text
stringlengths 14
5.22M
| meta
dict | __index_level_0__
int64 0
9.97k
| input_ids
listlengths 128
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| attention_mask
listlengths 128
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| labels
listlengths 128
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|
|---|---|---|---|---|---|
package cmp
type Sender interface {
Send(interface{}) error
}
type Receiver interface {
Receive() (interface{}, error)
}
type Communicator interface {
Sender
Receiver
}
| {
"redpajama_set_name": "RedPajamaGithub"
} | 2,406 | [
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Remix, a tech startup that offers data and planning tools for public transportation officials, has raised $15 million in investment.
The Series B round, led by Energy Impact Partners with participation from Sequoia Capital, brings Remix's total funding up to $27 million, according to Crunchbase. The company didn't get into specific plans for how it will use the influx of money, but it did use a blog post announcing the round to outline the challenges it sees facing its customers — chiefly, the need to be ready despite not knowing how self-driving vehicles, ride-sharing, bike- and scooter-sharing and a host of other technologies might change things.
"The short answer is that we'll use the money to continue investing in our technology and our team, maintaining our focus on the needs of cities and continuing to solve pressing challenges in the transportation industry," CEO Sam Hashemi wrote in the post.
Honolulu Turns to Remix to Plan Future Transportation NeedsLime and Spin to Share Detailed Use Data with LADOTData Sharing in Cities: What's the Worst That Could Happen?
The company offers a variety of software-as-a-service products designed to help governments do things like design streets, plan transit routes and keep an eye on how people are using new options like electric scooters. More than 300 cities around the world have used the company's technology, according to its website. They include King County, Wash.; Hillsborough Area Regional Transit in Tampa, Fla.; and the transit agency in the city of Rochester, Minn.
In a separate blog post, EIP Senior Vice President of Research and Strategy Shayle Kann specifically pointed to new mobility options as a major reason for investing in Remix. | {
"redpajama_set_name": "RedPajamaC4"
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Are you experiencing iPhone 4 Wi-Fi issues?
Get your iPhone 4 repaired fast at RepairZoom!
Just click Add To Cart to purchase this diagnostic service right now. Our free shipping is included in the price. How nice is that? We also offer some expedited shipping choices for a small upgrade fee during check out. Need more information? Read below for more details about this iPhone 4 Wireless Repair Diagnostic. Or call us at 877-274-5964 for any other questions about this iPhone 4 Wireless Repair Diagnostic.
Does your iPhone 4 have wireless problems? We love the Apple iPhone 4. It is an amazing iPhone with multiple wireless radio technologies. In fact, there are three wireless systems running inside your Verizon iPhone 4. These three systems are called the Bluetooth system, the WiFi system, and the GSM system. If you hare having issues in any of these wireless areas, let the experts at RepairZoom diagnose and repair your iPhone 4 problems.The RepairZoom experts are some of the most experienced technicians you can find anywhere to diagnose and repair your iPhone 4 wireless problems. Nearly all of our iPhone services and repairs are completed and shipped back to you the SAME DAY we receive your device. We also offer FREE SHIPPING both ways for this Wi-Fi repair diagnostic service. (Note: Your customized free shipping label will be available to print when you check-out of the online store.) The fastest way to get this iPhone 4 wireless problems diagnostic service started is to add this item to your cart, OR call us toll free right now at 877-274-5964 to set up the order by phone.Cool -- all that makes sense. Finally, a company that get's it. RepairZoom! | {
"redpajama_set_name": "RedPajamaC4"
} | 4,084 | [
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|
from __future__ import annotations
from pants.core.util_rules.config_files import ConfigFilesRequest
from pants.core.util_rules.external_tool import TemplatedExternalTool
from pants.engine.platform import Platform
from pants.option.option_types import ArgsListOption, BoolOption, FileOption, SkipOption
from pants.util.strutil import softwrap
class GolangciLint(TemplatedExternalTool):
options_scope = "golangci-lint"
name = "golangci-lint"
help = "A fast Go linters runner"
default_version = "1.50.1"
default_known_versions = [
"1.50.1|macos_arm64 |3ca9753d7804b34f9165427fbe339dbea69bd80be8a10e3f02c6037393b2e1c4|9726190", # noqa: E501
"1.50.1|macos_x86_64|0f615fb8c364f6e4a213f2ed2ff7aa1fc2b208addf29511e89c03534067bbf57|10007042", # noqa: E501
"1.50.1|linux_arm64 |3ea0a6d5946340f6831646e2c67a317dd9b35bdc4e09b2df953a86f09ba05d74|8911583", # noqa: E501
"1.50.1|linux_x86_64|4ba1dc9dbdf05b7bdc6f0e04bdfe6f63aa70576f51817be1b2540bbce017b69a|9682295", # noqa: E501
]
default_url_template = (
"https://github.com/golangci/golangci-lint/releases/download/v{version}/"
"golangci-lint-{version}-{platform}.tar.gz"
)
default_url_platform_mapping = {
"macos_arm64": "darwin-arm64",
"macos_x86_64": "darwin-amd64",
"linux_arm64": "linux-arm64",
"linux_x86_64": "linux-amd64",
}
skip = SkipOption("lint")
args = ArgsListOption(example="--enable gocritic")
config = FileOption(
"--config",
default=None,
advanced=True,
help=lambda cls: softwrap(
f"""
Path to a YAML config file understood by golangci-lint
(https://golangci-lint.run/usage/configuration/#config-file).
Setting this option will disable `[{cls.options_scope}].config_discovery`.
Use this option if the config is located in a non-standard location.
"""
),
)
config_discovery = BoolOption(
"--config-discovery",
default=True,
advanced=True,
help=lambda cls: softwrap(
f"""
If true, Pants will include all relevant config files during runs
(`.golangci.yml`, `.golangci.yaml`, `golangci.toml`, and `golangci.json`).
Use `[{cls.options_scope}].config` instead if your config is in a
non-standard location.
"""
),
)
def config_request(self) -> ConfigFilesRequest:
# Refer to https://golangci-lint.run/usage/configuration
# for how config files are discovered.
return ConfigFilesRequest(
specified=self.config,
specified_option_name=f"[{self.options_scope}].config",
discovery=self.config_discovery,
check_existence=[
".golangci.json",
".golangci.toml",
".golangci.yaml",
".golangci.yml",
],
)
def generate_exe(self, platform: Platform) -> str:
return (
f"./golangci-lint-{self.version}-"
f"{self.url_platform_mapping[platform.value]}/golangci-lint"
)
| {
"redpajama_set_name": "RedPajamaGithub"
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Cloudy skies, moderate fog expected in Delhi on R-Day
New Delhi, Jan 25 (PTI) Overcast conditions are predicted in Delhi on Republic Day and moderate fog is expected to lower visibility levels to 200 metres.
The maximum and minimum temperatures are likely to settle around 9 degrees Celsius and 19 degrees Celsius, respectively, the India Meteorological Department said.
"Moderate fog is likely in the city on Thursday morning. Cloudy conditions will prevail during the day," an official said.
According to the weather office, 'very dense' fog is when visibility is between 0 and 50 metres, 51 and 200 metres is 'dense', 201 and 500 metres 'moderate', and 501 and 1,000 metres 'shallow'.
Delhi witnessed overcast skies and logged a minimum temperature of 10.6 degrees Celsius, five notches above normal, on Wednesday.
The maximum temperature settled at 19.3 degrees Celsius, two notches below normal.
The Safdarjung Observatory, Delhi's primary weather station, had logged a minimum temperature of 12.3 degrees Celsius, the highest this month so far, on Tuesday.
The maximum temperature had settled at 21.6 degrees Celsius.
The city had recorded a maximum temperature of 25.9 degrees Celsius on Monday -- the highest in the month in four years -- according to the weather department.
Clouds trap heat that gets through during the day, keeping night-time temperatures above normal.
However, cloudy weather reduces daytime temperatures by preventing exposure to the sun.
Delhi is likely to see cloudy skies for the next four to five days.
A fresh western disturbance may lead to light rainfall on January 29, it said. Delhi has not recorded any rainfall this winter season so far. The Met department attributed it to the lack of strong western disturbances in November and December.
Last year, the city had recorded 82.2 mm rainfall in January, the highest in the month since 1901. The capital logged eight cold wave days in January this year, the most in the month in 15 years. It saw seven cold wave days in January 2020 while it did not record any such day last year.
The city recorded two intense coldwave spells -- from January 16 to January 18 and January 5 to 9, according to IMD data.
It, however, did not record any cold days. Delhi has also logged over 50 hours of dense fog this month so far, the highest since 2019. PTI GVS TDS TDS | {
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How will MPs amend Theresa May's Brexit plan B?
A complete guide to the amendments to the 29 January vote.
MPs will vote on Theresa May's dubiously-titled Plan B for Brexit this evening – with another defeat a foregone conclusion.
But this time, unlike the first iteration of the meaningful vote, the substantive, consequential action will come not on the government's main motion, but on a host of backbench amendments tabled in the hope of forcing ministers to change direction.
Some aim to do so by giving MPs unprecedented control over parliamentary business; others solicit conclusive expressions of opinion on the potential options ahead. A comprehensive rolling guide follows.
Corbyn's amendment would compel ministers to hold parliamentary debates – and votes – on options that would prevent a no-deal Brexit. Two, corresponding to the remaining paths Labour frontbenchers say are still open, are mentioned specifically: the party's official Brexit model of high single market alignment and a permanent customs union; and a "public vote on a deal or a proposition that has commanded the support of the House of Commons".
The second option has prompted the sort of celebrations one would expect from supporters of a second referendum within and without the Parliamentary Labour Party – that is to say, premature ones. What the amendment does not do is bind the leadership to whipping its MPs to support the referendum option if such a vote takes place under the terms it sets out, which it won't.
That said, Labour MPs will, naturally, be whipped to vote for this amendment by the leadership; that imprimatur alone will be enough to preclude the necessary support it needs from opposition parties, especially pro-EU Conservatives, to pass. The explicit mention of a second referendum is likely to repel some of the several dozen Labour MPs who are opposed to one, too.
This cross-party initiative spearheaded by the Home Affairs Select Committee chair and Nick Boles, the Conservative MP championing a Norway-style Brexit, would tear up the parliamentary rulebook instituted after the obstructionist campaign of Irish Parliamentary Party leader Charles Stewart Parnell in the 1880s, in the hope of stopping no-deal.
To do so, the amendment would revoke Standing Order 14 – the parliamentary rule that gives precedence to government business – for the duration of 5 February. In its absence, a Brexit bill sponsored by at least 10 MPs from four different parties would usurp everything else on the Commons order paper.
Cooper and Boles intend to use said powers to table legislative proposals to extend Article 50 for nine months in the event that a Withdrawal Agreement is not approved by parliament by 26 February – in effect, a backstop that would allow MPs to defer a no-deal exit.
Given the support it commands from pro-EU Conservatives, the plan stands a fighting chance if it secures the backing of the Labour leadership, which told frontbenchers yesterday it was supporting the plan. Doing so risks setting a precedent that could hobble its command of the parliamentary agenda should it come to power as a minority government, however, and some MPs in Leave constituencies in the North and Midlands are understood to have serious reservations. Amber Rudd has suggested that up to 40 government ministers could resign to vote for Cooper's proposals if collective responsibility is not suspended for the vote, but support for the amendment from MPs who explicitly advocate stopping Brexit could dissuade Tories.
The Tory Remainer had originally proposed a radical amendment that would have allowed a qualified minority of 300 MPs, provided representatives from four separate parties were among their number, to dictate the business of the Commons.
Unfavourable press coverage and with it backlash from parliamentary colleagues saw him drop that plan and in its place table an amendment – with the support of Tory Remainers, Labour backbenchers, the SNP, Liberal Democrats and Greens – that would force ministers to give MPs six full days of debate on alternative Brexit plans before March 26.
It would use the same mechanism proposed by Cooper's amendment to take control of the parliamentary timetable on 5 and 12 February and 5, 12, 19 and 26 March, allowing for a series of debates and indicative votes.
Only if Labour whips for it.
The 1922 Committee chairman - who surprised Westminster when he voted against the Withdrawal Agreement earlier this month - has tabled an amendment that would require the backstop to be replaced by alternative arrangements.
As with Murrison's amendment, it could not bind Brussels - but is instead intended to give May a renewed negotiating mandate ahead of a return to Brussels.
Likely to win the approval of the DUP and European Research Group, and could yet be accepted by the government given the support it enjoys from May loyalists like Damian Green.
"requires the Northern Ireland backstop to be replaced with alternative arrangements to avoid a hard border; supports leaving the European Union with a deal and would therefore support the Withdrawal Agreement subject to this change".
Tabled by Labour frontbencher Jack Dromey and Tory Caroline Spelman, the amendment straightforwardly asks MPs to reject no deal. It does not, however, propose a procedure for doing so.
Rejecting no-deal in the abstract is an uncontentious ask of MPs. Almost certainly.
The Walthamstow MP's cross-party amendment – also signed by her Labour colleagues Lisa Nandy, Liz Kendall, Alison McGovern; the Lib Dems' Norman Lamb and Christine Jardine; the Greens' Caroline Lucas, and others – would require ministers to seek an Article 50 extension and establish a Citizens' Assembly of 250 members to consider a range of Brexit options. Its advocates compare it to the body that considered reform of Ireland's constitutional ban on abortion.
Creasy's Assembly would be required to report to Parliament within 10 weeks. The government would be obliged to respond within a fortnight, and, if accepting its recommendations, would have to lay its plans for their implementation before MPs. There is no mention of it being bound to do so, however.
No. Despite the high profile of its more thoughtful advocates, and favourable coverage in the Guardian, this is the sort of idea that is unlikely to ever get much of a hearing outside of its comment pages. The identity of its lead backers, among other things, as good as guarantees it will be ignored by Team Corbyn, to say nothing of the seven Conservative MPs anyone seeking a Commons majority for anything requires. Its champions have nonetheless been buoyed by apparently positive responses from Tory ministers such as David Lidington, May's de facto deputy.
The Brexit Select Committee chairman's amendment demands ministers hold a series of non-binding votes on four options: leaving the EU under the terms of the Withdrawal Agreement and Political Declaration negotiated by Theresa May; leaving without a deal; directing the government to renegotiate the Irish backstop, a Canada-style free trade agreement or joining the EFTA pillar of the EEA; and a second referendum.
Indicative votes have significant support from MPs across the Commons, including a number of government ministers. Its best hope would come with a free vote, which may yet be forthcoming.
The former Labour member for Birkenhead's proposal is essentially the same as that proposed by Benn, albeit with a broader range of options. Co-sponsored by former Tory minister Ed Vaisey, the amendment proposes indicative votes on renegotiating the backstop; no-deal; extending Article 50; negotiating a customs union; a Canada-style free trade agreement; an EEA-style arrangment similar to Norway's; and a second referendum. Its list is not exhaustive, however.
Though his proposal is less well-supported than Benn's, indicative votes have significant support from MPs across the Commons, including a number of government ministers. Its best hope would come with a free vote, which may yet be forthcoming.
Backed by several backbench Labour MPs as well as Norman Lamb and the SNP's Drew Hendry, the Business Select Committee chairwoman calls upon ministers to seek an Article 50 extension of unspecified length for unspecified purposes.
"…and, in the event that the House of Commons has not passed a resolution approving the negotiated withdrawal agreement and the framework for the future relationship for the purposes of section 13(1)(b) of the European Union (Withdrawal) Act 2018 by 26 February 2019, requires the Prime Minister to seek an extension to the period of two years specified in Article 50(3) of the Treaty on European Union.
Baron, a pro-Brexit Conservative backbencher, was the only MP to push their amendment to the first meaningful vote motion to a divison. His proposal to give the UK the right to unilaterally terminate the backstop was overwhelmingly defeated by 600 votes to 24. That experience, however, has not stopped him from tabling a further two along similar lines.
The first would withhold parliamentary approval from a backstop whose provisions lasted longer than six months; while the second demands a unilateral exit clause.
Unlikely, given that opposition to the backstop is a mainly Tory preoccupation. But its proponents would argue that securing a majority is not the point. Rather the objective is to demonstrate the strength and breadth of Conservative opposition to the backstop.
That said, however, Baron's amendments lack the wide support enjoyed by his colleague Andrew Murrison, so it is concievable that they will do less well. The constituency of Tories who want to ditch the backstop entirely, rather than circumscribe the way it works, is also relatively small.
The Liberal Democrat leader's amendment instructs ministers to rule out a no-deal scenario and hold a second referendum, one of whose options would be remaining in the EU.
The Liberal Democrat MP has proposed that a committee of 17 MPs from all parties -- with seats allocated in proportionate with vote shares at the 2017 election, denying the government a majority -- be given powers to determine future Commons business on Brexit and sit around the clock. He also hints that it would have the power to negotiate with Brussels.
Unlikely to win support from either the Labour leadership or a significant number of Tory rebels.
Tabled by the Westminster leaders of the SNP and Plaid Cymru, this amendment urges the government to take note of the rejection of the withdrawal agreement by the devolved legislatures in Wales and Scotland and extend Article 50.
The SNP chair of the International Trade Select Committee proposes the government brings forward the legislation required to withdraw the UK's Article 50 notification before March 29.
MacNeil's amendment bears only his signature and that of an SNP colleague, Pete Wishart, meaning its chances of selection are slim. As for its chances of passing, few Remainers would be willing to take the nuclear option of calling for the revocation of Article 50 when other amendments propose a less controversial extension.
The following amendments were also tabled but have since been pulled ahead of tonight's vote.
The Conservative chairman of the Northern Ireland Affairs select committee has proposed an amendment that would make parliament's approval of the Withdrawal Agreement conditional on the insertion of a time limit on the Irish backstop – which, if secured, would win over the DUP and with them a substantial number of Tory Brexiteers.
Its approval, of course, would not bind Brussels, who have hitherto insisted that the divorce deal is not up for renegotiation. Instead, it would give the prime minister a quantifiable indicator of the mood of the Commons that might help her make a case for the EU's allowing so when she returns to Brussels.
Murrison agreed not to table his amendment after Theresa May told Tory MPs she would support Graham Brady's, in the hope of increasing its chances of selection by the Speaker and success in the Commons.
The first of three amendments originally tabled by the Tory Brexiteer, it aimed to deny parliamentary approval to a Withdrawal Agreement that contained any kind of backstop.
Like Andrew Murrison, Baron agreed not to table this amendment after Theresa May told Tory MPs she would support Graham Brady's, in the hope of increasing its chances of selection by the Speaker and success in the Commons. | {
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posted in PHP Leadership and tagged application deployment, application development, downtime, PHP 7, php 7.1, Zend Server on July 6, 2017 by Zeev Suraski.
Back in the old days, when PHP was in its infancy – deployment details were "left as an exercise to the reader," in this case, developers. There was no standardized deployment model, guidelines, or best practices on how deployment should be done. Early on, in the vast majority of cases – deployment simply meant copying the updated PHP files to the right directory in the server – relying on PHP's behavior to instantly start using these new files.
As PHP and the types of applications it's being used for matured, this simplistic approach started showing its limits, especially for business-critical apps. The problem had to do with the fact that PHP loads individual files as they are needed, and PHP applications typically involve hundreds, and sometimes even thousands of files in the context of a single request. Therefore, the files in a request may change during execution, resulting in the request beginning to execute with one set of files, and continuing execution with a different set of files. In some cases it could even result in a partially-changed file (one that has not yet been fully updated) being loaded. Depending on the nature of changes in the new version and the specific point in time the app happened to load specific individual files, this could result in nothing at all, fatal errors, and or possibly execution of flawed logic which arguably is the most problematic outcome.
In addition to not providing atomicity, these simplistic mechanisms also provided no mechanisms for management (which version is deployed?), rollback, or cross-cluster synchronization.
When we released the Zend deployment technology as a part of Zend Server, it aimed to solve these drawbacks. It placed emphasis on being atomic – apps would never be served by a mix of both new and old files, it allowed for easy management of apps supporting installation, updating, and rollback workflows – and provided seamless cross-cluster synchronization.
However, the atomic nature of the Zend deployment technology came at a cost – it required a web server restart for every application update. Initially, this was a reasonable cost to pay, as application updates weren't that frequent, and Zend Server also provided ways to ensure that at any given time, only a small subset of the servers in the cluster would be undergoing a restart – so the cluster as a whole continued responding properly.
With the growing popularity of continuous delivery, it became increasingly problematic to require web server restarts for every update. Therefore in Zend Server 9.1, we've rolled out a new mechanism that allows for zero downtime application updates, not just at the cluster level – but at each server level too.
The archive containing the new version is extracted into a new location on the server's filesystem.
The web server configuration is updated to point to the new location.
The web server process (Apache or nginx) is restarted for the new configuration to take effect.
The same process was repeated in every server in the cluster, at a configurable level of parallelism – in order to ensure that not all servers in the cluster are restarted at the same time, so that the cluster as a whole continues to respond.
The zero downtime approach tackles the job a bit differently. First, from the very first deployment, the web server is configured not to point to the actual location on the filesystem where the application files reside but rather, to a symbolic link, which in turn points to the application files' location.
The archive containing the new version is extracted into a new location on the server's filesystem (identical to the previous method).
The symbolic link pointer is moved to point to the new application location on the filesystem. The web server configuration remains untouched.
This is simple enough, but in order to ensure a fully atomic behavior, there's one extra step that needs to happen. Without it, it's still possible for requests to begin executing with an old set of files, and continue execution with a new set of files – with all of the potential risks associated.
To be truly atomic, we must ensure that there's a way for every request to finish execution using the same set of files it began execution with, and thankfully, zend_deployment_application_path() API does exactly that.
Regardless of when it's called during the request lifetime, this API will always return the base path from which the request began executing – even if a new version was deployed in the meantime. Using this path as the base path for loading all subsequent PHP files into memory ensures that we're using just one set of files the entire time. And given most PHP applications nowadays use autoloaders, introducing this base path across the entire application typically involves only minor changes to that single autoloading function.
The new deployment strategy in Zend Server 9.1 allows companies to update their applications a lot more frequently and without affecting end-user service. All servers remain working in full capacity without interruption or performance degradation. As such, it's a perfect fit for continuous delivery, as well as any other scenario where frequent updates are needed.
While the 'last mile' of ensuring the atomic nature of updates requires a tiny bit of manual intervention (in the form of one-time minor code changes), the outcome is well worth it, and we recommend all our customers switch to this strategy.
As always, our teams are here to help if you have any questions or need any help or guidance implementing this!
See what else is new in Zend Server 9.1.
Is the problem with opcache/realpath ttl solved for this symlink-based deployments ?
see: https://codeascraft.com/2013/07/01/atomic-deploys-at-etsy/ – opcache is NOT inode-based! | {
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Recent narrative fiction and film increasingly exploit, explore and thematize the embodied mind, revealing the tenacity of a certain brand of humanism. The presence of narratively based concepts of personal identity even in texts which explore posthuman possibilities is strong proof that our basic understanding of what it means to be human has, despite appearances, remained mostly unchanged. This is so even though our perception of time has been greatly modified by the same technology which both interrupts and allows for the rearrangement of our experience of time at a rate and a level of ease which, until recently, had never been possible.
Basing his views on a long line of philosophers and literary theorists such as Paul Ricoeur, Daniel Dennett and Francisco Varela, Escobar maintains in The Persistence of the Human that narrative plays an essential role in the process of constituting and maintaining a sense of self. It is narrative's effect on the embodied mind which gives it such force. Narrative projects us into possible spaces, shaping a temporary corporeality termed the "meta-body," a hybrid shared by the lived body and an imagined corporeal sense. The meta-body is a secondary embodiment that we inhabit for however long our narrative immersion lasts – something which, in today's world, may be a question of milliseconds or hours. The more agreeable the meta-body is, the less happy we are upon being abruptly removed from it, though the return is essential.
We want to be able to slip back and forth between this secondary embodiment and that of our lived body; each move entails both forgetting and remembering different subject positions (loss and recuperation being salient themes in the works which highlight this process). The negotiation of the transfer between these states is shaped by culture and technology and this is something which is precisely in flux now as multiple, ephemeral narrative immersion experiences are created by the different screens we come into contact with.
Matthew Escobar, Ph.D. Princeton University, is Associate Professor of Languages, Literatures and Cultures and Director of Latin American and Latino/a Studies at Seton Hall University.
All those interested in contemporary literature and film in English, French and Spanish as well as questions of consciousness, the human, corporeality, narrative and personal identity. | {
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I combine exotic tropical plants and cactus with up-cycled, recycled, vintage, found and foraged materials to design living wall and table top sculptures that surprise and entertain and celebrate ecology and the natural environment. The materials I use are sourced from the woods and waters around my country home, from charity oriented thrift shops, on the street, and the occasional dumpster dive. I have a small scale home-based plant nursery and these living beings are in and of themselves the ultimate in artistry – nature is the true crafter here, I am just in partnership. I feel privileged to care for these green beings, give them funky habitats, and send them out in the world to live with other people. Likewise with the findings I pair them with; forlorn toys, pieces of craftwork from the past, river stones and gnarly driftwood, thrift store kitsch and construction site scraps and whatever catches my eye from having spirit in it. Sky House: organic, low-tech, funky, junky, earthy, living sculptures. | {
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When it comes to developing their own youth, few teams in the world can compete with Ajax. When you are talking about a production line of real world-class talent, Ajax is one of the first club names that comes to mind. The Football Manager database has seen many great Ajax youth players in the past, but what about Football Manager 2018?
In this article we will taking a look at 6 of these Ajax wonderkids. And for all of these we can say; you will sign them eventually.
19-year-old Carel Eiting has made the jump from the Ajax U19 to the Jong Ajax team this season and he has captained the side on more than one occasion. In FM18 Eiting is seen as one of the bigger young talents at the club. He starts off in Jong Ajax, but will be able to make the jump soon. He is a versatile player that can play as a centre-back, a defensive midfielder and a central midfielder. He will be on his best on the MC position as a Deep Lying Playmaker.
18-year-old Matthijs de Ligt was a U19 player last season when former manager Peter Bosz decided to give him his debut. The young defender impressed enough to feature in eleven league games and even the Europa League final (2-0 loss against Man. United). The Football Manager 2018 database reflects the talent that was shown last season. De Ligt is already one of the better defenders at Ajax and he has the potential to be an elite defender. He can play on more than one position and he is a ball-playing defender. In a 3-man defense, De Ligt would be an ideal addition.
After Davy Klaassen made a big money move to Everton, Donny van de Beek jumped right into Ajax's first team. The young central midfielder has even been called up for the Dutch national team in recent months. In the FM18 database Van de Beek could be a very good player. He is 20-years-old and will attract some of the big teams right away. We have seen him end up at clubs like Paris Saint-Germain and Tottenham Hotspur, making him one of the elite players in Europe. Van de Beek is one of the real gems at Ajax.
Whilst Ajax is well known for its own youth set-up, the club decided to splash the cash last winter on Brazilian winger David Neres. The club paid 13.25M, making Neres one of the most expensive players in the club's history. Despite a difficult first 6 months at Ajax, the Brazilian has settled in well, claiming a spot in the first team. Neres is a good player in FM18, but we feel he won't live up to other great Brazilian players like Neymar, Gabriel Jesus and Philippe Coutinho. Whilst Neres could be player that can shine in a big league like the Premier League, we don't think he will be one of the elite players in the game.
Justin Kluivert followed his fathers footsteps at Ajax, making his debut before he turned 18. Whilst his father made the winning goal in the Champions League final in 1995, the young Kluivert has yet to impress in the Ajax first team. In Football Manager 2018 Kluivert is a really good dribbler with a lot of speed. Being only 18-years-old there is much potential to be explored. He has the quality to feature in the Ajax first team right away and he will only become better as the years progress. We are sure he will develop into a Dutch national player, but we fear the European elite might be a step too big for Kluivert.
Danish striker Kasper Dolberg got his big break last season and showed on more than one occasion he is a very gifted football player. He was nominated for the European Golden Boy earlier this year and also made his debut for the Danish national team. Dolberg was consdered a big wonderkid in FM17 and he has continued that trend in Football Manager 2018. The young Dane is one of the best strikers under 20 and will become one of the elite strikers in almost every save you will play.
Although we have named 6 of the best wonderkids at Ajax, the club has several other very talented players at the club. A small list with talented players to watch during your games.
Would you like to see all Football Manager 2018 Wonderkids? We have created the Ultimate Wonderkids List for Football Manager 2018. | {
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Asterisk Hotel offers 3-star superior accommodation in 2 restored 19th century buildings in the centre of Amsterdam. It is situated at 10 minutes walking distance from the Rijksmuseum and offers free WiFi in the entire property. Guests can relax in the garden or lobby and explore the surroundings where one can find cafes and restaurants.
All rooms are accessible by lift and are equipped with a flat-screen TV a safe work desk and a private bathroom. A 24-hour check-in front desk is available and in the lobby guests can enjoy water and a small snack in the afternoon.
The hotel offers a paid airport shuttle and taxi service upon request. A tour desk where excursions tours museum tickets souvenirs and toiletries can be bought is also present. Breakfast includes a.o. fresh baked eggs: fried omelette scrambled or cooked pancakes bacon salmon mozzarella various french cheeses fresh fruit salad different types of bread cereals toppings and fruit juices.
Many attractions can be found in the vicinity such as The Heineken Experience (350 metres) Muntplein (11 km) Van Gogh Museum (11 km) and the Hermitage (11 km). The hotel is only 250 metres from the Weteringcircuit Tram Stop where 4 tram lines run. | {
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Ski Spree in Sainte Foy, France
Will Ross, September 18, 2013
The small French ski resort of Sainte Foy in the Savoie department of the Rhône-Alpes is known by a select few for the quality and quantity of its off-piste areas, all serviced by three end-to-end chair lifts. Backcountry routes slip off the sides of the piste, making for an easy-to-access powder hunting experience.
Thanks to its north-west facing slopes, snow hangs around for longer in Sainte Foy than other larger ski areas. Once the snowline drops down the mountain as far as the village, Sainte Foy becomes a furious tree skiing hub.
When it comes to thinking about lift passes, Sainte Foy is way cheaper than other resorts with a 6-day adult pass at €191.50, and a 6-day infant at €154 (full 2015/16 prices). Yes, lifts aren't as developed as many of the larger resorts, but the rustic charm of his European village is still intact.
Navigating the terrain
Three lifts get you to the Col de l'Aiguille (2620m) from where you can find untracked powder to the left and right. From the Rocher de Pierre d'Arbine (2647m) there are three more routes, one of which leads down the the Refuge le Monal (accommodation). Also grin and bear a moderate climb along the to the left of the top chair lift to the Pointe de la Foglietta (2930m) for 1700 metres of top class off piste vertical descent.
If you're looking to combine some of your own routes with some inspiration from elite freeride skiers, who have passed through the mountain for Freeride World Tour Qualifiers. through Sainte Foy on 19th March 2016 – the Freeride World Tour Qualifiers. Download the off-piste winter map and get planning your routes.
Image: Philippe Royer / OT Sainte Foy
Those looking for ski guides or tuition should seek out Tarentaise Tours is a slick adventure company operating out of Sainte Foy. Their winter activities include an array of alpine treats, including single-day ski tours in the Tarentaise Valley and multi-day hut-to-hut options. Additionally, the ESF Sainte-Foy has a group of instructors that specialise in off-piste guiding. Find out how to book an ESF off-piste guide.
Sainte Foy Accommodation
For large, catered groups, check out Chalet Rassel – outrageous decor with sumptuous 4-course meals in the evening. Another chalet option is the hotel/chalet Yellowstone Ski Lodge which also wins points for design.
Yellowstone Ski Lodge
Getting to Sainte Foy by train
During the winter, Eurostar has a direct service to Bourg-Saint-Maurice from London leaving on Friday evenings and Saturday mornings. Over the Christmas and New Year periods there are trains on Sundays too.
Direct trains return to London from the French Alps on Saturday mornings and Saturday afternoons during the ski season and again on Sunday during the Christmas and New Year periods.
To get from Bourg Saint-Maurice, a taxi of 55 euros. Failing this buses run regularly between the station and the resort. | {
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ADDIS ABABA, May 11 (Xinhua) -- The United Nations Office for the Coordination of Humanitarian Affairs (UNOCHA) on Friday said ethnic clashes in Southern Ethiopia have displaced more than 200,000 people.
UNOCHA said it's working with officials from Southern regional state, home area of ethnic Gedeos and officials from Oromia regional state, home area of ethnic Oromos, to repatriate the internally displaced people, the office said in a statement.
Clashes between ethnic Gedeos and ethnic Oromos started on April 13, apparently over utilization of resources along the shared border of the two communities, the statement said.
As of May 1, 85,000 displaced people from both communities have returned to their homes, UNOCHA said, adding that further work is being undertaken to rehabilitate the remaining displaced people.
However, critics say the model magnifies ethnic diversity at the expense of national unity, leading to occasional ethnic tension and clashes. | {
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The Residents Initiative is pleased to inform you about the exhibition of cultural historical photos in the Nieuwe Uilenburgerstraat at the 'Nuon'-square number 27.
After completion of the renovation of the square in the summer of 2009, the Residents Initiative in October 2009 developed the plan to exhibit historical photos in public space of the Nieuwe Uilenburgerstraat.
In the City Archives we found documentary photos in black and white of the Jewish market in the Nieuwe Uilenburgerstraat, which in 1935 had been taken by the Jewish Austrian born photographer Wolf Suschitzky. . Mr. Suschitzky, now 98 years, is delighted that the inhabitants of the Nieuwe Uilenburgerstraat realised the exhibition of his photos into public space where they had been taken 75 years ago.
After eight months of preparation on June 28, 2010 three photos of Wolf Suschitsky where placed in large format on canvas in steel frames at the facade of the building from Alliander (formerly Nuon) right infront of the square in the Nieuwe Uilenburgerstraat. The sizes: 3.43 x 2.75 meters (2x) and 1.70 x 2.75 meters (1x).
In addition, on the wall next to the facade of Alliander, on July 13, 2010 a plate with information about the photo exhibition was placed.
On this plate, the three pictures of Wolf Suschitsky are engraved, along with one photo from the City Archives from 1943, showing a virtually empty Nieuwe Uilenburgerstraat with the ghetto signs 'Jewish district / Judenviertel'.
The exhibition aims to residents, the neighborhood and especially tourists to celebrate the cultural history of the area and at the same time wants to draw attention to the historical facts by the plate.
The photo project has been funded by the Community Centre 'The Old City' and the Amsterdam Fund for the Arts.
The project of the Residents Initiative is legally represented by Foundation JAM.
The intention is to place also other cultural historical photos in rotation. The plate will remain a permanent part of the exhibition. | {
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In the forming process of glassware products, the stress caused by temperature difference is called thermal stress.
How to distinguish the quality of glass wine glasses? Do you know?
We all know that wine culture has a long time in our history. Today, people still inherit. When it comes to wine, we all go to drink. No matter what kind of wine, we will use wine glasses when we drink.
Some of the names of the cups we touched in our daily life includes:shot glasses, goblets, squat cups, Bordeaux wine glasses, cocktail glasses, white wine glasses, Burgundy wine glasses, etc.
WHY DRINK DIFFERENT KINDS OF RED WINE IN DIFFERENT GLASS CUP?
10 kinds of classic beer cups, which one is commonly used? | {
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Samsung SGH-X120 — стільниковий телефон фірми Samsung Electronics.
Схожі моделі
Samsung SGH-C100
Samsung SGH-C110
LG G5310
Samsung SGH-C200
Samsung SGH-X140
Див. також
Samsung Electronics
Посилання
Опис на сайті Samsung
X
Мобільні телефони, представлені в 2004 році
Мобільні телефони з інфрачервоним передавачем | {
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Sleep is important to ensure our health and fitness. However, thousands if not countless people struggle with insomnia every day or, more appropriately, every night. Due to sleep deprivation, these individuals establish some illnesses that, in turn, adversely affect their work, service, relationships, and general lifestyle.
Chamomile is an herb that people have been utilizing for centuries. It is known to promote sleep and deal with other ailments like indigestion.
Exercising and taking part in extreme physical activities a few hours before going to sleep can increase the adrenaline levels in the body and cause sleep disturbances.
Potatoes are complex carbohydrates that are suggested to be consumed before going to bed for natural, relaxing sleep.
Milk includes high levels of melatonin while honey is said to have sleep-inducing homes and may serve as a sedative.
Naps are usually suggested to be not over one hour because taking a snooze too much might interfere with sleep during the night.
Meditation is a practice where one focuses on a specific sound, item, or idea. Visualization, breathing, and controlled body movements all comprise the health-giving practice of meditation. Numerous medical studies suggest that this activity actually alleviates tension and promotes relaxation.
Its recommended that you will meditate at least for 10 minute a day.
These beverages are high in caffeine, a compound that is known to reduce the capability to sleep. For some, caffeine may also increase stress and anxiety and anxiety at high doses.
Dosages of about 250 milligrams may induce sleep. Taking in magnesium-rich foods like kelp, wheat bran, almonds, and cashew nuts might assist promote sound sleep.
Checking out, sewing, playing card games, and other activities need to be done before going to sleep. Health experts suggest that any action that is ritually done before going to sleep assists indicate the body that sleeping time is turning up.
Sleep apnea is a sleep condition in which breathing stops a few seconds throughout sleep. This condition is one of the reasons for daytime sleepiness.
This type of amino acid induces relaxation and promotes sound sleep.
One of the popular ways to use binaural beats is hacking your way to much better sleep. Paying attention to a Delta binaural beats session right before your head strikes the pillow, and proceeding right into your bedtime, can prep your brain for better (and deeper) sleep.
Melatonin is a hormonal agent that is produced in the pineal gland, a small gland in the brain that is responsible for sleep policy and wake cycles. Medical research studies show that high levels of this hormonal agent may promote sleep. Melatonin supplements are commonly considered as a safe and effective sleep aid.
Sleeping should be your way leading to happy dreams and not disturbing nightmares. Doing the above tips can welcome sandman's bag of sweet dreams during sleep. | {
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Watch one of the best photo of Vanessa Hudgens – it is 7 photo from all 2756 we have.
A picture Vanessa Hudgens can be downloaded for your laptop, tablet, computer, or mobile phone. Your devices must maintain Mac or Android OS. You may also use all wallpapers on IPhone and IPad.
If resolution 1200x1800 is less than your mobile device screen size, then you need to find another picture. All Vanessa Hudgens images has resolution of 1200x1800, and the filesize is 280 KB. | {
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Q: Missing Reference to Navigation Controller in Monotouch I am new to Monotouch and attempting to understand how some of the basics hang together. Hopefully someone out there will be able to assist.
I've created a test project in MonoDevelop based on the Multi-Screened Apps tutorial on the Xamarin site and have extended it to include a tableView. I am having issues with referencing the Navigation Controller in a view that I need to push a detail view onto to display the detail of an item tapped in the table via an accessory button. I know some of the coding is scrappy, just been trying to get it working at this stage rather than the clarity in the code! (I'm using the latest versions of all Mono tools/libraries etc and XCode 4 on Lion). Starting at the beginning here's the code in FinishedLaunching in AppDelegate.
window = new UIWindow (UIScreen.MainScreen.Bounds);
this.rootNavigationController = new UINavigationController();
// Create a new homescreen
HomeScreen homeScreen = new HomeScreen();
// Add the homescreen to the root navigation controller
this.rootNavigationController.PushViewController(homeScreen, false);
// Set the root view controller on the window - the navigation controller
// will handle the rest.
this.window.RootViewController = this.rootNavigationController;
// make the window visible
this.window.MakeKeyAndVisible ();
homeScreen just contains a button which loads a new view containing a table view (OrderList). Here's the button event handler.
void HandleOrdersButtonhandleTouchUpInside (object sender, EventArgs e)
{
if (orderListScreen == null)
orderListScreen = new OrderList();
NavigationController.PushViewController(orderListScreen, true);
}
This all works fine. I've got some dummy data that loads into the table view, which also works fine. OrderData is a simple class for testing which just contains a couple of properties. I've added an AccessoryButton to the cells and am trying to load a detail view when this is tapped. Here's the code that does this - comment in code where issue is! (I'd previously tested the AccessoryButtonTapped functionilty was working by just displaying an alert).
public override void AccessoryButtonTapped (UITableView tableView, NSIndexPath indexPath)
{
var dataSource = (OrdersTableViewDataSource)tableView.DataSource;
if (detailScreen == null)
detailScreen = new OrderDetailScreen();
OrderData theOrder = dataSource.OrdersData[indexPath.Row];
detailScreen.currentOrder = theOrder;
// Cant get a reference to NavigationController here to push the detail view!
// this.NavigationController is not available
this.NavigationController.PushViewController(detailScreen, true);
}
My understanding of NavigationControllers from what I've read so far is that this reference should be available through all views that originate from the root ViewController/NavigationController without the need to pass the reference from AppDelegate through the various view constructors?
Can anyone tell me what I might be missing here?
Thanks in advance.
** An update after reviewing Jason's comment: (Please let me know if this is the incorrect way to post updates)
So, I tried the following:
I saved a reference to the NavigationController in the constructor for the ViewController that contains the table view as follows:
public partial class OrderList : UIViewController
{
UINavigationController navController;
public OrderList () : base ("OrderList", null)
{
this.Title = "Orders";
navController = this.NavigationController;
}
Then passed that into the TableViewDelegate, where the AccessoryButtonTapped is handled, in the ViewDidLoad method.
public override void ViewDidLoad ()
{
orderTableView.DataSource = new OrdersTableViewDataSource();
orderTableView.Delegate = new OrdersTableViewDelegate(navController);
base.ViewDidLoad ();
}
Then referenced that in the TableViewDelegate:
public class OrdersTableViewDelegate : UITableViewDelegate
{
UINavigationController navController;
public OrdersTableViewDelegate(UINavigationController controller)
{
navController = controller;
}
// Rest of class definition
}
Then the reference to the NavigationController using navController compiles with the code as previously described using the following in the AccessoryButtonTapped method:
navController.PushViewController(detailScreen, true);
When I run this and tap on the AccessoryButton I get a null reference exception on navController. The reference to this.NavigationController in the ViewController constructor is null. Am I doing something in the wrong place or sequence?
Cheers
A: The NavigationController property is on your table's view controller. If you are trying to reference it from your table's datasource, you need to pass a reference to the controller when you create the datasource.
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Ramadan History - Why Ramadan is Important?
Considered the most sacred Muslim occassion, Ramadan is observed throughout the ninth month (also known as Ramadan) of the Islamic calendar. Held since ancient times, this holy event has pious Muslims fasting, practicing extreme self-restraint, praying, doing charitable activities and all such actions that are recommended by Islam. Go through our informative article on the "History of Ramadan" to know when Ramadan originated and how it came to be established. If you like reading about the fascinating history of Ramadan and want to share it with your friends and loved ones, please click here and refer it to the. Wish you a sacred Ramadan!
Ramadan is a time of spiritual reflection, improvement and increased devotion and worship. Muslims are expected to put more effort into following the teachings of Islam. The fast begins at dawn and ends at sunset. Ramadan also teaches Muslims how to better practice self-discipline, self-control, sacrifice, and empathy for those who are less fortunate and thus encouraging actions of generosity and charity. It becomes compulsory for Muslims to start fasting when they reach puberty, so long as they are healthy, sane and have no disabilities or illnesses. | {
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|
476 The Long Lost Tale (Part XXII)
Abigail and Alex lay on the bed, chests heaving, drawing much needed air.
Find authorized novels in Webnovel, faster updates, better experience, Please click <a href>www.webnovel.com/book/hellbound-with-you_16699683105884505/the-long-lost-tale-(part-xxii)_49349154182321990 for visiting.
Even though Abigail was tired, she didn't want to succumb to sleep, afraid that he would disappear once she closed her eyes. She raised herself up slightly and rested on her elbow, gazing down at his gorgeous face.
Silently, she traced every contour of his face with a featherlike touch of her finger, as if she was engraving everything to her memory. She did just that for a while until Alex spoke. "Abigail…" he uttered her name as he lifted his hand and caressed her cheek. Emotions were swirling around in his tantalizing eyes. His eyes were more beautiful and mesmerising than the starry night sky that Abi didn't want to look away.
"Hmm?" she smiled slightly but when she saw the serious look in his face, her smile slowly faded.
"I…" he paused, looking torn, as if he was making a decision right then on whether to tell her the truth or not. "I have something important to tell you." | {
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|
In case you haven't been following the "PEBBLE-GRAIN" THREAD because it doesn't apply to you, I've started one for you owners of 69 Camaro smooth steering wheels!
Ed, I have an early Oct 68 build Z. Do you need my info?? I alway thought it was smooth, but now I'm not sure what I have. It has had one of those vinyl? wheel covering on it for a long time, so I'll have to take it off partially to look if need be. I do know that it is the original wheel.
Jimmy, yes, if you would remove the cover and see what you have, I'd appreciate it. Look close because the graining wore off fairly quickly and it might appear to be smooth. The best way to check is looking over the entire wheel. Not all areas will be as worn as others.
Ed, will do. Not sure, it may take week or so for me to get a look.
I was able to check my '69's interior over this weekend. Although I am not the original owner I am almost positive that the interior is all original due to the age it is showing, and I have verified that the engine, trans, and rear end are all original. It has the Z/28 option and Rally Sport also. The steering wheel is definitely a plastic "smooth" one; I could find no trace of "pebbling" anywhere on it. The build date is 01C. The interior is 712 black standard. It has a console with the wood grain and also wood grain on the lower left part of the dash where the light and wiper switches are and where the radio control dials are. The steering wheel has wood grain with a rs emblem in chrome. It has no wood grain where the ashtray and glove box doors are. It does have a grab handle above the dash and chrome trim on the accellerator, brake, and clutch pedals. Hope this info helps.
I caught a typo. The interior is 711, not 712; it is a standard black interior. Sorry.
I finally took time to check a column from a 69 I bought as a parts car back in 84. It was very complete and original but rusted to bad to fix. Even today I wouldn't want to try it. It is a Rally Green/white vinyl top SS 350 with floor shift turbo 350, with 727 interior and no Z23. S/N# is 124379N550686 and was added to the data base many years ago. It has a non x code cowl tag with a 11D build date. It has a standard steering column with the "ss" emblem and no trim. Column date is 324. Now for the word you are all waiting to hear. It is a "smooth" wheel. I was not expecting to find this as I was going to use it for my 02D L78, which had a small diameter chrome spoke cushion grip wheel when I bought it. My L78 has a 711 interior with Z23. The "ss" wheel has cracks on the back side where the spokes meet the rim. Is that worth fixing?
I have a 69 Z 08E 676923 no console car. Thats close. | {
"redpajama_set_name": "RedPajamaC4"
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package org.jbehave.mojo;
import static org.apache.commons.lang.ArrayUtils.isNotEmpty;
import java.io.File;
import java.net.MalformedURLException;
import java.net.URL;
import java.util.ArrayList;
import java.util.List;
import java.util.Properties;
import java.util.concurrent.ExecutorService;
import org.apache.maven.plugin.AbstractMojo;
import org.jbehave.core.ConfigurableEmbedder;
import org.jbehave.core.InjectableEmbedder;
import org.jbehave.core.embedder.Embedder;
import org.jbehave.core.embedder.EmbedderClassLoader;
import org.jbehave.core.embedder.EmbedderControls;
import org.jbehave.core.embedder.EmbedderMonitor;
import org.jbehave.core.embedder.MetaFilter;
import org.jbehave.core.embedder.NullEmbedderMonitor;
import org.jbehave.core.embedder.UnmodifiableEmbedderControls;
import org.jbehave.core.embedder.executors.ExecutorServiceFactory;
import org.jbehave.core.failures.BatchFailures;
import org.jbehave.core.io.StoryFinder;
import org.jbehave.core.junit.AnnotatedEmbedderRunner;
import org.jbehave.core.model.Meta;
import org.jbehave.core.model.Scenario;
import org.jbehave.core.model.Story;
import org.jbehave.core.model.StoryDuration;
import org.jbehave.core.model.StoryMaps;
import org.jbehave.core.reporters.ReportsCount;
/**
* Abstract mojo that holds all the configuration parameters to specify and load
* stories.
*
* @requiresDependencyResolution test
*/
public abstract class AbstractEmbedderMojo extends AbstractMojo {
static final String TEST_SCOPE = "test";
/**
* @parameter expression="${project.build.sourceDirectory}"
* @required
*/
String sourceDirectory;
/**
* @parameter expression="${project.build.testSourceDirectory}"
* @required
*/
String testSourceDirectory;
/**
* @parameter expression="${project.build.outputDirectory}"
* @required
*/
String outputDirectory;
/**
* @parameter expression="${project.build.testOutputDirectory}"
* @required
*/
String testOutputDirectory;
/**
* The scope of the mojo classpath, either "compile" or "test"
*
* @parameter default-value="compile"
*/
String scope;
/**
* Include filters, relative to the root source directory determined by the
* scope
*
* @parameter
*/
List<String> includes;
/**
* Exclude filters, relative to the root source directory determined by the
* scope
*
* @parameter
*/
List<String> excludes;
/**
* Compile classpath.
*
* @parameter expression="${project.compileClasspathElements}"
* @required
* @readonly
*/
List<String> compileClasspathElements;
/**
* Test classpath.
*
* @parameter expression="${project.testClasspathElements}"
* @required
* @readonly
*/
List<String> testClasspathElements;
/**
* The boolean flag to skip stories
*
* @parameter default-value="false"
*/
boolean skip = false;
/**
* The boolean flag to run in batch mode
*
* @parameter default-value="false"
*/
boolean batch = false;
/**
* The boolean flag to ignore failure in stories
*
* @parameter default-value="false"
*/
boolean ignoreFailureInStories = false;
/**
* The boolean flag to ignore failure in view
*
* @parameter default-value="false"
*/
boolean ignoreFailureInView = false;
/**
* The boolean flag to generate view after stories are run
*
* @parameter default-value="true"
*/
boolean generateViewAfterStories = true;
/**
* The boolean flag to output failures in verbose mode
*
* @parameter default-value="false"
*/
boolean verboseFailures = false;
/**
* The boolean flag to output filtering in verbose mode
*
* @parameter default-value="false"
*/
boolean verboseFiltering = false;
/**
* The story timeouts
*
* @parameter
*/
String storyTimeouts;
/**
* The story timeout in secs
*
* @parameter
* @deprecated Use storyTimeouts
*/
long storyTimeoutInSecs;
/**
* The story timeout in secs by path
*
* @parameter
* @deprecated Use storyTimeouts
*/
String storyTimeoutInSecsByPath;
/**
* The boolean flag to fail on story timeout
*
* @parameter default-value="false"
*/
boolean failOnStoryTimeout = false;
/**
* The number of threads
*
* @parameter default-value="1"
*/
int threads = 1;
/**
* The embedder class
*
* @parameter default-value="org.jbehave.core.embedder.Embedder"
*/
String embedderClass = Embedder.class.getName();
/**
* The implementation class of the {@link ExecutorServiceFactory}
*
* @parameter
*/
String executorsClass;
/**
* The class that is injected with the embedder
*
* @parameter
*/
String injectableEmbedderClass;
/**
* The annotated embedder runner class
*
* @parameter default-value="org.jbehave.core.junit.AnnotatedEmbedderRunner"
* @deprecated Obsolete
*/
String annotatedEmbedderRunnerClass = AnnotatedEmbedderRunner.class.getName();
/**
* Used to find story paths and class names
*
* @parameter
*/
String storyFinderClass = StoryFinder.class.getName();
/**
* The meta filter
*
* @parameter
*/
String[] metaFilters;
/**
* The system properties
*
* @parameter
*/
Properties systemProperties = new Properties();
/**
* The class loader
*/
private EmbedderClassLoader classLoader;
/**
* Determines if the scope of the mojo classpath is "test"
*
* @return A boolean <code>true</code> if test scoped
*/
boolean isTestScope() {
return TEST_SCOPE.equals(scope);
}
String searchDirectory() {
if (isTestScope()) {
return testSourceDirectory;
}
return sourceDirectory;
}
String outputDirectory() {
if (isTestScope()) {
return testOutputDirectory;
}
return outputDirectory;
}
URL codeLocation() {
String outputDirectory = outputDirectory();
try {
return outputDirectory != null ? new File(outputDirectory).toURI().toURL() : null;
} catch (MalformedURLException e) {
throw new IllegalArgumentException("Failed to create code location from " + outputDirectory, e);
}
}
/**
* Returns the EmbedderClassLoader with the classpath element of the
* selected scope.
*
* @return An EmbedderClassLoader
*/
protected EmbedderClassLoader classLoader() {
if (classLoader == null) {
classLoader = new EmbedderClassLoader(classpathElements());
}
return classLoader;
}
List<String> classpathElements() {
List<String> classpathElements = compileClasspathElements;
if (isTestScope()) {
classpathElements = testClasspathElements;
}
return classpathElements;
}
/**
* Finds story paths, using the {@link #newStoryFinder()}, in the
* {@link #searchDirectory()} given specified {@link #includes} and
* {@link #excludes}.
*
* @return A List of story paths found
*/
protected List<String> storyPaths() {
getLog().debug("Searching for story paths including " + includes + " and excluding " + excludes);
List<String> storyPaths = newStoryFinder().findPaths(searchDirectory(), includes, excludes);
getLog().info("Found story paths: " + storyPaths);
return storyPaths;
}
/**
* Finds class names, using the {@link #newStoryFinder()}, in the
* {@link #searchDirectory()} given specified {@link #includes} and
* {@link #excludes}.
*
* @return A List of class names found
*/
protected List<String> classNames() {
getLog().debug("Searching for class names including " + includes + " and excluding " + excludes);
List<String> classNames = newStoryFinder().findClassNames(searchDirectory(), includes, excludes);
getLog().info("Found class names: " + classNames);
return classNames;
}
/**
* Creates an instance of StoryFinder, using the {@link #storyFinderClass}
*
* @return A StoryFinder
*/
protected StoryFinder newStoryFinder() {
return classLoader().newInstance(StoryFinder.class, storyFinderClass);
}
/**
* Creates an instance of Embedder, either using
* {@link #injectableEmbedderClass} (if set) or defaulting to
* {@link #embedderClass}.
*
* @return An Embedder
*/
protected Embedder newEmbedder() {
Embedder embedder = null;
EmbedderClassLoader classLoader = classLoader();
if (injectableEmbedderClass != null) {
embedder = classLoader.newInstance(InjectableEmbedder.class, injectableEmbedderClass).injectedEmbedder();
} else {
embedder = classLoader.newInstance(Embedder.class, embedderClass);
}
URL codeLocation = codeLocation();
if (codeLocation != null) {
embedder.configuration().storyReporterBuilder().withCodeLocation(codeLocation);
}
embedder.useClassLoader(classLoader);
embedder.useEmbedderControls(embedderControls());
if ( executorsClass != null ){
ExecutorServiceFactory executorServiceFactory = classLoader.newInstance(ExecutorServiceFactory.class, executorsClass);
embedder.useExecutorService(executorServiceFactory.create(embedder.embedderControls()));
}
embedder.useEmbedderMonitor(embedderMonitor());
if (isNotEmpty(metaFilters)) {
List<String> filters = new ArrayList<String>();
for (String filter : metaFilters) {
if (filter != null) {
filters.add(filter);
}
}
embedder.useMetaFilters(filters);
}
if (!systemProperties.isEmpty()) {
embedder.useSystemProperties(systemProperties);
}
return embedder;
}
protected EmbedderMonitor embedderMonitor() {
return new MavenEmbedderMonitor();
}
protected EmbedderControls embedderControls() {
EmbedderControls embedderControls = new EmbedderControls().doBatch(batch).doSkip(skip)
.doGenerateViewAfterStories(generateViewAfterStories).doIgnoreFailureInStories(ignoreFailureInStories)
.doIgnoreFailureInView(ignoreFailureInView).doVerboseFailures(verboseFailures)
.doVerboseFiltering(verboseFiltering)
.doFailOnStoryTimeout(failOnStoryTimeout).useThreads(threads);
if ( storyTimeoutInSecs != 0 ){
embedderControls.useStoryTimeoutInSecs(storyTimeoutInSecs);
}
if ( storyTimeoutInSecsByPath != null ){
embedderControls.useStoryTimeoutInSecsByPath(storyTimeoutInSecsByPath);
}
if ( storyTimeouts != null ){
embedderControls.useStoryTimeouts(storyTimeouts);
}
return new UnmodifiableEmbedderControls(embedderControls);
}
protected class MavenEmbedderMonitor extends NullEmbedderMonitor {
public void batchFailed(BatchFailures failures) {
getLog().warn("Failed to run batch " + failures);
}
public void beforeOrAfterStoriesFailed() {
getLog().warn("Failed to run before or after stories steps");
}
public void embeddableFailed(String name, Throwable cause) {
getLog().warn("Failed to run embeddable " + name, cause);
}
public void embeddableNotConfigurable(String name) {
getLog().warn("Embeddable " + name + " must be an instance of " + ConfigurableEmbedder.class);
}
public void embeddablesSkipped(List<String> classNames) {
getLog().info("Skipped embeddables " + classNames);
}
public void metaNotAllowed(Meta meta, MetaFilter filter) {
getLog().debug(meta + " excluded by filter '" + filter.asString() + "'");
}
public void runningEmbeddable(String name) {
getLog().info("Running embeddable " + name);
}
public void runningStory(String path) {
getLog().info("Running story " + path);
}
public void storyFailed(String path, Throwable cause) {
getLog().warn("Failed to run story " + path, cause);
}
public void storiesSkipped(List<String> storyPaths) {
getLog().info("Skipped stories " + storyPaths);
}
public void storiesNotAllowed(List<Story> stories, MetaFilter filter, boolean verbose) {
StringBuffer sb = new StringBuffer();
sb.append(stories.size() + " stories excluded by filter: " + filter.asString() + "\n");
if (verbose) {
for (Story story : stories) {
sb.append(story.getPath()).append("\n");
}
}
getLog().info(sb.toString());
}
public void scenarioNotAllowed(Scenario scenario, MetaFilter filter) {
StringBuffer sb = new StringBuffer();
sb.append("Scenario '"+scenario.getTitle()+"' excluded by filter: " + filter.asString() + "\n");
getLog().info(sb.toString());
}
public void runningWithAnnotatedEmbedderRunner(String className) {
getLog().info("Running with AnnotatedEmbedderRunner '" + className + "'");
}
public void annotatedInstanceNotOfType(Object annotatedInstance, Class<?> type) {
getLog().warn("Annotated instance " + annotatedInstance + " not of type " + type);
}
public void generatingReportsView(File outputDirectory, List<String> formats, Properties viewProperties) {
getLog().info(
"Generating reports view to '" + outputDirectory + "' using formats '" + formats + "'"
+ " and view properties '" + viewProperties + "'");
}
public void reportsViewGenerationFailed(File outputDirectory, List<String> formats, Properties viewProperties,
Throwable cause) {
String message = "Failed to generate reports view to '" + outputDirectory + "' using formats '" + formats
+ "'" + " and view properties '" + viewProperties + "'";
getLog().warn(message, cause);
}
public void reportsViewGenerated(ReportsCount count) {
getLog().info(
"Reports view generated with " + count.getStories() + " stories (of which "
+ count.getStoriesPending() + " pending) containing " + count.getScenarios()
+ " scenarios (of which " + count.getScenariosPending() + " pending)");
if (count.getStoriesNotAllowed() > 0 || count.getScenariosNotAllowed() > 0) {
getLog().info(
"Meta filters excluded " + count.getStoriesNotAllowed() + " stories and "
+ count.getScenariosNotAllowed() + " scenarios");
}
}
public void reportsViewFailures(ReportsCount count) {
getLog().warn("Failures in reports view: " + count.getScenariosFailed() + " scenarios failed");
}
public void reportsViewNotGenerated() {
getLog().info("Reports view not generated");
}
public void mappingStory(String storyPath, List<String> metaFilters) {
getLog().info("Mapping story " + storyPath + " with meta filters " + metaFilters);
}
public void generatingMapsView(File outputDirectory, StoryMaps storyMaps, Properties viewProperties) {
getLog().info(
"Generating maps view to '" + outputDirectory + "' using story maps '" + storyMaps + "'"
+ " and view properties '" + viewProperties + "'");
}
public void mapsViewGenerationFailed(File outputDirectory, StoryMaps storyMaps, Properties viewProperties,
Throwable cause) {
getLog().warn(
"Failed to generate maps view to '" + outputDirectory + "' using story maps '" + storyMaps + "'"
+ " and view properties '" + viewProperties + "'", cause);
}
public void generatingNavigatorView(File outputDirectory, Properties viewProperties) {
getLog().info(
"Generating navigator view to '" + outputDirectory + "' using view properties '" + viewProperties
+ "'");
}
public void navigatorViewGenerationFailed(File outputDirectory, Properties viewProperties, Throwable cause) {
getLog().warn(
"Failed to generate navigator view to '" + outputDirectory + "' using view properties '"
+ viewProperties + "'", cause);
}
public void navigatorViewNotGenerated() {
getLog().warn(
"Navigator view not generated, as the CrossReference has not been declared in the StoryReporterBuilder");
}
public void processingSystemProperties(Properties properties) {
getLog().info("Processing system properties " + properties);
}
public void systemPropertySet(String name, String value) {
getLog().info("System property '" + name + "' set to '" + value + "'");
}
public void storyTimeout(Story story, StoryDuration storyDuration) {
getLog().warn(
"Story " + story.getPath() + " duration of " + storyDuration.getDurationInSecs()
+ " seconds has exceeded timeout of " + storyDuration.getTimeoutInSecs() + " seconds");
}
public void usingThreads(int threads) {
getLog().info("Using " + threads + " threads");
}
public void usingExecutorService(ExecutorService executorService) {
getLog().info("Using executor service " + executorService);
}
public void usingControls(EmbedderControls embedderControls) {
getLog().info("Using controls " + embedderControls);
}
public void invalidTimeoutFormat(String path) {
getLog().warn("Failed to set specific story timeout for story " + path + " because 'storyTimeoutInSecsByPath' has incorrect format");
getLog().warn("'storyTimeoutInSecsByPath' must be a CSV of regex expressions matching story paths. E.g. \"*/long/*.story:5000,*/short/*.story:200\"");
}
public void usingTimeout(String path, long timeout) {
getLog().info("Using timeout for story " + path + " of "+timeout+" secs.");
}
@Override
public String toString() {
return this.getClass().getSimpleName();
}
}
}
| {
"redpajama_set_name": "RedPajamaGithub"
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Twentieth-century semiotician Roland Barthes believed that fashion is a form of non-verbal communication that is totally subjective. Barthes Vestimentary Code suggests that meaning is communicated through the interpretation of signs. The sign is a combination of the signifier (the tangible garment) and the signified (the mental representation). When clothing is translated into this rhetorical code, fashion becomes more than just clothing, but rather a reflection of society. When it comes to semiotics, the little black dress is a garment with an extensive system of signs spanning centuries of changing perceptions (Barthes, R. 1967).
The Little Black Dress is a fashion staple and one which is closely associated with Coco Chanel. Here, you see her in the 1926 little black dress. At the time, Vogue compared this dress to the Ford Model-T - the first car to be industrially manufactured. To reduce costs, the car was painted only in black, and so blacks association with the industrial revolution and modernism was born. In fashion, the 20s are often referred to as the Androgynous era because of the way that couture shifted towards cleaner lines and away from the emphasis on women's breast and butts. The signifiers of Chanel's little black dress are a long, straight cut with a flat chest and straight waist. The signified, therefore, is of an androgynous, boylike figure. The signifier black was used by Chanel as an unambiguous indication of sexual impropriety, modernity and authority, mimicking that of men, clearly demonstrating that women were prepared to enter the workforce. In this way, she shifted the signified of black from a purely male, authoritarian, and mournful colour to a mature, distinguishing, gender-neutral and authoritative colour (Marcangeli, S. 2015). In this way, the LBD became not only a symbol of feminism but a weapon for liberated womanhood. In recent history, I believe that this was no better epitomised than when Princess Diana wore her iconic black "revenge dress" following Prince Charles' adultery scandal.
Chanel claims to have invented the LBD, that's not true, she simply helped popularise it because it was greatly associated with the modern woman of the 20s and who better epitomised that than Ms Chanel?
It's often been said also that Chanel is the one who took the black dress from being a gesture of mourning to being considered fashion. That too was naïve. Black clothing in general has undeniably been associated with mourning for a long time. Here, we see a mid-19th-century painting of a governess who is sitting alone, wearing black, presumably in mourning. Notice how the other girls are in light, bright colours connoting carefree girlhood whilst she is in black.
Black also had many extensive associations in the West with abstinence; members of the clergy, for example, will be wearing black as a signified of their submission to God and authority (Pastereau, M). Black became known as the colour of respectability.
In 1957, Vogue said, black is 'worldly, elegant, plainly alluring, indispensable'. This notion went back a long way. In the Middle Ages, black was not only seen as a colour for elite mourning but also as a very expensive, prestigious, elegant colour. Many aristocrats would wear black to indicate a sense of prestige - a dandiacal elegance which made them stand out amongst the peacock-coloured ensembles characteristic of the Middle Ages.
Black also very much had this sense of being an elegant colour in the 19th century. We think of the 19th century as all people in mourning black and that Chanel was the first to make elegant, fashionable black. Nothing could be further from the truth, black was already a colour which was seen as being extremely elegant. As
La Mode Paris put it in 1885, "Of course black, which can look very economical, can also be on the contrary, very expensive. And yet, the most distinguished dress, the most becoming dress that can be worn by any woman on any occasion is certainly a black dress".
But Black also, and for a long way back, was also associated with sex and power. So, in addition to the idea of death and mourning, it had the suggestion of the Devil (aka, The Prince of Darkness) and hell as the world was presumed to have started from nothing, just darkness (Pastereau, M). In one of Edith Wharton's novels, there is a woman who 'goes to bed' with a man and someone says of her, "What can you expect of someone who was allowed to wear black at her coming-out party?" Black had this connotation of sexiness and eroticism. We see it in the portrait of Madame X, a painting that caused outrage at the time of its reveal, and you see it as well in novels like Anna Karenina where the black velvet that she wears is contrasted with the ivory of her skin. Black's association with power, again goes right back to the Middle Ages to judges and executioners; it's been linked with crime and deviance. In Reservoir Dogs, there's a scene where Mr Pink asks why they can't pick out their own colours, and Joe remarks, "I tried that once, it don't work. You get four guys fighting over who's going to be Mr Black." Black is associated with the charisma of deviance as well as with the idea of sexualised women. In politics, you have the black of fascism and the black of anarchy.
Furthermore, as Valerie Mendez, the fashion historian, points out, black was fashionable long before the 1920s. In particular, she writes that the little black dress was born in the early 1900s, especially after the death of Edward the 7th in 1909. Then, during World War I, black became ubiquitous for mourning but also as a fashion colour. Black was a symbol of the nations shared grief caused by the war, but it was also a more practical colour as women were joining the war effort through taking over industrial job roles.
Chanel emphasised the quote, 'Scheherazade is easy, the little black dress is difficult'. This was in retaliation to the brilliant colours which were popular in the early 19 teens - reds, greens, and oranges. She said they made her feel nauseous and she went over to the other extreme by only using white, cream, black, and dark navy blue.
Black also has long antecedents as a bohemian, artistic colour. You can find it associated with beatniks, or with black leather jackets. But then you had also the chic cocktail dresses, the high fashion, elegant blacks. Balenciaga, for example, was described as creating dresses in Spanish black which is described as like a deep night without stars. Or Audrey Hepburn - of course - famously wore a plethora of little black dresses.
Christian Dior said of black, you can wear black at any age under virtually any circumstances. He also pointed out, as have many other designers, the black dress is appealing for designers because once you take away the colour you can focus on the silhouette, the texture, and other aspects of the dress, just as you would with line drawing for an artist instead of colour.
In the 1980s, the Japanese fashion revolution made black the dominant avant-garde colour in fashion. Yohji Yamamoto said the Samurai spirit is black. The Samurai must be able to throw his body into nothingness, the colour and image of which is black. Rei Kawakubo put it more simply when she said there are seven shades of black. And, of course, again, as it always sounded cryptic, a black velvet dress is completely different from a black satin dress or a black linen dress, etc.
One of the reasons why black is such a powerful colour is because there are so many layers of meaning. It's like a palimpsest, everything from elegance, evil, desirability, sexiness, power. And for all these layers of meaning, it means that a designer can create a wide variety of clothes, all of which end up having some of the modernity and allure of the little black dress. The little black dress can be whatever the wearer wants, or needs, it to be. In a sense, the little black dress is not a style per se but rather a concept. They're entirely versatile. There are many ways to design it. It's modern, it changes but it's always the same and it's always a kind of chic armour.
▼ January 2021 ( 1 )
► May 2020 ( 5 ) | {
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A Fresh Take on Transparency
Garden Fresh ambassadors interact with customers to share company's supply story.
Web Exclusive March 11, 2015 By Jill Watral
Garden Fresh CEO John Morberg, left, joins "Broccoli Bob" Campbell to share the story about Souplantation/Sweet Tomatoes' supply sources.
When Technomic released a study last year that researched transparency in the supply chain, Garden Fresh Restaurant Corporation CEO John Morberg took the data seriously. The study found that most consumers want restaurants to be more transparent about ingredients, and Morberg knew customers at Garden Fresh's Sweet Tomatoes and Souplantation restaurants were no different.
"Guests ask us all the time, 'Where does this come from?'" Morberg says. The answer is that the brands' ingredients come from local farms and ranches—no middlemen involved—but Morberg believed the company wasn't doing enough to share that story with customers.
Inspired by Garden Fresh's recent "Discover Fresh" campaign, which is a store remodel and marketing program focused on the brand's dedication to farm-to-table food, Morberg developed what Garden Fresh calls "Farm Teams." The Teams are employee duos in each store that serve as brand ambassadors, sharing the company's authentic story of healthy, sustainable foods.
When the company launched the endeavor in November, it also invited Garden Fresh farmers to one of the chain's 12 San Diego locations to converse face-to-face with transparency-hungry guests.
Bob Campbell, a fourth-generation grower at Campbell Ranches in Lompoc, California—also known as "Broccoli Bob" to the Garden Fresh family—spoke with consumers about the importance of generating appeal for healthy foods.
"I think the more people you can introduce to freshness, good quality, and a more flavorful product, then the more people are going to be attracted to vegetables," Campbell says.
"All we have to do is just authentically tell the story. We have nothing to hide."
And he's willing to take the transparency process a step further: Campbell invites customers to his farm to show them exactly how the broccoli they eat at Garden Fresh restaurants makes it to their plates. A few days after the initial event, one family took Campbell up on his offer.
"This family drove up from San Diego to see how we grow broccoli," he says. "It was a great experience for me." Campbell took the family on a tour of the entire ranch, allowing them to experience first-hand the growing, harvesting, packing, cooling, and delivery processes for broccoli production.
But not all customers can afford to make the five-hour trip from San Diego to Campbell Ranches. That's why Garden Fresh's Farm Teams provide customers with a smaller-scale version of the farm-to-table experience, Morberg says.
"The intention of the Farm Team is to help teach [guests], enlighten them, and let them know what we're doing with our partner farmers that are out there, and the type of quality produce that we receive from them," he says.
Sustainability innovation advocate Nancy Himmelfarb says the Farm Teams are a great direction for a restaurant company.
"They certainly are capitalizing on consumer interest in local foods," Himmelfarb says. She points to the National Restaurant Association's "What's Hot" trend list in its 2015 Forecast as proof that these types of campaigns are what customers are interested in. The chef survey found that locally sourced, environmentally sustainable, minimally processed, and healthy foods were in the top five food trends chefs expected this year.
The Farm Teams test phase is underway in San Diego, consisting of six brand ambassador teams that rotate weekly throughout Souplantation and Sweet Tomatoes restaurants at peak hours. Team members wear bright green T-shirts to stand out among restaurant visitors. Some teams meet and greet patrons at the door, while others chat directly with guests via table-to-table interactions.
Without millions of dollars to spend on advertising and public relations, Morberg says, these word-of-mouth interactions are cost-efficient ways to spread the Garden Fresh story. The Farm Teams also publicize the Garden Fresh story via radio advertisements and through informative coloring sheets for younger restaurant guests.
"A lot of kids are saying they want to be part of the Farm Teams," he says. "We're thinking it could go in really great directions. I'm going to send busloads of kids to see Bob."
Based on positive guest feedback thus far, Morberg feels optimistic about expanding the program. He aims to plant Farm Teams in locations in Los Angeles and Orange County in the coming months. If efforts continue to prove successful, the company will expand the Farm Team concept across the U.S.
As Garden Fresh expands its Farm Team reach, Himmelfarb says, the company must continue to practice what it preaches. "There is nothing to lose and everything to gain from being open and honest about what's in your food," she says. "If they're saying, 'We're fresh and we're doing all this great stuff,' that is fantastic. But then they need to be able to back it up."
Morberg is more than ready to heed Himmelfarb's advice. "All we have to do is just authentically tell the story," he says. "We have nothing to hide. We only have great things to tell, and we think that's the best way to serve the freshest meal and experience we can for our guests."
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Naturally, you want to record your gigs, as well as producing studio projects, podcasts, and so on. It's smart to record your rehearsals, too. So StudioLive AR mixers offer two different ways to record. Connect a StudioLive AR16 USB mixer to your computer via USB 2.0, and you have an 18x4 multitrack digital recorder, ready to capture all input channels plus the main mix to a Mac or Windows PC with professional, 24-bit/96 kHz quality. An onboard stereo SD recorder lets you record the main mix without a computer—just hit Record and go. Recording can't get much easier than this!
To get a great mix, you need high-quality effects. The StudioLive AR16 USB has you covered with an internal stereo effects processor with 16 presets, including an assortment of room, hall, and plate reverbs; chorus and delay effects; even a preset that emulates an acoustically treated studio room to provide a warmer, more intimate tone. A dedicated effects return, complete with master level fader and dedicated monitor sends, lets you adjust the amount of the effects in your main and monitor mixes. You can even bypass the effects with a footswitch (optional). It's just another way that StudioLive AR mixers enable you to build professional-quality mixes and recordings quickly and easily.
Compact and built for the road, the StudioLive AR16 USB is an easy-to-use, all-in-one solution for audio mixing and recording. With a wide variety of connections, two ways to record, and a simple, elegant mixing surface, it will quickly become the heart of your live and studio sound systems. | {
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Stock futures are derivative contracts that give you the power to buy or sell a set of stocks at a fixed price by a certain date. Once you buy the contract, you are obligated to maintain the terms of the agreement.
The contracts are traded on a futures exchange. The party agreeing to take delivery of the underlying stock in the future, the "buyer" of the contract, is said to be "long", and the party agreeing to deliver the stock in the future, the "seller" of the contract, is said to be "short".
The theoretical price of a future contract is sum of the current spot price and cost of carry. However, the actual price of futures contract very much depends upon the demand and supply of the underlying stock. Generally, the futures prices are higher than the spot prices of the underlying stocks.
Cost of carry is the interest cost of a similar position in cash market and carried to maturity of the futures contract less any dividend expected till the expiry of the contract.
Spot Price of Infosys = 1600, Interest Rate = 7% p.a. Futures Price of 1 month contract=1600 + 1600*0.07*30/365 = 1600 + 11.51 = 1611.51.
South Africa currently hosts the largest single-stock futures market in the world, trading on average 700,000 contracts daily.
The profits and losses would depend upon the difference between the price at which the position is opened and the price at which it is closed. Let an investor have a long position of one November Stock "A" Futures @ 430. If the investor square up his position by selling November Stock "A" futures @ 450, the profit would be Rs. 20 per share. In case, the investor squares up his position by selling November Stock "A" futures @ 400, the loss would be Rs. 30 per share. | {
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Q: Agregar Publicidad Admob en app con Android Studio estoy intentando implementar publicidad a una aplicación pero no aparece cuando agrego el id que me da ADMOB y eso que seguí los pasos tal y como están en la pagina
https://developers.google.com/admob/android/quick-start
solo me aparece el banner pero con el id de prueba de ADMOB , por favor ayuda, llevo buscando alguna solución por un largo tiempo y nada...
A: Inicializa AdMob en la actividad principal
MobileAds.initialize(thisActivity, "xx-xxx-pub-0000000000000000/0000000000"); //
adView = findViewById(R.id.adView);
AdRequest adReuest = new AdRequest.Builder().build();
adView.loadAd(adReuest);
Pero recuerda que también lo tienes que cambiar en AndroidManifest.xml
<meta-data
android:name="com.google.android.gms.ads.APPLICATION_ID"
android:value="xx-xxx-pub-0000000000000000/0000000000"/>
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Splash Magazines
Scenes From Life: Cuba! Review - A truly historic night
By Keith Gerbosi
View the Full Article | Return to the Site
Friday night at the Auditorium Theatre felt historic. Just being in the 125 year-old gorgeous theater makes one feel that way, but this was more. This was a once in a lifetime show. One that Emmy award winning musician, composer and conductor of the Chicago Jazz Philharmonic, Orbert Davis, looked forward to for a long time. One that couldn't have taken place just a few months ago.
The US and Cuban flags proudly hung together
The show started with a brief video to explain how this night came about. Davis, in his role as an educator and musical ambassador, traveled to Cuba in December 2014 on a cultural exchange. While there Davis visited The Universidad de las Artes (ISA) in Havana. ISA was established by the Cuban government to be the premier school for music talent on the island. Orbert Davis went to Havana to share Chicago Jazz as well as to learn about Cuba's musical heritage. The sessions went so well that the educators wanted to expand the relationship which, given the history between the two countries, seemed unlikely. However, as the video said, "Timing is everything." The very next day President Barrack Obama and Cuban President Raul Castro made the historic announcement to normalize relations between the two countries. And with it the seed of collaboration was planted.
Hurdles still had to be cleared, but in the end joining the 55 piece Chicago Jazz Philharmonic on stage on Friday were 36 Cuban music students from The Universidad de las Artes. This made for a crowded stage, but the more the merrier. Cubans and Americans making music together for the first time in the United States ushered in a new era of collaboration between the two former adversaries – and it was wonderful to hear.
The Super-Sized Orchestra
During the first act Orbert Davis conducted the super-sized orchestra through music he composed during his visits to Cuba. The extra flavor that the Cuban musicians added helped create more layers to the songs which somehow punctuated the theme of partnership on the night. Davis also made sure that the students were able to solo right along with his regulars – which was fun to see.
Mr. Davis takes a turn soloing
With all due respect to Mr. Davis, the best part of the night was the beginning of the second act. This was when he stepped aside and let the students take the stage by themselves. The first number was five young ladies with five string instruments performing a beautifully melodic number that could have lasted the rest of the night.
Six Young Students with six stringed instruments
After that, Ernesto Lima Parets came out to direct his fellow countrymen and women in traditional Cuban numbers.
Orbert Davis turns the stage over to Ernesto Lima Parets
His style as a conductor was a little different than what we are used to in this country. His hips swayed to the music and his head bobbed to the beat and at one point, joined by others from on stage and off, he danced in front of the orchestra. Cubans believe that music exists to dance to, and these students put that belief on full display. The music even got the audience to bounce in their seats.
Dancing and Singing Traditional Cuban Songs
To end the historic show, Davis performed a four part composition which he said wasn't completely finished. The final composition would be improvised right there on stage by the multi-national orchestra. The percussionists lead the way – with the drummers taking turns providing the Cuban rhythms that made the audience's hearts skip a beat.
This show was truly historic – but it had even deeper meaning. The collaboration between the American and Cuban musicians on display Friday night in Chicago should be looked upon as an example of how US-Cuban relationship should move forward: a collaboration of partnership, harmony and a whole lot of rhythm!
Photos by Darron Jones | {
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A comprehensive range of activities is organised in educational establishments with the road safety staff acting as facilitators and advisors.
The road safety section provides all primary schools with a programme of educational resources from Early Years through to Secondary.
Special needs - the road safety staff provides assistance and materials to these establishments. Resource available a2b Safely.
Road safety is thought by many as a subject only relevant to young children. However pedestrian crash statistics peak around 13 years of age. The road safety staff work on a number of projects to cover transition from primary to secondary.
Practical child pedestrian training: It has been recognised through extensive research that road safety lessons are more effective if taught in a real traffic environment rather than in the classroom.
'Urban Roadeo' Theatre Tour. Those in the mature road user category (55+) can enjoy 45 minutes of fun and laughter to learn about road safety. To find out more contact Road Safety. | {
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Children and Pesticides: New Approach to Considering Risk Is Partly in Place
HEHS-00-175 Published: Sep 11, 2000. Publicly Released: Sep 11, 2000.
Skip to Highlights
Pursuant to a congressional request, GAO provided information on the Environmental Protection Agency's (EPA) efforts to reduce children's exposure to pesticides by implementing the requirements of the Food Quality Protection Act (FQPA), focusing on the: (1) approach EPA has developed for making decisions about applying the new safety factor; (2) progress that has been made in considering aggregate exposure and cumulative effects; and (3) progress that has been made in reassessing tolerances for pesticide residues.
Full Report (40 pages)
Chuck Young
[email protected]
Agricultural chemicalsChildrenFood and drug lawPesticide regulationProduct safetySafety regulationSafety standardsPesticidesRisk assessmentPotable water | {
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Kayla was born and raised in St Augustine, Florida. She and her husband share two Siberian Huskies, Aiden and Sasha, and are excited for the arrival of their first child in May of 2015. As a graduate of Flagler College, she worked hard to earn an MBA by the age of 21. Her education and professional experience focuses on marketing with an emphasis in social media.
As a former Director of Marketing and self-taught graphic designer, Kayla strives to provide effective marketing solutions for business owners with services including social media marketing, blogging, copywriting, graphic design and brand management. She currently manages social media and marketing accounts for several clients including Herbie Wiles Insurance and MenuMax. Previously, she worked for Community Income Tax, assisting in the growth of the company to 90+ offices within the first year of operation. She was also contracted corporately by Hurricane Grill & Wings for a co-op marketing campaign for eight Northeast Florida franchise locations. In addition to her many marketing endeavors, Kayla is co-owner and Character Coordinator for Girly-Girl Partea's Inc, Northeast Florida's #1 choice for themed children's parties and character entertainment. She manages all character performers including hiring, training, scheduling and costuming, in addition to running the company website and furthering the Girly-Girl brand through social media and other marketing initiatives.
For six years Kayla served in many capacities with the St Augustine High School cheer program and helped secure a FHSAA competitive finalist placement for the first time in school history in 2013. She is also active with the Police Athletic League cheer program and has helped choreograph their competition routines since 2011. Kayla is available for freelance and non-profit marketing opportunities. | {
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Covid Turbulence – how countries got cancellations under control
Written by Becca Rowland |06 August 2020| 0 Comments
The past 30 weeks have seen the number of cancelled flights go through the roof as a result of the global pandemic, causing disruption to passengers, airlines and airports
Last week we looked at how airlines managed schedules during Covid. This week take a look the cancellation disruption and management at country level and how they got it under control.
In usual times airlines avoid flight cancellations in the 72 hours running up to the scheduled departure time for a flight. Typically, flight cancellations are an unavoidable consequence of technical failures, such as problems with an aircraft, or due to weather disruption. The proportion of flights cancelled isone of those key metrics that management and operations staff would be keeping an eye on.
However, as spikes in cases of the virus led to new lockdowns, airlines were forced to cancel hundreds of flights at short notice. Using OAG's cancellation dashboard we have analysed:
The unprecedented scale of cancellations and the timing of when they had most impact by country
When cancellations became a routine element of each region's capacity share
How long it took to stabilise so travellers could be confident that the public schedule would be the one that would fly
Early Warnings From China
Weeks 1-10: 1st January to 10 March
2020 was a fairly typical start to the year for flight cancellations. Across a basket of 24 countries, including many of the largest aviation markets in the world, fewer than 1% of flights were cancelled in the first week. The proportion of flights which were cancelled varied between a high of 2.73% (Canada) and a low of 0.02% (Thailand). The remainder of January was similar although the higher proportion of flights that were cancelled rose to 1.59% in the second week, and 1.66% in the third week before lowering to closer to 1% by the end of the month.
Through January covid-19 had been spreading in China and by 1st February countries around the world were closing their borders to arrivals from China. This is when the number of flight cancellations in China started to rise rapidly. In 2019 only 10% of departing flights from China were to international destinations, but flight cancellations rose as high as 22%, an indication that the impact was being felt far more widely than just on international air services to and from China as restrictions on movement within China took hold and demand for air travel plummeted.
By mid-March, none of the other countries in our basket were showing any flight cancellations effect from covid-19 with the exception of South Korea which had seen the proportion of cancelled flights rise steadily for a month.
April Turbulence
Weeks 11-20: 11 March to 19 May
It was the week of 18th March (Week 12) when the impact of covid-19 on commercial flying made it's weight known. 17 of these 24 countries saw the proportion of cancelled flights rise into double digits as countries rushed to close borders. The following 3-4 weeks were chaotic as travellers tried to return home, airlines operated repatriation flights, but demand fell through the floor and airlines consolidated flights, grounded planes and changed their operating schedule at short notice.
For some countries the chaotic phases was relatively short lived. The Netherlands, had a three-week period when flight cancellations rose to unprecedented levels – 46% for the very end of March - before falling to under 10%. Various other countries followed a smilar pattern – Spain, Australia, Colombia, Norway, dealing with the crisis and quickly adapting their schedule to become more realistic.
Some countries, or airlines, took a different path. In North America the number of cancellations remained high over a period of 7 weeks but by mid May (Week 20) cancellations were under control.
By then, China too appeared to have brought the number of cancellations under control, though they had been running at over 10% for 16 weeks. Japan, which saw cancellations start to rise a full 11 weeks later than China, followed a similar path to China with flight cancellations running at over 10% of scheduled flights for 16 weeks until the end of July.
China and Japan, widely known for the high density of flights on key city pair corridors
chose to continue with their pre-existing schedule, knowing they could cancel flights and reallocate passengers to another flight on the same route without too much impact on passenger travel plans.
Airlines Schedules Realistic
Weeks 21-30: 20 May to 28 July
As we moved into June and July it is clear than airlines had got their schedules under control, albeit with massively reduced numbers of flights. As a consequence, the number of flight cancellations has returned to a more normal level except where there are localised spikes in coronavirus, as was seen in China in Beijing in mid June, where the effect of new travel restrictions led to a short-lived increase in cancelled flights.
Until March airlines had never been in a position before where they had to consider cancelling large parts of their schedule for weeks and even months ahead, in tandem with all other airlines. The scale of making so many schedule adjustments in such a short space of time, with the uncertainty of not knowing when they'd be able to resume flying, was a massive logistical challenge.
Further cancellations are inevitable whenever spikes in covid-19 cases occur. As an example, on July 27th an infection spike in Northern Spain prompted the UK government to require holidaymakers to self-isolate for two weeks on returning from Spain, a move which affected travellers already in Spain and those about to travel. TUI, a leading airline and travel company, promptly cancelled all flights to the Spanish Mainland for a two-week period.
Rather than widespread cancellations, this pattern of handling cancellations is short-lived and regionally specific actions will be more likely in future, especially given how much more data is available now about the prevalence of covid-19. Airlines are no longer being taken by surprise and have time to plan on how to handle such events.
New Year, New Hope, Despite Challenges Ahead in 2023
An Overview of Airline Capacity from 2019-2022 as the Travel Recovery Continues
Airports See a Ten-Fold Increase in Flight Cancellations as Snow Hits Europe | {
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Provincial Administrator Eugenio Payongayong (leftmost) and Officer-in-charge Ma. Victoria Marcelo of the Provincial Youth, Sports and Public Employment Service Office (rightmost) present during the Monday Flag Raising Ceremony at the Bulacan Capitol Gymnasium, City of Malolos, Bulacan this morning the winners and National Qualifiers for Athletics category (L-R) Karen Mae Pelegria, 2nd place in both 200 and 400 meters, girls division and Marvilyn Canion, 1st place in both Long Jump and Triple Jump for girls in the 2019 Batang Pinoy Luzon Qualifying Leg Sports Competition held last March 16 – 23, 2019 in Isabela Province. Also in the photo is their coach Mr. Lamberto Nicolas. | {
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Due to the current Coronavirus outbreak, many attractions are closed and event organisers are cancelling or postponing their events. While we will try to update the information on this site as much as possible, we cannot guarantee to have all the information we would like. Therefore we urge you to check the latest information on the attraction or event's website or Facebook pages, and to contact them before travelling to avoid disappointment.
Please note: England is currently in a lockdown until at least 2nd December so no events will take place until after that date.
Museums & Attractions > South and South East > West Sussex
Amberley Museum
Museums & Steam Centres
Dedicated to the industrial heritage of the South East, charting the history of local industry and crafts in this part of Sussex. There is a diverse collection of exhibits, including a narrow-gauge railway and bus service (both provide free nostalgic travel around the site), Connected Earth Telecommunications Hall, Milne Electricity Hall, Printing Workshop and much more. The 36 acre open air museum is also home to traditional crafts people, such as the blacksmith and potter.
Address: New Barn Road Amberley Nr Arundel West Sussex BN18 9LT
Website: View website
Open Days & Times
Reopened 29th July. Visit website for details and advance booking.
By Rail: Amberley / 250 yards
Full disabled access
Register or log in to view location maps
Go to your account
Events at Amberley Museum | {
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IC 2689 ist eine Spiralgalaxie in Kantenstellung vom Hubble-Typ Sc? im Sternbild Löwe auf der Ekliptik. Sie ist rund 280 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 50.000 Lichtjahren. Sie bildet mit IC 2690 am Himmel ein optisches Doppel.
Entdeckt wurde das Objekt am 27. März 1906 von Max Wolf.
Einzelnachweise
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"doctor we are running out of time" teh soldier yelled.
"I know, I know, I'm almost done" she replied as she continued typing on the computer. "Gardener"
a pale blue figure materialized from thin air in the form of a woman in a black gown. "yes doctor?" she asked in a smooth, calm voice.
"status on the defense drones?" the doctor asked quickly.
"reports indicate that seventy-two of them remain, the infected are moving much faster than we had planned for." the hologram replied.
"ok then, relay all objectives that are to proceed upon our entry into stasis." the doctor asked again.
"upon stasis entry defense drones are to return to the lock-down perimeter and the facility is to be put into immediate lock-down until furhter notice, if infected individuals should enter the facility drones are to enter search and destroy mode to find and eradicate them."
The doctor had a satisfied look on her countenance, "good now we ju....."
"doctor Blair!" yelled the soldier again.
Doctor Blair looked up with a start. she had been so focused on ensuring Gardeners programming was set she forgot about everything; the desecrators, the banging on the door. the facility they were in housed the last known untainted humans in the world and kept them in suspended animation until the desecrators were eliminated or another intelligent race came and released them.
The soldier gave a look of agrivation and continued through another door that was open and was lost from sight. Dr. Blair finished typing and looked back at the stationay holographic woman and said; "take care of us." she said sadly.
"you know I will doctor." was here only reply.
When dr. Blair entered the next room she felt a chill creep over her from the several hundred cryo-pods. aside for the Six soldiers the other three people were already closing their pods and entering stasis. She walked up to one of the last pods and stepped in, the soldier that had yelled at her came to her and before he could say anything she asked; "sergeant are you sure you want to do this?"
"we don't know if the desecrators will ever recede, or if another intelligent species will ever come to earth much less let us out of stasis."
"but are you sure?" she asked again.
The soldier stood up a little straighter, "sure enough to die ma'am" he said in a more confident voice.
he tapped a few keys on the datapad built into the pods side and the hatch began to close. just before it shut there was a loud bang as the six soldiers ran back to the room they just left. The door shut quickly behind them as they were lost from sight. A small window on the door became full of flashes coming from the other side of it. A deep cold began to crawl up Casandras leg as the Pod hissed shut. When the Cold got to her head she was still watching the door when the window was blotted out by a smear of red. A tear rolled down her cheek and froze as the ice surrounded the rest of her body and she entered a deep cold slumber. | {
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May 23, 2011 at 7:11 pm EDT | by Chris Johnson
White House issues statement on Minn. marriage amendment
The White House (Blade file photo by Michael Key)
The White House on Monday issued a statement in response to a proposed measure in Minnesota that would make a ban on same-sex marriage part of the state constitution.
The complete statement follows:
"The President has long opposed divisive and discriminatory efforts to deny rights and benefits to same sex couples or to take such rights away. While he believes this is an issue best addressed by the states, he also believes that committed gay couples should have the same rights and responsibilities afforded to any married couple in this country."
White House spokesperson Shin Inouye provided the statement to the Washington Blade via e-mail in response to a question on President Obama's position on the marriage amendment, which will come before Minnesota voters in 2012.
The statement doesn't explicitly mention the proposed constitutional amendment in Minnesota, but states that the president "has long opposed divisive and discriminatory efforts" that would restrict rights for gay couples.
Additionally, the statement reaffirms Obama's lack of support for same-sex marriage rights by saying the issue is "best addressed by the states." Obama has said he's "wrestling" with the marriage issue, but has yet to make an endorsement for marriage equality.
Homepage HeadlinesmarriageMinnesotaWhite House
Chris Johnson is Chief Political & White House Reporter for the Washington Blade. Johnson is a member of the White House Correspondents' Association. Follow Chris
Jon John
May 23, 2011 at 7:54 pm EDT at 7:54 pm
Straight people should worry about the divorce rate and all of the people who have children without the benefit of marriage.
evolutionisfact
So exactly what is our fearless leader saying here? Re-hashing the same old blah, blah, blah he's always been saying. Pull yer head outta yer arse mr. President and actually take a stand on something for a change! jeeeeeeezus!!!
May 23, 2011 at 11:00 pm EDT at 11:00 pm
Time for the federal Government to step in…: TENNESSEE: Governor Signs Bill Banning All Local LGBT Rights Laws
Patrick Connors
Hey LOOKIE! President Fierce's flack almost says something!
tiredofyourBS!
action speaks louder than words Mr. President.. stop repeating yourself.. youve been saying those BS since you became our president. repeal DOMA if you really hate discrimination. we are not kids anymore to believe in your bedtime stories.
May 24, 2011 at 11:24 am EDT at 11:24 am
It's not discrimantion. two gays can't marry. Marriage is for heterosexuals. I guess next year you want man and boy 'marriages' and then woman and boy, and then german shepherd and woman. You can't change the definition of a word. Move on.
Jerry in Chapel Hill
May 24, 2011 at 8:03 am EDT at 8:03 am
Well, we saw how that approach worked out with another civil rights issue in the 1860s.
Did anyone notice the statement was sent only to the Washington blade …and via email. At least tell the people.
Walter Zimmerman
This is a deplorable move on the part of the state of Minnesota, and a tepid response from the President of the United States. Imagine the outcry, if it were interracial couples who were going to be denied their basic civil rights.
This is California's PROP H8 de ja vu. Why is it that EQUALITY is only a straight person's right? The Tyranny of a (bigoted) MAJORITY is allowed to deny us our RIGHTS! Time for all states to get out of the marriage business. Let churches "marry" whomever they wish. Grant SS Couples the SAME FEDERAL RIGHTS & PRIVILEGES as our straight counter-parts. And if the CHURCH continues to invest time & energy & $$ in Social Issues like this, time to TAX them!
I don't think Obama's support for gay marriage could be more crystal clear in this statement. These political manueverings while handling societal shifts are hard to deal with. I'm not a politician but I'm certainly engrossed in it. To me, this is similar to the birther movement and Donald Trump's demands to see Obama's birth certificate. Obama has shown his birth certificate up to three times prior before the White House Correspondents Dinner but not everyone believes he was born in the United States because they don't want to believe it. I feel the same way about people who think that Obama is against gay marriage. He's certainly for it but to actually enact a change in policy takes time and a lot of policy influencing. When the time is right, I have every faith that gay marriage will become federal law.
Donna Hutton
WHY IS THIS STILL AN ISSUE?? Why are we STILL listening to the so-called Moral Majority?? Especially since they've shown they're neither Moral OR a Majority?? If two people are committed to each other then let them marry. IT'S NONE OF THE STATE's OR ANYONE ELSE's BUSINESS! Aren't we living in U.S. of America? Aren't ALL "people" created equal in this country?? Isn't this the 21st century?? Get some BACKBONE Mr. President. Do what's RIGHT not what's easy.
Vato Lavino
June 15, 2011 at 7:08 pm EDT at 7:08 pm
"…the statement reaffirms Obama's lack of support for same-sex marriage rights"
"…committed gay couples should have the same rights and responsibilities afforded to any married couple in this country."
What else can he be saying here other than that he supports same-sex marriage? This is double-talk…and it's not even good double-talk. | {
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The safe level for ear corn in the crib is higher than for shelled corn because air passes through to remove heat and to dry the corn. In northern corn growing areas, the upper limit in narrow cribs (4 1/2 feet) is about 25% moisture in the grain. If late fall and winter are so damp that grain does not dry, spoilage will begin with the onset of warm weather in the spring. In the central Corn Belt where cribs are wider in order to handle higher yields, the safe limit is about 20%. Corn should be down to 18.5% by March 1 to avoid spoilage with the onset of warm weather.
A bushel of corn at 15.5% moisture consists of 47.32 pounds of dry matter and 8.68 pounds of water.
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The eastern and southern portions of the region need higher air flows because of higher humidities and somewhat warmer temperatures at harvest.
200 lb / (62.4 lb/cu.ft.) = 3.2 cu.ft. If the grain flow out of the bin is 1500 bu per hour, that is equivalent to 1500 bu x 1.244 cu ft/bu x 1/3600 hr/s = 0.518 cu ft/sec. So the human, if he/she is at the center of grain flow, will be buried in the grain in 3.2 cu ft/(0.518 cu ft/s) = 6.17 seconds.
Picking sites that are elevated and have good drainage is the key to storing grain on the ground. The risk of crop loss is higher when grain is stored on the ground than in bins, so ground piles should be considered short-term storage and monitored frequently.
The success of storing grain on the ground depends on a combination of variables that can be controlled, such as site preparation, storage design, use of aeration and storage management, and factors that can't, such as the weather.
Try to separate spoiled grain from the pile to limit the amount of grain that needs cleaning, drying and blending with other grain stored in outdoor piles.
Check with the building's manufacturer on how deep to fill the structure with grain.
Does not meet the requirements for the grades U.S. Numbers 1, 2, 3, 4, or 5; or In a 1,000 gram sample, contain 8 or more stones which have an aggregated weight in excess of 0.20 percent of the sample weight, 2 or more pieces of glass, 3 or more crotalaria seeds (Crotalaria ssp.), 2 or more castor beans (Ricinus communis), 8 or more cockleburs, 4 or more particles of an unknown foreign substance(s), or a commonly recognized harmful or toxic substance(s), or animal filth in excess of 0.20 percent; or has a musty, sour, or commercially objectionable foreign odor; or is heating or otherwise of distinctly low quality.
MidWest Plan Service - Available from AgriculturalEngineering Plan Service, 219A L.W.Chase Hall, University of Nebraska, 68583-0727 phone 402-472-6718. There is a charge for the publications and a fee for handling and postage. | {
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module Rapidfire
class QuestionsController < Rapidfire::ApplicationController
before_filter :authenticate_administrator!
respond_to :html, :js
before_filter :find_question_group!
before_filter :find_question!, :only => [:edit, :update, :destroy]
def index
@questions = @question_group.questions
respond_with(@questions)
end
def sort
item = Question.find(params[:id])
item.position = params[:thing][:position]
item.save
render nothing: true
end
def new
@question = QuestionForm.new(:question_group => @question_group)
respond_with(@question)
end
def create
form_params = params[:question].merge(:question_group => @question_group)
@question = QuestionForm.new(form_params)
@question.save
respond_with(@question, location: index_location)
end
def edit
@question = QuestionForm.new(:question => @question)
respond_with(@question)
end
def update
form_params = params[:question].merge(:question => @question)
@question = QuestionForm.new(form_params)
@question.save
respond_with(@question, location: index_location)
end
def destroy
@question.destroy
respond_with(@question, location: index_location)
end
private
def find_question_group!
@question_group = QuestionGroup.find(params[:question_group_id])
end
def find_question!
@question = @question_group.questions.find(params[:id])
end
def index_location
rapidfire.question_group_questions_url(@question_group)
end
end
end
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Welcome to our global equities blog
Our global equities blog lifts the lid on what we do and shows you how our investment engine works. From describing company visits and snapshots of the work we do, to exploring the major themes and trends shaping markets.
Natasha Ebtehadj
Portfolio Manager, Global Equities
What does market regulation mean for Chinese equities?
Recent regulatory action around China's after-school education companies and big tech firms is raising questions over the investability of the country.
Read time - 4 min
Pauline Grange
Fashion, Adidas and the circular economy
Adidas has been a core holding since the inception of the Threadneedle Global Sustainable Equity strategy. Its production and promotion of technical sports performance products contributes positively to our social theme of "Good Health and Wellbeing".
Japan sets its sights on a software revolution
The use of software solutions by companies to improve competitiveness, efficiency and productivity, and reduce costs, is picking up pace – just in time, as a shortage of skilled workers continues to bite
Scott Woods
Masts, manufacturing and meetings – 2021 so far in the global smaller companies universe
Visiting companies is key to small cap investing in particular. Scott Woods looks at how the pandemic has changed this.
Neil Robson
Head of Global Equities
Electric vehicles help power growing decarbonisation trend
Why understanding new ways of thinking and a changing world is critical to our investment process.
David Dudding
The destruction of creatives
Advertising spend was huge during lockdown, but it's not the traditional players who are benefiting. This changing market highlights some of the difficulties with 'value investing' at a time of technological change.
1210, 1107, 2964, 1147, 2651, 2962, 1175, 11343, 11373, 11374, 1108, 10938, 11345
Alex Beavis
Global Small Cap Analyst
Alex Beavis is an analyst within the Global Equities team, focusing on global smaller companies. He began this role in 2019. Prior to this, Alex worked as a client portfolio analyst within the Global Equities team, assisting with client servicing, sales and articulation of the team's investment views and capabilities.
Alex joined the company in 2016 and worked in Finance for six months on a graduate scheme rotation. In March 2017, he joined the Global Equities team, where he has remained since.
Alex holds a BSc (Hons) in Economics and Management Sciences from the University of Southampton.
Alex joined is a portfolio manager in the Global Equities team. Alex joined the company in 2016 as a portfolio manager on the Japan Equities desk and moved to the Global Equities team in 2018. He is now a portfolio manager on the Global Focus strategy and lead manager of a number of segregated Japan equity mandates.
Whilst working on the Japan desk, Alex assisted the Global Equities team with idea generation and analysis of Japanese companies across all sectors.
Before joining the company, Alex was a Senior Fund Manager at Canada Life Investments, where he managed the Japan fund and supported the management of the US and Global funds.
Alex has a BSc in economics from the London School of Economics. He also holds the Chartered Financial Analyst designation.
Ashish Kochar
Ashish Kochar is a portfolio manager within the Global Equities team. Ashish joined the company in 2008 and the Global Equities team in 2010. He is the co-portfolio manager for the Threadneedle Global Extended Alpha strategy, as well as the American Extended Alpha, American Absolute Alpha and American Select strategies.
Ashish joined the company as a senior analyst within the US Equities team. He joined the company from a 'Tiger Cub' hedge fund and previously worked as an analyst for Merrill Lynch in New York.
Ashish holds an MBA from Mason School of Business, The College of William and Mary.
Simon Haines
Simon Haines is a portfolio manager in the Global Equities team. He took up this role in November 2013 and is currently lead manager across the desk's EAFE and Shariah portfolios. He also has research responsibility for the industrials sector and for the Asia-Pacific region.
Simon joined the company in 1999 as a trainee UK Equities portfolio manager, progressing to portfolio manager in January 2005, where he managed the Threadneedle UK Mid 250 Fund and co-managed the Threadneedle UK Extended Alpha Fund.
Simon graduated with a degree in biology from Oxford University in 1999 and also holds the Chartered Financial Analyst designation.
David Dudding is a senior portfolio manager at Columbia Threadneedle Investments. He joined the company as an equity research analyst in 1999 moving on to manage the European Smaller Companies strategy for 10 years until December 2012. He is currently responsible for the European Select and Global Focus strategies.
David previously worked for John Swire and Sons in Hong Kong and for Investors Chronicle as a financial journalist.
He holds a Modern History degree and a European Politics Masters degree from Oxford University. He also holds the Chartered Financial Analyst designation and is a member of the CFA Society of the UK.
Pauline Grange is a portfolio manager within the Global Equities team. She took up this role in 2007 and is currently lead portfolio manager of the Threadneedle Global Sustainable Outcomes and Threadneedle World Equity strategies and deputy portfolio manager of the Columbia Select Global Equity fund. She also heads the telecoms and utilities sector research team and is the deputy head of the technology sector research team.
Before joining the company, Pauline was a global equity portfolio manager for Investec Asset Management.
Pauline has a Bachelor of Business Science (Honours) in Finance from the University of Cape Town. She also holds the Chartered Financial Analyst designation.
Georgina Hellyer
Georgina Hellyer is a portfolio manager within the Global Equities team. Georgina joined the company in 2011 and the Global Equities team in 2017. She is a portfolio manager on the Global Equity Income strategy and the International Dividend Income strategy.
Previously, Georgina worked as an analyst on the Emerging Markets Equity team, covering the materials and energy sectors and becoming a portfolio manager in 2013. Before joining the company, Georgina worked at Aviva Investors as an analyst covering the materials and energy sectors on the company's Emerging Market and Asian equities team.
Georgina has a degree in Philosophy, Politics & Economics from the University of Oxford and holds the Chartered Financial Analyst and Certified Market Technician designations.
Bronwyn Curran
Client Portfolio Analyst
Bronwyn Curran is a client portfolio analyst in the Global Equities team. In this role, she is responsible for providing detailed information on the company's global equity views and capabilities to clients, prospects and consultants.
She joined the company in 2018 as part of its graduate programme before joining her current team in 2020.
Jonathan Crown
Jonathan Crown is lead portfolio manager on the Global Equity Income Strategy and manages a number of pooled and institutional mandates including the Threadneedle Global Equity Income Fund. Jonathan joined the company in 2005 as an investment analyst on the credit team. In 2008, he moved from the Fixed Income team to the Global Equities team and has managed global equity portfolios since 2010 and global equity income portfolios since 2011. Jonathan is also deputy head of the financials sector research team.
Before joining the company, he worked at Dresdner Kleinwort Wasserstein as an investment grade credit analyst covering financials.
Jonathan has an MA (Hons) Degree in Economics from the University of St Andrews.
Scott Woods is a portfolio manager within the Global equities team and has been lead manager of the Threadneedle Global Smaller Companies strategy since April 2019. Scott joined the Global equities team in 2015 as an equity analyst with responsibility for researching small cap companies, focusing in particular on US small caps. He was subsequently made deputy portfolio manager on both the Threadneedle Global Smaller Companies strategy and the Threadneedle US Smaller Companies strategy.
Before joining the company, Scott spent three years with Ecclesiastical Investment Management, an SRI-focused asset manager, where he worked as an investment analyst within the global equities team.
Scott holds a Masters degree in Chemistry from the University of Oxford. He also holds the Chartered Financial Analyst designation and the Investment Management Certificate.
Andrew Harvie
Client Portfolio Manager, Global Equities
Andrew Harvie is a Client Portfolio Manager within the Global Equities team. His role is to articulate the team's investment views and capabilities to existing and prospective clients, consultants and intermediaries.
Andrew re-joined the company and the team in 2018 from Schroders where he was a client portfolio manager and head of product in the QEP investment team. He has previously worked as a client portfolio manager at Man AHL, Man Group's quantitative investment division, having originally joined as an investment analyst in 2007. Andrew was also involved in due diligence and product strategy during Man's acquisition of GLG Partners in 2010.
Prior to working in asset management, Andrew worked as an equity capital markets analyst at Bloomberg and started his career within wealth management.
Andrew holds a BSc (Hons) in Economics with Statistics from the University of Bristol.
Neil Robson is Head of Global Equities at Columbia Threadneedle Investments. He took up this role in July 2017. He joined the company in 2011 as a portfolio manager within the Global Equities team. He is the deputy manager of the Threadneedle Global Select Fund and manages a number of global equity mandates for institutional clients. He is also the co-manager of the Threadneedle Global Extended Alpha Fund.
Before joining the company, Neil worked as a fund manager at companies including Martin Currie, Barings and Citibank. In addition, he was Head of Global Equity at Pioneer Investments from 2003 to 2009.
Neil has an Economics degree from the University of Bristol.
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Mark William Bedders Bedford (Londen, 24 augustus 1961) is bassist van de Britse ska-popband Madness en tevens grafisch ontwerper.
Biografie
Bedford begon zijn carrière met het spelen van Beatles- en Motown-covers. In 1978 sloot hij zich aan bij The North London Invaders, zoals Madness toen nog heette, en regelde optredens op zowel zijn school als op zijn werk. Bedford volgde een opleiding zeefdrukken maar stopte daarmee toen de belangstelling voor Madness groter werd. De band groeide uit tot een van de kopstukken van de ska-revival en specialiseerde zich in humoristische clips met een onderliggende boodschap.
Van alle zeven leden was Bedford destijds het meest actief buiten Madness; zo produceerde hij een demo van 23 Skidoo en speelde hij mee op singles van Strawberry Switchblade, Robert Wyatt (Shipbuilding), The Inspirational Choir... (naar aanleiding van hun bijdrage aan de hit Wings of a Dove) en Tracey Ullmans verketterde cover van Madness' My Girl.
Ondertussen ging Madness serieuzere muziek maken met als gevolg dat de fans afhaakten en in 1986 het einde werd aangekondigd. Samen met drummer Daniel 'Woody' Woodgate ging Bedford verder bij The Voice of The Beehive waarmee hij in 1987 de single Just A City uitbracht en een handvol BBC-sessies deed. Geheel volgens plan vertrok hij na zes maanden om via een Japanse tournee met The Blockheads (zonder hun leadzanger Ian Dury) zijn nieuwe ambitie te verwezenlijken; filmsoundtracks schrijven.
Dit resulteerde slechts in Our Lady At The Laundromat waarvoor hij hulp kreeg van Terry Edwards, een saxofonist die eveneens een verleden had op het 2-Tone-label als lid van de Britfunkformatie The Higsons. Samen met pianist Seamus Beaghan (bij Madness de plaatsvervanger van Mike Barson) richtten ze het jazz-collectief Butterfield 8 op. In 1988 verscheen het album Blow! met daarop de single Watermelon Man. Optredens vonden sporadisch plaats omdat Bedford zijn grafische studie weer had opgepakt.
In het examenjaar 1992 gaf genoemd drietal twee concerten met de Terry Edwards Ska Extravaganza waaraan ook Madness-leden Chris Foreman en Lee Thompson (inmiddels actief met hun eigen band The Nutty Boys) meededen. Dit, en de re-release van It Must Be Love als voorbode op de verzamelaar Divine Madness voedden de geruchten over een op handen zijnde reünie. Na lang twijfelen en ontkennen werd de reünie eind dit juni daadwerkelijk bevestigd. De concerten in Den Haag en Finsbury Park waren zo'n succes dat Madness besloot om er een vervolg aan te geven. Afgezien van de live opgenomen Jimmy Cliff-cover The Harder They Come en het door Barson geschreven uitprobeerseltje Moondance bleef nieuw materiaal uit en al snel ging Madness over op greatest hits-shows met weinig verrassingen. Bedford had er op deze manier geen zin meer in en liet verstek gaan voor de concerten van 1995-1996; zijn nieuwe bedrijf en zijn gezin gingen voor.
In 1998 keerde hij terug en ging Madness eindelijk een nieuw album opnemen dat een jaar later werd uitgebracht. Bedford leverde geen compositorische/tekstuele bijdragen meer, zoals hij dat in de hoogtijdagen nog weleens deed, en bij sommige optredens liet hij zich vervangen door een lookalike. In de periode 2010-2012 was Bedford enkel aanwezig bij het 60-jarig jubileum van Koningin Elizabeth, maar begin 2013 keerde hij weer terug.
Naast Madness sloot Bedford zich aan bij Terry Edwards's Near-Jazz Experience en de Lee Thompson Ska Orchestra; beide acts hebben sinds 2013 twee albums uitgebracht. In 2014 verleende hij met de supergroep The Values zijn medewerking aan de Madness-tribute cd Mad Not Cancer. Voor het in 2016 verschenen tweede album van Lee Thompson Ska Orchestra schreef Bedford het titelnummer Bite the Bullet; zijn eerste compositie sinds jaren.
Datzelfde jaar kwam Madness met een nieuw album, Can't Touch Us Now, waarop Bedford in een nummer tuba speelde.
Tijdens de coronacrisis stond Bedford Foreman bij in een zoom-sessie met fans; deze verving de uitgestelde sloteditie van de House of Fun Weekender die Madness sinds 2011 organiseerde.
In juni 2021 bracht Bedford met Near Jazz Experience de ep Nought To 60 uit.
Brits bassist
Madness | {
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3 murder cases remain unsolved from 2022
by: Jaron Spor
WICHITA FALLS (KFDX/KJTL) — While 2022 is in the rearview mirror, three unsolved murder cases are still at the forefront.
2022 saw 18 homicides, 15 of those were classified as murders and three of those cases are still open.
"The first one was on the 1000 block of Covington," Sgt. Charlie Eipper said. "The second one was at the Haystack bar on N. Scott and then the third was on the 1300 block of 11th St."
Victim identified in fatal motorcycle crash
The one on Covington took place on May 22, 2022, around 2:00 A.M. Wichita Falls Fire Department was first called to the scene about a medical call but the WFPD was later called as well. That's when the WFPD found Andrew Lopez, 32.
"They found a deceased in the vehicle," Eipper said. I can't really share a lot of the details because an arrest has not been made but it's still moving forward, it's pending. It's an ongoing investigation."
A search warrant was served at a house and people inside were interviewed at the police station. But no arrests were made.
The next murder took place on Aug. 1, 2022, around 12:10 A.M. Officers were dispatched to investigate an assault with a weapon at the Haystack Bar. Once there, officers found Cordera Sherrard Walker, 34.
"We were called out there, there was a victim there inside of a car who had been killed so that's also labeled as a murder," Eipper said. "That's also pending an investigation and we are looking for tips. We are looking for any information if somebody wants to call into Crime Stoppers or call into our department that would be great."
The final homicide happened on Oct. 26, 2022, at 3:30 P.M. in the 1300 block of 11th St. Police were sent to a report of a deceased person. When they arrived, they located James Shierling, 70, inside the apartment.
"Officers were called out on that one as well and found Mr. Shierling deceased and he had been murdered," Eipper said. "So, that's still a pending investigation. People have been interviewed as well through that."
Search for missing 4-year-old Oklahoma girl now considered recovery operation
Since each of those incidents, detectives have worked hard to find the answers so these cases do not go cold.
"By law, a murder has no statute of limitation so it's always an ongoing case," Eipper said. "It may stop or come cold because of lack of leads but no, our detectives know the law but they also have this personal drive that they do want to solve this case for the victim and for the victim's family."
As we are in the new year, hopefully, that closure comes to each of those families, soon.
As Eipper said if you have any information on those cases you are urged to call Crime Stoppers. You never have to give your name and if your information leads to an arrest you could earn a cash reward. | {
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Getting an hourglass figure is something that everyone will enjoy. It is not too difficult as well, as long as you are ready to take care of fitness nutrition. If you just keep on eating to appease your appetite without caring much about what the food contains, a perfect figure will just remain a dream forever.
Different people have different pressures in life that may make it difficult for them to stick to a certain diet or do the necessary amount of exercises. Some people are into office jobs that will keep them tied to their chairs the whole day so that the body does not get exercised at all. Others may have to hurry through their meals or might have to rely on junk food joints for their lunches.
Those who are keen on keeping the body fit should try to alter this lifestyle and introduce fitness nutrition into their lives. The most practical way to go about it is by keeping track of the daily intake of food. You can start with noticing down on a daily basis all that you have eaten on that day. Quite a lot of it could be junk food especially in the case of those who have to go for something from a nearby joint during lunch break.
Proper fitness nutrition consists of eating the right way and exercising the right way. Fat and too many carbohydrates should be avoided. Proteins, fresh vegetables and fruits should be taken. How to balance your food intake is a science but it is not difficult. You owe it to you and your family to acquire more of this knowledge.It is necessary to squeeze in a little time for exercising every day even if you have gotten a tight work schedule. And those who are overweight may have to find more time for it. There are small exercises that you can do even while working in an office. You can take a few minutes break from the work and stand up and sit down a dozen times. Or you can stand up and shrink your shoulders and raise yourself on your toes now and then. All these will make a lot of difference.
Following the rules of fitness nutrition will help you to keep yourself fit without working out at a gym. Make a diet chart and try to stick to it as much as you can by taking a packed lunch or a few snacks to office so that rushing to eateries during lunch breaks can be reduced.
The good thing about getting started on a fitness nutrition is that you will start feeling good soon. Once you start enjoying that sense of energy and freshness, you are inadvertently to go back to the earlier pattern of unhealthy diet and limited exercising. | {
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Hexaprotodon, rod Parnoprstaša iz porodice Hippopotamidae koji danas obuhvaća samo jednu živu vrstu, Hexaprotodon liberiensis, a ostale su poznate iz fosilnih nalaza s tipičnom vrstom Hexaprotodon sivalensis koju su opisali Falconer i Cautley, 1836.
Fosilne vrste
†Hexaprotodon bruneti Boisserie and White 2004
†Hexaprotodon coryndoni Geze 1985
†Hexaprotodon crusafonti Aguire 1963
†Hexaprotodon dulu Boisserie 2004
†Hexaprotodon garyam Boisserie et al. 2005
†Hexaprotodon hipponensis Gaudry 1867
†Hexaprotodon imaguncula Hopwood 1926
†Hexaprotodon iravticus Falconer and Cautley 1847
†Hexaprotodon mingoz Boisserie et al. 2003
†Hexaprotodon namadicus Falconer and Cautley 1847
†Hexaprotodon palaeindicus Falconer and Cautley 1847
†Hexaprotodon pantanellii Joleaud 1920
†Hexaprotodon primaevus Crusafont et al. 1964
†Hexaprotodon sahabiensis Gaziry 1987
†Hexaprotodon shungurensis Geze 1985
†Hexaprotodon siculus Hooijer 1946
†Hexaprotodon sivalensis Falconer and Cautley 1836
Izvori za fosilne vrste
Izvori
Vodenkonji | {
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Turkish Language Center
Türkçe العربية
Faculty of Islamic Sciences
Faculty of Business and Management Sciences
Sports Science Faculty
Graduate Education Institute
School of Languages
Coordinatorship of Foreign Languages
Arabic Preparatory School
English Preparatory School
Turkish Preparatory School
IZU TOEFL Test Center
IZUSEM (Continuing Education Center)
IZUTEM (Turkish Language Center)
Turkish Language Education and Teaching Application and Research Center (İZUTEM)
Food and Agricultural Research Center
Halil İnalcık History and Society Science
Halal Food Ar-Ge Center of Excellence
Silk Road Civilizations Research and Application Center
CIGA (Center for Islam and Global Affairs)
Istanbul Research Center
M. Akif Ersoy Art, History, Literature and Civilization Research and Application Center
IZU Nuclear Detectors and Robotics Application and Research Center
Special Talented Children Education Research and Application Center
IRCIEF (International Research Center for Islamic Economics and Finance)
Local and Regional Policy Research and Application Center
Management, Entrepreneurship and Leadership Research and Application Center
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About IZU
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Who is Mehmet Akif Ersoy?
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Corporate Identity Details
Post-Covid19 Education for International Students
These past months, in Turkey as well as all around the world, the COVID19 pandemic has generated an unprecedented crisis that has changed the world at an incredible pace. The challenges it has presented have not only been medical, but have extended to economic, cultural, and financial activities, significantly disrupting all levels of educational institutions as well. The crisis will soon be over, but its indelible mark on our lives will persist in the coming years. In this new reality, the rules and habits of the past no longer hold; at least, not in their old forms. However, the response given by the people, institutions, and countries in the face of this global crisis stands as an indicator of what lies ahead.
In this critical time, Istanbul Sabahattin Zaim University encouraged order and understanding while continuing its research and educational missions. It quickly adapted its operations, and took health and social measures against the pandemic, with education shifting online uninterrupted. Both students and lecturers of our academic community have reacted competently to this change, and to the use of online applications and remote communication tools for lectures, seminars, and evaluation. Students have become increasingly involved in the new form of learning, expressing their satisfaction with the new strategies.
IZU manages an online infrastructure, which has grown essential to teaching during the COVID-19 crisis. It employed an integrated system of platforms dedicated to distance education, to facilitate students' access to lecture materials and online bibliographic resources, remote communication between students and lecturers (via messaging, discussion forums, video calls), assignment of homework and real-time tasks, as well as effective evaluation and feedback processes. All teaching-learning-evaluating activities are, consequently, made possible by the online infrastructure, which facilitates distance learning for Turkish and international students alike.
We know that Istanbul Zaim University offers one of the best campus environments and our applicants wish to live the IZU campus life. We are sure that there will continue to be countless social activities, sports courses and contests, cultural events, trips, and academic gatherings. In the meantime, IZU shall continue to fulfill its role for the community by undertaking social solidarity projects. The university's efforts towards the public bears special importance, especially in these crucial times. To ensure continuity of its positive impact, the university guarantees uninterrupted education, even, unfortunately, at the expense of suspending campus life.
Applicants for the upcoming fall semester 2020-21 will be able to start their education by September, in any case. In case you cannot travel due to the post-pandemic measures, you will still be able to follow distant online courses for your first semester and join us on campus in the second. If you graduate late, and are concerned that you will not be able to make it for the fall semester, you can start your education under a pre-registration status. You will be completely registered once you officially graduate. Regarding any other unforeseen circumstances that you may encounter, you will, at worst, be able to register for the second semester.
The university, in dealing with the crisis, adopted an approach that prioritizes the wellbeing of its students, ensuring that its international students experience minimal or no negative effects. Those who could not travel, stay at the university's on-campus student halls. The student dormitory management provides every service they need while ensuring that they stay safe, healthy, and indoors.
It is, therefore, a priority for myself and my colleagues to reassure you that we have taken the necessary measures to best look after all international students who presently study at our university. Apart from regular teaching activities, they are provided with additional support and counseling. In hope of continued improvement of the current situation, I wish to emphasize that the light of academic and research communities comes from their perseverance, and illuminates the world with optimism towards the future, regardless of physical location.
I would like to welcome you to Istanbul Zaim University, where together we can overcome challenges of the future.
On behalf of Istanbul Sabahattin Zaim University, with my best wishes
Prof. Mehmet BULUT, PhD
2018 © Istanbul Sabahattin Zaim University | {
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[S10] Snuffers|, James L. Wood, Jr., THE SNUFFERS, (BJW Printers; Beckley, WV : 1989), 929.273Sn72., p.7 (Reliability: 3).
[S103] FindaGrave|, FindaGrave.com, (www.FindAGrave.com), 191891783.
[S10] Snuffers|, James L. Wood, Jr., THE SNUFFERS, (BJW Printers; Beckley, WV : 1989), 929.273Sn72., p.6. | {
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Annadale humbled St. Rose's while Queenstown and Dolphin battled to a draw, when the Guyoil/Tradewind Tankers Under-18 Secondary School Football Championship continued yesterday at the Ministry of Education ground, Carifesta Avenue.
Annandale mauled St. Rose's 8-2. Colin Henriques and Omari Glasgow scored two goals each. Henriques tallied a double in the 13th and 18th, while Glasgow fashioned a double in the 27th and 45th minute.
Chipping in with goals in the 15th, 32nd, 60th and 69th minute respectively were Jamar Harrigon, ROn Robinson, Jerome Harrigon and Rondel Maxwell.
On the other side, standout Ravon Bailey recorded a double in the 53rd and 57th minute. Meanwhile, Queenstown and Dolphin battled to a 1-1 stalemate.
Kieron Dazzell netted in the 21st minute for Dolphin, while Kester Stewart equalised for Queenstown eight minutes onward. The event continues on Sundat October 28th at the same venue with four matches. | {
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2019 is a big year for the United States Women's National Team. Not only will they be participating in the eighth FIFA Women's World Cup in June looking to defend their 2015 title, but when play begins on January 19, it will kick off the 35th year of the USWNT and is the 20th anniversary of the 1999 FIFA Women's World Cup title.
With such a monumental year about to unfold and to celebrate the history of the USWNT, I thought I'd put together an All-Time Best XI squad. To qualify, players must have registered over 100 caps and been part of a victory in a major tournament (World Cup, Olympics).
The team will be chosen in a 4-3-3 formation, with four defenders, three midfielders, three forwards and a goalkeeper occupying the eleven spots.
With the kickoff to 2019 just hours away and the World Cup getting closer and closer, here are my picks for the top eleven players in the history of the U.S. Women's National Team.
The obvious choice for the goalkeeper on the team, Solo registered 202 caps in 17 years with the WNT while recording 102 shutouts. She helped the U.S. capture gold at both the 2008 and 2012 Olympic Games, as well as claiming victory in the 2015 FIFA Women's World Cup.
Solo also received numerous individual accolades throughout her career, including the Golden Glove at both the 2011 and 2015 World Cups, while also taking home the 2011 tournament's Bronze Ball. She was also named the 2009 U.S. Soccer Female Player of the Year and was chosen as the 2015 CONCACAF Women's Goalkeeper of the Year.
During an 18-year run with the WNT, Fawcett became one of the U.S.'s all-time best players, appearing in 241 games, while helping the U.S. capture two World Cup titles (1991, 1999).
The 1988 U.S. Soccer Female Player of the Year also helped the U.S. win three Olympic medals, winning gold at the 1996 and 2004 Games. Following her career, Fawcett was inducted into the National Soccer Hall of Fame in 2009 and was named to the USSF USWNT All-Time Best XI in 2013.
With 192 caps, Chastain left her mark on the WNT. During her career she helped the U.S. win three Olympic medals (two gold) and two World Cup titles. As part of the 1999 World Cup champions, Chastain converted the winning kick in a penalty shootout that gave the U.S. the win, which she followed up with one of the most iconic celebrations in sports. After her career, Chastain was inducted into the National Soccer Hall of Fame in 2017.
During a 13-year run with the USWNT, Overbeck won a gold medal at the 1996 Olympic Games, as well as World Cup titles in 1991 and as the captain of the 1999 squad. She was one of just two players to play every minute of each of the team's games at the 1995 FIFA Women's World Cup, the 1996 Summer Olympics, and the 1999 Women's World Cup. After leading the U.S. to a silver medal at the 2000 Olympics, Overbeck retired. She was inducted into the National Soccer Hall of Fame in 2006.
With 311 caps in 19 years, Rampone ranks second in WNT history in appearances. During her historic run, she played in nine major tournaments – five Women's World Cups and four Olympic Games – the most in team history. Rampone helped the U.S. win Olympic gold on three occasions (2004, 2008, 2012) as well as silver in 2000 while also winning two World Cup titles, captaining the 2015 team to victory in Canada.
The most-capped player in women's soccer history (354 caps), Lilly was a staple in the midfield of the WNT for 24 years. She ranks third in U.S. history is goals (130) and second in assists (106) and was named the U.S. Soccer Female Player of the Year in 1993, 2005 and 2006. During her time with the WNT, Lilly helped the team capture three Olympic medals (two gold) and two World Cup titles in 1991 and 1999. After she retired, Lilly was inducted into the National Soccer Hall of Fame in 2014.
With 265 caps and 105 goals, Lloyd ranks fifth in WNT history in both categories. After winning Olympic gold medals in 2004 and 2008, Lloyd carried the team to the 2015 FIFA Women's World Cup title, netting a hat-trick in the final against Japan and taking home the World Cup Golden Ball and Silver Boot. More hardware came after the World Cup triumph as she was named the U.S. Soccer Female Player of the Year for the first time since 2008 while also being named the CONCACAF Women's Player of the Year and the 2015 FIFA Women's World Player of the Year. She again received the World Player of the Year award in 2016 and in 2018 reached the coveted 100-goal club in April before helping the U.S. clinch a spot in the 2019 FIFA Women's World Cup in the fall.
The co-FIFA Women's Player of the Century, Akers tallied 107 goals (4th in U.S. history) while helping the U.S. will the inaugural FIFA Women's World Cup in 1991, where she took home the Golden Boot and Silver Ball. A three-time U.S. Soccer Female Player of the Year (1990-91, 1999), Akers also led the WNT to a gold medal at the 1996 Olympics before winning a second World Cup title in 1999, where she received the Bronze Ball. After her storied career, she was named to the FIFA 100 – a list of the 100 greatest footballers – and was inducted into the National Soccer Hall of Fame in 2004.
One of just two women named to the FIFA 100 list, Hamm is arguably the greatest player in the history of women's soccer. During an 18-year run with the WNT, she made 276 appearances (3rd all-time) while scoring 158 goals (2nd) and tallying 145 assists (1st) and was named the U.S. Soccer Female Player of the Year five times (1994-98). Hamm was also a member of both the 1991 and 1999 World Cup champions, also winning two Olympic gold medals (1996, 20004) and one silver medal. The 2001 and 2002 FIFA Women's World Player of the Year retired as the all-time leading goal-scorer in international football history – men or women – and was inducted into the National Soccer Hall of Fame in 2007.
The all-time leading goal scorer in international soccer history, Wambach rewrote the record books during her storied career, finishing sixth in WNT history in caps (256) and third in assists (73) while winning the U.S. Soccer Female Player of the Year award a record six times (2003-04, 2007, 2010-11, 2013).
After leading the U.S. to a runner-up finish at the 2011 World Cup – where she received the Silver Ball and Bronze Boot -, Wambach led the U.S. to the World Cup title in 2015. She also helped the WNT claim gold medals at the 2004 and 2012 Olympic games.
Along with records and team success, Wambach was named the FIFA Women's World Player of the Year in 2012 and took home the 2014 CONCACAF Women's Player of the Year and in 2011 became the first soccer player to receive the AP Female Athlete of the Year award.
The author of perhaps the greatest goal in U.S. soccer history, Morgan was named to the USSF All-Time Best XI in 2013 – at just 24 years of age. During a breakout 2012 campaign, she led the WNT to an Olympic gold medal and was named the 2012 U.S. Soccer Female Player of the Year and was a finalist for the FIFA Women's World Player of the Year award.
After taking home the CONCACAF Women's Player of the Year in 2013, Morgan helped guide the U.S. to victory at the 2015 FIFA Women's World Cup while also taking home the CONCACAF Women's Player of the Year award in both 2016 and 2017.
After another spectacular season in 2018, Morgan received her third consecutive CONCACAF Women's Player of the Year award and was named the 2018 U.S. Soccer Female Player of the Year while leading the WNT to a berth in the 2019 FIFA Women's World Cup.
Currently sitting seventh in U.S. history in goals (98) and just two shy of the 100-goal club, Morgan should have plenty of good soccer ahead of her as she aims to lead the U.S. to another World Cup title. | {
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Kid's party means fun, balloons and laughter. It is unlike any regular party. You will never get bored even with all the kids play. A birthday is an important day for any child. They wait all year to celebrate this day with their friends and families. And why not, the burdens from their academic institute have blocked them from having their fair share of fun and amusement. As parents we often forget that amusement for a child is equally important as their education. It is very important to balance out both. Education is very important and many are not privileged to have that. But overdoing something can be very harmful. You certainly don't want your child to have a life without happiness. A child forced into study at all times can result badly. So in order to give them a little break you can throw them a party where they can enjoy with their friends. It can be any party; just a medium of celebration is enough to let them know you care. We often miss out the effort they put in everything and forget to appreciate them for that. This can dishearten any child and their performance can fall. But a celebration party in their honor is just the thing to let them know how much you love and appreciate them.
You can throw them a big party on their upcoming birthday. Take interest in their likings and they are going to love you for that. But it is a tough job to throw a party that too for a child. There are so many details to take care off. And after the day's job it seems like it is impossible. So in order to get some help you can call in the professional planners who can create an elegant party for your kids in no time at al. They are talented and experienced and understand what your child may like. They take firm notes on their interest and create exactly something your child will love. A child needs to express themselves, and some of them express through their interests, hobbies or collections. And as parents you should always encourage your child's diverse interest. So, for the themes it is best to leave it in the hands of the experts. They can bring out the very best of a child's party, with balloons, colors, flags, garlands and lights. They can turn any party into a breathing and living one. Their arrays of services are endless. Kids Parties are loaded with fun activities as well.
The games and activities are ladles with enjoyment. From ball games to dance competitions and from arts and crafts session to storytelling, they can provide it all. You also get the professional magicians, clowns, jugglers and many more. An evening filled with laughter and enjoyment is necessary for any child. The more they get to spend time with their friends, the more expressive they become. It is a very important part of growing up. | {
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I am 'Guest Posting" at the Catholic Bloggers Network on the Scripture, Sunday Readings and Reflections contributor page. Come and check out my post: How do YOU see God?
My priest friend just gently responded "smiling".
Read more of this post, illustrated by Kelly Comics and while you are clicking around, come and visit Equipping Catholic Families for Catholic activities and traditions and our newly renovated Arma Dei Shoppe, full of Catholic craft kits (now available by download to copy for your whole class), Catholic books and quizzing cards!
Monica is a wife, Mom of 5+ kids, a designer, an architecture school survivor, an author and a crafter who thinks that it's cool to be Catholic! Check out the Arma Dei Shoppe for solid Catholic, fun teaching tools and gifts to celebrate and teach the Catholic Faith and subscribe to Equipping Catholic Families for family-building and Faith-centred crafts! | {
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Home > Films > F > Fifty Shades Of Grey
Fifty Shades Of Grey | 2015
Fifty Shades Of Grey location: the exterior of Christian Grey's Seattle penthouse: Escala Building, 4th Avenue, Seattle | Photograph: wikimedia / Joe Mabel
British Columbia;
Dakota Johnson,
Jamie Dornan,
Jennifer Ehle,
Marcia Gay Harden,
Max Martini,
The one-time piece of online Twilight fan fiction replaced Harry Potter books and The Da Vinci Code as the necessary adjunct to a long train/bus/plane journey, and the film adaptation happily trots through its by-the-numbers format without expending needless energy on plot, characterisation or dialogue.
As with the series that inspired it, the story is set in the damp and fittingly grey-skied Pacific Northwest of the USA around Portland and Seattle but, apart from some Second Unit scene setting, was made in Vancouver, largely around the city's historic downtown core, Gastown, and in the North Shore Studios (formerly Lionsgate Studios), 555 Brooksbank Avenue in North Vancouver.
So Christian Grey (Jamie Dornan) is first seen jogging not around Seattle or Portland, but in Vancouver's Coal Harbour seafront area and down the steps at Oceanic Plaza on Hastings Street.
It does get a little confusing here, as there are two Vancouvers. Although the film is made in the famous Canadian city in British Columbia, there is another smaller city of the same name in Washington State (not really such a coincidence – they were both named after British sea captain George Vancouver who explored much of the Pacific Northwest coast).
It happens that Washington State University has a campus in the US Vancouver, and it's here that Anastasia Steele (Dakota Johnson) is studying journalism. So Vancouver, BC, gets to play 'Vancouver, WA', as these university scenes were filmed on the campus of the University of British Columbia, 2329 West Mall, using classrooms in the Liu Institute for Global Issues on Northwest Marine Drive, and exteriors of the Student Union Building and the Irving K Barber Learning Centre on East Mall.
Fortuitously standing in for her sick roommate, Kate, Ana heads off to the intimidating hi-rise 'Grey House' to interview mysterious Christian Grey, CEO of Grey Enterprises, who has amassed a mind-boggling fortune seemingly by shouting "That is not acceptable!" into the phone.
Fifty Shades Of Grey location: Ana interviews Christian at 'Grey House': Bentall 5, Burrard Street, Vancouver | Photograph: wikimedia / timsdad
As residents of Vancouver will have spotted, Grey's HQ is part of the Bentall Centre complex in Downtown. The 35-story Bentall 5 (or Five Bentall Centre), 550 Burrard Street between Dunsmuir and West Pender Streets, was the last tower of the complex when it was completed in 2007.
With the film's tag line, "Mr Grey will see you now", Ana nervously conducts the interview. They lock eyes; he sees her hidden passions; she sees his hidden pain, and we see an unashamedly old-fashioned romance, modishly tricked out with primly tasteful S&M accessories. And Ana comes away with Mr Grey's business card.
Fifty Shades Of Grey location: 'Clayton's' hardware store: Ladner Village Hardware, Delta Street, Delta | Photograph: Google Maps
Christian Grey is clearly a thrifty billionaire, shopping for his 'personal' equipment not at some fancy specialist emporium (I'm shocked to learn there are such places), but at his local hardware store. And – crikey! – whom should he find financing her college education by working in the store but Anastasia, ready to supply him with various widths of duct tape and yards of photogenically blood-red rope.
'Clayton's', the reassuringly well-stocked store, is Ladner Village Hardware, 4821 Delta Street, between Bridge Street at 48 Avenue in Delta, way south of Vancouver across the Fraser River.
Fifty Shades Of Grey location: Christian Grey's 'Heathman Hotel': Fairmount Hotel, West Georgia Street, Vancouver | Photograph: Google Maps
Away from his Seattle home, Grey is staying at 'Portland's' fictitious 'Heathman Hotel', which is the Fairmount Hotel, 900 West Georgia Street, just a few blocks southwest of Bentall 5. It's in the hotel's British Columbia Ballroom that Grey obligingly poses for a photoshoot by Ana's college chum, Jose.
After the session, Ana accompanies Christian to a 'Portland' coffee house where the pair tentatively get to know each other. The cool, bare brick-walled hangout was Rainier Provisions, since closed, which stood at 2 West Cordova Street, housed in the historic 106-year-old Rainier Hotel building in Gastown.
As they exit the coffee house and walk along Abbott Street, Christian grabs Ana from the path of an oncoming bike. After a brief clinch, he has a flicker of doubt "I'm not the man for you. I have to let you go." But of course he doesn't.
They're at the corner of street corner of Water Street, near the statue of Gassy Jack, from whom Gastown gets its name, and the eagle eyed will have spotted that they're outside Peckinpah Restaurant. This isn't a movie in-joke by the Production Designer, by the way, it's a real Gastown restaurant.
Like all good students, Ana celebrates the end of her finals by getting well and truly trashed with her friends. Sadly, the bar was just a set built in the Burrard Iron Works building, 235 Alexander Street at Main Street, near CRAB Park.
A drunken phone call brings the concerned Christian hurrying over in time to catch her barfing spectacularly in the street. The bar entrance was the rear of the Burrard Iron Works (which now houses an exhibition space) beneath the curve of the Main Street Overpass. The same complex was later used as Ajax's lair in Deadpool.
Ana wakes up from her alcoholic haze, inevitably sans clothes, in Christian's hotel room. He's quick to reassure her that nothing happened, adding that nothing will happen without her written consent – his tastes being, as he admits with an archaically Victorian flourish, "very singular".
Nevertheless, he's soon showing up, with chauffeur, at the hardware store and whisks Ana off in a waiting 'copter for a night flight to Seattle.
Just as in the book, Grey's penthouse turns out to be atop the city's Escala Tower, 1920 4th Avenue at Virginia Street in Belltown.
The tower's real penthouse was sold for a massive $6.2 million – supposedly the highest price paid for a Seattle condo in many years. I hope the new owner wasn't too disappointed to discover that it doesn't really come with a locked Red Room (author EL James has admitted she'd never set foot in the place).
The play room was built in the studio and other interiors for the Escala were filmed in 36-story Jameson House, 838 West Hastings Street, back in downtown Vancouver.
It's here that Christian finally gives Ana a little taste of his singularity, and the next day drives her home, briefly stopping off at Stanley Park, Pipeline Road. The wooden pier on which they talk is at Beaver Lake.
Fifty Shades Of Grey location: Ana's apartment: Powell Street, Vancouver | Photograph: Google Maps
Ana's new 'Portland' apartment, outside which Christian hands her the written contract for her consideration, and later delivers a posh replacement for her beloved VW, is 120 Powell Street, barely a block west of the Iron Works bar location.
Fifty Shades Of Grey location: the graduation ceremony: Chan Sun Concert Hall, Chan Centre for the Performing Arts, Vancouver | Photograph: wikimedia / TedxVancouver c/o Maurice Li
Soon Ana is graduating at a ceremony held in the Chan Sun Concert Hall of the UBC Chan Centre For The Performing Arts, 6265 Crescent Road, where Christian makes a speech (did I forget to mention he's also a benefactor of Ana's college?) letting slip the tantalising hint that he knows what it's like to go hungry.
The Chan Centre has become something of a staple for TV sci-fi shows, having appeared in The 4400, Fringe, Stargate Atlantis and Battlestar Galactica.
At the subsequent reception party in the university's nearby Frederic Wood Theatre, Ana now introduces Christian as her boyfriend.
She goes on to join Christian, his mother (Marcia Gay Harden) and family for dinner at the Grey home, which is Casa Mia, 1920 Southwest Marine Drive in Vancouver's Southlands neighbourhood. The Spanish Revival/art deco mansion, built in 1932 for brewery magnate George Reifel – during Prohibition – was also seen in the pilot show for TV's Psych.
The wonderful glass-roofed swimming pool, where Ana questions the nature of their relationship, is the Pompeii Pool at the nearby Rio Vista estate, 2170 Southwest Marine Drive.
Control-freak Christian is taken aback at Ana's sudden announcement that the next day she's off to visit her mother in Savannah, Georgia.
The 'Savannah' hotel bar in which Ana discusses her new relationship with her mother (Jennifer Ehle) is The Fish House in Stanley Park (which has also closed – oh dear, the curse of Fifty Shades?), 8901 Stanley Park Drive. When Christian suddenly shows up, many women might think it's time to consider taking out a restraining order, but Ana is happy to take off for another mystery trip, this time looping and rolling in a glider at Boundary Bay Airport, a few miles southeast of the hardware store in Delta.
An urgent phone call summons the two back to the Escala, where Ana pushes the limits of what she's willing to do and, depending on your level of cynicism, the film ends with either a daring structural shock, or a blatantly contrived teaser for the sequel.
Visit: British Columbia
Visit: Vancouver
Flights: Vancouver International Airport, 3211 Grant McConachie Way, Richmond, BC V7B 0A4 (tel: 604.207.7077)
Stay at: the Fairmount Hotel, 900 West Georgia Street, Vancouver, BC V6C 2W6 (tel: 604.684.3131)
Visit: Washington State
Visit: Seattle
Flights: Seattle–Tacoma International Airport, 17801 International Boulevard, Seattle, WA 98158 (tel: 206.787.5388) | {
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Fabulous Journeys
8/27/2007 — By Robert Firpo-Cappiello
1 / 7 Photos
In the late 1500s, European artists depicted foreign cultures in ways that mixed myth, Christian theology, and newly discovered facts. For an example, look at this page from one the earliest illustrated books, the Nuremberg Chronicle. (National Gallery of Art, Washington, D.C., Paul Mellon Collection)
Europeans relished fanciful images like this 17th-century one that portrays the Greek god Dionysus as a leopard returning from India with followers in tow. (National Gallery of Art, Washington, D.C., Ailsa Mellon Bruce Fund)
Here's a detail from the first widely printed road map of Central Europe. This south-on-top map was created for pilgrims traveling to the holy city of Rome. Each dot stands for about 7.5 kilometers. When used with a pocket sun compass, it's quite accurate. (National Gallery of Art, Washington, D.C., Rosenwald Collection)
In this celebrated print from 1513, the German artist Albrecht Durer portrays a rider on horseback as a symbol of moral virtue moving steadfastly through darkness. The print's title is Knight, Death, and Devil. (National Gallery of Art, Washington, D.C., Rosenwald Collection)
This impressive 16-foot-long panorama depicts the overland journey from Europe through the Balkans to Constantinople, which was the capital of the Ottoman Empire. In the early 1500s, this journey would have taken between 30 and 45 days. (National Gallery of Art, Washington, D.C., Rosenwald Collection)
European encounters with the New World fueled a lively market for prints and images of America, such as this 1590 one titled "Dance of the Virginians" from The Wonderful but True Report on the Manners and Customs of the Savages of Virginia. (Private Collection)
In 1710, four Iroquois chiefs traveled to London to solicit Queen Anne's help in battling tribes allied with the French. They quickly became the subjects of numerous works of art, plays, and poems. This print shows Etow oh Koam, head of a Mohican tribe. (National Gallery of Art, Washington, D.C., Paul Mellon Fund)
9 Ethnic Neighborhoods With Incredible Internation...
Northeast Wineries: 10 Vineyards That Are Changing...
10 Delicious Food Factory Tours
7 Exceptional American Food Halls
Cocktails at Your Service: 8 Hotels With Amazing M... | {
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"Not surprisingly, the federal judiciary nearly always rules in favor of the federal government. Judicial review, contrary to the assurances of its advocates, has hardly restrained Congress at all. Instead it has progressively stripped the states of their traditional powers, while allowing federal power to grow unchecked." Joseph Sobran, (1946-2010) Columnist. Source: Usurpation of power is routine, Conservative Chronicle, October 25, 1995.
Al on Has the King of the North Been Pushed Too Far in American Politics?
Marcy on Has the King of the North Been Pushed Too Far in American Politics? | {
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WHERE IS MY BROTHER JOHN SPIRA?
MISSING SINCE FEBRUARY 23, 2007
Many Thanks To Lamar Advertising for Two Tenth Anniversary Billboards!
Tweets by @FindJohnSpira
Click Here to open the Searching For John Spira Blog in a new window.
Click Here to go to John's Facebook Page "Missing John Spira".
Please click on John's picture below to view my first video from 2007 asking for your help!
Please help me find my brother John!
He has been missing since February 23, 2007!
News Story Links
CLICK PLAY below to hear LOVE REACTION (Featuring my brother John Spira on guitar):
Please Watch "When the Music Stopped" Promo
Thank you to everyone who watches John's story on "DISAPPEARED"!
If you want to watch all of "Disappeared: When The Music Stopped" right now,
John's episode is available for purchase at this link:
When-the-Music-Stopped
THE SEARCH CONTINUES!
John Spira, Chicago Johnny Is Missing: Please Help Us Find Him!
PLEASE KEEP CHECKING THESE AREAS --
ESPECIALLY IF YOU OWN PRIVATE PROPERTY IN THESE AREAS:
THANK YOU TO AMERICA'S MOST WANTED FOR COVERING JOHN'S CASE!
CLICK HERE TO WATCH AMW CLIP!
John Michael Spira, 45 years old, 5'8", 165 pounds, brown hair, brown eyes.He has been missing since Friday, February 23, 2007, 7:00 pm. from West Chicago, Illinois.
Resident of St. Charles, Illinois. Last seen wearing blue jeans, black turtleneck sweater, black shoes, olive green aviator jacket.
This is no ordinary guy; as hundreds of friends and relatives will attest. Everyone has something wonderful to say about John Spira who has been missing since Friday, February 23, 2007; last seen at 7:00 pm at his workplace on County Farm Road near North Avenue in unincorporated West Chicago, Illinois.
To report information,
CALL Dupage County Sheriff Investigations:
Click Here to download John's Flyer: Download Now!
Please take a moment to view and add to John's Weblog
Do You Know John Spira? He's No Ordinary Guy!
John Spira is a very talented man. You may know him.
Hundreds of friends and relatives will attest that John was no ordinary guy; everyone has something wonderful to say about John Spira.
Owner of Universal Cable Construction in West Chicago, Illinois,John was active in community affairs. John, a U.S. Army veteran, was a tank driver stationed at Fort Carson,Colorado,
An electronics and machinery aficionado, a race car builder and driver, and a private pilot;
About to launch a promising aviation venture with Marchetti and warbird training. John Spira was an active, fun-loving guy with a straight-forward approach to life; loved,respected, and admired by all; always helping anyone in need.
Music was John Spira's passion; he has been mesmerizing listeners with his hard-driving, soulful blues for 30 years. John was an accomplished guitar and slide-guitar player with the Rabble Rousers Band prior to his mysterious disappearance.
UPDATED POINTS of INTEREST:
John placed a cell phone call to a friend at 7:09pm confirming that he would meet for dinner in Oak Brook, IL at 8:30pm, but he was never to arrive. THE LAST PERSON TO SEE JOHN ALIVE WAS HIS "FRIEND"AND BUSINESS PARTNER OF 20 YEARS, DAVID STUBBEN AT 7:15 pm AT THEIR OFFICE. JOHN'S CAR NEVER LEFT THE OFFICE PARKING LOT. JOHN AND DAVE WERE HAVING SERIOUS FINANCIAL ISSUES AT THE TIME OF JOHN'S DISAPPEARANCE. Whatever happened to John could only have happened between 7:10 and 7:45; a very short time frame. When DuPage County and St. Charles police initially investigated the matter in theearly morning hours of Sunday, 2/25/07, John's employees at Universal Cable officially reported a large piece of heavy duty plastic sheeting material missing from the premises. DAVE, the last person to see John alive, HAS REFUSED A LIE DETECTOR TEST AND WILL NOT SPEAK WITH THE POLICE. WHY?
John and his estranged wife, Suzanne, had agreed on the final details of their divorce settlement on the morning of February 23rd, a FACT she has since denied. Why? They had been going through a nasty divorce for 2 years. SUZANNE WAS THE PETIONER. She was FINALLY COAXED into filing an official missing person's report with the St. Charles Police Department at 5:30am of the following Sunday,February 25th, 2007. Their divorce was to be official on March the 8th. Within the first 2 weeks of John's disappearance Suzanne tried to have John's amplifiers appraised at a local music store. Why?The person at the music store refused and reported this to the police. By September of 2007, SUZANNE SOLD ALL THEIR BELONGINGS AND MOVED TO NEW YORK. (She has since been found dead in her home in New York.) SUZANNE FILED PLEADINGS IN THE KANE COUNTYPROBATE COURT AND STOOD TO POTENTIALLY GAIN A SUBSTANTIAL SUM OF MONEY AS WELL AS PROCEEDS FROM A LIFE INSURANCE POLICY IF AND WHEN JOHN WAS DECLARED DEAD. SUZANNE ALSO REFUSED A LIE DETECTOR TEST. WHY
Another interesting fact: On 9/14/07 around 7:30 p.m. some friends erected a very large, 5' x 20' banner attached by 10x4's and 2x4s and solidly placed in the ground, directly across the street fromand facing UCC, WITH PERMISSION of the landowners. The banner had 2 large pictures of John and his missing information. At the time the banner/billboard was being erected, several people were standing in front of UCC but no one offered help. WAS DAVE WATCHING? It was near dark when the billboard went up. John's Business was burned to the ground 48 hours later on Sunday, September 16, 2007. The billboard was nowhere to be found and we do not know when it was removed or if it was burned in the fire. Another billboard put up in the same place shortly thereafter was dismantled. The(now) gutted building that was once home to former Du Page County "Business of the year" nominee, Universal Cable Construction Inc., was co-owned by John's estranged wife and the wife of John's business partner, David W. Stubben. Firemen could not enter the building at the time of the fire because TOO MANY BULLETS were exploding?????
THIS IS A HOMICIDE CASE. The police still call it a missing person's case but those of us who know John, know that he never, ever would have walked away from his life, not ever. In fact, he was very happy on the 23rd because a settlement agreement had finally been reached in his divorce; again, a fact Suzanne denied. We will not give up in our efforts to see that John gets the justice he deserves and that those responsible pay dearly for their horrendous crime against John, his family and those that knew and loved him.
If you would like to contribute to our search efforts please make a donation via the paypal link below
The John Spira Search Fund - at Chase Bank, IL1-2520 c/o - John Spira Search Fund - 1825 West Lawrence Ave. Chicago, IL 60640 (ACCOUNT NUMBER: 734664360).
Click Here to download a printable Missing Persons Poster
File Name: poster_johnspira.pdf 140 KB
The Spira family is very grateful for all of your help.
Help find John. Keep your hope and your prayers constant. | {
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Biografia
Figlia del critico cinematografico Filippo Sacchi e di Josepha Gianzana (zia di Giangiacomo Feltrinelli), moglie dell'attore Vittorio Mezzogiorno e madre dell'attrice Giovanna Mezzogiorno, ha recitato nella pièce di Maurizio Costanzo Vuoti a perdere.
Ha lavorato anche in televisione (conducendo pure il programma per i bambini Giocagiò) e in lavori prodotti da Lucio Ardenzi, recitando a fianco di noti attori, fra cui Domenico Modugno.
Dopo l'incontro con Mezzogiorno, avvenuto nel 1969 al Teatro Greco di Segesta, e la nascita della figlia Giovanna, nel 1974, si è ritirata dal mondo dello spettacolo, tranne che per partecipare a ruoli televisivi negli anni novanta. È deceduta dopo una lunga malattia il 29 ottobre 2010. Le sue ceneri riposano col marito nel cimitero di Griante, sul Lago di Como, sede di una villa ereditata dal nonno materno, il banchiere Mino Gianzana. Nello stesso cimitero sono sepolti i genitori.
Filmografia
Attrice
Le avventure di Laura Storm (1966) - serie TV
Vivere insieme episodio Un padre superfluo (1968) - serie TV
Processi a porte aperte episodio Losey il bugiardo (1968) - serie TV
I fratelli Karamazov (1969) - miniserie TV
Don Giovanni in Sicilia, regia di Guglielmo Morandi (1977) - miniserie TV
Hors saison, regia di Daniel Schmid (1992)
Più leggero non basta, regia di Elisabetta Lodoli (1998)
Negli occhi, regia di Daniele Anzellotti e Francesco Del Grosso (2009) - documentario
Aiuto regista
Il giorno dei cristalli, regia di Giacomo Battiato (1979) - film TV
Note
Collegamenti esterni
Attori teatrali italiani
Attori televisivi italiani | {
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The Organising Committee is pleased to announce the 3rd International Whitefly Symposium will be held in Fremantle, Western Australia from the 16 - 21 September 2018.
The 2018 Symposium theme is "Putting Farmers First" keeping this at the forefront whilst working together to share openly and form new collaborations.
Join us for what promises to be a successful and world-class Symposium, with a series of stimulating presentations by international keynote speakers and nationally recognised experts taking place across 6 days.
Savour the culture and tradition of Western Australia's premier tourist destination when staying at the re-imagined Esplanade Hotel Fremantle by Rydges.
building while looking over the iconic port city, creating an environment that is rich, warm and sophisticated for business and leisure travelers alike.
Accommodation rates will be available - please register your interest to receive regular updates.
For maximum brand positioning, exposure and interactive networking opportunities, we are delighted to offer numerous sponsorship opportunities.
Save the Date in your calendars by clicking on the image below. | {
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There is a lots of competition in online business and everybody wishes to stay on the top. So, Search Engine Optimization (SEO) is the only way to climb above the competition also to enhance the occurrence of your business online. Our SEO specialists know well how to upgrade the traffic of your website and get your rank higher. | {
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"use strict";
var _interopRequireWildcard = require("@babel/runtime/helpers/interopRequireWildcard");
exports.__esModule = true;
exports.createDbQueriesFromObject = createDbQueriesFromObject;
exports.prefixResolvedFields = prefixResolvedFields;
exports.dbQueryToSiftQuery = dbQueryToSiftQuery;
exports.toDottedFields = toDottedFields;
exports.objectToDottedField = objectToDottedField;
exports.liftResolvedFields = liftResolvedFields;
exports.DbComparator = void 0;
var _ = _interopRequireWildcard(require("lodash"));
let DbComparator;
exports.DbComparator = DbComparator;
(function (DbComparator) {
DbComparator["EQ"] = "$eq";
DbComparator["NE"] = "$ne";
DbComparator["GT"] = "$gt";
DbComparator["GTE"] = "$gte";
DbComparator["LT"] = "$lt";
DbComparator["LTE"] = "$lte";
DbComparator["IN"] = "$in";
DbComparator["NIN"] = "$nin";
DbComparator["REGEX"] = "$regex";
DbComparator["GLOB"] = "$glob";
})(DbComparator || (exports.DbComparator = DbComparator = {}));
const DB_COMPARATOR_VALUES = new Set(Object.values(DbComparator));
function isDbComparator(value) {
return DB_COMPARATOR_VALUES.has(value);
}
/**
* Converts a nested mongo args object into array of DbQuery objects,
* structured representation of each distinct path of the query. We convert
* nested objects with multiple keys to separate instances.
*/
function createDbQueriesFromObject(filter) {
return createDbQueriesFromObjectNested(filter);
}
function createDbQueriesFromObjectNested(filter, path = []) {
const keys = Object.getOwnPropertyNames(filter);
return _.flatMap(keys, key => {
if (key === `$elemMatch`) {
const queries = createDbQueriesFromObjectNested(filter[key]);
return queries.map(query => {
return {
type: `elemMatch`,
path: path,
nestedQuery: query
};
});
} else if (isDbComparator(key)) {
return [{
type: `query`,
path,
query: {
comparator: key,
value: filter[key]
}
}];
} else {
return createDbQueriesFromObjectNested(filter[key], path.concat([key]));
}
});
}
function prefixResolvedFields(queries, resolvedFields) {
const dottedFields = objectToDottedField(resolvedFields);
const dottedFieldKeys = Object.getOwnPropertyNames(dottedFields);
queries.forEach(query => {
const prefixPath = query.path.join(`.`);
if (dottedFields[prefixPath] || dottedFieldKeys.some(dottedKey => dottedKey.startsWith(prefixPath)) && query.type === `elemMatch` || dottedFieldKeys.some(dottedKey => prefixPath.startsWith(dottedKey))) {
query.path.unshift(`__gatsby_resolved`);
}
});
return queries;
}
function dbQueryToSiftQuery(query) {
const result = {};
if (query.type === `elemMatch`) {
result[query.path.join(`.`)] = {
$elemMatch: dbQueryToSiftQuery(query.nestedQuery)
};
} else if (query.path.length) {
result[query.path.join(`.`)] = {
[query.query.comparator]: query.query.value
};
} else {
return {
[query.query.comparator]: query.query.value
};
}
return result;
} // Most of the below can be gone after we decide to remove loki
// Converts a nested mongo args object into a dotted notation. acc
// (accumulator) must be a reference to an empty object. The converted
// fields will be added to it. E.g
//
// {
// internal: {
// type: {
// $eq: "TestNode"
// },
// content: {
// $regex: new MiniMatch(v)
// }
// },
// id: {
// $regex: newMiniMatch(v)
// }
// }
//
// After execution, acc would be:
//
// {
// "internal.type": {
// $eq: "TestNode"
// },
// "internal.content": {
// $regex: new MiniMatch(v)
// },
// "id": {
// $regex: // as above
// }
// }
function toDottedFields(filter, acc = {}, path = []) {
Object.keys(filter).forEach(key => {
const value = filter[key];
const nextValue = _.isPlainObject(value) && value[Object.keys(value)[0]];
if (key === `$elemMatch`) {
acc[path.join(`.`)] = {
[`$elemMatch`]: toDottedFields(value)
};
} else if (_.isPlainObject(nextValue)) {
toDottedFields(value, acc, path.concat(key));
} else {
acc[path.concat(key).join(`.`)] = value;
}
});
return acc;
} // Like above, but doesn't handle $elemMatch
function objectToDottedField(obj, path = []) {
let result = {};
Object.keys(obj).forEach(key => {
const value = obj[key];
if (_.isPlainObject(value)) {
const pathResult = objectToDottedField(value, path.concat(key));
result = { ...result,
...pathResult
};
} else {
result[path.concat(key).join(`.`)] = value;
}
});
return result;
}
function liftResolvedFields(args, resolvedFields) {
const dottedFields = objectToDottedField(resolvedFields);
const dottedFieldKeys = Object.keys(dottedFields);
const finalArgs = {};
Object.keys(args).forEach(key => {
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//# sourceMappingURL=query.js.map | {
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Q: How to change Page Title with Tag Manager in order to show different title in Analytics? The best solution would be to modify website that is being tracked and change it to generate more valuable Page Titles.
However, that isn't possible and I would like to use breadcrumbs to provide new Page Title for Analytics.
I've created new variable for title in Tag Manager and added a Trigger for it in a Tag.
And yet the Page Title isn't changing and therefore I ended up wondering should this tag be fired before Analytics tag?
EDIT:
I've now used it with Preview mode and I can see that it is at least trying to set a new value for title. However, the value seems a bit too "unescaped" and I think that there's some hidden characters that cause problems.
EDIT 2:
function() {
var a = jQuery('.breadcrumb_container a');
delete a[0];
var textValues = jQuery(a).map(function() {
return jQuery(this).text();
}).get();
var str = textValues.join(' > ');
return str;
}
A: There is no need to create a new trigger. You should edit your existing pageview tag and set field of title as indicated below:
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SuprBay: The PirateBay Forum › Member Forums › Economics, Law & Politics
The scramble to earn a living in Gaza starts at school age thanks to Israel's siege
Last Active: Yesterday
Written by Motasem A Dalloul for Middle East Monitor
The start of the new school year in the besieged Gaza Strip saw just under 300,000 students aged between six and 17 turn up for classes; more than 20,000 are attending school for the first time, often in overcrowded classrooms. Despite the difficult situation in Gaza and the repeated Israeli military offensives, Gaza children generally enjoy going to school.
However, there are hundreds who get up early every day, but do not go to school. They roam the streets looking for work in order to earn some money for their families. Mahmoud Al-Borsh, 13, is one of them. He leaves his house at 6am every day and doesn't get back until 6pm with not even enough money to buy the soap needed to wash his clothes.
13-year-old Mahmoud Al-Borsh
Quote: "I get up as soon as I feel the sun in the sky, get ready for work and go out," he told me.
"I do not always know where to go, but I start with the rubbish bags and bins in the area near my house."
His job, such as it is, sees him trying to collect scrap metal and plastic. It is very difficult, and he works all day, often ending up with as little as 10 shekels ($3) in his pocket. It is also very dangerous, because the scrap metal could have been used to hold dangerous chemicals and hazardous liquids.
In the occupied territories, domestic rubbish is not disposed of in separate containers, with one for cans, one for plastic and cardboard, and one for perishable and other stuff. Everything goes into a nylon bag and put at the door to be collected by the cleaning workers. That's why dozens of youngsters like Mahmoud Al-Borsh leave home early, to check the bags before the cleaning team arrives. Many then follow the rubbish truck to the dump and scavenge for saleable items there.
According to the Palestinian Central Bureau of Statistics, almost 5,000 out of 372,600 children were working in Gaza in 2018, aged between 10 and 17. Almost 2,000 children were working part-time before or after school.
Al-Borsh braves the hot weather and traffic congestion to go to work when other children are going to school. "I am sad when I see the other children going to school, because I hope that one day I can join them. However, I am very happy that I can earn some money for food for my family." There are ten people in his immediate family, so whatever he brings home is most welcome.
He is losing hope about his education prospects, though.
Quote: "How can I learn to read and write after missing all the primary and preparatory lessons?"
Moreover, he has heard about someone who studied computer engineering at university and is now selling boiled corn on the streets. What good is education when there are no jobs at the end of it under the Israeli-led siege of Gaza?
Scrap metal and plastic dealer Abu Yahya told me that he buys items from at least 50 children every day.
Quote: "All of them are of school age."
The difficult living conditions, he explained, have pushed these children to get any kind of work, even if they do not make much money out of it.
Quote: "The most they can expect," said Abu Yahya, "is probably 15 shekels ($4.50) a day. But for a family living under the poverty line and in desperate need of food, that is an important contribution to the budget."
I looked for the computer engineer mentioned by Al Borsh and found him on the corniche alongside the Mediterranean. His name is Hamdi Lubbad and he is 26 years old. He studied computer engineering at one of Gaza's universities, but couldn't find a job, so sells boiled corn to support his family.
Palestinian computer engineer, Hamdi Lubbad
Quote: "After completing my BA degree, I spent two years looking for work but I could not find any," he explained.
"I needed a job because I have to get food and medicine for my mother, who has cancer. So I thought about having this cart. I use it to sell boiled corn in summer and sahlab — a hot Palestinian drink — in winter."
Lubbad trades under the name of "The Engineer"; he doesn't want people to think that he is uneducated. It is important for him that they know that he is an engineer and selling corn is not his preferred employment option. Most people will understand that the Israeli blockade imposed since 2007 is to blame for the lack of job opportunities.
According to Lubbad, he is not the only university graduate who has a job on the corniche. He counted off dozens who sell corn, household appliances, cigarettes, hot or cold drinks and so on.
Quote: "People like us do not need much money to get us going in such small businesses," he added.
Quote: "The disastrous economic situation in the Gaza Strip is the direct result of the Israeli siege," said Mohammad Abu Jayyab, chief editor of Al-Eqtisadiyeh newspaper.
"Unemployment is at record levels." The whole situation, he warned, is almost "unrepairable".
Mohammad Abu Jayyab, chief editor of Al-Eqtisadiyeh newspaper
International humanitarian aid, he pointed out, is for emergencies, not long term.
Quote: "After a couple of weeks, families need things other than food. They need clothes, household appliances, house repairs, electricity, fresh water; things that are not being offered by donors and charities."
Jamal Al-Khodari MP is the head of the Popular Committee against the Israeli Siege on Gaza. He told me that more than 85 per cent of the Palestinian families in Gaza suffer from food insecurity.
Quote: "They live under the official poverty line and have nothing at home to eat or drink just days after receiving food coupons from the international charities."
Moreover, as the Deputy Labour Minister in Gaza, Ihab Al-Ghussein, noted, "There are 270,000 professionals and university graduates who are looking for jobs in the Gaza Strip." New graduates join the search for those elusive jobs at the end of every academic year.
All three — Abu Jayyab, Al-Khodari and Al-Ghussein — reiterated that Israel must end the siege imposed on Gaza. If it doesn't, the besieged enclave is heading for an even more disastrous economic and social situation, and nobody knows where that will lead us. We can't say that we haven't been warned.
https://www.middleeastmonitor.com/202109...uel-siege/
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Qatar resumes aid to thousands of Gaza families Resurgence 0 2,563 Sep 16, 2021, 01:24 am | {
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First day begins with stay at hotel in Jaipur after arrival. In the afternoon, viewing monuments and tourist spots are planned. In the next morning, visit Amber Fort and other magnificent palaces. You will be driving to Bikaner from Jaipur, next day to witness Junagarh Fort and National Camel Breeding Farm. On the next day, travel to Jaisalmer from Bikaner to visit temple, fort and havelis. Fifth day ends with visit the Sand Dunes in the evening. Visit Blue city, Jodhpur on the next day and watch Mehrangarh Fort and Jaswant Thada in the afternoon. Move to Udaipur on the next day. Travel to City Palace and Museum in Udaipur, next morning. After the breakfast, drive to Pushkar, on the Ninth morning and get blessings from Lord Brahma Temple. On the last day, you will onward journey to Jaipur is planned after breakfast.
Hotel Accommodation on a twin- sharing basis.
For 02 Pax A/C Indigo & for 04 Pax, 06 Pax A/C Innova.
Government Service Tax (GST) 3.09% extra.
Reach hotel after arrival in Jaipur. Visit the City Palace and the Palace Museum in the afternoon. Jantar Mantar of 17th century can be seen too while driving past the Hawa Mahal. Rest overnight at the hotel.
Visit to Amer Fort is followed by traveling towards magnificent palaces with walls covered with mirrored mosaics, in the morning. Enjoy an elephant ride at Amer. Stay overnight after evening leisure.
Drive to the imposing walled city of Bikaner (321 kms / 7-8 hrs), early this morning. Visit the unusual Junagarh Fort, built on the desert plains itself, unlike other hill-top forts. National Camel Breeding Farm is shown too offering you a view of spectacular desert sunset in the background. Overnight stay at the hotel!
Drive to Deshnok to visit the Karni Mata Mandir in the morning. Visit desert town of Jaisalmer (332 kms / 7-8 hrs) is planned in the latter half of the day. Stay overnight at the hotel after evening's leisure.
Visit the spectacular Jaisalmer Fort, today! Besides, walk around the countless havelis of Jaisalmer regarded as city's reputed real showpieces. Visit to Sand Dunes, best known for spectacular sunset in the evening. Overnight stay marks day-end.
Travel to Blue City, Jodhpur (285 kms / 6-7 hrs) in the morning. You will visit Mehrangarh Fort and Jaswant Thada in the afternoon followed by overnight stay at the hotel.
Drive to Udaipur (259 kms / 6 hrs) visiting Ranekpur on your way. Ranekpur is famous for its exquisitely carved Jain temples and a hall of 1444 pillars. Boat ride can be enjoyed in the picturesque Lake Pichola, later this evening. Day ends with overnight stay at the hotel.
Sightseeing tour of city covers visit to City Palace and museum at the day-start. Jagdish temple and the Sahelion Ki Bari are also shown and overnight stay at the hotel marks end of the day.
Check out from the hotel and proceed to Pushkar from Udaipur in the morning. Seek blessings from Lord Brahma Temple and enjoy the day in Pushkar. Stay overnight at the hotel.
Onward journey to Jaipur is planned after breakfast at the hotel. You will reach Jaipur after 3 hours' drive (180 Km) from Pushkar. | {
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Archive for category: Jobs
You are here: Home / News / Jobs
Facebook to add 1,000 jobs in Ireland in 2019
January 23, 2019 /1 Comment/in Jobs /by News Desk
Facebook is to hire an additional 1,000 people in Ireland over the course of 2019.
The extra roles will be created across 60 teams, including the social media giants' engineering, safety, legal, policy, marketing and sales teams.
The roles will based on its Ballsbridge campus which was previously home to AIB.
The expansion will bring the total number of people employed across its centres in Cork, Dublin and Meath to 5,000.
The announcement was made in Dublin today by the company's chief operating officer, Sheryl Sandberg, while she attended Facebook's Gather event in Croke Park.
More than 500 small and medium businesses from Ireland and across the EMEA region attended the event.
Speaking on one of Facebook's priorities in 2019 to earn users' trust, Ms Sandberg said: "Facebook is a very different company to what it was in 2016 or even a year ago".
She detailed the steps the company has taken, and will be taking, in key priority areas including "the safety and security of Facebook's users; the commitment to cracking down on fake accounts and false news; strengthening defences against election interference; and being even more transparent in how it operates and makes decisions, to make itself more publicly accountable".
Meanwhile, Head of Facebook Ireland, Gareth Lambe, admitted today that the company is concerned about the current housing crisis gripping the country.
However, he says it is not something which has stunted Facebook's growth, and insists he has faith in how the government is tackling the problem.
"We're concerned, of course; to date, it hasn't been a blocker for us hiring, we have over 4,000 people here in Ireland and announcing another 1,000 today is a big investment," he said.
POP OUT We support all the government's initiatives, we think they're doing all the right things around planning, reform and cost benchmarking and all the infrastructure reform that we're doing.
"We think that will release this glut in a few years, we see it being not as bad in a few years," he said.
It was also announced today that Facebook would triple its investment in online safety programmes run by the National Anti-Bullying Centre (ABC) and SpunOut.ie, bringing the total investment to €1m.
The funding will go towards research and an online training program for teachers and parents of secondary school students.
An online safety resource for teenagers will also be created in partnership with SpunOut.ie.
https://www.advisoryexcellence.com/wp-content/uploads/2019/01/FB-LOGO.jpg 1080 1920 News Desk https://advisoryexcellence.com/wp-content/uploads/2017/08/Advisory-Excellence-logo.png News Desk2019-01-23 08:38:342019-01-23 08:38:34Facebook to add 1,000 jobs in Ireland in 2019
Elite Big 4 boutique seeking Audit and Advisory manager
October 29, 2018 /0 Comments/in Jobs /by News Desk
This firm offers the quality and benefits of a large firm in a smaller environment where there is more opportunity to use your initiative and gain responsibility early on.
They provide wide-ranging work experience in fields including investigation litigation support, business planning, financial modelling, tax planning, audit and general business advice. You will have the opportunity to deal with everything from an entrepreneur just setting up a business, to a large established company.
Clients include high street names, AIM-listed companies, film distributors, retailers and travel firms. They also specialise in working with hedge fund managers regulated by the FCA.
You will take responsibility for developing a wide ranging portfolio, building and driving excellent client relationships, delivering a quality service. You will manage the team and look to support and develop junior individuals. Alongside this you will have a development focus to your role, looking to identify opportunities for planning/further services etc. The firm is growing and planning for future developments and therefore the business is seeking individuals, who are career focused and looking to progress in level and responsibility. You will have genuine opportunity progress and develop in your career within this leading firm.
The Successful Applicant
ACA qualified accountant or equivalent
Currently working as an Audit Manager or Senior Manager
Intellectually ambitious
Aspirations to develop and one day achieve partnership
Curious and keen to offer clients a range of creative solutions
Focus on excellence in all you do
Enjoy building client relationships
Professional, friendly and supportive in approach
Company support, professional growth and partner prospects
£60,000 – £80,000 salary
Opportunity to study CTA (+ other qualifications)
Genuine work life balance
Opportunity to work with and learn from high quality senior advisers
Contact: Lorraine Twist
Quote job ref: 13915109
https://www.advisoryexcellence.com/wp-content/uploads/2018/10/MP.png 788 1400 News Desk https://advisoryexcellence.com/wp-content/uploads/2017/08/Advisory-Excellence-logo.png News Desk2018-10-29 07:01:242018-10-29 10:23:18Elite Big 4 boutique seeking Audit and Advisory manager
International organisation seeking Derivatives lawyer
September 21, 2018 /1 Comment/in Jobs /by News Desk
Based in London and reporting into the Head of Legal your main role will be to review, analyse and negotiate ISDA Master Agreements related to product and loan offerings, including Credit Agreements, Common Terms Agreement, Intercreditor Agreements, relevant Security Agreements as well as other project finance documentation. On a day to day basis this would include:
Draft and negotiate ISDA Master Agreements and any associated Credit Support Annex/collateral documents with various types of counterparty such as Financial Institutions and Corporates.
Review and analyse finance and security documents for derivatives hedging related to secured financing/project finance transactions.
Provide legal support and advice on laws, rules and regulations applicable to global transactions (including netting opinions for foreign jurisdictions and EMIR).
The successful candidate will need to be a qualified derivatives lawyer with experience from a top tier law firm and ideally a comparative banking organisation.
In depth understanding of ISDA documentation is essential and any exposure to loan and project finance hedging documentation would be highly advantageous.
A basic salary of up to £100,000 + excellent benefits + discretionary annual bonus.
Contact: Thomas Watson
https://www.advisoryexcellence.com/wp-content/uploads/2018/09/DV-PHOTO.jpg 853 1280 News Desk https://advisoryexcellence.com/wp-content/uploads/2017/08/Advisory-Excellence-logo.png News Desk2018-09-21 08:39:002018-09-21 09:27:39International organisation seeking Derivatives lawyer
Baker McKenzie law firm to create 150 jobs in Belfast
July 5, 2018 /3 Comments/in Jobs /by News Desk
GLOBAL law firm Baker McKenzie is to create 150 new jobs in Belfast as part of major expansion plans.
The legal company, who first opened in the city back in 2014, has entered into an agreement with Belfast Harbour Commissioners to take additional office space in the City Quays development. The deal will see Baker McKenzie lease a floor in City Quays 2, a move which will see staff numbers in Northern Ireland grow from just under 300 to 450.
The expansion also allows the legal firm to develop and grow the services it currently provides in Belfast.
Baker McKenzie was the first tenant to move to grade A office space within City Quays 1 in June 2015, but is now nearing capacity in its existing premises.
Since setting up in late 2014 the Belfast office, one of 77 around the world, has grown rapidly and now provides over 30 legal and business services, including finance, corporate support, marketing and IT.
Executive director at Baker McKenzie, James Richards said the expansion underlines the firm's commitment to Belfast and Northern Ireland.
"The growth of our Belfast office has been a remarkable success story which would not have been possible without the exceptional pool of talent here from both legal and business backgrounds, which has allowed us to create highly skilled and specialised opportunities in Northern Ireland."
"Our lawyers and professional staff around the globe have been really impressed at what we have created in Belfast and we have become a major innovation hub for the firm. We have introduced a number of initiatives here that are not only benefitting our clients but have a direct impact on our financial performance," he added.
Belfast Harbour CEO, Joe O'Neill believes Baker McKenzie's expansion in the city is testament to the offering provided in the City Quays development.
"Cementing our relationship even further with Baker McKenzie and facilitating their ability to grow is something which makes us very proud," he said.
"City Quays 2 is Belfast Harbour's response to ongoing demand by inward investors and indigenous firms for new Grade A office space in Belfast. The development has already established itself as the preferred destination for local and international business leaders and Baker McKenzie's decision to expand into City Quays 2 is a clear testament to the quality of the space provided, its location for business and the infrastructure around it."
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Good fight. This tournament doesn't seem like much because it has already had a season at 200, and there aren't many names, but when you do some research, you see, this has the makings of 4 good fights for an entertaining quarterfinal round.
Both these guys are undefeated, both are young, under 30, so probably in their primes or nearing that time, but Tabiti is a couple of years older than Fayfer, and has had 7 less fights, which isn't a good combination, but Tabiti might be the favourite in this fight, because he fought Steve Cunningham, biggest name on eiether record, and fought him on the Mayweather vs McGregor undercard as well, so he has more of a reputation.
Tabiti trains at the Mayweather gym, which says a lot about what he is learning in the gym, the quality sparring, the value of the advice he gets, it doesn't necessarily mean he is world level, but it is definitely a great place for a fighter to train. Tabiti has the better resume, with his last two wins, beating Cunningham and Kayode, I don't recognise a single name on Fayfer's record, he has had a few title fights, Baltic, International, Asian title (no idea why he fought for an Asian title, as a Russian based Russian), and Tabiti has had USA title fights, North American Title fights, so title wise, there isn't much in it, although Tabiti probably has the edge, but in terms of sheer calibre of opponent, records of opponents, levels opponents have been at, Tabiti has the much better experience, fought the much better opponents, but still, both these guys, unproven at world level.
These guys can punch, but I think given Tabiti has fought the better opponents, and he has 11% more KOs, we can assume he hits harder.
Neither of these guys were great amateurs, there is no record of any amateur success on Fayfer's BoxRec, and not much on Tabiti's, only had 38 fights, but he did compete in the Golden Gloves, so he was probably the better amateur.
There is no record of either being dropped on BoxRec, so we can assume they have good chins, but on the other hand, I don't think their chins have been really tested, especially not Fayfer's.
Fayfer has had 7 more fights, done 30 more rounds than Tabiti, so Fayfer has more general professional experience.
If this goes past 10 rounds, it will be unfamiliar territory for Tabiti, but not for Fayfer, because he has been 12 rounds once before.
Fayfer fought 4 times in 2017, and fought 4 months ago, he hasn't been that active, hasn't been past 4 rounds in oevr a year, but still, fought in June, and had plenty of fights last year, so he hasn't been inactive. Tabiti beat Cunningham 14 months ago, has had one fight since, stopped Kayode in 6 in May, so he hasn't been inactive, maybe not quite as active as ideal at this stage of his career, but still, inactivity shouldn't be an issue for him. I don't think activity will really be a factor in this fight.
I rate Tabiti, I was impressed with his performance against Cunningham, trains in the Mayweather gym, has fought the better opposition, and I think he is the better fighter, so I think he'll win this fight, but not easy, because Fayfer is young, fresh, and, is 23-0, can punch, it should be a competitive fight.
I think round after round, Fayfer will be competing, but Tabiti will be faster, busier, have better footwork, prove to be the more complete fighter, and he will be winning the rounds, I think Fayfer might have some success, late, but he won't be able to put Tabiti down as he needs to, to win the fight, and Tabiti will win a landslide UD.
Love this report - are you on twitter at all?
Welcome to eye on the ring.
No I'm not, I don't do social media.
My god I regret watching this fight. Worst fight I've seen all year. Tabiti fought completely defensively, and Fayfer held so much he should have been DQed. Hard to say too much based on an ugly fight, but I wasn't impressed with Tabiti at all.
Worse than Okolie vs. Askin?
I didn't watch that one, I usually catch UK fights after the results happen since I'm in the states. Result got leaked to me before I watched it, and obviously I wasn't going to subject myself to that torment when I know the result beforehand.
Fair enough, I wish I didn't watch it live myself.
I might only watch highlights of this one, based on what people have been saying about the lack of entertainment value.
I decided to watch this since I have some free time, but only because I want to write a half-decent prediction breakdown for Dorticos vs Tabiti.
I think with the point deduction (which was overdue, let's be honest), I think that sealed the fate of Ruslan Fayfer, a lot of those rounds were close, it was what you liked. It was a shame, because on paper, this fight was going to be a fantastic little scrap, but the styles didn't gel, didn't quite take off the way we hoped. Tabiti didn't use his speed as well as he could have, he was well aware of Fayfer's power, might have had to much respect, but I thought he was nicking those early rounds, I thought in the middle part of the fight he just took his foot off the gas amd didn't do enough work, even though he did the cleaner work, there wasn't enough, and Fayfer's scrappier work won those middle rounds, but in the last few rounds there, Tabiti picked up the pace, landed cleaner shots, and I think the nail in the coffin for Fayfer was that well warranted point deduction, because of all the head clashes, and I think Tabiti is the rightful winner. | {
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Stiletto Fire is a premier wedding and events band based out of Royal Oak, Michigan. The musicians can range from a small ensemble to a nine-member band, based on your preferences and the size of your wedding. The band offers an extensive song list that will appeal to guests of all ages. They play pop music, dance music and Top 40 hits. In addition to music entertainment, the band offers a state-of-the-art sound system and lighting array that will amaze and excite your guests. The band members are professional musicians who love interacting with their audience and bringing people up on stage.
Best Band!! Beyond all my Expectations!
Everything that is written about this band is true, Jeff and Stiletto Fire were amazing and better than I expected. They worked with me on whatever I needed the day of, entertained the crowd all night long, and made the overall reception the best it could be. People still haven't stopped talking about how great the band was at our wedding. I would recommend them in a heartbeat!
When my wife and I started planning our wedding, we both wanted to put on a high energy celebration and this meant live music. We spent a great deal of time watching videos and reading reviews on bands in the Detroit/Windsor area. There was a pretty consistent message and that was Stiletto Fire, and we are very grateful that they played our wedding.
From the very first inquiry, Jeff, was always on top of his game. A true professional through and through, making our night special was his number one goal and he lived that through the entire process. After some quick discussions about what genre of music we wanted and any specific requests (even the obscure song we chose, they nailed it), Jeff conjured up an amazing set list. Live music was coordinated for our ceremony and reception and it was amazing - people definitely loved the Beatles before the ceremony. Then there was the reception; Stiletto Fire brought the party and we danced the entire night away. At weddings, I'm used to things dying down as the night draws to a close, but we had a huge number of people on the dance floor right up to when they turned the lights on!
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Weddings can be stressful and things don't always go to plan. With Stiletto fire, they do go to plan and they'll exceed your expectations. If you are getting married; do not hesitate to give Jeff and Stiletto Fire a call for your wedding. We are extremely glad that we did!
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Stiletto Fire MADE our wedding. Hands down our best decision of our entire wedding was hiring them as both our band and ceremony music. Jeff and the entire band rocked the house and had the dance floor packed from the beginning of the night all the way until the last dance (encores included). Jeff was timely in all communications, very organized, and was also a great MC during the ceremony. We are still receiving compliments from our guests. You won't be sorry booking Stiletto Fire!
We have worked with Stiletto Fire a few times now and really enjoyed it! They are a super fun group and really know how to get the party started! They are super talented, energetic, and professional. We can't wait until we work with them again!!! | {
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The Counts of Celje
Permanent event at the Pokrajinski muzej Celje in Celje, Slovenia
The Counts of Celje. Courtesy of Pokrajinski muzej Celje
The Princely Palace now houses the permanent exhibition – The Counts of Celje. The Counts of Celje were one of the most influential noble families in the Slovenian lands in the Late Middle Ages. The Celje Counts were the focus of the museum since its beginnings; the museum carefully collected material remains, excavated by archaeologists at the Old Castle (Stari grad) in Celje and other locations. In 1956, the skulls of the Celje Counts – safely guarded in the Minorite church in Celje, the former tomb of the counts – were transferred to the museum. Due to lack of space, the synoptic exhibition the Celje Counts, set up in 1999, was stored in a depot for a few years. The Princely Palace is the new exhibition grounds for the presentation on the Celje Counts.
The beginnings of the Celje Counts reach back into the period of the free lords of Žovnek, their family seat being the Žovnek Castle in Lower Savinja Valley. By the year 1333, the Žovnek lords inherited the Huenburg property in Savinja Valley, their seat now being in Celje. The accumulation of feudal estates and the establishment of political connections reinforced Žovnek's status to such a degree that the emperor Louis the Bavarian elevated them to the status of the counts of Celje. Charles IV of Luxembourg bestowed them the same status. The foundation of their power was the vast property in Styria, Carinthia, and Carniola.
The House of Celje experienced the summit of power during the reign of Herman II; due to his desire to become liberated from the hegemony of the House of Habsburg, he established close connection with the Hungarian king Sigismund of Luxembourg in 1396, who later became the German and Bohemian king, as well as the Holy Roman emperor. The Celje Counts acquired a plethora of territories and titles in the area of today's Croatia. Herman II became the Slavonian, Croatian, and Dalmatian Ban (civil governor); governor of the Croatian diocese with the right to bestow the title of Vicar; moreover, he was a close member of Sigismund Luxembourg's council. During their peak of power, the House of Celje established family relations with the Houses of Hungary (Barbara of Celje), Poland (Anne of Celje), Serbia (Ulrich II), and Bavaria (Herman III).
Herman II's goal of attaining power, for which he spent five decades, was achieved when Sigismund of Luxembourg elevated Frederick II and Ulrich II of Celje to the status of stately princes in Prague in 1436. Their lordship over Celje and Sternberg-Ortenburg properties became the independent principality of Celje, in which they obtained the right to mint their own money as well as having their own provincial court for the nobility (in German Landschrannengericht). At that point, the Celje Counts stood on an equal footing with the Habsburgs. Soon after their elevation to the status of princes, the Houses were engaged in a family feud – the Celje Counts became a serious threat to the interests of Habsburgs concerning Inner Austria. The peace treaty between the two Houses, finalized in 1443, enabled the House of Celje to preserve the princely status; however, the princely rights were taken away from them, which spelt the end of the initial formation of the independent land of Celje. The most important document regarding the compromise between the Houses was the contract of mutual inheritance, which later enabled the Habsburgs to acquire all of the property of Celje within the Holy Roman Empire.
Henceforth, the House of Celje directed their political ambition towards Hungary, in which Ulrich II managed to acquire the title of regent in 1456 for the Hungarian king Ladislaus the Posthumous. The high title, which the noble Ladislaus Hunyadi also fought for, simultaneously brought imminent death to the last male descendant of the Celje family. Within a year, the Hunyadi henchmen murdered Ulrich II of Celje.
The House of Celje was the last important medieval dynasty which rose to the heights of European aristocracy. Their princely palace in Celje was, besides Trieste, the only location in the lands of Slovenia where the European cultural and artistic streams flew.
In less than a century, the name of Celje was firmly stamped into the political sphere of the Central European area. The Celje Counts approved of many cultural creations of their time. They were the founders of monasteries, and were known for their church donations; they were also actively engaged in building and reconstructing castles, which they owned more than a hundred at the height of their power. Numerous architectural monuments of the late Middle Ages within and outside today's borders of Slovenia are connected with the names of the Counts.
The Celje Counts are still part and parcel of the collective memory of Slovenians. With the help of literature, various genres, and contributions of amateur and scholarly writers, the dramatic life stories of certain Celje family members have survived for the last 500 years – no other Slovenian noble family can claim such an achievement. Throughout the centuries, there has been a persistent notion about the affluent and uncomprising family, willing to go to extreme lengths to reach any goal; in the 19th century, there was also the historical myth about the Celje Counts as the first bearers of Slovenian nationality.
Pokrajinski muzej Celje
The museum offers a versatile view into the cultural heritage of the Celje region, spanning over 3000 m2 of exhibition grounds and 10 locations outside Celje.
Museum profile
More from Pokrajinski muzej Celje
Ethnological Exhibition
Permanent event
The Cultural History Collection
Alma M. Karlin
More in Celje, Slovenia
From a bone needle to Celje stars
Permanent event at Pokrajinski muzej Celje
From the Gothic to Historicism in Steps
Celeia: a town beneath today's town
More in Slovenia
Živa Božičnik Rebec
19 Dec 2019 — 16 Feb 2020 at MG+MSUM in Ljubljana
Dimitry Orlač
28 Nov 2019 — 16 Feb 2020 at MG+MSUM in Ljubljana
14 Nov 2019 — 9 Feb 2020 at MG+MSUM in Ljubljana
Arteast 2000+ collection
19 Aug 2019 — 30 Aug 2020 at MG+MSUM in Ljubljana | {
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64th Berlin International Film Festival
Highlights of the Berlinale 2014
Facts & Figures 2014
"The Berlinale has an incomparable atmosphere. I look forward to it every year anew. To the films I see, to the people I meet. [...] The Berlinale is a village made up of people from hundreds of countries. Here, we share our life stories with each other." – Andres Veiel, Berliner Morgenpost, February 6, 2014
The 64th Berlinale began unusually: No snow fell on Opening Night. Instead, a warm February evening welcomed the national and international stars and guests on the red carpet. Ten days later, feelings ran high again at the Awards Ceremony, but not due to the weather. Instead of the highly praised Boyhood by Richard Linklater, a top contender in the Competition programme, Bai Ri Yan Huo (Black Coal, Thin Ice) by Diao Yinan received the Golden Bear for Best Film. In addition, Black Coal, Thin Ice leading actor Liao Fan received the Silver Bear for Best Actor. The decision by 2014 Jury President James Schamus and his fellow jurors - Barbara Broccoli, Trine Dyrholm, Mitra Faharani, Greta Gerwig, Michel Gondry, Tony Leung and Christoph Waltz - confirmed last year's trend of boldly pushing cinematic areas seldom recognised at A festivals into the spotlight. "A remarkable designation, a signal. It says, take a look at China, the market is booming there, film art is alive and well there, the world is all wrong there, China is where it's at" ( Christiane Peitz, Der Tagesspiegel, February 16, 2014). Variety head critic Scott Foundas agreed seamlessly with that assessment: "Unencumbered by Cannes and Venice's reputations as ground zero for the latest work of the world's most important name-brand auteurs, Berlin has the ability to think a little bit more radically, and to put films and filmmakers in competition who would almost certainly be relegated to a sidebar at one of those other fests" (February 16, 2014).
The team of Bai Ri Yan Huo in the Berlinale Palast
Director Diao Yinan himself was amazed: "It's really hard to believe that this dream has come true," he exclaimed to the audience at Berlinale Palast. Bai Ri Yan Huo (Black Coal, Thin Ice) illustrates the uncertainties of his home country, a genre film strongly reminiscent of film noir that can be read as a mirror of Chinese society, even though the director rejected that interpretation in his official statements. The significance of the triumph for Chinese cinema was evident in interviews following the award ceremony: "The Chinese film market is a very large one. We're already the second-largest worldwide. That's partially due to the size of our population, of course. But I'm sure that this magnitude will also lead to more diversity, that there will be a multitude of forms and genres for a wide array of market sectors in the future. I'm confident that a lot is going to happen." (dpa, February 16,2014)
Canonised filmmakers from the US took home the Silver Bear for Best Director (Richard Linklater) and the Silver Bear Grand Jury Prize, awarded to Wes Anderson for The Grand Budapest Hotel, the film that opened the 64th Berlinale. Since Anderson was no longer in Berlin to accept the award, Greta Gerwig read the audience a message in which the director articulated - in all modesty, and in his unmistakably ironic style - his joy at finally winning a real award made of real metal. Two more Silver Bears went to Asia. Actress Haru Kuroki was recognised for her performance in Chiisai Ouchi (The Little House) by Yoji Yamada and expressed her happiness with enchanting reserve; Zeng Jian received a Silver Bear for his camera work in Tui Na (Blind Massage) by Lou Ye.
Winner of the Silver Bear: actress Haru Kuroki
The winner of the Silver Bear Alfred Bauer Prize for a film that opens new perspectives seemed an odd selection. It was awarded to Aimer, boire et chanter (Life of Riley) director and French film doyen Alain Resnais - at age 91! The sad news that Resnais - who couldn't be in Berlin to accept his award personally - died just two weeks after the festival reinforced the impression that one of the cinema's most unusual and significant artists had been honoured for his seminal life's work.
Four German productions found their way to Competition in 2014, and one of them won the Silver Bear for Best Script: Kreuzweg (Stations of the Cross) by siblings Anna and Dietrich Brüggemann. French-born Berlin resident Guillaume Cailleau pocketed the Silver Bear for his 22-minute film LABORAT, while the Golden Bear for Best Short Film went to his home country - to Tant qu'il nous reste des fusils à pompe (As long as shotguns remain) by Caroline Poggi and Jonathan Vinel.
Madness with a method
Aside from the Award Ceremony, memorable Festival moments were most often provided by Hollywood stars. George Clooney set off a week-long press mania in which even Paul Katzenberger - author for the sombre publication Süddeutsche Zeitung - perpetrated a typo and tried to stay cool: "For the makers of the Berlinale, Clooney's appearance of Clooney is of course important as well, and the same somehow goes for audiences." (on February 7, 2014) At the photo call for Monuments Men, directed by Clooney, the film team - including Matt Damon, John Goodman and Bill Murray - danced to the Press Conference in conga line style.
"I am not famous any more": actor Shia LaBoeuf
Another Hollywood heavyweight made headlines in a more outrageous, off-putting way: To broach the issue of his 'ambivalent' relationship with the press, Shia LaBoeuf quoted footballer Eric Cantona ("When the seagulls follow the trawler, it is because they think sardines will be thrown into the sea") before wordlessly leaving the podium. Later that evening, he appeared on the Red Carpet wearing a brown paper bag stating "I am not famous any more" on his head, ensuring everyone's continued and undiminished attention. By contrast, director Lars von Trier played with the scandals surrounding his person in ironic and self-deprecating style. He wore a t-shirt bearing the Cannes logo and "Persona non grata - Official Selection" to the Photo Call. His work Nymphomaniac Vol. I was enthusiastically received by audiences - especially since actors Christian Slater, Uma Thurman and Stacey Martin were also in attendance on the Red Carpet.
Speaking of Eric Cantona: The Manchester United legend was also in the programme - as a performer in Looking for Eric by Ken Loach, the 2014 recipient of the Honorary Golden Bear and subject of the Homage. The tribute to one of the most committed realists in British cinema received unanimous and joyful approval, as exemplified by Georg Seeßlen in Freitag on February 6, 2014: "Hardly anyone is more deserving of a push to the centre of cinematic attention." As opposed to previous years, only one Berlinale Camera was awarded in 2014. It went to German producer and distributor Karl Baumgartner, whose company Pandora Film discovered art house heavyweights like Andrej Tarkovsky, Jim Jarmusch, Kim Ki-duk and Aki Kaurismäki for the national market. Just one month later, more sad news reached the Berlinale: Karl Baumgartner had died on March 8.
Ken Loach was awarded the Honorary Golden Bear
Cinematic heritage threatened
Digitisation of screening copies reached over 95%, and when a film was submitted as a 35mm copy, EFM Director Beki Probst remarked laconically: "I'm going to have the registration form framed and hang it in my office as a memento" (Blickpunkt Film 8/2, 2014). Of course, this development also carries a risk for the heritage of cinematic history. Ernst Szebedits, director of the Friedrich Wilhelm Murnau Foundation, was outspoken: "What isn't made available today is threatened with extinction in the digital age" (filmecho/filmwoche 8/2, 2014). Hence, the Berlinale once again set striking standards in the Berlinale Classics programme. The absolute highlights were the presentations of two cinematographic milestones: The restored version of Robert Wiene's The Cabinet of Dr. Caligari at the Berliner Philharmonie under the musical direction of New York avant-gardist John Zorn, and the international premiere of the 4K-DCPA copy of Nicolas Ray's Rebel Without a Cause. The film, which embodies the definitive triumph of youth culture like no other, was personally introduced by Martin Scorsese. His company "The Film Foundation" was involved in the restoration of the classic.
But the seasoned master also brought a film of his own to Berlin and presented it as a work in progress: Untitled New York Review of Books Documentary. Scorsese, himself a long-time subscriber, co-directed with cutter David Tedeschi, with whom he worked on Shine a Light (Competition 2008). Untitled New York Review of Books Documentary was shown at the Haus der Berliner Festspiele, where the festival series Film + Talk was successfully continued in 2014. Among the guests returning to the Berlinale was Erroll Morris, who put a spotlight on one of American politics' grand old hardliners in The Unknown Known: Donald Rumsfeld. The film continues Morris's processing of post 9/11 military interventions and their outgrowths: His 2008 Competition film Standard Operating Procedure focused an uncompromising eye on the human rights violations at Abu Ghraib prison, for which former US Defense Secretary Rumsfeld accepted responsibility.
Seolguk-yeolcha premiere with Tilda Swinton and John Hurt
Films about film
Another high point of the Berlinale Special programme at Haus der Berliner Festspiele was the presentation of André Singer's Night Will Fall. The documentary delves into the bizarre and convoluted creation history of another film, German Concentration Camps Factual Survey, a movie made with the raw footage of liberated concentration camps filmed by Allied cameramen in 1945. Political interests prevented the film's completion - despite cloak-and-dagger help from directing legend Alfred Hitchcock - leading German Concentration Camps Factual Survey to celebrate its world premiere in 2014 in Forum, whose section head Christoph Terhechte was very pleased to be able to present the final version. Fragments of the material were first shown in Forum in 1984 under the title Memory of the Camps. Forum also boasted the most lavish Korean production of all time. Seolguk-yeolcha (Snowpiercer) by Bong Joon Ho is a cinematic end-of-days vision with Tilda Swinton and John Hurt, who both attended the premiere. One of contemporary literature's most prominent authors also visited Berlin to celebrate the world premiere of L'enlèvement de Michel Houellebecq (The Kidnapping of Michel Houellebecq) with Forum audiences. Director Guillaume Nicloux presents Michel Houellebecq as a chain-smoking cameo who is more than grateful for a temporary escape from his bourgeois Parisian life. Though the section's diversity can hardly be conceived concisely, Forum named "The absurdities of the cultural establishment and merciless working environments" as its guidelines in 2014, and fulfilled it with such diverse contributions as Que ta joie demeure (Joy of Man's Desiring) by Denis Côté, who won a Silver Bear in Competition 2013.
Panorama was as fierce as ever. "Changing the world is a matter near and dear to the Panorama heart" was curator Wieland Speck's battle cry. As always, the programme explored the status quo of international cinema, with political undertones clearly resonating in every film shown. One of the few exceptions was 20,000 Days on Earth by Iain Forsyth and Jane Pollard, whose protagonist Nick Cave was enthusiastically received in Berlin. Transfilm, a Panorama staple theme from the start, was once again confirmed in its significance through global political events in February 2014. One day after the start of the 64th Berlinale, the 2014 Winter Olympics began. The venue: Sochi, Russia. In the run-up to the event, Russian president Vladimir Putin had repeatedly begged for attention by using hate speech against homosexuals. The 2014 Panorama programme was also proud to present the winner of the First Feature Award: Güeros by Alonso Ruizpalacios from Mexico. But Panorama also displayed the same tendency clearly visible in the awards towards the end of the festival: a striking array of Asian productions. The main programme, for example, opened with Nước (2030), a post- catastrophe thriller by Nghiêm-Minh Nguyễn-Võ.
The Zoo Palast: 2014 again a festival venue
Wieland Speck was personally very pleased about the return to Zoo Palast, which reopened in November 2013 after a three-year restoration and served as a premiere venue at the 64th Berlinale. On its website, the venue introduces itself: "The new, lovingly restored Zoo Palast recalls the grand old days of film theatre with its architecture, atmosphere and service". Evoking the glamour of movie palaces past is normally far from Forum Expanded's mind, since the section focuses on the thresholds of film art to visual arts and to the public space. But section head Stefanie Schulte Strathaus emphasised that the movie palace is an integral part of the former and current cinema landscape, and thus a part of the focus for the Forum Expanded 2014 programme. "What Do We Know When We Know Where Something Is?" was the central query, and answers appeared in panels and discussion rounds as well as in the exhibits and films. A feeling of unease with the complete digitisation of the moving image was clearly recognisable in some works that directly focused on the (disappearing) material celluloid. A similar theme was visible in Berlinale Shorts, where nearly a third of all productions were either made with analogue media or focused on the medium of film as a vehicle, and whose theme guideline assigned by curator Maike Mia Höhne was "Mourning".
Forum Expanded awarded a prize for the first time in 2014: the Think:Film Award. It went to Amie Siegel and her film Provenance, which stood out due to its interplay with Lot 248, also in the programme, which shows the auction of Provenance at Christie's in London, both creating and staging reality. As such, it was an example of the emphasis chosen for the 2014 Berlinale: the documental form. A connection was consistently visible in interviews with the section heads: The separation of documentary and fiction film is outdated, and yet can't be completely abandoned, as the relationship between image and reality requires constant renewed reflection. The European Film Market was especially active within the theme, hosting numerous panels and discussions dealing with the status and possibilities of the documental form.
Premiere in the JVA Tegel
The full extent of the festival's diversity
The workshop character of Retrospective 2014, under the title "Aesthetics of Shadow. Lighting Styles 1915 - 1950" met with positive feedback. Lukas Foerster wrote in die tageszeitung on February 6, 2014: "A film programme such as "The Aesthetics of Shadow" isn't about developing a finished body of work, it's about making new paths in film history visible."
Perspektive Deutsches Kino revived the Midnight Movie, harking back to the American cult films of the 1970s, which permanently expanded the limits of film representation by eschewing cinematic convention. Two films celebrated late-night premieres, and the rest of the 2014 Perspektive Deutsches Kino programme was a success as well: "It's a good year. Very diverse - even previously seldom-seen genres like horror and black comedy are represented - at an artistcally advanced level" (Kirsten Riesselmann in die tageszeitung on February 6, 2014). Furthermore, Perspektive 2014 ventured to a location unusual for the venues of the Berlinale - Raumfahrer (Spacemen) by Georg Nonnenmacher, the depiction of an inmate's inner world, was presented at the JVA Tegel penitentiary as a special screening.
Berlinale Talent Campus renamed itself in 2013, operating under the title Berlinale Talents in February 2014. The name change reflects the professionalism of the programme, as programme manager Matthijs Wouter Knol explained - moving away from a scholastic, academic connotation. The 2014 programme carried on with the workshops Summit, Studios, Project Labs and Talent Press, under the theme "Ready to Play - Breaking the Rules". The talents were challenged to think about playful paths in film development and design, as well as to question entrenched structures within the film business.
Kulinarisches Kino Goes Kiez in the Markthalle Neun in Berlin Kreuzberg
Two special Berlinale sections joined forces for a debut event called Culinary Cinema Goes Kiez - a screening of I Cavalieri della Laguna (The Knights of the Lagoon) by Walter Bencini at the independent cinema Eiszeit, followed by dinner and discussion at Markthalle Neun in Kreuzberg. Culinary Cinema provided both gourmet cinephiles with the traditional programme of sumptuous feasts for eye and palate, as well as Berlinale visitors with the Street Food fair on Potsdamer Platz. The Berlinale Goes Kiez screenings sold out at lightning speed as always, not least thanks to prominent cinema mentors like Christian Petzold.
The same procedure as every year
Eleven breathless days - that's perhaps the best way to sum up the Berlinale 2014. The festival was bursting at the seams with energy, events were set up on the fly right before the festival - like the Berlinale Open House format - with storytelling slams, discussions, etc. - in the new Audi Berlinale Lounge near the Red Carpet, or a free special screening of the first two episodes of Season Two of House of Cards was scheduled. The list goes on and on. The voices of those spoilt for choice didn't take long to make themselves heard: "The sheer size of the mammoth event came under criticism once again this year. It's just too big for the critic who at Cannes or Venice only needs to take notice of 50 films, not 200." (Christiane Peitz in Der Tagesspiegel on February 16, 2014) But success speaks for itself - and more than 325,000 tickets sold can certainly be counted as a success. Thus voices were also heard regarding the positive festival developments through Dieter Kosslick's accomplishments to date: "In 2001, he began running the Berlinale in a city in the midst of a metamorphosis - from square and snooty West Berliner affluence to a liberal-progressive governed, 'poor but sexy' metropolis that was suddenly on everyone's itinerary - with its raw unfinished charm, its spooky breaks in history, its wild and dime-a-dozen party world. And Kosslick turned the slightly stiff-necked cultural affair Berlinale into a debonair event with esprit and glamour - and economic significance." (Katja Bauer in Stuttgarter Zeitung, February 6, 2014)
Facts & Figures of the Berlinale 2014
Total amount of theater visits 491,316
Tickets sold 325,262
Accredited guests (press excl.) 16,148
Countries of origin 131
Journalists 3,742
Countries of origin 81
Number of films in the public programme 370
(incl. 106 short films)
Total amount of screenings 902
European Film Market
Film industry participants 8,396
Number of films 784
Number of screenings 1,109
EFM-Stands
(Martin-Gropius-Bau & Business Offices) 183
Number of exhibitors 487
Berlinale Co-Production Market
Participants 510
Berlinale Talent Campus
Annual budget € 21 million
The Berlin International Film Festival receives € 6.5 million in institutional funding from the Federal Government Commissioner for Culture and the Media in accordance with a decision by the German Bundestag. | {
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Friday, September 7: Once more markets opened on the back foot as trade troubles continued to induce investors to run for cover. Financials, energy and mining stocks weighed heaviest on the FTSE 100(-0.56%) as markets slid lower ahead of the afternoon's US Jobs report.
IAG(-4.21%)continued to lose altitude as it acknowledged the theft of financial and personal data over a 15-day data breach. 380,000 card payments were reported to have been compromised, with customers trying to cancel their credit cards to negate further negative impacts. British Airways admitted "criminal activity" had compromised the personal and financial details of customers who made bookings on its website or app from just before 11pm on August 21 until 9.45pm on Wednesday.
The US economy continued on its record-breaking run as it added 201,000 jobs, ahead of a consensus 192,000 and marking the 95th consecutive month of uninterrupted growth. Wage growth also picked up marginally in August, rising 2.9% from a year earlier, though it hasn't surpassed the 3% mark since 2009 despite the record number of jobs added.
Sterling leapt to a one-week high against the dollar after EU negotiator Michel Barnier said the EU was open to discussing other "backstops" on the Brexit issue. The EU has made the Irish "backstop" a condition for any divorce deal before Britain leaves the EU on March 29, 2019.
At the close European equities were mixed with the FTSE 100 -0.56%, the CAC 40 +0.16% and the DAX +0.04%. | {
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Jul 26, 2017 at 07:04 PM | 109 Views | Last edit Jul 26, 2017 at 07:07 PM 2 rev.
I'm searching for the VDA XSD-Generator.
For all the Formats it is availible. But not for VDA.
I'm sure I imported the tables.
Do you need some other message type other than the data types included in the B2B Mapping Toolkit? Each time we have applied patches for the B2B add-on I have had to import updates for VDA into that SWCV for the ESR. | {
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/ Spring Easter Bunny Pennant Banner, 14 Ft.
Spring Easter Bunny Pennant Banner, 14 Ft.
Get your guests in the celebrating spirit with this Spring Easter Bunny Pennant Banner. Hang this flag banner from a doorway to greet guests as they arrive, or attach to the corners of your food table for a charming Easter brunch display. With a bright and cheery Easter bunny design kids will love, this party banner is ideal for all of your Easter celebrations.
• Happy Easter Banner measures 14 ft. | {
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Q: closing multiple GLUT windows independently In my GLUT program i have created two windows. when i try to close one window entire program shuts down. can anyone tell how to avoid it.
My code to create window is as follows
int main(int argc, char **argv)
{
glutInit(&argc, argv);
glutInitDisplayMode(GLUT_DEPTH | GLUT_DOUBLE | GLUT_RGBA);
glutInitWindowPosition(100,100);
glutInitWindowSize(ww,wh);
window1 = glutCreateWindow("sample");
glutReshapeFunc(changeSize);
glutIdleFunc(renderScene);
glutDisplayFunc(renderScene);
window3 = glutCreateWindow("sample2");
glutReshapeFunc(changeSize);
glutDisplayFunc(renderScene2);
glutIdleFunc(renderScene2);
glutMouseFunc(mouse);
glutPostRedisplay();
glutMainLoop();
return 1;
}
A: I don't recall GLUT being able to close windows independently in the same thread, like that. As you only use a single glutMainLoop() call to get them going, thereby when the main loop is killed for one window, it's killed for all of them.
You could try creating the windows in their own Thread. That might work, but I'm not entirely sure.
Something else you could try, is to use GLFW instead, using GLFW, you need to create the main loop etc, yourself. Bottom line, that's much easier to use and it gives you a lot more control, over your OpenGL programs. Also if you don't already have it, you should get something like GLEW.
A: You've just left the capabilities of GLUT with this demand. But you're lucky: GLUT =/= OpenGL and there are many other frameworks that will satisfy your needs. How about you take a look at Qt, which offers you not only a runtime environment and a OpenGL widget, but also a large set of widgets to draw UI elements with.
| {
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Law Makes NY Schools Safer for Students
For a long time, teacher unions in New York pushed for a law to protect teachers from students. At the same time, schools boards pushed for a fingerprinting law to help them protect students from teachers with a criminal background.
On July 24, both sides got most of what they wanted when New York Governor George Pataki signed into law a series of comprehensive school violence measures. Looking on and applauding were three teachers injured in classroom assaults by students or their parents.
Under the new law, which takes effect in July 2001, teachers will have more power to banish troublemakers from their classrooms, and students or parents who assault teachers will face felony rather than misdemeanor charges. By the same token, teachers who assault students will face similar felony charges. Parents will be better informed about school safety with the inclusion of statistics about school violence in each school's Annual Report Card.
The new law enhances student safety by requiring teaching applicants to be fingerprinted for a criminal background check. It also makes school administrators subject to a felony charge if they cover up student-abuse cases by allowing school employees to resign without reporting the incidents. However, students will find more expected of them under new codes of conduct that administrators will write, and students will be schooled in character and civility. School officials are also required by the law to write more detailed safety plans for their facilities.
"These new laws will give parents, teachers, and students the confidence that their schools are safe and that their schools are creating an environment where disruption and violence are simply not tolerated," said Pataki.
But NYC School Buildings Still Pose Dangers
Last year, the New York Post ran an exposé revealing that one in three of city school cafeterias was crawling with vermin, exposing students to diseases carried by mice, roaches, and flies. "If you were a restaurant, you could be closed down for that–but people still have to send their kids to school," said Jill Chaifetz, executive director of Advocates for Children. The newspaper also ran a series of stories about student-on-student sex attacks in the schools, with a former school safety chief advising students not to walk alone in the hallways or go to the bathroom alone.
New York Post reporter Carl Campanile revealed recently there's yet another danger to students in the city's public schools: the school buildings themselves.
Complaint files reviewed by the newspaper revealed that the 10-year-old agency responsible for building and maintaining the schools, the School Construction Authority, had bungled repair jobs and endangered the safety of students and staff.
Last summer, for example, loose bricks from PS 57 in The Bronx fell off and landed in a playground, fortunately not hitting anyone. Other incidents included:
Faulty sash balances caused windows to crash down on the hands of two students in IS 52 in The Bronx.
A wooden beam fell on to a school safety officer in IS 135 in The Bronx.
A boy was injured when he fell into an unsealed construction hole at PS 113.
A roofing contractor allowed leaking rainwater to do extensive damage to classrooms, books, and computer equipment.
Contractors blocked a fire exit at one school, forcing students and staff to exit through a smoke-filled hallway.
School officials and neighbors charged the School Construction Authority with endangering their health by stirring up dust that then infiltrated classrooms and homes.
Unfortunately, the problem is not a new one. Last July, The New York Times detailed how students are put at risk by careless and inept contractors who are given second chances and, in some cases, sixth and seventh chances. In 1997, a student was killed by falling bricks because of contractor ineptitude; in March 1998, a construction worker was killed and two students injured when a brick wall collapsed.
"We're much better than we were, but we're still a far cry from where we need to be," city Schools Chancellor Harold Levy told Campanile.
In early 1999, New York Governor Pataki established a state commission to investigate possible mismanagement in the New York City school system. When the commission issued its first report in June this year, it charged the Board of Education with delaying the repair of conditions that were hazardous for both staff and students. According to the commission's report, the Board failed to conduct required safety inspections and repeatedly violated other requirements to include the public in the planning of school construction and repair.
Research & Commentary: Utah Fits All Scholarship Program Would Be Game-Changer for Beehive State Families
Research & Commentary: Universal ESA Would Be a Game-Changer for Virginia Families | {
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Sept. 15 — Dylan James Houser, 513 E. Beer Road, Milford, arrested for sexual misconduct with a minor. Bond: $26,000 surety and cash.
Sept. 15 — Mario M. Martinez, 34, 340 E. Levi Lee Road, Warsaw, arrested for operator never licensed. Bond: $500 cash.
Sept. 15 — Randy K. Skinner, 51, 109 Boys City Drive, Winona Lake, arrested for public intoxication. Bond: $600 cash.
Sept. 14 — Jermesha Lanae Baker, 23, 1201 CR 15 Lot 190, Elkhart, arrested for driving while suspended. Bond: $183.50.
Sept. 14 — Neil Clark Bryant, 34, 18370 Gyr Court, New Paris, arrested as a habitual traffic violator, possession of methamphetamine, and possession of legend drug injection devices. No bond listed.
Sept. 14 — Rahul Kumar Palta, 35, Carmel, arrested for resisting law enforcement with a vehicle, resisting law enforcement, refusal to identify and battery.
Sept. 13 — Zachary Dean Cowger, 22, Plymouth, arrested for battery against a public safety official engaged in duty. | {
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Fans Website
Your Daily Dose of Movies News
Upcoming Best Pakistani Top Movies |
Bollywood Hindi Cinema Film Industry |
Recently Released Movies in Pakistan |
Most Recent Hollywood Releases – For the Year 2020 |
Bollywood Movies That Have Released Just Yet |
Upcoming Best Pakistani Top Movies
August 27, 2019 January 2, 2020 http://fanwebsite.co.uk
Pakistani cinema industry has been on a break for so long. However, it made a comeback about a decade ago and coming up with more exciting drama stories and epic laugh punch comedies. Pakistani cinema covers all the genres be it social issues, war stories, army man ship, comedy, drama and thriller as well.Upcoming best Pakistani top movies are helping Pakistani cinema industry.
Pakistani film industry was initially based on Lahore and initially it spread from there being the largest film industry representing the whole nation. Thus, the names Lahore and Hollywood when combined, gave out the name Lollywood for the whole Pakistani cinema.
Pakistani cinema is based in the two biggest and the most metropolitan cities if Pakistan that are Karachi and Lahore. Both cities are home to one of the biggest cinema homes and film studios. The industry as the whole started declining back in late 70s till early years of 21st century. But it has started flourishing again with the efforts of the industry men.
History of Pakistani Cinema
The Pakistani film industry flourished explicitly back in the early years after the state's freedom. There are almost above 10000 movies in Urdu that have been released till day after 1948. Also, the numbers are similar when we talk about Pashto movies, Sindhi and also the Punjabi movies which is 6000, 2000 and 8000 movies respectively.
Producers of Driver of Pakistani Cinema
The major industry drivers are a few names of the producing studios that have played there major and much needed part in the revival of the Pakistani cinema industry. The names are:
ARY Films
GEO Films
Hum Films
Urdu 1 Pictures
Upcoming Best Pakistani Top Movies in Later Part of the Year 2020
The Pakistani audience and viewers are a tasteful bunch of individuals. They love entertainment and watched movies since very long. The generation X and generation Y individuals, if you consider within Pakistan, they have been watching Hollywood and Bollywood all their lives till early years of the 21st century until the Pakistani cinema industry made a solid comeback.
As per seeing the cinema stats within Pakistan, it was to be said with absolutely no doubt that Pakistan needed this revival of the film industry. From the ages ago when industry had big names like Waheed Murad, Nadeem Baig and Noor Jahan till now when we have Mahira Khan, Saba Qamar and Humayoun Saeed kind of legends. Pakistani cinema has indeed made an epic comeback.
Let us see which movies are in the filming phase in the Pakistani cinema and at what dates we all have to mark our calendars so we do not miss them by any chance:
1. Upcoming best Pakistani top movie Durj
Durj is a Pakistani thriller movie which is going to be released very soon in October, 2019. Most probably the exact date is going to be October 11th. The Urdu movie is directed by the super talented Shamoon Abbasi and is produced by none other than Sherry Shah under the banner of the studio i.e. Shaam Films Production. The initial release will be done in Canada.
Durj is going to bring a lot of thrill along with mystery plots and of course a lot of drama. It is another film being shot to highlight the social issues in Pakistan. There are security concerns to every individual within Pakistan that there are crimes happening in Pakistan on a large scale. Such crimes involve theft, rape and kidnapping on a large scale. The movie portrays the same storyline that a wife is finding her kidnapped husband.
The cast stars popular PTV actress Maira Khan costarring Shamoon Abbasi along with Nouman Javaid. Everything about the movie sounds interesting, I think we should give it a chance watching.
2. Kaaf Kangana
Directorship and the screenplay by the legendary Khalil Ur Rehman Qamar and distribution done by the ARY Films, the upcoming movie Kaaf Kangana is expected to be a big hit. The movie stars Sami Khan costarring Eshal Fayyaz and the beautiful Ayesha Omer.
Kaaf Kangana is expected to be a light romantic movie yet filled with a lot of drama as well. The main songs are also one of the hype for the movie. The singers are very popular and loved worldwide and they are: the electrifying Aima Baig, the soothing Shafqat Amanat Ali Khan and also the all-time Sufi singer Rahat Fateh Ali Khan.
The movie is expected to release on October 25th, 2019 so guys, do nothing but mark your calendars because the date is not that far.
3. The Evil Marriage
The Evil Marriage is written and directed by Rana Abrar and is going to be Pakistan's newest action and fantasy mix movie. The movie is expected to release in November in 2019 and was produced by WBJ Movies along with the Messenger2050.
The movie plot carries fantasy along with action as we discussed before. It starts with dramatic and mystery music with a bit of haunting flavor, this creates the audience interest on another level. The movie is the quest in between a girl and an Evil King. Movie was shot partially in Turkey, Malaysia and Pakistan and languages are going to be Urdu and Malay.
Lollywood, Movies lollywood upcoming movies 2020, pakistani movies list 2020
Bollywood Hindi Cinema Film Industry
Recently Released Movies in Pakistan
Most Recent Hollywood Releases – For the Year 2020
Bollywood Movies That Have Released Just Yet
Most Popular Netflix Movies of 2020
Must Watch Animated Movies of All Times
Most Horrifying and Thrilling Hollywood Movies
Space Travel Hollywood Movies of All Times
Exciting Upcoming Hollywood Movies | {
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Mar 13, 2014. I own a WD MyBook 4TB hard drive, which I've used on Windows for the past. I have the same problem that after inserting to mac my usb disk.
Feb 22, 2015 · Hello, i have a problem with my external hard drive, when i plug it in my laptop. i takes too long to acknowledge it and when i open a file it would hung, i tried to reformat my external hard. Ideally, you should have a 2TB or higher hard drive for recording. shows on any of your extenders.
After you have connected your external hard drive on you Mac, launch the "Disk Utility" application which can be found under "Applications". Once the application is open, you would be able to see a list of available drives on the left side of the window.
If you think having scads of open Chrome tabs clutters up your screen, just wait till you've got a dozen plugins running in tandem: That 15-inch laptop screen can fill up awfully fast. If you're using.
If your Toshiba external hard drive has been partitioned with the wrong file system, you will also encounter the "external hard drive not recognized" issue. For instance, you may have formatted the drive with the ext4 file system from Linux or the HFS Plus file system from a Mac.
My toshiba laptop cd drive wont open. It makes a sound like it is trying but it i guess is jammed. I tried the paper clip tric Forum; Laptop won't run Sims 3 without an external hard drive Forum.
According to the court, Doe voluntarily handed over the password for an Apple iPhone 5S, but he refused to provide the passwords to decrypt his Mac or the external hard drives. images or to actuall.
Dec 09, 2009 · Connect your external hard drive to your mac 2. Open Disk Utility (command+F and type 'disk utility') 3. Click the drive you want to format in the left hand pannel 4. Click the 'partition' tab 5. Select under Volume Scheme '1 partition' 6.
Yes, there are high chances that you will successfully be able to retrieve most data that has been deleted / lost from a corrupt external hard disk drive using a Macintosh, even if you have reformatted your portable hard drive or if its file system is damaged.
A common task that arises for the end-user is to find stored passwords on a computer in order to recover lost. is located under the "Applications" section on the Mac hard drive. Step 2 – Open the ".
More memory is also helpful for people that keep multiple windows open simultaneously. "You can determine how much memory is installed by right-clicking on 'My Computer' or. Move the large files to.
I spent about $100 to get hundreds of files off of more than a dozen disks, and another $25 on an external drive that. most of my files were old Microsoft Word documents, but there were also Final.
My 1TB Seagate external hard drive cannot be detected by my computer and the light is blinking, can you help me fix this problem? And I do need to get my data back. Most of my personal files and some important files were all stored in the drive, help please.
In 2004 I bought the first line of the G5 white iMacs and I upgraded a few years later to a Mac Pro tower with dual processors. In 2008 I bought a Macbook Pro and after that a 27-inch iMac i7 with an.
Prep your hard drive. First up, you'll need an external hard drive, preferably a USB 3 one, as they'll transfer your data faster. A USB 2 drive will do just fine, as will a Thunderbolt one.
Jan 24, 2011. External drives allow you to quickly moves large files between computers. Open disk Utility on your Mac. I thought I was going to have to return my 1TB hard drive but these instructions prevented that from happening.
My one gripe: You hit the Space bar to open. s on the Mac, too. (Well, at least it's on Macs with solid-state drives like MacBook laptops. APFS doesn't yet auto-convert traditional spinning hard dr.
My thesis holds that the global Bubble. in Brazil's presidential election Sunday, marking a hard pivot to the right that p.
These steps can also be applied to partitioning an external hard drive connected to your Mac computer. Just select the outside drive rather than the internal one and follow the steps above.
Dec 1, 2015. Use these steps to format external hard drives for both operating systems. This will allow you to use the hard drive on both a Mac and PC. Open Disk Utility. 4. One of my personal tricks is naming all drives after an actor.
Feb 6, 2018. What to do if an External Hard Drive is not recognized on Windows and Mac? The article. Now, see if it is present there in the My Computer window. If not. To mount a drive, open Disk Utility and look for the drive in the list.
In order to copy files to your laptop or PC's hard disk, select the ones you want and click the Extract button. Browse to a folder on your local hard disk (or a different external drive) and click.
However, if your Mac runs OS X 10.10 Yosemite, installing Java is a little trickier. You will first need to install the distribution from Apple's support site, and then install the version from Oracle.
The best external drives for Mac computers are undoubtably G-DRIVE ones. They're reliable. Go to Finder and open up your applications folder. I found that it was saving my Library backups to a folder called FCB on my internal hard drive.
Mar 20, 2012. Thread: my macbook doesn't read my external hard drive anymore. the restoring menu. click restore hard drive. open terminal and enter reset.
An external hard drive hooks up to your Mac via a cable or built-in connector that connects. If you select a drive in the Finder and press "Cmd-I" to open a Get Info window, you can. Ask Dave Taylor: My New External Mac Drive Is Read-Only.
It supports both 2.4 and 5 Ghz wireless clients simultaneously and is designed to serve as a network-attached storage device when connected to an external hard drive via USB. "1-4" on the Linksys r.
Feb 25, 2014 · My hard drive finally went kaput on my mac, and it is in the mac hospital getting a replacement. I knew this was going to happen soon, so earlier this year I purchased an external to put everything on.
Jan 04, 2012 · For whatever reason the Mac commonly struggles with USB hubs, I think because they are not powered. I get similar errors constantly when using USB hubs on Mac with external drives, but when plugged directly into Mac the hard drives work. Also make sure the external drive is not locked.
In addition, regularly back up your data onto a USB drive or an external hard drive. without any effort on your part. Mac users can also automate the process of finding and installing available upd.
If I were to be completely honest though, I think Samsung stole my idea. Just about a year ago, I ripped open a MyDigitalSSD OTG External SSD. compatible with both PC and Mac Systems and Samsung's.
ExFat drives, in my experience, behave strangely under Mac OS X after they are. malfunctions (ie, your computer hard crashed while the drive was inserted). Open terminal and enter the following: defaults write com.apple.
Also I'd disconnect all drives, speakers, external. changes on Mac computers that have this feature. The computer doesn't respond to the power button when pressed. A portable Mac doesn't appear to.
Mar 31, 2015. When you connect an external hard drive to your Mac, it appears on. Click the "Finder" icon on the Dock to open the Finder application.
Windows or Mac. next to Open Internet Explorer Tiles on the Desktop. You should now go straight into Desktop IE instead of having to use Metro IE. 5 – USB drives freeze To preserve power Windows su.
Visit our Easy Guide to learn more about this completely free platform, test drive. to my GitHub project "TensorFlow Serving + gRPC + Java + Kafka Streams." Managing data at scale doesn't have to b.
To make a Mac act as an external hard disk, you can put it in Target Disk Mode and connect it to another Mac with a FireWire or Thunderbolt cable, as follows:. Note: Target Disk Mode is available on most recent Macs; however, computers that do not have FireWire or Thunderbolt ports are excluded. Shut down the computer you want to use as an external hard disk (i.e., the target computer).
Why my Android device heats? what can I do to prevent my device. But the important thing to remember when your device running Android overheats, is to check the external climatic conditions before.
The new My Passport design picks up on many of the same elements seen in the My Passport for Mac and the My Passport Studio. we were able to split the case open without damaging it, exposing custom.
Neither console supports USB 3.1 Gen 2, but even over USB 3.0's 5-Gbps constraints, the Exo should run rings around external hard drives. Speaking of cracking things open, the Savage Exo didn't yield. | {
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Q4 is well under way and you know what that means – it's time for Sales Kickoff planning!
In a former life, I was in charge of creating content for our company's annual Sales Kickoff. The three-day event included somewhere in the neighborhood of 40 presentations on success stories, best practices, and product training. We also killed a few trees to produce thick packets of collateral so our sales team could reference what they learned.
But no matter how early we started planning, getting all the content complete always came down to the wire. Sound familiar? Anyone? Bueller?
If you are tasked with creating content for your Sales Kickoff, here are five ways to get the most out of this year's event by incorporating online video presentations into your Kickoff agenda.
#1. Make it on-demand. It's a good idea to create on-demand video presentations that attendees can view at their convenience before your meeting. Since online videos can be accessed on-the-go via most mobile devices, they are a great way for reps to refresh their knowledge anytime, anywhere. Brainshark makes it easy to quickly create video presentations using materials as simple as PowerPoint. For more details on how online video can improve your Sales Kickoff meetings, check out the video below.
#2 Involve others. Nothing is created in a vacuum. To take some of the content creation burden off of your plate, try tapping your top sales people for content on how they got that big deal to go through. You could also get your service team to talk about what part of your solution is resonating with clients and what your customers are requesting. Hearing directly from the people who have success with your client base is more likely to have a powerful and memorable effect on your audience.
#3 Give homework. Instead of cramming your event with back-to-back presentations, give your team some required on-demand video viewing beforehand. This will free up valuable meeting time to focus on subject matter expert (SME) presentations, Q&As and the all-important team-building exercises.
#4 Measure knowledge. During a packed schedule of live presentations, it's only natural that your audience's minds will tend to wander. But you still need to make sure your team is learning their stuff! Create an on-demand presentation that summarizes the day's important lessons and include a quiz. By having your team view and take the quiz at the end of the day, you can help ensure they'll remember the right information.
#5 Be competitive. Salespeople by nature tend to be a competitive bunch. You can hold them accountable by making their quiz responses public or giving prizes for the highest scores. Remember, there's nothing like a little friendly competition to get people to pay attention and drive home your messages.
By including on-demand presentations into your Sales Kickoff event, you can open up the agenda to more interactive sessions and even shorten your meeting to save money. You'll also be able to lock in more content ahead of time, give your team a convenient way to absorb information, and ensure they learn the material. | {
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I wasn't going to succumb to the turkey crisps this year because the ones I have tried in previous years have either been too salty, or just take like roast chicken crisps. So what swung it this year? Well the M&S Turkey Feast Hand Cooked Crisps were saying all the right things.
Yes these roast turkey and all the trimmings proclaim to deliver potato crisps flavoured with turkey and cranberry, and carrot and parsnip crisps. I love veggie crisps they are scrummy so I am a happy bunny that M&S have included these too.
I can't for the life of me remember how much these were, I am going to say in the region of £2.00 and were a reasonably sized bag. They are also gluten free which is good to see. Opening up the Santa coloured red bag and the familiar meaty salty smell was evident but this time with a touch of sweetness.
Each crisp was identifiable and blended well together. The turkey stuffing crisps were pretty meaty and more on the side of turkey and less on the chicken flavour that usually comes through. I couldn't detect the cranberry at all, it would have nice to have seen how this would have tasted but I can't say I am overly sad that I can't. On the other hand I love love love the parsnip and carrot crisps, they are sweet, crunchy and delicious and they are a welcome change to just having the turkey crisps.
These M&S Turkey Feast Hand Cooked Crisps are certainly one of the better Turkey crisps I have tried but be prepared for the taste to linger for quite some time. I do wish they had included sprouts, yes this maybe an unpopular opinion but I love them and would love to see them added to the veggie crisp family, at least for Christmas.
This looks like such a nice and unique packet of crisps. Is it worthy enough for the nibbles table (despite everyone being in food comas!) at Christmas!? | {
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Home » Sports » 2018 Ballon d'Or to air live on StarTimes
2018 Ballon d'Or to air live on StarTimes
On November 23, 2018 1:00 amIn Sportsby Emmanuel Okogba
Africa's leading digital TV operator StarTimes has concluded plans to broadcast the 2018 Ballon d'Or ceremony on 3rd December when the winner of the annual football award is to be unveiled.
Ballon d'Or is considered by many as the highest honor for football players. And the past 10 years has seen only two players win the Ballon d'Or – Lionel Messi and Christiano Ronaldo. But this year's Ballon d'Or may see the emergence of a new winner, with reports suggesting that Luka Modric is likely to win the top gong, following his Best FIFA Men's Player award
The live broadcast of the 2018 Ballon d'Or Ceremony is to start at 20:00 GMT on 3rd December,
"This year' Ballon d'Or Ceremony definitely attracts wide attention of football fans and we may see a historic moment that a new winner of the award in 10 years," said Shi Maochu, StarTimes Sports Director.
"Live broadcast of the 2018 Ballon d'Or shows our commitment to fans that StarTimes always search for best football contents. We brought all 64 HD World Cup matches to African fans this summer, and we continuously offer top international football matches to audience, such as Bundesliga, Ligue 1 and Coppa Italia."
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Awolowo coup of January 1966103
Supreme court judgement meant to cause trouble in Imo State, Igbo land — IGA11 | {
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Q: Scala - Overloading method in implicit class I currently have an issue where I am trying to overload a method contained within quill using an implicit class, normally this is possible with the simple case, i.e. if you have something like
class Test {
def rawr(string: String): String = string
}
You can easily overload this definition of rawr using a different type like so
implicit final class RawrExt(val t: Test) {
def rawr(int: Int): Int = int
}
And this compiles as expected, i.e.
val t = new Test
t.rawr(5)
Even if Test has more complex type parameters, this still works, i.e.
class Test[T <: Number] {
def rawr(string: String): String = string
}
implicit final class RawrExt[N <: Number](val t: Test[N]) {
def rawr(int: Int): Int = int
}
val t = new Test[BigDecimal]
t.rawr(5)
Where I am getting a problem is when I am trying to implement the exact same overloading for the quill-monix-jdbc's transaction. When using monix-quill-jdbc, you have a transaction method that has the following signature
def transaction[A](f: Task[A]): Task[A]
The issue is that we are using TaskResult in our application logic which is Monad Transformer of Either and Task using cats, i.e.
type TaskResult[T] = EitherT[Task, GeneralError, T]
What I am trying to do is to provide an override for transaction which takes TaskResult rather than Task, defining this in an implicit class is quite straight forward
object TaskResultSupport {
implicit final class TaskResultCtxSupport[Dialect <: SqlIdiom, Naming <: NamingStrategy](
val value: MonixJdbcContext[Dialect, Naming]) {
def transaction[A](f: TaskResult[A]): TaskResult[A] =
EitherT(value.transaction(f.value))
}
}
And then when we try to use it we get a compilation error, it can't seem to pick up the implicit class.
val ctx: PostgresMonixJdbcContext[SnakeCase] =
new PostgresMonixJdbcContext(SnakeCase, "database")
val taskResult: TaskResult[Unit] = TaskResult(())
ctx.transaction(taskResult) // This doesn't compile
I tried all various permutations of defining the implicit class, i.e. as an example
implicit final class TaskResultCtxSupport(val value: MonixJdbcContext[_, _]) extends AnyVal
And none seem to work. Here is the compilation error
type mismatch;
found : Playground.this.Implicits.TaskResult[Unit]
(which expands to) cats.data.EitherT[monix.eval.Task,Playground.this.GeneralError,Unit]
required: monix.eval.Task[?]
A scastie demonstrating the problem can be found here https://scastie.scala-lang.org/pqAn8fUPTbmBqToCVIXDXA. Thanks to Martjin Hoekstra, there is a further minimized example here https://scastie.scala-lang.org/4YrhP0HSRzu7F9numrqAGQ. Scala contributors thread can be found here https://contributors.scala-lang.org/t/scala-compiler-unable-to-overload-methods-with-type-parameters/3761
A: Turns out this was a bug with the current Scala compiler, a solution is slated for 2.13. See https://github.com/scala/scala/pull/7396 for more details.
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Extremely loud noises can cause permanent damage to the tiny hair cells inside the cochlea. Even moderately loud noise over a period of time can be damaging. But just how loud is loud? Studies show that prolonged exposure to sounds at or above 90dB can damage hearing. Protect your hearing and wear earplugs when exposed to loud noise.
To view a chart that graphically illustrates some common noises and their respective dB levels click here.
Protect your hearing whenever your surroundings are so loud you must raise your voice to be heard. It doesn't matter what the source of the loud sounds are – music (radios, live music, and headphones), machinery, conversation (bar or restaurant). If it's too loud for you to hear yourself, the sound is potentially damaging to your hearing. If you can't avoid the situation, wear ear plugs.
Mention any ringing or buzzing in your ears or in your head to your doctor.
Ears are self-cleaning. Normal bathing is all most people have to do to keep their ears clean and healthy.
If ear wax does need to be "cleaned out" only a qualified professional should do so.
Any sudden change in hearing should be reported to your doctor. | {
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- Painting should cause massive weight loss. According to my estimates, I should be a size 2 by now.
- The color I chose? The entire idea to paint this very day? Total impulse. I purchased three cans of paint, color... sight unseen. I planned to get a swatch, see it in different lights, just generally scrutinize the crap out of it. No. The color I wanted to look at was discontinued. I'd only seen pictures of it online. I was feeling sassy, so I just bought it.
- Since it was a 'discontinued' color, I got to choose what brand of paint the color was mixed into. The guy asked "Glidden or Behr?" [blank stare] It was then he gave me a third option: The cheapest thing possible. It was like this paint guy in the dirty apron was daring me. Not one to turn down a dare, I went with the cheapest thing possible. The brand? Speed Wall. White can, stark black lettering. Twelve bucks a gallon. (what could possibly go wrong? It's all just paint... right?!) Everything about it screams generic. As in Cheerios are to Toasted Oat Cereal as Paint is to Speed Wall.
- Can I have paint and paint accessories in my house for more than an hour without painting? No. I had every intent of saving it for the next day. As soon as I got home and dropped the cans on the table, the paint started calling. I threw some up on a couple walls at 9pm. After everyone had gone to bed, I was rolling on paint in really poor lighting- (as not to wake the sleeping children) the next morning proved this to be a really bad idea.
- I freaked out that night because the color looked REALLY BAD with my carpet, cabinetry, and tile. It looked like baby barf. Baby barf on my wall. But being the cheapness that I am, decided- too bad. I was painting the majority of my house this color. Luckily, it dries into a more beigey creaminess and less of a greenish barf.
- The cheapest paint possible? It's not like the Glidden or the Behr. It's like painting your house with water. I'm undecided on whether this is good or bad. It seems to get into the little crevices pretty well. It's kind of annoying though. The paint barely hangs onto the brush. Cheap paint... hmmmm. I think time will tell.
- I really don't understand the paint categories. Flat, Satin, Semi-gloss? I read that Flat is good for most areas like bedrooms and living rooms, etc. Satin is the same, but is a bit more scrub-able. Semi-gloss they reserve for kitchens and baths... because you can really clean it.
My ENTIRE house is semi-gloss. Who doesn't want the ability to really clean a wall? When does NOT being able to clean something become a selling-feature? Especially with small children, with their sticky jam-hands. I can see a trail of dirt and stickiness at their height that goes right along up the stairs. The lady at the home builder's design studio called it "washable flat." I wish to drive to her house at 2 am, ring her doorbell until she wakes up, then give her the stink eye.
- I am going to have to climb onto a 10 ft. tall ladder and paint a 2 story wall in the stairwell... with a roller on a long stick. Does anything about that sound a little sketchy to you, too? I've been avoiding this task. But it feels like a gigantic elephant in the room- no matter how much progress I make on the rest of the house, the stairwell will still be there... waiting for me.
- My helper, Trent (also known as my little brother) is apparently afraid of heights. He twitched a little bit just looking off the balcony at the two towering walls I was hoping to paint. I'm pretty sure I'm going to be the one on the ladder. I'm also fairly certain that as long as someone is there to call an ambulance when/if I fall, I'll only break an arm, or a leg, or something. Unlike Trent, I'm somewhat confident that it won't kill me.
- I don't believe in taping, masking, or dropcloths. They're for sissies. Plus, if a can of paint just happened to fall onto my crap builder-grade carpet... I would just have to replace it with hardwood.... and that would be a real tragedy.
- I'm playing it fast and loose with the paint. Except for my shutters. Those will be sealed up like Fort Knox. My shutters reside in a very special place in my heart. If they are even slightly tarnished with paint, someone is going to feel the wrath.
Then, last night, I heard the girls fighting over who got to let the puppies outside (yes, big problems. Totally worthy of bopping a sister on the head... totally) I threatened them that I would have to stop painting and come down there. Bunny's response was a loud, "No! You need to paint a my house! You no stop paint! You paint that wall!" Ok, my tiny taskmasters, I'll get right on that. They are kind of peeved that I haven't completed the whole job yet. I mean really, I've had the whole duration of Toy Stories 1 and 2... and a Tinker Bell.
- Painting is always something that seems totally do-able... until you're doing it.
- This has turned into quite the long list of thoughts. Kudos to you for hanging on this long. You guys are the strong, the brave, the resilient, true readers of my crazy babble. Gold stars all around!
I fear I will never be able to finish, or reach the top of the ceiling, and my house will look like this forever.
Can you even tell that it's a different color? It's the yellowy-tone. When dry, it is a very subtle beige. But it is soooo high up. I'm doing everything but climbing the ladder.
Big self-painters here at our house. Why just last weekend I decided that the hubby and I were going to repaint the boys bedrooms downstairs, one of his favorite pastimes. I always tell him that I will just do it myself, but the guilt always gets to him and he ends up doing most of the work. It's really his fault that he is so stinkin tall and handy:) I wanna see pics of your paint job! Way to go girl!!!
I am impressed! Both sisters are fans of painting--not me! But, they got to me. Marne' insisted it would "make my fireplace show up better." 3 trips to WAL-MART and I have a caramel, diarrhea-ish wall. fun.
Go you! Yet again, accomplishing the impossible.
Where do you find the time for these projects??
My first house was half-painted for the entire two years we lived there. You better believe I will hire a painter from now on! | {
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Liberals call for a dementia friendly Canberra
Shadow Minister for Seniors Nicole Lawder will move a motion in the Legislative Assembly today, calling on the Labor-Greens Government to investigate and implement changes to the Age-Friendly City Plan 2020-2024, to improve accessibility for those living with dementia in Canberra.
Ms Lawder said introducing and normalising dementia friendly design practises doesn't have to be difficult or come at a significant financial cost.
"It can be as simple as selecting carpet that doesn't have patterns or installing additional lighting," said Ms Lawder.
"Dementia is a terrible, debilitating disease which unfortunately is a lot more common than most people realise.
"Sadly, there is still a stigma around dementia, people don't like talking about it. The reality is most people are going to encounter it either themselves or through a loved one.
"Until there is a cure for dementia, there is always more we can do to make life easier for those living with the disease and supporting their carers.
"Canberra is a city that should be inclusive to all, especially for those most vulnerable in our community.
"If this Labor-Greens Government means what it says about diversity and inclusivity, they must support this motion," Ms Lawder concluded.
According to Dementia Australia, there are an estimated 472,000 Australians living with dementia in 2021.It is the second leading cause of death of Australians.
Nicole Lawder Shadow Minister for City Services; Shadow Minister for Seniors; Shadow Minister for Women; Shadow Minister for Arts; Liberal Member for Brindabella | {
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Jeannette Koger is Vice President, Advisory Services and Credentialing at the American Institute of CPAs. Jeannette joined the AICPA in 2006 and is responsible for providing strategic and tactical direction for the vision and management of AICPA's advisory services.
In this role she is responsible for leading the domestic and international growth and success of four distinct disciplines and related credentials including forensics, valuation, personal financial planning and information management and technology assurance. Her team also helps members demonstrate their expertise in these areas through the ABV, CEIV, CFF, CITP and PFS credential programs.
During her time at the Institute, Jeannette has been integral in building the highly technical Advisory Services and Credentialing team to lead the advocacy efforts and development of education and resources that enable members practicing in these disciplines to be successful. The depth offered in these areas has grown exponentially under Jeannette's leadership.
Jeannette has been instrumental in moving the ABV, CEIV, CFF, CITP and PFS credentials to a global model. She has worked to develop and refine AICPA's business valuation standards to ensure they are at the forefront of global standards. She played a key role in establishing standard setting authority on behalf of the Personal Financial Planning Executive Committee, and led the effort to redefine the CITP body of knowledge.
A licensed CPA in North Carolina, Jeannette earned her BA in Accounting from North Carolina State University and holds an MBA from Cornell University's Johnson Graduate School of Management. | {
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Located approximately 104-miles east of Austin and 170-miles south of the Dallas/Fort Worth Metroplex, Bryan and neighboring College Station real estate offers residents access to a wealth of amenities ranging from world-class sporting events in Houston to shopping in San Antonio, and award-winning festivals in Austin. But you don't have to go far from home to experience a wealth of incredible amenities, attractions and activities. In fact, Bryan is within a three-hour drive from more than 80 percent of the Texas population. Despite the availability of nearby metropolitan areas, many choose to spend their time right here in Bryan.
Spend a Saturday sipping wine and Texas' most awarded premium winery, the Messina Hof Winery. Take the kids to the Gibbons Creek Reservoir for a hike or to enjoy swimming and camping in the summer. Love the relaxation of the golf course? Check out Pebble Creek Country Club, Pecan Lakes Golf Club, Miramont, and the Traditions Golf and Country Club to name just a few. Spend an evening at a Texas A&M sporting event with the family. However, one of the main attractions in the area is Lake Bryan. Home to miles of hiking trails, campsites, a swimming area, fishing areas, and a pavilion for events, residents of all ages enjoy this Bryan amenity. When you choose to secure any of the Bryan TX rentals available to you, all this and more can be steps from your front door.
Another main draw to Bryan TX rentals, as well as nearby College Station rentals, is the excellent school districts that service these areas. The Bryan Independent School District serves the communities of Bryan, Kurten and Wixon Valley as well as the rural areas of northern Brazos County and is consistently rated "Academically Acceptable" by the Texas Education Agency. Below is a list of the schools that service this area.
Bonham, Bowen, Mary Branch, Carver, Crockett, Fannin, Henderson, Houston, Johnson, Anson Jones, E.A. Kemp, Ben Milam, Harvey Mitchell, Navarro, Robert C. Neal, and Sul Ross Elementary Schools.
Similar to the homes for sale available in Bryan, the rental market is filled with single-family homes and condominiums ideal for residents of all tastes and budgets. Whether you're looking for a single-family home to rent while your family searches for a new home, a urban condominium close to the area's finest amenities, or a quiet retreat close to Lake Bryan, Realtor Myke Leatham and her team of real estate experts can help you find the rental property you desire. They will listen to your needs and expectations, and with budget and location in mind, will find you the rental that best suits you and your family.
When you're ready to learn more about the options available to you, Myke invites you to start your search by using the state-of-the-art search tools within this website. Should you see a property of interest or would like more information, she is always just a phone call away. Don't see what you're looking for? Call her today to discuss your specific needs and let her find the Bryan TX rentals that best suit them. She looks forward to hearing from you and to helping you make the most out of your housing experience here in Bryan.
With more than 25 years of experience and as a Realtor who consistently is ranked among the Top 1% of Realtors nationwide, there is no better real estate professional to assist you with your Bryan rental needs. When you're ready to start your search, do not hesitate to contact Myke and her team. Connect today to get started! | {
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Home » Jazz Musicians » Junior Wells
Junior Wells
Junior Wells was considered the direct musical descendant of modern blues harmonica legends John Lee "Sonny Boy" Williamson, "Sonny Boy" Williamson II (Rice Miller) and Little Walter Jacobs. An exponent of blues, funk and soul music, Wells developed a style incorporating all of those genres, and was a consummate stage performer who could back it all up.
Born Amos Blakemore in 1934, Junior was raised on a farm in rural West Memphis and Marion, Arkansas. He became intensely interested in the music flowing from the fertile blues culture of Memphis and learned harmonica from his cousin Little Junior Parker. After his parents separated, the wild and rebellious Junior moved with his mother to Chicago in 1946. There he discovered that music would be the most important thing in his life.
His teenage years were spent playing hooky from school, scrambling change from odd jobs and practicing his harmonica. His interest in the local blues musicians found the underage Junior sneaking into various clubs, vying to "sit-in" with bands. His earliest such escapade was in 1948 sneaking into the C & T Lounge where Tampa Red and Johnny Jones let the young harpist show his skills. A now famous incident was when Junior convinced his sister and her then-boyfriend, a Chicago policeman, to escort him to Sam's Ebony Lounge where the celebrated Muddy Waters band (with Little Walter Jacobs and Jimmy Rogers) were playing. "I went up to Muddy and told him I played harp...Muddy said he'd let me try. Little Walter said, "That little shrimp." They stood me on a coke box to reach the mike and I made $45 in tips....Walter asked me if I ever played the sax before!"
When Little Water left the Muddy Waters band to tour with his new found fame, Junior was called to replace him. Junior stayed on with Waters until 1952. In 1953, Wells was inducted into the army, but he didn't let this get in the way of his music career - some of his first recording sessions done for the States label were done while he was AWOL. Upon his return from the army in 1955, Willie Dixon introduced Junior to Mel London, who recorded classic Wells' songs "Messin' With The Kid," "Come On In This House," and "Little By Little" for the Chief and Profile labels.
The 1960's found Junior working frequently with Chicago blues guitarist Buddy Guy. The duo gigged the clubs and became a regular fixture in the city. In 1965, Delmark Records released Junior's first album, the classic "Hoodoo Man Blues," with Buddy Guy on guitar. The celebrated duo of Wells and Guy toured the world with the Rolling Stones in 1970, and went into the Atlantic studios in '72 to record "Buddy Guy & Jr. Wells Play the Blues." This album garnered them recognition, and the pair continued a long association of recording and playing through the late 1980's.
In 1974, Guy and Wells played the Montreaux Jazz Festival backed by Rolling Stones' bassist Bill Wyman, Terry Taylor, Dallas Taylor and Chicago blues pianist Pinetop Perkins. The explosive performance was captured on tape and released on Blind Pig Records in 1982. "Drinkin' TNT 'N' Smokin' Dynamite," finds Guy and Wells in extraordinary form. Both artists went on to become internationally acclaimed blues legends and this stellar recording remains one of Blind Pig's most popular releases.
Wells was reunited with Delmark in the late '70's where he released "On Tap," ('75) and "Blues Hit Big Town." ('77) He did one album for Alligator "Alone and Acoustic," in 1991. Junior signed with Telarc in '93 and proceeded to put out records for them peaking with "Come On In This House," in '96, his most unadulterated blues record since his highly acclaimed "Hoodoo Man Blues," of more than 30 years vintage. The idea was to team Wells with some of the era's top younger traditional blues guitarists - - Corey Harris, Alvin Youngblood Hart, Sonny Landreth, Bob Margolin, and John Mooney; to have those musicians, in various combinations, accompany Wells on a variety of slide guitars; and to concentrate on vintage Chicago and Delta blues. The result is a demonstration of the timeless appeal of classic blues done well. Wells' vocals are deep and manly; his harp playing is high- pitched, and in synch with the true feeling of the session. A well received and acknowledged recording, which was nominated for a Grammy.
To say that Wells is the genuine article is to understate the matter. He hailed from the hard knock school of blues harp masters. His is the sound of the Chicago streets, the Maxwell Street market, the juke joints, the after-hours sessions, the road-weary gigs and the hostile territory into which any artist must go to prove his worth. The beauty of it is that after all those years, in the end Junior Wells didn't have anything at all to prove.
Junior Wells passed away in 1998. Show less
Junior Wells harmonica
Live In Boston 1966 by Nic Jones
Hoodoo Man Blues by Nic Jones
Junior Wells, with Buddy Guy - Hoodoo Man Blues (1965, Reissue)
Junior Wells and the Aces - Live in Boston 1966 (Delmark, 2010)
Junior Wells/Buddy Guy - Southside Blues Jam (1970)
Hoodoo Man Blues
Delmark Records
Live In Boston 1966
Live at Theresa's...
Vietnam-Blues /...
guitar, electric
Sonny Boy Williamson II
Earl Hooker
guitar, slide
Jimmy Rogers
Billy Boy Arnold
Instrument: Harmonica
Died: 1998
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Contact Junior Wells | {
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Erna Dorothea Luise Sack, z domu Weber (ur. 6 lutego 1898 w Spandau, zm. 2 marca 1972 w Moguncji) – niemiecka śpiewaczka, sopran.
Życiorys
Studiowała w Pradze oraz w Berlinie u Oscara Daniela. Początkowo występowała jako kontralt, później jako sopran koloraturowy. Zadebiutowała w 1925 roku w Städtische Oper w Berlinie. W następnych latach występowała w Bielefeldzie (1930–1932), Wiesbaden (1932–1934) i Wrocławiu (1934–1935). Od 1935 do 1941 roku związana była z Operą w Dreźnie, gdzie w 1935 roku wystąpiła jako Isotta w prapremierze Die schweigsame Frau Richarda Straussa. W 1936 roku debiutowała w Covent Garden Theatre w Londynie w roli Zerbinetty w Ariadnie na Naksos Straussa pod batutą kompozytora. Śpiewała gościnnie w Mediolanie, Paryżu, Wiedniu i Salzburgu. W 1947 roku wyjechała do Stanów Zjednoczonych. W latach 1947–1952 odbyła światowe tournée. W 1956 roku wróciła do Niemiec, w 1966 roku osiadła w Wiesbaden.
Obdarzona była unikatowym głosem, sięgającym do c4, o naturalnej lekkości koloratury, osiągając dźwięk nieosiągalny dla większości sopranów. Specjalizowała się w lżejszym repertuarze: ariach operetkowych, wokalnych opracowaniach walców Straussa i Lehára oraz pieśniach. Grete von Zieritz skomponowała z myślą o niej Vogellieder. Wystąpiła w filmach Blumen aus Nizza Augusto Geniny (1936) i Nanon Herberta Maischa (1938).
Przypisy
Niemieckie soprany
Niemieckie śpiewaczki operowe
Urodzeni w 1898
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Questa voce raccoglie le informazioni riguardanti il Wisła Płock nelle competizioni ufficiali della stagione 2020-2021.
Stagione
Rosa
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Pocket Editing
All your writing and editing needs in the palm of your hand
Pocket Blog
Letters from Lily
In 2021 I was the editor for C.E. Corrales and Michael Jaymes' novel Letters from Lily.
What once gave me nightmares now gave me lustful dreams. I thought maybe it was just my curiosity at first, but now I was beginning to think there was a deeper desire. Something inside of me didn't just want to know more about the picture. Something told me I wanted to partake…
With only a few weeks left of senior year, Zach can't wait to be out of high school. He's never been part of a clique, had a girlfriend, or felt accepted. With no direction, Zach sought the perfect opportunity to make himself feel noticed. But he never imagined that chance to come in the form of an unexpected letter. What Zach didn't know is that each mysterious letter depicted the image of an impending murder. With every new drawing, Zach discovers dark secrets within himself. How long can he hide from the truth before he's caught red-handed?
Find it on Amazon Here: Letters from Lily
The Executioners Book One
From 2018 to 2020 I worked with Vanora Belmont on the first two novels in The Executioners series. Below is the first novel in the series:
As an Executioner, it's Anora's job to hunt down dangerous supernaturals that threaten the human race. She loves her job, despite the constant threats and hatred towards her kind. Feeding the disquiet between the races, a powerful warlock emerges, seeking to fuel the humans' rage against the witches. Torn between living the life she wants and the life expected of her, one thing is certain: dark times lie ahead, and Anora's biggest secret is about to be revealed.
Find it on Amazon Here: The Executioners: Book 1
Making "New Rich" Books Work for You
In 2018 and 2019 I was the main editor for Kevin Price's book Making "New Rich" Books Work for You.
So you have read Four Hour Work Week, The E Myth Revisited, and Rich Dad Poor Dad, but have little to show for it but a good read. Kevin Price, host of the nationally syndicated Price of Business radio show, explains why this happens and what one can do about it in his compelling book, Making New Rich Books Work for You. It is based entirely on his own struggles.
Find it on Amazon Here: Making "New Rich" Books Work for You
In 2018 I was the editor for M.A. Lorie's second novel Reminiscence.
A powerful, ancient magic, passed down through generations, lands in the hands of a young demon hunter.
The aftermath of Richelle's devastating betrayal still lingers throughout Bryson Agencies, affecting Brent the most. Though he claims to be handling it, he's not, leaving the rest of the group no choice but to take drastic measures. Meanwhile, bits and pieces of the past begin trickling into the present, causing Stephen, Brent, and Marc to question everything they were ever told. As tensions flare and secrets are slowly unearthed, Stephen loses faith in Denny. Will their pasts come back to haunt them? Will the discovery of new information regarding a powerful amulet lead them down a more dangerous path? What will become of the Power of Three? Can they keep it safe?
Find it on Amazon Here: Reminiscence
Pocket Editing, Create a website or blog at WordPress.com | {
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- Girls; Conduct of life; Juvenile literature.
- Role models; Juvenile literature.
Contributor Bio(s): Julie Merberg is the author of MY FAVORITE SHOES, TURN THE KEY, and TURN THE KEY AROUND TOWN and the mother of 4 super-hero loving boys. Illustrations are classic DC character art. | {
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|
FILM /
Film Features /
Who Cares if Films are Historically Inaccurate? /
Who Cares if Films are Historically Inaccurate?
It's just a movie, right?
Meg Hanson
Films "based on a true story" tend to blur the line between fiction and reality as thoroughly as Trump's Twitter account.
But history is not a social construct that can be upended as long as there are witnesses to hold us accountable. From biopics to period dramas, films recounting true events call for closer scrutiny than just taking their stories at face value. Should we expect historical accuracy? Not in all cases. Sometimes embellishments are justified if they produce a better movie. Not to mention, some details frankly aren't important. The fact that 300 depicts fit Spartan soldiers in loincloths rather than body armor, or Braveheart's battle scenes make 13th century Scottish soldiers look like tactical buffoons, doesn't skew our perception of the world.
And despite our culture's love of skepticism, historical accuracy seems to matter less and less the better a film is received. We can overlook fumbled facts if the film is seen as a great cinematic achievement. Many laud how A Beautiful Mind depicts schizophrenia, despite it being largely inaccurate about John Nash's life. Depending on the subject, filmmakers and viewers feel they owe different forms of deference to the material. After all, we're still cool with Pocahontas as a children's movie, for which we set a low bar. Aside from the erasure of genocide and indigenous slavery, the real-life Pocahontas was 12 years old when she met Disney's OG colonizer John Rolfe, who thankfully wasn't into it (at least until she was 19 and a slave).
Many of this year's Oscar-nominated films were based on true events but spun off the tracks of history. Sometimes, those creative liberties were justified. In other cases, they were pretty fucked up.
1. BlacKkKlansman (2018)
Spike Lee's film opens with the title card, "Dis joint is based on some fo' real, fo' real shit." Indeed, the movie's adapted from real Colorado cop Ron Stallworth's 2014 memoir. The gist of the movie is true: between 1978 and 1979, Stallworth infiltrated his local chapter of the Ku Klux Klan by striking up a friendship with the Klan's Grand Wizard, David Duke.
The film's creative liberties primarily involve invented altercations between Stallworth and the Klan members and a significant change of identity for his fellow cop. In the film, Stallworth's partner in the ruse, played by Adam Driver, is Jewish, resulting in immediate suspicion from the Klan, heightened stakes for the characters, and an action-packed climax. In reality, his partner wasn't Jewish, and the entire investigation occurred without Klan members casting any doubt on the two cops. But that's a boring movie.
Blackkklansman isn't entirely accurateVanity Fair
So does it matter that the real infiltration was easier–and less violent–than it was portrayed? In this case, no. Not only does Stallworth approve of the adaptation, but the white supremacist he duped feels insulted, so everybody else wins. "The film even changes the facts in Ron Stallworth's book, Black Klansman, to demonize me," Duke, the KKK Grand Wizard, said. "They brag about how this guy conned me. Somebody calls me on the phone, I tend to trust people, I talk to people, I've got nothing to hide." Stallworth agrees, "Spike made him look kind of stupid, but he was stupid in how this whole thing transpired 40 years ago."
The film's creative liberties are justified for the sake of enhancing drama, because they don't alter its broader narrative about anti-black racism in the U.S, which is ultimately the point of Spike Lee's film.
2. Green Book (2018)
While BlacKkKlansman isn't a perfect movie, many of us related to Spike Lee when he tried to storm out of the Oscars when Green Book won Best Picture. Unlike Lee's film, the Academy's pick is co-written by the son of its real-life subject, Tony "Lip" Vallelonga. The simple premise is following along Tony's job as the driver for piano virtuoso Dr. Donald Shirley on his tour through the Jim Crow South in 1962. The movie would have us believe that Tony became enlightened to change his racist views under Shirley's guidance, and the two formed a lifelong friendship.
Neither Vallelonga and Shirley lived to see the film, but Shirley's brother condemned it as "a symphony of lies." In fact, Vallelonga's son co-wrote the script based on his father's notes–with no input from Shirley's surviving family members. It's true that the men bonded while Vallelonga drove Shirley through a contemptuous South just one year after the Freedom Riders were arrested and attacked on a similar route. The musician reflected in a 2010 documentary about the tour, "We never had an employer-employee relationship, you don't have time for that foolishness. My life is in this man's hands, do you understand me? So we got to be friendly with one another."
The real Shirley with Mahershala AliHistory vs. Hollywood
However, Shirley's family members dispute the film's loose interpretation of "friendly" as the kind of transformative lifelong friendship depicted in the film. While Shirley's siblings and nephew take issue with the cold and distant portrayal of the musician, the most offensive inaccuracy is how the film stages the men's friendship as another White Savior narrative. Vallelonga protects Shirley from racism in the Deep South; in return, Shirley shares his exotic wisdom. Mahershala Ali, who portrayed Shirley, even called the family members after the film's release to apologize. Shirley's nephew recalls it was a "very, very respectful phone call...What he said was, 'I did the best I could with the material I had. I was not aware that there were close relatives with whom I could have consulted to add some nuance to the character.'"
In this case, straying from the source material just to create a Feel Good Movie About Racism is a cheap, lazy move that romanticizes racism as being curable on a nine-day road trip. As a result, not only does the man who wrote Shallow Hal have an Oscar, but Hollywood bastardized what was probably a genuine, unconventional connection between two people who experienced racism from opposing perspectives.
3. Bohemian Rhapsody (2018)
Would Freddie Mercury be pleased with Bohemian Rhapsody? We obviously can't know. Does the film inform Mercury's cultural legacy? With Rami Malek named the Academy's Best Actor of 2019 for his high-profile portrayal of the man, absolutely. With that being said, the Queen bio-pic sacrifices true-to-life details for what is essentially a two-hour-long music video. From the band's early development to Mercury launching a solo career and the group "reuniting" to perform in the 1985 Live Aid broadcast, nothing depicted in the film is accurate. But for general viewers who aren't die-hard Queen fans, that's pretty dismissible.
The most controversial–and justified–grievance about Bohemian Rhapsody is how Freddie Mercury's bisexuality and HIV diagnosis are mishandled. While the film implies that Mercury had romantic relationships with both men and women, it manages to both erase the icon's bisexuality and negatively depict homosexuality. From his lifelong bond with the "love of his life," Mary Austin, to his final relationship with Jim Hutton, the film suggests Mercury was a capricious and nervous man prone to vainglory and promiscuity. Similarly, the film changes the timeline of his HIV diagnosis in order to dramatize the Live Aid performance with the implication that the band was inspired to reunite (in fact, they weren't separated) to support Mercury in his battle.
Rami Malek wins best actor.Hollywood Reporter
In reality, the performance was years before he was diagnosed, and altering the timeline conflates Mercury's legacy with his disease. Indiewire critiqued, "It's inexplicably perverse that the movie retcons Mercury's HIV diagnosis as the band's motivation for Live Aid." Writer Kevin Fallon calls the whole film "an insult to Freddie Mercury" as "a cruel and manipulative version of tragedy porn that is inaccurate and perpetuates the trope of AIDS as punishment for gay promiscuity."
While we can't expect biopics to flawlessly capture the personality and legacy of its subject, the point of the genre is to contextualize individuals in history and modern culture. In doing so, it's a given that films sensationalize events, personalities are exaggerated, and reality is reduced to a tagline. But questioning historical accuracy is important if for no other reason than to hold filmmakers accountable for manipulating the truth. Who's being served by re-writing history? What messages are being manufactured? Ultimately, blanket dismissal of those questions can spiral into a strange and lazy relationship with media, like Trump mistaking a movie for current events or someone who solely relies on Twitter for the news. Spike Lee puts it simply, "You have to do the research. If you don't know about something, then you ask the right people who do."
Meg Hanson is a Brooklyn-based writer, teacher and jaywalker. Find Meg at her website and on Twitter @megsoyung.
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historical accurate films | {
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A scene from the 2013 Horse Lake Trail Run in the Wenatchee Foothills.
WENATCHEE — RunWenatchee has some really cool news: We will be holding this spring the first official trail run series along the east slopes of the Cascades in Washington state.
The Wenatchee Valley Trail Run Series, presented by Volyn Law of Wenatchee, will combine two existing events — the May 10 Horse Lake Trail Runs in the Wenatchee Foothills and the June 8 Red Devil Challenge Trail Runs in the Devil's Gulch area of the Wenatchee National Forest near Cashmere — with a new race, the June 22 Bavarian Battle Trail Runs at the Leavenworth Ski Hill.
The trail series will include prize money as well.
Each of these runs will take place on single-track, well-maintained trails, set amid a crush of wildflowers and views of the North Cascades.
The Red Devil Challenge Trail Runs are set in the Wenatchee National Forest near Cashmere.
"With the Leavenworth event, we have a true trail run series now, and one that stretches from one end of the valley to the other," said Steve Maher, a partner in RunWenatchee. "The communities of Wenatchee, Cashmere and Leavenworth will each be featured as will their local trail systems."
According to Matt Kearny, sports tourism coordinator with the Wenatchee Valley Chamber of Commerce, the estimated economic impact from the trail run series will be in the $95,000 to $100,000 range. That figure include funds being raised for the trail series' three beneficiaries — the Chelan-Douglas Land Trust, Chelan County Mountain Rescue and the Leavenworth Winter Sports Club.
"Trail running is one of the fastest growing segments of running, with long distance trail running (half-marathons or greater) up 200 percent in the last five years," said Joel Rhyner, race director of the series. "The Wenatchee Valley is perfectly positioned to offer world-class trail running right out our back door."
As part of the series, RunWenatchee will be offering prize money to the winners (male and female) of the overall series in both short-course and long-course divisions. For details and rules: https://www.runwenatchee.com/wenatchee-valley-trail-run-series/
"Having the ability to offer prize money has been a goal of ours, and we are fortunate to have the support of our presenting sponsor, Volyn Law, to allow this to happen," Rhyner said.
The Horse Lake Trail Runs, which benefit the Chelan-Douglas Land Trust, include half-marathon and 5-mile distances. The Red Devil Trail Runs, held in the Wenatchee National Forest south of Cashmere and benefitting Chelan County Mountain Rescue, include 10K and 25K distances and a kids race. And the Bavarian Battle event, with proceeds going to the Leavenworth Winter Sports Club, will feature 10-mile and 8K runs, plus a kids race.
The Bavarian Battle Trail Runs also are being held in conjunction with the June 21 Bavarian Battle Adventure Race at the same site. For more on the adventure race — which includes a festive beer garden, music and food — please visit: http://www.skileavenworth.com/events/BavarianBattle.
"The Leavenworth Winter Sports Club is excited to be teaming up with RunWenatchee to bring the community a couple of challenging and fun races on June 21 and 22," said Corey McKenna, LWSC marketing director. "These two races are going to challenge athletes' skills and endurance, and all in the same weekend."
In addition to Volyn Law, sponsors include Project Groundwork, Arlberg Sports, Cashmere Valley Bank, Liberty Orchards (Orchard Bars), Crunch-Pak, Milepost 111 Brewery, and Great Harvest Bread Co. of Wenatchee.
— RunWenatchee.com
Visit Wenatchee announced as sponsor of RunWenatchee's trail running events
Written on Mar 3rd, 2018 by Steve, Category News, Trail Running
River Run 2014 results
Written on Sep 20th, 2014 by Steve, Category Events, Race Results, Training | {
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\section{Introduction}
Despite observational advances in characterising exoplanets and the environments in which they form (protoplanetary discs), a coherent picture that explains the origin and diversity of planets from their disky forebears remains elusive. We know planets must sculpt the discs in which they form, and indeed we see structures in observed protoplanetary discs; however, a lack of understanding means that using these observed structures to learn about the details planet formation is challenging.
There is a handful of disc-systems which show IR colours and SEDs that are inconsistent with primordial discs: discs that are optically thick from small to large radii \citep[e.g.][]{Strom1989,Skrutskie1990}. Instead, these objects show inner regions that are heavily depleted in dust, while returning to primordial levels in the outer regions \citep[e.g.][]{Calvet2005,Espaillat2014,Owen2016}. Given these discs are partially cleared (in at least the dust) they have been termed ``transition'' discs.
It is now known that transition discs do not represent a homogeneous class \citep[e.g.][]{OC12}. While many transition discs are believed to be protoplanetary discs caught in the act of clearing through photoevaporation \citep{Cieza2008,Merin2010,Owen2011}, a significant subset do not match any of the characteristics that would be associated with a protoplanetary disc in the throes of destruction \citep[e.g.][]{Kim2009,Espaillat2010,OC12}. { Approximately half} of transition discs { surveyed by \citet{OC12} had} large accretion rates ($\dot{M}\gtrsim10^{-9}$ M$_\odot$~yr$^{-1}$), large cleared dust cavities (out to $\gtrsim 10$~AU) and they { were} often the brightest of all class II discs at mm wavelengths \citep{Andrews2011,OC12,Ansdell2016}; for this reason they have been termed ``mm-bright transition discs" \citep{Owen2016}.
The majority of mechanisms invoked to create a transition disc signature do so by removing dust from the inner regions, and preventing its resupply, by trapping dust outside some radius in a pressure enabled dust trap. Indeed this is true for the two most commonly invoked mechanisms: photoevaporation \citep[e.g.][]{Clarke2001,Alexander2007,Owen2011,Gorti2015} and gap formation by giant planets \citep[e.g.][]{Calvet2005,Rice2006,Zhu2011,Zhu2012,Owen2014}.
Several of the mm-bright transition discs have been imaged at high resolution using {\it ALMA}, and in these high resolution images they show strong axisymmetric {\it and} non-axisymmetric emission features \citep[e.g.][]{Casassus2013,vanderMarel2013,Perez2014,vanderMarel2015,Andrews2016,Canovas2016} and see \citet{Casassus2016} for a recent review. These features have been linked to signs of planet formation, although as yet there is no clear understanding of how to link these observations to theory. A common interpretation of the non-axisymmetric structures is that they caused by large-scale vortices \citep[e.g.][]{vanderMarel2013,Ataiee2013,LyraLin2013}. Since these vortices represent local pressure maxima that orbit the star with roughly the local Keplerian velocity they can efficiently trap dust particles \citep[e.g.][]{Meheut2012,LyraLin2013,Zhu2014}. The strong dust density contrast that can result from dust particle trapping in vortices can lead to strong azimuthal surface brightness differences. The Rossby Wave Instability \citep[RWI][]{Lovelace1999,Li2000} provides a mechanism to generate vortices in astrophysical discs that contain radial structure. Sharp radial features give rise to an extremum in potential vorticity that leads to vortex formation. Non-linear hydrodynamic simulations \citep[e.g.][]{Li2001} show that several small scale vortices grow from the linear instability before they begin to grow and merge resulting in one large scale vortex, which can trap particles \citep[e.g.][]{Lyra2009,Meheut2012,Zhu2014}.
Transition discs are believed to contain a cavity edge in the gas, and such drops in gas surface density have recently been observed in CO emission \citep{vanderMarel2015,vanderMarel2016}\footnote{ Note: CO is likely to be optically thick, and at this stage it is still difficult to directly transform CO structures into gas structures.} . Such an axisymmetric gas structure is necessary to explain many of the observed features of transition discs, however, it remains to be seen whether the observed density drops are steep enough to trigger the RWI. While massive planets {(of order Jupiter mass and higher)} inserted into discs in simulations are known to produce deep and sharp cavities, sharp enough to trigger the RWI, it is unclear whether this is likely to occur in reality. This is because massive planets are inserted into disc simulations instantaneously (or grown over several orbits), necessarily producing a transient phase with a very sharp cavity which is RWI unstable.
In a realistic scenario, however, a planet accretes and grows on a time-scale comparable to the evolution of the protoplanetary disc itself. Viscosity present in the disc and, in fact, vortices created by any planet gap initially, can relax the gas to a much smoother distribution, which would be {\it stable} to the RWI over the long-term. This raises the intriguing question: if a transition disc cavity is stable to the RWI, or only unstable for a short period of time, why do transition discs, that are observable on time-scales $\gtrsim 10^4$ orbits, display non-axisymmetric structures generated by RWI vortices? This question is perhaps the biggest weakness of the RWI mechanism in explaining the observed transition disc structures \citep{Hammer2016}.
{ The RWI can also be triggered in protoplanetary discs at the edge of the dead-zone \citep[e.g.][]{Lyra2009}, where the change in viscosity leads to a sharp change in the surface density \citep[e.g.][]{Gammie1996}. Recent hydrodynamic simulations have shown that large-scale vortices can also be produced this way \citep[e.g.][]{Regaly2012,Flock2015,Lyra2015,Ruge2016} through the RWI. { Recent work \citep{Ruge2016,Pinilla2016} has shown that the dead-zone model can produce rings and gaps in scattered-light and mm images, although it remains to be seen if the model can explain the large drops in dust-opacity in the inner disc sufficient to reproduce the SEDs of transition discs.} Finally, vortices can also be formed through baroclinic instabilities \citep[e.g.][]{Klahr2003,Lesur2010,Raettig2015}.}
By trapping dust at some radius, while it continues to drift in from larger radii, transition discs will have significant increases in the dust-to-gas ratio in the dust trap, from the standard ISM value of 0.01, to values that can approach unity \citep[e.g.][]{Pinilla2012}. Therefore, it has been suggested that these transition disc dust traps are likely to sites of increased planetesimal and planet formation. Indeed \citet{Lyra2008}, demonstrated that it is possible to get direct collapse to form planetary embryos in RWI generated vortices.
One interesting advance in the theory of planet formation is the concept of pebble accretion \citep[e.g.][]{Ormel2010,Johansen2010,Lambrechts2012}. Dust particles that have gas-drag induced stopping times comparable to their orbital times can be rapidly accreted by planetary embryos. This is because gas pressure gradients induced by the planetary embryo's presence cause dust particles to be accreted if they approach within the proto-planet's Hill sphere, decreasing the growth time to $\sim 10^{4}$~years --- significantly faster than the standard planetesimal accretion times. Since pebble accretion is very sensitive to dust particle size --- it is only efficient for dust particles that are close to optimally coupled to the gas --- it can only work where there are large numbers of dust particles close to this size. The dust traps in transition discs {\it inevitably} provide a reservoir of these pebbles, as those dust particles that are most efficiently accreted are also those most efficiently trapped.
Here we explore the possibility of low-mass planet formation in the pressure traps of transition discs, and argue that it is likely to naturally arise, while perhaps also explaining a variety of observational signatures that are now commonly associated with transition discs. We are agnostic about the mechanism that creates the transition disc itself, but argue that if low-mass planet formation begins in transition discs as we suggest it is: i) likely to be rapid and ii) if the disc is sufficiently massive, it is able to generate vortices that can lead to non-axisymmetric structures similar to those recently observed.
We structure our work as follows: in Section~\ref{sec:mechanism} we discuss the physical picture and motivate the basic principles of our new mechanism. In Section~\ref{sec:sims} we present numerical simulations to look at the non-linear long term evolution. We discuss our results in Section~\ref{sec:results} and summarise in Section~\ref{sec:summary}.
\section{Physical Mechanism}
\label{sec:mechanism}
The characteristic feature of transition discs is the significant drop in opacity at small radii relative to a primordial disc with a return to primordial values at larger radii. This opacity drop is interpreted as a significant removal of dust (and hence opacity) close-in, while returning to standard values further out in the disc. The changeover from the optically-thin dust in the inner regions to the optically-thick outer regions is known to be sharp \citep[e.g.][]{Andrews2011}. Thus the standard explanation for such a dust distribution is that there is a ``dust-trap'', where a pressure maximum can overcome the gas accretion flow and trap dust particles in the vicinity of the pressure maximum due to gas-drag. This is in contrast to a gradual change in the dust properties that might result from, for example, dust evolution \citep[e.g.][]{Dullemond2005,Birnstiel2012}.
By generating an axisymmetric maximum in the gas surface density, which in turn creates a pressure maximum, dust particles will drift towards this pressure maximum where the dust particles feel no gas drag. The time-scale on which dust particles drift towards, and are trapped within the pressure trap, is determined by the particles' Stokes number, or the non-dimensional stopping time ($\tau_s$). Dust particles with $\tau_s$ { greater than the viscous $\alpha$ can become trapped \citep[e.g.][]{Birnstiel2013}. However, it is those particles with $\tau_s$ near unity $\sim10^{-1}-10$ that are {\it rapidly} and {\it efficiently}} trapped in a pressure maximum on a time-scale $\lesssim100$ orbits. However particles with Stokes numbers far from unity are not strongly trapped, with diffusion and advection dominating for particles with very small Stokes numbers, meaning the dust closely follows the gas distribution. The size of a dust particle $s$ can be related to the Stokes number (in the Epstein drag limit - relevant for small dust particles in the outer disc) as:
\begin{equation}
s\approx2\,{\rm mm}\, \tau_s\left(\frac{\Sigma_g}{1~{\rm g~cm}^{-2}}\right)\left(\frac{\rho_d}{3~{\rm g}~{\rm cm}^{-3}}\right)^{-1}
\end{equation}
where $\Sigma_g$ is the local gas surface density and $\rho_d$ is the dust density. Thus for typical parameters found in most transition discs, we find it is the mm to cm sized grains that are trapped in the pressure traps. This back of the envelope argument agrees with early mm observations of transition discs \citep[e.g.][]{Andrews2011}, which showed that the mm sized grain population was confined to narrow rings indicative of pressure trapping \citep{Pinilla2012}.
Dust trapping can increase the surface density of particles with stopping times close to unity to very high values, of the order of 10~g~cm$^{-2}$ \citep[e.g.][]{Pinilla2012} in the most massive transition discs. Thus, the dust-to-gas ratio in the trap is significantly enhanced above the standard ISM value of 0.01. Such environments are ripe for the formation and growth of planetesimals and planetary embryos, either through coagulation or direct collapse through mechanisms such as the streaming instability \citep[e.g.][]{Youdin2005,Johansen2007}. The streaming instability is likely to be important in these dust traps since it is typically strongly triggered in environments with large dust-to-gas ratios \citep{Johansen2009}. We suggest here that should a planetary embryo reach high enough mass such that it can undergoing pebble accretion, this planetary embryo will grow incredibly rapidly, as we now demonstrate.
\subsection{Pebble Accretion in a Dust Trap}
Pebble accretion is a mechanism by which a planetary embryo can rapidly grow to significant mass \citep[e.g.][]{Lambrechts2012}. For dust particles that are coupled to the gas on time-scales comparable to the orbital time (i.e. $\tau_s\sim 1$), the embryo can accrete particles from impact parameters significantly larger than its physical radius or effective radius due to gravitational focussing. In fact, gas-drag enables the embryo to accrete particles from a radius out to its Hill sphere ($R_H=a(M_p/3M_*)^{1/3}$), with all particles with $\tau_s$ in the range 0.1-1, being accreted if they approach the embryo's Hill sphere \citep{Ormel2010,Lambrechts2012}.
The rate at which embryos accrete through pebble accretion depends on whether it occurs in a largely planar or spherical manner \citep{Morbidelli2015,Bitsch2015}. In the planar case, the embryo accretes from the full height of the disc, whereas in the spherical case it just accretes from a fraction of the disc's height, and is therefore less efficient. The transition from spherical to planar accretion occurs approximately when the Hill sphere is larger than the scale height of the pebbles \citep{Morbidelli2015}. Or:
\begin{equation}
M_p \gtrsim 0.03~{\rm M}_\oplus \left(\frac{M_*}{1~{\rm M}_\odot}\right)\left(\frac{H/R}{0.1}\right)^3\left(\frac{\alpha}{10^{-3}}\right)^{3/2}
\end{equation}
As we shall see later, we are mainly concerned with accretion onto embryos with masses $\gtrsim 1$~M$_\oplus$ here, thus for simplicity, we assume pebble accretion will always take place in a 2D fashion with an accretion rate approximately given by:
\begin{equation}
\dot{M}_{\rm peb}\approx 2\Omega R_H^2 \Sigma_{\rm peb}
\end{equation}
As $R_H\propto M_p^{1/3}$, this means that at late times the planet mass will grow as $t^3$, provided it does not locally reduce the pebble surface density. With a typical growth time-scale of:
\begin{eqnarray}
t_{\rm acc}&\approx& 3\times 10^{3}\,\,{\rm yrs}\,\left(\frac{\Sigma_p}{3\,{\rm g~cm}^{-2}}\right)^{-1}\left(\frac{M_p}{5\,{\rm M}_\oplus}\right)^{1/3}\nonumber \\ &&\times \left(\frac{a}{20~{\rm AU}}\right)^{-1/2}\left(\frac{M_*}{1~{\rm M}_\odot}\right)^{1/6}
\end{eqnarray}
Such a time-scale is clearly very rapid, it could deplete the local reservoir of pebbles significantly, by turning them all into a low-mass planet and, as we shall argue in the next section, such a rapid accretion rate will have a significant thermal impact on the surrounding disc.
Firstly, however, we will explore the time to deplete the dust trap using a simple model. Assuming that the dust trap is in a balance between turbulent diffusion and gas-drag and contains a mass in pebbles $M_{\rm peb}$, then the surface density of pebbles in the trap is given by $\Sigma_p=M_{\rm peb}/(2\pi R H_p)$, where $H_p$ is the radial width of the dust trap. Without considering the feedback on the gas $H_p$ could, in principle, be very thin compared to the disc's vertical scale height ($H$). Such a small $H_p$ would result in a dust-to-gas ratio well above unity, meaning dust drag becomes much less effective, and as such the assumptions in deriving a thin $H_p$ break-down. Thus, we expect $H_p$ is likely to be fixed to the gas radial scale length when the dust-to-gas ratio approaches unity. As the dust-traps in transition discs are ordinarily expected to have dust-to-gas ratios well above the ISM value, for simplicity we set $H_p\sim H$ and leave a more detailed calculation to further work. Therefore, both the pebble reservoir and forming planet in a transition disc dust trap will evolve according to the following coupled equations:
\begin{eqnarray}
\frac{{\rm d}M_p}{{\rm d}t}&=&2\Omega a^2 \left(\frac{M_p}{3M_*}\right)^{2/3}\Sigma_p\label{eqn:planet_evolve}\\
\frac{{\rm d}\Sigma_p}{{\rm d}t}&=&\left(\frac{H}{R}\right)^{-1}\frac{\dot{M_p}}{2\pi a^2}\label{eqn:pebble_evolve}
\end{eqnarray}
Equation~\ref{eqn:pebble_evolve} implies that at late times the pebble surface density drops exponentially, with a characteristic time-scale comparable to $t_{\rm acc}$ for a planet mass of roughly $M_{\rm peb}$. Therefore, we expect the planet mass to grow as $t^3$ until its mass becomes comparable to the mass originally in the pebble reservoir, at which point the reservoir is rapidly depleted in an exponential fashion.
We are agnostic about the initial embryo mass since the strong temporal scaling of the growth makes our calculations largely insensitive to this value particularly at late times when the $t^3$ growth effectively erases the initial condition depleting all of the available mass into the planet. Depending on the pebble surface density and separation, however, the absolute time-scale over which this occurs varies. Nonetheless, this is always a rapid evolution occurring in under $\sim 10^5$ years for a wide range of plausible surface densities and separations.
{ Pure coagulation could give rise to the initial embryo; bypassing the fragmentation barrier (which resides at sizes of order cm's) by the sweep-up mechanism (e.g.} Windmark 2012ab, Dr{\c a}{\.z}kowska et al. 2013{), where larger particles can break through the fragmentation barrier by ``sweeping-up'' smaller ones. We also highlight two other possible avenues for the formation of the initial embryos that could be present in transition disc dust traps}. First, direct gravitational collapse itself could proceed; while in a slightly different scenario (inside a RWI vortex) the dust surface densities are not too dissimilar \citet{Lyra2008} showed one could directly collapse to embryo sizes of order $10^{-2}$~M$_\oplus$ and above. Second, as we have hinted to above the dust traps are also prime sites for planetesimal and embryo formation through the streaming instability. \citet{Johansen2015} and \citet{Simon2016} showed through numerical simulations that one can grow embryos up to masses $\sim 10^{-4}$ M$_\oplus$. { The streaming stability and coaugulation can also work together to promote embryo formation \citep{Drakowska2014}.} Certainly either of these scenarios or perhaps others could generate embryos large enough in mass to begin pebble accretion. Further, since the growth time drops as one approaches higher masses, accretion proceeds in a state that the first ``lucky'' embryo to start accreting will always be considerably more massive than all others. In the following calculations, we will assume the starting embryo masses are in the range $10^{-4}$-$10^{-3}$ M$_\oplus$, in accord with the values from the embryo formation models described above. The gestation of these embryos into planets in our scenario is demonstrated in Figure~\ref{fig:evolve_res}, where we numerically evaluate Equations~\ref{eqn:planet_evolve} \& \ref{eqn:pebble_evolve} for parameters expected in transition discs.
\begin{figure*}
\centering
\includegraphics[width=\textwidth]{Evolution_2}
\caption{The evolution of the planet mass (top row) and pebble surface density (bottom row) as a function of time. The solid lines show a starting embryo mass of $10^{-4}$~M$_\oplus$ and the dashed lines show a starting embryo mass of $10^{-3}$~M$_\oplus$. The line colour indicates the initial pebble surface density of 0.1 (red), 1.0 (blue) \& 10.0 (black) g~cm$^{-2}$. Each column show the calculations performed at separations of 10, 20 \& 50 AU.}\label{fig:evolve_res}
\end{figure*} Therefore, in this picture the embryos grow and deplete the local pebbles on a rapid time-scale that can reach planetary mass objects very quickly ($\sim 10^5$~years). As seen in the Figure, this model naturally and rapidly produces super-Earth and Neptune-mass planets in these dust traps at large ($ \gtrsim 10$AU) radius from the host star. This formation channel could be one of the dominant modes of low-mass planet formation at large separations.
\subsection{Thermal Consequences}\label{sec:thermal}
Apart from providing the ideal site for the rapid formation of low-mass planets, and thereby exploiting the well-known virtues of pebble accretion, perhaps the most interesting and new consequence of this scenario is the thermal feedback from the rapid accretion.
The energy resulting from the rapid accretion of pebbles will be liberated as radiation at the planet's surface, necessarily resulting in a large accretion luminosity. What we will argue is that if the low-mass planet can disrupt the thermal structure of the disc outside its Hill sphere (inside which the planet's gravity dominants) this can give rise to a source of vorticity strong enough to grow large scale vortices. In the outer regions of a protoplanetary disc we suspect it be optically thin to IR radiation \citep[e.g.][]{Chiang1997}. Thus, the temperature structure of the optically thin disc at a background temperature ($T_d$) surrounding a luminosity source is given by:
\begin{equation}
T=T_d\left[1+\left(\frac{R_T}{r}\right)^2\right]^{1/4}\label{eqn:temp_profile}
\end{equation}
where $R_T$ is the radius at which the black-body temperature due to just the irradiation from the planet is equal to the background disc temperature, and is given by:
\begin{equation}
R_T=\left(\frac{L}{16\pi\sigma T_d^4}\right)^{1/2}
\end{equation}
Thus assuming an accretion luminosity of $L=GM_p\dot{M}_{\rm peb}/R_p$ we can find the ratio of $R_T$ to the Hill radius as:
\begin{eqnarray}
\frac{R_T}{R_H}&=&\left(\frac{2GM_p\Omega\Sigma_{\rm peb}}{16\pi\sigma T_d^4R_p}\right)^{1/2}\\
&\approx & 5 \left(\frac{M_p}{5~{\rm M}_\oplus}\right)^{1/2}\left(\frac{R_p}{1.5~{\rm R}_\oplus}\right)^{-1/2}\left(\frac{\Omega}{3\times10^{-9}~{\rm s}^{-1}}\right)^{1/2}\nonumber \\&&\times \left(\frac{T_d}{30~{\rm K}}\right)^{-2}\left(\frac{\Sigma_{\rm peb}}{3~{\rm g~cm}^{-2}}\right)^{1/2}
\end{eqnarray}
Since the pressure trap can enhance $\Sigma_{\rm peb}$ to high values \citep[in some cases $\gtrsim 10$g~cm$^{-2}$, e.g.][]{Pinilla2012} the accreting planet will disrupt the temperature of the disc in regions significantly outside the Hill sphere of the planet. In fact in the above case, at the edge of the Hill sphere the temperature will be roughly three times the local disc temperature. Another relevant scale is $R_T/H$, which, for the above case, are roughly comparable.
\begin{eqnarray}
\frac{R_T}{H}&=&\left[\frac{2GM_p^{4/3}\Omega \Sigma_{\rm peb}}{16(3M_*)^{1/3} \pi\sigma T_d^4R_p(H/R)^2}\right]^{1/2}\\
&\approx&1.0 \left(\frac{H/R}{0.1}\right)^{-1}\left(\frac{M_p}{5~{\rm M}_\oplus}\right)^{2/3}\left(\frac{M_*}{1~{\rm M}_\odot}\right)^{-1/6}\nonumber\\&\times&\left(\frac{R_p}{1.5~{\rm R}_\oplus}\right)^{-1/2}\left(\frac{\Omega}{3\times10^{-9}~{\rm s}^{-1}}\right)^{1/2}\nonumber\\&\times&\left(\frac{T_d}{30~{\rm K}}\right)^{-2}\left(\frac{\Sigma_{\rm peb}}{3~{\rm g~cm}^{-2}}\right)^{1/2}
\end{eqnarray}
For distances from the planet $\gtrsim H$, the background Keplerian velocity, due to the shear, is supersonic with respect to the planet. If the temperature can disrupt the disc out to this radius it could cause wave breaking and significantly adjust the disc structure. However, given the weak scaling of $R_T/H$ on the parameters of the problem this is only likely to occur in the most extreme cases.
\subsection{Radiative and advective time-scales}
Since the gas in the neighbourhood of the planet is orbiting at slightly different velocities to the planet due to the background shear, there is the obvious question of whether there is time for the gas parcels to be heated to the equilibrium temperature given by Equation~\ref{eqn:temp_profile}. One requires the advective time-scale to be shorter than the radiative timescale to be close to local radiative equilibrium. To first order the relative azimuthal velocity of a gas parcel with respect to the planet is given by:
\begin{equation}
v_{\rm rel}=\frac{3}{2}\Omega x_p
\end{equation}
where $x_p=|R-a|$ is the distance from the planet along the radial co-ordinate connecting star and planet. So the advective time $t_{\rm adv}\approx x_p/ v_{\rm rel}$ is independent of distance from the planet. Whereas the radiative time-scale is approximately:
\begin{equation}
t_{\rm rad}\approx\frac{4\pi r^2 k_bT_d}{\mu L \kappa}
\end{equation}
The ratio of radiative to advective time-scales is thus:
\begin{eqnarray}
\frac{t_{\rm rad}}{t_{\rm adv}}&=&\frac{3k_b\Omega}{2\mu \sigma T_d^3 \kappa} \left(\frac{r}{R_T}\right)^2\\
&\approx& 0.16 \left(\frac{r}{R_T}\right)^2 \left(\frac{\Omega}{3\times10^{-9}~{\rm s}^{-1}}\right)\\
&&\times\left(\frac{T_d}{30~{\rm K}}\right)^{-3}\left(\frac{\kappa}{0.1~{\rm cm^2~g^{-1}}}\right)^{-1}
\end{eqnarray}
Therefore, for nominal parameters we expect the surrounding gas to be in radiative equilibrium in the entire region which is actively heated by the planet, unless the opacity is low, but since we are in a dust trap with a high dust-to-gas ratio we would expect the opacity to be high, rather than low. { For example, for a MRN particle distribution ($n(a)\propto a^{-3.5}$, as expected for a collisional cascade) that has a maximum particle size of 1~mm, \citet{dalessio2001} find an opacity of $\sim 0.1$~g~cm$^{-2}$ at FIR and mm wavelengths when the dust-to-gas ratio is $\sim 100$}. We thus conclude that the gas will indeed reach the equilibrium temperature given by Equation~\ref{eqn:temp_profile} and the disc will have a ``hot-spot" associated with the rapid planet formation.
\subsection{Implications of hot-spot}
The fact the flow is no longer barotropic means no steady-state solution exists and, as we shall see in the numerical calculations, the temperature disturbance launches waves. However, we can gain a great deal of insight by considering how a temperature bump effects the flow structure along a closed streamline in the disc\footnote{Note the following argument is {\it not} strictly a correct solution of the fluid equations in a rotating disc - we will use numerical simulations for that later - but is merely an illustrative calculation to gain insight.}. The vertically integrated steady-state fluid equations along a streamline with path length, ${\rm d}\ell$, are given by:
\begin{eqnarray}
\frac{\partial}{\partial \ell}\left(\Sigma u \right)&=&0\label{eqn:cont2d}\\
u\frac{\partial u}{\partial \ell}+\frac{1}{\Sigma}\frac{\partial \mathcal{P}}{\partial \ell}&=&0\label{eqn:euler2d}
\end{eqnarray}
where $\mathcal{P}$ is the vertically integrated 2D pressure. Adopting a locally isothermal equation of state, such that the 2D pressure is given by $\mathcal{P}=\Sigma c_s^2$, where $c_s$ is the isothermal sound speed, we can combine Equations~\ref{eqn:cont2d} \& \ref{eqn:euler2d} to obtain a standard ``nozzle'' expression:
\begin{equation}
\left(\frac{u^2}{c_s^2}-1\right)\frac{\partial \log u}{\partial \ell}=-\frac{\partial \log c_s^2}{\partial \ell} \label{eqn:euler_mom}
\end{equation}
As discussed above the relative velocity of gas parcels with respect to the planet does not become transonic until a distance of $\sim H$; therefore, the majority of the heated gas will have a significantly sub-sonic velocity with respect to the planet and temperature bump. This is crucial, as for the flow to adjust to the new temperature profile and reach dynamical equilibrium we require the flow time to be shorter than the sound crossing time, a condition obviously satisfied in the sub-sonic limit.
Working in the sub-sonic limit with $r\lesssim H$, Equation~\ref{eqn:euler_mom} implies that $\partial \log u/\partial \ell \approx \partial \log c_s^2/\partial \ell$. Since Equation~\ref{eqn:cont2d} relates the gradient of the surface density to the velocity, along with the equation of state we find:
\begin{eqnarray}
\frac{\partial \log \Sigma}{\partial \ell}&\approx&-\frac{\partial \log c_s^2}{\partial \ell}\\
\frac{\partial \log \mathcal{P}}{\partial \ell}&=&\frac{\partial \log \Sigma}{\partial \ell}+\frac{\partial \log c_s^2}{\partial \ell}\approx 0
\end{eqnarray}
Namely, the 2D pressure remains approximately constant as the gas parcel passes through the temperature bump, while the surface density drops, inversely tracking the temperature profile. This is an important result as it means the flow in the vicinity of the planet has become {\it baroclinic}. The implications of this fact become clear if we inspect the inviscid vortencity equation for a 2D disc:
\begin{equation}
\frac{D}{Dt}\left(\frac{\bm{\omega}}{\Sigma}\right)=\frac{\bm{\nabla}\Sigma\times\bm{\nabla} \mathcal{P}}{\Sigma^3}
\end{equation}
where $\bm{\omega}$ is the vorticity, which is only non-zero in the $\bm{\hat{z}}$ direction in our 2D disc. Therefore, if the flow was completely barotropic then vortencity ($\bm{\omega}/\Sigma$) would be conserved. However, along a gas parcel orbit, in the vicinity of the planet, $\bm{\nabla}\Sigma\times\bm{\nabla}\mathcal{P}\ne\bm{0}$ and the hot spot can source vortencity, allowing vortex structures to grow.
Therefore, in this work we present a mechanism for the generation and maintenance of vortices in astrophysical accretion discs. We discuss the picture specifically within the case of transition discs as this is likely to be observationally relevant; however, we note it should occur more generally, whenever $R_T\gtrsim R_H$ for a forming planet, or for cases where there is a luminosity point source in an astrophysical accretion disc.\footnote{Our framework describes the general phenomenon of hot-spot induced anti-cyclones in astrophysical accretion discs. Here, the vortex is induced by planet-formation in a transition disc but in other systems, we anticipate a different heat source and different disc type.}
\section{Numerical Calculations}
\label{sec:sims}
In order to investigate the long term evolution of a disc with a planet induced temperature bump and to see if we can grow large scale vortices we must perform numerical simulations. We work in 2D and use the {\sc fargo} code \citep{Masset2000} and adopt a locally isothermal equation of state ($\mathcal{P}=\Sigma c_s^2$), where we have modified the code to include a 2D locally isothermal temperature distribution. We consider the evolution of a low-mass planet that induces a temperature bump within a transition disc like gas structure. { To construct the simplest possible model, in order to isolate and investigate the physics of our new process, we neglect planet migration, dust-gas coupling, dust evolution, and cooling, all of which should be addressed in future work.}
\subsection{Setup}
As the starting point for our background transition disc gas structure we take a standard protoplanetary disc model with a surface density and passively heated temperature profile:
\begin{eqnarray}
\Sigma_b&=&\Sigma_1\left(\frac{R}{R_1}\right)^{-1}\\
T_b&=&T_1\left(\frac{R}{R_1}\right)^{-1/2}
\end{eqnarray}
where the normalising temperature at $R_1$ is chosen such that $H/R=0.1$ at $R_1$. In order to insert a gas cavity into the disc to mimic the possible gas structure that is likely present in a transition disc, we modify our background surface density structure ($\Sigma_b$) to the form:
\begin{equation}
\Sigma=\frac{\Sigma_b}{2}\left[1+\erf\left(\frac{R-R_0}{\sqrt{2}\sigma}\right)+\epsilon\right]
\end{equation}
where $R_0$ is a parameter that can be used to set the location of the peak of the surface density distribution, which we take to occur at $R_1$, such that $R_0\approx0.75 R_1$, and $\epsilon$ is a small number chosen to prevent the surface density from becoming zero at small radius { in the initial surface density distribution}, which we set to $10^{-3}$. The parameter $\sigma$ controls the smoothness over which the surface density declines. If $\sigma$ is too small then the disc will be unstable to the standard RWI and will naturally form vortices. This is obviously not what we want to investigate here, and we choose a value of $\sigma=0.3R_1$. We note we are not appealing to any physical model here (e.g. photoevaporation or giant planets), rather we want to remain agnostic and study a disc that has the general features one might expect in a transition disc, while not starting from a disc structure that is RWI unstable.
The angular velocity is initially set to the Keplerian value, { suitably adjusted for the pressure gradient to maintain radial dynamical balance, using the numerical procedure suplied in {\sc fargo}.} We also adopt wave damping boundary conditions. We have checked that our initial surface density and temperature profile is stable by evolving it forward for 500 orbits at $R_1$. In order to isolate the physics of our new mechanism we ignore disc self-gravity and the indirect potential at this stage, meaning our choice of surface density normalisation is arbitrary and we scale all results in terms of $\Sigma_1$.
We insert a planet in the disc with mass ratio $q=M_p/M_*$ on a fixed circular orbit at $R_1$, and the local temperature is modified such that it has the profile:
\begin{equation}
T=T_b\left[1+\left(\frac{R_L^2}{r^2+s^2}\right)\exp\left(\frac{-r^2}{2(fR_L)^2}\right)\right]^{1/4}\label{eqn:T_numerics}
\end{equation}
where $r$ is the distance from the centre of the planet. The temperature expression (Equation~\ref{eqn:T_numerics}) contains two additional terms not present in Equation~\ref{eqn:temp_profile}. The factor $s$ is a smoothing distance so that the temperature profile does not diverge on the grid and the exponential term provides a cut-off in the temperature profile at radii so far from the planet that gas parcels do not spend sufficient time in the planet's vicinity such that they are heated, with the cut-off radius occurring at a radius of $fR_T$. While we shall see the choice of $f$ does affect our results, $s$ doesn't as the smoothing occurs on the grid scale, well inside the planet's Hill sphere.
\begin{table*}
\centering
\begin{tabular}{l|ccccccc}
Simulation & $N_R\times N_\phi$ & $q$ & $R_T/R_1$ & $R_T/R_H$ & $f$ & $s$ & $\alpha$ \\
\hline
Ctrl1 & $768\times1024$ & 0 & --- & --- & ---& ---& $1\times10^{-6}$ \\
Ctrl2 & $768\times1024$ & $1.5\times10^{-5}$ & 0 & 0 & ---& ---& $1\times10^{-6}$ \\
Standard & $1024 \times 1408$ & $1.5\times10^{-5}$ & 0.06 & 3.5 & $\infty$ & $9\times10^{-3}$ & $1\times10^{-6}$ \\
CutOff & $1024 \times 1408$ & $1.5\times10^{-5}$ & 0.06 & 3.5 & 1 & $9\times10^{-3}$ & $1\times10^{-6}$ \\
LowLum & $1532 \times 2056$ & $4.5\times10^{-5}$ & 0.01 & 0.4 & 1 & $5\times10^{-3}$ & $1\times10^{-6}$ \\
Viscous1 & $1024 \times 1408$ & $1.5\times10^{-5}$ & 0.06 & 3.5 & $\infty$ & $9\times10^{-3}$ & $1\times10^{-4}$ \\
Viscous2 & $1024 \times 1408$ & $1.5\times10^{-5}$ & 0.06 & 3.5 & $\infty$ & $9\times10^{-3}$ & $5\times10^{-4}$ \\
Viscous3 & $1024 \times 1408$ & $1.5\times10^{-5}$ & 0.06 & 3.5 & $\infty$ & $9\times10^{-3}$ & $1\times10^{-3}$ \\
\hline
\end{tabular}
\caption{Description of simulation parameters run. The second column lists the simulation resolution, columns 3--7 list physical and numerical parameters described above and the final column lists the $\alpha$ viscosity included.}\label{tab:sim_params}
\end{table*}
All simulations are performed on a polar grid with logarithmic-spaced cells in the radial direction and uniform-spaced cells in the azimuthal direction. This choice keeps the ratio of the cell side lengths approximately square over the entire domain. The radial grid stretches from 0.1$R_1$ to 10$R_1$, and we consider the full $2\pi$ in the azimuthal direction. We use the {\sc fargo} transport algorithm to speed up time-stepping, and work in a frame that is co-rotating with the planet. An explicit viscosity is included using an $\alpha$ viscosity law. The parameters for the simulation runs are described in Table~\ref{tab:sim_params}. We pick our temperature smoothing length $s$ to correspond to approximately two grid cells and we also smooth the planet's potential with a length scale of 0.5 the planet's Hill radius using the {\sc RocheSmoothing} facility implemented in {\sc fargo}. The planets are inserted at zero time with their full masses whereas the temperature hot spot's size $R_T$ is grown linearly over the first 50 orbits to the desired value.
\subsection{Simulation Results}
We evolved all of our simulations for 300 orbits to asses the impact of a hot spot around a planet in a transition disc-like gas structure. As discussed in Section~\ref{sec:thermal} the hot spot results in a surface density decrease that scales with the temperature increase. The resulting flow properties in the vicinity of the planet for our Standard case are shown in Figure~\ref{fig:baroclinic}. The properties are shown after 50 orbits; once the hot spot has grown to its full size, but before the resulting dynamics begin to dominate the flow.
\begin{figure*}
\centering
\includegraphics[width=\textwidth]{Baroclinic_2}
\caption{Zoom-in on the planet showing the surface density (left), temperature (centre) and magnitude of the baroclinic vector (right). The simulation shown is the Standard case with $R_T/R_H=3.5$ and $f=\infty$, and is shown after 50 orbits once the hot spot has grown to its full size, but before large scale vortex formation has occurred. { The units $\Sigma_1$ and $T_1$ are defined in Equations 24 \& 25 respectively as the surface density and temperature at $R_1$ of the backgroud, power-law disc profile.}}\label{fig:baroclinic}
\end{figure*}
Figure~\ref{fig:baroclinic} shows the surface density (left), temperature (centre) and baroclinic vector (right) for a zoom-in on the planet in the Standard run. We see a significant reduction in the surface density in the vicinity of the planet that mirrors the temperature increase as expected. We also note that the temperature hot-spot also launches waves that dominate over the density waves that are purely driven by the planet's gravity. This surface density drop and temperature increase correspondingly results in a significant baroclinic term that is 2-3 orders of magnitude larger than those arising from the planetary wakes. This source of vorticity extends well outside the planet's Hill sphere (which has a radius of $\sim 0.17R_1$) and thus gas parcel orbits intersect this region every orbit, allowing for the growth of vorticity.
\begin{figure*}
\centering
\includegraphics[width=\textwidth]{Standard_surf_evol}
\caption{Snapshots of the surface density distribution every 60 planetary orbits for the Standard run with $M_p/M_*=1.5\times10^{-5}$, $R_T/R_H=3.5$ and very low viscosity of $\alpha=10^{-6}$. The planet is located at a position $[0,-1]$.}\label{fig:Standard_Sevol}
\end{figure*}
\begin{figure*}
\centering
\includegraphics[width=\textwidth]{Standard_vortencity_evol}
\caption{Snapshots of the vortensity (scaled to the value of the disc with a Keplerian velocity profile) shown every 60 orbits for the Standard run. The planet is located at a position $[0,-1]$.}\label{fig:vortensity_evol}
\end{figure*}
The evolution of the surface density and vortencity of the Standard run are shown every 60 orbits in Figures~\ref{fig:Standard_Sevol} \& \ref{fig:vortensity_evol} respectively. These show that the hot spot rapidly produces a number of small scale vortices that grow (thorough interactions with the hot spot) and merge. After approximately 150 orbits (100 orbits since the hot spot reached full size), the disc contains a significant large scale anti-cyclonic vortex that has grown to the maximal width of $\sim 2H$. The azimuthal surface density enchantment has reached roughly a factor of two over the original transition disc gas structure. Over the continued evolution, the vortex grows in strength and after 300 orbits the vortex has begun to migrate. Once the vortices have merged to result in a single large scale vortex it has pattern speed with respect to the planet in the range $|\Omega_{\rm pattern}/\Omega_p-1|\approx0.01-0.05$, close enough to Keplerian such that it should efficiently trap particles \citep{Ataiee2013}.
\begin{figure*}
\centering
\includegraphics[width=\textwidth]{Panel_big_2}
\caption{Snapshots of the surface density distribution for each simulation shown after 150 and 300 orbits. The planet is located at a position $[0,-1]$. The simulation parameters are indicated in Table~\ref{tab:sim_params}.}\label{fig:evol_all}
\end{figure*}
The surface density snapshots at 150 and 300 orbits are shown for all our simulations in Figure~\ref{fig:evol_all}. In the three cases where there is no significant source of baroclinicity -- Ctrl1, Ctrl2, LowLum -- no large scale vortex forms as expected. In Ctrl1, where we have no planet, as in all simulations we have deliberately selected a starting gas profile that is not steep enough to be RWI unstable, and as such the disc profile evolves unchanged for many hundreds of orbits. In Ctrl2, the planet has a mass of $M_p/M_*=1\times10^{-5}$ (which is well below the thermal gap opening mass), while the planet launches standard density waves as expected, it does not effect the large scale dynamics of the disc. In simulation LowLum, we have $R_T<R_H$ and the thermal impact of the planet is contained well within the Hill sphere of the planet. As such no source of significant baroclinicty intersects with circular gas parcel orbits and, as expected, no large scale vortex is generated.
In the CutOff simulation, where we mimic the effect of the finite thermal inertia of the gas with an exponential cut-off to the temperature profile, the weakened source of vorticity results in a slightly weaker vortex; however, the general differences are small and a large scale vortex still forms after $\sim 100$ orbits.
\subsubsection{Effect of Viscosity}
Viscosity is known to effect vortex growth and survival in protoplanetary discs and indeed this is what our simulations with significant viscosity indicate. We find that with $\alpha=10^{-4}$ in the Viscosity1 run, the vortex growth is barely suppressed compared to the Standard run with negligible viscosity. In Viscosity2 with $\alpha=5\times10^{-4}$, large scale vortex formation still does occur but it is suppressed with an azimuthal surface density contrast of $\sim 1.3$ compared with $\sim 2$ in the Standard run.
In the most viscous run - Viscosity3 - with $\alpha=10^{-3}$, we find that there is a weak vortex present at 150 orbits, with an azimuthal density contrast of $\sim 1.05-1.1$; however, it does not grow to become a strong large scale vortex and after 300 orbits the disc has returned to being close to axisymmetric. At this high viscosity the gas surface density bump is also significantly weakened due to standard radial viscous transport, allowing the small vortices initially generated to migrate into the inner regions of the disc. Thus, while the higher viscosity certainly makes large scale vortex formation more difficult, it is unclear whether if some process existed to maintain the gas profile during the simulation (e.g. photoevaporation, a dead-zone or a massive planet) a large scale vortex would have indeed formed.
\section{Discussion}
\label{sec:results}
We have shown that ``transition'' discs are prime sites for the growth of low-mass planets by pebble accretion. This planet formation scenario has two important -- perhaps mutually exclusive -- implications. Firstly, if the planet were able to accrete pebbles at the standard rate for the entire time planet formation is occurring, then it could quickly deplete the local pebble reservoir in a very rapid $\lesssim 10^{5}$~year time-scale. Secondly, if the accretion rate results in a large accretion luminosity, such that it can heat the disc material outside its Hill radius, then it can lead to large scale vortex formation. The first implication begs an interesting question: if the pebble depletion time-scale is so fast $\lesssim 10^{5}$~years, how is it we see a number of transition discs with large mm-fluxes (and hence large reservoirs of pebbles) that almost certainly have lifetimes $\gtrsim 10^{5}$ years?
We hypothesise the answer to this question lies in the second consequence. The observed, probably long lived, ``transition'' discs that have large mm-fluxes \citep[e.g.][]{Andrews2011,OC12,Owen2016}, are those discs which are likely to have the highest pebble accretion rates, and as such the discs most prone to vortex formation. Vortex formation, results in an azimuthal pressure trap that can very efficiently trap pebbles \citep[e.g.][]{Meheut2012,Ataiee2013,Birnstiel2013,Zhu2014}. After all, the same dust particles that are likely to be trapped in the dust trap, are those which will accrete onto the planet, and are also those most likely to be trapped in the vortex. Since the vortex can migrate slightly, and does not necessarily have a pattern speed that is exactly Keplerian (as seen in our simulations), then the pebbles that can accrete on to the planet are trapped in the vortex and can only accrete onto the planet for a small fraction of time, or none if the vortex and planet have migrated apart.
Therefore, vortex formation and subsequent particle trapping may be the only way to ensure that these mm-bright transition discs remain long-lived. In fact, we can calculate the critical pebble surface density for a transition disc to form a vortex, and in principle remain long lived. We do this by assuming this threshold occurs when $R_T/R_H>1$. Since the Hill radius scales with planet mass as $M_p^{1/3}$ and $R_T$ scales as $M_p^{17/24}$ (where the solid planet mass-radius relationship can be approximated as $M_p=A_{\rm MR}R_p^4$ in the range 1-10 M$_\oplus$ using the profiles from \citealt{Fortney2007}). Thus, the limiting case when a disc can cross the $R_T/R_H>1$ threshold will be at the highest mass the planet can possibly reach. Therefore, if we approximate the maximum mass a pebble accreting planet can reach as $M_p\approx\Sigma_{\rm peb}/2\pi aH_p$ (i.e. the mass it would reach if it had accreted all the pebbles) and assume it is accreting from a reservoir of pebbles with surface density $\Sigma_{\rm peb}$, then we estimate the critical pebble surface density for vortex formation to occur before the entire reservoir is sequestered into a planet as:
\begin{equation}
\Sigma^{\rm crit}_{\rm peb}=\left[\frac{16\pi\sigma T_d^4A_{\rm MR}^{1/4}}{2G\Omega\left(2\pi a H_p\right)^{3/4}}\right]^{4/7}\label{eqn:sigma_crit}
\end{equation}
Given a $T\propto R^{-1/2}$ temperature profile for the passively heated, flared disc \citep[e.g.][]{Kenyon1987}, Equation~\ref{eqn:sigma_crit} only depends on a few parameters such that:
\begin{equation}
\Sigma^{\rm crit}_{\rm peb}\approx 0.3\, {\rm g\, cm^{-2}} \left(\frac{H_p}{H}\right)^{-3/7}\left(\frac{a}{20\,{\rm AU}}\right)^{-5/7}\left(\frac{M_*}{1\,{\rm M}_\odot}\right)^{-4/7}\label{eqn:sigma_crit2}
\end{equation}
where we have left $H_p/H$ as a free parameter here, but we suspect it to close to unity as discussed above. This critical surface density threshold can be compared to many of the well known mm bright transition discs. This comparison is shown in Figure~\ref{fig:Sigma_crit_compare}, where we plot the peak surface density at the edge of the cavity determined from mm imaging by \citet{Andrews2011} (using their model fits), compared to the result from Equation~\ref{eqn:sigma_crit2}. { This is done by taking the surface density models provided in \citet{Andrews2011}, which are obtained from fits to the mm image and spectral energy distribution. The pebble surface density is then taken to be the surface density in mm-sized particles at the peak of the profile. As such the values are uncertain due to several factors: (i) the simple surface density profile assumed by \citet{Andrews2011}; (ii) uncertainties in the underlying dust-particle distribution which could contribute to the mm-flux and (iii) the trap could be optically thick. }
\begin{figure}
\centering
\includegraphics[width=\columnwidth]{Threshold_compare_2}
\caption{The peak surface density of mm particles determined from mm imaging for well known mm-bright ``transition'' discs taken from \citet{Andrews2011} shown as points. The point sizes indicate the stellar mass. The lines show the minimum pebble surface density for vortex formation to be possible indicated by Equation~\ref{eqn:sigma_crit2}, the lines show different stellar masses: 0.5 (dot-dashed), 1.0 (solid) \& 2.0 M$_\odot$ (dashed). { The labels show the individual source names.} }\label{fig:Sigma_crit_compare}
\end{figure}
Figure~\ref{fig:Sigma_crit_compare} shows that the vast majority of mm-bright ``transition'' discs have mm size particle surface densities sufficiently high that vortex formation due to low-mass planet formation is possible.
Finally, it is well known that high viscosities can prevent vortex formation in the planet induced RWI mechanism and can also dissipate vortices \citep[e.g.][]{ValBorro2007,Fu2014b,ZhuStone14}. Our results are also consistent with the previous RWI results, in that large scale vortex formation is suppressed when the typical viscous alpha parameter is $>10^{-3}$. While typical values to explain the global evolution of the protoplanetary discs are of this order \citep[e.g.][]{Hartmann1998,Owen2011} there is every reason to expect the viscosity is likely to be lower in dust-traps and the outer regions of protoplanetary discs. Firstly, non-ideal MHD effects are important in the outer regions of protoplanetary discs \citep[e.g.][]{Armitage2011} and in the case of ambipolar diffusion dominated discs, vortices are known to form and survive for an observable length of time \citep{ZhuStone14}. Secondly, the enhanced dust content in the dust trap is known to suppress the strength of MRI turbulence \citep[e.g.][]{Jacquet2012}. Therefore, it is not unreasonable to assume that the viscosity in the neighbourhood of the dust-trap is sufficiently low to allow the formation of vortices.
\subsection{Long term evolution}
The long term evolution of the disc will be strongly controlled by whether it is able to form a vortex or not. As discussed above, if a large scale vortex is able to form it will trap all the pebbles in the vortex itself. As none of the vortices seen in the simulations are co-located with the orbiting planet \citep[see][for a discussion of how the planet and vortex may interact]{Ataiee2014}, then the vortex will starve the planet of pebbles and the rapid pebble accretion will cease.
Our simulations suggested that vortex formation is fairly rapid $\sim 100$ orbits. This is similar to the dust trapping time-scale, thus we suspect that the pebbles will become easily trapped in the vortex. At this stage the pebbles will no longer be available to rapidly accrete onto the planet. If the planet's accretion source is quickly shut-off then it will still be luminous for a short period of time, as the gaseous envelope previously supported by the accretion contracts towards the planet. This contraction will maintain its luminosity for a time-scale roughly similar to the gaseous envelopes Kelvin-Helmholtz time-scale ($t_{\rm KH}$), which for a planet with an envelope mass considerably less than the solid mass is given by, \citep[e.g.][]{Lee2015}:
\begin{equation}
t_{\rm KH}=\frac{GM_p^2X_{\rm env}}{R_pL}=X_{\rm env}t_{\rm acc}
\end{equation}
Thus, the Kelvin-Helmhotz time-scale is shorter than the accretion time-scale by the gas envelope to planet mass ratio. For these masses and luminosities $X_{\rm env}$ will be in the range $\sim$0.01, indicating that the luminosity output of the planet will drop on a time-scale $\sim 10-100$ orbits. This means that once the large scale vortex has trapped the majority of pebbles, the source of the barcolinicity generating the vortex will disappear on a comparable time-scale to the vortex formation time-scale, approximately as $R_T\propto t_{\rm KH}^{-1/2}$. Since a gravitationally contracting object will follow an evolution such that $t_{\rm KH}$ is approximately the time it has been cooling, then $R_T$ will decrease as the square root of time.
Now, since the vortex lifetime is finite, as without a source of barcolinicty, viscosity, instabilities \citep[e.g.][]{Lesur2009} or even the inertia of the dust itself \citep[e.g.][]{Fu2014} can destroy a large scale vortex on a time-scale of roughly 1000s of orbits, which is short compared to the disc's lifetime (e.g. $> 10^4$ orbits). We can therefore expect that vortex generation and dissipation occurs several times during the disc's lifetime, where pebble accretion onto a planet generates a vortex, which traps the pebbles hence suppressing the accretion and vortex generation. The vortex then dissipates after some time-scale, releasing the dust particles into an axi-symmetric ring that can then undergo pebble accretion onto a planet again, forming another vortex. The entire process can repeat for a long time-scale until the pebble reservoir is too heavily depleted to permit vortex formation.
If the pebble reservoir is too small to permit vortex formation, { although as demonstrated by Equation~\ref{eqn:sigma_crit2} still significant to make the disc appear as a mm-bright disc.} As discussed in Section~2, pebble accretion onto a planet will then rapidly deplete its local reservoir on a time-scale $\lesssim 10^{5}$~years. { This means the time-scale that a disc in this model would appear at intermediate mm-fluxes would be short.} Once the planet has depleted its local reservoir, particles at larger orbital separations will continue to drift into the dust trap. At large radii the maximum dust particle size is limited by drag rather than fragmentation \citep[e.g.][]{Birnstiel2012b}. Therefore, we can imagine that as dust particles drift from large radii in the disc, they will begin to grow and when they arrive in the vicinity of the planet they will be accreted readily as they will have naturally reached a size with $\tau_s=1$ at the planet's radius. In this stage, the planet's accretion rate will be limited by the accretion rate of dust particles into the trap due to drift, rather than the standard pebble accretion rate. Since these planets will necessary be low-mass ($< 10$~M$_\oplus$) they are unlikely to be able to accrete a significant gas envelope \citep[e.g.][]{Rafikov2006,Piso2014}. Thus, unlike the dust particles that could in principle be rapidly sequestered into low-mass planets, the gas will remain largely unchanged. This means this process may ultimately result in a low-mass dust-poor, gas-rich, low-mass-planet-rich disc, a type of disc for which there are poor observational constraints.
Finally, the last concern is migration. These planets are low enough mass that they are unlikely to open a gap in the gas disc, where the gap opening mass is more typically $\sim 0.1$M$_J$ at tens of AU \citep[e.g.][]{Crida2006}. Therefore, migration is likely to take place in the type-I regime. While the migration rates for low-mass planets are still greatly uncertain in realistic protoplanetary discs, even the isothermal type-I migration rates, which are likely to strongly over-predict the migration rates, give rates $\sim 10^5$~years for a few earth mass planet at 10s of AU \citep[e.g.][]{Ward1997}. This means that a forming planet is able to initiate vortex formation and it will not migrate away in on the time scale for vortex formation to occur. However, migration might push the formed planet inside the transition disc cavity after the vortex has formed but before it has dissipated. The vortex will certainly qualitatively effect the migration of such a low-mass planet (we note again we do not consider migration of our planet in our simulations presented here), as demonstrated by \citet{Ataiee2014}. This might mean that over a Myr lifetime of planet formation, the cycles of vortex generation and dissipation in the disc may dump a handful of low-mass planets inside the transition disc cavity, which could subsequently scatter.
\subsection{Observational implications}
While we have suggested that transition discs are prime sites for planet formation through pebble accretion, the fact that it is so rapid means that if it was left to proceed as normal in discs with the parameters of standard mm-bright transition discs ($a\sim 10-50$~AU, $\Sigma_{\rm peb}\sim 1-10$g cm$^{-2}$), it would rapidly deplete the entire disc on an incredible short time $\lesssim 10^{5}$~years. We suggest the fact that these mm-bright transition discs can exist for a long enough time-scale to be observable, is that at the expected dust surface densities in these discs, the act of low-mass planet formation in their dust traps should result in large-scale vortex formation.
As discussed above these dust traps should trap all the pebbles within the vortex itself and prevent further planet growth. Therefore, many of these discs should spend { some} fraction of their lifetimes with large scale vortices, which will be observable as large scale asymmetries when the discs are imaged at mm wavelengths. { For the mm-bright transition discs imaged at high resolution IRS48 \citet{vanderMarel2013} and HD142527 \cite{Casassus2013} show strong asymmetries, and LkH$\alpha$330 \citep{Isella2013} and SAO2016462 \citep{Perez2014} show weaker asymmetries. Many other observed transition discs do not show any evidence of an asymmetry (e.g. LkCa15, SR24S \citealt{vanderMarel2015}, Sz91 \citealt{Canovas2016}, DoAr 44 \citealt{vanderMarel2016}). In recent ALMA surveys of protoplanetary discs \citep[e.g.][]{Pascucci2016,Ansdell2016} several more transition disc like structures have been detected, many of which show no evidence for an asymmetry at $\sim 0.3"$ resolution. To date it is unclear exactly what fraction of transition discs show asymmetries. The reason for this is partly due to unsystematic observations at a variety of resolutions and partly due to the fluid definition of a ``transition disc'': for example should discs with large mm-holes but primordial SEDs be counted in this sample? \citep[See][for a discussion of these discs.]{Andrews2011,Owen2016}. What can be said with any confidence is that a moderate fraction of mm-bright transition discs show asymmetries.} Finally, exactly what kind of asymmetry our vortices produce will depend on the observational wavelength, surface density distribution and other factors (e.g. dust-growth and destruction) we do not consider here. Therefore, we must wait until dust-gas simulations are performed, before we can draw any hard conclusions from the (incomplete) transition disc statistics we have today.
We suspect the hot-spot generated by the planet will fade on a time-scale of $\sim 100$ orbits. Thus if the vortex lifetime is significantly longer than 100 orbits, it would be very unlikely to directly observe the effect of the increase in local disc temperature in the continuum image as $R_T$ will have contracted to well inside the planet's Hill sphere once the vortex had trapped all the dust particles. However, it may be possible that the hot spot would generate some chemical fingerprint, that would last longer than the hot spot, spread into a ring, and possibly be a signature of this process.
The critical pebble surface density for vortex formation derived in Equation~\ref{eqn:sigma_crit2} is similar to the value required to give a mm-flux at 140pc of $\sim 30$ mJy \citep[e.g.][]{Andrews2005}. This mm-flux value is the discriminating value between mm-bright and mm-faint transition discs determined by \citet{OC12}. \citet{OC12} and \citet{Owen2016} argued that mm-bright transition discs are likely to be rare and long lived (lifetimes $> 10^{5}-10^{6}$ years), whereas mm-faint transition discs are thought to be common (in the sense that all discs experience this phase) and short lived with lifetimes $\lesssim 10^{5}$~years. Here we suggest that this critical pebble surface density for vortex formation could provide the link as to why mm-bright transition discs are likely long lived and mm-faint transition discs are likely short lived. Since mm-bright transition discs can form vortices, they can prevent the dust from being rapidly turned into planets, producing many cycles of planet formation, vortex formation and subsequent destruction.
Finally, one obvious consequence of this mechanism is the production of low-mass ($\lesssim$ Neptune mass) planets with orbital separations of tens of AU. There is currently limited observational sensitivity to the low-mass exoplanet population at large separations. However, mirco-lensing surveys have detected Neptune mass planets at separations $\sim$10~AU \citep[e.g.][]{Gaudi2012, Shvartzvald2016} and have suggested that such planets are common \citep[e.g.][]{Gould2006}. The sensitivity of these experiments will only improve with future surveys hopefully revealing the full mass-spectrum and semi-major axis distribution of these systems.
\subsection{Future Directions}
In this work we have mainly argued that transition disc dust traps are likely to be prime sites of planet formation by pebble accretion. The rapid nature of the planetary accretion is likely to have many interesting consequences. Here we have argued that by modifying the temperature structure outside the gravitational influence of the planet it can provide a source of vorticity, which allows the growth of large scale vortices.
In the simulations performed in this work we have described a very ideal setup, where we impose a local hot-spot that is not coupled to the subsequent dynamics. Specifically, we do not to attempt to model the coupled evolution of the dust, gas and planetary accretion in a self consistent way. While the time-scales suggest that large scale vortex formation is likely to occur the finer details of the results require further investigation. The vortex strength, how it traps dust particles, and when and how accretion onto the planet is shut-off due to the fact the pebbles are now trapped in the vortex requires coupled dust and gas simulations, possibly including grain growth. Such simulations will be able to investigate the cycle of planet formation, vortex growth, planet migration and dissipation that allows these discs to exist for the $>10^5-10^6$~years that we have postulated above.
Furthermore, in-order to isolate the physics of the problem at hand we have neglected the self-gravity of the disc and the indirect potential that could effect the planetary dynamics and migration. In massive discs, vortex formation could result in the vortices transitioning to global ``fast'' modes \citep{Mittal2015}, similar to the transition of RWI generated vortices into fast modes discussed by \citep{Zhu16a,Zhu16b}. It maybe interesting to investigate the interaction between pebble accretion generated vortices and the indirect potential to see if fast modes can be triggered in this case, even without the original transition disc cavity.
Finally, we note that while we have primarily focused on pebble accretion and vortex generation in transition discs, the mechanism of vorticity generation is not limited specifically to transition discs. Indeed, pebble accretion has been invoked to solve numerous planet formation problems at various locations and rates throughout primordial protoplanetary discs \citep[e.g.][]{Bitsch2015}. In our work, the gas cavity prevents the vortices from rapidly migrating allowing them to grow to large sizes. In a primordial disc, we speculate that smaller vortices may be generated which can still trap particles and migrate. By trapping particles this could affect the assumed pebble accretion rates in such calculations. This may be particularly important at smaller radii, as our critical vortex formation threshold scales as $R^{-5/7}$, whereas disc surface densities are thought to fall in a steeper manner with radius, with mm observations of protoplanetary discs suggesting an $R^{-1}$ \citep{Andrews2009} decline, and the Minimum Mass Solar Nebula (MMSN) scaling as $R^{-3/2}$. Therefore, investigating the prospects of vortex generation in a primordial disc that is forming planets through pebble accretion is certainly a worthwhile investigation.
\section{Summary}
We have argued that the dust-traps created within ``transition'' discs can serve as planet incubators, and consequently vortex generators.
If a small $\gtrsim 10^{-4}$~M$_\oplus$ embryo forms, it would undergo rapid accretion through ``pebble accretion''. The dust-trap naturally filters the dust particles size distribution within the trap, such that most of the dust mass in the trap will be at the preferred size to undergo pebble accretion, namely those particles with Stokes numbers $\sim 1$. The high surface density of pebbles means accretion is extremely rapid, and the embyro can grow to masses $>1$~M$_\oplus$ on short time-scales ($10^4-10^5$~years). Thus, massive transition discs are prime site for the formation of low-mass $\lesssim 10$~M$_\oplus$ planets. Depending on the exact frequency of massive transition discs, planet formation in a transition disc induced dust trap could be a dominant mechanism of low-mass planet formation at large separation.
Furthemore, we argue that the accretion luminosity liberated during the formation of the planet is large enough to heat the surrounding disc, well outside the planet's gravitational influence. This makes the disc {\it locally} baroclinic and unstable to vortex formation. By performing numerical simulations we show that these vortices will grow and merge until one large scale vortex is formed in about 100 orbits, only if the temperature of the disc can be increased by the planetary accretion outside the planet's Hill sphere.
We suggest that this mechanism naturally explains the observed asymmetries in transition discs, as planet formation and rapid pebble accretion is difficult to prevent in the dust densities expected in transition disc dust trap and thus seemingly inevitable. Furthermore, our mechanism doesn't suffer from the requirement of a sharp density contrast required by the Rossby Wave Instability which may be difficult to generate in an actual protoplanetary disc.
{ This new mechanism hinges on the production of a low-mass embryo to start undergoing pebble accretion (once the embryo forms it is difficult to imagine it could not undergo pebble accretion). We have not attempted to directly address the issue of the embryo's formation here. Several mechanisms do exist which would produces embryo's of the correct size (such as coagulation, the streaming instability of direct gravitational collapse, or some combination of them), they do require certain conditions be met. For example, the streaming stability requires low turbulence and high dust-to-gas ratios. The pressure traps to qualitatively provide many of these special conditions, it is impossible to say without quantitative calculations whether the observed ``transition'' discs satisfy these requirements all the time. }
Finally, we hypothesise a cycle of planet formation, vortex generation, dust-trapping and vortex dispersal where the duty cycle of vortex observability will be high. Rapid planet formation will heat the disc and generate a large scale vortex. This large scale vortex will then trap the dust particles and prevent further pebble accretion and vortex growth. The vortex will then live for some time before being destroyed releasing all the dust particles in the axisymmetric dust-trap allowing the cycle to restart. Thus, our mechanism does not suffer from the problem that we require a long vortex lifetime for it to be observable, just a lifetime greater than a few hundred orbits. Calculating this cycle end-to-end will require more detailed, probably coupled dust and gas simulations, however it presently offers a promising resolution to a number of outstanding observational and theoretical puzzles.
\section*{Acknowledgements}
The authors are grateful to the referee for advice that improved the manuscript. We are grateful to Richard Booth, Subo Dong, Ruobing Dong, Kaitlin Kratter, Tim Morton, Ruth Murray-Clay, Roman Rafikov, Giovanni Rosotti and Zhaohuan Zhu for interesting discussions. JEO acknowledges support by NASA through
Hubble Fellowship grant HST-HF2-51346.001-A awarded
by the Space Telescope Science Institute, which is operated by the Association of Universities for Research
in Astronomy, Inc., for NASA, under contract NAS 5-26555. JAK gratefully acknowledges support from the Institute for Advanced Study.
\label{sec:summary}
\input{ref.tex}
\bsp
\label{lastpage}
\end{document}
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Q: My enemy isn't moving when my character is standing still I'm currently coding a game on python, and I need a way for the enemy to run towards the player. It has to have a constant velocity of 5 pixels a cycle and this is my current code:
def move(self,character):
characterposition = Vector(character.posx,character.posy)
self.position = Vector(self.posx,self.posy)
dist = characterposition.subtract(self.position)
dist.normal(dist.length())
length = dist.length()
ratio = self.speed/math.sqrt(length)
self.posx += dist.x * ratio
self.posy += dist.y * ratio
this seems to be working until my character stops moving. When the character stops moving, the enemy stops as well. This is a problem and I would appreciate any suggestions.
Edit: Heres my loop.
while True:
for event in pygame.event.get():
if event.type == pygame.QUIT:
pygame.quit()
run = False
continue
updatecharacterposition()
collided = checkforbarriercollision()
badguy.move(character)
if collided:
print("YOU LOST")
pygame.quit()
time.sleep(5)
redrawgamewindow()
A: Is the indenting in the code above correct? It shows updatecharacterposition() and the lines after it inside the for event in pygame.event.get(): loop.
If that is really the case, then none of that code will get called if you are not getting any events. That would cause all of the movement to stop.
Try this:
while True:
for event in pygame.event.get():
if event.type == pygame.QUIT:
pygame.quit()
run = False
continue
updatecharacterposition()
collided = checkforbarriercollision()
badguy.move(character)
if collided:
print("YOU LOST")
pygame.quit()
time.sleep(5)
redrawgamewindow()
On a side note, it seems odd to me that badguy.move(character) is after the collision check. Usually you would move everything (the player and the 'badguy') and then do the collision check.
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GSERB District Selection of Secondary Sikshan Sahayak 2016. Check all official updates of GSERB District Selection process as per official gserb.org Site. Lets check more Details Like Education, Fees, Application form, Pay scale are given below.
Check above link for Details, kindly Stay updated with us for Latest GSERB bharti / Recruitment updates. | {
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ACCEPTED
#### According to
Index Fungorum
#### Published in
Nova Hedwigia 55(1-2): 205 (1992)
#### Original name
Porina rugosa Ach.
### Remarks
null | {
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Like the Gimlet, the Dark 'n Stormy is a cocktail for which we have British sailors to thank. In the mid-1800s, English brothers James and Ambrose Gosling ran a thriving distillery in Bermuda famous for its dark-colored rum. British ships back then always carried booze for their sailors, along with ginger beer, which is an excellent remedy for seasickness. It's only natural that someone would combine the two at some point.
"I love the simplicity of the Dark 'n Stormy," says Chad Solomon, who co-owns Midnight Rambler in Dallas with Christy Pope. Solomon and Pope are both Southern—he grew up in Texas, she in Louisiana and Florida—but they got in on the ground floor of the twenty-first-century cocktail revival in New York, where both worked at several influential cocktail bars in the early 2000s, eventually starting the city's first drinks-only catering company, Cuffs & Buttons.
Making ginger syrup is simple: Juice some fresh ginger, and add sugar. Another technique Solomon and Pope recommend for this drink is dry-shaking: Combine the rum, ginger syrup, and lime juice in a shaker and shake without ice before assembling the drink. "This adds a little aeration and makes the texture of the drink a little lighter," Solomon says. Just be sure everything else is chilled: he recommends sticking the glass in the freezer for a few hours, and topping the blended mix with club soda that's as crisp and cold as possible.
Though you can fiddle with the ratios of ingredients in the Dark 'n Stormy, you absolutely cannot substitute the Gosling's Black Seal Rum. The drink is one of a handful whose names have been trademarked, and Gosling's has not been shy about taking legal action against competitors and bars who call for different brands of rum. Thankfully, the rich and molasses-y Bermudan spirit is ideal for a Dark 'n Stormy.
Add the rum, ginger syrup, and lime juice to shaker and shake without ice. Pour into a frozen highball glass filled with ice. Fill with club soda and garnish with a lime wheel and a piece of candied ginger on a cocktail pick.
*To make fresh ginger syrup, wash a large chunk of fresh ginger and chop into 1-inch pieces (no need to peel). Run through a juicer and fine-strain the juice. Measure the ginger juice and stir in an equal volume of sugar (e.g. for 1 cup of ginger juice, add 1 cup of sugar). Store in the refrigerator for up to 3 days. | {
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Puddings | Anyone For Seconds?
I don't know where I found this recipe but it is a very nice light pudding. The alcohol can be left out to no real detriment to the taste, but you will need 2 lemons if you do not use it. It can be made very quickly if guests turn up unexpectedly. Since making it a few times now, it has become a summer family favourite.
Bring a taste of Italy to your table with this delicious gluten free pud!
1 Mix the the Limoncello, most of the zest from 2 lemons and the juice of one to two lemons (whatever your preference) together.
2 Pour the cream into a large bowl and softly whip with the sugar. It's important not to over-whip the cream, so whisk it until it just starts to thicken.
3 Then drizzle in the lemon mixture and whisk again.
4 Divide between 4-6 small glasses and refrigerate for at least an hour.
5 Just before serving, put six biscuits in a plastic bag. Crush with a rolling pin and sprinkle them over each dessert with a little lemon zest.
If you like, serve each with a ratafia biscuit.
N.B. Check the biscuits are gluten free.
This has got to be one of the best Christmas treats ever and I have had them homemade as far back as I can remember! They are one thing I love coming back to the family home for, over the festive period. I have even had my Brother in Canada asking me to get this recipe on my blog.
This is my recipe for mince pies, everyone has their own I feel, but these freeze well and my family seem to like them. In fact when my eldest son (me) was at primary school he used to take one for break. This led to me making them for his form teacher too!
You do need a light hand for pastry or make it in a mixer but watch it carefully as it should not be over-mixed. I use my homemade mincemeat that I make with the apples from the garden, but if you use shop-bought mincemeat add a little brandy or rum to it as it adds a certain something to the pies.
I make the pastry with what flour I have in the cupboard – plain, self-raising or a mixture of both. The amounts shown below can be doubled in quantity or even halved.
Preheat oven to 200C/400F Gas 6 or 180C Fan Oven.
1 Cut the butter into cubes and rub into the flour until it resembles breadcrumbs. If using a mixer do not over mix.
2 Add the egg and some water; continue mixing until the mixture comes together. If you only use the egg the pastry will be more difficult to work with but that is ok.
3 Remove from the bowl, wrap in cling-film and refrigerate for ½/1 hour.
4 Place onto a floured board, roll out thinly and cut out rounds to fit your tins.
5 Fill with the mincemeat and dampen the edges of the lids with water and press them lightly on top.
6 Brush with either beaten egg, milk or a mixture of both and cut a slit in the top. This can be with a knife or scissors. I am a bit of a traditionalist and put a cross.
7 Bake in the oven for 20/30 minutes or until golden. Cool on a wire tray.
8 Serve warm sprinkled with icing sugar and cream or brandy butter.
9 If freezing I find it is better to freeze the mince-pies uncooked. Freeze in the tin, and when frozen remove from the tin and put into a freezer bag. To cook, remove from the freezer put back into the tin, allow to defrost, brush with an egg mixture and cook as before.
If allergic to either eggs or milk just leave them out.
NB I will post my recipe for homemade mincemeat at a later date. | {
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Q: Keep calling activity and clear other activities before that I am calling activities in the following order A>B>C>D, now I want to call Activity A and clear B and C but keep D. I am calling A with Intent.FLAG_ACTIVITY_CLEAR_TOP | Intent.FLAG_ACTIVITY_SINGLE_TOP. But all the activities apart from A is getting cleared. Any body has any idea how to clear B and C and keep D>A.
A: You can move A to the top (from D) by doing this in D:
Intent intent = new Intent(this, A.class);
intent.addFlags(Intent.FLAG_ACTIVITY_REORDER_TO_FRONT);
startActivity(intent);
There aren't any simple flags you can use to get rid of B and C. I would suggest that you have B and C register a BroadcastReceiver that listens for a specific ACTION. After you launch A from D, you can then send a broadcast Intent that will cause B and C to finish themselves. For example, in B and C do this:
// Declare receiver as member variable
BroadcastReceiver exitReceiver = new BroadcastReceiver() {
@Override
void onReceive (Context context, Intent intent) {
// This Activity is no longer needed, finish it
finish();
}
}
in onCreate() register the receiver:
registerReceiver(exitReceiver, new IntentFilter(ACTION_EXIT));
don't forget to unregister the receiver in onDestroy()!
In D, when you launch A, send a broadcast Intent containing ACTION_EXIT to make B and C finish, like this:
sendBroadcast(new Intent(ACTION_EXIT));
A: Add this in your manifest for Class B, C.
<activity
android:name=".AnyActivity"
android:noHistory="true" />
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Rannvijay Singha Defends Bigg Boss 11 Contestant Priyank Sharma!
Bigg Boss 11: Priyank Sharma And Vikas Gupta's Friendship Turns Sour!
Bigg Boss 11: Priyank Sharma Gets Nominated For BREAKING Rules!
Bigg Boss 11: Akash Dadlani Provokes Priyank Sharma Again- Watch Video!
Bigg Boss 11: Evicted Contestant Jyoti Kumari Makes Some Shocking Revelations! | {
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home Dogs Up To What Age Do Dogs Have Estrus
Up To What Age Do Dogs Have Estrus
How old are dogs in estrus?
First estrus in dogs.
A cat's heat: a natural process that requires special attention
Heat in dogs
First estrus in dogs: duration and characteristics
Owner rules
Problems during estrus
Techka: main features
Duration and frequency of estrus in a dog
Hygiene rules during estrus
When a dog starts to heat
Preparation for mating
How to tell if your dog is in heat soon
Overview of Canine Heat
Possible problems during estrus in dogs
How to behave if a dog is in heat
What to do if dogs are not in heat
How long does a Yorkie in heat last?
Normally, estrus lasts 3 weeks, and from the 9th to the 13th day the brood bitch can be fertilized. The 12th day is considered the best day for mating. But this is not a mandatory rule. If there are deviations in the duration of estrus, then the onset of the period during which the bitch can be fertilized also changes. Therefore, it is recommended to keep a close eye on the breeding bitch during the entire estrus and record the dates of her beginning and end. This plays an extremely important role in choosing the right mating day for Yorkshire Terriers. Preventive breeding vaccinations must be done no later than a month before the expected estrus and no earlier than a month after its end or a month after the distribution of puppies. In addition, you need to check the York girl for the presence of worms.
As soon as you establish a breeder's bitch in heat that you intend to mate, contact the breed leader or Breeding Director. He tells you which dog your dog should be mated with, and tells you the address of its owner, as well as tell you what day it is best to mate. If you and your dog are going to mate in another city, choose the appropriate mode of transport so that the breeding bitch does not inconvenience and does not get lost.
When dogs are in heat?
The first estrus in dogs usually begins after the change of teeth, but it is impossible to predict the exact time, because K. The techka completes a certain stage in the development of the body of a young bitch. Each dog has its own. In large breeds, the development of the dog takes longer and there are frequent cases of a shift in the first heat up to the age of one year of the dog. Even within one breed, for example, the Caucasian Shepherd Dog, we had the timing of the onset of the first estrus from 6 months to 13 months (a very powerful and large bitch)!
What can help in guessing the deadline?
You should ask when your dog's mother started her first heat and how it went. Features, behavior, the course of pregnancy and childbirth are passed from mothers to daughters and, according to experience, in most cases, this is confirmed.
There is no unambiguous age indicator, since everything is individual. The breeds are different and the weight categories are different. Which leaves its mark. Large dogs live much less than dogs of small breeds, respectively, and the manifestations of a full-fledged sexual cycle are different.
When examining a patient, the doctor comes first with his diagnostic concept, which he will prove using special research methods.
" A correct diagnosis does not mean a cure"
You have a young bitch in your house and now you have to learn how to periodically go through the estrus cycle with her and adapt to this inevitable process.
How to notice the onset of heat or signs of heat in dogs?
The approaching heat can be noticed while walking the dog. The dog urinates frequently.
Behavior can change, often the dog becomes active, playful, and disobedient. Hormones begin "play", and instinct pushes her towards free behavior. The bitch makes frequent marks. Odorless "bait" for males.
The bitch wants to explore more and more vast territories, thereby spreading its smell, luring potential "suitors". Bitches often shed before heat.
Males during this period come up to the bitch, sniff at her, but they do not bind the bitch, and the bitch herself behaves more aggressively towards males.
When examining the dog, the owner notices a change in the female genitals. The loop becomes more and more swollen, when pressed, you can see the discharge lightly. Pink or unclear. Color pink.
If you notice changes in the dog's behavior, do not be lazy and check the dog every day for heat by blotting the noose of the bitch with a napkin or toilet paper. The pinkish discharge will be the beginning of estrus. Mark this day in the dog's notebook.
In order for a future breeding bitch to be used for breeding, she must receive at the show an assessment of at least "very well". The obvious requirement for a breeding bitch is her health and good shape. A bitch is allowed to mate at the age of 18 months. It is generally recommended to knit a Yorkie in third heat.
When Yorkies start their first heat?
Yorkies usually start estrus at the age of 8-10 months. The following are repeated at intervals of six months. There are many bitches whose first estrus begins much later. at 12-14 months. The interval between estrus in Yorkies also varies greatly. from 5 to 10 months. It even happens that a Yorkie is in heat only once a year. In the same bitch, the duration of the heat interval may also change. By old age, as a rule, the interval between estrus increases.
If you intend to have a cat, and not a cat, you should prepare from the very first days for the fact that at a certain age she will begin to estrus. This is a natural process in the body of an animal, however, you need to prepare in advance for its beginning, because the owner of the animal must not only know how the cat behaves during estrus, but also be able to help his pet prepare for "an adult" life. And don't think that caring for a cat during estrus will be easier and easier than caring for a cat in a similar situation.!
What is a cat's estrus?
In another way, this phenomenon is called estrus and involves a change not only in the physical state of the animal, but also the occurrence of certain changes in its psyche. Heat begins when the follicles in the ovaries ripen in a cat, and it is this symptom that is the first evidence that the animal is ready to bear offspring and to subsequent childbirth.
As a rule, estrus in cats lasts several days, and you can determine its onset by the following signs:
Change in animal behavior. It can become either very aggressive or, on the contrary, very affectionate.,
The appearance of uterine and inviting cries (sometimes the cat can scream all day and night),
Swelling of the genitals (practically insignificant, therefore only a specialist can often determine its presence),
Frequent urination,
Decreased or even complete lack of appetite (observed either during the entire period of estrus in cats, or only in the first days),
Change in cat gait. She begins to walk on bent hind legs, tail raised,
The appearance of transparent discharge from the genitals. To remove them, the cat begins to wash much more often (at the same time, unlike dogs, cats do not have spotting!).
These signs of estrus in a cat can alternate, or they can be observed in combination. However, in any case, the owners of the animal need to be prepared for the fact that sometimes the cat marks its territory during estrus.!
What are the signs that you can tell if a dog is in heat?
Droplets of blood on the couch and floor, frequent urination, strange behavior uncharacteristic for a dog. all these symptoms indicate that the female is in heat.
Signs of heat:
Favorite more often than usual to ask to go to the toilet. In this case, the female can mark with her urine every bush and every tree. In rare cases, the dog begins to write in the house, trying to mark all corners and pieces of furniture with its scent.
Bloody discharge with a specific odor oozes from the female's genitals. In all places where the pet sat or lay, there are bloody drops, indicating that she is in heat.
Sometimes animals during this period begin to shed intensively, leaving scraps of hair throughout the house.
When the dog is taken out for a walk, he takes an active interest in all the males running by. In this case, the pet may try to break off the leash and escape from the owner.
During estrus, the character of the animal also changes. Sometimes the pet becomes overly excited and playful or behaves disobediently, not responding to the owner's comments and commands. Some females, on the contrary, become lethargic and sad, do not want to play and even lose their appetite.
A sign of estrus can also be the fact that the dog often licks its genitals, in particular after each trip to the toilet.
Representatives of large breeds can behave viciously and aggressively even towards the owner. Therefore, it is advisable to limit walking with the dog, especially in those places where children walk.
Frequent urination may be a symptom of estrus.
Are there norms?
It is worth noting that the duration of estrus, the cyclical nature of this process are individual for each female. Of course, there are norms. But they are very conditional. There is a framework for how many days a dog is in heat, exceeding which indicates the presence of health problems. Any caring owner should know the duration and frequency of estrus, what changes occur in the dog's body during this difficult period, how behavior changes.
When a dog first starts to estrus?
Sexual maturity of four-fingered pets occurs at the age of seven to twelve months. Therefore, the first estrus can begin both in a seven-month-old pet and in a female who is twelve or fourteen months old. In some animals up to a year and a half, there are no signs of estrus at all and this is considered the norm, and not a deviation.
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Puberty in dogs begins at 7-12 months of age.
About the determination of estrus in dogs. When a dog starts to heat
The first estrus in a dog, at what age. this question is of interest to many owners. Usually the onset falls within a period of six months to two years. This is normal. Usually, the first estrus begins after the period of tooth change. Nobody knows the exact time. In animals of small breeds, blood begins to flow at the age of 6 to 10 months. For representatives of medium and large breeds, the timing is slightly different. A dog's first estrus can begin between six months and 13 months.
When a dog's first heat occurs, it is not difficult to notice it. The beginning takes place in conjunction with the following symptoms:
Behavior change;
Interest in the pet from males;
The appearance of bloody discharge;
Sometimes females are prone to molt during this period.
Heat is often quite noticeable in small breeds. But sometimes the first estrus begins imperceptibly and passes inactively, without noticeable signs. But even in this case, you must not lose your vigilance. it's still a full heat.
An owner wishing to breed offspring should remember when the female starts bleeding. Puberty occurs in the third period, it is for the third time that a pet can be knitted. In order to choose the most favorable days for mating in the future, the owner should record the behavior of the animal during this period of time.
A dog's sexual cycle consists of several parts. Let's consider each of them in more detail:
Proestrus is a period that takes from a week to 10 days in which the behavior of the female changes noticeably. The pet is excited, playful and active. During walks, she marks the territory, listens poorly to the owner and more often pays attention to males.
Estrus itself. Ovulation occurs. The female allows the dog to come to her, takes away the tail.
Metaestrus is the third period lasting several days. The flow ends, the blood stops flowing, and the female loses interest in the males and stops letting them in.
During anestrus (the fourth cycle), sexual rest occurs, lasting up to 150 days.
What should the owner do when the dog's first estrus begins? It should be remembered when it started, note how many days it lasts, as well as the peculiarities of the pet's behavior during this period of time. This data will help predict the approximate time of the next estrus, as well as determine the favorable time for mating if further breeding of the offspring is planned.
If the owner does not want to mix a bitch with a dog, the main rule for him is not to let the dog off the leash for a while, while it is in heat. Even if the pet knows all the commands and obeys the owner, during this period of time it can become uncontrollable, run away, not approach on command. And it will be very difficult to drag the dog away from the bitch, in which case.
While estrus lasts, the owner should restrict his pet from participating in exhibitions for two reasons: firstly, at this time the dog's behavior changes, and the owner cannot predict what she will do; and secondly, it can be dangerous due to the risk of accidental mating.
During the period when the dog is estrus, it should be protected from infections. Their animal can pick up, for example, after swimming in a pond.
Heat in dogs or estrus is an important process that helps to plan mating or, on the contrary, to prevent the appearance of unwanted offspring. Any deviations from the norm are a reason to visit a veterinary clinic to prevent possible health problems.
Estrus can be determined by the behavior of the pet, which varies greatly. The female is active, plays a lot, may not follow the usual commands. All these are the consequences of hormonal changes. Other signs include:
Frequent urination. this is how the animal marks the territory and attracts males;
Bloody issues;
The dog constantly licks the area under the tail;
The bitch tries to run away to the males, and they reciprocate her;
Molting. this often precedes estrus.
At first, dogs do not allow males to come near them and can be quite aggressive, since their bodies are not yet ready for mating. After about a week, sexual desire arises, the loop noticeably increases in size. A bitch can stay in this state for up to seven days.
The dog tends to lick the area under the tail
But your pet's breed matters.
The first phase of estrus is a period of bloody discharge, a gradual increase in the loop and constant rushing towards persistent suitors. It is important to remember how long the dog's estrus does not cause hunting: with the onset of the time of "love", the most dangerous or most desirable (if mating is planned) days come. Estrus or the second phase of estrus. mucous transparent discharge, soft yielding noose, inviting games and characteristic postures when meeting males. The girl often asks for a walk, is disobedient during a walk, she can run away in search of love. The third phase of estrus in a dog lasts as long as it takes for the body to return to its normal state: the loop decreases, the discharge stops, the level of most sex hormones drops. As a rule, the duration of the phases is conditionally equal, plus or minus a couple of days.
It would seem that everything is easy to calculate, but many different factors affect the duration of estrus in dogs. First of all, these are individual characteristics and heredity, therefore, with the question of the period of love, it is wiser to contact the breeder if he has enough experience. In addition, the size of the bitch is important: large girls mature later and "walk" longer, estrus in small dogs is shorter and occurs earlier, sometimes already at the age of five months. The constitution also plays a role: wide bone, square format, bulky muscles. late maturation and less prolonged estrus, light bones and general harmony, leanness. earlier maturation and longer estrus.
How many days a dog's estrus lasts is also influenced by the conditions of detention. If different-sex animals are kept in the same house, estrus can be delayed. If the bitch is exhausted by excessive exertion, contract. Heat is shorter in winter, longer in spring and summer, which is especially noticeable when it comes to booth or enclosure dogs. The season has almost no effect on a girl living in an apartment, therefore, the duration and frequency of estrus in dogs rarely change with the change in day length and temperature.
Among other things, the general condition of the bitch is important. There are many congenital pathologies that often do not affect health in any way, but determine how long dogs are in heat. This is not necessarily a pathology of the development of the reproductive system, the pituitary gland, the thyroid gland, the adrenal glands, and other organs are responsible for the production of hormones, and therefore for the sexual cycle. Chronic diseases can also change the duration of the cycle. systemic diseases, tumors, infections, "female" ailments, etc.
How long a dog will take in heat depends on age. Young healthy bitches run longer than adolescent and aging dogs. With age, not only the duration of the leaks decreases, but also their frequency. the resting phase gradually increases from year to year. Although some girls remain active until old age. But there is no complete cessation of leaks just due to aging.
Do not forget to record how estrus affects the girl's behavior, how many days the dog's estrus does not cause a desire for love, how long the arousal phase and the rest phase lasts. This data will help if any changes happen. And remember that a veterinarian is the only competent person whose advice can truly be trusted.
Estrus, scientifically or simply, estrus is a process that indicates the onset of puberty in a female. He says that the dog is ready to mate and bear offspring. First blood occurs as early as six months to a year. Normally. up to two years. It happens once or twice a year. frequent bleeding may indicate the presence of hormonal disorders in the dog. How many days does it bleed, when estrus begins in representatives of different breeds, what measures should be taken by the owner during estrus in dogs. more on this in more detail.
If the owner does not want to mix a bitch with a dog, the main rule for him is not to let the dog off the leash for a while, while it is in heat. Even if the pet knows all the commands and obeys the owner, during this period of time it can become uncontrollable, run away, not approach on command. And it will be very difficult to drag the dog away, in which case, from the bitch.
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While estrus lasts, the owner should restrict his pet from participating in exhibitions for two reasons: firstly, at this time the behavior of the dog changes, and the owner cannot predict what she will do; and secondly, it can be dangerous due to the risk of accidental mating.
Some owners, having waited for the period when the dog's first estrus should begin approximately, do not notice it. Often in decorative dogs (sometimes in representatives of large breeds) bloodless estrus begins. During such a period, there are all signs of estrus, except for discharge: they are either not, or they are invisible. It also happens: there are no signs of heat, but she is coming.
In this case, the owner also needs to be on the lookout. Even if there is no discharge, the dog is ready for mating, and the males around him feel it.
Special tests will help determine if an animal is in bloodless heat. In any case, the animal should be shown to the veterinarian, as heat without blood is unnatural. The specialist will determine whether the dog's hormonal background is normal, and, if necessary, will prescribe a course of treatment.
Unusual estrus (longer than usual, no discharge, onset at the wrong time) in older dogs may be indicative of a tumor or disease.
How long dogs are in heat. the answer to this question is not very different for representatives of different breeds. Both in representatives of large and medium-sized breeds, and in small breeds, its duration is on average 20-30 days. Blood comes at intervals of 1-2 times a year.
During this period, the owner should be more careful about his pet. Only joint efforts can ease this difficult period.
How many times a year does a dog have estrus, how long does it last and what are its features. every dog breeder thinks about this. Heat usually occurs twice a year or three times in 14 months. For some breeds, it is individual and does not happen so often, but only once a year.
It is bad if the animal does not bleed for more than 8 months, or, on the contrary, it appears too often, with interruptions of less than 4 months. This may indicate the development of an animal's disease. Therefore, in this case, it is better to show the four-legged pet to the veterinarian.
The exact cycle of a dog of large or medium breeds is determined by 2 years. In decorative breeds a little earlier. at about the age of 18 months.
When a pet grows (up to a period of 1.5-2 years), different periods between estrus are the norm. Older dogs have a clearer cycle, although it may deviate by several weeks.
The dates when estrus begins and ends are shifted throughout the year, since its duration is not exactly one month. Therefore, the owner must record the beginning and end of estrus every time.
The frequency of estrus in dogs may differ depending on whether they are courtyard or domesticated. So, for the former, it takes place once a year, more often in early spring. The latter can have blood once or twice a year: in winter and autumn.
How long dogs are in heat. there is no one answer to this question. The duration may vary depending on a number of factors. For example, conditions of detention. So, if the bitch lives with animals of the opposite sex, the duration of estrus may be longer. If the pet is too loaded (training, training, physical exercise), then this period ends earlier than usual.
The duration of estrus in dogs may vary depending on the season. It often ends earlier in winter, while in summer its duration increases. But this does not apply to animals living in the apartment.
How long estrus lasts can be influenced by the girl's general well-being. Various diseases, pathologies, chronic diseases can affect the duration of the cycle.
In aged animals, the duration of the cycle is reduced, the "resting phase" increases from year to year. At the same time, estrus does not stop at all even in older bitches. Young people have a longer cycle.
During this period, the owner should record all manifestations: the beginning, how long it takes, what behavior the pet demonstrates. This data will help you notice any changes at some point.
Many owners are wondering if their pet needs special underpants for the estrus period. In their use, both pros and cons can be distinguished.
So, experts do not recommend using this hygienic device during estrus, since the animal must lick itself at this time.
But in some cases, owners use dog shorts during estrus. For example, if the dog is used to sleeping on the bed, or when traveling on public transport. to protect the dog from dirt during the period when it is most vulnerable.
When choosing hygienic pants, you should pay attention to the material: they must be sewn from natural fabrics, have a hole for the tail, and also be adjustable in volume. There should be no seams on the underpants so that they do not irritate the skin of the animal. Also, the thing should fit in size. the dog should be comfortable in it. There are options with Velcro, fasteners, and even overalls or suspenders. Depending on whether the dog is used to wearing clothes, the choice of model also depends. For girls-dogs, shorts are sewn with a special on the inside. It is designed for special gaskets.
Sometimes, in order to save money and if necessary, you can make such panties yourself, using cropped sliders or baby shorts.
The first estrus in a dog, at what age. this question is of interest to many owners. Usually the onset falls within a period of six months to two years. This is normal. Usually, the first estrus begins after the period of tooth change. Nobody knows the exact time. In animals of small breeds, blood begins to flow at the age of 6 to 10 months. In representatives of medium and large breeds, the timing is slightly different. the first estrus in a dog can begin in a period of time from six months to 13 months.
When a dog is in heat, the owner who plans to breed offspring should think about mating a pet. How many days should pass from the onset of estrus is an individual question for each dog. Records and observations of the dog during the previous period will help to understand when to send a pet for mating. With their help, you can determine auspicious days. This is usually 11-15 days from the onset of estrus.
It is better to mate before feeding the pets. Prerequisite: the bitch is brought to the male, and not vice versa. During this process, the animals should be in a calm environment, with as few people around as possible. Usually the dogs themselves deal with their amorous affairs. In rare cases, requires the participation of an instructor and a knitting specialist.
So, the owners of a girl dog should know the following: in the period from six months to two years, the animal should start estrus. If this does not happen, you must show the pet to the veterinarian. The owner should know how long the dog is in heat. This knowledge will help determine the most appropriate time for mating. The owner should be more attentive to the animal at this time. to walk exclusively on a leash, to protect it from participation in exhibitions and competitions. Some pets may have some character changes, this should also be taken into account.
Experienced owners know how to determine if a dog is in heat. And what about beginners who keep a pet girl for the first time? If the animal is over 6 months old, you should be on the lookout. To understand that the dog is in heat in the near future, the following signs will help:
The dog began to shed;
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The girl pees often;
Blood blotches may be present in the urine of an animal;
The behavior of the animal changes radically: an affectionate dog usually becomes a real fury, and a person with character turns into a submissive shy;
The behavior of the dog before heat can be aggressive towards other bitches;
Tags may appear in the apartment.
The listed signs of estrus in dogs are not present in every case. It happens that the pet does not behave suspiciously before the time "x". If the dog has reached the age of six months, the owner will have to be especially vigilant, watching the behavior of the animal, impurities in the urine, the state of the coat.
Pregnancy in dogs
Sometimes people, choosing a dog for themselves, refuse to buy a female animal because of fear of leaks, pregnancies, unwillingness to attach baby puppies to good hands. However, many problems can be avoided if, ahead of time, when the dog's first estrus has not yet begun, know about the intricacies of the processes taking place in the body of a sexually mature pet. So, let's look at the age at which estrus begins in dogs, what are its signs and how the dog behaves in such a difficult period, what kind of assistance should be provided to the animal, what can and cannot be done if the pet is in heat.
First, let's find out when to expect a "surprise" from the female. It's believed that the first estrus in dogs begins between 6 months and 2 years of age. over, in dogs of small breeds, estrus (the correct name for estrus) begins early. at 6, and sometimes even at 5 months. In medium-sized dogs, estrus usually begins at 8-12 months. And in large dogs, estrus occurs later than all. at 1-1.5 years, but sometimes even at 2 years. At the same time, it is impossible to name the exact time when the girl-dog will be ready for procreation.
AND how old do dogs have estrus? Theoretically, a pet can be ready for future fertilization up to a very respectable age. That is, at 10, and at 15, and even at 20 years old (if the animal manages to live to such an old age) there may be estrus, because the menopause in dogs simply does not exist.
Now it's time to find out the duration of this difficult period. How long does estrus last for dogs? small breeds? They usually have estrus for 20 days. In medium-sized dogs and large dogs, estrus can occasionally last up to 30 days. The duration of estrus in dogs may be slightly less than the indicated periods if the pet is elderly, moreover, the amount of discharge from her may be very small.
In this case, it is customary to divide the cycle into 4 stages, including:
Proestrus. the period when the canine vulva begins to swell. Lasts about 6-10 days. During proestrus, the canine body is preparing for ovulation, special hormones are released. estrogens, which contribute to the appearance of bloody discharge;
Estrus. in fact, this is the time when the pet develops an increased interest in doggies-boys. The loop becomes soft, puffiness decreases, the discharge changes to transparent or light pink. This stage in dogs usually lasts 7-9 days, and ovulation occurs on the 2-3rd day of the estrus period. Those owners who do not know on what day of estrus the dog should mate do it from the very first day of estrus, but it is better to wait 2 days after ovulation, when the eggs are formed;
Metestrus. in the body, ovulation gradually fades away with the help of the hormone progesterone produced. Discharge in the dog during metestrus gradually disappears. The animal ceases to look at males lustfully. This phase lasts for about 7-20 days;
Anestrus. dormant time, when the female either bears offspring, or is falsely pregnant, or simply does not want to communicate with four-legged "gentlemen", if fertilization for some reason did not occur. The duration of anestrus is approximately 5.5 months.
To the question, how often dogs are in heat also cannot be answered unequivocally. Usually, domestic bitches have a difficult period twice a year, mainly in spring and autumn (but it also happens in winter and summer). Yard dogs may be in heat once a year (more often in spring).
Heat in itself is not a disease, but sometimes bitches have problems during this period, which should be reported to the doctor as soon as possible. So, it is not good if the dog has:
Vomiting and categorical refusal to eat. with estrus the appetite of some bitches decreases, but does not disappear completely. When, after a small snack, the animal's stomach literally turns inside out, it's bad. Perhaps the pet has been poisoned, caught an infection, or has a disorder in the work of its internal organs;
If the time has come for metestrus, and the dog's discharge does not stop in any way, a hormonal failure may occur;
Normally, the discharge cannot be green, bright yellow, black. The fetid smell should also alert you. The dog may have an infection or genital inflammation;
When a dog's temperature rises above 39.5 during estrus. 40 degrees is a mess. Most likely, the animal got sick (viral and bacterial infections, allergies, oncology, poisoning, etc.).
To prevent estrus from becoming a nightmare, the owner of a girl dog will need these tips:
In order for the pet not to stain furniture, household clothes and carpets with secretions, the animal can wear special protective diapers. Pampers for girls in estrus are chosen in the appropriate size (from the smallest Small to the largest XXL). However, not all pets happily agree to wearing absorbent diapers. To prevent the animal from pulling the diaper with its teeth, it is better to wear overalls, pants or underpants for the dog during estrus;
If the tailed "lady" is categorically against diapers, it will be necessary to secure all the fabric surfaces in the house if possible: roll up carpets, cover sofas and beds with blankets;
During estrus, the pet attracts males like a magnet. During the period of "women's affairs" the dog should be walked only on a leash, reducing the time of the promenade so that the animal has time to fulfill its needs and run a little. Small dogs, accustomed to a home litter box, may not be allowed out into the street at all;
The behavior of a dog during estrus can unpleasantly surprise its owner: the pet may suddenly "forget" all the commands, although it previously strictly followed them. The owner needs to minimize the contact of the animal with the outside world during estrus;
During estrus, the canine genitals are prone to infections. Felting in the dust and swimming in open water should be excluded if the animal has estrus;
Bitches that mature should not participate in shows or competitions, and should not be taken on trips. If you neglect this rule, there will be harm to both the female and the dog, who will certainly feel that there is a "friend" nearby, ready to mate;
Have you ever seen funny short-legged mestizos born from the union of a large female and a short male (or vice versa)? Do not expect mating to fail if a dog of the "wrong" size is running on the court. It is better to keep the dog on a leash outside the apartment;
Even if the owner does not mind that the pet becomes pregnant, it is possible to rush to allow the dog to "meet" the males only after the third, at least second estrus, when the dog is older than 1.5 years (otherwise, a too young animal may even die during childbirth or have problems carrying puppies);
It is pointless to scold a dog that marks furniture and wallpaper, howls, ignores the words of the owner. It is better to distract the animal, for example, with some kind of game, a kind conversation. It is permissible to slightly soothe the animal with a remedy based on motherwort, valerian, passionflower or Scutellaria baikal (it is advisable to consult a veterinarian before use).
Sometimes the dog's discharge is too sparse for the owner to notice. If against the background of this, the pet behaves quietly, then it happens that the owner does not even know that the dog is in heat. Conversations about the fact that a dog can get pregnant without estrus is sometimes conducted by inexperienced dog breeders. So, pregnancy occurs only during ovulation, which takes place only during estrus. If an inexperienced (in appearance) bitch becomes pregnant, most likely, the owner simply did not notice the discharge.
In some situations, the owner does not want the animal to be in heat (for example, when the dog perceives abstinence from mating too painfully, has poor health for bearing offspring, etc.). To deprive the animal of the opportunity to give birth, sterilization is often carried out by ligating the fallopian tubes. But after such an intervention, estrus will still be present. If you remove the ovaries and uterus at the same time, there will be no heat. When sterilization is carried out correctly, the dog will cease to be of interest to individuals of the opposite sex and will forever lose the opportunity to have offspring.
Many owners of pet girls are interested in the question: is it possible to spay a dog during estrus? Veterinarians believe that it is better to carry out the intervention to remove the genitals when the hormonal background of the dog returns to normal, that is, during anestrus. Although sometimes sterilization is carried out during estrus, but resorting to the method of laparoscopy, when internal organs are removed through a small incision in the belly of the dog.
http://yorki-strizhka.ru/sobak/u-sobak-do-skolki-let-techka-do-kakogo-vozrasta-byvaet-techka-u-sobak-kogda-zakanchivaetsya.html
http://vmiresobak.com/uhod-za-sobakami/pervaya-techka-u-sobak-prodolzhitelnost-i-osobennosti.html
http://dogcatfan.com/352-techka-u-sobak.html
TAGS: dogs estrus | {
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