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annotations_creators: |
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- no-annotation |
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language: |
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- en |
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language_creators: |
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- other |
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license: |
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- mit |
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multilinguality: |
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- monolingual |
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pretty_name: LIFD Magnetic Fields |
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size_categories: [] |
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source_datasets: [gufm1 model] |
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tags: [] |
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task_categories: |
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- feature-extraction |
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- image-to-image |
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- time-series-forecasting |
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- object-detection |
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- unconditional-image-generation |
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task_ids: |
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- multivariate-time-series-forecasting |
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You will need the package |
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https://chaosmagpy.readthedocs.io/en/master/ |
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A description of the dataset: |
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The gufm1 model is a global geomagnetic model based on spherical harmonics, covering the period 1590 - 1990, and is described in the publication: |
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Andrew Jackson, Art R. T. Jonkers and Matthew R. Walker (2000), “Four centuries of geomagnetic secular variation from historical records”, Phil. Trans. R. Soc. A.358957–990, http://doi.org/10.1098/rsta.2000.0569 |
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The native model representation is converted into a discrete dataset in physical space and time, using the Python package https://chaosmagpy.readthedocs.io/en/master/ |
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The dataset has dimension (181, 361, 401) whose axes represent co-latitude, longitude, time, and whose values are the radial magnetic field at the core-mantle boundary (radius 3485km) in nT. |
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The colatitude takes values (in degrees): 0,1,2,3,…180; longitude (degrees) takes values -180,-179,….180; and time is yearly 1590, 1591, …1990. |