text:   From Microphysical Cloud Modeling",9,"['Inhomogeneous clouds can be observed in transmission even with limited wavelength coverage, uncertainty on limb darkening coefficients, and imprecise transit times in a way that is statistically robust! See my new paper to learn why and how: <LINK>', 'Both the east and west limb often form clouds, but that the different properties of these clouds enhances the limb to limb differences compared to the clear atmosphere case. https://t.co/x3XRvqZnDx', 'Using JWST it should be possible to detect the presence of cloud inhomogeneities by comparing the shape of the transit lightcurve at multiple wavelengths because inhomogeneous clouds impart a characteristic, wavelength dependent signature https://t.co/MUIodCPjrZ', 'Probing limb inhomogeneity on hot Jupiters due to clouds can be statistically robust even with limited wavelength coverage, uncertainty on limb darkening coefficients, and imprecise transit times! https://t.co/gQW2OUDYg2', 'The signatures due to clouds in these models are key in observing inhomogeneity! Check out the paper for predictions about cloud properties and their impact on the observed spectra!', ""Also don't forget to consider cloud particle size distributions!  Using the area or mass weighted particle size significantly alters the relative strength of the cloud spectral features compared to using the predicted size distribution. https://t.co/R0MTSaVyW1"", 'In short, we can use cloud physics to probe fundamental atmospheric properties like limb inhomogeneity! This work was done in collaboration with @TomLouden_b, @lkreidberg, Xi Zhang, @PlanetaryGao, and @V_Parmentier \n\n#dreamteam #cloudsarefriends\nhttps://t.co/GqurZ0jzHb', '@henrifdrake thank you!!!', '@Of_FallingStars @TomLouden_b @lkreidberg @PlanetaryGao @V_Parmentier thank you!!!']",19,10,1665