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#474990
Sun 23 Sep 2018 08:18:PM
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Joined: Feb 2001
Posts: 381,904
Launch Director
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Joined: Feb 2001
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Abstract: Condensation clouds in substellar atmospheres have been widely inferred from spectra and photometric variability. Up until now, their horizontally averaged vertical distribution and mean particle size have been largely characterized using models, one of which is the eddy diffusion-sedimentation model from Ackerman and Marley that relies on a sedimentation efficiency parameter, f(sub sed), to determine the vertical extent of clouds in the atmosphere. However, the physical processes controlling... Source: Sedimentation Efficiency of Condensation Clouds in Substellar Atmospheres
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Sedimentation Efficiency of Condensation Clouds in Substellar Atmospheres
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Sun 23 Sep 2018 08:18:PM
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