Modeling cloud microphysics using a two-moments hybrid bulk/bin scheme for use in Titan’s climate models: Application to the annual and diurnal cycles
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference38 articles.
1. Cloud formation along mountain ridges on Titan;Barth;Planet. Space Sci.,2010
2. TRAMS: A new dynamic cloud model for Titan’s methane clouds;Barth;Geophys. Res. Lett.,2007
3. Convective cloud heights as a diagnostic for methane environment on Titan;Barth;Icarus,2010
4. Microphysical modeling of ethane ice clouds in titan’s atmosphere;Barth;Icarus,2003
5. Properties of methane clouds on Titan: Results from microphysical modeling;Barth;Geophys. Res. Lett.,2004
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1. Development of a new cloud model for Venus (MAD-VenLA) using the Modal Aerosol Dynamics approach;Advances in Space Research;2023-01
2. Superrotation on Venus, on Titan, and Elsewhere;Annual Review of Earth and Planetary Sciences;2018-05-30
3. Brownian coagulation of a bi-modal distribution of both spherical and fractal aerosols;Journal of Aerosol Science;2017-03
4. GCM simulations of Titan’s middle and lower atmosphere and comparison to observations;Icarus;2015-04
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