Wind-induced atmospheric escape: Titan
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/gl1216/2012GL052774/2012GL052774.pdf
Reference30 articles.
1. Simulating the one-dimensional structure of Titan's upper atmosphere: 2. Alternative scenarios for escape;Bell;J. Geophys. Res.,2010
2. Distribution and escape of molecular hydrogen in Titan's thermosphere and exosphere;Cui;J. Geophys. Res.,2008
3. The implications of the H2 variability in Titan's exosphere;Cui;J. Geophys. Res.,2011
4. Wind enhanced planetary escape: Collisional modifications;Curtis;J. Geophys. Res.,1977
5. Cassini ion and neutral mass spectrometer data in Titan's upper atmosphere and exosphere: Observation of a suprathermal corona;De La Haye;J. Geophys. Res.,2007
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1. Enhanced Hydrogen Escape on Mars during the 2018 Global Dust Storm: Impact of Horizontal Wind Field;The Astrophysical Journal;2023-08-01
2. Wind‐Enhanced Hydrogen Escape on Mars;Geophysical Research Letters;2022-05-13
3. The thermal structure of Titan’s upper atmosphere, II: Energetics;Icarus;2014-01
4. Diffusion and thermal escape of H2 from Titan’s atmosphere: Monte Carlo simulations;Icarus;2013-01
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