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Escape of Planetary Atmospheres
2012The extreme radiation and plasma environments during the period of the young active Sun/Stars have important implications for the evolution of planetary atmospheres and may be responsible that planets with a low gravity like early Mars most likely could never build up a dense atmosphere during the first few 100 Myr after their origin. On the other hand
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Izvestiya, Atmospheric and Oceanic Physics, 2017
A. Vigasin, I. I. Mokhov
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A. Vigasin, I. I. Mokhov
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Motions in planetary atmospheres
Quarterly Journal of the Royal Meteorological Society, 1976openaire +2 more sources
Comparative planetary nitrogen atmospheres: Density and thermal structures of Pluto and Triton
, 2017D. Strobel, Xun Zhu
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