Cosmic Ray and UV Radiation Models on the Ancient Martian Surface

The atmospheric evolution on Mars is influenced by nonthermal loss processes of heavy atmospheric constituents. Since Mars does not have an appreciable intrinsic magnetic field at present and a comparatively small gravitational acceleration, all known atmospheric loss processes can be active and sev...

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Veröffentlicht in:	Icarus (New York, N.Y. 1962) N.Y. 1962), 2001-11, Vol.154 (1), p.216-222
Hauptverfasser:	Molina-Cuberos, G.J, Stumptner, W, Lammer, H, Kömle, N.I, O'Brien, K
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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