Three‐dimensional, multispecies, high spatial resolution MHD studies of the solar wind interaction with Mars

By Yingjuan Ma, A. Nagy, Igor M. Sokolov, K. Hansen. 2004

274 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/14c9bbc4eaec4b469c24e9236a99973b6fc06577

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In Astronomy and Astrophysics

1. Matthias Grott
2. A. Morschhauser
3. H. Lammer
4. Ernst Hauber
5. Yingjuan Ma
6. C. Dong
7. P. Odert
8. O. Cohen

Citations in the corpus

• Influence of the solar EUV flux on the Martian plasma environment (2005, unknown): “The present understanding of this interaction has been recently reviewed by Mazelle et al. (2004) and Nagy et al. (2004).”
• Outgassing History and Escape of the Martian Atmosphere and Water Inventory (2015, result): “The value suggested initially by Melosh and Vickery (1989), n = 1, has been revised by more recent studies to n= 10 (Vickery 1990; Manning et al. 2006). On the other hand, the more recent hydrocode simulations performed by Shuvalov and Artemieva (2001), Ivanov et al.”
• Is Proxima Centauri b Habitable? A Study of Atmospheric Loss (2017, methodology): “One of the primary scientific goals of NASA’s Mars Atmosphere and Volatile EvolutioN (MAVEN) mission is to determine the escape rates, which are crucial because of their potential impact on the long-term evolution of the Martian atmosphere (e.g., loss of water).”
• Electron pitch angle distributions as indicators of magnetic field topology near Mars (2007, unknown): “A global MHD simulation showed closed field lines on the nightside [Ma et al., 2002, 2004], and test particles traced in this model demonstrate how photoelectrons from the Martian dayside might travel along field lines and be observed in the induced magnetotail [Liemohn et al., 2006].”
• The plasma Environment of Mars (2004, methodology): “Some of this trans-terminator flux, will flow down on the nightside and help to maintain the nightside ionosphere, while the rest will escape through the tail (Ma et al., 2002; 2004).”