Three-dimensional multispecies MHD studies of the solar wind interaction with Mars in the presence of crustal fields

By Yingjuan Ma, A. Nagy, K. Hansen, D. Dezeeuw, Tamas I. Gombosi, Kenneth G. Powell. 2002

166 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/c755890193002a14e4e86a752a44d00f637ce8cd

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In Astronomy and Astrophysics

1. H. Lammer
2. I. Ribas
3. J. Owen
4. Yingjuan Ma
5. H. Lichtenegger
6. Igor M. Sokolov
7. R. Abart
8. E. Guinan

Citations in the corpus

• Loss of water from Mars: Implications for the oxidation of the soil (2003, background): “Based on numerical studies, McElroy (1972), McElr and Donahue (1972), and Liu and Donahue (1976) fo”
• 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].”
• Influence of the solar EUV flux on the Martian plasma environment (2005, unknown): “These studies have been carried out using different approaches like gas dynamics models ( Spreiter and Stahara , 1992), MHD models ( Tanaka, 1993; Liu et al., 1999; Liu et al., 2001; Ma et al., 2002; Ma et al., 2004), and a bi-ion MHD model (Sauer et al.”
• Three‐dimensional, multispecies, high spatial resolution MHD studies of the solar wind interaction with Mars (2004, methodology): “We started out with singlespecies, axisymmetric assumptions, and in our last paper we presented results from a three-species, three-dimensional (3-D) model of the solar wind interaction with Mars, including the effects of the crustal magnetic field and mass loading [ Ma et al., 2002 ].”
• 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).”