期刊
GEOPHYSICAL RESEARCH LETTERS
卷 31, 期 22, 页码 -出版社
AMER GEOPHYSICAL UNION
DOI: 10.1029/2004GL020953
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A hybrid simulation of the solar wind-Mars interaction and a test particle simulation of heavy ion trajectories near Mars are used to compute the contribution from solar wind charge exchange processes to the X-ray emission from Mars. It is found that the X-ray halo observed by the Chandra X-ray observatory can be explained by emissions from heavy, highly charged, ions in the solar wind undergoing charge exchange collisions in the upper atmosphere of Mars.
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