The depletion of the solar wind near Mars

Details The depletion of the solar wind near Mars The depletion of the solar wind near Mars

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..143l&link_type=abstract

Advances in Space Research, vol. 20, p. 143

Computer Science

2

Solar Wind, Mars Atmosphere, Charge Exchange, Helium Ions, Oxygen Ions, Magnetospheric Ion Density, Radiation Absorption, Hydrogen Ions, Magnetosheath

Scientific paper

The present investigation of the charge exchange-mediated absorption of the solar wind by the Martian atmosphere notes that the H(+) + O yields H + O(+) can result in significant depletion of the solar wind in a small region above subsolar space. The He(+) ions created by charge exchange have no function in the total He(+) outflow at Mars. A comparison is conducted between the flux of O(+) ions with Phobos 2 data.

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