Computer Science
Scientific paper
May 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010eguga..12.5308b&link_type=abstract
EGU General Assembly 2010, held 2-7 May, 2010 in Vienna, Austria, p.5308
Computer Science
Scientific paper
For the solar system planets the non-thermal atmospheric escape exceeds by far the Jean escape for particles heavier than helium. In this talk we consider only ion escape and compare the total ion escape rates for Venus, Earth, and Mars caused by the interaction with the solar wind. The most recent data on the escape rates based on measurements from Mars Express, Venus Express, and Cluster show that despite large differences in the atmospheric masses (a factor of 100 - 200), different types of the interactions with the solar wind, the escape rates for Mars ,Venus, and the Earth are within the range 1024 - 1025s-1 . Surprisingly, the expected shielding of the Earth atmosphere by the intrinsic magnetic field is not as efficient as one may assume. The reason for this is the non-thermal escape caused by the solar wind interaction is an energy - limited process. The larger Earth's magnetosphere intercepts and tunnels down to the ionosphere more energy from the solar wind than more compact interaction regions of non-magnetized planets.
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