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| Detailed Reference Information |
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Nagy, A.F., Kim, J., Cravens, T.E. and Kliore, A.J. (1998). Hot oxygen corona at Europa. Geophysical Research Letters 25: doi: 10.1029/1998GL900139. issn: 0094-8276. |
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A model of the hot oxygen exosphere at Europa was constructed. The source term for the hot atoms was assumed to be dissociative recombination of O2+ and Liouville's theorem was used to calculate their altitude distribution. It was found that near the surface the hot oxygen density is in excess of 200 cm-3, dropping to a value on the order of 50 cm-3 at 1500 km. These calculations indicate that the hot atomic oxygen densities are considerably less than the thermal molecular oxygen ones, but slightly larger than the measured sodium values. The escape flux of the hot oxygen atoms was calculated to be on the order of 1.4¿108 atoms cm-2 sec-1. This corresponds to a global escape rate of 4.4¿1025 atoms sec-1, which is more than an order of magnitude less than the estimated atmospheric sputtering rate. ¿ 1998 American Geophysical Union |
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Abstract |
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Keywords
Planetology, Solar System Objects, Jovian satellites, Planetology, Solid Surface Planets, Atmospheres—evolution, Planetology, Solid Surface Planets, Composition, Ionosphere, Planetary ionospheres (5435, 5729, 6026, 6027, 6028) |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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