Europa's sodium atmosphere: An ocean source?

被引:42
|
作者
Leblanc, F [2 ]
Johnson, RE
Brown, ME
机构
[1] Univ Virginia, Charlottesville, VA USA
[2] CNRS, Serv Aeron, F-91371 Verrieres Le Buisson, France
[3] CALTECH, Pasadena, CA 91125 USA
基金
美国国家科学基金会;
关键词
Europa; surface; satellite; atmosphere; composition;
D O I
10.1006/icar.2002.6934
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Sputtering and decomposition of Europa's surface by energetic ions and electrons produce an atmosphere. Here we use a 3D Monte Carlo simulation, including collisions with the background O-2 atmosphere, to describe recent measurements of the sodium component of the atmosphere. By constraining the model with the observational data, we attempt to reconstruct the source processes, the energy distribution, and the flux of the ejected sodium. We confirm that electronic sputtering from ice-rich regions dominates the ejecta and that Europa loses between 5 and 10 x 10(6) Na cm(-2) s(-1). This is about one order of magnitude more sodium than that implanted from the jovian magnetosphere. (C) 2002 Elsevier Science (USA).
引用
收藏
页码:132 / 144
页数:13
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