Evidence for negative charging of the lunar surface in shadow -: art. no. 1435

被引:79
|
作者
Halekas, JS [1 ]
Mitchell, DL
Lin, RP
Hood, LL
Acuña, MH
Binder, AB
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] Lunar Res Inst, Tucson, AZ 85747 USA
关键词
D O I
10.1029/2001GL014428
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
[1] Observations of electron distributions above the shadowed surface of the Moon show energy-dependent loss cones which indicate reflection by both magnetic and electric fields. At the same time, low energy (less than or similar to100 eV) field aligned upward-going electron beams are observed. Together, these observations imply average night-side potential differences between the surface and the Lunar Prospector (LP) spacecraft of 35 V. The lunar surface may be at an even higher negative potential relative to the ambient plasma, since LP will likely also charge negative. The potential difference is consistent with simple current balance models which include secondary emission. No clear dependence is found on surface terrane type and age, or on ambient electron density and temperature. Instead, the potential difference is found to depend strongly on the angle from the subsolar point and the angle between the magnetic field and the normal to the lunar surface.
引用
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页码:77 / 1
页数:4
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