Magnetic field draping around Mars:: Mars global surveyor results

被引:20
|
作者
Crider, D [1 ]
Acuña, M
Connerney, J
Mitchell, D
Lin, R
Cloutier, P
Rème, H
Mazelle, C
Brain, D
Ness, N
Bauer, S
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA
[3] Rice Univ, Houston, TX 77251 USA
[4] Ctr Etud Spatiale Rayonnements, Toulouse, France
[5] Univ Colorado, Boulder, CO 80309 USA
[6] Univ Delaware, Bartol Res Inst, Newark, DE USA
[7] Graz Univ, Graz, Austria
来源
PLANETARY IONOSPHERES | 2001年 / 27卷 / 11期
关键词
D O I
10.1016/S0273-1177(01)00333-7
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We investigate the contribution of the radial component of the magnetic field in the solar wind interaction with Mars. We use Mars Global Surveyor Magnetometer and Electron Reflectometer data during the Science Phasing Orbits to gain a qualitative understanding of the magnitude of the radial magnetic field from the solar wind draping around the dayside of Mars. Using only data far away, from the strong crustal magnetic sources, we find that the angle the magnetic field makes to the horizontal within the martian ionosphere has an average closer to zero than that outside the ionosphere. However, we find a much larger spread in angles inside the ionosphere. In addition, we find that the angle of inclination increases with increasing altitude and local time, but more spatial coverage is needed to quantify these relationships. (C) 2001 COSPAR. Published by Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:1831 / 1836
页数:6
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