The Lunar X-ray Observatory (LXO)/Magnetosheath Explorer in X-rays (MagEX)

被引:0
|
作者
Collier, M. R. [1 ]
Abbey, T. F. [2 ]
Bannister, N. P. [2 ]
Carter, J. A.
Choi, M. [1 ]
Cravens, T. [3 ]
Evans, M. [2 ]
Fraser, G. W.
Hills, H. K. [4 ]
Kuntz, K. [5 ]
Lyons, J. [1 ]
Omidi, N. [6 ]
Porter, F. S. [1 ]
Read, A. M. [2 ]
Robertson, I. [3 ]
Rozmarynowski, P. [1 ]
Sembay, S.
Sibeck, D. G. [1 ]
Snowden, S. L. [1 ]
Stubbs, T. [7 ]
Travnicek, P. [8 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Univ Leicester, Leicester, Leics, England
[3] Univ Kansas, Lawrence, KS 66045 USA
[4] Perot Syst Gov Serv, Fairfax, VA 22031 USA
[5] Johns Hopkins Univ, Baltimore, MD 21218 USA
[6] Solana Sci, Solomons, MD 92075 USA
[7] Goddard Earth Sci & Technol, Baltimore, MD 21250 USA
[8] Acad Sci Czech Republic, Prague, Czech Republic
来源
LOCAL BUBBLE AND BEYOND II | 2009年 / 1156卷
基金
美国国家航空航天局;
关键词
X-rays:diffuse background; EMISSION;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
X-ray observations of solar wind charge exchange (SWCX) emission, a nuisance to astrophysicists, will dramatically enhance our ability to determine the structure and variability of the Earth's magnetosheath. Such observations could be made from the lunar surface or an Earth-orbiting spacecraft and will resolve key controversies about magnetopause physics as well as better characterize SWCX emission with the aim of avoiding or removing it from astrophysical observations.
引用
收藏
页码:105 / +
页数:2
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