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

页码：105 / +

页数：2

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