The Lunar X-ray Observatory (LXO)∕Magnetosheath Explorer in X-rays (MagEX)
Author(s) -
M. R. Collier,
Tony Abbey,
N. Bannister,
Jennifer Carter,
Michael K. Choi,
T. E. Cravens,
Megan Evans,
G.W. Fraser,
H. K. Hills,
K. D. Küntz,
J. Lyons,
N. Omidi,
F. S. Porter,
A. M. Read,
I. P. Robertson,
P. Rozmarynowski,
S. Sembay,
D. G. Sibeck,
S. L. Snowden,
T. J. Stubbs,
P. Trávnı́ček,
Randall K. Smith
Publication year - 2009
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.177
H-Index - 75
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.3211802
Subject(s) - magnetosheath , magnetopause , physics , observatory , spacecraft , solar wind , charge exchange , astronomy , astrobiology , astrophysics , plasma , ion , quantum mechanics
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.
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