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Solar Wind Change Exchange from the MagnetosheathWe report the results of a long (approximately 100 ks) XMM-Newton observation designed to observe solar wind charge exchange emission (SWCX) from Earth's magnetosheath. By luck, the observation took place during a period of minimal solar wind flux so the SWCX emission was also minimal. Never-the-less, there is a significant if not stunning correlation between the observed O VIII count rate and our model for magnetosheath emission. We also report on the observed O VII and O VII emission.
Document ID
20080043891
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Snowden, Steve (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 24, 2013
Publication Date
April 20, 2008
Subject Category
Solar Physics
Meeting Information
Meeting: Local Bubble and Beyond II conference
Location: Philadelphia, PA
Country: United States
Start Date: April 20, 2008
End Date: April 24, 2008
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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