NASA NTRS ยท 20080043891
Solar Wind Change Exchange from the Magnetosheath
Abstract
We 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.
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Snowden, Steve. 2008-04-20. Solar Wind Change Exchange from the Magnetosheath. https://ntrs.nasa.gov/citations/20080043891
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