Solar Wind Charge Exchange in the Chandra Deep Field-South During Solar Max and Min

Details Solar Wind Charge Exchange in the Chandra Deep Field-South During Solar Max and Min Solar Wind Charge Exchange in the Chandra Deep Field-South During Solar Max and Min

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.205w&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Computer Science

Solar

Scientific paper

Uniquely among X-ray deep field observations, the Chandra Deep Field-South contains data collected both during Solar Maximum (1999 and 2000) and during Solar Minimum (2007). These 2 Ms of data also sample lines of sight through and to the side of the solar helium focusing cone. When combined with data on solar wind composition from the ACE satellite, these observations permit studies of the effects of solar wind variability and viewing geometry (through the heliosphere and geocorona) on SWCX emission, and strongly constrain the level of hot-gas emission from the Local Bubble.

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