Understanding the Solar Wind interactions with the Venusian boundary layers

Details Understanding the Solar Wind interactions with the Venusian boundary layers Understanding the Solar Wind interactions with the Venusian boundary layers

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009eguga..11.4712w&link_type=abstract

"EGU General Assembly 2009, held 19-24 April, 2009 in Vienna, Austria http://meetings.copernicus.org/egu2009, p.4712"

Physics

Scientific paper

The ASPERA-4 (Analyser of Space Plasmas and Energetic Atoms) instrument onboard Venus Express is used to investigate Bow Shock and Ionopause positions. The movement of these layers during Fast-Slow stream Solar Wind interaction is looked at as well as during Solar events. The methods of determining Solar events from the data are shown as well as a brief discussion on how the data has been specifically cleaned up.

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