The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.

Details The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere. The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufm.p13b1311w&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #P13B-1311

Physics

2102 Corotating Streams, 2154 Planetary Bow Shocks, 2164 Solar Wind Plasma, 2194 Instruments And Techniques

Scientific paper

Using the ASPERA-4 instrument onboard Venus Express the change in the atmospheric boundary layers are investigated. Using the instrument when it is in the apoapsis period of the polar orbit allows pure Solar Wind measurements to be taken. Composition ratios are determined thus identifying periods of fast and slow solar wind. This is then applied to ion maps of the Venusian atmosphere to determine the response after noise calibration methods. The Species reactions to the differing Solar Wind are also used to investigate the inner boundary movements.

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