The Geoeffectiveness of High Speed Solar Wind Streams: Ionospheric Effects

Details The Geoeffectiveness of High Speed Solar Wind Streams: Ionospheric Effects The Geoeffectiveness of High Speed Solar Wind Streams: Ionospheric Effects

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsa31b..03t&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SA31B-03

Physics

2134 Interplanetary Magnetic Fields, 2164 Solar Wind Plasma, 2407 Auroral Ionosphere (2704), 2431 Ionosphere/Magnetosphere Interactions (2736), 2441 Ionospheric Storms (7949)

Scientific paper

There are a number of different coupling mechanisms for getting solar wind energy into the magnetosphere during high speed solar wind intervals. These will be reviewed. Specifically recent time intervals have been empirically studied to quantify these effects and the effects of coordinate transformations of the interplanetary parameters. The results of this recent study will be presented together with possible interpretations.

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