Stream Interactions in STEREO and THEMIS Data and Resulting Geomagnetic Activity

Details Stream Interactions in STEREO and THEMIS Data and Resulting Geomagnetic Activity Stream Interactions in STEREO and THEMIS Data and Resulting Geomagnetic Activity

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm31b1535m&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SM31B-1535

Physics

[2102] Interplanetary Physics / Corotating Streams, [2784] Magnetospheric Physics / Solar Wind/Magnetosphere Interactions, [2788] Magnetospheric Physics / Magnetic Storms And Substorms

Scientific paper

During this unusual solar minimum the decrease in solar activity has resulted in less geomagnetic activity. The observed activity, which ultimately arises from changes in the solar wind, has been from stream interaction regions (SIRs), shocks, and a few interplanetary coronal mass ejections (ICMEs). Stream interactions and shocks are identified in STEREO PLASTIC and ACE data and CMEs are identified in STEREO SECCHI. These events are studied in THEMIS data when the spacecraft are in dayside configuration. The propagation of these structures to the magnetopause, the resulting magnetospheric response, and any storm and substorm activity is discussed.

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