Physics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsa21b0448z&link_type=abstract
American Geophysical Union, Fall Meeting 2002, abstract #SA21B-0448
Physics
2704 Auroral Phenomena (2407), 2716 Energetic Particles, Precipitating, 2736 Magnetosphere/Ionosphere Interactions, 2784 Solar Wind/Magnetosphere Interactions, 2788 Storms And Substorms
Scientific paper
During the major magnetic storms on April 17-20, 2002, TIMED/GUVI observed a new feature of dayside auroras: a separated diffused auroral oval at magnetic latitudes below 70 degrees. Such auroral feature was very dynamic and did not exist all the time. Energetic electrons/protons drifting from the night side magnetosphere may be the source of the auroras. We will discuss the IMF and magnetospheric conditions for the auroras to occur.
Avery S.
Christensen A.
Craven J.
Crowley Geoff
Kil Hyosub
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