Observations of Energetic Particles From the Polar Cap to the Equator During the April 2002 Storms

Details Observations of Energetic Particles From the Polar Cap to the Equator During the April 2002 Storms Observations of Energetic Particles From the Polar Cap to the Equator During the April 2002 Storms

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsa21b0438a&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SA21B-0438

Physics

2716 Energetic Particles, Precipitating, 2730 Magnetosphere: Inner, 2731 Magnetosphere: Outer, 2778 Ring Current, 2788 Storms And Substorms

Scientific paper

Geomagnetic storms can be studied from the polar cap to the equator at several local times using low-altitude spacecraft data. The unique data coverage offered by NOAA-15 and 16 is indeed very useful, since huge geomagnetic storms are affecting the ionosphere both at high and low latitudes. In the polar cap intense precipitation of MeV protons takes place, and at low L-values a Storm Time Equatorial Belt (STEB) of trapped protons and energetic neutral atoms appears. In this paper we employ multi-spacecraft data to study the April 2002 storms.

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