Observations of energetic helium ions in the earth's radiation belts during a sequence of geomagnetic storms

Details Observations of energetic helium ions in the earth's radiation belts during a sequence of geomagnetic storms Observations of energetic helium ions in the earth's radiation belts during a sequence of geomagnetic storms

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jgr....86.2317s&link_type=abstract

Journal of Geophysical Research, vol. 86, Apr. 1, 1981, p. 2317-2328.

Physics

19

Energetic Particles, Geomagnetism, Helium Ions, Magnetic Storms, Magnetospheric Instability, Radiation Belts, Charge Exchange, Distribution Functions, Energy Dissipation, Equatorial Regions, Explorer 45 Satellite, Ionic Collisions, Ionic Diffusion, Solar Flares, Solar Terrestrial Interactions

Scientific paper

Observations of energetic (MeV) helium ions made with Explorer 45 during a sequence of magnetic storms during June through December of 1972 are presented. It is noted that the first of these storms started on June 17 and had a Dst index excursion to -190 gamma and that the MeV helium ions were perturbed primarily beyond 3 earth radii in the equatorial radiation belts with a typical flux increase of an order of magnitude at L equal to 4. The second storm period was in August and was associated with very major solar flare activity. While the Dst extremum was at best 35 gamma less than the June storm, this period can be characterized as irregular (or multi-storm) with strong compression of the magnetosphere and very large (order of magnitude) MeV helium ion flux enhancements down to L approximately equal to 2. After this injection, the trapped helium ion fluxes showed positive spherical slope with the peak beyond 3.15 MeV at L equal to 2.5; at the lowest observable L shells, little flux decay was seen during the remainder of the year.

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