Quasi-drift effects of high-energy solar cosmic rays in the magnetosphere

Details Quasi-drift effects of high-energy solar cosmic rays in the magnetosphere Quasi-drift effects of high-energy solar cosmic rays in the magnetosphere

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....9817423s&link_type=abstract

Journal of Geophysical Research, Volume 98, Issue A10, p. 17423-17428

Astronomy and Astrophysics

Astrophysics

2

Interplanetary Physics: Cosmic Rays, Magnetospheric Physics: Energetic Particles, Precipitating, Solar Physics, Astrophysics, And Astronomy: Energetic Particles

Scientific paper

The structure of high-energy solar proton penetration zones in the polar and subpolar regions using data from riometers, transpolar satellite DMSP-F6, and neutron monitors during an extremely anisotropic solar proton event on February 16, 1984, has been studied. Particular emphasis was placed upon interpretation of the solar proton intensity maximum located at the auroral and nearby latitudes. Precipitation of quasi-trapped particles drifting along the latitudinal direction from the entry site of the anisotropic flux at the dawnside of the magnetosphere is discussed as a cause of this maximum.

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