Angular distributions of solar protons and electrons

Details Angular distributions of solar protons and electrons Angular distributions of solar protons and electrons

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975p%26ss...23.1179n&link_type=abstract

Planetary and Space Science, vol. 23, Aug. 1975, p. 1179-1194.

Physics

1

Angular Distribution, Interplanetary Magnetic Fields, Solar Electrons, Solar Protons, Anisotropy, Lines Of Force, Ogo-5, Solar Flares, Time Response

Scientific paper

High angular-resolution measurements of directional fluxes of solar particles in space have been obtained with detectors aboard OGO-5 during the cosmic ray event of Nov. 18, 1968. This is the only case on record for which sharply-defined directional observations of protons and electrons covering a wide rigidity range (0.3 MV to 1.5 GV) are available. The satellite experiment provided data for determining pitch-angle distributions with respect to the direction of the local interplanetary magnetic field lines during the lengthy highly anisotropic phase of the event. The results have been interpreted in the light of the temporal flux profiles and the state of the interplanetary medium.

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