The pitch-angle anisotropy of solar protons according to stratospheric measurements

Details The pitch-angle anisotropy of solar protons according to stratospheric measurements The pitch-angle anisotropy of solar protons according to stratospheric measurements

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982izssr..46.1709b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Samarkand, Uzbek SSR, Oct. 27-29, 1981.) Akademiia Nauk SSSR, Izvestiia, Ser

Computer Science

Sound

Anisotropic Media, Balloon Sounding, Pitch (Inclination), Solar Protons, Angular Distribution, Satellite Observation, Solar Flares, Stratosphere

Scientific paper

The pitch-angle distribution of solar protons in the 100-300 MeV energy range was investigated on the basis of balloon data acquired over the Apatity. A number of spectra obtained by a single Geiger counter and a coincidence telescope at the beginning of August 1972 are presented. The data indicate that the appearance of anisotropy with a maximum at large pitch angles corresponds to a closed magnetosphere. An open magnetosphere is characterized by an isotropy of particles with energies not less than 100 MeV penetrating into the geomagnetic field before the atmospheric boundary.

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