A study of the pitch-angular anisotropy of cosmic rays using data from a world-wide station network

Details A study of the pitch-angular anisotropy of cosmic rays using data from a world-wide station network A study of the pitch-angular anisotropy of cosmic rays using data from a world-wide station network

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izssr..48.1447d&link_type=abstract

(Vsesoiuznaia Konferentsiia po Optike Lazerov, 4th, Leningrad, USSR, Jan. 13-18, 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fi

Physics

Cosmic Ray Showers, Forbush Decreases, Interplanetary Magnetic Fields, Angular Distribution, Anisotropy, Energy Spectra, Particle Flux Density, Radiation Counters, Spectrographs

Scientific paper

Reference is made to recent studies in which attention has been given to the effect of strong cosmic ray anisotropy in pitch-angular space during Forbush decreases. The existence of such an anisotropy makes it possible to determine the electromagnetic conditions prevailing in the interplanetary space. In particular, a method (based on global spectrographic survey) is proposed which provides information on the interplanetary magnetic field orientation in addition to information on the variance of the angular and energy distribution of cosmic rays.

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