Stationary and nonstationary modulation of cosmic rays

Details Stationary and nonstationary modulation of cosmic rays Stationary and nonstationary modulation of cosmic rays

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2103a&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Statistics

Computation

Computational Astrophysics, Cosmic Rays, Energy Spectra, Forbush Decreases, Interplanetary Magnetic Fields, Modulation, Particle Energy, Radiant Flux Density, Solar Cycles, Temporal Distribution

Scientific paper

The stationary and nonstationary equations of cosmic ray propagation are solved depending on primary particle energy in an investigation of cosmic-ray variations in a wide range of energies (high-energy for nonstationary modulation and low-energy for stationary modulation). An analysis is then made of the effect of the sector structure of the interplanetary magnetic field on cosmic-ray anisotropy at the minimum of the 20th solar cycle. Also studied are time variations of the energy spectrum of Forbush effects for the initial phase of cosmic-ray intensity decrease according to data from neutron monitors for 1969-1971.

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