Origin of cosmic ray fluctuations

Details Origin of cosmic ray fluctuations Origin of cosmic ray fluctuations

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..391k&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, May-June 1980, p. 391-395. In Russian.

Computer Science

3

Cosmic Rays, Galactic Radiation, Interplanetary Medium, Neutrons, Arctic Regions, Forbush Decreases, Interplanetary Magnetic Fields, Magnetohydrodynamic Waves, Plasma Turbulence, Shock Wave Propagation

Scientific paper

The origin of neutron-component fluctuations with periods ranging from 10 min to 10 hr, observed during the passage of interplanetary shock waves, is examined. An analysis of the energy-dependence of the pulsation amplitude during magnetically disturbed periods indicates that the structure of Forbush decreases of galactic cosmic rays is produced by modulation of the cosmic ray gas by a packet of interacting hydromagnetic waves of various scales.

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