North-south asymmetry in the distribution of galactic cosmic rays

Details North-south asymmetry in the distribution of galactic cosmic rays North-south asymmetry in the distribution of galactic cosmic rays

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1817s&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1817-1819. In Russian.

Computer Science

Asymmetry, Galactic Cosmic Rays, Particle Motion, Interplanetary Magnetic Fields, Solar Wind Velocity, Velocity Distribution

Scientific paper

The global survey technique is used to determine the solar wind velocity, the isotropic intensity of galactic cosmic rays (GCRs), and the north-south component of the GCR current for two successive revolutions of the sun during June-August 1974. The direction of the north-south component of the GCR current is shown to depend on the sign of the interplanetary magnetic field. In addition, a scheme for the formation of the radial density gradient of cosmic rays in high-velocity solar-wind streams is presented.

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