Expected contribution of Hall-type diffusion to cosmic ray anisotropy and comparison with experiment

Details Expected contribution of Hall-type diffusion to cosmic ray anisotropy and comparison with experiment Expected contribution of Hall-type diffusion to cosmic ray anisotropy and comparison with experiment

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979sogru..93...49a&link_type=abstract

Akademiia Nauk Gruzinskoi SSR, Soobshcheniia, vol. 93, Jan. 1979, p. 49-52. In Russian.

Physics

Cosmic Rays, Hall Effect, Interplanetary Magnetic Fields, Magnetic Diffusion, Anisotropy, Differential Equations, Diurnal Variations, Neutron Counters, Radiant Flux Density, Solar Wind Velocity

Scientific paper

Data from neutron counters at the Deep River station from 1964 were used to determine the contribution of Hall-type diffusion to the anisotropy of cosmic rays in interplanetary space. The first harmonic coefficients of the solar-diurnal variations of cosmic ray intensity were calculated and averaged as a function of IMF direction. It is found that the occurrence of Hall-type diffusion is associated with changes of the IMF sector structure.

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