Dependence of the north-south anisotropy of cosmic rays on the orientation of interplanetary shock waves

Details Dependence of the north-south anisotropy of cosmic rays on the orientation of interplanetary shock waves Dependence of the north-south anisotropy of cosmic rays on the orientation of interplanetary shock waves

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ge%26ae..15..401r&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 15, May-June 1975, p. 401-404.) Geomagnetism and Aeronomy, vol. 15, Oct. 1975, p. 332-334. Tra

Physics

Geophysics

Cosmic Rays, Forbush Decreases, Interplanetary Magnetic Fields, Radiation Distribution, Shock Waves, Anisotropy, Geophysics, Solar Wind

Scientific paper

The north-south anisotropy of cosmic rays at onset times of Forbush decreases is analyzed as a function of the azimuth angles of normals to interplanetary shock fronts. The difference between onset times of Forbush decreases detected at northern and southern stations is calculated using a simple geometric model of a field with normal vectors and an interplanetary magnetic field lying strictly in the plane of the ecliptic. It is shown that the gradient cosmic-ray flux is an important factor in the observed anisotropy.

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