Heliographic-latitude dependence of the cosmic-ray intensity

Details Heliographic-latitude dependence of the cosmic-ray intensity Heliographic-latitude dependence of the cosmic-ray intensity

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974georl...1..302a&link_type=abstract

Geophysical Research Letters, vol. 1, Nov. 1974, p. 302-304.

Physics

6

Cosmic Rays, Galactic Radiation, Particle Flux Density, Radiation Distribution, Solar Cycles, Annual Variations, Earth Orbits, Radiant Flux Density, Solar Wind Velocity, Spectroheliographs

Scientific paper

Evidence for a semiannual variation in the galactic cosmic-ray intensity is presented. This effect can be associated with the heliographic latitude excursion of the earth during its orbital motion. Therefore the phase evaluation of the semiannual variation can be used to infer the direction of the cosmic-ray gradient perpendicular to the solar equatorial plane through the solar cycle.

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