Solar influence on galactic cosmic ray anisotropy measurements

Details Solar influence on galactic cosmic ray anisotropy measurements Solar influence on galactic cosmic ray anisotropy measurements

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.260..507k&link_type=abstract

Nature, vol. 260, Apr. 8, 1976, p. 507, 508.

Physics

1

Cosmic Rays, Galactic Radiation, Magnetic Effects, Particle Flux Density, Solar Wind, Anisotropy, Electromagnetic Fields, Particle Intensity, Particle Trajectories, Periodic Variations, Solar Activity Effects, Solar Magnetic Field

Scientific paper

The phase of sidereal intensity variation in the energy range 100 billion to 1 trillion electron volts was observed to shift from about 1800 to about 330 LST when the solar magnetic field reversed in 1969 (Hill and Silk, 1975). Based on an examination of individual particle trajectories a model is proposed which attributes the observed anisotropy to the electromagnetic field embedded in the solar wind.

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