Cosmic ray gradients in the heliosphere and particle drifts

Details Cosmic ray gradients in the heliosphere and particle drifts Cosmic ray gradients in the heliosphere and particle drifts

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981georl...8..619n&link_type=abstract

Geophysical Research Letters, vol. 8, June 1981, p. 619-622.

Physics

26

Cosmic Rays, Heliosphere, Particle Motion, Protons, Coronal Holes, Galactic Radiation, Gradients, Latitude, Particle Trajectories, Solar Wind

Scientific paper

K-coronameter, solar wind, and neutron monitor data are used to estimate the latitudinal gradient of protons of approximately 5 GeV in the heliosphere at 1 AU during 1965 and 1975. The reversal of sign of the gradient between 1965 and 1975 and the strong positive latitudinal gradient in 1975 predicted by models in which drifts are dominant are not observed.

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