Cosmic ray anisotropy relevant to high-velocity solar wind fluxes

Details Cosmic ray anisotropy relevant to high-velocity solar wind fluxes Cosmic ray anisotropy relevant to high-velocity solar wind fluxes

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10..178k&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 10 (A85-22801

Physics

Coronal Holes, Galactic Cosmic Rays, Solar Wind Velocity, Anisotropy, Isotropy, Solar Flux Density

Scientific paper

The behavior of galactic cosmic rays in the periods when the earth traverses high-velocity solar wind fluxes (HVF) is examined. A network of neutron monitors was used to study the value and direction of the anisotropy arising in the region of HVF interaction with steady solar wind. Magnetic field in HVF is shown to be of a more regular character than in a steady solar wind.

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