Solar polar coronal holes and galactic cosmic ray intensities

Details Solar polar coronal holes and galactic cosmic ray intensities Solar polar coronal holes and galactic cosmic ray intensities

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85.6845a&link_type=abstract

Journal of Geophysical Research, vol. 85, Dec. 1, 1980, p. 6845-6852. Natural Sciences and Engineering Research Council of Cana

Physics

4

Coronal Holes, Cosmic Rays, Galactic Radiation, Solar Activity Effects, Solar Terrestrial Interactions, Asymmetry, Data Correlation, Neutron Counters, Particle Intensity, Polar Regions, Solar Corona

Scientific paper

A comparison between the areas of solar polar coronal holes and N-S cosmic ray asymmetries measured by polar region neutron monitors showed that the N-S asymmetries during 1973-74 were related to asymmetries in the dimensions of solar polar holes. The hemisphere with the smaller hole has a larger cosmic ray flux; the N-S asymmetry is small in the presence of a symmetric coronal region about the solar equator. Various mechanisms relating to a N-S asymmetry are discussed.

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