Solar-polar coronal holes and the north-south cosmic ray gradient

Details Solar-polar coronal holes and the north-south cosmic ray gradient Solar-polar coronal holes and the north-south cosmic ray gradient

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978georl...5..589a&link_type=abstract

Geophysical Research Letters, vol. 5, July 1978, p. 589-591. National Research Council of Canada

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Cosmic Rays, Radiation Distribution, Solar Corona, Ogo-5, Skylab Program, Solar Rotation, Spatial Distribution, Vela Satellites

Scientific paper

We show, using Skylab measures of solar polar coronal hole areas, that
during non-disturbed periods the north-south gradient of galactic cosmic
rays as measured at 1 AU depends upon the difference in areas of the
polar coronal holes. Higher cosmic ray fluxes are observed from the
polar direction with the smaller coronal hole area.

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