Polar Coronal Holes and Cosmic-Ray Modulation
A. J. HUNDHAUSEN 1,
D. G. SIME 1,
R. T. HANSEN 1, and
S. F. HANSEN 1
1 High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado 80307
A comparison of the size of polar coronal holes with the cosmic-ray intensity observed during the most recent sunspot cycle shows close correspondence. This lends support to recent suggestions that the well-known sunspot-cycle modulation of cosmic rays is a three-dimensional effect, probably related to the global character of the interplanetary magnetic field.
Submitted on September 14, 1979