Storm-time increase in cosmic ray intensity and its characteristics.

Details Storm-time increase in cosmic ray intensity and its characteristics. Storm-time increase in cosmic ray intensity and its characteristics.

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992chjss..12..270y&link_type=abstract

Chin. J. Space Sci., Vol. 12, No. 4, p. 270 - 278

Physics

Scientific paper

The cosmic ray increases due to considerable depressions of cosmic ray cut off rigidity during large geomagnetic storms are investigate. Data from 11 superneutron monitors in world network are analyzed for six geomagnetic storms of various type during 1984 - 1989. The results show that the storm-time increases are due to the existence of westward equatorial ring currents developing or intensifying during geomagnetic storms.

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