A high-energy increase in cosmic-ray intensity

Details A high-energy increase in cosmic-ray intensity A high-energy increase in cosmic-ray intensity

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991cajph..69..984v&link_type=abstract

Canadian Journal of Physics (ISSN 0008-4204), vol. 69, Aug.-Sept. 1991, p. 984-987.

Physics

Cosmic Rays, High Energy Interactions, Neutron Counters, Forbush Decreases, Solar Flares

Scientific paper

The increase in cosmic rays observed by neutron monitors with high-energy cutoff, on April 29, 1973, is interpreted to be a definite high-energy phenomenon. This is not associated with any solar flare or interplanetary disturbance. The association of the increase in intensity with geomagnetic index Dst variation indicates a possibility that the high-energy event was caused by a magnetospheric phenomenon.

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