Cosmic-Ray Intensity Following a Solar Flare

Details Cosmic-Ray Intensity Following a Solar Flare Cosmic-Ray Intensity Following a Solar Flare

May 1950

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1950phrv...78..411b&link_type=abstract

Physical Review, vol. 78, Issue 4, pp. 411-414

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Scientific paper

Continuous records of the cosmic-ray intensity measured by a heavily shielded, high pressure ion chamber, were obtained during and following an intense solar flare (of importance 3+) and a subsequent intense magnetic storm. No increase in C-R intensity was observed at or near the time of the flare, such as have been observed by others on similar occasions. At the peak of the magnetic storm there was a decrease of about 1.5 percent in C-R intensity, with full recovery requiring 2 or 3 days. Unshielded C-R telescope readings of low accuracy are included. These indicate that there were no prolonged alterations in the intensity (without shielding) of magnitude much greater than 14 percent associated with either the flare or the storm.

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