Post-storm cosmic ray increases and the radiation belt

Details Post-storm cosmic ray increases and the radiation belt Post-storm cosmic ray increases and the radiation belt

May 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965jatp...27..635t&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 27, no. 5, pp. 635-640

Physics

Scientific paper

Post-storm cosmic ray increases observed recently by (1961a) have been studied following a Chree analysis for the neutron intensity data of fourteen selected stations for the I.G.Y. period. These increases are shown to be the general feature of all geomagnetic storms specially those followed by a long quiet-period. They may have their origin in the outer radiation belt. The local acceleration mechanism in the outer radiation belt has been developed which correlates these increases with the recent satellite observations of the outer radiation belt during a geomagnetic storm.

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