Ground-level energetic solar particle event on 24 May 1990 - Possibility of direct solar neutron detection

Details Ground-level energetic solar particle event on 24 May 1990 - Possibility of direct solar neutron detection Ground-level energetic solar particle event on 24 May 1990 - Possibility of direct solar neutron detection

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..144..195k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 144, no. 1, p. 195-198.

Physics

7

Solar Flares, Solar Neutrons, Solar Physics, Neutron Counters, Solar Atmosphere

Scientific paper

The first increase in neutron monitor count rate during the ground-level event on 24 May 1990 was interpreted by Shea et al. (1991) as a consequence of an arrival of flare neutrons. Debrunner et al. (1991) rejected the neutron hypothesis and proposed that the first neutron monitor increase was due to the arrival of primary protons. We have shown that neutron monitor data do not contradict the hypothesis of a neutron origin of the first increase of ground-level event on 24 May 1990.

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