Spectra of solar proton ground level events using neutron monitor and neutron moderated detector recordings

Details Spectra of solar proton ground level events using neutron monitor and neutron moderated detector recordings Spectra of solar proton ground level events using neutron monitor and neutron moderated detector recordings

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..114s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 114-117 (SEE N85-34729 23-92)

Physics

Cosmic Ray Showers, Helium Ions, Neutron Counters, Relativistic Velocity, Solar Flares, Solar Protons, Solar Spectra, Alpha Particles, Least Squares Method, Remote Sensing

Scientific paper

Recordings on relativistic solar flare protons observed at Sanae, Antarctic, show that the percentage increase in counting rates of the neutron moderated detector (4NMD) is larger than the percentage increase in counting rates of the 3NM64 neutron monitor. These relative increases are described by solar proton differential spectra js(P) = AP(beta). The power beta is determined for each event and the hardnesses of the temporal variations of beta, found for the ground level events (GLE) of 7 May, 1978 and 22 November, 1977.

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