GeV Proton Detection in the 8 November 2000 Solar Event

UNIVERSE(2022)

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摘要
In this study, we analyze the L3 precision muon spectrometer data from November 2000. The results showed that a 4.7 sigma muon excess appeared at a time coincident with the solar flare of 8 November 2000. This muon excess corresponded to primary protons above 40 GeV, coming from a sky cell of solid angle 0.048 sr. The probability of being a background fluctuation was estimated to be about 0.1%. It is interesting and noteworthy that an M-class solar flare may also accelerate solar protons to such high energies.
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关键词
solar flares, solar energetic protons, ground level enhancement (GLE), muon enhancements, muon drift chamber, neutron monitor (NM)
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