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- W2181825918 abstract "Using nitrate enhancements in the polar ice as a proxy for solar proton events, we have determined the proton fluence above 30 MeV for 31 solar cycles between 1610 and 1954 (cycle -12 through cycle 18). Our results show a wide range of solar proton fluences over these 31 solar cycles, from three cycles with no significant proton events above 10 9 cm -2 to a high of 38 x 10 9 cm -2 . In a comparison of the two cycles with the highest solar proton fluence, we find that cycle 10 was dominated by one major event (the Carrington event in 1859) while cycle 13 had 7 major events contributing to the total fluence. The to- tal fluence for most cycles is within a factor of 2 of the maximum fluence per cycle meas- ured by spacecraft since 1965. Until new deep ice cores are available for both calibration with known fluences and for verification of the original results, these derived solar proton fluences over a number of solar cycles represent the only available values as upper limits for space exploration experiments." @default.
- W2181825918 created "2016-06-24" @default.
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- W2181825918 date "2007-01-01" @default.
- W2181825918 modified "2023-09-27" @default.
- W2181825918 title "SOLAR PROTON FLUENCE FOR 31 SOLAR CYCLES DERIVED FROM NITRATE ENHANCEMENTS IN POLAR ICE" @default.
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