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Solar flare particle fluences during solar cycles 19, 20 and 21Satellite data for solar flare particle events during solar cycle 21 (up to July 1982) have been analyzed to obtain event-integrated fluxes of energetic protons and alpha particles. Thirty nine events with proton fluences (E greater than 10 MeV) greater than 10-million/sq cm occurred during 1976-1982. The average flux of protons with kinetic energy greater than 10 MeV is 65 per sq cm/s for this period. The event averaged alpha to proton ratio, in the energy interval 1-22 MeV/n, varies between 0.006 to 0.04, with an average value of about 0.02 for the whole cycle. The flux of protons (with energies greater than 10 MeV) averaged over cycle 21 is lower than those for solar-cycle 20 per sq cm/s based on satellite data, and for solar-cycle 19 378 per sq cm/s based on lunar sample data. There is no definitive correlation between solar-cycle averaged proton fluxes and sunspot numbers.
Document ID
19850040720
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Mcguire, R. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Goswami, J. N.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Jha, R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lal, D.
(Physical Research Laboratory Ahmedabad, India)
Reedy, R. C.
(Max-Planck-Institut fuer Chemie, Mainz, West Germany; Los Alamos National Laboratory, Los Alamos NM, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1983
Subject Category
Solar Physics
Meeting Information
Meeting: International Cosmic Ray Conference
Location: Bangalore
Country: India
Start Date: August 22, 1983
End Date: September 3, 1983
Accession Number
85A22871
Distribution Limits
Public
Copyright
Other

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