NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Nuclear processes and neutrino production in solar flaresThe determination of flare neutrino flux is approached from the standpoint of recent observations and theoretical results on the nuclear processes in solar flares. Attention is given to the energy spectra and total numbers of accelerated particles in flares, as well as their resulting production of beta(+)-emitting radionuclei and pions; these should be the primary sources of neutrinos. The observed 0.511 MeV line flux for the June 21, 1980 flare is compared with the expected from the number and spectrum of accelerated particles.
Document ID
19860052900
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lingenfelter, R. E.
(California, University La Jolla, United States)
Ramaty, R.
(California Univ. La Jolla, CA, United States)
Murphy, R. J.
(California Univ. La Jolla, CA, United States)
Kozlovsky, S.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Subject Category
Solar Physics
Accession Number
86A37638
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available