Nuclear gamma-ray line ratios as spectral diagnostics for protons accelerated in solar flares

Details Nuclear gamma-ray line ratios as spectral diagnostics for protons accelerated in solar flares Nuclear gamma-ray line ratios as spectral diagnostics for protons accelerated in solar flares

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..170..240c&link_type=abstract

AIP Conference Proceedings, Volume 170, pp. 240-245 (1988).

Physics

1

Scientific paper

New and revised gamma-ray production cross sections are employed to calculate the expected 15.10- to 4.438-MeV line ratio for proton interactions with carbon and oxygen as a function of parameters characterizing the incident proton spectrum in a solar flare. The additional cross sections for which inadequate determinations cause significant uncertainties in the results of this calculation are identified.

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