Nuclear line spectroscopy of solar flares

Details Nuclear line spectroscopy of solar flares Nuclear line spectroscopy of solar flares

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..118..123f&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 118, no. 1-2, 1988, p. 123-135.

Astronomy and Astrophysics

Astrophysics

16

Energy Spectra, Gamma Ray Spectra, Line Spectra, Nuclear Astrophysics, Solar Flares, Abundance, Astronomical Models, Energetic Particles, Line Shape

Scientific paper

The study of nuclear line spectra from solar flares holds a rich promise for elucidating the properties of both the accelerated particles and the interaction or target region. The authors review the observations and the analysis of the large nuclear line rich flare which occurred near the west limb starting at 08:03 UT on 27 April, 1981. The observed spectrum from this flare contains three intense and isolated gamma-ray lines which can be analyzed in a model independent way. Elemental abundances of the ambient gas at the site of gamma-ray line production in the solar atmosphere are deduced. The resultant abundances are different from local galactic abundances which are thought to be similar to photospheric abundances.

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