Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...371..793m&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 371, April 20, 1991, p. 793-803.
Astronomy and Astrophysics
Astrophysics
108
Gamma Ray Spectra, Particle Emission, Photosphere, Solar Corona, Solar Flares, Energetic Particles, Solar Atmosphere, Solar Spectra, Spectrum Analysis
Scientific paper
Accelerated particle and ambient gas abundances have been derived using solar flare gamma-ray spectroscopy. The results with photospheric and coronal abundances, as well as with solar energetic particle abundances. This is the first time that the composition of accelerated particles interacting in an astrophysical source has been compared with the composition of particles escaping from the source. The analysis shows that the derived composition of the accelerated particles is different from the composition of particles observed in large proton flares; rather, it resembles the composition observed in He-3-rich flares. The analysis also suggests an ambient gas composition which differs from the composition of both the photosphere and the corona.
Kozlovsky Benz
Murphy Ronald J.
Ramaty Reuven
Reames Donald. V.
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