Solar abundances from gamma-ray spectroscopy: Comparisons with energetic particle, photospheric, and coronal abundances

Details Solar abundances from gamma-ray spectroscopy: Comparisons with energetic particle, photospheric, and coronal abundances Solar abundances from gamma-ray spectroscopy: Comparisons with energetic particle, photospheric, and coronal abundances

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..232..439m&link_type=abstract

Gamma-ray line astrophysics. AIP Conference Proceedings, Volume 232, pp. 439-444 (1991).

Astronomy and Astrophysics

Astrophysics

Composition

Scientific paper

We have derived accelerated particle and ambient gas abundances using solar flare gamma-ray spectroscopy. We find that the derived accelerated particle composition is different from the composition observed in large proton flares; rather, it resemble that observed in 3He-rich flares. Our analysis also suggests that the ambient composition differs from the composition of both the photosphere and the corona.

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