Solar abundances using gamma-ray line spectroscopy of a solar flare

Details Solar abundances using gamma-ray line spectroscopy of a solar flare Solar abundances using gamma-ray line spectroscopy of a solar flare

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..170..228m&link_type=abstract

AIP Conference Proceedings, Volume 170, pp. 228-233 (1988).

Computer Science

Abundances, Chemical Composition

Scientific paper

Elemental abundance of the ambient gas at the site of gamma-ray line
production in the solar atmosphere are deduced using gamma-ray line
observations of a solar flare. The resultant abundances are different
from local galactic abundances which are thought to be similar to
photospheric abundances.

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