Abundances from solar-flare gamma-ray line spectroscopy

Details Abundances from solar-flare gamma-ray line spectroscopy Abundances from solar-flare gamma-ray line spectroscopy

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..249m&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 4 p 249-252 (SEE N85-34729 23-92)

Physics

1

Abundance, Galactic Radiation, Gamma Ray Spectra, Line Spectra, Nuclear Particles, Nuclear Radiation, Photosphere, Solar Flares, Ambient Temperature, Emission Spectra, Gamma Ray Bursts, Ionized Gases, Ionizing Radiation, Solar Atmosphere, Solar Cosmic Rays

Scientific paper

Elemental abundances of the ambient gas at the site of gamma-ray line
production in the solar atmosphere are deduced using gamma-ray line
observations from 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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