Solar neon abundances from gamma-ray spectroscopy and He-3-rich particle events

Details Solar neon abundances from gamma-ray spectroscopy and He-3-rich particle events Solar neon abundances from gamma-ray spectroscopy and He-3-rich particle events

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...332l..87r&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 332, Sept. 15, 1988, p. L87-L91.

Astronomy and Astrophysics

Astrophysics

18

Gamma Ray Spectrometers, Helium, Neon, Solar Atmosphere, Solar Flares, Solar Wind, Abundance, Coronal Loops, Radio Emission, X Ray Spectroscopy

Scientific paper

The authors compare ambient solar atmospheric abundances derived from gamma-ray spectroscopy with observations of solar energetic particles. They find agreement between the gamma-ray derived Ne/O ratio and the corresponding mean ratio for 3He-rich flares. Both of these values are significantly higher than inferred coronal Ne/O ratios. It is suggested that the mean Ne/O ratio in 3He-rich flares reflects the composition of the flare plasma rather than the acceleration process.

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