Solar abundances from gamma‐ray spectroscopy: Comparisons with energetic particle, photospheric, and coronal abundances
作者:
R. J. Murphy,
R. Ramaty,
B. Kozlovsky,
期刊:
AIP Conference Proceedings
(AIP Available online 1991)
卷期:
Volume 232,
issue 1
页码: 439-444
ISSN:0094-243X
年代: 1991
DOI:10.1063/1.40918
出版商: AIP
数据来源: AIP
摘要:
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 in3He‐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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