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The Calculation of Solar Gamma-Rays by TALYS
Chen Wei ; Gan wei-qun
Source PublicationChinese Astronomy and Astrophysics
AbstractSolar gamma-ray lines, produced from nuclear reactions of accelerated particles interacting with the solar atmospheric medium, are the most direct diagnosis for the acceleration and transportation of energetic electrons and ions in solar flares. Much information about composition, spectrum, and angular distribution of the accelerated ions, as well as the elemental abundances of the ambient solar atmosphere can be derived from solar gamma-ray line spectra. A new gamma-ray calculation program has been developed by using an efficient nuclear code − TALYS. The theory of gamma-ray production in solar flares is treated in detail. The characteristics of gamma-ray spectrum are also presented.
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Recommended Citation
GB/T 7714
Chen Wei,Gan wei-qun. The Calculation of Solar Gamma-Rays by TALYS[J]. Chinese Astronomy and Astrophysics,2012,36(1):49-62.
APA Chen Wei,&Gan wei-qun.(2012).The Calculation of Solar Gamma-Rays by TALYS.Chinese Astronomy and Astrophysics,36(1),49-62.
MLA Chen Wei,et al."The Calculation of Solar Gamma-Rays by TALYS".Chinese Astronomy and Astrophysics 36.1(2012):49-62.
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