Cosmic γ-spectroscopy

I.L. Rozental’^a, V.V. Usov, I.V. Éstulin
^aSpace Research Institute, Russian Academy of Sciences, Profsoyuznaya str. 84/32, Moscow, 117997, Russian Federation

Features of the origin of $\gamma$-lines under cosmic conditions, the methodology of cosmic $\gamma$-spectroscopy, and the characteristics of $\gamma$-spectrometers are discussed. Observational data are provided on discrete ylines caused by solar flares as well as on those arising in cosmic objects outside the solar system. A possible interpretation of the detected $\gamma$-lines is discussed. In closing the article, the prospects of cosmic $\gamma$-spectroscopy are analyzed.

PACS: 94.40.Lx, 95.75.Fg, 95.85.Qx, 94.40.Cn
DOI: 10.1070/PU1979v022n01ABEH005415
URL: https://ufn.ru/en/articles/1979/1/c/
Citation: Rozental’ I L, Usov V V, Éstulin I V "Cosmic γ-spectroscopy" Sov. Phys. Usp. 22 46–60 (1979)

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Оригинал: Розенталь И Л, Усов В В, Эстулин И В «Космическая γ-спектроскопия» УФН 127 135–161 (1979); DOI: 10.3367/UFNr.0127.197901f.0135

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