Background conditions aboard the KORONAS-I satellite as measured by the AVS instrument

Yu D. Kotov, A. S. Glyanenko, S. V. Bogovalov, I. V. Belousova, V. Yu Kovalen', V. D. Malashkevich, A. Yu Sokolov, A. V. Dmitriev, S. N. Kuznetsov, S. P. Ryumin, A. S. Udalov, S. I. Boldyrev, V. Yu Klepikov, A. I. Stepanov

研究成果: 雜誌貢獻期刊論文同行評審

摘要

Data concerning the spectra of background x-ray and gamma-ray radiations at various segments of an orbit of the KORONAS-I satellite in the range from 30 keV to 50 MeV are presented. The background spectra were measured by a detector with a crystal CsI(Tl). At a minimum counting rate, the background is approximated by a function with two power law exponents. When compared to the SMM satellite, the experimental background conditions aboard KORONAS-I are shown to be only slightly worse: the background counting rate of the AVS instrument insignificantly exceeds the corresponding SMM counting rate. Thereby, good conditions for recording solar flares and gamma ray bursts are provided.

原文???core.languages.en_GB???
頁(從 - 到)155
頁數1
期刊Cosmic Research
37
發行號2
出版狀態已出版 - 3月 1999

指紋

深入研究「Background conditions aboard the KORONAS-I satellite as measured by the AVS instrument」主題。共同形成了獨特的指紋。

引用此