Instruments for the Observation of Galactic X-Rays
スポンサーリンク
概要
- 論文の詳細を見る
Three types of rocket-borne X-ray instruments were constructed; they consists of a scintillation counter, four proportional counters, and twenty-three GM counters respectively. The scintillation counter was used to observe isotropic X-rays in the energy ranges of 5∼10, 10∼15, 15∼20 and >__-20 KeV, and the proportional counters to observe the intensities of X-rays from several sources in the energy ranges of 2∼4, 4∼8 and 7∼11 Å. Their properties were tested by radioactive sources and were found to be suitable for analyzing the energy spectrum of galactic X-rays while rejecting charged particles. Two of the counter systems were used for the observations of X-rays, and the method of data analysis as well as some of the raw data are discribed.
- 社団法人応用物理学会の論文
- 1966-08-15
著者
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Matsuoka Masaru
Department Of Physics Nagoya University:(present Address) Institute Of Space And Aeronautical Scienc
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Matsuoka Masaru
Department Of Applied Chemistry College Of Engineering University Of Osaka Prefecture
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