Intensity and Energy Spectrum of Fast Neutrons in Cosmic Radiation
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概要
- 論文の詳細を見る
The intensity and the energy spectrum of low energy neutrons at Mt. Norikura (2740m above sea level and 25°N geomagnetic latitude) were obtained by observing recoil protons with the randomly operated high pressure cloud chamber filled with hydrogen gas at the pressure of 92 atm. The differential energy spectrum for neutrons in the energy range from I Mev to 15 Mev was found to be expressed by (1.2±40%) × 10^<-3> × E^<-1・25±0.10>cm^<-2> sec^<-1> sterad^<-1> Mev^<-1>. The neutron flux is in conformity with what one would expect from the density of thermal neutrons. Connecting the present data with the others which were obtained by many investigations in different energy ranges, the energy spectrum of neutrons ranging from 1ev to 10Bev are discussed.
- 1957-02-05
著者
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HINOTANI Kensaku
Institute of Polytechnics, Osaka City University
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Miyake Saburo
Institute Of Polytechnics Osaka City University
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Hinotani Kensaku
Institute Of Polytechnics Osaka City University
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NUNOGAKI Kan-ichi
Institute of Polytechnics, Osaka City University
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Nunogaki Kan-ichi
Institute Of Polytechnics Osaka City University
関連論文
- All Experimental Study of Extensive Air Showers
- Cosmic Ray Nuclear Interactions in Nitrogen GaS
- Intensity and Energy Spectrum of Fast Neutrons in Cosmic Radiation
- A Cloud Chamber Study of the Cosmic-Ray Hard Showers
- An Analysis of Experimental Data on Extensive Air Showers