Applicability of Polyimide Films as Etched-Track Detectors for Ultra-Heavy Cosmic Ray Components
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概要
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The track registration property in polyimide Kapton has been examined for heavy ions, including 2.3 GeV Fe and 24 GeV Xe ions. Conventional track formation criteria fail to predict the thresholds of etch pit formation, while a chemical criterion stating that etchable tracks are formed when two adjacent diphenyl ethers are broken in the vicinity of the ion's trajectory should be more appropriate. Discriminative detections of ultra-heavy components in cosmic rays, such as Bi, Th, and U ions, are possible by measuring the recorded track length.
- 2013-04-25
著者
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Yasuda Nakahiro
Research Center For Radiation Safety National Institute Of Radiological Sciences
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Barillon Rémi
Institute Pluridisciplinaire Hubert Curien (UMR7178), Strasbourg Cedex 2, France
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ODA Keiji
Graduate School of Maritime Sciences, Kobe University
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MATAI Yuri
Graduate School of Maritime Sciences, Kobe University
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KODAIRA Satoshi
National Institute of Radiological Sciences
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KANASAKI Masato
Graduate School of Maritime Sciences, Kobe University
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Kitamura Hisashi
National Institute for Radiological Sciences, 4-9-1 Anagawa, Inage, Chiba 263-8555, Japan
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KONISHI Teruaki
National Institute of Radiological Sciences
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MATSUKAWA Kenya
Graduate School of Maritime Sciences, Kobe University
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YAMAUCHI Tomoya
Graduate School of Maritime Sciences, Kobe University
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HATTORI Atsuto
Graduate School of Maritime Sciences, Kobe University
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MORI Yutaka
Graduate School of Maritime Sciences, Kobe University
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Tao Akira
Graduate School of Maritime Sciences, Kobe University, Kobe 658-0022, Japan
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Kusumoto Tamon
Graduate School of Maritime Sciences, Kobe University, Kobe 658-0022, Japan
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