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The JEM-EUSO Project: Observing Extremely High Energy Cosmic Rays and Neutrinos from the International Space Station
https://repo.qst.go.jp/records/45189
https://repo.qst.go.jp/records/451895e206978-d173-4ebc-800d-84f9bbe43f20
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2008-06-11 | |||||
タイトル | ||||||
タイトル | The JEM-EUSO Project: Observing Extremely High Energy Cosmic Rays and Neutrinos from the International Space Station | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
Ebisuzaki, T.
× Ebisuzaki, T.× Bertaina, M.E.× Uchihori, Yukio× et.al× 内堀 幸夫 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The Japanese Experiment Module - Extreme Universe Space Observatory (JEM-EUSO) is a super wide-field telescope to observe Extremely High Energy Cosmic Rays (EHECR) and neutrinos with energy above 1019eV from the International Space Station (ISS), orbiting at an altitude of about 430 km from ground. JEM-EUSO will image the fluorescence light emitted by the atmospheric molecules of nitrogen excited during the development of the Extensive Air Shower (EAS) generated by the interaction of a EHECR or neutrino at the top of the atmosphere. It will also detect part of the ˇCerenkov light produced during the shower development and reflected at the impact point (land, sea or clouds). |
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書誌情報 |
Nuclear Physics B - Proceedings Supplements 巻 175/176, p. 237-240, 発行日 2008-01 |
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ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0920-5632 |