電子飛跡検出型広視野コンプトンカメラによるsub-MeV および MeV ガンマ線観測気球実験の結果と展望: SMILE 実験

• 資料種別: 規格・テクニカルリポート類
• タイトル: 電子飛跡検出型広視野コンプトンカメラによるsub-MeV および MeV ガンマ線観測気球実験の結果と展望: SMILE 実験
• 著者・編者: 谷森, 達; 服部, 香里; 株木, 重人; 窪, 秀利; 黒澤, 俊介; 井田, 知宏; 岩城, 智; 身内, 賢太郎; 水田, 栄一; 永吉, 勉; 西村, 広展; 野中, 直樹; 岡田, 葉子; 折戸, 玲子; 高田, 淳史; 高橋, 慶在; 上野, 一樹; Tanimori, Toru; Hattori, Kaori; Kabuki, Shigeto; Kubo, Hidetoshi; Kurosawa, Shunsuke; Ida, Chihiro; Iwaki, Satoru; Miuchi, Kentaro; Mizuta, Eiichi; Nagayoshi, Tsutomu; Nishimura, Hironobu; Nonaka, Naoki; Okada, Yoko; Orito, Reiko; Takada, Atsushi; Takahashi, Michiaki; Ueno, Kazuki
• 著者標目: 谷森, 達; 服部, 香里; 株木, 重人; 窪, 秀利; 黒澤, 俊介; 井田, 知宏; 岩城, 智; 身内, 賢太郎; 水田, 栄一; 永吉, 勉; 西村, 広展; 野中, 直樹; 岡田, 葉子; 折戸, 玲子; 高田, 淳史; 高橋, 慶在; 上野, 一樹; Tanimori, Toru; Hattori, Kaori; Kabuki, Shigeto; Kubo, Hidetoshi; Kurosawa, Shunsuke; Ida, Chihiro; Iwaki, Satoru; Miuchi, Kentaro; Mizuta, Eiichi; Nagayoshi, Tsutomu; Nishimura, Hironobu; Nonaka, Naoki; Okada, Yoko; Orito, Reiko; Takada, Atsushi; Takahashi, Michiaki; Ueno, Kazuki
• 出版事項: 宇宙航空研究開発機構
• 出版年月日等: 2010-03-31
• 出版年（W3CDTF）: 2010-03-31
• 並列タイトル等: Result and Prospect for Balloon-Borne Experiments of Sub-MeV and MeV Gamma-ray Astronomy using an Electron-Tracking Compton Camera
• タイトル（掲載誌）: 宇宙航空研究開発機構研究開発報告: 大気球研究報告
• 巻号年月日等（掲載誌）: JAXA-RR-09-007
• 掲載巻: JAXA-RR-09-007
• ISSN（掲載誌）: ISSN : 1349-1113
• 本文の言語コード: jpn
• 件名標目: MeV Gamma-ray Astronomy, Compton Gamma-ray Camera, Micro-Pixel Gas Chamber
• 対象利用者: 一般
• 一般注記: We developed the Electron-Tracking Compton Camera (ETCC) with reconstructing the track of a recoil electron in Compton process for both sub-MeV and MeV gamma rays to explore MeV gamma-ray astronomy in space. By adding the direction of a recoil electron to Compton reconstruction method, the direction of the incident gamma ray is determined for each individual photon. Also, an angle between the recoil electron and scattered gamma ray is powerful for the kinematical background-rejection. Since MeV gamma-ray astronomy has suffered from huge background so far, this new method is expected to increase the sensitivity. In the simulation, a 50 cm cubic ETCC would provide about 10 times better sensitivity than that of COMPTEL for one year observation in space. As a first step, we observed diffuse cosmic and atmospheric gamma rays at balloon altitudes with an ETCC consisting of the 10 cm cubic Time Projection Chamber (micro-TPC) and the GSO crystal pixel arrays surrounding the micro-TPC (SMILE-I). This instrument was launched on 1st September, 2006 from the Sanriku Balloon Center, and we successfully carried out about 3-hour observation time at an altitude of 32-35 km, and consequently obtained the both gamma-ray spectra between 0.1 and 1 MeV. In addition, this result indicates that the expected detection sensitivity of a future SMILE experiment between 150 keV and 20 MeV would provide a ten times better sensitivity than those of other missions at around 1 MeV. For the next balloon-borne experiment, we are developing a larger ETCC for detecting sub-MeV gamma rays from celestial point sources such as Crab and Cygnus X-1 during a few hours observation.; 形態: カラー図版あり; 著者人数: 17人; Physical characteristics: Original contains color illustrations; 資料番号: AA0064759002; レポート番号: JAXA-RR-09-007
• オンライン閲覧公開範囲: インターネット公開
• 掲載誌（NCID）: AA1192675X; https://ci.nii.ac.jp/ncid/AA1192675X
• 連携機関・データベース: 国立情報学研究所 : 学術機関リポジトリデータベース（IRDB）（機関リポジトリ）; https://irdb.nii.ac.jp
• 提供元機関・データベース: 宇宙航空研究開発機構 : 宇宙航空研究開発機構リポジトリ