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1 チベット高原での高エネルギー 宇宙線の研究 瀧田正人東京大学宇宙線研究所平成 17 宇宙線研究所 16/12/2005 (For Tibet Asγcollaboration)
2 平成 17 年度チベット実験関係の共同利 用研究採択課題一覧 1. チベット高原での高エネルギー宇宙線の研究 ( 瀧田正人東京大学宇宙線研究所 ) 2. 宇宙線による太陽の影を用いた太陽周辺磁場の時間変動の観測 ( 山本嘉昭甲南大学理工学部 ) 3. 定常的または一時的ガンマ線放射の点源及び天体の探索 ( 坂田通徳甲南大学理工学部 ) 4. チベット空気シャワーアレイによる超新星残骸及びその他の活動的天体からのガンマ線の探索 ( 水谷興平埼玉大学理学部 ) 5.Knee 領域一次宇宙線組成の研究 ( 柴田槇雄横浜国立大学大学院工学研究院 ) 6.Knee 領域一次宇宙線全粒子スペクトルの研究 ( 堀田直己宇都宮大学教育学部 ) 7.Sidereal daily variation of ~10TeV galactic cosmic ray intensity observed by the Tibet air shower array ( 宗像一起信州大学理学部 )
3 チベットグループ共同利用研究 経費執行状況 校費 : 申請額 495 万円 -> 配分額 220 万円 2002 年に完成した Tibet-III の維持 運転及び将来計画のための R&D 費用の一部に使用 旅費 : 申請額 805 万円 -> 配分額 265 万円 宇宙線研でのグループミーティング (25 人程度 ) 開催 /1-2 ヶ月宇宙線研での解析ミーティング / 必要な時チベット出張海外旅費
4 The Tibet ASγ Collaboration Papers (in refereed journals): Are protons still dominant at the knee of the cosmic-ray energy spectrum?, to be published in Phys. Lett B. Observation of PeV Gamma Rays from the Monogem Ring with the Tibet Air Shower Array, ApJ 635, L53-L56. A Northern Sky Survey for Steady Tera-Electron Volt Gamma-Ray Point Sources Using the Tibet Air Shower Array, ApJ, 633, p Large-Scale Sidereal Anisotropy of Galactic Cosmic-Ray Intensity Observed by the Tibet Air Shower Array, ApJ, 626, L29-L32. International Conference/Proceedings: 29th International Cosmic Ray Conference (Pune, India 2005) 17 talks/posters and proceedings papers Aspen2005 (Aspen, U.S.A. 2005) 1 talk and proceedings paper
5 研究目的 大気チェレンコフ望遠鏡と相補的な広視野 ( 約 2sr2 sr) 連続観測高エネルギー宇宙線望遠鏡 3~100TeV の高エネルギーガンマ線放射天体の探索 ~10 17 の一次宇宙線の観測から 宇宙線の起源 加速機構の研究を行う 太陽活動期における 太陽の影 ( 太陽による宇宙線の遮蔽効果 ) を観測し 太陽近傍および惑星間磁場の大局的構造を知る
6 Collaborators The Tibet ASγ Collaboration M. Amenomori 1, S.Ayabe 2, S.W. Cui 3, Danzengluobu 4, L.K. Ding 3, X.H. Ding 4, C.F. Feng 5, Z.Y. Feng 6, X.Y. Gao 7, Q.X. Geng 7, H.W. Guo 4, M. He 5, K. Hibino 8, N. Hotta 9, H.B. Hu 3, J. Huang 9, Q. Huang 6, H.Y.Jia 6, F.Kajino 11, K. Kasahara 12, Y. Katayose 13, K.Kawata 11, Labaciren 4, C.L. Lan 3, G.M. Le 14, J.Y. Li 5, H.Lu 3, S.L. Lu 3, X.R. Meng 4, K. Mizutani 2, J.Mu 7, H. Nanjo 1, M. Nishizawa 15, M. Ohnishi 10, I. Ohta 9, T. Ouchi 10, S. Ozawa 9, J.R. Ren 3, T. Saito 16, M. Sakata 11, T. Sasaki 8, M. Shibata 13, A. Shiomi 10, T. Shirai 8, H. Sugimoto 17, K. Taira 17, M. Takita 10, Y.H. Tan 3, N.Tateyama 8, S. Torii 8, H. Tsuchiya 10, S.Udo 2, T. Utsugi 8, B.S. Wang 3, H. Wang 3, Y.G. Wang 5, L. Xue 5, X.X. Zhou 6, X.C. Yang 7, Y. Yamamoto 11, Z.H.Ye 14, G.C.Yu 6, A.F. Yuan 4, T. Yuda 18, H.M. Zhang 3, J.L. Zhang 3, N.J. Zhang 5, X.Y. Zhang 5, and Zhaxisangzhu 4 1 Department of Physics, Hirosaki University, Hirosaki , Japan 2 Department of Physics, Saitama University, Saitama , Japan 3 Laboratory of Cosmic Ray and High Energy Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing , China 4 Department of Mathematics and Physics, Tibet University, Lhasa , China 5 Department of Physics, Shangdong University, Jinan , China 6 Institute of Modern Physics, South West Jiaotong University, Chengdu , China 7 Department of Physics, Yunnan University, Kunming , China 8 Faculty of Engineering, Kanagawa University, Yokohama , Japan 9 Faculty of Education, Utsunomiya University, Utsunomiya , Japan 10 Institute for Cosmic Ray Research, University of Tokyo, Kashiwa , Japan 11 Department of Physics, Konan University, Kobe , Japan 12 Faculty of Systems Engineering, Shibaura Institute of Technology, Saitama , Japan 13 Faculty of Engineering, Yokohama National University, Yokohama , Japan 14 Center of Space Science and Application Research, Chinese Academy of Sciences, Beijing , China 15 National Institute for Informatics, Tokyo , Japan 16 Tokyo Metropolitan College of Aeronautical Engineering, Tokyo , Japan 17 Shonan Institute of Technology, Fujisawa , Japan 18 Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya , Japan
7 Our site : Tibet Yangbajing, Tibet, China 90 53E, 30 11N, 4,300 m a.s.l. (606g/cm 2 )
8 Tibet Airshower Array Tibet III (37000m 2 ) Yangbajing (4300a.s.l.=606g/cm 2 ), Tibet, China Total 789 detectors Mode Energy ~3 TeV Angular Resolution ~0.9 Trigger Rate ~1700 Hz
9 月の影 と 地磁気効果 観測された月の影 影の南北のズレ 影の西へのズレ
10 ~1000 days Tibet-HD (555.9 Crab days) Mrk421 北天探査 ( 最頻エネルギー約 2TeV) 0.1 刻み 2,160,000(3600x600) 点 Dec. Crab Tibet-III (456.8 days) R.A. HD + III Crab Mrk421
11 北天 TeV ガンマ線 90% フラックス上限値 2-3 TeV ApJ, 633, , (2005) Milagrito U.L. 90% (2001) Crab Milagro U.L. 95% (2004) Tibet 5.0 σ Whipple(1998) Milagro(2004) 6.0σ This Work 推定 Milagro U.L. 90% AIROBICC U.L. 90% (2002) 10-16TeV Crab Tibet 2.5 σ This Work (95%U.L x 90%U.L) イベント天頂角 >6.8 度制限のため
12 Search for PeV signal from Monogem Ring MAKET-ANI 6 σ signal from Monogem 3 O x3 O bin, However, Tibet ~ x 100 statistics x 10 sensitivity No significant signal <4.0x10-12 /cm 2 /sec/sr above ApJ, 635, L53-L56, (2005)
13 TIBET Hybrid Experiment
14 How to obtain proton spectrum? AS+ECfamily matching event (Eγ,Nγ,< R >,<ER>,sec(θ), Ne ) Data: ~200 ev DATA ANN (Correlations) Proton identification ~100 ev. Location(x, y) Direction(θ, φ) Time (t) Measurement Parameter EC(γ family) AS BD Eγ,Nγ,< R >,<ER>,sec(θ) Ne E0 N b
15 Primary Cosmic Ray Energy Spectrum CORSIKA_QGSJET CORSIKA_SIBYLL Proton モデル依存性小 (30 %) All (p+he) All Accepted by PL B
16 Cosmic Ray Anisotropy at Sidereal Time (ApJL 626, L29-L32, 2005) 1999Nov-2003Nov 918 live days ~3x10 10 ev Differential Integral= (Physical Quantity)
17 恒星時日周変動と宇宙線異方性 Multi-TeV 宇宙線の全天強度分布 Tail-In Loss-Cone Cygnus Region ApJ, 626,L29-L32, (2005) Tail-in 10TeV 領域までアリ 加速モデル? Loss cone 何処で消えるか? 銀河宇宙線異方性のモデル
18 惑星間磁場 太陽の影 宇宙線は太陽によって遮蔽される 正電荷をもった宇宙線は太陽磁場 惑星間磁場によって曲げられ 観測される へこみ は磁場の変動によって 移動 する 太陽活動は 11 年周期で極大期を迎え 磁場の変動も活発になる この へこみ の 移動 を観測することによって 太陽磁気圏の大局的磁場構造を知ることができる
19 Monthly Sunspots Tibet-I Tibet-II Tibet-III Tibet-II HD 1992_Jan 1992_Jul 1993_Jan 1993_Jul 1994_Jan 1994_Jul 1995_Jan 1995_Jul 1996_Jan 1996_Jul 1997_Jan 1997_Jul 1998_Jan 1998_Jul 1999_Jan 1999_Jul 2000_Jan 2000_Jul 2001_Jan 2001_Jul 2002_Jan 2002_Jul 1991_Jul Date 1990_Jul 1991_Jan 1990_Jan Sunspots #
20 20
21 太陽近傍磁場変動と太陽の影 太陽の影の変動 10TeV Cosmic Rays 静穏期上昇期 最盛期
22 太陽活動と銀河宇宙線 太陽の影 3TeV 2000 年 2001 年 2002 年 2003 年
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