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Primary cosmic-ray proton and helium spectra at the knee energy region measured by the Tibet hybrid AS experiment

Primary cosmic-ray proton and helium spectra at the knee ene...

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29th International Cosmic Ray Conference, ICRC 2005

作者： Amenomori, M. Ayabe, S. Chen, D. Cui, S.W. Danzengluobu Ding, L.K. Ding, X.H. Feng, C.F. Feng, Z.Y. Gao, X.Y. Geng, Q.X. Guo, H.W. He, H.H. He, M. Hibino, K. Hotta, N. Hu, Haibing Hu, H.B. Huang, J. Huang, Q. Jia, H.Y. Kajino, F. Kasahara, K. Katayose, Y. Kato, C. Kawata, K. labaciren Le, G.M. Li, J.Y. Lu, H. Lu, S.L. Meng, X.R. Mizutani, K. Mu, J. Munakata, K. Nagai, A. Nanjo, H. Nishizawa, M. Ohnishi, M. Ohta, I. Onuma, H. Ouchi, T. Ozawa, S. Ren, J.R. Saito, T. Sakata, M. Sasaki, T. Shibata, M. Shiomi, A. Shirai, T. Sugimoto, H. Takita, M. Tan, Y.H. Tateyama, N. Torii, S. Tsuchiya, H. Udo, S. Wang, H. Wang, X. Wang, Y.G. Wu, H.R. Xue, L. Yamamoto, Y. Yan, C.T. Yang, X.C. Yasue, S. Ye, Z.H. Yu, G.C. Yuan, A.F. Yuda, T. Zhang, H.M. Zhang, J.L. Zhang, N.J. Zhang, X.Y. Zhang, Y. Zhang, Yi Zhaxisangzhu Zhou, X.X. Department of Physics Hirosaki University Hirosaki 036-8561 Japan Department of Physics Saitama University Saitama 338-8570 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Key Lab. of Particle Astrophys. Chinese Academy of Sciences Institute of High Energy Physics Beijing 100049 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics South West Jiaotong University Chengdu 610031 China Department of Physics Yunnan University Kunming 650091 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Department of Physics Konan University Kobe 658-8501 Japan Faculty of Systems Engineering Shibaura Institute of Technology Saitama 337-8570 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Center of Space Science and Application Research Chinese Academy of Sciences Beijing 100080 China Advanced Media Network Center Utsunomiya University Utsunomiya 321-8585 Japan National Institute of Informatics Tokyo 101-8430 Japan Tokyo Metropolitan College of Aeronautical Engineering Tokyo 116-0003 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Advanced Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan RIKEN Wako 351-0198 Japan

A hybrid experiment was carried out to study the cosmic-ray primary composition in the 'knee' energy region. The experimental set-up consists of the Tibet-II air shower array( AS ), the emulsion chamber ( EC ) and the burst detector ( BD ) which are operated simulteneously and provides us information on the primary species. For three-year operation, we have observed 177 γ -families ( ∑Eγ 20 TeV ) accompanying air showers with the shower size Ne × 105. Using this data set and a neural network method to select proton and helium induced events, the primary proton and helium energy spectra are obtained between 1015 and 1016. The proton spectrum, thus obtained, can be expressed by a single power-law function with a differential index of -3.01 ± 0.11 and -3.05 ± 0.12 based on the QGSJET+HD and SIBYLL+HD models, respectively, which are steeper than that extrapolated from the direct observations of -2.74 ± 0.01 vin the energy range below (1014eV. Our experiment suggests that the main component responsible for making the knee structure of the all-particle spectrum is composed of nuclei heavier than helium.

关键词： Helium

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Multiwavelength searches of the Shell-like SNR G40.5-0.5

Multiwavelength searches of the Shell-like SNR G40.5-0.5

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29th International Cosmic Ray Conference, ICRC 2005

作者： Amenomori, M. Ayabe, S. Chen, D. Cui, S.W. Danzengluobu Ding, L.K. Ding, X.H. Feng, C.F. Feng, Z.Y. Gao, X.Y. Geng, Q.X. Guo, H.W. He, H.H. He, M. Hibino, K. Hotta, N. Hu, Haibing Hu, H.B. Huang, J. Huang, Q. Jia, H.Y. Kajino, F. Kasahara, K. Katayose, Y. Kato, C. Kawata, K. labaciren Le, G.M. Li, J.Y. Lu, H. Lu, S.L. Meng, X.R. Mizutani, K. Mu, J. Munakata, K. Nagai, A. Nanjo, H. Nishizawa, M. Ohnishi, M. Ohta, I. Onuma, H. Ouchi, T. Ozawa, S. Ren, J.R. Saito, T. Sakata, M. Sasaki, T. Shibata, M. Shiomi, A. Shirai, T. Sugimoto, H. Takita, M. Tan, Y.H. Tateyama, N. Torii, S. Tsuchiya, H. Udo, S. Wang, H. Wang, X. Wang, Y.G. Wu, H.R. Xue, L. Yamamoto, Y. Yan, C.T. Yang, X.C. Yasue, S. Ye, Z.H. Yu, G.C. Yuan, A.F. Yuda, T. Zhang, H.M. Zhang, J.L. Zhang, N.J. Zhang, X.Y. Zhang, Y. Zhang, Y.I. Zhaxisangzhu Zhou, X.X. Department of Physics Hirosaki University Hirosaki 036-8561 Japan Department of Physics Saitama University Saitama 338-8570 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Key Lab. of Particle Astrophys Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics South West Jiaotong University Chengdu 610031 China Department of Physics Yunnan University Kunming 650091 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Department of Physics Konan University Kobe 658-8501 Japan Faculty of Systems Engineering Shibaura Institute of Technology Saitama 337-8570 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Center of Space Science and Application Research Chinese Academy of Sciences Beijing 100080 China Advanced Media Network Center Utsunomiya University Utsunomiya 321-8585 Japan National Institute for Informatics Tokyo 101-8430 Japan Tokyo Metropolitan College of Aeronautical Engineering Tokyo 116-0003 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Advanced Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan RIKEN Wako 351-0198 Japan

Using observation data of the extended Tibet air shower array from October 2000 to September 2001, a region around the shell-like SNR G40.5-0.5 direction with the highest excess of 4.4 sigma was found using two dimension analysis method. In this article we presented some work done to understanding the nature of the G40.5-0.5 using a multiwavelength approach. In order to look for a site of the CR accelerators, a survey of the CO(J=1-0) line to G40.5-0.5 region will be conducting with the 13.7m radio telescope at Delingha, the millimeter-wave radio observatory of Purple Mountain Observatory this year.

关键词： Observatories

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Absolute energy scale calibration of multi-TeV cosmic rays using the moon's shadow observed by the Tibet air shower array

Absolute energy scale calibration of multi-TeV cosmic rays u...

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29th International Cosmic Ray Conference, ICRC 2005

The Tibet air shower array has been in operation since 1999 as Tibet III with an energy threshold of a few TeV. As primary cosmic rays are shielded by the Moon having the finite size of 0.5° in diameter, we observe a deficit in cosmic rays called the Moon's shadow with a significance of 40 α level for 1041 live days. The center of the Moon's shadow shifts westward depending on primary cosmic-ray energies due to the geomagnetic field. We calibrate the absolute energy scale of the primary cosmic rays observed by the Tibet III array using this effect. The Moon's shadow simulation, including a precise calculation of the geomagnetic effect, shows a good agreement with observational data. As a result, the systematic error in the absolute energy scale is estimated to be less than approximately ± 8% level by means of the geomagnetic field as a spectrometer.

关键词： Cosmic rays

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Search for TeV transient gamma-ray sources of the northern sky using the Tibet- III air shower array

Search for TeV transient gamma-ray sources of the northern s...

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29th International Cosmic Ray Conference, ICRC 2005

作者： Amenomori, M. Ayabe, S. Chen, D. Cui, S.W. Danzengluobu Ding, L.K. Ding, X.H. Feng, C.F. Feng, Z.Y. Gao, X.Y. Geng, Q.X. Guo, H.W. He, H.H. He, M. Hibino, K. Hotta, N. Hu, Haibing Hu, H.B. Huang, J. Huang, Q. Jia, H.Y. Kajino, F. Kasahara, K. Katayose, Y. Kato, C. Kawata, K. labaciren Le, G.M. Li, J.Y. Lu, H. Lu, S.L. Meng, X.R. Mizutani, K. Mu, J. Munakata, K. Nagai, A. Nanjo, H. Nishizawa, M. Ohnishi, M. Ohta, I. Onuma, H. Ouchi, T. Ozawa, S. Ren, J.R. Saito, T. Sakata, M. Sasaki, T. Shibata, M. Shiomi, A. Shirai, T. Sugimoto, H. Takita, M. Tan, Y.H. Tateyama, N. Torii, S. Tsuchiya, H. Udo, S. Wang, H. Wang, X. Wang, Y.G. Wu, H.R. Xue, L. Yamamoto, Y. Yan, C.T. Yang, X.C. Yasue, S. Ye, Z.H. Yu, G.C. Yuan, A.F. Yuda, T. Zhang, H.M. Zhang, J.L. Zhang, N.J. Zhang, X.Y. Zhang, Y. Zhang, Yi Zhaxisangzhu Zhou, X.X. Department of Physics Hirosaki Univ Ersity Hirosaki 036-8561 Japan Department of Physics Saitama University Saitama 338-8570 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Key Lab. of Particle Astrophys Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics South West Jiaotong University Chengdu 610031 China Department of Physics Yunnan University Kunming 650091 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Department of Physics Konan University Kobe 658-8501 Japan Faculty of Systems Engineering Shibaura Institute of Technology Saitama 337-8570 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Center of Space Science and Application Research Chinese Academy of Sciences Beijing 100080 China Advanced Media Network Center Utsunomiya University Utsunomiya 321-8585 Japan National Institute of Informatics Tokyo 101-8430 Japan Tokyo Metropolitan College of Aeronautical Engineering Tokyo 116-0003 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Advanced Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan RIKEN Wako 351-0198 Japan

The Tibet III air shower array has a wide field of view greater than one steradian and a high duty cycle. Using the Tibet III (Nov. 1999 - Oct. 2004) data, we search for TeV transient gamma-ray point sources on the time scale of 120 days, 30 days, 10 days and 3 days. No new source was found at sufficiently high significance on any time scale in the field of view during the live time. The 90% confidence level upper limits on the integral flux above 3 TeV assuming an energy spectrum of E-1.6 and of E-1.0 are obtained.

关键词： Gamma rays

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The energy spectrum of the light components (P+He) at the knee obtained by the Tibet air shower core detector

The energy spectrum of the light components (P+He) at the kn...

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29th International Cosmic Ray Conference, ICRC 2005

作者： Katayose, Y. Amenomori, M. Ayabe, S. Chen, D. Cui, S.W. Danzengluobu Ding, L.K. Ding, X.H. Feng, C.F. Feng, Z.Y. Gao, X.Y. Geng, Q.X. Guo, H.W. He, H.H. He, M. Hibino, K. Hotta, N. Hu, Haibing Hu, H.B. Huang, J. Huang, Q. Jia, H.Y. Kajino, F. Kasahara, K. Kato, C. Kawata, K. labaciren Le, G.M. Li, J.Y. Lu, H. Lu, S.L. Meng, X.R. Mizutani, K. Mu, J. Munakata, K. Nagai, A. Nanjo, H. Nishizawa, M. Ohnishi, M. Ohta, I. Onuma, H. Ouchi, T. Ozawa, S. Ren, J.R. Saito, T. Sakata, M. Sasaki, T. Shibata, M. Shiomi, A. Shirai, T. Sugimoto, H. Takita, M. Tan, Y.H. Tateyama, N. Torii, S. Tsuchiya, H. Udo, S. Wang, H. Wang, X. Wang, Y.G. Wu, H.R. Xue, L. Yamamoto, Y. Yan, C.T. Yang, X.C. Yasue, S. Ye, Z.H. Yu, G.C. Yuan, A.F. Yuda, T. Zhang, H.M. Zhang, J.L. Zhang, N.J. Zhang, X.Y. Zhang, Y. Zhang, Yi Zhaxisangzhu Zhou, X.X. Department of Physics Hirosaki University Hirosaki 036-8561 Japan Department of Physics Saitama University Saitama 338-8570 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Key Lab. of Particle Astrophys. Chinese Academy of Sciences Institute of High Energy Physics Beijing 100049 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics South West Jiaotong University Chengdu 610031 China Department of Physics Yunnan University Kunming 650091 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Department of Physics Konan University Kobe 658-8501 Japan Faculty of Systems Engineering Shibaura Institute of Technology Saitama 337-8570 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Center of Space Science and Application Research Chinese Academy of Sciences Beijing 100080 China Advanced Media Network Center Utsunomiya University Utsunomiya 321-8585 Japan National Institute of Informatics Tokyo 101-8430 Japan Tokyo Metropolitan College of Aeronautical Engineering Tokyo 116-0003 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Advanced Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan RIKEN Wako 351-0198 Japan

A hybrid experiment was carried out to study the cosmic-ray primary composition in the 'knee' energy region. The experimental set-up consists of the Tibet-II air shower array( AS ), the emulsion chamber ( EC ) and the burst detector ( BD ) which are operated simulteneously and provides us information on the primary species. For three-year operation, we have observed 177 γ -families ( ∑Eγ 20 TeV ) accompanying air showers with the shower size Ne≥ × 105. Using this data set and a neural network method to select proton and helium induced events, the primary proton and helium energy spectra are obtained between 1015 and 10 16. The proton spectrum, thus obtained, can be expressed by a single power-law function with a differential index of -3.01 ± 0.11 and -3.05 ± 0.12 based on the QGSJET+HD and SIBYLL+HD models, respectively, which are steeper than that extrapolated from the direct observations of -2.74 ± 0.01 vin the energy range below (1014eV. Our experiment suggests that the main component responsible for making the knee structure of the all-particle spectrum is composed of nuclei heavier than helium.

关键词： Helium

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Sidereal anisotropy of galactic cosmic-ray intensity observed with the Tibet air shower array

Sidereal anisotropy of galactic cosmic-ray intensity observe...

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29th International Cosmic Ray Conference, ICRC 2005

作者： Kawata, K. Amenomori, M. Ayabe, S. Chen, D. Cui, S.W. Danzengluobu Ding, L.K. Ding, X.H. Feng, C.F. Feng, Z.Y. Gao, X.Y. Geng, Q.X. Guo, H.W. He, H.H. He, M. Hibino, K. Hotta, N. Hu, Haibing Hu, H.B. Huang, J. Huang, Q. Jia, H.Y. Kajino, F. Kasahara, K. Katayose, Y. Kato, C. Kawata, K. labaciren Le, G.M. Li, J.Y. Lu, H. Lu, S.L. Meng, X.R. Mizutani, K. Mu, J. Munakata, K. Nagai, A. Nanjo, H. Nishizawa, M. Ohnishi, M. Ohta, I. Onuma, H. Ouchi, T. Ozawa, S. Ren, J.R. Saito, T. Saito, T.Y. Sakata, M. Sasaki, T. Shibata, M. Shiomi, A. Shirai, T. Sugimoto, H. Takita, M. Tan, Y.H. Tateyama, N. Torii, S. Tsuchiya, H. Udo, S. Wang, H. Wang, X. Wang, Y.G. Wu, H.R. Xue, L. Yamamoto, Y. Yan, C.T. Yang, X.C. Yasue, S. Ye, Z.H. Yu, G.C. Yuan, A.F. Yuda, T. Zhang, H.M. Zhang, J.L. Zhang, N.J. Zhang, X.Y. Zhang, Y. Zhang, Yi Zhaxisangzhu Zhou, X.X. Department of Physics Hirosaki University Hirosaki 036-8561 Japan Department of Physics Saitama University Saitama 338-8570 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Key Lab. of Particle Astrophys. Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics South West Jiaotong University Chengdu 610031 China Department of Physics Yunnan University Kunming 650091 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Department of Physics Konan University Kobe 658-8501 Japan Faculty of Systems Engineering Shibaura Institute of Technology Saitama 337-8570 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Center of Space Science and Application Research Chinese Academy of Sciences Beijing 100080 China Advanced Media Network Center Utsunomiya University Utsunomiya 321-8585 Japan National Institute of Informatics Tokyo 101-8430 Japan Tokyo Metropolitan College of Aeronautical Engineering Tokyo 116-0003 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Advanced Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan RIKEN Wako 351-0198 Japan

We report the large-scale sidereal anisotropy of galactic cosmic-ray intensity in the multi-TeV region obtained with the Tibet III air shower array in the period from 1999 through 2003. The sidereal daily variation of cosmic rays observed with Tibet III clearly indicates the excess of relative intensity around 4 ∼ 7 hours local sidereal time, as well as the deficit around 12 hours local sidereal time. The amplitude of the excess is not significant when averaged over the declination, however it becomes larger and clearer as the declination of viewing direction moves toward the south. The maximum phase of the excess intensity shifts from ∼ 7 to ∼ 4 hours according to the declination moving from the northern hemisphere to the equatorial region. Furthermore.

关键词： Anisotropy

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An upper limit on cosmic-ray p¯/p flux ratio estimated by the Moon's shadow with the Tibet III air shower array

An upper limit on cosmic-ray p¯/p flux ratio estimated by t...

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29th International Cosmic Ray Conference, ICRC 2005

作者： Amenomori, M. Ayabe, S. Chen, D. Cui, W. Danzengluobu Ding, L.K. Ding, X.H. Feng, C.F. Feng, Z.Y. Gao, X.Y. Geng, Q.X. Guo, H.W. He, H.H. He, M. Ohta, I. Hotta, N. Hu, Haibing Hu, H.B. Huang, J. Huang, Q. Jia, H.Y. Kajino, F. Saito, T. Katayose, Y. Kato, C. Kasahara, K. labaciren Le, G.M. Li, J.Y. Lu, H. Lu, S.L. Meng, X.R. Mizutani, K. Mu, J. Munakata, K. Nagai, A. Nanjo, H. Nishizawa, M. Ohnishi, M. Onuma, H. Ouchi, T. Ozawa, S. Ren, J.R. Kawata, K. Zhaxisangzhu Sasaki, T. Shibata, M. Shiomi, A. Shirai, T. Sugimoto, H. Zhang, H.M. Tateyama, N. Torii, S. Tsuchiya, H. Wang, H. Wang, X. Wang, Y.G. Wu, H.R. Xue, L. Takita, M. Yamamoto, Y. Yan, C.T. Yang, X.C. Yasue, S. Ye, Z.H. Yu, G.C. Udo, S. Yuda, T. Zhang, J.L. Zhang, N.J. Zhang, X.Y. Zhang, Y. Zhang, Yi Sakata, M. Yuan, A.F. Tan, Y.H. Hibino, K. Zhou, X.X. Department of Physics Hirosaki University Hirosaki 036-8561 Japan Department of Physics Saitama University Saitama 338-8570 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Key Lab. of Particle Astrophys. Chinese Academy of Sciences Institute of High Energy Physics Beijing 100049 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics South West Jiaotong University Chengdu 610031 China Department of Physics Yunnan University Kunming 650091 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Department of Physics Konan University Kobe 658-8501 Japan Faculty of Systems Engineering Shibaura Institute of Technology Saitama 337-8570 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Center of Space Science and Application Research Chinese Academy of Sciences Beijing 100080 China Advanced Media Network Center Utsunomiya University Utsunomiya 321-8585 Japan National Institute of Informatics Tokyo 101-8430 Japan Tokyo Metropolitan College of Aeronautical Engineering Tokyo 116-0003 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Advanced Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan RIKEN Wako 351-0198 Japan

The Tibet air shower array has been in operation since 1999 as Tibet III (22,050m2) with energy threshold of a few TeV. As primary cosmic rays are shielded by the Moon having the finite size of 0.5 degree in diameter, we observe a deficit in cosmic rays called the Moon's shadow with sufficient statistical significance. The center of the Moon's shadow shifts westwardly due to the geomagnetic field. By analyzing this energy-dependent westward displacement carefully, we set an upper limit of about 5% at 90% confidence level on the cosmic-ray antiproton/proton ratio at multi-TeV energies.

关键词： Cosmic rays

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Two dimensional observation on TeV Cosmic-ray large scale anisotropy using the Tibet Air Shower Array

Two dimensional observation on TeV Cosmic-ray large scale an...

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29th International Cosmic Ray Conference, ICRC 2005

作者： Amenomori, M. Ayabe, S. Chen, D. Cui, S.W. Danzengluobu Ding, L.K. Ding, X.H. Feng, C.F. Feng, Z.Y. Gao, X.Y. Geng, Q.X. Guo, H.W. He, H.H. He, M. Hibino, K. Hotta, N. Hu, Haibing Hu, H.B. Huang, J. Huang, Q. Jia, H.Y. Kajino, F. Kasahara, K. Katayose, Y. Kato, C. Kawata, K. labaciren Le, G.M. Li, J.Y. Lu, H. Lu, S.L. Meng, X.R. Mizutani, K. Mu, J. Munakata, K. Nagai, A. Nanjo, H. Nishizawa, M. Ohnishi, M. Ohta, I. Onuma, H. Ouchi, T. Ozawa, S. Ren, J.R. Saito, T. Sakata, M. Sasaki, T. Shibata, M. Shiomi, A. Shirai, T. Sugimoto, H. Takita, M. Tan, Y.H. Tateyama, N. Torii, S. Tsuchiya, H. Udo, S. Wang, H. Wang, X. Wang, Y.G. Wu, H.R. Xue, L. Yamamoto, Y. Yan, C.T. Yang, X.C. Yasue, S. Ye, Z.H. Yu, G.C. Yuan, A.F. Yuda, T. Zhang, H.M. Zhang, J.L. Zhang, N.J. Zhang, X.Y. Zhang, Y. Zhang, Yi Zhaxisangzhu Zhou, X.X. Department of Physics Hirosaki University Hirosaki 036-8561 Japan Department of Physics Saitama University Saitama 338-8570 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Key Lab. of Particle Astrophys. Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics South West Jiaotong University Chengdu 610031 China Department of Physics Yunnan University Kunming 650091 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Department of Physics Konan University Kobe 658-8501 Japan Faculty of Systems Engineering Shibaura Institute of Technology Saitama 337-8570 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Center of Space Science and Application Research Chinese Academy of Sciences Beijing 100080 China Advanced Media Network Center Utsunomiya University Utsunomiya 321-8585 Japan National Institute of Informatics Tokyo 101-8430 Japan Tokyo Metropolitan College of Aeronautical Engineering Tokyo 116-0003 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Advanced Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan RIKEN Wako 351-0198 Japan

The two-dimensional large scale anisotropy of cosmic-ray intensity in a magnitude about 0.1% is observed in TeV energy range using data taken from Tibet-III (Nov.1999-Oct.2003). The anisotropy due to the terrestrial o... 详细信息

关键词： Anisotropy

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Security and Privacy in Web 3.0 1

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丛书名： Digital Privacy and Security

1000年

作者： Meng Shen Liehuang Zhu Xiangyun Tang Wei Wang

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