Large-Scale Sidereal Anisotropy of Galactic Cosmic-Ray Intensity Observed by the Tibet Air Shower Array
M. Amenomori,S. Ayabe,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,Cunfeng Feng,Zhenyong Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,Hongbo Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,J. Y. Li,Hong-peng Lu,S. L. Lu,X. R. Meng,K. Mizutani,J. Mu,Kazuoki Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,To. Saito,M. Sakata,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,T. Utsugi,B. S. Wang,Huanyu Wang,X. Wang,Yu Wang,Hong Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,HongMei Zhang,J. L. Zhang,N. J. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +78 more
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TLDR
In this paper, the sidereal anisotropy of cosmic ray intensity in the multi-TeV region observed with the Tibet-III air shower array during the period from 1999 through 2003 was analyzed.Abstract:
We present the large-scale sidereal anisotropy of Galactic cosmic-ray intensity in the multi-TeV region observed with the Tibet-III air shower array during the period from 1999 through 2003. The sidereal daily variation of cosmic rays observed in this experiment shows an excess of relative intensity around 4-7 hr local sidereal time as well as a deficit around 12 hr local sidereal time. While the amplitude of the excess is not significant when averaged over all declinations, the excess in individual declination bands becomes larger and clearer as the viewing direction moves toward the south. The maximum phase of the excess intensity changes from ~7 hr at the Northern Hemisphere to ~4 hr at the equatorial region. We also show that both the amplitude and the phase of the first harmonic vector of the daily variation are remarkably independent of primary energy in the multi-TeV region. This is the first result determining the energy and declination dependences of the full 24 hr profiles of the sidereal daily variation in the multi-TeV region with a single air shower experiment.read more
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Journal ArticleDOI
Cosmic-Ray Propagation and Interactions in the Galaxy
TL;DR: A survey of the theory and experimental tests for the propagation of cosmic rays in the Galaxy up to energies of 10 15 eV is given in this article, followed by an exposition of basic principles.
Journal ArticleDOI
Anisotropy and corotation of galactic cosmic rays.
M. Amenomori,S. Ayabe,X. J. Bi,D. Chen,Shuwang Cui,Danzengluobu,Liming Ding,X. H. Ding,Cunfeng Feng,Zhaoyang Feng,Zhenyong Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,Hailan Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,A. F. Li,J. Y. Li,Y. Q. Lou,Hong-peng Lu,S. L. Lu,X. R. Meng,K. Mizutani,K. Mizutani,J. Mu,Kazuoki Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,To. Saito,Takashi Saito,M. Sakata,Takashi Sako,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,B. Wang,H. Wang,X. Wang,Y. G. Wang,Hong Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,J. L. Zhang,Ning Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +85 more
TL;DR: Two-dimensional high-precision anisotropy measurement for energies from a few to several hundred teraelectronvolts (TeV) is presented, using the large data sample of the Tibet Air Shower Arrays, revealing finer details of the known anisotropies.
Journal ArticleDOI
Diffusive propagation of cosmic rays from supernova remnants in the Galaxy. II: anisotropy
Pasquale Blasi,Elena Amato +1 more
TL;DR: In this article, the effects of stochasticity in the spatial and temporal distribution of supernova remnants on the anisotropy of cosmic rays observed at Earth were investigated for different choices of the diffusion coefficient D(E) experienced by cosmic rays during propagation in the Galaxy.
Journal ArticleDOI
Observation of anisotropy in the arrival directions of galactic cosmic rays at multiple angular scales with IceCube
Rasha Abbasi,Y. Abdou,T. Abu-Zayyad,Jenni Adams,Juanan Aguilar,Markus Ahlers,D. Altmann,Karen Andeen,J. Auffenberg,Xinhua Bai,Michael J. Baker,S. W. Barwick,R. C. Bay,J. L. Bazo Alba,K. Beattie,J. J. Beatty,S. Bechet,J. K. Becker,K.-H. Becker,M. L. Benabderrahmane,Segev BenZvi,J. Berdermann,P. Berghaus,D. Berley,Elisa Bernardini,D. Bertrand,D. Z. Besson,Daniel Bindig,M. Bissok,E. Blaufuss,J. Blumenthal,D. J. Boersma,C. Bohm,D. Bose,S. Böser,Olga Botner,A. M. Brown,Stijn Buitink,Karen S. Caballero-Mora,M. J. Carson,Dmitry Chirkin,B. Christy,J. M. Clem,F. Clevermann,S. Cohen,C. Colnard,D. F. Cowen,M. V. D'Agostino,M. Danninger,J. Daughhetee,J. C. Davis,C. De Clercq,L. Demirörs,T. Denger,O. Depaepe,F. Descamps,Paolo Desiati,G. de Vries-Uiterweerd,Tyce DeYoung,Juan Carlos Diaz-Velez,M. Dierckxsens,J. Dreyer,J. P. Dumm,R. Ehrlich,J. Eisch,R. W. Ellsworth,O. Engdegård,S. Euler,Paul Evenson,O. Fadiran,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,T. Feusels,Kirill Filimonov,Chad Finley,T. Fischer-Wasels,M. M. Foerster,B. D. Fox,A. Franckowiak,R. Franke,Thomas K. Gaisser,J. C. Gallagher,L. Gerhardt,L. Gerhardt,L. Gladstone,T. Glüsenkamp,A. Goldschmidt,J. A. Goodman,Dariusz Gora,Darren Grant,T. Griesel,Axel Groß,Axel Groß,S. Grullon,M. Gurtner,C. Ha,A. Hajismail,Allan Hallgren,Francis Halzen,K. Han,Kael Hanson,Kael Hanson,D. Heinen,K. Helbing,Ph. Herquet,S. Hickford,G. C. Hill,Kara Hoffman,A. Homeier,K. Hoshina,D. Hubert,W. Huelsnitz,J.-P. Hülß,P. O. Hulth,K. Hultqvist,S. Hussain,A. Ishihara,J. E. Jacobsen,George Japaridze,Henrik J. Johansson,J. M. Joseph,Karl-Heinz Kampert,Alexander Kappes,Timo Karg,Albrecht Karle,Paraic A. Kenny,Joanna Kiryluk,Joanna Kiryluk,Fabian Kislat,Spencer Klein,Spencer Klein,J.-H. Köhne,G. Kohnen,Hermann Kolanoski,L. Köpke,Sandro Kopper,D. J. Koskinen,M. Kowalski,T. Kowarik,M. Krasberg,T. Krings,G. Kroll,N. Kurahashi,Takao Kuwabara,M. Labare,S.J. Lafebre,K. Laihem,H. Landsman,M. J. Larson,R. J. Lauer,J. Lünemann,B. Madajczyk,James Madsen,Pratik Majumdar,A. Marotta,Reina H. Maruyama,K. Mase,H. S. Matis,K. Meagher,M. Merck,Peter Mészáros,Thomas Meures,E. Middell,N. Milke,J. Miller,Teresa Montaruli,Teresa Montaruli,R. Morse,S. M. Movit,R. Nahnhauer,J. W. Nam,U. Naumann,P. Nießen,D. R. Nygren,S. Odrowski,A. Olivas,M. Olivo,Aongus O'Murchadha,M. Ono,S. Panknin,Larissa Paul,C. Pérez de los Heros,J. Petrovic,A. Piegsa,Damian Pieloth,R. Porrata,J. Posselt,Craig Price,P. B. Price,Gerald Przybylski,K. Rawlins,P. Redl,Elisa Resconi,Wolfgang Rhode,M. Ribordy,A. Rizzo,J. P. Rodrigues,P. Roth,F. Rothmaier,Carsten Rott,Tim Ruhe,D. Rutledge,B. Ruzybayev,Dirk Ryckbosch,H. G. Sander,Marcos Santander,Subir Sarkar,K. Schatto,T. O. B. Schmidt,A. Schönwald,A. Schukraft,A. Schultes,O. Schulz,M. Schunck,D. Seckel,B. Semburg,S. H. Seo,Y. Sestayo,S. Seunarine,A. Silvestri,A. Slipak,Glenn Spiczak,Christian Spiering,M. Stamatikos,M. Stamatikos,Todor Stanev,G. Stephens,T. Stezelberger,R. G. Stokstad,A. Stössl,S. Stoyanov,E. A. Strahler,T. Straszheim,M. Stür,G. W. Sullivan,Q. Swillens,H. Taavola,I. Taboada,A. Tamburro,A. Tepe,Samvel Ter-Antonyan,S. Tilav,P. A. Toale,Simona Toscano,D. Tosi,D. Turcan,N. van Eijndhoven,Justin Vandenbroucke,A. Van Overloop,J. van Santen,M. Vehring,M. Voge,C. Walck,T. Waldenmaier,M. Wallraff,M. Walter,Ch. Weaver,C. Wendt,S. Westerhoff,Nathan Whitehorn,K. Wiebe,Christopher Wiebusch,David A. Williams,R. Wischnewski,H. Wissing,Martin Wolf,T. R. Wood,Kurt Woschnagg,Chun Xu,Xianwu Xu,G. B. Yodh,S. Yoshida,P. Zarzhitsky,M. Zoll +274 more
TL;DR: In this paper, a power spectrum analysis was performed on the relative intensity map of the cosmic ray flux in the southern hemisphere, and it was shown that the arrival direction distribution is not isotropic, but shows significant structure on several angular scales.
Journal ArticleDOI
Diffusive propagation of cosmic rays from supernova remnants in the Galaxy. II: anisotropy
Pasquale Blasi,Elena Amato +1 more
TL;DR: In this article, the effects of stochasticity in the spatial and temporal distribution of supernova remnants on the anisotropy of cosmic rays observed at Earth were investigated for different choices of the diffusion coefficient D(E) for propagation in the Galaxy.
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Anisotropy and corotation of galactic cosmic rays.
M. Amenomori,S. Ayabe,X. J. Bi,D. Chen,Shuwang Cui,Danzengluobu,Liming Ding,X. H. Ding,Cunfeng Feng,Zhaoyang Feng,Zhenyong Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,Hailan Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,A. F. Li,J. Y. Li,Y. Q. Lou,Hong-peng Lu,S. L. Lu,X. R. Meng,K. Mizutani,K. Mizutani,J. Mu,Kazuoki Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,To. Saito,Takashi Saito,M. Sakata,Takashi Sako,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,B. Wang,H. Wang,X. Wang,Y. G. Wang,Hong Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,J. L. Zhang,Ning Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +85 more