Anisotropy and corotation of galactic cosmic rays

Science

Volumn 314, Issue 5798, 2006, Pages 439-443

  Amenomori, M ^a   Ayabe, S ^b   Bi, X J ^c   Chen, D ^d   Cui, S W ^e   Danzengluobu, ^f   Ding, L K ^c   Ding, X H ^f   Feng, C F ^g   Feng, Zhaoyang ^c   Feng, Z Y ^h   Gao, X Y ⁱ   Geng, Q X ⁱ   Guo, H W ^f   He, H H ^c   He, M ^g   Hibino, K ^j   Hotta, N ^k   Hu, Haibing ^f   Hu, H B ^c   Huang, J ^l   Huang, Q ^h   Jia, H Y ^h   Kajino, F ^m   Kasahara, K ⁿ   Katayose, Y ^d   Kato, C ^o   Kawata, K ^l   Labaciren, ^f   Le, G M ^p   Li, A F ^g   Li, J Y ^g   Lou, Y Q ^q   Lu, H ^c   Lu, S L ^c   Meng, X R ^f   Mizutani, K ^b,r   Mu, J ⁱ   Munakata, K ^o   Nagai, A ^k   Nanjo, H ^a   Mishizawa, M ^s   Ohnishi, M ^l   Ohta, I ^t   Onuma, H ^b   Ouchi, T ^j   Ozawa, S ^l   Ren, J R ^c   Saito, T ^u   Saito, T Y ^l   Sakata, M ^m   Sako, T K ^l   Sasaki, T ^j   Shibata, M ^d   Shiomi, A ^l   Shirai, T ^j   Sugimoto, H ^v   Takita, M ^l   Tan, Y H ^c   Tateyama, N ^j   Torii, S ^r   Tsuchiya, H ^w   Udo, S ^l   Wang, B ⁱ   Wang, H ^c   Wang, X ^l   Wang, Y G ^g   Wu, H R ^c   Xue, L ^g   Yamamoto, Y ^m   Yan, C T ^l   Yang, X C ⁱ   Yasue, S ^o   Ye, Z H ^p   Yu, G C ^h   Yuan, A F ^f   Yuda, T ^j   Zhang, H M ^c   Zhang, J L ^c   Zhang, N J ^g   Zhang, X Y ^g   Zhang, Y ^c   Zhang, Yi ^c   Zhaxisangzhu, ^f   Zhou, X X ^h   more..

^a HIROSAKI UNIVERSITY   (Japan)

^b SAITAMA UNIVERSITY   (Japan)

^c INSTITUTE OF HIGH ENERGY PHYSICS   (China)

^d YOKOHAMA NATIONAL UNIVERSITY   (Japan)

^e HEBEI NORMAL UNIVERSITY   (China)

^f TIBET UNIVERSITY   (China)

^g SHANDONG UNIVERSITY   (China)

^h SOUTHWEST JIAOTONG UNIVERSITY   (China)

ⁱ YUNNAN UNIVERSITY   (China)

^j KANAGAWA UNIVERSITY   (Japan)

^k UTSUNOMIYA UNIVERSITY   (Japan)

^l UNIVERSITY OF TOKYO   (Japan)

^m KONAN UNIVERSITY   (Japan)

ⁿ SHIBAURA INSTITUTE OF TECHNOLOGY   (Japan)

^o SHINSHU UNIVERSITY   (Japan)

^p CENTER FOR SPACE SCIENCE AND APPLIED RESEARCH   (China)

^q TSINGHUA UNIVERSITY   (China)

^r WASEDA UNIVERSITY   (Japan)

^s NATIONAL INSTITUTE OF INFORMATICS   (Japan)

^t OPEN UNIVERSITY OF JAPAN   (Japan)

^u TOKYO METROPOLITAN COLLEGE OF INDUSTRIAL TECHNOLOGY   (Japan)

^v SHONAN INSTITUTE OF TECHNOLOGY   (Japan)

^w RIKEN   (Japan)

more..

Author keywords

[No Author keywords available]

Indexed keywords

ELECTRON ENERGY LEVELS; GALAXIES; MAGNETIC ANISOTROPY; MAGNETIC FIELD EFFECTS;

CYGNUS REGION; GALACTIC COSMIC RAYS; SUPERNOVAE; TERAELECTRONVOLTS (TEV);

COSMIC RAYS;

COSMIC RAY; COSMOLOGY; ENERGY; MAGNETIC ANISOTROPY; MAGNETIC FIELD;

ANISOTROPY; ARTICLE; ASTRONOMY; COSMIC RADIATION; ENERGY; MAGNETIC FIELD; PRIORITY JOURNAL;

CYGNUS;

EID: 33750311775     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1131702     Document Type: Article

References (41)

1. H. J. Voelk, in Frontiers of Cosmic Ray Science, T. Kajita, Y. Asaoka, A. Kawachi, Y. Matsubara, M. Sasaki, Eds. (Universal Academy Press, Tokyo, 2003), pp. 29-48.
2. Y.-Q. Lou, Astrophys. J. 428, L21 (1994).
3. A. Dar, Nuovo Cim. B 120, 767 (2005).
4. C. Yu, Y.-Q. Lou, F. Y. Bian, Y. Wu, Mon. Not. R. Astron. Soc. 370, 121 (2006).
5. A. D. Erlykin, A. W. Wolfendale, Astropart. Phys. 25, 183 (2006).
6. G. F. Krymsky, Geomagn. Aeron. 977, 763 (1964).
7. E. N. Parker, Planet. Space Sci. 13, 9 (1965).
8. B. Heber, in Proc. 27th Int. Cosmic Ray Conf., M. Simon, E. Lorenz, M. Pohl, Eds., Invited, Rapporteur and High-lighted papers (CDROM, 2002) pp. 118-135.
9. A. H. Compton, I. A. Getting, Phys. Rev. 47, 817 (1935).
10. D. J. Cutler, D. E. Groom, Nature 322, L434 (1986).
11. M. Amenomori et al., Phys. Rev. Lett. 93, 061101 (2004).
12. K. Nagashima, S. Mori, in Proc. Int. Cosmic Ray Symp. on High Energy Cosmic Ray Modulation, Univ. of Tokyo, Tokyo, Japan, 326 (1976).
13. K. Nagashima, K. Fujimoto, R. M. Jacklyn, J. Geophys. Res. 103, 17429 (1998).
14. K. Munakata et al., Phys. Rev. D56, 23 (1997).
15. M. Ambrosio et al., Phys. Rev. D67, 042002 (2003).
16. M. Aglietta et al., in Proc. 28th Int. Cosmic Ray Conf., T. Kajita, Y. Asaoka, A. Kawachi, Y. Matsubara, M. Sasaki, Eds., (Universal Academy Press, Tokyo, 2003) 4, pp. 183-186.
17. T. Antonr et al., Astrophys. J. 604, 687 (2004).
18. G. Guillian et al., Phys. Rev. D, in press (see http:// arxiv.org/astro-ph/0508468).
19. M. Amenomori et al., Astrophys. J. 626, L29 (2005).
20. D. L. Hall et al., J. Geophys. Res. 103, 367 (1998).
21. D. L. Hall et al., J. Geophys. Res. 104, 6737 (1999).
22. M. L. Duldig, PASA 18 (1), 12 (2001).
23. M. Amenomori et al., Phys. Rev. Lett. 69, 2468 (1992).
24. M. Amenomori et al., in International Symposium on High Energy Gamma-Ray Astronomy, F. A. Aharoman, H. J. Voelk, Eds., AIP Conf. Proc. 558, 557 (2001).
25. M. Amenomori et ol., in Proc. 27th Int. Cosmic Ray Conf., M. Siḿon, E. Lorenz, M. Pohl, Eds. (Copernicus Gesellschaft, 2002), 2, pp. 573-576.
26. M. Amenomori et al., Phys. Rev. D47, 2675 (1993).
27. M. Amenomori et al., Astrophys. J. 598, 242 (2003).
28. M. Amenomori et al., Nucl. Instrum. Methods Phys. Res. A 288, 619 (1990).
29. K. Kasahara, http://cosmos.n.kanagawa-u.ac.jp/EPICSHome/.
30. M. Amenomori et al., Astrophys. J. 633, 1005 (2005).
31. F. A. Aharonian et al., A & A 393, L37 (2002).
32. S. D. Hunter et al., Astrophys. J. 481, 205 (1997).
33. R. Atkins et al., Phys. Rev. Lett. 95, 251103 (2005).
34. G. Walker, R. Atkins, D. Kieda, Astrophys. J. 614, L93 (2004).
35. L. Bergamasco et al., in Proc. 21th Int. Cosmic Ray Conf. (Adelaide), 6, 372-375 (1990).
36. E. N. Parker, Astrophys. J. 145, 811 (1966).
37. Z. H. Fan, Y.-Q. Lou, Nature 383, 800 (1996).
38. Y.-Q. Lou, Z. H. Fan, Mon. Not. R. Astron. Soc. 341, 909 (2003).
39. Y.-Q. Lou, X. N. Bai, Mon. Not. R. Astron. Soc., in press, astro-ph/0607328 (2006).
40. Unless otherwise stated, images in Figs. 1 to 4 are presented using pixels in a radius of 5° and are sampled over a square grid of side width 2°; the modal energy is 3 TeV.
41. The collaborative experiment of the Tibet Air Shower Arrays has been performed under the auspices of the Ministry of Science and Technology of China and the Ministry of Foreign Affairs of Japan. This work was supported in part by Grants-in-Aid for Scientific Research on Priority Areas (712) (MEXT), by the Japan Society for the Promotion of Science, by the National Natural Science Foundation of China, and by the Chinese Academy of Sciences. The authors thank J. Kota for reading the manuscript and for critical comments.