@article{oai:nagoya.repo.nii.ac.jp:00007167,
 author = {Guillian, G. and Hosaka, J. and Ishihara, K. and Kameda, J. and Koshio, Y. and Minamino, A. and Mitsuda, C. and Miura, M. and Moriyama, S. and Nakahata, M. and Namba, T. and Nishijima, K. and Ishino, H. and Watanabe, Y. and Koshiba, M. and Kielczewska, D. and Berns, H. G. and Gran, R. and Ogawa, H. and Shiraishi, K. K. and Stachyra, A. L. and Okada, A. and Washburn, K. and Wilkes, R. J. and Munakata, K. and Shiozawa, M. and Suzuki, Y. and Takeda, A. and Takeuchi, Y. and Yamada, S. and Higuchi, I. and Ishitsuka, M. and Okumura, K. and Kajita, T. and Kaneyuki, K. and Mitsuka, G. and Nakayama, S. and Nishino, H. and Saji, C. and Takenaga, Y. and Desai, S. and Kearns, E. and Stone, J.L. and Sulak, L.R. and Wang, W. and Goldhaber, M. and Tasaka, S. and Casper, D. and Gajewski, W. and Griskevich, J. and Kropp, W. R. and Liu, D.W. and Mine, S. and Smy, M. B. and Sobel, H.W. and Vagins, M. R. and Ganezer, K. S. and Kibayashi, A. and Hill, J. and Keig, W. E. and Scholberg, K. and Walter, C.W. and Ellsworth, R.W. and Learned, J. G. and Matsuno, S. and Messier, M. D. and Hayato, Y. and Ichikawa, A. K. and Ishida, T. and Ishii, T. and Iwashita, T. and Haines, T. J. and Kobayashi, T. and Nakadaira, T. and Nakamura, K. and Nitta, K. and Oyama, Y. and Totsuka, Y. and Suzuki, A. T. and Hasegawa, M. and Kato, I. and Maesaka, H. and Dazeley, S. and Nakaya, T. and Nishikawa, K. and Sato, H. and Yamamoto, S. and Yokoyama, M. and Hatakeyama, S. and Svoboda, R. and Blaufuss, E. and Goodman, J. A. and Sullivan, G.W. and Turcan, D. and Habig, A. and Fukuda, Y. and Gando, Y. and Itow, Y. and Sakuda, M. and Yoshida, M. and Kim, S. B. and Yoo, J. and Okazawa, H. and Ishizuka, T. and Jung, C. K. and Kato, T. and Kobayashi, K. and Hasegawa, T. and Malek, M. and Mauger, C. and McGrew, C. and Sharkey, E. and Yanagisawa, C. and Inoue, K. and Shirai, J. and Suzuki, A. and Nishijima, K. and Ishino, H. and Watanabe, Y. and Koshiba, M. and Hasegawa, T. and Obayashi, Y. and Inoue, K. and Shirai, J. and Suzuki, A.},
 issue = {6},
 journal = {PHYSICAL REVIEW D},
 month = {Mar},
 note = {The relative sidereal variation in the arrival direction of primary cosmic ray nuclei of median energy 10 TeV was measured using downward, through-going muons detected with the Super-Kamiokande-I detector. The projection of the anisotropy map onto the right ascension axis has a first harmonic amplitude of (6.64±0.98 stat±0.55 syst) ×10^-4 and a phase at maximum at (33.2±8.2 stat± 5.1°syst) right ascension. A sky map in equatorial coordinates indicates an excess region in the constellation of Taurus and a deficit region toward Virgo. The excess region is centered at (αT, δT)=(75±7, -5±9) with a half-opening angle χT =(39±7)°; the excess flux is (0.104±0.020)% above the isotropic expectation. The corresponding parameters for the deficit region are (αV, δV)=(205±7, 5±10), χV = (54±7), and (-0.094±0.014)%. The data do not allow us to rule out a pure dipole form for the anisotropy (allowed at 13% confidence level); they are better described by the excess and deficit cones described above. We explored the implications under the assumption that the true anisotropy is not distorted too much by the analysis filter so that it is well-described by the observed excess and deficit cones.},
 pages = {062003--062003},
 title = {Observation of the anisotropy of 10 TeV primary cosmic ray nuclei flux with the Super-Kamiokande-I detector},
 volume = {75},
 year = {2007}
}