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Study on the cosmic ray intensity variation using scintillation counters for air shower observation

Authors
Nonaka, T.Oshima, A.Yamazaki, K.Abbasi, R.U.Abu-Zayyad, T.Allen, M.Arai, Y.Arimura, R.Barcikowski, E.Belz, J.W.Bergman, D.R.Blake, S.A.Buckland, I.Cady, R.Cheon, B.G.Chiba, J.Chikawa, M.Fujii, T.Fujisue, K.Fujita, K.Fujiwara, R.Fukushima, M.Fukushima, R.Furlich, G.Gonzalez, R.Hanlon, W.Hayashi, M.Hayashida, N.Hibino, K.Higuchi, R.Honda, K.Ikeda, D.Inadomi, T.Inoue, N.Ishii, T.Ito, H.Ivanov, D.Iwakura, H.Iwasaki, A.Jeong, H.M.Jeong, S.Jui, C.C.H.Kadota, K.Kakimoto, F.Kalashev, O.Kasahara, K.Kasami, S.Kawai, H.Kawakami, S.Kawana, S.Kawata, K.Kharuk, I.Kido, E.Kim, H.B.Kim, J.H.Kim, J.H.Kim, M.H.Kim, S.W.Kimura, Y.Kishigami, S.Kubota, Y.Kurisu, S.Kuzmin, V.Kuznetsov, M.Kwon, Y.J.Lee, K.H.Lubsandorzhiev, B.Lundquist, J.P.Machida, K.Matsumiya, H.Matsuyama, T.Matthews, J.N.Mayta, R.Minamino, M.Mukai, K.Myers, I.Nagataki, S.Nakai, K.Nakamura, R.Nakamura, T.Nakamura, T.Nakamura, Y.Nakazawa, A.Nishio, E.Nonaka, T.Oda, H.Ogio, S.Ohnishi, M.Ohoka, H.Oku, Y.Okuda, T.Omura, Y.Ono, M.Onogi, R.Oshima, A.Ozawa, S.Park, I.H.Potts, M.Pshirkov, M.S.Remington, J.Rodriguez, D.C.Rubtsov, G.I.Ryu, D.Sagawa, H.Sahara, R.Saito, Y.Sakaki, N.Sako, T.Sakurai, N.Sano, K.Sato, K.Seki, T.Sekino, K.Shah, P.D.Shibasaki, Y.Shibata, F.Shibata, N.Shibata, T.Shimodaira, H.Shin, B.K.Shin, H.S.Shinto, D.Smith, J.D.Sokolsky, P.Sone, N.Stokes, B.T.Stroman, T.A.Takagi, Y.Takahashi, Y.Takamura, M.Takeda, M.Takeishi, R.Taketa, A.Takita, M.Tameda, Y.Tanaka, H.Tanaka, K.Tanaka, M.Tanoue, Y.Thomas, S.B.Thomson, G.B.Tinyakov, P.Tkachev, I.Tokuno, H.Tomida, T.Troitsky, S.Tsuda, R.Tsunesada, Y.Uchihori, Y.Udo, S.Uehama, T.Urban, F.Wong, T.Yada, K.Yamamoto, M.Yamazaki, K.Yang, J.Yashiro, K.Yoshida, F.Yoshioka, Y.Zhezher, Y.Zundel, Z.Telescope ArrayTelescope Array Collaboration
Issue Date
Mar-2022
Publisher
Sissa Medialab Srl
Citation
Proceedings of Science, v.395, pp.1 - 9
Indexed
SCOPUS
Journal Title
Proceedings of Science
Volume
395
Start Page
1
End Page
9
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/182215
ISSN
1824-8039
Abstract
We report a study on the conversion of a giant cosmic ray observatory for air shower observation to observe cosmic ray intensity variations caused by solar activity, anisotropy associated with interplanetary disturbances, and detection of sudden cosmic ray events on the earth’s surface. In this report, we use data from the surface detectors operated by the Telescope Array experiment located at 39°N, 112°W (total detector area: 2250 m2). In order to evaluate the cosmic ray intensity variations, we will compare the data with some of the corrections considered and with available world wide database such as Nagoya Muon detector and other observatories that have been in stable operation at different geographic longitudes. Finally, we will report on the intensity variations due to weather and solar activity recorded during the observation period.
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