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The atmospheric transparency of Telescope Array observation site by the CLF

Authors
Tomida, T.Nakamura, T.Yamazaki, K.Matthews, J.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.the Telescope Array collaboration on behalf of the Telescope Array Collaboration
Issue Date
Mar-2022
Publisher
Sissa Medialab Srl
Citation
Proceedings of Science, v.395, pp.1 - 8
Indexed
SCOPUS
Journal Title
Proceedings of Science
Volume
395
Start Page
1
End Page
8
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/182209
ISSN
1824-8039
Abstract
The Telescope Array (TA) experiment continues to observe Ultra High Energy Cosmic Rays (UHECRs) both with its original TA detectors as well as with the new TAx4 expansion detectors. These observations employ Fluorescence Detectors (FDs) to capture the air shower induced by the primary UHECRs. The FD observes fluorescence light emitted from atmospheric nitrogen molecules excited by air shower particles. The observation of the FD extends over tens of kilometers, and the fluorescence light is attenuated by scattering from atmospheric molecules and aerosols during the propagation process. Seasonal dependence was found when assessing the attenuation of fluorescence by aerosols. We also captured the weather characteristics. We report on the effect of aerosols on the atmospheric transparency of the TA sites.
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