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Effects of atmospheric transparency on Telescope Array air shower analysisopen accessEffects of atmospheric transparency on TA air shower analysis

Other Titles
Effects of atmospheric transparency on TA air shower analysis
Authors
Mizuno, K.Tomida, T.Yamazaki, K.Abbasi, R.U.Abe, Y.Abu-Zayyad, T.Allen, M.Arai, Y.Arimura, R.Barcikowski, E.Belz, J.W.Bergman, D.R.Blake, S.A.Buckland, I.Cheon, B.G.Chikawa, M.Fedynitch, A.Fujii, T.Fujisue, K.Fujita, K.Fujiwara, R.Fukushima, M.Furlich, G.Gerber, Z.Globus, N.Hanlon, W.Hayashida, N.He, H.Hibi, R.Hibino, K.Higuchi, R.Honda, K.Ikeda, D.Inoue, N.Ishii, T.Ito, H.Ivanov, D.Iwasaki, A.Jeong, H.M.Jeong, S.Jui, C.C.H.Kadota, K.Kakimoto, F.Kalashev, O.Kasahara, K.Kasami, S.Kawakami, S.Kawata, K.Kharuk, I.Kido, E.Kim, H.B.Kim, J.H.Kim, J.H.Kim, S.W.Kimura, Y.Komae, I.Komori, K.Kusumori, Y.Kuznetsov, M.Kwon, Y.J.Lee, K.H.Lee, M.J.Lubsandorzhiev, B.Lundquist, J.P.Matsuyama, T.Matthews, J.A.Matthews, J.N.Mayta, R.Miyashita, K.Mizuno, K.Mori, M.Murakami, M.Myers, I.Nagataki, S.Nakai, K.Nakamura, T.Nishio, E.Nonaka, T.Ogio, S.Ohoka, H.Okazaki, N.Oku, Y.Okuda, T.Omura, Y.Onishi, M.Ono, M.Oshima, A.Oshima, H.Ozawa, S.Park, I.H.Park, K.Y.Potts, M.Pshirkov, M.S.Remington, J.Rodriguez, D.C.Rott, C.Rubtsov, G.I.Ryu, D.Sagawa, H.Saito, R.Sakaki, N.Sako, T.Sakurai, N.Sato, D.Sato, K.Sato, S.Sekino, K.Shah, P.D.Shibata, N.Shibata, T.Shikita, J.Shimodaira, H.Shin, B.K.Shin, H.S.Shinto, D.Smith, J.D.Sokolsky, P.Stokes, B.T.Stroman, T.A.Takagi, Y.Takahashi, K.Takamura, M.Takeda, M.Takeishi, R.Taketa, A.Takita, M.Tameda, Y.Tanaka, K.Tanaka, M.Thomas, S.B.Thomson, G.B.Tinyakov, P.Tkachev, I.Tokuno, H.Tomida, T.Troitsky, S.Tsuda, R.Tsunesada, Y.Udo, S.Urban, F.Vaiman, I.A.Warren, D.Wong, T.Yamazaki, K.Yashiro, K.Yoshida, F.Zhezher, Y.Zundel, Z.
Issue Date
Sep-2024
Citation
Proceedings of Science, v.444, pp 1 - 9
Pages
9
Indexed
SCOPUS
Journal Title
Proceedings of Science
Volume
444
Start Page
1
End Page
9
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/204178
DOI
10.22323/1.444.0226
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. 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 evaluating the attenuation of fluorescence by aerosols. We will report on the effects of this seasonal dependence on TA air shower analysis.
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