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The bursts of high energy events observed by the telescope array surface detector
- Authors
- Abbasi, R.U.[Abbasi, R.U.]; Abe, M.[ Abe, M.]; Abu-Zayyad, T.[ Abu-Zayyad, T.]; Allen, M.[ Allen, M.]; Anderson, R.[ Anderson, R.]; Azuma, R.[ Azuma, R.]; Barcikowski, E.[ Barcikowski, E.]; Belz, J.W.[ Belz, J.W.]; Bergman, D.R.[ Bergman, D.R.]; Blake, S.A.[ Blake, S.A.]; Cady, R.[ Cady, R.]; Cheon, B.G.[ Cheon, B.G.]; Chiba, J.[ Chiba, J.]; Chikawa, M.[ Chikawa, M.]; Fujii, T.[ Fujii, T.]; Fukushima, M.[ Fukushima, M.]; Goto, T.[ Goto, T.]; Hanlon, W.[ Hanlon, W.]; Hayashi, Y.[ Hayashi, Y.]; Hayashida, N.[ Hayashida, N.]; Hibino, K.[ Hibino, K.]; Honda, K.[ Honda, K.]; Ikeda, D.[ Ikeda, D.]; Inoue, N.[ Inoue, N.]; Ishii, T.[ Ishii, T.]; Ishimori, R.[ Ishimori, R.]; Ito, H.[ Ito, H.]; Ivanov, D.[ Ivanov, D.]; Jui, C.C.H.[ Jui, C.C.H.]; Kadota, K.[ Kadota, K.]; Kakimoto, F.[ Kakimoto, F.]; Kalashev, O.[ Kalashev, O.]; Kasahara, K.[ Kasahara, K.]; Kawai, H.[ Kawai, H.]; Kawakami, S.[ Kawakami, S.]; Kawana, S.[ Kawana, S.]; Kawata, K.[ Kawata, K.]; Kido, E.[ Kido, E.]; Kim, H.B.[ Kim, H.B.]; Kim, J.H.[ Kim, J.H.]; Kim, J.H.[ Kim, J.H.]; Kishigami, S.[ Kishigami, S.]; Kitamura, S.[ Kitamura, S.]; Kitamura, Y.[ Kitamura, Y.]; Kuzmin, V.[ Kuzmin, V.]; Kwon, Y.J.[ Kwon, Y.J.]; Lan, J.[ Lan, J.]; Lundquist, J.P.[ Lundquist, J.P.]; Machida, K.[ Machida, K.]; Martens, K.[ Martens, K.]; Matsuda, T.[ Matsuda, T.]; Matsuyama, T.[ Matsuyama, T.]; Matthews, J.N.[ Matthews, J.N.]; Minamino, M.[ Minamino, M.]; Mukai, K.[ Mukai, K.]; Myers, I.[ Myers, I.]; Nagasawa, K.[ Nagasawa, K.]; Nagataki, S.[ Nagataki, S.]; Nakamura, T.[ Nakamura, T.]; Nonaka, T.[ Nonaka, T.]; Nozato, A.[ Nozato, A.]; Ogio, S.[ Ogio, S.]; Ogura, J.[ Ogura, J.]; Ohnishi, M.[ Ohnishi, M.]; Ohoka, H.[ Ohoka, H.]; Oki, K.[ Oki, K.]; Okuda, T.[ Okuda, T.]; Ono, M.[ Ono, M.]; Onogi, R.[ Onogi, R.]; Oshima, A.[ Oshima, A.]; Ozawa, S.[ Ozawa, S.]; Park, I.H.[Park, I.H.]; Pshirkov, M.S.[ Pshirkov, M.S.]; Rodriguez, D.C.[ Rodriguez, D.C.]; Rubtsov, G.[ Rubtsov, G.]; Ryu, D.[ Ryu, D.]; Sagawa, H.[ Sagawa, H.]; Saito, K.[ Saito, K.]; Saito, Y.[ Saito, Y.]; Sakaki, N.[ Sakaki, N.]; Sakurai, N.[ Sakurai, N.]; Sampson, A.L.[ Sampson, A.L.]; Scott, L.M.[ Scott, L.M.]; Sekino, K.[ Sekino, K.]; Shah, P.D.[ Shah, P.D.]; Shibata, F.[ Shibata, F.]; Shibata, T.[ Shibata, T.]; Shimodaira, H.[ Shimodaira, H.]; Shin, B.K.[ Shin, B.K.]; Shin, H.S.[ Shin, H.S.]; Smith, J.D.[ Smith, J.D.]; Sokolsky, P.[ Sokolsky, P.]; Springer, R.W.[ Springer, R.W.]; Stokes, B.T.[ Stokes, B.T.]; Stratton, S.R.[ Stratton, S.R.]; Stroman, T.A.[ Stroman, T.A.]; Suzawa, T.[ Suzawa, T.]; Takamura, M.[ Takamura, M.]; Takeda, M.[ Takeda, M.]; Takeishi, R.[ Takeishi, R.]; Taketa, A.[ Taketa, A.]; Takita, M.[ Takita, M.]; Tameda, Y.[ Tameda, Y.]; Tanaka, H.[ Tanaka, H.]; Tanaka, K.[ Tanaka, K.]; Tanaka, M.[ Tanaka, M.]; Thomas, S.B.[ Thomas, S.B.]; Thomson, G.B.[ Thomson, G.B.]; Tinyakov, P.[ Tinyakov, P.]; Tkachev, I.[ Tkachev, I.]; Tokuno, H.[ Tokuno, H.]; Tomida, T.[ Tomida, T.]; Troitsky, S.[ Troitsky, S.]; Tsunesada, Y.[ Tsunesada, Y.]; Tsutsumi, K.[ Tsutsumi, K.]; Uchihori, Y.[ Uchihori, Y.]; Udo, S.[ Udo, S.]; Urban, F.[ Urban, F.]; Vasiloff, G.[ Vasiloff, G.]; Wong, T.[ Wong, T.]; Yamane, R.[ Yamane, R.]; Yamaoka, H.[ Yamaoka, H.]; Yamazaki, K.[ Yamazaki, K.]; Yang, J.[ Yang, J.]; Yashiro, K.[ Yashiro, K.]; Yoneda, Y.[ Yoneda, Y.]; Yoshida, S.[ Yoshida, S.]; Yoshii, H.[ Yoshii, H.]; Zollinger, R.[ Zollinger, R.]; Zundel, Z.[ Zundel, Z.]
- Issue Date
- 28-Aug-2017
- Publisher
- ELSEVIER SCIENCE BV
- Keywords
- High energy radiation; Lightning; Terrestrial gamma-ray flash
- Citation
- PHYSICS LETTERS A, v.381, no.32, pp.2565 - 2572
- Indexed
- SCIE
SCOPUS
- Journal Title
- PHYSICS LETTERS A
- Volume
- 381
- Number
- 32
- Start Page
- 2565
- End Page
- 2572
- ISSN
- 0375-9601
- Abstract
- The Telescope Array (TA) experiment is designed to detect air showers induced by ultra high energy cosmic rays. The TA ground Surface particle Detector (TASD) observed several short-time bursts of air shower like events. These bursts are not likely due to chance coincidence between single shower events. The expectation of chance coincidence is less than 10(-4) for five-year's observation. We checked the correlation between these bursts of events and lightning data, and found evidence for correlations in timing and position. Some features of the burst events are similar to those of a normal cosmic ray air shower, and some are not. On this paper, we report the observed bursts of air shower like events and their correlation with lightning. (C) 2017 Elsevier B.V. All rights reserved.
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