First High-speed Camera Observations of the Optical Counterpart of a Terrestrial Gamma-ray Flash

R. U. Abbasi,J. W. Belz,M. M. F. Saba,P. R. Krehbiel,J. Remington,M. A. Stanley,D. R. da Silva,W. Rison,Dan Rodeheffer, N. Kieu, J. Mazich, R. LeVon, K. Smout, A. Petrizze, T. Abu-Zayyad,M. Allen,Y. Arai,R. Arimura,E. Barcikowski,D. R. Bergman,S. A. Blake, I. Buckland,B. G. Cheon,M. Chikawa, T. Fujii, K. Fujisue,K. Fujita,R. Fujiwara,M. Fukushima,G. Furlich,N. Globus, R. Gonzalez,W. Hanlon,N. Hayashida,H. He,K. Hibino,R. Higuchi, K. Honda, D. Ikeda,N. Inoue,T. Ishii, H. Ito,D. Ivanov, H. Iwakura,A. Iwasaki, H. M. Jeong,S. Jeong,C. C. H. Jui, K. Kadota,F. Kakimoto,O. Kalashev,K. Kasahara, S. Kasami, S. Kawakami,K. Kawata,I. Kharuk, E. Kido,H. B. Kim,J. H. Kim,S. W. Kim,Y. Kimura, I. Komae,Y. Kubota,V. Kuzmin,M. Kuznetsov,Y. J. Kwon, K. H. Lee, B. Lubsandorzhiev,J. P. Lundquist, H. Matsumiya,T. Matsuyama, J. N. Matthews, R. Mayta,I. Myers,S. Nagataki,K. Nakai,R. Nakamura,T. Nakamura, Y. Nakamura,A. Nakazawa, E. Nishio, T. Nonaka,H. Oda,S. Ogio,M. Ohnishi,H. Ohoka,Y. Oku, T. Okuda,Y. Omura, M. Ono,A. Oshima,S. Ozawa, I. H. Park,M. Potts,M. S. Pshirkov,J. Remington, D. C. Rodriguez,C. Rott, G. I. Rubtsov,D. Ryu,H. Sagawa,N. Sakaki,T. Sako, N. Sakurai,K. Sato,T. Seki,K. Sekino,P. D. Shah, Y. Shibasaki,N. Shibata,T. Shibata, J. Shikita, H. Shimodaira,B. K. Shin,H. S. Shin, D. Shinto,J. D. Smith,P. Sokolsky,B. T. Stokes,T. A. Stroman, K. Takahashi, M. Takamura, M. Takeda, R. Takeishi,A. Taketa,M. Takita, Y. Tameda,K. Tanaka, M. Tanaka, Y. Tanoue, S. B. Thomas,G. B. Thomson, P. Tinyakov,I. Tkachev,H. Tokuno,T. Tomida,S. Troitsky, R. Tsuda,Y. Tsunesada,S. Udo, T. Uehama,F. Urban, D. Warren,T. Wong,M. Yamamoto,K. Yamazaki,K. Yashiro,F. Yoshida, Y. Zhezher, Z. Zundel

arxiv(2022)

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摘要
In this paper, we present the first observation of optical emission of a downward-directed terrestrial gamma ray flash (TGF). The optical emission was observed by a high-speed video camera Phantom v2012 in conjunction with the Telescope Array (TA) surface detector, lightning mapping array, interferrometer, fast antenna, and the national lightning detection network. The suite of gamma and lightning instruments, timing resolution, and source proximity offers us an unprecedented look at the TGF phenomena. On September 11 of 2021 we observed a storm above the TA detector. The storm resulted in six extremely energetic TGF events that were produced by flashes with return stroke peak currents up to 223 kA. The observed TGFs were found to correlate directly to the initial burst pulse signal of the lightning flash while producing an intense optical signature. Results from this study allow us to furthers the understanding regarding the initiation mechanism of TGFs.
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flash,high-speed,gamma-ray
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