# Gamma-ray Showers Observed at Ground Level in Coincidence With Downward   Lightning Leaders

**Authors:** R.U. Abbasi, T.Abu-Zayyad, M. Allen, E. Barcikowski, J.W. Belz, D.R., Bergman, S.A. Blake, M. Byrne, R. Cady, B.G. Cheon, J. Chiba, M. Chikawa, T., Fujii, M. Fukushima, G. Furlich, T. Goto, W. Hanlon, Y. Hayashi, N., Hayashida, K. Hibino, K. Honda, D. Ikeda, N. Inoue, T. Ishii, H. Ito, D., Ivanov, S. Jeong, C.C.H. Jui, K. Kadota, F. Kakimoto, O. Kalashev, K., Kasahara, H. Kawai, S. Kawakami, K. Kawata, E. Kido, H.B. Kim, J.H. Kim, J.H., Kim, S.S. Kishigami, P.R. Krehbiel, V. Kuzmin, Y.J. Kwon, J. Lan, R. LeVon,, J.P. Lundquist, K. Machida, K. Martens, T. Matuyama, J.N. Matthews, M., Minamino, K. Mukai, I. Myers, S. Nagataki, R. Nakamura, T. Nakamura, T., Nonaka, S. Ogio, M. Ohnishi, H. Ohoka, K. Oki, T. Okuda, M. Ono, R. Onogi, A., Oshima, S. Ozawa, I.H. Park, M.S. Pshirkov, J. Remington, W. Rison, D., Rodeheffer, D.C. Rodriguez, G. Rubtsov, D. Ryu, H. Sagawa, K. Saito, N., Sakaki, N. Sakurai, T. Seki, K. Sekino, P.D. Shah, F. Shibata, T. Shibata, H., Shimodaira, B.K. Shin, H.S. Shin, J.D. Smith, P. Sokolsky, R.W. Springer,, B.T. Stokes, T.A. Stroman, H. Takai, M. Takeda, R. Takeishi, A. Taketa, M., Takita, Y. Tameda, H. Tanaka, K. Tanaka, M. Tanaka, R.J. Thomas, S.B. Thomas,, G.B. Thomson, P. Tinyakov, I. Tkachev, H. Tokuno, T. Tomida, S. Troitsky, Y., Tsunesada, Y. Uchihori, S. Udo, F. Urban, G. Vasiloff, T. Wong, M. Yamamoto,, R. Yamane, H. Yamaoka, K. Yamazaki, J. Yang, K. Yashiro, Y. Yoneda, S., Yoshida, H. Yoshii, Z. Zundel

arXiv: 1705.06258 · 2018-05-22

## TL;DR

This study reports ground-based detection of gamma-ray showers coinciding with downward lightning leaders, revealing detailed temporal and spatial characteristics of terrestrial gamma-ray flashes (TGFs) during lightning events.

## Contribution

It provides the first detailed ground-based observations of TGFs associated with lightning, including structure, timing, and origin altitude, supported by simulations and multi-instrument data.

## Key findings

- Gamma-ray showers occur at 3-5 km altitude during initial lightning breakdown.
- Showers consist mainly of downward-beamed gamma radiation.
- Ground-based detection is more sensitive than satellite observations.

## Abstract

Bursts of gamma ray showers have been observed in coincidence with downward propagating negative leaders in lightning flashes by the Telescope Array Surface Detector (TASD). The TASD is a 700~square kilometer cosmic ray observatory located in southwestern Utah, U.S.A. In data collected between 2014 and 2016, correlated observations showing the structure and temporal development of three shower-producing flashes were obtained with a 3D lightning mapping array, and electric field change measurements were obtained for an additional seven flashes, in both cases co-located with the TASD. National Lightning Detection Network (NLDN) information was also used throughout. The showers arrived in a sequence of 2--5 short-duration ($\le$10~$\mu$s) bursts over time intervals of several hundred microseconds, and originated at an altitude of $\simeq$3--5 kilometers above ground level during the first 1--2 ms of downward negative leader breakdown at the beginning of cloud-to-ground lightning flashes. The shower footprints, associated waveforms and the effect of atmospheric propagation indicate that the showers consist primarily of downward-beamed gamma radiation. This has been supported by GEANT simulation studies, which indicate primary source fluxes of $\simeq$$10^{12}$--$10^{14}$ photons for $16^{\circ}$ half-angle beams. We conclude that the showers are terrestrial gamma-ray flashes (TGFs), similar to those observed by satellites, but that the ground-based observations are more representative of the temporal source activity and are also more sensitive than satellite observations, which detect only the most powerful TGFs.

## Full text

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## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1705.06258/full.md

## References

55 references — full list in the complete paper: https://tomesphere.com/paper/1705.06258/full.md

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Source: https://tomesphere.com/paper/1705.06258