We provide an updated analysis of the gamma ray signature of a terrestrial gamma ray flash (TGF) detected by the Fermi Gamma ray Burst Monitor first reported by Pu et al. (2020,
In 2015, Bowers et al. (2018,
- Award ID(s):
- 1613028
- NSF-PAR ID:
- 10457807
- Publisher / Repository:
- DOI PREFIX: 10.1029
- Date Published:
- Journal Name:
- Journal of Geophysical Research: Atmospheres
- Volume:
- 125
- Issue:
- 6
- ISSN:
- 2169-897X
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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https://doi.org/10.1029/2011GL048099 ; Lu et al., 2011,https://doi.org/10.1029/2010JA016141 ; Pu et al., 2019,https://doi.org/10.1029/2019GL082743 ; Pu et al., 2020,https://doi.org/10.1029/2020GL089427 ), a −EIP (Lyu et al., 2016,https://doi.org/10.1002/2016GL070154 ; Lyu et al., 2021,https://doi.org/10.1029/2021GL093627 ; Wada et al., 2020,https://doi.org/10.1029/2019JD031730 ), and a double peak TGF associated with an extraordinarily powerful and complicated positive‐polarity sferic, where each TGF peak is possibly preceded by a short burst of stepped leader emission. -
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