Observation of Terrestrial gamma-ray flashes in the RELEC space experiment on the Vernov satellite
- Authors: Bogomolov V.V.1,2, Panasyuk M.I.1,2, Svertilov S.I.1,2, Bogomolov A.V.1, Garipov G.K.1, Iyudin A.F.1, Klimov P.A.1, Klimov S.I.3, Mishieva T.M.1,2, Minaev P.Y.3, Morozenko V.S.1, Morozov O.V.1, Posanenko A.S.3, Prokhorov A.V.1,2, Rotkel H.4
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Affiliations:
- Skobeltsyn Research Institute of Nuclear Physics
- Department of Physics
- Space Research Institute of the Russian Academy of Sciences
- Space Research Center of the Polish Academy of Sciences
- Issue: Vol 55, No 3 (2017)
- Pages: 159-168
- Section: Article
- URL: https://journal-vniispk.ru/0010-9525/article/view/153386
- DOI: https://doi.org/10.1134/S0010952517030017
- ID: 153386
Cite item
Abstract
The RELEС scientific payload of the Vernov satellite launched on July 8, 2014 includes the DRGE spectrometer of gamma-rays and electrons. This instrument comprises a set of scintillator phoswich-detectors, including four identical X-ray and gamma-ray detector with an energy range of 10 kev to 3 MeV with a total area of ~500 cm2 directed to the atmosphere, as well as an electron spectrometer containing three mutually orthogonal detector units with a geometric factor of ~2 cm2 sr. The aim of a space experiment with the DRGE instrument is the study of fast phenomena, in particular Terrestrial gamma-ray flashes (TGF) and magnetospheric electron precipitation. In this regard, the instrument provides the transmission of both monitoring data with a time resolution of 1 s, and data in the event-by-event mode, with a recording of the time of detection of each gamma quantum or electron to an accuracy of ~15 μs. This makes it possible to not only conduct a detailed analysis of the variability in the gamma-ray range, but also compare the time profiles with the results of measurements with other RELEC instruments (the detector of optical and ultraviolet flares, radio-frequency and low-frequency analyzers of electromagnetic field parameters), as well as with the data of ground-based facility for thunderstorm activity. This paper presents the first catalog of Terrestrial gamma-ray flashes. The criterion for selecting flashes required in order to detect no less than 5 hard quanta in 1 ms by at least two independent detectors. The TGFs included in the catalog have a typical duration of ~400 μs, during which 10–40 gamma-ray quanta were detected. The time profiles, spectral parameters, and geographic position, as well as a result of a comparison with the output data of other Vernov instruments, are presented for each of candidates. The candidate for Terrestrial gamma-ray flashes detected in the near-polar region over Antarctica is discussed.
About the authors
V. V. Bogomolov
Skobeltsyn Research Institute of Nuclear Physics; Department of Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899; Moscow, 119991
M. I. Panasyuk
Skobeltsyn Research Institute of Nuclear Physics; Department of Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899; Moscow, 119991
S. I. Svertilov
Skobeltsyn Research Institute of Nuclear Physics; Department of Physics
Author for correspondence.
Email: sis@coronas.ru
Russian Federation, Moscow, 119899; Moscow, 119991
A. V. Bogomolov
Skobeltsyn Research Institute of Nuclear Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899
G. K. Garipov
Skobeltsyn Research Institute of Nuclear Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899
A. F. Iyudin
Skobeltsyn Research Institute of Nuclear Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899
P. A. Klimov
Skobeltsyn Research Institute of Nuclear Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899
S. I. Klimov
Space Research Institute of the Russian Academy of Sciences
Email: sis@coronas.ru
Russian Federation, Moscow, 117997
T. M. Mishieva
Skobeltsyn Research Institute of Nuclear Physics; Department of Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899; Moscow, 119991
P. Yu. Minaev
Space Research Institute of the Russian Academy of Sciences
Email: sis@coronas.ru
Russian Federation, Moscow, 117997
V. S. Morozenko
Skobeltsyn Research Institute of Nuclear Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899
O. V. Morozov
Skobeltsyn Research Institute of Nuclear Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899
A. S. Posanenko
Space Research Institute of the Russian Academy of Sciences
Email: sis@coronas.ru
Russian Federation, Moscow, 117997
A. V. Prokhorov
Skobeltsyn Research Institute of Nuclear Physics; Department of Physics
Email: sis@coronas.ru
Russian Federation, Moscow, 119899; Moscow, 119991
H. Rotkel
Space Research Center of the Polish Academy of Sciences
Email: sis@coronas.ru
Poland, Warsaw
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