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Observation of Terrestrial gamma-ray flashes in the RELEC space experiment on the Vernov satellite
Authors:V.?V.?Bogomolov,M.?I.?Panasyuk,S.?I.?Svertilov  mailto:sis@coronas.ru"   title="  sis@coronas.ru"   itemprop="  email"   data-track="  click"   data-track-action="  Email author"   data-track-label="  "  >Email author,A.?V.?Bogomolov,G.?K.?Garipov,A.?F.?Iyudin,P.?A.?Klimov,S.?I.?Klimov,T.?M.?Mishieva,P.?Yu.?Minaev,V.?S.?Morozenko,O.?V.?Morozov,A.?S.?Posanenko,A.?V.?Prokhorov,H.?Rotkel
Affiliation:1.Skobeltsyn Research Institute of Nuclear Physics,Moscow State University,Moscow,Russia;2.Department of Physics,Lomonosov Moscow State University,Moscow,Russia;3.Space Research Institute of the Russian Academy of Sciences,Moscow,Russia;4.Space Research Center of the Polish Academy of Sciences,Warsaw,Poland
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.
Keywords:
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