Observation of Terrestrial gamma-ray flashes in the RELEC space experiment on the Vernov satellite


Дәйексөз келтіру

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Аннотация

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.

Авторлар туралы

V. Bogomolov

Skobeltsyn Research Institute of Nuclear Physics; Department of Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899; Moscow, 119991

M. Panasyuk

Skobeltsyn Research Institute of Nuclear Physics; Department of Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899; Moscow, 119991

S. Svertilov

Skobeltsyn Research Institute of Nuclear Physics; Department of Physics

Хат алмасуға жауапты Автор.
Email: sis@coronas.ru
Ресей, Moscow, 119899; Moscow, 119991

A. Bogomolov

Skobeltsyn Research Institute of Nuclear Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899

G. Garipov

Skobeltsyn Research Institute of Nuclear Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899

A. Iyudin

Skobeltsyn Research Institute of Nuclear Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899

P. Klimov

Skobeltsyn Research Institute of Nuclear Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899

S. Klimov

Space Research Institute of the Russian Academy of Sciences

Email: sis@coronas.ru
Ресей, Moscow, 117997

T. Mishieva

Skobeltsyn Research Institute of Nuclear Physics; Department of Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899; Moscow, 119991

P. Minaev

Space Research Institute of the Russian Academy of Sciences

Email: sis@coronas.ru
Ресей, Moscow, 117997

V. Morozenko

Skobeltsyn Research Institute of Nuclear Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899

O. Morozov

Skobeltsyn Research Institute of Nuclear Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899

A. Posanenko

Space Research Institute of the Russian Academy of Sciences

Email: sis@coronas.ru
Ресей, Moscow, 117997

A. Prokhorov

Skobeltsyn Research Institute of Nuclear Physics; Department of Physics

Email: sis@coronas.ru
Ресей, Moscow, 119899; Moscow, 119991

H. Rotkel

Space Research Center of the Polish Academy of Sciences

Email: sis@coronas.ru
Польша, Warsaw

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