Increases in the Gamma-Ray Background: General Properties and Statistical Characteristics


Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
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Аннотация

A special system is designed and produced at the Polar Geophysical Institute to monitor the soft gamma radiation induced by cosmic rays in the atmosphere. The radiation is registered in two ranges: 20−400 keV and 0.2−0.8 MeV. Monitoring begins in 2010 at cosmic-ray stations at Apatity and Barentsburg (Spitsbergen Archipelago). A new phenomenon is discovered at the start of observations: the gamma background grows during precipitation. At the same time, no radionuclides are found in the precipitates. The large volume of data on these increases allows analysis of them and identification of their characteristic features

Авторлар туралы

Ju. Balabin

Polar Geophysical Institute

Хат алмасуға жауапты Автор.
Email: balabin@pgia.ru
Ресей, Apatity, Murmansk oblast, 184209

B. Gvozdevsky

Polar Geophysical Institute

Email: balabin@pgia.ru
Ресей, Apatity, Murmansk oblast, 184209

A. Germanenko

Polar Geophysical Institute

Email: balabin@pgia.ru
Ресей, Apatity, Murmansk oblast, 184209

E. Maurchev

Polar Geophysical Institute

Email: balabin@pgia.ru
Ресей, Apatity, Murmansk oblast, 184209

E. Mikhalko

Polar Geophysical Institute

Email: balabin@pgia.ru
Ресей, Apatity, Murmansk oblast, 184209

A. Lukovnikova

Institute of Solar–Terrestrial Physics, Siberian Branch, Russian Academy of Sciences

Email: balabin@pgia.ru
Ресей, Irkutsk, 664033

A. Toropov

Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences

Email: balabin@pgia.ru
Ресей, Yakutsk, 677980

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