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


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

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

About the authors

Ju. V. Balabin

Polar Geophysical Institute

Author for correspondence.
Email: balabin@pgia.ru
Russian Federation, Apatity, Murmansk oblast, 184209

B. B. Gvozdevsky

Polar Geophysical Institute

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

A. V. Germanenko

Polar Geophysical Institute

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

E. A. Maurchev

Polar Geophysical Institute

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

E. A. Mikhalko

Polar Geophysical Institute

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

A. A. Lukovnikova

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

Email: balabin@pgia.ru
Russian Federation, Irkutsk, 664033

A. A. Toropov

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

Email: balabin@pgia.ru
Russian Federation, Yakutsk, 677980

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2019 Allerton Press, Inc.