Thunderstorm effects according to data from a comprehensive study of variations in secondary cosmic ray particles
- Authors: Kanonidi K.K.1, Kurenya A.N.2, Lidvansky A.S.2, Khaerdinov M.N.2, Khaerdinov N.S.2
-
Affiliations:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
- Institute for Nuclear Research
- Issue: Vol 81, No 2 (2017)
- Pages: 222-225
- Section: Proceedings of the 34th All-Russian Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/184975
- DOI: https://doi.org/10.3103/S1062873817020216
- ID: 184975
Cite item
Abstract
Thunderstorms have been studied at the Baksan Neutrino Observatory (Institute for Nuclear Research, Russian Academy of Sciences) since the summer of 2013 using a measuring instrumentation complex. During the period of observation, three events of continuous night-sky airglow correlating with the disturbances in the flux of energetic particles have been recorded during thunderstorms. It is established that there is interaction between a thunderstorm’s front and the precipitation of protons from the Earth’s radiation belt into the atmosphere due to seismic activity.
About the authors
K. Kh. Kanonidi
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
Email: khaerdinovns@yandex.ru
Russian Federation, Troitsk, Moscow, 108840
A. N. Kurenya
Institute for Nuclear Research
Email: khaerdinovns@yandex.ru
Russian Federation, Moscow, 117312
A. S. Lidvansky
Institute for Nuclear Research
Email: khaerdinovns@yandex.ru
Russian Federation, Moscow, 117312
M. N. Khaerdinov
Institute for Nuclear Research
Email: khaerdinovns@yandex.ru
Russian Federation, Moscow, 117312
N. S. Khaerdinov
Institute for Nuclear Research
Author for correspondence.
Email: khaerdinovns@yandex.ru
Russian Federation, Moscow, 117312
Supplementary files
