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Real-time monitoring of the behavior of the daily anisotropy vector of cosmic rays according to the data of neutron monitors at Yakutsk and Tiksi stations
- Authors: Zverev A.S.1, Starodubtsev S.A.1, Grigoryev V.G.1, Gololobov P.Y.1
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Affiliations:
- Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
- Issue: Vol 88, No 2 (2024)
- Pages: 311-313
- Section: Physics of Cosmic Rays
- URL: https://rjpbr.com/0367-6765/article/view/654769
- DOI: https://doi.org/10.31857/S0367676524020254
- EDN: https://elibrary.ru/RQAGPN
- ID: 654769
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Abstract
Since 2022, the Institute of Cosmophysical Research and Aeronomy (SB RAS) for the first time has been continuously monitoring the forecast of terrestrial winds of space weather based on data from neutron monitors in Yakutsk and Tiksi. Preliminary studies during periods of geomagnetic disturbances in 2022. The peculiarity is that the results of this may provide an additional opportunity for their use for the purpose of forecasting large geomagnetic storms.
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About the authors
A. S. Zverev
Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
Author for correspondence.
Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk
S. A. Starodubtsev
Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk
V. G. Grigoryev
Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk
P. Yu. Gololobov
Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk
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