Abstract
The station-ring method makes it possible to isolate and study the specific angular distributions of cosmic-ray variations that are poorly described by the sum of the first spherical harmonics. Examples of the use of the station-ring method are given and described in detail. The application of the method to study precursors of Forbush effects and the behavior of cosmic rays inside the perturbations of the solar wind is shown.
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ACKNOWLEDGMENTS
The authors are grateful to the teams of the world network of CR stations providing data for the continuous recording of the neutron component (http://cr0.izmiran.ru/ ThankYou/Our_Acknowledgment.pdf) and to the Neutron Monitor Database (www.nmdb.eu). The work is based on experimental data from the Unique Scientific Facility “Russian National Network of Cosmic Ray Stations.”
Funding
This work was partially supported by the Fundamental Research Program of the Presidium of the Russian Academy of Sciences no. 3 and the Russian Foundation for Basic Research (grant nos. 17-02-00508 and RNF no. 15-12-20001).
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Abunina, M.A., Belov, A.V., Eroshenko, E.A. et al. Station-Ring Method in the Study of Cosmic-Ray Variations: 2. Examples of Its Use. Geomagn. Aeron. 60, 184–191 (2020). https://doi.org/10.1134/S0016793220020024
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DOI: https://doi.org/10.1134/S0016793220020024