Vestnik КRAUNC. Fiz.-Mat. nauki. 2024. vol. 49. no. 4. P. 112-124. ISSN 2079-6641
INFORMATION AND COMPUTING TECHNOLOGIES
https://doi.org/10.26117/2079-6641-2024-49-4-112-124
Research Article
Full text in Russian
MSC 65
Analysis of Geomagnetic Field Variations Based on the Results of the «Aurora» Interactive System
Y. A. Polozov^{\ast}, O. V. Mandrikova
Institute of Cosmophysical Research and Radio Wave Propagation FEB RAS, Russia, 684034, Paratunka, Mirnay St. 7
Abstract. This paper describes the geomagnetic component of the Aurora system, which assesses the state of the Earth’s magnetic field using data from the Paratunka (Kamchatka Krai, 52.97^{\circ} N, 158.24^{\circ} E) and Khabarovsk (47.61^{\circ} N, 134.69^{\circ} E) stations. The data were obtained by direct measurements at magnetic observatories. The geomagnetic component of the Aurora system was developed at IKIR FEB RAS. The functions of this component are based on new approaches and methods developed by the team of scientists of the System Analysis Laboratory. The developed methods are based on the synthesis of elements of wavelet transform theory with methods of probability theory and mathematical statistics. The system provides a comprehensive assessment of the state of the Earth’s magnetic field in disturbed and calm periods and enables the study of spatial and temporal features and dynamics of processes in the Earth’s magnetosphere. The conclusion about the state of the magnetic field is formed in the operational mode. The analysis of the system operation during the periods of the events considered in the article confirmed the possibility of weak short-period synchronous geomagnetic disturbances preceding the onset of magnetic storms. The geomagnetic component considered in the article complements the complex analysis of geophysical monitoring data in the system. The results of the geomagnetic component of the Aurora system can be used as an additional tool in the tasks of operational space weather forecasting.
Key words: geomagnetic field, data analysis, wavelets, magnetic storms.
Received: 28.10.2024; Revised: 21.11.2024; Accepted: 25.11.2024; First online: 28.11.2024
For citation. Polozov Y. A., Mandrikova O. V. Analysis of geomagnetic field variations based on the results of the «Aurora» interactive system. Vestnik KRAUNC. Fiz.-mat. nauki. 2024, 49: 4, 112-124. EDN: IVINBR. https://doi.org/10.26117/2079-6641-2024-49-4-112-124.
Funding. The work was supported by IKIR FEB RAS State Task (subject registration No. 124012300245-2). Competing interests. The authors declare that there are no conflicts of interest regarding authorship and publication.
Contribution and Responsibility. All authors contributed to this article. Authors are solely responsible for providing the final version of the article in print. The final version of the manuscript was approved by all authors.
^{\ast}Correspondence: E-mail: polozov@ikir.ru
The content is published under the terms of the Creative Commons Attribution 4.0 International License
© Polozov Y. A., Mandrikova O. V., 2024
© Institute of Cosmophysical Research and Radio Wave Propagation, 2024 (original layout, design, compilation)
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Information about the authors
Yurii Alexandrovich Polozov – Ph. D. (Tech.), Senior Researcher Laboratory of System Analysis, IKIR FEB RAS, Russia, ORCID 0000-0001-6960-8784
Mandrikova Oksana Viktorovna – D. Sci. (Tech.), Professor, Head Laboratory of System Analysis, IKIR FEB RAS, Russia, ORCID 0000-0002-6172-1827.