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JOURNALS // Vestnik KRAUNC. Fiziko-Matematicheskie Nauki // Archive

Vestnik KRAUNC. Fiz.-Mat. Nauki, 2024 Volume 49, Number 4, Pages 157–170 (Mi vkam671)

INFORMATION AND COMPUTATION TECHNOLOGIES

Analysis of the ionospheric parameter dynamics during disturbed periods based on Aurora system results

N. V. Fetisova, O. V. Mandrikova

Institute of Cosmophysical Researches and Radio Wave Propagation, Far East Division, Russian Academy of Sciences

Abstract: The paper describes an ionospheric component of “Aurora” interactive system. The “Aurora” system implements new methods of data analysis based on the combination of modern means of digital signal processing with classical methods of data analysis. The paper presents the results of the ionospheric component based on a generalized multicomponent model of ionospheric parameters developed by the authors. The model and numerical algorithms based on it make it possible to study the ionospheric parameter dynamics during disturbed periods (to detect anomalous periods and estimate their parameters) in detail. The ionospheric component of “Aurora” system performs processing and analysis of the foF2 ionospheric critical frequency parameters recorded at Paratunka station (Kamchatka Territory) and forms a conclusion on the state of the ionosphere above Kamchatka. This development was carried out by a team of the system analysis laboratory of IKIR FEB RAS. The paper presents numerical algorithms implemented in the system and system results during increased geomagnetic activity (as an example of a weak magnetic storm from June 15, 2024) and seismic processes in Kamchatka (as an example of the November 2, 2018 earthquake). During the periods of the considered events, anomalous changes were detected in the ionosphere, which were accompanied with both the increase and decrease of the electron concentration.

Keywords: ionospheric disturbances, wavelet transform, autoregressive models.

UDC: 519.65

MSC: 41A99

Received: 08.11.2024
Accepted: 26.11.2024

DOI: 10.26117/2079-6641-2024-49-4-157-170



© Steklov Math. Inst. of RAS, 2025