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Relationship between the Fluence of Magnetospheric Electrons with Energies above 2 MeV and Geomagnetic and Interplanetary Characteristics in 1987–2021

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

Coefficients of correlation are calculated for the daily electron fluence, solar wind velocity, and the Ар-index of geomagnetic activity with different delays, along with electron fluences obtained for subsequent days using a dataset from 35 years (1987–2021) of measuring magnetospheric electron fluxes with energies of more than 2 MeV in geostationary orbits, solar wind velocity, and geomagnetic activity. A three-parameter model is developed that allows the fluence of high-energy magnetospheric electrons for the next day to be predicted on the basis of the prehistory of the behavior of the fluence, data on the Ap-index of geomagnetic activity, and measurements of the solar wind speed. Model calculations are in good agreement with experimental data with a high coefficient of correlation (0.82) for the period 1987–2021.

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Funding

This work was supported by the Science Committee of the RK Ministry of Education and Science, project no. АР08855916; and by the Aerospace Committee of the RK Ministry of Digital Development, Innovation, and the Aerospace Industry, program no. BR11265408.

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Correspondence to O. N. Kryakunova.

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The authors declare they have no conflicts of interest.

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Translated by G. Dedkov

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Kryakunova, O.N., Belov, A.V., Yakovets, A.F. et al. Relationship between the Fluence of Magnetospheric Electrons with Energies above 2 MeV and Geomagnetic and Interplanetary Characteristics in 1987–2021. Bull. Russ. Acad. Sci. Phys. 86, 1532–1536 (2022). https://doi.org/10.3103/S106287382212019X

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  • DOI: https://doi.org/10.3103/S106287382212019X

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