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Dynamics of High-Energy Proton Fluxes in the South Atlantic Anomaly Region According to ARINA and VSPLESK Satellite Experiment Data

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Abstract

This paper studies the dynamics of proton flux in the South Atlantic Anomaly (SAA) region according to ARINA (was operated on the Resurs-DK1 satellite from 2006 to 2015) and VSPLESK (which was mounted on the ISS from 2008 to 2013) satellite experiment data. Both spectrometers have the same scheme. The SAA drift is determined by the position of the maximum flux of high-energy protons with energies in the range from 30 to 100 MeV at the altitude of the Resurs-DK1 satellite (about 580 km) and the ISS (380–420 km). Part of the time the instruments operated simultaneously.

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Funding

This work was supported by ongoing institutional funding. No additional grants to carry out or direct this particular research were obtained.

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Authors and Affiliations

  1. National Research Nuclear University ‘‘MEPhI’’, Moscow, Russia

    S. Yu. Aleksandrin, V. M. Grachev & E. I. Olshevsky

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  1. S. Yu. Aleksandrin
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  2. V. M. Grachev
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  3. E. I. Olshevsky
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Correspondence to S. Yu. Aleksandrin.

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Translated by E. Oborin

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Aleksandrin, S.Y., Grachev, V.M. & Olshevsky, E.I. Dynamics of High-Energy Proton Fluxes in the South Atlantic Anomaly Region According to ARINA and VSPLESK Satellite Experiment Data. Phys. Atom. Nuclei 86, 1138–1142 (2023). https://doi.org/10.1134/S1063778824010058

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  • DOI: https://doi.org/10.1134/S1063778824010058

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