Reaction of the high-latitude lower ionosphere to solar proton events from observations in the ELF range
- Authors: Lebed’ O.M.1, Larchenko A.V.1, Pil’gaev S.V.1, Fedorenko Y.V.1
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Affiliations:
- Polar Geophysical Institute
- Issue: Vol 57, No 1 (2017)
- Pages: 51-57
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156137
- DOI: https://doi.org/10.1134/S0016793217010078
- ID: 156137
Cite item
Abstract
The reaction of the lower ionosphere to the solar proton events that occurred in 2011–2012 is studied in this paper based on the results of measurements of the propagation velocity and the Ez/Hτ ratio of the low-frequency electromagnetic pulses (atmospherics) in the ELF range at the high-latitude observatories Lovozero and Barentsburg. With numerical modeling methods, it is shown that horizontal local irregularities of the lower ionosphere conductivity profile could be a cause of the splashes in the Ez/Hτ ratio observed in the experiment during the solar proton event of March 7, 2012, which was a unique event in both the proton flux value and energy.
About the authors
O. M. Lebed’
Polar Geophysical Institute
Author for correspondence.
Email: olgamihsh@yandex.ru
Russian Federation, Apatity, 184200
A. V. Larchenko
Polar Geophysical Institute
Email: olgamihsh@yandex.ru
Russian Federation, Apatity, 184200
S. V. Pil’gaev
Polar Geophysical Institute
Email: olgamihsh@yandex.ru
Russian Federation, Apatity, 184200
Yu. V. Fedorenko
Polar Geophysical Institute
Email: olgamihsh@yandex.ru
Russian Federation, Apatity, 184200
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