Paper
13 December 2018 the numerical simulation of the 2017 september solar X-flares impact on the midlatitude lower ionosphere
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Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 108339M (2018) https://doi.org/10.1117/12.2504292
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
Abstract
The progress in the physics and chemistry of the lower ionosphere depends on the verification of the numerical models on the experimental data. We establish the framework, that the lower ionosphere model can be considered as a valid one, only if the prediction for the VLF-LF radiowave propagation coincides with evidence both in amplitude and phase temporal dynamics. The extremely strong X-flares 06 and 10 September 2017 were chosen as a testbed for the empirical and theoretical models of the midlatitude lower ionosphere. Both models used GOES-15 X-ray flux measurements. Empirical model captures only the time moment of disturbance. Theoretical model captures the main feature in VLF response. We summarize the observed problems in simulation and prospective solutions as well.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrey N. Lyakhov, Julia A. Korsunskaya, Yuri V. Poklad, Boris G. Gavrilov, Ilya A. Ryakhovsky, Julius I. Zetzer, Tatiana V. Losseva, M. A. Bisyarin, V. V. Kirillov, A. B. Orlov, and A. E. Pronin "the numerical simulation of the 2017 september solar X-flares impact on the midlatitude lower ionosphere", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 108339M (13 December 2018); https://doi.org/10.1117/12.2504292
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Cited by 2 scholarly publications.
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KEYWORDS
Solar radiation models

Solar processes

Ionization

Transmitters

Numerical simulations

X-rays

Data modeling

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