Paper
12 November 2020 Dependence of variation of parameters of the D-layer of the ionosphere during x-ray flashes of M and X classes from their energy
Author Affiliations +
Proceedings Volume 11560, 26th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics; 115608P (2020) https://doi.org/10.1117/12.2575607
Event: 26th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics, 2020, Moscow, Russian Federation
Abstract
The paper presents the variations in the parameters of the ionosphere D-layer during x-ray flares of M and X classes on the propagation path of signals from the superluminal waves of the GQD and GBZ transmitters, as well as those adopted by the Mikhnevo State Educational Center. It is shown that, within the framework of the two-parameter Ferguson-White model, the effective reflection height of the VLF signal h’ and the gradient of increase in the electron concentration β at the leading edge of the flare are related to the x-ray energy in the range 0.05–0.4 nm.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yu. V. Poklad, B. G. Gavrilov, V. M. Ermak, A. N. Lyakhov, I. A. Ryakhovskiy, and V. A. Rybakov "Dependence of variation of parameters of the D-layer of the ionosphere during x-ray flashes of M and X classes from their energy", Proc. SPIE 11560, 26th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics, 115608P (12 November 2020); https://doi.org/10.1117/12.2575607
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
X-rays

Solar radiation models

Transmitters

Atmospheric propagation

Solar radiation

Sun

Wave propagation

Back to Top