29 November 2016 Estimation of effective height changes of Earth-ionosphere waveguide by VLF radio signals phase variations during a solar eclipse
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Proceedings Volume 10035, 22nd International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 100351J (2016) https://doi.org/10.1117/12.2248802
Event: XXII International Symposium Atmospheric and Ocean Optics. Atmospheric Physics, 2016, Tomsk, Russian Federation
Abstract
During the solar eclipse of May 20 - 21, 2012 in Yakutsk VLF radio signal phase variations are recorded. The variations are 0.77 and 0.54 radians for JJY40 and NPM radio stations respectively. By the radio signals phase variations a normalization factor is determined. The normalization coefficients are 3,27 ± 0,08 and 2,27 ± 0,05 km for paths JJY40 - Yakutsk and NPM - Yakutsk respectively. The effective height of the Earth-ionosphere waveguide changing for the maximum shading the path JJY40 - Yakutsk (22:47 UT) is 4.63 km. For the path NPM - Yakutsk the effective height changes in maximum shading (23:52 UT) are 4.25 km.
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Alexey A. Korsakov, Alexey A. Korsakov, Vladimir I. Kozlov, Vladimir I. Kozlov, Rustam R. Karimov, Rustam R. Karimov, } "Estimation of effective height changes of Earth-ionosphere waveguide by VLF radio signals phase variations during a solar eclipse", Proc. SPIE 10035, 22nd International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 100351J (29 November 2016); doi: 10.1117/12.2248802; https://doi.org/10.1117/12.2248802
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