1 November 2006 Influence of a solar eclipse on Doppler frequency shift of signal from upper atmosphere
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Proceedings Volume 6522, Thirteenth Joint International Symposium on Atmospheric and Ocean Optics/ Atmospheric Physics; 652224 (2006) https://doi.org/10.1117/12.723269
Event: Thirteenth Joint International Symposium on Atmospheric and Ocean Optics/ Atmospheric Physics, 2006, Tomsk, Russian Federation
Abstract
The Doppler shift frequency (DSF) method and based on it the interference goniometric techniques are effectively applied in ionospheric researches [1-3]. The long-time continuous measurements are required for research the ionospheric processes and rare events, such as solar flashes and solar eclipses. In this article we present the results of measurements which were spent in measuring equipment "Spectr" of Kazan University.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
V. Yu. Teplov, V. Yu. Teplov, V. V. Bochkarev, V. V. Bochkarev, R. R. Latipov, R. R. Latipov, I. R. Petrova, I. R. Petrova, } "Influence of a solar eclipse on Doppler frequency shift of signal from upper atmosphere", Proc. SPIE 6522, Thirteenth Joint International Symposium on Atmospheric and Ocean Optics/ Atmospheric Physics, 652224 (1 November 2006); doi: 10.1117/12.723269; https://doi.org/10.1117/12.723269
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