Paper
17 October 2023 Solar eclipse effects on 10 June 2021 in amplitude variations of VLF signals registering in Yakutsk
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Proceedings Volume 12780, 29th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 1278071 (2023) https://doi.org/10.1117/12.2689627
Event: XXIX International Symposium "Atmospheric and Ocean Optics, Atmospheric Physics", 2023, Moscow, Russian Federation
Abstract
The VLF signals from DHO and JXN registering in Yakutsk. During the solar eclipse on June 10, 2021 the maximum VLF amplitudes increased by 1.62 dB (11:39:18 UTC) and 1.4 dB (11:26:42 UTC) respectively. The relative changes of the ionizing radiation flux during an eclipse is characterized by the ratio of the areas of the open solar disk part to the total solar disk S(Φ)/S0. Along the DHO – Yakutsk and JXN – Yakutsk propagation paths the minimum average values S(Φ)/S0 are 0.532 (11:39:18 UTC) and 0.411 (11:33:00 UTC) respectively. The time of radio paths overlapping by the lunar shadow does not contradict the time interval of VLF amplitude variations registering in Yakutsk during the solar eclipse.
© (2023) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alexey A. Korsakov, Vladimir I. Kozlov, and Rustam R. Karimov "Solar eclipse effects on 10 June 2021 in amplitude variations of VLF signals registering in Yakutsk", Proc. SPIE 12780, 29th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 1278071 (17 October 2023); https://doi.org/10.1117/12.2689627
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KEYWORDS
Shadows

Radio propagation

Wave propagation

Transmitters

Waveguides

Analog to digital converters

Ionizing radiation

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