VLF radio signal perturbations during two recent solar eclipses observed from a VLF receiving station, Cooch Behar, India

B. Das, S. Pal, P. K. Haldar
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Abstract

Effects of two recent solar eclipses of December 2019 and June 2020 on the Very Low Frequency (VLF) radio signal amplitudes, observed from a single receiving station at Cooch Behar (CHB), India, have been presented in this paper. Signal amplitudes of VLF transmitters such as VTX (18.2 kHz), NWC (19.8 kHz), JJI (22.2 kHz), and DHO (23.4 kHz) experienced both enhancement and reduction during the eclipse period. Depending on the eclipse obscuration over the propagation path, propagation distance, and frequency of the signal, increase and decrease of signal amplitudes were observed. The amplitude perturbation on the VLF signals was also opposite for the two eclipses on each propagation path. The possible reason behind the amplitude perturbations is the changes induced in the earth ionosphere waveguide during the solar eclipses and corresponding constructive or destructive interference that occurred between the waveguide modes of the received signal at each frequency.
在印度Cooch Behar的VLF接收站观测到的最近两次日食期间的VLF无线电信号扰动
本文介绍了2019年12月和2020年6月最近两次日食对印度Cooch Behar (CHB)单个接收站观测到的甚低频(VLF)无线电信号幅度的影响。在日食期间,VTX (18.2 kHz)、NWC (19.8 kHz)、JJI (22.2 kHz)和DHO (23.4 kHz)等VLF发射机的信号幅度既有增强又有降低。根据日食遮挡对信号传播路径、传播距离和频率的影响,观测到信号幅度的增减。在每条传播路径上,两次日食对VLF信号的振幅扰动也是相反的。振幅扰动背后的可能原因是日食期间地球电离层波导的变化以及在每个频率接收信号的波导模式之间发生的相应的建设性或破坏性干涉。
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