Effect of total lunar eclipse of 27th July 2018 on the D-region ionosphere by using VLF observations

In this report, an effort for the first time has been made to investigate the effect of the total Lunar Eclipse that occurred on 27th July 2018 (the longest lunar eclipse in the 21st century) on the D-region ionosphere. Very Low Frequency (VLF) navigational transmitter signals recorded at Prayagraj (formally Allahabad) station in India is the primary dataset used. The signals from two VLF transmitters: NWC (19.8 kHz) from Australia, and JJI (22.2 kHz) from Japan, have been utilized. When compared to unperturbed night, NWC signal amplitude showed an anomalous decrease of similar to 0.86 dB, while JJI amplitude showed an anomalous increase similar to 0.26 dB during the lunar eclipse. The Wait's lower ionospheric parameters: reflection height (H') and sharpness factor (beta) are estimated by using a rather coarse method of modeling of VLF signals anomalies on eclipse day, which comes out to be H' = 85.25 km & beta = 0.689 km(-1) and H' = 84.59 km & beta = 0.683 km(-1) respectively for NWC and JJI path. Using wait parameters, the electron density (N-e) profile is estimated and this showed a decrease in N-e during eclipse time with reference to the nighttime ambient values. The N-e values for the NWC path, showed relatively higher decrease compared to the JJI path. The plausible reasons for observed N-e decrease on lunar eclipse night could be due to the reflected lunar Lyman-c( and X-ray's radiation which may contribute to the nighttime ionization is blocked during the lunar eclipse, thereby decreasing the nighttime lower ionospheric N-e. (C) 2021 COSPAR. Published by Elsevier B.V. All rights reserved.

Automated summary

This study investigated the impact of a total Lunar Eclipse on the D-region ionosphere using VLF signals recorded in India. The study found anomalous changes in signal amplitudes during the eclipse and estimated lower ionospheric parameters. The decrease in electron density during the eclipse may be due to blocked nighttime ionization by reflected lunar radiation.