Virtual Reflection Height of Nighttime Equatorial Ionosphere Estimated With Low‐Frequency Magnetic Sferics Measured in Malacca

Author:

Wang Yongping12,Lu Gaopeng2ORCID,Cheng Zhengwei3ORCID,Niu Ziru2,Chen Yazhou4,Peng Kang‐Ming2,York Seah Boon2,Ahmad Mohd Riduan5ORCID

Affiliation:

1. Key Laboratory for Polar Science, Ministry of Natural Resources Polar Research Institute of China Shanghai China

2. School of Earth and Space Sciences University of Science and Technology of China Hefei China

3. State Key Laboratory of Space Weather National Space Science Center Chinese Academy of Sciences Beijing China

4. National Key Laboratory of Electromagnetic Environment Effects Army Engineering University Shijiazhuang China

5. Department of Computer Engineering Universiti Teknikal Malaysia Melaka Malacca Malaysia

Abstract

AbstractThe return stroke of cloud‐to‐ground (CG) lightning is an impulsive radiator of very low‐frequency/low‐frequency (VLF/LF) electromagnetic signals allowing for the remote sensing of lower ionosphere over large spatial coverage. In this study, we examined the LF magnetic fields measured in Malacca, Malaysia, to probe reflection heights of the lower ionosphere near the equator on three different nights in 2021. The results show that the virtual ionospheric height at nighttime typically ranged from 82.0 to 90.0 km, with a mean value of 85.3 km. Our measurements also revealed significant variations in the virtual ionospheric height across different regions over a spatial scale of about 800 km. The maximum height difference was about 5.0 km. Moreover, the fluctuation characteristics are observed in both estimated ionospheric height and calculated peak reflection ratio during similar periods. This fluctuation may be related to atmospheric gravity waves in the nighttime ionosphere. In addition, we compared the virtual ionospheric height estimated from CG strokes of different polarities, and the results showed that the virtual reflection height for positive CG strokes is lower than that for negative ones.

Funder

National Key Research and Development Program of China

National Natural Science Foundation of China

Chinese Academy of Sciences

Publisher

American Geophysical Union (AGU)

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