Ionospheric Perturbations Due to Large Thunderstorms and the Resulting Mechanical and Acoustic Signatures

Author:

Ogunsua Babalola O.12,Qie Xiushu13,Srivastava Abhay14,Abe Oladipo Emmanuel5,Owolabi Charles26,Jiang Rubin1,Yang Jing1

Affiliation:

1. Key Laboratory for Middle Atmosphere and Global Environment Observation (LAGEO), Institute of Atmospheric Physics (IAP), Chinese Academy of Sciences, Beijing 100029, China

2. Department of Physics, Federal University of Technology, Akure 340252, Nigeria

3. College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China

4. Space and Atmospheric Science Division, North Eastern Space Applications Centre, Umiam 793103, India

5. Department of Physics, Federal University Oye Ekiti, Oye 370111, Nigeria

6. Geophysical Institute, University of Alaska, Fairbanks, AK 99775, USA

Abstract

Perturbations from thunderstorms can play a notable role in the dynamics of the ionosphere. In this work, ionospheric perturbation effects due to thunderstorms were extracted and studied. Thunderstorm-associated lightning activities and their locations were detected by the World-Wide Lightning Location Network (WWLLN). The mechanical components of ionospheric perturbations due to thunderstorms were extracted from the total electron content (TEC), which was measured at selected thunderstorm locations using the polynomial filtering method. Further analyses were conducted using wavelet analysis and Discrete Fourier Transform (DFT) to study the frequency modes and periodicities of TEC deviation. It was revealed that the highest magnitudes of TEC deviations could reach up to ~2.2 TECUs, with dominant modes of frequency in the range of ~0.2 mHz to ~1.2 mHz, falling within the gravity wave range and the second dominant mode in the acoustic range of >1 mHz to <7.5 mHz. Additionally, a 20–60 min time delay was observed between the sprite events, the other high-energy electrical discharges, and the time of occurrence at the highest peak of acoustic-gravity wave perturbations extracted from TEC deviations. The possible mechanism responsible for this phenomenon is further proposed and discussed.

Funder

National Natural Science Foundation of China

Publisher

MDPI AG

Subject

General Earth and Planetary Sciences

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