JOURNAL ARTICLE
An Investigation on the Ionospheric Response to the Volcanic Explosion at Hunga Ha'apai in 2021.
Published In: Journal of Geophysical Research. Space Physics, 2023, v. 128, n. 11. P. 1 1 of 3
Database: Applied Science & Technology Source Ultimate 2 of 3
Authored By: Qiu, Shican; Zhang, Zhanming; Soon, Willie; Velasco Herrera, Victor Manuel; Dou, Xiankang 3 of 3
Abstract
The Hunga Ha'apai volcano eruption (20.536°S, 175.382°W in Tonga), which started intermittently around December 2021 and most violently erupted on 15 January 2022, is considered to be the largest volcanic outbreak in recent decades. In this research, we derived the ionospheric total electron content (TEC) over Sanya (18.400°N, 109.600°E), Wuhan (30.530°N, 114.610°E), and Mohe (53.500°N, 122.370°E), from the Global Navigation Satellite System observations. Then we investigated the coupling between the volcano eruption and ionosphere through the TEC variations. The TEC anomaly decayed from about 10 days before main eruption of the Hunga Ha'apai volcano, and showed obvious fluctuations during the eruption phase. The TEC anomaly propagated periodically, with its autocorrelation‐analyzed period of about 16.5 hr during the intermittent outbreak and about 8 hr during the main outbreak phase. Its independently derived wavelet‐analyzed periods are about 9.4 hr during the intermittent outbreak and about 9.4 and 18.8 hr during the main outbreak phase. The propagation is mainly expressed in low frequencies, with energy concentrated in the range of 0–10−3 Hz. This study highlights that the preeruption activities may play an important role in the coupling between the volcanic eruption and ionosphere disturbances. Plain Language Summary: In this research, we study the response of ionosphere to the volcanic explosion of Hunga Ha'apai through the total electron content (TEC) over Sanya (18.400°N, 109.600°E), Wuhan (30.530°N, 114.610°E), and Mohe (53.500°N, 122.370°E), from the Global Navigation Satellite System. We investigated the coupling between the volcano eruption and ionosphere through the TEC variations. We found that the TEC anomalies are propagated periodically with periods of about 8–9 hr and 16–19 hr during the intermittent activity phase and the main eruptive phase, respectively. We envision that these signals probably reflect the nature of the impacts of Hunga Ha'apai volcano eruption processes on the ionosphere. Key Points: The ionospheric total electron content decayed starting 10 days before the main eruption and showed obvious fluctuations during the eruption phaseThe anomaly propagated with autocorrelation‐analyzed period of ∼16.5 and ∼8 hr during intermittent and main outbreak phases, respectivelyThe anomaly propagation is mainly expressed by low frequencies, with energy concentrated in the range of 0–10−3 Hz [ABSTRACT FROM AUTHOR]
Additional Information
- Source:Journal of Geophysical Research. Space Physics. 2023/11, Vol. 128, Issue 11, p1
- Document Type:Article
- Subject Area:History
- Publication Date:2023
- ISSN:21699380
- DOI:10.1029/2023JA031731
- Accession Number:173893343
- Copyright Statement:Copyright of Journal of Geophysical Research. Space Physics is the property of Wiley-Blackwell and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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