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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/109985


    題名: 2022年東加火山噴發引發之電離層擾動:觀測與數值模擬研究;Ionospheric Disturbances Induced by the 2022 Tonga Volcano Eruption: Observations and Numerical Simulations
    作者: 劉天祺;LIU, TIEN-CHI
    貢獻者: 太空科學與工程學系
    關鍵詞: 東加火山;電離層;大氣移行擾動;電離層移行擾動;Tonga volcano;ionosphere;traveling atmospheric disturbance;traveling ionospheric disturbance
    日期: 2026-07-28
    上傳時間: 2026-10-20 14:51:15 (UTC+8)
    出版者: 國立中央大學
    摘要: 2022年1月15日,宏加東加-宏加哈派(Hunga Tonga–Hunga Ha′apai)火山發生大規模噴發,產生強烈的大氣擾動,並由地表向上傳遞至高層大氣。此次火山噴發釋放大量能量,使包含蘭姆波(Lamb wave)、移行大氣擾動(traveling atmospheric disturbances, TADs)以及移行電離層擾動(traveling ionospheric disturbances, TIDs)在內的多種大氣與電離層擾動在全球各地皆有觀測紀錄,成為研究極端地球物理事件下大氣-電離層耦合過程的重要案例。

    本研究結合地表、衛星觀測資料與數值模擬結果,探討2022年東加火山噴發引發之電離層變化及其物理機制。使用之觀測資料包含電離層探測儀(ionosonde)、高頻都卜勒探測系統(HF Doppler sounding system)、氣壓計、潮位計、向日葵 8 號(Himawari-8)衛星影像、全球電離層圖(Global Ionosphere Maps, GIMTEC)、福爾摩沙衛星七號(FORMOSAT-7/COSMIC-2, F7C2)無線電掩星(radio occultation)與離子速度儀(Ion Velocity Meter, IVM)觀測、福爾摩沙衛星五號(FORMOSAT-5, Fs-5)先進電離層探測儀(Advanced Ionospheric Probe, AIP)資料,以及全球電離層再分析系統(Global Ionospheric Specification, GIS)之電子密度重建結果。此外,本研究亦利用全球電離層-熱氣層模式(Global Ionosphere–Thermosphere Model, GITM)進行數值模擬,探討觀測之電離層擾動形成機制。

    針對火山周圍之近場區域,全球電離層圖觀測顯示噴發後形成半徑約1650公里的傘狀擾動結構,於當地夜間呈現長時間之電漿密度消散區,並在日間轉變為電漿增強現象。夜間期間,全電子濃度(total electron content)減少約5–10 TECU,而F7C2與Fs-5觀測則分別顯示電漿密度下降約30–97% 與72–95%。隨著進入日間,原先的電漿耗損區轉變為增強區,其中TEC增加約2–18 TECU,離子密度則增加約234–532%。GIS 電子密度重建結果進一步指出,此擾動分布於約200至600公里高度,涵蓋大部分F層。GITM模擬結果重現大尺度電漿耗損之形成,並顯示火山噴發造成電漿由源區向外重新分布。綜合觀測與模擬結果顯示,傘狀電離層結構的形成與大氣膨脹、電離層抬升、分子離子復合反應增強,以及大尺度電漿傳輸等過程密切相關。

    針對遠場區域,本研究分析火山噴發產生之大氣與電離層擾動傳播特性。氣壓資料顯示,移行大氣擾動以300.8 ± 3.9 m/s的速度傳播至西太平洋區域,而臺灣與日本的電離層探測儀及高頻都卜勒觀測亦記錄到相對應的電離層變化。分析結果顯示,兩組不同TID分別以539.0 ± 22.3 m/s與338.3 ± 4.0 m/s的速度傳播,分別對應於熱氣層與對流層蘭姆波波前。這些擾動造成約86–155公里及50–110公里的電離層抬升,且TID抵達時間較相對應之蘭姆波波前提前約14–39分鐘,顯示蘭姆波之傳播可產生艏波(bow wave)並影響電離層。數值模擬亦成功重現此大尺度傳播特徵,說明火山噴發所產生之大氣波動可有效耦合至電離層。

    綜合觀測與模擬結果顯示,2022年東加火山噴發對熱氣層–電離層系統造成由區域至全球尺度之顯著且長時間影響。近場結果指出,極端火山事件可透過大氣動力過程、電漿傳輸及電離層化學反應之共同作用,造成大尺度的電漿耗損與增強;遠場結果則顯示,火山產生之蘭姆波能有效將能量傳遞至高層大氣,並在遠離火山之區域引發顯著電離層抬升。本論文透過整合多種觀測資料與數值模擬,釐清極端火山事件引發之大氣–電離層耦合過程,進而理解低層大氣擾動對太空環境之影響。;The major eruption of the Hunga Tonga–Hunga Ha′apai volcano on 15 January 2022 generated atmospheric disturbances that propagated from the Earth′s surface into the upper atmosphere and ionosphere. Due to the enormous energy released by the eruption, various atmospheric waves, including Lamb waves, traveling atmospheric disturbances (TADs), and traveling ionospheric disturbances (TIDs), are observed globally. The eruption therefore provides a unique opportunity to study atmosphere–ionosphere coupling processes triggered by an extreme geophysical event.

    This study examines the ionospheric responses to the 2022 Tonga volcanic eruption using a combination of ground-based and space-borne observations together with numerical simulations. Multiple observational datasets are employed, including ionosondes, HF Doppler sounding systems, barometers, tide gauges, Himawari-8 satellite observations, Global Ionosphere Maps (GIMTEC), FORMOSAT-7/COSMIC-2 (F7C2) radio occultation and ion -velocity meter (IVM) measurements, FORMOSAT-5 (Fs-5) Advanced Ionospheric Probe (AIP) observations, and Global Ionospheric Specification (GIS) electron density reconstructions. In addition, the Global Ionosphere–Thermosphere Model (GITM) is conducted to investigate the physical mechanisms responsible for the observed ionospheric perturbations.

    The first part of this dissertation investigates the near-field ionospheric response surrounding the eruption source region. GIMTEC reveals a long-lived umbrella-shaped plasma depletion during local nighttime and a subsequent daytime plasma enhancement extending approximately 1650 km from the volcano. During nighttime, TEC decreases by approximately 5–10 TECU, while F7C2 and Fs-5 observations indicate plasma density reductions of 30–97% and 72–95%, respectively. During daytime, the depleted region transitions into a broad plasma enhancement characterized by TEC increases of 2–18 TECU and ion density increases of 234–532%. Electron density reconstructions show that the disturbance extends from approximately 200 to 500 km altitude throughout much of the F-region ionosphere. Numerical simulations performed using the GITM reproduce the development of large-scale plasma depletion and reveal substantial plasma redistribution away from the eruption source region. Comparisons between observations and simulations suggest that atmospheric expansion, ionospheric uplift, enhanced molecular-ion recombination, and large-scale plasma transport collectively contribute to the formation of the observed umbrella-shaped ionospheric signatures.

    The second part of this dissertation examines the far-field propagation of eruption-generated atmospheric and ionospheric disturbances. Surface pressure observations identify a tropospheric Lamb wave propagating at 300.8 ± 3.9 m/s across the western Pacific region. Corresponding ionospheric responses are detected by ionosondes and HF Doppler sounding systems in Taiwan and Japan. Two distinct TIDs are identified with propagation speeds of 539.0 ± 22.3 m/s and 338.3 ± 4.0 m/s, respectively, and are associated with thermospheric and tropospheric Lamb-wave modes. These disturbances produce ionospheric uplifts of approximately 86–155 km and 50–110 km and are observed 14–39 min prior to the arrival of the corresponding Lamb-wave fronts, indicating the presence of bow-wave structures. Numerical simulations successfully reproduce the large-scale propagation characteristics of the disturbances and provide further evidence of atmosphere–ionosphere coupling driven by eruption-generated Lamb waves.

    The findings of this study demonstrate that the 2022 Tonga volcanic eruption produced profound and long-lasting modifications of the thermosphere–ionosphere system from regional to global scales. The near-field observations reveal that extreme volcanic forcing can generate large-scale plasma depletion and enhancement through the combined effects of atmospheric expansion, plasma transport, and ionospheric chemistry. The far-field observations further show that eruption-generated Lamb waves can couple efficiently into the ionosphere, producing substantial ionospheric uplift far from the source. By integrating multi-instrument observations with numerical simulations, this dissertation provides new insights into atmosphere–ionosphere coupling processes associated with extreme volcanic eruptions and improves our understanding of how disturbances originating in the lower atmosphere influence the space environment.
    顯示於類別:[太空科學研究所 ] 博碩士論文

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