Tsunami detection using early-stage traveling ionospheric disturbances and machine learning based on GNSS measurements

IF 3.2 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Advances in Space Research Pub Date : 2026-07-15 Epub Date: 2026-05-05 DOI:10.1016/j.asr.2026.04.117
Danial Abdollahi, M. Mahdi Alizadeh
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引用次数: 0

Abstract

Natural hazards, such as earthquakes and tsunamis produce shock waves that travel into the ionosphere and produce traveling ionospheric disturbances (TIDs). TIDs should be detected in the case of earthquakes and tsunamis, as they can assist in monitoring natural hazards and provide early warning for tsunamis. A key challenge in detection is that TIDs also occur in the ionosphere as ordinary phenomena that are not caused by tsunamis. To address this issue, it must be noted that after a tsunami, TIDs are generated by two sources: acoustic waves from the earthquake shock, and gravity waves from tsunami propagation. Usually, tsunami TID detection is performed using gravity waves; however, gravity waves are weaker than acoustic waves and are more similar to ordinary ionospheric TIDs. Thus, to reduce false detections in near-field regions where tsunamis are strong and acoustic waves are present, this study focuses on early-stage TIDs—believed to be generated by acoustic waves—and incorporates their characteristics into a Levenberg–Marquardt backpropagation neural network for detection. GNSS time series of two giant tsunami events, the 2011 Tohoku and the 2004 Sumatra earthquakes and tsunamis, were considered. Because of the dense GNSS receiver coverage, the 2011 data were considered as the training and testing datasets, and the 2004 Sumatra dataset served as an independent validation case. The observations were classified into two categories: tsunami TIDs and non-tsunami TIDs. The test showed an accuracy of 99.8% in tsunami detection, and validation with observations from another region confirmed the model’s capacity to detect tsunami TIDs. This accuracy is higher than that of most previous detection systems and demonstrates its promising potential. Incorporating early-stage TID properties into a neural network enhances the practical reliability of tsunami detection.
利用早期电离层扰动和基于GNSS测量的机器学习进行海啸探测
自然灾害,如地震和海啸,会产生进入电离层的冲击波,并产生电离层扰动(TIDs)。在发生地震和海啸的情况下,应检测到tid,因为它们有助于监测自然灾害和提供海啸预警。探测方面的一个关键挑战是,TIDs也作为普通现象发生在电离层,不是由海啸引起的。为了解决这个问题,必须注意到海啸发生后,tid由两个来源产生:地震冲击的声波和海啸传播的重力波。通常,海啸TID探测是利用重力波进行的;然而,重力波比声波弱,更类似于普通的电离层tid。因此,为了减少在海啸强烈且声波存在的近场区域的错误检测,本研究侧重于早期的tid -被认为是由声波产生的-并将其特征合并到Levenberg-Marquardt反向传播神经网络中进行检测。考虑了2011年东北和2004年苏门答腊地震和海啸这两个巨大海啸事件的GNSS时间序列。由于GNSS接收机覆盖较密,将2011年数据作为训练和测试数据集,2004年苏门答腊数据作为独立验证案例。观测结果分为两类:海啸TIDs和非海啸TIDs。该测试表明,海啸探测的准确率为99.8%,并且与其他地区的观测数据进行验证,证实了该模型探测海啸TIDs的能力。这种精度高于大多数以前的检测系统,并显示出其良好的潜力。将早期海啸特征纳入神经网络,提高了海啸探测的实际可靠性。
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来源期刊
Advances in Space Research
Advances in Space Research 地学天文-地球科学综合
CiteScore
5.20
自引率
11.50%
发文量
800
审稿时长
5.8 months
期刊介绍: The COSPAR publication Advances in Space Research (ASR) is an open journal covering all areas of space research including: space studies of the Earth''s surface, meteorology, climate, the Earth-Moon system, planets and small bodies of the solar system, upper atmospheres, ionospheres and magnetospheres of the Earth and planets including reference atmospheres, space plasmas in the solar system, astrophysics from space, materials sciences in space, fundamental physics in space, space debris, space weather, Earth observations of space phenomena, etc. NB: Please note that manuscripts related to life sciences as related to space are no more accepted for submission to Advances in Space Research. Such manuscripts should now be submitted to the new COSPAR Journal Life Sciences in Space Research (LSSR). All submissions are reviewed by two scientists in the field. COSPAR is an interdisciplinary scientific organization concerned with the progress of space research on an international scale. Operating under the rules of ICSU, COSPAR ignores political considerations and considers all questions solely from the scientific viewpoint.
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