利用星群卫星研究土耳其和希腊随时间变化的磁异常变化:对 2017 年至 2020 年 M≥6 级地震的前兆多轨综合分析

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-03-26 DOI:10.1016/j.jastp.2024.106210
İlkin Özsöz , Oya Ankaya Pamukçu , Erdinç Timoçin
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引用次数: 0

摘要

本文介绍了一项全面的多轨道分析,旨在研究 2017 年 1 月至 2020 年 10 月期间发生的五次 M≥6 级地震在土耳其和希腊造成的随时间变化的磁异常变化。该研究利用了 Swarm 卫星的数据,并采用了各种分析技术,包括首次导数计算、长波分量去除和移动均方根滤波器,以构建每个磁分量的累积异常计数图。通过消除外部磁场的影响,我们只关注磁分量(X、Y、Z 和 F)。我们仔细解读了地震前、地震期间和地震后磁异常的变化。研究系统分析了普洛马里地震(2017 年 6 月 12 日)、科斯地震(2017 年 7 月 20 日)、Doğanyol 地震(2020 年 1 月 24 日)、Özalp 地震(2020 年 2 月 23 日)和 Karlovasion 地震(2020 年 10 月 30 日),考虑了每个磁分量的主震和余震反应。研究结果揭示了一些耐人寻味的模式,其中最引人注目的是在各种磁性成分中出现了独特的 S 型异常。此外,该研究还强调了普洛马利和科斯等重大地震对累积异常轨迹的影响,为了解磁场行为提供了重要依据。此外,研究还调查了厄扎尔普地震对在多安约尔地震中观测到的磁场异常的潜在影响,并探讨了多安约尔地震的发生与导致厄扎尔普地震主震的前兆异常之间的关系。此外,对 Karlovasion 地震的分析确定了主震前的磁异常。最后,研究对五次地震的横向和纵向得分进行了主观评估,以确定 S 型模式的表现能力。普洛马里地震和科斯地震分别获得了第三和第四高分,而多安约尔地震获得了最高分,并明显呈现出 S 形模式,这表明了其在磁场行为中的重要性。Özalp地震得分次之,呈明显的S形图案,而Karlovasion地震得分最低,没有明显的S形图案。此外,垂直分值表明 Y 和 Z 分量具有更明显的 S 形模式,而 X 和 F 分量的分值较低。值得注意的是,陆上 Doğanyol 地震在所有磁性成分中表现出最明显的 S 型模式,这归因于其位于 10 千米深处的浅走向滑动断层,而由位于 21 千米深处的正断层产生的离岸 Karlovasion 地震则表现出最分散的模式,为构造环境对磁场行为的影响提供了有价值的信息。总之,这项研究为了解与该地区地震事件相关的磁场异常提供了宝贵的信息,大大有助于更好地了解地震前兆和地震模式,加强地震风险评估和减灾战略。
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Time-dependent magnetic anomaly variations in Turkey and Greece using swarm satellites: A comprehensive precursory multi-track analysis of M≥6 earthquakes from 2017 to 2020

This article presents a comprehensive multi-track analysis aimed at investigating time-dependent magnetic anomaly variations in Turkey and Greece resulting from five M ≥ 6 earthquakes occurring between January 2017 and October 2020. The study utilizes data from the Swarm satellites and employs various analytical techniques, including first-time derivative calculations, long-wavelength component removal, and moving RMS filters, to construct cumulative anomaly count graphs for each magnetic component. By eliminating the influence of the external magnetic field, we focus solely on the magnetic components (X, Y, Z, and F). The changes in magnetic anomalies before, during, and immediately after the earthquakes are carefully interpreted. The research systematically analyses the Plomari (June 12, 2017), Kos (July 20, 2017), Doğanyol (January 24, 2020), Özalp (February 23, 2020), and Karlovasion (October 30, 2020) Earthquakes, considering the mainshock and aftershock responses for each magnetic component. The findings reveal intriguing patterns, most notably the emergence of distinctive S-shaped anomalies in various magnetic components. Moreover, the study highlights the influence of significant earthquakes, such as Plomari and Kos, on cumulative anomalous tracks, providing critical insights into magnetic field behavior. Additionally, the study investigates the potential impact of the Özalp Earthquake on the magnetic anomalies observed in the Doğanyol earthquake and explores the relationship between the occurrence of the Doğanyol Earthquake and the precursory anomalies leading to the mainshock of the Özalp Earthquake. Furthermore, the analysis of the Karlovasion earthquake identifies magnetic anomalies preceding the mainshock. Finally, the research subjectively assesses the lateral and vertical scores of the five earthquakes to capability to represent the S-shaped pattern. The Plomari and Kos earthquakes score third and fourth highest, respectively, while the Doğanyol Earthquake achieves the top score and distinctly displays an S-shaped pattern, indicating its significance in the magnetic field behavior. The Özalp Earthquake scores second-best with a distinct S-shaped pattern, while the Karlovasion Earthquake receives the lowest score with no evident S-shaped pattern. Additionally, vertical scores indicate the Y and Z components with more pronounced S-shaped patterns, while the X and F components receive lower scores. Notably, the onshore Doğanyol Earthquake exhibits the most pronounced S-shaped pattern across all magnetic components, attributable to its shallow strike-slip fault at 10 km depth, while the offshore Karlovasion Earthquake, generated by a normal fault at 21 km depth, displays the most scattered pattern, providing valuable information on the influence of tectonic settings on magnetic field behaviour. In conclusion, this study provides valuable insights into the magnetic anomalies associated with seismic events in the region, significantly contributing to a better understanding of earthquake precursors and seismicity patterns, and enhancing seismic risk assessment and mitigation strategies.

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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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