2020年1月24日土耳其地震的地磁效应

Q4 Physics and Astronomy
Y. Luo, L. Chernogor, K. Garmash
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It is considered that the EQ action is caused by cracking of rocks, fluctuating motion in the pore fluid, static electricity discharges, etc. In the course of EQs, the seismic, acoustic, atmospheric gravity waves (AGWs), and magnetohydrodynamic (MHD) waves are generated. The purpose of this paper is to describe the magnetic effects of the EQ, which took place in Turkey on 24 January 2020. Design/methodology/approach: The measurements are taken with the fluxmeter magnetometer delivering 0.5-500 pT sensitivity in the 1-1000 s period range, respectively, and in a wide enough studied frequency band within 0.001 to 1 Hz. The EM-II magnetometer with the embedded microcontroller digitizes the magnetometer signals and performs preliminary filtering over 0.5 s time intervals, while the external flash memory is used to store the filtered out magnetometer signals and the times of their acquisition. 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The quasi-periodic variations in the level of the H and D components of the geomagnetic field, which followed 75 min after the EQ, were caused by a magnetic disturbance produced by the traveling ionospheric disturbances due to the AGWs launched by the EQ. The magnetic effect amplitude was estimated to be close to 0.3 nT, and the quasi-period to be 700-900 s. The amplitude of the disturbances in the electron density in the AGW field was estimated to be about 8 % and the period of 700-900 s. Damping oscillations in both components of the magnetic field were detected to occur with a period of approximately 120 s. This effect is supposed to be due to the shock wave generated in the atmosphere in the course of the EQ. Conclusions: The magnetic variations associated with the EQ and occurring before and during the EQ have been studied in the 1-1000 s period range. 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引用次数: 1

摘要

目的:地磁扰动的主要原因是宇宙源、作用于太阳风和行星际介质的过程,以及进入地球大气层的大型天体。地震也会产生地磁效应。根据系统范式,地球-大气层-电离层-磁层系统(EAIMS)构成了一个统一的系统,在这个系统中,子系统之间发生了正负耦合,系统组件之间也发生了反馈和前提。岩石圈中EQ和过程对地磁场的作用机制尚不清楚。认为EQ作用是由岩石破裂、孔隙流体波动、静电放电等引起的。在EQs过程中,会产生地震、声波、大气重力波(AGW)和磁流体动力学(MHD)波。本文的目的是描述2020年1月24日在土耳其举行的EQ的磁效应。设计/方法/方法:使用磁通计磁强计进行测量,磁强计分别在1-1000s的周期范围内提供0.5-500pT的灵敏度,并在0.001至1Hz的足够宽的研究频带内进行测量。带有嵌入式微控制器的EM-II磁力计将磁力计信号数字化,并在0.5 s的时间间隔内执行初步滤波,而外部闪存用于存储过滤掉的磁力计信号及其采集时间。为了详细研究准周期过程,将地磁场H和D分量水平的时间变化应用于系统频谱分析,该分析利用了短时傅立叶变换、以Morlet小波为基函数的小波变换、,以及在宽度被调整为等于固定数量的谐波周期的滑动窗口中的傅立叶变换。研究结果:在2020年1月23日EQ前25.5小时观察到的D分量水平的一系列振荡被认为与磁性前兆有关。2020年1月24日观察到的H分量中的双向脉冲可能是由于EQ的活塞作用,EQ产生了MHD脉冲。EQ后75分钟,地磁场H和D分量水平的准周期性变化是由EQ发射的AGW引起的电离层移动扰动产生的磁扰动引起的。磁效应振幅估计接近0.3 nT,准周期为700-900 s。AGW场中电子密度扰动的振幅估计约为8%,周期为700-900秒。检测到磁场两个分量中的阻尼振荡发生的周期约为120秒。这种影响被认为是由于EQ过程中大气中产生的冲击波。结论:已经研究了在1-1000s周期范围内与EQ相关的以及在EQ之前和期间发生的磁变化。关键词:地震、磁通计磁强计、准周期扰动、地震波、重力声波、磁流体脉冲
本文章由计算机程序翻译,如有差异,请以英文原文为准。
GEOMAGNETIC EFFECT OF TURKISH EARTHQUAKE OF JANUARY 24, 2020
Purpose:The main cause of geomagnetic disturbances are cosmic sources, processes acting in the solar wind and in the interplanetary medium, as well as large celestial bodies entering the terrestrial atmosphere. Earthquakes (EQs) also act to produce geomagnetic effects. In accordance with the systems paradigm, the Earth–atmosphere–ionosphere–magnetosphere system (EAIMS) constitute a unified system, where positive and negative couplings among the subsystems, as well as feedbacks and precondition among the system components take place. The mechanisms for the action of EQs and processes acting in the lithosphere on the geomagnetic field are poorly understood. It is considered that the EQ action is caused by cracking of rocks, fluctuating motion in the pore fluid, static electricity discharges, etc. In the course of EQs, the seismic, acoustic, atmospheric gravity waves (AGWs), and magnetohydrodynamic (MHD) waves are generated. The purpose of this paper is to describe the magnetic effects of the EQ, which took place in Turkey on 24 January 2020. Design/methodology/approach: The measurements are taken with the fluxmeter magnetometer delivering 0.5-500 pT sensitivity in the 1-1000 s period range, respectively, and in a wide enough studied frequency band within 0.001 to 1 Hz. The EM-II magnetometer with the embedded microcontroller digitizes the magnetometer signals and performs preliminary filtering over 0.5 s time intervals, while the external flash memory is used to store the filtered out magnetometer signals and the times of their acquisition. To investigate quasi-periodic processes in detail, the temporal variations in the level of the H and D components of the geomagnetic field were applied to the systems spectral analysis, which makes use of the short-time Fourier transform, the wavelet transform using the Morlet wavelet as a basis function, and the Fourier transform in a sliding window with a width adjusted to be equal to a fixed number of harmonic periods. Findings: The train of oscillations in the level of the D component observed 25.5 h before the EQ on 23 January 2020 is supposed to be associated with the magnetic precursor. The bidirectional pulse in the H component observed on 24 January 2020 could be due to the piston action of the EQ, which had generated an MHD pulse. The quasi-periodic variations in the level of the H and D components of the geomagnetic field, which followed 75 min after the EQ, were caused by a magnetic disturbance produced by the traveling ionospheric disturbances due to the AGWs launched by the EQ. The magnetic effect amplitude was estimated to be close to 0.3 nT, and the quasi-period to be 700-900 s. The amplitude of the disturbances in the electron density in the AGW field was estimated to be about 8 % and the period of 700-900 s. Damping oscillations in both components of the magnetic field were detected to occur with a period of approximately 120 s. This effect is supposed to be due to the shock wave generated in the atmosphere in the course of the EQ. Conclusions: The magnetic variations associated with the EQ and occurring before and during the EQ have been studied in the 1-1000 s period range. Key words: earthquake, fluxmeter magnetometer, quasi-periodic disturbance, seismic wave, acoustic-gravity wave, MHD pulse
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来源期刊
Radio Physics and Radio Astronomy
Radio Physics and Radio Astronomy Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
0.60
自引率
0.00%
发文量
18
审稿时长
8 weeks
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