Signal-Processing Investigations on the Precursors of Strong Earthquakes Using GPS-TEC, ULF, and VLF Data

IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS
Swati, Manish Awasthi, Raj Pal Singh, Nitin Dubey, Devbrat Pundhir
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引用次数: 0

Abstract

The seismo-electromagnetic studies have been in progress since 1998 at Agra station. In the present paper, ionospheric GPS-TEC, ground-based ULF/VLF measurements were investigated in light of four strong earthquakes (M ≥ 6.8) that occurred around the Indian subcontinent in different periods. These three datasets are processed by using advanced signal-processing techniques in time and frequency domains. To analyze these datasets, a period of 16 days (including the day of the earthquake) was considered. For each day, only one minute of data was taken into account, with the time of the earthquake being the midpoint of that minute. The precursors are obtained in all the datasets considered before the occurrence of earthquakes. In TEC, ULF, and VLF data, significant changes are observed 2 to 15, 2 to 7, and 5 to 13 days before earthquakes, respectively. Significant results are obtained in time and frequency domains and the variations of solar and magnetic storm activities have also been examined thoroughly to check the validity of these variations. Further, these variations are interpreted in terms of lithosphere-atmosphere-ionosphere coupling mechanisms available in the literature.

Abstract Image

基于GPS-TEC、ULF和VLF数据的强震前兆信号处理研究
自1998年以来,阿格拉站的地震电磁研究一直在进行中。本文针对发生在印度次大陆不同时期的4次强震(M≥6.8),研究了电离层GPS-TEC、地面ULF/VLF测量结果。这三个数据集使用先进的信号处理技术在时域和频域进行处理。为了分析这些数据集,我们考虑了16天的时间段(包括地震当天)。每天只考虑一分钟的数据,地震时间为该分钟的中点。前兆是在地震发生前考虑的所有数据集中获得的。在TEC、ULF和VLF资料中,分别在地震前2 ~ 15天、2 ~ 7天和5 ~ 13天观测到显著变化。在时域和频域得到了重要的结果,太阳和磁暴活动的变化也被彻底地检查了这些变化的有效性。此外,根据文献中可用的岩石圈-大气-电离层耦合机制来解释这些变化。
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来源期刊
Geomagnetism and Aeronomy
Geomagnetism and Aeronomy Earth and Planetary Sciences-Space and Planetary Science
CiteScore
1.30
自引率
33.30%
发文量
65
审稿时长
4-8 weeks
期刊介绍: Geomagnetism and Aeronomy is a bimonthly periodical that covers the fields of interplanetary space; geoeffective solar events; the magnetosphere; the ionosphere; the upper and middle atmosphere; the action of solar variability and activity on atmospheric parameters and climate; the main magnetic field and its secular variations, excursion, and inversion; and other related topics.
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