Preseismic Ionospheric Electric Field Irregularities Detected by the Double Probes Method

IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS
S. Makhlouf, M. Djebli
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引用次数: 0

Abstract

Based on the double probe method, we investigated the ionospheric preseismic electric effects for the strong Chile earthquake of magnitude M = 8.8 that occurred on February 27, 2010, at 06:3414 universal time (UT). To correlate the electrical disturbance to natural geophysical activities in the ionosphere associated with the earthquake, we used a new approach to analyze these disturbances a few days before the event, based on DEMETER spacecraft collected data in the ultra low frequency (ULF) band. The double probes method and the calculated preseismic ionospheric electric field resulting from the potential difference between two electrical probes of ICE (Instrument Champ Electrique) onboard the DEMETER satellite are investigated. Once the effect of the satellite motion is canceled, it is found that the disturbance is caused only by the telluric activity. Moreover, the investigation of the collected data illustrates a clear correlation between preseismic electrical disturbances and ionospheric plasma parameters recorded near the future epicenter. The strongest ionospheric electrical disturbances are located near the future epicenter and close to the geomagnetic conjugate points.

Abstract Image

双探头法探测到的地震前电离层电场不规则现象
基于双探头方法,我们研究了 2010 年 2 月 27 日世界时 06:3414 发生的 M = 8.8 级智利强烈地震的电离层震前电效应。为了将电扰动与地震相关的电离层中的自然地球物理活动联系起来,我们使用了一种新方法,根据 DEMETER 航天器收集的超低频(ULF)波段数据,在地震发生前几天对这些扰动进行分析。研究了双探头方法和由 DEMETER 卫星上的两个电探头 ICE(Instrument Champ Electrique)之间的电位差产生的地震前电离层电场的计算结果。一旦消除了卫星运动的影响,就会发现扰动仅由碲活动引起。此外,对所收集数据的研究表明,震前电扰动与未来震中附近记录的电离层等离子参数之间存在明显的相关性。最强的电离层电扰动位于未来震中附近和地磁共轭点附近。
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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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