2020年牙买加MW7.7地震前蜂群卫星磁场的时变背景场与异常分析

朱凯光 贺小丹 樊蒙璇 Dedalo Marchetti 王婷 温佳咪 张逸群

朱凯光,贺小丹,樊蒙璇,Dedalo Marchetti,王婷,温佳咪,张逸群. 2023. 2020年牙买加MW7.7地震前蜂群卫星磁场的时变背景场与异常分析. 地震学报,45(2):315−327 doi: 10.11939/jass.20210172
引用本文: 朱凯光,贺小丹,樊蒙璇,Dedalo Marchetti,王婷,温佳咪,张逸群. 2023. 2020年牙买加MW7.7地震前蜂群卫星磁场的时变背景场与异常分析. 地震学报,45(2):315−327 doi: 10.11939/jass.20210172
Zhu K G,He X D,Fan M X,Marchetti D,Wang T,Wen J M,Zhang Y Q. 2023. Time-varying background field and anomaly analysis of Swarm satellite magnetic field data before the 2020 Jamaica MW7.7 earthquake. Acta Seismologica Sinica,45(2):315−327 doi: 10.11939/jass.20210172
Citation: Zhu K G,He X D,Fan M X,Marchetti D,Wang T,Wen J M,Zhang Y Q. 2023. Time-varying background field and anomaly analysis of Swarm satellite magnetic field data before the 2020 Jamaica MW7.7 earthquake. Acta Seismologica Sinica45(2):315−327 doi: 10.11939/jass.20210172

2020年牙买加MW7.7地震前蜂群卫星磁场的时变背景场与异常分析

doi: 10.11939/jass.20210172
基金项目: 国家自然科学基金(41974084)和吉林省自然科学基金(20230101091JC)联合资助
详细信息
    通讯作者:

    朱凯光,博士,教授,主要研究方向为航空电磁探测技术及信号处理与地震前兆监测数据以及电磁卫星数据处理,e-mail:zhukaiguang@jlu.edu.cn

  • 中图分类号: P315.72

Time-varying background field and anomaly analysis of Swarm satellite magnetic field data before the 2020 Jamaica MW7.7 earthquake

  • 摘要: 蜂群卫星磁场数据受地磁活动和地方时的影响,本文先通过变分模态分解去除地磁活动对数据的影响,再建立时变背景场以消除地方时对数据的影响。基于建立的时变背景场,我们利用蜂群卫星磁场数据对2020年牙买加MW7.7地震进行震前异常分析,计算地震影响区域内轨道数据的能量值,利用时变背景场设置阈值提取异常。结果表明:牙买加地震影响区域内的异常轨道累计数量在震前50天至震前43天出现加速增长的现象。此外,基于时变背景场与昼、夜侧背景场提取异常的结果对比显示:由于昼、夜侧背景场的建立混合了多个当地时间的磁场数据,高值背景场会被低值背景场拉低,导致部分非异常的轨道被错误地识别为异常轨道;而低值背景场会被高值背景场抬高,导致部分异常轨道不能被识别。而时变背景场针对每一个地方时建立了更为准确的背景,其时间分辨率高,能凸显出不同地方时卫星磁场数据的背景值差异,这对异常轨道的准确提取十分重要。进一步对岩石层、大气层和电离层多圈层的参量进行了震前异常分析,并对三个圈层的异常出现时间进行解释,证明了这些异常可能与牙买加地震的孕育有关。

     

  • 图  1  2020年牙买加 MW7.7地震的地理位置和地震影响区(USGS,2020a

    Figure  1.  Location of the 2020 Jamaica MW7.7 earthquake and related earthquake affected areas (USGS,2020a

    图  2  两个模态的平均能量与对应的$a_p $指数

    (a) 轨道第一个模态的能量;(b) 轨道第二个模态的能量;(c) 轨道对应的$a_p $指数

    Figure  2.  Results of average energy of the two modes and their corresponding $a_p $ index

    (a) The average energy of the first mode of all the tracks;(b) The average energy of the second mode of all the tracks; (c) The $a_p $ index at the moment corresponding to the time of the track

    图  3  模态的平均能量与对应的$\overline a_p $的相关系数

    Figure  3.  The correlation coefficients between $\overline \varphi_{\rm{IMF1}} $ and $\overline a_p $ and those between $\overline \varphi_{\rm{IMF2}} $ and $\overline a_p $

    图  4  牙买加地震影响区域在不同地方时(LT)的时变背景场

    Figure  4.  The time-varying background field at different local time inside the earthquake affected areas of the Jamaica earthquake

    图  5  牙买加地震影响区域内24个地方时的平均背景值

    Figure  5.  The average background values of 24 local times inside the earthquake-affected area of the Jamaica earthquake

    图  6  基于时变背景场(a)与昼侧、夜侧背景场(b)分别提取的异常轨道累计结果

    Figure  6.  The cumulative number of anomalous tracks over time based on the time-varying background field (a) and the day-side and the night-side background field (b)

    图  7  地方时为白天(a)和夜晚(b)时昼侧、夜侧的两个背景场对比

    Figure  7.  Comparison between dayside and night side background field in the day time (a) and the night time (b)

    图  8  时变背景场与昼侧、夜侧背景场提取异常的阈值(a)及其对比图(b)

    Figure  8.  The threshold (a) of the time-varying background field and the day-side and the night-side background field used to extract anomalous tracks and its comparison (b)

    图  9  岩石层能量(a)、大气层总水气柱(b)和电离层磁场异常轨道(c)累计结果

    Figure  9.  Accumulative number of anomalies of the lithospheric energy (a), the total column water vapourof atmosphere (b) and the ionosphere magnetic field (c)

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出版历程
  • 收稿日期:  2021-11-15
  • 修回日期:  2022-02-10
  • 网络出版日期:  2023-03-20
  • 刊出日期:  2023-03-15

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