日本地球惑星科学連合2023年大会

講演情報

[E] 口頭発表

セッション記号 S (固体地球科学) » S-SS 地震学

[S-SS03] New trends in data acquisition, analysis and interpretation of seismicity

2023年5月23日(火) 09:00 〜 10:15 201A (幕張メッセ国際会議場)

コンビーナ:Enescu Bogdan(京都大学 大学院 理学研究科 地球惑星科学専攻 地球物理学教室)、Francesco Grigoli(University of Pisa)、青木 陽介(東京大学地震研究所)、座長:青木 陽介(東京大学地震研究所)、Enescu Bogdan(京都大学 大学院 理学研究科 地球惑星科学専攻 地球物理学教室)、庄 建倉(統計数理研究所)


09:15 〜 09:30

[SSS03-02] Directly Polarity Correction for Microseismic Event Location Using Hilbert Transform

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*Zhiyi Zeng1Peng Han1、Jincheng Xu1、Ying Chang2 (1.Southern University of Science and Technology, Shenzhen, China、2. Institute of Mining Engineering, BGRIMM Technology Group)


キーワード:Microseismic event, Migration diffraction stacking (MDS) imaging, Polarity correction

Microseismic events can delineate fault and fracture distribution in natural and induced earthquakes. Migration diffraction stacking (MDS) imaging implicitly assumes that the traveltime corrected seismic waveforms will stack coherently, making it a practical method to detect and locate microseismic events simultaneously. However, the polarity reversal caused by source radiation patterns interferes with the coherence stack. We develop a method of directly transforming the original signal polarity to consistency using the Hilbert transform, rather than aiming to identify and correct the polarity. The method can refocus the dispersed energy and preserves time-domain noise incoherence to suppress spatial-domain imaging noise. We have demonstrated its effectiveness with synthetic data. Application to real data from the coal-bed methane (CBM) fracture experiment locates more microseismic events in the practical fracturing depth. Since the polarity correction is completed in the data domain before imaging, this method is adapted to various seismic monitoring projects.

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