日本地球惑星科学連合2021年大会

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セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG39] Science of slow earthquakes: Toward unified understandings of whole earthquake process

2021年6月5日(土) 13:45 〜 15:15 Ch.21 (Zoom会場21)

コンビーナ:井出 哲(東京大学大学院理学系研究科地球惑星科学専攻)、廣瀬 仁(神戸大学都市安全研究センター)、氏家 恒太郎(筑波大学生命環境系)、波多野 恭弘(大阪大学理学研究科)、座長:波多野 恭弘(大阪大学理学研究科)

13:45 〜 14:00

[SCG39-07] 線形臨界安定性解析の観点による滑り端伝播速度の統一的理解

*鈴木 岳人1 (1.青山学院大学理工学部物理・数理学科)

キーワード:滑り端伝播速度、摩擦則、線形臨界安定性解析

Slip-front-propagation on an interface between two media has attracted interests of many researchers in scientific and industrial fields. In particular, the slip-front-propagation velocity has been obtained using some friction laws such as the slip-velocity-dependent law. Notably, to obtain the propagation velocity, Linear Marginal Stability Hypothesis (LMSH) has been widely employed. First, LMSH assumes the plane wave solution for the slip profile near the slip front, i.e., u~exp(i (k x-omega t)), where u is the slip and k and omega are the complex wave number and frequency, respectively. The imaginary parts of k and omega are written as ki and omegai, respectively, and the slip-front-propagation velocity is given by v=omegai/ki. We consider the friction law depending on both the slip and slip velocity, leading to two model parameters in the governing equation. We therefore assume that the terms C1 u and C2 \dot{u}, where C1 and C2 are the constants, emerge in the governing equation for u. We have obtained the cubic equation for omegai using LMSH, and found that the numbers of the solutions for omegai can be categorized into 12 regions on the C1-C2 phase space. Here, we aim to categorize the slip-front-propagation velocity on the C1-C2 phase space, and give some implications associated with slow earthquakes.

We should emphasize that the slip front has two forms: the intruding and extruding fronts (see details in Suzuki and Matsukawa, 2019). Actually, we have obtained the analytical solutions for omegai, and they are called omegain1, omegain2, and omegain3 for the intruding front, and omegaex1, omegaex2, and omegaex3 for the extruding front. Using these values and the relationship between ki and omegai, we have also obtained the analytical forms of ki, which are called kin1, kin2, and kin3 for the intruding front, and kex1, kex2, and kex3 for the extruding front. Therefore, we can write analytical forms for the intruding and extruding slip-front-propagation velocities, vinj=omegainj/kinj and vexj=omegaexj/kexj (j=1,2,3), respectively.

In terms of the solutions of vinj and vexj, the C1-C2 phase space is divided into 7 regions. They are the regions with (A) vin1, (B) vex1, (C) vin1 and vex2, (D) vex1 and vex3, (E) vin1, vex2, and vin3, (F) vin1, vex2, and vex3, and (G) no propagation velocity. In particular, we emphasize that there exists the region where vinj or vexj does not exist. This region cannot generate the steady slip-front-propagation, and may imply the generation of slow earthquakes from seismological viewpoint.