日本地球惑星科学連合2014年大会

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セッション記号 S (固体地球科学) » S-SS 地震学

[S-SS29_28PM2] 地震発生の物理・震源過程

2014年4月28日(月) 16:15 〜 17:30 416 (4F)

コンビーナ:*加瀬 祐子(産業技術総合研究所 活断層・地震研究センター)、座長:麻生 尚文(東京大学大学院理学系研究科)、矢部 康男(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)

16:30 〜 16:45

[SSS29-09] Stress concentration ahead of supershear rupture

*福山 英一1徐 世慶1溝口 一生2山下 太1 (1.防災科学技術研究所、2.電力中央研究所)

キーワード:Earthquake rupture, Stress concentration, Supershear rupture

We report the shear strain field ahead of a supershear rupture. The strain data was obtained during the large-scale biaxial friction experiments conducted at NIED in March 2013. We conducted friction experiments using a pair of meter-scale gabbro rock specimens whose fault area was 1.5m x 0.1m. We applied 2.6MPa normal stress and loading velocity of 0.1mm/s. At the long side of the fault edge, which is parallel to the slip direction, 32 2-component semi-conductor strain gauges were installed at an interval of 50mm and 10mm off the fault. The data are conditioned by high frequency strain amplifiers (<0.5MHz) and continuously recorded at an interval of 1MHz with 16-bit resolution. Many stick slip events were observed and a unilateral rupture event was chosen in this analysis that propagated with supershear rupture velocity. By focusing at the rupture front, stress concentration was observed and sharp stress drop occurred immediately inside the rupture. We found that the stress concentration becomes mild as the rupture propagates and length of the stress concentration area becomes longer. This observation is quite interesting because the rupture propagates at a constant speed close to square root two times the shear wave velocity and thus a longer stress concentration region suggests more energy dissipation. We might speculate that such longer stress concentration area suggests longer plastic region ahead of the rupture (or longer cohesive distance). I.e. The cohesive zone length might be longer as the rupture propagates to maintain constant rupture velocity propagation.