Fault ‘scratches’ offer clues to rupture direction

Temblor ◽  
2020 ◽  
Author(s):  
Jennifer Schmidt ◽  
Keyword(s):  
Rupture Direction

Rupture direction study of two Tonghai Ms 5.0 earthquakes on August 13 and 14, 2018

2019 ◽  
pp. 573-580
Author(s):  
Xueliang Chen* ◽  
Quanbo Luo ◽  
Mengtan Gao ◽  
Sen Qiao ◽  
Shicheng Li ◽  
...  
Keyword(s):  
Rupture Direction

Curved slickenlines preserve direction of rupture propagation

Geology ◽  
2019 ◽  
Vol 47 (9) ◽  
pp. 838-842
Author(s):  
Jesse Kearse ◽  
Yoshihiro Kaneko ◽  
Tim Little ◽  
Russ Van Dissen
Keyword(s):  
Cohesive Zone ◽  
Strike Slip ◽  
Rupture Propagation ◽  
Dynamic Rupture ◽  
Slip Direction ◽  
Rupture Dynamics ◽  
Earthquake Rupture Dynamics ◽  
Kaikoura Earthquake ◽  
Rupture Direction ◽  
Dextral Strike Slip

Abstract Slip-parallel grooves (striations) on fault surfaces are considered a robust indicator of fault slip direction, yet their potential for recording aspects of earthquake rupture dynamics has received little attention. During the 2016 Kaikōura earthquake (South Island, New Zealand), >10 m of dextral strike-slip on the steeply dipping Kekerengu fault exhumed >200 m2 of fresh fault exposure (free faces) where it crossed bedrock canyons. Inscribed upon these surfaces, we observed individual striae up to 6 m long, all of which had formed during the earthquake. These were typically curved. Using simulations of spontaneous dynamic rupture on a vertical strike-slip fault, we reproduce the curved morphology of striae on the Kekerengu fault. Assuming strike-slip pre-stress, our models demonstrate that vertical tractions induced by slip in the so-called cohesive zone result in transient changes in slip direction. We show that slip-path convexity is sensitive to the direction of rupture propagation. To match the convexity of striae formed in 2016 requires the rupture to have propagated in a northeast direction, a prediction that matches the known rupture direction of the Kaikōura earthquake. Our study highlights the potential for fault striae to record aspects of rupture dynamics, including the rupture direction of paleo strike-slip earthquakes.

XFEM SIMULATION OF RUPTURE DIRECTION ON BRANCHING FAULT

2020 ◽  
Vol 76 (2) ◽  
pp. I_217-I_224
Author(s):  
Daiki YAMASHITA ◽  
Hiroyuki GOTO ◽  
Sumio SAWADA
Keyword(s):  
Rupture Direction

scholarly journals Rupture velocity inferred from near-field shear strain analysis

2014 ◽  
Vol 199 (3) ◽  
pp. 1709-1712 ◽  
Author(s):  
M. Causse ◽  
C. Cornou ◽  
J. Bécasse
Keyword(s):  
Shock Waves ◽  
Phase Velocity ◽  
Shear Strain ◽  
Fractured Rock ◽  
Near Field ◽  
Strain Analysis ◽  
Rupture Velocity ◽  
Fault Trace ◽  
A New Technique ◽  
Rupture Direction

Abstract We propose a new technique to determine the rupture velocity of large strike slip earthquakes. By means of simple numerical ground motion simulations, we show that when the rupture penetrates a shallow layer of sediment or fractured rock, shock waves propagate along the surface fault trace in the forward rupture direction. Such shock waves, which are insensitive to the complexity of slip over the fault plane, propagate at a phase velocity equal to the rupture speed. We show that those shock waves can be easily isolated in the frequency domain, and that phase velocity can then be simply obtained from shear strain.

Near-field source parameters by finite-source theoretical seismograms

1977 ◽  
Vol 67 (3) ◽  
pp. 631-640 ◽  
Author(s):  
Moshe Israel ◽  
Moshe Vered
Keyword(s):  
Epicentral Distance ◽  
Near Field ◽  
Source Parameters ◽  
Dynamics Model ◽  
Field Source ◽  
San Andreas ◽  
Fault Parameters ◽  
Calculated Amplitude ◽  
Hypocentral Location ◽  
Rupture Direction

abstract Near-field seismograms due to finite faulting in a half-space were calculated. An attempt is made to evaluate near-field fault parameters by using two criteria: (1) agreement of observed and theoretical pulse width; and (2) agreement of observed and calculated amplitude ratios of the horizontal components of motion. Using this method we have investigated possible fault parameters of an earthquake along the San Andreas fault (source depth 12.5 km), recorded at two stations (epicentral distance 2.3, 5.5 km). It is found that computed seismograms are strongly dependent on the point in which a unilateral fracture begins. Assuming different initial failure points within the uncertainty region of the hypocentral location may effect fault parameter solutions. Thus, fault parameters obtained in this study should not be viewed as unique. However, we have shown, that for an assumed point and dynamics model, it is possible to determine rupture direction and source parameters. The seismic moment found in this study is weakly dependent on the dynamics model assumed.

Within and Between-Events Variability of Strong-Velocity Pulses

2020 ◽  
Author(s):  
Ming-Hsuan Yen ◽  
Kuo-Fong Ma ◽  
Fabrice Cotton ◽  
Yen-Yu Lin ◽  
Ya-Ting Lee
Keyword(s):  
Seismic Hazard ◽  
Hazard Assessment ◽  
Structural Engineering ◽  
Ground Motions ◽  
Hanging Wall ◽  
Seismic Hazard Assessment ◽  
Foot Wall ◽  
Complete Understanding ◽  
Significant Damage ◽  
Rupture Direction

<p>Ground motions with strong pulses often bring significant damage to structures. The period and the amplitude of the strong-velocity pulses are critical for structural engineering and seismic hazard assessment. The scaling of pulses periods with magnitudes and the within-event variability of pulses is however poorly understood. In this study, we analyze two moderate earthquakes, namely 2016 Meinong earthquake and 2018 Hualien earthquake, using Shahi and Baker’s criteria (2014) to detect pulses. The observations in this study show that the amplitudes of the pulse decay with the distance from the source to the stations, and is also associated with the rupture direction from the asperity instead of the direction from the hypocenter. In addition, we further perform simulations using a simple FK method to clarify the causes of the variability of the pulse periods within and between events. We test the effect of faults dipping angles and the impacts of the asperity location and size. Through our simulations, we reveal that the amplitudes of the pulses in the shallow dipping fault are larger on the hanging wall than on the foot wall, and that the asperity properties has a large impact on the pulses periods and the amplitudes at the nearby stations. The results show that the asperity characteristics are critical for the occurrence of the strong-velocity pulses. The complete understanding of the kinematics of the rupture is then important for clarifying the effects of the strong-velocity pulses and improving ground-motions predictions.</p>

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