Sample records for earthquake fault systems

  1. Quasi-dynamic earthquake fault systems with rheological heterogeneity

    NASA Astrophysics Data System (ADS)

    Brietzke, G. B.; Hainzl, S.; Zoeller, G.; Holschneider, M.

    2009-12-01

    Seismic risk and hazard estimates mostly use pure empirical, stochastic models of earthquake fault systems tuned specifically to the vulnerable areas of interest. Although such models allow for reasonable risk estimates, such models cannot allow for physical statements of the described seismicity. In contrary such empirical stochastic models, physics based earthquake fault systems models allow for a physical reasoning and interpretation of the produced seismicity and system dynamics. Recently different fault system earthquake simulators based on frictional stick-slip behavior have been used to study effects of stress heterogeneity, rheological heterogeneity, or geometrical complexity on earthquake occurrence, spatial and temporal clustering of earthquakes, and system dynamics. Here we present a comparison of characteristics of synthetic earthquake catalogs produced by two different formulations of quasi-dynamic fault system earthquake simulators. Both models are based on discretized frictional faults embedded in an elastic half-space. While one (1) is governed by rate- and state-dependent friction with allowing three evolutionary stages of independent fault patches, the other (2) is governed by instantaneous frictional weakening with scheduled (and therefore causal) stress transfer. We analyze spatial and temporal clustering of events and characteristics of system dynamics by means of physical parameters of the two approaches.

  2. Scaling Relations of Earthquakes on Inland Active Mega-Fault Systems

    NASA Astrophysics Data System (ADS)

    Murotani, S.; Matsushima, S.; Azuma, T.; Irikura, K.; Kitagawa, S.

    2010-12-01

    Since 2005, The Headquarters for Earthquake Research Promotion (HERP) has been publishing 'National Seismic Hazard Maps for Japan' to provide useful information for disaster prevention countermeasures for the country and local public agencies, as well as promote public awareness of disaster prevention of earthquakes. In the course of making the year 2009 version of the map, which is the commemorate of the tenth anniversary of the settlement of the Comprehensive Basic Policy, the methods to evaluate magnitude of earthquakes, to predict strong ground motion, and to construct underground structure were investigated in the Earthquake Research Committee and its subcommittees. In order to predict the magnitude of earthquakes occurring on mega-fault systems, we examined the scaling relations for mega-fault systems using 11 earthquakes of which source processes were analyzed by waveform inversion and of which surface information was investigated. As a result, we found that the data fit in between the scaling relations of seismic moment and rupture area by Somerville et al. (1999) and Irikura and Miyake (2001). We also found that maximum displacement of surface rupture is two to three times larger than the average slip on the seismic fault and surface fault length is equal to length of the source fault. Furthermore, compiled data of the source fault shows that displacement saturates at 10m when fault length(L) is beyond 100km, L>100km. By assuming the fault width (W) to be 18km in average of inland earthquakes in Japan, and the displacement saturate at 10m for length of more than 100 km, we derived a new scaling relation between source area and seismic moment, S[km^2] = 1.0 x 10^-17 M0 [Nm] for mega-fault systems that seismic moment (M0) exceeds 1.8×10^20 Nm.

  3. Synthetic earthquake catalogs simulating seismic activity in the Corinth Gulf, Greece, fault system

    NASA Astrophysics Data System (ADS)

    Console, Rodolfo; Carluccio, Roberto; Papadimitriou, Eleftheria; Karakostas, Vassilis

    2015-01-01

    The characteristic earthquake hypothesis is the basis of time-dependent modeling of earthquake recurrence on major faults. However, the characteristic earthquake hypothesis is not strongly supported by observational data. Few fault segments have long historical or paleoseismic records of individually dated ruptures, and when data and parameter uncertainties are allowed for, the form of the recurrence distribution is difficult to establish. This is the case, for instance, of the Corinth Gulf Fault System (CGFS), for which documents about strong earthquakes exist for at least 2000 years, although they can be considered complete for M ≥ 6.0 only for the latest 300 years, during which only few characteristic earthquakes are reported for individual fault segments. The use of a physics-based earthquake simulator has allowed the production of catalogs lasting 100,000 years and containing more than 500,000 events of magnitudes ≥ 4.0. The main features of our simulation algorithm are (1) an average slip rate released by earthquakes for every single segment in the investigated fault system, (2) heuristic procedures for rupture growth and stop, leading to a self-organized earthquake magnitude distribution, (3) the interaction between earthquake sources, and (4) the effect of minor earthquakes in redistributing stress. The application of our simulation algorithm to the CGFS has shown realistic features in time, space, and magnitude behavior of the seismicity. These features include long-term periodicity of strong earthquakes, short-term clustering of both strong and smaller events, and a realistic earthquake magnitude distribution departing from the Gutenberg-Richter distribution in the higher-magnitude range.

  4. Upper crustal fault reactivation and the potential of triggered earthquakes on the Atacama Fault System, N-Chile

    NASA Astrophysics Data System (ADS)

    Victor, Pia; Ewiak, Oktawian; Thomas, Ziegenhagen; Monika, Sobiesiak; Bernd, Schurr; Gabriel, Gonzalez; Onno, Oncken

    2016-04-01

    The Atacama Fault System (AFS) is an active trench-parallel fault system, located in the forearc of N-Chile directly above the subduction zone interface. Due to its well-exposed position in the hyper arid forearc of N-Chile it is the perfect target to investigate the interaction between the deformation cycle in the overriding forearc and the subduction zone seismic cycle of the underlying megathrust. Although the AFS and large parts of the upper crust are devoid of any noteworthy seismicity, at least three M=7 earthquakes in the past 10 ky have been documented in the paleoseismological record, demonstrating the potential of large events in the future. We apply a two-fold approach to explore fault activation and reactivation patterns through time and to investigate the triggering potential of upper crustal faults. 1) A new methodology using high-resolution topographic data allows us to investigate the number of past earthquakes for any given segment of the fault system as well as the amount of vertical displacement of the last increment. This provides us with a detailed dataset of past earthquake rupture of upper plate faults which is potentially linked to large subduction zone earthquakes. 2) The IPOC Creepmeter array (http://www.ipoc-network.org/index.php/observatory/creepmeter.html) provides us with high-resolution time series of fault displacement accumulation for 11 stations along the 4 most active branches of the AFS. This array monitors the displacement across the fault with 2 samples/min with a resolution of 1μm. Collocated seismometers record the seismicity at two of the creepmeters, whereas the regional seismicity is provided by the IPOC Seismological Networks. Continuous time series of the creepmeter stations since 2009 show that the shallow segments of the fault do not creep permanently. Instead the accumulation of permanent deformation occurs by triggered slip caused by local or remote earthquakes. The 2014 Mw=8.2 Pisagua Earthquake, located close to

  5. Significant earthquakes on the Enriquillo fault system, Hispaniola, 1500-2010: Implications for seismic hazard

    USGS Publications Warehouse

    Bakun, William H.; Flores, Claudia H.; ten Brink, Uri S.

    2012-01-01

    Historical records indicate frequent seismic activity along the north-east Caribbean plate boundary over the past 500 years, particularly on the island of Hispaniola. We use accounts of historical earthquakes to assign intensities and the intensity assignments for the 2010 Haiti earthquakes to derive an intensity attenuation relation for Hispaniola. The intensity assignments and the attenuation relation are used in a grid search to find source locations and magnitudes that best fit the intensity assignments. Here we describe a sequence of devastating earthquakes on the Enriquillo fault system in the eighteenth century. An intensity magnitude MI 6.6 earthquake in 1701 occurred near the location of the 2010 Haiti earthquake, and the accounts of the shaking in the 1701 earthquake are similar to those of the 2010 earthquake. A series of large earthquakes migrating from east to west started with the 18 October 1751 MI 7.4–7.5 earthquake, probably located near the eastern end of the fault in the Dominican Republic, followed by the 21 November 1751 MI 6.6 earthquake near Port-au-Prince, Haiti, and the 3 June 1770 MI 7.5 earthquake west of the 2010 earthquake rupture. The 2010 Haiti earthquake may mark the beginning of a new cycle of large earthquakes on the Enriquillo fault system after 240 years of seismic quiescence. The entire Enriquillo fault system appears to be seismically active; Haiti and the Dominican Republic should prepare for future devastating earthquakes.

  6. Large earthquakes and creeping faults

    USGS Publications Warehouse

    Harris, Ruth A.

    2017-01-01

    Faults are ubiquitous throughout the Earth's crust. The majority are silent for decades to centuries, until they suddenly rupture and produce earthquakes. With a focus on shallow continental active-tectonic regions, this paper reviews a subset of faults that have a different behavior. These unusual faults slowly creep for long periods of time and produce many small earthquakes. The presence of fault creep and the related microseismicity helps illuminate faults that might not otherwise be located in fine detail, but there is also the question of how creeping faults contribute to seismic hazard. It appears that well-recorded creeping fault earthquakes of up to magnitude 6.6 that have occurred in shallow continental regions produce similar fault-surface rupture areas and similar peak ground shaking as their locked fault counterparts of the same earthquake magnitude. The behavior of much larger earthquakes on shallow creeping continental faults is less well known, because there is a dearth of comprehensive observations. Computational simulations provide an opportunity to fill the gaps in our understanding, particularly of the dynamic processes that occur during large earthquake rupture and arrest.

  7. Strong ground motions generated by earthquakes on creeping faults

    USGS Publications Warehouse

    Harris, Ruth A.; Abrahamson, Norman A.

    2014-01-01

    A tenet of earthquake science is that faults are locked in position until they abruptly slip during the sudden strain-relieving events that are earthquakes. Whereas it is expected that locked faults when they finally do slip will produce noticeable ground shaking, what is uncertain is how the ground shakes during earthquakes on creeping faults. Creeping faults are rare throughout much of the Earth's continental crust, but there is a group of them in the San Andreas fault system. Here we evaluate the strongest ground motions from the largest well-recorded earthquakes on creeping faults. We find that the peak ground motions generated by the creeping fault earthquakes are similar to the peak ground motions generated by earthquakes on locked faults. Our findings imply that buildings near creeping faults need to be designed to withstand the same level of shaking as those constructed near locked faults.

  8. Determining on-fault earthquake magnitude distributions from integer programming

    NASA Astrophysics Data System (ADS)

    Geist, Eric L.; Parsons, Tom

    2018-02-01

    Earthquake magnitude distributions among faults within a fault system are determined from regional seismicity and fault slip rates using binary integer programming. A synthetic earthquake catalog (i.e., list of randomly sampled magnitudes) that spans millennia is first formed, assuming that regional seismicity follows a Gutenberg-Richter relation. Each earthquake in the synthetic catalog can occur on any fault and at any location. The objective is to minimize misfits in the target slip rate for each fault, where slip for each earthquake is scaled from its magnitude. The decision vector consists of binary variables indicating which locations are optimal among all possibilities. Uncertainty estimates in fault slip rates provide explicit upper and lower bounding constraints to the problem. An implicit constraint is that an earthquake can only be located on a fault if it is long enough to contain that earthquake. A general mixed-integer programming solver, consisting of a number of different algorithms, is used to determine the optimal decision vector. A case study is presented for the State of California, where a 4 kyr synthetic earthquake catalog is created and faults with slip ≥3 mm/yr are considered, resulting in >106 variables. The optimal magnitude distributions for each of the faults in the system span a rich diversity of shapes, ranging from characteristic to power-law distributions.

  9. Determining on-fault earthquake magnitude distributions from integer programming

    USGS Publications Warehouse

    Geist, Eric L.; Parsons, Thomas E.

    2018-01-01

    Earthquake magnitude distributions among faults within a fault system are determined from regional seismicity and fault slip rates using binary integer programming. A synthetic earthquake catalog (i.e., list of randomly sampled magnitudes) that spans millennia is first formed, assuming that regional seismicity follows a Gutenberg-Richter relation. Each earthquake in the synthetic catalog can occur on any fault and at any location. The objective is to minimize misfits in the target slip rate for each fault, where slip for each earthquake is scaled from its magnitude. The decision vector consists of binary variables indicating which locations are optimal among all possibilities. Uncertainty estimates in fault slip rates provide explicit upper and lower bounding constraints to the problem. An implicit constraint is that an earthquake can only be located on a fault if it is long enough to contain that earthquake. A general mixed-integer programming solver, consisting of a number of different algorithms, is used to determine the optimal decision vector. A case study is presented for the State of California, where a 4 kyr synthetic earthquake catalog is created and faults with slip ≥3 mm/yr are considered, resulting in >106  variables. The optimal magnitude distributions for each of the faults in the system span a rich diversity of shapes, ranging from characteristic to power-law distributions. 

  10. The 2015 M w 6.0 Mt. Kinabalu earthquake: an infrequent fault rupture within the Crocker fault system of East Malaysia

    NASA Astrophysics Data System (ADS)

    Wang, Yu; Wei, Shengji; Wang, Xin; Lindsey, Eric O.; Tongkul, Felix; Tapponnier, Paul; Bradley, Kyle; Chan, Chung-Han; Hill, Emma M.; Sieh, Kerry

    2017-12-01

    The M w 6.0 Mt. Kinabalu earthquake of 2015 was a complete (and deadly) surprise, because it occurred well away from the nearest plate boundary in a region of very low historical seismicity. Our seismological, space geodetic, geomorphological, and field investigations show that the earthquake resulted from rupture of a northwest-dipping normal fault that did not reach the surface. Its unilateral rupture was almost directly beneath 4000-m-high Mt. Kinabalu and triggered widespread slope failures on steep mountainous slopes, which included rockfalls that killed 18 hikers. Our seismological and morphotectonic analyses suggest that the rupture occurred on a normal fault that splays upwards off of the previously identified normal Marakau fault. Our mapping of tectonic landforms reveals that these faults are part of a 200-km-long system of normal faults that traverse the eastern side of the Crocker Range, parallel to Sabah's northwestern coastline. Although the tectonic reason for this active normal fault system remains unclear, the lengths of the longest fault segments suggest that they are capable of generating magnitude 7 earthquakes. Such large earthquakes must occur very rarely, though, given the hitherto undetectable geodetic rates of active tectonic deformation across the region.

  11. Earthquake behavior along the Levant fault from paleoseismology (Invited)

    NASA Astrophysics Data System (ADS)

    Klinger, Y.; Le Beon, M.; Wechsler, N.; Rockwell, T. K.

    2013-12-01

    The Levant fault is a major continental structure 1200 km-long that bounds the Arabian plate to the west. The finite offset of this left-lateral strike-slip fault is estimated to be 105 km for the section located south of the restraining bend corresponding roughly to Lebanon. Along this southern section the slip-rate has been estimated over a large range of time scales, from few years to few hundreds thousands of years. Over these different time scales, studies agree for the slip-rate to be 5mm/yr × 2 mm/yr. The southern section of the Levant fault is particularly attractive to study earthquake behavior through time for several reasons: 1/ The fault geometry is simple and well constrained. 2/ The fault system is isolated and does not interact with obvious neighbor fault systems. 3/ The Middle-East, where the Levant fault is located, is the region in the world where one finds the longest and most complete historical record of past earthquakes. About 30 km north of the city of Aqaba, we opened a trench in the southern part of the Yotvata playa, along the Wadi Araba fault segment. The stratigraphy presents silty sand playa units alternating with coarser sand sediments from alluvial fans flowing westwards from the Jordan plateau. Two fault zones can be recognized in the trench and a minimum of 8 earthquakes can be identified, based on upward terminations of ground ruptures. Dense 14C dating through the entire exposure allows matching the 4 most recent events with historical events in AD1458, AD1212, AD1068 and AD748. Size of the ground rupture suggests a bi-modal distribution of earthquakes with earthquakes rupturing the entire Wadi Araba segment and earthquakes ending in the extensional jog forming the playa. Timing of earthquakes shows that no earthquakes occurred at this site since about 600 years, suggesting earthquake clustering along this section of the fault and potential for a large earthquake in the near future. 3D paleoseismological trenches at the Beteiha

  12. Computing and Visualizing the Complex Dynamics of Earthquake Fault Systems: Towards Ensemble Earthquake Forecasting

    NASA Astrophysics Data System (ADS)

    Rundle, J.; Rundle, P.; Donnellan, A.; Li, P.

    2003-12-01

    We consider the problem of the complex dynamics of earthquake fault systems, and whether numerical simulations can be used to define an ensemble forecasting technology similar to that used in weather and climate research. To effectively carry out such a program, we need 1) a topological realistic model to simulate the fault system; 2) data sets to constrain the model parameters through a systematic program of data assimilation; 3) a computational technology making use of modern paradigms of high performance and parallel computing systems; and 4) software to visualize and analyze the results. In particular, we focus attention of a new version of our code Virtual California (version 2001) in which we model all of the major strike slip faults extending throughout California, from the Mexico-California border to the Mendocino Triple Junction. We use the historic data set of earthquakes larger than magnitude M > 6 to define the frictional properties of all 654 fault segments (degrees of freedom) in the model. Previous versions of Virtual California had used only 215 fault segments to model the strike slip faults in southern California. To compute the dynamics and the associated surface deformation, we use message passing as implemented in the MPICH standard distribution on a small Beowulf cluster consisting of 10 cpus. We are also planning to run the code on significantly larger machines so that we can begin to examine much finer spatial scales of resolution, and to assess scaling properties of the code. We present results of simulations both as static images and as mpeg movies, so that the dynamical aspects of the computation can be assessed by the viewer. We also compute a variety of statistics from the simulations, including magnitude-frequency relations, and compare these with data from real fault systems.

  13. Dynamic rupture scenarios from Sumatra to Iceland - High-resolution earthquake source physics on natural fault systems

    NASA Astrophysics Data System (ADS)

    Gabriel, Alice-Agnes; Madden, Elizabeth H.; Ulrich, Thomas; Wollherr, Stephanie

    2017-04-01

    Capturing the observed complexity of earthquake sources in dynamic rupture simulations may require: non-linear fault friction, thermal and fluid effects, heterogeneous fault stress and fault strength initial conditions, fault curvature and roughness, on- and off-fault non-elastic failure. All of these factors have been independently shown to alter dynamic rupture behavior and thus possibly influence the degree of realism attainable via simulated ground motions. In this presentation we will show examples of high-resolution earthquake scenarios, e.g. based on the 2004 Sumatra-Andaman Earthquake, the 1994 Northridge earthquake and a potential rupture of the Husavik-Flatey fault system in Northern Iceland. The simulations combine a multitude of representations of source complexity at the necessary spatio-temporal resolution enabled by excellent scalability on modern HPC systems. Such simulations allow an analysis of the dominant factors impacting earthquake source physics and ground motions given distinct tectonic settings or distinct focuses of seismic hazard assessment. Across all simulations, we find that fault geometry concurrently with the regional background stress state provide a first order influence on source dynamics and the emanated seismic wave field. The dynamic rupture models are performed with SeisSol, a software package based on an ADER-Discontinuous Galerkin scheme for solving the spontaneous dynamic earthquake rupture problem with high-order accuracy in space and time. Use of unstructured tetrahedral meshes allows for a realistic representation of the non-planar fault geometry, subsurface structure and bathymetry. The results presented highlight the fact that modern numerical methods are essential to further our understanding of earthquake source physics and complement both physic-based ground motion research and empirical approaches in seismic hazard analysis.

  14. Ground Motions Due to Earthquakes on Creeping Faults

    NASA Astrophysics Data System (ADS)

    Harris, R.; Abrahamson, N. A.

    2014-12-01

    We investigate the peak ground motions from the largest well-recorded earthquakes on creeping strike-slip faults in active-tectonic continental regions. Our goal is to evaluate if the strong ground motions from earthquakes on creeping faults are smaller than the strong ground motions from earthquakes on locked faults. Smaller ground motions might be expected from earthquakes on creeping faults if the fault sections that strongly radiate energy are surrounded by patches of fault that predominantly absorb energy. For our study we used the ground motion data available in the PEER NGA-West2 database, and the ground motion prediction equations that were developed from the PEER NGA-West2 dataset. We analyzed data for the eleven largest well-recorded creeping-fault earthquakes, that ranged in magnitude from M5.0-6.5. Our findings are that these earthquakes produced peak ground motions that are statistically indistinguishable from the peak ground motions produced by similar-magnitude earthquakes on locked faults. These findings may be implemented in earthquake hazard estimates for moderate-size earthquakes in creeping-fault regions. Further investigation is necessary to determine if this result will also apply to larger earthquakes on creeping faults. Please also see: Harris, R.A., and N.A. Abrahamson (2014), Strong ground motions generated by earthquakes on creeping faults, Geophysical Research Letters, vol. 41, doi:10.1002/2014GL060228.

  15. Geodetic Finite-Fault-based Earthquake Early Warning Performance for Great Earthquakes Worldwide

    NASA Astrophysics Data System (ADS)

    Ruhl, C. J.; Melgar, D.; Grapenthin, R.; Allen, R. M.

    2017-12-01

    GNSS-based earthquake early warning (EEW) algorithms estimate fault-finiteness and unsaturated moment magnitude for the largest, most damaging earthquakes. Because large events are infrequent, algorithms are not regularly exercised and insufficiently tested on few available datasets. The Geodetic Alarm System (G-larmS) is a GNSS-based finite-fault algorithm developed as part of the ShakeAlert EEW system in the western US. Performance evaluations using synthetic earthquakes offshore Cascadia showed that G-larmS satisfactorily recovers magnitude and fault length, providing useful alerts 30-40 s after origin time and timely warnings of ground motion for onshore urban areas. An end-to-end test of the ShakeAlert system demonstrated the need for GNSS data to accurately estimate ground motions in real-time. We replay real data from several subduction-zone earthquakes worldwide to demonstrate the value of GNSS-based EEW for the largest, most damaging events. We compare predicted ground acceleration (PGA) from first-alert-solutions with those recorded in major urban areas. In addition, where applicable, we compare observed tsunami heights to those predicted from the G-larmS solutions. We show that finite-fault inversion based on GNSS-data is essential to achieving the goals of EEW.

  16. Understanding Earthquake Fault Systems Using QuakeSim Analysis and Data Assimilation Tools

    NASA Technical Reports Server (NTRS)

    Donnellan, Andrea; Parker, Jay; Glasscoe, Margaret; Granat, Robert; Rundle, John; McLeod, Dennis; Al-Ghanmi, Rami; Grant, Lisa

    2008-01-01

    We are using the QuakeSim environment to model interacting fault systems. One goal of QuakeSim is to prepare for the large volumes of data that spaceborne missions such as DESDynI will produce. QuakeSim has the ability to ingest distributed heterogenous data in the form of InSAR, GPS, seismicity, and fault data into various earthquake modeling applications, automating the analysis when possible. Virtual California simulates interacting faults in California. We can compare output from long time history Virtual California runs with the current state of strain and the strain history in California. In addition to spaceborne data we will begin assimilating data from UAVSAR airborne flights over the San Francisco Bay Area, the Transverse Ranges, and the Salton Trough. Results of the models are important for understanding future earthquake risk and for providing decision support following earthquakes. Improved models require this sensor web of different data sources, and a modeling environment for understanding the combined data.

  17. Fault Rupture Model of the 2016 Gyeongju, South Korea, Earthquake and Its Implication for the Underground Fault System

    NASA Astrophysics Data System (ADS)

    Uchide, Takahiko; Song, Seok Goo

    2018-03-01

    The 2016 Gyeongju earthquake (ML 5.8) was the largest instrumentally recorded inland event in South Korea. It occurred in the southeast of the Korean Peninsula and was preceded by a large ML 5.1 foreshock. The aftershock seismicity data indicate that these earthquakes occurred on two closely collocated parallel faults that are oblique to the surface trace of the Yangsan fault. We investigate the rupture properties of these earthquakes using finite-fault slip inversion analyses. The obtained models indicate that the ruptures propagated NNE-ward and SSW-ward for the main shock and the large foreshock, respectively. This indicates that these earthquakes occurred on right-step faults and were initiated around a fault jog. The stress drops were up to 62 and 43 MPa for the main shock and the largest foreshock, respectively. These high stress drops imply high strength excess, which may be overcome by the stress concentration around the fault jog.

  18. Dynamic rupture scenarios from Sumatra to Iceland - High-resolution earthquake source physics on natural fault systems

    NASA Astrophysics Data System (ADS)

    Gabriel, A. A.; Madden, E. H.; Ulrich, T.; Wollherr, S.

    2016-12-01

    Capturing the observed complexity of earthquake sources in dynamic rupture simulations may require: non-linear fault friction, thermal and fluid effects, heterogeneous fault stress and strength initial conditions, fault curvature and roughness, on- and off-fault non-elastic failure. All of these factors have been independently shown to alter dynamic rupture behavior and thus possibly influence the degree of realism attainable via simulated ground motions. In this presentation we will show examples of high-resolution earthquake scenarios, e.g. based on the 2004 Sumatra-Andaman Earthquake and a potential rupture of the Husavik-Flatey fault system in Northern Iceland. The simulations combine a multitude of representations of source complexity at the necessary spatio-temporal resolution enabled by excellent scalability on modern HPC systems. Such simulations allow an analysis of the dominant factors impacting earthquake source physics and ground motions given distinct tectonic settings or distinct focuses of seismic hazard assessment. Across all simulations, we find that fault geometry concurrently with the regional background stress state provide a first order influence on source dynamics and the emanated seismic wave field. The dynamic rupture models are performed with SeisSol, a software package based on an ADER-Discontinuous Galerkin scheme for solving the spontaneous dynamic earthquake rupture problem with high-order accuracy in space and time. Use of unstructured tetrahedral meshes allows for a realistic representation of the non-planar fault geometry, subsurface structure and bathymetry. The results presented highlight the fact that modern numerical methods are essential to further our understanding of earthquake source physics and complement both physic-based ground motion research and empirical approaches in seismic hazard analysis.

  19. Earthquake geology and paleoseismology of major strands of the San Andreas fault system: Chapter 38

    USGS Publications Warehouse

    Rockwell, Thomas; Scharer, Katherine M.; Dawson, Timothy E.

    2016-01-01

    The San Andreas fault system in California is one of the best-studied faults in the world, both in terms of the long-term geologic history and paleoseismic study of past surface ruptures. In this paper, we focus on the Quaternary to historic data that have been collected from the major strands of the San Andreas fault system, both on the San Andreas Fault itself, and the major subparallel strands that comprise the plate boundary, including the Calaveras-Hayward- Rogers Creek-Maacama fault zone and the Concord-Green Valley-Bartlett Springs fault zone in northern California, and the San Jacinto and Elsinore faults in southern California. The majority of the relative motion between the Pacific and North American lithospheric plates is accommodated by these faults, with the San Andreas slipping at about 34 mm/yr in central California, decreasing to about 20 mm/yr in northern California north of its juncture with the Calaveras and Concord faults. The Calaveras-Hayward-Rogers Creek-Maacama fault zone exhibits a slip rate of 10-15 mm/yr, whereas the rate along the Concord-Green Valley-Bartlett Springs fault zone is lower at about 5 mm/yr. In southern California, the San Andreas exhibits a slip rate of about 35 mm/yr along the Mojave section, decreasing to as low as 10-15 mm/yr along its juncture with the San Jacinto fault, and about 20 mm/yr in the Coachella Valley. The San Jacinto and Elsinore fault zones exhibit rates of about 15 and 5 mm/yr, respectively. The average recurrence interval for surface-rupturing earthquakes along individual elements of the San Andreas fault system range from 100-500 years and is consistent with slip rate at those sites: higher slip rates produce more frequent or larger earthquakes. There is also evidence of short-term variations in strain release (slip rate) along various fault sections, as expressed as “flurries” or clusters of earthquakes as well as periods of relatively fewer surface ruptures in these relatively short records. This

  20. The 2017 Jiuzhaigou Earthquake: A Complicated Event Occurred in a Young Fault System

    NASA Astrophysics Data System (ADS)

    Sun, Jianbao; Yue, Han; Shen, Zhengkang; Fang, Lihua; Zhan, Yan; Sun, Xiangyu

    2018-03-01

    The Minshan Uplift Zone (MUZ) is located at the eastern margin of the Tibetan Plateau, which is the junction of three tectonic terranes. The observed discrepancy between a high uplifting and low shortening rate over the MUZ is attributed to the intrusion of a viscous lower crust. In the last 50 years, several significant earthquakes occurred at the boundaries of the MUZ, that is, the Huya and Mingjiang faults. On 8 August 2017, the Jiuzhaigou earthquake (Mw 6.5) occurred on the northern extension of the Huya fault. We adopt a joint inversion of the interferometric synthetic aperture radar and teleseismic body wave data to investigate the rupture process of this event. The obtained slip model is dominated by left-lateral strike slips on a subvertical fault presenting significant shallow slip deficit. The rupture initiation is composed of both thrust and strike-slip mechanisms producing a non-double-couple solution. We also resolve a secondary fault branch forming an obtuse angle with the main fault plane at its northern end. These phenomena indicate that the northern Huya fault is a young (less mature) fault system. Focal mechanisms of the regional earthquakes demonstrate that the northern and southern Huya faults present different combinations of strike-slip and reversed motion. We attribute such discrepancy to the lateral extension of the viscous lower crust, which appears to extrude to the east beyond the northern Huya fault, in comparison with that confined under the MUZ near the southern Huya fault. This conceptual model is also supported by geomorphological and magnetotelluric observations.

  1. UCERF3: A new earthquake forecast for California's complex fault system

    USGS Publications Warehouse

    Field, Edward H.; ,

    2015-01-01

    With innovations, fresh data, and lessons learned from recent earthquakes, scientists have developed a new earthquake forecast model for California, a region under constant threat from potentially damaging events. The new model, referred to as the third Uniform California Earthquake Rupture Forecast, or "UCERF" (http://www.WGCEP.org/UCERF3), provides authoritative estimates of the magnitude, location, and likelihood of earthquake fault rupture throughout the state. Overall the results confirm previous findings, but with some significant changes because of model improvements. For example, compared to the previous forecast (Uniform California Earthquake Rupture Forecast 2), the likelihood of moderate-sized earthquakes (magnitude 6.5 to 7.5) is lower, whereas that of larger events is higher. This is because of the inclusion of multifault ruptures, where earthquakes are no longer confined to separate, individual faults, but can occasionally rupture multiple faults simultaneously. The public-safety implications of this and other model improvements depend on several factors, including site location and type of structure (for example, family dwelling compared to a long-span bridge). Building codes, earthquake insurance products, emergency plans, and other risk-mitigation efforts will be updated accordingly. This model also serves as a reminder that damaging earthquakes are inevitable for California. Fortunately, there are many simple steps residents can take to protect lives and property.

  2. Homogeneity of small-scale earthquake faulting, stress, and fault strength

    USGS Publications Warehouse

    Hardebeck, J.L.

    2006-01-01

    Small-scale faulting at seismogenic depths in the crust appears to be more homogeneous than previously thought. I study three new high-quality focal-mechanism datasets of small (M < ??? 3) earthquakes in southern California, the east San Francisco Bay, and the aftershock sequence of the 1989 Loma Prieta earthquake. I quantify the degree of mechanism variability on a range of length scales by comparing the hypocentral disctance between every pair of events and the angular difference between their focal mechanisms. Closely spaced earthquakes (interhypocentral distance faults of many orientations may or may not be present, only similarly oriented fault planes produce earthquakes contemporaneously. On these short length scales, the crustal stress orientation and fault strength (coefficient of friction) are inferred to be homogeneous as well, to produce such similar earthquakes. Over larger length scales (???2-50 km), focal mechanisms become more diverse with increasing interhypocentral distance (differing on average by 40-70??). Mechanism variability on ???2- to 50 km length scales can be explained by ralatively small variations (???30%) in stress or fault strength. It is possible that most of this small apparent heterogeneity in stress of strength comes from measurement error in the focal mechanisms, as negligibble variation in stress or fault strength (<10%) is needed if each earthquake is assigned the optimally oriented focal mechanism within the 1-sigma confidence region. This local homogeneity in stress orientation and fault strength is encouraging, implying it may be possible to measure these parameters with enough precision to be useful in studying and modeling large earthquakes.

  3. Sedimentary evidence of historical and prehistorical earthquakes along the Venta de Bravo Fault System, Acambay Graben (Central Mexico)

    NASA Astrophysics Data System (ADS)

    Lacan, Pierre; Ortuño, María; Audin, Laurence; Perea, Hector; Baize, Stephane; Aguirre-Díaz, Gerardo; Zúñiga, F. Ramón

    2018-03-01

    The Venta de Bravo normal fault is one of the longest structures in the intra-arc fault system of the Trans-Mexican Volcanic Belt. It defines, together with the Pastores Fault, the 80 km long southern margin of the Acambay Graben. We focus on the westernmost segment of the Venta de Bravo Fault and provide new paleoseismological information, evaluate its earthquake history, and assess the related seismic hazard. We analyzed five trenches, distributed at three different sites, in which Holocene surface faulting offsets interbedded volcanoclastic, fluvio-lacustrine and colluvial deposits. Despite the lack of known historical destructive earthquakes along this fault, we found evidence of at least eight earthquakes during the late Quaternary. Our results indicate that this is one of the major seismic sources of the Acambay Graben, capable of producing by itself earthquakes with magnitudes (MW) up to 6.9, with a slip rate of 0.22-0.24 mm yr- 1 and a recurrence interval between 1940 and 2390 years. In addition, a possible multi-fault rupture of the Venta de Bravo Fault together with other faults of the Acambay Graben could result in a MW > 7 earthquake. These new slip rates, earthquake recurrence rates, and estimation of slips per event help advance our understanding of the seismic hazard posed by the Venta de Bravo Fault and provide new parameters for further hazard assessment.

  4. Effects of Strike-Slip Fault Segmentation on Earthquake Energy and Seismic Hazard

    NASA Astrophysics Data System (ADS)

    Madden, E. H.; Cooke, M. L.; Savage, H. M.; McBeck, J.

    2014-12-01

    Many major strike-slip faults are segmented along strike, including those along plate boundaries in California and Turkey. Failure of distinct fault segments at depth may be the source of multiple pulses of seismic radiation observed for single earthquakes. However, how and when segmentation affects fault behavior and energy release is the basis of many outstanding questions related to the physics of faulting and seismic hazard. These include the probability for a single earthquake to rupture multiple fault segments and the effects of segmentation on earthquake magnitude, radiated seismic energy, and ground motions. Using numerical models, we quantify components of the earthquake energy budget, including the tectonic work acting externally on the system, the energy of internal rock strain, the energy required to overcome fault strength and initiate slip, the energy required to overcome frictional resistance during slip, and the radiated seismic energy. We compare the energy budgets of systems of two en echelon fault segments with various spacing that include both releasing and restraining steps. First, we allow the fault segments to fail simultaneously and capture the effects of segmentation geometry on the earthquake energy budget and on the efficiency with which applied displacement is accommodated. Assuming that higher efficiency correlates with higher probability for a single, larger earthquake, this approach has utility for assessing the seismic hazard of segmented faults. Second, we nucleate slip along a weak portion of one fault segment and let the quasi-static rupture propagate across the system. Allowing fractures to form near faults in these models shows that damage develops within releasing steps and promotes slip along the second fault, while damage develops outside of restraining steps and can prohibit slip along the second fault. Work is consumed in both the propagation of and frictional slip along these new fractures, impacting the energy available

  5. Fault lubrication during earthquakes.

    PubMed

    Di Toro, G; Han, R; Hirose, T; De Paola, N; Nielsen, S; Mizoguchi, K; Ferri, F; Cocco, M; Shimamoto, T

    2011-03-24

    The determination of rock friction at seismic slip rates (about 1 m s(-1)) is of paramount importance in earthquake mechanics, as fault friction controls the stress drop, the mechanical work and the frictional heat generated during slip. Given the difficulty in determining friction by seismological methods, elucidating constraints are derived from experimental studies. Here we review a large set of published and unpublished experiments (∼300) performed in rotary shear apparatus at slip rates of 0.1-2.6 m s(-1). The experiments indicate a significant decrease in friction (of up to one order of magnitude), which we term fault lubrication, both for cohesive (silicate-built, quartz-built and carbonate-built) rocks and non-cohesive rocks (clay-rich, anhydrite, gypsum and dolomite gouges) typical of crustal seismogenic sources. The available mechanical work and the associated temperature rise in the slipping zone trigger a number of physicochemical processes (gelification, decarbonation and dehydration reactions, melting and so on) whose products are responsible for fault lubrication. The similarity between (1) experimental and natural fault products and (2) mechanical work measures resulting from these laboratory experiments and seismological estimates suggests that it is reasonable to extrapolate experimental data to conditions typical of earthquake nucleation depths (7-15 km). It seems that faults are lubricated during earthquakes, irrespective of the fault rock composition and of the specific weakening mechanism involved.

  6. Numerical simulations of earthquakes and the dynamics of fault systems using the Finite Element method.

    NASA Astrophysics Data System (ADS)

    Kettle, L. M.; Mora, P.; Weatherley, D.; Gross, L.; Xing, H.

    2006-12-01

    Simulations using the Finite Element method are widely used in many engineering applications and for the solution of partial differential equations (PDEs). Computational models based on the solution of PDEs play a key role in earth systems simulations. We present numerical modelling of crustal fault systems where the dynamic elastic wave equation is solved using the Finite Element method. This is achieved using a high level computational modelling language, escript, available as open source software from ACcESS (Australian Computational Earth Systems Simulator), the University of Queensland. Escript is an advanced geophysical simulation software package developed at ACcESS which includes parallel equation solvers, data visualisation and data analysis software. The escript library was implemented to develop a flexible Finite Element model which reliably simulates the mechanism of faulting and the physics of earthquakes. Both 2D and 3D elastodynamic models are being developed to study the dynamics of crustal fault systems. Our final goal is to build a flexible model which can be applied to any fault system with user-defined geometry and input parameters. To study the physics of earthquake processes, two different time scales must be modelled, firstly the quasi-static loading phase which gradually increases stress in the system (~100years), and secondly the dynamic rupture process which rapidly redistributes stress in the system (~100secs). We will discuss the solution of the time-dependent elastic wave equation for an arbitrary fault system using escript. This involves prescribing the correct initial stress distribution in the system to simulate the quasi-static loading of faults to failure; determining a suitable frictional constitutive law which accurately reproduces the dynamics of the stick/slip instability at the faults; and using a robust time integration scheme. These dynamic models generate data and information that can be used for earthquake forecasting.

  7. The Active Fault Parameters for Time-Dependent Earthquake Hazard Assessment in Taiwan

    NASA Astrophysics Data System (ADS)

    Lee, Y.; Cheng, C.; Lin, P.; Shao, K.; Wu, Y.; Shih, C.

    2011-12-01

    Taiwan is located at the boundary between the Philippine Sea Plate and the Eurasian Plate, with a convergence rate of ~ 80 mm/yr in a ~N118E direction. The plate motion is so active that earthquake is very frequent. In the Taiwan area, disaster-inducing earthquakes often result from active faults. For this reason, it's an important subject to understand the activity and hazard of active faults. The active faults in Taiwan are mainly located in the Western Foothills and the Eastern longitudinal valley. Active fault distribution map published by the Central Geological Survey (CGS) in 2010 shows that there are 31 active faults in the island of Taiwan and some of which are related to earthquake. Many researchers have investigated these active faults and continuously update new data and results, but few people have integrated them for time-dependent earthquake hazard assessment. In this study, we want to gather previous researches and field work results and then integrate these data as an active fault parameters table for time-dependent earthquake hazard assessment. We are going to gather the seismic profiles or earthquake relocation of a fault and then combine the fault trace on land to establish the 3D fault geometry model in GIS system. We collect the researches of fault source scaling in Taiwan and estimate the maximum magnitude from fault length or fault area. We use the characteristic earthquake model to evaluate the active fault earthquake recurrence interval. In the other parameters, we will collect previous studies or historical references and complete our parameter table of active faults in Taiwan. The WG08 have done the time-dependent earthquake hazard assessment of active faults in California. They established the fault models, deformation models, earthquake rate models, and probability models and then compute the probability of faults in California. Following these steps, we have the preliminary evaluated probability of earthquake-related hazards in certain

  8. Transform fault earthquakes in the North Atlantic: Source mechanisms and depth of faulting

    NASA Technical Reports Server (NTRS)

    Bergman, Eric A.; Solomon, Sean C.

    1987-01-01

    The centroid depths and source mechanisms of 12 large earthquakes on transform faults of the northern Mid-Atlantic Ridge were determined from an inversion of long-period body waveforms. The earthquakes occurred on the Gibbs, Oceanographer, Hayes, Kane, 15 deg 20 min, and Vema transforms. The depth extent of faulting during each earthquake was estimated from the centroid depth and the fault width. The source mechanisms for all events in this study display the strike slip motion expected for transform fault earthquakes; slip vector azimuths agree to 2 to 3 deg of the local strike of the zone of active faulting. The only anomalies in mechanism were for two earthquakes near the western end of the Vema transform which occurred on significantly nonvertical fault planes. Secondary faulting, occurring either precursory to or near the end of the main episode of strike-slip rupture, was observed for 5 of the 12 earthquakes. For three events the secondary faulting was characterized by reverse motion on fault planes striking oblique to the trend of the transform. In all three cases, the site of secondary reverse faulting is near a compression jog in the current trace of the active transform fault zone. No evidence was found to support the conclusions of Engeln, Wiens, and Stein that oceanic transform faults in general are either hotter than expected from current thermal models or weaker than normal oceanic lithosphere.

  9. Retardations in fault creep rates before local moderate earthquakes along the San Andreas fault system, central California

    USGS Publications Warehouse

    Burford, R.O.

    1988-01-01

    Records of shallow aseismic slip (fault creep) obtained along parts of the San Andreas and Calaveras faults in central California demonstrate that significant changes in creep rates often have been associated with local moderate earthquakes. An immediate postearthquake increase followed by gradual, long-term decay back to a previous background rate is generally the most obvious earthquake effect on fault creep. This phenomenon, identified as aseismic afterslip, usually is characterized by above-average creep rates for several months to a few years. In several cases, minor step-like movements, called coseismic slip events, have occurred at or near the times of mainshocks. One extreme case of coseismic slip, recorded at Cienega Winery on the San Andreas fault 17.5 km southeast of San Juan Bautista, consisted of 11 mm of sudden displacement coincident with earthquakes of ML=5.3 and ML=5.2 that occurred 2.5 minutes apart on 9 April 1961. At least one of these shocks originated on the main fault beneath the winery. Creep activity subsequently stopped at the winery for 19 months, then gradually returned to a nearly steady rate slightly below the previous long-term average. The phenomena mentioned above can be explained in terms of simple models consisting of relatively weak material along shallow reaches of the fault responding to changes in load imposed by sudden slip within the underlying seismogenic zone. In addition to coseismic slip and afterslip phenomena, however, pre-earthquake retardations in creep rates also have been observed. Onsets of significant, persistent decreases in creep rates have occurred at several sites 12 months or more before the times of moderate earthquakes. A 44-month retardation before the 1979 ML=5.9 Coyote Lake earthquake on the Calaveras fault was recorded at the Shore Road creepmeter site 10 km northwest of Hollister. Creep retardation on the San Andreas fault near San Juan Bautista has been evident in records from one creepmeter site for

  10. Retardations in fault creep rates before local moderate earthquakes along the San Andreas fault system, central California

    NASA Astrophysics Data System (ADS)

    Burford, Robert O.

    1988-06-01

    Records of shallow aseismic slip (fault creep) obtained along parts of the San Andreas and Calaveras faults in central California demonstrate that significant changes in creep rates often have been associated with local moderate earthquakes. An immediate postearthquake increase followed by gradual, long-term decay back to a previous background rate is generally the most obvious earthquake effect on fault creep. This phenomenon, identified as aseismic afterslip, usually is characterized by above-average creep rates for several months to a few years. In several cases, minor step-like movements, called coseismic slip events, have occurred at or near the times of mainshocks. One extreme case of coseismic slip, recorded at Cienega Winery on the San Andreas fault 17.5 km southeast of San Juan Bautista, consisted of 11 mm of sudden displacement coincident with earthquakes of M L =5.3 and M L =5.2 that occurred 2.5 minutes apart on 9 April 1961. At least one of these shocks originated on the main fault beneath the winery. Creep activity subsequently stopped at the winery for 19 months, then gradually returned to a nearly steady rate slightly below the previous long-term average. The phenomena mentioned above can be explained in terms of simple models consisting of relatively weak material along shallow reaches of the fault responding to changes in load imposed by sudden slip within the underlying seismogenic zone. In addition to coseismic slip and afterslip phenomena, however, pre-earthquake retardations in creep rates also have been observed. Onsets of significant, persistent decreases in creep rates have occurred at several sites 12 months or more before the times of moderate earthquakes. A 44-month retardation before the 1979 M L =5.9 Coyote Lake earthquake on the Calaveras fault was recorded at the Shore Road creepmeter site 10 km northwest of Hollister. Creep retardation on the San Andreas fault near San Juan Bautista has been evident in records from one creepmeter

  11. Geometry and earthquake potential of the shoreline fault, central California

    USGS Publications Warehouse

    Hardebeck, Jeanne L.

    2013-01-01

    The Shoreline fault is a vertical strike‐slip fault running along the coastline near San Luis Obispo, California. Much is unknown about the Shoreline fault, including its slip rate and the details of its geometry. Here, I study the geometry of the Shoreline fault at seismogenic depth, as well as the adjacent section of the offshore Hosgri fault, using seismicity relocations and earthquake focal mechanisms. The Optimal Anisotropic Dynamic Clustering (OADC) algorithm (Ouillon et al., 2008) is used to objectively identify the simplest planar fault geometry that fits all of the earthquakes to within their location uncertainty. The OADC results show that the Shoreline fault is a single continuous structure that connects to the Hosgri fault. Discontinuities smaller than about 1 km may be undetected, but would be too small to be barriers to earthquake rupture. The Hosgri fault dips steeply to the east, while the Shoreline fault is essentially vertical, so the Hosgri fault dips towards and under the Shoreline fault as the two faults approach their intersection. The focal mechanisms generally agree with pure right‐lateral strike‐slip on the OADC planes, but suggest a non‐planar Hosgri fault or another structure underlying the northern Shoreline fault. The Shoreline fault most likely transfers strike‐slip motion between the Hosgri fault and other faults of the Pacific–North America plate boundary system to the east. A hypothetical earthquake rupturing the entire known length of the Shoreline fault would have a moment magnitude of 6.4–6.8. A hypothetical earthquake rupturing the Shoreline fault and the section of the Hosgri fault north of the Hosgri–Shoreline junction would have a moment magnitude of 7.2–7.5.

  12. Earthquake epicenters and fault intersections in central and southern California

    NASA Technical Reports Server (NTRS)

    Abdel-Gawad, M. (Principal Investigator); Silverstein, J.

    1972-01-01

    The author has identifed the following significant results. ERTS-1 imagery provided evidence for the existence of short transverse fault segments lodged between faults of the San Andreas system in the Coast Ranges, California. They indicate that an early episode of transverse shear has affected the Coast Ranges prior to the establishment of the present San Andreas fault. The fault has been offset by transverse faults of the Transverse Ranges. It appears feasible to identify from ERTS-1 imagery geomorphic criteria of recent fault movements. Plots of historic earthquakes in the Coast Ranges and western Transverse Ranges show clusters in areas where structures are complicated by interaction of tow active fault systems. A fault lineament apparently not previously mapped was identified in the Uinta Mountains, Utah. Part of the lineament show evidence of recent faulting which corresponds to a moderate earthquake cluster.

  13. Fault healing promotes high-frequency earthquakes in laboratory experiments and on natural faults

    USGS Publications Warehouse

    McLaskey, Gregory C.; Thomas, Amanda M.; Glaser, Steven D.; Nadeau, Robert M.

    2012-01-01

    Faults strengthen or heal with time in stationary contact and this healing may be an essential ingredient for the generation of earthquakes. In the laboratory, healing is thought to be the result of thermally activated mechanisms that weld together micrometre-sized asperity contacts on the fault surface, but the relationship between laboratory measures of fault healing and the seismically observable properties of earthquakes is at present not well defined. Here we report on laboratory experiments and seismological observations that show how the spectral properties of earthquakes vary as a function of fault healing time. In the laboratory, we find that increased healing causes a disproportionately large amount of high-frequency seismic radiation to be produced during fault rupture. We observe a similar connection between earthquake spectra and recurrence time for repeating earthquake sequences on natural faults. Healing rates depend on pressure, temperature and mineralogy, so the connection between seismicity and healing may help to explain recent observations of large megathrust earthquakes which indicate that energetic, high-frequency seismic radiation originates from locations that are distinct from the geodetically inferred locations of large-amplitude fault slip

  14. Late Holocene earthquakes on the Toe Jam Hill fault, Seattle fault zone, Bainbridge Island, Washington

    USGS Publications Warehouse

    Nelson, A.R.; Johnson, S.Y.; Kelsey, H.M.; Wells, R.E.; Sherrod, B.L.; Pezzopane, S.K.; Bradley, L.A.; Koehler, R. D.; Bucknam, R.C.

    2003-01-01

    Five trenches across a Holocene fault scarp yield the first radiocarbon-measured earthquake recurrence intervals for a crustal fault in western Washington. The scarp, the first to be revealed by laser imagery, marks the Toe Jam Hill fault, a north-dipping backthrust to the Seattle fault. Folded and faulted strata, liquefaction features, and forest soil A horizons buried by hanging-wall-collapse colluvium record three, or possibly four, earthquakes between 2500 and 1000 yr ago. The most recent earthquake is probably the 1050-1020 cal. (calibrated) yr B.P. (A.D. 900-930) earthquake that raised marine terraces and triggered a tsunami in Puget Sound. Vertical deformation estimated from stratigraphic and surface offsets at trench sites suggests late Holocene earthquake magnitudes near M7, corresponding to surface ruptures >36 km long. Deformation features recording poorly understood latest Pleistocene earthquakes suggest that they were smaller than late Holocene earthquakes. Postglacial earthquake recurrence intervals based on 97 radiocarbon ages, most on detrital charcoal, range from ???12,000 yr to as little as a century or less; corresponding fault-slip rates are 0.2 mm/yr for the past 16,000 yr and 2 mm/yr for the past 2500 yr. Because the Toe Jam Hill fault is a backthrust to the Seattle fault, it may not have ruptured during every earthquake on the Seattle fault. But the earthquake history of the Toe Jam Hill fault is at least a partial proxy for the history of the rest of the Seattle fault zone.

  15. Stafford fault system: 120 million year fault movement history of northern Virginia

    USGS Publications Warehouse

    Powars, David S.; Catchings, Rufus D.; Horton, J. Wright; Schindler, J. Stephen; Pavich, Milan J.

    2015-01-01

    The Stafford fault system, located in the mid-Atlantic coastal plain of the eastern United States, provides the most complete record of fault movement during the past ~120 m.y. across the Virginia, Washington, District of Columbia (D.C.), and Maryland region, including displacement of Pleistocene terrace gravels. The Stafford fault system is close to and aligned with the Piedmont Spotsylvania and Long Branch fault zones. The dominant southwest-northeast trend of strong shaking from the 23 August 2011, moment magnitude Mw 5.8 Mineral, Virginia, earthquake is consistent with the connectivity of these faults, as seismic energy appears to have traveled along the documented and proposed extensions of the Stafford fault system into the Washington, D.C., area. Some other faults documented in the nearby coastal plain are clearly rooted in crystalline basement faults, especially along terrane boundaries. These coastal plain faults are commonly assumed to have undergone relatively uniform movement through time, with average slip rates from 0.3 to 1.5 m/m.y. However, there were higher rates during the Paleocene–early Eocene and the Pliocene (4.4–27.4 m/m.y), suggesting that slip occurred primarily during large earthquakes. Further investigation of the Stafford fault system is needed to understand potential earthquake hazards for the Virginia, Maryland, and Washington, D.C., area. The combined Stafford fault system and aligned Piedmont faults are ~180 km long, so if the combined fault system ruptured in a single event, it would result in a significantly larger magnitude earthquake than the Mineral earthquake. Many structures most strongly affected during the Mineral earthquake are along or near the Stafford fault system and its proposed northeastward extension.

  16. The 1868 Hayward fault, California, earthquake: Implications for earthquake scaling relations on partially creeping faults

    USGS Publications Warehouse

    Hough, Susan E.; Martin, Stacey

    2015-01-01

    The 21 October 1868 Hayward, California, earthquake is among the best-characterized historical earthquakes in California. In contrast to many other moderate-to-large historical events, the causative fault is clearly established. Published magnitude estimates have been fairly consistent, ranging from 6.8 to 7.2, with 95% confidence limits including values as low as 6.5. The magnitude is of particular importance for assessment of seismic hazard associated with the Hayward fault and, more generally, to develop appropriate magnitude–rupture length scaling relations for partially creeping faults. The recent reevaluation of archival accounts by Boatwright and Bundock (2008), together with the growing volume of well-calibrated intensity data from the U.S. Geological Survey “Did You Feel It?” (DYFI) system, provide an opportunity to revisit and refine the magnitude estimate. In this study, we estimate the magnitude using two different methods that use DYFI data as calibration. Both approaches yield preferred magnitude estimates of 6.3–6.6, assuming an average stress drop. A consideration of data limitations associated with settlement patterns increases the range to 6.3–6.7, with a preferred estimate of 6.5. Although magnitude estimates for historical earthquakes are inevitably uncertain, we conclude that, at a minimum, a lower-magnitude estimate represents a credible alternative interpretation of available data. We further discuss implications of our results for probabilistic seismic-hazard assessment from partially creeping faults.

  17. Coulomb stress transfer and tectonic loading preceding the 2002 Denali fault earthquake

    USGS Publications Warehouse

    Bufe, Charles G.

    2006-01-01

    Pre-2002 tectonic loading and Coulomb stress transfer are modeled along the rupture zone of the M 7.9 Denali fault earthquake (DFE) and on adjacent segments of the right-lateral Denali–Totschunda fault system in central Alaska, using a three-dimensional boundary-element program. The segments modeled closely follow, for about 95°, the arc of a circle of radius 375 km centered on an inferred asperity near the northeastern end of the intersection of the Patton Bay fault with the Alaskan megathrust under Prince William Sound. The loading model includes slip of 6 mm/yr below 12 km along the fault system, consistent with rotation of the Wrangell block about the asperity at a rate of about 1°/m.y. as well as slip of the Pacific plate at 5 cm/yr at depth along the Fairweather–Queen Charlotte transform fault system and on the Alaska megathrust. The model is consistent with most available pre-2002 Global Positioning System (GPS) displacement rate data. Coulomb stresses induced on the Denali–Totschunda fault system (locked above 12 km) by slip at depth and by transfer from the M 9.2 Prince William Sound earthquake of 1964 dominated the changing Coulomb stress distribution along the fault. The combination of loading (∼70–85%) and coseismic stress transfer from the great 1964 earthquake (∼15–30%) were the principal post-1900 stress factors building toward strike-slip failure of the northern Denali and Totschunda segments in the M 7.9 earthquake of November 2002. Postseismic stresses transferred from the 1964 earthquake may also have been a significant factor. The M 7.2–7.4 Delta River earthquake of 1912 (Carver et al., 2004) may have delayed or advanced the timing of the DFE, depending on the details and location of its rupture. The initial subevent of the 2002 DFE earthquake was on the 40-km Susitna Glacier thrust fault at the western end of the Denali fault rupture. The Coulomb stress transferred from the 1964 earthquake moved the Susitna Glacier thrust

  18. Comparative study of two active faults in different stages of the earthquake cycle in central Japan -The Atera fault (with 1586 Tensho earthquake) and the Nojima fault (with 1995 Kobe earthquake)-

    NASA Astrophysics Data System (ADS)

    Matsuda, T.; Omura, K.; Ikeda, R.

    2003-12-01

    National Research Institute for Earth Science and Disaster Prevention (NIED) has been conducting _gFault zone drilling_h. Fault zone drilling is especially important in understanding the structure, composition, and physical properties of an active fault. In the Chubu district of central Japan, large active faults such as the Atotsugawa (with 1858 Hietsu earthquake) and the Atera (with 1586 Tensho earthquake) faults exist. After the occurrence of the 1995 Kobe earthquake, it has been widely recognized that direct measurements in fault zones by drilling. This time, we describe about the Atera fault and the Nojima fault. Because, these two faults are similar in geological situation (mostly composed of granitic rocks), so it is easy to do comparative study of drilling investigation. The features of the Atera fault, which have been dislocated by the 1586 Tensho earthquake, are as follows. Total length is about 70 km. That general trend is NW45 degree with a left-lateral strike slip. Slip rate is estimated as 3-5 m / 1000 years. Seismicity is very low at present and lithologies around the fault are basically granitic rocks and rhyolite. Six boreholes have been drilled from the depth of 400 m to 630 m. Four of these boreholes (Hatajiri, Fukuoka, Ueno and Kawaue) are located on a line crossing in a direction perpendicular to the Atera fault. In the Kawaue well, mostly fractured and alternating granitic rock continued from the surface to the bottom at 630 m. X-ray fluorescence analysis (XRF) is conducted to estimate the amount of major chemical elements using the glass bead method for core samples. The amounts of H20+ are about from 0.5 to 2.5 weight percent. This fractured zone is also characterized by the logging data such as low resistivity, low P-wave velocity, low density and high neutron porosity. The 1995 Kobe (Hyogo-ken Nanbu) earthquake occurred along the NE-SW-trending Rokko-Awaji fault system, and the Nojima fault appeared on the surface on Awaji Island when this

  19. Apparent stress, fault maturity and seismic hazard for normal-fault earthquakes at subduction zones

    USGS Publications Warehouse

    Choy, G.L.; Kirby, S.H.

    2004-01-01

    The behavior of apparent stress for normal-fault earthquakes at subduction zones is derived by examining the apparent stress (?? a = ??Es/Mo, where E s is radiated energy and Mo is seismic moment) of all globally distributed shallow (depth, ?? 1 MPa) are also generally intraslab, but occur where the lithosphere has just begun subduction beneath the overriding plate. They usually occur in cold slabs near trenches where the direction of plate motion across the trench is oblique to the trench axis, or where there are local contortions or geometrical complexities of the plate boundary. Lower ??a (< 1 MPa) is associated with events occurring at the outer rise (OR) complex (between the OR and the trench axis), as well as with intracrustal events occurring just landward of the trench. The average apparent stress of intraslab-normal-fault earthquakes is considerably higher than the average apparent stress of interplate-thrust-fault earthquakes. In turn, the average ?? a of strike-slip earthquakes in intraoceanic environments is considerably higher than that of intraslab-normal-fault earthquakes. The variation of average ??a with focal mechanism and tectonic regime suggests that the level of ?? a is related to fault maturity. Lower stress drops are needed to rupture mature faults such as those found at plate interfaces that have been smoothed by large cumulative displacements (from hundreds to thousands of kilometres). In contrast, immature faults, such as those on which intraslab-normal-fault earthquakes generally occur, are found in cold and intact lithosphere in which total fault displacement has been much less (from hundreds of metres to a few kilometres). Also, faults on which high ??a oceanic strike-slip earthquakes occur are predominantly intraplate or at evolving ends of transforms. At subduction zones, earthquakes occurring on immature faults are likely to be more hazardous as they tend to generate higher amounts of radiated energy per unit of moment than

  20. Modelling earthquake ruptures with dynamic off-fault damage

    NASA Astrophysics Data System (ADS)

    Okubo, Kurama; Bhat, Harsha S.; Klinger, Yann; Rougier, Esteban

    2017-04-01

    Earthquake rupture modelling has been developed for producing scenario earthquakes. This includes understanding the source mechanisms and estimating far-field ground motion with given a priori constraints like fault geometry, constitutive law of the medium and friction law operating on the fault. It is necessary to consider all of the above complexities of a fault systems to conduct realistic earthquake rupture modelling. In addition to the complexity of the fault geometry in nature, coseismic off-fault damage, which is observed by a variety of geological and seismological methods, plays a considerable role on the resultant ground motion and its spectrum compared to a model with simple planer fault surrounded by purely elastic media. Ideally all of these complexities should be considered in earthquake modelling. State of the art techniques developed so far, however, cannot treat all of them simultaneously due to a variety of computational restrictions. Therefore, we adopt the combined finite-discrete element method (FDEM), which can effectively deal with pre-existing complex fault geometry such as fault branches and kinks and can describe coseismic off-fault damage generated during the dynamic rupture. The advantage of FDEM is that it can handle a wide range of length scales, from metric to kilometric scale, corresponding to the off-fault damage and complex fault geometry respectively. We used the FDEM-based software tool called HOSSedu (Hybrid Optimization Software Suite - Educational Version) for the earthquake rupture modelling, which was developed by Los Alamos National Laboratory. We firstly conducted the cross-validation of this new methodology against other conventional numerical schemes such as the finite difference method (FDM), the spectral element method (SEM) and the boundary integral equation method (BIEM), to evaluate the accuracy with various element sizes and artificial viscous damping values. We demonstrate the capability of the FDEM tool for

  1. HOT Faults", Fault Organization, and the Occurrence of the Largest Earthquakes

    NASA Astrophysics Data System (ADS)

    Carlson, J. M.; Hillers, G.; Archuleta, R. J.

    2006-12-01

    We apply the concept of "Highly Optimized Tolerance" (HOT) for the investigation of spatio-temporal seismicity evolution, in particular mechanisms associated with largest earthquakes. HOT provides a framework for investigating both qualitative and quantitative features of complex feedback systems that are far from equilibrium and punctuated by rare, catastrophic events. In HOT, robustness trade-offs lead to complexity and power laws in systems that are coupled to evolving environments. HOT was originally inspired by biology and engineering, where systems are internally very highly structured, through biological evolution or deliberate design, and perform in an optimum manner despite fluctuations in their surroundings. Though faults and fault systems are not designed in ways comparable to biological and engineered structures, feedback processes are responsible in a conceptually comparable way for the development, evolution and maintenance of younger fault structures and primary slip surfaces of mature faults, respectively. Hence, in geophysical applications the "optimization" approach is perhaps more aptly replaced by "organization", reflecting the distinction between HOT and random, disorganized configurations, and highlighting the importance of structured interdependencies that evolve via feedback among and between different spatial and temporal scales. Expressed in the terminology of the HOT concept, mature faults represent a configuration optimally organized for the release of strain energy; whereas immature, more heterogeneous fault networks represent intermittent, suboptimal systems that are regularized towards structural simplicity and the ability to generate large earthquakes more easily. We discuss fault structure and associated seismic response pattern within the HOT concept, and outline fundamental differences between this novel interpretation to more orthodox viewpoints like the criticality concept. The discussion is flanked by numerical simulations of a

  2. Active Fault Topography and Fault Outcrops in the Central Part of the Nukumi fault, the 1891 Nobi Earthquake Fault System, Central Japan

    NASA Astrophysics Data System (ADS)

    Sasaki, T.; Ueta, K.; Inoue, D.; Aoyagi, Y.; Yanagida, M.; Ichikawa, K.; Goto, N.

    2010-12-01

    It is important to evaluate the magnitude of earthquake caused by multiple active faults, taking into account the simultaneous effects. The simultaneity of adjacent active faults are often decided on the basis of geometric distances except for known these paleoseismic records. We have been studied the step area between the Nukumi fault and the Neodani fault, which appeared as consecutive ruptures in the 1891 Nobi earthquake, since 2009. The purpose of this study is to establish innovation in valuation technique of the simultaneity of adjacent active faults in addition to the paleoseismic record and the geometric distance. Geomorphological, geological and reconnaissance microearthquake surveys are concluded. The present work is intended to clarify the distribution of tectonic geomorphology along the Nukumi fault and the Neodani fault by high-resolution interpretations of airborne LiDAR DEM and aerial photograph, and the field survey of outcrops and location survey. The study area of this work is the southeastern Nukumi fault and the northwestern Neodani fault. We interpret DEM using shaded relief map and stereoscopic bird's-eye view made from 2m mesh DEM data which is obtained by airborne laser scanner of Kokusai Kogyo Co., Ltd. Aerial photographic survey is for confirmation of DEM interpretation using 1/16,000 scale photo. As a result of topographic survey, we found consecutive tectonic topography which is left lateral displacement of ridge and valley lines and reverse scarplets along the Nukumi fault and the Neodani fault . From Ogotani 2km southeastern of Nukumi pass which is located at the southeastern end of surface rupture along the Nukumi fault by previous study to Neooppa 9km southeastern of Nukumi pass, we can interpret left lateral topographies and small uphill-facing fault scarps on the terrace surface by detail DEM investigation. These topographies are unrecognized by aerial photographic survey because of heavy vegetation. We have found several new

  3. Deformation of the 2002 Denali Fault earthquakes, mapped by Radarsat-1 interferometry

    USGS Publications Warehouse

    Lu, Zhong; Wright, Tim; Wicks, Chuck

    2003-01-01

    The magnitude 7.9 earthquake that struck central Alaska on 3 November 2002 was the largest strike-slip earthquake in North America for more than 150 years. The earthquake ruptured about 340 km of the Denali Fault system with observed right-lateral offsets of up to 9 m [Eberhart-Phillips et al., 2003] (Figure l). The rupture initiated with slip on a previously unknown thrust fault, the 40-km-long Susitna Glacier Fault. The rupture propagated eastward for about 220 km along the right-lateral Denali Fault where right-lateral slip averaged ˜5 m, before stepping southeastward onto the Totschunda Fault for about 70 km, with offsets as large as 2 m. The 3 November earthquake was preceded by a magnitude 6.7 shock on 23 October—the Nenana Mountain Earthquake—which was located about 25 km to the west of the 3 November earthquake.

  4. Phase response curves for models of earthquake fault dynamics

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Franović, Igor, E-mail: franovic@ipb.ac.rs; Kostić, Srdjan; Perc, Matjaž

    We systematically study effects of external perturbations on models describing earthquake fault dynamics. The latter are based on the framework of the Burridge-Knopoff spring-block system, including the cases of a simple mono-block fault, as well as the paradigmatic complex faults made up of two identical or distinct blocks. The blocks exhibit relaxation oscillations, which are representative for the stick-slip behavior typical for earthquake dynamics. Our analysis is carried out by determining the phase response curves of first and second order. For a mono-block fault, we consider the impact of a single and two successive pulse perturbations, further demonstrating how themore » profile of phase response curves depends on the fault parameters. For a homogeneous two-block fault, our focus is on the scenario where each of the blocks is influenced by a single pulse, whereas for heterogeneous faults, we analyze how the response of the system depends on whether the stimulus is applied to the block having a shorter or a longer oscillation period.« less

  5. Fault Interaction and Stress Accumulation in Chaman Fault System, Balouchistan, Pakistan, Since 1892

    NASA Astrophysics Data System (ADS)

    Riaz, M. S.; Shan, B.; Xiong, X.; Xie, Z.

    2017-12-01

    The curved-shaped left-lateral Chaman fault is the Western boundary of the Indian plate, which is approximately 1000 km long. The Chaman fault is an active fault and also locus of many catastrophic earthquakes. Since the inception of strike-slip movement at 20-25Ma along the western collision boundary between Indian and Eurasian plates, the average geologically constrained slip rate of 24 to 35 mm/yr accounts for a total displacement of 460±10 km along the Chaman fault system (Beun et al., 1979; Lawrence et al., 1992). Based on earthquake triggering theory, the change in Coulomb Failure Stress (DCFS) either halted (shadow stress) or advances (positive stress) the occurrence of subsequent earthquakes. Several major earthquakes occurred in Chaman fault system, and this region is poorly studied to understand the earthquake/fault interaction and hazard assessment. In order to do so, we have analyzed the earthquakes catalog and collected significant earthquakes with M ≥6.2 since 1892. We then investigate the evolution of DCFS in the Chaman fault system is computed by integration of coseismic static and postseismic viscoelastic relaxation stress transfer since the 1892, using the codePSGRN/PSCMP (Wang et al., 2006). Moreover, for postseismic stress transfer simulation, we adopted linear Maxwell rheology to calculate the viscoelastic effects in this study. Our results elucidate that three out of four earthquakes are triggered by the preceding earthquakes. The 1892-earthquake with magnitude Mw6.8, which occurred on the North segment of Chaman fault has not influence the 1935-earthquake which occurred on Ghazaband fault, a parallel fault 20km east to Chaman fault. The 1935-earthquake with magnitude Mw7.7 significantly loaded the both ends of rupture with positive stress (CFS ≥0.01 Mpa), which later on triggered the 1975-earthquake with 23% of its rupture length where CFS ≥0.01 Mpa, on Chaman fault, and 1990-earthquke with 58% of its rupture length where CFS ≥0

  6. Fault weakening and earthquake instability by powder lubrication

    USGS Publications Warehouse

    Reches, Z.; Lockner, D.A.

    2010-01-01

    Earthquake instability has long been attributed to fault weakening during accelerated slip1, and a central question of earthquake physics is identifying the mechanisms that control this weakening2. Even with much experimental effort2-12, the weakening mechanisms have remained enigmatic. Here we present evidence for dynamic weakening of experimental faults that are sheared at velocities approaching earthquake slip rates. The experimental faults, which were made of room-dry, solid granite blocks, quickly wore to form a fine-grain rock powder known as gouge. At modest slip velocities of 10-60mms-1, this newly formed gouge organized itself into a thin deforming layer that reduced the fault's strength by a factor of 2-3. After slip, the gouge rapidly 'aged' and the fault regained its strength in a matter of hours to days. Therefore, only newly formed gouge can weaken the experimental faults. Dynamic gouge formation is expected to be a common and effective mechanism of earthquake instability in the brittle crust as (1) gouge always forms during fault slip5,10,12-20; (2) fault-gouge behaves similarly to industrial powder lubricants21; (3) dynamic gouge formation explains various significant earthquake properties; and (4) gouge lubricant can form for a wide range of fault configurations, compositions and temperatures15. ?? 2010 Macmillan Publishers Limited. All rights reserved.

  7. Surface and Subsurface Fault Displacements from the September 2010 Darfield (Canterbury) Earthquake

    NASA Astrophysics Data System (ADS)

    Meyers, B.; Furlong, K. P.; Hayes, G. P.; Herman, M. W.; Quigley, M.

    2012-12-01

    On September 3, 2010 a Magnitude 7.1 earthquake struck near Darfield, New Zealand. This was to be the first earthquake in an ongoing, damaging sequence near the city of Christchurch. The earthquake produced a surface rupture with measurable offsets of up to 5.3m along a 30km surface fault system. The spatial pattern of slip during this rupture has been determined by various groups using a range of approaches and several independent data sets. Surface fault rupture was measured in the field and fault slip at depth has been inferred from a seismologic finite fault model (FFM) and various geodetic observations including GPS and InSAR. Here we compare the observed segmented surface displacements with fault slip inferred from the other data. Measurements of the surface rupture show segmented faulting consistent with subsurface slip in the FFM. In the FFM, the main slip patch near the hypocenter can be directly correlated to the region of maximum surface displacement. The FFM and some evidence in the InSAR data also indicate that the Greendale fault system, the structure responsible for the bulk of the rupture, continues at depth closer towards Christchurch than is seen in surface rupture patterns. There is an additional 20km long patch with up to 3m of modeled slip seen in the eastern end of the inverted fault, offset to the south from the Greendale fault trace. This additional fault segment is consistent with a zone of aftershock activity of the main Darfield event, and with local patterns of strong motion. It thus appears that slip recorded at the surface does not describe the entire fault system. This eastward extension of the September rupture means that there is only a short segment of unruptured crust remaining along the entire fault system involved in the Canterbury earthquake sequence.

  8. The Pawnee earthquake as a result of the interplay among injection, faults and foreshocks.

    PubMed

    Chen, Xiaowei; Nakata, Nori; Pennington, Colin; Haffener, Jackson; Chang, Jefferson C; He, Xiaohui; Zhan, Zhongwen; Ni, Sidao; Walter, Jacob I

    2017-07-10

    The Pawnee M5.8 earthquake is the largest event in Oklahoma instrument recorded history. It occurred near the edge of active seismic zones, similar to other M5+ earthquakes since 2011. It ruptured a previously unmapped fault and triggered aftershocks along a complex conjugate fault system. With a high-resolution earthquake catalog, we observe propagating foreshocks leading to the mainshock within 0.5 km distance, suggesting existence of precursory aseismic slip. At approximately 100 days before the mainshock, two M ≥ 3.5 earthquakes occurred along a mapped fault that is conjugate to the mainshock fault. At about 40 days before, two earthquakes clusters started, with one M3 earthquake occurred two days before the mainshock. The three M ≥ 3 foreshocks all produced positive Coulomb stress at the mainshock hypocenter. These foreshock activities within the conjugate fault system are near-instantaneously responding to variations in injection rates at 95% confidence. The short time delay between injection and seismicity differs from both the hypothetical expected time scale of diffusion process and the long time delay observed in this region prior to 2016, suggesting a possible role of elastic stress transfer and critical stress state of the fault. Our results suggest that the Pawnee earthquake is a result of interplay among injection, tectonic faults, and foreshocks.

  9. Unraveling the Earthquake History of the Denali Fault System, Alaska: Filling a Blank Canvas With Paleoearthquakes

    NASA Astrophysics Data System (ADS)

    Schwartz, D. P.; Haeussler, P. J.; Seitz, G. G.; Dawson, T. E.; Stenner, H. D.; Matmon, A.; Crone, A. J.; Personius, S.; Burns, P. B.; Cadena, A.; Thoms, E.

    2005-12-01

    Developing accurate rupture histories of long, high-slip-rate strike-slip faults is is especially challenging where recurrence is relatively short (hundreds of years), adjacent segments may fail within decades of each other, and uncertainties in dating can be as large as, or larger than, the time between events. The Denali Fault system (DFS) is the major active structure of interior Alaska, but received little study since pioneering fault investigations in the early 1970s. Until the summer of 2003 essentially no data existed on the timing or spatial distribution of past ruptures on the DFS. This changed with the occurrence of the M7.9 2002 Denali fault earthquake, which has been a catalyst for present paleoseismic investigations. It provided a well-constrained rupture length and slip distribution. Strike-slip faulting occurred along 290 km of the Denali and Totschunda faults, leaving unruptured ?140km of the eastern Denali fault, ?180 km of the western Denali fault, and ?70 km of the eastern Totschunda fault. The DFS presents us with a blank canvas on which to fill a chronology of past earthquakes using modern paleoseismic techniques. Aware of correlation issues with potentially closely-timed earthquakes we have a) investigated 11 paleoseismic sites that allow a variety of dating techniques, b) measured paleo offsets, which provide insight into magnitude and rupture length of past events, at 18 locations, and c) developed late Pleistocene and Holocene slip rates using exposure age dating to constrain long-term fault behavior models. We are in the process of: 1) radiocarbon-dating peats involved in faulting and liquefaction, and especially short-lived forest floor vegetation that includes outer rings of trees, spruce needles, and blueberry leaves killed and buried during paleoearthquakes; 2) supporting development of a 700-900 year tree-ring time-series for precise dating of trees used in event timing; 3) employing Pb 210 for constraining the youngest ruptures in

  10. Development of the Global Earthquake Model’s neotectonic fault database

    USGS Publications Warehouse

    Christophersen, Annemarie; Litchfield, Nicola; Berryman, Kelvin; Thomas, Richard; Basili, Roberto; Wallace, Laura; Ries, William; Hayes, Gavin P.; Haller, Kathleen M.; Yoshioka, Toshikazu; Koehler, Richard D.; Clark, Dan; Wolfson-Schwehr, Monica; Boettcher, Margaret S.; Villamor, Pilar; Horspool, Nick; Ornthammarath, Teraphan; Zuñiga, Ramon; Langridge, Robert M.; Stirling, Mark W.; Goded, Tatiana; Costa, Carlos; Yeats, Robert

    2015-01-01

    The Global Earthquake Model (GEM) aims to develop uniform, openly available, standards, datasets and tools for worldwide seismic risk assessment through global collaboration, transparent communication and adapting state-of-the-art science. GEM Faulted Earth (GFE) is one of GEM’s global hazard module projects. This paper describes GFE’s development of a modern neotectonic fault database and a unique graphical interface for the compilation of new fault data. A key design principle is that of an electronic field notebook for capturing observations a geologist would make about a fault. The database is designed to accommodate abundant as well as sparse fault observations. It features two layers, one for capturing neotectonic faults and fold observations, and the other to calculate potential earthquake fault sources from the observations. In order to test the flexibility of the database structure and to start a global compilation, five preexisting databases have been uploaded to the first layer and two to the second. In addition, the GFE project has characterised the world’s approximately 55,000 km of subduction interfaces in a globally consistent manner as a basis for generating earthquake event sets for inclusion in earthquake hazard and risk modelling. Following the subduction interface fault schema and including the trace attributes of the GFE database schema, the 2500-km-long frontal thrust fault system of the Himalaya has also been characterised. We propose the database structure to be used widely, so that neotectonic fault data can make a more complete and beneficial contribution to seismic hazard and risk characterisation globally.

  11. Stress before and after the 2002 Denali fault earthquake

    USGS Publications Warehouse

    Wesson, R.L.; Boyd, O.S.

    2007-01-01

    Spatially averaged, absolute deviatoric stress tensors along the faults ruptured during the 2002 Denali fault earthquake, both before and after the event, are derived, using a new method, from estimates of the orientations of the principal stresses and the stress change associated with the earthquake. Stresses are estimated in three regions along the Denali fault, one of which also includes the Susitna Glacier fault, and one region along the Totschunda fault. Estimates of the spatially averaged shear stress before the earthquake resolved onto the faults that ruptured during the event range from near 1 MPa to near 4 MPa. Shear stresses estimated along the faults in all these regions after the event are near zero (0 ?? 1 MPa). These results suggest that deviatoric stresses averaged over a few tens of km along strike are low, and that the stress drop during the earthquake was complete or nearly so.

  12. Lacustrine Paleoseismology Reveals Earthquake Segmentation of the Alpine Fault, New Zealand

    NASA Astrophysics Data System (ADS)

    Howarth, J. D.; Fitzsimons, S.; Norris, R.; Langridge, R. M.

    2013-12-01

    Transform plate boundary faults accommodate high rates of strain and are capable of producing large (Mw>7.0) to great (Mw>8.0) earthquakes that pose significant seismic hazard. The Alpine Fault in New Zealand is one of the longest, straightest and fastest slipping plate boundary transform faults on Earth and produces earthquakes at quasi-periodic intervals. Theoretically, the fault's linearity, isolation from other faults and quasi-periodicity should promote the generation of earthquakes that have similar magnitudes over multiple seismic cycles. We test the hypothesis that the Alpine Fault produces quasi-regular earthquakes that contiguously rupture the southern and central fault segments, using a novel lacustrine paleoseismic proxy to reconstruct spatial and temporal patterns of fault rupture over the last 2000 years. In three lakes located close to the Alpine Fault the last nine earthquakes are recorded as megaturbidites formed by co-seismic subaqueous slope failures, which occur when shaking exceeds Modified Mercalli (MM) VII. When the fault ruptures adjacent to a lake the co-seismic megaturbidites are overlain by stacks of turbidites produced by enhanced fluvial sediment fluxes from earthquake-induced landslides. The turbidite stacks record shaking intensities of MM>IX in the lake catchments and can be used to map the spatial location of fault rupture. The lake records can be dated precisely, facilitating meaningful along strike correlations, and the continuous records allow earthquakes closely spaced in time on adjacent fault segments to be distinguished. The results show that while multi-segment ruptures of the Alpine Fault occurred during most seismic cycles, sequential earthquakes on adjacent segments and single segment ruptures have also occurred. The complexity of the fault rupture pattern suggests that the subtle variations in fault geometry, sense of motion and slip rate that have been used to distinguish the central and southern segments of the Alpine

  13. Methodology for earthquake rupture rate estimates of fault networks: example for the western Corinth rift, Greece

    NASA Astrophysics Data System (ADS)

    Chartier, Thomas; Scotti, Oona; Lyon-Caen, Hélène; Boiselet, Aurélien

    2017-10-01

    Modeling the seismic potential of active faults is a fundamental step of probabilistic seismic hazard assessment (PSHA). An accurate estimation of the rate of earthquakes on the faults is necessary in order to obtain the probability of exceedance of a given ground motion. Most PSHA studies consider faults as independent structures and neglect the possibility of multiple faults or fault segments rupturing simultaneously (fault-to-fault, FtF, ruptures). The Uniform California Earthquake Rupture Forecast version 3 (UCERF-3) model takes into account this possibility by considering a system-level approach rather than an individual-fault-level approach using the geological, seismological and geodetical information to invert the earthquake rates. In many places of the world seismological and geodetical information along fault networks is often not well constrained. There is therefore a need to propose a methodology relying on geological information alone to compute earthquake rates of the faults in the network. In the proposed methodology, a simple distance criteria is used to define FtF ruptures and consider single faults or FtF ruptures as an aleatory uncertainty, similarly to UCERF-3. Rates of earthquakes on faults are then computed following two constraints: the magnitude frequency distribution (MFD) of earthquakes in the fault system as a whole must follow an a priori chosen shape and the rate of earthquakes on each fault is determined by the specific slip rate of each segment depending on the possible FtF ruptures. The modeled earthquake rates are then compared to the available independent data (geodetical, seismological and paleoseismological data) in order to weight different hypothesis explored in a logic tree.The methodology is tested on the western Corinth rift (WCR), Greece, where recent advancements have been made in the understanding of the geological slip rates of the complex network of normal faults which are accommodating the ˜ 15 mm yr-1 north

  14. Normal fault earthquakes or graviquakes

    PubMed Central

    Doglioni, C.; Carminati, E.; Petricca, P.; Riguzzi, F.

    2015-01-01

    Earthquakes are dissipation of energy throughout elastic waves. Canonically is the elastic energy accumulated during the interseismic period. However, in crustal extensional settings, gravity is the main energy source for hangingwall fault collapsing. Gravitational potential is about 100 times larger than the observed magnitude, far more than enough to explain the earthquake. Therefore, normal faults have a different mechanism of energy accumulation and dissipation (graviquakes) with respect to other tectonic settings (strike-slip and contractional), where elastic energy allows motion even against gravity. The bigger the involved volume, the larger is their magnitude. The steeper the normal fault, the larger is the vertical displacement and the larger is the seismic energy released. Normal faults activate preferentially at about 60° but they can be shallower in low friction rocks. In low static friction rocks, the fault may partly creep dissipating gravitational energy without releasing great amount of seismic energy. The maximum volume involved by graviquakes is smaller than the other tectonic settings, being the activated fault at most about three times the hypocentre depth, explaining their higher b-value and the lower magnitude of the largest recorded events. Having different phenomenology, graviquakes show peculiar precursors. PMID:26169163

  15. Synthetic Earthquake Statistics From Physical Fault Models for the Lower Rhine Embayment

    NASA Astrophysics Data System (ADS)

    Brietzke, G. B.; Hainzl, S.; Zöller, G.

    2012-04-01

    As of today, seismic risk and hazard estimates mostly use pure empirical, stochastic models of earthquake fault systems tuned specifically to the vulnerable areas of interest. Although such models allow for reasonable risk estimates they fail to provide a link between the observed seismicity and the underlying physical processes. Solving a state-of-the-art fully dynamic description set of all relevant physical processes related to earthquake fault systems is likely not useful since it comes with a large number of degrees of freedom, poor constraints on its model parameters and a huge computational effort. Here, quasi-static and quasi-dynamic physical fault simulators provide a compromise between physical completeness and computational affordability and aim at providing a link between basic physical concepts and statistics of seismicity. Within the framework of quasi-static and quasi-dynamic earthquake simulators we investigate a model of the Lower Rhine Embayment (LRE) that is based upon seismological and geological data. We present and discuss statistics of the spatio-temporal behavior of generated synthetic earthquake catalogs with respect to simplification (e.g. simple two-fault cases) as well as to complication (e.g. hidden faults, geometric complexity, heterogeneities of constitutive parameters).

  16. Segmentation of the Calaveras-Hayward Fault System Based on 3-D Geometry and Geology at Large-Earthquake Depth

    NASA Astrophysics Data System (ADS)

    Graymer, R. W.; Simpson, R. W.; Jachens, R. C.; Ponce, D. A.; Phelps, G. A.; Watt, J. T.; Wentworth, C. M.

    2007-12-01

    For the purpose of estimating seismic hazard, the Calaveras and Hayward Faults have been considered as separate structures and analyzed and segmented based largely on their surface-trace geometry and the extent of the 1868 Hayward Fault earthquake. Recent relocations of earthquakes and 3-D geologic mapping have shown, however, that at depths associated with large earthquakes (>5 km) the fault geology and geometry is quite different than that at the surface. Using deep fault geometry inferred from these studies we treat the Hayward and Calaveras Faults as a single system and divide the system into segments that differ from the previously accepted segments as follows: 1. The Hayward Fault connects directly to the central Calaveras Fault at depth, as opposed to the 5 km wide restraining stepover zone of multiple imbricate oblique right-lateral reverse faults at the surface east of Fremont and San Jose (between about 37.25°-37.6°N). 2. The segment boundary between the Hayward, central Calaveras, and northern Calaveras is based on their Y- shaped intersection at depth near 37.40°N, 121.76°W (Cherry Flat Reservoir), about 8 km south of the previously accepted central-northern Calaveras Fault segment boundary. 3. The central Calaveras Fault is divided near 37.14°N, 121.56°W (southern end of Anderson Lake) into two subsegments based on a large discontinuity at depth seen in relocated seismicity. 4. The Hayward Fault is divided near 37.85°N, 122.23°W (Lake Temescal) into two segments based on a large contrast in fault face geology. This segmentation is similar to that based on the extent of 1868 fault rupture, but is now related to an underlying geologic cause. The direct connection of the Hayward and central Calaveras Faults at depth suggests that earthquakes larger than those previously modeled should be considered (~M6.9 for the southern Hayward, ~M7.2 for the southern Hayward plus northern central Calaveras). A NEHRP study by Witter and others (2003; NEHRP 03

  17. Dynamics of folding: Impact of fault bend folds on earthquake cycles

    NASA Astrophysics Data System (ADS)

    Sathiakumar, S.; Barbot, S.; Hubbard, J.

    2017-12-01

    Earthquakes in subduction zones and subaerial convergent margins are some of the largest in the world. So far, forecasts of future earthquakes have primarily relied on assessing past earthquakes to look for seismic gaps and slip deficits. However, the roles of fault geometry and off-fault plasticity are typically overlooked. We use structural geology (fault-bend folding theory) to inform fault modeling in order to better understand how deformation is accommodated on the geological time scale and through the earthquake cycle. Fault bends in megathrusts, like those proposed for the Nepal Himalaya, will induce folding of the upper plate. This introduces changes in the slip rate on different fault segments, and therefore on the loading rate at the plate interface, profoundly affecting the pattern of earthquake cycles. We develop numerical simulations of slip evolution under rate-and-state friction and show that this effect introduces segmentation of the earthquake cycle. In crustal dynamics, it is challenging to describe the dynamics of fault-bend folds, because the deformation is accommodated by small amounts of slip parallel to bedding planes ("flexural slip"), localized on axial surface, i.e. folding axes pinned to fault bends. We use dislocation theory to describe the dynamics of folding along these axial surfaces, using analytic solutions that provide displacement and stress kernels to simulate the temporal evolution of folding and assess the effects of folding on earthquake cycles. Studies of the 2015 Gorkha earthquake, Nepal, have shown that fault geometry can affect earthquake segmentation. Here, we show that in addition to the fault geometry, the actual geology of the rocks in the hanging wall of the fault also affect critical parameters, including the loading rate on parts of the fault, based on fault-bend folding theory. Because loading velocity controls the recurrence time of earthquakes, these two effects together are likely to have a strong impact on the

  18. How fault geometry controls earthquake magnitude

    NASA Astrophysics Data System (ADS)

    Bletery, Q.; Thomas, A.; Karlstrom, L.; Rempel, A. W.; Sladen, A.; De Barros, L.

    2016-12-01

    Recent large megathrust earthquakes, such as the Mw9.3 Sumatra-Andaman earthquake in 2004 and the Mw9.0 Tohoku-Oki earthquake in 2011, astonished the scientific community. The first event occurred in a relatively low-convergence-rate subduction zone where events of its size were unexpected. The second event involved 60 m of shallow slip in a region thought to be aseismicaly creeping and hence incapable of hosting very large magnitude earthquakes. These earthquakes highlight gaps in our understanding of mega-earthquake rupture processes and the factors controlling their global distribution. Here we show that gradients in dip angle exert a primary control on mega-earthquake occurrence. We calculate the curvature along the major subduction zones of the world and show that past mega-earthquakes occurred on flat (low-curvature) interfaces. A simplified analytic model demonstrates that shear strength heterogeneity increases with curvature. Stress loading on flat megathrusts is more homogeneous and hence more likely to be released simultaneously over large areas than on highly-curved faults. Therefore, the absence of asperities on large faults might counter-intuitively be a source of higher hazard.

  19. Dynamic 3D simulations of earthquakes on en echelon faults

    USGS Publications Warehouse

    Harris, R.A.; Day, S.M.

    1999-01-01

    One of the mysteries of earthquake mechanics is why earthquakes stop. This process determines the difference between small and devastating ruptures. One possibility is that fault geometry controls earthquake size. We test this hypothesis using a numerical algorithm that simulates spontaneous rupture propagation in a three-dimensional medium and apply our knowledge to two California fault zones. We find that the size difference between the 1934 and 1966 Parkfield, California, earthquakes may be the product of a stepover at the southern end of the 1934 earthquake and show how the 1992 Landers, California, earthquake followed physically reasonable expectations when it jumped across en echelon faults to become a large event. If there are no linking structures, such as transfer faults, then strike-slip earthquakes are unlikely to propagate through stepovers >5 km wide. Copyright 1999 by the American Geophysical Union.

  20. Earthquake rupture process recreated from a natural fault surface

    USGS Publications Warehouse

    Parsons, Thomas E.; Minasian, Diane L.

    2015-01-01

    What exactly happens on the rupture surface as an earthquake nucleates, spreads, and stops? We cannot observe this directly, and models depend on assumptions about physical conditions and geometry at depth. We thus measure a natural fault surface and use its 3D coordinates to construct a replica at 0.1 m resolution to obviate geometry uncertainty. We can recreate stick-slip behavior on the resulting finite element model that depends solely on observed fault geometry. We clamp the fault together and apply steady state tectonic stress until seismic slip initiates and terminates. Our recreated M~1 earthquake initiates at contact points where there are steep surface gradients because infinitesimal lateral displacements reduce clamping stress most efficiently there. Unclamping enables accelerating slip to spread across the surface, but the fault soon jams up because its uneven, anisotropic shape begins to juxtapose new high-relief sticking points. These contacts would ultimately need to be sheared off or strongly deformed before another similar earthquake could occur. Our model shows that an important role is played by fault-wall geometry, though we do not include effects of varying fluid pressure or exotic rheologies on the fault surfaces. We extrapolate our results to large fault systems using observed self-similarity properties, and suggest that larger ruptures might begin and end in a similar way, though the scale of geometrical variation in fault shape that can arrest a rupture necessarily scales with magnitude. In other words, fault segmentation may be a magnitude dependent phenomenon and could vary with each subsequent rupture.

  1. Has El Salvador Fault Zone produced M ≥ 7.0 earthquakes? The 1719 El Salvador earthquake

    NASA Astrophysics Data System (ADS)

    Canora, C.; Martínez-Díaz, J.; Álvarez-Gómez, J.; Villamor, P.; Ínsua-Arévalo, J.; Alonso-Henar, J.; Capote, R.

    2013-05-01

    Historically, large earthquakes, Mw ≥ 7.0, in the Εl Salvador area have been attributed to activity in the Cocos-Caribbean subduction zone. Τhis is correct for most of the earthquakes of magnitude greater than 6.5. However, recent paleoseismic evidence points to the existence of large earthquakes associated with rupture of the Εl Salvador Fault Ζone, an Ε-W oriented strike slip fault system that extends for 150 km through central Εl Salvador. Τo calibrate our results from paleoseismic studies, we have analyzed the historical seismicity of the area. In particular, we suggest that the 1719 earthquake can be associated with paleoseismic activity evidenced in the Εl Salvador Fault Ζone. Α reinterpreted isoseismal map for this event suggests that the damage reported could have been a consequence of the rupture of Εl Salvador Fault Ζone, rather than rupture of the subduction zone. Τhe isoseismal is not different to other upper crustal earthquakes in similar tectonovolcanic environments. We thus challenge the traditional assumption that only the subduction zone is capable of generating earthquakes of magnitude greater than 7.0 in this region. Τhis result has broad implications for future risk management in the region. Τhe potential occurrence of strong ground motion, significantly higher and closer to the Salvadorian populations that those assumed to date, must be considered in seismic hazard assessment studies in this area.

  2. Earthquake hypocenters and focal mechanisms in central Oklahoma reveal a complex system of reactivated subsurface strike-slip faulting

    USGS Publications Warehouse

    McNamara, Daniel E.; Benz, Harley M.; Herrmann, Robert B.; Bergman, Eric A.; Earle, Paul S.; Holland, Austin F.; Baldwin, Randy W.; Gassner, A.

    2015-01-01

    The sharp increase in seismicity over a broad region of central Oklahoma has raised concern regarding the source of the activity and its potential hazard to local communities and energy industry infrastructure. Since early 2010, numerous organizations have deployed temporary portable seismic stations in central Oklahoma in order to record the evolving seismicity. In this study, we apply a multiple-event relocation method to produce a catalog of 3,639 central Oklahoma earthquakes from late 2009 through 2014. RMT source parameters were determined for 195 of the largest and best-recorded earthquakes. Combining RMT results with relocated seismicity enabled us to determine the length, depth and style-of-faulting occurring on reactivated subsurface fault systems. Results show that the majority of earthquakes occur on near vertical, optimally oriented (NE-SW and NW-SE), strike-slip faults in the shallow crystalline basement. These are necessary first order observations required to assess the potential hazards of individual faults in Oklahoma.

  3. Implications of fault constitutive properties for earthquake prediction

    USGS Publications Warehouse

    Dieterich, J.H.; Kilgore, B.

    1996-01-01

    The rate- and state-dependent constitutive formulation for fault slip characterizes an exceptional variety of materials over a wide range of sliding conditions. This formulation provides a unified representation of diverse sliding phenomena including slip weakening over a characteristic sliding distance D(c), apparent fracture energy at a rupture front, time- dependent healing after rapid slip, and various other transient and slip rate effects. Laboratory observations and theoretical models both indicate that earthquake nucleation is accompanied by long intervals of accelerating slip. Strains from the nucleation process on buried faults generally could not be detected if laboratory values of D, apply to faults in nature. However, scaling of D(c) is presently an open question and the possibility exists that measurable premonitory creep may precede some earthquakes. Earthquake activity is modeled as a sequence of earthquake nucleation events. In this model, earthquake clustering arises from sensitivity of nucleation times to the stress changes induced by prior earthquakes. The model gives the characteristic Omori aftershock decay law and assigns physical interpretation to aftershock parameters. The seismicity formulation predicts large changes of earthquake probabilities result from stress changes. Two mechanisms for foreshocks are proposed that describe observed frequency of occurrence of foreshock-mainshock pairs by time and magnitude. With the first mechanism, foreshocks represent a manifestation of earthquake clustering in which the stress change at the time of the foreshock increases the probability of earthquakes at all magnitudes including the eventual mainshock. With the second model, accelerating fault slip on the mainshock nucleation zone triggers foreshocks.

  4. Implications of fault constitutive properties for earthquake prediction.

    PubMed Central

    Dieterich, J H; Kilgore, B

    1996-01-01

    The rate- and state-dependent constitutive formulation for fault slip characterizes an exceptional variety of materials over a wide range of sliding conditions. This formulation provides a unified representation of diverse sliding phenomena including slip weakening over a characteristic sliding distance Dc, apparent fracture energy at a rupture front, time-dependent healing after rapid slip, and various other transient and slip rate effects. Laboratory observations and theoretical models both indicate that earthquake nucleation is accompanied by long intervals of accelerating slip. Strains from the nucleation process on buried faults generally could not be detected if laboratory values of Dc apply to faults in nature. However, scaling of Dc is presently an open question and the possibility exists that measurable premonitory creep may precede some earthquakes. Earthquake activity is modeled as a sequence of earthquake nucleation events. In this model, earthquake clustering arises from sensitivity of nucleation times to the stress changes induced by prior earthquakes. The model gives the characteristic Omori aftershock decay law and assigns physical interpretation to aftershock parameters. The seismicity formulation predicts large changes of earthquake probabilities result from stress changes. Two mechanisms for foreshocks are proposed that describe observed frequency of occurrence of foreshock-mainshock pairs by time and magnitude. With the first mechanism, foreshocks represent a manifestation of earthquake clustering in which the stress change at the time of the foreshock increases the probability of earthquakes at all magnitudes including the eventual mainshock. With the second model, accelerating fault slip on the mainshock nucleation zone triggers foreshocks. Images Fig. 3 PMID:11607666

  5. Implications of fault constitutive properties for earthquake prediction.

    PubMed

    Dieterich, J H; Kilgore, B

    1996-04-30

    The rate- and state-dependent constitutive formulation for fault slip characterizes an exceptional variety of materials over a wide range of sliding conditions. This formulation provides a unified representation of diverse sliding phenomena including slip weakening over a characteristic sliding distance Dc, apparent fracture energy at a rupture front, time-dependent healing after rapid slip, and various other transient and slip rate effects. Laboratory observations and theoretical models both indicate that earthquake nucleation is accompanied by long intervals of accelerating slip. Strains from the nucleation process on buried faults generally could not be detected if laboratory values of Dc apply to faults in nature. However, scaling of Dc is presently an open question and the possibility exists that measurable premonitory creep may precede some earthquakes. Earthquake activity is modeled as a sequence of earthquake nucleation events. In this model, earthquake clustering arises from sensitivity of nucleation times to the stress changes induced by prior earthquakes. The model gives the characteristic Omori aftershock decay law and assigns physical interpretation to aftershock parameters. The seismicity formulation predicts large changes of earthquake probabilities result from stress changes. Two mechanisms for foreshocks are proposed that describe observed frequency of occurrence of foreshock-mainshock pairs by time and magnitude. With the first mechanism, foreshocks represent a manifestation of earthquake clustering in which the stress change at the time of the foreshock increases the probability of earthquakes at all magnitudes including the eventual mainshock. With the second model, accelerating fault slip on the mainshock nucleation zone triggers foreshocks.

  6. Fault Zone Permeability Decrease Following Large Earthquakes in a Hydrothermal System

    NASA Astrophysics Data System (ADS)

    Shi, Zheming; Zhang, Shouchuan; Yan, Rui; Wang, Guangcai

    2018-02-01

    Seismic wave shaking-induced permeability enhancement in the shallow crust has been widely observed. Permeability decrease, however, is seldom reported. In this study, we document coseismic discharge and temperature decrease in a hot spring following the 1996 Lijiang Mw 7.0 and the 2004 Mw 9.0 earthquakes in the Balazhang geothermal field. We use three different models to constrain the permeability change and the mechanism of coseismic discharge decrease, and we use an end-member mixing model for the coseismic temperature change. Our results show that the earthquake-induced permeability decrease in the fault zone reduced the recharge from deep hot water, which may be the mechanism that explains the coseismic discharge and temperature responses. The changes in the hot spring response reflect the dynamic changes in the hydrothermal system; in the future, the earthquake-induced permeability decrease should be considered when discussing controls on permeability.

  7. Earthquake Nucleation and Fault Slip: Possible Experiments on a Natural Fault

    NASA Astrophysics Data System (ADS)

    Germanovich, L. N.; Murdoch, L. C.; Garagash, D.; Reches, Z.; Martel, S. J.; Johnston, M. J.; Ebenhack, J.; Gwaba, D.

    2011-12-01

    High-resolution deformation and seismic observations are usually made only near the Earths' surface, kilometers away from where earthquake nucleate on active faults and are limited by inverse-cube-distance attenuation and ground noise. We have developed an experimental approach that aims at reactivating faults in-situ using thermal techniques and fluid injection, which modify in-situ stresses and the fault strength until the fault slips. Mines where in-situ stresses are sufficient to drive faulting present an opportunity to conduct such experiments. The former Homestake gold mine in South Dakota is a good example. During our recent field work in the Homestake mine, we found a large fault that intersects multiple mine levels. The size and distinct structure of this fault make it a promising target for in-situ reactivation, which would likely to be localized on a crack-like patch. Slow patch propagation, moderated by the injection rate and the rate of change of the background stresses, may become unstable, leading to the nucleation of a dynamic earthquake rupture. Our analyses for the Homestake fault conditions indicate that this transition occurs for a patch size ~1 m. This represents a fundamental limitation for laboratory experiments and necessitates larger-scale field tests ~10-100 m. The opportunity to observe earthquake nucleation on the Homestake Fault is feasible because slip could be initiated at a pre-defined location and time with instrumentation placed as close as a few meters from the nucleation site. Designing the experiment requires a detailed assessment of the state-of-stress in the vicinity of the fault. This is being conducted by simulating changes in pore pressure and effective stresses accompanying dewatering of the mine, and by evaluating in-situ stress measurements in light of a regional stress field modified by local perturbations caused by the mine workings.

  8. Earthquake Clustering on Normal Faults: Insight from Rate-and-State Friction Models

    NASA Astrophysics Data System (ADS)

    Biemiller, J.; Lavier, L. L.; Wallace, L.

    2016-12-01

    Temporal variations in slip rate on normal faults have been recognized in Hawaii and the Basin and Range. The recurrence intervals of these slip transients range from 2 years on the flanks of Kilauea, Hawaii to 10 kyr timescale earthquake clustering on the Wasatch Fault in the eastern Basin and Range. In addition to these longer recurrence transients in the Basin and Range, recent GPS results there also suggest elevated deformation rate events with recurrence intervals of 2-4 years. These observations suggest that some active normal fault systems are dominated by slip behaviors that fall between the end-members of steady aseismic creep and periodic, purely elastic, seismic-cycle deformation. Recent studies propose that 200 year to 50 kyr timescale supercycles may control the magnitude, timing, and frequency of seismic-cycle earthquakes in subduction zones, where aseismic slip transients are known to play an important role in total deformation. Seismic cycle deformation of normal faults may be similarly influenced by its timing within long-period supercycles. We present numerical models (based on rate-and-state friction) of normal faults such as the Wasatch Fault showing that realistic rate-and-state parameter distributions along an extensional fault zone can give rise to earthquake clusters separated by 500 yr - 5 kyr periods of aseismic slip transients on some portions of the fault. The recurrence intervals of events within each earthquake cluster range from 200 to 400 years. Our results support the importance of stress and strain history as controls on a normal fault's present and future slip behavior and on the characteristics of its current seismic cycle. These models suggest that long- to medium-term fault slip history may influence the temporal distribution, recurrence interval, and earthquake magnitudes for a given normal fault segment.

  9. Real-time Estimation of Fault Rupture Extent for Recent Large Earthquakes

    NASA Astrophysics Data System (ADS)

    Yamada, M.; Mori, J. J.

    2009-12-01

    Current earthquake early warning systems assume point source models for the rupture. However, for large earthquakes, the fault rupture length can be of the order of tens to hundreds of kilometers, and the prediction of ground motion at a site requires the approximated knowledge of the rupture geometry. Early warning information based on a point source model may underestimate the ground motion at a site, if a station is close to the fault but distant from the epicenter. We developed an empirical function to classify seismic records into near-source (NS) or far-source (FS) records based on the past strong motion records (Yamada et al., 2007). Here, we defined the near-source region as an area with a fault rupture distance less than 10km. If we have ground motion records at a station, the probability that the station is located in the near-source region is; P = 1/(1+exp(-f)) f = 6.046log10(Za) + 7.885log10(Hv) - 27.091 where Za and Hv denote the peak values of the vertical acceleration and horizontal velocity, respectively. Each observation provides the probability that the station is located in near-source region, so the resolution of the proposed method depends on the station density. The information of the fault rupture location is a group of points where the stations are located. However, for practical purposes, the 2-dimensional configuration of the fault is required to compute the ground motion at a site. In this study, we extend the methodology of NS/FS classification to characterize 2-dimensional fault geometries and apply them to strong motion data observed in recent large earthquakes. We apply a cosine-shaped smoothing function to the probability distribution of near-source stations, and convert the point fault location to 2-dimensional fault information. The estimated rupture geometry for the 2007 Niigata-ken Chuetsu-oki earthquake 10 seconds after the origin time is shown in Figure 1. Furthermore, we illustrate our method with strong motion data of the

  10. Static stress changes associated with normal faulting earthquakes in South Balkan area

    NASA Astrophysics Data System (ADS)

    Papadimitriou, E.; Karakostas, V.; Tranos, M.; Ranguelov, B.; Gospodinov, D.

    2007-10-01

    Activation of major faults in Bulgaria and northern Greece presents significant seismic hazard because of their proximity to populated centers. The long recurrence intervals, of the order of several hundred years as suggested by previous investigations, imply that the twentieth century activation along the southern boundary of the sub-Balkan graben system, is probably associated with stress transfer among neighbouring faults or fault segments. Fault interaction is investigated through elastic stress transfer among strong main shocks ( M ≥ 6.0), and in three cases their foreshocks, which ruptured distinct or adjacent normal fault segments. We compute stress perturbations caused by earthquake dislocations in a homogeneous half-space. The stress change calculations were performed for faults of strike, dip, and rake appropriate to the strong events. We explore the interaction between normal faults in the study area by resolving changes of Coulomb failure function ( ΔCFF) since 1904 and hence the evolution of the stress field in the area during the last 100 years. Coulomb stress changes were calculated assuming that earthquakes can be modeled as static dislocations in an elastic half-space, and taking into account both the coseismic slip in strong earthquakes and the slow tectonic stress buildup associated with major fault segments. We evaluate if these stress changes brought a given strong earthquake closer to, or sent it farther from, failure. Our modeling results show that the generation of each strong event enhanced the Coulomb stress on along-strike neighbors and reduced the stress on parallel normal faults. We extend the stress calculations up to present and provide an assessment for future seismic hazard by identifying possible sites of impending strong earthquakes.

  11. Static stress transfer during the 2002 Nenana Mountain-Denali Fault, Alaska, earthquake sequence

    USGS Publications Warehouse

    Anderson, G.; Ji, C.

    2003-01-01

    On 23 October 2002, the Mw 6.7 Nenana Mountain earthquake occurred in central Alaska. It was followed on 3 November 2002 by the Mw 7.9 Denali Fault mainshock, the largest strike-slip earthquake to occur in North America during the past 150 years. We have modeled static Coulomb stress transfer effects during this sequence. We find that the Nenana Mountain foreshock transferred 30-50 kPa of Coulomb stress to the hypocentral region of the Denali Fault mainshock, encouraging its occurrence. We also find that the two main earthquakes together transferred more than 400 kPa of Coulomb stress to the Cross Creek segment of the Totschunda fault system and to the Denali fault southeast of the mainshock rupture, and up to 80 kPa to the Denali fault west of the Nenana Mountain rupture. Other major faults in the region experienced much smaller static Coulomb stress changes.

  12. Along-strike variations in fault frictional properties along the San Andreas Fault near Cholame, California from joint earthquake and low-frequency earthquake relocations

    USGS Publications Warehouse

    Harrington, Rebecca M.; Cochran, Elizabeth S.; Griffiths, Emily M.; Zeng, Xiangfang; Thurber, Clifford H.

    2016-01-01

    Recent observations of low‐frequency earthquakes (LFEs) and tectonic tremor along the Parkfield–Cholame segment of the San Andreas fault suggest slow‐slip earthquakes occur in a transition zone between the shallow fault, which accommodates slip by a combination of aseismic creep and earthquakes (<15  km depth), and the deep fault, which accommodates slip by stable sliding (>35  km depth). However, the spatial relationship between shallow earthquakes and LFEs remains unclear. Here, we present precise relocations of 34 earthquakes and 34 LFEs recorded during a temporary deployment of 13 broadband seismic stations from May 2010 to July 2011. We use the temporary array waveform data, along with data from permanent seismic stations and a new high‐resolution 3D velocity model, to illuminate the fine‐scale details of the seismicity distribution near Cholame and the relation to the distribution of LFEs. The depth of the boundary between earthquakes and LFE hypocenters changes along strike and roughly follows the 350°C isotherm, suggesting frictional behavior may be, in part, thermally controlled. We observe no overlap in the depth of earthquakes and LFEs, with an ∼5  km separation between the deepest earthquakes and shallowest LFEs. In addition, clustering in the relocated seismicity near the 2004 Mw 6.0 Parkfield earthquake hypocenter and near the northern boundary of the 1857 Mw 7.8 Fort Tejon rupture may highlight areas of frictional heterogeneities on the fault where earthquakes tend to nucleate.

  13. Dynamic Evolution Of Off-Fault Medium During An Earthquake: A Micromechanics Based Model

    NASA Astrophysics Data System (ADS)

    Thomas, Marion Y.; Bhat, Harsha S.

    2018-05-01

    Geophysical observations show a dramatic drop of seismic wave speeds in the shallow off-fault medium following earthquake ruptures. Seismic ruptures generate, or reactivate, damage around faults that alter the constitutive response of the surrounding medium, which in turn modifies the earthquake itself, the seismic radiation, and the near-fault ground motion. We present a micromechanics based constitutive model that accounts for dynamic evolution of elastic moduli at high-strain rates. We consider 2D in-plane models, with a 1D right lateral fault featuring slip-weakening friction law. The two scenarios studied here assume uniform initial off-fault damage and an observationally motivated exponential decay of initial damage with fault normal distance. Both scenarios produce dynamic damage that is consistent with geological observations. A small difference in initial damage actively impacts the final damage pattern. The second numerical experiment, in particular, highlights the complex feedback that exists between the evolving medium and the seismic event. We show that there is a unique off-fault damage pattern associated with supershear transition of an earthquake rupture that could be potentially seen as a geological signature of this transition. These scenarios presented here underline the importance of incorporating the complex structure of fault zone systems in dynamic models of earthquakes.

  14. Dynamic Evolution Of Off-Fault Medium During An Earthquake: A Micromechanics Based Model

    NASA Astrophysics Data System (ADS)

    Thomas, M. Y.; Bhat, H. S.

    2017-12-01

    Geophysical observations show a dramatic drop of seismic wave speeds in the shallow off-fault medium following earthquake ruptures. Seismic ruptures generate, or reactivate, damage around faults that alter the constitutive response of the surrounding medium, which in turn modifies the earthquake itself, the seismic radiation, and the near-fault ground motion. We present a micromechanics based constitutive model that accounts for dynamic evolution of elastic moduli at high-strain rates. We consider 2D in-plane models, with a 1D right lateral fault featuring slip-weakening friction law. The two scenarios studied here assume uniform initial off-fault damage and an observationally motivated exponential decay of initial damage with fault normal distance. Both scenarios produce dynamic damage that is consistent with geological observations. A small difference in initial damage actively impacts the final damage pattern. The second numerical experiment, in particular, highlights the complex feedback that exists between the evolving medium and the seismic event. We show that there is a unique off-fault damage pattern associated with supershear transition of an earthquake rupture that could be potentially seen as a geological signature of this transition. These scenarios presented here underline the importance of incorporating the complex structure of fault zone systems in dynamic models of earthquakes.

  15. Surface fault rupture during the Mw 7.8 Kaikoura earthquake, New Zealand, with specific comment on the Kekerengu Fault - one of the country's fastest slipping onland active faults

    NASA Astrophysics Data System (ADS)

    Van Dissen, Russ; Little, Tim

    2017-04-01

    received surface fault rupture, and are now dextrally offset by about 9 m, while the third trench did not have any 2016 surface rupture pass through it. In this instance, ground-surface rupture along this trace of the fault died out within tens of metres of the trench. Another salient aspect of the Kaikoura earthquake is that the determined (or estimated) recurrence intervals of the faults that ruptured the ground surface vary by an order of magnitude or more. This strongly implies that the ensemble of faults that ruptured with the Kekerengu Fault in the 2016 earthquake has not always been the same for past earthquakes. Possible reasons for this could include the state of stress at the time of a specific earthquake, the direction of rupture propagation, and whether or not rupture on one fault system cascades into rupture on another as is suspected to have happened in the Kaikoura earthquake.

  16. A fault is born: The Landers-Mojave earthquake line

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Nur, A.; Ron, H.

    1993-04-01

    The epicenter and the southern portion of the 1992 Landers earthquake fell on an approximately N-S earthquake line, defined by both epicentral locations and by the rupture directions of four previous M>5 earthquakes in the Mojave: The 1947 Manix; 1975 Galway Lake; 1979 Homestead Valley: and 1992 Joshua Tree events. Another M 5.2 earthquake epicenter in 1965 fell on this line where it intersects the Calico fault. In contrast, the northern part of the Landers rupture followed the NW-SE trending Camp Rock and parallel faults, exhibiting an apparently unusual rupture kink. The block tectonic model (Ron et al., 1984) combiningmore » fault kinematic and mechanics, explains both the alignment of the events, and their ruptures (Nur et al., 1986, 1989), as well as the Landers kink (Nur et al., 1992). Accordingly, the now NW oriented faults have rotated into their present direction away from the direction of maximum shortening, close to becoming locked, whereas a new fault set, optimally oriented relative to the direction of shortening, is developing to accommodate current crustal deformation. The Mojave-Landers line may thus be a new fault in formation. During the transition of faulting from the old, well developed and wak but poorly oriented faults to the strong, but favorably oriented new ones, both can slip simultaneously, giving rise to kinks such as Landers.« less

  17. Ergodicity in natural earthquake fault networks

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Tiampo, K. F.; Rundle, J. B.; Holliday, J.

    2007-06-15

    Numerical simulations have shown that certain driven nonlinear systems can be characterized by mean-field statistical properties often associated with ergodic dynamics [C. D. Ferguson, W. Klein, and J. B. Rundle, Phys. Rev. E 60, 1359 (1999); D. Egolf, Science 287, 101 (2000)]. These driven mean-field threshold systems feature long-range interactions and can be treated as equilibriumlike systems with statistically stationary dynamics over long time intervals. Recently the equilibrium property of ergodicity was identified in an earthquake fault system, a natural driven threshold system, by means of the Thirumalai-Mountain (TM) fluctuation metric developed in the study of diffusive systems [K. F.more » Tiampo, J. B. Rundle, W. Klein, J. S. Sa Martins, and C. D. Ferguson, Phys. Rev. Lett. 91, 238501 (2003)]. We analyze the seismicity of three naturally occurring earthquake fault networks from a variety of tectonic settings in an attempt to investigate the range of applicability of effective ergodicity, using the TM metric and other related statistics. Results suggest that, once variations in the catalog data resulting from technical and network issues are accounted for, all of these natural earthquake systems display stationary periods of metastable equilibrium and effective ergodicity that are disrupted by large events. We conclude that a constant rate of events is an important prerequisite for these periods of punctuated ergodicity and that, while the level of temporal variability in the spatial statistics is the controlling factor in the ergodic behavior of seismic networks, no single statistic is sufficient to ensure quantification of ergodicity. Ergodicity in this application not only requires that the system be stationary for these networks at the applicable spatial and temporal scales, but also implies that they are in a state of metastable equilibrium, one in which the ensemble averages can be substituted for temporal averages in studying their

  18. Rare normal faulting earthquake induced by subduction megaquake: example from 2011 Tohoku-oki earthquake

    NASA Astrophysics Data System (ADS)

    Ishiyama, T.; Sugito, N.; Echigo, T.; Sato, H.; Suzuki, T.

    2012-04-01

    A month after March 11 gigantic M9.0 Tohoku-oki earthquake, M7.0 intraplate earthquake occurred at a depth of 5 km on April 11 beneath coastal area of near Iwaki city, Fukushima prefecture. Focal mechanism of the mainshock indicates that this earthquake is a normal faulting event. Based on field reconnaissance and LIDAR mapping by Geospatial Information Authority of Japan, we recognized coseismic surface ruptures, presumably associated with the main shock. Coseismic surface ruptures extend NNW for about 11 km in a right-stepping en echelon manner. Geomorphic expressions of these ruptures commonly include WWS-facing normal fault scarps and/or drape fold scarp with open cracks on their crests, on the hanging wall sides of steeply west-dipping normal fault planes subparallel to Cretaceous metamorphic rocks. Highest topographic scarp height is about 2.3 m. In this study we introduce preliminary results of a trenching survey across the coseismic surface ruptures at Shionohira site, to resolve timing of paleoseismic events along the Shionohira fault. Trench excavations were carried out at two sites (Ichinokura and Shionohira sites) in Iwaki, Fukushima. At Shionohira site a 2-m-deep trench was excavated across the coseismic fault scarp emerged on the alluvial plain on the eastern flank of the Abukuma Mountains. On the trench walls we observed pairs of steeply dipping normal faults that deform Neogene to Paleogene conglomerates and unconformably overlying, late Quaternary to Holocene fluvial units. Sense of fault slip observed on the trench walls (large dip-slip with small sinistral component) is consistent with that estimated from coseismic surface ruptures. Fault throw estimated from separation of piercing points on lower Unit I and vertical structural relief on folded upper Unit I is consistent with topographic height of the coseismic fault scarp at the trench site. In contrast, vertical separation of Unit II, unconformably overlain by Unit I, is measured as about 1.5 m

  19. How does the 2010 El Mayor - Cucapah Earthquake Rupture Connect to the Southern California Plate Boundary Fault System

    NASA Astrophysics Data System (ADS)

    Donnellan, A.; Ben-Zion, Y.; Arrowsmith, R.

    2016-12-01

    The Pacific - North American plate boundary in southern California is marked by several major strike slip faults. The 2010 M7.2 El Mayor - Cucapah earthquake ruptured 120 km of upper crust in Baja California to the US-Mexico border. The earthquake triggered slip along an extensive network of faults in the Salton Trough from the Mexican border to the southern end of the San Andreas fault. Earthquakes >M5 were triggered in the gap between the Laguna Salada and Elsinore faults at Ocotillo and on the Coyote Creek segment of the San Jacinto fault 20 km northwest of Borrego Springs. UAVSAR observations, collected since October of 2009, measure slip associated with the M5.7 Ocotillo aftershock with deformation continuing into 2014. The Elsinore fault has been remarkably quiet, however, with only M5.0 and M5.2 earthquakes occurring on the Coyote Mountains segment of the fault in 1940 and 1968 respectively. In contrast, the Imperial Valley has been quite active historically with numerous moderate events occurring since 1935. Moderate event activity is increasing along the San Jacinto fault zone (SJFZ), especially the trifurcation area, where 6 of 12 historic earthquakes in this 20 km long fault zone have occurred since 2000. However, no recent deformation has been detected using UAVSAR measurements in this area, including the recent M5.2 June 2016 Borrego earthquake. Does the El Mayor - Cucapah rupture connect to and transfer stress primarily to a single southern California fault or several? What is its role relative to the background plate motion? UAVSAR observations indicate that the southward extension of the Elsinore fault has recently experienced the most localized deformation. Seismicity suggests that the San Jacinto fault is more active than neighboring major faults, and geologic evidence suggests that the Southern San Andreas fault has been the major plate boundary fault in southern California. Topographic data with 3-4 cm resolution using structure from motion from

  20. Stress Interactions Between the 1976 Magnitude 7.8 Tangshan Earthquake and Adjacent Fault Systems in Northern China

    NASA Astrophysics Data System (ADS)

    Zhang, Z.; Lin, J.; Chen, Y. J.

    2004-12-01

    The 28 July 1976 ML = 7.8 Tangshan earthquake struck a highly populated metropolitan center in northern China and was one of the most devastating earthquakes in modern history. Its occurrence has significantly changed the Coulomb stresses on a complex network of strike-slip, normal, and thrust faults in the region, potentially heightened the odds of future earthquakes on some of these fault segments. We have conducted a detailed analysis of the 3D stress effects of the Tangshan earthquake on its neighboring faults, the relationship between stress transfer and aftershock locations, and the implications for future seismic hazard in the region. Available seismic and geodetic data, although limited, indicate that the Tangshan main shock sequence is composed of complex rupture on 2-3 fault segments. The dominant rupture mode is right-lateral strike-slip on two adjoining sub-segments that strike N5¡aE and N35¡aE, respectively. We calculated that the Tangshan main shock sequence has increased the Coulomb failure stress by more than 1 bar in the vicinity of the Lunanxian district to the east, where the largest aftershock (ML = 7.1) occurred 15 hours after the Tangshan main event. The second largest aftershock (ML = 6.8) occurred on the Ninghe fault to the southwest of the main rupture, in a transitional region between the calculated Coulomb stress increase and decrease. The majority of the ML > 5.0 aftershocks also occurred in areas of calculated Coulomb stress increase. Our analyses further indicate that the Coulomb stress on portions of other fault segments, including the Leting and Lulong fault to the east and Yejito fault to the north, may also have been increased. Thus it is critical to obtain estimates of earthquake repeat times on these and other tectonic faults and to acquire continuous GPS and space geodetic measurements. Investigation of stress interaction and earthquake triggering in northern China is not only highly societal relevant but also important for

  1. The effect of segmented fault zones on earthquake rupture propagation and termination

    NASA Astrophysics Data System (ADS)

    Huang, Y.

    2017-12-01

    A fundamental question in earthquake source physics is what can control the nucleation and termination of an earthquake rupture. Besides stress heterogeneities and variations in frictional properties, damaged fault zones (DFZs) that surround major strike-slip faults can contribute significantly to earthquake rupture propagation. Previous earthquake rupture simulations usually characterize DFZs as several-hundred-meter-wide layers with lower seismic velocities than host rocks, and find earthquake ruptures in DFZs can exhibit slip pulses and oscillating rupture speeds that ultimately enhance high-frequency ground motions. However, real DFZs are more complex than the uniform low-velocity structures, and show along-strike variations of damages that may be correlated with historical earthquake ruptures. These segmented structures can either prohibit or assist rupture propagation and significantly affect the final sizes of earthquakes. For example, recent dense array data recorded at the San Jacinto fault zone suggests the existence of three prominent DFZs across the Anza seismic gap and the south section of the Clark branch, while no prominent DFZs were identified near the ends of the Anza seismic gap. To better understand earthquake rupture in segmented fault zones, we will present dynamic rupture simulations that calculate the time-varying rupture process physically by considering the interactions between fault stresses, fault frictional properties, and material heterogeneities. We will show that whether an earthquake rupture can break through the intact rock outside the DFZ depend on the nucleation size of the earthquake and the rupture propagation distance in the DFZ. Moreover, material properties of the DFZ, stress conditions along the fault, and friction properties of the fault also have a critical impact on rupture propagation and termination. We will also present scenarios of San Jacinto earthquake ruptures and show the parameter space that is favorable for

  2. Using Earthquake Analysis to Expand the Oklahoma Fault Database

    NASA Astrophysics Data System (ADS)

    Chang, J. C.; Evans, S. C.; Walter, J. I.

    2017-12-01

    The Oklahoma Geological Survey (OGS) is compiling a comprehensive Oklahoma Fault Database (OFD), which includes faults mapped in OGS publications, university thesis maps, and industry-contributed shapefiles. The OFD includes nearly 20,000 fault segments, but the work is far from complete. The OGS plans on incorporating other sources of data into the OFD, such as new faults from earthquake sequence analyses, geologic field mapping, active-source seismic surveys, and potential fields modeling. A comparison of Oklahoma seismicity and the OFD reveals that earthquakes in the state appear to nucleate on mostly unmapped or unknown faults. Here, we present faults derived from earthquake sequence analyses. From 2015 to present, there has been a five-fold increase in realtime seismic stations in Oklahoma, which has greatly expanded and densified the state's seismic network. The current seismic network not only improves our threshold for locating weaker earthquakes, but also allows us to better constrain focal plane solutions (FPS) from first motion analyses. Using nodal planes from the FPS, HypoDD relocation, and historic seismic data, we can elucidate these previously unmapped seismogenic faults. As the OFD is a primary resource for various scientific investigations, the inclusion of seismogenic faults improves further derivative studies, particularly with respect to seismic hazards. Our primal focus is on four areas of interest, which have had M5+ earthquakes in recent Oklahoma history: Pawnee (M5.8), Prague (M5.7), Fairview (M5.1), and Cushing (M5.0). Subsequent areas of interest will include seismically active data-rich areas, such as the central and northcentral parts of the state.

  3. Aftershocks of the 2014 South Napa, California, Earthquake: Complex faulting on secondary faults

    USGS Publications Warehouse

    Hardebeck, Jeanne L.; Shelly, David R.

    2016-01-01

    We investigate the aftershock sequence of the 2014 MW6.0 South Napa, California, earthquake. Low-magnitude aftershocks missing from the network catalog are detected by applying a matched-filter approach to continuous seismic data, with the catalog earthquakes serving as the waveform templates. We measure precise differential arrival times between events, which we use for double-difference event relocation in a 3D seismic velocity model. Most aftershocks are deeper than the mainshock slip, and most occur west of the mapped surface rupture. While the mainshock coseismic and postseismic slip appears to have occurred on the near-vertical, strike-slip West Napa fault, many of the aftershocks occur in a complex zone of secondary faulting. Earthquake locations in the main aftershock zone, near the mainshock hypocenter, delineate multiple dipping secondary faults. Composite focal mechanisms indicate strike-slip and oblique-reverse faulting on the secondary features. The secondary faults were moved towards failure by Coulomb stress changes from the mainshock slip. Clusters of aftershocks north and south of the main aftershock zone exhibit vertical strike-slip faulting more consistent with the West Napa Fault. The northern aftershocks correspond to the area of largest mainshock coseismic slip, while the main aftershock zone is adjacent to the fault area that has primarily slipped postseismically. Unlike most creeping faults, the zone of postseismic slip does not appear to contain embedded stick-slip patches that would have produced on-fault aftershocks. The lack of stick-slip patches along this portion of the fault may contribute to the low productivity of the South Napa aftershock sequence.

  4. Can diligent and extensive mapping of faults provide reliable estimates of the expected maximum earthquakes at these faults? No. (Invited)

    NASA Astrophysics Data System (ADS)

    Bird, P.

    2010-12-01

    The hope expressed in the title question above can be contradicted in 5 ways, listed below. To summarize, an earthquake rupture can be larger than anticipated either because the fault system has not been fully mapped, or because the rupture is not limited to the pre-existing fault network. 1. Geologic mapping of faults is always incomplete due to four limitations: (a) Map-scale limitation: Faults below a certain (scale-dependent) apparent offset are omitted; (b) Field-time limitation: The most obvious fault(s) get(s) the most attention; (c) Outcrop limitation: You can't map what you can't see; and (d) Lithologic-contrast limitation: Intra-formation faults can be tough to map, so they are often assumed to be minor and omitted. If mapping is incomplete, fault traces may be longer and/or better-connected than we realize. 2. Fault trace “lengths” are unreliable guides to maximum magnitude. Fault networks have multiply-branching, quasi-fractal shapes, so fault “length” may be meaningless. Naming conventions for main strands are unclear, and rarely reviewed. Gaps due to Quaternary alluvial cover may not reflect deeper seismogenic structure. Mapped kinks and other “segment boundary asperities” may be only shallow structures. Also, some recent earthquakes have jumped and linked “separate” faults (Landers, California 1992; Denali, Alaska, 2002) [Wesnousky, 2006; Black, 2008]. 3. Distributed faulting (“eventually occurring everywhere”) is predicted by several simple theories: (a) Viscoelastic stress redistribution in plate/microplate interiors concentrates deviatoric stress upward until they fail by faulting; (b) Unstable triple-junctions (e.g., between 3 strike-slip faults) in 2-D plate theory require new faults to form; and (c) Faults which appear to end (on a geologic map) imply distributed permanent deformation. This means that all fault networks evolve and that even a perfect fault map would be incomplete for future ruptures. 4. A recent attempt

  5. The 2011 Hawthorne, Nevada, Earthquake Sequence; Shallow Normal Faulting

    NASA Astrophysics Data System (ADS)

    Smith, K. D.; Johnson, C.; Davies, J. A.; Agbaje, T.; Knezevic Antonijevic, S.; Kent, G.

    2011-12-01

    An energetic sequence of shallow earthquakes that began in early March 2011 in western Nevada, near the community of Hawthorne, has slowly decreased in intensity through mid-2011. To date about 1300 reviewed earthquake locations have been compiled; we have computed moment tensors for the larger earthquakes and have developed a set of high-precision locations for all reviewed events. The sequence to date has included over 50 earthquakes ML 3 and larger with the largest at Mw 4.6. Three 6-channel portable stations configured with broadband sensors and accelerometers were installed by April 20. Data from the portable instruments is telemetered through NSL's microwave backbone to Reno where it is integrated with regional network data for real-time notifications, ShakeMaps, and routine event analysis. The data is provided in real-time to NEIC, CISN and the IRIS DMC. The sequence is located in a remote area about 15-20 km southwest of Hawthorne in the footwall block of the Wassuk Range fault system. An initial concern was that the sequence might be associated with volcanic processes due to the proximity of late Quaternary volcanic flows; there have been no volcanic signatures observed in near source seismograms. An additional concern, as the sequence has proceeded, was a clear progression eastward toward the Wassuk Range front fault. The east dipping range bounding fault is capable of M 7+ events, and poses a significant hazard to the community of Hawthorne and local military facilities. The Hawthorne Army Depot is an ordinance storage facility and the nation's storage site for surplus mercury. The sequence is within what has been termed the 'Mina Deflection' of the Central Walker Lane Belt. Faulting along the Whiskey Flat section of the Wassuk front fault would be primarily down-to-the-east, with an E-W extension direction; moment tensors for the 2011 earthquake show a range of extension directions from E-W to NW-SE, suggesting a possible dextral component to the Wassuk

  6. The 2013, Mw 7.7 Balochistan earthquake, energetic strike-slip reactivation of a thrust fault

    NASA Astrophysics Data System (ADS)

    Avouac, Jean-Philippe; Ayoub, Francois; Wei, Shengji; Ampuero, Jean-Paul; Meng, Lingsen; Leprince, Sebastien; Jolivet, Romain; Duputel, Zacharie; Helmberger, Don

    2014-04-01

    We analyse the Mw 7.7 Balochistan earthquake of 09/24/2013 based on ground surface deformation measured from sub-pixel correlation of Landsat-8 images, combined with back-projection and finite source modeling of teleseismic waveforms. The earthquake nucleated south of the Chaman strike-slip fault and propagated southwestward along the Hoshab fault at the front of the Kech Band. The rupture was mostly unilateral, propagated at 3 km/s on average and produced a 200 km surface fault trace with purely strike-slip displacement peaking to 10 m and averaging around 6 m. The finite source model shows that slip was maximum near the surface. Although the Hoshab fault is dipping by 45° to the North, in accordance with its origin as a thrust fault within the Makran accretionary prism, slip was nearly purely strike-slip during that earthquake. Large seismic slip on such a non-optimally oriented fault was enhanced possibly due to the influence of the free surface on dynamic stresses or to particular properties of the fault zone allowing for strong dynamic weakening. Strike-slip faulting on thrust fault within the eastern Makran is interpreted as due to eastward extrusion of the accretionary prism as it bulges out over the Indian plate. Portions of the Makran megathrust, some thrust faults in the Kirthar range and strike-slip faults within the Chaman fault system have been brought closer to failure by this earthquake. Aftershocks cluster within the Chaman fault system north of the epicenter, opposite to the direction of rupture propagation. By contrast, few aftershocks were detected in the area of maximum moment release. In this example, aftershocks cannot be used to infer earthquake characteristics.

  7. The Mechanics of Transient Fault Slip and Slow Earthquakes

    NASA Astrophysics Data System (ADS)

    Marone, C.; Leeman, J.; Scuderi, M.; Saffer, D. M.; Collettini, C.

    2015-12-01

    Earthquakes are understood as frictional stick-slip instabilities in which stored elastic energy is released suddenly, driving catastrophic failure. In normal (fast) earthquakes the rupture zone expands at a rate dictated by elastic wave speeds, a few km/s, and fault slip rates reach 1-10 m/s. However, tectonic faults also fail in slow earthquakes with rupture durations of months and fault slip speeds of ~100 micron/s or less. We know very little about the mechanics of slow earthquakes. What determines the rupture propagation velocity in slow earthquakes and in other forms of quasi-dynamic rupture? What processes limit stress drop and fault slip speed in slow earthquakes? Existing lab studies provide some help via observations of complex forms of stick-slip, creep-slip, or, in a few cases, slow slip. However, these are mainly anecdotal and rarely include examples of repetitive slow slip or systematic measurements that could be used to isolate the underlying mechanisms. Numerical studies based on rate and state friction also shed light on transiently accelerating slip, showing that slow slip can occur if: 1) fault rheology involves a change in friction rate dependence (a-b) with velocity or unusually large values of the frictional weakening distance Dc, or 2) fault zone elastic stiffness equals the critical frictional weakening rate kc = (b-a)/Dc. Recent laboratory work shows that the latter can occur much more commonly that previously thought. We document the complete spectrum of stick-slip behaviors from transient slow slip to fast stick-slip for a narrow range of conditions around k/kc = 1.0. Slow slip occurs near the threshold between stable and unstable failure, controlled by the interplay of fault zone frictional properties, normal stress, and elastic stiffness of the surrounding rock. Our results provide a generic mechanism for slow earthquakes, consistent with the wide range of conditions for which slow slip has been observed.

  8. Earthquake geology of the Bulnay Fault (Mongolia)

    USGS Publications Warehouse

    Rizza, Magali; Ritz, Jean-Franciois; Prentice, Carol S.; Vassallo, Ricardo; Braucher, Regis; Larroque, Christophe; Arzhannikova, A.; Arzhanikov, S.; Mahan, Shannon; Massault, M.; Michelot, J-L.; Todbileg, M.

    2015-01-01

    The Bulnay earthquake of July 23, 1905 (Mw 8.3-8.5), in north-central Mongolia, is one of the world's largest recorded intracontinental earthquakes and one of four great earthquakes that occurred in the region during the 20th century. The 375-km-long surface rupture of the left-lateral, strike-slip, N095°E trending Bulnay Fault associated with this earthquake is remarkable for its pronounced expression across the landscape and for the size of features produced by previous earthquakes. Our field observations suggest that in many areas the width and geometry of the rupture zone is the result of repeated earthquakes; however, in those areas where it is possible to determine that the geomorphic features are the result of the 1905 surface rupture alone, the size of the features produced by this single earthquake are singular in comparison to most other historical strike-slip surface ruptures worldwide. Along the 80 km stretch, between 97.18°E and 98.33°E, the fault zone is characterized by several meters width and the mean left-lateral 1905 offset is 8.9 ± 0.6 m with two measured cumulative offsets that are twice the 1905 slip. These observations suggest that the displacement produced during the penultimate event was similar to the 1905 slip. Morphotectonic analyses carried out at three sites along the eastern part of the Bulnay fault, allow us to estimate a mean horizontal slip rate of 3.1 ± 1.7 mm/yr over the Late Pleistocene-Holocene period. In parallel, paleoseismological investigations show evidence for two earthquakes prior to the 1905 event with recurrence intervals of ~2700-4000 years.

  9. Earthquake nucleation on faults with rate-and state-dependent strength

    USGS Publications Warehouse

    Dieterich, J.H.

    1992-01-01

    Dieterich, J.H., 1992. Earthquake nucleation on faults with rate- and state-dependent strength. In: T. Mikumo, K. Aki, M. Ohnaka, L.J. Ruff and P.K.P. Spudich (Editors), Earthquake Source Physics and Earthquake Precursors. Tectonophysics, 211: 115-134. Faults with rate- and state-dependent constitutive properties reproduce a range of observed fault slip phenomena including spontaneous nucleation of slip instabilities at stresses above some critical stress level and recovery of strength following slip instability. Calculations with a plane-strain fault model with spatially varying properties demonstrate that accelerating slip precedes instability and becomes localized to a fault patch. The dimensions of the fault patch follow scaling relations for the minimum critical length for unstable fault slip. The critical length is a function of normal stress, loading conditions and constitutive parameters which include Dc, the characteristic slip distance. If slip starts on a patch that exceeds the critical size, the length of the rapidly accelerating zone tends to shrink to the characteristic size as the time of instability approaches. Solutions have been obtained for a uniform, fixed-patch model that are in good agreement with results from the plane-strain model. Over a wide range of conditions, above the steady-state stress, the logarithm of the time to instability linearly decreases as the initial stress increases. Because nucleation patch length and premonitory displacement are proportional to Dc, the moment of premonitory slip scales by D3c. The scaling of Dc is currently an open question. Unless Dc for earthquake faults is significantly greater than that observed on laboratory faults, premonitory strain arising from the nucleation process for earthquakes may by too small to detect using current observation methods. Excluding the possibility that Dc in the nucleation zone controls the magnitude of the subsequent earthquake, then the source dimensions of the smallest

  10. Source model of an earthquake doublet that occurred in a pull-apart basin along the Sumatran fault, Indonesia

    NASA Astrophysics Data System (ADS)

    Nakano, M.; Kumagai, H.; Toda, S.; Ando, R.; Yamashina, T.; Inoue, H.; Sunarjo

    2010-04-01

    On 2007 March 6, an earthquake doublet occurred along the Sumatran fault, Indonesia. The epicentres were located near Padang Panjang, central Sumatra, Indonesia. The first earthquake, with a moment magnitude (Mw) of 6.4, occurred at 03:49 UTC and was followed two hours later (05:49 UTC) by an earthquake of similar size (Mw = 6.3). We studied the earthquake doublet by a waveform inversion analysis using data from a broadband seismograph network in Indonesia (JISNET). The focal mechanisms of the two earthquakes indicate almost identical right-lateral strike-slip faults, consistent with the geometry of the Sumatran fault. Both earthquakes nucleated below the northern end of Lake Singkarak, which is in a pull-apart basin between the Sumani and Sianok segments of the Sumatran fault system, but the earthquakes ruptured different fault segments. The first earthquake occurred along the southern Sumani segment and its rupture propagated southeastward, whereas the second one ruptured the northern Sianok segment northwestward. Along these fault segments, earthquake doublets, in which the two adjacent fault segments rupture one after the other, have occurred repeatedly. We investigated the state of stress at a segment boundary of a fault system based on the Coulomb stress changes. The stress on faults increases during interseismic periods and is released by faulting. At a segment boundary, on the other hand, the stress increases both interseismically and coseismically, and may not be released unless new fractures are created. Accordingly, ruptures may tend to initiate at a pull-apart basin. When an earthquake occurs on one of the fault segments, the stress increases coseismically around the basin. The stress changes caused by that earthquake may trigger a rupture on the other segment after a short time interval. We also examined the mechanism of the delayed rupture based on a theory of a fluid-saturated poroelastic medium and dynamic rupture simulations incorporating a

  11. Characterizing the recent behavior and earthquake potential of the blind western San Cayetano and Ventura fault systems

    NASA Astrophysics Data System (ADS)

    McAuliffe, L. J.; Dolan, J. F.; Hubbard, J.; Shaw, J. H.

    2011-12-01

    The recent occurrence of several destructive thrust fault earthquakes highlights the risks posed by such events to major urban centers around the world. In order to determine the earthquake potential of such faults in the western Transverse Ranges of southern California, we are studying the activity and paleoearthquake history of the blind Ventura and western San Cayetano faults through a multidisciplinary analysis of strata that have been folded above the fault tiplines. These two thrust faults form the middle section of a >200-km-long, east-west belt of large, interconnected reverse faults that extends across southern California. Although each of these faults represents a major seismic source in its own right, we are exploring the possibility of even larger-magnitude, multi-segment ruptures that may link these faults to other major faults to the east and west in the Transverse Ranges system. The proximity of this large reverse-fault system to several major population centers, including the metropolitan Los Angeles region, and the potential for tsunami generation during offshore ruptures of the western parts of the system, emphasizes the importance of understanding the behavior of these faults for seismic hazard assessment. During the summer of 2010 we used a mini-vibrator source to acquire four, one- to three-km-long, high-resolution seismic reflection profiles. The profiles were collected along the locus of active folding above the blind, western San Cayetano and Ventura faults - specifically, across prominent fold scarps that have developed in response to recent slip on the underlying thrust ramps. These high-resolution data overlap with the uppermost parts of petroleum-industry seismic reflection data, and provide a near-continuous image of recent folding from several km depth to within 50-100 m of the surface. Our initial efforts to document the earthquake history and slip-rate of this large, multi-fault reverse fault system focus on a site above the blind

  12. The 1954 and 1980 Algerian earthquakes: implications for the characteristic-displacement model of fault behavior

    USGS Publications Warehouse

    Dewey, J.W.

    1991-01-01

    Joint epicenter determination of earthquakes that occurred in northern Algeria near Ech Cheliff (named Orleansville in 1954 and El Asnam in 1980) shows that the earthquake of 9 September 1954 (M=6.5) occurred at nearly the same location as the earthquake of 10 October 1980 (M=7.3). The 1954 main shock and earliest aftershocks were concentrated close to the boundaries of segment B (nomenclature of Deschamps et al., 1982; King and Yielding, 1984) of the 1980 fault system, which was to experience approximately 8 m of slip in the 1980 earthquake. Later aftershocks of the 1954 earthquake were spread over a broad area, notably in a region north of the 1980 fault system that also experienced many aftershocks to the 1980 earthquake. The closeness of the 1954 main shock and earliest aftershocks to the 1980 segment B implies that the 1954 earthquake involved either 1) rupture of segment B proper, or 2) rupture of a distinct fault in the hanging wall of footwall block of segment B. -from Author

  13. Detection of postseismic fault-zone collapse following the Landers earthquake

    USGS Publications Warehouse

    Massonnet, D.; Thatcher, W.; Vadon, H.

    1996-01-01

    Stress changes caused by fault movement in an earthquake induce transient aseismic crustal movements in the earthquake source region that continue for months to decades following large events. These motions reflect aseismic adjustments of the fault zone and/or bulk deformation of the surroundings in response to applied stresses, and supply information regarding the inelastic behaviour of the Earth's crust. These processes are imperfectly understood because it is difficult to infer what occurs at depth using only surface measurements, which are in general poorly sampled. Here we push satellite radar interferometry to near its typical artefact level, to obtain a map of the postseismic deformation field in the three years following the 28 June 1992 Landers, California earthquake. From the map, we deduce two distinct types of deformation: afterslip at depth on the fault that ruptured in the earthquake, and shortening normal to the fault zone. The latter movement may reflect the closure of dilatant cracks and fluid expulsion from a transiently over-pressured fault zone.

  14. Earthquake precursory events around epicenters and local active faults; the cases of two inland earthquakes in Iran

    NASA Astrophysics Data System (ADS)

    Valizadeh Alvan, H.; Mansor, S.; Haydari Azad, F.

    2012-12-01

    source and propagation of seismic waves. In many cases, active faults are capable of buildup and sudden release of tectonic stress. Hence, monitoring the active fault systems near epicentral regions of past earthquakes would be a necessity. In this paper, we try to detect possible anomalies in SLHF and AT during two moderate earthquakes of 6 - 6.5 M in Iran and explain the relationships between the seismic activities prior to these earthquake and active faulting in the area. Our analysis shows abnormal SLHF 5~10 days before these earthquakes. Meaningful anomalous concentrations usually occurred in the epicentral area. On the other hand, spatial distributions of these variations were in accordance with the local active faults. It is concluded that the anomalous increase in SLHF shows great potential in providing early warning of a disastrous earthquake, provided that there is a better understanding of the background noise due to the seasonal effects and climatic factors involved. Changes in near surface air temperature along nearby active faults, one or two weeks before the earthquakes, although not as significant as SLHF changes, can be considered as another earthquake indicator.

  15. The 2002 Denali fault earthquake, Alaska: A large magnitude, slip-partitioned event

    USGS Publications Warehouse

    Eberhart-Phillips, D.; Haeussler, Peter J.; Freymueller, J.T.; Frankel, A.D.; Rubin, C.M.; Craw, P.; Ratchkovski, N.A.; Anderson, G.; Carver, G.A.; Crone, A.J.; Dawson, T.E.; Fletcher, H.; Hansen, R.; Harp, E.L.; Harris, R.A.; Hill, D.P.; Hreinsdottir, S.; Jibson, R.W.; Jones, L.M.; Kayen, R.; Keefer, D.K.; Larsen, C.F.; Moran, S.C.; Personius, S.F.; Plafker, G.; Sherrod, B.; Sieh, K.; Sitar, N.; Wallace, W.K.

    2003-01-01

    The MW (moment magnitude) 7.9 Denali fault earthquake on 3 November 2002 was associated with 340 kilometers of surface rupture and was the largest strike-slip earthquake in North America in almost 150 years. It illuminates earthquake mechanics and hazards of large strike-slip faults. It began with thrusting on the previously unrecognized Susitna Glacier fault, continued with right-slip on the Denali fault, then took a right step and continued with right-slip on the Totschunda fault. There is good correlation between geologically observed and geophysically inferred moment release. The earthquake produced unusually strong distal effects in the rupture propagation direction, including triggered seismicity.

  16. Continuous permeability measurements record healing inside the Wenchuan earthquake fault zone.

    PubMed

    Xue, Lian; Li, Hai-Bing; Brodsky, Emily E; Xu, Zhi-Qing; Kano, Yasuyuki; Wang, Huan; Mori, James J; Si, Jia-Liang; Pei, Jun-Ling; Zhang, Wei; Yang, Guang; Sun, Zhi-Ming; Huang, Yao

    2013-06-28

    Permeability controls fluid flow in fault zones and is a proxy for rock damage after an earthquake. We used the tidal response of water level in a deep borehole to track permeability for 18 months in the damage zone of the causative fault of the 2008 moment magnitude 7.9 Wenchuan earthquake. The unusually high measured hydraulic diffusivity of 2.4 × 10(-2) square meters per second implies a major role for water circulation in the fault zone. For most of the observation period, the permeability decreased rapidly as the fault healed. The trend was interrupted by abrupt permeability increases attributable to shaking from remote earthquakes. These direct measurements of the fault zone reveal a process of punctuated recovery as healing and damage interact in the aftermath of a major earthquake.

  17. Width of surface rupture zone for thrust earthquakes: implications for earthquake fault zoning

    NASA Astrophysics Data System (ADS)

    Boncio, Paolo; Liberi, Francesca; Caldarella, Martina; Nurminen, Fiia-Charlotta

    2018-01-01

    The criteria for zoning the surface fault rupture hazard (SFRH) along thrust faults are defined by analysing the characteristics of the areas of coseismic surface faulting in thrust earthquakes. Normal and strike-slip faults have been deeply studied by other authors concerning the SFRH, while thrust faults have not been studied with comparable attention. Surface faulting data were compiled for 11 well-studied historic thrust earthquakes occurred globally (5.4 ≤ M ≤ 7.9). Several different types of coseismic fault scarps characterize the analysed earthquakes, depending on the topography, fault geometry and near-surface materials (simple and hanging wall collapse scarps, pressure ridges, fold scarps and thrust or pressure ridges with bending-moment or flexural-slip fault ruptures due to large-scale folding). For all the earthquakes, the distance of distributed ruptures from the principal fault rupture (r) and the width of the rupture zone (WRZ) were compiled directly from the literature or measured systematically in GIS-georeferenced published maps. Overall, surface ruptures can occur up to large distances from the main fault ( ˜ 2150 m on the footwall and ˜ 3100 m on the hanging wall). Most of the ruptures occur on the hanging wall, preferentially in the vicinity of the principal fault trace ( > ˜ 50 % at distances < ˜ 250 m). The widest WRZ are recorded where sympathetic slip (Sy) on distant faults occurs, and/or where bending-moment (B-M) or flexural-slip (F-S) fault ruptures, associated with large-scale folds (hundreds of metres to kilometres in wavelength), are present. A positive relation between the earthquake magnitude and the total WRZ is evident, while a clear correlation between the vertical displacement on the principal fault and the total WRZ is not found. The distribution of surface ruptures is fitted with probability density functions, in order to define a criterion to remove outliers (e.g. 90 % probability of the cumulative distribution

  18. Fault healing and earthquake spectra from stick slip sequences in the laboratory and on active faults

    NASA Astrophysics Data System (ADS)

    McLaskey, G. C.; Glaser, S. D.; Thomas, A.; Burgmann, R.

    2011-12-01

    Repeating earthquake sequences (RES) are thought to occur on isolated patches of a fault that fail in repeated stick-slip fashion. RES enable researchers to study the effect of variations in earthquake recurrence time and the relationship between fault healing and earthquake generation. Fault healing is thought to be the physical process responsible for the 'state' variable in widely used rate- and state-dependent friction equations. We analyze RES created in laboratory stick slip experiments on a direct shear apparatus instrumented with an array of very high frequency (1KHz - 1MHz) displacement sensors. Tests are conducted on the model material polymethylmethacrylate (PMMA). While frictional properties of this glassy polymer can be characterized with the rate- and state- dependent friction laws, the rate of healing in PMMA is higher than room temperature rock. Our experiments show that in addition to a modest increase in fault strength and stress drop with increasing healing time, there are distinct spectral changes in the recorded laboratory earthquakes. Using the impact of a tiny sphere on the surface of the test specimen as a known source calibration function, we are able to remove the instrument and apparatus response from recorded signals so that the source spectrum of the laboratory earthquakes can be accurately estimated. The rupture of a fault that was allowed to heal produces a laboratory earthquake with increased high frequency content compared to one produced by a fault which has had less time to heal. These laboratory results are supported by observations of RES on the Calaveras and San Andreas faults, which show similar spectral changes when recurrence time is perturbed by a nearby large earthquake. Healing is typically attributed to a creep-like relaxation of the material which causes the true area of contact of interacting asperity populations to increase with time in a quasi-logarithmic way. The increase in high frequency seismicity shown here

  19. Near-fault peak ground velocity from earthquake and laboratory data

    USGS Publications Warehouse

    McGarr, A.; Fletcher, Joe B.

    2007-01-01

    We test the hypothesis that peak ground velocity (PGV) has an upper bound independent of earthquake magnitude and that this bound is controlled primarily by the strength of the seismogenic crust. The highest PGVs, ranging up to several meters per second, have been measured at sites within a few kilometers of the causative faults. Because the database for near-fault PGV is small, we use earthquake slip models, laboratory experiments, and evidence from a mining-induced earthquake to investigate the factors influencing near-fault PGV and the nature of its scaling. For each earthquake slip model we have calculated the peak slip rates for all subfaults and then chosen the maximum of these rates as an estimate of twice the largest near-fault PGV. Nine slip models for eight earthquakes, with magnitudes ranging from 6.5 to 7.6, yielded maximum peak slip rates ranging from 2.3 to 12 m/sec with a median of 5.9 m/sec. By making several adjustments, PGVs for small earthquakes can be simulated from peak slip rates measured during laboratory stick-slip experiments. First, we adjust the PGV for differences in the state of stress (i.e., the difference between the laboratory loading stresses and those appropriate for faults at seismogenic depths). To do this, we multiply both the slip and the peak slip rate by the ratio of the effective normal stresses acting on fault planes measured at 6.8 km depth at the KTB site, Germany (deepest available in situ stress measurements), to those acting on the laboratory faults. We also adjust the seismic moment by replacing the laboratory fault with a buried circular shear crack whose radius is chosen to match the experimental unloading stiffness. An additional, less important adjustment is needed for experiments run in triaxial loading conditions. With these adjustments, peak slip rates for 10 stick-slip events, with scaled moment magnitudes from -2.9 to 1.0, range from 3.3 to 10.3 m/sec, with a median of 5.4 m/sec. Both the earthquake and

  20. Fault Structural Control on Earthquake Strong Ground Motions: The 2008 Wenchuan Earthquake as an Example

    NASA Astrophysics Data System (ADS)

    Zhang, Yan; Zhang, Dongli; Li, Xiaojun; Huang, Bei; Zheng, Wenjun; Wang, Yuejun

    2018-02-01

    Continental thrust faulting earthquakes pose severe threats to megacities across the world. Recent events show the possible control of fault structures on strong ground motions. The seismogenic structure of the 2008 Wenchuan earthquake is associated with high-angle listric reverse fault zones. Its peak ground accelerations (PGAs) show a prominent feature of fault zone amplification: the values within the 30- to 40-km-wide fault zone block are significantly larger than those on both the hanging wall and the footwall. The PGA values attenuate asymmetrically: they decay much more rapidly in the footwall than in the hanging wall. The hanging wall effects can be seen on both the vertical and horizontal components of the PGAs, with the former significantly more prominent than the latter. All these characteristics can be adequately interpreted by upward extrusion of the high-angle listric reverse fault zone block. Through comparison with a low-angle planar thrust fault associated with the 1999 Chi-Chi earthquake, we conclude that different fault structures might have controlled different patterns of strong ground motion, which should be taken into account in seismic design and construction.

  1. Earthquakes and faults in southern California (1970-2010)

    USGS Publications Warehouse

    Sleeter, Benjamin M.; Calzia, James P.; Walter, Stephen R.

    2012-01-01

    The map depicts both active and inactive faults and earthquakes magnitude 1.5 to 7.3 in southern California (1970–2010). The bathymetry was generated from digital files from the California Department of Fish And Game, Marine Region, Coastal Bathymetry Project. Elevation data are from the U.S. Geological Survey National Elevation Database. Landsat satellite image is from fourteen Landsat 5 Thematic Mapper scenes collected between 2009 and 2010. Fault data are reproduced with permission from 2006 California Geological Survey and U.S. Geological Survey data. The earthquake data are from the U.S. Geological Survey National Earthquake Information Center.

  2. New insights into seismic faulting during the 2008 Mw7.9 Wenchuan earthquake

    NASA Astrophysics Data System (ADS)

    Li, H.; Wang, H.; Si, J.; Sun, Z.; Pei, J.; Lei, Z.; He, X.

    2017-12-01

    The WFSD project was implemented promptly after the 2008 Mw 7.9 Wenchuan earthquake. A series of research results on the seismogenic structure, fault deformation, sliding mechanism and fault healing have been obtained, which provide new insights into seismic faulting and mechanisms of the Wenchuan earthquake. The WFSD-1 and -2 drilling core profiles reveal that the Longmen Shan thrust belt is composed of multiple thrust sheets. The 2008 Wenchuan earthquake took place in such tectonic setting with strong horizontal shortening. The two ruptured faults have different deformation mechanisms. The Yingxiu-Beichuan fault (YBF) is a stick-slip fault characterized by fault gouge with high magnetic susceptibility, Guanxian-Anxian fault (GAF) with creeping features and characterized by fault gouge with low magnetic susceptibility. Two PSZs were found in WFSD-1 and -2 cores in the southern segment of YBF. The upper PSZ1 is a low-angle thrust fault characterized by coseisimc graphitization with an extremely low frictional coefficient. The lower PSZ2 is an oblique dextral-slip thrust fault characterized by frictional melt lubrication. In the northern segment of YBF, the PSZ in WFSD-4S cores shows a high-angle thrust feature with fresh melt as well. Therefore, the oblique dextral-slip thrust faulting with frictional melt lubrication is the main faulting of Wenchuan earthquake. Fresh melt with quenching texture was formed in Wenchuan earthquake implying vigorous fluid circulation occurred during the earthquake, which quenched high-temperature melt, hamper the aftermost fault slip and welding seismic fault. Therefore, fluids in the fault zone not only promotes fault weakening, but also suppress slipping in theWenchuan earthquake. The YBF has an extremely high hydraulic diffusivity (2.4×10-2 m2s-1), implying a vigorous fluid circulation in the Wenchuan fault zone. the permeability of YBF has reduced 70% after the shock, reflecting a rapid healing for the YBF. However, the water

  3. Repeating Marmara Sea earthquakes: indication for fault creep

    NASA Astrophysics Data System (ADS)

    Bohnhoff, Marco; Wollin, Christopher; Domigall, Dorina; Küperkoch, Ludger; Martínez-Garzón, Patricia; Kwiatek, Grzegorz; Dresen, Georg; Malin, Peter E.

    2017-07-01

    Discriminating between a creeping and a locked status of active faults is of central relevance to characterize potential rupture scenarios of future earthquakes and the associated seismic hazard for nearby population centres. In this respect, highly similar earthquakes that repeatedly activate the same patch of an active fault portion are an important diagnostic tool to identify and possibly even quantify the amount of fault creep. Here, we present a refined hypocentre catalogue for the Marmara region in northwestern Turkey, where a magnitude M up to 7.4 earthquake is expected in the near future. Based on waveform cross-correlation for selected spatial seismicity clusters, we identify two magnitude M ∼ 2.8 repeater pairs. These repeaters were identified as being indicative of fault creep based on the selection criteria applied to the waveforms. They are located below the western part of the Marmara section of the North Anatolian Fault Zone and are the largest reported repeaters for the larger Marmara region. While the eastern portion of the Marmara seismic gap has been identified to be locked, only sparse information on the deformation status has been reported for its western part. Our findings indicate that the western Marmara section deforms aseismically to a substantial extent, which reduces the probability for this region to host a nucleation point for the pending Marmara earthquake. This is of relevance, since a nucleation of the Marmara event in the west and subsequent eastward rupture propagation towards the Istanbul metropolitan region would result in a substantially higher seismic hazard and resulting risk than if the earthquake would nucleate in the east and thus propagate westward away from the population centre Istanbul.

  4. Slip maxima at fault junctions and rupturing of barriers during the 2008 Wenchuan earthquake

    USGS Publications Warehouse

    Shen, Z.-K.; Sun, Jielun; Zhang, P.; Wan, Y.; Wang, M.; Burgmann, R.; Zeng, Y.; Gan, Weijun; Liao, H.; Wang, Q.

    2009-01-01

    The disastrous 12 May 2008 Wenchuan earthquake in China took the local population as well as scientists by surprise. Although the Longmen Shan fault zonewhich includes the fault segments along which this earthquake nucleatedwas well known, geologic and geodetic data indicate relatively low (<3 mm yr -1) deformation rates. Here we invert Global Positioning System and Interferometric Synthetic Aperture Radar data to infer fault geometry and slip distribution associated with the earthquake. Our analysis shows that the geometry of the fault changes along its length: in the southwest, the fault plane dips moderately to the northwest but becomes nearly vertical in the northeast. Associated with this is a change in the motion along the fault from predominantly thrusting to strike-slip. Peak slip along the fault occurs at the intersections of fault segments located near the towns of Yingxiu, Beichuan and Nanba, where fatalities and damage were concentrated. We suggest that these locations represent barriers that failed in a single event, enabling the rupture to cascade through several fault segments and cause a major moment magnitude (Mw) 7.9 earthquake. Using coseismic slip distribution and geodetic and geological slip rates, we estimate that the failure of barriers and rupture along multiple segments takes place approximately once in 4,000 years. ?? 2009 Macmillan Publishers Limited. All rights reserved.

  5. Surface faults on Montague Island associated with the 1964 Alaska earthquake: Chapter G in The Alaska earthquake, March 27, 1964: regional effects

    USGS Publications Warehouse

    Plafter, George

    1967-01-01

    Two reverse faults on southwestern Montague Island in Prince William Sound were reactivated during the earthquake of March 27, 1964. New fault scarps, fissures, cracks, and flexures appeared in bedrock and unconsolidated surficial deposits along or near the fault traces. Average strike of the faults is between N. 37° E. and N. 47° E.; they dip northwest at angles ranging from 50° to 85°. The dominant motion was dip slip; the blocks northwest of the reactivated faults were relatively upthrown, and both blocks were upthrown relative to sea level. No other earthquake faults have been found on land. The Patton Bay fault on land is a complex system of en echelon strands marked by a series of spectacular landslides along the scarp and (or) by a zone of fissures and flexures on the upthrown block that locally is as much as 3,000 feet wide. The fault can be traced on land for 22 miles, and it has been mapped on the sea floor to the southwest of Montague Island an additional 17 miles. The maximum measured vertical component of slip is 20 to 23 feet and the maximum indicated dip slip is about 26 feet. A left-lateral strike-slip component of less than 2 feet occurs near the southern end of the fault on land where its strike changes from northeast to north. Indirect evidence from the seismic sea waves and aftershocks associated with the earthquake, and from the distribution of submarine scarps, suggests that the faulting on and near Montague Island occurred at the northeastern end of a reactivated submarine fault system that may extend discontinuously for more than 300 miles from Montague Island to the area offshore of the southeast coast of Kodiak Island. The Hanning Bay fault is a minor rupture only 4 miles long that is marked by an exceptionally well defined almost continuous scarp. The maximum measured vertical component of slip is 16⅓ feet near the midpoint, and the indicated dip slip is about 20 feet. There is a maximum left-lateral strike-slip component of one

  6. Change in failure stress on the southern San Andreas fault system caused by the 1992 magnitude = 7.4 Landers earthquake

    USGS Publications Warehouse

    Stein, R.S.; King, G.C.P.; Lin, J.

    1992-01-01

    The 28 June Landers earthquake brought the San Andreas fault significantly closer to failure near San Bernardino, a site that has not sustained a large shock since 1812. Stress also increased on the San Jacinto fault near San Bernardino and on the San Andreas fault southeast of Palm Springs. Unless creep or moderate earthquakes relieve these stress changes, the next great earthquake on the southern San Andreas fault is likely to be advanced by one to two decades. In contrast, stress on the San Andreas north of Los Angeles dropped, potentially delaying the next great earthquake there by 2 to 10 years.

  7. Reading a 400,000-year record of earthquake frequency for an intraplate fault

    NASA Astrophysics Data System (ADS)

    Williams, Randolph T.; Goodwin, Laurel B.; Sharp, Warren D.; Mozley, Peter S.

    2017-05-01

    Our understanding of the frequency of large earthquakes at timescales longer than instrumental and historical records is based mostly on paleoseismic studies of fast-moving plate-boundary faults. Similar study of intraplate faults has been limited until now, because intraplate earthquake recurrence intervals are generally long (10s to 100s of thousands of years) relative to conventional paleoseismic records determined by trenching. Long-term variations in the earthquake recurrence intervals of intraplate faults therefore are poorly understood. Longer paleoseismic records for intraplate faults are required both to better quantify their earthquake recurrence intervals and to test competing models of earthquake frequency (e.g., time-dependent, time-independent, and clustered). We present the results of U-Th dating of calcite veins in the Loma Blanca normal fault zone, Rio Grande rift, New Mexico, United States, that constrain earthquake recurrence intervals over much of the past ˜550 ka—the longest direct record of seismic frequency documented for any fault to date. The 13 distinct seismic events delineated by this effort demonstrate that for >400 ka, the Loma Blanca fault produced periodic large earthquakes, consistent with a time-dependent model of earthquake recurrence. However, this time-dependent series was interrupted by a cluster of earthquakes at ˜430 ka. The carbon isotope composition of calcite formed during this seismic cluster records rapid degassing of CO2, suggesting an interval of anomalous fluid source. In concert with U-Th dates recording decreased recurrence intervals, we infer seismicity during this interval records fault-valve behavior. These data provide insight into the long-term seismic behavior of the Loma Blanca fault and, by inference, other intraplate faults.

  8. Influence of fault steps on rupture termination of strike-slip earthquake faults

    NASA Astrophysics Data System (ADS)

    Li, Zhengfang; Zhou, Bengang

    2018-03-01

    A statistical analysis was completed on the rupture data of 29 historical strike-slip earthquakes across the world. The purpose of this study is to examine the effects of fault steps on the rupture termination of these events. The results show good correlations between the type and length of steps with the seismic rupture and a poor correlation between the step number and seismic rupture. For different magnitude intervals, the smallest widths of the fault steps (Lt) that can terminate the rupture propagation are variable: Lt = 3 km for Ms 6.5 6.9, Lt = 4 km for Ms 7.0 7.5, Lt = 6 km for Ms 7.5 8.0, and Lt = 8 km for Ms 8.0 8.5. The dilational fault step is easier to rupture through than the compression fault step. The smallest widths of the fault step for the rupture arrest can be used as an indicator to judge the scale of the rupture termination of seismic faults. This is helpful for research on fault segmentation, as well as estimating the magnitude of potential earthquakes, and is thus of significance for the assessment of seismic risks.

  9. Earthquake Clustering in Noisy Viscoelastic Systems

    NASA Astrophysics Data System (ADS)

    Dicaprio, C. J.; Simons, M.; Williams, C. A.; Kenner, S. J.

    2006-12-01

    Geologic studies show evidence for temporal clustering of earthquakes on certain fault systems. Since post- seismic deformation may result in a variable loading rate on a fault throughout the inter-seismic period, it is reasonable to expect that the rheology of the non-seismogenic lower crust and mantle lithosphere may play a role in controlling earthquake recurrence times. Previously, the role of rheology of the lithosphere on the seismic cycle had been studied with a one-dimensional spring-dashpot-slider model (Kenner and Simons [2005]). In this study we use the finite element code PyLith to construct a two-dimensional continuum model a strike-slip fault in an elastic medium overlying one or more linear Maxwell viscoelastic layers loaded in the far field by a constant velocity boundary condition. Taking advantage of the linear properties of the model, we use the finite element solution to one earthquake as a spatio-temporal Green's function. Multiple Green's function solutions, scaled by the size of each earthquake, are then summed to form an earthquake sequence. When the shear stress on the fault reaches a predefined yield stress it is allowed to slip, relieving all accumulated shear stress. Random variation in the fault yield stress from one earthquake to the next results in a temporally clustered earthquake sequence. The amount of clustering depends on a non-dimensional number, W, called the Wallace number. For models with one viscoelastic layer, W is equal to the standard deviation of the earthquake stress drop divided by the viscosity times the tectonic loading rate. This definition of W is modified from the original one used in Kenner and Simons [2005] by using the standard deviation of the stress drop instead of the mean stress drop. We also use a new, more appropriate, metric to measure the amount of temporal clustering of the system. W is the ratio of the viscoelastic relaxation rate of the system to the tectonic loading rate of the system. For values of

  10. Geophysical Characterization of the Hilton Creek Fault System

    NASA Astrophysics Data System (ADS)

    Lacy, A. K.; Macy, K. P.; De Cristofaro, J. L.; Polet, J.

    2016-12-01

    The Long Valley Caldera straddles the eastern edge of the Sierra Nevada Batholith and the western edge of the Basin and Range Province, and represents one of the largest caldera complexes on Earth. The caldera is intersected by numerous fault systems, including the Hartley Springs Fault System, the Round Valley Fault System, the Long Valley Ring Fault System, and the Hilton Creek Fault System, which is our main region of interest. The Hilton Creek Fault System appears as a single NW-striking fault, dipping to the NE, from Davis Lake in the south to the southern rim of the Long Valley Caldera. Inside the caldera, it splays into numerous parallel faults that extend toward the resurgent dome. Seismicity in the area increased significantly in May 1980, following a series of large earthquakes in the vicinity of the caldera and a subsequent large earthquake swarm which has been suggested to be the result of magma migration. A large portion of the earthquake swarms in the Long Valley Caldera occurs on or around the Hilton Creek Fault splays. We are conducting an interdisciplinary geophysical study of the Hilton Creek Fault System from just south of the onset of splay faulting, to its extension into the dome of the caldera. Our investigation includes ground-based magnetic field measurements, high-resolution total station elevation profiles, Structure-From-Motion derived topography and an analysis of earthquake focal mechanisms and statistics. Preliminary analysis of topographic profiles, of approximately 1 km in length, reveals the presence of at least three distinct fault splays within the caldera with vertical offsets of 0.5 to 1.0 meters. More detailed topographic mapping is expected to highlight smaller structures. We are also generating maps of the variation in b-value along different portions of the Hilton Creek system to determine whether we can detect any transition to more swarm-like behavior towards the North. We will show maps of magnetic anomalies, topography

  11. Earthquake Prediction in Large-scale Faulting Experiments

    NASA Astrophysics Data System (ADS)

    Junger, J.; Kilgore, B.; Beeler, N.; Dieterich, J.

    2004-12-01

    We study repeated earthquake slip of a 2 m long laboratory granite fault surface with approximately homogenous frictional properties. In this apparatus earthquakes follow a period of controlled, constant rate shear stress increase, analogous to tectonic loading. Slip initiates and accumulates within a limited area of the fault surface while the surrounding fault remains locked. Dynamic rupture propagation and slip of the entire fault surface is induced when slip in the nucleating zone becomes sufficiently large. We report on the event to event reproducibility of loading time (recurrence interval), failure stress, stress drop, and precursory activity. We tentatively interpret these variations as indications of the intrinsic variability of small earthquake occurrence and source physics in this controlled setting. We use the results to produce measures of earthquake predictability based on the probability density of repeating occurrence and the reproducibility of near-field precursory strain. At 4 MPa normal stress and a loading rate of 0.0001 MPa/s, the loading time is ˜25 min, with a coefficient of variation of around 10%. Static stress drop has a similar variability which results almost entirely from variability of the final (rather than initial) stress. Thus, the initial stress has low variability and event times are slip-predictable. The variability of loading time to failure is comparable to the lowest variability of recurrence time of small repeating earthquakes at Parkfield (Nadeau et al., 1998) and our result may be a good estimate of the intrinsic variability of recurrence. Distributions of loading time can be adequately represented by a log-normal or Weibel distribution but long term prediction of the next event time based on probabilistic representation of previous occurrence is not dramatically better than for field-observed small- or large-magnitude earthquake datasets. The gradually accelerating precursory aseismic slip observed in the region of

  12. Paleo-earthquake Analysis from the Morphologic Features of Unconsolidated-sediment Fault Scarp: An Example from Dushanzi Thrust Fault in the Northern Tianshan, China

    NASA Astrophysics Data System (ADS)

    Wei, Z.; He, H.

    2016-12-01

    Fault scarp is important specific tectonic landform caused by surface-rupture earthquake. The morphology of the fault scarp in unconsolidated sediment could evolve in a predictable, time-dependent diffusion model. As a result, the investigation of fault-generated fault scarps is a prevalent technique used to study fault activity, geomorphic evolution, and the recurrence of faulting events. Addition to obtainment of cumulative displacement, gradient changes, i.e. slope breaks, in the morphology of fault scarps could indicate multiple rupture events along an active fault. In this study, we exacted a large set of densely spaced topographic profiles across fault scarp from LiDAR-derive DEM to detect subtle changes in the fault scarp geometry at the Dushanzi trust fault in the Northern Tianshan, China. Several slope breaks in topographic profiles can be identified, which may represent repeated rupture at the investigated fault. The number of paleo-earthquakes derived from our analysis is 4-3, well in agreement with the investigation results from the paleoseismological trenches. Statistical analysis results show that the scarp height of fault scarp with one slope break is 0.75±0.12 (mean value ±1 standard deviation) m representing the last incremental displacement during earthquakes; the height of fault scarp with two slope breaks is 1.86±0.32 m, and the height of fault scarp with three-four slope break is 6.45±1.44 m. Our approach enables us to obtain paleo-earthquake information from geomorphological analysis of fault scarps, and to assess the multiple rupture history of a complex fault system.

  13. Detection of postseismic fault-zone collapse following the Landers earthquake

    NASA Astrophysics Data System (ADS)

    Massonnet, Didier; Thatcher, Wayne; Vadon, Hélèna

    1996-08-01

    STRESS changes caused by fault movement in an earthquake induce transient aseismic crustal movements in the earthquake source region that continue for months to decades following large events1-4. These motions reflect aseismic adjustments of the fault zone and/or bulk deformation of the surroundings in response to applied stresses2,5-7, and supply information regarding the inelastic behaviour of the Earth's crust. These processes are imperfectly understood because it is difficult to infer what occurs at depth using only surface measurements2, which are in general poorly sampled. Here we push satellite radar interferometry to near its typical artefact level, to obtain a map of the postseismic deformation field in the three years following the 28 June 1992 Landers, California earthquake. From the map, we deduce two distinct types of deformation: afterslip at depth on the fault that ruptured in the earthquake, and shortening normal to the fault zone. The latter movement may reflect the closure of dilatant cracks and fluid expulsion from a transiently over-pressured fault zone6-8.

  14. Surface faulting along the Superstition Hills fault zone and nearby faults associated with the earthquakes of 24 November 1987

    USGS Publications Warehouse

    Sharp, R.V.

    1989-01-01

    The M6.2 Elmore Desert Ranch earthquake of 24 November 1987 was associated spatially and probably temporally with left-lateral surface rupture on many northeast-trending faults in and near the Superstition Hills in western Imperial Valley. Three curving discontinuous principal zones of rupture among these breaks extended northeastward from near the Superstition Hills fault zone as far as 9km; the maximum observed surface slip, 12.5cm, was on the northern of the three, the Elmore Ranch fault, at a point near the epicenter. Twelve hours after the Elmore Ranch earthquake, the M6.6 Superstition Hills earthquake occurred near the northwest end of the right-lateral Superstition Hills fault zone. We measured displacements over 339 days at as many as 296 sites along the Superstition Hills fault zone, and repeated measurements at 49 sites provided sufficient data to fit with a simple power law. The overall distributions of right-lateral displacement at 1 day and the estimated final slip are nearly symmetrical about the midpoint of the surface rupture. The average estimated final right-lateral slip for the Superstition Hills fault zone is ~54cm. The average left-lateral slip for the conjugate faults trending northeastward is ~23cm. The southernmost ruptured member of the Superstition Hills fault zone, newly named the Wienert fault, extends the known length of the zone by about 4km. -from Authors

  15. Normal Fault Type Earthquakes Off Fukushima Region - Comparison of the 1938 Events and Recent Earthquakes -

    NASA Astrophysics Data System (ADS)

    Murotani, S.; Satake, K.

    2017-12-01

    Off Fukushima region, Mjma 7.4 (event A) and 6.9 (event B) events occurred on November 6, 1938, following the thrust fault type earthquakes of Mjma 7.5 and 7.3 on the previous day. These earthquakes were estimated as normal fault earthquakes by Abe (1977, Tectonophysics). An Mjma 7.0 earthquake occurred on July 12, 2014 near event B and an Mjma 7.4 earthquake occurred on November 22, 2016 near event A. These recent events are the only M 7 class earthquakes occurred off Fukushima since 1938. Except for the two 1938 events, normal fault earthquakes have not occurred until many aftershocks of the 2011 Tohoku earthquake. We compared the observed tsunami and seismic waveforms of the 1938, 2014, and 2016 earthquakes to examine the normal fault earthquakes occurred off Fukushima region. It is difficult to compare the tsunami waveforms of the 1938, 2014 and 2016 events because there were only a few observations at the same station. The teleseismic body wave inversion of the 2016 earthquake yielded with the focal mechanism of strike 42°, dip 35°, and rake -94°. Other source parameters were as follows: source area 70 km x 40 km, average slip 0.2 m, maximum slip 1.2 m, seismic moment 2.2 x 1019 Nm, and Mw 6.8. A large slip area is located near the hypocenter, and it is compatible with the tsunami source area estimated from tsunami travel times. The 2016 tsunami source area is smaller than that of the 1938 event, consistent with the difference in Mw: 7.7 for event A estimated by Abe (1977) and 6.8 for the 2016 event. Although the 2014 epicenter is very close to that of event B, the teleseismic waveforms of the 2014 event are similar to those of event A and the 2016 event. While Abe (1977) assumed that the mechanism of event B was the same as event A, the initial motions at some stations are opposite, indicating that the focal mechanisms of events A and B are different and more detailed examination is needed. The normal fault type earthquake seems to occur following the

  16. Study on the Evaluation Method for Fault Displacement: Probabilistic Approach Based on Japanese Earthquake Rupture Data - Principal fault displacements -

    NASA Astrophysics Data System (ADS)

    Kitada, N.; Inoue, N.; Tonagi, M.

    2016-12-01

    The purpose of Probabilistic Fault Displacement Hazard Analysis (PFDHA) is estimate fault displacement values and its extent of the impact. There are two types of fault displacement related to the earthquake fault: principal fault displacement and distributed fault displacement. Distributed fault displacement should be evaluated in important facilities, such as Nuclear Installations. PFDHA estimates principal fault and distributed fault displacement. For estimation, PFDHA uses distance-displacement functions, which are constructed from field measurement data. We constructed slip distance relation of principal fault displacement based on Japanese strike and reverse slip earthquakes in order to apply to Japan area that of subduction field. However, observed displacement data are sparse, especially reverse faults. Takao et al. (2013) tried to estimate the relation using all type fault systems (reverse fault and strike slip fault). After Takao et al. (2013), several inland earthquakes were occurred in Japan, so in this time, we try to estimate distance-displacement functions each strike slip fault type and reverse fault type especially add new fault displacement data set. To normalized slip function data, several criteria were provided by several researchers. We normalized principal fault displacement data based on several methods and compared slip-distance functions. The normalized by total length of Japanese reverse fault data did not show particular trend slip distance relation. In the case of segmented data, the slip-distance relationship indicated similar trend as strike slip faults. We will also discuss the relation between principal fault displacement distributions with source fault character. According to slip distribution function (Petersen et al., 2011), strike slip fault type shows the ratio of normalized displacement are decreased toward to the edge of fault. However, the data set of Japanese strike slip fault data not so decrease in the end of the fault

  17. Fluid-rock interaction during a large earthquake recorded in fault gouge: A case study of the Nojima fault, Japan

    NASA Astrophysics Data System (ADS)

    Bian, D.; Lin, A.

    2016-12-01

    Distinguishing the seismic ruptures during the earthquake from a lot of fractures in borehole core is very important to understand rupture processes and seismic efficiency. In particular, a great earthquake like the 1995 Mw 7.2 Kobe earthquake, but again, evidence has been limited to the grain size analysis and the color of fault gouge. In the past two decades, increasing geological evidence has emerged that seismic faults and shear zones within the middle to upper crust play a crucial role in controlling the architectures of crustal fluid migration. Rock-fluid interactions along seismogenic faults give us a chance to find the seismic ruptures from the same event. Recently, a new project of "Drilling into Fault Damage Zone" has being conducted by Kyoto University on the Nojima Fault again after 20 years of the 1995 Kobe earthquake for an integrated multidisciplinary study on the assessment of activity of active faults involving active tectonics, geochemistry and geochronology of active fault zones. In this work, we report on the signature of slip plane inside the Nojima Fault associated with individual earthquakes on the basis of trace element and isotope analyses. Trace element concentrations and 87Sr/86Sr ratios of fault gouge and host rocks were determined by an inductively coupled plasma mass spectrometer (ICP-MS) and thermal ionization mass spectrometry (TIMS). Samples were collected from two trenches and an outcrop of Nojima Fault which. Based on the geochemical result, we interpret these geochemical results in terms of fluid-rock interactions recorded in fault friction during earthquake. The trace-element enrichment pattern of the slip plane can be explained by fluid-rock interactions at high temperature. It also can help us find the main coseismic fault slipping plane inside the thick fault gouge zone.

  18. Evaluation of Earthquake-Induced Effects on Neighbouring Faults and Volcanoes: Application to the 2016 Pedernales Earthquake

    NASA Astrophysics Data System (ADS)

    Bejar, M.; Alvarez Gomez, J. A.; Staller, A.; Luna, M. P.; Perez Lopez, R.; Monserrat, O.; Chunga, K.; Herrera, G.; Jordá, L.; Lima, A.; Martínez-Díaz, J. J.

    2017-12-01

    It has long been recognized that earthquakes change the stress in the upper crust around the fault rupture and can influence the short-term behaviour of neighbouring faults and volcanoes. Rapid estimates of these stress changes can provide the authorities managing the post-disaster situation with a useful tool to identify and monitor potential threads and to update the estimates of seismic and volcanic hazard in a region. Space geodesy is now routinely used following an earthquake to image the displacement of the ground and estimate the rupture geometry and the distribution of slip. Using the obtained source model, it is possible to evaluate the remaining moment deficit and to infer the stress changes on nearby faults and volcanoes produced by the earthquake, which can be used to identify which faults and volcanoes are brought closer to failure or activation. Although these procedures are commonly used today, the transference of these results to the authorities managing the post-disaster situation is not straightforward and thus its usefulness is reduced in practice. Here we propose a methodology to evaluate the potential influence of an earthquake on nearby faults and volcanoes and create easy-to-understand maps for decision-making support after an earthquake. We apply this methodology to the Mw 7.8, 2016 Ecuador earthquake. Using Sentinel-1 SAR and continuous GPS data, we measure the coseismic ground deformation and estimate the distribution of slip. Then we use this model to evaluate the moment deficit on the subduction interface and changes of stress on the surrounding faults and volcanoes. The results are compared with the seismic and volcanic events that have occurred after the earthquake. We discuss potential and limits of the methodology and the lessons learnt from discussion with local authorities.

  19. The July 11, 1995 Myanmar-China earthquake: A representative event in the bookshelf faulting system of southeastern Asia observed from JERS-1 SAR images

    NASA Astrophysics Data System (ADS)

    Ji, Lingyun; Wang, Qingliang; Xu, Jing; Ji, Cunwei

    2017-03-01

    On July 11, 1995, an Mw 6.8 earthquake struck eastern Myanmar near the Chinese border; hereafter referred to as the 1995 Myanmar-China earthquake. Coseismic surface displacements associated with this event are identified from JERS-1 (Japanese Earth Resources Satellite-1) SAR (Synthetic Aperture Radar) images. The largest relative displacement reached 60 cm in the line-of-sight direction. We speculate that a previously unrecognized dextral strike-slip subvertical fault striking NW-SE was responsible for this event. The coseismic slip distribution on the fault planes is inverted based on the InSAR-derived deformation. The results indicate that the fault slip was confined to two lobes. The maximum slip reached approximately 2.5 m at a depth of 5 km in the northwestern part of the focal region. The inverted geodetic moment was approximately Mw = 6.69, which is consistent with seismological results. The 1995 Myanmar-China earthquake is one of the largest recorded earthquakes that has occurred around the "bookshelf faulting" system between the Sagaing fault in Myanmar and the Red River fault in southwestern China.

  20. Near real-time finite fault source inversion for moderate-large earthquakes in Taiwan using teleseismic P waveform

    NASA Astrophysics Data System (ADS)

    Wong, T. P.; Lee, S. J.; Gung, Y.

    2017-12-01

    Taiwan is located at one of the most active tectonic regions in the world. Rapid estimation of the spatial slip distribution of moderate-large earthquake (Mw6.0) is important for emergency response. It is necessary to have a real-time system to provide the report immediately after earthquake happen. The earthquake activities in the vicinity of Taiwan can be monitored by Real-Time Moment Tensor Monitoring System (RMT) which provides the rapid focal mechanism and source parameters. In this study, we follow up the RMT system to develop a near real-time finite fault source inversion system for the moderate-large earthquakes occurred in Taiwan. The system will be triggered by the RMT System when an Mw6.0 is detected. According to RMT report, our system automatically determines the fault dimension, record length, and rise time. We adopted one segment fault plane with variable rake angle. The generalized ray theory was applied to calculate the Green's function for each subfault. The primary objective of the system is to provide the first order image of coseismic slip pattern and identify the centroid location on the fault plane. The performance of this system had been demonstrated by 23 big earthquakes occurred in Taiwan successfully. The results show excellent data fits and consistent with the solutions from other studies. The preliminary spatial slip distribution will be provided within 25 minutes after an earthquake occurred.

  1. Recurrent Holocene movement on the Susitna Glacier Thrust Fault: The structure that initiated the Mw 7.9 Denali Fault earthquake, central Alaska

    USGS Publications Warehouse

    Personius, Stephen; Crone, Anthony J.; Burns, Patricia A.; Reitman, Nadine G.

    2017-01-01

    We conducted a trench investigation and analyzed pre‐ and postearthquake topography to determine the timing and size of prehistoric surface ruptures on the Susitna Glacier fault (SGF), the thrust fault that initiated the 2002 Mw 7.9 Denali fault earthquake sequence in central Alaska. In two of our three hand‐excavated trenches, we found clear evidence for a single pre‐2002 earthquake (penultimate earthquake [PE]) and determined an age of 2210±420  cal. B.P. (2σ) for this event. We used structure‐from‐motion software to create a pre‐2002‐earthquake digital surface model (DSM) from 1:62,800‐scale aerial photography taken in 1980 and compared this DSM with postearthquake 5‐m/pixel Interferometric Synthetic Aperature Radar topography taken in 2010. Topographic profiles measured from the pre‐earthquake DSM show features that we interpret as fault and fold scarps. These landforms were about the same size as those formed in 2002, so we infer that the PE was similar in size to the initial (Mw 7.2) subevent of the 2002 sequence. A recurrence interval of 2270 yrs and dip slip of ∼4.8  m yield a single‐interval slip rate of ∼1.8  mm/yr. The lack of evidence for pre‐PE deformation indicates probable episodic (clustering) behavior on the SGF that may be related to strain migration among other similarly oriented thrust faults that together accommodate shortening south of the Denali fault. We suspect that slip‐partitioned thrust‐triggered earthquakes may be a common occurrence on the Denali fault system, but documenting the frequency of such events will be very difficult, given the lack of long‐term paleoseismic records, the number of potential thrust‐earthquake sources, and the pervasive glacial erosion in the region.

  2. Association of earthquakes and faults in the San Francisco Bay area using Bayesian inference

    USGS Publications Warehouse

    Wesson, R.L.; Bakun, W.H.; Perkins, D.M.

    2003-01-01

    Bayesian inference provides a method to use seismic intensity data or instrumental locations, together with geologic and seismologic data, to make quantitative estimates of the probabilities that specific past earthquakes are associated with specific faults. Probability density functions are constructed for the location of each earthquake, and these are combined with prior probabilities through Bayes' theorem to estimate the probability that an earthquake is associated with a specific fault. Results using this method are presented here for large, preinstrumental, historical earthquakes and for recent earthquakes with instrumental locations in the San Francisco Bay region. The probabilities for individual earthquakes can be summed to construct a probabilistic frequency-magnitude relationship for a fault segment. Other applications of the technique include the estimation of the probability of background earthquakes, that is, earthquakes not associated with known or considered faults, and the estimation of the fraction of the total seismic moment associated with earthquakes less than the characteristic magnitude. Results for the San Francisco Bay region suggest that potentially damaging earthquakes with magnitudes less than the characteristic magnitudes should be expected. Comparisons of earthquake locations and the surface traces of active faults as determined from geologic data show significant disparities, indicating that a complete understanding of the relationship between earthquakes and faults remains elusive.

  3. Use of Fault Displacement Vector to Identify Future Zones of Seismicity: An Example from the Earthquakes of Nepal Himalayas.

    NASA Astrophysics Data System (ADS)

    Naim, F.; Mukherjee, M. K.

    2017-12-01

    Earthquakes occur due to fault slip in the subsurface. They can occur either as interplate or intraplate earthquakes. The region of study is the Nepal Himalayas that defines the boundary of Indian-Eurasian plate and houses the focus of the most devastating earthquakes. The aim of the study was to analyze all the earthquakes that occurred in the Nepal Himalayas upto May 12, 2015 earthquake in order to mark the regions still under stress and vulnerable for future earthquakes. Three different fault systems in the Nepal Himalayas define the tectonic set up of the area. They are: (1) Main Frontal Thrust(MFT), (2) Main Central Thrust(MCT) and (3) Main Boundary Thrust(MBT) that extend from NW to SE. Most of the earthquakes were observed to occur between the MBT and MCT. Since the thrust faults are dipping towards NE, the focus of most of the earthquakes lies on the MBT. The methodology includes estimating the dip of the fault by considering the depths of different earthquake events and their corresponding distance from the MBT. In order to carry out stress analysis on the fault, the beach ball diagrams associated with the different earthquakes were plotted on a map. Earthquakes in the NW and central region of the fault zone were associated with reverse fault slip while that on the South-Eastern part were associated with a strike slip component. The direction of net slip on the fault associated with the different earthquakes was known and from this a 3D slip diagram of the fault was constructed. The regions vulnerable for future earthquakes in the Nepal Himalaya were demarcated on the 3D slip diagram of the fault. Such zones were marked owing to the fact that the slips due to earthquakes cause the adjoining areas to come under immense stress and this stress is directly proportional to the amount of slip occuring on the fault. These vulnerable zones were in turn projected on the map to show their position and are predicted to contain the epicenter of the future earthquakes.

  4. Aseismic Transform Fault Slip at the Mendocino Triple Junction From Characteristically Repeating Earthquakes

    NASA Astrophysics Data System (ADS)

    Materna, Kathryn; Taira, Taka'aki; Bürgmann, Roland

    2018-01-01

    The Mendocino Triple Junction (MTJ), at the northern terminus of the San Andreas Fault system, is an actively deforming plate boundary region with poorly constrained estimates of seismic coupling on most offshore fault surfaces. Characteristically repeating earthquakes provide spatial and temporal descriptions of aseismic creep at the MTJ, including on the oceanic transform Mendocino Fault Zone (MFZ) as it subducts beneath North America. Using a dataset of earthquakes from 2008 to 2017, we find that the easternmost segment of the MFZ displays creep during this period at about 65% of the long-term slip rate. We also find creep at slower rates on the shallower strike-slip interface between the Pacific plate and the North American accretionary wedge, as well as on a fault that accommodates Gorda subplate internal deformation. After a nearby M5.7 earthquake in 2015, we observe a possible decrease in aseismic slip on the near-shore MFZ that lasts from 2015 to at least early 2017.

  5. Fault failure with moderate earthquakes

    USGS Publications Warehouse

    Johnston, M.J.S.; Linde, A.T.; Gladwin, M.T.; Borcherdt, R.D.

    1987-01-01

    High resolution strain and tilt recordings were made in the near-field of, and prior to, the May 1983 Coalinga earthquake (ML = 6.7, ?? = 51 km), the August 4, 1985, Kettleman Hills earthquake (ML = 5.5, ?? = 34 km), the April 1984 Morgan Hill earthquake (ML = 6.1, ?? = 55 km), the November 1984 Round Valley earthquake (ML = 5.8, ?? = 54 km), the January 14, 1978, Izu, Japan earthquake (ML = 7.0, ?? = 28 km), and several other smaller magnitude earthquakes. These recordings were made with near-surface instruments (resolution 10-8), with borehole dilatometers (resolution 10-10) and a 3-component borehole strainmeter (resolution 10-9). While observed coseismic offsets are generally in good agreement with expectations from elastic dislocation theory, and while post-seismic deformation continued, in some cases, with a moment comparable to that of the main shock, preseismic strain or tilt perturbations from hours to seconds (or less) before the main shock are not apparent above the present resolution. Precursory slip for these events, if any occurred, must have had a moment less than a few percent of that of the main event. To the extent that these records reflect general fault behavior, the strong constraint on the size and amount of slip triggering major rupture makes prediction of the onset times and final magnitudes of the rupture zones a difficult task unless the instruments are fortuitously installed near the rupture initiation point. These data are best explained by an inhomogeneous failure model for which various areas of the fault plane have either different stress-slip constitutive laws or spatially varying constitutive parameters. Other work on seismic waveform analysis and synthetic waveforms indicates that the rupturing process is inhomogeneous and controlled by points of higher strength. These models indicate that rupture initiation occurs at smaller regions of higher strength which, when broken, allow runaway catastrophic failure. ?? 1987.

  6. Spatial and Temporal Variations in Earthquake Stress Drop on Gofar Transform Fault, East Pacific Rise: Implications for Fault Strength

    NASA Astrophysics Data System (ADS)

    Moyer, P. A.; Boettcher, M. S.; McGuire, J. J.; Collins, J. A.

    2017-12-01

    During the last five seismic cycles on Gofar transform fault on the East Pacific Rise, the largest earthquakes (6.0 ≤ Mw ≤ 6.2) have repeatedly ruptured the same fault segment (rupture asperity), while intervening fault segments host swarms of microearthquakes. Previous studies on Gofar have shown that these segments of low (≤10%) seismic coupling contain diffuse zones of seismicity and P-wave velocity reduction compared with the rupture asperity; suggesting heterogeneous fault properties control earthquake behavior. We investigate the role systematic differences in material properties have on earthquake rupture along Gofar using waveforms from ocean bottom seismometers that recorded the end of the 2008 Mw 6.0 seismic cycle.We determine stress drop for 117 earthquakes (2.4 ≤ Mw ≤ 4.2) that occurred in and between rupture asperities from corner frequency derived using an empirical Green's function spectral ratio method and seismic moment obtained by fitting the omega-square source model to the low frequency amplitude of earthquake spectra. We find stress drops from 0.03 to 2.7 MPa with significant spatial variation, including 2 times higher average stress drop in the rupture asperity compared to fault segments with low seismic coupling. We interpret an inverse correlation between stress drop and P-wave velocity reduction as the effect of damage on earthquake rupture. Earthquakes with higher stress drops occur in more intact crust of the rupture asperity, while earthquakes with lower stress drops occur in regions of low seismic coupling and reflect lower strength, highly fractured fault zone material. We also observe a temporal control on stress drop consistent with log-time healing following the Mw 6.0 mainshock, suggesting a decrease in stress drop as a result of fault zone damage caused by the large earthquake.

  7. Stress transfer to the Denali and other regional faults from the M 9.2 Alaska earthquake of 1964

    USGS Publications Warehouse

    Bufe, C.G.

    2004-01-01

    Stress transfer from the great 1964 Prince William Sound earthquake is modeled on the Denali fault, including the Denali-Totschunda fault segments that ruptured in 2002, and on other regional fault systems where M 7.5 and larger earthquakes have occurred since 1900. The results indicate that analysis of Coulomb stress transfer from the dominant earthquake in a region is a potentially powerful tool in assessing time-varying earthquake hazard. Modeled Coulomb stress increases on the northern Denali and Totschunda faults from the great 1964 earthquake coincide with zones that ruptured in the 2002 Denali fault earthquake, although stress on the Susitna Glacier thrust plane, where the 2002 event initiated, was decreased. A southeasterlytrending Coulomb stress transect along the right-lateral Totschunda-Fairweather-Queen Charlotte trend shows stress transfer from the 1964 event advancing slip on the Totschunda, Fairweather, and Queen Charlotte segments, including the southern Fairweather segment that ruptured in 1972. Stress transfer retarding right-lateral strike slip was observed from the southern part of the Totschunda fault to the northern end of the Fairweather fault (1958 rupture). This region encompasses a gap with shallow thrust faulting but with little evidence of strike-slip faulting connecting the segments to the northwest and southeast. Stress transfer toward failure was computed on the north-south trending right-lateral strike-slip faults in the Gulf of Alaska that ruptured in 1987 and 1988, with inhibitory stress changes at the northern end of the northernmost (1987) rupture. The northern Denali and Totschunda faults, including the zones that ruptured in the 2002 earthquakes, follow very closely (within 3%), for about 90??, an arc of a circle of radius 375 km. The center of this circle is within a few kilometers of the intersection at depth of the Patton Bay fault with the Alaskan megathrust. This inferred asperity edge may be the pole of counterclockwise

  8. Distributing Earthquakes Among California's Faults: A Binary Integer Programming Approach

    NASA Astrophysics Data System (ADS)

    Geist, E. L.; Parsons, T.

    2016-12-01

    Statement of the problem is simple: given regional seismicity specified by a Gutenber-Richter (G-R) relation, how are earthquakes distributed to match observed fault-slip rates? The objective is to determine the magnitude-frequency relation on individual faults. The California statewide G-R b-value and a-value are estimated from historical seismicity, with the a-value accounting for off-fault seismicity. UCERF3 consensus slip rates are used, based on geologic and geodetic data and include estimates of coupling coefficients. The binary integer programming (BIP) problem is set up such that each earthquake from a synthetic catalog spanning millennia can occur at any location along any fault. The decision vector, therefore, consists of binary variables, with values equal to one indicating the location of each earthquake that results in an optimal match of slip rates, in an L1-norm sense. Rupture area and slip associated with each earthquake are determined from a magnitude-area scaling relation. Uncertainty bounds on the UCERF3 slip rates provide explicit minimum and maximum constraints to the BIP model, with the former more important to feasibility of the problem. There is a maximum magnitude limit associated with each fault, based on fault length, providing an implicit constraint. Solution of integer programming problems with a large number of variables (>105 in this study) has been possible only since the late 1990s. In addition to the classic branch-and-bound technique used for these problems, several other algorithms have been recently developed, including pre-solving, sifting, cutting planes, heuristics, and parallelization. An optimal solution is obtained using a state-of-the-art BIP solver for M≥6 earthquakes and California's faults with slip-rates > 1 mm/yr. Preliminary results indicate a surprising diversity of on-fault magnitude-frequency relations throughout the state.

  9. The regional structural setting of the 2008 Wells earthquake and Town Creek Flat Basin: implications for the Wells earthquake fault and adjacent structures

    USGS Publications Warehouse

    Henry, Christopher S.; Colgan, Joseph P.

    2011-01-01

    The 2008 Wells earthquake occurred on a northeast-striking, southeast-dipping fault that is clearly delineated by the aftershock swarm to a depth of 10-12 km below sea level. However, Cenozoic rocks and structures around Wells primarily record east-west extension along north- to north-northeast-striking, west-dipping normal faults that formed during the middle Miocene. These faults are responsible for the strong eastward tilt of most basins and ranges in the area, including the Town Creek Flat basin (the location of the earthquake) and the adjacent Snake Mountains and western Windermere Hills. These older west-dipping faults are locally overprinted by a younger generation of east-dipping, high-angle normal faults that formed as early as the late Miocene and have remained active into the Quaternary. The most prominent of these east-dipping faults is the set of en-échelon, north-striking faults that bounds the east sides of the Ruby Mountains, East Humboldt Range, and Clover Hill (about 5 km southwest of Wells). The northeastern-most of these faults, the Clover Hill fault, projects northward along strike toward the Snake Mountains and the approximately located surface projection of the Wells earthquake fault as defined by aftershock locations. The Clover Hill fault also projects toward a previously unrecognized, east-facing Quaternary fault scarp and line of springs that appear to mark a significant east-dipping normal fault along the western edge of Town Creek Flat. Both western and eastern projections may be northern continuations of the Clover Hill fault. The Wells earthquake occurred along this east-dipping fault system. Two possible alternatives to rupture of a northern continuation of the Clover Hill fault are that the earthquake fault (1) is antithetic to an active west-dipping fault or (2) reactivated a Mesozoic thrust fault that dips east as a result of tilting by the west-dipping faults along the west side of the Snake Mountains. Both alternatives are

  10. The history of late holocene surface-faulting earthquakes on the central segments of the Wasatch fault zone, Utah

    USGS Publications Warehouse

    Duross, Christopher; Personius, Stephen; Olig, Susan S; Crone, Anthony J.; Hylland, Michael D.; Lund, William R; Schwartz, David P.

    2017-01-01

    The Wasatch fault (WFZ)—Utah’s longest and most active normal fault—forms a prominent eastern boundary to the Basin and Range Province in northern Utah. To provide paleoseismic data for a Wasatch Front regional earthquake forecast, we synthesized paleoseismic data to define the timing and displacements of late Holocene surface-faulting earthquakes on the central five segments of the WFZ. Our analysis yields revised histories of large (M ~7) surface-faulting earthquakes on the segments, as well as estimates of earthquake recurrence and vertical slip rate. We constrain the timing of four to six earthquakes on each of the central segments, which together yields a history of at least 24 surface-faulting earthquakes since ~6 ka. Using earthquake data for each segment, inter-event recurrence intervals range from about 0.6 to 2.5 kyr, and have a mean of 1.2 kyr. Mean recurrence, based on closed seismic intervals, is ~1.1–1.3 kyr per segment, and when combined with mean vertical displacements per segment of 1.7–2.6 m, yield mean vertical slip rates of 1.3–2.0 mm/yr per segment. These data refine the late Holocene behavior of the central WFZ; however, a significant source of uncertainty is whether structural complexities that define the segments of the WFZ act as hard barriers to ruptures propagating along the fault. Thus, we evaluate fault rupture models including both single-segment and multi-segment ruptures, and define 3–17-km-wide spatial uncertainties in the segment boundaries. These alternative rupture models and segment-boundary zones honor the WFZ paleoseismic data, take into account the spatial and temporal limitations of paleoseismic data, and allow for complex ruptures such as partial-segment and spillover ruptures. Our data and analyses improve our understanding of the complexities in normal-faulting earthquake behavior and provide geological inputs for regional earthquake-probability and seismic hazard assessments.

  11. Continuous Record of Permeability inside the Wenchuan Earthquake Fault Zone

    NASA Astrophysics Data System (ADS)

    Xue, Lian; Li, Haibing; Brodsky, Emily

    2013-04-01

    Faults are complex hydrogeological structures which include a highly permeable damage zone with fracture-dominated permeability. Since fractures are generated by earthquakes, we would expect that in the aftermath of a large earthquake, the permeability would be transiently high in a fault zone. Over time, the permeability may recover due to a combination of chemical and mechanical processes. However, the in situ fault zone hydrological properties are difficult to measure and have never been directly constrained on a fault zone immediately after a large earthquake. In this work, we use water level response to solid Earth tides to constrain the hydraulic properties inside the Wenchuan Earthquake Fault Zone. The transmissivity and storage determine the phase and amplitude response of the water level to the tidal loading. By measuring phase and amplitude response, we can constrain the average hydraulic properties of the damage zone at 800-1200 m below the surface (~200-600 m from the principal slip zone). We use Markov chain Monte Carlo methods to evaluate the phase and amplitude responses and the corresponding errors for the largest semidiurnal Earth tide M2 in the time domain. The average phase lag is ~ 30o, and the average amplitude response is 6×10-7 strain/m. Assuming an isotropic, homogenous and laterally extensive aquifer, the average storage coefficient S is 2×10-4 and the average transmissivity T is 6×10-7 m2 using the measured phase and the amplitude response. Calculation for the hydraulic diffusivity D with D=T/S, yields the reported value of D is 3×10-3 m2/s, which is two orders of magnitude larger than pump test values on the Chelungpu Fault which is the site of the Mw 7.6 Chi-Chi earthquake. If the value is representative of the fault zone, then this means the hydrology processes should have an effect on the earthquake rupture process. This measurement is done through continuous monitoring and we could track the evolution for hydraulic properties

  12. High-precision relocation for aftershocks of the 2016 ML 5.8 Gyeongju earthquake in South Korea: Stress partitioning controlled by complex fault systems

    NASA Astrophysics Data System (ADS)

    Woo, J. U.; Rhie, J.; Kang, T. S.; Kim, S.; Chai, G.; Cho, E.

    2017-12-01

    Complex inherent fault system is one of key factors controlling the main shock occurrence and the pattern of aftershock sequence. Many field studies have shown that the fault systems in the Korean Peninsula are complex because they formed by various tectonic events since Proterozoic. Apart from that the mainshock is the largest one (ML 5.8) ever recorded in South Korea, the Gyeongju earthquake sequence shows particularly interesting features: ML 5.1 event preceded ML 5.8 event by 50 min and they are located closely to each other ( 1 km). In addition, ML 4.5 event occurred 2 3 km away from the two events after a week of the mainshock. Considering reported focal mechanisms and hypocenters of the three major events, it is unlikely that the earthquake sequence occurs on a single fault plane. To depict the detailed fault geometry associated with the sequence, we precisely determine the relative locations of 1,400 aftershocks recorded by 27 broadband stations, which started to be deployed less than one hour after the mainshock. Double difference algorithm is applied using relative travel time measurements by a waveform cross-correlation method. Relocated hypocenters show that a major fault striking NE-SW and some minor faults get involved in the sequence. In particular, aftershocks immediately following ML 4.5 event seem to occur on a fault striking NW-SE, which is orthogonal to the strike of a major fault. We expect that the Gyeongju earthquake sequence resulted from the stress transfer controlled by the complex inherent fault system in this region.

  13. Active arc-continent collision: Earthquakes, gravity anomalies, and fault kinematics in the Huon-Finisterre collision zone, Papua New Guinea

    NASA Astrophysics Data System (ADS)

    Abers, Geoffrey A.; McCaffrey, Robert

    1994-04-01

    The Huon-Finisterre island arc terrane is actively colliding with the north edge of the Australian continent. The collision provides a rare opportunity to study continental accretion while it occurs. We examine the geometry and kinematics of the collision by comparing earthquake source parameters to surface fault geometries and plate motions, and we constrain the forces active in the collision by comparing topographic loads to gravity anomalies. Waveform inversion is used to constrain focal mechanisms for 21 shallow earthquakes that occurred between 1966 and 1992 (seismic moment 1017 to 3 × 1020 N m). Twelve earthquakes show thrust faulting at 22-37 km depth. The largest thrust events are on the north side of the Huon Peninsula and are consistent with slip on the Ramu-Markham thrust fault zone, the northeast dipping thrust fault system that bounds the Huon-Finisterre terrane. Thus much of the terrane's crust but little of its mantle is presently being added to the Australian continent. The large thrust earthquakes also reveal a plausible mechanism for the uplift of Pleistocene coral terraces on the north side of the Huon Peninsula. Bouguer gravity anomalies are too negative to allow simple regional compensation of topography and require large additional downward forces to depress the lower plate beneath the Huon Peninsula. With such forces, plate configurations are found that are consistent with observed gravity and basin geometry. Other earthquakes give evidence of deformation above and below the Ramu-Markham thrust system. Four thrust events, 22-27 km depth directly below the Ramu-Markham fault outcrop, are too deep to be part of a planar Ramu-Markham thrust system and may connect to the north dipping Highlands thrust system farther south. Two large strike-slip faulting earthquakes and their aftershocks, in 1970 and 1987, show faulting within the upper plate of the thrust system. The inferred fault planes show slip vectors parallel to those on nearby thrust

  14. Crustal structure and fault geometry of the 2010 Haiti earthquake from temporary seismometer deployments

    USGS Publications Warehouse

    Douilly, Roby; Haase, Jennifer S.; Ellsworth, William L.; Bouin, Marie‐Paule; Calais, Eric; Symithe, Steeve J.; Armbruster, John G.; Mercier de Lépinay, Bernard; Deschamps, Anne; Mildor, Saint‐Louis; Meremonte, Mark E.; Hough, Susan E.

    2013-01-01

    Haiti has been the locus of a number of large and damaging historical earthquakes. The recent 12 January 2010 Mw 7.0 earthquake affected cities that were largely unprepared, which resulted in tremendous losses. It was initially assumed that the earthquake ruptured the Enriquillo Plantain Garden fault (EPGF), a major active structure in southern Haiti, known from geodetic measurements and its geomorphic expression to be capable of producing M 7 or larger earthquakes. Global Positioning Systems (GPS) and Interferometric Synthetic Aperture Radar (InSAR) data, however, showed that the event ruptured a previously unmapped fault, the Léogâne fault, a north‐dipping oblique transpressional fault located immediately north of the EPGF. Following the earthquake, several groups installed temporary seismic stations to record aftershocks, including ocean‐bottom seismometers on either side of the EPGF. We use data from the complete set of stations deployed after the event, on land and offshore, to relocate all aftershocks from 10 February to 24 June 2010, determine a 1D regional crustal velocity model, and calculate focal mechanisms. The aftershock locations from the combined dataset clearly delineate the Léogâne fault, with a geometry close to that inferred from geodetic data. Its strike and dip closely agree with the global centroid moment tensor solution of the mainshock but with a steeper dip than inferred from previous finite fault inversions. The aftershocks also delineate a structure with shallower southward dip offshore and to the west of the rupture zone, which could indicate triggered seismicity on the offshore Trois Baies reverse fault. We use first‐motion focal mechanisms to clarify the relationship of the fault geometry to the triggered aftershocks.

  15. Refinements on the inferred causative faults of the great 2012 Indian Ocean earthquakes

    NASA Astrophysics Data System (ADS)

    Revathy, P. M.; Rajendran, K.

    2014-12-01

    As the largest known intra-plate strike-slip events, the pair of 2012 earthquakes in the Wharton Basin is a rarity. Separated in time by 2 hours these events rouse interest also because of their short inter-event duration, complex rupture mechanism, and spatial-temporal proximity to the great 2004 Sumatra plate boundary earthquake. Reactivation of fossil ridge-transform pairs is a favoured mechanism for large oceanic plate earthquakes and their inherent geometry triggers earthquakes on conjugate fault systems, as observed previously in the Wharton Basin. The current debate is whether the ruptures occurred on the WNW-ESE paleo ridges or the NNE-SSW paleo transforms. Back-projection models give a complex rupture pattern that favours the WNW-ESE fault [1]. However, the static stress changes due to the 2004 Sumatra earthquake and 2005 Nias earthquake favour the N15°E fault [2]. We use the Teleseismic Body-Wave Inversion Program [3] and waveform data from Global Seismic Network, to obtain the best fit solutions using P and S-wave synthetic modelling. The preliminary P-wave analysis of both earthquakes gives source parameters that are consistent with the Harvard CMT solutions. The obtained slip distribution complies with the NNE-SSW transforms. Both these earthquakes triggered small tsunamis which appear as two distinctive pulses on 13 Indian Ocean tide gauges and buoys. Frequency spectra of the tsunami recordings from various azimuths provide additional constraint for the choice of the causative faults. References: [1] Yue, H., T. Lay, and K. D. Koper (2012), En echelon and orthogonal fault ruptures of the 11 April 2012 great intraplate earthquakes, Nature, 490, 245-249, doi:10.1038/nature11492 [2] Delescluse, M., N. Chamot-Rooke, R. Cattin, L. Fleitout, O. Trubienko and C. Vigny April 2012 intra-oceanic seismicity off Sumatra boosted by the Banda-Aceh megathrust, Nature, 490(2012), pp. 240-244, doi:10.1038/nature11520 [3] M. Kikuchi and H. Kanamori, Note on

  16. Satellite Geodetic Constraints On Earthquake Processes: Implications of the 1999 Turkish Earthquakes for Fault Mechanics and Seismic Hazards on the San Andreas Fault

    NASA Technical Reports Server (NTRS)

    Reilinger, Robert

    2005-01-01

    Our principal activities during the initial phase of this project include: 1) Continued monitoring of postseismic deformation for the 1999 Izmit and Duzce, Turkey earthquakes from repeated GPS survey measurements and expansion of the Marmara Continuous GPS Network (MAGNET), 2) Establishing three North Anatolian fault crossing profiles (10 sitedprofile) at locations that experienced major surface-fault earthquakes at different times in the past to examine strain accumulation as a function of time in the earthquake cycle (2004), 3) Repeat observations of selected sites in the fault-crossing profiles (2005), 4) Repeat surveys of the Marmara GPS network to continue to monitor postseismic deformation, 5) Refining block models for the Marmara Sea seismic gap area to better understand earthquake hazards in the Greater Istanbul area, 6) Continuing development of models for afterslip and distributed viscoelastic deformation for the earthquake cycle. We are keeping close contact with MIT colleagues (Brad Hager, and Eric Hetland) who are developing models for S. California and for the earthquake cycle in general (Hetland, 2006). In addition, our Turkish partners at the Marmara Research Center have undertaken repeat, micro-gravity measurements at the MAGNET sites and have provided us estimates of gravity change during the period 2003 - 2005.

  17. Effects of Fault Segmentation, Mechanical Interaction, and Structural Complexity on Earthquake-Generated Deformation

    NASA Astrophysics Data System (ADS)

    Haddad, David Elias

    Earth's topographic surface forms an interface across which the geodynamic and geomorphic engines interact. This interaction is best observed along crustal margins where topography is created by active faulting and sculpted by geomorphic processes. Crustal deformation manifests as earthquakes at centennial to millennial timescales. Given that nearly half of Earth's human population lives along active fault zones, a quantitative understanding of the mechanics of earthquakes and faulting is necessary to build accurate earthquake forecasts. My research relies on the quantitative documentation of the geomorphic expression of large earthquakes and the physical processes that control their spatiotemporal distributions. The first part of my research uses high-resolution topographic lidar data to quantitatively document the geomorphic expression of historic and prehistoric large earthquakes. Lidar data allow for enhanced visualization and reconstruction of structures and stratigraphy exposed by paleoseismic trenches. Lidar surveys of fault scarps formed by the 1992 Landers earthquake document the centimeter-scale erosional landforms developed by repeated winter storm-driven erosion. The second part of my research employs a quasi-static numerical earthquake simulator to explore the effects of fault roughness, friction, and structural complexities on earthquake-generated deformation. My experiments show that fault roughness plays a critical role in determining fault-to-fault rupture jumping probabilities. These results corroborate the accepted 3-5 km rupture jumping distance for smooth faults. However, my simulations show that the rupture jumping threshold distance is highly variable for rough faults due to heterogeneous elastic strain energies. Furthermore, fault roughness controls spatiotemporal variations in slip rates such that rough faults exhibit lower slip rates relative to their smooth counterparts. The central implication of these results lies in guiding the

  18. Source characteristics of 2000 small earthquakes nucleating on the Alto Tiberina fault system (central Italy).

    NASA Astrophysics Data System (ADS)

    Munafo, I.; Malagnini, L.; Tinti, E.; Chiaraluce, L.; Di Stefano, R.; Valoroso, L.

    2014-12-01

    The Alto Tiberina Fault (ATF) is a 60 km long east-dipping low-angle normal fault, located in a sector of the Northern Apennines (Italy) undergoing active extension since the Quaternary. The ATF has been imaged by analyzing the active source seismic reflection profiles, and the instrumentally recorded persistent background seismicity. The present study is an attempt to separate the contributions of source, site, and crustal attenuation, in order to focus on the mechanics of the seismic sources on the ATF, as well on the synthetic and the antithetic structures within the ATF hanging-wall (i.e. Colfiorito fault, Gubbio fault and Umbria Valley fault). In order to compute source spectra, we perform a set of regressions over the seismograms of 2000 small earthquakes (-0.8 < ML< 4) recorded between 2010 and 2014 at 50 permanent seismic stations deployed in the framework of the Alto Tiberina Near Fault Observatory project (TABOO) and equipped with three-components seismometers, three of which located in shallow boreholes. Because we deal with some very small earthquakes, we maximize the signal to noise ratio (SNR) with a technique based on the analysis of peak values of bandpass-filtered time histories, in addition to the same processing performed on Fourier amplitudes. We rely on a tool called Random Vibration Theory (RVT) to completely switch from peak values in the time domain to Fourier spectral amplitudes. Low-frequency spectral plateau of the source terms are used to compute moment magnitudes (Mw) of all the events, whereas a source spectral ratio technique is used to estimate the corner frequencies (Brune spectral model) of a subset of events chosen over the analysis of the noise affecting the spectral ratios. So far, the described approach provides high accuracy over the spectral parameters of earthquakes of localized seismicity, and may be used to gain insights into the underlying mechanics of faulting and the earthquake processes.

  19. Potential earthquake faults offshore Southern California, from the eastern Santa Barbara Channel south to Dana Point

    USGS Publications Warehouse

    Fisher, M.A.; Sorlien, C.C.; Sliter, R.W.

    2009-01-01

    Urban areas in Southern California are at risk from major earthquakes, not only quakes generated by long-recognized onshore faults but also ones that occur along poorly understood offshore faults. We summarize recent research findings concerning these lesser known faults. Research by the U.S. Geological Survey during the past five years indicates that these faults from the eastern Santa Barbara Channel south to Dana Point pose a potential earthquake threat. Historical seismicity in this area indicates that, in general, offshore faults can unleash earthquakes having at least moderate (M 5-6) magnitude. Estimating the earthquake hazard in Southern California is complicated by strain partitioning and by inheritance of structures from early tectonic episodes. The three main episodes are Mesozoic through early Miocene subduction, early Miocene crustal extension coeval with rotation of the Western Transverse Ranges, and Pliocene and younger transpression related to plate-boundary motion along the San Andreas Fault. Additional complication in the analysis of earthquake hazards derives from the partitioning of tectonic strain into strike-slip and thrust components along separate but kinematically related faults. The eastern Santa Barbara Basin is deformed by large active reverse and thrust faults, and this area appears to be underlain regionally by the north-dipping Channel Islands thrust fault. These faults could produce moderate to strong earthquakes and destructive tsunamis. On the Malibu coast, earthquakes along offshore faults could have left-lateral-oblique focal mechanisms, and the Santa Monica Mountains thrust fault, which underlies the oblique faults, could give rise to large (M ??7) earthquakes. Offshore faults near Santa Monica Bay and the San Pedro shelf are likely to produce both strike-slip and thrust earthquakes along northwest-striking faults. In all areas, transverse structures, such as lateral ramps and tear faults, which crosscut the main faults, could

  20. Coseismic deformation of the 2001 El Salvador and 2002 Denali fault earthquakes from GPS geodetic measurements

    NASA Astrophysics Data System (ADS)

    Hreinsdottir, Sigrun

    2005-07-01

    GPS geodetic measurements are used to study two major earthquakes, the 2001 MW 7.7 El Salvador and 2002 MW 7.9 Denali Fault earthquakes. The 2001 MW 7.7 earthquake was a normal fault event in the subducting Cocos plate offshore El Salvador. Coseismic displacements of up to 15 mm were measured at permanent GPS stations in Central America. The GPS data were used to constrain the location of and slip on the normal fault. One month later a MW 6.6 strike-slip earthquake occurred in the overriding Caribbean plate. Coulomb stress changes estimated from the M W 7.7 earthquake suggest that it triggered the MW 6.6 earthquake. Coseismic displacement from the MW 6.6 earthquake, about 40 mm at a GPS station in El Salvador, indicates that the earthquake triggered additional slip on a fault close to the GPS station. The MW 6.6 earthquake further changed the stress field in the overriding Caribbean plate, with triggered seismic activity occurring west and possibly also to the east of the rupture in the days to months following the earthquake. The MW 7.9 Denali Fault earthquake ruptured three faults in the interior of Alaska. It initiated with a thrust motion on the Susitna Glacier fault but then ruptured the Denali and Totschunda faults with predominantly right-lateral strike-slip motion unilaterally from west to east. GPS data measured in the two weeks following the earthquake suggest a complex coseismic rupture along the faults with two main regions of moment release along the Denali fault. A large amount of additional data were collected in the year following the earthquake which greatly improved the resolution on the fault, revealing more details of the slip distribution. We estimate a total moment release of 6.81 x 1020 Nm in the earthquake with a M W 7.2 thrust subevent on Susitna Glacier fault. The slip on the Denali fault is highly variable, with 4 main pulses of moment release. The largest moment pulse corresponds to a MW 7.5 subevent, about 40 km west of the Denali

  1. Frictional stability and earthquake triggering during fluid pressure stimulation of an experimental fault

    NASA Astrophysics Data System (ADS)

    Scuderi, M. M.; Collettini, C.; Marone, C.

    2017-11-01

    It is widely recognized that the significant increase of M > 3.0 earthquakes in Western Canada and the Central United States is related to underground fluid injection. Following injection, fluid overpressure lubricates the fault and reduces the effective normal stress that holds the fault in place, promoting slip. Although, this basic physical mechanism for earthquake triggering and fault slip is well understood, there are many open questions related to induced seismicity. Models of earthquake nucleation based on rate- and state-friction predict that fluid overpressure should stabilize fault slip rather than trigger earthquakes. To address this controversy, we conducted laboratory creep experiments to monitor fault slip evolution at constant shear stress while the effective normal stress was systematically reduced via increasing fluid pressure. We sheared layers of carbonate-bearing fault gouge in a double direct shear configuration within a true-triaxial pressure vessel. We show that fault slip evolution is controlled by the stress state acting on the fault and that fluid pressurization can trigger dynamic instability even in cases of rate strengthening friction, which should favor aseismic creep. During fluid pressurization, when shear and effective normal stresses reach the failure condition, accelerated creep occurs in association with fault dilation; further pressurization leads to an exponential acceleration with fault compaction and slip localization. Our work indicates that fault weakening induced by fluid pressurization can overcome rate strengthening friction resulting in fast acceleration and earthquake slip. Our work points to modifications of the standard model for earthquake nucleation to account for the effect of fluid overpressure and to accurately predict the seismic risk associated with fluid injection.

  2. Continuous Record of Permeability inside the Wenchuan Earthquake Fault Zone

    NASA Astrophysics Data System (ADS)

    Xue, L.; Li, H.; Brodsky, E. E.; Wang, H.; Pei, J.

    2012-12-01

    Faults are complex hydrogeological structures which include a highly permeable damage zone with fracture-dominated permeability. Since fractures are generated by earthquakes, we would expect that in the aftermath of a large earthquake, the permeability would be transiently high in a fault zone. Over time, the permeability may recover due to a combination of chemical and mechanical processes. However, the in situ fault zone hydrological properties are difficult to measure and have never been directly constrained on a fault zone immediately after a large earthquake. In this work, we use water level response to solid Earth tides to constrain the hydraulic properties inside the Wenchuan Earthquake Fault Zone. The transmissivity and storage determine the phase and amplitude response of the water level to the tidal loading. By measuring phase and amplitude response, we can constrain the average hydraulic properties of the damage zone at 800-1200 m below the surface (˜200-600 m from the principal slip zone). We use Markov chain Monte Carlo methods to evaluate the phase and amplitude responses and the corresponding errors for the largest semidiurnal Earth tide M2 in the time domain. The average phase lag is ˜30°, and the average amplitude response is 6×10-7 strain/m. Assuming an isotropic, homogenous and laterally extensive aquifer, the average storage coefficient S is 2×10-4 and the average transmissivity T is 6×10-7 m2 using the measured phase and the amplitude response. Calculation for the hydraulic diffusivity D with D=T/S, yields the reported value of D is 3×10-3 m2/s, which is two orders of magnitude larger than pump test values on the Chelungpu Fault which is the site of the Mw 7.6 Chi-Chi earthquake. If the value is representative of the fault zone, then this means the hydrology processes should have an effect on the earthquake rupture process. This measurement is done through continuous monitoring and we could track the evolution for hydraulic properties

  3. Earthquake hazards to domestic water distribution systems in Salt Lake County, Utah

    USGS Publications Warehouse

    Highland, Lynn M.

    1985-01-01

    A magnitude-7. 5 earthquake occurring along the central portion of the Wasatch Fault, Utah, may cause significant damage to Salt Lake County's domestic water system. This system is composed of water treatment plants, aqueducts, distribution mains, and other facilities that are vulnerable to ground shaking, liquefaction, fault movement, and slope failures. Recent investigations into surface faulting, landslide potential, and earthquake intensity provide basic data for evaluating the potential earthquake hazards to water-distribution systems in the event of a large earthquake. Water supply system components may be vulnerable to one or more earthquake-related effects, depending on site geology and topography. Case studies of water-system damage by recent large earthquakes in Utah and in other regions of the United States offer valuable insights in evaluating water system vulnerability to earthquakes.

  4. Quasi-periodic recurrence of large earthquakes on the southern San Andreas fault

    USGS Publications Warehouse

    Scharer, Katherine M.; Biasi, Glenn P.; Weldon, Ray J.; Fumal, Tom E.

    2010-01-01

    It has been 153 yr since the last large earthquake on the southern San Andreas fault (California, United States), but the average interseismic interval is only ~100 yr. If the recurrence of large earthquakes is periodic, rather than random or clustered, the length of this period is notable and would generally increase the risk estimated in probabilistic seismic hazard analyses. Unfortunately, robust characterization of a distribution describing earthquake recurrence on a single fault is limited by the brevity of most earthquake records. Here we use statistical tests on a 3000 yr combined record of 29 ground-rupturing earthquakes from Wrightwood, California. We show that earthquake recurrence there is more regular than expected from a Poisson distribution and is not clustered, leading us to conclude that recurrence is quasi-periodic. The observation of unimodal time dependence is persistent across an observationally based sensitivity analysis that critically examines alternative interpretations of the geologic record. The results support formal forecast efforts that use renewal models to estimate probabilities of future earthquakes on the southern San Andreas fault. Only four intervals (15%) from the record are longer than the present open interval, highlighting the current hazard posed by this fault.

  5. Width of the Surface Rupture Zone for Thrust Earthquakes and Implications for Earthquake Fault Zoning: Chi-Chi 1999 and Wenchuan 2008 Earthquakes

    NASA Astrophysics Data System (ADS)

    Boncio, P.; Caldarella, M.

    2016-12-01

    We analyze the zones of coseismic surface faulting along thrust faults, whit the aim of defining the most appropriate criteria for zoning the Surface Fault Rupture Hazard (SFRH) along thrust faults. Normal and strike-slip faults were deeply studied in the past, while thrust faults were not studied with comparable attention. We analyze the 1999 Chi-Chi, Taiwan (Mw 7.6) and 2008 Wenchuan, China (Mw 7.9) earthquakes. Several different types of coseismic fault scarps characterize the two earthquakes, depending on the topography, fault geometry and near-surface materials. For both the earthquakes, we collected from the literature, or measured in GIS-georeferenced published maps, data about the Width of the coseismic Rupture Zone (WRZ). The frequency distribution of WRZ compared to the trace of the main fault shows that the surface ruptures occur mainly on and near the main fault. Ruptures located away from the main fault occur mainly in the hanging wall. Where structural complexities are present (e.g., sharp bends, step-overs), WRZ is wider then for simple fault traces. We also fitted the distribution of the WRZ dataset with probability density functions, in order to define a criterion to remove outliers (e.g., by selecting 90% or 95% probability) and define the zone where the probability of SFRH is the highest. This might help in sizing the zones of SFRH during seismic microzonation (SM) mapping. In order to shape zones of SFRH, a very detailed earthquake geologic study of the fault is necessary. In the absence of such a very detailed study, during basic (First level) SM mapping, a width of 350-400 m seems to be recommended (95% of probability). If the fault is carefully mapped (higher level SM), one must consider that the highest SFRH is concentrated in a narrow zone, 50 m-wide, that should be considered as a "fault-avoidance (or setback) zone". These fault zones should be asymmetric. The ratio of footwall to hanging wall (FW:HW) calculated here ranges from 1:5 to 1:3.

  6. Unexpected earthquake hazard revealed by Holocene rupture on the Kenchreai Fault (central Greece): Implications for weak sub-fault shear zones

    NASA Astrophysics Data System (ADS)

    Copley, Alex; Grützner, Christoph; Howell, Andy; Jackson, James; Penney, Camilla; Wimpenny, Sam

    2018-03-01

    High-resolution elevation models, palaeoseismic trenching, and Quaternary dating demonstrate that the Kenchreai Fault in the eastern Gulf of Corinth (Greece) has ruptured in the Holocene. Along with the adjacent Pisia and Heraion Faults (which ruptured in 1981), our results indicate the presence of closely-spaced and parallel normal faults that are simultaneously active, but at different rates. Such a configuration allows us to address one of the major questions in understanding the earthquake cycle, specifically what controls the distribution of interseismic strain accumulation? Our results imply that the interseismic loading and subsequent earthquakes on these faults are governed by weak shear zones in the underlying ductile crust. In addition, the identification of significant earthquake slip on a fault that does not dominate the late Quaternary geomorphology or vertical coastal motions in the region provides an important lesson in earthquake hazard assessment.

  7. Probing failure susceptibilities of earthquake faults using small-quake tidal correlations.

    PubMed

    Brinkman, Braden A W; LeBlanc, Michael; Ben-Zion, Yehuda; Uhl, Jonathan T; Dahmen, Karin A

    2015-01-27

    Mitigating the devastating economic and humanitarian impact of large earthquakes requires signals for forecasting seismic events. Daily tide stresses were previously thought to be insufficient for use as such a signal. Recently, however, they have been found to correlate significantly with small earthquakes, just before large earthquakes occur. Here we present a simple earthquake model to investigate whether correlations between daily tidal stresses and small earthquakes provide information about the likelihood of impending large earthquakes. The model predicts that intervals of significant correlations between small earthquakes and ongoing low-amplitude periodic stresses indicate increased fault susceptibility to large earthquake generation. The results agree with the recent observations of large earthquakes preceded by time periods of significant correlations between smaller events and daily tide stresses. We anticipate that incorporating experimentally determined parameters and fault-specific details into the model may provide new tools for extracting improved probabilities of impending large earthquakes.

  8. Fault interaction and stress triggering of twentieth century earthquakes in Mongolia

    USGS Publications Warehouse

    Pollitz, F.; Vergnolle, M.; Calais, E.

    2003-01-01

    A cluster of exceptionally large earthquakes in the interior of Asia occurred from 1905 to 1967: the 1905 M7.9 Tsetserleg and M8.4 Bolnai earthquakes, the 1931 M8.0 Fu Yun earthquake, the 1957 M8.1 Gobi-Altai earthquake, and the 1967 M7.1 Mogod earthquake (sequence). Each of the larger (M ??? 8) earthquakes involved strike-slip faulting averaging more than 5 m and rupture lengths of several hundred kilometers. Available geologic data indicate that recurrence intervals on the major source faults are several thousands of years and distances of about 400 km separate the respective rupture areas. We propose that the occurrences of these and many smaller earthquakes are related and controlled to a large extent by stress changes generated by the compounded static deformation of the preceding earthquakes and subsequent viscoelastic relaxation of the lower crust and upper mantle beneath Mongolia. We employ a spherically layered viscoelastic model constrained by the 1994-2002 GPS velocity field in western Mongolia [Vergnolle et al., 2003]. Using the succession of twentieth century earthquakes as sources of deformation, we then analyze the time-dependent change in Coulomb failure stress (????f). At remote interaction distances, static ????f values are small. However, modeled postseismic stress changes typically accumulate to several tenths of a bar over time intervals of decades. Almost all significant twentieth century regional earthquakes (M ??? 6) with well-constrained fault geometry lie in positive ????f lobes of magnitude about +0.5 bar. Our results suggest that significant stress transfer is possible among continental faults separated by hundreds of kilometers and on timescales of decades. Copyright 2003 by the American Geophysical Union.

  9. Earthquake cycle modeling of multi-segmented faults: dynamic rupture and ground motion simulation of the 1992 Mw 7.3 Landers earthquake.

    NASA Astrophysics Data System (ADS)

    Petukhin, A.; Galvez, P.; Somerville, P.; Ampuero, J. P.

    2017-12-01

    We perform earthquake cycle simulations to study the characteristics of source scaling relations and strong ground motions and in multi-segmented fault ruptures. For earthquake cycle modeling, a quasi-dynamic solver (QDYN, Luo et al, 2016) is used to nucleate events and the fully dynamic solver (SPECFEM3D, Galvez et al., 2014, 2016) is used to simulate earthquake ruptures. The Mw 7.3 Landers earthquake has been chosen as a target earthquake to validate our methodology. The SCEC fault geometry for the three-segmented Landers rupture is included and extended at both ends to a total length of 200 km. We followed the 2-D spatial correlated Dc distributions based on Hillers et. al. (2007) that associates Dc distribution with different degrees of fault maturity. The fault maturity is related to the variability of Dc on a microscopic scale. Large variations of Dc represents immature faults and lower variations of Dc represents mature faults. Moreover we impose a taper (a-b) at the fault edges and limit the fault depth to 15 km. Using these settings, earthquake cycle simulations are performed to nucleate seismic events on different sections of the fault, and dynamic rupture modeling is used to propagate the ruptures. The fault segmentation brings complexity into the rupture process. For instance, the change of strike between fault segments enhances strong variations of stress. In fact, Oglesby and Mai (2012) show the normal stress varies from positive (clamping) to negative (unclamping) between fault segments, which leads to favorable or unfavorable conditions for rupture growth. To replicate these complexities and the effect of fault segmentation in the rupture process, we perform earthquake cycles with dynamic rupture modeling and generate events similar to the Mw 7.3 Landers earthquake. We extract the asperities of these events and analyze the scaling relations between rupture area, average slip and combined area of asperities versus moment magnitude. Finally, the

  10. Characterizing the structural maturity of fault zones using high-resolution earthquake locations.

    NASA Astrophysics Data System (ADS)

    Perrin, C.; Waldhauser, F.; Scholz, C. H.

    2017-12-01

    We use high-resolution earthquake locations to characterize the three-dimensional structure of active faults in California and how it evolves with fault structural maturity. We investigate the distribution of aftershocks of several recent large earthquakes that occurred on immature faults (i.e., slow moving and small cumulative displacement), such as the 1992 (Mw7.3) Landers and 1999 (Mw7.1) Hector Mine events, and earthquakes that occurred on mature faults, such as the 1984 (Mw6.2) Morgan Hill and 2004 (Mw6.0) Parkfield events. Unlike previous studies which typically estimated the width of fault zones from the distribution of earthquakes perpendicular to the surface fault trace, we resolve fault zone widths with respect to the 3D fault surface estimated from principal component analysis of local seismicity. We find that the zone of brittle deformation around the fault core is narrower along mature faults compared to immature faults. We observe a rapid fall off of the number of events at a distance range of 70 - 100 m from the main fault surface of mature faults (140-200 m fault zone width), and 200-300 m from the fault surface of immature faults (400-600 m fault zone width). These observations are in good agreement with fault zone widths estimated from guided waves trapped in low velocity damage zones. The total width of the active zone of deformation surrounding the main fault plane reach 1.2 km and 2-4 km for mature and immature faults, respectively. The wider zone of deformation presumably reflects the increased heterogeneity in the stress field along complex and discontinuous faults strands that make up immature faults. In contrast, narrower deformation zones tend to align with well-defined fault planes of mature faults where most of the deformation is concentrated. Our results are in line with previous studies suggesting that surface fault traces become smoother, and thus fault zones simpler, as cumulative fault slip increases.

  11. Fault Branching and Long-Term Earthquake Rupture Scenario for Strike-Slip Earthquake

    NASA Astrophysics Data System (ADS)

    Klinger, Y.; CHOI, J. H.; Vallage, A.

    2017-12-01

    Careful examination of surface rupture for large continental strike-slip earthquakes reveals that for the majority of earthquakes, at least one major branch is involved in the rupture pattern. Often, branching might be either related to the location of the epicenter or located toward the end of the rupture, and possibly related to the stopping of the rupture. In this work, we examine large continental earthquakes that show significant branches at different scales and for which ground surface rupture has been mapped in great details. In each case, rupture conditions are described, including dynamic parameters, past earthquakes history, and regional stress orientation, to see if the dynamic stress field would a priori favor branching. In one case we show that rupture propagation and branching are directly impacted by preexisting geological structures. These structures serve as pathways for the rupture attempting to propagate out of its shear plane. At larger scale, we show that in some cases, rupturing a branch might be systematic, hampering possibilities for the development of a larger seismic rupture. Long-term geomorphology hints at the existence of a strong asperity in the zone where the rupture branched off the main fault. There, no evidence of throughgoing rupture could be seen along the main fault, while the branch is well connected to the main fault. This set of observations suggests that for specific configurations, some rupture scenarios involving systematic branching are more likely than others.

  12. Using focal mechanism solutions to correlate earthquakes with faults in the Lake Tahoe-Truckee area, California and Nevada, and to help design LiDAR surveys for active-fault reconnaissance

    NASA Astrophysics Data System (ADS)

    Cronin, V. S.; Lindsay, R. D.

    2011-12-01

    Geomorphic analysis of hillshade images produced from aerial LiDAR data has been successful in identifying youthful fault traces. For example, the recently discovered Polaris fault just northwest of Lake Tahoe, California/Nevada, was recognized using LiDAR data that had been acquired by local government to assist land-use planning. Subsequent trenching by consultants under contract to the US Army Corps of Engineers has demonstrated Holocene displacement. The Polaris fault is inferred to be capable of generating a magnitude 6.4-6.9 earthquake, based on its apparent length and offset characteristics (Hunter and others, 2011, BSSA 101[3], 1162-1181). Dingler and others (2009, GSA Bull 121[7/8], 1089-1107) describe paleoseismic or geomorphic evidence for late Neogene displacement along other faults in the area, including the West Tahoe-Dollar Point, Stateline-North Tahoe, and Incline Village faults. We have used the seismo-lineament analysis method (SLAM; Cronin and others, 2008, Env Eng Geol 14[3], 199-219) to establish a tentative spatial correlation between each of the previously mentioned faults, as well as with segments of the Dog Valley fault system, and one or more earthquake(s). The ~18 earthquakes we have tentatively correlated with faults in the Tahoe-Truckee area occurred between 1966 and 2008, with magnitudes between 3 and ~6. Given the focal mechanism solution for a well-located shallow-focus earthquake, the nodal planes can be projected to Earth's surface as represented by a DEM, plus-or-minus the vertical and horizontal uncertainty in the focal location, to yield two seismo-lineament swaths. The trace of the fault that generated the earthquake is likely to be found within one of the two swaths [1] if the fault surface is emergent, and [2] if the fault surface is approximately planar in the vicinity of the focus. Seismo-lineaments from several of the earthquakes studied overlap in a manner that suggests they are associated with the same fault. The surface

  13. Fluid-faulting interactions: Fracture-mesh and fault-valve behavior in the February 2014 Mammoth Mountain, California, earthquake swarm

    USGS Publications Warehouse

    Shelly, David R.; Taira, Taka’aki; Prejean, Stephanie; Hill, David P.; Dreger, Douglas S.

    2015-01-01

    Faulting and fluid transport in the subsurface are highly coupled processes, which may manifest seismically as earthquake swarms. A swarm in February 2014 beneath densely monitored Mammoth Mountain, California, provides an opportunity to witness these interactions in high resolution. Toward this goal, we employ massive waveform-correlation-based event detection and relative relocation, which quadruples the swarm catalog to more than 6000 earthquakes and produces high-precision locations even for very small events. The swarm's main seismic zone forms a distributed fracture mesh, with individual faults activated in short earthquake bursts. The largest event of the sequence, M 3.1, apparently acted as a fault valve and was followed by a distinct wave of earthquakes propagating ~1 km westward from the updip edge of rupture, 1–2 h later. Late in the swarm, multiple small, shallower subsidiary faults activated with pronounced hypocenter migration, suggesting that a broader fluid pressure pulse propagated through the subsurface.

  14. Fault structure and mechanics of the Hayward Fault, California from double-difference earthquake locations

    USGS Publications Warehouse

    Waldhauser, F.; Ellsworth, W.L.

    2002-01-01

    The relationship between small-magnitude seismicity and large-scale crustal faulting along the Hayward Fault, California, is investigated using a double-difference (DD) earthquake location algorithm. We used the DD method to determine high-resolution hypocenter locations of the seismicity that occurred between 1967 and 1998. The DD technique incorporates catalog travel time data and relative P and S wave arrival time measurements from waveform cross correlation to solve for the hypocentral separation between events. The relocated seismicity reveals a narrow, near-vertical fault zone at most locations. This zone follows the Hayward Fault along its northern half and then diverges from it to the east near San Leandro, forming the Mission trend. The relocated seismicity is consistent with the idea that slip from the Calaveras Fault is transferred over the Mission trend onto the northern Hayward Fault. The Mission trend is not clearly associated with any mapped active fault as it continues to the south and joins the Calaveras Fault at Calaveras Reservoir. In some locations, discrete structures adjacent to the main trace are seen, features that were previously hidden in the uncertainty of the network locations. The fine structure of the seismicity suggest that the fault surface on the northern Hayward Fault is curved or that the events occur on several substructures. Near San Leandro, where the more westerly striking trend of the Mission seismicity intersects with the surface trace of the (aseismic) southern Hayward Fault, the seismicity remains diffuse after relocation, with strong variation in focal mechanisms between adjacent events indicating a highly fractured zone of deformation. The seismicity is highly organized in space, especially on the northern Hayward Fault, where it forms horizontal, slip-parallel streaks of hypocenters of only a few tens of meters width, bounded by areas almost absent of seismic activity. During the interval from 1984 to 1998, when digital

  15. The response of creeping parts of the San Andreas fault to earthquakes on nearby faults: Two examples

    USGS Publications Warehouse

    Simpson, R.W.; Schulz, S.S.; Dietz, L.D.; Burford, R.O.

    1988-01-01

    Rates of shallow slip on creeping sections of the San Andreas fault have been perturbed on a number of occasions by earthquakes occurring on nearby faults. One example of such perturbations occurred during the 26 January 1986 magnitude 5.3 Tres Pinos earthquake located about 10 km southeast of Hollister, California. Seven creepmeters on the San Andreas fault showed creep steps either during or soon after the shock. Both left-lateral (LL) and right-lateral (RL) steps were observed. A rectangular dislocation in an elastic half-space was used to model the coseismic fault offset at the hypocenter. For a model based on the preliminary focal mechanism, the predicted changes in static shear stress on the plane of the San Andreas fault agreed in sense (LL or RL) with the observed slip directions at all seven meters; for a model based on a refined focal mechanism, six of the seven meters showed the correct sense of motion. Two possible explanations for such coseismic and postseismic steps are (1) that slip was triggered by the earthquake shaking or (2) that slip occurred in response to the changes in static stress fields accompanying the earthquake. In the Tres Pinos example, the observed steps may have been of both the triggered and responsive kinds. A second example is provided by the 2 May 1983 magnitude 6.7 Coalinga earthquake, which profoundly altered slip rates at five creepmeters on the San Andreas fault for a period of months to years. The XMM1 meter 9 km northwest of Parkfield, California recorded LL creep for more than a year after the event. To simulate the temporal behavior of the XMM1 meter and to view the stress perturbation provided by the Coalinga earthquake in the context of steady-state deformation on the San Andreas fault, a simple time-evolving dislocation model was constructed. The model was driven by a single long vertical dislocation below 15 km in depth, that was forced to slip at 35 mm/yr in a RL sense. A dislocation element placed in the

  16. Break of slope in earthquake size distribution and creep rate along the San Andreas Fault system

    NASA Astrophysics Data System (ADS)

    Shebalin, P.; Narteau, C.; Vorobieva, I.

    2017-12-01

    Crustal faults accommodate slip either by a succession of earthquakes or continuous slip, andin most instances, both these seismic and aseismic processes coexist. Recorded seismicity and geodeticmeasurements are therefore two complementary data sets that together document ongoing deformationalong active tectonic structures. Here we study the influence of stable sliding on earthquake statistics.We show that creep along the San Andreas Fault is responsible for a break of slope in the earthquake sizedistribution. This slope increases with an increasing creep rate for larger magnitude ranges, whereas itshows no systematic dependence on creep rate for smaller magnitude ranges. This is interpreted as a deficitof large events under conditions of faster creep where seismic ruptures are less likely to propagate. Theseresults suggest that the earthquake size distribution does not only depend on the level of stress but also onthe type of deformation.

  17. Modeling Crustal Deformation Due to the Landers, Hector Mine Earthquakes Using the SCEC Community Fault Model

    NASA Astrophysics Data System (ADS)

    Gable, C. W.; Fialko, Y.; Hager, B. H.; Plesch, A.; Williams, C. A.

    2006-12-01

    More realistic models of crustal deformation are possible due to advances in measurements and modeling capabilities. This study integrates various data to constrain a finite element model of stress and strain in the vicinity of the 1992 Landers earthquake and the 1999 Hector Mine earthquake. The geometry of the model is designed to incorporate the Southern California Earthquake Center (SCEC), Community Fault Model (CFM) to define fault geometry. The Hector Mine fault is represented by a single surface that follows the trace of the Hector Mine fault, is vertical and has variable depth. The fault associated with the Landers earthquake is a set of seven surfaces that capture the geometry of the splays and echelon offsets of the fault. A three dimensional finite element mesh of tetrahedral elements is built that closely maintains the geometry of these fault surfaces. The spatially variable coseismic slip on faults is prescribed based on an inversion of geodetic (Synthetic Aperture Radar and Global Positioning System) data. Time integration of stress and strain is modeled with the finite element code Pylith. As a first step the methodology of incorporating all these data is described. Results of the time history of the stress and strain transfer between 1992 and 1999 are analyzed as well as the time history of deformation from 1999 to the present.

  18. Simulate earthquake cycles on the oceanic transform faults in the framework of rate-and-state friction

    NASA Astrophysics Data System (ADS)

    Wei, M.

    2016-12-01

    Progress towards a quantitative and predictive understanding of the earthquake behavior can be achieved by improved understanding of earthquake cycles. However, it is hindered by the long repeat times (100s to 1000s of years) of the largest earthquakes on most faults. At fast-spreading oceanic transform faults, the typical repeating time ranges from 5-20 years, making them a unique tectonic environment for studying the earthquake cycle. One important observation on OTFs is the quasi-periodicity and the spatial-temporal clustering of large earthquakes: same fault segment ruptured repeatedly at a near constant interval and nearby segments ruptured during a short time period. This has been observed on the Gofar and Discovery faults in the East Pacific Rise. Between 1992 and 2014, five clusters of M6 earthquakes occurred on the Gofar and Discovery fault system with recurrence intervals of 4-6 years. Each cluster consisted of a westward migration of seismicity from the Discovery to Gofar segment within a 2-year period, providing strong evidence for spatial-temporal clustering of large OTFs earthquakes. I simulated earthquake cycles of oceanic transform fault in the framework of rate-and-state friction, motivated by the observations at the Gofar and Discovery faults. I focus on a model with two seismic segments, each 20 km long and 5 km wide, separated by an aseismic segment of 10 km wide. This geometry is set based on aftershock locations of the 2008 M6.0 earthquake on Gofar. The repeating large earthquake on both segments are reproduced with similar magnitude as observed. I set the state parameter differently for the two seismic segments so initially they are not synchornized. Results also show that synchronization of the two seismic patches can be achieved after several earthquake cycles when the effective normal stress or the a-b parameter is smaller than surrounding aseismic areas, both having reduced the resistance to seismic rupture in the VS segment. These

  19. Transfer fault earthquake in compressionally reactivated back-arc failed rift: 1948 Fukui earthquake (M7.1), Japan

    NASA Astrophysics Data System (ADS)

    Ishiyama, Tatsuya; Kato, Naoko; Sato, Hiroshi; Koshiya, Shin

    2017-04-01

    Back-arc rift structures in many subduction zones are recognized as mechanically and thermally weak zones that possibly play important roles in strain accommodation at later post-rift stages within the overriding plates. In case of Miocene back-arc failed rift structures in the Sea of Japan in the Eurasian-Pacific subduction system, the mechanical contrasts between the crustal thrust wedges of the pre-rift continental crust and high velocity lower crust have fundamentally controlled the styles of post-rift, Quaternary active deformation (Ishiyama et al. 2016). In this study, we show a possibility that strike-slip M>7 devastating earthquakes in this region have been gregion enerated by reactivation of transfer faults highly oblique to the rift axes. The 1948 Fukui earthquake (M7.1), onshore shallow seismic event with a strike-slip faulting mechanism (Kanamori, 1973), resulted in more than 3,500 causalities and destructive damages on the infrastructures. While geophysical analyses on geodetic measurements based on leveling and triangulation networks clearly show coseismic left-lateral fault slip on a NNW striking vertical fault plane beneath the Fukui plain (Sagiya, 1999), no evidence for coseismic surface rupture has been identified based on both post-earthquake intensive fieldwork and recent reexamination of stereopair interpretations using 1/3,000 aerial photographs taken in 1948 (Togo et al., 2000). To find recognizable fault-related structures that deform Neogene basin fill sediments, we collected new 9.6-km-long high-resolution seismic reflection data across the geodetically estimated fault plane and adjacent subparallel active strike slip faults, using 925 offline recorders and Envirovib truck as a seismic source. A depth-converted section to 1.5 km depth contains discontinuous seismic reflectors correlated to Miocene volcaniclastic deposits and depression of the overlying Plio-Pleistocene sediments above the geodetically determined fault plane. We interpreted

  20. Earthquakes and aseismic creep associated with growing fault-related folds

    NASA Astrophysics Data System (ADS)

    Burke, C. C.; Johnson, K. M.

    2017-12-01

    Blind thrust faults overlain by growing anticlinal folds pose a seismic risk to many urban centers in the world. A large body of research has focused on using fold and growth strata geometry to infer the rate of slip on the causative fault and the distribution of off-fault deformation. However, because we have had few recorded large earthquakes on blind faults underlying folds, it remains unclear how much of the folding occurs during large earthquakes or during the interseismic period accommodated by aseismic creep. Numerous kinematic and mechanical models as well as field observations demonstrate that flexural slip between sedimentary layering is an important mechanism of fault-related folding. In this study, we run boundary element models of flexural-slip fault-related folding to examine the extent to which energy is released seismically or aseismically throughout the evolution of the fold and fault. We assume a fault imbedded in viscoelastic mechanical layering under frictional contact. We assign depth-dependent frictional properties and adopt a rate-state friction formulation to simulate slip over time. We find that in many cases, a large percentage (greater than 50%) of fold growth is accomplished by aseismic creep at bedding and fault contacts. The largest earthquakes tend to occur on the fault, but a significant portion of the seismicity is distributed across bedding contacts through the fold. We are currently working to quantify these results using a large number of simulations with various fold and fault geometries. Result outputs include location, duration, and magnitude of events. As more simulations are completed, these results from different fold and fault geometries will provide insight into how much folding occurs from these slip events. Generalizations from these simulations can be compared with observations of active fault-related folds and used in the future to inform seismic hazard studies.

  1. Finite element models of earthquake cycles in mature strike-slip fault zones

    NASA Astrophysics Data System (ADS)

    Lynch, John Charles

    The research presented in this dissertation is on the subject of strike-slip earthquakes and the stresses that build and release in the Earth's crust during earthquake cycles. Numerical models of these cycles in a layered elastic/viscoelastic crust are produced using the finite element method. A fault that alternately sticks and slips poses a particularly challenging problem for numerical implementation, and a new contact element dubbed the "Velcro" element was developed to address this problem (Appendix A). Additionally, the finite element code used in this study was bench-marked against analytical solutions for some simplified problems (Chapter 2), and the resolving power was tested for the fault region of the models (Appendix B). With the modeling method thus developed, there are two main questions posed. First, in Chapter 3, the effect of a finite-width shear zone is considered. By defining a viscoelastic shear zone beneath a periodically slipping fault, it is found that shear stress concentrates at the edges of the shear zone and thus causes the stress tensor to rotate into non-Andersonian orientations. Several methods are used to examine the stress patterns, including the plunge angles of the principal stresses and a new method that plots the stress tensor in a manner analogous to seismic focal mechanism diagrams. In Chapter 4, a simple San Andreas-like model is constructed, consisting of two great earthquake producing faults separated by a freely-slipping shorter fault. The model inputs of lower crustal viscosity, fault separation distance, and relative breaking strengths are examined for their effect on fault communication. It is found that with a lower crustal viscosity of 1018 Pa s (in the lower range of estimates for California), the two faults tend to synchronize their earthquake cycles, even in the cases where the faults have asymmetric breaking strengths. These models imply that postseismic stress transfer over hundreds of kilometers may play a

  2. Kinematics, mechanics, and potential earthquake hazards for faults in Pottawatomie County, Kansas, USA

    USGS Publications Warehouse

    Ohlmacher, G.C.; Berendsen, P.

    2005-01-01

    Many stable continental regions have subregions with poorly defined earthquake hazards. Analysis of minor structures (folds and faults) in these subregions can improve our understanding of the tectonics and earthquake hazards. Detailed structural mapping in Pottawatomie County has revealed a suite consisting of two uplifted blocks aligned along a northeast trend and surrounded by faults. The first uplift is located southwest of the second. The northwest and southeast sides of these uplifts are bounded by northeast-trending right-lateral faults. To the east, both uplifts are bounded by north-trending reverse faults, and the first uplift is bounded by a north-trending high-angle fault to the west. The structural suite occurs above a basement fault that is part of a series of north-northeast-trending faults that delineate the Humboldt Fault Zone of eastern Kansas, an integral part of the Midcontinent Rift System. The favored kinematic model is a contractional stepover (push-up) between echelon strike-slip faults. Mechanical modeling using the boundary element method supports the interpretation of the uplifts as contractional stepovers and indicates that an approximately east-northeast maximum compressive stress trajectory is responsible for the formation of the structural suite. This stress trajectory suggests potential activity during the Laramide Orogeny, which agrees with the age of kimberlite emplacement in adjacent Riley County. The current stress field in Kansas has a N85??W maximum compressive stress trajectory that could potentially produce earthquakes along the basement faults. Several epicenters of seismic events (faults, is similar to that mapped in the New Madrid Seismic Zone, and both areas currently feature roughly east-west maximum

  3. Seismicity in the source areas of the 1896 and 1933 Sanriku earthquakes and implications for large near-trench earthquake faults

    NASA Astrophysics Data System (ADS)

    Obana, Koichiro; Nakamura, Yasuyuki; Fujie, Gou; Kodaira, Shuichi; Kaiho, Yuka; Yamamoto, Yojiro; Miura, Seiichi

    2018-03-01

    In the northern part of the Japan Trench, the 1933 Showa-Sanriku earthquake (Mw 8.4), an outer-trench, normal-faulting earthquake, occurred 37 yr after the 1896 Meiji-Sanriku tsunami earthquake (Mw 8.0), a shallow, near-trench, plate-interface rupture. Tsunamis generated by both earthquakes caused severe damage along the Sanriku coast. Precise locations of earthquakes in the source areas of the 1896 and 1933 earthquakes have not previously been obtained because they occurred at considerable distances from the coast in deep water beyond the maximum operational depth of conventional ocean bottom seismographs (OBSs). In 2015, we incorporated OBSs designed for operation in deep water (ultradeep OBSs) in an OBS array during two months of seismic observations in the source areas of the 1896 and 1933 Sanriku earthquakes to investigate the relationship of seismicity there to outer-rise normal-faulting earthquakes and near-trench tsunami earthquakes. Our analysis showed that seismicity during our observation period occurred along three roughly linear trench-parallel trends in the outer-trench region. Seismic activity along these trends likely corresponds to aftershocks of the 1933 Showa-Sanriku earthquake and the Mw 7.4 normal-faulting earthquake that occurred 40 min after the 2011 Tohoku-Oki earthquake. Furthermore, changes of the clarity of reflections from the oceanic Moho on seismic reflection profiles and low-velocity anomalies within the oceanic mantle were observed near the linear trends of the seismicity. The focal mechanisms we determined indicate that an extensional stress regime extends to about 40 km depth, below which the stress regime is compressional. These observations suggest that rupture during the 1933 Showa-Sanriku earthquake did not extend to the base of the oceanic lithosphere and that compound rupture of multiple or segmented faults is a more plausible explanation for that earthquake. The source area of the 1896 Meiji-Sanriku tsunami earthquake is

  4. The Hayward-Rodgers Creek Fault System: Learning from the Past to Forecast the Future

    NASA Astrophysics Data System (ADS)

    Schwartz, D. P.; Lienkaemper, J. J.; Hecker, S.

    2007-12-01

    The San Francisco Bay area is located within the Pacific-North American plate boundary. As a result, the region has the highest density of active faults per square kilometer of any urban center in the US. Between the Farallon Islands and Livermore, the faults of the San Andreas fault system are slipping at a rate of about 40 mm/yr. Approximately 25 percent of this rate is accommodated by the Hayward fault and its continuation to the north, the Rodgers Creek fault. The Hayward fault extends 88 km from Warm Springs on the south into San Pablo Bay on the north, traversing the most heavily urbanized part of the Bay Area. The Rodgers Creek fault extends another 63 km, passing through Santa Rosa and ending south of Healdsburg. Geologic, seismologic, and geodetic studies during the past ten years have significantly increased our knowledge of this system. In particular, paleoseismic studies of the timing of past earthquakes have provided critical new information for improving our understanding of how these faults may work in time and space, and for estimating the probability of future earthquakes. The most spectacular result is an 11-earthquake record on the southern Hayward fault that extends back to A.D. 170. It suggests an average time interval between large earthquakes of 170 years for this period, with a shorter interval of 140 years for the five most recent earthquakes. Paleoseismic investigations have also shown that prior to the most recent large earthquake on the southern Hayward fault in 1868, large earthquakes occurred on the southern Hayward fault between 1658 and1786, on the northern Hayward fault between 1640 and 1776, and on the Rodgers Creek fault between 1690 and 1776. These could have been three separate earthquakes. However, the overlapping radiocarbon dates for these paleoearthquakes allow the possibility that these faults may have ruptured together in several different combinations: a combined southern and northern Hayward fault earthquake, a Rodgers

  5. Identification of repeating earthquakes and spatio-temporal variations of fault zone properties around the Parkfield section of the San Andreas fault and the central Calaveras fault

    NASA Astrophysics Data System (ADS)

    Zhao, P.; Peng, Z.

    2008-12-01

    We systemically identify repeating earthquakes and investigate spatio-temporal variations of fault zone properties associated with the 2004 Mw6.0 Parkfield earthquake along the Parkfield section of the San Andreas fault, and the 1984 Mw6.2 Morgan Hill earthquake along the central Calaveras fault. The procedure for identifying repeating earthquakes is based on overlapping of the source regions and the waveform similarity, and is briefly described as follows. First, we estimate the source radius of each event based on a circular crack model and a normal stress drop of 3 MPa. Next, we compute inter-hypocentral distance for events listed in the relocated catalog of Thurber et al. (2006) around Parkfield, and Schaff et al. (2002) along the Calaveras fault. Then, we group all events into 'initial' clusters by requiring the separation distance between each event pair to be less than the source radius of larger event, and their magnitude difference to be less than 1. Next, we calculate the correlation coefficients between every event pair within each 'initial' cluster using a 3-s time window around the direct P waves for all available stations. The median value of the correlation coefficients is used as a measure of similarity between each event pair. We drop an event if the median similarity to the rest events in that cluster is less than 0.9. After identifying repeating clusters in both regions, our next step is to apply a sliding window waveform cross-correlation technique (Niu et al., 2003; Peng and Ben-Zion, 2006) to calculate the delay time and decorrelation index for each repeating cluster. By measuring temporal changes in waveforms of repeating clusters at different locations and depth, we hope to obtain a better constraint on spatio-temporal variations of fault zone properties and near-surface layers associated with the occurrence of major earthquakes.

  6. Foreshock sequences and short-term earthquake predictability on East Pacific Rise transform faults.

    PubMed

    McGuire, Jeffrey J; Boettcher, Margaret S; Jordan, Thomas H

    2005-03-24

    East Pacific Rise transform faults are characterized by high slip rates (more than ten centimetres a year), predominantly aseismic slip and maximum earthquake magnitudes of about 6.5. Using recordings from a hydroacoustic array deployed by the National Oceanic and Atmospheric Administration, we show here that East Pacific Rise transform faults also have a low number of aftershocks and high foreshock rates compared to continental strike-slip faults. The high ratio of foreshocks to aftershocks implies that such transform-fault seismicity cannot be explained by seismic triggering models in which there is no fundamental distinction between foreshocks, mainshocks and aftershocks. The foreshock sequences on East Pacific Rise transform faults can be used to predict (retrospectively) earthquakes of magnitude 5.4 or greater, in narrow spatial and temporal windows and with a high probability gain. The predictability of such transform earthquakes is consistent with a model in which slow slip transients trigger earthquakes, enrich their low-frequency radiation and accommodate much of the aseismic plate motion.

  7. Intra-caldera active fault: An example from the Mw 7.0 2016 Kumamoto, Japan, earthquake

    NASA Astrophysics Data System (ADS)

    Toda, S.; Murakami, T.; Takahashi, N.

    2017-12-01

    A NE-trending 30-km-long surface rupture with up to 2.4 m dextral slip emerged during the Mw=7.0 16 April 2016 Kumamoto earthquake along the previously mapped Futagawa and northern Hinagu fault systems. The 5-km-long portion of the northeast rupture end, which was previously unidentified, crossed somma and extended to the 20-km-diameter Aso Caldera, one of the major active volcanoes, central Kyushu. We here explore geologic exposures of interplays of active faulting and active volcanism, and then argue the Futagawa fault system has been influenced by the ring fault system associated with the caldera forming gigantic eruptions since 270 ka, last of which occurred 90 ka ejecting a huge amount of ignimbrite. To understand the interplays, together with the mapping of the 2016 rupture, we employed an UAV to capture numerous photos of the exposures along the canyon and developed 3D orthochromatic topographic model using PhotoScan. One-hundred-meter-deep Kurokawa River canyon by the Aso Caldera rim exposes two lava flow units of 50 ka vertically offset by 10 m by the Futatawa fault system. Reconstructions of the collapsed bridges across the Kurokawa River also reveal cross sections of a 30-meter-high tectonic bulge and 10-m-scale negative flower structure deformed by the frequent fault movements. We speculate two fault developing models across the Aso Caldera. One is that the NE edge of the Futagawa fault system was cut and reset by the caldera forming ring fault, which indicates the 3-km-long rupture extent within the Aso Caldera would be a product of the fault growth since the last Aso-4 eruption of 90 ka. It enables us to estimate the 33 mm/yr of the fault propagation speed. An alternative model is that subsurface rupture of the Kumamoto earthquake extended further to the NE rim, the other side of the caldera edge, which is partially supported by the geodetic and seismic inversions. With respect to the model, the clear surface rupture of the 2016 Kumamoto earthquake

  8. Earthquake imprints on a lacustrine deltaic system: the Kürk Delta along the East Anatolian Fault (Turkey)

    NASA Astrophysics Data System (ADS)

    Hubert-Ferrari, Aurélia; El-Ouahabi, Meriam; Garcia-Moreno, David; Avsar, Ulas; Altinok, Sevgi; Schmidt, Sabine; Cagatay, Namik

    2016-04-01

    Delta contains a sedimentary record primarily indicative of water level changes, but particularly sensitive to earthquake shaking, which results generally in soft-sediment-deformation structures. The Kürk Delta adjacent to a major strike-slip fault displays this type of deformation (Hempton and Dewey, 1983) as well as other types of earthquake fingerprints that are specifically investigated. This lacustrine delta stands at the south-western extremity of the Hazar Lake and is bound by the East Anatolian Fault (EAF), which generated earthquakes of magnitude 7 in eastern Turkey. Water level changes and earthquake shaking affecting the Kurk Delta have been reevaluated combining geophysical data (seismic-reflection profiles and side-scan sonar), remote sensing images, historical data, onland outcrops and offshore coring. The history of water level changes provides a temporal framework regarding the sedimentological record. In addition to the commonly soft-sediment-deformation previously documented, the onland outcrops reveal a record of deformation (faults and clastic dykes) linked to large earthquake-induced liquefactions. The recurrent liquefaction structures can be used to obtain a paleoseismological record. Five event horizons were identified that could be linked to historical earthquakes occurring in the last 1000 years along the EAF. Sedimentary cores sampling the most recent subaqueous sedimentation revealed the occurrence of another type of earthquake fingerprint. Based on radionuclide dating (137Cs and 210Pb), two major sedimentary events were attributed to the 1874-1875 earthquake sequence along the EAF. Their sedimentological characteristics were inferred based X-ray imagery, XRD, LOI, grain-size distribution, geophysical measurements. The events are interpreted to be hyperpycnal deposits linked to post-seismic sediment reworking of earthquake-triggered landslides. A time constraint regarding this sediment remobilization process could be achieved thanks to

  9. Thermodynamic method for generating random stress distributions on an earthquake fault

    USGS Publications Warehouse

    Barall, Michael; Harris, Ruth A.

    2012-01-01

    This report presents a new method for generating random stress distributions on an earthquake fault, suitable for use as initial conditions in a dynamic rupture simulation. The method employs concepts from thermodynamics and statistical mechanics. A pattern of fault slip is considered to be analogous to a micro-state of a thermodynamic system. The energy of the micro-state is taken to be the elastic energy stored in the surrounding medium. Then, the Boltzmann distribution gives the probability of a given pattern of fault slip and stress. We show how to decompose the system into independent degrees of freedom, which makes it computationally feasible to select a random state. However, due to the equipartition theorem, straightforward application of the Boltzmann distribution leads to a divergence which predicts infinite stress. To avoid equipartition, we show that the finite strength of the fault acts to restrict the possible states of the system. By analyzing a set of earthquake scaling relations, we derive a new formula for the expected power spectral density of the stress distribution, which allows us to construct a computer algorithm free of infinities. We then present a new technique for controlling the extent of the rupture by generating a random stress distribution thousands of times larger than the fault surface, and selecting a portion which, by chance, has a positive stress perturbation of the desired size. Finally, we present a new two-stage nucleation method that combines a small zone of forced rupture with a larger zone of reduced fracture energy.

  10. Spatiotemporal earthquake clusters along the North Anatolian fault zone offshore Istanbul

    USGS Publications Warehouse

    Bulut, Fatih; Ellsworth, William L.; Bohnhoff, Marco; Aktar, Mustafa; Dresen, Georg

    2011-01-01

    We investigate earthquakes with similar waveforms in order to characterize spatiotemporal microseismicity clusters within the North Anatolian fault zone (NAFZ) in northwest Turkey along the transition between the 1999 ??zmit rupture zone and the Marmara Sea seismic gap. Earthquakes within distinct activity clusters are relocated with cross-correlation derived relative travel times using the double difference method. The spatiotemporal distribution of micro earthquakes within individual clusters is resolved with relative location accuracy comparable to or better than the source size. High-precision relative hypocenters define the geometry of individual fault patches, permitting a better understanding of fault kinematics and their role in local-scale seismotectonics along the region of interest. Temporal seismic sequences observed in the eastern Sea of Marmara region suggest progressive failure of mostly nonoverlapping areas on adjacent fault patches and systematic migration of microearthquakes within clusters during the progressive failure of neighboring fault patches. The temporal distributions of magnitudes as well as the number of events follow swarmlike behavior rather than a mainshock/aftershock pattern.

  11. Influence of the Saros Fault on the Periodicity of Earthquake Activity (Gelibolu Peninsula, NW Turkey)

    NASA Astrophysics Data System (ADS)

    İpek Gültekin, Derya; Karakoç, Okan; Şahin, Murat; Elitez, İrem; Yaltırak, Cenk

    2017-04-01

    Active faults are vital in terms of settlement and socio-economic aspects of a region. For this reason, it is important to determine the characteristics and impact areas of active faults correctly. The Marmara region is a tectonically active region located in the northwestern Anatolia. The northern part of the North Anatolian Fault, which was named the Saros Fault, passes through the westernmost part of this region. The Saros Fault is a 52 km-long and NE-SW-trending right-lateral strike-slip fault. In this study, the seismicity of the Gelibolu Peninsula has been examined in the light of historical records. When considering the historical records, 545, 986, 1354 and 1756 earthquakes led to damage on the settlements close to the Saros Fault. The dates of historical earthquakes were calculated by integration of previously published empirical formulas, year difference between events and velocity of GPS vectors. The acceleration map (PGA MAPS) of the region has been produced by taking into account these earthquake magnitudes, fault geometry and geology of the region, and consequently, it was seen that these maps overlap quite well with the damage records of historical earthquakes. Considering the periodicity of the Saros Fault, which majorly controls the seismicity in the region, it is aimed to find an answer to the question "how does a recent earthquake affect the region?" by the help of historical earthquake records and PGA modelling. In conclusion, our data showed that PGA values are dominant in the northern side of the Gelibolu Peninsula and this region may be affected by a magnitude 7.3 earthquake.

  12. Fluid-driven normal faulting earthquake sequences in the Taiwan orogen

    NASA Astrophysics Data System (ADS)

    Wang, Ling-hua; Rau, Ruey-Juin; Lee, En-Jui

    2017-04-01

    Seismicity in the Central Range of Taiwan shows normal faulting mechanisms with T-axes directing NE, subparallel to the strike of the mountain belt. We analyze earthquake sequences occurred within 2012-2015 in the Nanshan area of northern Taiwan which indicating swarm behavior and migration characteristics. We select events larger than 2.0 from Central Weather Bureau catalog and use the double-difference relocation program hypoDD with waveform cross-correlation in the Nanshan area. We obtained a final count of 1406 (95%) relocated earthquakes. Moreover, we compute focal mechanisms using USGS program HASH by P-wave first motion and S/P ratio picking and 114 fault plane solutions with M 3.0-5.87 were determined. To test for fluid diffusion, we model seismicity using the equation of Shapiro et al. (1997) by fitting earthquake diffusing rate D during the migration period. According to the relocation result, seismicity in the Taiwan orogenic belt present mostly N25E orientation parallel to the mountain belt with the same direction of the tension axis. In addition, another seismic fracture depicted by seismicity rotated 35 degree counterclockwise to the NW direction. Nearly all focal mechanisms are normal fault type. In the Nanshan area, events show N10W distribution with a focal depth range from 5-12 km and illustrate fault plane dipping about 45-60 degree to SW. Three months before the M 5.87 mainshock which occurred in March, 2013, there were some foreshock events occurred in the shallow part of the fault plane of the mainshock. Half a year following the mainshock, earthquakes migrated to the north and south, respectively with processes matched the diffusion model at a rate of 0.2-0.6 m2/s. This migration pattern and diffusion rate offer an evidence of 'fluid-driven' process in the fault zone. We also find the upward migration of earthquakes in the mainshock source region. These phenomena are likely caused by the opening of the permeable conduit due to the M 5

  13. Modeling earthquake magnitudes from injection-induced seismicity on rough faults

    NASA Astrophysics Data System (ADS)

    Maurer, J.; Dunham, E. M.; Segall, P.

    2017-12-01

    It is an open question whether perturbations to the in-situ stress field due to fluid injection affect the magnitudes of induced earthquakes. It has been suggested that characteristics such as the total injected fluid volume control the size of induced events (e.g., Baisch et al., 2010; Shapiro et al., 2011). On the other hand, Van der Elst et al. (2016) argue that the size distribution of induced earthquakes follows Gutenberg-Richter, the same as tectonic events. Numerical simulations support the idea that ruptures nucleating inside regions with high shear-to-effective normal stress ratio may not propagate into regions with lower stress (Dieterich et al., 2015; Schmitt et al., 2015), however, these calculations are done on geometrically smooth faults. Fang & Dunham (2013) show that rupture length on geometrically rough faults is variable, but strongly dependent on background shear/effective normal stress. In this study, we use a 2-D elasto-dynamic rupture simulator that includes rough fault geometry and off-fault plasticity (Dunham et al., 2011) to simulate earthquake ruptures under realistic conditions. We consider aggregate results for faults with and without stress perturbations due to fluid injection. We model a uniform far-field background stress (with local perturbations around the fault due to geometry), superimpose a poroelastic stress field in the medium due to injection, and compute the effective stress on the fault as inputs to the rupture simulator. Preliminary results indicate that even minor stress perturbations on the fault due to injection can have a significant impact on the resulting distribution of rupture lengths, but individual results are highly dependent on the details of the local stress perturbations on the fault due to geometric roughness.

  14. It's Our Fault: better defining earthquake risk in Wellington, New Zealand

    NASA Astrophysics Data System (ADS)

    Van Dissen, R.; Brackley, H. L.; Francois-Holden, C.

    2012-12-01

    The Wellington region, home of New Zealand's capital city, is cut by a number of major right-lateral strike slip faults, and is underlain by the currently locked west-dipping subduction interface between the down going Pacific Plate, and the over-riding Australian Plate. In its short historic period (ca. 160 years), the region has been impacted by large earthquakes on the strike-slip faults, but has yet to bear the brunt of a subduction interface rupture directly beneath the capital city. It's Our Fault is a comprehensive study of Wellington's earthquake risk. Its objective is to position the capital city of New Zealand to become more resilient through an encompassing study of the likelihood of large earthquakes, and the effects and impacts of these earthquakes on humans and the built environment. It's Our Fault is jointly funded by New Zealand's Earthquake Commission, Accident Compensation Corporation, Wellington City Council, Wellington Region Emergency Management Group, Greater Wellington Regional Council, and Natural Hazards Research Platform. The programme has been running for six years, and key results to date include better definition and constraints on: 1) location, size, timing, and likelihood of large earthquakes on the active faults closest to Wellington; 2) earthquake size and ground shaking characterization of a representative suite of subduction interface rupture scenarios under Wellington; 3) stress interactions between these faults; 4) geological, geotechnical, and geophysical parameterisation of the near-surface sediments and basin geometry in Wellington City and the Hutt Valley; and 5) characterisation of earthquake ground shaking behaviour in these two urban areas in terms of subsoil classes specified in the NZ Structural Design Standard. The above investigations are already supporting measures aimed at risk reduction, and collectively they will facilitate identification of additional actions that will have the greatest benefit towards further

  15. The 26 May 2006 Yogyakarta earthquake fault observed by seismic data and satellite data based surface features

    NASA Astrophysics Data System (ADS)

    Anggraini, Ade; Sobiesiak, Monika; Walter, Thomas R.

    2010-05-01

    The Mw 6.3 May 26, 2006 Yogyakarta Earthquake caused severe damage and claimed thousands lives in the Yogyakarta Special Province and Klaten District of Central Java Province. The nearby Opak River fault was thought to be the source of this earthquake disaster. However, no significant surface movement was observed along the fault which could confirm that this fault was really the source of the earthquake. To investigate the earthquake source and to understand the earthquake mechanism, a rapid response team of the German Task Force for Earthquake, together with the Seismological Division of Badan Meteorologi Klimatologi dan Geofisika and Gadjah Mada University in Yogyakarta, had installed a temporary seismic network of 12 short period seismometers. More than 3000 aftershocks were recorded during the 3-month campaign. Here we present the result of several hundred processed aftershocks. We used integrated software package GIANTPitsa to pick P and S phases manually and HYPO71 to determine the hypocenters. HypoDD software was used for hypocenters relocation to obtain high precision aftershock locations. Our aftershock distribution shows a system of lineaments in southwest-northeast direction, about 10 km east to Opak River fault, at 5-18 km depth. The b-value map from the aftershocks shows that the main lineaments have relatively low b-value at the middle part which suggests this part is still under stress. We also observe several aftershock clusters cutting these lineaments in nearly perpendicular direction. To verify the interpretation of our aftershocks analysis, we will overlay it on surface feature we delineate from satellite data. Hopefully our result will give significant contribution to understand the near surface fault systems around Yogyakarta Area in order to mitigate similar earthquake hazard in the future.

  16. Cumulative co-seismic fault damage and feedbacks on earthquake rupture

    NASA Astrophysics Data System (ADS)

    Mitchell, T. M.; Aben, F. M.; Ostermeijer, G.; Rockwell, T. K.; Doan, M. L.

    2017-12-01

    The importance of the damage zone in the faulting and earthquake process is widely recognized, but our understanding of how damage zones are created, what their properties are, and how they feed back into the seismic cycle, is remarkably poorly known. Firstly, damaged rocks have reduced elastic moduli, cohesion and yield strength, which can cause attenuation and potentially non-linear wave propagation effects during ruptures. Secondly, damaged fault rocks are generally more permeable than intact rocks, and hence play a key role in the migration of fluids in and around fault zones over the seismic cycle. Finally, the dynamic generation of damage as the earthquake propagates can itself influence the dynamics of rupture propagation, by increasing the amount of energy dissipation, decreasing the rupture velocity, modifying the size of the earthquake, changing the efficiency of weakening mechanisms such as thermal pressurisation of pore fluids, and even generating seismic waves itself . All of these effects imply that a feedback exists between the damage imparted immediately after rupture propagation, at the early stages of fault slip, and the effects of that damage on subsequent ruptures dynamics. In recent years, much debate has been sparked by the identification of so-called `pulverized rocks' described on various crustal-scale faults, a type of intensely damaged fault rock which has undergone minimal shear strain, and the occurrence of which has been linked to damage induced by transient high strain-rate stress perturbations during earthquake rupture. Damage induced by such transient stresses, whether compressional or tensional, likely constitute heterogeneous modulations of the remote stresses that will impart significant changes on the strength, elastic and fluid flow properties of a fault zone immediately after rupture propagation, at the early stage of fault slip. In this contribution, we will demonstrate laboratory and field examples of two dynamic mechanisms

  17. Tidal triggering of earthquakes suggests poroelastic behavior on the San Andreas Fault

    DOE PAGES

    Delorey, Andrew A.; van der Elst, Nicholas J.; Johnson, Paul Allan

    2016-12-28

    Tidal triggering of earthquakes is hypothesized to provide quantitative information regarding the fault's stress state, poroelastic properties, and may be significant for our understanding of seismic hazard. To date, studies of regional or global earthquake catalogs have had only modest successes in identifying tidal triggering. We posit that the smallest events that may provide additional evidence of triggering go unidentified and thus we developed a technique to improve the identification of very small magnitude events. We identify events applying a method known as inter-station seismic coherence where we prioritize detection and discrimination over characterization. Here we show tidal triggering ofmore » earthquakes on the San Andreas Fault. We find the complex interaction of semi-diurnal and fortnightly tidal periods exposes both stress threshold and critical state behavior. Lastly, our findings reveal earthquake nucleation processes and pore pressure conditions – properties of faults that are difficult to measure, yet extremely important for characterizing earthquake physics and seismic hazards.« less

  18. Tidal triggering of earthquakes suggests poroelastic behavior on the San Andreas Fault

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Delorey, Andrew A.; van der Elst, Nicholas J.; Johnson, Paul Allan

    Tidal triggering of earthquakes is hypothesized to provide quantitative information regarding the fault's stress state, poroelastic properties, and may be significant for our understanding of seismic hazard. To date, studies of regional or global earthquake catalogs have had only modest successes in identifying tidal triggering. We posit that the smallest events that may provide additional evidence of triggering go unidentified and thus we developed a technique to improve the identification of very small magnitude events. We identify events applying a method known as inter-station seismic coherence where we prioritize detection and discrimination over characterization. Here we show tidal triggering ofmore » earthquakes on the San Andreas Fault. We find the complex interaction of semi-diurnal and fortnightly tidal periods exposes both stress threshold and critical state behavior. Lastly, our findings reveal earthquake nucleation processes and pore pressure conditions – properties of faults that are difficult to measure, yet extremely important for characterizing earthquake physics and seismic hazards.« less

  19. Tidal triggering of earthquakes suggests poroelastic behavior on the San Andreas Fault

    USGS Publications Warehouse

    Delorey, Andrew; Van Der Elst, Nicholas; Johnson, Paul

    2017-01-01

    Tidal triggering of earthquakes is hypothesized to provide quantitative information regarding the fault's stress state, poroelastic properties, and may be significant for our understanding of seismic hazard. To date, studies of regional or global earthquake catalogs have had only modest successes in identifying tidal triggering. We posit that the smallest events that may provide additional evidence of triggering go unidentified and thus we developed a technique to improve the identification of very small magnitude events. We identify events applying a method known as inter-station seismic coherence where we prioritize detection and discrimination over characterization. Here we show tidal triggering of earthquakes on the San Andreas Fault. We find the complex interaction of semi-diurnal and fortnightly tidal periods exposes both stress threshold and critical state behavior. Our findings reveal earthquake nucleation processes and pore pressure conditions – properties of faults that are difficult to measure, yet extremely important for characterizing earthquake physics and seismic hazards.

  20. The 7.9 Denali Fault Earthquake: Damage to Structures and Lifelines

    NASA Astrophysics Data System (ADS)

    Cox, T.; Hreinsdöttir, S.; Larsen, C.; Estes, S.

    2002-12-01

    In the early afternoon of Sunday, November 3rd, the residents of many interior Alaska towns were shaken up by a magnitude 7.9 earthquake. The shaking lasted an average of three minutes and when it stopped, nearly 300 km of the Denali Fault had ruptured. In the hours that followed, the Alaska Earthquake Information Center (AEIC) fielded reports of structural damage from Cantwell to Tok and other earthquake effects as far away as Louisiana. Upon investigation, the most severe effects were found in the village of Mentasta where basic utilities were interrupted and the school and several houses suffered major damage. Almost 3000 reports submitted to a community internet intensity map show a maximum Mercalli intensity VIII along the eastern end of the rupture area. The Richardson and Parks Highways, two main north-south thoroughfares in Alaska, both buckled and split as a result of the fault rupture. Traffic was stopped for a few hours while repairs were made. Between the Richardson Highway the Tok Cutoff, a section of the Glenn Highway that connects Tok and Glennallen, the maximum offsets on the Denali Fault were observed. Designed to withstand a magnitude 8.5 earthquake at the Denali Fault crossing, the 800-mile long Trans-Alaska Pipeline suffered relatively minor damage. According to Alyeska Pipeline Service Company press releases, the pipeline was shut down shortly after the earthquake occurred. Repairs to pipeline supports and engineering evaluations began immediately thereafter, and oil began flowing through the pipeline Thursday, November 7th . Through it all, the AEIC has collected and archived many photographs, emails, and eyewitness accounts of those who experienced the destruction firsthand. We will detail the effects that the M7.9 Denali Fault earthquake had from near and far.

  1. Earthquakes and faults in the San Francisco Bay area (1970-2003)

    USGS Publications Warehouse

    Sleeter, Benjamin M.; Calzia, James P.; Walter, Stephen R.; Wong, Florence L.; Saucedo, George J.

    2004-01-01

    The map depicts both active and inactive faults and earthquakes magnitude 1.5 to 7.0 in the greater San Francisco Bay area. Twenty-two earthquakes magnitude 5.0 and greater are indicated on the map and listed chronologically in an accompanying table. The data are compiled from records from 1970-2003. The bathymetry was generated from a digital version of NOAA maps and hydrogeographic data for San Francisco Bay. Elevation data are from the USGS National Elevation Database. Landsat satellite image is from seven Landsat 7 Enhanced Thematic Mapper Plus scenes. Fault data are reproduced with permission from the California Geological Survey. The earthquake data are from the Northern California Earthquake Catalog.

  2. Near-surface versus fault zone damage following the 1999 Chi-Chi earthquake: Observation and simulation of repeating earthquakes

    USGS Publications Warehouse

    Chen, Kate Huihsuan; Furumura, Takashi; Rubinstein, Justin L.

    2015-01-01

    We observe crustal damage and its subsequent recovery caused by the 1999 M7.6 Chi-Chi earthquake in central Taiwan. Analysis of repeating earthquakes in Hualien region, ~70 km east of the Chi-Chi earthquake, shows a remarkable change in wave propagation beginning in the year 2000, revealing damage within the fault zone and distributed across the near surface. We use moving window cross correlation to identify a dramatic decrease in the waveform similarity and delays in the S wave coda. The maximum delay is up to 59 ms, corresponding to a 7.6% velocity decrease averaged over the wave propagation path. The waveform changes on either side of the fault are distinct. They occur in different parts of the waveforms, affect different frequencies, and the size of the velocity reductions is different. Using a finite difference method, we simulate the effect of postseismic changes in the wavefield by introducing S wave velocity anomaly in the fault zone and near the surface. The models that best fit the observations point to pervasive damage in the near surface and deep, along-fault damage at the time of the Chi-Chi earthquake. The footwall stations show the combined effect of near-surface and the fault zone damage, where the velocity reduction (2–7%) is twofold to threefold greater than the fault zone damage observed in the hanging wall stations. The physical models obtained here allow us to monitor the temporal evolution and recovering process of the Chi-Chi fault zone damage.

  3. On fault evidence for a large earthquake in the late fifteenth century, Eastern Kunlun fault, China

    NASA Astrophysics Data System (ADS)

    Junlong, Zhang

    2017-11-01

    The EW-trending Kunlun Fault System (KFS) is one of the major left-lateral strike-slip faults on the Tibetan Plateau. It forms the northern boundary of the Bayan Har block. Heretofore, no evidence has been provided for the most recent event (MRE) of the 70-km-long eastern section of the KFS. The studied area is located in the north of the Zoige Basin (northwest Sichuan province) and was recognized by field mapping. Several trenches were excavated and revealed evidence of repeated events in late Holocene. The fault zone is characterized by a distinct 30-60-cm-thick clay fault gouge layer juxtaposing the hanging wall bedrock over unconsolidated late Holocene footwall colluvium and alluvium. The fault zone, hanging wall, and footwall were conformably overlain by undeformed post-MRE deposits. Samples of charred organic material were obtained from the top of the faulted sediments and the base of the unfaulted sediments. Modeling of the age of samples, earthquake yielded a calibrated 2σ radiocarbon age of A.D. 1489 ± 82. Combined with the historical earthquake record, the MRE is dated at A.D. 1488. Based on the over 50 km-long surface rupture, the magnitude of this event is nearly M w 7.0. Our data suggests that a 200-km-long seismic gap could be further divided into the Luocha and Maqu sections. For the last 1000 years, the Maqu section has been inactive, and hence, it is likely that the end of its seismic cycle is approaching, and that there is a potentially significant seismic hazard in eastern Tibet.

  4. Earthquake behavior of the Enriquillo fault zone, Haiti revealed by interactive terrain visualization

    NASA Astrophysics Data System (ADS)

    Cowgill, E.; Bernardin, T. S.; Oskin, M. E.; Bowles, C. J.; Yikilmaz, M. B.; Kreylos, O.; Elliott, A. J.; Bishop, M. S.; Gold, R. D.; Morelan, A.; Bawden, G. W.; Hamann, B.; Kellogg, L. H.

    2010-12-01

    The Mw 7.0 January 12, 2010 Haiti earthquake ended 240 years of relative quiescence following earthquakes that destroyed Port-au-Prince in 1751 and 1770. We place the 2010 rupture in the context of past earthquakes and future hazards by using remote analysis of airborne LiDAR to observe the topographic expression of active faulting and develop a new conceptual model for the earthquake behavior of the eastern Enriquillo fault zone (EFZ). In this model, the 2010 event occupies a long-lived segment boundary at a stepover within the EFZ separating fault segments that likely ruptured in 1751 and 1770, explaining both past clustering and the lack of 2010 surface rupture. Immediately following the 2010 earthquake, an airborne LiDAR point cloud containing over 2.7 billion point measurements of surface features was collected by the Rochester Inst. of Technology. To analyze these data, we capitalize on the human capacity to visually identify meaningful patterns embedded in noisy data by conducting interactive visual analysis of the entire 66.8 GB Haiti terrain data in a 4-sided, 800 ft3 immersive virtual-reality environment at the UC Davis KeckCAVES using the software tools LiDAR Viewer (to analyze point cloud data) and Crusta (for 3D surficial geologic mapping on DEM data). We discovered and measured landforms displaced by past surface-rupturing earthquakes and remotely characterized the regional fault geometry. Our analysis of the ~50 km long reach of EFZ spanning the 2010 epicenter indicates that geomorphic evidence of active faulting is clearer east of the epicenter than to the west. West of the epicenter, and in the region of the 2010 rupture, the fault is poorly defined along an embayed, low-relief range front, with little evidence of recent surface rupture. In contrast, landform offsets of 6 to 50 m along the reach of the EFZ east of the epicenter and closest to Port-au-Prince attest to repeated recent surface-rupturing earthquakes here. Specifically, we found and

  5. Slip rate and slip magnitudes of past earthquakes along the Bogd left-lateral strike-slip fault (Mongolia)

    USGS Publications Warehouse

    Rizza, M.; Ritz, J.-F.; Braucher, R.; Vassallo, R.; Prentice, C.; Mahan, S.; McGill, S.; Chauvet, A.; Marco, S.; Todbileg, M.; Demberel, S.; Bourles, D.

    2011-01-01

    earthquakes along the different segments of the western Bogd Fault. This suggests that the three western segments of the Bogd Fault and the Gurvan Bulag thrust fault (a reverse fault bounding the southern side of the Ih Bogd range that ruptured during the 1957 earthquake) have similar average recurrence times, and therefore may have ruptured together in previous earthquakes as they did in 1957. These results suggest that the western part of the Bogd Fault system, including the Gurvan Bulag thrust fault, usually behaves in a 'characteristic earthquake' mode. ?? 2011 The Authors Geophysical Journal International ?? 2011 RAS.

  6. Controls of earthquake faulting style on near field landslide triggering: The role of coseismic slip

    NASA Astrophysics Data System (ADS)

    Tatard, L.; Grasso, J. R.

    2013-06-01

    compare the spatial distributions of seven databases of landslides triggered by Mw=5.6-7.9 earthquakes, using distances normalized by the earthquake fault length. We show that the normalized landslide distance distributions collapse, i.e., the normalized distance distributions overlap whatever the size of the earthquake, separately for the events associated with dip-slip, buried-faulting earthquakes, and surface-faulting earthquakes. The dip-slip earthquakes triggered landslides at larger normalized distances than the oblique-slip event of Loma Prieta. We further identify that the surface-faulting earthquakes of Wenchuan, Chi-Chi, and Kashmir triggered landslides at normalized distances smaller than the ones expected from their Mw ≥ 7.6 magnitudes. These results support a control of the seismic slip (through amplitude, rake, and surface versus buried slip) on the distances at which landslides are triggered. In terms of coseismic landslide management in mountainous areas, our results allow us to propose distances at which 95 and 75% of landslides will be triggered as a function of the earthquake focal mechanism.

  7. M ≥ 7.0 earthquake recurrence on the San Andreas fault from a stress renewal model

    USGS Publications Warehouse

    Parsons, Thomas E.

    2006-01-01

     Forecasting M ≥ 7.0 San Andreas fault earthquakes requires an assessment of their expected frequency. I used a three-dimensional finite element model of California to calculate volumetric static stress drops from scenario M ≥ 7.0 earthquakes on three San Andreas fault sections. The ratio of stress drop to tectonic stressing rate derived from geodetic displacements yielded recovery times at points throughout the model volume. Under a renewal model, stress recovery times on ruptured fault planes can be a proxy for earthquake recurrence. I show curves of magnitude versus stress recovery time for three San Andreas fault sections. When stress recovery times were converted to expected M ≥ 7.0 earthquake frequencies, they fit Gutenberg-Richter relationships well matched to observed regional rates of M ≤ 6.0 earthquakes. Thus a stress-balanced model permits large earthquake Gutenberg-Richter behavior on an individual fault segment, though it does not require it. Modeled slip magnitudes and their expected frequencies were consistent with those observed at the Wrightwood paleoseismic site if strict time predictability does not apply to the San Andreas fault.

  8. Earthquake triggering at alaskan volcanoes following the 3 November 2002 denali fault earthquake

    USGS Publications Warehouse

    Moran, S.C.; Power, J.A.; Stihler, S.D.; Sanchez, J.J.; Caplan-Auerbach, J.

    2004-01-01

    The 3 November 2002 Mw 7.9 Denali fault earthquake provided an excellent opportunity to investigate triggered earthquakes at Alaskan volcanoes. The Alaska Volcano Observatory operates short-period seismic networks on 24 historically active volcanoes in Alaska, 247-2159 km distant from the mainshock epicenter. We searched for evidence of triggered seismicity by examining the unfiltered waveforms for all stations in each volcano network for ???1 hr after the Mw 7.9 arrival time at each network and for significant increases in located earthquakes in the hours after the mainshock. We found compelling evidence for triggering only at the Katmai volcanic cluster (KVC, 720-755 km southwest of the epicenter), where small earthquakes with distinct P and 5 arrivals appeared within the mainshock coda at one station and a small increase in located earthquakes occurred for several hours after the mainshock. Peak dynamic stresses of ???0.1 MPa at Augustine Volcano (560 km southwest of the epicenter) are significantly lower than those recorded in Yellowstone and Utah (>3000 km southeast of the epicenter), suggesting that strong directivity effects were at least partly responsible for the lack of triggering at Alaskan volcanoes. We describe other incidents of earthquake-induced triggering in the KVC, and outline a qualitative magnitude/distance-dependent triggering threshold. We argue that triggering results from the perturbation of magmatic-hydrothermal systems in the KVC and suggest that the comparative lack of triggering at other Alaskan volcanoes could be a result of differences in the nature of magmatic-hydrothermal systems.

  9. Subduction of thick oceanic plateau and high-angle normal-fault earthquakes intersecting the slab

    NASA Astrophysics Data System (ADS)

    Arai, Ryuta; Kodaira, Shuichi; Yamada, Tomoaki; Takahashi, Tsutomu; Miura, Seiichi; Kaneda, Yoshiyuki; Nishizawa, Azusa; Oikawa, Mitsuhiro

    2017-06-01

    The role of seamounts on interplate earthquakes has been debated. However, its impact on intraslab deformation is poorly understood. Here we present unexpected evidence for large normal-fault earthquakes intersecting the slab just ahead of a subducting seamount. In 1995, a series of earthquakes with maximum magnitude of 7.1 occurred in northern Ryukyu where oceanic plateaus are subducting. The aftershock distribution shows that conjugate faults with an unusually high dip angle of 70-80° ruptured the entire subducting crust. Seismic reflection images reveal that the plate interface is displaced over 1 km along one of the fault planes of the 1995 events. These results suggest that a lateral variation in slab buoyancy can produce sufficient differential stress leading to near-vertical normal-fault earthquakes within the slab. On the contrary, the upper surface of the seamount (plate interface) may correspond to a weakly coupled region, reflecting the dual effects of seamounts/plateaus on subduction earthquakes.

  10. Mapping apparent stress and energy radiation over fault zones of major earthquakes

    USGS Publications Warehouse

    McGarr, A.; Fletcher, Joe B.

    2002-01-01

    Using published slip models for five major earthquakes, 1979 Imperial Valley, 1989 Loma Prieta, 1992 Landers, 1994 Northridge, and 1995 Kobe, we produce maps of apparent stress and radiated seismic energy over their fault surfaces. The slip models, obtained by inverting seismic and geodetic data, entail the division of the fault surfaces into many subfaults for which the time histories of seismic slip are determined. To estimate the seismic energy radiated by each subfault, we measure the near-fault seismic-energy flux from the time-dependent slip there and then multiply by a function of rupture velocity to obtain the corresponding energy that propagates into the far-field. This function, the ratio of far-field to near-fault energy, is typically less than 1/3, inasmuch as most of the near-fault energy remains near the fault and is associated with permanent earthquake deformation. Adding the energy contributions from all of the subfaults yields an estimate of the total seismic energy, which can be compared with independent energy estimates based on seismic-energy flux measured in the far-field, often at teleseismic distances. Estimates of seismic energy based on slip models are robust, in that different models, for a given earthquake, yield energy estimates that are in close agreement. Moreover, the slip-model estimates of energy are generally in good accord with independent estimates by others, based on regional or teleseismic data. Apparent stress is estimated for each subfault by dividing the corresponding seismic moment into the radiated energy. Distributions of apparent stress over an earthquake fault zone show considerable heterogeneity, with peak values that are typically about double the whole-earthquake values (based on the ratio of seismic energy to seismic moment). The range of apparent stresses estimated for subfaults of the events studied here is similar to the range of apparent stresses for earthquakes in continental settings, with peak values of about

  11. Estimation of recurrence interval of large earthquakes on the central Longmen Shan fault zone based on seismic moment accumulation/release model.

    PubMed

    Ren, Junjie; Zhang, Shimin

    2013-01-01

    Recurrence interval of large earthquake on an active fault zone is an important parameter in assessing seismic hazard. The 2008 Wenchuan earthquake (Mw 7.9) occurred on the central Longmen Shan fault zone and ruptured the Yingxiu-Beichuan fault (YBF) and the Guanxian-Jiangyou fault (GJF). However, there is a considerable discrepancy among recurrence intervals of large earthquake in preseismic and postseismic estimates based on slip rate and paleoseismologic results. Post-seismic trenches showed that the central Longmen Shan fault zone probably undertakes an event similar to the 2008 quake, suggesting a characteristic earthquake model. In this paper, we use the published seismogenic model of the 2008 earthquake based on Global Positioning System (GPS) and Interferometric Synthetic Aperture Radar (InSAR) data and construct a characteristic seismic moment accumulation/release model to estimate recurrence interval of large earthquakes on the central Longmen Shan fault zone. Our results show that the seismogenic zone accommodates a moment rate of (2.7 ± 0.3) × 10¹⁷ N m/yr, and a recurrence interval of 3900 ± 400 yrs is necessary for accumulation of strain energy equivalent to the 2008 earthquake. This study provides a preferred interval estimation of large earthquakes for seismic hazard analysis in the Longmen Shan region.

  12. Estimation of Recurrence Interval of Large Earthquakes on the Central Longmen Shan Fault Zone Based on Seismic Moment Accumulation/Release Model

    PubMed Central

    Zhang, Shimin

    2013-01-01

    Recurrence interval of large earthquake on an active fault zone is an important parameter in assessing seismic hazard. The 2008 Wenchuan earthquake (Mw 7.9) occurred on the central Longmen Shan fault zone and ruptured the Yingxiu-Beichuan fault (YBF) and the Guanxian-Jiangyou fault (GJF). However, there is a considerable discrepancy among recurrence intervals of large earthquake in preseismic and postseismic estimates based on slip rate and paleoseismologic results. Post-seismic trenches showed that the central Longmen Shan fault zone probably undertakes an event similar to the 2008 quake, suggesting a characteristic earthquake model. In this paper, we use the published seismogenic model of the 2008 earthquake based on Global Positioning System (GPS) and Interferometric Synthetic Aperture Radar (InSAR) data and construct a characteristic seismic moment accumulation/release model to estimate recurrence interval of large earthquakes on the central Longmen Shan fault zone. Our results show that the seismogenic zone accommodates a moment rate of (2.7 ± 0.3) × 1017 N m/yr, and a recurrence interval of 3900 ± 400 yrs is necessary for accumulation of strain energy equivalent to the 2008 earthquake. This study provides a preferred interval estimation of large earthquakes for seismic hazard analysis in the Longmen Shan region. PMID:23878524

  13. Pulverization provides a mechanism for the nucleation of earthquakes at low stress on strong faults

    USGS Publications Warehouse

    Felzer, Karen R.

    2014-01-01

    An earthquake occurs when rock that has been deformed under stress rebounds elastically along a fault plane (Gilbert, 1884; Reid, 1911), radiating seismic waves through the surrounding earth. Rupture along the entire fault surface does not spontaneously occur at the same time, however. Rather the rupture starts in one tiny area, the rupture nucleation zone, and spreads sequentially along the fault. Like a row of dominoes, one bit of rebounding fault triggers the next. This triggering is understood to occur because of the large dynamic stresses at the tip of an active seismic rupture. The importance of these crack tip stresses is a central question in earthquake physics. The crack tip stresses are minimally important, for example, in the time predictable earthquake model (Shimazaki and Nakata, 1980), which holds that prior to rupture stresses are comparable to fault strength in many locations on the future rupture plane, with bits of variation. The stress/strength ratio is highest at some point, which is where the earthquake nucleates. This model does not require any special conditions or processes at the nucleation site; the whole fault is essentially ready for rupture at the same time. The fault tip stresses ensure that the rupture occurs as a single rapid earthquake, but the fact that fault tip stresses are high is not particularly relevant since the stress at most points does not need to be raised by much. Under this model it should technically be possible to forecast earthquakes based on the stress-renewaql concept, or estimates of when the fault as a whole will reach the critical stress level, a practice used in official hazard mapping (Field, 2008). This model also indicates that physical precursors may be present and detectable, since stresses are unusually high over a significant area before a large earthquake.

  14. Dynamic rupture simulations of the 2016 Mw7.8 Kaikōura earthquake: a cascading multi-fault event

    NASA Astrophysics Data System (ADS)

    Ulrich, T.; Gabriel, A. A.; Ampuero, J. P.; Xu, W.; Feng, G.

    2017-12-01

    The Mw7.8 Kaikōura earthquake struck the Northern part of New Zealand's South Island roughly one year ago. It ruptured multiple segments of the contractional North Canterbury fault zone and of the Marlborough fault system. Field observations combined with satellite data suggest a rupture path involving partly unmapped faults separated by large stepover distances larger than 5 km, the maximum distance usually considered by the latest seismic hazard assessment methods. This might imply distant rupture transfer mechanisms generally not considered in seismic hazard assessment. We present high-resolution 3D dynamic rupture simulations of the Kaikōura earthquake under physically self-consistent initial stress and strength conditions. Our simulations are based on recent finite-fault slip inversions that constrain fault system geometry and final slip distribution from remote sensing, surface rupture and geodetic data (Xu et al., 2017). We assume a uniform background stress field, without lateral fault stress or strength heterogeneity. We use the open-source software SeisSol (www.seissol.org) which is based on an arbitrary high-order accurate DERivative Discontinuous Galerkin method (ADER-DG). Our method can account for complex fault geometries, high resolution topography and bathymetry, 3D subsurface structure, off-fault plasticity and modern friction laws. It enables the simulation of seismic wave propagation with high-order accuracy in space and time in complex media. We show that a cascading rupture driven by dynamic triggering can break all fault segments that were involved in this earthquake without mechanically requiring an underlying thrust fault. Our prefered fault geometry connects most fault segments: it does not features stepover larger than 2 km. The best scenario matches the main macroscopic characteristics of the earthquake, including its apparently slow rupture propagation caused by zigzag cascading, the moment magnitude and the overall inferred slip

  15. Examining Structural Controls on Earthquake Rupture Dynamics Along the San Andreas Fault

    NASA Astrophysics Data System (ADS)

    McGuire, J. J.; Ben-Zion, Y.

    2002-12-01

    Recent numerical simulations of dynamic rupture [Andrews and Ben-Zion, 1997; Harris and Day, 1997] have confirmed earlier analytical results [Weertman, 1980; Adams, 1995] that a contrast in elastic properties between the two sides of a fault will generate an interaction between the normal stress and fault slip that is not present in a homogeneous medium. It has been shown that for a range of frictional parameters and initial conditions, this interaction produces a statistical preference for unilateral rupture propagation in the direction of slip of the more compliant medium [Ben-Zion and Andrews, 1998; Cochard and Rice, 2000; Ben-Zion and Huang 2002]. Thus, the directivity of earthquake ruptures on large faults with well-developed material interfaces may be controlled by material contrasts of the rocks within and across the fault zone. One of the largest known velocity contrasts across a major crustal fault occurs along the Bear Valley section of the San Andreas where high velocity materials on the SW side (P-velocity >5 km/s) are juxtaposed with low-velocity material on the NE side (P-velocity <4 km/s) down to a depth of about 4 km with a less dramatic contrast continuing to about 8 km [Thurber et al., 1997]. This boundary is strong enough to generate significant head-waves refracted along it that are recorded as the first arrivals at stations close to the fault on the NE side [McNally and McEvilly, 1977]. Rubin and Gillard [2000] and Rubin [2002] relocated the events in this region using NCSN waveform data and found that more than twice as many immediate aftershocks to small earthquakes occurred to the NW of the mainshock as to the SE, which they interpreted as being consistent with a preferred rupture direction to the SE. Their interpretation that aftershocks to microearthquakes occur preferentially in the direction opposite of rupture propagation has not been directly tested and is inconsistent with observations from moderate [Fletcher and Spudich, 1998] and

  16. Delineating Concealed Faults within Cogdell Oil Field via Earthquake Detection

    NASA Astrophysics Data System (ADS)

    Aiken, C.; Walter, J. I.; Brudzinski, M.; Skoumal, R.; Savvaidis, A.; Frohlich, C.; Borgfeldt, T.; Dotray, P.

    2016-12-01

    Cogdell oil field, located within the Permian Basin of western Texas, has experienced several earthquakes ranging from magnitude 1.7 to 4.6, most of which were recorded since 2006. Using the Earthscope USArray, Gan and Frohlich [2013] relocated some of these events and found a positive correlation in the timing of increased earthquake activity and increased CO2 injection volume. However, focal depths of these earthquakes are unknown due to 70 km station spacing of the USArray. Accurate focal depths as well as new detections can delineate subsurface faults and establish whether earthquakes are occurring in the shallow sediments or in the deeper basement. To delineate subsurface fault(s) in this region, we first detect earthquakes not currently listed in the USGS catalog by applying continuous waveform-template matching algorithms to multiple seismic data sets. We utilize seismic data spanning the time frame of 2006 to 2016 - which includes data from the U.S. Geological Survey Global Seismographic Network, the USArray, and the Sweetwater, TX broadband and nodal array located 20-40 km away. The catalog of earthquakes enhanced by template matching reveals events that were well recorded by the large-N Sweetwater array, so we are experimenting with strategies for optimizing template matching using different configurations of many stations. Since earthquake activity in the Cogdell oil field is on-going (a magnitude 2.6 occurred on May 29, 2016), a temporary deployment of TexNet seismometers has been planned for the immediate vicinity of Cogdell oil field in August 2016. Results on focal depths and detection of small magnitude events are pending this small local network deployment.

  17. Paleoseismology of Sinistral-Slip Fault System, Focusing on the Mae Chan Fault, on the Shan Plateau, SE Asia.

    NASA Astrophysics Data System (ADS)

    Curtiss, E. R.; Weldon, R. J.; Wiwegwin, W.; Weldon, E. M.

    2017-12-01

    The Shan Plateau, which includes portions of Myanmar, China, Thailand, Laos, and Vietnam lies between the dextral NS-trending Sagaing and SE-trending Red River faults and contains 14 active E-W sinistral-slip faults, including the Mae Chan Fault (MCF) in northern Thailand. The last ground-rupturing earthquake to occur on the broader sinistral fault system was the M6.8 Tarlay earthquake in Myanmar in March 2011 on the Nam Ma fault immediately north of the MCF the last earthquake to occur on the MCF was a M4.0 in the 5th century that destroyed the entire city of Wiang Yonok (Morley et al., 2011). We report on a trenching study of the MCF, which is part of a broader study to create a regional seismic hazard map of the entire Shan Plateau. By studying the MCF, which appears to be representative of the sinistral faults, and easy to work on, we hope to characterize both it and the other unstudied faults in the system. As part of a paleoseismology training course we dug two trenches at the Pa Tueng site on the MCF, within an offset river channel and the trenches exposed young sediment with abundant charcoal (in process of dating), cultural artifacts, and evidence for the last two (or three) ground-rupturing earthquakes on the fault. We hope to use the data from this site to narrow the recurrence interval, which is currently to be 2,000-4,000 years and the slip rate of 1-2 mm/year, being developed at other sites on the fault. By extrapolating the data of the MCF to the other faults we will have a better understanding of the whole fault system. Once we have characterized the MCF, we plan to use geomorphic offsets and strain rates from regional GPS to relatively estimate the activity of the other faults in this sinistral system.

  18. The origin of high frequency radiation in earthquakes and the geometry of faulting

    NASA Astrophysics Data System (ADS)

    Madariaga, R.

    2004-12-01

    In a seminal paper of 1967 Kei Aki discovered the scaling law of earthquake spectra and showed that, among other things, the high frequency decay was of type omega-squared. This implies that high frequency displacement amplitudes are proportional to a characteristic length of the fault, and radiated energy scales with the cube of the fault dimension, just like seismic moment. Later in the seventies, it was found out that a simple explanation for this frequency dependence of spectra was that high frequencies were generated by stopping phases, waves emitted by changes in speed of the rupture front as it propagates along the fault, but this did not explain the scaling of high frequency waves with fault length. Earthquake energy balance is such that, ignoring attenuation, radiated energy is the change in strain energy minus energy released for overcoming friction. Until recently the latter was considered to be a material property that did not scale with fault size. Yet, in another classical paper Aki and Das estimated in the late 70s that energy release rate also scaled with earthquake size, because earthquakes were often stopped by barriers or changed rupture speed at them. This observation was independently confirmed in the late 90s by Ide and Takeo and Olsen et al who found that energy release rates for Kobe and Landers were in the order of a MJ/m2, implying that Gc necessarily scales with earthquake size, because if this was a material property, small earthquakes would never occur. Using both simple analytical and numerical models developed by Addia-Bedia and Aochi and Madariaga, we examine the consequence of these observations for the scaling of high frequency waves with fault size. We demonstrate using some classical results by Kostrov, Husseiny and Freund that high frequency energy flow measures energy release rate and is generated when ruptures change velocity (both direction and speed) at fault kinks or jogs. Our results explain why super shear ruptures are

  19. Temporal variation in fault friction and its effects on the slip evolution of a thrust fault over several earthquake cycles

    NASA Astrophysics Data System (ADS)

    Hampel, Andrea; Hetzel, Ralf

    2013-04-01

    The friction coefficient is a key parameter for the slip evolution of faults, but how temporal changes in friction affect fault slip is still poorly known. By using three-dimensional numerical models with a thrust fault that is alternately locked and released, we show that variations in the friction coefficient affect both coseismic and long-term fault slip (Hampel and Hetzel, 2012). Decreasing the friction coefficient by 5% while keeping the duration of the interseismic phase constant leads to a four-fold increase in coseismic slip, whereas a 5% increase nearly suppresses slip. A gradual decrease or increase of friction over several earthquake cycles (1-5% per earthquake) considerably alters the cumulative fault slip. In nature, the slip deficit (surplus) resulting from variations in the friction coefficient would presumably be compensated by a longer (shorter) interseismic phase, but the magnitude of the changes required for compensation render variations of the friction coefficient of >5% unlikely. Reference Hampel, A., R. Hetzel (2012) Temporal variation in fault friction and its effects on the slip evolution of a thrust fault over several earthquake cycles. Terra Nova, 24, 357-362, doi: 10.1111/j.1365-3121.2012.01073.x.

  20. 12 May 2008 M = 7.9 Wenchuan, China, earthquake calculated to increase failure stress and seismicity rate on three major fault systems

    USGS Publications Warehouse

    Toda, S.; Lin, J.; Meghraoui, M.; Stein, R.S.

    2008-01-01

    The Wenchuan earthquake on the Longmen Shan fault zone devastated cities of Sichuan, claiming at least 69,000 lives. We calculate that the earthquake also brought the Xianshuihe, Kunlun and Min Jiang faults 150-400 km from the mainshock rupture in the eastern Tibetan Plateau 0.2-0.5 bars closer to Coulomb failure. Because some portions of these stressed faults have not ruptured in more than a century, the earthquake could trigger or hasten additional M > 7 earthquakes, potentially subjecting regions from Kangding to Daofu and Maqin to Rangtag to strong shaking. We use the calculated stress changes and the observed background seismicity to forecast the rate and distribution of damaging shocks. The earthquake probability in the region is estimated to be 57-71% for M ??? 6 shocks during the next decade, and 8-12% for M ??? 7 shocks. These are up to twice the probabilities for the decade before the Wenchuan earthquake struck. Copyright 2008 by the American Geophysical Union.

  1. Sensitivity analysis of tall buildings in Semarang, Indonesia due to fault earthquakes with maximum 7 Mw

    NASA Astrophysics Data System (ADS)

    Partono, Windu; Pardoyo, Bambang; Atmanto, Indrastono Dwi; Azizah, Lisa; Chintami, Rouli Dian

    2017-11-01

    Fault is one of the dangerous earthquake sources that can cause building failure. A lot of buildings were collapsed caused by Yogyakarta (2006) and Pidie (2016) fault source earthquakes with maximum magnitude 6.4 Mw. Following the research conducted by Team for Revision of Seismic Hazard Maps of Indonesia 2010 and 2016, Lasem, Demak and Semarang faults are three closest earthquake sources surrounding Semarang. The ground motion from those three earthquake sources should be taken into account for structural design and evaluation. Most of tall buildings, with minimum 40 meter high, in Semarang were designed and constructed following the 2002 and 2012 Indonesian Seismic Code. This paper presents the result of sensitivity analysis research with emphasis on the prediction of deformation and inter-story drift of existing tall building within the city against fault earthquakes. The analysis was performed by conducting dynamic structural analysis of 8 (eight) tall buildings using modified acceleration time histories. The modified acceleration time histories were calculated for three fault earthquakes with magnitude from 6 Mw to 7 Mw. The modified acceleration time histories were implemented due to inadequate time histories data caused by those three fault earthquakes. Sensitivity analysis of building against earthquake can be predicted by evaluating surface response spectra calculated using seismic code and surface response spectra calculated from acceleration time histories from a specific earthquake event. If surface response spectra calculated using seismic code is greater than surface response spectra calculated from acceleration time histories the structure will stable enough to resist the earthquake force.

  2. Holocene slip rates along the San Andreas Fault System in the San Gorgonio Pass and implications for large earthquakes in southern California

    NASA Astrophysics Data System (ADS)

    Heermance, Richard V.; Yule, Doug

    2017-06-01

    The San Gorgonio Pass (SGP) in southern California contains a 40 km long region of structural complexity where the San Andreas Fault (SAF) bifurcates into a series of oblique-slip faults with unknown slip history. We combine new 10Be exposure ages (Qt4: 8600 (+2100, -2200) and Qt3: 5700 (+1400, -1900) years B.P.) and a radiocarbon age (1260 ± 60 years B.P.) from late Holocene terraces with scarp displacement of these surfaces to document a Holocene slip rate of 5.7 (+2.7, -1.5) mm/yr combined across two faults. Our preferred slip rate is 37-49% of the average slip rates along the SAF outside the SGP (i.e., Coachella Valley and San Bernardino sections) and implies that strain is transferred off the SAF in this area. Earthquakes here most likely occur in very large, throughgoing SAF events at a lower recurrence than elsewhere on the SAF, so that only approximately one third of SAF ruptures penetrate or originate in the pass.Plain Language SummaryHow large are <span class="hlt">earthquakes</span> on the southern San Andreas <span class="hlt">Fault</span>? The answer to this question depends on whether or not the <span class="hlt">earthquake</span> is contained only along individual <span class="hlt">fault</span> sections, such as the Coachella Valley section north of Palm Springs, or the rupture crosses multiple sections including the area through the San Gorgonio Pass. We have determined the age and offset of <span class="hlt">faulted</span> stream deposits within the San Gorgonio Pass to document slip rates of these <span class="hlt">faults</span> over the last 10,000 years. Our results indicate a long-term slip rate of 6 mm/yr, which is almost 1/2 of the rates east and west of this area. These new rates, combined with <span class="hlt">faulted</span> geomorphic surfaces, imply that large magnitude <span class="hlt">earthquakes</span> must occasionally rupture a 300 km length of the San Andreas <span class="hlt">Fault</span> from the Salton Sea to the Mojave Desert. Although many ( 65%) <span class="hlt">earthquakes</span> along the southern San Andreas <span class="hlt">Fault</span> likely do not rupture through the pass, our new results suggest that large >Mw 7.5 <span class="hlt">earthquakes</span> are possible</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S21D..04W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S21D..04W"><span>Irregular <span class="hlt">earthquake</span> recurrence patterns and slip variability on a plate-boundary <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wechsler, N.; Rockwell, T. K.; Klinger, Y.</p> <p>2015-12-01</p> <p>The Dead Sea <span class="hlt">fault</span> in the Levant represents a simple, segmented plate boundary from the Gulf of Aqaba northward to the Sea of Galilee, where it changes its character into a complex plate boundary with multiple sub-parallel <span class="hlt">faults</span> in northern Israel, Lebanon and Syria. The studied Jordan Gorge (JG) segment is the northernmost part of the simple section, before the <span class="hlt">fault</span> becomes more complex. Seven <span class="hlt">fault</span>-crossing buried paleo-channels, offset by the Dead Sea <span class="hlt">fault</span>, were investigated using paleoseismic and geophysical methods. The mapped offsets capture the long-term rupture history and slip-rate behavior on the JG <span class="hlt">fault</span> segment for the past 4000 years. The ~20 km long JG segment appears to be more active (in term of number of <span class="hlt">earthquakes</span>) than its neighboring segments to the south and north. The rate of movement on this segment varies considerably over the studied period: the long-term slip-rate for the entire 4000 years is similar to previously observed rates (~4 mm/yr), yet over shorter time periods the rate varies from 3-8 mm/yr. Paleoseismic data on both timing and displacement indicate a high COV >1 (clustered) with displacement per event varying by nearly an order of magnitude. The rate of <span class="hlt">earthquake</span> production does not produce a time predictable pattern over a period of 2 kyr. We postulate that the seismic behavior of the JG <span class="hlt">fault</span> is influenced by stress interactions with its neighboring <span class="hlt">faults</span> to the north and south. Coulomb stress modelling demonstrates that an <span class="hlt">earthquake</span> on any neighboring <span class="hlt">fault</span> will increase the Coulomb stress on the JG <span class="hlt">fault</span> and thus promote rupture. We conclude that deriving on-<span class="hlt">fault</span> slip-rates and <span class="hlt">earthquake</span> recurrence patterns from a single site and/or over a short time period can produce misleading results. The definition of an adequately long time period to resolve slip-rate is a question that needs to be addressed and requires further work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70042525','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70042525"><span>Slip rate and slip magnitudes of past <span class="hlt">earthquakes</span> along the Bogd left-lateral strike-slip <span class="hlt">fault</span> (Mongolia)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prentice, Carol S.; Rizza, M.; Ritz, J.F.; Baucher, R.; Vassallo, R.; Mahan, S.</p> <p>2011-01-01</p> <p>5200 yr for past <span class="hlt">earthquakes</span> along the different segments of the western Bogd <span class="hlt">Fault</span>. This suggests that the three western segments of the Bogd <span class="hlt">Fault</span> and the Gurvan Bulag thrust <span class="hlt">fault</span> (a reverse <span class="hlt">fault</span> bounding the southern side of the Ih Bogd range that ruptured during the 1957 <span class="hlt">earthquake</span>) have similar average recurrence times, and therefore may have ruptured together in previous <span class="hlt">earthquakes</span> as they did in 1957. These results suggest that the western part of the Bogd <span class="hlt">Fault</span> <span class="hlt">system</span>, including the Gurvan Bulag thrust <span class="hlt">fault</span>, usually behaves in a ‘characteristic earthquake’ mode.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H13F1045G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H13F1045G"><span>A Controllable <span class="hlt">Earthquake</span> Rupture Experiment on the Homestake <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Germanovich, L. N.; Murdoch, L. C.; Garagash, D.; Reches, Z.; Martel, S. J.; Gwaba, D.; Elsworth, D.; Lowell, R. P.; Onstott, T. C.</p> <p>2010-12-01</p> <p><span class="hlt">Fault</span>-slip is typically simulated in the laboratory at the cm-to-dm scale. Laboratory results are then up-scaled by orders of magnitude to understand <span class="hlt">faulting</span> and <span class="hlt">earthquakes</span> processes. We suggest an experimental approach to reactivate <span class="hlt">faults</span> in-situ at scales ~10-100 m using thermal techniques and fluid injection to modify in situ stresses and the <span class="hlt">fault</span> strength to the point where the rock fails. Mines where the modified in-situ stresses are sufficient to drive <span class="hlt">faulting</span>, present an opportunity to conduct such experiments. During our recent field work in the former Homestake gold mine in the northern Black Hills, South Dakota, we found a large <span class="hlt">fault</span> present on multiple mine levels. The <span class="hlt">fault</span> is subparallel to the local foliation in the Poorman formation, a Proterozoic metamorphic rock deformed into regional-scale folds with axes plunging ~40° to the SSE. The <span class="hlt">fault</span> extends at least 1.5 km along strike and dip, with a center ~1.5 km deep. It strikes ~320-340° N, dips ~45-70° NE, and is recognized by a ~0.3-0.5 m thick distinct gouge that contains crushed host rock and black material that appears to be graphite. Although we could not find clear evidence for <span class="hlt">fault</span> displacement, secondary features suggest that it is a normal <span class="hlt">fault</span>. The size and distinct structure of this <span class="hlt">fault</span> make it a promising target for in-situ experimentation of <span class="hlt">fault</span> strength, hydrological properties, and slip nucleation processes. Most <span class="hlt">earthquakes</span> are thought to be the result of unstable slip on existing <span class="hlt">faults</span>, Activation of the Homestake <span class="hlt">fault</span> in response to the controlled fluid injection and thermally changing background stresses is likely to be localized on a crack-like patch. Slow patch propagation, moderated by the injection rate and the rate of change of the background stresses, may become unstable, leading to the nucleation of a small <span class="hlt">earthquake</span> (dynamic) rupture. This controlled instability is intimately related to the dependence of the <span class="hlt">fault</span> strength on the slip process and has been</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060028502&hterms=earthquakes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dearthquakes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060028502&hterms=earthquakes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dearthquakes"><span>The 2003 Bam (Iran) <span class="hlt">earthquake</span>: Rupture of a blind strike-slip <span class="hlt">fault</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Talebian, M.; Fielding, E. J.; Funning, G. J.; Ghorashi, M.; Jackson, J.; Nazari, H.; Parsons, B.; Priestley, K.; Rosen, P. A.; Walker, R.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20060028502'); toggleEditAbsImage('author_20060028502_show'); toggleEditAbsImage('author_20060028502_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20060028502_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20060028502_hide"></p> <p>2004-01-01</p> <p>A magnitude 6.5 <span class="hlt">earthquake</span> devastated the town of Bam in southeast Iran on 26 December 2003. Surface displacements and decorrelation effects, mapped using Envisat radar data, reveal that over 2 m of slip occurred at depth on a <span class="hlt">fault</span> that had not previously been identified. It is common for <span class="hlt">earthquakes</span> to occur on blind <span class="hlt">faults</span> which, despite their name, usually produce long-term surface effects by which their existence may be recognised. However, in this case there is a complete absence of morphological features associated with the seismogenic <span class="hlt">fault</span> that destroyed Bam.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028656','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028656"><span>Slip on the San Andreas <span class="hlt">fault</span> at Parkfield, California, over two <span class="hlt">earthquake</span> cycles, and the implications for seismic hazard</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Murray, J.; Langbein, J.</p> <p>2006-01-01</p> <p>Parkfield, California, which experienced M 6.0 <span class="hlt">earthquakes</span> in 1934, 1966, and 2004, is one of the few locales for which geodetic observations span multiple <span class="hlt">earthquake</span> cycles. We undertake a comprehensive study of deformation over the most recent <span class="hlt">earthquake</span> cycle and explore the results in the context of geodetic data collected prior to the 1966 event. Through joint inversion of the variety of Parkfield geodetic measurements (trilateration, two-color laser, and Global Positioning <span class="hlt">System</span>), including previously unpublished two-color data, we estimate the spatial distribution of slip and slip rate along the San Andreas using a <span class="hlt">fault</span> geometry based on precisely relocated seismicity. Although the three most recent Parkfield <span class="hlt">earthquakes</span> appear complementary in their along-strike distributions of slip, they do not produce uniform strain release along strike over multiple seismic cycles. Since the 1934 <span class="hlt">earthquake</span>, more than 1 m of slip deficit has accumulated on portions of the <span class="hlt">fault</span> that slipped in the 1966 and 2004 <span class="hlt">earthquakes</span>, and an average of 2 m of slip deficit exists on the 33 km of the <span class="hlt">fault</span> southeast of Gold Hill to be released in a future, perhaps larger, <span class="hlt">earthquake</span>. It appears that the <span class="hlt">fault</span> is capable of partially releasing stored strain in moderate <span class="hlt">earthquakes</span>, maintaining a disequilibrium through multiple <span class="hlt">earthquake</span> cycles. This complicates the application of simple <span class="hlt">earthquake</span> recurrence models that assume only the strain accumulated since the most recent event is relevant to the size or timing of an upcoming <span class="hlt">earthquake</span>. Our findings further emphasize that accumulated slip deficit is not sufficient for <span class="hlt">earthquake</span> nucleation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGP44A..02W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGP44A..02W"><span>Frictional melt generated by the 2008 Mw 7.9 Wenchuan <span class="hlt">earthquake</span> and its <span class="hlt">faulting</span> mechanisms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, H.; Li, H.; Si, J.; Sun, Z.; Zhang, L.; He, X.</p> <p>2017-12-01</p> <p><span class="hlt">Fault</span>-related pseudotachylytes are considered as fossil <span class="hlt">earthquakes</span>, conveying significant information that provide improved insight into <span class="hlt">fault</span> behaviors and their mechanical properties. The WFSD project was carried out right after the 2008 Wenchuan <span class="hlt">earthquake</span>, detailed research was conducted in the drilling cores. 2 mm rigid black layer with fresh slickenlines was observed at 732.6 m in WFSD-1 cores drilled at the southern Yingxiu-Beichuan <span class="hlt">fault</span> (YBF). Evidence of optical microscopy, FESEM and FIB-TEM show it's frictional melt (pseudotachylyte). In the northern part of YBF, 4 mm fresh melt was found at 1084 m with similar structures in WFSD-4S cores. The melts contain numerous microcracks. Considering that (1) the highly unstable property of the frictional melt (easily be altered or devitrified) under geological conditions; (2) the unfilled microcracks; (3) fresh slickenlines and (4) recent large <span class="hlt">earthquake</span> in this area, we believe that 2-4 mm melt was produced by the 2008 Wenchuan <span class="hlt">earthquake</span>. This is the first report of fresh pseudotachylyte with slickenlines in natural <span class="hlt">fault</span> that generated by modern <span class="hlt">earthquake</span>. Geochemical analyses show that <span class="hlt">fault</span> rocks at 732.6 m are enriched in CaO, Fe2O3, FeO, H2O+ and LOI, whereas depleted in SiO2. XRF results show that Ca and Fe are enriched obviously in the 2.5 cm fine-grained <span class="hlt">fault</span> rocks and Ba enriched in the slip surface. The melt has a higher magnetic susceptibility value, which may due to neoformed magnetite and metallic iron formed in <span class="hlt">fault</span> frictional melt. Frictional melt visible in both southern and northern part of YBF reveals that frictional melt lubrication played a major role in the Wenchuan <span class="hlt">earthquake</span>. Instead of vesicles and microlites, numerous randomly oriented microcracks in the melt, exhibiting a quenching texture. The quenching texture suggests the frictional melt was generated under rapid heat-dissipation condition, implying vigorous fluid circulation during the <span class="hlt">earthquake</span>. We surmise that during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.G23B0820G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.G23B0820G"><span>Implications for stress changes along the Motagua <span class="hlt">fault</span> and other nearby <span class="hlt">faults</span> using GPS and seismic constraints on the M=7.3 2009 Swan Islands <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Graham, S. E.; Rodriguez, M.; Rogers, R. D.; Strauch, W.; Hernandez, D.; Demets, C.</p> <p>2010-12-01</p> <p>The May 28, 2009 M=7.3 Swan Islands <span class="hlt">earthquake</span> off the north coast of Honduras caused significant damage in the northern part of the country, including seven deaths. This event, the largest in the region for several decades, ruptured the offshore continuation of the Motagua-Polochic <span class="hlt">fault</span> <span class="hlt">system</span>, whose 1976 <span class="hlt">earthquake</span> (located several hundred kilometers to the southwest of the 2009 epicenter) caused more than 23,000 deaths in Central America and left homeless 20% of Guatemala’s population. We use elastic half-space modeling of coseismic offsets measured at 39 GPS stations in Honduras, El Salvador, and Guatemala to better understand the slip source of the recent Swan Islands <span class="hlt">earthquake</span>. Measured offsets range from .32 meters at a campaign site near the Motagua <span class="hlt">fault</span> in northern Honduras to 4 millimeters at five continuous sites in El Salvador. Coulomb stress calculations based on the estimated distribution of coseismic slip will be presented and compared to <span class="hlt">earthquake</span> focal mechanisms and aftershock locations determined from a portable seismic network that was installed in northern Honduras after the main shock. Implications of the Swan Islands rupture for the seismically hazardous Motagua-Polochic <span class="hlt">fault</span> <span class="hlt">system</span> will be described.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH21A0165S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH21A0165S"><span>Long-Term <span class="hlt">Fault</span> Memory: A New Time-Dependent Recurrence Model for Large <span class="hlt">Earthquake</span> Clusters on Plate Boundaries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salditch, L.; Brooks, E. M.; Stein, S.; Spencer, B. D.; Campbell, M. R.</p> <p>2017-12-01</p> <p>A challenge for <span class="hlt">earthquake</span> hazard assessment is that geologic records often show large <span class="hlt">earthquakes</span> occurring in temporal clusters separated by periods of quiescence. For example, in Cascadia, a paleoseismic record going back 10,000 years shows four to five clusters separated by approximately 1,000 year gaps. If we are still in the cluster that began 1700 years ago, a large <span class="hlt">earthquake</span> is likely to happen soon. If the cluster has ended, a great <span class="hlt">earthquake</span> is less likely. For a Gaussian distribution of recurrence times, the probability of an <span class="hlt">earthquake</span> in the next 50 years is six times larger if we are still in the most recent cluster. <span class="hlt">Earthquake</span> hazard assessments typically employ one of two recurrence models, neither of which directly incorporate clustering. In one, <span class="hlt">earthquake</span> probability is time-independent and modeled as Poissonian, so an <span class="hlt">earthquake</span> is equally likely at any time. The <span class="hlt">fault</span> has no "memory" because when a prior <span class="hlt">earthquake</span> occurred has no bearing on when the next will occur. The other common model is a time-dependent <span class="hlt">earthquake</span> cycle in which the probability of an <span class="hlt">earthquake</span> increases with time until one happens, after which the probability resets to zero. Because the probability is reset after each <span class="hlt">earthquake</span>, the <span class="hlt">fault</span> "remembers" only the last <span class="hlt">earthquake</span>. This approach can be used with any assumed probability density function for recurrence times. We propose an alternative, Long-Term <span class="hlt">Fault</span> Memory (LTFM), a modified <span class="hlt">earthquake</span> cycle model where the probability of an <span class="hlt">earthquake</span> increases with time until one happens, after which it decreases, but not necessarily to zero. Hence the probability of the next <span class="hlt">earthquake</span> depends on the <span class="hlt">fault</span>'s history over multiple cycles, giving "long-term memory". Physically, this reflects an <span class="hlt">earthquake</span> releasing only part of the elastic strain stored on the <span class="hlt">fault</span>. We use the LTFM to simulate <span class="hlt">earthquake</span> clustering along the San Andreas <span class="hlt">Fault</span> and Cascadia. In some portions of the simulated <span class="hlt">earthquake</span> history, events would</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027729','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027729"><span><span class="hlt">Earthquake</span> fracture energy inferred from kinematic rupture models on extended <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tinti, E.; Spudich, P.; Cocco, M.</p> <p>2005-01-01</p> <p>We estimate fracture energy on extended <span class="hlt">faults</span> for several recent <span class="hlt">earthquakes</span> by retrieving dynamic traction evolution at each point on the <span class="hlt">fault</span> plane from slip history imaged by inverting ground motion waveforms. We define the breakdown work (Wb) as the excess of work over some minimum traction level achieved during slip. Wb is equivalent to "seismological" fracture energy (G) in previous investigations. Our numerical approach uses slip velocity as a boundary condition on the <span class="hlt">fault</span>. We employ a three-dimensional finite difference algorithm to compute the dynamic traction evolution in the time domain during the <span class="hlt">earthquake</span> rupture. We estimate Wb by calculating the scalar product between dynamic traction and slip velocity vectors. This approach does not require specifying a constitutive law and assuming dynamic traction to be collinear with slip velocity. If these vectors are not collinear, the inferred breakdown work depends on the initial traction level. We show that breakdown work depends on the square of slip. The spatial distribution of breakdown work in a single <span class="hlt">earthquake</span> is strongly correlated with the slip distribution. Breakdown work density and its integral over the <span class="hlt">fault</span>, breakdown energy, scale with seismic moment according to a power law (with exponent 0.59 and 1.18, respectively). Our estimates of breakdown work range between 4 ?? 105 and 2 ?? 107 J/m2 for <span class="hlt">earthquakes</span> having moment magnitudes between 5.6 and 7.2. We also compare our inferred values with geologic surface energies. This comparison might suggest that breakdown work for large <span class="hlt">earthquakes</span> goes primarily into heat production. Copyright 2005 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S11B0574F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S11B0574F"><span>Multiple geophysical observations indicate possible splay <span class="hlt">fault</span> activation during the 2006 Java Tsunami <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fan, W.; Bassett, D.; Denolle, M.; Shearer, P. M.; Ji, C.; Jiang, J.</p> <p>2017-12-01</p> <p>The 2006 Mw 7.8 Java <span class="hlt">earthquake</span> was a tsunami <span class="hlt">earthquake</span>, exhibiting frequency-dependent seismic radiation along strike. High-frequency global back-projection results suggest two distinct rupture stages. The first stage lasted 65 s with a rupture speed of 1.2 km/s, while the second stage lasted from 65 to 150 s with a rupture speed of 2.7 km/s. In addition, P-wave high-frequency radiated energy and fall-off rates indicate a rupture transition at 60 s. High-frequency radiators resolved with back-projection during the second stage spatially correlate with splay <span class="hlt">fault</span> traces mapped from residual free-air gravity anomalies. These splay <span class="hlt">faults</span> also collocate with a major tsunami source associated with the <span class="hlt">earthquake</span> inferred from tsunami first-crest back-propagation simulation. These correlations suggest that the splay <span class="hlt">faults</span> may have been reactivated during the Java <span class="hlt">earthquake</span>, as has been proposed for other tsunamigenic <span class="hlt">earthquakes</span>, such as the 1944 Mw 8.1 Tonankai <span class="hlt">earthquake</span> in the Nankai Trough.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026407','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026407"><span>Evidence for Late Holocene <span class="hlt">earthquakes</span> on the Utsalady Point <span class="hlt">fault</span>, Northern Puget Lowland, Washington</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Johnson, S.Y.; Nelson, A.R.; Personius, S.F.; Wells, R.E.; Kelsey, H.M.; Sherrod, B.L.; Okumura, K.; Koehler, R.; Witter, R.C.; Bradley, L.A.; Harding, D.J.</p> <p>2004-01-01</p> <p>Trenches across the Utsalady Point <span class="hlt">fault</span> in the northern Puget Lowland of Washington reveal evidence of at least one and probably two late Holocene <span class="hlt">earthquakes</span>. The "Teeka" and "Duffers" trenches were located along a 1.4-km-long, 1-to 4-m-high, northwest-trending, southwest-facing, topographic scarp recognized from Airborne Laser Swath Mapping. Glaciomarine drift exposed in the trenches reveals evidence of about 95 to 150 cm of vertical and 200 to 220 cm of left-lateral slip in the Teeka trench. Radiocarbon ages from a buried soil A horizon and overlying slope colluvium along with the historical record of <span class="hlt">earthquakes</span> suggest that this <span class="hlt">faulting</span> occurred 100 to 400 calendar years B.P. (A.D. 1550 to 1850). In the Duffers trench, 370 to 450 cm of vertical separation is accommodated by <span class="hlt">faulting</span> (???210 cm) and folding (???160 to 240 cm), with probable but undetermined amounts of lateral slip. Stratigraphic relations and radiocarbon ages from buried soil, colluvium, and fissure fill in the hanging wall suggest the deformation at Duffers is most likely from two <span class="hlt">earthquakes</span> that occurred between 100 to 500 and 1100 to 2200 calendar years B.P., but deformation during a single <span class="hlt">earthquake</span> is also possible. For the two-<span class="hlt">earthquake</span> hypothesis, deformation at Teeka trench in the first event involved folding but not <span class="hlt">faulting</span>. Regional relations suggest that the <span class="hlt">earthquake(s</span>) were M ??? ???6.7 and that offshore rupture may have produced tsunamis. Based on this investigation and related recent studies, the maximum recurrence interval for large ground-rupturing crustal-<span class="hlt">fault</span> <span class="hlt">earthquakes</span> in the Puget Lowland is about 400 to 600 years or less.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.2734C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.2734C"><span>Potential for larger <span class="hlt">earthquakes</span> in the East San Francisco Bay Area due to the direct connection between the Hayward and Calaveras <span class="hlt">Faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chaussard, E.; Bürgmann, R.; Fattahi, H.; Nadeau, R. M.; Taira, T.; Johnson, C. W.; Johanson, I.</p> <p>2015-04-01</p> <p>The Hayward and Calaveras <span class="hlt">Faults</span>, two strike-slip <span class="hlt">faults</span> of the San Andreas <span class="hlt">System</span> located in the East San Francisco Bay Area, are commonly considered independent structures for seismic hazard assessment. We use Interferometric Synthetic Aperture RADAR to show that surface creep on the Hayward <span class="hlt">Fault</span> continues 15 km farther south than previously known, revealing new potential for rupture and damage south of Fremont. The extended trace of the Hayward <span class="hlt">Fault</span>, also illuminated by shallow repeating micro-<span class="hlt">earthquakes</span>, documents a surface connection with the Calaveras <span class="hlt">Fault</span>. At depths greater than 3-5 km, repeating micro-<span class="hlt">earthquakes</span> located 10 km north of the surface connection highlight the 3-D wedge geometry of the junction. Our new model of the Hayward and Calaveras <span class="hlt">Faults</span> argues that they should be treated as a single <span class="hlt">system</span> with potential for <span class="hlt">earthquake</span> ruptures generating events with magnitudes greater than 7, posing a higher seismic hazard to the East San Francisco Bay Area than previously considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T42A..07D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T42A..07D"><span>Repetition of large stress drop <span class="hlt">earthquakes</span> on Wairarapa <span class="hlt">fault</span>, New Zealand, revealed by LiDAR data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delor, E.; Manighetti, I.; Garambois, S.; Beaupretre, S.; Vitard, C.</p> <p>2013-12-01</p> <p>We have acquired high-resolution LiDAR topographic data over most of the onland trace of the 120 km-long Wairarapa strike-slip <span class="hlt">fault</span>, New Zealand. The Wairarapa <span class="hlt">fault</span> broke in a large <span class="hlt">earthquake</span> in 1855, and this historical <span class="hlt">earthquake</span> is suggested to have produced up to 18 m of lateral slip at the ground surface. This would make this <span class="hlt">earthquake</span> a remarkable event having produced a stress drop much higher than commonly observed on other <span class="hlt">earthquakes</span> worldwide. The LiDAR data allowed us examining the ground surface morphology along the <span class="hlt">fault</span> at < 50 cm resolution, including in the many places covered with vegetation. In doing so, we identified more than 900 alluvial features of various natures and sizes that are clearly laterally offset by the <span class="hlt">fault</span>. We measured the about 670 clearest lateral offsets, along with their uncertainties. Most offsets are lower than 100 m. Each measurement was weighted by a quality factor that quantifies the confidence level in the correlation of the paired markers. Since the slips are expected to vary along the <span class="hlt">fault</span>, we analyzed the measurements in short, 3-5 km-long <span class="hlt">fault</span> segments. The PDF statistical analysis of the cumulative offsets per segment reveals that the alluvial morphology has well recorded, at every step along the <span class="hlt">fault</span>, no more than a few (3-6), well distinct cumulative slips, all lower than 80 m. Plotted along the entire <span class="hlt">fault</span>, the statistically defined cumulative slip values document four, fairly continuous slip profiles that we attribute to the four most recent large <span class="hlt">earthquakes</span> on the Wairarapa <span class="hlt">fault</span>. The four slip profiles have a roughly triangular and asymmetric envelope shape that is similar to the coseismic slip distributions described for most large <span class="hlt">earthquakes</span> worldwide. The four slip profiles have their maximum slip at the same place, in the northeastern third of the <span class="hlt">fault</span> trace. The maximum slips vary from one event to another in the range 7-15 m; the most recent 1855 <span class="hlt">earthquake</span> produced a maximum coseismic slip</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035037','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035037"><span><span class="hlt">Earthquake</span> stress drops and inferred <span class="hlt">fault</span> strength on the Hayward <span class="hlt">Fault</span>, east San Francisco Bay, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hardebeck, J.L.; Aron, A.</p> <p>2009-01-01</p> <p>We study variations in <span class="hlt">earthquake</span> stress drop with respect to depth, <span class="hlt">faulting</span> regime, creeping versus locked <span class="hlt">fault</span> behavior, and wall-rock geology. We use the P-wave displacement spectra from borehole seismic recordings of M 1.0-4.2 <span class="hlt">earthquakes</span> in the east San Francisco Bay to estimate stress drop using a stack-and-invert empirical Green's function method. The median stress drop is 8.7 MPa, and most stress drops are in the range between 0.4 and 130 MPa. An apparent correlation between stress drop and magnitude is entirely an artifact of the limited frequency band of 4-55 Hz. There is a trend of increasing stress drop with depth, with a median stress drop of ~5 MPa for 1-7 km depth, ~10 MPa for 7-13 km depth, and ~50 MPa deeper than 13 km. We use S=P amplitude ratios measured from the borehole records to better constrain the first-motion focal mechanisms. High stress drops are observed for a deep cluster of thrust-<span class="hlt">faulting</span> <span class="hlt">earthquakes</span>. The correlation of stress drops with depth and <span class="hlt">faulting</span> regime implies that stress drop is related to the applied shear stress. We compare the spatial distribution of stress drops on the Hayward <span class="hlt">fault</span> to a model of creeping versus locked behavior of the <span class="hlt">fault</span> and find that high stress drops are concentrated around the major locked patch near Oakland. This also suggests a connection between stress drop and applied shear stress, as the locked patch may experience higher applied shear stress as a result of the difference in cumulative slip or the presence of higher-strength material. The stress drops do not directly correlate with the strength of the proposed wall-rock geology at depth, suggesting that the relationship between <span class="hlt">fault</span> strength and the strength of the wall rock is complex.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1610572G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1610572G"><span>Simulating Large-Scale <span class="hlt">Earthquake</span> Dynamic Rupture Scenarios On Natural <span class="hlt">Fault</span> Zones Using the ADER-DG Method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gabriel, Alice; Pelties, Christian</p> <p>2014-05-01</p> <p>In this presentation we will demonstrate the benefits of using modern numerical methods to support physic-based ground motion modeling and research. For this purpose, we utilize SeisSol an arbitrary high-order derivative Discontinuous Galerkin (ADER-DG) scheme to solve the spontaneous rupture problem with high-order accuracy in space and time using three-dimensional unstructured tetrahedral meshes. We recently verified the method in various advanced test cases of the 'SCEC/USGS Dynamic <span class="hlt">Earthquake</span> Rupture Code Verification Exercise' benchmark suite, including branching and dipping <span class="hlt">fault</span> <span class="hlt">systems</span>, heterogeneous background stresses, bi-material <span class="hlt">faults</span> and rate-and-state friction constitutive formulations. Now, we study the dynamic rupture process using 3D meshes of <span class="hlt">fault</span> <span class="hlt">systems</span> constructed from geological and geophysical constraints, such as high-resolution topography, 3D velocity models and <span class="hlt">fault</span> geometries. Our starting point is a large scale <span class="hlt">earthquake</span> dynamic rupture scenario based on the 1994 Northridge blind thrust event in Southern California. Starting from this well documented and extensively studied event, we intend to understand the ground-motion, including the relevant high frequency content, generated from complex <span class="hlt">fault</span> <span class="hlt">systems</span> and its variation arising from various physical constraints. For example, our results imply that the Northridge <span class="hlt">fault</span> geometry favors a pulse-like rupture behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.8073Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.8073Z"><span><span class="hlt">Fault</span> geometric complexity and how it may cause temporal slip-rate variation within an interacting <span class="hlt">fault</span> <span class="hlt">system</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zielke, Olaf; Arrowsmith, Ramon</p> <p>2010-05-01</p> <p>Slip-rates along individual <span class="hlt">faults</span> may differ as a function of measurement time scale. Short-term slip-rates may be higher than the long term rate and vice versa. For example, vertical slip-rates along the Wasatch <span class="hlt">Fault</span>, Utah are 1.7+/-0.5 mm/yr since 6ka, <0.6 mm/yr since 130ka, and 0.5-0.7 mm/yr since 10Ma (Friedrich et al., 2003). Following conventional <span class="hlt">earthquake</span> recurrence models like the characteristic <span class="hlt">earthquake</span> model, this observation implies that the driving strain accumulation rates may have changed over the respective time scales as well. While potential explanations for such slip-rate variations may be found for example in the reorganization of plate tectonic motion or mantle flow dynamics, causing changes in the crustal velocity field over long spatial wavelengths, no single geophysical explanation exists. Temporal changes in <span class="hlt">earthquake</span> rate (i.e., event clustering) due to elastic interactions within a complex <span class="hlt">fault</span> <span class="hlt">system</span> may present an alternative explanation that requires neither variations in strain accumulation rate or nor changes in <span class="hlt">fault</span> constitutive behavior for frictional sliding. In the presented study, we explore this scenario and investigate how <span class="hlt">fault</span> geometric complexity, <span class="hlt">fault</span> segmentation and <span class="hlt">fault</span> (segment) interaction affect the seismic behavior and slip-rate along individual <span class="hlt">faults</span> while keeping tectonic stressing-rate and frictional behavior constant in time. For that, we used FIMozFric--a physics-based numerical <span class="hlt">earthquake</span> simulator, based on Okada's (1992) formulations for internal displacements and strains due to shear and tensile <span class="hlt">faults</span> in a half-space. <span class="hlt">Faults</span> are divided into a large number of equal-sized <span class="hlt">fault</span> patches which communicate via elastic interaction, allowing implementation of geometrically complex, non-planar <span class="hlt">faults</span>. Each patch has assigned a static and dynamic friction coefficient. The difference between those values is a function of depth--corresponding to the temperature-dependence of velocity-weakening that is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S13A2256D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S13A2256D"><span>Improving the resolution of the 2010 Haiti <span class="hlt">earthquake</span> <span class="hlt">fault</span> geometry using temporary seismometer deployments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Douilly, R.; Haase, J. S.; Ellsworth, W. L.; Bouin, M.; Calais, E.; Armbruster, J. G.; Mercier De Lepinay, B. F.; Deschamps, A.; Saint Louis, M.; Meremonte, M. E.; Hough, S. E.</p> <p>2011-12-01</p> <p>Haiti has several active <span class="hlt">faults</span> that are capable of producing large <span class="hlt">earthquakes</span> such as the 2010 Mw 7.0 Haiti <span class="hlt">earthquake</span>. This <span class="hlt">earthquake</span> was not unexpected, given geodetic measurements showing strain accumulation on the Enriquillo Plantain Garden <span class="hlt">Fault</span> Zone, the major <span class="hlt">fault</span> <span class="hlt">system</span> in southern Haiti (Manaker et al. 2008). GPS and INSAR data (Calais et al., 2010) show, however, that this rupture occurred on the previously unmapped Léogâne <span class="hlt">fault</span>, a 60° north dipping oblique blind thrust located immediately north of the Enriquillo <span class="hlt">Fault</span>. Following the <span class="hlt">earthquake</span>, several groups installed temporary seismic stations to record aftershocks. Natural Resources Canada installed three broadband seismic stations, Géoazur installed 21 ocean bottom seismometers, L'Institut de Physique du Globe de Paris installed 5 broadband seismometers, and the United States Geological Survey deployed 17 short period and strong motion seismometers in and around Port-au-Prince. We use data from this complete set of stations, along with data from permanent regional stations, to relocate all of the events from March 17 to June 24, to determine the regional one-dimensional crustal structure and determine focal mechanisms. The aftershock locations from the combined data set clearly delineate the Léogâne <span class="hlt">fault</span>. The strike and dip closely agrees with that of the global centroid moment tensor solution, but appears to be more steeply dipping than the finite <span class="hlt">fault</span> inversions. The aftershocks also delineate a flat structure on the west side of the rupture zone and may indicate triggered seismicity on the Trois Baies <span class="hlt">fault</span>, although the depths of these events are not as well constrained. There is no clear evidence for aftershocks on the other rupture segments inferred in the Hayes et al. (2010) mainshock rupture model. There is a cluster of aftershocks in the hanging wall near the western patch of high slip identified by Calais et al. (2010) and Meng et al. (2011), or central patch in the Hayes et al</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012765','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012765"><span><span class="hlt">Earthquake</span> swarms and local crustal spreading along major strike-slip <span class="hlt">faults</span> in California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Weaver, C.S.; Hill, D.P.</p> <p>1978-01-01</p> <p><span class="hlt">Earthquake</span> swarms in California are often localized to areas within dextral offsets in the linear trend in active <span class="hlt">fault</span> strands, suggesting a relation between <span class="hlt">earthquake</span> swarms and local crustal spreading. Local crustal spereading is required by the geometry of dextral offsets when, as in the San Andreas <span class="hlt">system</span>, <span class="hlt">faults</span> have dominantly strike-slip motion with right-lateral displacement. Three clear examples of this relation occur in the Imperial Valley, Coso Hot Springs, and the Danville region, all in California. The first two of these areas are known for their Holocene volcanism and geothermal potential, which is consistent with crustal spreading and magmatic intrusion. The third example, however, shows no evidence for volcanism or geothermal activity at the surface. ?? 1978 Birkha??user Verlag.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.3305F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.3305F"><span>Coseismic and postseismic deformation due to the 2007 M5.5 Ghazaband <span class="hlt">fault</span> <span class="hlt">earthquake</span>, Balochistan, Pakistan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fattahi, H.; Amelung, F.; Chaussard, E.; Wdowinski, S.</p> <p>2015-05-01</p> <p>Time series analysis of interferometric synthetic aperture radar data reveals coseismic and postseismic surface displacements associated with the 2007 M5.5 <span class="hlt">earthquake</span> along the southern Ghazaband <span class="hlt">fault</span>, a major but little studied <span class="hlt">fault</span> in Pakistan. Modeling indicates that the coseismic surface deformation was caused by ~9 cm of strike-slip displacement along a shallow subvertical <span class="hlt">fault</span>. The <span class="hlt">earthquake</span> was followed by at least 1 year of afterslip, releasing ~70% of the moment of the main event, equivalent to a M5.4 <span class="hlt">earthquake</span>. This high aseismic relative to the seismic moment release is consistent with previous observations for moderate <span class="hlt">earthquakes</span> (M < 6) and suggests that smaller <span class="hlt">earthquakes</span> are associated with a higher aseismic relative to seismic moment release than larger <span class="hlt">earthquakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S11B0580S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S11B0580S"><span>Characterization of Aftershock Sequences from Large Strike-Slip <span class="hlt">Earthquakes</span> Along Geometrically Complex <span class="hlt">Faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sexton, E.; Thomas, A.; Delbridge, B. G.</p> <p>2017-12-01</p> <p>Large <span class="hlt">earthquakes</span> often exhibit complex slip distributions and occur along non-planar <span class="hlt">fault</span> geometries, resulting in variable stress changes throughout the region of the <span class="hlt">fault</span> hosting aftershocks. To better discern the role of geometric discontinuities on aftershock sequences, we compare areas of enhanced and reduced Coulomb failure stress and mean stress for systematic differences in the time dependence and productivity of these aftershock sequences. In strike-slip <span class="hlt">faults</span>, releasing structures, including stepovers and bends, experience an increase in both Coulomb failure stress and mean stress during an <span class="hlt">earthquake</span>, promoting fluid diffusion into the region and further failure. Conversely, Coulomb failure stress and mean stress decrease in restraining bends and stepovers in strike-slip <span class="hlt">faults</span>, and fluids diffuse away from these areas, discouraging failure. We examine spatial differences in seismicity patterns along structurally complex strike-slip <span class="hlt">faults</span> which have hosted large <span class="hlt">earthquakes</span>, such as the 1992 Mw 7.3 Landers, the 2010 Mw 7.2 El-Mayor Cucapah, the 2014 Mw 6.0 South Napa, and the 2016 Mw 7.0 Kumamoto events. We characterize the behavior of these aftershock sequences with the Epidemic Type Aftershock-Sequence Model (ETAS). In this statistical model, the total occurrence rate of aftershocks induced by an <span class="hlt">earthquake</span> is λ(t) = λ_0 + \\sum_{i:t_i</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026874','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026874"><span>Surface rupture of the 2002 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span> and comparison with other strike-slip ruptures</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Haeussler, Peter J.; Schwartz, D.P.; Dawson, T.E.; Stenner, Heidi D.; Lienkaemper, J.J.; Cinti, F.; Montone, Paola; Sherrod, B.; Craw, P.</p> <p>2004-01-01</p> <p>On 3 November 2002, an M7.9 <span class="hlt">earthquake</span> produced 340 km of surface rupture on the Denali and two related <span class="hlt">faults</span> in Alaska. The rupture proceeded from west to east and began with a 40-km-long break on a previously unknown thrust <span class="hlt">fault</span>. Estimates of surface slip on this thrust are 3-6 m. Next came the principal surface break along ???218 km of the Denali <span class="hlt">fault</span>. Right-lateral offsets averaged around 5 m and increased eastward to a maximum of nearly 9 m. The <span class="hlt">fault</span> also ruptured beneath the trans-Alaska oil pipeline, which withstood almost 6 m of lateral offset. Finally, slip turned southeastward onto the Totschunda <span class="hlt">fault</span>. Right-lateral offsets are up to 3 m, and the surface rupture is about 76 km long. This three-part rupture ranks among the longest strike-slip events of the past two centuries. The <span class="hlt">earthquake</span> is typical when compared to other large <span class="hlt">earthquakes</span> on major intracontinental strike-slip <span class="hlt">faults</span>. ?? 2004, <span class="hlt">Earthquake</span> Engineering Research Institute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026732','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026732"><span>Geotechnical reconnaissance of the 2002 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kayen, R.; Thompson, E.; Minasian, D.; Moss, R.E.S.; Collins, B.D.; Sitar, N.; Dreger, D.; Carver, G.</p> <p>2004-01-01</p> <p>The 2002 M7.9 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> resulted in 340 km of ruptures along three separate <span class="hlt">faults</span>, causing widespread liquefaction in the fluvial deposits of the alpine valleys of the Alaska Range and eastern lowlands of the Tanana River. Areas affected by liquefaction are largely confined to Holocene alluvial deposits, man-made embankments, and backfills. Liquefaction damage, sparse surrounding the <span class="hlt">fault</span> rupture in the western region, was abundant and severe on the eastern rivers: the Robertson, Slana, Tok, Chisana, Nabesna and Tanana Rivers. Synthetic seismograms from a kinematic source model suggest that the eastern region of the rupture zone had elevated strong-motion levels due to rupture directivity, supporting observations of elevated geotechnical damage. We use augered soil samples and shear-wave velocity profiles made with a portable apparatus for the spectral analysis of surface waves (SASW) to characterize soil properties and stiffness at liquefaction sites and three trans-Alaska pipeline pump station accelerometer locations. ?? 2004, <span class="hlt">Earthquake</span> Engineering Research Institute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.S72F1335W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.S72F1335W"><span>Character and Significance of Surface Rupture Near the Intersection of the Denali and Totschunda <span class="hlt">Faults</span>, M7.9 Denali <span class="hlt">Fault</span> <span class="hlt">Earthquake</span>, Alaska, November 3, 2002</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wallace, W. K.; Sherrod, B. L.; Dawson, T. E.</p> <p>2002-12-01</p> <p>Preliminary observations suggest that right-lateral strike-slip on the Denali <span class="hlt">fault</span> is transferred to the Totschunda <span class="hlt">fault</span> via an extensional bend in the Little Tok River valley. Most of the surface rupture during the Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> was along an east- to east-southeast striking, gently curved segment of the Denali <span class="hlt">fault</span>. However, in the Little Tok River valley, rupture transferred to the southeast-striking Totschunda <span class="hlt">fault</span> and continued to the southeast for another 75 km. West of the Little Tok River valley, 5-7 m of right-lateral slip and up to 2 m of vertical offset occurred on the main strand of the Denali <span class="hlt">fault</span>, but no apparent displacement occurred on the Denali <span class="hlt">fault</span> east of the valley. Rupture west of the intersection also occurred on multiple discontinuous strands parallel to and south of the main strand of the Denali <span class="hlt">fault</span>. In the Little Tok River valley, the northern part of the Totschunda <span class="hlt">fault</span> <span class="hlt">system</span> consists of multiple discontinuous southeast-striking strands that are connected locally by south-striking stepover <span class="hlt">faults</span>. <span class="hlt">Faults</span> of the northern Totschunda <span class="hlt">system</span> display 0-2.5 m of right-lateral slip and 0-2.75 m of vertical offset, with the largest vertical offset on a dominantly extensional stepover <span class="hlt">fault</span>. The strands of the Totschunda <span class="hlt">system</span> converge southeastward to a single strand that had up to 2 m of slip. Complex and discontinuous <span class="hlt">faulting</span> may reflect in part the immaturity of the northern Totschunda <span class="hlt">system</span>, which is known to be younger and have much less total slip than the Denali. The Totschunda <span class="hlt">fault</span> forms an extensional bend relative to the dominantly right-lateral Denali <span class="hlt">fault</span> to the west. The <span class="hlt">fault</span> geometry and displacements at the intersection suggest that slip on the Denali <span class="hlt">fault</span> during the <span class="hlt">earthquake</span> was accommodated largely by extension in the northern Totschunda <span class="hlt">fault</span> <span class="hlt">system</span>, allowing a significant decrease in strike-slip relative to the Denali <span class="hlt">fault</span>. Strands to the southwest in the area of the bend may represent shortcut</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T11F..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T11F..01B"><span>Multi-Scale Structure and <span class="hlt">Earthquake</span> Properties in the San Jacinto <span class="hlt">Fault</span> Zone Area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ben-Zion, Y.</p> <p>2014-12-01</p> <p>I review multi-scale multi-signal seismological results on structure and <span class="hlt">earthquake</span> properties within and around the San Jacinto <span class="hlt">Fault</span> Zone (SJFZ) in southern California. The results are based on data of the southern California and ANZA networks covering scales from a few km to over 100 km, additional near-<span class="hlt">fault</span> seismometers and linear arrays with instrument spacing 25-50 m that cross the SJFZ at several locations, and a dense rectangular array with >1100 vertical-component nodes separated by 10-30 m centered on the <span class="hlt">fault</span>. The structural studies utilize <span class="hlt">earthquake</span> data to image the seismogenic sections and ambient noise to image the shallower structures. The <span class="hlt">earthquake</span> studies use waveform inversions and additional time domain and spectral methods. We observe pronounced damage regions with low seismic velocities and anomalous Vp/Vs ratios around the <span class="hlt">fault</span>, and clear velocity contrasts across various sections. The damage zones and velocity contrasts produce <span class="hlt">fault</span> zone trapped and head waves at various locations, along with time delays, anisotropy and other signals. The damage zones follow a flower-shape with depth; in places with velocity contrast they are offset to the stiffer side at depth as expected for bimaterial ruptures with persistent propagation direction. Analysis of PGV and PGA indicates clear persistent directivity at given <span class="hlt">fault</span> sections and overall motion amplification within several km around the <span class="hlt">fault</span>. Clear temporal changes of velocities, probably involving primarily the shallow material, are observed in response to seasonal, <span class="hlt">earthquake</span> and other loadings. Full source tensor properties of M>4 <span class="hlt">earthquakes</span> in the complex trifurcation area include statistically-robust small isotropic component, likely reflecting dynamic generation of rock damage in the source volumes. The dense <span class="hlt">fault</span> zone instruments record seismic "noise" at frequencies >200 Hz that can be used for imaging and monitoring the shallow material with high space and time details, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=39445','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=39445"><span>Geometric incompatibility in a <span class="hlt">fault</span> <span class="hlt">system</span>.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gabrielov, A; Keilis-Borok, V; Jackson, D D</p> <p>1996-01-01</p> <p>Interdependence between geometry of a <span class="hlt">fault</span> <span class="hlt">system</span>, its kinematics, and seismicity is investigated. Quantitative measure is introduced for inconsistency between a fixed configuration of <span class="hlt">faults</span> and the slip rates on each <span class="hlt">fault</span>. This measure, named geometric incompatibility (G), depicts summarily the instability near the <span class="hlt">fault</span> junctions: their divergence or convergence ("unlocking" or "locking up") and accumulation of stress and deformations. Accordingly, the changes in G are connected with dynamics of seismicity. Apart from geometric incompatibility, we consider deviation K from well-known Saint Venant condition of kinematic compatibility. This deviation depicts summarily unaccounted stress and strain accumulation in the region and/or internal inconsistencies in a reconstruction of block- and <span class="hlt">fault</span> <span class="hlt">system</span> (its geometry and movements). The estimates of G and K provide a useful tool for bringing together the data on different types of movement in a <span class="hlt">fault</span> <span class="hlt">system</span>. An analog of Stokes formula is found that allows determination of the total values of G and K in a region from the data on its boundary. The phenomenon of geometric incompatibility implies that nucleation of strong <span class="hlt">earthquakes</span> is to large extent controlled by processes near <span class="hlt">fault</span> junctions. The junctions that have been locked up may act as transient asperities, and unlocked junctions may act as transient weakest links. Tentative estimates of K and G are made for each end of the Big Bend of the San Andreas <span class="hlt">fault</span> <span class="hlt">system</span> in Southern California. Recent strong <span class="hlt">earthquakes</span> Landers (1992, M = 7.3) and Northridge (1994, M = 6.7) both reduced K but had opposite impact on G: Landers unlocked the area, whereas Northridge locked it up again. Images Fig. 1 Fig. 2 PMID:11607673</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189777','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189777"><span>Late Holocene slip rate and ages of prehistoric <span class="hlt">earthquakes</span> along the Maacama <span class="hlt">Fault</span> near Willits, Mendocino County, northern California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prentice, Carol S.; Larsen, Martin C.; Kelsey, Harvey M.; Zachariasen, Judith</p> <p>2014-01-01</p> <p>The Maacama <span class="hlt">fault</span> is the northward continuation of the Hayward–Rodgers Creek <span class="hlt">fault</span> <span class="hlt">system</span> and creeps at a rate of 5.7±0.1  mm/yr (averaged over the last 20 years) in Willits, California. Our paleoseismic studies at Haehl Creek suggest that the Maacama <span class="hlt">fault</span> has produced infrequent large <span class="hlt">earthquakes</span> in addition to creep. <span class="hlt">Fault</span> terminations observed in several excavations provide evidence that a prehistoric surface‐rupturing <span class="hlt">earthquake</span> occurred between 1060 and 1180 calibrated years (cal) B.P. at the Haehl Creek site. A folding event, which we attribute to a more recent large <span class="hlt">earthquake</span>, occurred between 790 and 1060 cal B.P. In the last 560–690 years, a buried channel deposit has been offset 4.6±0.2  m, giving an average slip rate of 6.4–8.6  mm/yr, which is higher than the creep rate over the last 20 years. The difference between this slip rate and the creep rate suggests that coseismic slip up to 1.7 m could have occurred after the formation of the channel deposit and could be due to a paleoearthquake known from paleoseismic studies in the Ukiah Valley, about 25 km to the southeast. Therefore, we infer that at least two, and possibly three, large <span class="hlt">earthquakes</span> have occurred at the Haehl Creek site since 1180 cal B.P. (770 C.E.), consistent with earlier studies suggesting infrequent, large <span class="hlt">earthquakes</span> on the Maacama <span class="hlt">fault</span>. The short‐term geodetic slip rate across the Maacama <span class="hlt">fault</span> zone is approximately twice the slip rate that we have documented at the Haehl Creek site, which is averaged over the last approximately 600 years. If the geodetic rate represents the long‐term slip accumulation across the <span class="hlt">fault</span> zone, then we infer that, in the last ∼1200 years, additional <span class="hlt">earthquakes</span> may have occurred either on the Haehl Creek segment of the Maacama <span class="hlt">fault</span> or on other active <span class="hlt">faults</span> within the Maacama <span class="hlt">fault</span> zone at this latitude.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T21C0577H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T21C0577H"><span>Causative <span class="hlt">Fault</span> of 2016 ML 5.8 Gyeongju <span class="hlt">Earthquake</span> (SE Korea): Structural and Seismic characteristics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ha, S.; Cheon, Y.; Lee, Y.; Kim, J.; Kim, K. H.; Son, M.</p> <p>2017-12-01</p> <p>A ML 5.8 <span class="hlt">earthquake</span>, the largest instrumental <span class="hlt">earthquake</span> in the Korean peninsula, occurred on 12 September 2016 in the Gyeongju-city, SE Korea, where is regarded as a stable intraplate region. The <span class="hlt">earthquake</span> was widely felt in the southern peninsula and had a maximum MMI VIII in the epicentral region. Most of the intraplate <span class="hlt">earthquakes</span> occur along preexisting weaknesses, but the potentially seismogenic structures are mostly not exposed at the surface. This study focuses on (1) the structural features in the neighboring area of the epicenter, (2) the distribution of <span class="hlt">earthquake</span> hypocenter locations during the first 10 days of the aftershock sequence of the Gyeongju <span class="hlt">earthquake</span>, and (3) the focal mechanism solution of select events to reveal the geometry and kinematics of its causative <span class="hlt">fault</span>. The <span class="hlt">earthquake</span> hypocenters in plan view clearly show a linear distribution of N 28°E, which extends about 7 km southwestward from the Yangsan <span class="hlt">Fault</span> to the Deokcheon <span class="hlt">Fault</span>. In cross-sectional views along N28°E and perpendicularly, the hypocenters at depths between 11 and 16 km clearly delineate a subsurface <span class="hlt">fault</span> which has a rupturing size of about 3 ´ 3 km2 and a dip of 78°SE. Based on focal mechanism solutions, the <span class="hlt">fault</span> acted as dextral strike-slip <span class="hlt">fault</span> under ENE-WSW compressional stress that has been widely known as the major component of current stress field in and around Korean peninsula. The general trend, N 28°E, of the seismogenic <span class="hlt">fault</span> slightly differs from the strike of the adjacent NNE-striking Yangsan <span class="hlt">Fault</span> with an angular difference of 15°. The Yangsan <span class="hlt">fault</span> is the most prominent dextral strike-slip <span class="hlt">fault</span> in SE Korea, which can be traced for 170 km with a right-lateral offset of 30 km. The strike-slip movement is well-reported to have occurred during the Paleogene. At that time, probably numerous subsidiary fractures, such as Y-, R-, R'-, and T fractures, in various directions were produced along the Yangsan master <span class="hlt">fault</span>. It is thus interpreted that a large R</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T22A..08J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T22A..08J"><span>Numerical simulation of <span class="hlt">faulting</span> in the Sunda Trench shows that seamounts may generate megathrust <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiao, L.; Chan, C. H.; Tapponnier, P.</p> <p>2017-12-01</p> <p>The role of seamounts in generating <span class="hlt">earthquakes</span> has been debated, with some studies suggesting that seamounts could be truncated to generate megathrust events, while other studies indicate that the maximum size of megathrust <span class="hlt">earthquakes</span> could be reduced as subducting seamounts could lead to segmentation. The debate is highly relevant for the seamounts discovered along the Mentawai patch of the Sunda Trench, where previous studies have suggested that a megathrust <span class="hlt">earthquake</span> will likely occur within decades. In order to model the dynamic behavior of the Mentawai patch, we simulated forearc <span class="hlt">faulting</span> caused by seamount subducting using the Discrete Element Method. Our models show that rupture behavior in the subduction <span class="hlt">system</span> is dominated by stiffness of the overriding plate. When stiffness is low, a seamount can be a barrier to rupture propagation, resulting in several smaller (M≤8.0) events. If, however, stiffness is high, a seamount can cause a megathrust <span class="hlt">earthquake</span> (M8 class). In addition, we show that a splay <span class="hlt">fault</span> in the subduction environment could only develop when a seamount is present, and a larger offset along a splay <span class="hlt">fault</span> is expected when stiffness of the overriding plate is higher. Our dynamic models are not only consistent with previous findings from seismic profiles and <span class="hlt">earthquake</span> activities, but the models also better constrain the rupture behavior of the Mentawai patch, thus contributing to subsequent seismic hazard assessment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70190212','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70190212"><span>Imaging of <span class="hlt">earthquake</span> <span class="hlt">faults</span> using small UAVs as a pathfinder for air and space observations</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Donnellan, Andrea; Green, Joseph; Ansar, Adnan; Aletky, Joseph; Glasscoe, Margaret; Ben-Zion, Yehuda; Arrowsmith, J. Ramón; DeLong, Stephen B.</p> <p>2017-01-01</p> <p>Large <span class="hlt">earthquakes</span> cause billions of dollars in damage and extensive loss of life and property. Geodetic and topographic imaging provide measurements of transient and long-term crustal deformation needed to monitor <span class="hlt">fault</span> zones and understand <span class="hlt">earthquakes</span>. <span class="hlt">Earthquake</span>-induced strain and rupture characteristics are expressed in topographic features imprinted on the landscapes of <span class="hlt">fault</span> zones. Small UAVs provide an efficient and flexible means to collect multi-angle imagery to reconstruct fine scale <span class="hlt">fault</span> zone topography and provide surrogate data to determine requirements for and to simulate future platforms for air- and space-based multi-angle imaging.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..12210220V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..12210220V"><span>Mixed-Mode Slip Behavior of the Altotiberina Low-Angle Normal <span class="hlt">Fault</span> <span class="hlt">System</span> (Northern Apennines, Italy) through High-Resolution <span class="hlt">Earthquake</span> Locations and Repeating Events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Valoroso, Luisa; Chiaraluce, Lauro; Di Stefano, Raffaele; Monachesi, Giancarlo</p> <p>2017-12-01</p> <p>We generated a 4.5-year-long (2010-2014) high-resolution <span class="hlt">earthquake</span> catalogue, composed of 37,000 events with ML < 3.9 and MC = 0.5 completeness magnitude, to report on the seismic activity of the Altotiberina (ATF) low-angle normal <span class="hlt">fault</span> <span class="hlt">system</span> and to shed light on the mechanical behavior and seismic potential of this <span class="hlt">fault</span>, which is capable of generating a M7 event. Seismicity defines the geometry of the <span class="hlt">fault</span> <span class="hlt">system</span> composed of the low-angle (15°-20°) ATF, extending for 50 km along strike and between 4 and 16 km at depth showing an 1.5 km thick <span class="hlt">fault</span> zone made of multiple subparallel slipping planes, and a complex network of synthetic/antithetic higher-angle segments located in the ATF hanging wall (HW) that can be traced along strike for up to 35 km. Ninety percent of the recorded seismicity occurs along the high-angle HW <span class="hlt">faults</span> during a series of minor, sometimes long-lasting (months) seismic sequences with multiple MW3+ mainshocks. Remaining <span class="hlt">earthquakes</span> (ML < 2.4) are released instead along the low-angle ATF at a constant rate of 2.2 events per day. Within the ATF-related seismicity, we found 97 clusters of repeating <span class="hlt">earthquakes</span> (RE), mostly consisting of doublets occurring during short interevent time (hours). RE are located within the geodetically recognized creeping portions of the ATF, around the main locked asperity. The rate of occurrence of RE seems quite synchronous with the ATF-HW seismic release, suggesting that creeping may guide the strain partitioning in the ATF <span class="hlt">system</span>. The seismic moment released by the ATF seismicity accounts for 30% of the geodetic one, implying aseismic deformation. The ATF-seismicity pattern is thus consistent with a mixed-mode (seismic and aseismic) slip behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.721..143F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.721..143F"><span>Rupture evolution of the 2006 Java tsunami <span class="hlt">earthquake</span> and the possible role of splay <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fan, Wenyuan; Bassett, Dan; Jiang, Junle; Shearer, Peter M.; Ji, Chen</p> <p>2017-11-01</p> <p>The 2006 Mw 7.8 Java <span class="hlt">earthquake</span> was a tsunami <span class="hlt">earthquake</span>, exhibiting frequency-dependent seismic radiation along strike. High-frequency global back-projection results suggest two distinct rupture stages. The first stage lasted ∼65 s with a rupture speed of ∼1.2 km/s, while the second stage lasted from ∼65 to 150 s with a rupture speed of ∼2.7 km/s. High-frequency radiators resolved with back-projection during the second stage spatially correlate with splay <span class="hlt">fault</span> traces mapped from residual free-air gravity anomalies. These splay <span class="hlt">faults</span> also colocate with a major tsunami source associated with the <span class="hlt">earthquake</span> inferred from tsunami first-crest back-propagation simulation. These correlations suggest that the splay <span class="hlt">faults</span> may have been reactivated during the Java <span class="hlt">earthquake</span>, as has been proposed for other tsunamigenic <span class="hlt">earthquakes</span>, such as the 1944 Mw 8.1 Tonankai <span class="hlt">earthquake</span> in the Nankai Trough.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/unnumbered/70114624/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/unnumbered/70114624/report.pdf"><span><span class="hlt">Earthquake</span> damage to transportation <span class="hlt">systems</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McCullough, Heather</p> <p>1994-01-01</p> <p><span class="hlt">Earthquakes</span> represent one of the most destructive natural hazards known to man. A large magnitude <span class="hlt">earthquake</span> near a populated area can affect residents over thousands of square kilometers and cause billions of dollars in property damage. Such an event can kill or injure thousands of residents and disrupt the socioeconomic environment for months, sometimes years. A serious result of a large-magnitude <span class="hlt">earthquake</span> is the disruption of transportation <span class="hlt">systems</span>, which limits post-disaster emergency response. Movement of emergency vehicles, such as police cars, fire trucks and ambulances, is often severely restricted. Damage to transportation <span class="hlt">systems</span> is categorized below by cause including: ground failure, <span class="hlt">faulting</span>, vibration damage, and tsunamis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70197851','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70197851"><span>Statistical relations among <span class="hlt">earthquake</span> magnitude, surface rupture length, and surface <span class="hlt">fault</span> displacement</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bonilla, Manuel G.; Mark, Robert K.; Lienkaemper, James J.</p> <p>1984-01-01</p> <p>In order to refine correlations of surface-wave magnitude, <span class="hlt">fault</span> rupture length at the ground surface, and <span class="hlt">fault</span> displacement at the surface by including the uncertainties in these variables, the existing data were critically reviewed and a new data base was compiled. <span class="hlt">Earthquake</span> magnitudes were redetermined as necessary to make them as consistent as possible with the Gutenberg methods and results, which make up much of the data base. Measurement errors were estimated for the three variables for 58 moderate to large shallow-focus <span class="hlt">earthquakes</span>. Regression analyses were then made utilizing the estimated measurement errors.The regression analysis demonstrates that the relations among the variables magnitude, length, and displacement are stochastic in nature. The stochastic variance, introduced in part by incomplete surface expression of seismogenic <span class="hlt">faulting</span>, variation in shear modulus, and regional factors, dominates the estimated measurement errors. Thus, it is appropriate to use ordinary least squares for the regression models, rather than regression models based upon an underlying deterministic relation in which the variance results primarily from measurement errors.Significant differences exist in correlations of certain combinations of length, displacement, and magnitude when events are grouped by <span class="hlt">fault</span> type or by region, including attenuation regions delineated by Evernden and others.Estimates of the magnitude and the standard deviation of the magnitude of a prehistoric or future <span class="hlt">earthquake</span> associated with a <span class="hlt">fault</span> can be made by correlating Ms with the logarithms of rupture length, <span class="hlt">fault</span> displacement, or the product of length and displacement.<span class="hlt">Fault</span> rupture area could be reliably estimated for about 20 of the events in the data set. Regression of Ms on rupture area did not result in a marked improvement over regressions that did not involve rupture area. Because no subduction-zone <span class="hlt">earthquakes</span> are included in this study, the reported results do not apply to such</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T23F0689M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T23F0689M"><span>Stress and Strain Rates from <span class="hlt">Faults</span> Reconstructed by <span class="hlt">Earthquakes</span> Relocalization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morra, G.; Chiaraluce, L.; Di Stefano, R.; Michele, M.; Cambiotti, G.; Yuen, D. A.; Brunsvik, B.</p> <p>2017-12-01</p> <p>Recurrence of main <span class="hlt">earthquakes</span> on the same <span class="hlt">fault</span> depends on kinematic setting, hosting lithologies and <span class="hlt">fault</span> geometry and population. Northern and central Italy transitioned from convergence to post-orogenic extension. This has produced a unique and very complex tectonic setting characterized by superimposed normal <span class="hlt">faults</span>, crossing different geologic domains, that allows to investigate a variety of seismic manifestations. In the past twenty years three seismic sequences (1997 Colfiorito, 2009 L'Aquila and 2016-17 Amatrice-Norcia-Visso) activated a 150km long normal <span class="hlt">fault</span> <span class="hlt">system</span> located between the central and northern apennines and allowing the recordings of thousands of seismic events. Both the 1997 and the 2009 main shocks were preceded by a series of small pre-shocks occurring in proximity to the future largest events. It has been proposed and modelled that the seismicity pattern of the two foreshocks sequences was caused by active dilatancy phenomenon, due to fluid flow in the source area. Seismic activity has continued intensively until three events with 6.0</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U23B..02N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U23B..02N"><span>Interaction between <span class="hlt">fault</span> <span class="hlt">systems</span> in a complex tectonic setting: Insights from InSAR and Teleseismic analysis of the 2015 Lake Saurez and 2016 Muji <span class="hlt">fault</span> <span class="hlt">earthquake</span> sequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nanjundiah, P.; Barbot, S.; Wei, S.; Tapponnier, P.; Feng, W.; Wang, T.</p> <p>2017-12-01</p> <p>The Pamir Plateau is a complex and important component of the India-Eurasia Collision zone. Despite being similar to the Tibetan plateau in elevation and collision processes, quite a bit is still unknown about the structure and the tectonic processes occurring in this region. We aim to better understand the structure, stress and deformation patterns in the northern and central Pamir plateau by analysing InSAR, teleseismic, and optical data for two large <span class="hlt">earthquakes</span> that occurred in this region between December 2015 (Mw 7.2, Lake Saurez) and November 2016 (Mw 6.6 Muji <span class="hlt">Fault</span>). We constrain the <span class="hlt">fault</span> geometry by precisely relocating aftershocks using the double difference technique implemented in HypoDD (Waldhauser & Ellsworth 2000). We used Okada's (1992) Green Functions to invert for slip on the <span class="hlt">fault</span> with a rectangular dislocation and edgreen to numerically invert for the slip in a layered medium (Wang et al. 2005). The combined datasets highlight the existence of an oblique <span class="hlt">fault</span> between two major thrust <span class="hlt">fault</span> <span class="hlt">systems</span> i.e. the Darwas & the Karakoram <span class="hlt">faults</span>. The December 2015 event highlights complexity in this <span class="hlt">fault</span> <span class="hlt">system</span>. The combination of data sets used in this study highlights the existence of a seismic gap south of Lake Karakul as well as coupling between the Muji and Darwas-Karakoram <span class="hlt">fault</span> <span class="hlt">systems</span>. We emphasise the role of smaller <span class="hlt">faults</span> and their interactions in accommodating the overall strain and tectonics in the Pamir region and their effect on estimating local seismic hazard.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028373','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028373"><span>Association of the 1886 Charleston, South Carolina, <span class="hlt">earthquake</span> and seismicity near Summervile with a 12º bend in the East Coast <span class="hlt">fault</span> <span class="hlt">system</span> and triple-<span class="hlt">fault</span> junctions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Marple, R.; Miller, R.</p> <p>2006-01-01</p> <p>Seismic-reflection data were integrated with other geophysical, geologic, and seismicity data to better determine the location and nature of buried <span class="hlt">faults</span> in the Charleston, South Carolina, region. Our results indicate that the 1886 Charleston, South Carolina, <span class="hlt">earthquake</span> and seismicity near Summerville are related to local stresses caused by a 12?? bend in the East Coast <span class="hlt">fault</span> <span class="hlt">system</span> (ECFS) and two triple-<span class="hlt">fault</span> junctions. One triple junction is formed by the intersection of the northwest-trending Ashley River <span class="hlt">fault</span> with the two segments of the ECFS north and south of the bend. The other triple junction is formed by the intersection of the northeast-trending Summerville <span class="hlt">fault</span> and a newly discovered northwest-trending Berkeley <span class="hlt">fault</span> with the ECFS about 10 km north of the bend. The Summerville <span class="hlt">fault</span> is a northwest-dipping border <span class="hlt">fault</span> of the Triassic-age Jedburg basin that is undergoing reverse-style reactivation. This reverse-style reactivation is unusual because the Summerville <span class="hlt">fault</span> parallels the regional stress field axis, suggesting that the reactivation is from stresses applied by dextral motion on the ECFS. The southwest-dip and reverse-type motion of the Berkeley <span class="hlt">fault</span> are interpreted from seismicity data and a seismic-reflection profile in the western part of the study area. Our results also indicate that the East Coast <span class="hlt">fault</span> <span class="hlt">system</span> is a Paleozoic basement <span class="hlt">fault</span> and that its reactivation since early Mesozoic time has fractured through the overlying allochthonous terranes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.712..156S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.712..156S"><span>Field- to nano-scale evidence for weakening mechanisms along the <span class="hlt">fault</span> of the 2016 Amatrice and Norcia <span class="hlt">earthquakes</span>, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smeraglia, Luca; Billi, Andrea; Carminati, Eugenio; Cavallo, Andrea; Doglioni, Carlo</p> <p>2017-08-01</p> <p>In August and October 2016, two normal <span class="hlt">fault</span> <span class="hlt">earthquakes</span> (Mw 6.0 and Mw 6.5, respectively) struck the Amatrice-Norcia area in the central Apennines, Italy. The mainshocks nucleated at depths of 7-9 km with the co-seismic slip propagating upward along the Mt. Gorzano <span class="hlt">Fault</span> (MGF) and Mt. Vettore <span class="hlt">Fault</span> <span class="hlt">System</span> (MVFS). To recognize possible weakening mechanisms along the carbonate-hosted seismogenic <span class="hlt">faults</span> that generated the Amatrice-Norcia <span class="hlt">earthquakes</span>, the fresh co-seismic <span class="hlt">fault</span> exposure (i.e., "nastrino") exposed along the Mt. Vettoretto <span class="hlt">Fault</span> was sampled and analyzed. This exposed <span class="hlt">fault</span> belongs to the MVFS and was exhumed from 2-3 km depth. Over the fresh <span class="hlt">fault</span> surface, phyllosilicates concentrated and localized along mm- to μm-thick layers, and truncated clasts and fluid-like structures were found. At the nano-scale, instead of their common platy-lamellar crystallographic texture, the analyzed phyllosilicates consist of welded nm-thick nanospherules and nanotubes similar to phyllosilicates deformed in rotary shear apparatus at seismic velocities or altered under high hydrothermal temperatures (> 250 °C). Moreover, the attitude of the Mt. Vettoretto <span class="hlt">Fault</span> and its kinematics inferred from exposed slickenlines are consistent with the co-seismic <span class="hlt">fault</span> and slip vectors obtained from the focal mechanisms computed for the 2016 mainshocks. All these pieces of evidence suggest that the Mt. Vettoretto <span class="hlt">Fault</span> slipped seismically during past <span class="hlt">earthquakes</span> and that co-seismic slip was assisted and facilitated at depths of < 3 km by phyllosilicate-rich layers and overpressured fluids. The same weakening processes may also have been decisive in facilitating the co-seismic slip propagation during the 2016 Mw 6.0 Amatrice and Mw 6.5 Norcia <span class="hlt">earthquakes</span>. The microstructures found along the Mt. Vettoretto <span class="hlt">Fault</span>, which is certainly a seismogenic <span class="hlt">fault</span>, provide a realistic synoptic picture of co-seismic processes and weakening mechanisms that may occur in carbonate-hosted seismogenic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.S14B..07B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.S14B..07B"><span>The 1868 Hayward <span class="hlt">Earthquake</span> Alliance: A Case Study - Using an <span class="hlt">Earthquake</span> Anniversary to Promote <span class="hlt">Earthquake</span> Preparedness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brocher, T. M.; Garcia, S.; Aagaard, B. T.; Boatwright, J. J.; Dawson, T.; Hellweg, M.; Knudsen, K. L.; Perkins, J.; Schwartz, D. P.; Stoffer, P. W.; Zoback, M.</p> <p>2008-12-01</p> <p>Last October 21st marked the 140th anniversary of the M6.8 1868 Hayward <span class="hlt">Earthquake</span>, the last damaging <span class="hlt">earthquake</span> on the southern Hayward <span class="hlt">Fault</span>. This anniversary was used to help publicize the seismic hazards associated with the <span class="hlt">fault</span> because: (1) the past five such <span class="hlt">earthquakes</span> on the Hayward <span class="hlt">Fault</span> occurred about 140 years apart on average, and (2) the Hayward-Rodgers Creek <span class="hlt">Fault</span> <span class="hlt">system</span> is the most likely (with a 31 percent probability) <span class="hlt">fault</span> in the Bay Area to produce a M6.7 or greater <span class="hlt">earthquake</span> in the next 30 years. To promote <span class="hlt">earthquake</span> awareness and preparedness, over 140 public and private agencies and companies and many individual joined the public-private nonprofit 1868 Hayward <span class="hlt">Earthquake</span> Alliance (1868alliance.org). The Alliance sponsored many activities including a public commemoration at Mission San Jose in Fremont, which survived the 1868 <span class="hlt">earthquake</span>. This event was followed by an <span class="hlt">earthquake</span> drill at Bay Area schools involving more than 70,000 students. The anniversary prompted the Silver Sentinel, an <span class="hlt">earthquake</span> response exercise based on the scenario of an <span class="hlt">earthquake</span> on the Hayward <span class="hlt">Fault</span> conducted by Bay Area County Offices of Emergency Services. 60 other public and private agencies also participated in this exercise. The California Seismic Safety Commission and KPIX (CBS affiliate) produced professional videos designed forschool classrooms promoting Drop, Cover, and Hold On. Starting in October 2007, the Alliance and the U.S. Geological Survey held a sequence of press conferences to announce the release of new research on the Hayward <span class="hlt">Fault</span> as well as new loss estimates for a Hayward <span class="hlt">Fault</span> <span class="hlt">earthquake</span>. These included: (1) a ShakeMap for the 1868 Hayward <span class="hlt">earthquake</span>, (2) a report by the U. S. Bureau of Labor Statistics forecasting the number of employees, employers, and wages predicted to be within areas most strongly shaken by a Hayward <span class="hlt">Fault</span> <span class="hlt">earthquake</span>, (3) new estimates of the losses associated with a Hayward <span class="hlt">Fault</span> <span class="hlt">earthquake</span>, (4) new ground motion</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011055','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011055"><span>Tilt precursors before <span class="hlt">earthquakes</span> on the San Andreas <span class="hlt">fault</span>, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Johnston, M.J.S.; Mortensen, C.E.</p> <p>1974-01-01</p> <p>An array of 14 biaxial shallow-borehole tiltmeters (at 10-7 radian sensitivity) has been installed along 85 kilometers of the San Andreas <span class="hlt">fault</span> during the past year. <span class="hlt">Earthquake</span>-related changes in tilt have been simultaneously observed on up to four independent instruments. At <span class="hlt">earthquake</span> distances greater than 10 <span class="hlt">earthquake</span> source dimensions, there are few clear indications of tilt change. For the four instruments with the longest records (>10 months), 26 <span class="hlt">earthquakes</span> have occurred since July 1973 with at least one instrument closer than 10 source dimensions and 8 <span class="hlt">earthquakes</span> with more than one instrument within that distance. Precursors in tilt direction have been observed before more than 10 <span class="hlt">earthquakes</span> or groups of <span class="hlt">earthquakes</span>, and no similar effect has yet been seen without the occurrence of an <span class="hlt">earthquake</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980029715','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980029715"><span>Systematic Underestimation of <span class="hlt">Earthquake</span> Magnitudes from Large Intracontinental Reverse <span class="hlt">Faults</span>: Historical Ruptures Break Across Segment Boundaries</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubin, C. M.</p> <p>1996-01-01</p> <p>Because most large-magnitude <span class="hlt">earthquakes</span> along reverse <span class="hlt">faults</span> have such irregular and complicated rupture patterns, reverse-<span class="hlt">fault</span> segments defined on the basis of geometry alone may not be very useful for estimating sizes of future seismic sources. Most modern large ruptures of historical <span class="hlt">earthquakes</span> generated by intracontinental reverse <span class="hlt">faults</span> have involved geometrically complex rupture patterns. Ruptures across surficial discontinuities and complexities such as stepovers and cross-<span class="hlt">faults</span> are common. Specifically, segment boundaries defined on the basis of discontinuities in surficial <span class="hlt">fault</span> traces, pronounced changes in the geomorphology along strike, or the intersection of active <span class="hlt">faults</span> commonly have not proven to be major impediments to rupture. Assuming that the seismic rupture will initiate and terminate at adjacent major geometric irregularities will commonly lead to underestimation of magnitudes of future large <span class="hlt">earthquakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016987','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016987"><span><span class="hlt">Earthquake</span> mechanism and predictability shown by a laboratory <span class="hlt">fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>King, C.-Y.</p> <p>1994-01-01</p> <p>Slip events generated in a laboratory <span class="hlt">fault</span> model consisting of a circulinear chain of eight spring-connected blocks of approximately equal weight elastically driven to slide on a frictional surface are studied. It is found that most of the input strain energy is released by a relatively few large events, which are approximately time predictable. A large event tends to roughen stress distribution along the <span class="hlt">fault</span>, whereas the subsequent smaller events tend to smooth the stress distribution and prepare a condition of simultaneous criticality for the occurrence of the next large event. The frequency-size distribution resembles the Gutenberg-Richter relation for <span class="hlt">earthquakes</span>, except for a falloff for the largest events due to the finite energy-storage capacity of the <span class="hlt">fault</span> <span class="hlt">system</span>. Slip distributions, in different events are commonly dissimilar. Stress drop, slip velocity, and rupture velocity all tend to increase with event size. Rupture-initiation locations are usually not close to the maximum-slip locations. ?? 1994 Birkha??user Verlag.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S51A4440M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S51A4440M"><span>Constraints on recent <span class="hlt">earthquake</span> source parameters, <span class="hlt">fault</span> geometry and aftershock characteristics in Oklahoma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McNamara, D. E.; Benz, H.; Herrmann, R. B.; Bergman, E. A.; McMahon, N. D.; Aster, R. C.</p> <p>2014-12-01</p> <p>In late 2009, the seismicity of Oklahoma increased dramatically. The largest of these <span class="hlt">earthquakes</span> was a series of three damaging events (Mw 4.8, 5.6, 4.8) that occurred over a span of four days in November 2011 near the town of Prague in central Oklahoma. Studies suggest that these <span class="hlt">earthquakes</span> were induced by reactivation of the Wilzetta <span class="hlt">fault</span> due to the disposal of waste water from hydraulic fracturing ("fracking") and other oil and gas activities. The Wilzetta <span class="hlt">fault</span> is a northeast trending vertical strike-slip <span class="hlt">fault</span> that is a well known structural trap for oil and gas. Since the November 2011 Prague sequence, thousands of small to moderate (M2-M4) <span class="hlt">earthquakes</span> have occurred throughout central Oklahoma. The most active regions are located near the towns of Stillwater and Medford in north-central Oklahoma, and Guthrie, Langston and Jones near Oklahoma City. The USGS, in collaboration with the Oklahoma Geological Survey and the University of Oklahoma, has responded by deploying numerous temporary seismic stations in the region in order to record the vigorous aftershock sequences. In this study we use data from the temporary seismic stations to re-locate all Oklahoma <span class="hlt">earthquakes</span> in the USGS National <span class="hlt">Earthquake</span> Information Center catalog using a multiple-event approach known as hypo-centroidal decomposition that locates <span class="hlt">earthquakes</span> with decreased uncertainty relative to one another. Modeling from this study allows us to constrain the detailed geometry of the reactivated <span class="hlt">faults</span>, as well as source parameters (focal mechanisms, stress drop, rupture length) for the larger <span class="hlt">earthquakes</span>. Preliminary results from the November 2011 Prague sequence suggest that subsurface rupture lengths of the largest <span class="hlt">earthquakes</span> are anomalously long with very low stress drop. We also observe very high Q (~1000 at 1 Hz) that explains the large felt areas and we find relatively low b-value and a rapid decay of aftershocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T41C0644C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T41C0644C"><span>The 2014 Mw6.9 Gokceada and 2017 Mw6.3 Lesvos <span class="hlt">Earthquakes</span> in the Northern Aegean Sea: The Transition from Right-Lateral Strike-Slip <span class="hlt">Faulting</span> on the North Anatolian <span class="hlt">Fault</span> to Extension in the Central Aegean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cetin, S.; Konca, A. O.; Dogan, U.; Floyd, M.; Karabulut, H.; Ergintav, S.; Ganas, A.; Paradisis, D.; King, R. W.; Reilinger, R. E.</p> <p>2017-12-01</p> <p>The 2014 Mw6.9 Gokceada (strike-slip) and 2017 Mw6.3 Lesvos (normal) <span class="hlt">earthquakes</span> represent two of the set of <span class="hlt">faults</span> that accommodate the transition from right-lateral strike-slip <span class="hlt">faulting</span> on the North Anatolian <span class="hlt">Fault</span> (NAF) to normal <span class="hlt">faulting</span> along the Gulf of Corinth. The Gokceada <span class="hlt">earthquake</span> was a purely strike-slip event on the western extension of the NAF where it enters the northern Aegean Sea. The Lesvos <span class="hlt">earthquake</span>, located roughly 200 km south of Gokceada, occurred on a WNW-ESE-striking normal <span class="hlt">fault</span>. Both <span class="hlt">earthquakes</span> respond to the same regional stress field, as indicated by their sub-parallel seismic tension axis and far-field coseismic GPS displacements. Interpretation of GPS-derived velocities, active <span class="hlt">faults</span>, crustal seismicity, and <span class="hlt">earthquake</span> focal mechanisms in the northern Aegean indicates that this pattern of complementary <span class="hlt">faulting</span>, involving WNW-ESE-striking normal <span class="hlt">faults</span> (e.g. Lesvos <span class="hlt">earthquake</span>) and SW-NE-striking strike-slip <span class="hlt">faults</span> (e.g. Gokceada <span class="hlt">earthquake</span>), persists across the full extent of the northern Aegean Sea. The combination of these two "families" of <span class="hlt">faults</span>, combined with some <span class="hlt">systems</span> of conjugate left-lateral strike-slip <span class="hlt">faults</span>, complement one another and culminate in the purely extensional rift structures that form the large Gulfs of Evvia and Corinth. In addition to being consistent with seismic and geodetic observations, these <span class="hlt">fault</span> geometries explain the increasing velocity of the southern Aegean and Peloponnese regions towards the Hellenic subduction zone. Alignment of geodetic extension and seismic tension axes with motion of the southern Aegean towards the Hellenic subduction zone suggests a direct association of Aegean extension with subduction, possibly by trench retreat, as has been suggested by prior investigators.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T21A0547H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T21A0547H"><span>Creeping Guanxian-Anxian <span class="hlt">Fault</span> ruptured in the 2008 Mw 7.9 Wenchuan <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>He, X.; Li, H.; Wang, H.; Zhang, L.; Si, J.</p> <p>2017-12-01</p> <p>Crustal active <span class="hlt">faults</span> can slide either steadily by aseismic creep, or abruptly by <span class="hlt">earthquake</span> rupture. Creep can relax continuously the stress and reduce the occurrence of large <span class="hlt">earthquakes</span>. Identifying the behaviors of active <span class="hlt">faults</span> plays a crucial role in predicting and preventing <span class="hlt">earthquake</span> disasters. Based on multi-scale structural analyses for <span class="hlt">fault</span> rocks from the GAF surface rupture zone and the Wenchuan <span class="hlt">Earthquake</span> <span class="hlt">Fault</span> Zone Science Drilling borehole 3P, we detect the analogous "mylonite structures" develop pervasively in GAF <span class="hlt">fault</span> rocks. Such specious "ductile deformations", showing intensive foliation, spindly clasts, tailing structure, "boudin structure", "augen structure" and S-C fabrics, are actually formed in brittle <span class="hlt">faulting</span>, which indicates the creeping behavior of the GAF. Furthermore, some special structures hint the creeping mechanism. The cracks and veins developed in fractured clasts imply pressure and fluid control in the <span class="hlt">faulting</span>. Under the effect of fluid, clasts are dissolved in pressing direction, and solutions are transferred to stress vacancy area at both ends of clasts and deposit to regenerate clay minerals. The clasts thus present spindly shape and are surrounded by orientational clay minerals constituting continuous foliation structure. The clay minerals are dominated by phyllosilicates that can weaken <span class="hlt">faults</span> and promote pressure solution. Therefore, pressure solution creep and phyllosilicates weakening reasonably interpret the creeping of GAF. Additionally, GPS velocity data show slip rates of the GAF are respectively 1.5 and 12 mm/yr during 1998-2008 and 2009-2011, which also indicate the GAF is in creeping during interseismic period. According to analysis on aftershocks distribution and P-wave velocity with depth and geological section in the Longmenshan thrust belt, we suggest the GAF is creeping in shallow (<10 km) and locked in deep (10-20 km). Comprehensive research shows stress propagated from the west was concentrated near the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1984/of84-256/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1984/of84-256/"><span>Statistical relations among <span class="hlt">earthquake</span> magnitude, surface rupture length, and surface <span class="hlt">fault</span> displacement</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bonilla, M.G.; Mark, R.K.; Lienkaemper, J.J.</p> <p>1984-01-01</p> <p>In order to refine correlations of surface-wave magnitude, <span class="hlt">fault</span> rupture length at the ground surface, and <span class="hlt">fault</span> displacement at the surface by including the uncertainties in these variables, the existing data were critically reviewed and a new data base was compiled. <span class="hlt">Earthquake</span> magnitudes were redetermined as necessary to make them as consistent as possible with the Gutenberg methods and results, which necessarily make up much of the data base. Measurement errors were estimated for the three variables for 58 moderate to large shallow-focus <span class="hlt">earthquakes</span>. Regression analyses were then made utilizing the estimated measurement errors. The regression analysis demonstrates that the relations among the variables magnitude, length, and displacement are stochastic in nature. The stochastic variance, introduced in part by incomplete surface expression of seismogenic <span class="hlt">faulting</span>, variation in shear modulus, and regional factors, dominates the estimated measurement errors. Thus, it is appropriate to use ordinary least squares for the regression models, rather than regression models based upon an underlying deterministic relation with the variance resulting from measurement errors. Significant differences exist in correlations of certain combinations of length, displacement, and magnitude when events are qrouped by <span class="hlt">fault</span> type or by region, including attenuation regions delineated by Evernden and others. Subdivision of the data results in too few data for some <span class="hlt">fault</span> types and regions, and for these only regressions using all of the data as a group are reported. Estimates of the magnitude and the standard deviation of the magnitude of a prehistoric or future <span class="hlt">earthquake</span> associated with a <span class="hlt">fault</span> can be made by correlating M with the logarithms of rupture length, <span class="hlt">fault</span> displacement, or the product of length and displacement. <span class="hlt">Fault</span> rupture area could be reliably estimated for about 20 of the events in the data set. Regression of MS on rupture area did not result in a marked improvement</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EP%26S...70...62J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EP%26S...70...62J"><span>Coseismic and postseismic deformation associated with the 2016 Mw 7.8 Kaikoura <span class="hlt">earthquake</span>, New Zealand: <span class="hlt">fault</span> movement investigation and seismic hazard analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Zhongshan; Huang, Dingfa; Yuan, Linguo; Hassan, Abubakr; Zhang, Lupeng; Yang, Zhongrong</p> <p>2018-04-01</p> <p>The 2016 moment magnitude (Mw) 7.8 Kaikoura <span class="hlt">earthquake</span> demonstrated that multiple <span class="hlt">fault</span> segments can undergo rupture during a single seismic event. Here, we employ Global Positioning <span class="hlt">System</span> (GPS) observations and geodetic modeling methods to create detailed images of coseismic slip and postseismic afterslip associated with the Kaikoura <span class="hlt">earthquake</span>. Our optimal geodetic coseismic model suggests that rupture not only occurred on shallow crustal <span class="hlt">faults</span> but also to some extent at the Hikurangi subduction interface. The GPS-inverted moment release during the <span class="hlt">earthquake</span> is equivalent to a Mw 7.9 event. The near-field postseismic deformation is mainly derived from right-lateral strike-slip motions on shallow crustal <span class="hlt">faults</span>. The afterslip did not only significantly extend northeastward on the Needles <span class="hlt">fault</span> but also appeared at the plate interface, slowly releasing energy over the past 6 months, equivalent to a Mw 7.3 <span class="hlt">earthquake</span>. Coulomb stress changes induced by coseismic deformation exhibit complex patterns and diversity at different depths, undoubtedly reflecting multi-<span class="hlt">fault</span> rupture complexity associated with the <span class="hlt">earthquake</span>. The Coulomb stress can reach several MPa during coseismic deformation, which can explain the trigger mechanisms of afterslip in two high-slip regions and the majority of aftershocks. Based on the deformation characteristics of the Kaikoura <span class="hlt">earthquake</span>, interseismic plate coverage, and historical <span class="hlt">earthquakes</span>, we conclude that Wellington is under higher seismic threat after the <span class="hlt">earthquake</span> and great attention should be paid to potential large <span class="hlt">earthquake</span> disasters in the near future.[Figure not available: see fulltext.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S33A2754M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S33A2754M"><span>Evidence of Multiple Ground-rupturing <span class="hlt">Earthquakes</span> in the Past 4000 Years along the Pasuruan <span class="hlt">Fault</span>, East Java, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marliyani, G. I.; Arrowsmith, R.; Helmi, H.</p> <p>2015-12-01</p> <p>Instrumental and historical records of <span class="hlt">earthquakes</span>, supplemented by paleoeseismic constraints can help reveal the <span class="hlt">earthquake</span> potential of an area. The Pasuruan <span class="hlt">fault</span> is a high angle normal <span class="hlt">fault</span> with prominent youthful scarps cutting young deltaic sediments in the north coast of East Java, Indonesia and may pose significant hazard to the densely populated region. This <span class="hlt">fault</span> has not been considered a significant structure, and mapped as a lineament with no sense of motion. Information regarding past <span class="hlt">earthquakes</span> along this <span class="hlt">fault</span> is not available. The <span class="hlt">fault</span> is well defined both in the imagery and in the field as a ~13km long, 2-50m-high scarp. Open and filled fractures and natural exposures of the south-dipping <span class="hlt">fault</span> plane indicate normal sense of motion. We excavated two <span class="hlt">fault</span>-perpendicular trenches across a relay ramp identified during our surface mapping. Evidence for past <span class="hlt">earthquakes</span> (documented in both trenches) includes upward <span class="hlt">fault</span> termination with associated fissure fills, colluvial wedges and scarp-derived debris, folding, and angular unconformities. The ages of the events are constrained by 23 radiocarbon dates on detrital charcoal. We calibrated the dates using IntCal13 and used Oxcal to build the age model of the events. Our preliminary age model indicates that since 2006±134 B.C., there has been at least five ground rupturing <span class="hlt">earthquakes</span> along the <span class="hlt">fault</span>. The oldest event identified in the trench however, is not well-dated. Our modeled 95th percentile ranges of the next four earlier <span class="hlt">earthquakes</span> (and their mean) are A.D. 1762-1850 (1806), A.D. 1646-1770 (1708), A.D. 1078-1648 (1363), and A.D. 726-1092 (909), yielding a rough recurrence rate of 302±63 yrs. These new data imply that Pasuruan <span class="hlt">fault</span> is more active than previously thought. Additional well-dated <span class="hlt">earthquakes</span> are necessary to build a solid <span class="hlt">earthquake</span> recurrence model. Rupture along the whole section implies a minimum <span class="hlt">earthquake</span> magnitude of 6.3, considering 13km as the minimum surface rupture</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70197944','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70197944"><span>2014 M=6.0 South Napa <span class="hlt">earthquake</span> triggered widespread aftershocks and stressed several major <span class="hlt">faults</span> and exotic <span class="hlt">fault</span> clusters</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Toda, Shinji; Stein, Ross</p> <p>2015-01-01</p> <p>The strongest San Francisco Bay area <span class="hlt">earthquake</span> since the 1989 Mw 7.0 Loma Prieta shock struck near Napa on 24 August 2014. Field mapping (Dawson et al., 2014; <span class="hlt">Earthquake</span> Engineering Research Institute [EERI], 2014; Brocher et al., 2015) and seismic and geodetic source inversions (Barnhart et al., 2015; Dreger et al., 2015; Wei et al., 2015) indicate that a 15-km-long northwest-trending section of the West Napa Valley <span class="hlt">fault</span> ruptured in the <span class="hlt">earthquake</span>. Remarkably, it was the first indisputable surface rupture in the Bay area since 1906. The Napa event, along with other smaller <span class="hlt">earthquakes</span> such as the 1980 Mw 5.8 Livermore and 1984 Mw 6.2 Morgan Hill events on the Calaveras and Hayward <span class="hlt">faults</span> over the past 3–4 decades, may indicate that the Bay area region is emerging from the stress shadow of the 1906 Mw 7.8 San Francisco <span class="hlt">earthquake</span> (Harris and Simpson, 1998; Pollitz et al., 2004). Since 1979, there has been a 140% increase in the rate of Mw≥4.1 shocks (Fig. 1) in the broader Bay area, with most concentrated in a corridor extending north from the 1989 Loma Prieta aftershock zone through the Calaveras, Greenville, Green Valley, Napa, and Rodgers Creek <span class="hlt">faults</span> east of the San Francisco Bay (Fig. 1a). This corridor roughly coincides with the 1906 stress shadow that is being eroded away by more than a century of stress reaccumulation. The Napa event, as well as the surrounding <span class="hlt">faults</span> on which we calculate the resulting hazard increases, all lie within this zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JSG....32.1046W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JSG....32.1046W"><span>Active <span class="hlt">faulting</span>, <span class="hlt">earthquakes</span>, and restraining bend development near Kerman city in southeastern Iran</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walker, Richard Thomas; Talebian, Morteza; Saiffori, Sohei; Sloan, Robert Alastair; Rasheedi, Ali; MacBean, Natasha; Ghassemi, Abbas</p> <p>2010-08-01</p> <p>We provide descriptions of strike-slip and reverse <span class="hlt">faulting</span>, active within the late Quaternary, in the vicinity of Kerman city in southeastern Iran. The <span class="hlt">faults</span> accommodate north-south, right-lateral, shear between central Iran and the Dasht-e-Lut depression. The regions that we describe have been subject to numerous <span class="hlt">earthquakes</span> in the historical and instrumental periods, and many of the <span class="hlt">faults</span> that are documented in this paper constitute hazards for local populations, including the city of Kerman itself (population ˜200,000). <span class="hlt">Faults</span> to the north and east of Kerman are associated with the transfer of slip from the Gowk to the Kuh Banan right-lateral <span class="hlt">faults</span> across a 40 km-wide restraining bend. <span class="hlt">Faults</span> south and west of the city are associated with oblique slip on the Mahan and Jorjafk <span class="hlt">systems</span>. The patterns of <span class="hlt">faulting</span> observed along the Mahan-Jorjafk <span class="hlt">system</span>, the Gowk-Kuh Banan <span class="hlt">system</span>, and also the Rafsanjan-Rayen <span class="hlt">system</span> further to the south, appear to preserve different stages in the development of these oblique-slip <span class="hlt">fault</span> <span class="hlt">systems</span>. We suggest that the <span class="hlt">faulting</span> evolves through time. Topography is initially generated on oblique slip <span class="hlt">faults</span> (as is seen on the Jorjafk <span class="hlt">fault</span>). The shortening component then migrates to reverse <span class="hlt">faults</span> situated away from the high topography whereas strike-slip continues to be accommodated in the high, mountainous, regions (as is seen, for example, on the Rafsanjan <span class="hlt">fault</span>). The reverse <span class="hlt">faults</span> may then link together and eventually evolve into new, through-going, strike-slip <span class="hlt">faults</span> in a process that appears to be occurring, at present, in the bend between the Gowk and Kuh Banan <span class="hlt">faults</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014458','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014458"><span>The growth of geological structures by repeated <span class="hlt">earthquakes</span>: 2, Field examples of continental dip-slip <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Stein, R.S.; King, G.C.P.; Rundle, J.B.</p> <p>1988-01-01</p> <p>A strong test of our understanding of the <span class="hlt">earthquake</span> cycle is the ability to reproduce extant faultbounded geological structures, such as basins and ranges, which are built by repeated cycles of deformation. Three examples are considered for which the structure and <span class="hlt">fault</span> geometry are well known: the White Wolf reverse <span class="hlt">fault</span> in California, site of the 1952 Kern County M=7.3 <span class="hlt">earthquake</span>, the Lost River normal <span class="hlt">fault</span> in Idaho, site of the 1983 Borah Peak M=7.0 <span class="hlt">earthquake</span>, and the Cricket Mountain normal <span class="hlt">fault</span> in Utah, site of Quaternary slip events. Basin stratigraphy and seismic reflection records are used to profile the structure, and coseismic deformation measured by leveling surveys is used to estimate the <span class="hlt">fault</span> geometry. To reproduce these structures, we add the deformation associated with the <span class="hlt">earthquake</span> cycle (the coseismic slip and postseismic relaxation) to the flexure caused by the observed sediment load, treating the crust as a thin elastic plate overlying a fluid substrate. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189854','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189854"><span>High-resolution seismic profiling reveals <span class="hlt">faulting</span> associated with the 1934 Ms 6.6 Hansel Valley <span class="hlt">earthquake</span> (Utah, USA)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bruno, Pier Paolo G.; Duross, Christopher; Kokkalas, Sotirios</p> <p>2017-01-01</p> <p>The 1934 Ms 6.6 Hansel Valley, Utah, <span class="hlt">earthquake</span> produced an 8-km-long by 3-km-wide zone of north-south−trending surface deformation in an extensional basin within the easternmost Basin and Range Province. Less than 0.5 m of purely vertical displacement was measured at the surface, although seismologic data suggest mostly strike-slip <span class="hlt">faulting</span> at depth. Characterization of the origin and kinematics of <span class="hlt">faulting</span> in the Hansel Valley <span class="hlt">earthquake</span> is important to understand how complex <span class="hlt">fault</span> ruptures accommodate regions of continental extension and transtension. Here, we address three questions: (1) How does the 1934 surface rupture compare with <span class="hlt">faults</span> in the subsurface? (2) Are the 1934 <span class="hlt">fault</span> scarps tectonic or secondary features? (3) Did the 1934 <span class="hlt">earthquake</span> have components of both strike-slip and dip-slip motion? To address these questions, we acquired a 6.6-km-long, high-resolution seismic profile across Hansel Valley, including the 1934 ruptures. We observed numerous east- and west-dipping normal <span class="hlt">faults</span> that dip 40°−70° and offset late Quaternary strata from within a few tens of meters of the surface down to a depth of ∼1 km. Spatial correspondence between the 1934 surface ruptures and subsurface <span class="hlt">faults</span> suggests that ruptures associated with the <span class="hlt">earthquake</span> are of tectonic origin. Our data clearly show complex basin <span class="hlt">faulting</span> that is most consistent with transtensional tectonics. Although the kinematics of the 1934 <span class="hlt">earthquake</span> remain underconstrained, we interpret the disagreement between surface (normal) and subsurface (strike-slip) kinematics as due to slip partitioning during <span class="hlt">fault</span> propagation and to the effect of preexisting structural complexities. We infer that the 1934 <span class="hlt">earthquake</span> occurred along an ∼3-km wide, off-<span class="hlt">fault</span> damage zone characterized by distributed deformation along small-displacement <span class="hlt">faults</span> that may be alternatively activated during different <span class="hlt">earthquake</span> episodes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....7478M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....7478M"><span><span class="hlt">Earthquake</span> geology along the North Anatoli <span class="hlt">Fault</span> Zone in the Marmara Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McHugh, C. M.; Cormier, M.-H.; Seeber, L.; Cagatay, M. N.; Capotondi, L.; Polonia, A.; Lozefski, G.</p> <p>2003-04-01</p> <p>The feasibility of conducting submarine <span class="hlt">earthquake</span> geology along the North Anatolia <span class="hlt">Fault</span> Zone (NAFZ) was evaluated from sediment cores and geophysical data (multibeam bathymetry and high-resolution CHIRP) recently collected from the Marmara Sea. We have successfully begun to characterize the Holocene <span class="hlt">earthquake</span> record of the NAFZ in a small basin along the Ganos <span class="hlt">fault</span> east of the Gelibolu peninsula, and in Izmit Gulf (west of the Hersek promontory and in the Karamürsel basin). Evidence for seismic activity was derived from mass-wasting and gravity flow deposits including homogenites (deposits >10cm thick containing turbidites with resuspended sediment above) identified from core x-rays, grain size, organic carbon, and mineralogical analyses. Deposits were correlated to the historical <span class="hlt">earthquake</span> record of the Marmara Sea region by chronology derived from 14C, 210Pb and 137Cs. The basin near Ganos is ideal for the study of <span class="hlt">earthquake</span>-related activity. It is deep (>50m), bisected by the <span class="hlt">fault</span>, and isolated from other basins and distal from fluvial and alluvial fan input that may include weather-related events. Yet, its sedimentation rates are very high (>2m/1000 years). Homogenites, have been tentatively correlated to the 1912 Ganos <span class="hlt">earthquake</span> and to the mid-1960's and mid-1800's Saros Gulf <span class="hlt">earthquakes</span>. The Ganos <span class="hlt">earthquake</span> ruptured the entire 50km long segment across the Gelibolu peninsula plus submarine portions on either side. If the timing of these events is correct, it suggests frequent seismic activity for this region. On the Gulf of Izmit, west of Hersek, sandy-mass flows containing soft sediment deformation such as recumbent folds and sand injections have been linked to the 1509 <span class="hlt">earthquake</span>. Historical records indicate that the segment of the NAFZ in the Hersek Peninsula ruptured during this <span class="hlt">earthquake</span> and our findings suggest that the rupture may have continued beneath the Izmit Gulf. In the eastern portion of the Karamürsel basin, sandy turbidites have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5893D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5893D"><span>Deformation of conjugate compliant <span class="hlt">fault</span> zones induced by the 2013 Mw7.7 Baluchistan (Pakistan) <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dutta, Rishabh; Wang, Teng; Feng, Guangcai; Harrington, Jonathan; Vasyura-Bathke, Hannes; Jónsson, Sigurjón</p> <p>2017-04-01</p> <p>Strain localizations in compliant <span class="hlt">fault</span> zones (with elastic moduli lower than the surrounding rocks) induced by nearby <span class="hlt">earthquakes</span> have been detected using geodetic observations in a few cases in the past. Here we observe small-scale changes in interferometric Synthetic Aperture Radar (InSAR) measurements along multiple conjugate <span class="hlt">faults</span> near the rupture of the 2013 Mw7.7 Baluchistan (Pakistan) <span class="hlt">earthquake</span>. After removing the main coseismic deformation signal in the interferograms and correcting them for topography-related phase, we observe 2-3 cm signal along several conjugate <span class="hlt">faults</span> that are 15-30 km from the mainshock <span class="hlt">fault</span> rupture. These conjugate compliant <span class="hlt">faults</span> have strikes of N30°E and N45°W. The sense of motion indicates left-lateral deformation across the N30°E <span class="hlt">faults</span> and right-lateral deformation across the N45°W <span class="hlt">faults</span>, which suggests the conjugate <span class="hlt">faults</span> were subjected to extensional coseismic stresses along the WSW-ENE direction. The spacing between the different sets of <span class="hlt">faults</span> is around 5 to 8 km. We explain the observed strain localizations as an elastic response of the compliant conjugate <span class="hlt">faults</span> induced by the Baluchistan <span class="hlt">earthquake</span>. Using 3D Finite Element models (FEM), we impose coseismic static displacements due to the <span class="hlt">earthquake</span> along the boundaries of the FEM domain to reproduce the coseismic stress changes acting across the compliant <span class="hlt">faults</span>. The InSAR measurements are used to constrain the geometry and rigidity variations of the compliant <span class="hlt">faults</span> with respect to the surrounding rocks. The best fitting models show the compliant <span class="hlt">fault</span> zones to have a width of 0.5 km to 2 km and a reduction of the shear modulus by a factor of 3 to 4. Our study yields similar values as were found for compliant <span class="hlt">fault</span> zones near the 1992 Landers and the 1999 Hector Mine <span class="hlt">earthquakes</span> in California, although here the strain localization is occurring on more complex conjugate sets of <span class="hlt">faults</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027562','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027562"><span>Viscoelasticity, postseismic slip, <span class="hlt">fault</span> interactions, and the recurrence of large <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Michael, A.J.</p> <p>2005-01-01</p> <p>The Brownian Passage Time (BPT) model for <span class="hlt">earthquake</span> recurrence is modified to include transient deformation due to either viscoelasticity or deep post seismic slip. Both of these processes act to increase the rate of loading on the seismogenic <span class="hlt">fault</span> for some time after a large event. To approximate these effects, a decaying exponential term is added to the BPT model's uniform loading term. The resulting interevent time distributions remain approximately lognormal, but the balance between the level of noise (e.g., unknown <span class="hlt">fault</span> interactions) and the coefficient of variability of the interevent time distribution changes depending on the shape of the loading function. For a given level of noise in the loading process, transient deformation has the effect of increasing the coefficient of variability of <span class="hlt">earthquake</span> interevent times. Conversely, the level of noise needed to achieve a given level of variability is reduced when transient deformation is included. Using less noise would then increase the effect of known <span class="hlt">fault</span> interactions modeled as stress or strain steps because they would be larger with respect to the noise. If we only seek to estimate the shape of the interevent time distribution from observed <span class="hlt">earthquake</span> occurrences, then the use of a transient deformation model will not dramatically change the results of a probability study because a similar shaped distribution can be achieved with either uniform or transient loading functions. However, if the goal is to estimate <span class="hlt">earthquake</span> probabilities based on our increasing understanding of the seismogenic process, including <span class="hlt">earthquake</span> interactions, then including transient deformation is important to obtain accurate results. For example, a loading curve based on the 1906 <span class="hlt">earthquake</span>, paleoseismic observations of prior events, and observations of recent deformation in the San Francisco Bay region produces a 40% greater variability in <span class="hlt">earthquake</span> recurrence than a uniform loading model with the same noise level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/fs-096-03/pdf/fs-096-03.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/fs-096-03/pdf/fs-096-03.pdf"><span><span class="hlt">Earthquakes</span>-Rattling the Earth's Plumbing <span class="hlt">System</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sneed, Michelle; Galloway, Devin L.; Cunningham, William L.</p> <p>2003-01-01</p> <p>Hydrogeologic responses to <span class="hlt">earthquakes</span> have been known for decades, and have occurred both close to, and thousands of miles from <span class="hlt">earthquake</span> epicenters. Water wells have become turbid, dry or begun flowing, discharge of springs and ground water to streams has increased and new springs have formed, and well and surface-water quality have become degraded as a result of <span class="hlt">earthquakes</span>. <span class="hlt">Earthquakes</span> affect our Earth’s intricate plumbing system—whether you live near the notoriously active San Andreas <span class="hlt">Fault</span> in California, or far from active <span class="hlt">faults</span> in Florida, an <span class="hlt">earthquake</span> near or far can affect you and the water resources you depend on.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000GeoJI.141...43B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000GeoJI.141...43B"><span>Effects induced by an <span class="hlt">earthquake</span> on its <span class="hlt">fault</span> plane:a boundary element study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonafede, Maurizio; Neri, Andrea</p> <p>2000-04-01</p> <p>Mechanical effects left by a model <span class="hlt">earthquake</span> on its <span class="hlt">fault</span> plane, in the post-seismic phase, are investigated employing the `displacement discontinuity method'. Simple crack models, characterized by the release of a constant, unidirectional shear traction are investigated first. Both slip components-parallel and normal to the traction direction-are found to be non-vanishing and to depend on <span class="hlt">fault</span> depth, dip, aspect ratio and <span class="hlt">fault</span> plane geometry. The rake of the slip vector is similarly found to depend on depth and dip. The <span class="hlt">fault</span> plane is found to suffer some small rotation and bending, which may be responsible for the indentation of a transform tectonic margin, particularly if cumulative effects are considered. Very significant normal stress components are left over the shallow portion of the <span class="hlt">fault</span> surface after an <span class="hlt">earthquake</span>: these are tensile for thrust <span class="hlt">faults</span>, compressive for normal <span class="hlt">faults</span> and are typically comparable in size to the stress drop. These normal stresses can easily be computed for more realistic seismic source models, in which a variable slip is assigned; normal stresses are induced in these cases too, and positive shear stresses may even be induced on the <span class="hlt">fault</span> plane in regions of high slip gradient. Several observations can be explained from the present model: low-dip thrust <span class="hlt">faults</span> and high-dip normal <span class="hlt">faults</span> are found to be facilitated, according to the Coulomb failure criterion, in repetitive <span class="hlt">earthquake</span> cycles; the shape of dip-slip <span class="hlt">faults</span> near the surface is predicted to be upward-concave; and the shallower aftershock activity generally found in the hanging block of a thrust event can be explained by `unclamping' mechanisms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JAESc..96..123M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JAESc..96..123M"><span>Detailed <span class="hlt">fault</span> structure of the Tarutung Pull-Apart Basin in Sumatra, Indonesia, derived from local <span class="hlt">earthquake</span> data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muksin, Umar; Haberland, Christian; Nukman, Mochamad; Bauer, Klaus; Weber, Michael</p> <p>2014-12-01</p> <p>The Tarutung Basin is located at a right step-over in the northern central segment of the dextral strike-slip Sumatran <span class="hlt">Fault</span> <span class="hlt">System</span> (SFS). Details of the <span class="hlt">fault</span> structure along the Tarutung Basin are derived from the relocations of seismicity as well as from focal mechanism and structural geology. The seismicity distribution derived by a 3D inversion for hypocenter relocation is clustered according to a <span class="hlt">fault</span>-like seismicity distribution. The seismicity is relocated with a double-difference technique (HYPODD) involving the waveform cross-correlations. We used 46,904 and 3191 arrival differences obtained from catalogue data and cross-correlation analysis, respectively. Focal mechanisms of events were analyzed by applying a grid search method (HASH code). Although there is no significant shift of the hypocenters (10.8 m in average) and centroids (167 m in average), the application of the double difference relocation sharpens the <span class="hlt">earthquake</span> distribution. The <span class="hlt">earthquake</span> lineation reflects the <span class="hlt">fault</span> <span class="hlt">system</span>, the extensional duplex <span class="hlt">fault</span> <span class="hlt">system</span>, and the negative flower structure within the Tarutung Basin. The focal mechanisms of events at the edge of the basin are dominantly of strike-slip type representing the dextral strike-slip Sumatran <span class="hlt">Fault</span> <span class="hlt">System</span>. The almost north-south striking normal <span class="hlt">fault</span> events along extensional zones beneath the basin correlate with the maximum principal stress direction which is the direction of the Indo-Australian plate motion. The extensional zones form an en-echelon pattern indicated by the presence of strike-slip <span class="hlt">faults</span> striking NE-SW to NW-SE events. The detailed characteristics of the <span class="hlt">fault</span> <span class="hlt">system</span> derived from the seismological study are also corroborated by structural geology at the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNS33A0041D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNS33A0041D"><span>Fracture Modes and Identification of <span class="hlt">Fault</span> Zones in Wenchuan <span class="hlt">Earthquake</span> <span class="hlt">Fault</span> Scientific Drilling Boreholes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deng, C.; Pan, H.; Zhao, P.; Qin, R.; Peng, L.</p> <p>2017-12-01</p> <p>After suffering from the disaster of Wenchuan <span class="hlt">earthquake</span> on May 12th, 2008, scientists are eager to figure out the structure of formation, the geodynamic processes of <span class="hlt">faults</span> and the mechanism of <span class="hlt">earthquake</span> in Wenchuan by drilling five holes into the Yingxiu-Beichuan <span class="hlt">fault</span> zone and Anxian-Guanxian <span class="hlt">fault</span> zone. Fractures identification and in-situ stress determination can provide abundant information for formation evaluation and <span class="hlt">earthquake</span> study. This study describe all the fracture modes in the five boreholes on the basis of cores and image logs, and summarize the response characteristics of fractures in conventional logs. The results indicate that the WFSD boreholes encounter enormous fractures, including natural fractures and induced fractures, and high dip-angle conductive fractures are the most common fractures. The maximum horizontal stress trends along the borehole are deduced as NWW-SEE according to orientations of borehole breakouts and drilling-induced fractures, which is nearly parallel to the strikes of the younger natural fracture sets. Minor positive deviations of AC (acoustic log) and negative deviation of DEN (density log) demonstrate their responses to fracture, followed by CNL (neutron log), resistivity logs and GR (gamma ray log) at different extent of intensity. Besides, considering the fact that the reliable methods for identifying fracture zone, like seismic, core recovery and image logs, can often be hampered by their high cost and limited application, this study propose a method by using conventional logs, which are low-cost and available in even old wells. We employ wavelet decomposition to extract the high frequency information of conventional logs and reconstruction a new log in special format of enhance fracture responses and eliminate nonfracture influence. Results reveal that the new log shows obvious deviations in <span class="hlt">fault</span> zones, which confirm the potential of conventional logs in fracture zone identification.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17738534','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17738534"><span><span class="hlt">Earthquake</span> Swarm Along the San Andreas <span class="hlt">Fault</span> near Palmdale, Southern California, 1976 to 1977.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McNally, K C; Kanamori, H; Pechmann, J C; Fuis, G</p> <p>1978-09-01</p> <p>Between November 1976 and November 1977 a swarm of small <span class="hlt">earthquakes</span> (local magnitude </= 3) occurred on or near the San Andreas <span class="hlt">fault</span> near Palmdale, California. This swarm was the first observed along this section of the San Andreas since cataloging of instrumental data began in 1932. The activity followed partial subsidence of the 35-centimeter vertical crustal uplift known as the Palmdale bulge along this "locked" section of the San Andreas, which last broke in the great (surface-wave magnitude = 8(1/4)+) 1857 Fort Tejon <span class="hlt">earthquake</span>. The swarm events exhibit characteristics previously observed for some foreshock sequences, such as tight clustering of hypocenters and time-dependent rotations of stress axes inferred from focal mechanisms. However, because of our present lack of understanding of the processes that precede <span class="hlt">earthquake</span> <span class="hlt">faulting</span>, the implications of the swarm for future large <span class="hlt">earthquakes</span> on the San Andreas <span class="hlt">fault</span> are unknown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012399','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012399"><span><span class="hlt">Earthquake</span> swarm along the San Andreas <span class="hlt">fault</span> near Palmdale, Southern California, 1976 to 1977</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mcnally, K.C.; Kanamori, H.; Pechmann, J.C.; Fuis, G.</p> <p>1978-01-01</p> <p>Between November 1976 and November 1977 a swarm of small <span class="hlt">earthquakes</span> (local magnitude ??? 3) occurred on or near the San Andreas <span class="hlt">fault</span> near Palmdale, California. This swarm was the first observed along this section of the San Andreas since cataloging of instrumental data began in 1932. The activity followed partial subsidence of the 35-centimeter vertical crustal uplift known as the Palmdale bulge along this "locked" section of the San Andreas, which last broke in the great (surface-wave magnitude = 81/4+) 1857 Fort Tejon <span class="hlt">earthquake</span>. The swarm events exhibit characteristics previously observed for some foreshock sequences, such as tight clustering of hypocenters and time-dependent rotations of stress axes inferred from focal mechanisms. However, because of our present lack of understanding of the processes that precede <span class="hlt">earthquake</span> <span class="hlt">faulting</span>, the implications of the swarm for future large <span class="hlt">earthquakes</span> on the San Andreas <span class="hlt">fault</span> are unknown. Copyright ?? 1978 AAAS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031643','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031643"><span>The most recent large <span class="hlt">earthquake</span> on the Rodgers Creek <span class="hlt">fault</span>, San Francisco bay area</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hecker, S.; Pantosti, D.; Schwartz, D.P.; Hamilton, J.C.; Reidy, L.M.; Powers, T.J.</p> <p>2005-01-01</p> <p>The Rodgers Creek <span class="hlt">fault</span> (RCF) is a principal component of the San Andreas <span class="hlt">fault</span> <span class="hlt">system</span> north of San Francisco. No evidence appears in the historical record of a large <span class="hlt">earthquake</span> on the RCF, implying that the most recent <span class="hlt">earthquake</span> (MRE) occurred before 1824, when a Franciscan mission was built near the <span class="hlt">fault</span> at Sonoma, and probably before 1776, when a mission and presidio were built in San Francisco. The first appearance of nonnative pollen in the stratigraphic record at the Triangle G Ranch study site on the south-central reach of the RCF confirms that the MRE occurred before local settlement and the beginning of livestock grazing. Chronological modeling of <span class="hlt">earthquake</span> age using radiocarbon-dated charcoal from near the top of a <span class="hlt">faulted</span> alluvial sequence at the site indicates that the MRE occurred no earlier than A.D. 1690 and most likely occurred after A.D. 1715. With these age constraints, we know that the elapsed time since the MRE on the RCF is more than 181 years and less than 315 years and is probably between 229 and 290 years. This elapsed time is similar to published recurrence-interval estimates of 131 to 370 years (preferred value of 230 years) and 136 to 345 years (mean of 205 years), calculated from geologic data and a regional <span class="hlt">earthquake</span> model, respectively. Importantly, then, the elapsed time may have reached or exceeded the average recurrence time for the <span class="hlt">fault</span>. The age of the MRE on the RCF is similar to the age of prehistoric surface rupture on the northern and southern sections of the Hayward <span class="hlt">fault</span> to the south. This suggests possible rupture scenarios that involve simultaneous rupture of the Rodgers Creek and Hayward <span class="hlt">faults</span>. A buried channel is offset 2.2 (+ 1.2, - 0.8) m along one side of a pressure ridge at the Triangle G Ranch site. This provides a minimum estimate of right-lateral slip during the MRE at this location. Total slip at the site may be similar to, but is probably greater than, the 2 (+ 0.3, - 0.2) m measured previously at the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRB..119.6650C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRB..119.6650C"><span>Active <span class="hlt">faulting</span> in apparently stable peninsular India: Rift inversion and a Holocene-age great <span class="hlt">earthquake</span> on the Tapti <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Copley, Alex; Mitra, Supriyo; Sloan, R. Alastair; Gaonkar, Sharad; Reynolds, Kirsty</p> <p>2014-08-01</p> <p>We present observations of active <span class="hlt">faulting</span> within peninsular India, far from the surrounding plate boundaries. Offset alluvial fan surfaces indicate one or more magnitude 7.6-8.4 thrust-<span class="hlt">faulting</span> <span class="hlt">earthquakes</span> on the Tapti <span class="hlt">Fault</span> (Maharashtra, western India) during the Holocene. The high ratio of <span class="hlt">fault</span> displacement to length on the alluvial fan offsets implies high stress-drop <span class="hlt">faulting</span>, as has been observed elsewhere in the peninsula. The along-strike extent of the fan offsets is similar to the thickness of the seismogenic layer, suggesting a roughly equidimensional <span class="hlt">fault</span> rupture. The subsiding footwall of the <span class="hlt">fault</span> is likely to have been responsible for altering the continental-scale drainage pattern in central India and creating the large west flowing catchment of the Tapti river. A preexisting sedimentary basin in the uplifting hanging wall implies that the Tapti <span class="hlt">Fault</span> was active as a normal <span class="hlt">fault</span> during the Mesozoic and has been reactivated as a thrust, highlighting the role of preexisting structures in determining the rheology and deformation of the lithosphere. The slip sense of <span class="hlt">faults</span> and <span class="hlt">earthquakes</span> in India suggests that deformation south of the Ganges foreland basin is driven by the compressive force transmitted between India and the Tibetan Plateau. The along-strike continuation of <span class="hlt">faulting</span> to the east of the Holocene ruptures we have studied represents a significant seismic hazard in central India.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020550','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020550"><span>Absence of <span class="hlt">earthquake</span> correlation with Earth tides: An indication of high preseismic <span class="hlt">fault</span> stress rate</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Vidale, J.E.; Agnew, D.C.; Johnston, M.J.S.; Oppenheimer, D.H.</p> <p>1998-01-01</p> <p>Because the rate of stress change from the Earth tides exceeds that from tectonic stress accumulation, tidal triggering of <span class="hlt">earthquakes</span> would be expected if the final hours of loading of the <span class="hlt">fault</span> were at the tectonic rate and if rupture began soon after the achievement of a critical stress level. We analyze the tidal stresses and stress rates on the <span class="hlt">fault</span> planes and at the times of 13,042 <span class="hlt">earthquakes</span> which are so close to the San Andreas and Calaveras <span class="hlt">faults</span> in California that we may take the <span class="hlt">fault</span> plane to be known. We find that the stresses and stress rates from Earth tides at the times of <span class="hlt">earthquakes</span> are distributed in the same way as tidal stresses and stress rates at random times. While the rate of <span class="hlt">earthquakes</span> when the tidal stress promotes failure is 2% higher than when the stress does not, this difference in rate is not statistically significant. This lack of tidal triggering implies that preseismic stress rates in the nucleation zones of <span class="hlt">earthquakes</span> are at least 0.15 bar/h just preceding seismic failure, much above the long-term tectonic stress rate of 10-4 bar/h.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019787','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019787"><span>Geophysical setting of the Wabash Valley <span class="hlt">fault</span> <span class="hlt">system</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hildenbrand, T.G.; Ravat, D.</p> <p>1997-01-01</p> <p>Interpretation of existing regional magnetic and gravity data and new local high-resolution aeromagnetic data provides new insights on the tectonic history and structural development of the Wabash Valley <span class="hlt">Fault</span> <span class="hlt">System</span> in Illinois and Indiana. Enhancement of short-wavelength magnetic anomalies reveal numerous NW- to NNE-trending ultramafic dikes and six intrusive complexes (including those at Hicks Dome and Omaha Dome). Inversion models indicate that the interpreted dikes are narrow (???3 m), lie at shallow depths (500 km long and generally >50 km wide) and with deep basins (locally >3 km thick), the ancestral Wabash Valley <span class="hlt">faults</span> express, in comparison, minor tectonic structures and probably do not represent a failed rift arm. There is a lack of any obvious relation between the Wabash Valley <span class="hlt">Fault</span> <span class="hlt">System</span> and the epicenters of historic and prehistoric <span class="hlt">earthquakes</span>. Five prehistoric <span class="hlt">earthquakes</span> lie conspicuously near structures associated with the Commerce geophysical lineament, a NE-trending magnetic and gravity lineament lying oblique to the Wabash Valley <span class="hlt">Fault</span> <span class="hlt">System</span> and possibly extending over 600 km from NE Arkansas to central Indiana.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S44C..03E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S44C..03E"><span>Magnetotelluric Studies of <span class="hlt">Fault</span> Zones Surrounding the 2016 Pawnee, Oklahoma <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Evans, R. L.; Key, K.; Atekwana, E. A.</p> <p>2016-12-01</p> <p>Since 2008, there has been a dramatic increase in <span class="hlt">earthquake</span> activity in the central United States in association with major oil and gas operations. Oklahoma is now considered one the most seismically active states. Although seismic networks are able to detect activity and map its locus, they are unable to image the distribution of fluids in the <span class="hlt">fault</span> responsible for triggering seismicity. Electrical geophysical methods are ideally suited to image fluid bearing <span class="hlt">faults</span> since the injected waste-waters are highly saline and hence have a high electrical conductivity. To date, no study has imaged the fluids in the <span class="hlt">faults</span> in Oklahoma and made a direct link to the seismicity. The 2016 M5.8 Pawnee, Oklahoma <span class="hlt">earthquake</span> provides an unprecedented opportunity for scientists to provide that link. Several injection wells are located within a 20 km radius of the epicenter; and studies have suggested that injection of fluids in high-volume wells can trigger <span class="hlt">earthquakes</span> as far away as 30 km. During late October to early November, 2016, we are collecting magnetotelluric (MT) data with the aim of constraining the distribution of fluids in the <span class="hlt">fault</span> zone. The MT technique uses naturally occurring electric and magnetic fields measured at Earth's surface to measure conductivity structure. We plan to carry out a series of short two-dimensional (2D) profiles of wideband MT acquisition located through areas where the <span class="hlt">fault</span> recently ruptured and seismic activity is concentrated and also across the <span class="hlt">faults</span> in the vicinity that did not rupture. The integration of our results and ongoing seismic studies will lead to a better understanding of the links between fluid injection and seismicity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019068','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019068"><span>An <span class="hlt">earthquake</span> instability model based on <span class="hlt">faults</span> containing high fluid-pressure compartments</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lockner, D.A.; Byerlee, J.D.</p> <p>1995-01-01</p> <p>It has been proposed that large strike-slip <span class="hlt">faults</span> such as the San Andreas contain water in seal-bounded compartments. Arguments based on heat flow and stress orientation suggest that in most of the compartments, the water pressure is so high that the average shear strength of the <span class="hlt">fault</span> is less than 20 MPa. We propose a variation of this basic model in which most of the shear stress on the <span class="hlt">fault</span> is supported by a small number of compartments where the pore pressure is relatively low. As a result, the <span class="hlt">fault</span> gouge in these compartments is compacted and lithified and has a high undisturbed strength. When one of these locked regions fails, the <span class="hlt">system</span> made up of the neighboring high and low pressure compartments can become unstable. Material in the high fluid pressure compartments is initially underconsolidated since the low effective confining pressure has retarded compaction. As these compartments are deformed, fluid pressure remains nearly unchanged so that they offer little resistance to shear. The low pore pressure compartments, however, are overconsolidated and dilate as they are sheared. Decompression of the pore fluid in these compartments lowers fluid pressure, increasing effective normal stress and shear strength. While this effect tends to stabilize the <span class="hlt">fault</span>, it can be shown that this dilatancy hardening can be more than offset by displacement weakening of the <span class="hlt">fault</span> (i.e., the drop from peak to residual strength). If the surrounding rock mass is sufficiently compliant to produce an instability, slip will propagate along the <span class="hlt">fault</span> until the shear fracture runs into a low-stress region. Frictional heating and the accompanying increase in fluid pressure that are suggested to occur during shearing of the <span class="hlt">fault</span> zone will act as additional destabilizers. However, significant heating occurs only after a finite amount of slip and therefore is more likely to contribute to the energetics of rupture propagation than to the initiation of the instability. We present</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911966S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911966S"><span>Three dimensional modelling of <span class="hlt">earthquake</span> rupture cycles on frictional <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Simpson, Guy; May, Dave</p> <p>2017-04-01</p> <p>We are developing an efficient MPI-parallel numerical method to simulate <span class="hlt">earthquake</span> sequences on preexisting <span class="hlt">faults</span> embedding within a three dimensional viscoelastic half-space. We solve the velocity form of the elasto(visco)dynamic equations using a continuous Galerkin Finite Element Method on an unstructured pentahedral mesh, which thus permits local spatial refinement in the vicinity of the <span class="hlt">fault</span>. Friction sliding is coupled to the viscoelastic solid via rate- and state-dependent friction laws using the split-node technique. Our coupled formulation employs a picard-type non-linear solver with a fully implicit, first order accurate time integrator that utilises an adaptive time step that efficiently evolves the <span class="hlt">system</span> through multiple seismic cycles. The implementation leverages advanced parallel solvers, preconditioners and linear algebra from the Portable Extensible Toolkit for Scientific Computing (PETSc) library. The model can treat heterogeneous frictional properties and stress states on the <span class="hlt">fault</span> and surrounding solid as well as non-planar <span class="hlt">fault</span> geometries. Preliminary tests show that the model successfully reproduces dynamic rupture on a vertical strike-slip <span class="hlt">fault</span> in a half-space governed by rate-state friction with the ageing law.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027833','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027833"><span>Stress distribution along the Fairweather-Queen Charlotte transform <span class="hlt">fault</span> <span class="hlt">system</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bufe, C.G.</p> <p>2005-01-01</p> <p>Tectonic loading and Coulomb stress transfer are modeled along the right-lateral Fairweather-Queen Charlotte transform <span class="hlt">fault</span> <span class="hlt">system</span> using a threedimensional boundary element program. The loading model includes slip below 12 km along the transform as well as motion of the Pacific plate, and it is consistent with most available Global Positioning <span class="hlt">System</span> (GPS) displacement rate data. Coulomb stress transfer is shown to have been a weak contributing factor in the failure of the southeastern (Sitka) segment of the Fairweather <span class="hlt">fault</span> in 1972, hastening the occurrence of the <span class="hlt">earthquake</span> by only about 8 months. Failure of the Sitka segment was enhanced by a combination of cumulative loading from below (95%) by slip of about 5 cm/yr since 1848, by stress transfer (about 1%) from major <span class="hlt">earthquakes</span> on straddling segments of the Queen Charlotte <span class="hlt">fault</span> (M 8.1 in 1949) and the Fairweather <span class="hlt">fault</span> (M 7.8 in 1958), and by viscoelastic relaxation (about 4%) following the great 1964 Alaska <span class="hlt">earthquake</span>, modeled by Pollitz et al. (1998). Cumulative stress increases in excess of 7 MPa at a depth of 8 km are projected prior to the M 7.6 <span class="hlt">earthquake</span>. Coulomb stress transferred by the rupture of the great M 9.2 Alaska <span class="hlt">earthquake</span> in 1964 (Bufe, 2004a) also hastened the occurrence of the 1972 event, but only by a month or two. Continued tectonic loading over the last half century and stress transfer from the M 7.6 Sitka event has resulted in restressing of the adjacent segments by about 3 MPa at 8 km depth. The occurrence of a M 6.8 <span class="hlt">earthquake</span> on the northwestern part of the Queen Charlotte <span class="hlt">fault</span> on 28 June 2004, the largest since 1949, also suggests increased stress. The Cape St. James segment of the <span class="hlt">fault</span> immediately southeast of the 1949 Queen Charlotte rupture has accumulated about 6 MPa at 8 km through loading since 1900 and stress transfer in 1949. A continued rise in <span class="hlt">earthquake</span> hazard is indicated for the Alaska panhandle and Queen Charlotte Islands region in the decades ahead as the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.733...73Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.733...73Y"><span>Modeling <span class="hlt">earthquake</span> sequences along the Manila subduction zone: Effects of three-dimensional <span class="hlt">fault</span> geometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Hongyu; Liu, Yajing; Yang, Hongfeng; Ning, Jieyuan</p> <p>2018-05-01</p> <p>To assess the potential of catastrophic megathrust <span class="hlt">earthquakes</span> (MW > 8) along the Manila Trench, the eastern boundary of the South China Sea, we incorporate a 3D non-planar <span class="hlt">fault</span> geometry in the framework of rate-state friction to simulate <span class="hlt">earthquake</span> rupture sequences along the <span class="hlt">fault</span> segment between 15°N-19°N of northern Luzon. Our simulation results demonstrate that the first-order <span class="hlt">fault</span> geometry heterogeneity, the transitional-segment (possibly related to the subducting Scarborough seamount chain) connecting the steeper south segment and the flatter north segment, controls <span class="hlt">earthquake</span> rupture behaviors. The strong along-strike curvature at the transitional-segment typically leads to partial ruptures of MW 8.3 and MW 7.8 along the southern and northern segments respectively. The entire <span class="hlt">fault</span> occasionally ruptures in MW 8.8 events when the cumulative stress in the transitional-segment is sufficiently high to overcome the geometrical inhibition. <span class="hlt">Fault</span> shear stress evolution, represented by the S-ratio, is clearly modulated by the width of seismogenic zone (W). At a constant plate convergence rate, a larger W indicates on average lower interseismic stress loading rate and longer rupture recurrence period, and could slow down or sometimes stop ruptures that initiated from a narrower portion. Moreover, the modeled interseismic slip rate before whole-<span class="hlt">fault</span> rupture events is comparable with the coupling state that was inferred from the interplate seismicity distribution, suggesting the Manila trench could potentially rupture in a M8+ <span class="hlt">earthquake</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://geology.utah.gov/hazards/technical-information/paleoseismology-of-utah-series/','USGSPUBS'); return false;" href="https://geology.utah.gov/hazards/technical-information/paleoseismology-of-utah-series/"><span>Holocene surface-<span class="hlt">faulting</span> <span class="hlt">earthquakes</span> at the Spring Lake and North Creek Sites on the Wasatch <span class="hlt">Fault</span> Zone: Evidence for complex rupture of the Nephi Segment</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Duross, Christopher; Hylland, Michael D.; Hiscock, Adam; Personius, Stephen; Briggs, Richard; Gold, Ryan D.; Beukelman, Gregg; McDonald, Geg N; Erickson, Ben; McKean, Adam; Angster, Steve; King, Roselyn; Crone, Anthony J.; Mahan, Shannon</p> <p>2017-01-01</p> <p>The Nephi segment of the Wasatch <span class="hlt">fault</span> zone (WFZ) comprises two <span class="hlt">fault</span> strands, the northern and southern strands, which have evidence of recurrent late Holocene surface-<span class="hlt">faulting</span> <span class="hlt">earthquakes</span>. We excavated paleoseismic trenches across these strands to refine and expand their Holocene <span class="hlt">earthquake</span> chronologies; improve estimates of <span class="hlt">earthquake</span> recurrence, displacement, and <span class="hlt">fault</span> slip rate; and assess whether the strands rupture separately or synchronously in large <span class="hlt">earthquakes</span>. Paleoseismic data from the Spring Lake site expand the Holocene record of <span class="hlt">earthquakes</span> on the northern strand: at least five to seven <span class="hlt">earthquakes</span> ruptured the Spring Lake site at 0.9 ± 0.2 ka (2σ), 2.9 ± 0.7 ka, 4.0 ± 0.5 ka, 4.8 ± 0.8 ka, 5.7 ± 0.8 ka, 6.6 ± 0.7 ka, and 13.1 ± 4.0 ka, yielding a Holocene mean recurrence of ~1.2–1.5 kyr and vertical slip rate of ~0.5–0.8 mm/yr. Paleoseismic data from the North Creek site help refine the Holocene <span class="hlt">earthquake</span> chronology for the southern strand: at least five <span class="hlt">earthquakes</span> ruptured the North Creek site at 0.2 ± 0.1 ka (2σ), 1.2 ± 0.1 ka, 2.6 ± 0.9 ka, 4.0 ± 0.1 ka, and 4.7 ± 0.7 ka, yielding a mean recurrence of 1.1–1.3 kyr and vertical slip rate of ~1.9–2.0 mm/yr. We compare these Spring Lake and North Creek data with previous paleoseismic data for the Nephi segment and report late Holocene mean recurrence intervals of ~1.0–1.2 kyr for the northern strand and ~1.1–1.3 kyr for the southern strand. The northern and southern strands have similar late Holocene <span class="hlt">earthquake</span> histories, which allow for models of both independent and synchronous rupture. However, considering the <span class="hlt">earthquake</span> timing probabilities and per-event vertical displacements, we have the greatest confidence in the simultaneous rupture of the strands, including rupture of one strand with spillover rupture to the other. Ultimately, our results improve the surface-<span class="hlt">faulting</span> <span class="hlt">earthquake</span> history of the Nephi segment and enhance our understanding of how structural barriers</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JAESc..64..125Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JAESc..64..125Y"><span>Nonlinear dynamic failure process of tunnel-<span class="hlt">fault</span> <span class="hlt">system</span> in response to strong seismic event</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Zhihua; Lan, Hengxing; Zhang, Yongshuang; Gao, Xing; Li, Langping</p> <p>2013-03-01</p> <p>Strong <span class="hlt">earthquakes</span> and <span class="hlt">faults</span> have significant effect on the stability capability of underground tunnel structures. This study used a 3-Dimensional Discrete Element model and the real records of ground motion in the Wenchuan <span class="hlt">earthquake</span> to investigate the dynamic response of tunnel-<span class="hlt">fault</span> <span class="hlt">system</span>. The typical tunnel-<span class="hlt">fault</span> <span class="hlt">system</span> was composed of one planned railway tunnel and one seismically active <span class="hlt">fault</span>. The discrete numerical model was prudentially calibrated by means of the comparison between the field survey and numerical results of ground motion. It was then used to examine the detailed quantitative information on the dynamic response characteristics of tunnel-<span class="hlt">fault</span> <span class="hlt">system</span>, including stress distribution, strain, vibration velocity and tunnel failure process. The intensive tunnel-<span class="hlt">fault</span> interaction during seismic loading induces the dramatic stress redistribution and stress concentration in the intersection of tunnel and <span class="hlt">fault</span>. The tunnel-<span class="hlt">fault</span> <span class="hlt">system</span> behavior is characterized by the complicated nonlinear dynamic failure process in response to a real strong seismic event. It can be qualitatively divided into 5 main stages in terms of its stress, strain and rupturing behaviors: (1) strain localization, (2) rupture initiation, (3) rupture acceleration, (4) spontaneous rupture growth and (5) stabilization. This study provides the insight into the further stability estimation of underground tunnel structures under the combined effect of strong <span class="hlt">earthquakes</span> and <span class="hlt">faults</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S11B0570A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S11B0570A"><span><span class="hlt">Earthquake</span> bursts and <span class="hlt">fault</span> branching: lessons from the Carmel <span class="hlt">fault</span> branch (CFB) of the Dead Sea Transform (DST)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Agnon, A.; Rockwell, T. K.; Stein, S.; Raphael, K.</p> <p>2017-12-01</p> <p>The DST, accommodating most of the displacement across the boundary zone between the Arabian and Sinai plates, is an ideal plate boundary on which to study <span class="hlt">earthquake</span> sequences because of 1) a long (>2 kyr) record of historical <span class="hlt">earthquakes</span> (corroborated and extended several millennia back with ancient ruins); 2) deformed sediments and rockfalls, offering datable archives of strong shaking at various distances from the <span class="hlt">fault</span>, spanning 300 kyr; 3) a moderate <span class="hlt">fault</span> slip rate, allowing separation and dating of individual <span class="hlt">earthquakes</span> for comparison to the historical record, and 4) a growing body of paleoseismic trench data on both timing and displacement across some sectors of the <span class="hlt">fault</span>. Here we explore the role of a secondary <span class="hlt">fault</span> branch on clustering using a new approach for the analysis of <span class="hlt">earthquake</span> bursts. The CFZ is a ≥100 km long shear zone, branching northwestward from the N-S trending Jordan Valley segment of the DST. GPS monitoring of the CFZ indicates a slip rate of <1 mm/yr, absorbing up to 20% of the slip between Arabia Plate and the Sinai-Levant Block across the DST. CFZ seismicity is recorded by three datasets with different time scales and maximum magnitudes: 1) Instrumental seismicity, M≤5.3 (1984); 2) Historic documents suggesting a M>6 event in 363 CE, with ruins distributed up to 100 km from the CFZ; 3) 5 ka cave deposits showing damage greater than from any subsequent <span class="hlt">earthquake</span>, implying 6The CFZ branch events interact with ruptures on the main DST. At 5 ka destruction was widespread along the DST. The 363 CE <span class="hlt">earthquake</span> was accompanied by another event in the Arava Valley. The pair skipped the 100 km long Dead Sea segment of the DST. An earlier pair in the northern Levant preceded that pair by several decades: 303 & 347 CE, following a two-century long quiescence, and a harbinger for a shaky millennium. We suggest that the 363 CE pair reflects a rare state that enables a CFZ rupture. This oblique branch is unfavorably oriented for slip under</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U33A..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U33A..02S"><span>My Road to Transform <span class="hlt">Faulting</span> 1963; Long-Term Precursors to Recent Great <span class="hlt">Earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sykes, L. R.</p> <p>2017-12-01</p> <p>My road to plate tectonics started serendipitously in 1963 in a remote area of the southeast Pacific when I was studying the propagation of short-period seismic surface waves for my PhD. The <span class="hlt">earthquakes</span> I used as sources were poorly located. I discovered that my relocated epicenters followed the crest of the East Pacific Rise but then suddenly took a sharp turn to the east at what I interpreted to be a major fracture zone 1000 km long before turning again to the north near 55 degrees south. I noted that <span class="hlt">earthquakes</span> along that zone only occurred between the two ridge crests, an observation Tuzo Wilson used to develop his hypothesis of transform <span class="hlt">faulting</span>. Finding a great, unknown fracture zone led me to conclude that work on similar <span class="hlt">faults</span> that intersect the Mid-Oceanic Ridge <span class="hlt">System</span> was more important than my study of surface waves. I found similar great <span class="hlt">faults</span> over the next two years and obtained refined locations of <span class="hlt">earthquakes</span> along several island arcs. When I was in Fiji and Tonga during 1965 studying deep <span class="hlt">earthquakes</span>, James Dorman wrote to me about Wilson's paper and I thought about testing his hypothesis. I started work on it the spring of 1966 immediately after I learned about the symmetrical "magic magnetic anomaly profile" across the East Pacific Rise of Pitman and Heirtzler. I quickly obtained <span class="hlt">earthquake</span> mechanisms that verified the transform hypothesis and its related concepts of seafloor spreading and continental drift. As an undergraduate in the late 1950s, my mentor told me that respectable young earth scientists should not work on vague and false mobilistic concepts like continental drift since continents cannot plow through strong oceanic crust. Hence, until spring 1966, I did not take continental drift seriously. The second part of my presentation involves new evidence from seismology and GPS of what appear to be long-term precursors to a number of great <span class="hlt">earthquakes</span> of the past decade.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S31B2732X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S31B2732X"><span>Pore pressure may control rupture propagation of the 2001 Mw=7.8 Kokoxili <span class="hlt">earthquake</span> from the Kunlun <span class="hlt">fault</span> to the Kunlun Pass <span class="hlt">fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, J.; Wang, W.; He, J.</p> <p>2016-12-01</p> <p>The 2001 Mw=7.8 Kokoxili <span class="hlt">earthquake</span> nucleated on the west-east tending Kunlun strike-slip <span class="hlt">fault</span> in center of the Tibetan plateau. When the rupture propagated eastward near the Xidatan segment of the Kunlun <span class="hlt">fault</span>, this <span class="hlt">earthquake</span> jumped to the Kunlun Pass <span class="hlt">fault</span>, a less matured <span class="hlt">fault</span> that, due to the geometric orientation, was obviously clamped by the coseismic deformation before its rupture. To investigate the possible mechanism for the rupture jump, we updated the coseismic rupture model from a joint inversion of the geological, geodetic and seismic wave data. Constrained with the rupture process, a three-dimensional finite element model was developed to calculate the failure stress from elastic and poroelastic deformation of the crust during the rupture propagation. Results show that just before the rupture reached the conjunction of the Xidatan segment and the Kunlun Pass <span class="hlt">fault</span>, the failure stress induced by elastic deformation is indeed larger on Xidatan segment of the Kunlun <span class="hlt">fault</span> than on the Kunlun Pass <span class="hlt">fault</span>. However, if the pore pressure resulted from undrained poroelastic deformation was invoked, the failure stress is significantly increased on the Kunlun Pass <span class="hlt">fault</span>. Given a reasonable bound on <span class="hlt">fault</span> friction and on poroelastic parameters, it can be seen that the poroelastic failure stress is 0.3-0.9 Mpa greater on the Kunlun Pass <span class="hlt">fault</span> than on Xidatan segment of the Kunlun <span class="hlt">fault</span>. We therefore argue that during the rupture process of the 2001 Mw=7.8 Kokoxili <span class="hlt">earthquake</span>, pore pressure may play an important role on controlling the rupture propagation from the Kunlun <span class="hlt">fault</span> to the Kunlun Pass <span class="hlt">fault</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T24A..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T24A..05M"><span>Influence of <span class="hlt">fault</span> geometry and tectonic driving stress orientation on the mechanics of multifault <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Madden, E. H.; Maerten, F.; Pollard, D. D.</p> <p>2012-12-01</p> <p> times associated with running successive forward models. We apply the inverse method using aftershock, Interferometric Synthetic Aperture Radar (InSAR) and Global Positioning <span class="hlt">System</span> (GPS) data associated with the Landers <span class="hlt">earthquake</span> and address how <span class="hlt">fault</span> geometry and aftershock size, timing, and focal mechanism quality influence inversion results. The advantages of this new method are that: (1) coseismic displacement data can be used, (2) the underlying model is better constrained to find a solution in the parameter space in the presence of <span class="hlt">fault</span> slip perturbations, (3) absolute magnitudes can be recovered when using data with magnitude information such as GPS, InSAR and stress tensors inferred from aftershocks with known magnitudes. In addition, while one can choose to invert for an Andersonian <span class="hlt">fault</span> regime, the method is not restricted to that particular case with one vertical principal stress.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.S34A..03K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.S34A..03K"><span>Impact of a Large San Andreas <span class="hlt">Fault</span> <span class="hlt">Earthquake</span> on Tall Buildings in Southern California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krishnan, S.; Ji, C.; Komatitsch, D.; Tromp, J.</p> <p>2004-12-01</p> <p>In 1857, an <span class="hlt">earthquake</span> of magnitude 7.9 occurred on the San Andreas <span class="hlt">fault</span>, starting at Parkfield and rupturing in a southeasterly direction for more than 300~km. Such a unilateral rupture produces significant directivity toward the San Fernando and Los Angeles basins. The strong shaking in the basins due to this <span class="hlt">earthquake</span> would have had a significant long-period content (2--8~s). If such motions were to happen today, they could have a serious impact on tall buildings in Southern California. In order to study the effects of large San Andreas <span class="hlt">fault</span> <span class="hlt">earthquakes</span> on tall buildings in Southern California, we use the finite source of the magnitude 7.9 2001 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> in Alaska and map it onto the San Andreas <span class="hlt">fault</span> with the rupture originating at Parkfield and proceeding southward over a distance of 290~km. Using the SPECFEM3D spectral element seismic wave propagation code, we simulate a Denali-like <span class="hlt">earthquake</span> on the San Andreas <span class="hlt">fault</span> and compute ground motions at sites located on a grid with a 2.5--5.0~km spacing in the greater Southern California region. We subsequently analyze 3D structural models of an existing tall steel building designed in 1984 as well as one designed according to the current building code (Uniform Building Code, 1997) subjected to the computed ground motion. We use a sophisticated nonlinear building analysis program, FRAME3D, that has the ability to simulate damage in buildings due to three-component ground motion. We summarize the performance of these structural models on contour maps of carefully selected structural performance indices. This study could benefit the city in laying out emergency response strategies in the event of an <span class="hlt">earthquake</span> on the San Andreas <span class="hlt">fault</span>, in undertaking appropriate retrofit measures for tall buildings, and in formulating zoning regulations for new construction. In addition, the study would provide risk data associated with existing and new construction to insurance companies, real estate developers, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMMR33B2662Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMMR33B2662Z"><span>Magnetic properties of cores from the Wenchuan <span class="hlt">Earthquake</span> <span class="hlt">Fault</span> Scientific Drilling Hole-2 (WFSD-2), China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, L., Jr.; Sun, Z.; Li, H.; Cao, Y.; Ye, X.; Wang, L.; Zhao, Y.; Han, S.</p> <p>2015-12-01</p> <p>During an <span class="hlt">earthquake</span>, seismic slip and frictional heating may cause the physical and chemical alterations of magnetic minerals within the <span class="hlt">fault</span> zone. Rock magnetism provides a method for understanding <span class="hlt">earthquake</span> dynamics. The Wenchuan <span class="hlt">earthquake</span> <span class="hlt">Fault</span> Scientific Drilling Project (WFSD) started right after 2008 Mw7.9 Wenchuan <span class="hlt">earthquake</span>, to investigate the <span class="hlt">earthquake</span> <span class="hlt">faulting</span> mechanism. Hole 2 (WFSD-2) is located in the Pengguan Complex in the Bajiaomiao village (Dujiangyan, Sichuan), and reached the Yingxiu-Beichuan <span class="hlt">fault</span> (YBF). We measured the surface magnetic susceptibility of the cores in WFSD-2 from 500 m to 1530 m with an interval of 1 cm. Rocks at 500-599.31 m-depth and 1211.49-1530 m-depth are from the Neoproterozoic Pengguang Complex while the section from 599.31 m to 1211.49 m is composed of Late Triassic sediments. The magnetic susceptibility values of the first part of the Pengguan Complex range from 1 to 25 × 10-6 SI, while the second part ranges from 10 to 200 × 10-6 SI, which indicate that the two parts are not from the same rock units. The Late Triassic sedimentary rocks have a low magnetic susceptibility values, ranging from -5 to 20 × 10-6 SI. Most <span class="hlt">fault</span> zones coincide with the high value of magnetic susceptibility in the WFSD-2 cores. <span class="hlt">Fault</span> rocks, mainly <span class="hlt">fault</span> breccia, cataclasite, gouge and pseudotachylite within the WFSD-2 cores, and mostly display a significantly higher magnetic susceptibility than host rocks (5:1 to 20:1). In particular, in the YBF zone of the WFSD-2 cores (from 600 to 960 m), dozens of stages with high values of magnetic susceptibility have been observed. The multi-layered <span class="hlt">fault</span> rocks with high magnetic susceptibility values might indicate that the YBF is a long-term active <span class="hlt">fault</span>. The magnetic susceptibility values change with different types of <span class="hlt">fault</span> rocks. The gouge and pseudotachylite have higher values of magnetic susceptibility than other <span class="hlt">fault</span> rocks. Other primary rock magnetism analyses were then performed to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S51B2375M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S51B2375M"><span>Rupture Synchronicity in Complex <span class="hlt">Fault</span> <span class="hlt">Systems</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Milner, K. R.; Jordan, T. H.</p> <p>2013-12-01</p> <p>While most investigators would agree that the timing of large <span class="hlt">earthquakes</span> within a <span class="hlt">fault</span> <span class="hlt">system</span> depends on stress-mediated interactions among its elements, much of the debate relevant to time-dependent forecasting has been centered on single-<span class="hlt">fault</span> concepts, such as characteristic <span class="hlt">earthquake</span> behavior. We propose to broaden this discussion by quantifying the multi-<span class="hlt">fault</span> concept of rupture synchronicity. We consider a finite set of small, <span class="hlt">fault</span>-spanning volumes {Vk} within a <span class="hlt">fault</span> <span class="hlt">system</span> of arbitrary (fractal) complexity. We let Ck be the catalog of length tmax comprising Nk discrete times {ti(k)} that mark when the kth volume participates in a rupture of magnitude > M. The main object of our analysis is the complete set of event time differences {τij(kk') = ti(k) - tj(k')}, which we take to be a random process with an expected density function ρkk'(t). When k = k', we call this function the auto-catalog density function (ACDF); when k ≠ k', we call it the cross-catalog density function (CCDF). The roles of the ACDF and CCDF in synchronicity theory are similar to those of autocorrelation and cross-correlation functions in time-series analysis. For a renewal process, the ACDF can be written in terms of convolutions of the interevent-time distribution, and many of its properties (e.g., large-t asymptote) can be derived analytically. The interesting information in the CCDF, like that in the ACDF, is concentrated near t = 0. If two catalogs are completely asynchronous, the CCDF collapses to an asymptote given by the harmonic mean of the ACDF asymptotes. Synchronicity can therefore be characterized by the variability of the CCDF about this asymptote. The brevity of instrumental catalogs makes the identification of synchronicity at large M difficult, but we will illustrate potentially interesting behaviors through the analysis of a million-year California catalog generated by the <span class="hlt">earthquake</span> simulator, RSQSim (Deiterich & Richards-Dinger, 2010), which we sampled at a</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018540','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018540"><span>Role of stress triggering in <span class="hlt">earthquake</span> migration on the North Anatolian <span class="hlt">fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Stein, R.S.; Dieterich, J.H.; Barka, A.A.</p> <p>1996-01-01</p> <p>Ten M???6.7 <span class="hlt">earthquakes</span> ruptured 1,000 km of the North Anatolian <span class="hlt">fault</span> (Turkey) during 1939-92, providing an unsurpassed opportunity to study how one large shock sets up the next. Calculations of the change in Coulomb failure stress reveal that 9 out of 10 ruptures were brought closer to failure by the preceding shocks, typically by 5 bars, equivalent to 20 years of secular stressing. We translate the calculated stress changes into <span class="hlt">earthquake</span> probabilities using an <span class="hlt">earthquake</span>-nucleation constitutive relation, which includes both permanent and transient stress effects. For the typical 10-year period between triggering and subsequent rupturing shocks in the Anatolia sequence, the stress changes yield an average three-fold gain in the ensuing <span class="hlt">earthquake</span> probability. Stress is now calculated to be high at several isolated sites along the <span class="hlt">fault</span>. During the next 30 years, we estimate a 15% probability of a M???6.7 <span class="hlt">earthquake</span> east of the major eastern center of Erzincan, and a 12% probability for a large event south of the major western port city of Izmit. Such stress-based probability calculations may thus be useful to assess and update <span class="hlt">earthquake</span> hazards elsewhere. ?? 1997 Elsevier Science Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.T42A..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.T42A..03S"><span>A New Correlation of Large <span class="hlt">Earthquakes</span> Along the Southern San Andreas <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scharer, K. M.; Weldon, R. J.; Biasi, G. P.</p> <p>2010-12-01</p> <p>There are now three sites on the southern San Andreas <span class="hlt">fault</span> (SSAF) with records of 10 or more dated ground rupturing <span class="hlt">earthquakes</span> (Frazier Mountain, Wrightwood and Pallett Creek) and at least seven other sites with 3-5 dated events. Numerous sites have related information including geomorphic offsets caused by 1 to a few <span class="hlt">earthquakes</span>, a known amount of slip spanning a specific interval of time or number of <span class="hlt">earthquakes</span>, or the number (but not necessarily the exact ages) of <span class="hlt">earthquakes</span> in an interval of time. We use this information to construct a record of recent large <span class="hlt">earthquakes</span> on the SSAF. Strongly overlapping C-14 age ranges, especially between closely spaced sites like Pallett Creek and Wrightwood on the Mojave segment and Thousand Palms, Indio, Coachella and Salt Creek on the southernmost 100 kms of the <span class="hlt">fault</span>, and overlap between the more distant Frazier Mountain and Bidart Fan sites on the northernmost part of the <span class="hlt">fault</span> suggest that the paleoseismic data are robust and can be explained by a relatively small number of events that span substantial portions of the <span class="hlt">fault</span>. This is consistent with the extent of rupture of the two historic events (1857 was ~300 km long and 1812 was 100-200 km long); slip per event data that averages 3-5 m per event at most sites; and the long historical hiatus since 1857. While some sites have smaller offsets for individual events, correlation between sites suggests that many small offsets are near the end of long ruptures. While the long event series on the Mojave are quasi-periodic, individual intervals range about an order of magnitude, from a few decades up to ~200 years. This wide range of intervals and the apparent anti-slip predictable behavior of ruptures (small intervals are not followed by small events) suggest weak clustering or periods of time spanning multiple intervals when strain release is higher low lower than average. These properties defy the application of simple hazard analysis but need to be understood to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.482...44W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.482...44W"><span>The 2016 Kaikōura <span class="hlt">earthquake</span>: Simultaneous rupture of the subduction interface and overlying <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Teng; Wei, Shengji; Shi, Xuhua; Qiu, Qiang; Li, Linlin; Peng, Dongju; Weldon, Ray J.; Barbot, Sylvain</p> <p>2018-01-01</p> <p>The distribution of slip during an <span class="hlt">earthquake</span> and how it propagates among <span class="hlt">faults</span> in the subduction <span class="hlt">system</span> play a major role in seismic and tsunami hazards, yet they are poorly understood because offshore observations are often lacking. Here we derive the slip distribution and rupture evolution during the 2016 Mw 7.9 Kaikōura (New Zealand) <span class="hlt">earthquake</span> that reconcile the surface rupture, space geodetic measurements, seismological and tsunami waveform records. We use twelve <span class="hlt">fault</span> segments, with eleven in the crust and one on the megathrust interface, to model the geodetic data and match the major features of the complex surface ruptures. Our modeling result indicates that a large portion of the moment is distributed on the subduction interface, making a significant contribution to the far field surface deformation and teleseismic body waves. The inclusion of local strong motion and teleseismic waveform data in the joint inversion reveals a unilateral rupture towards northeast with a relatively low averaged rupture speed of ∼1.5 km/s. The first 30 s of the rupture took place on the crustal <span class="hlt">faults</span> with oblique slip motion and jumped between <span class="hlt">fault</span> segments that have large differences in strike and dip. The peak moment release occurred at ∼65 s, corresponding to simultaneous rupture of both plate interface and the overlying splay <span class="hlt">faults</span> with rake angle changes progressively from thrust to strike-slip. The slip on the Papatea <span class="hlt">fault</span> produced more than 2 m of offshore uplift, making a major contribution to the tsunami at the Kaikōura station, while the northeastern end of the rupture can explain the main features at the Wellington station. Our inversions and simulations illuminate complex up-dip rupture behavior that should be taken into consideration in both seismic and tsunami hazard assessment. The extreme complex rupture behavior also brings new challenges to the <span class="hlt">earthquake</span> dynamic simulations and understanding the physics of <span class="hlt">earthquakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021088','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021088"><span>Use of <span class="hlt">fault</span> striations and dislocation models to infer tectonic shear stress during the 1995 Hyogo-Ken Nanbu (Kobe) <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Spudich, P.; Guatteri, Mariagiovanna; Otsuki, K.; Minagawa, J.</p> <p>1998-01-01</p> <p>Dislocation models of the 1995 Hyogo-ken Nanbu (Kobe) <span class="hlt">earthquake</span> derived by Yoshida et al. (1996) show substantial changes in direction of slip with time at specific points on the Nojima and Rokko <span class="hlt">fault</span> <span class="hlt">systems</span>, as do striations we observed on exposures of the Nojima <span class="hlt">fault</span> surface on Awaji Island. Spudich (1992) showed that the initial stress, that is, the shear traction on the <span class="hlt">fault</span> before the <span class="hlt">earthquake</span> origin time, can be derived at points on the <span class="hlt">fault</span> where the slip rake rotates with time if slip velocity and stress change are known at these points. From Yoshida's slip model, we calculated dynamic stress changes on the ruptured <span class="hlt">fault</span> surfaces. To estimate errors, we compared the slip velocities and dynamic stress changes of several published models of the <span class="hlt">earthquake</span>. The differences between these models had an exponential distribution, not gaussian. We developed a Bayesian method to estimate the probability density function (PDF) of initial stress from the striations and from Yoshida's slip model. Striations near Toshima and Hirabayashi give initial stresses of about 13 and 7 MPa, respectively. We obtained initial stresses of about 7 to 17 MPa at depths of 2 to 10 km on a subset of points on the Nojima and Rokko <span class="hlt">fault</span> <span class="hlt">systems</span>. Our initial stresses and coseismic stress changes agree well with postearthquake stresses measured by hydrofracturing in deep boreholes near Hirabayashi and Ogura on Awaji Island. Our results indicate that the Nojima <span class="hlt">fault</span> slipped at very low shear stress, and fractional stress drop was complete near the surface and about 32% below depths of 2 km. Our results at depth depend on the accuracy of the rake rotations in Yoshida's model, which are probably correct on the Nojima <span class="hlt">fault</span> but debatable on the Rokko <span class="hlt">fault</span>. Our results imply that curved or cross-cutting <span class="hlt">fault</span> striations can be formed in a single <span class="hlt">earthquake</span>, contradicting a common assumption of structural geology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70190383','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70190383"><span>Tsunami simulations of the 1867 Virgin Island <span class="hlt">earthquake</span>: Constraints on epicenter location and <span class="hlt">fault</span> parameters</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barkan, Roy; ten Brink, Uri S.</p> <p>2010-01-01</p> <p>The 18 November 1867 Virgin Island <span class="hlt">earthquake</span> and the tsunami that closely followed caused considerable loss of life and damage in several places in the northeast Caribbean region. The <span class="hlt">earthquake</span> was likely a manifestation of the complex tectonic deformation of the Anegada Passage, which cuts across the Antilles island arc between the Virgin Islands and the Lesser Antilles. In this article, we attempt to characterize the 1867 <span class="hlt">earthquake</span> with respect to <span class="hlt">fault</span> orientation, rake, dip, <span class="hlt">fault</span> dimensions, and first tsunami wave propagating phase, using tsunami simulations that employ high-resolution multibeam bathymetry. In addition, we present new geophysical and geological observations from the region of the suggested <span class="hlt">earthquake</span> source. Results of our tsunami simulations based on relative amplitude comparison limit the <span class="hlt">earthquake</span> source to be along the northern wall of the Virgin Islands basin, as suggested by Reid and Taber (1920), or on the carbonate platform north of the basin, and not in the Virgin Islands basin, as commonly assumed. The numerical simulations suggest the 1867 <span class="hlt">fault</span> was striking 120°–135° and had a mixed normal and left-lateral motion. First propagating wave phase analysis suggests a <span class="hlt">fault</span> striking 300°–315° is also possible. The best-fitting rupture length was found to be relatively small (50 km), probably indicating the <span class="hlt">earthquake</span> had a moment magnitude of ∼7.2. Detailed multibeam echo sounder surveys of the Anegada Passage bathymetry between St. Croix and St. Thomas reveal a scarp, which cuts the northern wall of the Virgin Islands basin. High-resolution seismic profiles further indicate it to be a reasonable <span class="hlt">fault</span> candidate. However, the <span class="hlt">fault</span> orientation and the orientation of other subparallel <span class="hlt">faults</span> in the area are more compatible with right-lateral motion. For the other possible source region, no clear disruption in the bathymetry or seismic profiles was found on the carbonate platform north of the basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027461','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027461"><span>Stress triggering in thrust and subduction <span class="hlt">earthquakes</span> and stress interaction between the southern San Andreas and nearby thrust and strike-slip <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lin, J.; Stein, R.S.</p> <p>2004-01-01</p> <p>We argue that key features of thrust <span class="hlt">earthquake</span> triggering, inhibition, and clustering can be explained by Coulomb stress changes, which we illustrate by a suite of representative models and by detailed examples. Whereas slip on surface-cutting thrust <span class="hlt">faults</span> drops the stress in most of the adjacent crust, slip on blind thrust <span class="hlt">faults</span> increases the stress on some nearby zones, particularly above the source <span class="hlt">fault</span>. Blind thrusts can thus trigger slip on secondary <span class="hlt">faults</span> at shallow depth and typically produce broadly distributed aftershocks. Short thrust ruptures are particularly efficient at triggering <span class="hlt">earthquakes</span> of similar size on adjacent thrust <span class="hlt">faults</span>. We calculate that during a progressive thrust sequence in central California the 1983 Mw = 6.7 Coalinga <span class="hlt">earthquake</span> brought the subsequent 1983 Mw = 6.0 Nunez and 1985 Mw = 6.0 Kettleman Hills ruptures 10 bars and 1 bar closer to Coulomb failure. The idealized stress change calculations also reconcile the distribution of seismicity accompanying large subduction events, in agreement with findings of prior investigations. Subduction zone ruptures are calculated to promote normal <span class="hlt">faulting</span> events in the outer rise and to promote thrust-<span class="hlt">faulting</span> events on the periphery of the seismic rupture and its downdip extension. These features are evident in aftershocks of the 1957 Mw = 9.1 Aleutian and other large subduction <span class="hlt">earthquakes</span>. We further examine stress changes on the rupture surface imparted by the 1960 Mw = 9.5 and 1995 Mw = 8.1 Chile <span class="hlt">earthquakes</span>, for which detailed slip models are available. Calculated Coulomb stress increases of 2-20 bars correspond closely to sites of aftershocks and postseismic slip, whereas aftershocks are absent where the stress drops by more than 10 bars. We also argue that slip on major strike-slip <span class="hlt">systems</span> modulates the stress acting on nearby thrust and strike-slip <span class="hlt">faults</span>. We calculate that the 1857 Mw = 7.9 Fort Tejon <span class="hlt">earthquake</span> on the San Andreas <span class="hlt">fault</span> and subsequent interseismic slip brought</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.G44A..01N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.G44A..01N"><span>Repeating <span class="hlt">Earthquake</span> and Nonvolcanic Tremor Observations of Aseismic Deep <span class="hlt">Fault</span> Transients in Central California.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nadeau, R. M.; Traer, M.; Guilhem, A.</p> <p>2005-12-01</p> <p>Seismic indicators of <span class="hlt">fault</span> zone deformation can complement geodetic measurements by providing information on aseismic transient deformation: 1) from deep within the <span class="hlt">fault</span> zone, 2) on a regional scale, 3) with intermediate temporal resolution (weeks to months) and 4) that spans over 2 decades (1984 to early 2005), including pre- GPS and INSAR coverage. Along the San Andreas <span class="hlt">Fault</span> (SAF) in central California, two types of seismic indicators are proving to be particularly useful for providing information on deep <span class="hlt">fault</span> zone deformation. The first, characteristically repeating microearthquakes, provide long-term coverage (decades) on the evolution of aseismic <span class="hlt">fault</span> slip rates at seismogenic depths along a large (~175 km) stretch of the SAF between the rupture zones of the ~M8 1906 San Francisco and 1857 Fort Tejon <span class="hlt">earthquakes</span>. In Cascadia and Japan the second type of seismic indicator, nonvolcanic tremors, have shown a remarkable correlation between their activity rates and GPS and tiltmeter measurements of transient deformation in the deep (sub-seismogenic) <span class="hlt">fault</span> zone. This correlation suggests that tremor rate changes and deep transient deformation are intimately related and that deformation associated with the tremor activity may be stressing the seismogenic zone in both areas. Along the SAF, nonvolcanic tremors have only recently been discovered (i.e., in the Parkfield-Cholame area), and knowledge of their full spatial extent is still relatively limited. Nonetheless the observed temporal correlation between <span class="hlt">earthquake</span> and tremor activity in this area is consistent with a model in which sub-seismogenic deformation and seismogenic zone stress changes are closely related. We present observations of deep aseismic transient deformation associated with the 28 September 2004, M6 Parkfield <span class="hlt">earthquake</span> from both repeating <span class="hlt">earthquake</span> and nonvolcanic tremor data. Also presented are updated deep <span class="hlt">fault</span> slip rate estimates from prepeating quakes in the San Juan Bautista area with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.464..175C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.464..175C"><span>A plate boundary <span class="hlt">earthquake</span> record from a wetland adjacent to the Alpine <span class="hlt">fault</span> in New Zealand refines hazard estimates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cochran, U. A.; Clark, K. J.; Howarth, J. D.; Biasi, G. P.; Langridge, R. M.; Villamor, P.; Berryman, K. R.; Vandergoes, M. J.</p> <p>2017-04-01</p> <p>Discovery and investigation of millennial-scale geological records of past large <span class="hlt">earthquakes</span> improve understanding of <span class="hlt">earthquake</span> frequency, recurrence behaviour, and likelihood of future rupture of major active <span class="hlt">faults</span>. Here we present a ∼2000 year-long, seven-event <span class="hlt">earthquake</span> record from John O'Groats wetland adjacent to the Alpine <span class="hlt">fault</span> in New Zealand, one of the most active strike-slip <span class="hlt">faults</span> in the world. We linked this record with the 7000 year-long, 22-event <span class="hlt">earthquake</span> record from Hokuri Creek (20 km along strike to the north) to refine estimates of <span class="hlt">earthquake</span> frequency and recurrence behaviour for the South Westland section of the plate boundary <span class="hlt">fault</span>. Eight cores from John O'Groats wetland revealed a sequence that alternated between organic-dominated and clastic-dominated sediment packages. Transitions from a thick organic unit to a thick clastic unit that were sharp, involved a significant change in depositional environment, and were basin-wide, were interpreted as evidence of past surface-rupturing <span class="hlt">earthquakes</span>. Radiocarbon dates of short-lived organic fractions either side of these transitions were modelled to provide estimates for <span class="hlt">earthquake</span> ages. Of the seven events recognised at the John O'Groats site, three post-date the most recent event at Hokuri Creek, two match events at Hokuri Creek, and two events at John O'Groats occurred in a long interval during which the Hokuri Creek site may not have been recording <span class="hlt">earthquakes</span> clearly. The preferred John O'Groats-Hokuri Creek <span class="hlt">earthquake</span> record consists of 27 events since ∼6000 BC for which we calculate a mean recurrence interval of 291 ± 23 years, shorter than previously estimated for the South Westland section of the <span class="hlt">fault</span> and shorter than the current interseismic period. The revised 50-year conditional probability of a surface-rupturing <span class="hlt">earthquake</span> on this <span class="hlt">fault</span> section is 29%. The coefficient of variation is estimated at 0.41. We suggest the low recurrence variability is likely to be a feature of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GeoJI.190.1625G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GeoJI.190.1625G"><span>GPS and seismic constraints on the M = 7.3 2009 Swan Islands <span class="hlt">earthquake</span>: implications for stress changes along the Motagua <span class="hlt">fault</span> and other nearby <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Graham, Shannon E.; DeMets, Charles; DeShon, Heather R.; Rogers, Robert; Maradiaga, Manuel Rodriguez; Strauch, Wilfried; Wiese, Klaus; Hernandez, Douglas</p> <p>2012-09-01</p> <p>We use measurements at 35 GPS stations in northern Central America and 25 seismometers at teleseismic distances to estimate the distribution of slip, source time function and Coulomb stress changes of the Mw = 7.3 2009 May 28, Swan Islands <span class="hlt">fault</span> <span class="hlt">earthquake</span>. This event, the largest in the region for several decades, ruptured the offshore continuation of the seismically hazardous Motagua <span class="hlt">fault</span> of Guatemala, the site of the destructive Ms = 7.5 <span class="hlt">earthquake</span> in 1976. Measured GPS offsets range from 308 millimetres at a campaign site in northern Honduras to 6 millimetres at five continuous sites in El Salvador. Separate inversions of geodetic and seismic data both indicate that up to ˜1 m of coseismic slip occurred along a ˜250-km-long rupture zone between the island of Roatan and the eastern limit of the 1976 M = 7.5 Motagua <span class="hlt">fault</span> <span class="hlt">earthquake</span> in Guatemala. Evidence for slip ˜250 km west of the epicentre is corroborated independently by aftershocks recorded by a local seismic network and by the high concentration of damage to structures in areas of northern Honduras adjacent to the western limit of the rupture zone. Coulomb stresses determined from the coseismic slip distribution resolve a maximum of 1 bar of stress transferred to the seismically hazardous Motagua <span class="hlt">fault</span> and further indicate unclamping of normal <span class="hlt">faults</span> along the northern shore of Honduras, where two M > 5 normal-<span class="hlt">faulting</span> <span class="hlt">earthquakes</span> and numerous small <span class="hlt">earthquakes</span> were triggered by the main shock.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019873','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019873"><span>Progressive failure on the North Anatolian <span class="hlt">fault</span> since 1939 by <span class="hlt">earthquake</span> stress triggering</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Stein, R.S.; Barka, A.A.; Dieterich, J.H.</p> <p>1997-01-01</p> <p>10 M ??? 6.7 <span class="hlt">earthquakes</span> ruptured 1000 km of the North Anatolian <span class="hlt">fault</span> (Turkey) during 1939-1992, providing an unsurpassed opportunity to study how one large shock sets up the next. We use the mapped surface slip and <span class="hlt">fault</span> geometry to infer the transfer of stress throughout the sequence. Calculations of the change in Coulomb failure stress reveal that nine out of 10 ruptures were brought closer to failure by the preceding shocks, typically by 1-10 bar, equivalent to 3-30 years of secular stressing. We translate the calculated stress changes into <span class="hlt">earthquake</span> probability gains using an <span class="hlt">earthquake</span>-nucleation constitutive relation, which includes both permanent and transient effects of the sudden stress changes. The transient effects of the stress changes dominate during the mean 10 yr period between triggering and subsequent rupturing shocks in the Anatolia sequence. The stress changes result in an average three-fold gain in the net <span class="hlt">earthquake</span> probability during the decade after each event. Stress is calculated to be high today at several isolated sites along the <span class="hlt">fault</span>. During the next 30 years, we estimate a 15 per cent probability of a M ??? 6.7 <span class="hlt">earthquake</span> east of the major eastern centre of Ercinzan, and a 12 per cent probability for a large event south of the major western port city of Izmit. Such stress-based probability calculations may thus be useful to assess and update <span class="hlt">earthquake</span> hazards elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.T41C..04R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.T41C..04R"><span>The Non-Regularity of <span class="hlt">Earthquake</span> Recurrence in California: Lessons From Long Paleoseismic Records in Simple vs Complex <span class="hlt">Fault</span> Regions (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rockwell, T. K.</p> <p>2010-12-01</p> <p>A long paleoseismic record at Hog Lake on the central San Jacinto <span class="hlt">fault</span> (SJF) in southern California documents evidence for 18 surface ruptures in the past 3.8-4 ka. This yields a long-term recurrence interval of about 210 years, consistent with its slip rate of ~16 mm/yr and field observations of 3-4 m of displacement per event. However, during the past 3800 years, the <span class="hlt">fault</span> has switched from a quasi-periodic mode of <span class="hlt">earthquake</span> production, during which the recurrence interval is similar to the long-term average, to clustered behavior with the inter-event periods as short as a few decades. There are also some periods as long as 450 years during which there were no surface ruptures, and these periods are commonly followed by one to several closely-timed ruptures. The coefficient of variation (CV) for the timing of these <span class="hlt">earthquakes</span> is about 0.6 for the past 4000 years (17 intervals). Similar behavior has been observed on the San Andreas <span class="hlt">Fault</span> (SAF) south of the Transverse Ranges where clusters of <span class="hlt">earthquakes</span> have been followed by periods of lower seismic production, and the CV is as high as 0.7 for some portions of the <span class="hlt">fault</span>. In contrast, the central North Anatolian <span class="hlt">Fault</span> (NAF) in Turkey, which ruptured in 1944, appears to have produced ruptures with similar displacement at fairly regular intervals for the past 1600 years. With a CV of 0.16 for timing, and close to 0.1 for displacement, the 1944 rupture segment near Gerede appears to have been both periodic and characteristic. The SJF and SAF are part of a broad plate boundary <span class="hlt">system</span> with multiple parallel strands with significant slip rates. Additional <span class="hlt">faults</span> lay to the east (Eastern California shear zone) and west (<span class="hlt">faults</span> of the LA basin and southern California Borderland), which makes the southern SAF <span class="hlt">system</span> a complex and broad plate boundary zone. In comparison, the 1944 rupture section of the NAF is simple, straight and highly localized, which contrasts with the complex <span class="hlt">system</span> of parallel <span class="hlt">faults</span> in southern</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.T12C0474L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.T12C0474L"><span>Reevaluation of 1935 M 7.0 <span class="hlt">earthquake</span> <span class="hlt">fault</span>, Miaoli-Taichung Area, western Taiwan: a DEM and field study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, Y. N.; Chen, Y.; Ota, Y.</p> <p>2003-12-01</p> <p>A large <span class="hlt">earthquake</span> (M 7.0) took place in Miaoli area, western Taiwan on April 21st, 1935. Right to its south is the 1999 Chi-Chi <span class="hlt">earthquake</span> <span class="hlt">fault</span>, indicating it is not only tectonically but seismically active. As the previous study, the study area is located in the mature zone of a tectonic collision that occurred between Philippine sea Plate and Eurasia continental Plate. The associated surface ruptures of 1935 <span class="hlt">earthquake</span> daylighted Tungtsichiao <span class="hlt">Fault</span>, a tear <span class="hlt">fault</span> trending NE in the south and Chihhu <span class="hlt">Fault</span>, a back thrust trending N-S in the north, but no ruptures occurred in between. Strike-slip component was identified by the horizontal offset observed along Tungtsichiao <span class="hlt">Fault</span>; however, there are still disputes on the reported field evidence. Our purposes are (1) to identify the structural behaviors of these two <span class="hlt">faults</span>, (2) to find out what the seismogenic structure is, and (3) to reconstruct the regional geology by information given by this <span class="hlt">earthquake</span>. By DEM interpretation and field survey, we can clearly recognize a lot of the 1935 associated features. In the west of Chihhu <span class="hlt">Fault</span>, a series of N-S higher terraces can be identified with eastward tilted surfaces and nearly 200 m relative height. Another lower terrace is also believed being created during the 1935 <span class="hlt">earthquake</span>, showing an east-facing scarp with a height of ca. 1.5~2 m. Outcrop investigation reveals that the late-Miocene bedrock has been easterly thrusted over the Holocene conglomerates, indicating a west-dipping <span class="hlt">fault</span> plane. The Tungtsichiao <span class="hlt">Fault</span> cuts through a lateritic terrace at Holi, which is supposed developed in Pleistocene. The <span class="hlt">fault</span> scarp is only discernible in the northeastern ending. Other noticeable features are the <span class="hlt">fault</span> related antiforms that line up along the surface rupture. There is no outcrop to show the <span class="hlt">fault</span> geometry among bedrocks. We re-interpret the northern Chihhu <span class="hlt">Fault</span> as the back thrust generated from a main subsurface detachment, which may be the actual seismogenic <span class="hlt">fault</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70191859','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191859"><span>Ground-rupturing <span class="hlt">earthquakes</span> on the northern Big Bend of the San Andreas <span class="hlt">Fault</span>, California, 800 A.D. to Present</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Scharer, Katherine M.; Weldon, Ray; Biasi, Glenn; Streig, Ashley; Fumal, Thomas E.</p> <p>2017-01-01</p> <p>Paleoseismic data on the timing of ground-rupturing <span class="hlt">earthquakes</span> constrain the recurrence behavior of active <span class="hlt">faults</span> and can provide insight on the rupture history of a <span class="hlt">fault</span> if <span class="hlt">earthquakes</span> dated at neighboring sites overlap in age and are considered correlative. This study presents the evidence and ages for 11 <span class="hlt">earthquakes</span> that occurred along the Big Bend section of the southern San Andreas <span class="hlt">Fault</span> at the Frazier Mountain paleoseismic site. The most recent <span class="hlt">earthquake</span> to rupture the site was the Mw7.7–7.9 Fort Tejon <span class="hlt">earthquake</span> of 1857. We use over 30 trench excavations to document the structural and sedimentological evolution of a small pull-apart basin that has been repeatedly <span class="hlt">faulted</span> and folded by ground-rupturing <span class="hlt">earthquakes</span>. A sedimentation rate of 0.4 cm/yr and abundant organic material for radiocarbon dating contribute to a record that is considered complete since 800 A.D. and includes 10 paleoearthquakes. <span class="hlt">Earthquakes</span> have ruptured this location on average every ~100 years over the last 1200 years, but individual intervals range from ~22 to 186 years. The coefficient of variation of the length of time between <span class="hlt">earthquakes</span> (0.7) indicates quasiperiodic behavior, similar to other sites along the southern San Andreas <span class="hlt">Fault</span>. Comparison with the <span class="hlt">earthquake</span> chronology at neighboring sites along the <span class="hlt">fault</span> indicates that only one other 1857-size <span class="hlt">earthquake</span> could have occurred since 1350 A.D., and since 800 A.D., the Big Bend and Mojave sections have ruptured together at most 50% of the time in Mw ≥ 7.3 <span class="hlt">earthquakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA529678','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA529678"><span>Transportations <span class="hlt">Systems</span> Modeling and Applications in <span class="hlt">Earthquake</span> Engineering</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-07-01</p> <p>49 Figure 6 PGA map of a M7.7 <span class="hlt">earthquake</span> on all three New Madrid <span class="hlt">fault</span> segments (g)............... 50...Memphis, Tennessee. The NMSZ was responsible for the devastating 1811-1812 New Madrid <span class="hlt">earthquakes</span> , the largest <span class="hlt">earthquakes</span> ever recorded in the...Figure 6 PGA map of a M7.7 <span class="hlt">earthquake</span> on all three New Madrid <span class="hlt">fault</span> segments (g) Table 1 Fragility parameters for MSC steel bridge (Padgett 2007</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026158','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026158"><span>Constraining the slip distribution and <span class="hlt">fault</span> geometry of the Mw 7.9, 3 November 2002, Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> with Interferometric Synthetic Aperture Radar and Global Positioning <span class="hlt">System</span> data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wright, Tim J.; Lu, Z.; Wicks, Charles</p> <p>2004-01-01</p> <p>The Mw 7.9, Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> (DFE) is the largest continental strike-slip <span class="hlt">earthquake</span> to occur since the development of Interferometric Synthetic Aperture Radar (InSAR). We use five interferograms, constructed using radar images from the Canadian Radarsat-1 satellite, to map the surface deformation at the western end of the <span class="hlt">fault</span> rupture. Additional geodetic data are provided by displacements observed at 40 campaign and continuous Global Positioning <span class="hlt">System</span> (GPS) sites. We use the data to determine the geometry of the Susitna Glacier <span class="hlt">fault</span>, thrusting on which initiated the DFE, and to determine a slip model for the entire event that is consistent with both the InSAR and GPS data. We find there was an average of 7.3 ± 0.4 m slip on the Susitna Glacier <span class="hlt">fault</span>, between 1 and 9.5 km depth on a 29 km long <span class="hlt">fault</span> that dips north at 41 ± 0.7° and has a surface projection close to the mapped rupture. On the Denali <span class="hlt">fault</span>, a simple model with large slip patches finds a maximum of 8.7 ± 0.7 m of slip between the surface and 14.3 ± 0.2 km depth. A more complex distributed slip model finds a peak of 12.5 ± 0.8 m in the upper 4 km, significantly higher than the observed surface slip. We estimate a geodetic moment of 670 ± 10 × 1018 N m (Mw 7.9), consistent with seismic estimates. Lack of preseismic data resulted in an absence of InSAR coverage for the eastern half of the DFE rupture. A dedicated geodetic InSAR mission could obviate coverage problems in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036995','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036995"><span>San Andreas <span class="hlt">fault</span> geometry at Desert Hot Springs, California, and its effects on <span class="hlt">earthquake</span> hazards and groundwater</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Catchings, R.D.; Rymer, M.J.; Goldman, M.R.; Gandhok, G.</p> <p>2009-01-01</p> <p>The Mission Creek and Banning <span class="hlt">faults</span> are two of the principal strands of the San Andreas <span class="hlt">fault</span> zone in the northern Coachella Valley of southern California. Structural characteristics of the <span class="hlt">faults</span> affect both regional <span class="hlt">earthquake</span> hazards and local groundwater resources. We use seismic, gravity, and geological data to characterize the San Andreas <span class="hlt">fault</span> zone in the vicinity of Desert Hot Springs. Seismic images of the upper 500 m of the Mission Creek <span class="hlt">fault</span> at Desert Hot Springs show multiple <span class="hlt">fault</span> strands distributed over a 500 m wide zone, with concentrated <span class="hlt">faulting</span> within a central 200 m wide area of the <span class="hlt">fault</span> zone. High-velocity (up to 5000 m=sec) rocks on the northeast side of the <span class="hlt">fault</span> are juxtaposed against a low-velocity (6.0) <span class="hlt">earthquakes</span> in the area (in 1948 and 1986) occurred at or near the depths (~10 to 12 km) of the merged (San Andreas) <span class="hlt">fault</span>. Large-magnitude <span class="hlt">earthquakes</span> that nucleate at or below the merged <span class="hlt">fault</span> will likely generate strong shaking from guided waves along both <span class="hlt">fault</span> zones and from amplified seismic waves in the low-velocity basin between the two <span class="hlt">fault</span> zones. The Mission Creek <span class="hlt">fault</span> zone is a groundwater barrier with the top of the water table varying by 60 m in depth and the aquifer varying by about 50 m in thickness across a 200 m wide zone of concentrated <span class="hlt">faulting</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027453','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027453"><span>Geophysical investigation of the Denali <span class="hlt">fault</span> and Alaska Range orogen within the aftershock zone of the October-November 2002, M = 7.9 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fisher, M.A.; Nokleberg, W.J.; Ratchkovski, N.A.; Pellerin, L.; Glen, J.M.; Brocher, T.M.; Booker, J.</p> <p>2004-01-01</p> <p>The aftershock zone of the 3 November 2002, M = 7.9 <span class="hlt">earthquake</span> that ruptured along the right-slip Denali <span class="hlt">fault</span> in south-central Alaska has been investigated by using gravity and magnetic, magnetotelluric, and deep-crustal, seismic reflection data as well as outcrop geology and <span class="hlt">earthquake</span> seismology. Strong seismic reflections from within the Alaska Range orogen north of the Denali <span class="hlt">fault</span> dip as steeply as 25°N and extend to depths as great as 20 km. These reflections outline a relict crustal architecture that in the past 20 yr has produced little seismicity. The Denali <span class="hlt">fault</span> is nonreflective, probably because this <span class="hlt">fault</span> dips steeply to vertical. The most intriguing finding from geophysical data is that <span class="hlt">earthquake</span> aftershocks occurred above a rock body, with low electrical resistivity (>10 Ω·m), that is at depths below ∼10 km. Aftershocks of the Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> have mainly occurred shallower than 10 km. A high geothermal gradient may cause the shallow seismicity. Another possibility is that the low resistivity results from fluids, which could have played a role in locating the aftershock zone by reducing rock friction within the middle and lower crust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018183','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018183"><span>A slow <span class="hlt">earthquake</span> sequence on the San Andreas <span class="hlt">fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Linde, A.T.; Gladwin, M.T.; Johnston, M.J.S.; Gwyther, R.L.; Bilham, R.G.</p> <p>1996-01-01</p> <p><span class="hlt">EARTHQUAKES</span> typically release stored strain energy on timescales of the order of seconds, limited by the velocity of sound in rock. Over the past 20 years, observations and laboratory experiments have indicated that capture can also occur more slowly, with durations up to hours. Such events may be important in <span class="hlt">earthquake</span> nucleation and in accounting for the excess of plate convergence over seismic slip in subduction zones. The detection of events with larger timescales requires near-field deformation measurements. In December 1992, two borehole strainmeters close to the San Andreas <span class="hlt">fault</span> in California recorded a slow strain event of about a week in duration, and we show here that the strain changes were produced by a slow <span class="hlt">earthquake</span> sequence (equivalent magnitude 4.8) with complexity similar to that of regular <span class="hlt">earthquakes</span>. The largest <span class="hlt">earthquakes</span> associated with these slow events were small (local magnitude 3.7) and contributed negligible strain release. The importance of slow <span class="hlt">earthquakes</span> in the seismogenic process remains an open question, but these observations extend the observed timescale for slow events by two orders of magnitude.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S14B..08A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S14B..08A"><span>Insights into the <span class="hlt">Fault</span> Geometry and Rupture History of the 2016 MW 7.8 Kaikoura, New Zealand, <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adams, M.; Ji, C.</p> <p>2017-12-01</p> <p>The November 14th 2016 MW 7.8 Kaikoura, New Zealand <span class="hlt">earthquake</span> occurred along the east coast of the northern part of the South Island. The local tectonic setting is complicated. The central South Island is dominated by oblique continental convergence, whereas the southern part of this island experiences eastward subduction of the Australian plate. Available information (e.g., Hamling et al., 2017; Bradley et al., 2017) indicate that this <span class="hlt">earthquake</span> involved multiple <span class="hlt">fault</span> segments of the Marlborough <span class="hlt">fault</span> <span class="hlt">system</span> (MFS) as the rupture propagated northwards for more than 150 km. Additional slip might also occur on the subduction interface of the Pacific plate under the Australian plate, beneath the MFS. However, the exact number of involved <span class="hlt">fault</span> segments as well as the temporal co-seismic rupture sequence has not been fully determined with geodetic and geological observations. Knowledge of the kinematics of complex <span class="hlt">fault</span> interactions has important implications for our understanding of global seismic hazards, particularly to relatively unmodeled multisegment ruptures. Understanding the Kaikoura <span class="hlt">earthquake</span> will provide insight into how one incorporates multi-<span class="hlt">fault</span> ruptures in seismic-hazard models. We propose to apply a multiple double-couple inversion to determine the <span class="hlt">fault</span> geometry and spatiotemporal rupture history using teleseismic and strong motion waveforms, before constraining the detailed slip history using both seismic and geodetic data. The Kaikoura <span class="hlt">earthquake</span> will be approximated as the summation of multiple subevents—each represented as a double-couple point source, characterized by i) <span class="hlt">fault</span> geometry (strike, dip and rake), ii) seismic moment, iii) centroid time, iv) half-duration and v) location (latitude, longitude and depth), a total of nine variables. We progressively increase the number of point sources until the additional source cannot produce significant improvement to the observations. Our preliminary results using only teleseismic data indicate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.478..234T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.478..234T"><span>3D geometry of a plate boundary <span class="hlt">fault</span> related to the 2016 Off-Mie <span class="hlt">earthquake</span> in the Nankai subduction zone, Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsuji, Takeshi; Minato, Shohei; Kamei, Rie; Tsuru, Tetsuro; Kimura, Gaku</p> <p>2017-11-01</p> <p>We used recent seismic data and advanced techniques to investigate 3D <span class="hlt">fault</span> geometry over the transition from the partially coupled to the fully coupled plate interface inboard of the Nankai Trough off the Kii Peninsula, Japan. We found that a gently dipping plate boundary décollement with a thick underthrust layer extends beneath the entire Kumano forearc basin. The 1 April 2016 Off-Mie <span class="hlt">earthquake</span> (Mw6.0) and its aftershocks occurred, where the plate boundary décollement steps down close to the oceanic crust surface. This location also lies beneath the trenchward edge of an older accretionary prism (∼14 Ma) developed along the coast of the Kii peninsula. The strike of the 2016 rupture plane was similar to that of a formerly active splay <span class="hlt">fault</span> <span class="hlt">system</span> in the accretionary prism. Thus, the <span class="hlt">fault</span> planes of the 2016 <span class="hlt">earthquake</span> and its aftershocks were influenced by the geometry of the plate interface as well as splay <span class="hlt">faulting</span>. The 2016 <span class="hlt">earthquake</span> occurred within the rupture area of large interplate <span class="hlt">earthquakes</span> such as the 1944 Tonankai <span class="hlt">earthquake</span> (Mw8.1), although the 2016 rupture area was much smaller than that of the 1944 event. Whereas the hypocenter of the 2016 <span class="hlt">earthquake</span> was around the underplating sequence beneath the younger accretionary prism (∼6 Ma), the 1944 great <span class="hlt">earthquake</span> hypocenter was close to oceanic crust surface beneath the older accretionary prism. The variation of <span class="hlt">fault</span> geometry and lithology may influence the degree of coupling along the plate interface, and such coupling variation could hinder slip propagation toward the deeper plate interface in the 2016 event.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70193655','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70193655"><span>Constraints on the source parameters of low-frequency <span class="hlt">earthquakes</span> on the San Andreas <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Thomas, Amanda M.; Beroza, Gregory C.; Shelly, David R.</p> <p>2016-01-01</p> <p>Low-frequency <span class="hlt">earthquakes</span> (LFEs) are small repeating <span class="hlt">earthquakes</span> that occur in conjunction with deep slow slip. Like typical <span class="hlt">earthquakes</span>, LFEs are thought to represent shear slip on crustal <span class="hlt">faults</span>, but when compared to <span class="hlt">earthquakes</span> of the same magnitude, LFEs are depleted in high-frequency content and have lower corner frequencies, implying longer duration. Here we exploit this difference to estimate the duration of LFEs on the deep San Andreas <span class="hlt">Fault</span> (SAF). We find that the M ~ 1 LFEs have typical durations of ~0.2 s. Using the annual slip rate of the deep SAF and the average number of LFEs per year, we estimate average LFE slip rates of ~0.24 mm/s. When combined with the LFE magnitude, this number implies a stress drop of ~104 Pa, 2 to 3 orders of magnitude lower than ordinary <span class="hlt">earthquakes</span>, and a rupture velocity of 0.7 km/s, 20% of the shear wave speed. Typical <span class="hlt">earthquakes</span> are thought to have rupture velocities of ~80–90% of the shear wave speed. Together, the slow rupture velocity, low stress drops, and slow slip velocity explain why LFEs are depleted in high-frequency content relative to ordinary <span class="hlt">earthquakes</span> and suggest that LFE sources represent areas capable of relatively higher slip speed in deep <span class="hlt">fault</span> zones. Additionally, changes in rheology may not be required to explain both LFEs and slow slip; the same process that governs the slip speed during slow <span class="hlt">earthquakes</span> may also limit the rupture velocity of LFEs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995Tectp.249..249B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995Tectp.249..249B"><span><span class="hlt">Faulting</span> mechanism of the El Asnam (Algeria) 1954 and 1980 <span class="hlt">earthquakes</span> from modelling of vertical movements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bezzeghoud, M.; Dimitro, D.; Ruegg, J. C.; Lammali, K.</p> <p>1995-09-01</p> <p>Since 1980, most of the papers published on the El Asnam <span class="hlt">earthquake</span> concern the geological and seismological aspects of the <span class="hlt">fault</span> zone. Only one paper, published by Ruegg et al. (1982), constrains the <span class="hlt">faulting</span> mechanism with geodetic measurements. The purpose of this paper is to reexamine the <span class="hlt">faulting</span> mechanism of the 1954 and 1980 events by modelling the associated vertical movements. For this purpose we used all available data, and particularly those of the levelling profiles along the Algiers-Oran railway that has been remeasured after each event. The comparison between 1905 and 1976 levelling data shows observed vertical displacement that could have been induced by the 1954 <span class="hlt">earthquake</span>. On the basis of the 1954 and 1980 levelling data, we propose a possible model for the 1954 and 1980 <span class="hlt">fault</span> <span class="hlt">systems</span>. Our 1954 <span class="hlt">fault</span> model is parallel to the 1980 main thrust <span class="hlt">fault</span>, with an offset of 6 km towards the west. The 1980 dislocation model proposed in this study is based on a variable slip dislocation model and explains the observed surface break displacements given by Yielding et al. (1981). The Dewey (1991) and Avouac et al. (1992) models are compared with our dislocation model and discussed in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS43D..05O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS43D..05O"><span>Quantifying Coseismic Normal <span class="hlt">Fault</span> Rupture at the Seafloor: The 2004 Les Saintes <span class="hlt">Earthquake</span> Along the Roseau <span class="hlt">Fault</span> (French Antilles)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olive, J. A. L.; Escartin, J.; Leclerc, F.; Garcia, R.; Gracias, N.; Odemar Science Party, T.</p> <p>2016-12-01</p> <p>While >70% of Earth's seismicity is submarine, almost all observations of <span class="hlt">earthquake</span>-related ruptures and surface deformation are restricted to subaerial environments. Such observations are critical for understanding <span class="hlt">fault</span> behavior and associated hazards (including tsunamis), but are not routinely conducted at the seafloor due to obvious constraints. During the 2013 ODEMAR cruise we used autonomous and remotely operated vehicles to map the Roseau normal <span class="hlt">Fault</span> (Lesser Antilles), source of the 2004 Mw6.3 <span class="hlt">earthquake</span> and associated tsunami (<3.5m run-up). These vehicles acquired acoustic (multibeam bathymetry) and optical data (video and electronic images) spanning from regional (>1 km) to outcrop (<1 m) scales. These high-resolution submarine observations, analogous to those routinely conducted subaerially, rely on advanced image and video processing techniques, such as mosaicking and structure-from-motion (SFM). We identify sub-vertical <span class="hlt">fault</span> slip planes along the Roseau scarp, displaying coseismic deformation structures undoubtedly due to the 2004 event. First, video mosaicking allows us to identify the freshly exposed <span class="hlt">fault</span> plane at the base of one of these scarps. A maximum vertical coseismic displacement of 0.9 m can be measured from the video-derived terrain models and the texture-mapped imagery, which have better resolution than any available acoustic <span class="hlt">systems</span> (<10 cm). Second, seafloor photomosaics allow us to identify and map both additional sub-vertical <span class="hlt">fault</span> scarps, and cracks and fissures at their base, recording hangingwall damage from the same event. These observations provide critical parameters to understand the seismic cycle and long-term seismic behavior of this submarine <span class="hlt">fault</span>. Our work demonstrates the feasibility of extensive, high-resolution underwater surveys using underwater vehicles and novel imaging techniques, thereby opening new possibilities to study recent seafloor changes associated with tectonic, volcanic, or hydrothermal activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70048647','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70048647"><span>The Mw 5.8 Mineral, Virginia, <span class="hlt">earthquake</span> of August 2011 and aftershock sequence: constraints on <span class="hlt">earthquake</span> source parameters and <span class="hlt">fault</span> geometry</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McNamara, Daniel E.; Benz, H.M.; Herrmann, Robert B.; Bergman, Eric A.; Earle, Paul; Meltzer, Anne; Withers, Mitch; Chapman, Martin</p> <p>2014-01-01</p> <p>The Mw 5.8 <span class="hlt">earthquake</span> of 23 August 2011 (17:51:04 UTC) (moment, M0 5.7×1017  N·m) occurred near Mineral, Virginia, within the central Virginia seismic zone and was felt by more people than any other <span class="hlt">earthquake</span> in United States history. The U.S. Geological Survey (USGS) received 148,638 felt reports from 31 states and 4 Canadian provinces. The USGS PAGER <span class="hlt">system</span> estimates as many as 120,000 people were exposed to shaking intensity levels of IV and greater, with approximately 10,000 exposed to shaking as high as intensity VIII. Both regional and teleseismic moment tensor solutions characterize the <span class="hlt">earthquake</span> as a northeast‐striking reverse <span class="hlt">fault</span> that nucleated at a depth of approximately 7±2  km. The distribution of reported macroseismic intensities is roughly ten times the area of a similarly sized <span class="hlt">earthquake</span> in the western United States (Horton and Williams, 2012). Near‐source and far‐field damage reports, which extend as far away as Washington, D.C., (135 km away) and Baltimore, Maryland, (200 km away) are consistent with an <span class="hlt">earthquake</span> of this size and depth in the eastern United States (EUS). Within the first few days following the <span class="hlt">earthquake</span>, several government and academic institutions installed 36 portable seismograph stations in the epicentral region, making this among the best‐recorded aftershock sequences in the EUS. Based on modeling of these data, we provide a detailed description of the source parameters of the mainshock and analysis of the subsequent aftershock sequence for defining the <span class="hlt">fault</span> geometry, area of rupture, and observations of the aftershock sequence magnitude–frequency and temporal distribution. The observed slope of the magnitude–frequency curve or b‐value for the aftershock sequence is consistent with previous EUS studies (b=0.75), suggesting that most of the accumulated strain was released by the mainshock. The aftershocks define a rupture that extends between approximately 2–8 km in depth and 8–10 km along</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996JGR...10125459H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996JGR...10125459H"><span>The 1954 Rainbow Mountain-Fairview Peak-Dixie Valley <span class="hlt">earthquakes</span>: A triggered normal <span class="hlt">faulting</span> sequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hodgkinson, Kathleen M.; Stein, Ross S.; King, Geoffrey C. P.</p> <p>1996-11-01</p> <p>In 1954, four <span class="hlt">earthquakes</span> of M > 6.0 occurred within a 30 km radius in a period of six months. The Rainbow Mountain-Fairview Peak-Dixie Valley <span class="hlt">earthquakes</span> are among the largest to have been recorded geodetically in the Basin and Range province. The Fairview Peak <span class="hlt">earthquake</span> (M = 7.2, December 12, 1954) followed two events in the Rainbow Mountains (M = 6.2, July 6, and M = 6.5, August 24, 1954) by 6 months. Four minutes later the Dixie Valley <span class="hlt">fault</span> ruptured (M = 6.7, December 12, 1954). The changes in static stresses caused by the events are calculated using the Coulomb-Navier failure criterion and assuming uniform slip on rectangular dislocations embedded in an elastic half-space. Coulomb stress changes are resolved on optimally oriented <span class="hlt">faults</span> and on each of the <span class="hlt">faults</span> that ruptured in the chain of events. These calculations show that each <span class="hlt">earthquake</span> in the Rainbow Mountain-Fairview Peak-Dixie Valley sequence was preceded by a static stress change that encouraged failure. The magnitude of the stress increases transferred from one <span class="hlt">earthquake</span> to another ranged from 0.01 MPa (0.1 bar) to over 0.1 MPa (1 bar). Stresses were reduced by up to 0.1 MPa over most of the Rainbow Mountain-Fairview Peak area as a result of the <span class="hlt">earthquake</span> sequence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018658','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018658"><span>The 1954 Rainbow Mountain-Fairview Peak-Dixie Valley <span class="hlt">earthquakes</span>: A triggered normal <span class="hlt">faulting</span> sequence</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hodgkinson, K.M.; Stein, R.S.; King, G.C.P.</p> <p>1996-01-01</p> <p>In 1954, four <span class="hlt">earthquakes</span> of M > 6.0 occurred within a 30 km radius in a period of six months. The Rainbow Mountain-Fairview Peak-Dixie Valley <span class="hlt">earthquakes</span> are among the largest to have been recorded geodetically in the Basin and Range province. The Fairview Peak <span class="hlt">earthquake</span> (M=7.2, December 12, 1954) followed two events in the Rainbow Mountains (M=6.2, July 6, and M=6.5, August 24, 1954) by 6 months. Four minutes later the Dixie Valley <span class="hlt">fault</span> ruptured (M=6.7, December 12, 1954). The changes in static stresses caused by the events are calculated using the Coulomb-Navier failure criterion and assuming uniform slip on rectangular dislocations embedded in an elastic half-space. Coulomb stress changes are resolved on optimally oriented <span class="hlt">faults</span> and on each of the <span class="hlt">faults</span> that ruptured in the chain of events. These calculations show that each <span class="hlt">earthquake</span> in the Rainbow Mountain-Fairview Peak-Dixie Valley sequence was preceded by a static stress change that encouraged failure. The magnitude of the stress increases transferred from one <span class="hlt">earthquake</span> to another ranged from 0.01 MPa (0.1 bar) to over 0.1 MPa (1 bar). Stresses were reduced by up to 0.1 MPa over most of the Rainbow Mountain-Fairview Peak area as a result of the <span class="hlt">earthquake</span> sequence. Copyright 1996 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.S41A1898G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.S41A1898G"><span>Searching for the buried memory of past strong <span class="hlt">earthquakes</span> on strike-slip <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garambois, S.; Manighetti, I.; Malavieille, J.; Langridge, R. M.; Davies, T. R.</p> <p>2009-12-01</p> <p>On strike-slip <span class="hlt">faults</span>, the effect of a large <span class="hlt">earthquake</span> is to suddenly displace the ground surface laterally, often by up to several meters. A consequence is the lateral offset, hence lateral separation, of the preexisting ground features. In alluvial settings, the dominant surface features are the stream network and related sediments. Where ongoing sedimentation is significant, the surface imprints of an <span class="hlt">earthquake</span> may be rapidly buried under fresh sediments so that, when the next seismic event occurs (if not too close in time from the previous one), it offsets and deforms a younger soil layer possibly holding new markers such as newly formed drainage channels. Hence as <span class="hlt">earthquakes</span> repeat on a strike-slip <span class="hlt">fault</span> under ongoing sedimentation, the subsurface should keep part of their memory more or less buried in the form of distinctly offset markers, lying at various depths (0-10 m) in the ground. To search for that buried memory, we need non-invasive investigation methods, allowing imaging the sub-surface down to depths of several meters to 10s of meters. Ground penetrating radar (GPR) has appropriate resolution and acquisition time, provided that the subsurface layers are not too electrically conductive. We have performed serial 2D GPR profiles using 100 MHz antennas along several major strike-slip <span class="hlt">faults</span> in New Zealand. In particular, at the Mason river site on the Hope dextral <span class="hlt">fault</span>, four 450 m-long profiles were recorded parallel to the <span class="hlt">fault</span>, two on each northern and southern compartments of the <span class="hlt">fault</span>, whose surfaces are made of the 14-26 ka-old Terako alluvial terrace. The processed GPR data show the ground architecture only down to 5 meters in such conductive sediments. The profiles however reveal a number of places along the <span class="hlt">fault</span> where the reflector pile is deflected at depth to form concave-up patterns. Some of those buried features have their edges extending up to the ground surface, what suggests they may post-date the Terako terrace surface. Most of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028930','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028930"><span>Surface <span class="hlt">fault</span> slip associated with the 2004 Parkfield, California, <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rymer, M.J.; Tinsley, J. C.; Treiman, J.A.; Arrowsmith, J.R.; Ciahan, K.B.; Rosinski, A.M.; Bryant, W.A.; Snyder, H.A.; Fuis, G.S.; Toke, N.A.; Bawden, G.W.</p> <p>2006-01-01</p> <p>Surface fracturing occurred along the San Andreas <span class="hlt">fault</span>, the subparallel Southwest Fracture Zone, and six secondary <span class="hlt">faults</span> in association with the 28 September 2004 (M 6.0) Parkfield <span class="hlt">earthquake</span>. Fractures formed discontinuous breaks along a 32-km-long stretch of the San Andreas <span class="hlt">fault</span>. Sense of slip was right lateral; only locally was there a minor (1-11 mm) vertical component of slip. Right-lateral slip in the first few weeks after the event, early in its afterslip period, ranged from 1 to 44 mm. Our observations in the weeks following the <span class="hlt">earthquake</span> indicated that the highest slip values are in the Middle Mountain area, northwest of the mainshock epicenter (creepmeter measurements indicate a similar distribution of slip). Surface slip along the San Andreas <span class="hlt">fault</span> developed soon after the mainshock; field checks in the area near Parkfield and about 5 km to the southeast indicated that surface slip developed more than 1 hr but generally less than 1 day after the event. Slip along the Southwest Fracture Zone developed coseismically and extended about 8 km. Sense of slip was right lateral; locally there was a minor to moderate (1-29 mm) vertical component of slip. Right-lateral slip ranged from 1 to 41 mm. Surface slip along secondary <span class="hlt">faults</span> was right lateral; the right-lateral component of slip ranged from 3 to 5 mm. Surface slip in the 1966 and 2004 events occurred along both the San Andreas <span class="hlt">fault</span> and the Southwest Fracture Zone. In 1966 the length of ground breakage along the San Andreas <span class="hlt">fault</span> extended 5 km longer than that mapped in 2004. In contrast, the length of ground breakage along the Southwest Fracture Zone was the same in both events, yet the surface fractures were more continuous in 2004. Surface slip on secondary <span class="hlt">faults</span> in 2004 indicated previously unmapped structural connections between the San Andreas <span class="hlt">fault</span> and the Southwest Fracture Zone, further revealing aspects of the structural setting and <span class="hlt">fault</span> interactions in the Parkfield area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1212744D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1212744D"><span><span class="hlt">Fault</span> Lubrication and <span class="hlt">Earthquake</span> Propagation in Thermally Unstable Rocks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Paola, Nicola; Hirose, Takehiro; Mitchell, Tom; di Toro, Giulio; Viti, Cecilia; Shimamoto, Toshiko</p> <p>2010-05-01</p> <p>During <span class="hlt">earthquake</span> propagation in thermally unstable rocks, the frictional heat generated can induce thermal reactions which lead to chemical and physical changes in the slip zone. We performed laboratory friction experiments on thermally unstable minerals (gypsum, dolomite and calcite) at about 1 m/s slip velocities, more than 1 m displacements and calculated temperature rise above 500 C degrees. These conditions are typical during the propagation of large <span class="hlt">earthquakes</span>. The main findings of our experimental work are: 1) Dramatic <span class="hlt">fault</span> weakening is characterized by a dynamic frictional strength drop up to 90% of the initial static value in the Byerlee's range. 2) Seismic source parameters, calculated from our experimental results, match those obtained by modelling of seismological data from the 1997 Cofliorito <span class="hlt">earthquake</span> nucleated in carbonate rocks in Italy (i.e. same rocks used in the friction experiments). <span class="hlt">Fault</span> lubrication observed during the experiments is controlled by the superposition of multiple, thermally-activated, slip weakening mechanisms (e.g., flash heating, thermal pressurization and nanoparticle lubrication). The integration of mechanical and CO2 emission data, temperature rise calculations and XRPD analyses suggests that flash heating is not the main dynamic slip weakening process. This process was likely inhibited very soon (t < 1s) for displacements d < 0.20 m, when intense grain size reduction by both cataclastic and chemical/thermal processes took place. Conversely, most of the dynamic weakening observed was controlled by thermal pressurization and nanoparticle lubrication processes. The dynamic shear strength of experimental <span class="hlt">faults</span> was reduced when fluids (CO2, H2O) were trapped and pressurized within the slip zone, in accord with the effective normal stress principle. The fluids were not initially present in the slip zone, but were released by decarbonation (dolomite and Mg-rich calcite) and dehydration (gypsum) reactions, both activated by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T52A..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T52A..02D"><span><span class="hlt">Fault</span> Lubrication and <span class="hlt">Earthquake</span> Propagation in Thermally Unstable Rocks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Paola, N.; Hirose, T.; Mitchell, T. M.; di Toro, G.; Viti, C.; Shimamoto, T.</p> <p>2009-12-01</p> <p>During <span class="hlt">earthquake</span> propagation in thermally unstable rocks, the frictional heat generated can induce thermal reactions which lead to chemical and physical changes in the slip zone. We performed laboratory friction experiments on thermally unstable minerals (gypsum, dolomite and calcite) at about 1 m/s slip velocities, more than 1 m displacements and calculated temperature rise above 500 C degrees. These conditions are typical during the propagation of large <span class="hlt">earthquakes</span>. The main findings of our experimental work are: 1) Dramatic <span class="hlt">fault</span> weakening is characterized by a dynamic frictional strength drop up to 90% of the initial static value in the Byerlee’s range. 2) Seismic source parameters, calculated from our experimental results, match those obtained by modelling of seismological data from the 1997 Cofliorito <span class="hlt">earthquake</span> nucleated in carbonate rocks in Italy (i.e. same rocks used in the friction experiments). <span class="hlt">Fault</span> lubrication observed during the experiments is controlled by the superposition of multiple, thermally-activated, slip weakening mechanisms (e.g., flash heating, thermal pressurization and nanoparticle lubrication). The integration of mechanical and CO2 emission data, temperature rise calculations and XRPD analyses suggests that flash heating is not the main dynamic slip weakening process. This process was likely inhibited very soon (t < 1s) for displacements d < 0.20 m, when intense grain size reduction by both cataclastic and chemical/thermal processes took place. Conversely, most of the dynamic weakening observed was controlled by thermal pressurization and nanoparticle lubrication processes. The dynamic shear strength of experimental <span class="hlt">faults</span> was reduced when fluids (CO2, H2O) were trapped and pressurized within the slip zone, in accord with the effective normal stress principle. The fluids were not initially present in the slip zone, but were released by decarbonation (dolomite and Mg-rich calcite) and dehydration (gypsum) reactions, both activated by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017166','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017166"><span>An <span class="hlt">earthquake</span> mechanism based on rapid sealing of <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Blanpied, M.L.; Lockner, D.A.; Byerlee, J.D.</p> <p>1992-01-01</p> <p>RECENT seismological, heat flow and stress measurements in active <span class="hlt">fault</span> zones such as the San Andreas have led to the suggestion1,2 that such zones can be relatively weak. One explanation for this may be the presence of overpressured fluids along the <span class="hlt">fault</span>3-5, which would reduce the shear stress required for sliding by partially 'floating' the rock. Although several mechanisms have been proposed for overpressurizing <span class="hlt">fault</span> fluids3,4,6,7, we recall that 'pressure seals' are known to form in both sedimentary8 and igneous9 rocks by the redistribution of materials in solution; the formation of such a seal along the boundaries of a <span class="hlt">fault</span> will prevent the communication of fluids between the porous, deforming <span class="hlt">fault</span> zone and the surrounding country rock. Compaction of <span class="hlt">fault</span> gouge, under hydrostatic loading and/or during shear, elevates pore pressure in the sealed <span class="hlt">fault</span> and allows sliding at low shear stress. We report the results of laboratory sliding experiments on granite, which demonstrate that the sliding resistance of <span class="hlt">faults</span> can be significantly decreased by sealing and compaction. The weakening that results from shear-induced compaction can be rapid, and may provide an instability mechanism for <span class="hlt">earthquakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S23B2778L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S23B2778L"><span>Microearthquake detection at 2012 M4.9 Qiaojia <span class="hlt">earthquake</span> source area , the north of the Xiaojiang <span class="hlt">Fault</span> in Yunnan, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Y.; Yang, H.; Zhou, S.; Yan, C.</p> <p>2016-12-01</p> <p>We perform a comprehensive analysis in Yunnan area based on continuous seismic data of 38 stations of Qiaojia Network in Xiaojiang <span class="hlt">Fault</span> from 2012.3 to 2015.2. We use an effective method: Match and Locate (M&L, Zhang&Wen, 2015) to detect and locate microearthquakes to conduct our research. We first study dynamic triggering around the Xiaojiang <span class="hlt">Fault</span> in Yunnan. The triggered <span class="hlt">earthquakes</span> are identified as two impulsive seismic arrivals in 2Hz-highpass-filtered velocity seismograms during the passage of surface waves of large teleseismic <span class="hlt">earthquakes</span>. We only find two <span class="hlt">earthquakes</span> that may have triggered regional <span class="hlt">earthquakes</span> through inspecting their spectrograms: Mexico Mw7.4 <span class="hlt">earthquake</span> in 03/20/2012 and El Salvador Mw7.3 <span class="hlt">earthquake</span> in 10/14/2014. To confirm the two <span class="hlt">earthquakes</span> are triggered instead of coincidence, we use M&L to search if there are any repeating <span class="hlt">earthquakes</span>. The result of the coefficients shows that it is a coincidence during the surface waves of El Salvador <span class="hlt">earthquake</span> and whether 2012 Mexico have triggered <span class="hlt">earthquake</span> is under discussion. We then visually inspect the 2-8Hz-bandpass-filterd velocity envelopes of these years to search for non-volcanic tremor. We haven't detected any signals similar to non-volcanic tremors yet. In the following months, we are going to study the 2012 M4.9 Qiaojia <span class="hlt">earthquake</span>. It occurred only 30km west of the epicenter of the 2014 M6.5 Ludian <span class="hlt">earthquake</span>. We use Match and Locate (M&L) technique to detect and relocate microearthquakes that occurred 2 days before and 3 days after the mainshock. Through this, we could obtain several times more events than listed in the catalogs provided by NEIC and reduce the magnitude of completeness Mc. We will also detect microearthquakes along Xiaojiang <span class="hlt">Fault</span> using template <span class="hlt">earthquakes</span> listed in the catalogs to learn more about <span class="hlt">fault</span> shape and other properties of Xiaojiang <span class="hlt">Fault</span>. Analyzing seismicity near Xiaojiang <span class="hlt">Fault</span> systematically may cast insight on our understanding of the features of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1818112T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1818112T"><span>The numerical simulation study of the dynamic evolutionary processes in an <span class="hlt">earthquake</span> cycle on the Longmen Shan <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tao, Wei; Shen, Zheng-Kang; Zhang, Yong</p> <p>2016-04-01</p> <p>The Longmen Shan, located in the conjunction of the eastern margin the Tibet plateau and Sichuan basin, is a typical area for studying the deformation pattern of the Tibet plateau. Following the 2008 Mw 7.9 Wenchuan <span class="hlt">earthquake</span> (WE) rupturing the Longmen Shan <span class="hlt">Fault</span> (LSF), a great deal of observations and studies on geology, geophysics, and geodesy have been carried out for this region, with results published successively in recent years. Using the 2D viscoelastic finite element model, introducing the rate-state friction law to the <span class="hlt">fault</span>, this thesis makes modeling of the <span class="hlt">earthquake</span> recurrence process and the dynamic evolutionary processes in an <span class="hlt">earthquake</span> cycle of 10 thousand years. By analyzing the displacement, velocity, stresses, strain energy and strain energy increment fields, this work obtains the following conclusions: (1) The maximum coseismic displacement on the <span class="hlt">fault</span> is on the surface, and the damage on the hanging wall is much more serious than that on the foot wall of the <span class="hlt">fault</span>. If the detachment layer is absent, the coseismic displacement would be smaller and the relative displacement between the hanging wall and foot wall would also be smaller. (2) In every stage of the <span class="hlt">earthquake</span> cycle, the velocities (especially the vertical velocities) on the hanging wall of the <span class="hlt">fault</span> are larger than that on the food wall, and the values and the distribution patterns of the velocity fields are similar. While in the locking stage prior to the <span class="hlt">earthquake</span>, the velocities in crust and the relative velocities between hanging wall and foot wall decrease. For the model without the detachment layer, the velocities in crust in the post-seismic stage is much larger than those in other stages. (3) The maximum principle stress and the maximum shear stress concentrate around the joint of the <span class="hlt">fault</span> and detachment layer, therefore the <span class="hlt">earthquake</span> would nucleate and start here. (4) The strain density distribution patterns in stages of the <span class="hlt">earthquake</span> cycle are similar. There are two</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026864','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026864"><span>A teleseismic study of the 2002 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span> and implications for rapid strong-motion estimation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ji, C.; Helmberger, D.V.; Wald, D.J.</p> <p>2004-01-01</p> <p>Slip histories for the 2002 M7.9 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span> are derived rapidly from global teleseismic waveform data. In phases, three models improve matching waveform data and recovery of rupture details. In the first model (Phase I), analogous to an automated solution, a simple <span class="hlt">fault</span> plane is fixed based on the preliminary Harvard Centroid Moment Tensor mechanism and the epicenter provided by the Preliminary Determination of Epicenters. This model is then updated (Phase II) by implementing a more realistic <span class="hlt">fault</span> geometry inferred from Digital Elevation Model topography and further (Phase III) by using the calibrated P-wave and SH-wave arrival times derived from modeling of the nearby 2002 M6.7 Nenana Mountain <span class="hlt">earthquake</span>. These models are used to predict the peak ground velocity and the shaking intensity field in the <span class="hlt">fault</span> vicinity. The procedure to estimate local strong motion could be automated and used for global real-time <span class="hlt">earthquake</span> shaking and damage assessment. ?? 2004, <span class="hlt">Earthquake</span> Engineering Research Institute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T33D..05R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T33D..05R"><span>Could offset cluster reveal strong <span class="hlt">earthquake</span> pattern?——case study from Haiyuan <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, Z.; Zhang, Z.; Chen, T.; Yin, J.; Zhang, P. Z.; Zheng, W.; Zhang, H.; Li, C.</p> <p>2016-12-01</p> <p>Since 1990s, researchers tried to use offset clusters to study strong <span class="hlt">earthquake</span> patterns. However, due to the limitation of quantity of offset data, it was not widely used until recent years with the rapid development of high-resolution topographic data, such as remote sensing images, LiDAR. In this study, we use airborne LiDAR data to re-evaluate the cumulative offsets and co-seismic offset of the 1920 Haiyuan Ms 8.5 <span class="hlt">earthquake</span> along the western and middle segments of the co-seismic surface rupture zone. Our LiDAR data indicate the offset observations along both the western and middle segments fall into five groups. The group with minimum slip amount is associated with the 1920 Haiyuan Ms 8.5 <span class="hlt">earthquake</span>, which ruptured both the western and middle segments. Our research highlights two new interpretations: firstly, the previously reported maximum displacement of the 1920 <span class="hlt">Earthquake</span> is likely to be produced by at least two <span class="hlt">earthquakes</span>; secondly, Our results reveal that the Cumulative Offset Probability Density (COPD) peaks of same offset amount on western segment and middles segment did not corresponding to each other one by one. The ages of the paleoearthquakes indicate the offsets are not accumulated during same period. We suggest that any discussion of the rupture pattern of a certain <span class="hlt">fault</span> based on the offset data should also consider <span class="hlt">fault</span> segmentation and paleoseismological data; Therefore, using the COPD peaks for studying the number of palaeo-events and their rupture patterns, the COPD peaks should be computed and analyzed on <span class="hlt">fault</span> sub-sections and not entire <span class="hlt">fault</span> zones. Our results reveal that the rupture pattern on the western and middle segment of the Haiyuan <span class="hlt">Fault</span> is different from each other, which provide new data for the regional seismic potential analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7855W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7855W"><span>How large is the <span class="hlt">fault</span> slip at trench in the M=9 Tohoku-oki <span class="hlt">earthquake</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Kelin; Sun, Tianhaozhe; Fujiwara, Toshiya; Kodaira, Shuichi; He, Jiangheng</p> <p>2015-04-01</p> <p>It is widely known that coseismic slip breached the trench during the 2011 Mw=9 Tohoku-oki <span class="hlt">earthquake</span>, responsible for generating a devastating tsunami. For understanding both the mechanics of megathrust rupture and the mechanism of tsunami generation, it is important to know how much <span class="hlt">fault</span> slip actually occurred at the trench. But the answer has remained elusive because most of the data from this <span class="hlt">earthquake</span> do not provide adequate near-trench resolution. Seafloor GPS sites were located > 30 km from the trench. Near-trench seafloor pressure records suffered from complex vertical deformation at local scales. Seismic inversion does not have adequate accuracy at the trench. Inversion of tsunami data is highly dependent on the parameterization of the <span class="hlt">fault</span> near the trench. The severity of the issue is demonstrated by our compilation of rupture models for this <span class="hlt">earthquake</span> published by ~40 research groups using multiple sets of coseismic observations. In the peak slip area, <span class="hlt">fault</span> slip at the trench depicted by these models ranges from zero to >90 m. The <span class="hlt">faults</span> in many models do not reach the trench because of simplification of <span class="hlt">fault</span> geometry. In this study, we use high-resolution differential bathymetry, that is, bathymetric differences before and after the <span class="hlt">earthquake</span>, to constrain coseismic slip at and near the trench along a corridor in the area of largest moment release. We use a 3D elastic finite element model including real <span class="hlt">fault</span> geometry and surface topography to produce Synthetic Differential Bathymetry (SDB) and compare it with the observed differential bathymetry. <span class="hlt">Earthquakes</span> induce bathymetric changes by shifting the sloping seafloor seaward and by warping the seafloor through internal deformation of rocks. These effects are simulated by our SDB modeling, except for the permanent formation of the upper plate which is like to be limited and localized. Bathymetry data were collected by JAMSTEC in 1999, 2004, and in 2011 right after the M=9 <span class="hlt">earthquake</span>. Our SDB</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....13093A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....13093A"><span>Broadband Rupture Process of the 2001 Kunlun <span class="hlt">Fault</span> (Mw 7.8) <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Antolik, M.; Abercrombie, R.; Ekstrom, G.</p> <p>2003-04-01</p> <p>We model the source process of the 14 November, 2001 Kunlun <span class="hlt">fault</span> <span class="hlt">earthquake</span> using broadband body waves from the Global Digital Seismographic Network (P, SH) and both point-source and distributed slip techniques. The point-source mechanism technique is a non-linear iterative inversion that solves for focal mechanism, moment rate function, depth, and rupture directivity. The P waves reveal a complex rupture process for the first 30 s, with smooth unilateral rupture toward the east along the Kunlun <span class="hlt">fault</span> accounting for the remainder of the 120 s long rupture. The obtained focal mechanism for the main portion of the rupture is (strike=96o, dip=83o, rake=-8o) which is consistent with both the Harvard CMT solution and observations of the surface rupture. The seismic moment is 5.29×1020 Nm and the average rupture velocity is ˜3.5 km/s. However, the initial portion of the P waves cannot be fit at all with this mechanism. A strong pulse visible in the first 20 s can only be matched with an oblique-slip subevent (MW ˜ 6.8-7.0) involving a substantial normal <span class="hlt">faulting</span> component, but the nodal planes of this mechanism are not well constrained. The first-motion polarities of the P waves clearly require a strike mechanism with a similar orientation as the Kunlun <span class="hlt">fault</span>. Field observations of the surface rupture (Xu et al., SRL, 73, No. 6) reveal a small 26 km-long strike-slip rupture at the far western end (90.5o E) with a 45-km long gap and extensional step-over between this rupture and the main Kunlun <span class="hlt">fault</span> rupture. We hypothesize that the initial <span class="hlt">fault</span> break occurred on this segment, with release of the normal <span class="hlt">faulting</span> energy as a continuous rupture through the extensional step, enabling transfer of the slip to the main Kunlun <span class="hlt">fault</span>. This process is similar to that which occurred during the 2002 Denali <span class="hlt">fault</span> (MW 7.9) <span class="hlt">earthquake</span> sequence except that 11 days elapsed between the October 23 (M_W 6.7) foreshock and the initial break of the Denali <span class="hlt">earthquake</span> along a thrust <span class="hlt">fault</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914161P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914161P"><span>The Surface <span class="hlt">faulting</span> produced by the 30 October 2016 Mw 6.5 Central Italy <span class="hlt">earthquake</span>: the Open EMERGEO Working Group experience</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pantosti, Daniela</p> <p>2017-04-01</p> <p>The October 30, 2016 (06:40 UTC) Mw 6.5 <span class="hlt">earthquake</span> occurred about 28 km NW of Amatrice village as the result of upper crust normal <span class="hlt">faulting</span> on a nearly 30 km-long, NW-SE oriented, SW dipping <span class="hlt">fault</span> <span class="hlt">system</span> in the Central Apennines. This <span class="hlt">earthquake</span> is the strongest Italian seismic event since the 1980 Mw 6.9 Irpinia <span class="hlt">earthquake</span>. The Mw 6.5 event was the largest shock of a seismic sequence, which began on August 24 with a Mw 6.0 <span class="hlt">earthquake</span> and also included a Mw 5.9 <span class="hlt">earthquake</span> on October 26, about 9 and 35 km NW of Amatrice village, respectively. Field surveys of coseismic geological effects at the surface started within hours of the mainshock and were carried out by several national and international teams of earth scientists (about 120 people) from different research institutions and universities coordinated by the EMERGEO Working Group of the Istituto Nazionale di Geofisica e Vulcanologia. This collaborative effort was focused on the detailed recognition and mapping of: 1) the total extent of the October 30 coseismic surface ruptures, 2) their geometric and kinematic characteristics, 3) the coseismic displacement distribution along the activated <span class="hlt">fault</span> <span class="hlt">system</span>, including subsidiary and antithetic ruptures. The huge amount of collected data (more than 8000 observation points of several types of coseismic effects at the surface) were stored, managed and shared using a specifically designed spreadsheet to populate a georeferenced database. More comprehensive mapping of the details and extent of surface rupture was facilitated by Structure-from-Motion photogrammetry surveys by means of several helicopter flights. An almost continuous alignment of ruptures about 30 km long, N150/160 striking, mainly SW side down was observed along the already known active Mt. Vettore - Mt. Bove <span class="hlt">fault</span> <span class="hlt">system</span>. The mapped ruptures occasionally overlapped those of the August 24 Mw 6.0 and October 26 Mw 5.9 shocks. The coincidence between the observed surface ruptures and the trace of active</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoJI.tmp..186R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoJI.tmp..186R"><span>Accounting for uncertain <span class="hlt">fault</span> geometry in <span class="hlt">earthquake</span> source inversions - I: theory and simplified application</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ragon, Théa; Sladen, Anthony; Simons, Mark</p> <p>2018-05-01</p> <p>The ill-posed nature of <span class="hlt">earthquake</span> source estimation derives from several factors including the quality and quantity of available observations and the fidelity of our forward theory. Observational errors are usually accounted for in the inversion process. Epistemic errors, which stem from our simplified description of the forward problem, are rarely dealt with despite their potential to bias the estimate of a source model. In this study, we explore the impact of uncertainties related to the choice of a <span class="hlt">fault</span> geometry in source inversion problems. The geometry of a <span class="hlt">fault</span> structure is generally reduced to a set of parameters, such as position, strike and dip, for one or a few planar <span class="hlt">fault</span> segments. While some of these parameters can be solved for, more often they are fixed to an uncertain value. We propose a practical framework to address this limitation by following a previously implemented method exploring the impact of uncertainties on the elastic properties of our models. We develop a sensitivity analysis to small perturbations of <span class="hlt">fault</span> dip and position. The uncertainties in <span class="hlt">fault</span> geometry are included in the inverse problem under the formulation of the misfit covariance matrix that combines both prediction and observation uncertainties. We validate this approach with the simplified case of a <span class="hlt">fault</span> that extends infinitely along strike, using both Bayesian and optimization formulations of a static inversion. If epistemic errors are ignored, predictions are overconfident in the data and source parameters are not reliably estimated. In contrast, inclusion of uncertainties in <span class="hlt">fault</span> geometry allows us to infer a robust posterior source model. Epistemic uncertainties can be many orders of magnitude larger than observational errors for great <span class="hlt">earthquakes</span> (Mw > 8). Not accounting for uncertainties in <span class="hlt">fault</span> geometry may partly explain observed shallow slip deficits for continental <span class="hlt">earthquakes</span>. Similarly, ignoring the impact of epistemic errors can also bias estimates of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2017/5013/sir20175013ah_v1.1.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2017/5013/sir20175013ah_v1.1.pdf"><span>The HayWired <span class="hlt">Earthquake</span> Scenario—<span class="hlt">Earthquake</span> Hazards</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Detweiler, Shane T.; Wein, Anne M.</p> <p>2017-04-24</p> <p>The HayWired scenario is a hypothetical <span class="hlt">earthquake</span> sequence that is being used to better understand hazards for the San Francisco Bay region during and after an <span class="hlt">earthquake</span> of magnitude 7 on the Hayward <span class="hlt">Fault</span>. The 2014 Working Group on California <span class="hlt">Earthquake</span> Probabilities calculated that there is a 33-percent likelihood of a large (magnitude 6.7 or greater) <span class="hlt">earthquake</span> occurring on the Hayward <span class="hlt">Fault</span> within three decades. A large Hayward <span class="hlt">Fault</span> <span class="hlt">earthquake</span> will produce strong ground shaking, permanent displacement of the Earth’s surface, landslides, liquefaction (soils becoming liquid-like during shaking), and subsequent <span class="hlt">fault</span> slip, known as afterslip, and <span class="hlt">earthquakes</span>, known as aftershocks. The most recent large <span class="hlt">earthquake</span> on the Hayward <span class="hlt">Fault</span> occurred on October 21, 1868, and it ruptured the southern part of the <span class="hlt">fault</span>. The 1868 magnitude-6.8 <span class="hlt">earthquake</span> occurred when the San Francisco Bay region had far fewer people, buildings, and infrastructure (roads, communication lines, and utilities) than it does today, yet the strong ground shaking from the <span class="hlt">earthquake</span> still caused significant building damage and loss of life. The next large Hayward <span class="hlt">Fault</span> <span class="hlt">earthquake</span> is anticipated to affect thousands of structures and disrupt the lives of millions of people. <span class="hlt">Earthquake</span> risk in the San Francisco Bay region has been greatly reduced as a result of previous concerted efforts; for example, tens of billions of dollars of investment in strengthening infrastructure was motivated in large part by the 1989 magnitude 6.9 Loma Prieta <span class="hlt">earthquake</span>. To build on efforts to reduce <span class="hlt">earthquake</span> risk in the San Francisco Bay region, the HayWired <span class="hlt">earthquake</span> scenario comprehensively examines the <span class="hlt">earthquake</span> hazards to help provide the crucial scientific information that the San Francisco Bay region can use to prepare for the next large <span class="hlt">earthquake</span>, The HayWired <span class="hlt">Earthquake</span> Scenario—<span class="hlt">Earthquake</span> Hazards volume describes the strong ground shaking modeled in the scenario and the hazardous movements of</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017613','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017613"><span>Large mid-Holocene and late Pleistocene <span class="hlt">earthquakes</span> on the Oquirrh <span class="hlt">fault</span> zone, Utah</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Olig, S.S.; Lund, W.R.; Black, B.D.</p> <p>1994-01-01</p> <p>The Oquirrh <span class="hlt">fault</span> zone is a range-front normal <span class="hlt">fault</span> that bounds the east side of Tooele Valley and it has long been recognized as a potential source for large <span class="hlt">earthquakes</span> that pose a significant hazard to population centers along the Wasatch Front in central Utah. Scarps of the Oquirrh <span class="hlt">fault</span> zone offset the Provo shoreline of Lake Bonneville and previous studies of scarp morphology suggested that the most recent surface-<span class="hlt">faulting</span> <span class="hlt">earthquake</span> occurred between 9000 and 13,500 years ago. Based on a potential rupture length of 12 to 21 km from previous mapping, moment magnitude (Mw) estimates for this event range from 6.3 to 6.6 In contrast, our results from detailed mapping and trench excavations at two sites indicate that the most-recent event actually occurred between 4300 and 6900 yr B.P. (4800 and 7900 cal B.P.) and net vertical displacements were 2.2 to 2.7 m, much larger than expected considering estimated rupture lengths for this event. Empirical relations between magnitude and displacement yield Mw 7.0 to 7.2. A few, short discontinuous <span class="hlt">fault</span> scarps as far south as Stockton, Utah have been identified in a recent mapping investigation and our results suggest that they may be part of the Oquirrh <span class="hlt">fault</span> zone, increasing the total <span class="hlt">fault</span> length to 32 km. These results emphasize the importance of integrating stratigraphic and geomorphic information in <span class="hlt">fault</span> investigations for <span class="hlt">earthquake</span> hazard evaluations. At both the Big Canyon and Pole Canyon sites, trenches exposed <span class="hlt">faulted</span> Lake Bonneville sediments and thick wedges of <span class="hlt">fault</span>-scarp derived colluvium associated with the most-recent event. Bulk sediment samples from a <span class="hlt">faulted</span> debris-flow deposit at the Big Canyon site yield radiocarbon ages of 7650 ?? 90 yr B.P. and 6840 ?? 100 yr B.P. (all lab errors are ??1??). A bulk sediment sample from unfaulted fluvial deposits that bury the <span class="hlt">fault</span> scarp yield a radiocarbon age estimate of 4340 ?? 60 yr B.P. Stratigraphic evidence for a pre-Bonneville lake cycle penultimate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.489..135X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.489..135X"><span>Kinematics of the 2015 San Ramon, California <span class="hlt">earthquake</span> swarm: Implications for <span class="hlt">fault</span> zone structure and driving mechanisms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, Lian; Bürgmann, Roland; Shelly, David R.; Johnson, Christopher W.; Taira, Taka'aki</p> <p>2018-05-01</p> <p><span class="hlt">Earthquake</span> swarms represent a sudden increase in seismicity that may indicate a heterogeneous <span class="hlt">fault</span>-zone, the involvement of crustal fluids and/or slow <span class="hlt">fault</span> slip. Swarms sometimes precede major <span class="hlt">earthquake</span> ruptures. An <span class="hlt">earthquake</span> swarm occurred in October 2015 near San Ramon, California in an extensional right step-over region between the northern Calaveras <span class="hlt">Fault</span> and the Concord-Mt. Diablo <span class="hlt">fault</span> zone, which has hosted ten major swarms since 1970. The 2015 San Ramon swarm is examined here from 11 October through 18 November using template matching analysis. The relocated seismicity catalog contains ∼4000 events with magnitudes between - 0.2 <Md < 3.6. The swarm illuminated three sub-parallel, southwest striking and northwest dipping <span class="hlt">fault</span> segments of km-scale dimension and thickness of up to 200 m. The segments contain coexisting populations of different focal-mechanisms, suggesting a complex <span class="hlt">fault</span> zone structure with several sets of en échelon <span class="hlt">fault</span> orientations. The migration of events along the three planar structures indicates a complex fluid and <span class="hlt">faulting</span> interaction processes. We searched for correlations between seismic activity and tidal stresses and found some suggestive features, but nothing that we can be confident is statistically significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/pp1550/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/pp1550/"><span>The Loma Prieta, California, <span class="hlt">Earthquake</span> of October 17, 1989: <span class="hlt">Earthquake</span> Occurrence</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Coordinated by Bakun, William H.; Prescott, William H.</p> <p>1993-01-01</p> <p>Professional Paper 1550 seeks to understand the M6.9 Loma Prieta <span class="hlt">earthquake</span> itself. It examines how the <span class="hlt">fault</span> that generated the <span class="hlt">earthquake</span> ruptured, searches for and evaluates precursors that may have indicated an <span class="hlt">earthquake</span> was coming, reviews forecasts of the <span class="hlt">earthquake</span>, and describes the geology of the <span class="hlt">earthquake</span> area and the crustal forces that affect this geology. Some significant findings were: * Slip during the <span class="hlt">earthquake</span> occurred on 35 km of <span class="hlt">fault</span> at depths ranging from 7 to 20 km. Maximum slip was approximately 2.3 m. The <span class="hlt">earthquake</span> may not have released all of the strain stored in rocks next to the <span class="hlt">fault</span> and indicates a potential for another damaging <span class="hlt">earthquake</span> in the Santa Cruz Mountains in the near future may still exist. * The <span class="hlt">earthquake</span> involved a large amount of uplift on a dipping <span class="hlt">fault</span> plane. Pre-<span class="hlt">earthquake</span> conventional wisdom was that large <span class="hlt">earthquakes</span> in the Bay area occurred as horizontal displacements on predominantly vertical <span class="hlt">faults</span>. * The <span class="hlt">fault</span> segment that ruptured approximately coincided with a <span class="hlt">fault</span> segment identified in 1988 as having a 30% probability of generating a M7 <span class="hlt">earthquake</span> in the next 30 years. This was one of more than 20 relevant <span class="hlt">earthquake</span> forecasts made in the 83 years before the <span class="hlt">earthquake</span>. * Calculations show that the Loma Prieta <span class="hlt">earthquake</span> changed stresses on nearby <span class="hlt">faults</span> in the Bay area. In particular, the <span class="hlt">earthquake</span> reduced stresses on the Hayward <span class="hlt">Fault</span> which decreased the frequency of small <span class="hlt">earthquakes</span> on it. * Geological and geophysical mapping indicate that, although the San Andreas <span class="hlt">Fault</span> can be mapped as a through going <span class="hlt">fault</span> in the epicentral region, the southwest dipping Loma Prieta rupture surface is a separate <span class="hlt">fault</span> strand and one of several along this part of the San Andreas that may be capable of generating <span class="hlt">earthquakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..122.5691W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..122.5691W"><span>A 667 year record of coseismic and interseismic Coulomb stress changes in central Italy reveals the role of <span class="hlt">fault</span> interaction in controlling irregular <span class="hlt">earthquake</span> recurrence intervals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wedmore, L. N. J.; Faure Walker, J. P.; Roberts, G. P.; Sammonds, P. R.; McCaffrey, K. J. W.; Cowie, P. A.</p> <p>2017-07-01</p> <p>Current studies of <span class="hlt">fault</span> interaction lack sufficiently long <span class="hlt">earthquake</span> records and measurements of <span class="hlt">fault</span> slip rates over multiple seismic cycles to fully investigate the effects of interseismic loading and coseismic stress changes on the surrounding <span class="hlt">fault</span> network. We model elastic interactions between 97 <span class="hlt">faults</span> from 30 <span class="hlt">earthquakes</span> since 1349 A.D. in central Italy to investigate the relative importance of co-seismic stress changes versus interseismic stress accumulation for <span class="hlt">earthquake</span> occurrence and <span class="hlt">fault</span> interaction. This region has an exceptionally long, 667 year record of historical <span class="hlt">earthquakes</span> and detailed constraints on the locations and slip rates of its active normal <span class="hlt">faults</span>. Of 21 <span class="hlt">earthquakes</span> since 1654, 20 events occurred on <span class="hlt">faults</span> where combined coseismic and interseismic loading stresses were positive even though 20% of all <span class="hlt">faults</span> are in "stress shadows" at any one time. Furthermore, the Coulomb stress on the <span class="hlt">faults</span> that experience <span class="hlt">earthquakes</span> is statistically different from a random sequence of <span class="hlt">earthquakes</span> in the region. We show how coseismic Coulomb stress changes can alter <span class="hlt">earthquake</span> interevent times by 103 years, and <span class="hlt">fault</span> length controls the intensity of this effect. Static Coulomb stress changes cause greater interevent perturbations on shorter <span class="hlt">faults</span> in areas characterized by lower strain (or slip) rates. The exceptional duration and number of <span class="hlt">earthquakes</span> we model enable us to demonstrate the importance of combining long <span class="hlt">earthquake</span> records with detailed knowledge of <span class="hlt">fault</span> geometries, slip rates, and kinematics to understand the impact of stress changes in complex networks of active <span class="hlt">faults</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70182746','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70182746"><span>Fluid-<span class="hlt">faulting</span> evolution in high definition: Connecting <span class="hlt">fault</span> structure and frequency-magnitude variations during the 2014 Long Valley Caldera, California <span class="hlt">earthquake</span> swarm</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shelly, David R.; Ellsworth, William L.; Hill, David P.</p> <p>2016-01-01</p> <p>An extended <span class="hlt">earthquake</span> swarm occurred beneath southeastern Long Valley Caldera between May and November 2014, culminating in three magnitude 3.5 <span class="hlt">earthquakes</span> and 1145 cataloged events on 26 September alone. The swarm produced the most prolific seismicity in the caldera since a major unrest episode in 1997-1998. To gain insight into the physics controlling swarm evolution, we used large-scale cross-correlation between waveforms of cataloged <span class="hlt">earthquakes</span> and continuous data, producing precise locations for 8494 events, more than 2.5 times the routine catalog. We also estimated magnitudes for 18,634 events (~5.5 times the routine catalog), using a principal component fit to measure waveform amplitudes relative to cataloged events. This expanded and relocated catalog reveals multiple episodes of pronounced hypocenter expansion and migration on a collection of neighboring <span class="hlt">faults</span>. Given the rapid migration and alignment of hypocenters on narrow <span class="hlt">faults</span>, we infer that activity was initiated and sustained by an evolving fluid pressure transient with a low-viscosity fluid, likely composed primarily of water and CO2 exsolved from underlying magma. Although both updip and downdip migration were observed within the swarm, downdip activity ceased shortly after activation, while updip activity persisted for weeks at moderate levels. Strongly migrating, single-<span class="hlt">fault</span> episodes within the larger swarm exhibited a higher proportion of larger <span class="hlt">earthquakes</span> (lower Gutenberg-Richter b value), which may have been facilitated by fluid pressure confined in two dimensions within the <span class="hlt">fault</span> zone. In contrast, the later swarm activity occurred on an increasingly diffuse collection of smaller <span class="hlt">faults</span>, with a much higher b value.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S33F4934R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S33F4934R"><span>Pre-<span class="hlt">Earthquake</span> Paleoseismic Trenching in 2014 Along a Mapped Trace of the West Napa <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rubin, R. S.; Dawson, T. E.; Mareschal, M.</p> <p>2014-12-01</p> <p>Paleoseismic trenching in July 2014 across a previously mapped trace of the West Napa <span class="hlt">fault</span> in eastern Alston Park (EAP) was undertaken with NEHRP funding as part of an effort to better characterize activity of the <span class="hlt">fault</span> for regional seismic hazard assessments, and as part of an Alquist-Priolo <span class="hlt">Earthquake</span> <span class="hlt">Fault</span> Zoning (APEFZ) evaluation. The trench was excavated across a prominent escarpment that had been interpreted by others to represent evidence of Holocene <span class="hlt">fault</span> activity, based on <span class="hlt">faults</span> logged in an ~1-m-deep natural drainage exposure. Our trench was located ~3 m south of the drainage exposure and encompassed the interpreted <span class="hlt">fault</span> zone, and beyond. The trench exposed the same surficial units as the natural exposure, as well as additional Pleistocene and older stratigraphy at depth. Escarpment parallel channeling was evident within deposits along the base of the slope. <span class="hlt">Faulting</span> was not encountered, and is precluded by unbroken depositional contacts. Our preferred interpretation is that the escarpment in EAP is a result of fluvial and differential erosion, which is consistent with existence of channels along the base of the escarpment and a lack of <span class="hlt">faulting</span>. The location of surface rupture of the South Napa <span class="hlt">Earthquake</span> (SNE) of 8/24/14 occurred on <span class="hlt">fault</span> strands south and west of this study and crosses Alston Park approximately 800 m west of our trench site, at its nearest point. Pre- and post-<span class="hlt">earthquake</span> UAVSAR from NASA's JPL been useful in identifying major and minor ruptures of the SNE. Based on the imagery, a subtle lineament has been interpreted upslope from the trench. However, field observations along this feature yielded no visible surface deformation and the origin of this lineament is uncertain. The <span class="hlt">fault</span> rupture pattern expressed by the SNE, as reflected by detailed field mapping and UAVSAR imagery, provides a unique opportunity to better understand the complex nature of the West Napa <span class="hlt">fault</span>. Our study illustrates the value of subsurface investigations as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43.3134Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43.3134Z"><span>Mapping 3D <span class="hlt">fault</span> geometry in <span class="hlt">earthquakes</span> using high-resolution topography: Examples from the 2010 El Mayor-Cucapah (Mexico) and 2013 Balochistan (Pakistan) <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, Yu; Walker, Richard T.; Elliott, John R.; Parsons, Barry</p> <p>2016-04-01</p> <p><span class="hlt">Fault</span> dips are usually measured from outcrops in the field or inferred through geodetic or seismological modeling. Here we apply the classic structural geology approach of calculating dip from a <span class="hlt">fault</span>'s 3-D surface trace using recent, high-resolution topography. A test study applied to the 2010 El Mayor-Cucapah <span class="hlt">earthquake</span> shows very good agreement between our results and those previously determined from field measurements. To obtain a reliable estimate, a <span class="hlt">fault</span> segment ≥120 m long with a topographic variation ≥15 m is suggested. We then applied this method to the 2013 Balochistan <span class="hlt">earthquake</span>, getting dips similar to previous estimates. Our dip estimates show a switch from north to south dipping at the southern end of the main trace, which appears to be a response to local extension within a stepover. We suggest that this previously unidentified geometrical complexity may act as the endpoint of <span class="hlt">earthquake</span> ruptures for the southern end of the Hoshab <span class="hlt">fault</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S41A2401M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S41A2401M"><span>Source parameters of the 2013 Lushan, Sichuan, Ms7.0 <span class="hlt">earthquake</span> and estimation of the near-<span class="hlt">fault</span> strong ground motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meng, L.; Zhou, L.; Liu, J.</p> <p>2013-12-01</p> <p>Abstract: The April 20, 2013 Ms 7.0 <span class="hlt">earthquake</span> in Lushan city, Sichuan province of China occurred as the result of east-west oriented reverse-type motion on a north-south striking <span class="hlt">fault</span>. The source location suggests the event occurred on the Southern part of Longmenshan <span class="hlt">fault</span> at a depth of 13km. The Lushan <span class="hlt">earthquake</span> caused a great of loss of property and 196 deaths. The maximum intensity is up to VIII to IX at Boxing and Lushan city, which are located in the meizoseismal area. In this study, we analyzed the dynamic source process and calculated source spectral parameters, estimated the strong ground motion in the near-<span class="hlt">fault</span> field based on the Brune's circle model at first. A dynamical composite source model (DCSM) has been developed further to simulate the near-<span class="hlt">fault</span> strong ground motion with associated <span class="hlt">fault</span> rupture properties at Boxing and Lushan city, respectively. The results indicate that the frictional undershoot behavior in the dynamic source process of Lushan <span class="hlt">earthquake</span>, which is actually different from the overshoot activity of the Wenchuan <span class="hlt">earthquake</span>. Based on the simulated results of the near-<span class="hlt">fault</span> strong ground motion, described the intensity distribution of the Lushan <span class="hlt">earthquake</span> field. The simulated intensity indicated that, the maximum intensity value is IX, and region with and above VII almost 16,000km2, which is consistence with observation intensity published online by China <span class="hlt">Earthquake</span> Administration (CEA) on April 25. Moreover, the numerical modeling developed in this study has great application in the strong ground motion prediction and intensity estimation for the <span class="hlt">earthquake</span> rescue purpose. In fact, the estimation methods based on the empirical relationship and numerical modeling developed in this study has great application in the strong ground motion prediction for the <span class="hlt">earthquake</span> source process understand purpose. Keywords: Lushan, Ms7.0 <span class="hlt">earthquake</span>; near-<span class="hlt">fault</span> strong ground motion; DCSM; simulated intensity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780015706','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780015706"><span>Numerical and laboratory simulation of <span class="hlt">fault</span> motion and <span class="hlt">earthquake</span> occurrence</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cohen, S. C.</p> <p>1978-01-01</p> <p>Simple linear rheologies were used with elastic forces driving the main events and viscoelastic forces being important for aftershock and creep occurrence. Friction and its dependence on velocity, stress, and displacement also plays a key role in determining how, when, and where <span class="hlt">fault</span> motion occurs. The discussion of the qualitative behavior of the simulators focuses on the manner in which energy was stored in the <span class="hlt">system</span> and released by the unstable and stable sliding processes. The numerical results emphasize the statistics of <span class="hlt">earthquake</span> occurrence and the correlations among source parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.S13A0219S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.S13A0219S"><span>Automatic <span class="hlt">Earthquake</span> Shear Stress Measurement Method Developed for Accurate Time- Prediction Analysis of Forthcoming Major <span class="hlt">Earthquakes</span> Along Shallow Active <span class="hlt">Faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Serata, S.</p> <p>2006-12-01</p> <p>The Serata Stressmeter has been developed to measure and monitor <span class="hlt">earthquake</span> shear stress build-up along shallow active <span class="hlt">faults</span>. The development work made in the past 25 years has established the Stressmeter as an automatic stress measurement <span class="hlt">system</span> to study timing of forthcoming major <span class="hlt">earthquakes</span> in support of the current <span class="hlt">earthquake</span> prediction studies based on statistical analysis of seismological observations. In early 1982, a series of major Man-made <span class="hlt">earthquakes</span> (magnitude 4.5-5.0) suddenly occurred in an area over deep underground potash mine in Saskatchewan, Canada. By measuring underground stress condition of the mine, the direct cause of the <span class="hlt">earthquake</span> was disclosed. The cause was successfully eliminated by controlling the stress condition of the mine. The Japanese government was interested in this development and the Stressmeter was introduced to the Japanese government research program for <span class="hlt">earthquake</span> stress studies. In Japan the Stressmeter was first utilized for direct measurement of the intrinsic lateral tectonic stress gradient G. The measurement, conducted at the Mt. Fuji Underground Research Center of the Japanese government, disclosed the constant natural gradients of maximum and minimum lateral stresses in an excellent agreement with the theoretical value, i.e., G = 0.25. All the conventional methods of overcoring, hydrofracturing and deformation, which were introduced to compete with the Serata method, failed demonstrating the fundamental difficulties of the conventional methods. The intrinsic lateral stress gradient determined by the Stressmeter for the Japanese government was found to be the same with all the other measurements made by the Stressmeter in Japan. The stress measurement results obtained by the major international stress measurement work in the Hot Dry Rock Projects conducted in USA, England and Germany are found to be in good agreement with the Stressmeter results obtained in Japan. Based on this broad agreement, a solid geomechanical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.3918F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.3918F"><span>Surface <span class="hlt">faulting</span> along the inland Itozawa normal <span class="hlt">fault</span> (eastern Japan) and relation to the 2011 Tohoku-oki megathrust <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferry, Matthieu; Tsutsumi, Hiroyuki; Meghraoui, Mustapha; Toda, Shinji</p> <p>2013-04-01</p> <p>The 11 March 2011 Mw 9 Tohoku-oki <span class="hlt">earthquake</span> ruptured ~500 km length of the Japan Trench along the coast of eastern Japan and significantly impacted the stress regime within the crust. The resulting change in seismicity over the Japan mainland was exhibited by the 11 April 2011 Mw 6.6 Iwaki <span class="hlt">earthquake</span> that ruptured the Itozawa and Yunodake <span class="hlt">faults</span>. Trending NNW and NW, respectively, these 70-80° W-dipping <span class="hlt">faults</span> bound the Iwaki basin of Neogene age and have been reactivated simultaneously both along 15-km-long sections. Here, we present initial results from a paleoseismic excavation performed across the Itozawa <span class="hlt">fault</span> within the Tsunagi Valley at the northern third of the observed surface rupture. At the Tsunagi site, the rupture affects a rice paddy, which provides an ideally horizontal initial state to collect detailed and accurate measurements. The surface break is composed of a continuous 30-to-40-cm-wide purely extensional crack that separates the uplifted block from a gently dipping 1-to-2-m-wide strip affected by right-stepping en-echelon cracks and locally bounded by a ~0.1-m-high reverse scarplet. Total station across-<span class="hlt">fault</span> topographic profiles indicate the pre-<span class="hlt">earthquake</span> ground surface was vertically deformed by ~0.6 m while direct field examinations reveal that well-defined rice paddy limits have been left-laterally offset by ~0.1 m. The 12-m-long, 3.5-m-deep trench exposes the 30-to-40-cm-thick cultivated soil overlaying a 1-m-thick red to yellow silt unit, a 2-m-thick alluvial gravel unit and a basal 0.1-1-m-thick organic-rich silt unit. Deformation associated to the 2011 rupture illustrates down-dip movement along a near-vertical <span class="hlt">fault</span> with a well-expressed bending moment at the surface and generalized warping. On the north wall, the intermediate gravel unit displays a deformation pattern similar to granular flow with only minor discrete <span class="hlt">faulting</span> and no splay to be continuously followed from the main <span class="hlt">fault</span> to the surface. On the south wall, warping</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T13D2645F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T13D2645F"><span>Surface <span class="hlt">faulting</span> along the inland Itozawa normal <span class="hlt">fault</span> (eastern Japan) and relation to the 2011 Tohoku-oki megathrust <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferry, M.; Tsutsumi, H.; Meghraoui, M.; Toda, S.</p> <p>2012-12-01</p> <p>The 11 March 2011 Mw 9 Tohoku-oki <span class="hlt">earthquake</span> ruptured ~500 km length of the Japan Trench along the coast of eastern Japan and significantly impacted the stress regime within the crust. The resulting change in seismicity over the Japan mainland was exhibited by the 11 April 2011 Mw 6.6 Iwaki <span class="hlt">earthquake</span> that ruptured the Itozawa and Yunodake <span class="hlt">faults</span>. Trending NNW and NW, respectively, these 70-80° W-dipping <span class="hlt">faults</span> bound the Iwaki basin of Neogene age and have been reactivated simultaneously both along 15-km-long sections. Here, we present initial results from a paleoseismic excavation performed across the Itozawa <span class="hlt">fault</span> within the Tsunagi Valley at the northern third of the observed surface rupture. At the Tsunagi site, the rupture affects a rice paddy, which provides an ideally horizontal initial state to collect detailed and accurate measurements. The surface break is composed of a continuous 30-to-40-cm-wide purely extensional crack that separates the uplifted block from a gently dipping 1-to-2-m-wide strip affected by right-stepping en-echelon cracks and locally bounded by a ~0.1-m-high reverse scarplet. Total station across-<span class="hlt">fault</span> topographic profiles indicate the pre-<span class="hlt">earthquake</span> ground surface was vertically deformed by ~0.6 m while direct field examinations reveal that well-defined rice paddy limits have been left-laterally offset by ~0.1 m. The 12-m-long, 3.5-m-deep trench exposes the 30-to-40-cm-thick cultivated soil overlaying a 1-m-thick red to yellow silt unit, a 2-m-thick alluvial gravel unit and a basal 0.1-1-m-thick organic-rich silt unit. Deformation associated to the 2011 rupture illustrates down-dip movement along a near-vertical <span class="hlt">fault</span> with a well-expressed bending moment at the surface and generalized warping. On the north wall, the intermediate gravel unit displays a deformation pattern similar to granular flow with only minor discrete <span class="hlt">faulting</span> and no splay to be continuously followed from the main <span class="hlt">fault</span> to the surface. On the south wall, warping</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910006334','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910006334"><span>GPS measurements of deformation associated with the 1987 Superstition Hills <span class="hlt">earthquake</span>: Evidence for conjugate <span class="hlt">faulting</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Larsen, Shawn; Reilinger, Robert; Neugebauer, Helen; Strange, William</p> <p>1991-01-01</p> <p>Large station displacements observed from Imperial Valley Global Positioning <span class="hlt">System</span> (GPS) campaigns are attributed to the November 24, 1987 Superstition Hills <span class="hlt">earthquake</span> sequence. Thirty sites from a 42 station GPS network established in 1986 were reoccupied during 1988 and/or 1990. Displacements at three sites within 3 kilometers of the surface rupture approach 0.5 m. Eight additional stations within 20 km of the seismic zone are displaced at least 10 cm. This is the first occurrence of a large <span class="hlt">earthquake</span> (M(sub S) 6.6) within a preexisting GPS network. Best-fitting uniform slip models of rectangular dislocations in an elastic half-space indicate 130 + or - 8 cm right-lateral displacement along the northwest-trending Superstition Hills <span class="hlt">fault</span> and 30 + or - 10 cm left-lateral displacement along the conjugate northeast-trending Elmore Ranch <span class="hlt">fault</span>. The geodetic moments are 9.4 x 10(exp 25) dyne-cm and 2.3 x 10(exp 25) dyne-cm for the Superstition Hills and Elmore Ranch <span class="hlt">faults</span>, respectively, consistent with teleseismic source parameters. The data also suggest the post seismic slip along the Superstition Hills <span class="hlt">fault</span> is concentrated at shallow depths. Distributed slip solutions using Singular Value Decomposition indicate near uniform displacement along the Elmore Ranch <span class="hlt">fault</span> and concentrated slip to the northwest and southeast along the Superstition Hills <span class="hlt">fault</span>. A significant component of non-seismic displacement is observed across the Imperial Valley, which is attributed in part to interseismic plate-boundary deformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMED51B0528G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMED51B0528G"><span>Development of the Elastic Rebound Strike-slip (ERS) <span class="hlt">Fault</span> Model for Teaching <span class="hlt">Earthquake</span> Science to Non-science Students</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Glesener, G. B.; Peltzer, G.; Stubailo, I.; Cochran, E. S.; Lawrence, J. F.</p> <p>2009-12-01</p> <p>The Modeling and Educational Demonstrations Laboratory (MEDL) at the University of California, Los Angeles has developed a fourth version of the Elastic Rebound Strike-slip (ERS) <span class="hlt">Fault</span> Model to be used to educate students and the general public about the process and mechanics of <span class="hlt">earthquakes</span> from strike-slip <span class="hlt">faults</span>. The ERS <span class="hlt">Fault</span> Model is an interactive hands-on teaching tool which produces failure on a predefined <span class="hlt">fault</span> embedded in an elastic medium, with adjustable normal stress. With the addition of an accelerometer sensor, called the Joy Warrior, the user can experience what it is like for a field geophysicist to collect and observe ground shaking data from an <span class="hlt">earthquake</span> without having to experience a real <span class="hlt">earthquake</span>. Two knobs on the ERS <span class="hlt">Fault</span> Model control the normal and shear stress on the <span class="hlt">fault</span>. Adjusting the normal stress knob will increase or decrease the friction on the <span class="hlt">fault</span>. The shear stress knob displaces one side of the elastic medium parallel to the strike of the <span class="hlt">fault</span>, resulting in changing shear stress on the <span class="hlt">fault</span> surface. When the shear stress exceeds the threshold defined by the static friction of the <span class="hlt">fault</span>, an <span class="hlt">earthquake</span> on the model occurs. The accelerometer sensor then sends the data to a computer where the shaking of the model due to the sudden slip on the <span class="hlt">fault</span> can be displayed and analyzed by the student. The experiment clearly illustrates the relationship between <span class="hlt">earthquakes</span> and seismic waves. One of the major benefits to using the ERS <span class="hlt">Fault</span> Model in undergraduate courses is that it helps to connect non-science students with the work of scientists. When students that are not accustomed to scientific thought are able to experience the scientific process first hand, a connection is made between the scientists and students. Connections like this might inspire a student to become a scientist, or promote the advancement of scientific research through public policy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S33F4930G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S33F4930G"><span>Three-dimensional <span class="hlt">fault</span> framework of the 2014 South Napa <span class="hlt">Earthquake</span>, San Francisco Bay region, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Graymer, R. W.</p> <p>2014-12-01</p> <p>Assignment of the South Napa <span class="hlt">earthquake</span> to a mapped <span class="hlt">fault</span> is difficult, as it occurred where three large, northwest-trending <span class="hlt">faults</span> converge and may interact in the subsurface. The surface rupture did not fall on the main trace of any of these <span class="hlt">faults</span>, but instead between the Carneros and West Napa <span class="hlt">faults</span> and northwest along strike from the northern mapped end of the Franklin <span class="hlt">Fault</span>. The 2014 rupture plane appears to be nearly vertical, based on focal mechanisms of the mainshock and connection of the surface trace/rupture to the relocated hypocenter (J. Hardebeck, USGS). 3D surfaces constructed from published data show that the Carneros <span class="hlt">Fault</span> is a steeply west-dipping <span class="hlt">fault</span> that runs just west of the near-vertical 2014 rupture plane. The Carneros <span class="hlt">Fault</span> does not appear to have been involved in the <span class="hlt">earthquake</span>, although relocated aftershocks suggest possible minor triggered slip. The main West Napa <span class="hlt">Fault</span> is also steeply west-dipping and that its projection intersects the 2014 rupture plane at around the depth of the mainshock hypocenter. UAVSAR data (A. Donnellan, JPL) and relocated aftershocks suggest that the main West Napa <span class="hlt">Fault</span> experienced triggered slip/afterslip along a length of roughly 20 km. It is possible that the 2014 rupture took place along a largely unrecognized westerly strand of the West Napa <span class="hlt">Fault</span>. The Franklin <span class="hlt">Fault</span> is a steeply east-dipping <span class="hlt">fault</span> (with a steeply west-dipping subordinate trace east of Mare Island) that has documented late Quaternary offset. Given the generally aligned orientation of the 3D <span class="hlt">fault</span> surfaces, an alternative interpretation is that the South Napa <span class="hlt">earthquake</span> occurred on the northernmost reach of the Franklin <span class="hlt">Fault</span> within it's 3D junction with the West Napa <span class="hlt">Fault</span>. This interpretation is supported, but not proven, by a short but prominent linear feature in the UAVSAR data at Slaughterhouse Point west of Vallejo, along trend south-southeast of the observed coseismic surface rupture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoJI.198.1159H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoJI.198.1159H"><span>A smoothed stochastic <span class="hlt">earthquake</span> rate model considering seismicity and <span class="hlt">fault</span> moment release for Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hiemer, S.; Woessner, J.; Basili, R.; Danciu, L.; Giardini, D.; Wiemer, S.</p> <p>2014-08-01</p> <p>We present a time-independent gridded <span class="hlt">earthquake</span> rate forecast for the European region including Turkey. The spatial component of our model is based on kernel density estimation techniques, which we applied to both past <span class="hlt">earthquake</span> locations and <span class="hlt">fault</span> moment release on mapped crustal <span class="hlt">faults</span> and subduction zone interfaces with assigned slip rates. Our forecast relies on the assumption that the locations of past seismicity is a good guide to future seismicity, and that future large-magnitude events occur more likely in the vicinity of known <span class="hlt">faults</span>. We show that the optimal weighted sum of the corresponding two spatial densities depends on the magnitude range considered. The kernel bandwidths and density weighting function are optimized using retrospective likelihood-based forecast experiments. We computed <span class="hlt">earthquake</span> activity rates (a- and b-value) of the truncated Gutenberg-Richter distribution separately for crustal and subduction seismicity based on a maximum likelihood approach that considers the spatial and temporal completeness history of the catalogue. The final annual rate of our forecast is purely driven by the maximum likelihood fit of activity rates to the catalogue data, whereas its spatial component incorporates contributions from both <span class="hlt">earthquake</span> and <span class="hlt">fault</span> moment-rate densities. Our model constitutes one branch of the <span class="hlt">earthquake</span> source model logic tree of the 2013 European seismic hazard model released by the EU-FP7 project `Seismic HAzard haRmonization in Europe' (SHARE) and contributes to the assessment of epistemic uncertainties in <span class="hlt">earthquake</span> activity rates. We performed retrospective and pseudo-prospective likelihood consistency tests to underline the reliability of our model and SHARE's area source model (ASM) using the testing algorithms applied in the collaboratory for the study of <span class="hlt">earthquake</span> predictability (CSEP). We comparatively tested our model's forecasting skill against the ASM and find a statistically significant better performance for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5359594','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5359594"><span>Orogen-scale uplift in the central Italian Apennines drives episodic behaviour of <span class="hlt">earthquake</span> <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Cowie, P. A.; Phillips, R. J.; Roberts, G. P.; McCaffrey, K.; Zijerveld, L. J. J.; Gregory, L. C.; Faure Walker, J.; Wedmore, L. N. J.; Dunai, T. J.; Binnie, S. A.; Freeman, S. P. H. T.; Wilcken, K.; Shanks, R. P.; Huismans, R. S.; Papanikolaou, I.; Michetti, A. M.; Wilkinson, M.</p> <p>2017-01-01</p> <p>Many areas of the Earth’s crust deform by distributed extensional <span class="hlt">faulting</span> and complex <span class="hlt">fault</span> interactions are often observed. Geodetic data generally indicate a simpler picture of continuum deformation over decades but relating this behaviour to <span class="hlt">earthquake</span> occurrence over centuries, given numerous potentially active <span class="hlt">faults</span>, remains a global problem in hazard assessment. We address this challenge for an array of seismogenic <span class="hlt">faults</span> in the central Italian Apennines, where crustal extension and devastating <span class="hlt">earthquakes</span> occur in response to regional surface uplift. We constrain <span class="hlt">fault</span> slip-rates since ~18 ka using variations in cosmogenic 36Cl measured on bedrock scarps, mapped using LiDAR and ground penetrating radar, and compare these rates to those inferred from geodesy. The 36Cl data reveal that individual <span class="hlt">faults</span> typically accumulate meters of displacement relatively rapidly over several thousand years, separated by similar length time intervals when slip-rates are much lower, and activity shifts between <span class="hlt">faults</span> across strike. Our rates agree with continuum deformation rates when averaged over long spatial or temporal scales (104 yr; 102 km) but over shorter timescales most of the deformation may be accommodated by <30% of the across-strike <span class="hlt">fault</span> array. We attribute the shifts in activity to temporal variations in the mechanical work of <span class="hlt">faulting</span>. PMID:28322311</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28322311','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28322311"><span>Orogen-scale uplift in the central Italian Apennines drives episodic behaviour of <span class="hlt">earthquake</span> <span class="hlt">faults</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cowie, P A; Phillips, R J; Roberts, G P; McCaffrey, K; Zijerveld, L J J; Gregory, L C; Faure Walker, J; Wedmore, L N J; Dunai, T J; Binnie, S A; Freeman, S P H T; Wilcken, K; Shanks, R P; Huismans, R S; Papanikolaou, I; Michetti, A M; Wilkinson, M</p> <p>2017-03-21</p> <p>Many areas of the Earth's crust deform by distributed extensional <span class="hlt">faulting</span> and complex <span class="hlt">fault</span> interactions are often observed. Geodetic data generally indicate a simpler picture of continuum deformation over decades but relating this behaviour to <span class="hlt">earthquake</span> occurrence over centuries, given numerous potentially active <span class="hlt">faults</span>, remains a global problem in hazard assessment. We address this challenge for an array of seismogenic <span class="hlt">faults</span> in the central Italian Apennines, where crustal extension and devastating <span class="hlt">earthquakes</span> occur in response to regional surface uplift. We constrain <span class="hlt">fault</span> slip-rates since ~18 ka using variations in cosmogenic 36 Cl measured on bedrock scarps, mapped using LiDAR and ground penetrating radar, and compare these rates to those inferred from geodesy. The 36 Cl data reveal that individual <span class="hlt">faults</span> typically accumulate meters of displacement relatively rapidly over several thousand years, separated by similar length time intervals when slip-rates are much lower, and activity shifts between <span class="hlt">faults</span> across strike. Our rates agree with continuum deformation rates when averaged over long spatial or temporal scales (10 4  yr; 10 2  km) but over shorter timescales most of the deformation may be accommodated by <30% of the across-strike <span class="hlt">fault</span> array. We attribute the shifts in activity to temporal variations in the mechanical work of <span class="hlt">faulting</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S53D..07F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S53D..07F"><span>Toward a physics-based rate and state friction law for <span class="hlt">earthquake</span> nucleation processes in <span class="hlt">fault</span> zones with granular gouge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferdowsi, B.; Rubin, A. M.</p> <p>2017-12-01</p> <p>Numerical simulations of <span class="hlt">earthquake</span> nucleation rely on constitutive rate and state evolution laws to model <span class="hlt">earthquake</span> initiation and propagation processes. The response of different state evolution laws to large velocity increases is an important feature of these constitutive relations that can significantly change the style of <span class="hlt">earthquake</span> nucleation in numerical models. However, currently there is not a rigorous understanding of the physical origins of the response of bare rock or gouge-filled <span class="hlt">fault</span> zones to large velocity increases. This in turn hinders our ability to design physics-based friction laws that can appropriately describe those responses. We here argue that most <span class="hlt">fault</span> zones form a granular gouge after an initial shearing phase and that it is the behavior of the gouge layer that controls the <span class="hlt">fault</span> friction. We perform numerical experiments of a confined sheared granular gouge under a range of confining stresses and driving velocities relevant to <span class="hlt">fault</span> zones and apply 1-3 order of magnitude velocity steps to explore dynamical behavior of the <span class="hlt">system</span> from grain- to macro-scales. We compare our numerical observations with experimental data from biaxial double-direct-shear <span class="hlt">fault</span> gouge experiments under equivalent loading and driving conditions. Our intention is to first investigate the degree to which these numerical experiments, with Hertzian normal and Coulomb friction laws at the grain-grain contact scale and without any time-dependent plasticity, can reproduce experimental <span class="hlt">fault</span> gouge behavior. We next compare the behavior observed in numerical experiments with predictions of the Dieterich (Aging) and Ruina (Slip) friction laws. Finally, the numerical observations at the grain and meso-scales will be used for designing a rate and state evolution law that takes into account recent advances in rheology of granular <span class="hlt">systems</span>, including local and non-local effects, for a wide range of shear rates and slow and fast deformation regimes of the <span class="hlt">fault</span> gouge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.G13A0999A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.G13A0999A"><span>Slip distribution, strain accumulation and aseismic slip on the Chaman <span class="hlt">Fault</span> <span class="hlt">system</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Amelug, F.</p> <p>2015-12-01</p> <p>The Chaman <span class="hlt">fault</span> <span class="hlt">system</span> is a transcurrent <span class="hlt">fault</span> <span class="hlt">system</span> developed due to the oblique convergence of the India and Eurasia plates in the western boundary of the India plate. To evaluate the contemporary rates of strain accumulation along and across the Chaman <span class="hlt">Fault</span> <span class="hlt">system</span>, we use 2003-2011 Envisat SAR imagery and InSAR time-series methods to obtain a ground velocity field in radar line-of-sight (LOS) direction. We correct the InSAR data for different sources of systematic biases including the phase unwrapping errors, local oscillator drift, topographic residuals and stratified tropospheric delay and evaluate the uncertainty due to the residual delay using time-series of MODIS observations of precipitable water vapor. The InSAR velocity field and modeling demonstrates the distribution of deformation across the Chaman <span class="hlt">fault</span> <span class="hlt">system</span>. In the central Chaman <span class="hlt">fault</span> <span class="hlt">system</span>, the InSAR velocity shows clear strain localization on the Chaman and Ghazaband <span class="hlt">faults</span> and modeling suggests a total slip rate of ~24 mm/yr distributed on the two <span class="hlt">faults</span> with rates of 8 and 16 mm/yr, respectively corresponding to the 80% of the total ~3 cm/yr plate motion between India and Eurasia at these latitudes and consistent with the kinematic models which have predicted a slip rate of ~17-24 mm/yr for the Chaman <span class="hlt">Fault</span>. In the northern Chaman <span class="hlt">fault</span> <span class="hlt">system</span> (north of 30.5N), ~6 mm/yr of the relative plate motion is accommodated across Chaman <span class="hlt">fault</span>. North of 30.5 N where the topographic expression of the Ghazaband <span class="hlt">fault</span> vanishes, its slip does not transfer to the Chaman <span class="hlt">fault</span> but rather distributes among different <span class="hlt">faults</span> in the Kirthar range and Sulaiman lobe. Observed surface creep on the southern Chaman <span class="hlt">fault</span> between Nushki and north of City of Chaman, indicates that the <span class="hlt">fault</span> is partially locked, consistent with the recorded M<7 <span class="hlt">earthquakes</span> in last century on this segment. The Chaman <span class="hlt">fault</span> between north of the City of Chaman to North of Kabul, does not show an increase in the rate of strain</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27441248','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27441248"><span>Automatic generation of smart <span class="hlt">earthquake</span>-resistant building <span class="hlt">system</span>: Hybrid <span class="hlt">system</span> of base-isolation and building-connection.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kasagi, M; Fujita, K; Tsuji, M; Takewaki, I</p> <p>2016-02-01</p> <p>A base-isolated building may sometimes exhibit an undesirable large response to a long-duration, long-period <span class="hlt">earthquake</span> ground motion and a connected building <span class="hlt">system</span> without base-isolation may show a large response to a near-<span class="hlt">fault</span> (rather high-frequency) <span class="hlt">earthquake</span> ground motion. To overcome both deficiencies, a new hybrid control <span class="hlt">system</span> of base-isolation and building-connection is proposed and investigated. In this new hybrid building <span class="hlt">system</span>, a base-isolated building is connected to a stiffer free wall with oil dampers. It has been demonstrated in a preliminary research that the proposed hybrid <span class="hlt">system</span> is effective both for near-<span class="hlt">fault</span> (rather high-frequency) and long-duration, long-period <span class="hlt">earthquake</span> ground motions and has sufficient redundancy and robustness for a broad range of <span class="hlt">earthquake</span> ground motions.An automatic generation algorithm of this kind of smart structures of base-isolation and building-connection hybrid <span class="hlt">systems</span> is presented in this paper. It is shown that, while the proposed algorithm does not work well in a building without the connecting-damper <span class="hlt">system</span>, it works well in the proposed smart hybrid <span class="hlt">system</span> with the connecting damper <span class="hlt">system</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70188386','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70188386"><span>Kinematics of shallow backthrusts in the Seattle <span class="hlt">fault</span> zone, Washington State</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pratt, Thomas L.; Troost, K.G.; Odum, Jackson K.; Stephenson, William J.</p> <p>2015-01-01</p> <p>Near-surface thrust <span class="hlt">fault</span> splays and antithetic backthrusts at the tips of major thrust <span class="hlt">fault</span> <span class="hlt">systems</span> can distribute slip across multiple shallow <span class="hlt">fault</span> strands, complicating <span class="hlt">earthquake</span> hazard analyses based on studies of surface <span class="hlt">faulting</span>. The shallow expression of the <span class="hlt">fault</span> strands forming the Seattle <span class="hlt">fault</span> zone of Washington State shows the structural relationships and interactions between such <span class="hlt">fault</span> strands. Paleoseismic studies document an ∼7000 yr history of <span class="hlt">earthquakes</span> on multiple <span class="hlt">faults</span> within the Seattle <span class="hlt">fault</span> zone, with some backthrusts inferred to rupture in small (M ∼5.5–6.0) <span class="hlt">earthquakes</span> at times other than during <span class="hlt">earthquakes</span> on the main thrust <span class="hlt">faults</span>. We interpret seismic-reflection profiles to show three main thrust <span class="hlt">faults</span>, one of which is a blind thrust <span class="hlt">fault</span> directly beneath downtown Seattle, and four small backthrusts within the Seattle <span class="hlt">fault</span> zone. We then model <span class="hlt">fault</span> slip, constrained by shallow deformation, to show that the Seattle <span class="hlt">fault</span> forms a <span class="hlt">fault</span> propagation fold rather than the alternatively proposed roof thrust <span class="hlt">system</span>. <span class="hlt">Fault</span> slip modeling shows that back-thrust ruptures driven by moderate (M ∼6.5–6.7) <span class="hlt">earthquakes</span> on the main thrust <span class="hlt">faults</span> are consistent with the paleoseismic data. The results indicate that paleoseismic data from the back-thrust ruptures reveal the times of moderate <span class="hlt">earthquakes</span> on the main <span class="hlt">fault</span> <span class="hlt">system</span>, rather than indicating smaller (M ∼5.5–6.0) <span class="hlt">earthquakes</span> involving only the backthrusts. Estimates of cumulative shortening during known Seattle <span class="hlt">fault</span> zone <span class="hlt">earthquakes</span> support the inference that the Seattle <span class="hlt">fault</span> has been the major seismic hazard in the northern Cascadia forearc in the late Holocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2018/1093/ofr20181093.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2018/1093/ofr20181093.pdf"><span>Reexamination of the subsurface <span class="hlt">fault</span> structure in the vicinity of the 1989 moment-magnitude-6.9 Loma Prieta <span class="hlt">earthquake</span>, central California, using steep-reflection, <span class="hlt">earthquake</span>, and magnetic data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zhang, Edward; Fuis, Gary S.; Catchings, Rufus D.; Scheirer, Daniel S.; Goldman, Mark; Bauer, Klaus</p> <p>2018-06-13</p> <p>We reexamine the geometry of the causative <span class="hlt">fault</span> structure of the 1989 moment-magnitude-6.9 Loma Prieta <span class="hlt">earthquake</span> in central California, using seismic-reflection, <span class="hlt">earthquake</span>-hypocenter, and magnetic data. Our study is prompted by recent interpretations of a two-part dip of the San Andreas <span class="hlt">Fault</span> (SAF) accompanied by a flower-like structure in the Coachella Valley, in southern California. Initially, the prevailing interpretation of <span class="hlt">fault</span> geometry in the vicinity of the Loma Prieta <span class="hlt">earthquake</span> was that the mainshock did not rupture the SAF, but rather a secondary <span class="hlt">fault</span> within the SAF <span class="hlt">system</span>, because network locations of aftershocks defined neither a vertical plane nor a <span class="hlt">fault</span> plane that projected to the surface trace of the SAF. Subsequent waveform cross-correlation and double-difference relocations of Loma Prieta aftershocks appear to have clarified the <span class="hlt">fault</span> geometry somewhat, with steeply dipping <span class="hlt">faults</span> in the upper crust possibly connecting to the more moderately southwest-dipping mainshock rupture in the middle crust. Examination of steep-reflection data, extracted from a 1991 seismic-refraction profile through the Loma Prieta area, reveals three robust <span class="hlt">fault</span>-like features that agree approximately in geometry with the clusters of upper-crustal relocated aftershocks. The subsurface geometry of the San Andreas, Sargent, and Berrocal <span class="hlt">Faults</span> can be mapped using these features and the aftershock clusters. The San Andreas and Sargent <span class="hlt">Faults</span> appear to dip northeastward in the uppermost crust and change dip continuously toward the southwest with depth. Previous models of gravity and magnetic data on profiles through the aftershock region also define a steeply dipping SAF, with an initial northeastward dip in the uppermost crust that changes with depth. At a depth 6 to 9 km, upper-crustal <span class="hlt">faults</span> appear to project into the moderately southwest-dipping, planar mainshock rupture. The change to a planar dipping rupture at 6–9 km is similar to <span class="hlt">fault</span> geometry seen in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70141606','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70141606"><span>Aftershocks illuminate the 2011 Mineral, Virginia, <span class="hlt">earthquake</span> causative <span class="hlt">fault</span> zone and nearby active <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Horton, J. Wright; Shah, Anjana K.; McNamara, Daniel E.; Snyder, Stephen L.; Carter, Aina M</p> <p>2015-01-01</p> <p>Deployment of temporary seismic stations after the 2011 Mineral, Virginia (USA), <span class="hlt">earthquake</span> produced a well-recorded aftershock sequence. The majority of aftershocks are in a tabular cluster that delineates the previously unknown Quail <span class="hlt">fault</span> zone. Quail <span class="hlt">fault</span> zone aftershocks range from ~3 to 8 km in depth and are in a 1-km-thick zone striking ~036° and dipping ~50°SE, consistent with a 028°, 50°SE main-shock nodal plane having mostly reverse slip. This cluster extends ~10 km along strike. The Quail <span class="hlt">fault</span> zone projects to the surface in gneiss of the Ordovician Chopawamsic Formation just southeast of the Ordovician–Silurian Ellisville Granodiorite pluton tail. The following three clusters of shallow (<3 km) aftershocks illuminate other <span class="hlt">faults</span>. (1) An elongate cluster of early aftershocks, ~10 km east of the Quail <span class="hlt">fault</span> zone, extends 8 km from Fredericks Hall, strikes ~035°–039°, and appears to be roughly vertical. The Fredericks Hall <span class="hlt">fault</span> may be a strand or splay of the older Lakeside <span class="hlt">fault</span> zone, which to the south spans a width of several kilometers. (2) A cluster of later aftershocks ~3 km northeast of Cuckoo delineates a <span class="hlt">fault</span> near the eastern contact of the Ordovician Quantico Formation. (3) An elongate cluster of late aftershocks ~1 km northwest of the Quail <span class="hlt">fault</span> zone aftershock cluster delineates the northwest <span class="hlt">fault</span> (described herein), which is temporally distinct, dips more steeply, and has a more northeastward strike. Some aftershock-illuminated <span class="hlt">faults</span> coincide with preexisting units or structures evident from radiometric anomalies, suggesting tectonic inheritance or reactivation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70191101','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191101"><span>Continuity of the West Napa–Franklin <span class="hlt">fault</span> zone inferred from guided waves generated by <span class="hlt">earthquakes</span> following the 24 August 2014 Mw 6.0 South Napa <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Catchings, Rufus D.; Goldman, Mark R.; Li, Yong-Gang; Chan, Joanne</p> <p>2016-01-01</p> <p>We measure peak ground velocities from fault‐zone guided waves (FZGWs), generated by on‐<span class="hlt">fault</span> <span class="hlt">earthquakes</span> associated with the 24 August 2014 Mw 6.0 South Napa <span class="hlt">earthquake</span>. The data were recorded on three arrays deployed across north and south of the 2014 surface rupture. The observed FZGWs indicate that the West Napa <span class="hlt">fault</span> zone (WNFZ) and the Franklin <span class="hlt">fault</span> (FF) are continuous in the subsurface for at least 75 km. Previously published potential‐field data indicate that the WNFZ extends northward to the Maacama <span class="hlt">fault</span> (MF), and previous geologic mapping indicates that the FF extends southward to the Calaveras <span class="hlt">fault</span> (CF); this suggests a total length of at least 110 km for the WNFZ–FF. Because the WNFZ–FF appears contiguous with the MF and CF, these <span class="hlt">faults</span> apparently form a continuous Calaveras–Franklin–WNFZ–Maacama (CFWM) <span class="hlt">fault</span> that is second only in length (∼300  km) to the San Andreas <span class="hlt">fault</span> in the San Francisco Bay area. The long distances over which we observe FZGWs, coupled with their high amplitudes (2–10 times the S waves) suggest that strong shaking from large <span class="hlt">earthquakes</span> on any part of the CFWM <span class="hlt">fault</span> may cause far‐field amplified fault‐zone shaking. We interpret guided waves and seismicity cross sections to indicate multiple upper crustal splays of the WNFZ–FF, including a northward extension of the Southhampton <span class="hlt">fault</span>, which may cause strong shaking in the Napa Valley and the Vallejo area. Based on travel times from each <span class="hlt">earthquake</span> to each recording array, we estimate average P‐, S‐, and guided‐wave velocities within the WNFZ–FF (4.8–5.7, 2.2–3.2, and 1.1–2.8  km/s, respectively), with FZGW velocities ranging from 58% to 93% of the average S‐wave velocities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..915S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..915S"><span><span class="hlt">Fault</span>- and Area-Based PSHA in Nepal using OpenQuake: New Insights from the 2015 M7.8 Gorkha-Nepal <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stevens, Victoria</p> <p>2017-04-01</p> <p>The 2015 Gorkha-Nepal M7.8 <span class="hlt">earthquake</span> (hereafter known simply as the Gorkha <span class="hlt">earthquake</span>) highlights the seismic risk in Nepal, allows better characterization of the geometry of the Main Himalayan Thrust (MHT), and enables comparison of recorded ground-motions with predicted ground-motions. These new data, together with recent paleoseismic studies and geodetic-based coupling models, allow for good parameterization of the <span class="hlt">fault</span> characteristics. Other <span class="hlt">faults</span> in Nepal remain less well studied. Unlike previous PSHA studies in Nepal that are exclusively area-based, we use a mix of <span class="hlt">faults</span> and areas to describe six seismic sources in Nepal. For each source, the Gutenberg-Richter a and b values are found, and the maximum magnitude <span class="hlt">earthquake</span> estimated, using a combination of <span class="hlt">earthquake</span> catalogs, moment conservation principals and similarities to other tectonic regions. The MHT and Karakoram <span class="hlt">fault</span> are described as <span class="hlt">fault</span> sources, whereas four other sources - normal <span class="hlt">faulting</span> in N-S trending grabens of northern Nepal, strike-slip <span class="hlt">faulting</span> in both eastern and western Nepal, and background seismicity - are described as area sources. We use OpenQuake (http://openquake.org/) to carry out the analysis, and peak ground acceleration (PGA) at 2 and 10% chance in 50 years is found for Nepal, along with hazard curves at various locations. We compare this PSHA model with previous area-based models of Nepal. The Main Himalayan Thrust is the principal seismic hazard in Nepal so we study the effects of changing several parameters associated with this <span class="hlt">fault</span>. We compare ground shaking predicted from various <span class="hlt">fault</span> geometries suggested from the Gorkha <span class="hlt">earthquake</span> with each other, and with a simple model of a flat <span class="hlt">fault</span>. We also show the results from incorporating a coupling model based on geodetic data and microseismicity, which limits the down-dip extent of rupture. There have been no ground-motion prediction equations (GMPEs) developed specifically for Nepal, so we compare the results of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020700','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020700"><span>Evidence of shallow <span class="hlt">fault</span> zone strengthening after the 1992 M7.5 Landers, California, <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Li, Y.-G.; Vidale, J.E.; Aki, K.; Xu, Fei; Burdette, T.</p> <p>1998-01-01</p> <p>Repeated seismic surveys of the Landers, California, <span class="hlt">fault</span> zone that ruptured in the magnitude (M) 7.5 <span class="hlt">earthquake</span> of 1992 reveal an increase in seismic velocity with time. P, S, and <span class="hlt">fault</span> zone trapped waves were excited by near-surface explosions in two locations in 1994 and 1996, and were recorded on two linear, three-component seismic arrays deployed across the Johnson Valley <span class="hlt">fault</span> trace. The travel times of P and S waves for identical shot-receiver pairs decreased by 0.5 to 1.5 percent from 1994 to 1996, with the larger changes at stations located within the <span class="hlt">fault</span> zone. These observations indicate that the shallow Johnson Valley <span class="hlt">fault</span> is strengthening after the main shock, most likely because of closure of cracks that were opened by the 1992 <span class="hlt">earthquake</span>. The increase in velocity is consistent with the prevalence of dry over wet cracks and with a reduction in the apparent crack density near the <span class="hlt">fault</span> zone by approximately 1.0 percent from 1994 to 1996.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.S23D..08N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.S23D..08N"><span><span class="hlt">Earthquake</span> doublet that occurred in a pull-apart basin along the Sumatran <span class="hlt">fault</span> and its seismotectonic implication</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nakano, M.; Kumagai, H.; Yamashina, T.; Inoue, H.; Toda, S.</p> <p>2007-12-01</p> <p>On March 6, 2007, an <span class="hlt">earthquake</span> doublet occurred around Lake Singkarak, central Sumatra in Indonesia. An <span class="hlt">earthquake</span> with magnitude (Mw) 6.4 at 03:49 is followed two hours later (05:49) by a similar-size event (Mw 6.3). Lake Singkarak is located between the Sianok and Sumani <span class="hlt">fault</span> segments of the Sumatran <span class="hlt">fault</span> <span class="hlt">system</span>, and is a pull-apart basin formed at the segment boundary. We investigate source processes of the <span class="hlt">earthquakes</span> using waveform data obtained from JISNET, which is a broad-band seismograph network in Indonesia. We first estimate the centroid source locations and focal mechanisms by the waveform inversion carried out in the frequency domain. Since stations are distributed almost linearly in the NW-SE direction coincident with the Sumatran <span class="hlt">fault</span> strike direction, the estimated centroid locations are not well resolved especially in the direction orthogonal to the NW-SE direction. If we assume that these <span class="hlt">earthquakes</span> occurred along the Sumatran <span class="hlt">fault</span>, the first <span class="hlt">earthquake</span> is located on the Sumani segment below Lake Singkarak and the second event is located at a few tens of kilometers north of the first event on the Sianok segment. The focal mechanisms of both events point to almost identical right-lateral strike-slip vertical <span class="hlt">faulting</span>, which is consistent with the geometry of the Sumatran <span class="hlt">fault</span> <span class="hlt">system</span>. We next investigate the rupture initiation points using the particle motions of the P-waves of these <span class="hlt">earthquakes</span> observed at station PPI, which is located about 20 km north of the Lake Singkarak. The initiation point of the first event is estimated in the north of the lake, which corresponds to the northern end of the Sumani segment. The initiation point of the second event is estimated at the southern end of the Sianok segment. The observed maximum amplitudes at stations located in the SE of the source region show larger amplitudes for the first event than those for the second one. On the other hand, the amplitudes at station BSI located in the NW of the source</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.S53C..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.S53C..03C"><span>A Geophysical Study of the Cadell <span class="hlt">Fault</span> Scarp for <span class="hlt">Earthquake</span> Hazard Assessment in Southeast Australia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Collins, C. D.</p> <p>2004-12-01</p> <p>The historical record of seismicity in Australia is too short (less than 150 years) to confidently define seismic source zones, particularly the recurrence rates for large, potentially damaging <span class="hlt">earthquakes</span>, and this leads to uncertainty in hazard assessments. One way to extend this record is to search for evidence of <span class="hlt">earthquakes</span> in the landscape, including Quaternary <span class="hlt">fault</span> scarps, tilt blocks and disruptions to drainage patterns. A recent Geoscience Australia compilation of evidence of Quaternary tectonics identified over one hundred examples of potentially recent structures in Australia, testifying to the fact that a greater hazard may exist from large <span class="hlt">earthquakes</span> than is evident from the recorded history alone. Most of these structures have not been studied in detail and have not been dated, so the recurrence rate for damaging events is unknown. One example of recent tectonic activity lies on the Victoria-New South Wales border, where geologically recent uplift has resulted in the formation of the Cadell <span class="hlt">Fault</span> Scarp, damming Australia's largest river, the Murray River, and diverting its course. The scarp extends along a north-south strike for at least 50 km and reaches a maximum height of about 13 metres. The scarp displaces sands and clays of the Murray Basin sediments which overlie Palaeozoic bedrock at a depth of 100 to 250 m. There is evidence that the river <span class="hlt">system</span> has eroded the scarp and displaced the topographic expression away from the location where the <span class="hlt">fault</span>, or <span class="hlt">faults</span>, meets the surface. Thus, to locate potential sites for trenching which intersect the <span class="hlt">faults</span>, Geoscience Australia acquired ground-penetrating radar, resistivity and multi-channel high-resolution seismic reflection and refraction data along traverses across the scarp. The seismic data were acquired using an IVI T15000 MiniVib vibrator operating in p-wave mode, and a 24-channel Stratavisor acquisition <span class="hlt">system</span>. Four 10-second sweeps, with a frequency range of 10-240 Hz, were carried out</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GGG....16.1577M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GGG....16.1577M"><span>Quantifying near-field and off-<span class="hlt">fault</span> deformation patterns of the 1992 Mw 7.3 Landers <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Milliner, Christopher W. D.; Dolan, James F.; Hollingsworth, James; Leprince, Sebastien; Ayoub, Francois; Sammis, Charles G.</p> <p>2015-05-01</p> <p>Coseismic surface deformation in large <span class="hlt">earthquakes</span> is typically measured using field mapping and with a range of geodetic methods (e.g., InSAR, lidar differencing, and GPS). Current methods, however, either fail to capture patterns of near-field coseismic surface deformation or lack preevent data. Consequently, the characteristics of off-<span class="hlt">fault</span> deformation and the parameters that control it remain poorly understood. We develop a standardized method to fully measure the surface, near-field, coseismic deformation patterns at high resolution using the COSI-Corr program by correlating pairs of aerial photographs taken before and after the 1992 Mw 7.3 Landers <span class="hlt">earthquake</span>. COSI-Corr offers the advantage of measuring displacement across the entire zone of surface deformation and over a wider aperture than that available to field geologists. For the Landers <span class="hlt">earthquake</span>, our measured displacements are systematically larger than the field measurements, indicating the presence of off-<span class="hlt">fault</span> deformation. We show that 46% of the total surface displacement occurred as off-<span class="hlt">fault</span> deformation, over a mean deformation width of 154 m. The magnitude and width of off-<span class="hlt">fault</span> deformation along the rupture is primarily controlled by the macroscopic structural complexity of the <span class="hlt">fault</span> <span class="hlt">system</span>, with a weak correlation with the type of near-surface materials through which the rupture propagated. Both the magnitude and width of distributed deformation are largest in stepovers, bends, and at the southern termination of the surface rupture. We find that slip along the surface rupture exhibits a consistent degree of variability at all observable length scales and that the slip distribution is self-affine fractal with dimension of 1.56.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.3026S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.3026S"><span>Normal <span class="hlt">Faulting</span> in the 1923 Berdún <span class="hlt">Earthquake</span> and Postorogenic Extension in the Pyrenees</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stich, Daniel; Martín, Rosa; Batlló, Josep; Macià, Ramón; Mancilla, Flor de Lis; Morales, Jose</p> <p>2018-04-01</p> <p>The 10 July 1923 <span class="hlt">earthquake</span> near Berdún (Spain) is the largest instrumentally recorded event in the Pyrenees. We recover old analog seismograms and use 20 hand-digitized waveforms for regional moment tensor inversion. We estimate moment magnitude Mw 5.4, centroid depth of 8 km, and a pure normal <span class="hlt">faulting</span> source with strike parallel to the mountain chain (N292°E), dip of 66° and rake of -88°. The new mechanism fits into the general predominance of normal <span class="hlt">faulting</span> in the Pyrenees and extension inferred from Global Positioning <span class="hlt">System</span> data. The unique location of the 1923 <span class="hlt">earthquake</span>, near the south Pyrenean thrust front, shows that the extensional regime is not confined to the axial zone where high topography and the crustal root are located. Together with seismicity near the northern mountain front, this indicates that gravitational potential energy in the western Pyrenees is not extracted locally but induces a wide distribution of postorogenic deformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T42D..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T42D..04C"><span>Near-shore Evaluation of Holocene <span class="hlt">Faulting</span> and <span class="hlt">Earthquake</span> Hazard in the New York City Metropolitan Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cormier, M. H.; King, J. W.; Seeber, L.; Heil, C. W., Jr.; Caccioppoli, B.</p> <p>2016-12-01</p> <p>During its relatively short historic period, the Atlantic Seaboard of North America has experienced a few M6+ <span class="hlt">earthquakes</span>. These events raise the specter of a similar <span class="hlt">earthquake</span> occurring anywhere along the eastern seaboard, including in the greater New York City (NYC) metropolitan area. Indeed, the NYC Seismic Zone is one of several concentrations of <span class="hlt">earthquake</span> activity that stand out in the field of epicenters over eastern North America. Various lines of evidence point to a maximum magnitude in the M7 range for metropolitan NYC - a dramatic scenario that is counterbalanced by the low probability of such an event. Several <span class="hlt">faults</span> mapped near NYC strike NW, sub-normal to the NE-striking structural trends of the Appalachians, and all <span class="hlt">earthquake</span> sequences with well-established <span class="hlt">fault</span> sources in the NYC seismic zone originate from NW-striking <span class="hlt">faults</span>. With funding from the USGS <span class="hlt">Earthquake</span> Hazard Program, we recently (July 2016) collected 85 km of high-resolution sub-bottom (CHIRP) profiles along the north shore of western Long Island Sound, immediately adjacent to metropolitan NYC. This survey area is characterized by a smooth, 15.5 kyr-old erosional surface and overlying strata with small original relief. CHIRP sonar profiles of these reflectors are expected to resolve <span class="hlt">fault</span> or fold-related vertical relief (if present) greater than 50 cm. They would also resolve horizontal <span class="hlt">fault</span> displacements with similar resolution, as may be expressed by offsets of either sedimentary or geomorphic features. No sedimentary cover on the land portion of the metro area offers such ideal reference surfaces, which are continuous in both time and space. Seismic profiles have a spacing of 200 m and have been acquired mostly perpendicular to the NW-striking <span class="hlt">faults</span> mapped on land. These new data will be analyzed systematically for all resolvable features and then interpreted, distinguishing sedimentary, geomorphic, and tectonic features. The absence of evidence of post-glacial tectonic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH23A0213N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH23A0213N"><span>Continuous Fine-<span class="hlt">Fault</span> Estimation with Real-Time GNSS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norford, B. B.; Melbourne, T. I.; Szeliga, W. M.; Santillan, V. M.; Scrivner, C.; Senko, J.; Larsen, D.</p> <p>2017-12-01</p> <p>Thousands of real-time telemetered GNSS stations operate throughout the circum-Pacific that may be used for rapid <span class="hlt">earthquake</span> characterization and estimation of local tsunami excitation. We report on the development of a GNSS-based finite-<span class="hlt">fault</span> inversion <span class="hlt">system</span> that continuously estimates slip using real-time GNSS position streams from the Cascadia subduction zone and which is being expanded throughout the circum-Pacific. The <span class="hlt">system</span> uses 1 Hz precise point position streams computed in the ITRF14 reference frame using clock and satellite orbit corrections from the IGS. The software is implemented as seven independent modules that filter time series using Kalman filters, trigger and estimate coseismic offsets, invert for slip using a non-negative least squares method developed by Lawson and Hanson (1974) and elastic half-space Green's Functions developed by Okada (1985), smooth the results temporally and spatially, and write the resulting streams of time-dependent slip to a RabbitMQ messaging server for use by downstream modules such as tsunami excitation modules. Additional <span class="hlt">fault</span> models can be easily added to the <span class="hlt">system</span> for other circum-Pacific subduction zones as additional real-time GNSS data become available. The <span class="hlt">system</span> is currently being tested using data from well-recorded <span class="hlt">earthquakes</span> including the 2011 Tohoku <span class="hlt">earthquake</span>, the 2010 Maule <span class="hlt">earthquake</span>, the 2015 Illapel <span class="hlt">earthquake</span>, the 2003 Tokachi-oki <span class="hlt">earthquake</span>, the 2014 Iquique <span class="hlt">earthquake</span>, the 2010 Mentawai <span class="hlt">earthquake</span>, the 2016 Kaikoura <span class="hlt">earthquake</span>, the 2016 Ecuador <span class="hlt">earthquake</span>, the 2015 Gorkha <span class="hlt">earthquake</span>, and others. Test data will be fed to the <span class="hlt">system</span> and the resultant <span class="hlt">earthquake</span> characterizations will be compared with published <span class="hlt">earthquake</span> parameters. Seismic events will be assumed to occur on major <span class="hlt">faults</span>, so, for example, only the San Andreas <span class="hlt">fault</span> will be considered in Southern California, while the hundreds of other <span class="hlt">faults</span> in the region will be ignored. Rake will be constrained along each subfault to be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S53D..02O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S53D..02O"><span>Dynamic fracture network around <span class="hlt">faults</span>: implications for <span class="hlt">earthquake</span> ruptures, ground motion and energy budget</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Okubo, K.; Bhat, H. S.; Rougier, E.; Lei, Z.; Knight, E. E.; Klinger, Y.</p> <p>2017-12-01</p> <p>Numerous studies have suggested that spontaneous <span class="hlt">earthquake</span> ruptures can dynamically induce failure in secondary fracture network, regarded as damage zone around <span class="hlt">faults</span>. The feedbacks of such fracture network play a crucial role in <span class="hlt">earthquake</span> rupture, its radiated wave field and the total energy budget. A novel numerical modeling tool based on the combined finite-discrete element method (FDEM), which accounts for the main rupture propagation and nucleation/propagation of secondary cracks, was used to quantify the evolution of the fracture network and evaluate its effects on the main rupture and its associated radiation. The simulations were performed with the FDEM-based software tool, Hybrid Optimization Software Suite (HOSSedu) developed by Los Alamos National Laboratory. We first modeled an <span class="hlt">earthquake</span> rupture on a planar strike-slip <span class="hlt">fault</span> surrounded by a brittle medium where secondary cracks can be nucleated/activated by the <span class="hlt">earthquake</span> rupture. We show that the secondary cracks are dynamically generated dominantly on the extensional side of the <span class="hlt">fault</span>, mainly behind the rupture front, and it forms an intricate network of fractures in the damage zone. The rupture velocity thereby significantly decreases, by 10 to 20 percent, while the supershear transition length increases in comparison to the one with purely elastic medium. It is also observed that the high-frequency component (10 to 100 Hz) of the near-field ground acceleration is enhanced by the dynamically activated fracture network, consistent with field observations. We then conducted the case study in depth with various sets of initial stress state, and friction properties, to investigate the evolution of damage zone. We show that the width of damage zone decreases in depth, forming "flower-like" structure as the characteristic slip distance in linear slip-weakening law, or the fracture energy on the <span class="hlt">fault</span>, is kept constant with depth. Finally, we compared the fracture energy on the <span class="hlt">fault</span> to the energy</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.S72F1345R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.S72F1345R"><span>The 7.9 Denali <span class="hlt">Fault</span> <span class="hlt">Earthquake</span>: Aftershock Locations, Moment Tensors and Focal Mechanisms from the Regional Seismic Network Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ratchkovski, N. A.; Hansen, R. A.; Christensen, D.; Kore, K.</p> <p>2002-12-01</p> <p>The largest <span class="hlt">earthquake</span> ever recorded on the Denali <span class="hlt">fault</span> <span class="hlt">system</span> (magnitude 7.9) struck central Alaska on November 3, 2002. It was preceded by a magnitude 6.7 foreshock on October 23. This earlier <span class="hlt">earthquake</span> and its zone of aftershocks were located slightly to the west of the 7.9 quake. Aftershock locations and surface slip observations from the 7.9 quake indicate that the rupture was predominately unilateral in the eastward direction. Near Mentasta Lake, a village that experienced some of the worst damage in the quake, the surface rupture scar turns from the Denali <span class="hlt">fault</span> to the adjacent Totschunda <span class="hlt">fault</span>, which trends toward more southeasterly toward the Canadian border. Overall, the geologists found that measurable scarps indicate that the north side of the Denali <span class="hlt">fault</span> moved to the east and vertically up relative to the south. Maximum offsets on the Denali <span class="hlt">fault</span> were 8.8 meters at the Tok Highway cutoff, and were 2.2 meters on the Totschunda <span class="hlt">fault</span>. The Alaska regional seismic network consists of over 250 station sites, operated by the Alaska <span class="hlt">Earthquake</span> Information Center (AEIC), the Alaska Volcano Observatory (AVO), and the Pacific Tsunami Warning Center (PTWC). Over 25 sites are equipped with the broad-band sensors, some of which have in addition the strong motion sensors. The rest of the stations are either 1 or 3-component short-period instruments. The data from these stations are collected, processed and archived at the AEIC. The AEIC staff installed a temporary network with over 20 instruments following the 6.7 Nenana Mountain and the 7.9 events. Prior to the M 7.9 Denali <span class="hlt">Fault</span> event, the automatic <span class="hlt">earthquake</span> detection <span class="hlt">system</span> at AEIC was locating between 15 and 30 events per day. After the event, the <span class="hlt">system</span> had over 200-400 automatic locations per day for at least 10 days following the 7.9 event. The processing of the data is ongoing with the priority given to the larger events. The cumulative length of the 6.7 and 7.9 aftershock locations along the Denali</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021831','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021831"><span>On relating apparent stress to the stress causing <span class="hlt">earthquake</span> <span class="hlt">fault</span> slip</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGarr, A.</p> <p>1999-01-01</p> <p>Apparent stress ??a is defined as ??a = ??????, where ???? is the average shear stress loading the <span class="hlt">fault</span> plane to cause slip and ?? is the seismic efficiency, defined as Ea/W, where Ea is the energy radiated seismically and W is the total energy released by the <span class="hlt">earthquake</span>. The results of a recent study in which apparent stresses of mining-induced <span class="hlt">earthquakes</span> were compared to those measured for laboratory stick-slip friction events led to the hypothesis that ??a/???? ??? 0.06. This hypothesis is tested here against a substantially augmented data set of <span class="hlt">earthquakes</span> for which ???? can be estimated, mostly from in situ stress measurements, for comparison with ??a. The expanded data set, which includes <span class="hlt">earthquakes</span> artificially triggered at a depth of 9 km in the German Kontinentales Tiefbohrprogramm der Bundesrepublik Deutschland (KTB) borehole and natural tectonic <span class="hlt">earthquakes</span>, covers a broad range of hypocentral depths, rock types, pore pressures, and tectonic settings. Nonetheless, over ???14 orders of magnitude in seismic moment, apparent stresses exhibit distinct upper bounds defined by a maximum seismic efficiency of ???0.06, consistent with the hypothesis proposed before. This behavior of ??a and ?? can be expressed in terms of two parameters measured for stick-slip friction events in the laboratory: the ratio of the static to the dynamic coefficient of friction and the <span class="hlt">fault</span> slip overshoot. Typical values for these two parameters yield seismic efficiencies of ???0.06. In contrast to efficiencies for laboratory events for which ?? is always near 0.06, those for <span class="hlt">earthquakes</span> tend to be less than this bounding value because Ea for <span class="hlt">earthquakes</span> is usually underestimated due to factors such as band-limited recording. Thus upper bounds on ??a/???? appear to be controlled by just a few fundamental aspects of frictional stick-slip behavior that are common to shallow <span class="hlt">earthquakes</span> everywhere. Estimates of ???? from measurements of ??a for suites of <span class="hlt">earthquakes</span>, using ??a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29643366','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29643366"><span>Constant strain accumulation rate between major <span class="hlt">earthquakes</span> on the North Anatolian <span class="hlt">Fault</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hussain, Ekbal; Wright, Tim J; Walters, Richard J; Bekaert, David P S; Lloyd, Ryan; Hooper, Andrew</p> <p>2018-04-11</p> <p><span class="hlt">Earthquakes</span> are caused by the release of tectonic strain accumulated between events. Recent advances in satellite geodesy mean we can now measure this interseismic strain accumulation with a high degree of accuracy. But it remains unclear how to interpret short-term geodetic observations, measured over decades, when estimating the seismic hazard of <span class="hlt">faults</span> accumulating strain over centuries. Here, we show that strain accumulation rates calculated from geodetic measurements around a major transform <span class="hlt">fault</span> are constant for its entire 250-year interseismic period, except in the ~10 years following an <span class="hlt">earthquake</span>. The shear strain rate history requires a weak <span class="hlt">fault</span> zone embedded within a strong lower crust with viscosity greater than ~10 20  Pa s. The results support the notion that short-term geodetic observations can directly contribute to long-term seismic hazard assessment and suggest that lower-crustal viscosities derived from postseismic studies are not representative of the lower crust at all spatial and temporal scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2008/3019/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2008/3019/"><span>The Hayward <span class="hlt">Fault</span> - Is It Due for a Repeat of the Powerful 1868 <span class="hlt">Earthquake</span>?</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brocher, Thomas M.; Boatwright, Jack; Lienkaemper, James J.; Prentice, Carol S.; Schwartz, David P.; Bundock, Howard</p> <p>2008-01-01</p> <p>On October 21, 1868, a magnitude 6.8 <span class="hlt">earthquake</span> struck the San Francisco Bay region. Although the region was then sparsely populated, this quake on the Hayward <span class="hlt">Fault</span> was one of the most destructive in California?s history. Recent studies show that such powerful Hayward <span class="hlt">Fault</span> quakes have repeatedly jolted the region in the past. U.S. Geological Survey (USGS) scientists describe this <span class="hlt">fault</span> as a tectonic time bomb, due anytime for another magnitude 6.8 to 7.0 <span class="hlt">earthquake</span>. Because such a quake could cause hundreds of deaths, leave thousands homeless, and devastate the region?s economy, the USGS and other organizations are working together with new urgency to help prepare Bay Area communities for this certain future quake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S11C..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S11C..06G"><span>Active <span class="hlt">Faults</span> and Seismic Sources of the Middle East Region: <span class="hlt">Earthquake</span> Model of the Middle East (EMME) Project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gulen, L.; EMME WP2 Team*</p> <p>2011-12-01</p> <p>The <span class="hlt">Earthquake</span> Model of the Middle East (EMME) Project is a regional project of the GEM (Global <span class="hlt">Earthquake</span> Model) project (http://www.emme-gem.org/). The EMME project covers Turkey, Georgia, Armenia, Azerbaijan, Syria, Lebanon, Jordan, Iran, Pakistan, and Afghanistan. Both EMME and SHARE projects overlap and Turkey becomes a bridge connecting the two projects. The Middle East region is tectonically and seismically very active part of the Alpine-Himalayan orogenic belt. Many major <span class="hlt">earthquakes</span> have occurred in this region over the years causing casualties in the millions. The EMME project consists of three main modules: hazard, risk, and socio-economic modules. The EMME project uses PSHA approach for <span class="hlt">earthquake</span> hazard and the existing source models have been revised or modified by the incorporation of newly acquired data. The most distinguishing aspect of the EMME project from the previous ones is its dynamic character. This very important characteristic is accomplished by the design of a flexible and scalable database that permits continuous update, refinement, and analysis. An up-to-date <span class="hlt">earthquake</span> catalog of the Middle East region has been prepared and declustered by the WP1 team. EMME WP2 team has prepared a digital active <span class="hlt">fault</span> map of the Middle East region in ArcGIS format. We have constructed a database of <span class="hlt">fault</span> parameters for active <span class="hlt">faults</span> that are capable of generating <span class="hlt">earthquakes</span> above a threshold magnitude of Mw≥5.5. The EMME project database includes information on the geometry and rates of movement of <span class="hlt">faults</span> in a "<span class="hlt">Fault</span> Section Database", which contains 36 entries for each <span class="hlt">fault</span> section. The "<span class="hlt">Fault</span> Section" concept has a physical significance, in that if one or more <span class="hlt">fault</span> parameters change, a new <span class="hlt">fault</span> section is defined along a <span class="hlt">fault</span> zone. So far 6,991 <span class="hlt">Fault</span> Sections have been defined and 83,402 km of <span class="hlt">faults</span> are fully parameterized in the Middle East region. A separate "Paleo-Sites Database" includes information on the timing and amounts of <span class="hlt">fault</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoJI.208..748W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoJI.208..748W"><span><span class="hlt">Fault</span> geometry and slip distribution of the 2008 Mw 7.9 Wenchuan, China <span class="hlt">earthquake</span>, inferred from GPS and InSAR measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wan, Yongge; Shen, Zheng-Kang; Bürgmann, Roland; Sun, Jianbao; Wang, Min</p> <p>2017-02-01</p> <p>We revisit the problem of coseismic rupture of the 2008 Mw7.9 Wenchuan <span class="hlt">earthquake</span>. Precise determination of the <span class="hlt">fault</span> structure and slip distribution provides critical information about the mechanical behaviour of the <span class="hlt">fault</span> <span class="hlt">system</span> and <span class="hlt">earthquake</span> rupture. We use all the geodetic data available, craft a more realistic Earth structure and <span class="hlt">fault</span> model compared to previous studies, and employ a nonlinear inversion scheme to optimally solve for the <span class="hlt">fault</span> geometry and slip distribution. Compared to a homogeneous elastic half-space model and laterally uniform layered models, adopting separate layered elastic structure models on both sides of the Beichuan <span class="hlt">fault</span> significantly improved data fitting. Our results reveal that: (1) The Beichuan <span class="hlt">fault</span> is listric in shape, with near surface <span class="hlt">fault</span> dip angles increasing from ˜36° at the southwest end to ˜83° at the northeast end of the rupture. (2) The <span class="hlt">fault</span> rupture style changes from predominantly thrust at the southwest end to dextral at the northeast end of the <span class="hlt">fault</span> rupture. (3) <span class="hlt">Fault</span> slip peaks near the surface for most parts of the <span class="hlt">fault</span>, with ˜8.4 m thrust and ˜5 m dextral slip near Hongkou and ˜6 m thrust and ˜8.4 m dextral slip near Beichuan, respectively. (4) The peak slips are located around <span class="hlt">fault</span> geometric complexities, suggesting that <span class="hlt">earthquake</span> style and rupture propagation were determined by <span class="hlt">fault</span> zone geometric barriers. Such barriers exist primarily along restraining left stepping discontinuities of the dextral-compressional <span class="hlt">fault</span> <span class="hlt">system</span>. (5) The seismic moment released on the <span class="hlt">fault</span> above 20 km depth is 8.2×1021 N m, corresponding to an Mw7.9 event. The seismic moments released on the local slip concentrations are equivalent to events of Mw7.5 at Yingxiu-Hongkou, Mw7.3 at Beichuan-Pingtong, Mw7.2 near Qingping, Mw7.1 near Qingchuan, and Mw6.7 near Nanba, respectively. (6) The <span class="hlt">fault</span> geometry and kinematics are consistent with a model in which crustal deformation at the eastern margin of the Tibetan plateau is</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.9104H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.9104H"><span>An <span class="hlt">earthquake</span> rate forecast for Europe based on smoothed seismicity and smoothed <span class="hlt">fault</span> contribution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hiemer, Stefan; Woessner, Jochen; Basili, Roberto; Wiemer, Stefan</p> <p>2013-04-01</p> <p>The main objective of project SHARE (Seismic Hazard Harmonization in Europe) is to develop a community-based seismic hazard model for the Euro-Mediterranean region. The logic tree of <span class="hlt">earthquake</span> rupture forecasts comprises several methodologies including smoothed seismicity approaches. Smoothed seismicity thus represents an alternative concept to express the degree of spatial stationarity of seismicity and provides results that are more objective, reproducible, and testable. Nonetheless, the smoothed-seismicity approach suffers from the common drawback of being generally based on <span class="hlt">earthquake</span> catalogs alone, i.e. the wealth of knowledge from geology is completely ignored. We present a model that applies the kernel-smoothing method to both past <span class="hlt">earthquake</span> locations and slip rates on mapped crustal <span class="hlt">faults</span> and subductions. The result is mainly driven by the data, being independent of subjective delineation of seismic source zones. The core parts of our model are two distinct location probability densities: The first is computed by smoothing past seismicity (using variable kernel smoothing to account for varying data density). The second is obtained by smoothing <span class="hlt">fault</span> moment rate contributions. The <span class="hlt">fault</span> moment rates are calculated by summing the moment rate of each <span class="hlt">fault</span> patch on a fully parameterized and discretized <span class="hlt">fault</span> as available from the SHARE <span class="hlt">fault</span> database. We assume that the regional frequency-magnitude distribution of the entire study area is well known and estimate the a- and b-value of a truncated Gutenberg-Richter magnitude distribution based on a maximum likelihood approach that considers the spatial and temporal completeness history of the seismic catalog. The two location probability densities are linearly weighted as a function of magnitude assuming that (1) the occurrence of past seismicity is a good proxy to forecast occurrence of future seismicity and (2) future large-magnitude events occur more likely in the vicinity of known <span class="hlt">faults</span>. Consequently</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.733..108N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.733..108N"><span>Maximum magnitude of injection-induced <span class="hlt">earthquakes</span>: A criterion to assess the influence of pressure migration along <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norbeck, Jack H.; Horne, Roland N.</p> <p>2018-05-01</p> <p>The maximum expected <span class="hlt">earthquake</span> magnitude is an important parameter in seismic hazard and risk analysis because of its strong influence on ground motion. In the context of injection-induced seismicity, the processes that control how large an <span class="hlt">earthquake</span> will grow may be influenced by operational factors under engineering control as well as natural tectonic factors. Determining the relative influence of these effects on maximum magnitude will impact the design and implementation of induced seismicity management strategies. In this work, we apply a numerical model that considers the coupled interactions of fluid flow in <span class="hlt">faulted</span> porous media and quasidynamic elasticity to investigate the <span class="hlt">earthquake</span> nucleation, rupture, and arrest processes for cases of induced seismicity. We find that under certain conditions, <span class="hlt">earthquake</span> ruptures are confined to a pressurized region along the <span class="hlt">fault</span> with a length-scale that is set by injection operations. However, <span class="hlt">earthquakes</span> are sometimes able to propagate as sustained ruptures outside of the zone that experienced a pressure perturbation. We propose a <span class="hlt">faulting</span> criterion that depends primarily on the state of stress and the <span class="hlt">earthquake</span> stress drop to characterize the transition between pressure-constrained and runaway rupture behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.S12A0376V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.S12A0376V"><span>Spatial Based Integrated Assessment of Bedrock and Ground Motions, <span class="hlt">Fault</span> Offsets, and Their Effects for the October-November 2002 <span class="hlt">Earthquake</span> Sequence on the Denali <span class="hlt">Fault</span>, Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vinson, T. S.; Carlson, R.; Hansen, R.; Hulsey, L.; Ma, J.; White, D.; Barnes, D.; Shur, Y.</p> <p>2003-12-01</p> <p>A National Science Foundation (NSF) Small Grant Exploratory Research Grant was awarded to the University of Alaska Fairbanks to archive bedrock and ground motions and <span class="hlt">fault</span> offsets and their effects for the October-November 2002 <span class="hlt">earthquake</span> sequence on the Denali <span class="hlt">Fault</span>, Alaska. The scope of work included the accumulation of all strong motion records, satellite imagery, satellite remote sensing data, aerial and ground photographs, and structural response (both measured and anecdotal) that would be useful to achieve the objective. Several interesting data sets were archived including ice cover, lateral movement of stream channels, landslides, avalanches, glacial fracturing, "felt" ground motions, and changes in water quantity and quality. The data sources may be spatially integrated to provide a comprehensive assessment of the bedrock and ground motions and <span class="hlt">fault</span> offsets for the October-November 2002 <span class="hlt">earthquake</span> sequence. In the aftermath of the October-November 2002 <span class="hlt">earthquake</span> sequence on the Denali <span class="hlt">fault</span>, the Alaskan engineering community expressed a strong interest to understand why their structures and infrastructure were not substantially damaged by the ground motions they experienced during the October-November 2002 <span class="hlt">Earthquake</span> Sequence on the Denali <span class="hlt">Fault</span>. The research work proposed under this NSF Grant is a necessary prerequisite to this understanding. Furthermore, the proposed work will facilitate a comparison of Denali events with the Loma Prieta and recent Kocelli and Dozce events in Turkey, all of which were associated with strike-slip <span class="hlt">faulting</span>. Finally, the spatially integrated data will provide the basis for research work that is truly innovative. For example, is may be possible to predict the observed (1) landsliding and avalanches, (2) changes in water quantity and quality, (3) glacial fracturing, and (4) the widespread liquefaction and lateral spreading, which occurred along the Tok cutoff and Northway airport, with the bedrock and ground motions and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1211153V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1211153V"><span>Preliminary results on <span class="hlt">earthquake</span> triggered landslides for the Haiti <span class="hlt">earthquake</span> (January 2010)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van Westen, Cees; Gorum, Tolga</p> <p>2010-05-01</p> <p>This study presents the first results on an analysis of the landslides triggered by the Ms 7.0 Haiti <span class="hlt">earthquake</span> that occurred on January 12, 2010 in the boundary region of the Pacific Plate and the North American plate. The <span class="hlt">fault</span> is a left lateral strike slip <span class="hlt">fault</span> with a clear surface expression. According to the USGS <span class="hlt">earthquake</span> information the Enriquillo-Plantain Garden <span class="hlt">fault</span> <span class="hlt">system</span> has not produced any major <span class="hlt">earthquake</span> in the last 100 years, and historical <span class="hlt">earthquakes</span> are known from 1860, 1770, 1761, 1751, 1684, 1673, and 1618, though none of these has been confirmed in the field as associated with this <span class="hlt">fault</span>. We used high resolution satellite imagery available for the pre and post <span class="hlt">earthquake</span> situations, which were made freely available for the response and rescue operations. We made an interpretation of all co-seismic landslides in the epicentral area. We conclude that the <span class="hlt">earthquake</span> mainly triggered landslide in the northern slope of the <span class="hlt">fault</span>-related valley and in a number of isolated area. The <span class="hlt">earthquake</span> apparently didn't trigger many visible landslides within the slum areas on the slopes in the southern part of Port-au-Prince and Carrefour. We also used ASTER DEM information to relate the landslide occurrences with DEM derivatives.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S11A2753L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S11A2753L"><span><span class="hlt">Earthquake</span> relocation near the Leech River <span class="hlt">Fault</span>, southern Vancouver Island</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, G.; Liu, Y.; Regalla, C.</p> <p>2015-12-01</p> <p>The Leech River <span class="hlt">Fault</span> (LRF), a northeast dipping thrust, extends across the southern tip of Vancouver Island in Southwest British Columbia, where local tectonic regime is dominated by the subduction of the Juan de Fuca plate beneath the North American plate at the present rate of 40-50 mm/year. British Columbia geologic map (Geoscience Map 2009-1A) shows that this area also consists of many crosscutting minor <span class="hlt">faults</span> in addition to the San Juan <span class="hlt">Fault</span> north of the LRF. To investigate the seismic evidence of the subsurface structures of these minor <span class="hlt">faults</span> and of possible hidden active structures in this area, precise <span class="hlt">earthquake</span> locations are required. In this study, we relocate 941 <span class="hlt">earthquakes</span> reported by Canadian National Seismograph Network (CNSN) catalog from 2000 to 2015 within a 100km x 55km study area surrounding the LRF. We use HypoDD [Waldhauser, F., 2001] double-difference relocation method by combining P/S phase arrivals provided by the CNSN at 169 stations and waveform data with correlation coefficient values greater than 0.7 at 50 common stations and event separation less than 10km. A total of 900 out of the 931 events satisfy the above relocation criteria. Velocity model used is a 1-D model extracted from the Ramachandran et al. (2005) model. Average relative location errors estimated by the bootstrap method are 546.5m (horizontal) and 1128.6m (in depth). Absolute errors reported by SVD method for individual clusters are ~100m in both dimensions. We select 5 clusters visually according to their epicenters (see figure). Cluster 1 is parallel to the LRF and a thrust FID #60. Clusters 2 and 3 are bounded by two <span class="hlt">faults</span>: FID #75, a northeast dipping thrust marking the southwestern boundary of the Wrangellia terrane, and FID #2 marking the northern boundary. Clusters 4 and 5, to the northeast and northwest of Victoria respectively, however, do not represent the surface traces of any mapped <span class="hlt">faults</span>. The depth profile of Cluster 5 depicts a hidden northeast</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T23A0598W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T23A0598W"><span>New insights on active <span class="hlt">fault</span> geometries in the Mentawai region of Sumatra, Indonesia, from broadband waveform modeling of <span class="hlt">earthquake</span> source parameters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>WANG, X.; Wei, S.; Bradley, K. E.</p> <p>2017-12-01</p> <p>Global <span class="hlt">earthquake</span> catalogs provide important first-order constraints on the geometries of active <span class="hlt">faults</span>. However, the accuracies of both locations and focal mechanisms in these catalogs are typically insufficient to resolve detailed <span class="hlt">fault</span> geometries. This issue is particularly critical in subduction zones, where most great <span class="hlt">earthquakes</span> occur. The Slab 1.0 model (Hayes et al. 2012), which was derived from global <span class="hlt">earthquake</span> catalogs, has smooth <span class="hlt">fault</span> geometries, and cannot adequately address local structural complexities that are critical for understanding <span class="hlt">earthquake</span> rupture patterns, coseismic slip distributions, and geodetically monitored interseismic coupling. In this study, we conduct careful relocation and waveform modeling of <span class="hlt">earthquake</span> source parameters to reveal <span class="hlt">fault</span> geometries in greater detail. We take advantage of global data and conduct broadband waveform modeling for medium size <span class="hlt">earthquakes</span> (M>4.5) to refine their source parameters, which include locations and <span class="hlt">fault</span> plane solutions. The refined source parameters can greatly improve the imaging of <span class="hlt">fault</span> geometry (e.g., Wang et al., 2017). We apply these approaches to <span class="hlt">earthquakes</span> recorded since 1990 in the Mentawai region offshore of central Sumatra. Our results indicate that the uncertainty of the horizontal location, depth and dip angle estimation are as small as 5 km, 2 km and 5 degrees, respectively. The refined catalog shows that the 2005 and 2009 "back-thrust" sequences in Mentawai region actually occurred on a steeply landward-dipping <span class="hlt">fault</span>, contradicting previous studies that inferred a seaward-dipping backthrust. We interpret these <span class="hlt">earthquakes</span> as `unsticking' of the Sumatran accretionary wedge along a backstop <span class="hlt">fault</span> that separates accreted material of the wedge from the strong Sunda lithosphere, or reactivation of an old normal <span class="hlt">fault</span> buried beneath the forearc basin. We also find that the seismicity on the Sunda megathrust deviates in location from Slab 1.0 by up to 7 km, with along strike</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.S53A0179W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.S53A0179W"><span>The Relationships Between <span class="hlt">Earthquakes</span>, <span class="hlt">Faults</span>, and Recent Glacial Fluctuations in Southern Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wiest, K. R.; Sauber, J. M.; Doser, D. I.; Hurtado, J. M.; Velasco, A. A.</p> <p>2004-12-01</p> <p>In southern Alaska, northwestward-directed subduction of the Pacific plate is accompanied by accretion of the Yakutat terrane to continental Alaska. In the tectonically complex region between the transcurrent Fairweather <span class="hlt">fault</span> and the Alaska-Aleutian subduction zone, active crustal shortening and strike-slip <span class="hlt">faulting</span> occurs. Since a series of large <span class="hlt">earthquakes</span> in 1899 (Mw = 8.1, Yakataga; Mw=8.1 Yakutat), there has been only one large event (1979 St. Elias Mw = 7.4) in the Yakutat region between the aftershock zones of the 1964 Prince William Sound (Mw = 9.2) and 1958 Fairweather (Mw = 8.2) <span class="hlt">earthquakes</span>. In this region, the glaciers are extensive and many of them have undergone significant retreat in the last 100 years. This study investigates the relationships between small to moderate magnitude events, ongoing crustal deformation, active geological structures in the region, and recent glacial fluctuations. To map <span class="hlt">earthquake</span> locations with respect to current glacier positions, we will incorporate Ice Cloud and land Elevation Satellite (ICESat) data into an updated Digital Elevation Model (DEM) of key glaciated regions that has been created using Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) images in conjunction with Shuttle Radar Topography Mission (SRTM) data. For the seismological investigation, we focused on relocating events that have occurred since the last large <span class="hlt">earthquake</span> at St. Elias in 1979 using data obtained from the Alaska <span class="hlt">Earthquake</span> Information Center (AEIC). P-wave polarity first motion focal mechanisms were generated for the relocated events and evaluated. Our preliminary relocations suggest a dipping slab in cross-section and also show a number of shallow event clusters around local glaciers. The focal mechanisms are quite variable but, in general, indicate strike-slip and oblique-slip focal mechanisms. Some of our highest quality focal mechanisms show dip-slip <span class="hlt">faulting</span> and are from shallow events located near glacial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AIPC.1658c0010W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AIPC.1658c0010W"><span><span class="hlt">Earthquake</span> disaster mitigation of Lembang <span class="hlt">Fault</span> West Java with electromagnetic method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Widodo</p> <p>2015-04-01</p> <p>The Lembang <span class="hlt">fault</span> is located around eight kilometers from Bandung City, West Java, Indonesia. The existence of this <span class="hlt">fault</span> runs through densely populated settlement and tourism area. It is an active <span class="hlt">fault</span> structure with increasing seismic activity where the 28 August 2011 <span class="hlt">earthquake</span> occurred. The seismic response at the site is strongly influenced by local geological conditions. The ambient noise measurements from the western part of this <span class="hlt">fault</span> give strong implication for a complex 3-D tectonic setting. Hence, near surface Electromagnetic (EM) measurements are carried out to understand the location of the local active <span class="hlt">fault</span> of the research area. Hence, near surface EM measurements are carried out to understand the location of the local active <span class="hlt">fault</span> and the top of the basement structure of the research area. The Transientelectromagnetic (TEM) measurements are carried out along three profiles, which include 35 TEM soundings. The results indicate that TEM data give detailed conductivity distribution of <span class="hlt">fault</span> structure in the study area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22391571-earthquake-disaster-mitigation-lembang-fault-west-java-electromagnetic-method','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22391571-earthquake-disaster-mitigation-lembang-fault-west-java-electromagnetic-method"><span><span class="hlt">Earthquake</span> disaster mitigation of Lembang <span class="hlt">Fault</span> West Java with electromagnetic method</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Widodo, E-mail: widodo@gf.itb.ac.id</p> <p></p> <p>The Lembang <span class="hlt">fault</span> is located around eight kilometers from Bandung City, West Java, Indonesia. The existence of this <span class="hlt">fault</span> runs through densely populated settlement and tourism area. It is an active <span class="hlt">fault</span> structure with increasing seismic activity where the 28 August 2011 <span class="hlt">earthquake</span> occurred. The seismic response at the site is strongly influenced by local geological conditions. The ambient noise measurements from the western part of this <span class="hlt">fault</span> give strong implication for a complex 3-D tectonic setting. Hence, near surface Electromagnetic (EM) measurements are carried out to understand the location of the local active <span class="hlt">fault</span> of the research area. Hence,more » near surface EM measurements are carried out to understand the location of the local active <span class="hlt">fault</span> and the top of the basement structure of the research area. The Transientelectromagnetic (TEM) measurements are carried out along three profiles, which include 35 TEM soundings. The results indicate that TEM data give detailed conductivity distribution of <span class="hlt">fault</span> structure in the study area.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70120714','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70120714"><span>Holocene <span class="hlt">earthquakes</span> and right-lateral slip on the left-lateral Darrington-Devils Mountain <span class="hlt">fault</span> zone, northern Puget Sound, Washington</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Personius, Stephen F.; Briggs, Richard W.; Nelson, Alan R.; Schermer, Elizabeth R; Maharrey, J. Zebulon; Sherrod, Brian; Spaulding, Sarah A.; Bradley, Lee-Ann</p> <p>2014-01-01</p> <p>Sources of seismic hazard in the Puget Sound region of northwestern Washington include deep <span class="hlt">earthquakes</span> associated with the Cascadia subduction zone, and shallow <span class="hlt">earthquakes</span> associated with some of the numerous crustal (upper-plate) <span class="hlt">faults</span> that crisscross the region. Our paleoseismic investigations on one of the more prominent crustal <span class="hlt">faults</span>, the Darrington–Devils Mountain <span class="hlt">fault</span> zone, included trenching of <span class="hlt">fault</span> scarps developed on latest Pleistocene glacial sediments and analysis of cores from an adjacent wetland near Lake Creek, 14 km southeast of Mount Vernon, Washington. Trench excavations revealed evidence of a single <span class="hlt">earthquake</span>, radiocarbon dated to ca. 2 ka, but extensive burrowing and root mixing of sediments within 50–100 cm of the ground surface may have destroyed evidence of other <span class="hlt">earthquakes</span>. Cores in a small wetland adjacent to our trench site provided stratigraphic evidence (formation of a laterally extensive, prograding wedge of hillslope colluvium) of an <span class="hlt">earthquake</span> ca. 2 ka, which we interpret to be the same <span class="hlt">earthquake</span> documented in the trenches. A similar colluvial wedge lower in the wetland section provides possible evidence for a second <span class="hlt">earthquake</span> dated to ca. 8 ka. Three-dimensional trenching techniques revealed evidence for 2.2 ± 1.1 m of right-lateral offset of a glacial outwash channel margin, and 45–70 cm of north-side-up vertical separation across the <span class="hlt">fault</span> zone. These offsets indicate a net slip vector of 2.3 ± 1.1 m, plunging 14° west on a 286°-striking, 90°-dipping <span class="hlt">fault</span> plane. The dominant right-lateral sense of slip is supported by the presence of numerous Riedel R shears preserved in two of our trenches, and probable right-lateral offset of a distinctive bedrock <span class="hlt">fault</span> zone in a third trench. Holocene north-side-up, right-lateral oblique slip is opposite the south-side-up, left-lateral oblique sense of slip inferred from geologic mapping of Eocene and older rocks along the <span class="hlt">fault</span> zone. The cause of this slip reversal is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRB..121.8196R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRB..121.8196R"><span>Complex spatiotemporal evolution of the 2008 Mw 4.9 Mogul <span class="hlt">earthquake</span> swarm (Reno, Nevada): Interplay of fluid and <span class="hlt">faulting</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ruhl, C. J.; Abercrombie, R. E.; Smith, K. D.; Zaliapin, I.</p> <p>2016-11-01</p> <p>After approximately 2 months of swarm-like <span class="hlt">earthquakes</span> in the Mogul neighborhood of west Reno, NV, seismicity rates and event magnitudes increased over several days culminating in an Mw 4.9 dextral strike-slip <span class="hlt">earthquake</span> on 26 April 2008. Although very shallow, the Mw 4.9 main shock had a different sense of slip than locally mapped dip-slip surface <span class="hlt">faults</span>. We relocate 7549 <span class="hlt">earthquakes</span>, calculate 1082 focal mechanisms, and statistically cluster the relocated <span class="hlt">earthquake</span> catalog to understand the character and interaction of active structures throughout the Mogul, NV <span class="hlt">earthquake</span> sequence. Rapid temporary instrument deployment provides high-resolution coverage of microseismicity, enabling a detailed analysis of swarm behavior and <span class="hlt">faulting</span> geometry. Relocations reveal an internally clustered sequence in which foreshocks evolved on multiple structures surrounding the eventual main shock rupture. The relocated seismicity defines a <span class="hlt">fault</span>-fracture mesh and detailed <span class="hlt">fault</span> structure from approximately 2-6 km depth on the previously unknown Mogul <span class="hlt">fault</span> that may be an evolving incipient strike-slip <span class="hlt">fault</span> zone. The seismicity volume expands before the main shock, consistent with pore pressure diffusion, and the aftershock volume is much larger than is typical for an Mw 4.9 <span class="hlt">earthquake</span>. We group events into clusters using space-time-magnitude nearest-neighbor distances between events and develop a cluster criterion through randomization of the relocated catalog. Identified clusters are largely main shock-aftershock sequences, without evidence for migration, occurring within the diffuse background seismicity. The migration rate of the largest foreshock cluster and simultaneous background events is consistent with it having triggered, or having been triggered by, an aseismic slip event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S44B..06K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S44B..06K"><span>Active Tectonics of Himalayan <span class="hlt">Faults</span>/Thrusts <span class="hlt">System</span> in Northern India on the basis of recent & Paleo <span class="hlt">earthquake</span> Studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, S.; Biswal, S.; Parija, M. P.</p> <p>2016-12-01</p> <p>The Himalaya overrides the Indian plate along a decollement <span class="hlt">fault</span>, referred as the Main Himalayan Thrust (MHT). The 2400 km long Himalayan mountain arc in the northern boundary of the Indian sub-continent is one of the most seismically active regions of the world. The Himalayan Frontal Thrust (HFT) is characterized by an abrupt physiographic and tectonic break between the Himalayan front and the Indo-Gangetic plain. The HFT represents the southern surface expression of the MHT on the Himalayan front. The tectonic zone between the Main Boundary Thrust (MBT) and the HFT encompasses the Himalayan Frontal <span class="hlt">Fault</span> <span class="hlt">System</span> (HFFS). The zone indicates late Quaternary-Holocene active deformation. Late Quaternary intramontane basin of Dehradun flanked to the south by the Mohand anticline lies between the MBT and the HFT in Garhwal Sub Himalaya. Slip rate 13-15 mm/yr has been estimated on the HFT based on uplifted strath terrace on the Himalyan front (Wesnousky et al. 2006). An out of sequence active <span class="hlt">fault</span>, Bhauwala Thrust (BT), is observed between the HFT and the MBT. The Himalayan Frontal <span class="hlt">Fault</span> <span class="hlt">System</span> includes MBT, BT, HFT and PF active <span class="hlt">fault</span> structures (Thakur, 2013). The HFFS structures were developed analogous to proto-thrusts in subduction zone, suggesting that the plate boundary is not a single structure, but series of structures across strike. Seismicity recorded by WIHG shows a concentrated belt of seismic events located in the Main Central Thrust Zone and the physiographic transition zone between the Higher and Lesser Himalaya. However, there is quiescence in the Himalayan frontal zone where surface rupture and active <span class="hlt">faults</span> are reported. GPS measurements indicate the segment between the southern extent of microseismicity zone and the HFT is locked. The great <span class="hlt">earthquake</span> originating in the locked segment rupture the plate boundary <span class="hlt">fault</span> and propagate to the Himalaya front and are registered as surface rupture reactivating the <span class="hlt">fault</span> in the HFFS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026294','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026294"><span>The susitna glacier thrust <span class="hlt">fault</span>: Characteristics of surface ruptures on the <span class="hlt">fault</span> that initiated the 2002 denali <span class="hlt">fault</span> <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Crone, A.J.; Personius, S.F.; Craw, P.A.; Haeussler, P.J.; Staft, L.A.</p> <p>2004-01-01</p> <p>The 3 November 2002 Mw 7.9 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> sequence initiated on the newly discovered Susitna Glacier thrust <span class="hlt">fault</span> and caused 48 km of surface rupture. Rupture of the Susitna Glacier <span class="hlt">fault</span> generated scarps on ice of the Susitna and West Fork glaciers and on tundra and surficial deposits along the southern front of the central Alaska Range. Based on detailed mapping, 27 topographic profiles, and field observations, we document the characteristics and slip distribution of the 2002 ruptures and describe evidence of pre-2002 ruptures on the <span class="hlt">fault</span>. The 2002 surface <span class="hlt">faulting</span> produced structures that range from simple folds on a single trace to complex thrust-<span class="hlt">fault</span> ruptures and pressure ridges on multiple, sinuous strands. The deformation zone is locally more than 1 km wide. We measured a maximum vertical displacement of 5.4 m on the south-directed main thrust. North-directed backthrusts have more than 4 m of surface offset. We measured a well-constrained near-surface <span class="hlt">fault</span> dip of about 19?? at one site, which is considerably less than seismologically determined values of 35??-48??. Surface-rupture data yield an estimated magnitude of Mw 7.3 for the <span class="hlt">fault</span>, which is similar to the seismological value of Mw 7.2. Comparison of field and seismological data suggest that the Susitna Glacier <span class="hlt">fault</span> is part of a large positive flower structure associated with northwest-directed transpressive deformation on the Denali <span class="hlt">fault</span>. Prehistoric scarps are evidence of previous rupture of the Sustina Glacier <span class="hlt">fault</span>, but additional work is needed to determine if past failures of the Susitna Glacier <span class="hlt">fault</span> have consistently induced rupture of the Denali <span class="hlt">fault</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70041948','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70041948"><span>Afterslip, tremor, and the Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gomberg, Joan; Prejean, Stephanie; Ruppert, Natalia</p> <p>2012-01-01</p> <p>We tested the hypothesis that afterslip should be accompanied by tremor using observations of seismic and aseismic deformation surrounding the 2002 M 7.9 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span> (DFE). Afterslip happens more frequently than spontaneous slow slip and has been observed in a wider range of tectonic environments, and thus the existence or absence of tremor accompanying afterslip may provide new clues about tremor generation. We also searched for precursory tremor, as a proxy for posited accelerating slip leading to rupture. Our search yielded no tremor during the five days prior to the DFE or in several intervals in the three months after. This negative result and an array of other observations all may be explained by rupture penetrating below the presumed locked zone into the frictional transition zone. While not unique, such an explanation corroborates previous models of megathrust and transform <span class="hlt">earthquake</span> ruptures that extend well into the transition zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T41B2896I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T41B2896I"><span>Progressive failure during the 1596 Keicho <span class="hlt">earthquakes</span> on the Median Tectonic Line active <span class="hlt">fault</span> zone, southwest Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ikeda, M.; Toda, S.; Nishizaka, N.; Onishi, K.; Suzuki, S.</p> <p>2015-12-01</p> <p>Rupture patterns of a long <span class="hlt">fault</span> <span class="hlt">system</span> are controlled by spatial heterogeneity of <span class="hlt">fault</span> strength and stress associated with geometrical characteristics and stress perturbation history. Mechanical process for sequential ruptures and multiple simultaneous ruptures, one of the characteristics of a long <span class="hlt">fault</span> such as the North Anatolian <span class="hlt">fault</span>, governs the size and frequency of large <span class="hlt">earthquakes</span>. Here we introduce one of the cases in southwest Japan and explore what controls rupture initiation, sequential ruptures and <span class="hlt">fault</span> branching on a long <span class="hlt">fault</span> <span class="hlt">system</span>. The Median Tectonic Line active <span class="hlt">fault</span> zone (hereinafter MTL) is the longest and most active <span class="hlt">fault</span> in Japan. Based on historical accounts, a series of M ≥ 7 <span class="hlt">earthquakes</span> occurred on at least a 300-km-long portion of the MTL in 1596. On September 1, the first event occurred on the Kawakami <span class="hlt">fault</span> segment, in Central Shikoku, and the subsequent events occurred further west. Then on September 5, another rupture initiated from the Central to East Shikoku and then propagated toward the Rokko-Awaji <span class="hlt">fault</span> zone to Kobe, a northern branch of the MTL, instead of the eastern main extent of the MTL. Another rupture eventually extended to near Kyoto. To reproduce this progressive failure, we applied two numerical models: one is a coulomb stress transfer; the other is a slip-tendency analysis under the tectonic stress. We found that Coulomb stress imparted from historical ruptures have triggered the subsequent ruptures nearby. However, stress transfer does not explain beginning of the sequence and rupture directivities. Instead, calculated slip-tendency values show highly variable along the MTL: high and low seismic potential in West and East Shikoku. The initiation point of the 1596 progressive failure locates near the boundary in the slip-tendency values. Furthermore, the slip-tendency on the Rokko-Awaji <span class="hlt">fault</span> zone is far higher than that of the MTL in Wakayama, which may explain the rupture directivity toward Kobe-Kyoto.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43.4340H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43.4340H"><span>Comparative study of two tsunamigenic <span class="hlt">earthquakes</span> in the Solomon Islands: 2015 Mw 7.0 normal-<span class="hlt">fault</span> and 2013 Santa Cruz Mw 8.0 megathrust <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heidarzadeh, Mohammad; Harada, Tomoya; Satake, Kenji; Ishibe, Takeo; Gusman, Aditya Riadi</p> <p>2016-05-01</p> <p>The July 2015 Mw 7.0 Solomon Islands tsunamigenic <span class="hlt">earthquake</span> occurred ~40 km north of the February 2013 Mw 8.0 Santa Cruz <span class="hlt">earthquake</span>. The proximity of the two epicenters provided unique opportunities for a comparative study of their source mechanisms and tsunami generation. The 2013 <span class="hlt">earthquake</span> was an interplate event having a thrust focal mechanism at a depth of 30 km while the 2015 event was a normal-<span class="hlt">fault</span> <span class="hlt">earthquake</span> occurring at a shallow depth of 10 km in the overriding Pacific Plate. A combined use of tsunami and teleseismic data from the 2015 event revealed the north dipping <span class="hlt">fault</span> plane and a rupture velocity of 3.6 km/s. Stress transfer analysis revealed that the 2015 <span class="hlt">earthquake</span> occurred in a region with increased Coulomb stress following the 2013 <span class="hlt">earthquake</span>. Spectral deconvolution, assuming the 2015 tsunami as empirical Green's function, indicated the source periods of the 2013 Santa Cruz tsunami as 10 and 22 min.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70188388','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70188388"><span>Paleoseismologic evidence for large-magnitude (Mw 7.5-8.0) <span class="hlt">earthquakes</span> on the Ventura blind thrust <span class="hlt">fault</span>: Implications for multifault ruptures in the Transverse Ranges of southern California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McAuliffe, Lee J.; Dolan, James F.; Rhodes, Edward J.; Hubbard, Judith; Shaw, John H.; Pratt, Thomas L.</p> <p>2015-01-01</p> <p>Detailed analysis of continuously cored boreholes and cone penetrometer tests (CPTs), high-resolution seismic-reflection data, and luminescence and 14C dates from Holocene strata folded above the tip of the Ventura blind thrust <span class="hlt">fault</span> constrain the ages and displacements of the two (or more) most recent <span class="hlt">earthquakes</span>. These two <span class="hlt">earthquakes</span>, which are identified by a prominent surface fold scarp and a stratigraphic sequence that thickens across an older buried fold scarp, occurred before the 235-yr-long historic era and after 805 ± 75 yr ago (most recent folding event[s]) and between 4065 and 4665 yr ago (previous folding event[s]). Minimum uplift in these two scarp-forming events was ∼6 m for the most recent <span class="hlt">earthquake(s</span>) and ∼5.2 m for the previous event(s). Large uplifts such as these typically occur in large-magnitude <span class="hlt">earthquakes</span> in the range of Mw7.5–8.0. Any such events along the Ventura <span class="hlt">fault</span> would likely involve rupture of other Transverse Ranges <span class="hlt">faults</span> to the east and west and/or rupture downward onto the deep, low-angle décollements that underlie these <span class="hlt">faults</span>. The proximity of this large reverse-<span class="hlt">fault</span> <span class="hlt">system</span> to major population centers, including the greater Los Angeles region, and the potential for tsunami generation during ruptures extending offshore along the western parts of the <span class="hlt">system</span> highlight the importance of understanding the complex behavior of these <span class="hlt">faults</span> for probabilistic seismic hazard assessment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009E%26PSL.284...94N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009E%26PSL.284...94N"><span><span class="hlt">Faulting</span> and hydration of the Juan de Fuca plate <span class="hlt">system</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nedimović, Mladen R.; Bohnenstiehl, DelWayne R.; Carbotte, Suzanne M.; Pablo Canales, J.; Dziak, Robert P.</p> <p>2009-06-01</p> <p>Multichannel seismic observations provide the first direct images of crustal scale normal <span class="hlt">faults</span> within the Juan de Fuca plate <span class="hlt">system</span> and indicate that brittle deformation extends up to ~ 200 km seaward of the Cascadia trench. Within the sedimentary layering steeply dipping <span class="hlt">faults</span> are identified by stratigraphic offsets, with maximum throws of 110 ± 10 m found near the trench. <span class="hlt">Fault</span> throws diminish both upsection and seaward from the trench. Long-term throw rates are estimated to be 13 ± 2 mm/kyr. <span class="hlt">Faulted</span> offsets within the sedimentary layering are typically linked to larger offset scarps in the basement topography, suggesting reactivation of the normal <span class="hlt">fault</span> <span class="hlt">systems</span> formed at the spreading center. Imaged reflections within the gabbroic igneous crust indicate swallowing <span class="hlt">fault</span> dips at depth. These reflections require local alteration to produce an impedance contrast, indicating that the imaged <span class="hlt">fault</span> structures provide pathways for fluid transport and hydration. As the depth extent of imaged <span class="hlt">faulting</span> within this young and sediment insulated oceanic plate is primarily limited to approximately Moho depths, <span class="hlt">fault</span>-controlled hydration appears to be largely restricted to crustal levels. If dehydration embrittlement is an important mechanism for triggering intermediate-depth <span class="hlt">earthquakes</span> within the subducting slab, then the limited occurrence rate and magnitude of intraslab seismicity at the Cascadia margin may in part be explained by the limited amount of water imbedded into the uppermost oceanic mantle prior to subduction. The distribution of submarine <span class="hlt">earthquakes</span> within the Juan de Fuca plate <span class="hlt">system</span> indicates that propagator wake areas are likely to be more <span class="hlt">faulted</span> and therefore more hydrated than other parts of this plate <span class="hlt">system</span>. However, being largely restricted to crustal levels, this localized increase in hydration generally does not appear to have a measurable effect on the intraslab seismicity along most of the subducted propagator wakes at the Cascadia margin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T42A..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T42A..06C"><span>Long term <span class="hlt">fault</span> <span class="hlt">system</span> reorganization of convergent and strike-slip <span class="hlt">systems</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cooke, M. L.; McBeck, J.; Hatem, A. E.; Toeneboehn, K.; Beyer, J. L.</p> <p>2017-12-01</p> <p>Laboratory and numerical experiments representing deformation over many <span class="hlt">earthquake</span> cycles demonstrate that <span class="hlt">fault</span> evolution includes episodes of <span class="hlt">fault</span> reorganization that optimize work on the <span class="hlt">fault</span> <span class="hlt">system</span>. Consequently, the mechanical and kinematic efficiencies of <span class="hlt">fault</span> <span class="hlt">systems</span> do not increase monotonically through their evolution. New <span class="hlt">fault</span> configurations can optimize the external work required to accommodate deformation, suggesting that changes in <span class="hlt">system</span> efficiency can drive <span class="hlt">fault</span> reorganization. Laboratory evidence and numerical results show that <span class="hlt">fault</span> reorganization within accretion, strike-slip and oblique convergent <span class="hlt">systems</span> is associated with increasing efficiency due to increased <span class="hlt">fault</span> slip (frictional work and seismic energy) and commensurate decreased off-<span class="hlt">fault</span> deformation (internal work and work against gravity). Between episodes of <span class="hlt">fault</span> reorganization, <span class="hlt">fault</span> <span class="hlt">systems</span> may become less efficient as they produce increasing off <span class="hlt">fault</span> deformation. For example, laboratory and numerical experiments show that the interference and interaction between different <span class="hlt">fault</span> segments may increase local internal work or that increasing convergence can increase work against gravity produced by a <span class="hlt">fault</span> <span class="hlt">system</span>. This accumulation of work triggers <span class="hlt">fault</span> reorganization as stored work provides the energy required to grow new <span class="hlt">faults</span> that reorganize the <span class="hlt">system</span> to a more efficient configuration. The results of laboratory and numerical experiments reveal that we should expect crustal <span class="hlt">fault</span> <span class="hlt">systems</span> to reorganize following periods of increasing inefficiency, even in the absence of changes to the tectonic regime. In other words, <span class="hlt">fault</span> reorganization doesn't require a change in tectonic loading. The time frame of <span class="hlt">fault</span> reorganization depends on <span class="hlt">fault</span> <span class="hlt">system</span> configuration, strain rate and processes that relax stresses within the crust. For example, stress relaxation may keep pace with stress accumulation, which would limit the increase in the internal work and gravitational work so that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=earthquakes&pg=5&id=EJ782558','ERIC'); return false;" href="https://eric.ed.gov/?q=earthquakes&pg=5&id=EJ782558"><span>Redefining <span class="hlt">Earthquakes</span> and the <span class="hlt">Earthquake</span> Machine</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Hubenthal, Michael; Braile, Larry; Taber, John</p> <p>2008-01-01</p> <p>The <span class="hlt">Earthquake</span> Machine (EML), a mechanical model of stick-slip <span class="hlt">fault</span> <span class="hlt">systems</span>, can increase student engagement and facilitate opportunities to participate in the scientific process. This article introduces the EML model and an activity that challenges ninth-grade students' misconceptions about <span class="hlt">earthquakes</span>. The activity emphasizes the role of models…</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.2625E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.2625E"><span><span class="hlt">Faults</span> Get Colder Through Transient Granular Vortices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Einav, I.; Rognon, P.; Miller, T.; Sulem, J.</p> <p>2018-03-01</p> <p><span class="hlt">Fault</span> temperatures govern their weakening and control the dynamics of <span class="hlt">earthquakes</span> during slip. Despite predictions of significant temperature rise within <span class="hlt">fault</span> gouges during <span class="hlt">earthquake</span> events, observations of frictional melting zones along exhumed <span class="hlt">faults</span> are relatively rare. Could there be a heat transfer mechanism, previously not considered, that results in ubiquitously colder <span class="hlt">faults</span> during <span class="hlt">earthquakes</span>? We demonstrate that the remarkable, previously neglected mechanism of heat transfer through transient granular vortices may be at the core of this. We present and analyze results from perpetual simple shear experiments on a <span class="hlt">system</span> of granular disks with which we are able to quantify the sizes and lifetimes of granular vortices within <span class="hlt">fault</span> gouges during <span class="hlt">earthquakes</span>. We then develop a formula that captures the contribution these vortices have on heat transfer. Using this formula, we show that crustal <span class="hlt">faults</span> such as those in the San Andreas <span class="hlt">system</span> may experience a maximum temperature rise 5 to 10 times lower than previously thought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T21A2519Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T21A2519Z"><span>Active <span class="hlt">fault</span> <span class="hlt">systems</span> of the Kivu rift and Virunga volcanic province, and implications for geohazards</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zal, H. J.; Ebinger, C. J.; Wood, D. J.; Scholz, C. A.; d'Oreye, N.; Carn, S. A.; Rutagarama, U.</p> <p>2013-12-01</p> <p>H Zal, C Ebinger, D. Wood, C. Scholz, N. d'Oreye, S. Carn, U. Rutagarama The weakly magmatic Western rift <span class="hlt">system</span>, East Africa, is marked by <span class="hlt">fault</span>-bounded basins filled by freshwater lakes that record tectonic and climatic signals. One of the smallest of the African Great Lakes, Lake Kivu, represents a unique geohazard owing to the warm, saline bottom waters that are saturated in methane, as well as two of the most active volcanoes in Africa that effectively dam the northern end of the lake. Yet, the dynamics of the basin <span class="hlt">system</span> and the role of magmatism were only loosely constrained prior to new field and laboratory studies in Rwanda. In this work, we curated, merged, and analyzed historical and digital data sets, including spectral analyses of merged Shuttle Radar Topography Mission topography and high resolution CHIRP bathymetry calibrated by previously mapped <span class="hlt">fault</span> locations along the margins and beneath the lake. We quantitatively compare these <span class="hlt">fault</span> maps with the time-space distribution of <span class="hlt">earthquakes</span> located using data from a temporary array along the northern sector of Lake Kivu, as well as space-based geodetic data. During 2012, seismicity rates were highest beneath Nyiragongo volcano, where a range of low frequency (1-3 s peak frequency) to tectonic <span class="hlt">earthquakes</span> were located. Swarms of low-frequency <span class="hlt">earthquakes</span> correspond to periods of elevated gas emissions, as detected by Ozone Monitoring Instrument (OMI). <span class="hlt">Earthquake</span> swarms also occur beneath Karisimbi and Nyamuragira volcanoes. A migrating swarm of <span class="hlt">earthquakes</span> in May 2012 suggests a sill intrusion at the DR Congo-Rwanda border. We delineate two <span class="hlt">fault</span> sets: SW-NE, and sub-N-S. Excluding the volcano-tectonic <span class="hlt">earthquakes</span>, most of the <span class="hlt">earthquakes</span> are located along subsurface projections of steep border <span class="hlt">faults</span>, and intrabasinal <span class="hlt">faults</span> calibrated by seismic reflection data. Small magnitude <span class="hlt">earthquakes</span> also occur beneath the uplifted rift flanks. Time-space variations in seismicity patterns provide a baseline</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.S21B1721Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.S21B1721Z"><span>Strain-dependent Damage Evolution and Velocity Reduction in <span class="hlt">Fault</span> Zones Induced by <span class="hlt">Earthquake</span> Rupture</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhong, J.; Duan, B.</p> <p>2009-12-01</p> <p>Low-velocity <span class="hlt">fault</span> zones (LVFZs) with reduced seismic velocities relative to the surrounding wall rocks are widely observed around active <span class="hlt">faults</span>. The presence of such a zone will affect rupture propagation, near-field ground motion, and off-<span class="hlt">fault</span> damage in subsequent <span class="hlt">earth-quakes</span>. In this study, we quantify the reduction of seismic velocities caused by dynamic rup-ture on a 2D planar <span class="hlt">fault</span> surrounded by a low-velocity <span class="hlt">fault</span> zone. First, we implement the damage rheology (Lyakhovsky et al. 1997) in EQdyna (Duan and Oglesby 2006), an explicit dynamic finite element code. We further extend this damage rheology model to include the dependence of strains on crack density. Then, we quantify off-<span class="hlt">fault</span> continuum damage distribution and velocity reduction induced by <span class="hlt">earthquake</span> rupture with the presence of a preexisting LVFZ. We find that the presence of a LVFZ affects the tempo-spatial distribu-tions of off-<span class="hlt">fault</span> damage. Because lack of constraint in some damage parameters, we further investigate the relationship between velocity reduction and these damage prameters by a large suite of numerical simulations. Slip velocity, slip, and near-field ground motions computed from damage rheology are also compared with those from off-<span class="hlt">fault</span> elastic or elastoplastic responses. We find that the reduction in elastic moduli during dynamic rupture has profound impact on these quantities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.S44B..04K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.S44B..04K"><span>Geological process of the slow <span class="hlt">earthquakes</span> -A hypothesis from an ancient plate boundary <span class="hlt">fault</span> rock</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kitamura, Y.; Kimura, G.; Kawabata, K.</p> <p>2012-12-01</p> <p>We present an integrated model of the deformation along the subduction plate boundary from the trench to the seismogenic zone. Over years of field based research in the Shimanto Belt accretionary complex, southwest Japan, yielded breaking-through discoveries on plate boundary processes, for example, the first finding of pseudotachylyte in the accretionary prism (Ikesawa et al., 2003). Our aim here is to unveil the geological aspects of slow <span class="hlt">earthquakes</span> and the related plate boundary processes. Studied tectonic mélanges in the Shimanto Belt are regarded as fossils of plate boundary <span class="hlt">fault</span> zone in subduction zone. We traced material from different depths along subduction channel using samples from on-land outcrops and ocean drilling cores. As a result, a series of progressive deformation down to the down-dip limit of the seismogenic zone was revealed. Detailed geological survey and structural analyses enabled us to separate superimposed deformation events during subduction. Material involved in the plate boundary deformation is mainly an alternation of sand and mud. As they have different competency and are suffered by simple shear stress field, sandstones break apart in flowing mudstones. We distinguished several stages of these deformations in sandstones and recognized progress in the intensity of deformation with increment of underthrusting. It is also known that the studied Mugi mélange bears pseudotachylyte in its upper bounding <span class="hlt">fault</span>. Our conclusion illustrates that the subduction channel around the depth of the seismogenic zone forms a thick plate boundary <span class="hlt">fault</span> zone, where there is a clear segregation in deformation style: a fast and episodic slip at the upper boundary <span class="hlt">fault</span> and a slow and continuous deformation within the zone. The former fast deformation corresponds to the plate boundary <span class="hlt">earthquakes</span> and the latter to the slow <span class="hlt">earthquakes</span>. We further examined numerically whether this plate boundary <span class="hlt">fault</span> rock is capable of releasing seismic moment enough to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024275','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024275"><span>Evidence for large <span class="hlt">earthquakes</span> on the San Andreas <span class="hlt">fault</span> at the Wrightwood, California paleoseismic site: A.D. 500 to present</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fumal, T.E.; Weldon, R.J.; Biasi, G.P.; Dawson, T.E.; Seitz, G.G.; Frost, W.T.; Schwartz, D.P.</p> <p>2002-01-01</p> <p>We present structural and stratigraphic evidence from a paleoseismic site near Wrightwood, California, for 14 large <span class="hlt">earthquakes</span> that occurred on the southern San Andreas <span class="hlt">fault</span> during the past 1500 years. In a network of 38 trenches and creek-bank exposures, we have exposed a composite section of interbedded debris flow deposits and thin peat layers more than 24 m thick; fluvial deposits occur along the northern margin of the site. The site is a 150-m-wide zone of deformation bounded on the surface by a main <span class="hlt">fault</span> zone along the northwest margin and a secondary <span class="hlt">fault</span> zone to the southwest. Evidence for most of the 14 <span class="hlt">earthquakes</span> occurs along structures within both zones. We identify paleoearthquake horizons using infilled fissures, scarps, multiple rupture terminations, and widespread folding and tilting of beds. Ages of stratigraphic units and <span class="hlt">earthquakes</span> are constrained by historic data and 72 14C ages, mostly from samples of peat and some from plant fibers, wood, pine cones, and charcoal. Comparison of the long, well-resolved paleoseimic record at Wrightwood with records at other sites along the <span class="hlt">fault</span> indicates that rupture lengths of past <span class="hlt">earthquakes</span> were at least 100 km long. Paleoseismic records at sites in the Coachella Valley suggest that each of the past five large <span class="hlt">earthquakes</span> recorded there ruptured the <span class="hlt">fault</span> at least as far northwest as Wrightwood. Comparisons with event chronologies at Pallett Creek and sites to the northwest suggests that approximately the same part of the <span class="hlt">fault</span> that ruptured in 1857 may also have failed in the early to mid-sixteenth century and several other times during the past 1200 years. Records at Pallett Creek and Pitman Canyon suggest that, in addition to the 14 <span class="hlt">earthquakes</span> we document, one and possibly two other large <span class="hlt">earthquakes</span> ruptured the part of the <span class="hlt">fault</span> including Wrightwood since about A.D. 500. These observations and elapsed times that are significantly longer than mean recurrence intervals at Wrightwood and sites to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70193570','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70193570"><span><span class="hlt">Faulting</span> within the Mount St. Helens conduit and implications for volcanic <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pallister, John S.; Cashman, Katharine V.; Hagstrum, Jonathan T.; Beeler, Nicholas M.; Moran, Seth C.; Denlinger, Roger P.</p> <p>2013-01-01</p> <p>The 2004–2008 eruption of Mount St. Helens produced seven dacite spines mantled by cataclastic <span class="hlt">fault</span> rocks, comprising an outer <span class="hlt">fault</span> core and an inner damage zone. These <span class="hlt">fault</span> rocks provide remarkable insights into the mechanical processes that accompany extrusion of degassed magma, insights that are useful in forecasting dome-forming eruptions. The outermost part of the <span class="hlt">fault</span> core consists of finely comminuted <span class="hlt">fault</span> gouge that is host to 1- to 3-mm-thick layers of extremely fine-grained slickenside-bearing ultracataclasite. Interior to the <span class="hlt">fault</span> core, there is an ∼2-m-thick damage zone composed of cataclastic breccia and sheared dacite, and interior to the damage zone, there is massive to flow-banded dacite lava of the spine interior. Structures and microtextures indicate entirely brittle deformation, including rock breakage, tensional dilation, shearing, grain flow, and microfaulting, as well as gas and fluid migration through intergranular pores and fractures in the damage zone. Slickenside lineations and consistent orientations of Riedel shears indicate upward shear of the extruding spines against adjacent conduit wall rocks.Paleomagnetic directions, demagnetization paths, oxide mineralogy, and petrology indicate that cataclasis took place within dacite in a solidified steeply dipping volcanic conduit at temperatures above 500 °C. Low water content of matrix glass is consistent with brittle behavior at these relatively high temperatures, and the presence of tridymite indicates solidification depths of <1 km. Cataclasis was coincident with the eruption’s seismogenic zone at <1.5 km.More than a million small and low-frequency “drumbeat” <span class="hlt">earthquakes</span> with coda magnitudes (Md) <2.0 and frequencies <5 Hz occurred during the 2004–2008 eruption. Our field data provide a means with which to estimate slip-patch dimensions for shear planes and to compare these with estimates of slip patches based on seismic moments and shear moduli for dacite rock and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018498','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018498"><span>1957 Gobi-Altay, Mongolia, <span class="hlt">earthquake</span> as a prototype for southern California's most devastating <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bayarsayhan, C.; Bayasgalan, A.; Enhtuvshin, B.; Hudnut, K.W.; Kurushin, R.A.; Molnar, P.; Olziybat, M.</p> <p>1996-01-01</p> <p>The 1957 Gobi-Altay <span class="hlt">earthquake</span> was associated with both strike-slip and thrust <span class="hlt">faulting</span>, processes similar to those along the San Andreas <span class="hlt">fault</span> and the <span class="hlt">faults</span> bounding the San Gabriel Mountains just north of Los Angeles, California. Clearly, a major rupture either on the San Andreas <span class="hlt">fault</span> north of Los Angeles or on the thrust <span class="hlt">faults</span> bounding the Los Angeles basin poses a serious hazard to inhabitants of that area. By analogy with the Gobi-Altay <span class="hlt">earthquake</span>, we suggest that simultaneous rupturing of both the San Andreas <span class="hlt">fault</span> and the thrust <span class="hlt">faults</span> nearer Los Angeles is a real possibility that amplifies the hazard posed by ruptures on either <span class="hlt">fault</span> <span class="hlt">system</span> separately.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034198','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034198"><span>Stress transfer among en echelon and opposing thrusts and tear <span class="hlt">faults</span>: Triggering caused by the 2003 Mw = 6.9 Zemmouri, Algeria, <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lin, J.; Stein, R.S.; Meghraoui, M.; Toda, S.; Ayadi, A.; Dorbath, C.; Belabbes, S.</p> <p>2011-01-01</p> <p>The essential features of stress interaction among <span class="hlt">earthquakes</span> on en echelon thrusts and tear <span class="hlt">faults</span> were investigated, first through idealized examples and then by study of thrust <span class="hlt">faulting</span> in Algeria. We calculated coseismic stress changes caused by the 2003 Mw = 6.9 Zemmouri <span class="hlt">earthquake</span>, finding that a large majority of the Zemmouri afterslip sites were brought several bars closer to Coulomb failure by the coseismic stresses, while the majority of aftershock nodal planes were brought closer to failure by an average of ~2 bars. Further, we calculated that the shallow portions of the adjacent Thenia tear <span class="hlt">fault</span>, which sustained ~0.25 m slip, were brought >2 bars closer to failure. We calculated that the Coulomb stress increased by 1.5 bars on the deeper portions of the adjacent Boumerdes thrust, which lies just 10–20 km from the city of Algiers; both the Boumerdes and Thenia <span class="hlt">faults</span> were illuminated by aftershocks. Over the next 6 years, the entire south dipping thrust <span class="hlt">system</span> extending 80 km to the southwest experienced an increased rate of seismicity. The stress also increased by 0.4 bar on the east Sahel thrust <span class="hlt">fault</span> west of the Zemmouri rupture. Algiers suffered large damaging <span class="hlt">earthquakes</span> in A.D. 1365 and 1716 and is today home to 3 million people. If these shocks occurred on the east Sahel <span class="hlt">fault</span> and if it has a ~2 mm/yr tectonic loading rate, then enough loading has accumulated to produce a Mw = 6.6–6.9 shock today. Thus, these potentially lethal <span class="hlt">faults</span> need better understanding of their slip rate and <span class="hlt">earthquake</span> history.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026246','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026246"><span>Remotely triggered seismicity on the United States west coast following the Mw 7.9 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prejean, S.G.; Hill, D.P.; Brodsky, E.E.; Hough, S.E.; Johnston, M.J.S.; Malone, S.D.; Oppenheimer, D.H.; Pitt, A.M.; Richards-Dinger, K. B.</p> <p>2004-01-01</p> <p>The Mw 7.9 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span> in central Alaska of 3 November 2002 triggered <span class="hlt">earthquakes</span> across western North America at epicentral distances of up to at least 3660 km. We describe the spatial and temporal development of triggered activity in California and the Pacific Northwest, focusing on Mount Rainier, the Geysers geothermal field, the Long Valley caldera, and the Coso geothermal field.The onset of triggered seismicity at each of these areas began during the Love and Raleigh waves of the Mw 7.9 wave train, which had dominant periods of 15 to 40 sec, indicating that <span class="hlt">earthquakes</span> were triggered locally by dynamic stress changes due to low-frequency surface wave arrivals. Swarms during the wave train continued for ∼4 min (Mount Rainier) to ∼40 min (the Geysers) after the surface wave arrivals and were characterized by spasmodic bursts of small (M ≤ 2.5) <span class="hlt">earthquakes</span>. Dynamic stresses within the surface wave train at the time of the first triggered <span class="hlt">earthquakes</span> ranged from 0.01 MPa (Coso) to 0.09 MPa (Mount Rainier). In addition to the swarms that began during the surface wave arrivals, Long Valley caldera and Mount Rainier experienced unusually large seismic swarms hours to days after the Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span>. These swarms seem to represent a delayed response to the Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span>. The occurrence of spatially and temporally distinct swarms of triggered seismicity at the same site suggests that <span class="hlt">earthquakes</span> may be triggered by more than one physical process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....12497R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....12497R"><span>The 7.9 Denali <span class="hlt">Fault</span>, Alaska <span class="hlt">Earthquake</span> of November 3, 2002: Aftershock Locations, Moment Tensors and Focal Mechanisms from the Regional Seismic Network Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ratchkovski, N. A.; Hansen, R. A.; Kore, K. R.</p> <p>2003-04-01</p> <p>The largest <span class="hlt">earthquake</span> ever recorded on the Denali <span class="hlt">fault</span> <span class="hlt">system</span> (magnitude 7.9) struck central Alaska on November 3, 2002. It was preceded by a magnitude 6.7 <span class="hlt">earthquake</span> on October 23. This earlier <span class="hlt">earthquake</span> and its zone of aftershocks were located ~20 km to the west of the 7.9 quake. Aftershock locations and surface slip observations from the 7.9 quake indicate that the rupture was predominately unilateral in the eastward direction. The geologists mapped a ~300-km-long rupture and measured maximum offsets of 8.8 meters. The 7.9 event ruptured three different <span class="hlt">faults</span>. The rupture began on the northeast trending Susitna Glacier Thrust <span class="hlt">fault</span>, a splay <span class="hlt">fault</span> south of the Denali <span class="hlt">fault</span>. Then the rupture transferred to the Denali <span class="hlt">fault</span> and propagated eastward for 220 km. At about 143W the rupture moved onto the adjacent southeast-trending Totschunda <span class="hlt">fault</span> and propagated for another 55 km. The cumulative length of the 6.7 and 7.9 aftershock zones along the Denali and Totschunda <span class="hlt">faults</span> is about 380 km. The <span class="hlt">earthquakes</span> were recorded and processed by the Alaska <span class="hlt">Earthquake</span> Information Center (AEIC). The AEIC acquires and processes data from the Alaska Seismic Network, consisting of over 350 seismograph stations. Nearly 40 of these sites are equipped with the broad-band sensors, some of which also have strong motion sensors. The rest of the stations are either 1 or 3-component short-period instruments. The data from these stations are collected, processed and archived at the AEIC. The AEIC staff installed a temporary seismic network of 6 instruments following the 6.7 <span class="hlt">earthquake</span> and an additional 20 stations following the 7.9 <span class="hlt">earthquake</span>. Prior to the 7.9 Denali <span class="hlt">Fault</span> event, the AEIC was locating 35 to 50 events per day. After the event, the processing load increased to over 300 events per day during the first week following the event. In this presentation, we will present and interpret the aftershock location patterns, first motion focal mechanism solutions, and regional seismic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70192478','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70192478"><span>Periodic, chaotic, and doubled <span class="hlt">earthquake</span> recurrence intervals on the deep San Andreas <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shelly, David R.</p> <p>2010-01-01</p> <p><span class="hlt">Earthquake</span> recurrence histories may provide clues to the timing of future events, but long intervals between large events obscure full recurrence variability. In contrast, small <span class="hlt">earthquakes</span> occur frequently, and recurrence intervals are quantifiable on a much shorter time scale. In this work, I examine an 8.5-year sequence of more than 900 recurring low-frequency <span class="hlt">earthquake</span> bursts composing tremor beneath the San Andreas <span class="hlt">fault</span> near Parkfield, California. These events exhibit tightly clustered recurrence intervals that, at times, oscillate between ~3 and ~6 days, but the patterns sometimes change abruptly. Although the environments of large and low-frequency <span class="hlt">earthquakes</span> are different, these observations suggest that similar complexity might underlie sequences of large <span class="hlt">earthquakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.S33A2518T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.S33A2518T"><span>Dynamic Simulations for the Seismic Behavior on the Shallow Part of the <span class="hlt">Fault</span> Plane in the Subduction Zone during Mega-Thrust <span class="hlt">Earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsuda, K.; Dorjapalam, S.; Dan, K.; Ogawa, S.; Watanabe, T.; Uratani, H.; Iwase, S.</p> <p>2012-12-01</p> <p>The 2011 Tohoku-Oki <span class="hlt">earthquake</span> (M9.0) produced some distinct features such as huge slips on the order of several ten meters around the shallow part of the <span class="hlt">fault</span> and different areas with radiating seismic waves for different periods (e.g., Lay et al., 2012). These features, also reported during the past mega-thrust <span class="hlt">earthquakes</span> in the subduction zone such as the 2004 Sumatra <span class="hlt">earthquake</span> (M9.2) and the 2010 Chile <span class="hlt">earthquake</span> (M8.8), get attentions as the distinct features if the rupture of the mega-thrust <span class="hlt">earthquakes</span> reaches to the shallow part of the <span class="hlt">fault</span> plane. Although various kinds of observations for the seismic behavior (rupture process and ground motion characteristics etc.) on the shallow part of the <span class="hlt">fault</span> plane during the mega-trust <span class="hlt">earthquakes</span> have been reported, the number of analytical or numerical studies based on dynamic simulation is still limited. Wendt et al. (2009), for example, revealed that the different distribution of initial stress produces huge differences in terms of the seismic behavior and vertical displacements on the surface. In this study, we carried out the dynamic simulations in order to get a better understanding about the seismic behavior on the shallow part of the <span class="hlt">fault</span> plane during mega-thrust <span class="hlt">earthquakes</span>. We used the spectral element method (Ampuero, 2009) that is able to incorporate the complex <span class="hlt">fault</span> geometry into simulation as well as to save computational resources. The simulation utilizes the slip-weakening law (Ida, 1972). In order to get a better understanding about the seismic behavior on the shallow part of the <span class="hlt">fault</span> plane, some parameters controlling seismic behavior for dynamic <span class="hlt">faulting</span> such as critical slip distance (Dc), initial stress conditions and friction coefficients were changed and we also put the asperity on the <span class="hlt">fault</span> plane. These understandings are useful for the ground motion prediction for future mega-thrust <span class="hlt">earthquakes</span> such as the <span class="hlt">earthquakes</span> along the Nankai Trough.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMMR31B..07L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMMR31B..07L"><span>Structure, Frictional Melting and <span class="hlt">Fault</span> Weakening during the 2008 Mw 7.9 Wenchuan <span class="hlt">Earthquake</span> Slip: Observation from the WFSD Drilling Core Samples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, H.; Wang, H.; Li, C.; Zhang, J.; Sun, Z.; Si, J.; Liu, D.; Chevalier, M. L.; Han, L.; Yun, K.; Zheng, Y.</p> <p>2015-12-01</p> <p>The 2008 Mw7.9 Wenchuan <span class="hlt">earthquake</span> produced two co-seismic surface ruptures along Yingxiu-Beichuan <span class="hlt">fault</span> (~270 km) and the Guanxian-Anxian <span class="hlt">fault</span> (~80 km) simultaneously in the Longmen Shan thrust belt. Besides, two surface rupture zones were tracked in the southern segment of the Yingxiu-Beichuan rupture zone, one along the Yingxiu <span class="hlt">fault</span>, the other along the Shenxigou-Longchi <span class="hlt">fault</span>, which both converged into one rupture zone at the Bajiaomiao village, Hongkou town, where one distinct <span class="hlt">fault</span> plane with two striation orientations was exposed. The Wenchuan <span class="hlt">earthquake</span> <span class="hlt">Fault</span> Scientific Drilling project (WFSD) was carried out right after the <span class="hlt">earthquake</span> to investigate its <span class="hlt">faulting</span> mechanisms and rupture process. Six boreholes were drilled along the rupture zones with depths ranging from 600 to 2400 m. WFSD-1 and WFSD-2 are located at the Bajiaomiao area, the southern segment of the Yingxiu-Beichuan rupture zone, while WFSD-4 and WFSD-4S are in the Nanba town area, in the northern part of the rupture zone. Detailed research showed that ~1 mm thick Principal Slip Zone (PSZ) of the Wenchuan <span class="hlt">earthquake</span> is located at ~589 m-depth in the WFSD-1 cores. Graphite present in the PSZ indicates a low <span class="hlt">fault</span> strength. Long-term temperature monitoring shows an extremely low <span class="hlt">fault</span> friction coefficient during the <span class="hlt">earthquake</span>. Recently, another possible PSZ was found in WFSD-1 cores at ~732 m-depth, with a ~2 mm thick melt layer in the <span class="hlt">fault</span> gouge, where feldspar was melted but quartz was not, indicating that the frictional melting temperature was 1230°C < T < 1720°C. These two PSZs at depth may correspond to the two co-seismic surface rupture zones. Besides, the Wenchuan <span class="hlt">earthquake</span> PSZ was also recognized in the WFSD-4S cores, at ~1084 m-depth. About 200-400 μm thick melt layer (<span class="hlt">fault</span> vein, mainly feldspar), as well as melt injection veins, were observed in the slip zone, where oblique distinct striations were visible on the slip surface. Therefore, there are two PSZs in the shallow</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910315W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910315W"><span>Controls on the long term <span class="hlt">earthquake</span> behavior of an intraplate <span class="hlt">fault</span> revealed by U-Th and stable isotope analyses of syntectonic calcite veins</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, Randolph; Goodwin, Laurel; Sharp, Warren; Mozley, Peter</p> <p>2017-04-01</p> <p>U-Th dates on calcite precipitated in coseismic extension fractures in the Loma Blanca normal <span class="hlt">fault</span> zone, Rio Grande rift, NM, USA, constrain <span class="hlt">earthquake</span> recurrence intervals from 150-565 ka. This is the longest direct record of seismicity documented for a <span class="hlt">fault</span> in any tectonic environment. Combined U-Th and stable isotope analyses of these calcite veins define 13 distinct <span class="hlt">earthquake</span> events. These data show that for more than 400 ka the Loma Blanca <span class="hlt">fault</span> produced <span class="hlt">earthquakes</span> with a mean recurrence interval of 40 ± 7 ka. The coefficient of variation for these events is 0.40, indicating strongly periodic seismicity consistent with a time-dependent model of <span class="hlt">earthquake</span> recurrence. Stochastic statistical analyses further validate the inference that <span class="hlt">earthquake</span> behavior on the Loma Blanca was time-dependent. The time-dependent nature of these <span class="hlt">earthquakes</span> suggests that the seismic cycle was fundamentally controlled by a stress renewal process. However, this periodic cycle was punctuated by an episode of clustered seismicity at 430 ka. Recurrence intervals within the <span class="hlt">earthquake</span> cluster were as low as 5-11 ka. Breccia veins formed during this episode exhibit carbon isotope signatures consistent with having formed through pronounced degassing of a CO2 charged brine during post-failure, <span class="hlt">fault</span>-localized fluid migration. The 40 ka periodicity of the long-term <span class="hlt">earthquake</span> record of the Loma Blanca <span class="hlt">fault</span> is similar in magnitude to recurrence intervals documented through paleoseismic studies of other normal <span class="hlt">faults</span> in the Rio Grande rift and Basin and Range Province. We propose that it represents a background rate of failure in intraplate extension. The short-term, clustered seismicity that occurred on the <span class="hlt">fault</span> records an interruption of the stress renewal process, likely by elevated fluid pressure in deeper structural levels of the <span class="hlt">fault</span>, consistent with <span class="hlt">fault</span>-valve behavior. The relationship between recurrence interval and inferred fluid degassing suggests that pore fluid pressure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.bssaonline.org/content/84/3/892.abstract','USGSPUBS'); return false;" href="http://www.bssaonline.org/content/84/3/892.abstract"><span>Foreshocks, aftershocks, and <span class="hlt">earthquake</span> probabilities: Accounting for the landers <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jones, Lucile M.</p> <p>1994-01-01</p> <p>The equation to determine the probability that an <span class="hlt">earthquake</span> occurring near a major <span class="hlt">fault</span> will be a foreshock to a mainshock on that <span class="hlt">fault</span> is modified to include the case of aftershocks to a previous <span class="hlt">earthquake</span> occurring near the <span class="hlt">fault</span>. The addition of aftershocks to the background seismicity makes its less probable that an <span class="hlt">earthquake</span> will be a foreshock, because nonforeshocks have become more common. As the aftershocks decay with time, the probability that an <span class="hlt">earthquake</span> will be a foreshock increases. However, <span class="hlt">fault</span> interactions between the first mainshock and the major <span class="hlt">fault</span> can increase the long-term probability of a characteristic <span class="hlt">earthquake</span> on that <span class="hlt">fault</span>, which will, in turn, increase the probability that an event is a foreshock, compensating for the decrease caused by the aftershocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S11B2329N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S11B2329N"><span><span class="hlt">Faulting</span> type classification of small <span class="hlt">earthquakes</span> using a template approach and their hypocenter relocation along the Japan and Kuril trenches</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nakamura, W.; Uchida, N.; Matsuzawa, T.</p> <p>2013-12-01</p> <p>After the 2011 Tohoku-oki <span class="hlt">earthquake</span>, the number of interplate <span class="hlt">earthquakes</span> off Miyagi was dramatically decreased (e.g., Asano et al., 2011), while many normal <span class="hlt">faulting</span> <span class="hlt">earthquakes</span> occurred in the outer trench region (e.g., Obana et al., 2012). To understand the meaning of the seismicity change caused by the huge <span class="hlt">earthquake</span>, it is essential to know <span class="hlt">faulting</span> types of small offshore <span class="hlt">earthquakes</span> which cannot be determined using conventional methods. In this study, we developed a method to classify focal mechanisms of small <span class="hlt">earthquakes</span> by using template events whose focal mechanisms were known. Here, we made pairs of <span class="hlt">earthquakes</span> with inter-event distances of less than 20 km and difference in magnitude of less than 1.0, and calculated their waveform cross-correlation coefficients (CCs) in 1.5 and 5.0 sec windows for P and S waves, respectively. We first calculated 3D minimum rotation angle (Kagan's angle; Kagan, 1991) for pairs whose focal mechanisms were listed in the F-net catalogue, to examine the relationships among the Kagan's angles, CCs and inter-event distances. The CCs decrease with increasing inter-event distances and Kagan's angles. We set a CC threshold of 0.8 for Tohoku (to the south of 40° N), and 0.7 for Hokkaido (to the north of 40° N) regions to judge whether the two events have the same focal mechanisms. This is because more than 90% of event pairs whose CCs are greater than the thresholds show Kagan's angles of less than 30° when we calculated them for the mechanism-known <span class="hlt">earthquakes</span> (templates). In total, 4012 <span class="hlt">earthquakes</span> from 2003 to 2012 are newly classified and 60% and 30% of them are of interplate and normal <span class="hlt">faulting</span> types, respectively. In the area of large coseismic slip of the 2011 Tohoku-oki <span class="hlt">earthquake</span>, we found no interplate <span class="hlt">earthquakes</span> after the main shock, while many interplate <span class="hlt">earthquakes</span> occurred around the M9 coseismic slip area. We also found many normal <span class="hlt">faulting</span> <span class="hlt">earthquakes</span> near the trench after the 2011 main shock. Along the Kuril</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020193','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020193"><span>Non-double-couple <span class="hlt">earthquakes</span>. 1. Theory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Julian, B.R.; Miller, A.D.; Foulger, G.R.</p> <p>1998-01-01</p> <p>Historically, most quantitative seismological analyses have been based on the assumption that <span class="hlt">earthquakes</span> are caused by shear <span class="hlt">faulting</span>, for which the equivalent force <span class="hlt">system</span> in an isotropic medium is a pair of force couples with no net torque (a 'double couple,' or DC). Observations of increasing quality and coverage, however, now resolve departures from the DC model for many <span class="hlt">earthquakes</span> and find some <span class="hlt">earthquakes</span>, especially in volcanic and geothermal areas, that have strongly non-DC mechanisms. Understanding non-DC <span class="hlt">earthquakes</span> is important both for studying the process of <span class="hlt">faulting</span> in detail and for identifying nonshear-<span class="hlt">faulting</span> processes that apparently occur in some <span class="hlt">earthquakes</span>. This paper summarizes the theory of 'moment tensor' expansions of equivalent-force <span class="hlt">systems</span> and analyzes many possible physical non-DC <span class="hlt">earthquake</span> processes. Contrary to long-standing assumption, sources within the Earth can sometimes have net force and torque components, described by first-rank and asymmetric second-rank moment tensors, which must be included in analyses of landslides and some volcanic phenomena. Non-DC processes that lead to conventional (symmetric second-rank) moment tensors include geometrically complex shear <span class="hlt">faulting</span>, tensile <span class="hlt">faulting</span>, shear <span class="hlt">faulting</span> in an anisotropic medium, shear <span class="hlt">faulting</span> in a heterogeneous region (e.g., near an interface), and polymorphic phase transformations. Undoubtedly, many non-DC <span class="hlt">earthquake</span> processes remain to be discovered. Progress will be facilitated by experimental studies that use wave amplitudes, amplitude ratios, and complete waveforms in addition to wave polarities and thus avoid arbitrary assumptions such as the absence of volume changes or the temporal similarity of different moment tensor components.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S33E..04W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S33E..04W"><span>Stress drop variation of M > 4 <span class="hlt">earthquakes</span> on the Blanco oceanic transform <span class="hlt">fault</span> using a phase coherence method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, J. R.; Hawthorne, J.; Rost, S.; Wright, T. J.</p> <p>2017-12-01</p> <p><span class="hlt">Earthquakes</span> on oceanic transform <span class="hlt">faults</span> often show unusual behaviour. They tend to occur in swarms, have large numbers of foreshocks, and have high stress drops. We estimate stress drops for approximately 60 M > 4 <span class="hlt">earthquakes</span> along the Blanco oceanic transform <span class="hlt">fault</span>, a right-lateral <span class="hlt">fault</span> separating the Juan de Fuca and Pacific plates offshore of Oregon. We find stress drops with a median of 4.4±19.3MPa and examine how they vary with <span class="hlt">earthquake</span> moment. We calculate stress drops using a recently developed method based on inter-station phase coherence. We compare seismic records of co-located <span class="hlt">earthquakes</span> at a range of stations. At each station, we apply an empirical Green's function (eGf) approach to remove phase path effects and isolate the relative apparent source time functions. The apparent source time functions at each <span class="hlt">earthquake</span> should vary among stations at periods shorter than a P wave's travel time across the <span class="hlt">earthquake</span> rupture area. Therefore we compute the rupture length of the larger <span class="hlt">earthquake</span> by identifying the frequency at which the relative apparent source time functions start to vary among stations, leading to low inter-station phase coherence. We determine a stress drop from the rupture length and moment of the larger <span class="hlt">earthquake</span>. Our initial stress drop estimates increase with increasing moment, suggesting that <span class="hlt">earthquakes</span> on the Blanco <span class="hlt">fault</span> are not self-similar. However, these stress drops may be biased by several factors, including depth phases, trace alignment, and source co-location. We find that the inclusion of depth phases (such as pP) in the analysis time window has a negligible effect on the phase coherence of our relative apparent source time functions. We find that trace alignment must be accurate to within 0.05 s to allow us to identify variations in the apparent source time functions at periods relevant for M > 4 <span class="hlt">earthquakes</span>. We check that the alignments are accurate enough by comparing P wave arrival times across groups of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T31G..06V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T31G..06V"><span><span class="hlt">Fault</span> Weakening due to Erosion by Fluids: A Possible Origin of Intraplate <span class="hlt">Earthquake</span> Swarms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vavrycuk, V.; Hrubcova, P.</p> <p>2016-12-01</p> <p>The occurrence and specific properties of <span class="hlt">earthquake</span> swarms in geothermal areas are usually attributed to a highly fractured rock and/or heterogeneous stress within the rock mass being triggered by magmatic or hydrothermal fluid intrusion. The increase of fluid pressure destabilizes fractures and causes their opening and subsequent shear-tensile rupture. The spreading and evolution of the seismic activity is controlled by fluid flow due to diffusion in a permeable rock and/or by the redistribution of Coulomb stress. The `fluid-injection model', however, is not valid universally. We provide evidence that this model is inconsistent with observations of <span class="hlt">earthquake</span> swarms in West Bohemia, Czech Republic. Full seismic moment tensors of micro-<span class="hlt">earthquakes</span> in the 1997 and 2008 swarms in West Bohemia indicate that fracturing at the starting phase of the swarm was not associated with <span class="hlt">fault</span> openings caused by pressurized fluids but rather with <span class="hlt">fault</span> compactions. This can physically be explained by a `fluid-erosion model', when the essential role in the swarm triggering is attributed to chemical and hydrothermal fluid-rock interactions in the focal zone. Since the rock is exposed to circulating hydrothermal, CO2-saturated fluids, the walls of fractures are weakened by dissolving and altering various minerals. If <span class="hlt">fault</span> strength lowers to a critical value, the seismicity is triggered. The fractures are compacted during failure, the <span class="hlt">fault</span> strength recovers and a new cycle begins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.S43A2031R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.S43A2031R"><span>The seismic velocity structure of a foreshock zone on an oceanic transform <span class="hlt">fault</span>: Imaging a rupture barrier to the 2008 Mw 6.0 <span class="hlt">earthquake</span> on the Gofar <span class="hlt">fault</span>, EPR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roland, E. C.; McGuire, J. J.; Lizarralde, D.; Collins, J. A.</p> <p>2010-12-01</p> <p>East Pacific Rise (EPR) oceanic transform <span class="hlt">faults</span> are known to exhibit a number of unique seismicity characteristics, including abundant seismic swarms, a prevalence of aseismic slip, and high rates of foreshock activity. Until recently the details of how this behavior fits into the seismic cycle of large events that occur periodically on transforms have remained poorly understood. In 2008 the most recent seismic cycle of the western segment (G3) of the Gofar <span class="hlt">fault</span> (4 degrees South on the EPR) ended with a Mw 6.0 <span class="hlt">earthquake</span>. Seismicity associated with this event was recorded by a local array of ocean bottom seismometers, and <span class="hlt">earthquake</span> locations reveal several distinct segments with unique slip behavior on the G3 <span class="hlt">fault</span>. Preceding the Mw 6.0 event, a significant foreshock sequence was recorded just to the east of the mainshock rupture zone that included more than 20,000 detected <span class="hlt">earthquakes</span>. This foreshock zone formed the eastern barrier to the mainshock rupture, and following the mainshock, seismicity rates within the foreshock zone remained unchanged. Based on aftershock locations of events following the 2007 Mw 6.0 event that completed the seismic cycle on the eastern end of the G3 <span class="hlt">fault</span>, it appears that the same foreshock zone may have served as the western rupture barrier for that prior <span class="hlt">earthquake</span>. Moreover, mainshock rupture associated with each of the last 8 large (~ Mw 6.0) events on the G3 <span class="hlt">fault</span> seems to terminate at the same foreshock zone. In order to elucidate some of the structural controls on <span class="hlt">fault</span> slip and <span class="hlt">earthquake</span> rupture along transform <span class="hlt">faults</span>, we present a seismic P-wave velocity profile crossing the center of the foreshock zone of the Gofar <span class="hlt">fault</span>, as well as a profile for comparison across the neighboring Quebrada <span class="hlt">fault</span>. Although tectonically similar, Quebrada does not sustain large <span class="hlt">earthquakes</span> and is thought to accommodate slip primarily aseismically and with small magnitude <span class="hlt">earthquake</span> swarms. Velocity profiles were obtained using data collected</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..122.2085S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..122.2085S"><span>Seismic constraints on the architecture of the Newport-Inglewood/Rose Canyon <span class="hlt">fault</span>: Implications for the length and magnitude of future <span class="hlt">earthquake</span> ruptures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sahakian, Valerie; Bormann, Jayne; Driscoll, Neal; Harding, Alistair; Kent, Graham; Wesnousky, Steve</p> <p>2017-03-01</p> <p>The Newport-Inglewood/Rose Canyon (NIRC) <span class="hlt">fault</span> zone is an active strike-slip <span class="hlt">fault</span> <span class="hlt">system</span> within the Pacific-North American plate boundary in Southern California, located in close proximity to populated regions of San Diego, Orange, and Los Angeles counties. Prior to this study, the NIRC <span class="hlt">fault</span> zone's continuity and geometry were not well constrained. Nested marine seismic reflection data with different vertical resolutions are employed to characterize the offshore <span class="hlt">fault</span> architecture. Four main <span class="hlt">fault</span> strands are identified offshore, separated by three main stepovers along strike, all of which are 2 km or less in width. Empirical studies of historical ruptures worldwide show that <span class="hlt">earthquakes</span> have ruptured through stepovers with this offset. Models of Coulomb stress change along the <span class="hlt">fault</span> zone are presented to examine the potential extent of future <span class="hlt">earthquake</span> ruptures on the <span class="hlt">fault</span> zone, which appear to be dependent on the location of rupture initiation and <span class="hlt">fault</span> geometry at the stepovers. These modeling results show that the southernmost stepover between the La Jolla and Torrey Pines <span class="hlt">fault</span> strands may act as an inhibitor to throughgoing rupture due to the stepover width and change in <span class="hlt">fault</span> geometry across the stepover; however, these results still suggest that rupture along the entire <span class="hlt">fault</span> zone is possible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T31D0646L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T31D0646L"><span>Crustal Seismicity and Geomorphic Observations of the Chiripa-Haciendas <span class="hlt">Fault</span> <span class="hlt">System</span>: The Guanacaste Volcanic Arc Sliver of Western Costa Rica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, J. C.; Montero Pohly, W. K.; Araya, M. C.</p> <p>2017-12-01</p> <p>It has recently been shown that contemporary northwest motion of the Nicoya Peninsula of Costa Rica reflects a tectonic sliver that includes much of the upper-plate arc, referred to as the Guanacaste Volcanic Arc Sliver (GVAS). Here we characterize historical seismicity and geomorphic expressions of <span class="hlt">faults</span> that define the northeastern margin of the GVAS. Several crustal <span class="hlt">earthquakes</span> and their aftershocks provide constraints on the geometry and/or kinematics of the <span class="hlt">fault</span> <span class="hlt">system</span>. These include the Armenia <span class="hlt">earthquake</span> of July 12, 2011, the Bijagua <span class="hlt">earthquake</span> of January 27, 2002, the Tilarán <span class="hlt">earthquake</span> of April 13, 1973 and two much older events. We summarize these <span class="hlt">earthquakes</span> in the context of recent <span class="hlt">fault</span> mapping and focal mechanism solutions, and suggest that most of the deformation can be explained by slip on steeply dipping NW-striking <span class="hlt">fault</span> planes accommodating dextral slip. Streams that cross the major <span class="hlt">fault</span> traces we have mapped also show deflections consistent with dextral slip. These include map-view apparent offsets of 6.5 km for the Haciendas River, 1.0 km for the Orosi River and 0.6 km for the Pizote River. Although preservation is poor, we document stream terrace risers that reveal truncations and/or offsets consistent with dextral slip. Additional constraints on the <span class="hlt">fault</span> <span class="hlt">system</span> are apparent as it is traced into Lake Nicaragua. Previous workers have shown that <span class="hlt">earthquake</span> clusters accommodate a combination of dextral slip on NW-strike <span class="hlt">faults</span> and sinistral slip NE-strike <span class="hlt">faults</span>, the latter described as part of a <span class="hlt">system</span> of bookshelf <span class="hlt">fault</span> blocks. Whether the northeastern margin of the GVAS under Lake Nicaragua is a single <span class="hlt">fault</span> strand or an array of bookshelf blocks remains an open question. An equally important gap in our understanding is the kinematic link of the <span class="hlt">fault</span> <span class="hlt">system</span> to the east where the GVAS originates. Our results set the stage for expanded studies that will be essential to understanding the relative contributions of Cocos Ridge collision and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/413/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/413/"><span>Data Files for Ground-Motion Simulations of the 1906 San Francisco <span class="hlt">Earthquake</span> and Scenario <span class="hlt">Earthquakes</span> on the Northern San Andreas <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Aagaard, Brad T.; Barall, Michael; Brocher, Thomas M.; Dolenc, David; Dreger, Douglas; Graves, Robert W.; Harmsen, Stephen; Hartzell, Stephen; Larsen, Shawn; McCandless, Kathleen; Nilsson, Stefan; Petersson, N. Anders; Rodgers, Arthur; Sjogreen, Bjorn; Zoback, Mary Lou</p> <p>2009-01-01</p> <p>This data set contains results from ground-motion simulations of the 1906 San Francisco <span class="hlt">earthquake</span>, seven hypothetical <span class="hlt">earthquakes</span> on the northern San Andreas <span class="hlt">Fault</span>, and the 1989 Loma Prieta <span class="hlt">earthquake</span>. The bulk of the data consists of synthetic velocity time-histories. Peak ground velocity on a 1/60th degree grid and geodetic displacements from the simulations are also included. Details of the ground-motion simulations and analysis of the results are discussed in Aagaard and others (2008a,b).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035685','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035685"><span>Possible deep <span class="hlt">fault</span> slip preceding the 2004 Parkfield <span class="hlt">earthquake</span>, inferred from detailed observations of tectonic tremor</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shelly, David R.</p> <p>2009-01-01</p> <p><span class="hlt">Earthquake</span> predictability depends, in part, on the degree to which sudden slip is preceded by slow aseismic slip. Recently, observations of deep tremor have enabled inferences of deep slow slip even when detection by other means is not possible, but these data are limited to certain areas and mostly the last decade. The region near Parkfield, California, provides a unique convergence of several years of high-quality tremor data bracketing a moderate <span class="hlt">earthquake</span>, the 2004 magnitude 6.0 event. Here, I present detailed observations of tectonic tremor from mid-2001 through 2008 that indicate deep <span class="hlt">fault</span> slip both before and after the Parkfield <span class="hlt">earthquake</span> that cannot be detected with surface geodetic instruments. While there is no obvious short-term precursor, I find unidirectional tremor migration accompanied by elevated tremor rates in the 3 months prior to the <span class="hlt">earthquake</span>, which suggests accelerated creep on the <span class="hlt">fault</span> ∼16 km beneath the eventual <span class="hlt">earthquake</span> hypocenter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70192291','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70192291"><span>A comparison among observations and <span class="hlt">earthquake</span> simulator results for the allcal2 California <span class="hlt">fault</span> model</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tullis, Terry. E.; Richards-Dinger, Keith B.; Barall, Michael; Dieterich, James H.; Field, Edward H.; Heien, Eric M.; Kellogg, Louise; Pollitz, Fred F.; Rundle, John B.; Sachs, Michael K.; Turcotte, Donald L.; Ward, Steven N.; Yikilmaz, M. Burak</p> <p>2012-01-01</p> <p>In order to understand <span class="hlt">earthquake</span> hazards we would ideally have a statistical description of <span class="hlt">earthquakes</span> for tens of thousands of years. Unfortunately the ∼100‐year instrumental, several 100‐year historical, and few 1000‐year paleoseismological records are woefully inadequate to provide a statistically significant record. Physics‐based <span class="hlt">earthquake</span> simulators can generate arbitrarily long histories of <span class="hlt">earthquakes</span>; thus they can provide a statistically meaningful history of simulated <span class="hlt">earthquakes</span>. The question is, how realistic are these simulated histories? This purpose of this paper is to begin to answer that question. We compare the results between different simulators and with information that is known from the limited instrumental, historic, and paleoseismological data.As expected, the results from all the simulators show that the observational record is too short to properly represent the <span class="hlt">system</span> behavior; therefore, although tests of the simulators against the limited observations are necessary, they are not a sufficient test of the simulators’ realism. The simulators appear to pass this necessary test. In addition, the physics‐based simulators show similar behavior even though there are large differences in the methodology. This suggests that they represent realistic behavior. Different assumptions concerning the constitutive properties of the <span class="hlt">faults</span> do result in enhanced capabilities of some simulators. However, it appears that the similar behavior of the different simulators may result from the fault‐<span class="hlt">system</span> geometry, slip rates, and assumed strength drops, along with the shared physics of stress transfer.This paper describes the results of running four <span class="hlt">earthquake</span> simulators that are described elsewhere in this issue of Seismological Research Letters. The simulators ALLCAL (Ward, 2012), VIRTCAL (Sachs et al., 2012), RSQSim (Richards‐Dinger and Dieterich, 2012), and ViscoSim (Pollitz, 2012) were run on our most recent all‐California <span class="hlt">fault</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511818O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511818O"><span>Microearthquake sequences along the Irpinia normal <span class="hlt">fault</span> <span class="hlt">system</span> in Southern Apennines, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Orefice, Antonella; Festa, Gaetano; Alfredo Stabile, Tony; Vassallo, Maurizio; Zollo, Aldo</p> <p>2013-04-01</p> <p>Microearthquakes reflect a continuous readjustment of tectonic structures, such as <span class="hlt">faults</span>, under the action of local and regional stress fields. Low magnitude seismicity in the vicinity of active <span class="hlt">fault</span> zones may reveal insights into the mechanics of the <span class="hlt">fault</span> <span class="hlt">systems</span> during the inter-seismic period and shine a light on the role of fluids and other physical parameters in promoting or disfavoring the nucleation of larger size events in the same area. Here we analyzed several <span class="hlt">earthquake</span> sequences concentrated in very limited regions along the 1980 Irpinia <span class="hlt">earthquake</span> <span class="hlt">fault</span> zone (Southern Italy), a complex <span class="hlt">system</span> characterized by normal stress regime, monitored by the dense, multi-component, high dynamic range seismic network ISNet (Irpinia Seismic Network). On a specific single sequence, the May 2008 Laviano swarm, we performed accurate absolute and relative locations and estimated source parameters and scaling laws that were compared with standard stress-drops computed for the area. Additionally, from EGF deconvolution, we computed a slip model for the mainshock and investigated the space-time evolution of the events in the sequence to reveal possible interactions among <span class="hlt">earthquakes</span>. Through the massive analysis of cross-correlation based on the master event scanning of the continuous recording, we also reconstructed the catalog of repeated <span class="hlt">earthquakes</span> and recognized several co-located sequences. For these events, we analyzed the statistical properties, location and source parameters and their space-time evolution with the aim of inferring the processes that control the occurrence and the size of microearthquakes in a swarm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T21E..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T21E..02M"><span>Strike-slip <span class="hlt">fault</span> propagation and linkage via work optimization with application to the San Jacinto <span class="hlt">fault</span>, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Madden, E. H.; McBeck, J.; Cooke, M. L.</p> <p>2013-12-01</p> <p>Over multiple <span class="hlt">earthquake</span> cycles, strike-slip <span class="hlt">faults</span> link to form through-going structures, as demonstrated by the continuous nature of the mature San Andreas <span class="hlt">fault</span> <span class="hlt">system</span> in California relative to the younger and more segmented San Jacinto <span class="hlt">fault</span> <span class="hlt">system</span> nearby. Despite its immaturity, the San Jacinto <span class="hlt">system</span> accommodates between one third and one half of the slip along the boundary between the North American and Pacific plates. It therefore poses a significant seismic threat to southern California. Better understanding of how the San Jacinto <span class="hlt">system</span> has evolved over geologic time and of current interactions between <span class="hlt">faults</span> within the <span class="hlt">system</span> is critical to assessing this seismic hazard accurately. Numerical models are well suited to simulating kilometer-scale processes, but models of <span class="hlt">fault</span> <span class="hlt">system</span> development are challenged by the multiple physical mechanisms involved. For example, laboratory experiments on brittle materials show that <span class="hlt">faults</span> propagate and eventually join (hard-linkage) by both opening-mode and shear failure. In addition, <span class="hlt">faults</span> interact prior to linkage through stress transfer (soft-linkage). The new algorithm GROW (GRowth by Optimization of Work) accounts for this complex array of behaviors by taking a global approach to <span class="hlt">fault</span> propagation while adhering to the principals of linear elastic fracture mechanics. This makes GROW a powerful tool for studying <span class="hlt">fault</span> interactions and <span class="hlt">fault</span> <span class="hlt">system</span> development over geologic time. In GROW, <span class="hlt">faults</span> evolve to minimize the work (or energy) expended during deformation, thereby maximizing the mechanical efficiency of the entire <span class="hlt">system</span>. Furthermore, the incorporation of both static and dynamic friction allows GROW models to capture <span class="hlt">fault</span> slip and <span class="hlt">fault</span> propagation in single <span class="hlt">earthquakes</span> as well as over consecutive <span class="hlt">earthquake</span> cycles. GROW models with idealized <span class="hlt">faults</span> reveal that the initial <span class="hlt">fault</span> spacing and the applied stress orientation control <span class="hlt">fault</span> linkage propensity and linkage patterns. These models allow the gains in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRB..119.6372D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRB..119.6372D"><span>Seismicity, <span class="hlt">faulting</span>, and structure of the Koyna-Warna seismic region, Western India from local <span class="hlt">earthquake</span> tomography and hypocenter locations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dixit, Madan M.; Kumar, Sanjay; Catchings, R. D.; Suman, K.; Sarkar, Dipankar; Sen, M. K.</p> <p>2014-08-01</p> <p>Although seismicity near Koyna Reservoir (India) has persisted for ~50 years and includes the largest induced <span class="hlt">earthquake</span> (M 6.3) reported worldwide, the seismotectonic framework of the area is not well understood. We recorded ~1800 <span class="hlt">earthquakes</span> from 6 January 2010 to 28 May 2010 and located a subset of 343 of the highest-quality <span class="hlt">earthquakes</span> using the tomoDD code of Zhang and Thurber (2003) to better understand the framework. We also inverted first arrivals for 3-D Vp, Vs, and Vp/Vs and Poisson's ratio tomography models of the upper 12 km of the crust. Epicenters for the recorded <span class="hlt">earthquakes</span> are located south of the Koyna River, including a high-density cluster that coincides with a shallow depth (<1.5 km) zone of relatively high Vp and low Vs (also high Vp/Vs and Poisson's ratios) near Warna Reservoir. This anomalous zone, which extends near vertically to at least 8 km depth and laterally northward at least 15 km, is likely a water-saturated zone of <span class="hlt">faults</span> under high pore pressures. Because many of the <span class="hlt">earthquakes</span> occur on the periphery of the <span class="hlt">fault</span> zone, rather than near its center, the observed seismicity-velocity correlations are consistent with the concept that many of the <span class="hlt">earthquakes</span> nucleate in fractures adjacent to the main <span class="hlt">fault</span> zone due to high pore pressure. We interpret our velocity images as showing a series of northwest trending <span class="hlt">faults</span> locally near the central part of Warna Reservoir and a major northward trending <span class="hlt">fault</span> zone north of Warna Reservoir.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008IzPSE..44..839L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008IzPSE..44..839L"><span><span class="hlt">Earthquake</span> source nucleation process in the zone of a permanently creeping deep <span class="hlt">fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lykov, V. I.; Mostryukov, A. O.</p> <p>2008-10-01</p> <p>The worldwide practice of <span class="hlt">earthquake</span> prediction, whose beginning relates to the 1970s, shows that spatial manifestations of various precursors under real seismotectonic conditions are very irregular. As noted in [Kurbanov et al., 1980], zones of bending, intersection, and branching of deep <span class="hlt">faults</span>, where conditions are favorable for increasing tangential tectonic stresses, serve as “natural amplifiers” of precursory effects. The <span class="hlt">earthquake</span> of September 28, 2004, occurred on the Parkfield segment of the San Andreas deep <span class="hlt">fault</span> in the area of a local bending of its plane. The <span class="hlt">fault</span> segment about 60 km long and its vicinities are the oldest prognostic area in California. Results of observations before and after the <span class="hlt">earthquake</span> were promptly analyzed and published in a special issue of Seismological Research Letters (2005, Vol. 76, no. 1). We have an original method enabling the monitoring of the integral rigidity of seismically active rock massifs. The integral rigidity is determined from the relative numbers of brittle and viscous failure acts during the formation of source ruptures of background <span class="hlt">earthquakes</span> in a given massif. Fracture mechanisms are diagnosed from the steepness of the first arrival of the direct P wave. Principles underlying our method are described in [Lykov and Mostryukov, 1996, 2001, 2003]. Results of monitoring have been directly displayed at the site of the Laboratory (<ExternalRef> <RefSource>http://wwwbrk.adm.yar.ru/russian/1_512/index.html</RefSource> <RefTarget Address="http://wwwbrk.adm.yar.ru/russian/1_512/index.html" TargetType="URL"/> </ExternalRef>) since the mid-1990s. It seems that this information has not attracted the attention of American seismologists. This paper assesses the informativeness of the rigidity monitoring at the stage of formation of a strong <span class="hlt">earthquake</span> source in relation to other methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28676691','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28676691"><span>Near-field <span class="hlt">fault</span> slip of the 2016 Vettore Mw 6.6 <span class="hlt">earthquake</span> (Central Italy) measured using low-cost GNSS.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wilkinson, Maxwell W; McCaffrey, Ken J W; Jones, Richard R; Roberts, Gerald P; Holdsworth, Robert E; Gregory, Laura C; Walters, Richard J; Wedmore, Luke; Goodall, Huw; Iezzi, Francesco</p> <p>2017-07-04</p> <p>The temporal evolution of slip on surface ruptures during an <span class="hlt">earthquake</span> is important for assessing <span class="hlt">fault</span> displacement, defining seismic hazard and for predicting ground motion. However, measurements of near-field surface displacement at high temporal resolution are elusive. We present a novel record of near-field co-seismic displacement, measured with 1-second temporal resolution during the 30 th October 2016 M w 6.6 Vettore <span class="hlt">earthquake</span> (Central Italy), using low-cost Global Navigation Satellite <span class="hlt">System</span> (GNSS) receivers located in the footwall and hangingwall of the Mt. Vettore - Mt. Bove <span class="hlt">fault</span> <span class="hlt">system</span>, close to new surface ruptures. We observe a clear temporal and spatial link between our near-field record and InSAR, far-field GPS data, regional measurements from the Italian Strong Motion and National Seismic networks, and field measurements of surface ruptures. Comparison of these datasets illustrates that the observed surface ruptures are the propagation of slip from depth on a surface rupturing (i.e. capable) <span class="hlt">fault</span> array, as a direct and immediate response to the 30 th October <span class="hlt">earthquake</span>. Large near-field displacement ceased within 6-8 seconds of the origin time, implying that shaking induced gravitational processes were not the primary driving mechanism. We demonstrate that low-cost GNSS is an accurate monitoring tool when installed as custom-made, short-baseline networks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/677055','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/677055"><span>Winnetka deformation zone: Surface expression of coactive slip on a blind <span class="hlt">fault</span> during the Northridge <span class="hlt">earthquake</span> sequence, California. Evidence that coactive <span class="hlt">faulting</span> occurred in the Canoga Park, Winnetka, and Northridge areas during the 17 January 1994, Northridge, California <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Cruikshank, K.M.; Johnson, A.M.; Fleming, R.W.</p> <p>1996-12-31</p> <p>Measurements of normalized length changes of streets over an area of 9 km{sup 2} in San Fernando Valley of Los Angeles, California, define a distinctive strain pattern that may well reflect blind <span class="hlt">faulting</span> during the 1994 Northridge <span class="hlt">earthquake</span>. Strain magnitudes are about 3 {times} 10{sup {minus}4}, locally 10{sup {minus}3}. They define a deformation zone trending diagonally from near Canoga Park in the southwest, through Winnetka, to near Northridge in the northeast. The deformation zone is about 4.5 km long and 1 km wide. The northwestern two-thirds of the zone is a belt of extension of streets, and the southeastern one-thirdmore » is a belt of shortening of streets. On the northwest and southeast sides of the deformation zone the magnitude of the strains is too small to measure, less than 10{sup {minus}4}. Complete states of strain measured in the northeastern half of the deformation zone show that the directions of principal strains are parallel and normal to the walls of the zone, so the zone is not a strike-slip zone. The magnitudes of strains measured in the northeastern part of the Winnetka area were large enough to fracture concrete and soils, and the area of larger strains correlates with the area of greater damage to such roads and sidewalks. All parts of the pattern suggest a blind <span class="hlt">fault</span> at depth, most likely a reverse <span class="hlt">fault</span> dipping northwest but possibly a normal <span class="hlt">fault</span> dipping southeast. The magnitudes of the strains in the Winnetka area are consistent with the strains produced at the ground surface by a blind <span class="hlt">fault</span> plane extending to depth on the order of 2 km and a net slip on the order of 1 m, within a distance of about 100 to 500 m of the ground surface. The pattern of damage in the San Fernando Valley suggests a <span class="hlt">fault</span> segment much longer than the 4.5 km defined by survey data in the Winnetka area. The blind <span class="hlt">fault</span> segment may extend several kilometers in both directions beyond the Winnetka area. This study of the Winnetka area further supports</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51A0442K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51A0442K"><span>The M6 1799 Vendée intraplate <span class="hlt">earthquake</span> (France) : characterizing the active <span class="hlt">fault</span> with a multidisciplinary approach.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kaub, C.; Perrot, J.; Le Roy, P., Sr.; Authemayou, C.; Bollinger, L.; Hebert, H.; Geoffroy, L.</p> <p>2017-12-01</p> <p>The coastal Vendee (France) is located to the south of the intraplate Armorican area. This region is affected by a <span class="hlt">system</span> of dominantly NW-SE trending shear zones and <span class="hlt">faults</span> inherited from a long and poly-phased tectonic history since Variscan times. This area currently presents a moderate background seismic activity, but was affected by a significant historical <span class="hlt">earthquake</span> (magnitude M 6) on the 1799 January 25th. This event generated particularly strong site effects in a Neogene basin located along a major onshore/offshore discontinuity bounding the basin, the Machecoul <span class="hlt">fault</span>. The objective of this study is to identify and qualify active <span class="hlt">faults</span> potentially responsible for such major seismic event in order to better constrain the seismic hazard of this area. We adopt for this purpose a multidisciplinary approach including an onshore seismological survey, high-resolution low-penetration offshore seismic data (CHIRP echo sounder, Sparker source and single channel streamer), high-resolution interferometric sonar bathymetry (GeoSwath), compilation of onshore drilling database (BSS, BRGM), and quantitative geomorphology In the meantime, the seismicity of the area was characterized by a network of 10 REFTEK stations, deployed since January 2016 around the Bay of Bourgneuf (MACHE network). About 50 local <span class="hlt">earthquakes</span>, with coda magnitudes ranging from 0.5 to 3.1 and local magnitude ranging from 0.2 to 2.9 were identified so far. This new database complement a local <span class="hlt">earthquake</span> catalog acquired since 2011 from previous regional networks. We surveyed the <span class="hlt">fault</span> segments offshore, in the Bay of Bourgneuf, analyzing 700 km of high-resolution seismic profiles and 40 km² of high-resolution bathymetry acquired during the RETZ1 (2016) and RETZ2 (2017) campaigns, in addition to HR-bathymetry along the <span class="hlt">fault</span> scarp. Those data are interpreted in conjunction with onshore wells to determine if (and since when) the Machecoul <span class="hlt">fault</span> controlled tectonically the Neogene sedimentation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.726...86Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.726...86Z"><span>InSAR and GPS derived coseismic deformation and <span class="hlt">fault</span> model of the 2017 Ms7.0 Jiuzhaigou <span class="hlt">earthquake</span> in the Northeast Bayanhar block</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Dezheng; Qu, Chunyan; Shan, Xinjian; Gong, Wenyu; Zhang, Yingfeng; Zhang, Guohong</p> <p>2018-02-01</p> <p>On 8 August 2017, a Ms7.0 <span class="hlt">earthquake</span> stroke the city of Jiuzhaigou, Sichuan, China. The Jiuzhaigou <span class="hlt">earthquake</span> occurred on a buried <span class="hlt">fault</span> in the vicinity of three well-known active <span class="hlt">faults</span> and this event offers a unique opportunity to study tectonic structures in the epicentral region and stress transferring. Here we present coseismic displacement field maps for this <span class="hlt">earthquake</span> using descending and ascending Sentinel-1A Interferometric Synthetic Aperture Radar (InSAR) data. Deformation covered an area of approximately 50 × 50 km, with a maximum line-of-sight (LOS) displacement of 22 cm in ascending and 14 cm in descending observations on the west side of the source <span class="hlt">fault</span>. Based on InSAR and Global Positioning <span class="hlt">System</span> (GPS) measurements, both separately and jointly, we constructed a one-segment model to invert the coseismic slip distribution and dip angle of this event. Our final <span class="hlt">fault</span> slip model suggests that slip was concentrated at an upper depth of 15 km; there was a maximum slip of 1.3 m and the rupture was dominated by a left-lateral strike-slip motion. The inverted geodetic moment was approximately 6.75 × 1018 Nm, corresponding to a moment magnitude of Mw6.5, consistent with seismological results. The calculated static Coulomb stress changes indicate that most aftershocks occurred in stress increasing zones caused by the mainshock rupture; the Jiuzhaigou <span class="hlt">earthquake</span> has brought the western part of the Tazang <span class="hlt">fault</span> 0.1-0.4 MPa closer to failure, indicating an increasing seismic hazard in this region. The Coulomb stress changes caused by the 2008 Mw7.8 Wenchuan <span class="hlt">earthquake</span> suggest that stress loading from this event acted as a trigger for the Jiuzhaigou <span class="hlt">earthquake</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..188Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..188Y"><span><span class="hlt">Earthquake</span> Records of North Anatolian <span class="hlt">Fault</span> from Sapanca Lake Sediments, NW Anatolia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yalamaz, Burak; Cagatay, Namık; Acar, Dursun; Demirbag, Emin; Gungor, Emin; Gungor, Nurdan; Gulen, Levent</p> <p>2014-05-01</p> <p>We determined <span class="hlt">earthquake</span> records in sediment cores of Sapanca Lake which is a pull-apart basin located along the North Anatolian <span class="hlt">Fault</span> zone in NW Anatolia. The lake has a maximum depth of 55 m, and a surface area of 46.8 km2, measuring 16 km in E-W and 5 km in N-S directions. A systematic study of the sedimentological, physical and geochemical properties of three water-sediment interface cores, up to 75.7 cm long, located along depth transects ranging from 43 to 51.5 m water depths. The cores were analyzed using Geotek Multi Sensor Core Logger (MSCL) for physical properties, laser particle size analyzer for granulometry, TOC Analyzer for Total Organic Content (TOC) and Total Inorganic Carbon (TIC) analysis, Itrax-XRF Core Scanner for elemental analysis and digital X-RAY Radiography. The geochronology was determined using AMS radiocarbon and radionuclide methods. The Sapanca Lake <span class="hlt">earthquake</span> records are characterized by mass flow units consisting of grey or dark grey coarse to fine sand and silty mud with sharp basal and transional upper boundaries. The units commonly show normal size grading with their basal parts showing high density, and high magnetic susceptibility and enrichment in one or more elements, such as Si, Ca, Tİ, K, Rb, Zr and Fe, indicative of coarse detrial input. Based on radionuclide and radiocarbon analyses the mass flow units are correlated with 1999 İzmit and Düzce <span class="hlt">earthquakes</span> (Mw=7.4 and 7.2, respectively) , 1967 Mudurnu <span class="hlt">earthquake</span> (Mw= 6,8), and 1957 Abant (Mw= 7.1) <span class="hlt">earthquake</span>. Keywords: Sapanca Lake, North Anatolian <span class="hlt">Fault</span>, <span class="hlt">Earthquake</span>, Grain size, Itrax-XRF, MSCL</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA21210.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA21210.html"><span>Satellite Radar Show Complex Set of <span class="hlt">Faults</span> Moved in 2016 New Zealand <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-03-23</p> <p>NASA and its partners are contributing important observations and expertise to the ongoing response to the Nov. 14, 2016, magnitude 7.8 Kaikoura <span class="hlt">earthquake</span> in New Zealand. This shallow <span class="hlt">earthquake</span> was so complex and unusual, it is likely to change how scientists think about <span class="hlt">earthquake</span> hazards in plate boundary zones around the world. Scientists with the Advanced Rapid Imaging and Analysis project (ARIA), a collaboration between NASA's Jet Propulsion Laboratory, Pasadena, California, and Caltech in Pasadena, analyzed interferometric synthetic aperture radar images from the PALSAR-2 instrument on the ALOS-2 satellite operated by the Japan Aerospace Exploration Agency (JAXA) to calculate maps of the deformation of Earth's surface caused by the quake. Two maps show motion of the surface in two different directions. Each false-color map shows the amount of permanent surface movement caused almost entirely by the <span class="hlt">earthquake</span>, as viewed by the satellite, during a 28-day interval between two ALOS-2 wide-swath images acquired on Oct. 18 and Nov. 15, 2016. In these two new maps made from the wide-swath images, the colors of the surface displacements are proportional to the surface motion. The wide-swath images cover the entire 106-mile (170-kilometer) length of the complex set of <span class="hlt">earthquake</span> ruptures. The arrows show the direction of the radar motion measurement. In the left image, the blue and purple tones show the areas where the land around the Kaikoura peninsula in the Marlborough region of New Zealand's South Island has moved toward the satellite by up to 13.2 feet (4 meters), both eastward and upward. In the right image, the blue and purple tones show the areas that moved to the north by up to 30 feet (9 meters) and green tones show the area that moved to the south. The sharp line of color change is across the Kekerengu <span class="hlt">Fault</span>, which had the largest amount of motion in the <span class="hlt">earthquake</span>. Field studies found maximum rupture at the surface was measured at 39 feet (12 meters) of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5533536','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5533536"><span>Buried shallow <span class="hlt">fault</span> slip from the South Napa <span class="hlt">earthquake</span> revealed by near-field geodesy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Brooks, Benjamin A.; Minson, Sarah E.; Glennie, Craig L.; Nevitt, Johanna M.; Dawson, Tim; Rubin, Ron; Ericksen, Todd L.; Lockner, David; Hudnut, Kenneth; Langenheim, Victoria; Lutz, Andrew; Mareschal, Maxime; Murray, Jessica; Schwartz, David; Zaccone, Dana</p> <p>2017-01-01</p> <p><span class="hlt">Earthquake</span>-related <span class="hlt">fault</span> slip in the upper hundreds of meters of Earth’s surface has remained largely unstudied because of challenges measuring deformation in the near field of a <span class="hlt">fault</span> rupture. We analyze centimeter-scale accuracy mobile laser scanning (MLS) data of deformed vine rows within ±300 m of the principal surface expression of the M (magnitude) 6.0 2014 South Napa <span class="hlt">earthquake</span>. Rather than assuming surface displacement equivalence to <span class="hlt">fault</span> slip, we invert the near-field data with a model that allows for, but does not require, the <span class="hlt">fault</span> to be buried below the surface. The inversion maps the position on a preexisting <span class="hlt">fault</span> plane of a slip front that terminates ~3 to 25 m below the surface coseismically and within a few hours postseismically. The lack of surface-breaching <span class="hlt">fault</span> slip is verified by two trenches. We estimate near-surface slip ranging from ~0.5 to 1.25 m. Surface displacement can underestimate <span class="hlt">fault</span> slip by as much as 30%. This implies that similar biases could be present in short-term geologic slip rates used in seismic hazard analyses. Along strike and downdip, we find deficits in slip: The along-strike deficit is erased after ~1 month by afterslip. We find no evidence of off-<span class="hlt">fault</span> deformation and conclude that the downdip shallow slip deficit for this event is likely an artifact. As near-field geodetic data rapidly proliferate and will become commonplace, we suggest that analyses of near-surface <span class="hlt">fault</span> rupture should also use more sophisticated mechanical models and subsurface geomechanical tests. PMID:28782026</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28782026','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28782026"><span>Buried shallow <span class="hlt">fault</span> slip from the South Napa <span class="hlt">earthquake</span> revealed by near-field geodesy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brooks, Benjamin A; Minson, Sarah E; Glennie, Craig L; Nevitt, Johanna M; Dawson, Tim; Rubin, Ron; Ericksen, Todd L; Lockner, David; Hudnut, Kenneth; Langenheim, Victoria; Lutz, Andrew; Mareschal, Maxime; Murray, Jessica; Schwartz, David; Zaccone, Dana</p> <p>2017-07-01</p> <p><span class="hlt">Earthquake</span>-related <span class="hlt">fault</span> slip in the upper hundreds of meters of Earth's surface has remained largely unstudied because of challenges measuring deformation in the near field of a <span class="hlt">fault</span> rupture. We analyze centimeter-scale accuracy mobile laser scanning (MLS) data of deformed vine rows within ±300 m of the principal surface expression of the M (magnitude) 6.0 2014 South Napa <span class="hlt">earthquake</span>. Rather than assuming surface displacement equivalence to <span class="hlt">fault</span> slip, we invert the near-field data with a model that allows for, but does not require, the <span class="hlt">fault</span> to be buried below the surface. The inversion maps the position on a preexisting <span class="hlt">fault</span> plane of a slip front that terminates ~3 to 25 m below the surface coseismically and within a few hours postseismically. The lack of surface-breaching <span class="hlt">fault</span> slip is verified by two trenches. We estimate near-surface slip ranging from ~0.5 to 1.25 m. Surface displacement can underestimate <span class="hlt">fault</span> slip by as much as 30%. This implies that similar biases could be present in short-term geologic slip rates used in seismic hazard analyses. Along strike and downdip, we find deficits in slip: The along-strike deficit is erased after ~1 month by afterslip. We find no evidence of off-<span class="hlt">fault</span> deformation and conclude that the downdip shallow slip deficit for this event is likely an artifact. As near-field geodetic data rapidly proliferate and will become commonplace, we suggest that analyses of near-surface <span class="hlt">fault</span> rupture should also use more sophisticated mechanical models and subsurface geomechanical tests.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70192302','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70192302"><span>Buried shallow <span class="hlt">fault</span> slip from the South Napa <span class="hlt">earthquake</span> revealed by near-field geodesy</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brooks, Benjamin A.; Minson, Sarah E.; Glennie, Craig L.; Nevitt, Johanna; Dawson, Timothy E.; Rubin, Ron S.; Ericksen, Todd; Lockner, David A.; Hudnut, Kenneth W.; Langenheim, Victoria; Lutz, Andrew; Murray, Jessica R.; Schwartz, David P.; Zaccone, Dana</p> <p>2017-01-01</p> <p><span class="hlt">Earthquake</span>-related <span class="hlt">fault</span> slip in the upper hundreds of meters of Earth’s surface has remained largely unstudied because of challenges measuring deformation in the near field of a <span class="hlt">fault</span> rupture. We analyze centimeter-scale accuracy mobile laser scanning (MLS) data of deformed vine rows within ±300 m of the principal surface expression of the M (magnitude) 6.0 2014 South Napa <span class="hlt">earthquake</span>. Rather than assuming surface displacement equivalence to <span class="hlt">fault</span> slip, we invert the near-field data with a model that allows for, but does not require, the <span class="hlt">fault</span> to be buried below the surface. The inversion maps the position on a preexisting <span class="hlt">fault</span> plane of a slip front that terminates ~3 to 25 m below the surface coseismically and within a few hours postseismically. The lack of surface-breaching <span class="hlt">fault</span> slip is verified by two trenches. We estimate near-surface slip ranging from ~0.5 to 1.25 m. Surface displacement can underestimate <span class="hlt">fault</span> slip by as much as 30%. This implies that similar biases could be present in short-term geologic slip rates used in seismic hazard analyses. Along strike and downdip, we find deficits in slip: The along-strike deficit is erased after ~1 month by afterslip. We find no evidence of off-<span class="hlt">fault</span> deformation and conclude that the downdip shallow slip deficit for this event is likely an artifact. As near-field geodetic data rapidly proliferate and will become commonplace, we suggest that analyses of near-surface <span class="hlt">fault</span> rupture should also use more sophisticated mechanical models and subsurface geomechanical tests.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=128570','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=128570"><span>Self-organization in leaky threshold <span class="hlt">systems</span>: The influence of near-mean field dynamics and its implications for <span class="hlt">earthquakes</span>, neurobiology, and forecasting</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rundle, J. B.; Tiampo, K. F.; Klein, W.; Sá Martins, J. S.</p> <p>2002-01-01</p> <p>Threshold <span class="hlt">systems</span> are known to be some of the most important nonlinear self-organizing <span class="hlt">systems</span> in nature, including networks of <span class="hlt">earthquake</span> <span class="hlt">faults</span>, neural networks, superconductors and semiconductors, and the World Wide Web, as well as political, social, and ecological <span class="hlt">systems</span>. All of these <span class="hlt">systems</span> have dynamics that are strongly correlated in space and time, and all typically display a multiplicity of spatial and temporal scales. Here we discuss the physics of self-organization in <span class="hlt">earthquake</span> threshold <span class="hlt">systems</span> at two distinct scales: (i) The “microscopic” laboratory scale, in which consideration of results from simulations leads to dynamical equations that can be used to derive the results obtained from sliding friction experiments, and (ii) the “macroscopic” <span class="hlt">earthquake</span> <span class="hlt">fault-system</span> scale, in which the physics of strongly correlated <span class="hlt">earthquake</span> <span class="hlt">fault</span> <span class="hlt">systems</span> can be understood by using time-dependent state vectors defined in a Hilbert space of eigenstates, similar in many respects to the mathematics of quantum mechanics. In all of these <span class="hlt">systems</span>, long-range interactions induce the existence of locally ergodic dynamics. The existence of dissipative effects leads to the appearance of a “leaky threshold” dynamics, equivalent to a new scaling field that controls the size of nucleation events relative to the size of background fluctuations. At the macroscopic <span class="hlt">earthquake</span> <span class="hlt">fault-system</span> scale, these ideas show considerable promise as a means of forecasting future <span class="hlt">earthquake</span> activity. PMID:11875204</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..122.7879S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..122.7879S"><span>A Decade of Induced Slip on the Causative <span class="hlt">Fault</span> of the 2015 Mw 4.0 Venus <span class="hlt">Earthquake</span>, Northeast Johnson County, Texas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scales, Monique M.; DeShon, Heather R.; Magnani, M. Beatrice; Walter, Jacob I.; Quinones, Louis; Pratt, Thomas L.; Hornbach, Matthew J.</p> <p>2017-10-01</p> <p>On 7 May 2015, a Mw 4.0 <span class="hlt">earthquake</span> occurred near Venus, northeast Johnson County, Texas, in an area of the Bend Arch-Fort Worth Basin that reports long-term, high-volume wastewater disposal and that has hosted felt <span class="hlt">earthquakes</span> since 2009. In the weeks following the Mw 4.0 <span class="hlt">earthquake</span>, we deployed a local seismic network and purchased nearby active-source seismic reflection data to capture additional events, characterize the causative <span class="hlt">fault</span>, and explore potential links between ongoing industry activity and seismicity. Hypocenter relocations of the resulting local <span class="hlt">earthquake</span> catalog span 4-6 km depth and indicate a <span class="hlt">fault</span> striking 230°, dipping to the west, consistent with a nodal plane of the Mw 4.0 regional moment tensor. <span class="hlt">Fault</span> plane solutions indicate normal <span class="hlt">faulting</span>, with B axes striking parallel to maximum horizontal compressive stress. Seismic reflection data image the reactivated basement <span class="hlt">fault</span> penetrating the Ordovician disposal layer and Mississippian production layer, but not displacing post-Lower Pennsylvanian units. Template matching at regional seismic stations indicates that low-magnitude <span class="hlt">earthquakes</span> with similar waveforms began in April 2008, with increasing magnitude over time. Pressure data from five saltwater disposal wells within 5 km of the active <span class="hlt">fault</span> indicate a disposal formation that is 0.9-4.8 MPa above hydrostatic. We suggest that the injection of 28,000,000 m3 of wastewater between 2006 and 2015 at these wells led to an increase in subsurface pore fluid pressure that contributed to inducing this long-lived <span class="hlt">earthquake</span> sequence. The 2015 Mw 4.0 event represents the largest event in the continuing evolution of slip on the causative <span class="hlt">fault</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S53A2807Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S53A2807Z"><span>A N-S fossil transform <span class="hlt">fault</span> reactivated by the March 2, 2016 Mw7.8 southwest of Sumatra, Indonesia <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, H.; van der Lee, S.</p> <p>2016-12-01</p> <p>Warton Basin (WB) is characterized by N-S striking fossil transform <span class="hlt">faults</span> and E-W trending extinct ridges. The 2016 Mw7.8 southwest of Sumatra <span class="hlt">earthquake</span>, nearby the WB's center, was first imaged by back-projecting P-waves from three regional seismic networks in Europn, Japan, and Australia. Next, the rupture direction of the <span class="hlt">earthquake</span> was further determined using the rupture directivity analysis to P-waves from the global seismic network (GSN). Finally, we inverting these GSN waveforms on a defined N-S striking vertical <span class="hlt">fault</span> for a kinematic source model. The results show that the <span class="hlt">earthquake</span> reactivates a 190 degree N-S striking vertical fossil transform <span class="hlt">fault</span> and asymmetrically bilaterally ruptures a 65 km by 30 km asperity over 35 s. Specifically, the <span class="hlt">earthquake</span> first bilaterally ruptures northward and southward at a speed of 1.0 km/s over the first 12 s, and then mainly rupture northward at a speed of 1.6 km/s. Compared with two previous M≥7.8 WB <span class="hlt">earthquakes</span>, including the 2000 southern WB <span class="hlt">earthquake</span> and 2012 Mw8.6 Sumatra <span class="hlt">earthquake</span>, the lower seismic energy radiation efficiency and slower rupture velicity of the 2016 <span class="hlt">earthquake</span> indicate the rupture of the <span class="hlt">earthquake</span> is probably controlled by the warmer ambient slab and tectonic stress regime.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.4773B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.4773B"><span><span class="hlt">Fault</span> zone structure and seismic reflection characteristics in zones of slow slip and tsunami <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, Rebecca; Henrys, Stuart; Sutherland, Rupert; Barker, Daniel; Wallace, Laura; Holden, Caroline; Power, William; Wang, Xiaoming; Morgan, Joanna; Warner, Michael; Downes, Gaye</p> <p>2015-04-01</p> <p>Over the last couple of decades we have learned that a whole spectrum of different <span class="hlt">fault</span> slip behaviour takes place on subduction megathrust <span class="hlt">faults</span> from stick-slip <span class="hlt">earthquakes</span> to slow slip and stable sliding. Geophysical data, including seismic reflection data, can be used to characterise margins and <span class="hlt">fault</span> zones that undergo different modes of slip. In this presentation we will focus on the Hikurangi margin, New Zealand, which exhibits marked along-strike changes in seismic behaviour and margin characteristics. Campaign and continuous GPS measurements reveal deep interseismic coupling and deep slow slip events (~30-60 km) at the southern Hikurangi margin. The northern margin, in contrast, experiences aseismic slip and shallow (<10-15 km) slow slip events (SSE) every 18-24 months with equivalent moment magnitudes of Mw 6.5-6.8. Updip of the SSE region two unusual megathrust <span class="hlt">earthquakes</span> occurred in March and May 1947 with characteristics typical of tsunami <span class="hlt">earthquakes</span>. The Hikurangi margin is therefore an excellent natural laboratory to study differential <span class="hlt">fault</span> slip behaviour. Using 2D seismic reflection, magnetic anomaly and geodetic data we observe in the source areas of the 1947 tsunami <span class="hlt">earthquakes</span> i) low amplitude interface reflectivity, ii) shallower interface relief, iii) bathymetric ridges, iv) magnetic anomaly highs and in the case of the March 1947 <span class="hlt">earthquake</span> v) stronger geodetic coupling. We suggest that this is due to the subduction of seamounts, similar in dimensions to seamounts observed on the incoming Pacific plate, to depths of <10 km. We propose a source model for the 1947 tsunami <span class="hlt">earthquakes</span> based on geophysical data and find that extremely low rupture velocities (c. 300 m/s) are required to model the observed large tsunami run-up heights (Bell et al. 2014, EPSL). Our study suggests that subducted topography can cause the nucleation of moderate <span class="hlt">earthquakes</span> with complex, low velocity rupture scenarios that enhance tsunami waves, and the role of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhDT........59A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhDT........59A"><span>Self-organized criticality in complex <span class="hlt">systems</span>: Applicability to the interoccurrent and recurrent statistical behavior of <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abaimov, Sergey G.</p> <p></p> <p>The concept of self-organized criticality is associated with scale-invariant, fractal behavior; this concept is also applicable to <span class="hlt">earthquake</span> <span class="hlt">systems</span>. It is known that the interoccurrent frequency-size distribution of <span class="hlt">earthquakes</span> in a region is scale-invariant and obeys the Gutenberg-Richter power-law dependence. Also, the interoccurrent time-interval distribution is known to obey Poissonian statistics excluding aftershocks. However, to estimate the hazard risk for a region it is necessary to know also the recurrent behavior of <span class="hlt">earthquakes</span> at a given point on a <span class="hlt">fault</span>. This behavior has been investigated in the literature, however, major questions remain unresolved. The reason is the small number of <span class="hlt">earthquakes</span> in observed sequences. To overcome this difficulty this research utilizes numerical simulations of a slider-block model and a sand-pile model. Also, experimental observations of creep events on the creeping section of the San Andreas <span class="hlt">fault</span> are processed and sequences up to 100 events are studied. Then the recurrent behavior of <span class="hlt">earthquakes</span> at a given point on a <span class="hlt">fault</span> or at a given <span class="hlt">fault</span> is investigated. It is shown that both the recurrent frequency-size and the time-interval behaviors of <span class="hlt">earthquakes</span> obey the Weibull distribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T53B2715W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T53B2715W"><span>"The Big One" in Taipei: Numerical Simulation Study of the Sanchiao <span class="hlt">Fault</span> <span class="hlt">Earthquake</span> Scenarios</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Y.; Lee, S.; Ng, S.</p> <p>2012-12-01</p> <p>Sanchiao <span class="hlt">fault</span> is a western boundary <span class="hlt">fault</span> of the Taipei basin located in northern Taiwan, close to the densely populated Taipei metropolitan area. According to the report of Central Geological Survey, the terrestrial portion of the Sanchiao <span class="hlt">fault</span> can be divided into north and south segments. The south segment is about 13 km and north segment is about 21 km. Recent study demonstrated that there are about 40 km of the <span class="hlt">fault</span> trace that extended to the marine area offshore of northern Taiwan. Combined with the marine and terrestrial parts, the total <span class="hlt">fault</span> length of Sanchiao <span class="hlt">fault</span> could be nearly 70 kilometers. Based on the recipe proposed by IRIKURA and Miyake (2010), we estimate the Sanchiao <span class="hlt">fault</span> has the potential to produce an <span class="hlt">earthquake</span> with moment magnitude larger than Mw 7.2. The total area of <span class="hlt">fault</span> rupture is about 1323 km2, asperity to the total <span class="hlt">fault</span> plane is 22%, and the slips of the asperity and background are 2.8 m and 1.6 m respectively. Use the characteristic source model based on this assumption, the 3D spectral-element method simulation results indicate that Peak ground acceleration (PGA) is significantly stronger along the surface <span class="hlt">fault</span>-rupture. The basin effects play an important role when wave propagates in the Taipei basin which cause seismic wave amplified and prolong the shaking for a very long time. It is worth noting that, when the rupture starts from the southern tip of the <span class="hlt">fault</span>, i.e. the hypocenter locates in the basin, the impact of the Sanchiao <span class="hlt">fault</span> <span class="hlt">earthquake</span> to the Taipei metropolitan area will be the most serious. The strong shaking can cover the entire Taipei city, and even across the basin that extended to eastern-most part of northern Taiwan.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008Tectp.453..148M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008Tectp.453..148M"><span>Recognition of <span class="hlt">earthquake</span>-related damage in archaeological sites: Examples from the Dead Sea <span class="hlt">fault</span> zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marco, Shmuel</p> <p>2008-06-01</p> <p>Archaeological structures that exhibit seismogenic damage expand our knowledge of temporal and spatial distribution of <span class="hlt">earthquakes</span>, afford independent examination of historical accounts, provide information on local <span class="hlt">earthquake</span> intensities and enable the delineation of macroseismic zones. They also illustrate what might happen in future <span class="hlt">earthquakes</span>. In order to recover this information, we should be able to distinguish <span class="hlt">earthquake</span> damage from anthropogenic damage and from other natural processes of wear and tear. The present paper reviews several types of damage that can be attributed with high certainty to <span class="hlt">earthquakes</span> and discusses associated caveats. In the rare cases, where <span class="hlt">faults</span> intersect with archaeological sites, offset structures enable precise determination of sense and size of slip, and constrain its time. Among the characteristic off-<span class="hlt">fault</span> damage types, I consider horizontal shifting of large building blocks, downward sliding of one or several blocks from masonry arches, collapse of heavy, stably-built walls, chipping of corners of building blocks, and aligned falling of walls and columns. Other damage features are less conclusive and require additional evidence, e.g., fractures that cut across several structures, leaning walls and columns, warps and bulges in walls. Circumstantial evidence for catastrophic <span class="hlt">earthquake</span>-related destruction includes contemporaneous damage in many sites in the same area, absence of weapons or other anthropogenic damage, stratigraphic data on collapse of walls and ceilings onto floors and other living horizons and burial of valuable artifacts, as well as associated geological palaeoseismic phenomena such as liquefaction, land- and rock-slides, and <span class="hlt">fault</span> ruptures. Additional support may be found in reliable historical accounts. Special care must be taken in order to avoid circular reasoning by maintaining the independence of data acquisition methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918205C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918205C"><span>The 2016 central Italy <span class="hlt">earthquake</span> sequence: surface effects, <span class="hlt">fault</span> model and triggering scenarios</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chatzipetros, Alexandros; Pavlides, Spyros; Papathanassiou, George; Sboras, Sotiris; Valkaniotis, Sotiris; Georgiadis, George</p> <p>2017-04-01</p> <p>The results of fieldwork performed during the 2016 <span class="hlt">earthquake</span> sequence around the karstic basins of Norcia and La Piana di Castelluccio, at an altitude of 1400 m, on the Monte Vettore (altitude 2476 m) and Vettoretto, as well as the three mapped seismogenic <span class="hlt">faults</span>, striking NNW-SSW, are presented in this paper. Surface co-seismic ruptures were observed in the Vettore and Vettoretto segment of the <span class="hlt">fault</span> for several kilometres ( 7 km) in the August <span class="hlt">earthquakes</span> at high altitudes, and were re-activated and expanded northwards during the October <span class="hlt">earthquakes</span>. Coseismic ruptures and the neotectonic Mt. Vettore <span class="hlt">fault</span> zone were modelled in detail using images acquired from specifically planned UAV (drone) flights. Ruptures, typically with displacement of up to 20 cm, were observed after the August event both in the scree and weathered mantle (elluvium), as well as the bedrock, consisting mainly of fragmented carbonate rocks with small tectonic surfaces. These fractures expanded and new ones formed during the October events, typically of displacements of up to 50 cm, although locally higher displacements of up to almost 2 m were observed. Hundreds of rock falls and landslides were mapped through satellite imagery, using pre- and post- <span class="hlt">earthquake</span> Sentinel 2A images. Several of them were also verified in the field. Based on field mapping results and seismological information, the causative <span class="hlt">faults</span> were modelled. The model consists of five seismogenic sources, each one associated with a strong event in the sequence. The visualisation of the seismogenic sources follows INGV's DISS standards for the Individual Seismogenic Sources (ISS) layer, while strike, dip and rake of the seismic sources are obtained from selected focal mechanisms. Based on this model, the ground deformation pattern was inferred, using Okada's dislocation solution formulae, which shows that the maximum calculated vertical displacement is 0.53 m. This is in good agreement with the statistical analysis of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.G22A..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.G22A..08F"><span>Imaging Complex <span class="hlt">Fault</span> Slip of the 2016 MeiNong and Kumamoto <span class="hlt">Earthquakes</span> with Sentinel-1 InSAR and Other Geodetic and Seismic Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fielding, E. J.; Huang, M. H.; Liang, C.; Yue, H.; Agram, P. S.; Simons, M.; Fattahi, H.; Tung, H.; Hu, J. C.; Huang, C.</p> <p>2016-12-01</p> <p>We map complex <span class="hlt">fault</span> ruptures of the February 2016 MeiNong <span class="hlt">earthquake</span> in Taiwan and the April 2016 Kumamoto <span class="hlt">earthquake</span> sequence in Japan by analysis of Synthetic Aperture Radar (SAR) data from the Copernicus Sentinel-1A (S1A) satellite operated by the European Space Agency and the Advanced Land Observation Satellite-2 (ALOS-2) satellite operated by the Japanese Aerospace Exploration Agency (JAXA). Our analysis shows that the MeiNong main rupture at lower crustal depth triggered slip on another <span class="hlt">fault</span> at upper crustal depth and shallow slip on several <span class="hlt">faults</span> in the upper few km. The Kumamoto <span class="hlt">earthquake</span> sequence ruptured two major <span class="hlt">fault</span> <span class="hlt">systems</span> over two days and triggered shallow slip on a large number of shallow <span class="hlt">faults</span>. We combine less precise analysis of large scale displacements from the SAR images of the two satellites by pixel offset tracking or sub-pixel correlation, including the along-track component of surface motion, with the more precise SAR interferometry (InSAR) measurements in the radar line-of-sight direction to estimate all three components of the surface displacement for the events. Data was processed with customized workflows based on modules in the InSAR Scientific Computing Environment (ISCE). Joint inversion of S1A and ALOS-2 InSAR, GPS, and strong motion seismograms for the Mw6.4 MeiNong <span class="hlt">earthquake</span> shows that the main thrust rupture with N61°W strike and 15° dip at 15-20 km depth explains nearly all of the seismic waveforms but leaves a substantial uplift residual in the InSAR and GPS offsets estimated 4 hours after the <span class="hlt">earthquake</span>. We model this residual with slip on a N8°E-trending thrust <span class="hlt">fault</span> dipping 30° at depths between 5-10 km. This <span class="hlt">fault</span> strike is parallel to surface <span class="hlt">faults</span> and we interpret it as <span class="hlt">fault</span> slip within a mid-crustal duplex that was triggered by the main rupture within 4 hours of the mainshock. In addition, InSAR shows sharp discontinuities at many locations that are likely due to shallow triggered slip, but the timing of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.G51A0857M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.G51A0857M"><span><span class="hlt">Fault</span> model of the M7.1 intraslab <span class="hlt">earthquake</span> on April 7 following the 2011 Great Tohoku <span class="hlt">earthquake</span> (M9.0) estimated by the dense GPS network data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miura, S.; Ohta, Y.; Ohzono, M.; Kita, S.; Iinuma, T.; Demachi, T.; Tachibana, K.; Nakayama, T.; Hirahara, S.; Suzuki, S.; Sato, T.; Uchida, N.; Hasegawa, A.; Umino, N.</p> <p>2011-12-01</p> <p>We propose a source <span class="hlt">fault</span> model of the large intraslab <span class="hlt">earthquake</span> with M7.1 deduced from a dense GPS network. The coseismic displacements obtained by GPS data analysis clearly show the spatial pattern specific to intraslab <span class="hlt">earthquakes</span> not only in the horizontal components but also the vertical ones. A rectangular <span class="hlt">fault</span> with uniform slip was estimated by a non-linear inversion approach. The results indicate that the simple rectangular <span class="hlt">fault</span> model can explain the overall features of the observations. The amount of moment released is equivalent to Mw 7.17. The hypocenter depth of the main shock estimated by the Japan Meteorological Agency is slightly deeper than the neutral plane between down-dip compression (DC) and down-dip extension (DE) stress zones of the double-planed seismic zone. This suggests that the depth of the neutral plane was deepened by the huge slip of the 2011 M9.0 Tohoku <span class="hlt">earthquake</span>, and the rupture of the thrust M7.1 <span class="hlt">earthquake</span> was initiated at that depth, although more investigations are required to confirm this idea. The estimated <span class="hlt">fault</span> plane has an angle of ~60 degrees from the surface of subducting Pacific plate. It is consistent with the hypothesis that intraslab <span class="hlt">earthquakes</span> are thought to be reactivation of the preexisting hydrated weak zones made in bending process of oceanic plates around outer-rise regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T22A..03D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T22A..03D"><span>Mechanical properties of conjugate <span class="hlt">faults</span> in the Makran accretionary prism estimated from InSAR observations of coseismic deformation due to the 2013 Baluchistan (Mw 7.7) <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dutta, R.; Harrington, J.; Wang, T.; Feng, G.; Vasyura-Bathke, H.; Jonsson, S.</p> <p>2017-12-01</p> <p>Interferometric Synthetic Aperture Radar (InSAR) measurements allow us to study various mechanical and rheological properties around <span class="hlt">faults</span>. For example, strain localizations along <span class="hlt">faults</span> induced by nearby <span class="hlt">earthquakes</span> observed by InSAR have been explained by the elastic response of compliant <span class="hlt">fault</span> zones (CFZ) where the elastic moduli is reduced with respect to that of the surrounding rock. We observed similar strain localizations (up to 1-3 cm displacements in the line-of-sight direction of InSAR) along several conjugate <span class="hlt">faults</span> near the rupture of the 2013 Mw7.7 Baluchistan (Pakistan) <span class="hlt">earthquake</span> in the accretionary prism of the Makran subduction zone. These conjugate compliant <span class="hlt">faults</span>, which have strikes of N30°E and N45°W, are located 15-30 km from the mainshock <span class="hlt">fault</span> rupture in a N-S compressional stress regime. The long-term geologic slip direction of these <span class="hlt">faults</span> is left-lateral for the N30°E striking <span class="hlt">faults</span> and right-lateral for the N45°W striking <span class="hlt">faults</span>. The 2013 Baluchistan <span class="hlt">earthquake</span> caused WSW-ENE extensional coseismic stress changes across the conjugate <span class="hlt">fault</span> <span class="hlt">system</span> and the observed strain localizations shows opposite sense of motion to that of the geologic long-term slip. We use 3D Finite Element modeling (FEM) to study the effects extensional coseismic stresses have on the conjugate CFZs that is otherwise loaded in a compressional regional stress. We use coseismic static displacements due to the <span class="hlt">earthquake</span> along the FEM domain boundaries to simulate the extensional coseismic stress change acting across the <span class="hlt">fault</span> <span class="hlt">system</span>. Around 0.5-2 km wide CFZs with reduction in shear modulus by a factor of 3 to 4 can explain the observed InSAR strain localizations and the opposite sense of motion. The InSAR measurements were also used to constrain the ranges of the length, width and rigidity variations of the CFZs. The FEM solution shows that the N45°W striking <span class="hlt">faults</span> localize mostly extensional strain and a small amount of left-lateral shear (opposite sense to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/422/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/422/"><span>Surface Rupture Map of the 2002 M7.9 Denali <span class="hlt">Fault</span> <span class="hlt">Earthquake</span>, Alaska: Digital Data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Haeussler, Peter J.</p> <p>2009-01-01</p> <p>The November 3, 2002, Mw7.9 Denali <span class="hlt">Fault</span> <span class="hlt">earthquake</span> produced about 340 km of surface rupture along the Susitna Glacier Thrust <span class="hlt">Fault</span> and the right-lateral, strike-slip Denali and Totschunda <span class="hlt">Faults</span>. Digital photogrammetric methods were primarily used to create a 1:500-scale, three-dimensional surface rupture map, and 1:6,000-scale aerial photographs were used for three-dimensional digitization in ESRI's ArcMap GIS software, using Leica's StereoAnalyst plug in. Points were digitized 4.3 m apart, on average, for the entire surface rupture. <span class="hlt">Earthquake</span>-induced landslides, sackungen, and unruptured Holocene <span class="hlt">fault</span> scarps on the eastern Denali <span class="hlt">Fault</span> were also digitized where they lay within the limits of air photo coverage. This digital three-dimensional <span class="hlt">fault</span>-trace map is superior to traditional maps in terms of relative and absolute accuracy, completeness, and detail and is used as a basis for three-dimensional visualization. Field work complements the air photo observations in locations of dense vegetation, on bedrock, or in areas where the surface trace is weakly developed. Seventeen km of the <span class="hlt">fault</span> trace, which broke through glacier ice, were not digitized in detail due to time constraints, and air photos missed another 10 km of <span class="hlt">fault</span> rupture through the upper Black Rapids Glacier, so that was not mapped in detail either.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70196642','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70196642"><span>Numerical models of pore pressure and stress changes along basement <span class="hlt">faults</span> due to wastewater injection: Applications to the 2014 Milan, Kansas <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hearn, Elizabeth H.; Koltermann, Christine; Rubinstein, Justin R.</p> <p>2018-01-01</p> <p>We have developed groundwater flow models to explore the possible relationship between wastewater injection and the 12 November 2014 Mw 4.8 Milan, Kansas <span class="hlt">earthquake</span>. We calculate pore pressure increases in the uppermost crust using a suite of models in which hydraulic properties of the Arbuckle Formation and the Milan <span class="hlt">earthquake</span> <span class="hlt">fault</span> zone, the Milan <span class="hlt">earthquake</span> hypocenter depth, and <span class="hlt">fault</span> zone geometry are varied. Given pre‐<span class="hlt">earthquake</span> injection volumes and reasonable hydrogeologic properties, significantly increasing pore pressure at the Milan hypocenter requires that most flow occur through a conductive channel (i.e., the lower Arbuckle and the <span class="hlt">fault</span> zone) rather than a conductive 3‐D volume. For a range of reasonable lower Arbuckle and <span class="hlt">fault</span> zone hydraulic parameters, the modeled pore pressure increase at the Milan hypocenter exceeds a minimum triggering threshold of 0.01 MPa at the time of the <span class="hlt">earthquake</span>. Critical factors include injection into the base of the Arbuckle Formation and proximity of the injection point to a narrow <span class="hlt">fault</span> damage zone or conductive fracture in the pre‐Cambrian basement with a hydraulic diffusivity of about 3–30 m2/s. The maximum pore pressure increase we obtain at the Milan hypocenter before the <span class="hlt">earthquake</span> is 0.06 MPa. This suggests that the Milan <span class="hlt">earthquake</span> occurred on a <span class="hlt">fault</span> segment that was critically stressed prior to significant wastewater injection in the area. Given continued wastewater injection into the upper Arbuckle in the Milan region, assessment of the middle Arbuckle as a hydraulic barrier remains an important research priority.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.3523C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.3523C"><span>Landslides and the <span class="hlt">Fault</span> Surface Ruptures during the 2008 Wengchuan <span class="hlt">Earthquake</span>, Sichuan, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chigira, M.; Xiyong, Wu; Takashi, Inokuchi; Gonghui, Wang</p> <p>2009-04-01</p> <p>2008 Sichuan <span class="hlt">earthquake</span> with a magnitude of Mw 7.9 induced numerous mass movements around the <span class="hlt">fault</span> surface ruptures of which maximum separations we observed were 3.6 m vertical and 1.5 m horizontal (right lateral). In order to clarify the distribution of these landslides and to characterize them, we interpreted satellite images and made field investigation for 3 weeks by using these images. We used satellite ALOS images taken by the sensors AVNIR II with a resolution of 10 m and PRISM with a resolution of 2.5 m, both of which were taken on 4th in June. We also used satellite images of before and after the <span class="hlt">earthquake</span> provided by Google Earth. The affected area was mountainous areas with elevations from 1000 m to 4500 m on the west of the Sichuan Basin. Ridges and valleys are generally trending NE parallel to the trends of the geologic structures, while large rivers, such as the Minjiang River, and the Fujiang River are flowing from the north or northwest to the south or southeast, crossing these trends. The NE-trending Longmenshan <span class="hlt">fault</span> zone runs along the boundary between the mountains and the Sichuan basin (He and Tsukuda, 2003), of which Yinghsiuwan-Beichuan <span class="hlt">fault</span> was the main <span class="hlt">fault</span> that generated the 2008 <span class="hlt">earthquake</span> (Xu, 2008). The basement rocks of the mountainous areas range from Precambrian to Cretaceous in age. They are basaltic rocks, granite, phyllite, dolostone, limestone, alternating beds of sandstone and shale, etc. (Geologic map of China). Landslide distribution areas were mainly of two types: One was the area along the <span class="hlt">fault</span> that generated this <span class="hlt">earthquake</span>, and another was along the steep slopes of inner valleys along the Minjian River. Landslides were concentrated on the hanging wall of the <span class="hlt">earthquake</span> <span class="hlt">fault</span>, which appeared for more than 180 km along the Longmenshan <span class="hlt">fault</span> zone. The distribution area of landslides was wider around the middle and the southwest parts of the surface rupture trace and became narrower to the northeast. The directions of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G52A..07F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G52A..07F"><span>Postseismic Deformation Following the 2002 Mw7.9 Denali <span class="hlt">Fault</span> <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Freymueller, J. T.; Harper, H.; Hu, Y.</p> <p>2017-12-01</p> <p>An Mw7.9 strike slip <span class="hlt">earthquake</span> struck on November 3, 2002, in central Alaska, rupturing 325 km of the Denali <span class="hlt">fault</span> and two other <span class="hlt">faults</span>. The <span class="hlt">earthquake</span> caused a strong postseismic transient that continues to have a substantial effect today. Distinguishing between different mechanisms of postseismic deformation (e.g., afterslip, viscoelastic relaxation) remains a challenging problem for many <span class="hlt">earthquakes</span>. Early studies done in the first few years after the Denali event demonstrated that the observed postseismic response could not be explained by a single mechanism, but estimates of the contributions of afterslip and viscoelastic relaxation were plagued by tradeoffs between unknown parameters. As a result, the postseismic models determined using the first few years of data did not predict the future observations well. We use a homogeneously reprocessed time series of GPS data from before and after the <span class="hlt">earthquake</span> to reassess the postseismic deformation using as much as 15 years of data after the event. We analyze the variations in the time series themselves to identify subsets of the data in space and time for which a single postseismic mechanism is dominant. We also assess tradeoffs between the imprecisely known "steady" deformation and the postseismic transient. We compute the postseismic deformation using finite element models including realistic 3D elastic and viscoelastic structures, including the impact of the dipping slab to the south of the Denali <span class="hlt">fault</span>, and constrain models based on the observations. Coseismic and postseismic models are self-consistent, using the same earth structure, which eliminates an inconsistency in the previous studies. We compare models in which the afterslip distribution is estimated empirically and models in which the afterslip distribution is determined by the coseismic stress changes. The empirical afterslip models show that there was no shallow afterslip, only deep afterslip. We then simulate afterslip using a shear zone with low</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.S42B0153E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.S42B0153E"><span>Istanbul <span class="hlt">Earthquake</span> Early Warning and Rapid Response <span class="hlt">System</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Erdik, M. O.; Fahjan, Y.; Ozel, O.; Alcik, H.; Aydin, M.; Gul, M.</p> <p>2003-12-01</p> <p>As part of the preparations for the future <span class="hlt">earthquake</span> in Istanbul a Rapid Response and Early Warning <span class="hlt">system</span> in the metropolitan area is in operation. For the Early Warning <span class="hlt">system</span> ten strong motion stations were installed as close as possible to the <span class="hlt">fault</span> zone. Continuous on-line data from these stations via digital radio modem provide early warning for potentially disastrous <span class="hlt">earthquakes</span>. Considering the complexity of <span class="hlt">fault</span> rupture and the short <span class="hlt">fault</span> distances involved, a simple and robust Early Warning algorithm, based on the exceedance of specified threshold time domain amplitude levels is implemented. The band-pass filtered accelerations and the cumulative absolute velocity (CAV) are compared with specified threshold levels. When any acceleration or CAV (on any channel) in a given station exceeds specific threshold values it is considered a vote. Whenever we have 2 station votes within selectable time interval, after the first vote, the first alarm is declared. In order to specify the appropriate threshold levels a data set of near field strong ground motions records form Turkey and the world has been analyzed. Correlations among these thresholds in terms of the epicenter distance the magnitude of the <span class="hlt">earthquake</span> have been studied. The encrypted early warning signals will be communicated to the respective end users by UHF <span class="hlt">systems</span> through a "service provider" company. The users of the early warning signal will be power and gas companies, nuclear research facilities, critical chemical factories, subway <span class="hlt">system</span> and several high-rise buildings. Depending on the location of the <span class="hlt">earthquake</span> (initiation of <span class="hlt">fault</span> rupture) and the recipient facility the alarm time can be as high as about 8s. For the rapid response <span class="hlt">system</span> one hundred 18 bit-resolution strong motion accelerometers were placed in quasi-free field locations (basement of small buildings) in the populated areas of the city, within an area of approximately 50x30km, to constitute a network that will enable early</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.bssaonline.org/content/84/3/799.abstract','USGSPUBS'); return false;" href="http://www.bssaonline.org/content/84/3/799.abstract"><span>Continuous borehole strain in the San Andreas <span class="hlt">fault</span> zone before, during, and after the 28 June 1992, MW 7.3 Landers, California, <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Johnston, M.J.S.; Linde, A.T.; Agnew, D.C.</p> <p>1994-01-01</p> <p>High-precision strain was observed with a borehole dilational strainmeter in the Devil's Punchbowl during the 11:58 UT 28 June 1992 MW 7.3 Landers <span class="hlt">earthquake</span> and the large Big Bear aftershock (MW 6.3). The strainmeter is installed at a depth of 176 m in the <span class="hlt">fault</span> zone approximately midway between the surface traces of the San Andreas and Punchbowl <span class="hlt">faults</span> and is about 100 km from the 85-km-long Landers rupture. We have questioned whether unusual amplified strains indicating precursive slip or high <span class="hlt">fault</span> compliance occurred on the <span class="hlt">faults</span> ruptured by the Landers <span class="hlt">earthquake</span>, or in the San Andreas <span class="hlt">fault</span> zone before and during the <span class="hlt">earthquake</span>, whether static offsets for both the Landers and Big Bear <span class="hlt">earthquakes</span> agree with expectation from geodetic and seismologic models of the ruptures and with observations from a nearby two-color geodimeter network, and whether postseismic behavior indicated continued slip on the Landers rupture or local triggered slip on the San Andreas. We show that the strain observed during the <span class="hlt">earthquake</span> at this instrument shows no apparent amplification effects. There are no indications of precursive strain in these strain data due to either local slip on the San Andreas or precursive slip on the eventual Landers rupture. The observations are generally consistent with models of the <span class="hlt">earthquake</span> in which <span class="hlt">fault</span> geometry and slip have the same form as that determined by either inversion of the seismic data or inversion of geodetically determined ground displacements produced by the <span class="hlt">earthquake</span>. Finally, there are some indications of minor postseismic behavior, particularly during the month following the <span class="hlt">earthquake</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026926','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026926"><span>Response of a 14-story Anchorage, Alaska, building in 2002 to two close <span class="hlt">earthquakes</span> and two distant Denali <span class="hlt">fault</span> <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Celebi, M.</p> <p>2004-01-01</p> <p>The recorded responses of an Anchorage, Alaska, building during four significant <span class="hlt">earthquakes</span> that occurred in 2002 are studied. Two <span class="hlt">earthquakes</span>, including the 3 November 2002 M7.9 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span>, with epicenters approximately 275 km from the building, generated long trains of long-period (>1 s) surface waves. The other two smaller <span class="hlt">earthquakes</span> occurred at subcrustal depths practically beneath Anchorage and produced higher frequency motions. These two pairs of <span class="hlt">earthquakes</span> have different impacts on the response of the building. Higher modes are more pronounced in the building response during the smaller nearby events. The building responses indicate that the close-coupling of translational and torsional modes causes a significant beating effect. It is also possible that there is some resonance occurring due to the site frequency being close to the structural frequency. Identification of dynamic characteristics and behavior of buildings can provide important lessons for future <span class="hlt">earthquake</span>-resistant designs and retrofit of existing buildings. ?? 2004, <span class="hlt">Earthquake</span> Engineering Research Institute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T41C0638P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T41C0638P"><span>Imaging the crustal structure of Haiti's transpressional <span class="hlt">fault</span> <span class="hlt">system</span> using seismicity and tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Possee, D.; Keir, D.; Harmon, N.; Rychert, C.; Rolandone, F.; Leroy, S. D.; Stuart, G. W.; Calais, E.; Boisson, D.; Ulysse, S. M. J.; Guerrier, K.; Momplaisir, R.; Prepetit, C.</p> <p>2017-12-01</p> <p>Oblique convergence of the Caribbean and North American plates has partitioned strain across an extensive transpressional <span class="hlt">fault</span> <span class="hlt">system</span> that bisects Haiti. Most recently the 2010, MW7.0 <span class="hlt">earthquake</span> ruptured multiple thrust <span class="hlt">faults</span> in southern Haiti. However, while the rupture mechanism has been well studied, how these <span class="hlt">faults</span> are segmented and link to deformation across the plate boundary is still debated. Understanding the link between strain accumulation and <span class="hlt">faulting</span> in Haiti is also key to future modelling of seismic hazards. To assess seismic activity and <span class="hlt">fault</span> structures we used data from 31 broadband seismic stations deployed on Haiti for 16-months. Local <span class="hlt">earthquakes</span> were recorded and hypocentre locations determined using a 1D velocity model. A high-quality subset of the data was then inverted using travel-time tomography for relocated hypocentres and 2D images of Vp and Vp/Vs crustal structure. <span class="hlt">Earthquake</span> locations reveal two clusters of seismic activity, the first delineates <span class="hlt">faults</span> associated with the 2010 <span class="hlt">earthquake</span> and the second shows activity 100km further east along a thrust <span class="hlt">fault</span> north of Lake Enriquillo (Dominican Republic). The velocity models show large variations in seismic properties across the plate boundary; shallow low-velocity zones with a 5-8% decrease in Vp and high Vp/Vs ratios of 1.85-1.95 correspond to sedimentary basins that form the low-lying terrain on Haiti. We also image a region with a 4-5% decrease in Vp and an increased Vp/Vs ratio of 1.80-1.85 dipping south to a depth of 20km beneath southern Haiti. This feature matches the location of a major thrust <span class="hlt">fault</span> and suggests a substantial damage zone around this <span class="hlt">fault</span>. Beneath northern Haiti a transition to lower Vp/Vs values of 1.70-1.75 reflects a compositional change from mafic facies such as the Caribbean large igneous province in the south, to arc magmatic facies associated with the Greater Antilles arc in the north. Our seismic images are consistent with the <span class="hlt">fault</span> <span class="hlt">system</span> across</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017260','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017260"><span>Creep, compaction and the weak rheology of major <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sleep, Norman H.; Blanpied, M.L.</p> <p>1992-01-01</p> <p>Field and laboratory observations suggest that the porosity within <span class="hlt">fault</span> zones varies over <span class="hlt">earthquake</span> cycles so that fluid pressure is in long-term equilibrium with hydrostatic fluid pressure in the country rock. Between <span class="hlt">earthquakes</span>, ductile creep compacts the <span class="hlt">fault</span> zone, increasing fluid pressure, and finally allowing frictional failure at relatively low shear stress. <span class="hlt">Earthquake</span> <span class="hlt">faulting</span> restores porosity and decreases fluid pressure to below hydrostatic. This mechanism may explain why major <span class="hlt">faults</span>, such as the San Andreas <span class="hlt">system</span>, are weak.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMNG13A1860S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMNG13A1860S"><span>The Virtual Quake <span class="hlt">Earthquake</span> Simulator: <span class="hlt">Earthquake</span> Probability Statistics for the El Mayor-Cucapah Region and Evidence of Predictability in Simulated <span class="hlt">Earthquake</span> Sequences</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schultz, K.; Yoder, M. R.; Heien, E. M.; Rundle, J. B.; Turcotte, D. L.; Parker, J. W.; Donnellan, A.</p> <p>2015-12-01</p> <p>We introduce a framework for developing <span class="hlt">earthquake</span> forecasts using Virtual Quake (VQ), the generalized successor to the perhaps better known Virtual California (VC) <span class="hlt">earthquake</span> simulator. We discuss the basic merits and mechanics of the simulator, and we present several statistics of interest for <span class="hlt">earthquake</span> forecasting. We also show that, though the <span class="hlt">system</span> as a whole (in aggregate) behaves quite randomly, (simulated) <span class="hlt">earthquake</span> sequences limited to specific <span class="hlt">fault</span> sections exhibit measurable predictability in the form of increasing seismicity precursory to large m > 7 <span class="hlt">earthquakes</span>. In order to quantify this, we develop an alert based forecasting metric similar to those presented in Keilis-Borok (2002); Molchan (1997), and show that it exhibits significant information gain compared to random forecasts. We also discuss the long standing question of activation vs quiescent type <span class="hlt">earthquake</span> triggering. We show that VQ exhibits both behaviors separately for independent <span class="hlt">fault</span> sections; some <span class="hlt">fault</span> sections exhibit activation type triggering, while others are better characterized by quiescent type triggering. We discuss these aspects of VQ specifically with respect to <span class="hlt">faults</span> in the Salton Basin and near the El Mayor-Cucapah region in southern California USA and northern Baja California Norte, Mexico.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175906','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175906"><span>Seismicity, <span class="hlt">faulting</span>, and structure of the Koyna-Warna seismic region, Western India from local <span class="hlt">earthquake</span> tomography and hypocenter locations</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dixit, Madan M.; Kumar, Sanjay; Catchings, Rufus D.; Suman, K.; Sarkar, Dipankar; Sen, M.K.</p> <p>2014-01-01</p> <p>Although seismicity near Koyna Reservoir (India) has persisted for ~50 years and includes the largest induced <span class="hlt">earthquake</span> (M 6.3) reported worldwide, the seismotectonic framework of the area is not well understood. We recorded ~1800 <span class="hlt">earthquakes</span> from 6 January 2010 to 28 May 2010 and located a subset of 343 of the highest-quality <span class="hlt">earthquakes</span> using the tomoDD code of Zhang and Thurber (2003) to better understand the framework. We also inverted first arrivals for 3-D Vp, Vs, and Vp/Vs and Poisson's ratio tomography models of the upper 12 km of the crust. Epicenters for the recorded <span class="hlt">earthquakes</span> are located south of the Koyna River, including a high-density cluster that coincides with a shallow depth (<1.5 km) zone of relatively high Vp and low Vs (also high Vp/Vs and Poisson's ratios) near Warna Reservoir. This anomalous zone, which extends near vertically to at least 8 km depth and laterally northward at least 15 km, is likely a water-saturated zone of <span class="hlt">faults</span> under high pore pressures. Because many of the <span class="hlt">earthquakes</span> occur on the periphery of the <span class="hlt">fault</span> zone, rather than near its center, the observed seismicity-velocity correlations are consistent with the concept that many of the <span class="hlt">earthquakes</span> nucleate in fractures adjacent to the main <span class="hlt">fault</span> zone due to high pore pressure. We interpret our velocity images as showing a series of northwest trending <span class="hlt">faults</span> locally near the central part of Warna Reservoir and a major northward trending <span class="hlt">fault</span> zone north of Warna Reservoir.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8782A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8782A"><span>Dynamic modeling of normal <span class="hlt">faults</span> of the 2016 Central Italy <span class="hlt">earthquake</span> sequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aochi, Hideo</p> <p>2017-04-01</p> <p>The <span class="hlt">earthquake</span> sequence of the Central Italy in 2016 are characterized mainly by the Mw6.0 24th August, Mw5.9 26th October and Mw6.4 30th October as well as two Mw5.4 <span class="hlt">earthquakes</span> (24th August, 26th October) (catalogue INGV). They all show normal <span class="hlt">faulting</span> mechanisms corresponding to the Apennines's tectonics. They are aligned briefly along NNW-SSE axis, and they may not be on a single continuous <span class="hlt">fault</span> plane. Therefore, dynamic rupture modeling of sequences should be carried out supposing co-planar normal multiple segments. We apply a Boundary Domain Method (BDM, Goto and Bielak, GJI, 2008) coupling a boundary integral equation method and a domain-based method, namely a finite difference method in this study. The Mw6.0 24th August <span class="hlt">earthquake</span> is modeled. We use the basic information of hypocenter position, focal mechanism and potential ruptured dimension from the INGV catalogue and Tinti et al., GRL, 2016), and begin with a simple condition (homogeneous boundary condition). From our preliminary simulations, it is shown that a uniformly extended rupture model does not fit the near-field ground motions and localized heterogeneity would be required.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032823','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032823"><span><span class="hlt">Earthquake-by-earthquake</span> fold growth above the Puente Hills blind thrust <span class="hlt">fault</span>, Los Angeles, California: Implications for fold kinematics and seismic hazard</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Leon, L.A.; Christofferson, S.A.; Dolan, J.F.; Shaw, J.H.; Pratt, T.L.</p> <p>2007-01-01</p> <p>Boreholes and high-resolution seismic reflection data collected across the forelimb growth triangle above the central segment of the Puente Hills thrust <span class="hlt">fault</span> (PHT) beneath Los Angeles, California, provide a detailed record of incremental fold growth during large <span class="hlt">earthquakes</span> on this major blind thrust <span class="hlt">fault</span>. These data document fold growth within a discrete kink band that narrows upward from ???460 m at the base of the Quaternary section (200-250 m depth) to 82% at 250 m depth) folding and uplift occur within discrete kink bands, thereby enabling us to develop a paleoseismic history of the underlying blind thrust <span class="hlt">fault</span>. The borehole data reveal that the youngest part of the growth triangle in the uppermost 20 m comprises three stratigraphically discrete growth intervals marked by southward thickening sedimentary strata that are separated by intervals in which sediments do not change thickness across the site. We interpret the intervals of growth as occurring after the formation of now-buried paleofold scarps during three large PHT <span class="hlt">earthquakes</span> in the past 8 kyr. The intervening intervals of no growth record periods of structural quiescence and deposition at the regional, near-horizontal stream gradient at the study site. Minimum uplift in each of the scarp-forming events, which occurred at 0.2-2.2 ka (event Y), 3.0-6.3 ka (event X), and 6.6-8.1 ka (event W), ranged from ???1.1 to ???1.6 m, indicating minimum thrust displacements of ???2.5 to 4.5 m. Such large displacements are consistent with the occurrence of large-magnitude <span class="hlt">earthquakes</span> (Mw > 7). Cumulative, minimum uplift in the past three events was 3.3 to 4.7 m, suggesting cumulative thrust displacement of ???7 to 10.5 m. These values yield a minimum Holocene slip rate for the PHT of ???0.9 to 1.6 mm/yr. The borehole and seismic reflection data demonstrate that dip within the kink band is acquired incrementally, such that older strata that have been deformed by more <span class="hlt">earthquakes</span> dip more steeply than younger</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Tectp.691..375V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Tectp.691..375V"><span>New constraints shed light on strike-slip <span class="hlt">faulting</span> beneath the southern Apennines (Italy): The 21 August 1962 Irpinia multiple <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vannoli, Paola; Bernardi, Fabrizio; Palombo, Barbara; Vannucci, Gianfranco; Console, Rodolfo; Ferrari, Graziano</p> <p>2016-11-01</p> <p>On 21 August 1962 an <span class="hlt">earthquake</span> sequence set off near the city of Benevento, in Italy's southern Apennines. Three <span class="hlt">earthquakes</span>, the largest having Mw 6.1, struck virtually the same area in less than 40 min (at 18:09, 18:19 and 18:44 UTC, respectively). Several historical <span class="hlt">earthquakes</span> hit this region, and its seismic hazard is accordingly among the highest countrywide. Although poorly understood in the past, the seismotectonics of this region can be revealed by the 1962 sequence, being the only significant <span class="hlt">earthquake</span> in the area for which modern seismograms are available. We determine location, magnitude, and nodal planes of the first event (18:09 UTC) of the sequence. The focal mechanism exhibits dominant strike-slip rupture along a north-dipping, E-W striking plane or along a west-dipping, N-S striking plane. Either of these solutions is significantly different from the kinematics of the typical large <span class="hlt">earthquakes</span> occurring along the crest of the Southern Apennines, such as the 23 November 1980 Irpinia <span class="hlt">earthquake</span> (Mw 6.9), caused by predominant normal <span class="hlt">faulting</span> along NW-SE-striking planes. The epicentre of the 21 August 1962, 18:09 event is located immediately east of the chain axis, near one of the three north-dipping, E-W striking oblique-slip sources thought to have caused one of the three main events of the December 1456 sequence (Io XI MCS), the most destructive events in the southern Apennines known to date. We maintain that the 21 August 1962, 18:09 <span class="hlt">earthquake</span> occurred along the E-W striking <span class="hlt">fault</span> <span class="hlt">system</span> responsible for the southernmost event of the 1456 sequence and for two smaller but instrumentally documented events that occurred on 6 May 1971 (Mw 5.0) and 27 September 2012 (Mw 4.6), further suggesting that normal <span class="hlt">faulting</span> is not the dominant tectonic style in this portion of the Italian peninsula.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025485','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025485"><span>Imaging the complexity of an active normal <span class="hlt">fault</span> <span class="hlt">system</span>: The 1997 Colfiorito (central Italy) case study</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Chiaraluce, L.; Ellsworth, W.L.; Chiarabba, C.; Cocco, M.</p> <p>2003-01-01</p> <p>Six moderate magnitude <span class="hlt">earthquakes</span> (5 < Mw < 6) ruptured normal <span class="hlt">fault</span> segments of the southern sector of the North Apennine belt (central Italy) in the 1997 Colfiorito <span class="hlt">earthquake</span> sequence. We study the progressive activation of adjacent and nearby parallel <span class="hlt">faults</span> of this complex normal <span class="hlt">fault</span> <span class="hlt">system</span> using ???1650 <span class="hlt">earthquake</span> locations obtained by applying a double-difference location method, using travel time picks and waveform cross-correlation measurements. The lateral extent of the <span class="hlt">fault</span> segments range from 5 to 10 km and make up a broad, ???45 km long, NW trending <span class="hlt">fault</span> <span class="hlt">system</span>. The geometry of each segment is quite simple and consists of planar <span class="hlt">faults</span> gently dipping toward SW with an average dip of 40??-45??. The <span class="hlt">fault</span> planes are not listric but maintain a constant dip through the entire seismogenic volume, down to 8 km depth. We observe the activation of <span class="hlt">faults</span> on the hanging wall and the absence of seismicity in the footwall of the structure. The observed <span class="hlt">fault</span> segmentation appears to be due to the lateral heterogeneity of the upper crust: preexisting thrusts inherited from Neogene's compressional tectonic intersect the active normal <span class="hlt">faults</span> and control their maximum length. The stress tensor obtained by inverting the six main shock focal mechanisms of the sequence is in agreement with the tectonic stress active in the inner chain of the Apennine, revealing a clear NE trending extension direction. Aftershock focal mechanisms show a consistent extensional kinematics, 70% of which are mechanically consistent with the main shock stress field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T22B..08H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T22B..08H"><span>3D Constraints On <span class="hlt">Fault</span> Architecture and Strain Distribution of the Newport-Inglewood Rose Canyon and San Onofre Trend <span class="hlt">Fault</span> <span class="hlt">Systems</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holmes, J. J.; Driscoll, N. W.; Kent, G. M.</p> <p>2017-12-01</p> <p>The Inner California Borderlands (ICB) is situated off the coast of southern California and northern Baja. The structural and geomorphic characteristics of the area record a middle Oligocene transition from subduction to microplate capture along the California coast. Marine stratigraphic evidence shows large-scale extension and rotation overprinted by modern strike-slip deformation. Geodetic and geologic observations indicate that approximately 6-8 mm/yr of Pacific-North American relative plate motion is accommodated by offshore strike-slip <span class="hlt">faulting</span> in the ICB. The farthest inshore <span class="hlt">fault</span> <span class="hlt">system</span>, the Newport-Inglewood Rose Canyon (NIRC) <span class="hlt">Fault</span> is a dextral strike-slip <span class="hlt">system</span> that is primarily offshore for approximately 120 km from San Diego to the San Joaquin Hills near Newport Beach, California. Based on trenching and well data, the NIRC <span class="hlt">Fault</span> Holocene slip rate is 1.5-2.0 mm/yr to the south and 0.5-1.0 mm/yr along its northern extent. An <span class="hlt">earthquake</span> rupturing the entire length of the <span class="hlt">system</span> could produce an Mw 7.0 <span class="hlt">earthquake</span> or larger. West of the main segments of the NIRC <span class="hlt">Fault</span> is the San Onofre Trend (SOT) along the continental slope. Previous work concluded that this is part of a strike-slip <span class="hlt">system</span> that eventually merges with the NIRC <span class="hlt">Fault</span>. Others have interpreted this <span class="hlt">system</span> as deformation associated with the Oceanside Blind Thrust <span class="hlt">Fault</span> purported to underlie most of the region. In late 2013, we acquired the first high-resolution 3D Parallel Cable (P-Cable) seismic surveys of the NIRC and SOT <span class="hlt">faults</span> as part of the Southern California Regional <span class="hlt">Fault</span> Mapping project. Analysis of stratigraphy and 3D mapping of this new data has yielded a new kinematic <span class="hlt">fault</span> model of the area that provides new insight on deformation caused by interactions in both compressional and extensional regimes. For the first time, we can reconstruct <span class="hlt">fault</span> interaction and investigate how strain is distributed through time along a typical strike-slip margin using 3D constraints on <span class="hlt">fault</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037700','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037700"><span>Evidence for a twelfth large <span class="hlt">earthquake</span> on the southern hayward <span class="hlt">fault</span> in the past 1900 years</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lienkaemper, J.J.; Williams, P.L.; Guilderson, T.P.</p> <p>2010-01-01</p> <p>We present age and stratigraphic evidence for an additional paleoearthquake at the Tyson Lagoon site. The acquisition of 19 additional radiocarbon dates and the inclusion of this additional event has resolved a large age discrepancy in our earlier <span class="hlt">earthquake</span> chronology. The age of event E10 was previously poorly constrained, thus increasing the uncertainty in the mean recurrence interval (RI), a critical factor in seismic hazard evaluation. Reinspection of many trench logs revealed substantial evidence suggesting that an additional <span class="hlt">earthquake</span> occurred between E10 and E9 within unit u45. Strata in older u45 are <span class="hlt">faulted</span> in the main <span class="hlt">fault</span> zone and overlain by scarp colluviums in two locations.We conclude that an additional surfacerupturing event (E9.5) occurred between E9 and E10. Since 91 A.D. (??40 yr, 1??), 11 paleoearthquakes preceded the M 6:8 <span class="hlt">earthquake</span> in 1868, yielding a mean RI of 161 ?? 65 yr (1??, standard deviation of recurrence intervals). However, the standard error of the mean (SEM) is well determined at ??10 yr. Since ~1300 A.D., the mean rate has increased slightly, but is indistinguishable from the overall rate within the uncertainties. Recurrence for the 12-event sequence seems fairly regular: the coefficient of variation is 0.40, and it yields a 30-yr <span class="hlt">earthquake</span> probability of 29%. The apparent regularity in timing implied by this <span class="hlt">earthquake</span> chronology lends support for the use of time-dependent renewal models rather than assuming a random process to forecast <span class="hlt">earthquakes</span>, at least for the southern Hayward <span class="hlt">fault</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T11A4545R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T11A4545R"><span>Aftershock source properties of events following the 2013 Craig <span class="hlt">Earthquake</span>: new evidence for structural heterogeneity on the northern Queen Charlotte <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roland, E. C.; Walton, M. A. L.; Ruppert, N. A.; Gulick, S. P. S.; Christeson, G. L.; Haeussler, P. J.</p> <p>2014-12-01</p> <p>In January 2013, a Mw 7.5 <span class="hlt">earthquake</span> ruptured a segment of the Queen Charlotte <span class="hlt">Fault</span> offshore the town of Craig in southeast Alaska. The region of the <span class="hlt">fault</span> that slipped during the Craig <span class="hlt">earthquake</span> is adjacent to and possibly overlapping with the northern extent of the 1949 M 8.1 Queen Charlotte <span class="hlt">earthquake</span> rupture (Canada's largest recorded <span class="hlt">earthquake</span>), and is just south of the rupture area of the 1972 M 7.6 <span class="hlt">earthquake</span> near Sitka, Alaska. Here we present aftershock locations and focal mechanisms for events that occurred four months following the mainshock using data recorded on an Ocean Bottom Seismometer (OBS) array that was deployed offshore of Prince of Wales Island. This array consisted of 9 short period instruments surrounding the <span class="hlt">fault</span> segment, and recorded hundreds of aftershocks during the months of April and May, 2013. In addition to highlighting the primary mainshock rupture plane, aftershocks also appear to be occurring along secondary <span class="hlt">fault</span> structures adjacent to the main <span class="hlt">fault</span> trace, illuminating complicated structure, particularly toward the northern extent of the Craig rupture. Focal mechanisms for the larger events recorded during the OBS deployment show both near-vertical strike slip motion consistent with the mainshock mechanism, as well as events with varying strike and a component of normal <span class="hlt">faulting</span>. Although <span class="hlt">fault</span> structure along this northern segment of the QCF appears to be considerably simpler than to the south, where a higher degree of oblique convergence leads to sub-parallel compressional deformation structures, secondary <span class="hlt">faulting</span> structures apparent in legacy seismic reflection data near the Craig rupture may be consistent with the observed seismicity patterns. In combination, these data may help to characterize structural heterogeneity along the northern segment of the Queen Charlotte <span class="hlt">Fault</span> that contributes to rupture segmentation during large strike slip events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T31G..03F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T31G..03F"><span><span class="hlt">Earthquake</span>-driven fluid flow rates inferred from borehole temperature measurements within the Japan Trench plate boundary <span class="hlt">fault</span> zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fulton, P. M.; Brodsky, E. E.</p> <p>2016-12-01</p> <p>Using borehole sub-seafloor temperature measurements, we have recently identified signatures suggestive of <span class="hlt">earthquake</span>-driven fluid pulses within the Japan Trench plate boundary <span class="hlt">fault</span> zone during a major aftershock sequence. Here we use numerical models to show that these signatures are consistent with time-varying fluid flow rates out of permeable zones within the formation into the borehole annulus. In addition, we also identify an apparent time-varying sensitivity of whether suspected fluid pulses occur in response to <span class="hlt">earthquakes</span> of a given magnitude and distance. The results suggest a damage and healing process and therefore provides a mechanism to allow for a disproportionate amount of heat and chemical transport in the short time frame after an <span class="hlt">earthquake</span>. Our observations come from an observatory installed across the main plate boundary <span class="hlt">fault</span> as part of IODP's Japan Trench Fast Drilling Project (JFAST) following the March 2011 Mw 9.0 Tohoku-oki <span class="hlt">earthquake</span>. It operated from July 2012 - April 2013 during which a Mw 7.3 <span class="hlt">earthquake</span> and numerous aftershocks occurred. High-resolution temperature time series data reveal spatially correlated transients in response to <span class="hlt">earthquakes</span> with distinct patterns interpreted to reflect advection by transient pulses of fluid flow from permeable zones into the borehole annulus. Typical transients involve perturbations over 12 m with increases of 10 mK that build over 0.1 days at shallower depths and decreases at deeper depths. They are consistently centered around 792.5 m below seafloor (mbsf) where a secondary <span class="hlt">fault</span> and permeable zone have been independently identified within the damage zone above the main plate boundary <span class="hlt">fault</span> at 820 mbsf . Model simulations suggest transient flow rates of up to 10-3m/s from the formation that quickly decrease. Comparison of characteristics of <span class="hlt">earthquakes</span> identified in nearby ocean bottom pressure measurements suggest there is not a clear relationship between fluid pulses and static strain. There</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70191663','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191663"><span>A decade of induced slip on the causative <span class="hlt">fault</span> of the 2015 Mw 4.0 Venus <span class="hlt">earthquake</span>, northeast Johnson County, Texas</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Scales, Monique M.; DeShon, Heather R.; Magnani, M. Beatrice; Walter, Jacob I.; Quinones, Louis; Pratt, Thomas L.; Hornbach, Matthew J.</p> <p>2017-01-01</p> <p>On 7 May 2015, a Mw 4.0 <span class="hlt">earthquake</span> occurred near Venus, northeast Johnson County, Texas, in an area of the Bend Arch-Fort Worth Basin that reports long-term, high-volume wastewater disposal and that has hosted felt <span class="hlt">earthquakes</span> since 2009. In the weeks following the Mw 4.0 <span class="hlt">earthquake</span>, we deployed a local seismic network and purchased nearby active-source seismic reflection data to capture additional events, characterize the causative <span class="hlt">fault</span>, and explore potential links between ongoing industry activity and seismicity. Hypocenter relocations of the resulting local <span class="hlt">earthquake</span> catalog span ~4–6 km depth and indicate a <span class="hlt">fault</span> striking ~230°, dipping to the west, consistent with a nodal plane of the Mw 4.0 regional moment tensor. <span class="hlt">Fault</span> plane solutions indicate normal <span class="hlt">faulting</span>, with B axes striking parallel to maximum horizontal compressive stress. Seismic reflection data image the reactivated basement <span class="hlt">fault</span> penetrating the Ordovician disposal layer and Mississippian production layer, but not displacing post-Lower Pennsylvanian units. Template matching at regional seismic stations indicates that low-magnitude <span class="hlt">earthquakes</span> with similar waveforms began in April 2008, with increasing magnitude over time. Pressure data from five saltwater disposal wells within 5 km of the active <span class="hlt">fault</span> indicate a disposal formation that is 0.9–4.8 MPa above hydrostatic. We suggest that the injection of 28,000,000 m3 of wastewater between 2006 and 2015 at these wells led to an increase in subsurface pore fluid pressure that contributed to inducing this long-lived <span class="hlt">earthquake</span> sequence. The 2015 Mw 4.0 event represents the largest event in the continuing evolution of slip on the causative <span class="hlt">fault</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JSeis..11..311A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JSeis..11..311A"><span>Revised seismic history of the El Pilar <span class="hlt">fault</span>, Northeastern Venezuela, from the Cariaco 1997 <span class="hlt">earthquake</span> and recent preliminary paleoseismic results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Audemard, Franck A.</p> <p>2007-07-01</p> <p>In light of the July 9, 1997, Cariaco <span class="hlt">earthquake</span>, it is clearly understood now that damage in the city of Cumaná located in northeastern Venezuela and frequently destroyed by the largest <span class="hlt">earthquakes</span> since the first recorded event in 1530 is strongly enhanced by poor soil conditions that, in turn, are responsible for site amplification and widespread <span class="hlt">earthquake</span>-induced effects. Therefore, most previous macroseismic studies of historical <span class="hlt">earthquakes</span> must be revaluated because those localized high-intensity values at Cumaná surely led to the misestimation of past epicenters. Preliminary paleoseismic results, gathered at three exploratory trenches dug across the surface break of the Cariaco 1997 <span class="hlt">earthquake</span> in 1998, allow us to associate the 1684 <span class="hlt">earthquake</span> with this recently ruptured <span class="hlt">fault</span> segment that extends between the towns of San Antonio del Golfo and Río Casanay (roughly between the two gulfs of Cariaco and Paria, state of Sucre). Other major results from the reassessment of the seismic history of this <span class="hlt">fault</span> are: (a) the 1766 event seems to have generated in a different source to the El Pilar <span class="hlt">fault</span> because the size of the felt area suggests that it is an intermediate-depth <span class="hlt">earthquake</span>; (b) damage to Cumaná produced by the 1797 event suggests that this was a local <span class="hlt">earthquake</span>, perhaps equivalent to the 1929 <span class="hlt">earthquake</span>, which ruptured for some 30 km just east of Cumaná into the Gulf of Cariaco; and (c) seismogenic association of the 1530 and 1853 <span class="hlt">earthquakes</span> still remains unclear but it is very likely that these ruptures occurred offshore, as suggested by the rather large tsunami waves that both events have generated, placing their hypocenters west of Cumaná in the Cariaco Trough. This reassessment also sheds light into the El Pilar <span class="hlt">fault</span> segmentation and the behavior of its seismogenic barriers through time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17778631','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17778631"><span>Outward-dipping ring-<span class="hlt">fault</span> structure at rabaul caldera as shown by <span class="hlt">earthquake</span> locations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mori, J; McKee, C</p> <p>1987-01-09</p> <p>The locations of a large number of <span class="hlt">earthquakes</span> recorded at Rabaul caldera in Papua New Guinea from late 1983 to mid-1985 have produced a picture of this active caldera's structural boundary. The <span class="hlt">earthquake</span> epicenters form an elliptical annulus about 10 kilometers long by 4 kilometers wide, centered in the southern part of the Rabaul volcanic complex. A set of events with well-constrained depth determinations shows a ring-<span class="hlt">fault</span> structure that extends from the surface to a depth of about 4 kilometers and slopes steeply outward from the center of the caldera. This is the first geophysical data set that clearly outlines the orientation of an active caldera's bounding <span class="hlt">faults</span>. This orientation, however, conflicts with the configuration of many other calderas and is not in keeping with currently preferred models of caldera formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.3923G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.3923G"><span>Nonlinear waves in earth crust <span class="hlt">faults</span>: application to regular and slow <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gershenzon, Naum; Bambakidis, Gust</p> <p>2015-04-01</p> <p>The genesis, development and cessation of regular <span class="hlt">earthquakes</span> continue to be major problems of modern geophysics. How are <span class="hlt">earthquakes</span> initiated? What factors determine the rapture velocity, slip velocity, rise time and geometry of rupture? How do accumulated stresses relax after the main shock? These and other questions still need to be answered. In addition, slow slip events have attracted much attention as an additional source for monitoring <span class="hlt">fault</span> dynamics. Recently discovered phenomena such as deep non-volcanic tremor (NVT), low frequency <span class="hlt">earthquakes</span> (LFE), very low frequency <span class="hlt">earthquakes</span> (VLF), and episodic tremor and slip (ETS) have enhanced and complemented our knowledge of <span class="hlt">fault</span> dynamic. At the same time, these phenomena give rise to new questions about their genesis, properties and relation to regular <span class="hlt">earthquakes</span>. We have developed a model of macroscopic dry friction which efficiently describes laboratory frictional experiments [1], basic properties of regular <span class="hlt">earthquakes</span> including post-seismic stress relaxation [3], the occurrence of ambient and triggered NVT [4], and ETS events [5, 6]. Here we will discuss the basics of the model and its geophysical applications. References [1] Gershenzon N.I. & G. Bambakidis (2013) Tribology International, 61, 11-18, http://dx.doi.org/10.1016/j.triboint.2012.11.025 [2] Gershenzon, N.I., G. Bambakidis and T. Skinner (2014) Lubricants 2014, 2, 1-x manuscripts; doi:10.3390/lubricants20x000x; arXiv:1411.1030v2 [3] Gershenzon N.I., Bykov V. G. and Bambakidis G., (2009) Physical Review E 79, 056601 [4] Gershenzon, N. I, G. Bambakidis, (2014a), Bull. Seismol. Soc. Am., 104, 4, doi: 10.1785/0120130234 [5] Gershenzon, N. I.,G. Bambakidis, E. Hauser, A. Ghosh, and K. C. Creager (2011), Geophys. Res. Lett., 38, L01309, doi:10.1029/2010GL045225. [6] Gershenzon, N.I. and G. Bambakidis (2014) Bull. Seismol. Soc. Am., (in press); arXiv:1411.1020</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.8510Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.8510Z"><span>Source parameters of the 2013, Ms 7.0, Lushan <span class="hlt">earthquake</span> and the characteristics of the near-<span class="hlt">fault</span> strong ground motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Fengfan; Meng, Lingyuan</p> <p>2016-04-01</p> <p>The April 20, 2013 Ms 7.0, <span class="hlt">earthquake</span> in Lushan city, Sichuan province of China occurred as the result of east-west oriented reverse-type motion on a north-south striking <span class="hlt">fault</span>. The source location suggests the event occurred on the Southern part of Longmenshan <span class="hlt">fault</span> at a depth of 13km. The maximum intensity is up to VIII to IX at Boxing and Lushan city, which are located in the meizoseismal area. In this study, we analyzed the dynamic source process with the source mechanism and empirical relationships, estimated the strong ground motion in the near-<span class="hlt">fault</span> field based on the Brune's circle model. A dynamical composite source model (DCSM) has been developed to simulate the near-<span class="hlt">fault</span> strong ground motion with associated <span class="hlt">fault</span> rupture properties at Boxing and Lushan city, respectively. The results indicate that the frictional undershoot behavior in the dynamic source process of Lushan <span class="hlt">earthquake</span>, which is actually different from the overshoot activity of the Wenchuan <span class="hlt">earthquake</span>. Moreover, we discussed the characteristics of the strong ground motion in the near-<span class="hlt">fault</span> field, that the broadband synthetic seismogram ground motion predictions for Boxing and Lushan city produced larger peak values, shorter durations and higher frequency contents. It indicates that the factors in near-<span class="hlt">fault</span> strong ground motion was under the influence of higher effect stress drop and asperity slip distributions on the <span class="hlt">fault</span> plane. This work is financially supported by the Natural Science Foundation of China (Grant No. 41404045) and by Science for <span class="hlt">Earthquake</span> Resilience of CEA (XH14055Y).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1513800L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1513800L"><span>Development of fluid overpressures in crustal <span class="hlt">faults</span> and implications for <span class="hlt">earthquakes</span> mechanics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leclère, Henri; Cappa, Frédéric; Faulkner, Daniel; Armitage, Peter; Blake, Oshaine; Fabbri, Olivier</p> <p>2013-04-01</p> <p>The development and maintenance of fluid overpressures strongly influence the mechanical behavior of the crust and especially crustal <span class="hlt">fault</span> zones. The mechanisms allowing fluid pressure build-up are still open questions, and their influence on tectonic and <span class="hlt">fault</span> weakening processes remain unclear. The determination of the hydraulic and mechanical properties of crustal <span class="hlt">fault</span> zone elements is a key aspect to improve our understanding of the fluid-tectonic interactions and more particularly the role of fluids in <span class="hlt">fault</span> mechanics and <span class="hlt">earthquake</span> triggering. Here we address this question combining geological observations, laboratory experiments and hydromechanical models of an active crustal <span class="hlt">fault</span>-zone in the Ubaye-Argentera area (southeastern France). Previous studies showed that the fluids located in the <span class="hlt">fault</span> zone developed overpressures between 7 and 26 MPa, that triggered intense seismic swarms (i.e. 16,000 events in 2003-2004) (Jenatton et al., 2007; Daniel et al., 2011; Leclère et al., 2012). The <span class="hlt">fault</span>-zone studied here is located in the Argentera external crystalline massif and is connected to regional NW-SE steeply-dipping dextral strike-slip <span class="hlt">faults</span> with an offset of several kilometers. The <span class="hlt">fault</span> zone cuts through migmatitic gneisses composed of quartz, K-feldspar, plagioclase, biotite and minor muscovite. It exposes several anastomosed core zones surrounded by damage zones with a pluri-decametric total width. The core zones are made up of centimetric to pluridecimetric phyllosilicate-rich gouge layers while the damage zones are composed of pluri-metric phyllonitic rock derived from mylonite. The permeability and elastic moduli of the host rock, damage zone and <span class="hlt">fault</span> core were measured from plugs with a diameter of 20 mm and lengths between 26 to 51 mm, using a high-pressure hydrostatic fluid-flow apparatus. Measurements were made with confining pressures ranging from 30 to 210 MPa and using argon pore fluid pressure of 20 MPa. Data show a variation of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T31A0603S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T31A0603S"><span><span class="hlt">Earthquake</span> Clusters and Spatio-temporal Migration of <span class="hlt">earthquakes</span> in Northeastern Tibetan Plateau: a Finite Element Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Y.; Luo, G.</p> <p>2017-12-01</p> <p>Seismicity in a region is usually characterized by <span class="hlt">earthquake</span> clusters and <span class="hlt">earthquake</span> migration along its major <span class="hlt">fault</span> zones. However, we do not fully understand why and how <span class="hlt">earthquake</span> clusters and spatio-temporal migration of <span class="hlt">earthquakes</span> occur. The northeastern Tibetan Plateau is a good example for us to investigate these problems. In this study, we construct and use a three-dimensional viscoelastoplastic finite-element model to simulate <span class="hlt">earthquake</span> cycles and spatio-temporal migration of <span class="hlt">earthquakes</span> along major <span class="hlt">fault</span> zones in northeastern Tibetan Plateau. We calculate stress evolution and <span class="hlt">fault</span> interactions, and explore effects of topographic loading and viscosity of middle-lower crust and upper mantle on model results. Model results show that <span class="hlt">earthquakes</span> and <span class="hlt">fault</span> interactions increase Coulomb stress on the neighboring <span class="hlt">faults</span> or segments, accelerating the future <span class="hlt">earthquakes</span> in this region. Thus, <span class="hlt">earthquakes</span> occur sequentially in a short time, leading to regional <span class="hlt">earthquake</span> clusters. Through long-term evolution, stresses on some seismogenic <span class="hlt">faults</span>, which are far apart, may almost simultaneously reach the critical state of <span class="hlt">fault</span> failure, probably also leading to regional <span class="hlt">earthquake</span> clusters and <span class="hlt">earthquake</span> migration. Based on our model synthetic seismic catalog and paleoseismic data, we analyze probability of <span class="hlt">earthquake</span> migration between major <span class="hlt">faults</span> in northeastern Tibetan Plateau. We find that following the 1920 M 8.5 Haiyuan <span class="hlt">earthquake</span> and the 1927 M 8.0 Gulang <span class="hlt">earthquake</span>, the next big event (M≥7) in northeastern Tibetan Plateau would be most likely to occur on the Haiyuan <span class="hlt">fault</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026986','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026986"><span>Landslides triggered by the 2002 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span> and the inferred nature of the strong shaking</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jibson, R.W.; Harp, E.L.; Schulz, W.; Keefer, D.K.</p> <p>2004-01-01</p> <p>The 2002 M7.9 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span> triggered thousands of landslides, primarily rock falls and rock slides, that ranged in volume from rock falls of a few cubic meters to rock avalanches having volumes as great as 15 ?? 106 m3. The pattern of landsliding was unusual; the number of slides was less than expected for an <span class="hlt">earthquake</span> of this magnitude, and the landslides were concentrated in a narrow zone 30-km wide that straddled the <span class="hlt">fault</span> rupture over its entire 300-km length. The large rock avalanches all clustered along the western third of the rupture zone where acceleration levels and ground-shaking frequencies are thought to have been the highest. Inferences about near-field strong shaking characteristics drawn from the interpretation of the landslide distribution are consistent with results of recent inversion modeling that indicate high-frequency energy generation was greatest in the western part of the <span class="hlt">fault</span> rupture zone and decreased markedly to the east. ?? 2004, <span class="hlt">Earthquake</span> Engineering Research Institute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EP%26S...70...55N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EP%26S...70...55N"><span><span class="hlt">Fault</span> model of the 2017 Jiuzhaigou Mw 6.5 <span class="hlt">earthquake</span> estimated from coseismic deformation observed using Global Positioning <span class="hlt">System</span> and Interferometric Synthetic Aperture Radar data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nie, Zhaosheng; Wang, Di-Jin; Jia, Zhige; Yu, Pengfei; Li, Liangfa</p> <p>2018-04-01</p> <p>On August 8, 2017, the Jiuzhaigou Mw 6.5 <span class="hlt">earthquake</span> occurred in Sichuan province, southwestern China, along the eastern margin of the Tibetan Plateau. The epicenter is surrounded by the Minjiang, Huya, and Tazang <span class="hlt">Faults</span>. As the seismic activity and tectonics are very complicated, there is controversy regarding the accurate location of the epicenter and the seismic <span class="hlt">fault</span> of the Jiuzhaigou <span class="hlt">earthquake</span>. To investigate these aspects, first, the coseismic deformation field was derived from Global Positioning <span class="hlt">System</span> (GPS) and Interferometric Synthetic Aperture Radar (InSAR) measurements. Second, the <span class="hlt">fault</span> geometry, coseismic slip model, and Coulomb stress changes around the seismic region were calculated using a homogeneous elastic half-space model. The coseismic deformation field derived from InSAR measurements shows that this event was mainly dominated by a left-lateral strike-slip <span class="hlt">fault</span>. The maximal and minimal displacements were approximately 0.15 m and - 0.21 m, respectively, along line-of-sight observation. The whole deformation field follows a northwest-trending direction and is mainly concentrated west of the <span class="hlt">fault</span>. The coseismic slip is 28 km along the strike and 18 km along the dip. It is dominated by a left-lateral strike-slip <span class="hlt">fault</span>. The average and maximal <span class="hlt">fault</span> slip is 0.18 and 0.85 m, respectively. The rupture did not fully reach the ground surface. The focal mechanism derived from GPS and InSAR data is consistent with the kinematics and geometry of the Huya <span class="hlt">Fault</span>. Therefore, we conclude that the northern section or the Shuzheng segment of the Huya <span class="hlt">Fault</span> is the seismogenic <span class="hlt">fault</span>. The maximal <span class="hlt">fault</span> slip is located at 33.25°N and 103.82°E at a depth of 11 km, and the release moment is approximately 6.635 × 1018 Nm, corresponding to a magnitude of Mw 6.49, which is consistent with results reported by the US Geological Survey, Global Centroid Moment Tensor, and other researchers. The coseismic Coulomb stress changes enhanced the stress on the northwest and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Tectp.693..453F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Tectp.693..453F"><span>Structure and kinematics of the Sumatran <span class="hlt">Fault</span> <span class="hlt">System</span> in North Sumatra (Indonesia)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernández-Blanco, David; Philippon, Melody; von Hagke, Christoph</p> <p>2016-12-01</p> <p>Lithospheric-scale <span class="hlt">faults</span> related to oblique subduction are responsible for some of the most hazardous <span class="hlt">earthquakes</span> reported worldwide. The mega-thrust in the Sunda sector of the Sumatran oblique subduction has been intensively studied, especially after the infamous 2004 Mw 9.1 <span class="hlt">earthquake</span>, but its onshore kinematic complement within the Sumatran subduction, the transform Sumatran <span class="hlt">Fault</span> <span class="hlt">System</span>, has received considerably less attention. In this paper, we apply a combination of analysis of Digital Elevation Models (ASTER GDEM) and field evidence to resolve the kinematics of the leading edge of deformation of the northern sector of the Sumatran <span class="hlt">Fault</span> <span class="hlt">System</span>. To this end, we mapped the northernmost tip of Sumatra, including the islands to the northwest, between 4.5°N and 6°N. Here, major topographic highs are related to different <span class="hlt">faults</span>. Using field evidence and our GDEM structural mapping, we can show that in the area where the <span class="hlt">fault</span> bifurcates into two <span class="hlt">fault</span> strands, two independent kinematic regimes evolve, both consistent with the large-scale framework of the Sumatran <span class="hlt">Fault</span> <span class="hlt">System</span>. Whereas the eastern branch is a classic Riedel <span class="hlt">system</span>, the western branch features a fold-and-thrust belt. The latter contractional feature accommodated significant amounts (c. 20%) of shortening of the <span class="hlt">system</span> in the study area. Our field observations of the tip of the NSFS match a strain pattern with a western contractional domain (Pulau Weh thrust splay) and an eastern extensional domain (Pulau Aceh Riedel <span class="hlt">system</span>), which are together characteristic of the tip of a propagating strike-slip <span class="hlt">fault</span>, from a mechanical viewpoint. For the first time, we describe the strain partitioning resulting from the propagation of the NSFS in Sumatra mainland. Our study helps understanding complex kinematics of an evolving strike-slip <span class="hlt">system</span>, and stresses the importance of field studies in addition to remote sensing and geophysical studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7821S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7821S"><span>Active <span class="hlt">faults</span> <span class="hlt">system</span> and related potential seismic events near Ulaanbaatar, capital of Mongolia.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlupp, Antoine; Ferry, Matthieu; Munkhuu, Ulziibat; Sodnomsambuu, Demberel; Al-Ashkar, Abeer</p> <p>2013-04-01</p> <p>The region of Ulaanbaatar lies several hundred kilometers from large known active <span class="hlt">faults</span> that produced magnitude 6 to 8+ <span class="hlt">earthquakes</span> during the last century. Beside the Hustai <span class="hlt">fault</span>, which displays a clear morphological expression, no active <span class="hlt">fault</span> was previously described less than 100 km from the city. In addition, no large historical (i.e. more recent than the 16th c.) <span class="hlt">earthquakes</span> are known in this region. However, since 2005 a very dense seismic activity has developed over the Emeelt Township area, a mere 10 km from Ulaanbaatar. The activity is characterized by numerous low magnitude events (M<2.8), which are distributed linearly along several tens of kilometers where no active <span class="hlt">fault</span> has been identified. This raises several questions: Is this seismicity associated to a -yet- unknown active <span class="hlt">fault</span>? If so, are there other unknown active <span class="hlt">faults</span> near Ulaanbaatar? Hence, we deployed a multi-disciplinary approach including morpho-tectonic, near-surface geophysical and paleoseismological investigations. We describe four large active <span class="hlt">faults</span> west and south of Ulaanbaatar, three of them are newly discovered (Emeelt, Sharai, Avdar), one was previously known (Hustai) but without precise study on its seismic potential. The Emeelt seismicity can be mapped over 35 km along N150 and corresponds in the field to a smoothed, but clear, active <span class="hlt">fault</span> morphology that can be mapped along a 10-km-long section. The <span class="hlt">fault</span> dips at ~30° NE (GPR and surface morphology observations) and uplifts the eastern block. The age of the last surface rupture observed in trenches is about 10 ka (preliminary OSL dating). Considering a rupture length of 35 km, a full segment rupture would be comparable to the 1967 Mogod <span class="hlt">earthquake</span> with a magnitude as large as Mw 7. It has to be considered today as a possible scenario for the seismic risk of Ulaanbaatar. The 90-km-long Hustai Range <span class="hlt">Fault</span> <span class="hlt">System</span>, oriented WSW-ENE and located about 10 km west of Ulaanbaatar, displays continuous microseismicity with five</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27981074','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27981074"><span>Potential for a large <span class="hlt">earthquake</span> near Los Angeles inferred from the 2014 La Habra <span class="hlt">earthquake</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Donnellan, Andrea; Grant Ludwig, Lisa; Parker, Jay W; Rundle, John B; Wang, Jun; Pierce, Marlon; Blewitt, Geoffrey; Hensley, Scott</p> <p>2015-09-01</p> <p>Tectonic motion across the Los Angeles region is distributed across an intricate network of strike-slip and thrust <span class="hlt">faults</span> that will be released in destructive <span class="hlt">earthquakes</span> similar to or larger than the 1933  M 6.4 Long Beach and 1994  M 6.7 Northridge events. Here we show that Los Angeles regional thrust, strike-slip, and oblique <span class="hlt">faults</span> are connected and move concurrently with measurable surface deformation, even in moderate magnitude <span class="hlt">earthquakes</span>, as part of a <span class="hlt">fault</span> <span class="hlt">system</span> that accommodates north-south shortening and westerly tectonic escape of northern Los Angeles. The 28 March 2014 M 5.1 La Habra <span class="hlt">earthquake</span> occurred on a northeast striking, northwest dipping left-lateral oblique thrust <span class="hlt">fault</span> northeast of Los Angeles. We present crustal deformation observation spanning the <span class="hlt">earthquake</span> showing that concurrent deformation occurred on several structures in the shallow crust. The seismic moment of the <span class="hlt">earthquake</span> is 82% of the total geodetic moment released. Slip within the unconsolidated upper sedimentary layer may reflect shallow release of accumulated strain on still-locked deeper structures. A future M 6.1-6.3 <span class="hlt">earthquake</span> would account for the accumulated strain. Such an event could occur on any one or several of these <span class="hlt">faults</span>, which may not have been identified by geologic surface mapping.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5125407','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5125407"><span>Potential for a large <span class="hlt">earthquake</span> near Los Angeles inferred from the 2014 La Habra <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Grant Ludwig, Lisa; Parker, Jay W.; Rundle, John B.; Wang, Jun; Pierce, Marlon; Blewitt, Geoffrey; Hensley, Scott</p> <p>2015-01-01</p> <p>Abstract Tectonic motion across the Los Angeles region is distributed across an intricate network of strike‐slip and thrust <span class="hlt">faults</span> that will be released in destructive <span class="hlt">earthquakes</span> similar to or larger than the 1933 M6.4 Long Beach and 1994 M6.7 Northridge events. Here we show that Los Angeles regional thrust, strike‐slip, and oblique <span class="hlt">faults</span> are connected and move concurrently with measurable surface deformation, even in moderate magnitude <span class="hlt">earthquakes</span>, as part of a <span class="hlt">fault</span> <span class="hlt">system</span> that accommodates north‐south shortening and westerly tectonic escape of northern Los Angeles. The 28 March 2014 M5.1 La Habra <span class="hlt">earthquake</span> occurred on a northeast striking, northwest dipping left‐lateral oblique thrust <span class="hlt">fault</span> northeast of Los Angeles. We present crustal deformation observation spanning the <span class="hlt">earthquake</span> showing that concurrent deformation occurred on several structures in the shallow crust. The seismic moment of the <span class="hlt">earthquake</span> is 82% of the total geodetic moment released. Slip within the unconsolidated upper sedimentary layer may reflect shallow release of accumulated strain on still‐locked deeper structures. A future M6.1–6.3 <span class="hlt">earthquake</span> would account for the accumulated strain. Such an event could occur on any one or several of these <span class="hlt">faults</span>, which may not have been identified by geologic surface mapping. PMID:27981074</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026340','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026340"><span>Rupture process of the M 7.9 Denali <span class="hlt">fault</span>, Alaska, <span class="hlt">earthquake</span>: Subevents, directivity, and scaling of high-frequency ground motions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Frankel, A.</p> <p>2004-01-01</p> <p>Displacement waveforms and high-frequency acceleration envelopes from stations at distances of 3-300 km were inverted to determine the source process of the M 7.9 Denali <span class="hlt">fault</span> <span class="hlt">earthquake</span>. Fitting the initial portion of the displacement waveforms indicates that the <span class="hlt">earthquake</span> started with an oblique thrust subevent (subevent # 1) with an east-west-striking, north-dipping nodal plane consistent with the observed surface rupture on the Susitna Glacier <span class="hlt">fault</span>. Inversion of the remainder of the waveforms (0.02-0.5 Hz) for moment release along the Denali and Totschunda <span class="hlt">faults</span> shows that rupture proceeded eastward on the Denali <span class="hlt">fault</span>, with two strike-slip subevents (numbers 2 and 3) centered about 90 and 210 km east of the hypocenter. Subevent 2 was located across from the station at PS 10 (Trans-Alaska Pipeline Pump Station #10) and was very localized in space and time. Subevent 3 extended from 160 to 230 km east of the hypocenter and had the largest moment of the subevents. Based on the timing between subevent 2 and the east end of subevent 3, an average rupture velocity of 3.5 km/sec, close to the shear wave velocity at the average rupture depth, was found. However, the portion of the rupture 130-220 km east of the epicenter appears to have an effective rupture velocity of about 5.0 km/ sec, which is supershear. These two subevents correspond approximately to areas of large surface offsets observed after the <span class="hlt">earthquake</span>. Using waveforms of the M 6.7 Nenana Mountain <span class="hlt">earthquake</span> as empirical Green's functions, the high-frequency (1-10 Hz) envelopes of the M 7.9 <span class="hlt">earthquake</span> were inverted to determine the location of high-frequency energy release along the <span class="hlt">faults</span>. The initial thrust subevent produced the largest high-frequency energy release per unit <span class="hlt">fault</span> length. The high-frequency envelopes and acceleration spectra (>0.5 Hz) of the M 7.9 <span class="hlt">earthquake</span> can be simulated by chaining together rupture zones of the M 6.7 <span class="hlt">earthquake</span> over distances from 30 to 180 km east of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4145K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4145K"><span>Stress change and <span class="hlt">fault</span> interaction from a two century-long <span class="hlt">earthquake</span> sequence in the central Tell Atlas (Algeria)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kariche, Jughurta; Meghraoui, Mustapha; Ayadi, Abdelhakim; Salah Boughacha, Mohamed</p> <p>2017-04-01</p> <p>We study the role and distribution of stress transfer that may trigger destructive <span class="hlt">earthquakes</span> in the Central Tell Atlas (Algeria). A sequence of historical events reaching Ms 7.3 and related stress tensors with thrust <span class="hlt">faulting</span> mechanisms allows the modeling of the Coulomb Failure Function (deltaCFF). We explore here the physical parameters for a stress transfer along the Tell thrust-and-fold belt taking into account an eastward trending <span class="hlt">earthquake</span> migration from 1891 to 2003. The Computation integrated the seismicity rate in the deltaCFF computation, which is in good agreement with the migration seismicity. The stress transfer progression and increase of 0.1 to 0.8 bar are obtained on <span class="hlt">fault</span> planes at 7-km-depth with a friction coefficient µ' 0.4 showing stress loading lobes on targeted coseismic <span class="hlt">fault</span> zone and location of stress shadow across other thrust-and-fold regions. The Coulomb modeling suggests a distinction in <span class="hlt">earthquake</span> triggering between zones with moderate-sized and large <span class="hlt">earthquake</span> ruptures. Recent InSAR and levelling studies and aftershocks that document postseismic deformation of major <span class="hlt">earthquakes</span> are integrated into the static stress change calculations. The presence of fluid and related poroelastic deformation can be considered as an open question with regards to their contribution to major <span class="hlt">earthquakes</span> and their implications in the seismic hazard assessment of northern Algeria.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1615340D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1615340D"><span>Superplastic flow lubricates carbonate <span class="hlt">faults</span> during <span class="hlt">earthquake</span> slip</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Paola, Nicola; Holdsworth, Robert; Viti, Cecilia; Collettini, Cristiano; Faoro, Igor; Bullock, Rachael</p> <p>2014-05-01</p> <p>Tectonic <span class="hlt">earthquakes</span> are hosted in the shallower portion of crustal <span class="hlt">fault</span> zones, where fracturing and cataclasis are thought to be the dominant processes during frictional sliding. Aseismic shear in lower crust and lithospheric mantle shear zones is accomplished by crystal plasticity, including superplastic flow acting at low strain rates on ultrafine-grained rocks. Superplasticity has also been observed at high strain rates for a range of nano-phase alloys and ceramics, and could potentially occur in fine-grained geological materials, if deformed at high strain rates and temperatures. We performed a set of displacement-controlled experiments to explore whether superplastic flow can effectively weaken <span class="hlt">faults</span>, and facilitate <span class="hlt">earthquake</span> propagation. The experiments were performed on fine-grained synthetic gouges (63 < f < 93 μm) of undeformed, protolith carbonate rocks using a rotary shear apparatus, at target speed v = 1 ms-1, normal stresses σn = 12-18 MPa, displacements d from 0.009 to 1.46 m, room temperature and humidity conditions. Samples were recovered after each experiment to study the slip zone microstructures. The integration of experimental data and microstructural observations shows that during sliding at seismic velocity, brittle fracturing and cataclasis control shear localization and grain size reduction in the slip zone at relatively low temperatures (T ≤ 100 °C). Stress levels predicted by such behaviours match those measured during the experiments. As temperatures rise due to frictional heating (T ≥ 500 °C), dislocation creep mechanisms start to accommodate intragranular strain, and play a key role in producing nanoscale subgrains (< 200 nm) in the slip zone. At this stage, despite of the presence of nanoparticles in the slip zone and the attainment of seismic slip rates, the measured frictional strength of experimental <span class="hlt">faults</span> still lies within Byerlee's range of values μ = 0.8. This suggests that the slip zone bulk strength at this stage</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T21E..03F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T21E..03F"><span>Strike-slip <span class="hlt">Fault</span> Structure in the Salton Trough and Deformation During and After the 2010 M7.2 El Mayor-Cucapah <span class="hlt">Earthquake</span> from Geodetic and Seismic Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fielding, E. J.; Sun, J.; Gonzalez-Ortega, A.; González-Escobar, M.; Freed, A. M.; Burgmann, R.; Samsonov, S. V.; Gonzalez-Garcia, J.; Fletcher, J. M.; Hinojosa, A.</p> <p>2013-12-01</p> <p>The Pacific-North America plate boundary character changes southward from the strike-slip and transpressional configuration along most of California to oblique rifting in the Gulf of California, with a transitional zone of transtension beneath the Salton Trough in southernmost California and northern Mexico. The Salton Trough is characterized by extremely high heat flow and thin lithosphere with a thick fill of sedimentary material delivered by the Colorado River during the past 5-6 million years. Because of the rapid sedimentation, most of the <span class="hlt">faults</span> in Salton Trough are buried and reveal themselves when they slip either seismically or aseismically. They can also be located by refraction and reflection of seismic waves. The 4 April 2010 El Mayor-Cucapah <span class="hlt">earthquake</span> (Mw 7.2) in Baja California and Sonora, Mexico is probably the largest <span class="hlt">earthquake</span> in the Salton Trough for at least 120 years, and had primarily right-lateral strike-slip motion. The <span class="hlt">earthquake</span> ruptured a complex set of <span class="hlt">faults</span> that lie to the west of the main plate boundary <span class="hlt">fault</span>, the Cerro Prieto <span class="hlt">Fault</span>, and shows that the strike-slip <span class="hlt">fault</span> <span class="hlt">system</span> in the southern Salton Trough has multiple sub-parallel active <span class="hlt">faults</span>, similar to southern California. The Cerro Prieto <span class="hlt">Fault</span> is still likely absorbing the majority of strain in the plate boundary. We study the coseismic and postseismic deformation of the 2010 <span class="hlt">earthquake</span> with interferometric analysis of synthetic aperture radar (SAR) images (InSAR) and pixel tracking by subpixel correlation of SAR and optical images. We combine sampled InSAR and subpixel correlation results with GPS (Global Positioning <span class="hlt">System</span>) offsets at PBO (Plate Boundary Observatory) stations to estimate the likely subsurface geometry of the major <span class="hlt">faults</span> that slipped during the <span class="hlt">earthquake</span> and to derive a static coseismic slip model. We constrained the surface locations of the <span class="hlt">fault</span> segments to mapped locations in the Sierra Cucapah to the northwest of the epicenter. SAR along-track offsets</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70041774','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70041774"><span>Coulomb stress interactions among M≥5.9 <span class="hlt">earthquakes</span> in the Gorda deformation zone and on the Mendocino Fracture Zone, Cascadia megathrust, and northern San Andreas <span class="hlt">fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rollins, John C.; Stein, Ross S.</p> <p>2010-01-01</p> <p>The Gorda deformation zone, a 50,000 km2 area of diffuse shear and rotation offshore northernmost California, has been the site of 20 M ≥ 5.9 <span class="hlt">earthquakes</span> on four different <span class="hlt">fault</span> orientations since 1976, including four M ≥ 7 shocks. This is the highest rate of large <span class="hlt">earthquakes</span> in the contiguous United States. We calculate that the source <span class="hlt">faults</span> of six recent M ≥ 5.9 <span class="hlt">earthquakes</span> had experienced ≥0.6 bar Coulomb stress increases imparted by <span class="hlt">earthquakes</span> that struck less than 9 months beforehand. Control tests indicate that ≥0.6 bar Coulomb stress interactions between M ≥ 5.9 <span class="hlt">earthquakes</span> separated by Mw = 7.3 Trinidad <span class="hlt">earthquake</span> are consistent with the locations of M ≥ 5.9 <span class="hlt">earthquakes</span> in the Gorda zone until at least 1995, as well as <span class="hlt">earthquakes</span> on the Mendocino <span class="hlt">Fault</span> Zone in 1994 and 2000. Coulomb stress changes imparted by the 1980 <span class="hlt">earthquake</span> are also consistent with its distinct elbow-shaped aftershock pattern. From these observations, we derive generalized static stress interactions among right-lateral, left-lateral and thrust <span class="hlt">faults</span> near triple junctions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MsT.........33S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MsT.........33S"><span>A Decade of Induced Slip on the Causative <span class="hlt">Fault</span> of the 2015 MW 4.0 Venus <span class="hlt">Earthquake</span>, Northeast Johnson County, Texas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scales, Monique Maria</p> <p></p> <p>On 7 May 2015, a MW 4.0 <span class="hlt">earthquake</span> occurred near Venus, northeast Johnson County, Texas, in an area of the Bend Arch-Fort Worth Basin that reports long-term, high-volume wastewater disposal and has hosted felt <span class="hlt">earthquakes</span> since 2009. Scientists at SMU deployed a local seismic network and purchased nearby seismic reflection data to capture additional events, identify and image the causative <span class="hlt">fault</span>, and explore potential links between ongoing industry activity and seismicity. Double-difference derived hypocenter relocations of the local <span class="hlt">earthquake</span> catalog indicate a <span class="hlt">fault</span> striking 230ºN, dipping to the west, consistent with a nodal plane of the MW 4.0 regional moment tensor. <span class="hlt">Fault</span> plane solutions, calculated using a combination of P-wave first motions and S to P amplitude ratios, indicate normal <span class="hlt">faulting</span>, with B-axes oriented parallel to maximum horizontal stress. Based on seismic reflection data, the reactivated basement <span class="hlt">fault</span> penetrates the Ordovician disposal layer and Mississippian production layer, but does not displace post-Lower Pennsylvanian units. The <span class="hlt">fault</span> rotates counter-clockwise north of current seismicity to become non-critically oriented within the modern stress field. Template matching at regional stations indicates that low magnitude <span class="hlt">earthquakes</span> with similar waveforms began in April 2008. Pressure data from five saltwater disposal wells within 5 km of the active <span class="hlt">fault</span> indicate a disposal formation that is 0.9-4.8 MPa above hydrostatic. I suggest that the injection of 28,000,000 m3 of wastewater between 2006 and 2016 at these wells led to an increase in subsurface pore fluid pressure that contributed to the triggering of this long-lived <span class="hlt">earthquake</span> sequence. The 2015 MW 4.0 event represents the largest event of a continuing evolution of slip on a causative <span class="hlt">fault</span>, with increasing magnitude over time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/bul/1991/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/bul/1991/report.pdf"><span>Late Quaternary <span class="hlt">faulting</span> along the Death Valley-Furnace Creek <span class="hlt">fault</span> <span class="hlt">system</span>, California and Nevada</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brogan, George E.; Kellogg, Karl; Slemmons, D. Burton; Terhune, Christina L.</p> <p>1991-01-01</p> <p>The Death Valley-Furnace Creek <span class="hlt">fault</span> <span class="hlt">system</span>, in California and Nevada, has a variety of impressive late Quaternary neotectonic features that record a long history of recurrent <span class="hlt">earthquake</span>-induced <span class="hlt">faulting</span>. Although no neotectonic features of unequivocal historical age are known, paleoseismic features from multiple late Quaternary events of surface <span class="hlt">faulting</span> are well developed throughout the length of the <span class="hlt">system</span>. Comparison of scarp heights to amount of horizontal offset of stream channels and the relationships of both scarps and channels to the ages of different geomorphic surfaces demonstrate that Quaternary <span class="hlt">faulting</span> along the northwest-trending Furnace Creek <span class="hlt">fault</span> zone is predominantly right lateral, whereas that along the north-trending Death Valley <span class="hlt">fault</span> zone is predominantly normal. These observations are compatible with tectonic models of Death Valley as a northwest-trending pull-apart basin. The largest late Quaternary scarps along the Furnace Creek <span class="hlt">fault</span> zone, with vertical separation of late Pleistocene surfaces of as much as 64 m (meters), are in Fish Lake Valley. Despite the predominance of normal <span class="hlt">faulting</span> along the Death Valley <span class="hlt">fault</span> zone, vertical offset of late Pleistocene surfaces along the Death Valley <span class="hlt">fault</span> zone apparently does not exceed about 15 m. Evidence for four to six separate late Holocene <span class="hlt">faulting</span> events along the Furnace Creek <span class="hlt">fault</span> zone and three or more late Holocene events along the Death Valley <span class="hlt">fault</span> zone are indicated by rupturing of Q1B (about 200-2,000 years old) geomorphic surfaces. Probably the youngest neotectonic feature observed along the Death Valley-Furnace Creek <span class="hlt">fault</span> <span class="hlt">system</span>, possibly historic in age, is vegetation lineaments in southernmost Fish Lake Valley. Near-historic <span class="hlt">faulting</span> in Death Valley, within several kilometers south of Furnace Creek Ranch, is represented by (1) a 2,000-year-old lake shoreline that is cut by sinuous scarps, and (2) a <span class="hlt">system</span> of young scarps with free-faceted faces (representing several <span class="hlt">faulting</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27418504','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27418504"><span>Connecting slow <span class="hlt">earthquakes</span> to huge <span class="hlt">earthquakes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Obara, Kazushige; Kato, Aitaro</p> <p>2016-07-15</p> <p>Slow <span class="hlt">earthquakes</span> are characterized by a wide spectrum of <span class="hlt">fault</span> slip behaviors and seismic radiation patterns that differ from those of traditional <span class="hlt">earthquakes</span>. However, slow <span class="hlt">earthquakes</span> and huge megathrust <span class="hlt">earthquakes</span> can have common slip mechanisms and are located in neighboring regions of the seismogenic zone. The frequent occurrence of slow <span class="hlt">earthquakes</span> may help to reveal the physics underlying megathrust events as useful analogs. Slow <span class="hlt">earthquakes</span> may function as stress meters because of their high sensitivity to stress changes in the seismogenic zone. Episodic stress transfer to megathrust source <span class="hlt">faults</span> leads to an increased probability of triggering huge <span class="hlt">earthquakes</span> if the adjacent locked region is critically loaded. Careful and precise monitoring of slow <span class="hlt">earthquakes</span> may provide new information on the likelihood of impending huge <span class="hlt">earthquakes</span>. Copyright © 2016, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035881','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035881"><span>A 3000-year record of ground-rupturing <span class="hlt">earthquakes</span> along the central North Anatolian <span class="hlt">fault</span> near Lake Ladik, Turkey</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fraser, J.; Pigati, J.S.; Hubert-Ferrari, A.; Vanneste, K.; Avsar, U.; Altinok, S.</p> <p>2009-01-01</p> <p>The North Anatolian <span class="hlt">fault</span> (NAF) is a ???1500 km long, arcuate, dextral strike-slip <span class="hlt">fault</span> zone in northern Turkey that extends from the Karliova triple junction to the Aegean Sea. East of Bolu, the <span class="hlt">fault</span> zone exhibits evidence of a sequence of large (Mw >7) <span class="hlt">earthquakes</span> that occurred during the twentieth century that displayed a migrating <span class="hlt">earthquake</span> sequence from east to west. Prolonged human occupation in this region provides an extensive, but not exhaustive, historical record of large <span class="hlt">earthquakes</span> prior to the twentieth century that covers much of the last 2000 yr. In this study, we extend our knowledge of rupture events in the region by evaluating the stratigraphy and chronology of sediments exposed in a paleoseismic trench across a splay of the NAF at Destek, ???6:5 km east of Lake Ladik (40.868?? N, 36.121?? E). The trenched <span class="hlt">fault</span> strand forms an uphill-facing scarp and associated sediment trap below a small catchment area. The trench exposed a narrow <span class="hlt">fault</span> zone that has juxtaposed a sequence of weakly defined paleosols interbedded with colluvium against highly fractured bedrock. We mapped magnetic susceptibility variations on the trench walls and found evidence for multiple visually unrecognized colluvial wedges. This technique was also used to constrain a predominantly dip-slip style of displacement on this <span class="hlt">fault</span> splay. Sediments exposed in the trench were dated using both charcoal and terrestrial gastropod shells to constrain the timing of the <span class="hlt">earthquake</span> events. While the gastropod shells consistently yielded 14 C ages that were too old (by ???900 yr), we obtained highly reliable 14 C ages from the charcoal by dating multiple components of the sample material. Our radiocarbon chronology constrains the timing of seven large <span class="hlt">earthquakes</span> over the past 3000 yr prior to the 1943 Tosya <span class="hlt">earthquake</span>, including event ages of (2?? error): A.D. 1437-1788, A.D. 1034-1321, A.D. 549-719, A.D. 17-585 (1-3 events), 35 B.C.-A.D. 28, 700-392 B.C., 912-596 B.C. Our results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1437/g/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1437/g/"><span>Development of Final A-<span class="hlt">Fault</span> Rupture Models for WGCEP/ NSHMP <span class="hlt">Earthquake</span> Rate Model 2</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Field, Edward H.; Weldon, Ray J.; Parsons, Thomas; Wills, Chris J.; Dawson, Timothy E.; Stein, Ross S.; Petersen, Mark D.</p> <p>2008-01-01</p> <p>This appendix discusses how we compute the magnitude and rate of <span class="hlt">earthquake</span> ruptures for the seven Type-A <span class="hlt">faults</span> (Elsinore, Garlock, San Jacinto, S. San Andreas, N. San Andreas, Hayward-Rodgers Creek, and Calaveras) in the WGCEP/NSHMP <span class="hlt">Earthquake</span> Rate Model 2 (referred to as ERM 2. hereafter). By definition, Type-A <span class="hlt">faults</span> are those that have relatively abundant paleoseismic information (e.g., mean recurrence-interval estimates). The first section below discusses segmentation-based models, where ruptures are assumed be confined to one or more identifiable segments. The second section discusses an un-segmented-model option, the third section discusses results and implications, and we end with a discussion of possible future improvements. General background information can be found in the main report.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMDI11A4246D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMDI11A4246D"><span>Dynamic <span class="hlt">earthquake</span> rupture simulation on nonplanar <span class="hlt">faults</span> embedded in 3D geometrically complex, heterogeneous Earth models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duru, K.; Dunham, E. M.; Bydlon, S. A.; Radhakrishnan, H.</p> <p>2014-12-01</p> <p>Dynamic propagation of shear ruptures on a frictional interface is a useful idealization of a natural <span class="hlt">earthquake</span>.The conditions relating slip rate and <span class="hlt">fault</span> shear strength are often expressed as nonlinear friction laws.The corresponding initial boundary value problems are both numerically and computationally challenging.In addition, seismic waves generated by <span class="hlt">earthquake</span> ruptures must be propagated, far away from <span class="hlt">fault</span> zones, to seismic stations and remote areas.Therefore, reliable and efficient numerical simulations require both provably stable and high order accurate numerical methods.We present a numerical method for:a) enforcing nonlinear friction laws, in a consistent and provably stable manner, suitable for efficient explicit time integration;b) dynamic propagation of <span class="hlt">earthquake</span> ruptures along rough <span class="hlt">faults</span>; c) accurate propagation of seismic waves in heterogeneous media with free surface topography.We solve the first order form of the 3D elastic wave equation on a boundary-conforming curvilinear mesh, in terms of particle velocities and stresses that are collocated in space and time, using summation-by-parts finite differences in space. The finite difference stencils are 6th order accurate in the interior and 3rd order accurate close to the boundaries. Boundary and interface conditions are imposed weakly using penalties. By deriving semi-discrete energy estimates analogous to the continuous energy estimates we prove numerical stability. Time stepping is performed with a 4th order accurate explicit low storage Runge-Kutta scheme. We have performed extensive numerical experiments using a slip-weakening friction law on non-planar <span class="hlt">faults</span>, including recent SCEC benchmark problems. We also show simulations on fractal <span class="hlt">faults</span> revealing the complexity of rupture dynamics on rough <span class="hlt">faults</span>. We are presently extending our method to rate-and-state friction laws and off-<span class="hlt">fault</span> plasticity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.G14A..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.G14A..02B"><span>Crustal strain accumulation on Southern Basin and Range Province <span class="hlt">faults</span> modulated by distant plate boundary <span class="hlt">earthquakes</span>? Evidence from geodesy, seismic imaging, and paleoseismology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bennett, R. A.; Shirzaei, M.; Broermann, J.; Spinler, J. C.; Holland, A. A.; Pearthree, P.</p> <p>2014-12-01</p> <p>GPS in Arizona reveals a change in the pattern of crustal strain accumulation in 2010 and based on viscoelastic modeling appears to be associated with the distant M7.2 El Mayor-Cucapah (EMC) <span class="hlt">earthquake</span> in Baja California, Mexico. GPS data collected between 1999 and 2009 near the Santa Rita normal <span class="hlt">fault</span> in SE Arizona reveal a narrow zone of crustal deformation coincident with the <span class="hlt">fault</span> trace, delineated by W-NW facing Pleistocene <span class="hlt">fault</span> scarps of heights 1 to 7 m. The apparent deformation zone is also seen in a preliminary InSAR interferogram. Total motion across the zone inferred using an elastic block model constrained by the pre-2010 GPS measurements is ~1 mm/yr in a sense consistent with normal <span class="hlt">fault</span> motion. However, continuous GPS measurements throughout Arizona reveal pronounced changes in crustal velocity following the EMC <span class="hlt">earthquake</span>, such that the relative motion across the Santa Rita <span class="hlt">fault</span> post-2010 is negligible. Paleoseismic evidence indicates that mapped Santa Rita <span class="hlt">fault</span> scarps were formed by two or more large magnitude (M6.7 to M7.6) surface rupturing normal-<span class="hlt">faulting</span> <span class="hlt">earthquakes</span> 60 to 100 kyrs ago. Seismic refraction and reflection data constrained by deep (~800 m) well log data provide evidence of progressive, possibly intermittent, displacement on the <span class="hlt">fault</span> through time. The rate of strain accumulation observed geodetically prior to 2010, if constant over the past 60 to 100 kyrs, would imply an untenable minimum slip rate deficit of 60 to 100 m since the most recent <span class="hlt">earthquake</span>. One explanation for the available geodetic, seismic, and paleoseismic evidence is that strain accumulation is modulated by viscoelastic relaxation associated with frequent large magnitude <span class="hlt">earthquakes</span> in the Salton Trough region, episodically inhibiting the accumulation of elastic strain required to generate large <span class="hlt">earthquakes</span> on the Santa Rita and possibly other <span class="hlt">faults</span> in the Southern Basin and Range. An important question is thus for how long the postseismic velocity changes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMNH31B1352G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMNH31B1352G"><span><span class="hlt">Earthquake</span> Model of the Middle East (EMME) Project: Active <span class="hlt">Fault</span> Database for the Middle East Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gülen, L.; Wp2 Team</p> <p>2010-12-01</p> <p>The <span class="hlt">Earthquake</span> Model of the Middle East (EMME) Project is a regional project of the umbrella GEM (Global <span class="hlt">Earthquake</span> Model) project (http://www.emme-gem.org/). EMME project region includes Turkey, Georgia, Armenia, Azerbaijan, Syria, Lebanon, Jordan, Iran, Pakistan, and Afghanistan. Both EMME and SHARE projects overlap and Turkey becomes a bridge connecting the two projects. The Middle East region is tectonically and seismically very active part of the Alpine-Himalayan orogenic belt. Many major <span class="hlt">earthquakes</span> have occurred in this region over the years causing casualties in the millions. The EMME project will use PSHA approach and the existing source models will be revised or modified by the incorporation of newly acquired data. More importantly the most distinguishing aspect of the EMME project from the previous ones will be its dynamic character. This very important characteristic is accomplished by the design of a flexible and scalable database that will permit continuous update, refinement, and analysis. A digital active <span class="hlt">fault</span> map of the Middle East region is under construction in ArcGIS format. We are developing a database of <span class="hlt">fault</span> parameters for active <span class="hlt">faults</span> that are capable of generating <span class="hlt">earthquakes</span> above a threshold magnitude of Mw≥5.5. Similar to the WGCEP-2007 and UCERF-2 projects, the EMME project database includes information on the geometry and rates of movement of <span class="hlt">faults</span> in a “<span class="hlt">Fault</span> Section Database”. The “<span class="hlt">Fault</span> Section” concept has a physical significance, in that if one or more <span class="hlt">fault</span> parameters change, a new <span class="hlt">fault</span> section is defined along a <span class="hlt">fault</span> zone. So far over 3,000 <span class="hlt">Fault</span> Sections have been defined and parameterized for the Middle East region. A separate “Paleo-Sites Database” includes information on the timing and amounts of <span class="hlt">fault</span> displacement for major <span class="hlt">fault</span> zones. A digital reference library that includes the pdf files of the relevant papers, reports is also being prepared. Another task of the WP-2 of the EMME project is to prepare</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNH53C2007I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNH53C2007I"><span>Study on the Evaluation Method for <span class="hlt">Fault</span> Displacement: Probabilistic Approach Based on Japanese <span class="hlt">Earthquake</span> Rupture Data - Distributed <span class="hlt">fault</span> displacements -</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Inoue, N.; Kitada, N.; Tonagi, M.</p> <p>2016-12-01</p> <p>Distributed <span class="hlt">fault</span> displacements in Probabilistic <span class="hlt">Fault</span> Displace- ment Analysis (PFDHA) have an important rule in evaluation of important facilities such as Nuclear Installations. In Japan, the Nu- clear Installations should be constructed where there is no possibility that the displacement by the <span class="hlt">earthquake</span> on the active <span class="hlt">faults</span> occurs. Youngs et al. (2003) defined the distributed <span class="hlt">fault</span> as displacement on other <span class="hlt">faults</span> or shears, or fractures in the vicinity of the principal rup- ture in response to the principal <span class="hlt">faulting</span>. Other researchers treated the data of distribution <span class="hlt">fault</span> around principal <span class="hlt">fault</span> and modeled according to their definitions (e.g. Petersen et al., 2011; Takao et al., 2013 ). We organized Japanese <span class="hlt">fault</span> displacements data and constructed the slip-distance relationship depending on <span class="hlt">fault</span> types. In the case of reverse <span class="hlt">fault</span>, slip-distance relationship on the foot-wall indicated difference trend compared with that on hanging-wall. The process zone or damaged zone have been studied as weak structure around principal <span class="hlt">faults</span>. The density or number is rapidly decrease away from the principal <span class="hlt">faults</span>. We contrasted the trend of these zones with that of distributed slip-distance distributions. The subsurface FEM simulation have been carried out to inves- tigate the distribution of stress around principal <span class="hlt">faults</span>. The results indicated similar trend compared with the distribution of field obser- vations. This research was part of the 2014-2015 research project `Development of evaluating method for <span class="hlt">fault</span> displacement` by the Secretariat of Nuclear Regulation Authority (S/NRA), Japan.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhDT........22R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhDT........22R"><span>Deformation associated with continental normal <span class="hlt">faults</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Resor, Phillip G.</p> <p></p> <p>Deformation associated with normal <span class="hlt">fault</span> <span class="hlt">earthquakes</span> and geologic structures provide insights into the seismic cycle as it unfolds over time scales from seconds to millions of years. Improved understanding of normal <span class="hlt">faulting</span> will lead to more accurate seismic hazard assessments and prediction of associated structures. High-precision aftershock locations for the 1995 Kozani-Grevena <span class="hlt">earthquake</span> (Mw 6.5), Greece image a segmented master <span class="hlt">fault</span> and antithetic <span class="hlt">faults</span>. This three-dimensional <span class="hlt">fault</span> geometry is typical of normal <span class="hlt">fault</span> <span class="hlt">systems</span> mapped from outcrop or interpreted from reflection seismic data and illustrates the importance of incorporating three-dimensional <span class="hlt">fault</span> geometry in mechanical models. Subsurface <span class="hlt">fault</span> slip associated with the Kozani-Grevena and 1999 Hector Mine (Mw 7.1) <span class="hlt">earthquakes</span> is modeled using a new method for slip inversion on three-dimensional <span class="hlt">fault</span> surfaces. Incorporation of three-dimensional <span class="hlt">fault</span> geometry improves the fit to the geodetic data while honoring aftershock distributions and surface ruptures. GPS Surveying of deformed bedding surfaces associated with normal <span class="hlt">faulting</span> in the western Grand Canyon reveals patterns of deformation that are similar to those observed by interferometric satellite radar interferometry (InSAR) for the Kozani Grevena <span class="hlt">earthquake</span> with a prominent down-warp in the hanging wall and a lesser up-warp in the footwall. However, deformation associated with the Kozani-Grevena <span class="hlt">earthquake</span> extends ˜20 km from the <span class="hlt">fault</span> surface trace, while the folds in the western Grand Canyon only extend 500 m into the footwall and 1500 m into the hanging wall. A comparison of mechanical and kinematic models illustrates advantages of mechanical models in exploring normal <span class="hlt">faulting</span> processes including incorporation of both deformation and causative forces, and the opportunity to incorporate more complex <span class="hlt">fault</span> geometry and constitutive properties. Elastic models with antithetic or synthetic <span class="hlt">faults</span> or joints in association with a master</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S14B..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S14B..06C"><span>Rapid modeling of complex multi-<span class="hlt">fault</span> ruptures with simplistic models from real-time GPS: Perspectives from the 2016 Mw 7.8 Kaikoura <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crowell, B.; Melgar, D.</p> <p>2017-12-01</p> <p>The 2016 Mw 7.8 Kaikoura <span class="hlt">earthquake</span> is one of the most complex <span class="hlt">earthquakes</span> in recent history, rupturing across at least 10 disparate <span class="hlt">faults</span> with varying <span class="hlt">faulting</span> styles, and exhibiting intricate surface deformation patterns. The complexity of this event has motivated the need for multidisciplinary geophysical studies to get at the underlying source physics to better inform <span class="hlt">earthquake</span> hazards models in the future. However, events like Kaikoura beg the question of how well (or how poorly) such <span class="hlt">earthquakes</span> can be modeled automatically in real-time and still satisfy the general public and emergency managers. To investigate this question, we perform a retrospective real-time GPS analysis of the Kaikoura <span class="hlt">earthquake</span> with the G-FAST early warning module. We first perform simple point source models of the <span class="hlt">earthquake</span> using peak ground displacement scaling and a coseismic offset based centroid moment tensor (CMT) inversion. We predict ground motions based on these point sources as well as simple finite <span class="hlt">faults</span> determined from source scaling studies, and validate against true recordings of peak ground acceleration and velocity. Secondly, we perform a slip inversion based upon the CMT <span class="hlt">fault</span> orientations and forward model near-field tsunami maximum expected wave heights to compare against available tide gauge records. We find remarkably good agreement between recorded and predicted ground motions when using a simple <span class="hlt">fault</span> plane, with the majority of disagreement in ground motions being attributable to local site effects, not <span class="hlt">earthquake</span> source complexity. Similarly, the near-field tsunami maximum amplitude predictions match tide gauge records well. We conclude that even though our models for the Kaikoura <span class="hlt">earthquake</span> are devoid of rich source complexities, the CMT driven finite <span class="hlt">fault</span> is a good enough "average" source and provides useful constraints for rapid forecasting of ground motion and near-field tsunami amplitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS21A1945B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS21A1945B"><span>Recent deformation on the San Diego Trough and San Pedro Basin <span class="hlt">fault</span> <span class="hlt">systems</span>, offshore Southern California: Assessing evidence for <span class="hlt">fault</span> <span class="hlt">system</span> connectivity.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bormann, J. M.; Kent, G. M.; Driscoll, N. W.; Harding, A. J.</p> <p>2016-12-01</p> <p>The seismic hazard posed by offshore <span class="hlt">faults</span> for coastal communities in Southern California is poorly understood and may be considerable, especially when these communities are located near long <span class="hlt">faults</span> that have the ability to produce large <span class="hlt">earthquakes</span>. The San Diego Trough <span class="hlt">fault</span> (SDTF) and San Pedro Basin <span class="hlt">fault</span> (SPBF) <span class="hlt">systems</span> are active northwest striking, right-lateral <span class="hlt">faults</span> in the Inner California Borderland that extend offshore between San Diego and Los Angeles. Recent work shows that the SDTF slip rate accounts for 25% of the 6-8 mm/yr of deformation accommodated by the offshore <span class="hlt">fault</span> network, and seismic reflection data suggest that these two <span class="hlt">fault</span> zones may be one continuous structure. Here, we use recently acquired CHIRP, high-resolution multichannel seismic (MCS) reflection, and multibeam bathymetric data in combination with USGS and industry MCS profiles to characterize recent deformation on the SDTF and SPBF zones and to evaluate the potential for an end-to-end rupture that spans both <span class="hlt">fault</span> <span class="hlt">systems</span>. The SDTF offsets young sediments at the seafloor for 130 km between the US/Mexico border and Avalon Knoll. The northern SPBF has robust geomorphic expression and offsets the seafloor in the Santa Monica Basin. The southern SPBF lies within a 25-km gap between high-resolution MCS surveys. Although there does appear to be a through-going <span class="hlt">fault</span> at depth in industry MCS profiles, the low vertical resolution of these data inhibits our ability to confirm recent slip on the southern SPBF. Empirical scaling relationships indicate that a 200-km-long rupture of the SDTF and its southern extension, the Bahia Soledad <span class="hlt">fault</span>, could produce a M7.7 <span class="hlt">earthquake</span>. If the SDTF and the SPBF are linked, the length of the combined <span class="hlt">fault</span> increases to >270 km. This may allow ruptures initiating on the SDTF to propagate within 25 km of the Los Angeles Basin. At present, the paleoseismic histories of the <span class="hlt">faults</span> are unknown. We present new observations from CHIRP and coring surveys at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.731..131X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.731..131X"><span>Sentinel-1 observation of the 2017 Sangsefid <span class="hlt">earthquake</span>, northeastern Iran: Rupture of a blind reserve-slip <span class="hlt">fault</span> near the Eastern Kopeh Dagh</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Guangyu; Xu, Caijun; Wen, Yangmao</p> <p>2018-04-01</p> <p>New satellites are now revealing InSAR-based surface deformation within a week after natural hazard events. Quick hazard responses will be more publically accessible and provide information to responding agencies. Here we used Sentinel-1 interferometric synthetic aperture radar (InSAR) data to investigate coseismic deformation associated with the 2017 Sangsefid <span class="hlt">earthquake</span>, which occurred in the southeast margin of the Kopeh Dagh <span class="hlt">fault</span> <span class="hlt">system</span>. The ascending and descending interferograms indicate thrust-dominated slip, with the maximum line-of-sight displacement of 10.5 and 13.7 cm, respectively. The detailed slip-distribution of the 2017 Sangsefid Mw6.1 <span class="hlt">earthquake</span> inferred from geodetic data is presented here for the first time. Although the InSAR interferograms themselves do not uniquely constrain what the primary slip surface is, we infer that the source <span class="hlt">fault</span> dips to southwest by analyzing the 2.5 D displacement field decomposed from the InSAR observations. The determined uniform slip <span class="hlt">fault</span> model shows that the dip angle of the seimogenic <span class="hlt">fault</span> is approximately 40°, with a strike of 120° except for a narrower <span class="hlt">fault</span> width than that predicted by the empirical scaling law. We suggest that geometric complexities near the Kopeh Dagh <span class="hlt">fault</span> <span class="hlt">system</span> obstruct the rupture propagation, resulting in high slip occurred within a small area and much higher stress drop than global estimates. The InSAR-determined moment is 1.71 × 1018 Nm with a shear modulus of 3.32 × 1010 N/m2, equivalent to Mw 6.12, which is consistent with seismological results. The finite <span class="hlt">fault</span> model (the west-dipping <span class="hlt">fault</span> plane) reveals that the peak slip of 0.90 m occurred at a depth of 6.3 km, with substantial slip at a depth of 4-10 km and a near-uniform slip of 0.1 m at a depth of 0-2.5 km. We suggest that the Sangsefid <span class="hlt">earthquake</span> occurred on an unknown blind reverse <span class="hlt">fault</span> dipping southwest, which can also be recognised through observing the long-term surface effects due to the existence of the blind</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T54C..03M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T54C..03M"><span>Seismicity Pattern and <span class="hlt">Fault</span> Structure in the Central Himalaya Seismic Gap Using Precise <span class="hlt">Earthquake</span> Hypocenters and their Source Parameters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mendoza, M.; Ghosh, A.; Rai, S. S.</p> <p>2017-12-01</p> <p>The devastation brought on by the Mw 7.8 Gorkha <span class="hlt">earthquake</span> in Nepal on 25 April 2015, reconditioned people to the high <span class="hlt">earthquake</span> risk along the Himalayan arc. It is therefore imperative to learn from the Gorkha <span class="hlt">earthquake</span>, and gain a better understanding of the state of stress in this <span class="hlt">fault</span> regime, in order to identify areas that could produce the next devastating <span class="hlt">earthquake</span>. Here, we focus on what is known as the "central Himalaya seismic gap". It is located in Uttarakhand, India, west of Nepal, where a large (> Mw 7.0) <span class="hlt">earthquake</span> has not occurred for over the past 200 years [Rajendran, C.P., & Rajendran, K., 2005]. This 500 - 800 km long along-strike seismic gap has been poorly studied, mainly due to the lack of modern and dense instrumentation. It is especially concerning since it surrounds densely populated cities, such as New Delhi. In this study, we analyze a rich seismic dataset from a dense network consisting of 50 broadband stations, that operated between 2005 and 2012. We use the STA/LTA filter technique to detect <span class="hlt">earthquake</span> phases, and the latest tools contributed to the Antelope software environment, to develop a large and robust <span class="hlt">earthquake</span> catalog containing thousands of precise hypocentral locations, magnitudes, and focal mechanisms. By refining those locations in HypoDD [Waldhauser & Ellsworth, 2000] to form a tighter cluster of events using relative relocation, we can potentially illustrate <span class="hlt">fault</span> structures in this region with high resolution. Additionally, using ZMAP [Weimer, S., 2001], we perform a variety of statistical analyses to understand the variability and nature of seismicity occurring in the region. Generating a large and consistent <span class="hlt">earthquake</span> catalog not only brings to light the physical processes controlling the <span class="hlt">earthquake</span> cycle in an Himalayan seismogenic zone, it also illustrates how stresses are building up along the décollment and the <span class="hlt">faults</span> that stem from it. With this new catalog, we aim to reveal <span class="hlt">fault</span> structure, study</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SPIE.9057E..09O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SPIE.9057E..09O"><span>Design of isolated buildings with S-FBI <span class="hlt">system</span> subjected to near-<span class="hlt">fault</span> <span class="hlt">earthquakes</span> using NSGA-II algorithm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ozbulut, O. E.; Silwal, B.</p> <p>2014-04-01</p> <p>This study investigates the optimum design parameters of a superelastic friction base isolator (S-FBI) <span class="hlt">system</span> through a multi-objective genetic algorithm and performance-based evaluation approach. The S-FBI <span class="hlt">system</span> consists of a flat steel- PTFE sliding bearing and a superelastic NiTi shape memory alloy (SMA) device. Sliding bearing limits the transfer of shear across the isolation interface and provides damping from sliding friction. SMA device provides restoring force capability to the isolation <span class="hlt">system</span> together with additional damping characteristics. A three-story building is modeled with S-FBI isolation <span class="hlt">system</span>. Multiple-objective numerical optimization that simultaneously minimizes isolation-level displacements and superstructure response is carried out with a genetic algorithm (GA) in order to optimize S-FBI <span class="hlt">system</span>. Nonlinear time history analyses of the building with S-FBI <span class="hlt">system</span> are performed. A set of 20 near-field ground motion records are used in numerical simulations. Results show that S-FBI <span class="hlt">system</span> successfully control response of the buildings against near-<span class="hlt">fault</span> <span class="hlt">earthquakes</span> without sacrificing in isolation efficacy and producing large isolation-level deformations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S21C0754M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S21C0754M"><span>Geostatistical analysis of the power-law exponents of the size distribution of <span class="hlt">earthquakes</span>, Quaternary <span class="hlt">faults</span> and monogenetic volcanoes in the Central Trans-Mexican Volcanic Belt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mendoza-Ponce, A.; Perez Lopez, R.; Guardiola-Albert, C.; Garduño-Monroy, V. H.; Figueroa-Soto, Á.</p> <p>2017-12-01</p> <p>The Trans Mexican Volcanic Belt (TMVB) is related to the convergence between the Cocos and Rivera plates beneath the North American plate by the Middle America Trench (MAT). Moreover, there is also intraplate <span class="hlt">faulting</span> within the TMVB, which is responsible of important <span class="hlt">earthquakes</span> like the Acambay in 1912 (Mw 7.0) and Maravatío in 1979 (Mb 5.3). In this tectonic scheme, monogenetic volcanoes, active <span class="hlt">faulting</span> and <span class="hlt">earthquakes</span> configure a complex tectonic frame where different spatial anisotropy featured this activity. This complexity can be characterized by the power-law of the frequency-size distribution of the monogenetic volcanoes, the <span class="hlt">faults</span> and the <span class="hlt">earthquakes</span>. This power-law is determined by the b-value of the Gutenberg-Richter law in case of the <span class="hlt">earthquakes</span>. The novelty of this work is the application of geostatistics techniques (variograms) for the analysis of spatial distribution of the b-values obtained from the size distribution of the basal diameter for monogenetic volcanoes in the Michoacán-Guanajuato Volcanic Field (bmv), surface area for <span class="hlt">faults</span> in the Morelia-Acambay <span class="hlt">fault</span> <span class="hlt">system</span> (bf) and the seismicity in the Central TMVB (beq). Therefore, the anisotropy in each case was compared and a geometric tectonic model was proposed. The evaluation of the spatial distribution of the b-value maps gives us a general interpretation of the tectonic stress field and the seismic hazard in the zone. Hence, the beq-value map for the seismic catalog shows anomalously low and high values, reveling two different processes, one related to a typical tectonic rupture (low b-values) and the other one related to hydraulic fracturing (high b-values). The resulting bmv-map for the diameter basal cones indicates us the locations of the ages of the monogenetic volcanoes, giving important information about the volcanic hazard. High bmv-values are correlated with the presence of young cinder cones and an increasing probability of a new volcano. For the Morelia-Acambay <span class="hlt">fault</span> <span class="hlt">system</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T51H..01F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T51H..01F"><span>Mechanics of Multifault <span class="hlt">Earthquake</span> Ruptures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fletcher, J. M.; Oskin, M. E.; Teran, O.</p> <p>2015-12-01</p> <p>The 2010 El Mayor-Cucapah <span class="hlt">earthquake</span> of magnitude Mw 7.2 produced the most complex rupture ever documented on the Pacific-North American plate margin, and the network of high- and low-angle <span class="hlt">faults</span> activated in the event record systematic changes in kinematics with <span class="hlt">fault</span> orientation. Individual <span class="hlt">faults</span> have a broad and continuous spectrum of slip sense ranging from endmember dextral strike slip to normal slip, and even <span class="hlt">faults</span> with thrust sense of dip slip were commonly observed in the aftershock sequence. Patterns of coseismic slip are consistent with three-dimensional constrictional strain and show that integrated transtensional shearing can be accommodated in a single <span class="hlt">earthquake</span>. Stress inversions of coseismic surface rupture and aftershock focal mechanisms define two coaxial, but permuted stress states. The maximum (σ1) and intermediate (σ2) principal stresses are close in magnitude, but flip orientations due to topography- and density-controlled gradients in lithostatic load along the length of the rupture. Although most large <span class="hlt">earthquakes</span> throughout the world activate slip on multiple <span class="hlt">faults</span>, the mechanical conditions of their genesis remain poorly understood. Our work attempts to answer several key questions. 1) Why do complex <span class="hlt">fault</span> <span class="hlt">systems</span> exist? They must do something that simple, optimally-oriented <span class="hlt">fault</span> <span class="hlt">systems</span> cannot because the two types of <span class="hlt">faults</span> are commonly located in close proximity. 2) How are <span class="hlt">faults</span> with diverse orientations and slip senses prepared throughout the interseismic period to fail spontaneously together in a single <span class="hlt">earthquake</span>? 3) Can a single stress state produce multi-<span class="hlt">fault</span> failure? 4) Are variations in pore pressure, friction and cohesion required to produce simultaneous rupture? 5) How is the fabric of surface rupture affected by variations in orientation, kinematics, total geologic slip and <span class="hlt">fault</span> zone architecture?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S11B2241W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S11B2241W"><span>Comparing the stress change characteristics and aftershock decay rate of the 2011 Mineral, VA, <span class="hlt">earthquake</span> with similar <span class="hlt">earthquakes</span> from a variety of tectonic settings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walsh, L. S.; Montesi, L. G.; Sauber, J. M.; Watters, T. R.; Kim, W.; Martin, A. J.; Anderson, R.</p> <p>2011-12-01</p> <p>On August 23, 2011, the magnitude 5.8 Mineral, VA, <span class="hlt">earthquake</span> rocked the U.S. national capital region (Washington, DC) drawing worldwide attention to the occurrence of intraplate <span class="hlt">earthquakes</span>. Using regional Coulomb stress change, we evaluate to what extent slip on <span class="hlt">faults</span> during the Mineral, VA, <span class="hlt">earthquake</span> and its aftershocks may have increased stress on notable Cenozoic <span class="hlt">fault</span> <span class="hlt">systems</span> in the DC metropolitan area: the central Virginia seismic zone, the DC <span class="hlt">fault</span> zone, and the Stafford <span class="hlt">fault</span> <span class="hlt">system</span>. Our Coulomb stress maps indicate that the transfer of stress from the Mineral, VA, mainshock was at least 500 times greater than that produced from the magnitude 3.4 Germantown, MD, <span class="hlt">earthquake</span> that occurred northwest of DC on July 16, 2010. Overall, the Mineral, VA, <span class="hlt">earthquake</span> appears to have loaded <span class="hlt">faults</span> of optimum orientation in the DC metropolitan region, bringing them closer to failure. The distribution of aftershocks of the Mineral, VA, <span class="hlt">earthquake</span> will be compared with Coulomb stress change maps. We further characterize the Mineral, VA, <span class="hlt">earthquake</span> by comparing its aftershock decay rate with that of blind thrust <span class="hlt">earthquakes</span> with similar magnitude, focal mechanism, and depth from a variety of tectonic settings. In particular, we compare aftershock decay relations of the Mineral, VA, <span class="hlt">earthquake</span> with two well studied California reverse <span class="hlt">faulting</span> events, the August 4, 1985 Kettleman Hills (Mw = 6.1) and October 1, 1987 Whittier Narrow (Mw = 5.9) <span class="hlt">earthquakes</span>. Through these relations we test the hypothesis that aftershock duration is inversely proportional to <span class="hlt">fault</span> stressing rate, suggesting that aftershocks in active tectonic margins may last only a few years while aftershocks in intraplate regions could endure for decades to a century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026626','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026626"><span>Wrightwood and the <span class="hlt">earthquake</span> cycle: What a long recurrence record tells us about how <span class="hlt">faults</span> work</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Weldon, R.; Scharer, K.; Fumal, T.; Biasi, G.</p> <p>2004-01-01</p> <p>The concept of the <span class="hlt">earthquake</span> cycle is so well established that one often hears statements in the popular media like, "the Big One is overdue" and "the longer it waits, the bigger it will be." Surprisingly, data to critically test the variability in recurrence intervals, rupture displacements, and relationships between the two are almost nonexistent. To generate a long series of <span class="hlt">earthquake</span> intervals and offsets, we have conducted paleoseismic investigations across the San Andreas <span class="hlt">fault</span> near the town of Wrightwood, California, excavating 45 trenches over 18 years, and can now provide some answers to basic questions about recurrence behavior of large <span class="hlt">earthquakes</span>. To date, we have characterized at least 30 prehistoric <span class="hlt">earthquakes</span> in a 6000-yr-long record, complete for the past 1500 yr and for the interval 3000-1500 B.C. For the past 1500 yr, the mean recurrence interval is 105 yr (31-165 yr for individual intervals) and the mean slip is 3.2 m (0.7-7 m per event). The series is slightly more ordered than random and has a notable cluster of events, during which strain was released at 3 times the long-term average rate. Slip associated with an <span class="hlt">earthquake</span> is not well predicted by the interval preceding it, and only the largest two <span class="hlt">earthquakes</span> appear to affect the time interval to the next <span class="hlt">earthquake</span>. Generally, short intervals tend to coincide with large displacements and long intervals with small displacements. The most significant correlation we find is that <span class="hlt">earthquakes</span> are more frequent following periods of net strain accumulation spanning multiple seismic cycles. The extent of paleoearthquake ruptures may be inferred by correlating event ages between different sites along the San Andreas <span class="hlt">fault</span>. Wrightwood and other nearby sites experience rupture that could be attributed to overlap of relatively independent segments that each behave in a more regular manner. However, the data are equally consistent with a model in which the irregular behavior seen at Wrightwood</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T13D2647W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T13D2647W"><span>How Long Is Long Enough? Estimation of Slip-Rate and <span class="hlt">Earthquake</span> Recurrence Interval on a Simple Plate-Boundary <span class="hlt">Fault</span> Using 3D Paleoseismic Trenching</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wechsler, N.; Rockwell, T. K.; Klinger, Y.; Agnon, A.; Marco, S.</p> <p>2012-12-01</p> <p>Models used to forecast future seismicity make fundamental assumptions about the behavior of <span class="hlt">faults</span> and <span class="hlt">fault</span> <span class="hlt">systems</span> in the long term, but in many cases this long-term behavior is assumed using short-term and perhaps non-representative observations. The question arises - how long of a record is long enough to represent actual <span class="hlt">fault</span> behavior, both in terms of recurrence of <span class="hlt">earthquakes</span> and of moment release (aka slip-rate). We test <span class="hlt">earthquake</span> recurrence and slip models via high-resolution three-dimensional trenching of the Beteiha (Bet-Zayda) site on the Dead Sea Transform (DST) in northern Israel. We extend the <span class="hlt">earthquake</span> history of this simple plate boundary <span class="hlt">fault</span> to establish slip rate for the past 3-4kyr, to determine the amount of slip per event and to study the fundamental behavior, thereby testing competing rupture models (characteristic, slip-patch, slip-loading, and Gutenberg Richter type distribution). To this end we opened more than 900m of trenches, mapped 8 buried channels and dated more than 80 radiocarbon samples. By mapping buried channels, offset by the DST on both sides of the <span class="hlt">fault</span>, we obtained for each an estimate of displacement. Coupled with <span class="hlt">fault</span> crossing trenches to determine event history, we construct <span class="hlt">earthquake</span> and slip history for the <span class="hlt">fault</span> for the past 2kyr. We observe evidence for a total of 9-10 surface-rupturing <span class="hlt">earthquakes</span> with varying offset amounts. 6-7 events occurred in the 1st millennium, compared to just 2-3 in the 2nd millennium CE. From our observations it is clear that the <span class="hlt">fault</span> is not behaving in a periodic fashion. A 4kyr old buried channel yields a slip rate of 3.5-4mm/yr, consistent with GPS rates for this segment. Yet in spite of the apparent agreement between GPS, Pleistocene to present slip rate, and the lifetime rate of the DST, the past 800-1000 year period appears deficit in strain release. Thus, in terms of moment release, most of the <span class="hlt">fault</span> has remained locked and is accumulating elastic strain. In contrast, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26552964','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26552964"><span>Fast-moving dislocations trigger flash weakening in carbonate-bearing <span class="hlt">faults</span> during <span class="hlt">earthquakes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Spagnuolo, Elena; Plümper, Oliver; Violay, Marie; Cavallo, Andrea; Di Toro, Giulio</p> <p>2015-11-10</p> <p>Rupture fronts can cause <span class="hlt">fault</span> displacement, reaching speeds up to several ms(-1) within a few milliseconds, at any distance away from the <span class="hlt">earthquake</span> nucleation area. In the case of silicate-bearing rocks the abrupt slip acceleration results in melting at asperity contacts causing a large reduction in <span class="hlt">fault</span> frictional strength (i.e., flash weakening). Flash weakening is also observed in experiments performed in carbonate-bearing rocks but evidence for melting is lacking. To unravel the micro-physical mechanisms associated with flash weakening in carbonates, experiments were conducted on pre-cut Carrara marble cylinders using a rotary shear apparatus at conditions relevant to <span class="hlt">earthquakes</span> propagation. In the first 5 mm of slip the shear stress was reduced up to 30% and CO2 was released. Focused ion beam, scanning and transmission electron microscopy investigations of the slipping zones reveal the presence of calcite nanograins and amorphous carbon. We interpret the CO2 release, the formation of nanograins and amorphous carbon to be the result of a shock-like stress release associated with the migration of fast-moving dislocations. Amorphous carbon, given its low friction coefficient, is responsible for flash weakening and promotes the propagation of the seismic rupture in carbonate-bearing <span class="hlt">fault</span> patches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4639853','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4639853"><span>Fast-moving dislocations trigger flash weakening in carbonate-bearing <span class="hlt">faults</span> during <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Spagnuolo, Elena; Plümper, Oliver; Violay, Marie; Cavallo, Andrea; Di Toro, Giulio</p> <p>2015-01-01</p> <p>Rupture fronts can cause <span class="hlt">fault</span> displacement, reaching speeds up to several ms−1 within a few milliseconds, at any distance away from the <span class="hlt">earthquake</span> nucleation area. In the case of silicate-bearing rocks the abrupt slip acceleration results in melting at asperity contacts causing a large reduction in <span class="hlt">fault</span> frictional strength (i.e., flash weakening). Flash weakening is also observed in experiments performed in carbonate-bearing rocks but evidence for melting is lacking. To unravel the micro-physical mechanisms associated with flash weakening in carbonates, experiments were conducted on pre-cut Carrara marble cylinders using a rotary shear apparatus at conditions relevant to <span class="hlt">earthquakes</span> propagation. In the first 5 mm of slip the shear stress was reduced up to 30% and CO2 was released. Focused ion beam, scanning and transmission electron microscopy investigations of the slipping zones reveal the presence of calcite nanograins and amorphous carbon. We interpret the CO2 release, the formation of nanograins and amorphous carbon to be the result of a shock-like stress release associated with the migration of fast-moving dislocations. Amorphous carbon, given its low friction coefficient, is responsible for flash weakening and promotes the propagation of the seismic rupture in carbonate-bearing <span class="hlt">fault</span> patches. PMID:26552964</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70042527','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70042527"><span>Prehistoric <span class="hlt">earthquakes</span> on the Caribbean-South American plate boundary, central Range <span class="hlt">Fault</span>, Trinidad</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prentice, Carol S.; Crosby, Christopher J.; Weber, John C.; Ragona, Daniel</p> <p>2010-01-01</p> <p>Recent geodetic studies suggest that the Central Range <span class="hlt">fault</span> is the principal plate-boundary structure accommodating strike-slip motion between the Caribbean and South American plates. Our study shows that the <span class="hlt">fault</span> forms a topographically prominent lineament in central Trinidad. Results from a paleoseismic investigation at a site where Holocene sediments have been deposited across the Central Range <span class="hlt">fault</span> indicate that it ruptured the ground surface most recently between 2710 and 550 yr B.P. If the geodetic slip rate of 9–15 mm/yr is representative of Holocene slip rates, our paleoseismic data suggest that at least 4.9 m of potential slip may have accumulated on the <span class="hlt">fault</span> and could be released during a future large <span class="hlt">earthquake</span> (M > 7).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037375','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037375"><span>Prehistoric <span class="hlt">earthquakes</span> on the Caribbean-South American plate boundary, central range <span class="hlt">fault</span>, Trinidad</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prentice, C.S.; Weber, J.C.; Crosby, C.J.; Ragona, D.</p> <p>2010-01-01</p> <p>Recent geodetic studies suggest that the Central Range <span class="hlt">fault</span> is the principal plate-boundary structure accommodating strike-slip motion between the Caribbean and South American plates. Our study shows that the <span class="hlt">fault</span> forms a topographically prominent lineament in central Trinidad. Results from a paleoseismic investigation at a site where Holocene sediments have been deposited across the Central Range <span class="hlt">fault</span> indicate that it ruptured the ground surface most recently between 2710 and 550 yr B.P. If the geodetic slip rate of 9-15 mm/yr is representative of Holocene slip rates, our paleoseismic data suggest that at least 4.9 m of potential slip may have accumulated on the <span class="hlt">fault</span> and could be released during a future large <span class="hlt">earthquake</span> (M > 7). ?? 2010 Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.S72F1359P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.S72F1359P"><span>Triggered Seismicity in Utah from the November 3, 2002, Denali <span class="hlt">Fault</span> <span class="hlt">Earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pankow, K. L.; Nava, S. J.; Pechmann, J. C.; Arabasz, W. J.</p> <p>2002-12-01</p> <p>Coincident with the arrival of the surface waves from the November 3, 2002, Mw 7.9 Denali <span class="hlt">Fault</span>, Alaska <span class="hlt">earthquake</span> (DFE), the University of Utah Seismograph Stations (UUSS) regional seismic network detected a marked increase in seismicity along the Intermountain Seismic Belt (ISB) in central and north-central Utah. The number of <span class="hlt">earthquakes</span> per day in Utah located automatically by the UUSS's Earthworm <span class="hlt">system</span> in the week following the DFE was approximately double the long-term average during the preceding nine months. From these preliminary data, the increased seismicity appears to be characterized by small magnitude events (M = 3.2) and concentrated in five distinct spatial clusters within the ISB between 38.75°and 42.0° N. The first of these <span class="hlt">earthquakes</span> was an M 2.2 event located ~20 km east of Salt Lake City, Utah, which occurred during the arrival of the Love waves from the DFE. The increase in Utah <span class="hlt">earthquake</span> activity at the time of the arrival of the surface waves from the DFE suggests that these surface waves triggered <span class="hlt">earthquakes</span> in Utah at distances of more than 3,000 km from the source. We estimated the peak dynamic shear stress caused by these surface waves from measurements of their peak vector velocities at 43 recording sites: 37 strong-motion stations of the Advanced National Seismic <span class="hlt">System</span> and six broadband stations. (The records from six other broadband instruments in the region of interest were clipped.) The estimated peak stresses ranged from 1.2 bars to 3.5 bars with a mean of 2.3 bars, and generally occurred during the arrival of Love waves of ~15 sec period. These peak dynamic shear stress estimates are comparable to those obtained from recordings of the 1992 Mw 7.3 Landers, California, <span class="hlt">earthquake</span> in regions where the Landers <span class="hlt">earthquake</span> triggered increased seismicity. We plan to present more complete analyses of UUSS seismic network data, further testing our hypothesis that the DFE remotely triggered seismicity in Utah. This hypothesis is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22321937','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22321937"><span>Determination of the relationship between radon anomalies and <span class="hlt">earthquakes</span> in well waters on the Akşehir-Simav <span class="hlt">Fault</span> <span class="hlt">System</span> in Afyonkarahisar province, Turkey.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ali Yalım, Hüseyin; Sandıkcıoğlu, Ayla; Ertuğrul, Oğuz; Yıldız, Ahmet</p> <p>2012-08-01</p> <p>Radon concentrations were measured in water of 4 wells on the Akşehir-Simav <span class="hlt">Fault</span> <span class="hlt">System</span> (ASFS) in Afyonkarahisar province from August 2009 to September 2010 and the relationship between radon anomalies and <span class="hlt">earthquake</span> magnitudes was examined. Anomalous decreases in radon concentrations in the wells were observed to precede the <span class="hlt">earthquakes</span> of magnitudes ranging from 2.6 M to 3.9 M. The correlation coefficients (R(2)) were 0.79, 0.93, 0.98 and 0.90 for the wells from 1 to 4, respectively, indicating that radon minima and <span class="hlt">earthquake</span> magnitude were well correlated and suggesting that the groundwater radon, when observed at suitable sites, can be a sensitive tracer for strain changes in crust associated with <span class="hlt">earthquake</span> occurrences. The relationship between the two parameters can be further improved as additional radon anomalies precursor to possible large <span class="hlt">earthquakes</span> are recorded in the wells located on the ASFS in the future. This study strongly suggests that the continuous observations of radon concentrations in well water, especially at well 3, should be carried forward. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S23C0847E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S23C0847E"><span>Microseismic data records <span class="hlt">fault</span> activation before and after a Mw 4.1 induced <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyre, T.; Eaton, D. W. S.</p> <p>2017-12-01</p> <p>Several large <span class="hlt">earthquakes</span> (Mw 4) have been observed in the vicinity of the town of Fox Creek, Alberta. These events have been determined to be induced <span class="hlt">earthquakes</span> related to hydraulic fracturing in the region. The largest of these has a magnitude Mw = 4.1, and is associated with a hydraulic-fracturing treatment close to Crooked Lake, about 30 km west of Fox Creek. The underlying factors that lead to localization of the high numbers of hydraulic fracturing induced events in this area remain poorly understood. The treatment that is associated with the Mw 4.1 event was monitored by 93 shallow three-level borehole arrays of sensors. Here we analyze the temporal and spatial evolution of the microseismic and seismic data recorded during the treatment. Contrary to expected microseismic event clustering parallel to the principal horizontal stress (NE - SW), the events cluster along obvious <span class="hlt">fault</span> planes that align both NNE - SSW and N - S. As the treatment well is oriented N - S, it appears that each stage of the treatment intersects a new portion of the fracture network, causing seismicity to occur. Focal-plane solutions support a strike-slip failure along these <span class="hlt">faults</span>, with nodal planes aligning with the microseismic cluster orientations. Each <span class="hlt">fault</span> segment is activated with a cluster of microseismicity in the centre, gradually extending along the <span class="hlt">fault</span> as time progresses. Once a portion of a <span class="hlt">fault</span> is active, further seismicity can be induced, regardless if the present stage is distant from the <span class="hlt">fault</span>. However, the large events seem to occur in regions with a gap in the microseismicity. Interestingly, most of the seismicity is located above the reservoir, including the larger events. Although a shallow-well array is used, these results are believed to have relatively high depth resolution, as the perforation shots are correctly located with an average error of 26 m in depth. This information contradicts previously held views that large induced <span class="hlt">earthquakes</span> occur primarily</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034995','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034995"><span>The ShakeOut scenario: A hypothetical Mw7.8 <span class="hlt">earthquake</span> on the Southern San Andreas <span class="hlt">Fault</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Porter, K.; Jones, L.; Cox, D.; Goltz, J.; Hudnut, K.; Mileti, D.; Perry, S.; Ponti, D.; Reichle, M.; Rose, A.Z.; Scawthorn, C.R.; Seligson, H.A.; Shoaf, K.I.; Treiman, J.; Wein, A.</p> <p>2011-01-01</p> <p>In 2008, an <span class="hlt">earthquake</span>-planning scenario document was released by the U.S. Geological Survey (USGS) and California Geological Survey that hypothesizes the occurrence and effects of a Mw7.8 <span class="hlt">earthquake</span> on the southern San Andreas <span class="hlt">Fault</span>. It was created by more than 300 scientists and engineers. <span class="hlt">Fault</span> offsets reach 13 m and up to 8 m at lifeline crossings. Physics-based modeling was used to generate maps of shaking intensity, with peak ground velocities of 3 m/sec near the <span class="hlt">fault</span> and exceeding 0.5 m/sec over 10,000 km2. A custom HAZUS??MH analysis and 18 special studies were performed to characterize the effects of the <span class="hlt">earthquake</span> on the built environment. The scenario posits 1,800 deaths and 53,000 injuries requiring emergency room care. Approximately 1,600 fires are ignited, resulting in the destruction of 200 million square feet of the building stock, the equivalent of 133,000 single-family homes. Fire contributes $87 billion in property and business interruption loss, out of the total $191 billion in economic loss, with most of the rest coming from shakerelated building and content damage ($46 billion) and business interruption loss from water outages ($24 billion). Emergency response activities are depicted in detail, in an innovative grid showing activities versus time, a new format introduced in this study. ?? 2011, <span class="hlt">Earthquake</span> Engineering Research Institute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016934','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016934"><span>Wasatch <span class="hlt">fault</span> zone, Utah - segmentation and history of Holocene <span class="hlt">earthquakes</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Machette, Michael N.; Personius, Stephen F.; Nelson, Alan R.; Schwartz, David P.; Lund, William R.</p> <p>1991-01-01</p> <p>The Wasatch <span class="hlt">fault</span> zone (WFZ) forms the eastern boundary of the Basin and Range province and is the longest continuous, active normal <span class="hlt">fault</span> (343 km) in the United States. It underlies an urban corridor of 1.6 million people (80% of Utah's population) representing the largest <span class="hlt">earthquake</span> risk in the interior of the western United States. The authors have used paleoseismological data to identify 10 discrete segments of the WFZ. Five are active, medial segments with Holocene slip rates of 1-2 mm a-1, recurrence intervals of 2000-4000 years and average lengths of about 50 km. Five are less active, distal segments with mostly pre-Holocene surface ruptures, late Quaternary slip rates of <0.5 mm a-1, recurrence intervals of ???10,000 years and average lengths of about 20 km. Surface-<span class="hlt">faulting</span> events on each of the medial segments of the WFZ formed 2-4-m-high scarps repeatedly during the Holocene. Paleoseismological records for the past 6000 years indicate that a major surface-rupturing <span class="hlt">earthquake</span> has occurred along one of the medial segments about every 395 ?? 60 years. However, between about 400 and 1500 years ago, the WFZ experienced six major surface-rupturing events, an average of one event every 220 years, or about twice as often as expected from the 6000-year record. Evidence has been found that surface-rupturing events occurred on the WFZ during the past 400 years, a time period which is twice the average intracluster recurrence interval and equal to the average Holocene recurrence interval.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814251Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814251Y"><span>Deriving <span class="hlt">earthquake</span> history of the Knidos <span class="hlt">Fault</span> Zone, SW Turkey, using cosmogenic 36Cl surface exposure dating of the <span class="hlt">fault</span> scarp.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yildirim, Cengiz; Ersen Aksoy, Murat; Akif Sarikaya, Mehmet; Tuysuz, Okan; Genc, S. Can; Ertekin Doksanalti, Mustafa; Sahin, Sefa; Benedetti, Lucilla; Tesson, Jim; Aster Team</p> <p>2016-04-01</p> <p>Formation of bedrock <span class="hlt">fault</span> scarps in extensional provinces is a result of large and successive <span class="hlt">earthquakes</span> that ruptured the surface several times. Extraction of seismic history of such <span class="hlt">faults</span> is critical to understand the recurrence intervals and the magnitude of paleo-<span class="hlt">earthquakes</span> and to better constrain the regional seismic hazard. Knidos on the Datca Peninsula (SW Turkey) is one of the largest cities of the antique times and sits on a terraced hill slope formed by en-echelon W-SW oriented normal <span class="hlt">faults</span>. The Datça Peninsula constitutes the southern boundary of the Gulf of Gökova, one of the largest grabens developed on the southernmost part of the Western Anatolian Extensional Province. Our investigation relies on cosmogenic 36Cl surface exposure dating of limestone <span class="hlt">faults</span> scarps. This method is a powerful tool to reconstruct the seismic history of normal <span class="hlt">faults</span> (e.g. Schlagenhauf et al 2010, Benedetti et al. 2013). We focus on one of the most prominent <span class="hlt">fault</span> scarp (hereinafter Mezarlık <span class="hlt">Fault</span>) of the Knidos <span class="hlt">fault</span> zone cutting through the antique Knidos city. We collected 128 pieces of tablet size (10x20cm) 3-cm thick samples along the <span class="hlt">fault</span> dip and opened 4 conventional paleoseismic trenches at the base of the <span class="hlt">fault</span> scarp. Our 36Cl concentration profile indicates that 3 to 4 seismic events ruptured the Mezarlık <span class="hlt">Fault</span> since Last Glacial Maximum (LGM). The results from the paleoseismic trenching are also compatible with 36Cl results, indicating 3 or 4 seismic events that disturbed the colluvium deposited at the base of the scarp. Here we will present implications for the seismic history and the derived slip-rate of the Mezarlık <span class="hlt">Fault</span> based on those results. This project is supported by The Scientific and Technological Research Council of Turkey (TUBITAK, Grant number: 113Y436) and it was conducted with the Decision of the Council of Ministers with No. 2013/5387 on the date 30.09.2013 and was done with the permission of Knidos Presidency of excavation in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.U13A0010J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.U13A0010J"><span>Nearshore geophysical investigation of the underwater trace of the Enriquillo-Plantain Garden <span class="hlt">Fault</span> following the 12 January 2010 Haiti <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnson, H. E.; Hornbach, M.; Cormier, M.; McHugh, C. M.; Gulick, S. P.; Braudy, N.; Davis, M.; Dieudonne, N.; Diebold, J. B.; Douilly, R.; Mishkin, K.; Seeber, L.; Sorlien, C. C.; Steckler, M. S.; Symithe, S. J.; Templeton, J.</p> <p>2010-12-01</p> <p>In response to the January 12, 2010 <span class="hlt">earthquake</span> in Haiti, we investigated offshore structures where aftershocks, lateral spreading, and a small tsunami suggested a coseismic underwater rupture. One aspect of that expedition involved mapping the trace of the Enriquillo-Plantain Garden <span class="hlt">fault</span> (EPGF) very close to shore, in water as shallow as 2 m. For this, we deployed from the ship a small inflatable boat mounted with a sidescan sonar and a chirp subbottom profiler. These nearshore surveys focused on Grand Goave Bay and Petit Goave Bay, two areas 40-60 km west of Port-au-Prince where the EPGF briefly extends offshore. In Grand Goave Bay, the combination of shipboard multibeam bathymetric data and nearshore geophysical data highlights a series of en-echelon ridges striking about EW, sub-parallel to the expected <span class="hlt">fault</span> trend. These rise 50-80 m above the surrounding seafloor and some slumps occur on their steep flanks. Although the sidescan imagery does not capture any well-defined seafloor offset or mole tracks that could be attributed to a 2010 <span class="hlt">earthquake</span> rupture, the chirp profiles document <span class="hlt">faults</span> that clearly affect the upper 20 m of sediments. The chirp also imaged an EW-striking ridge that appears to be <span class="hlt">fault</span>-bounded on its north flank and is located about 1 km north of the onshore trace of the EPGF, suggesting that this <span class="hlt">fault</span> <span class="hlt">system</span> affects a relatively broad zone. In Petit Goave Bay, a series of textured, sub-circular mounds rising ~5 m above the sedimented bottom most likely indicate bioherms. These align roughly EW at the base of a 20-30 m-high ridge and may be forming at cold seeps associated with an active <span class="hlt">fault</span> strand, as reported for other offshore transform <span class="hlt">fault</span> <span class="hlt">systems</span>. Lateral spreading and slumps fringe the southern shoreline of that bay. Based on the sharp resolution of the sidescan imagery over the slumps, detailing individual fissures and angular blocks, we interpret these to have been triggered by the 2010 <span class="hlt">earthquake</span>, and that they therefore are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70005804','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70005804"><span>The effect of complex <span class="hlt">fault</span> rupture on the distribution of landslides triggered by the 12 January 2010, Haiti <span class="hlt">earthquake</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Harp, Edwin L.; Jibson, Randall W.; Dart, Richard L.; Margottini, Claudio; Canuti, Paolo; Sassa, Kyoji</p> <p>2013-01-01</p> <p>The MW 7.0, 12 January 2010, Haiti <span class="hlt">earthquake</span> triggered more than 7,000 landslides in the mountainous terrain south of Port-au-Prince over an area that extends approximately 50 km to the east and west from the epicenter and to the southern coast. Most of the triggered landslides were rock and soil slides from 25°–65° slopes within heavily fractured limestone and deeply weathered basalt and basaltic breccia. Landslide volumes ranged from tens of cubic meters to several thousand cubic meters. Rock slides in limestone typically were 2–5 m thick; slides within soils and weathered basalt typically were less than 1 m thick. Twenty to thirty larger landslides having volumes greater than 10,000 m3 were triggered by the <span class="hlt">earthquake</span>; these included block slides and rotational slumps in limestone bedrock. Only a few landslides larger than 5,000 m3 occurred in the weathered basalt. The distribution of landslides is asymmetric with respect to the <span class="hlt">fault</span> source and epicenter. Relatively few landslides were triggered north of the <span class="hlt">fault</span> source on the hanging wall. The densest landslide concentrations lie south of the <span class="hlt">fault</span> source and the Enriquillo-Plantain-Garden <span class="hlt">fault</span> zone on the footwall. Numerous landslides also occurred along the south coast west of Jacmél. This asymmetric distribution of landsliding with respect to the <span class="hlt">fault</span> source is unusual given the modeled displacement of the <span class="hlt">fault</span> source as mainly thrust motion to the south on a plane dipping to the north at approximately 55°; landslide concentrations in other documented thrust <span class="hlt">earthquakes</span> generally have been greatest on the hanging wall. This apparent inconsistency of the landslide distribution with respect to the <span class="hlt">fault</span> model remains poorly understood given the lack of any strong-motion instruments within Haiti during the <span class="hlt">earthquake</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S53A2808Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S53A2808Q"><span>Dynamic <span class="hlt">Earthquake</span> Triggering on Seismogenic <span class="hlt">Faults</span> in Oklahoma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qin, Y.; Chen, X.; Peng, Z.; Aiken, C.</p> <p>2016-12-01</p> <p>Regions with high pore pressure are generally more susceptible to dynamic triggering from transient stress change caused by surface wave of distant <span class="hlt">earthquakes</span>. The stress threshold from triggering studies can help understand the stress state of seismogenic <span class="hlt">faults</span>. The recent dramatic seismicity increase in central US provides a rich database for assessing dynamic triggering phenomena. We begin our study by conducting a systematic analysis of dynamic triggering for the continental U.S using ANSS catalog (with magnitude of completeness Mc=3) from 49 global mainshocks (Ms>6.5, depth<100km, estimated dynamic stress>1kPa). We calculate β value for each 1° by 1° bins in 30 days before and 10 days after the mainshock. To identify regions that experience triggering from a distant mainshock, we generate a stacked map using β≥2 - which represents significant seismicity rate increase. As expected, the geothermal and volcanic fields in California show clear response to distant <span class="hlt">earthquakes</span>. We also note areas in Oklahoma and north Texas show enhanced triggering, where wastewater-injection induced seismicity are occurring. Next we focus on Oklahoma and use a local catalog from Oklahoma Geological Survey with lower completeness threshold Mc to calculate the beta map in 0.2° by 0.2° bins for each selected mainshock to obtain finer spatial resolutions of the triggering behavior. For those grids with β larger than 2.0, we use waveforms from nearby stations to search for triggered events. The April 2015 M7.8 Nepal <span class="hlt">earthquake</span> causes a statistically significant increase of local seismicity (β=3.5) in the Woodward area (west Oklahoma) during an on-going <span class="hlt">earthquake</span> sequence. By visually examining the surface wave from the nearest station, we identify 3 larger local events, and 10 additional smaller events with weaker but discernable amplitude. Preliminary analysis shows that the triggering is related to Rayleigh wave, which would cause dilatational or shear stress changes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51J..08N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51J..08N"><span>­Tectonic and geomorphic setting of the Pamir Plateau: Insights from InSAR and teleseismic analysis of the 2015 Lake Saurez and 2016 Muji <span class="hlt">fault</span> <span class="hlt">earthquake</span> sequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nanjundiah, P.; Barbot, S.; Wei, S.; Tapponnier, P.; Feng, W.; Wang, T.</p> <p>2017-12-01</p> <p>The Pamir Plateau lies on the western edge of the India- Eurasia collision zone and has been the sight of complex subduction regime in the past 50 Ma. In our study, we focus on two <span class="hlt">earthquakes</span> and their aftershocks that occurred between December 2015 and December 2016. The first <span class="hlt">earthquake</span> (Mw7.2), on 7 December 2015 between the Karakoram and Darwas <span class="hlt">fault</span> <span class="hlt">systems</span>, was sinstral strike slip in nature. The <span class="hlt">earthquake</span> on 25 November (Mw6.6) occurred on the western end of Muji <span class="hlt">Fault</span>, a dextral strike slip <span class="hlt">fault</span> with an avg slip rate of 4mm/yr. We aim to better understand the structure, stress and deformation patterns in the northern and central Pamir plateau by analyzing InSAR, teleseismic, and optical data for these events and their aftershocks. We aim to better understand the structure, stress and deformation patterns in the northern and central Pamir plateau by analysing InSAR, teleseismic, and optical data for these events and their aftershocks. We constrain the <span class="hlt">fault</span> geometry by precisely relocating aftershocks using the double difference technique implemented in HypoDD (Waldhauser & Ellsworth 2000). We used the Green's functions of Okada (1992) to invert for slip on the <span class="hlt">fault</span> with rectangular dislocation and edgreen to numerically invert for the slip in a layered medium (Wang et al. 2003). The surface rupture of the December 2015 Lake Saurez <span class="hlt">earthquake</span> shows evidence of multiple segments and step-overs. The combination of data sets used in this study highlights the existence of a seismic gap south of Lake Karakul as well as coupling between the Muji and Darwas-Karakoram <span class="hlt">fault</span> <span class="hlt">systems</span>. Mapping of past ruptures shows that the Sarez <span class="hlt">fault</span> continues along the eastern coast of Lake Karakul almost until the Muji <span class="hlt">fault</span>. With near field geodetic data in the form of InSAR, we can get a better insight into complex <span class="hlt">fault</span> structures as well as post seismic slip and strain along the <span class="hlt">faults</span> and its surroundings. We emphasize the role of smaller <span class="hlt">faults</span> and their interactions in</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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