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Keck Combined Strong-Motion/Broadband Obs
KECK COMBINED STRONG-MOTION/BROADBAND OBS WHOI Ocean Bottom Seismograph Laboratory W.M. Keck Foundation Award to Understand Earthquake Predictability at East Pacific Rise Transform Faults. • In 2006, the W.M. Keck Foundation awarded funding to Jeff McGuire and John Collins to determine the physical mechanisms responsible for the observed capability to predict, using foreshocks, large (Mw ~6) transform-fault earthquakes at the East Pacific Rise, and to gain greater insight into the fundamentals of earthquake mechanics in general. • Achieving this objective required building 10 OBS of a new and unique type that could record, without saturation, the large ground motions generated by moderate to large earthquakes at distances of less than ~10 km. W.M. Keck OBS: Combined Broadband Seismometer and Strong-Motion Accelerometer • The broadband OBS available from OBSIP carry a broadband seismometer whose performance is optimized to resolve the earth’s background noise, which can be as small as 10-11 g r.m.s. in a bandwidth of width 1/6 decade at periods of about 100 s. Thus, these sensors are ideal for resolving ground motions from large distant earthquakes, necessary for structural seismology studies. • Ground motions from local, moderate to large earthquakes can generate accelerations of up a g or more, which would saturate or clip these sensors. Currently, there are no sensors (or data-loggers) that have a dynamic range to resolve this ~220 dB range of ground motion. • To overcome this limitation, we used Keck Foundation funding to build 10 OBS equipped with both a conventional broadband seismometer and a strong- motion accelerometer with a clip level of 2.5 g. -
STRUCTURE of EARTH S-Wave Shadow P-Wave Shadow P-Wave
STRUCTURE OF EARTH Earthquake Focus P-wave P-wave shadow shadow S-wave shadow P waves = Primary waves = Pressure waves S waves = Secondary waves = Shear waves (Don't penetrate liquids) CRUST < 50-70 km thick MANTLE = 2900 km thick OUTER CORE (Liquid) = 3200 km thick INNER CORE (Solid) = 1300 km radius. STRUCTURE OF EARTH Low Velocity Crust Zone Whole Mantle Convection Lithosphere Upper Mantle Transition Zone Layered Mantle Convection Lower Mantle S-wave P-wave CRUST : Conrad discontinuity = upper / lower crust boundary Mohorovicic discontinuity = base of Continental Crust (35-50 km continents; 6-8 km oceans) MANTLE: Lithosphere = Rigid Mantle < 100 km depth Asthenosphere = Plastic Mantle > 150 km depth Low Velocity Zone = Partially Melted, 100-150 km depth Upper Mantle < 410 km Transition Zone = 400-600 km --> Velocity increases rapidly Lower Mantle = 600 - 2900 km Outer Core (Liquid) 2900-5100 km Inner Core (Solid) 5100-6400 km Center = 6400 km UPPER MANTLE AND MAGMA GENERATION A. Composition of Earth Density of the Bulk Earth (Uncompressed) = 5.45 gm/cm3 Densities of Common Rocks: Granite = 2.55 gm/cm3 Peridotite, Eclogite = 3.2 to 3.4 gm/cm3 Basalt = 2.85 gm/cm3 Density of the CORE (estimated) = 7.2 gm/cm3 Fe-metal = 8.0 gm/cm3, Ni-metal = 8.5 gm/cm3 EARTH must contain a mix of Rock and Metal . Stony meteorites Remains of broken planets Planetary Interior Rock=Stony Meteorites ÒChondritesÓ = Olivine, Pyroxene, Metal (Fe-Ni) Metal = Fe-Ni Meteorites Core density = 7.2 gm/cm3 -- Too Light for Pure Fe-Ni Light elements = O2 (FeO) or S (FeS) B. -
Seismic Wavefield Imaging of Earth's Interior Across Scales
TECHNICAL REVIEWS Seismic wavefield imaging of Earth’s interior across scales Jeroen Tromp Abstract | Seismic full- waveform inversion (FWI) for imaging Earth’s interior was introduced in the late 1970s. Its ultimate goal is to use all of the information in a seismogram to understand the structure and dynamics of Earth, such as hydrocarbon reservoirs, the nature of hotspots and the forces behind plate motions and earthquakes. Thanks to developments in high- performance computing and advances in modern numerical methods in the past 10 years, 3D FWI has become feasible for a wide range of applications and is currently used across nine orders of magnitude in frequency and wavelength. A typical FWI workflow includes selecting seismic sources and a starting model, conducting forward simulations, calculating and evaluating the misfit, and optimizing the simulated model until the observed and modelled seismograms converge on a single model. This method has revealed Pleistocene ice scrapes beneath a gas cloud in the Valhall oil field, overthrusted Iberian crust in the western Pyrenees mountains, deep slabs in subduction zones throughout the world and the shape of the African superplume. The increased use of multi- parameter inversions, improved computational and algorithmic efficiency , and the inclusion of Bayesian statistics in the optimization process all stand to substantially improve FWI, overcoming current computational or data- quality constraints. In this Technical Review, FWI methods and applications in controlled- source and earthquake seismology are discussed, followed by a perspective on the future of FWI, which will ultimately result in increased insight into the physics and chemistry of Earth’s interior. -
Earthquake Measurements
EARTHQUAKE MEASUREMENTS The vibrations produced by earthquakes are detected, recorded, and measured by instruments call seismographs1. The zig-zag line made by a seismograph, called a "seismogram," reflects the changing intensity of the vibrations by responding to the motion of the ground surface beneath the instrument. From the data expressed in seismograms, scientists can determine the time, the epicenter, the focal depth, and the type of faulting of an earthquake and can estimate how much energy was released. Seismograph/Seismometer Earthquake recording instrument, seismograph has a base that sets firmly in the ground, and a heavy weight that hangs free2. When an earthquake causes the ground to shake, the base of the seismograph shakes too, but the hanging weight does not. Instead the spring or string that it is hanging from absorbs all the movement. The difference in position between the shaking part of the seismograph and the motionless part is Seismograph what is recorded. Measuring Size of Earthquakes The size of an earthquake depends on the size of the fault and the amount of slip on the fault, but that’s not something scientists can simply measure with a measuring tape since faults are many kilometers deep beneath the earth’s surface. They use the seismogram recordings made on the seismographs at the surface of the earth to determine how large the earthquake was. A short wiggly line that doesn’t wiggle very much means a small earthquake, and a long wiggly line that wiggles a lot means a large earthquake2. The length of the wiggle depends on the size of the fault, and the size of the wiggle depends on the amount of slip. -
BY JOHNATHAN EVANS What Exactly Is an Earthquake?
Earthquakes BY JOHNATHAN EVANS What Exactly is an Earthquake? An Earthquake is what happens when two blocks of the earth are pushing against one another and then suddenly slip past each other. The surface where they slip past each other is called the fault or fault plane. The area below the earth’s surface where the earthquake starts is called the Hypocenter, and the area directly above it on the surface is called the “Epicenter”. What are aftershocks/foreshocks? Sometimes earthquakes have Foreshocks. Foreshocks are smaller earthquakes that happen in the same place as the larger earthquake that follows them. Scientists can not tell whether an earthquake is a foreshock until after the larger earthquake happens. The biggest, main earthquake is called the mainshock. The mainshocks always have aftershocks that follow the main earthquake. Aftershocks are smaller earthquakes that happen afterwards in the same location as the mainshock. Depending on the size of the mainshock, Aftershocks can keep happening for weeks, months, or even years after the mainshock happened. Why do earthquakes happen? Earthquakes happen because all the rocks that make up the earth are full of fractures. On some of the fractures that are known as faults, these rocks slip past each other when the crust rearranges itself in a process known as plate tectonics. But the problem is, rocks don’t slip past each other easily because they are stiff, rough and their under a lot of pressure from rocks around and above them. Because of that, rocks can pull at or push on each other on either side of a fault for long periods of time without moving much at all, which builds up a lot of stress in the rocks. -
Characteristics of Foreshocks and Short Term Deformation in the Source Area of Major Earthquakes
Characteristics of Foreshocks and Short Term Deformation in the Source Area of Major Earthquakes Peter Molnar Massachusetts Institute of Technology 77 Massachusetts Avenue Cambridge, Massachusetts 02139 USGS CONTRACT NO. 14-08-0001-17759 Supported by the EARTHQUAKE HAZARDS REDUCTION PROGRAM OPEN-FILE NO.81-287 U.S. Geological Survey OPEN FILE REPORT This report was prepared under contract to the U.S. Geological Survey and has not been reviewed for conformity with USGS editorial standards and stratigraphic nomenclature. Opinions and conclusions expressed herein do not necessarily represent those of the USGS. Any use of trade names is for descriptive purposes only and does not imply endorsement by the USGS. Appendix A A Study of the Haicheng Foreshock Sequence By Lucile Jones, Wang Biquan and Xu Shaoxie (English Translation of a Paper Published in Di Zhen Xue Bao (Journal of Seismology), 1980.) Abstract We have examined the locations and radiation patterns of the foreshocks to the 4 February 1978 Haicheng earthquake. Using four stations, the foreshocks were located relative to a master event. They occurred very close together, no more than 6 kilo meters apart. Nevertheless, there appear to have been too clusters of foreshock activity. The majority of events seem to have occurred in a cluster to the east of the master event along a NNE-SSW trend. Moreover, all eight foreshocks that we could locate and with a magnitude greater than 3.0 occurred in this group. The're also "appears to be a second cluster of foresfiocks located to the northwest of the first. Thus it seems possible that the majority of foreshocks did not occur on the rupture plane of the mainshock, which trends WNW, but on another plane nearly perpendicualr to the mainshock. -
Chapter 2 the Evolution of Seismic Monitoring Systems at the Hawaiian Volcano Observatory
Characteristics of Hawaiian Volcanoes Editors: Michael P. Poland, Taeko Jane Takahashi, and Claire M. Landowski U.S. Geological Survey Professional Paper 1801, 2014 Chapter 2 The Evolution of Seismic Monitoring Systems at the Hawaiian Volcano Observatory By Paul G. Okubo1, Jennifer S. Nakata1, and Robert Y. Koyanagi1 Abstract the Island of Hawai‘i. Over the past century, thousands of sci- entific reports and articles have been published in connection In the century since the Hawaiian Volcano Observatory with Hawaiian volcanism, and an extensive bibliography has (HVO) put its first seismographs into operation at the edge of accumulated, including numerous discussions of the history of Kīlauea Volcano’s summit caldera, seismic monitoring at HVO HVO and its seismic monitoring operations, as well as research (now administered by the U.S. Geological Survey [USGS]) has results. From among these references, we point to Klein and evolved considerably. The HVO seismic network extends across Koyanagi (1980), Apple (1987), Eaton (1996), and Klein and the entire Island of Hawai‘i and is complemented by stations Wright (2000) for details of the early growth of HVO’s seismic installed and operated by monitoring partners in both the USGS network. In particular, the work of Klein and Wright stands and the National Oceanic and Atmospheric Administration. The out because their compilation uses newspaper accounts and seismic data stream that is available to HVO for its monitoring other reports of the effects of historical earthquakes to extend of volcanic and seismic activity in Hawai‘i, therefore, is built Hawai‘i’s detailed seismic history to nearly a century before from hundreds of data channels from a diverse collection of instrumental monitoring began at HVO. -
Formation and Evolution of a Population of Strike-Slip Faults in a Multiscale Cellular Automaton Model
Geophys. J. Int. (2007) 168, 723–744 doi: 10.1111/j.1365-246X.2006.03213.x Formation and evolution of a population of strike-slip faults in a multiscale cellular automaton model Cl´ement Narteau Laboratoire de Dynamique des Syst`emes G´eologiques, Institut de Physique du Globe de Paris, 4, Place Jussieu, Paris, Cedex 05, 75252, France. E-mail: [email protected] Accepted 2006 September 4. Received 2006 September 4; in original form 2004 August 10 SUMMARY This paper describes a new model of rupture designed to reproduce structural patterns observed in the formation and evolution of a population of strike-slip faults. This model is a multiscale cellular automaton with two states. A stable state is associated with an ‘intact’ zone in which the fracturing process is confined to a smaller length scale. An active state is associated with an actively slipping fault. At the smallest length scale of a fault segment, transition rates from one state to another are determined with respect to the magnitude of the local strain rate and a time-dependent stochastic process. At increasingly larger length scales, healing and faulting are described according to geometric rules of fault interaction based on fracture mechanics. A redistribution of the strain rates in the neighbourhood of active faults at all length scales ensures that long range interactions and non-linear feedback processes are incorporated in the fault growth mechanism. Typical patterns of development of a population of faults are presented and show nucleation, growth, branching, interaction and coalescence. The geometries of the fault populations spontaneously converge to a configuration in which strain is concentrated on a dominant fault. -
PEAT8002 - SEISMOLOGY Lecture 13: Earthquake Magnitudes and Moment
PEAT8002 - SEISMOLOGY Lecture 13: Earthquake magnitudes and moment Nick Rawlinson Research School of Earth Sciences Australian National University Earthquake magnitudes and moment Introduction In the last two lectures, the effects of the source rupture process on the pattern of radiated seismic energy was discussed. However, even before earthquake mechanisms were studied, the priority of seismologists, after locating an earthquake, was to quantify their size, both for scientific purposes and hazard assessment. The first measure introduced was the magnitude, which is based on the amplitude of the emanating waves recorded on a seismogram. The idea is that the wave amplitude reflects the earthquake size once the amplitudes are corrected for the decrease with distance due to geometric spreading and attenuation. Earthquake magnitudes and moment Introduction Magnitude scales thus have the general form: A M = log + F(h, ∆) + C T where A is the amplitude of the signal, T is its dominant period, F is a correction for the variation of amplitude with the earthquake’s depth h and angular distance ∆ from the seismometer, and C is a regional scaling factor. Magnitude scales are logarithmic, so an increase in one unit e.g. from 5 to 6, indicates a ten-fold increase in seismic wave amplitude. Note that since a log10 scale is used, magnitudes can be negative for very small displacements. For example, a magnitude -1 earthquake might correspond to a hammer blow. Earthquake magnitudes and moment Richter magnitude The concept of earthquake magnitude was introduced by Charles Richter in 1935 for southern California earthquakes. He originally defined earthquake magnitude as the logarithm (to the base 10) of maximum amplitude measured in microns on the record of a standard torsion seismograph with a pendulum period of 0.8 s, magnification of 2800, and damping factor 0.8, located at a distance of 100 km from the epicenter. -
Paper 4: Seismic Methods for Determining Earthquake Source
Paper 4: Seismic methods for determining earthquake source parameters and lithospheric structure WALTER D. MOONEY U.S. Geological Survey, MS 977, 345 Middlefield Road, Menlo Park, California 94025 For referring to this paper: Mooney, W. D., 1989, Seismic methods for determining earthquake source parameters and lithospheric structure, in Pakiser, L. C., and Mooney, W. D., Geophysical framework of the continental United States: Boulder, Colorado, Geological Society of America Memoir 172. ABSTRACT The seismologic methods most commonly used in studies of earthquakes and the structure of the continental lithosphere are reviewed in three main sections: earthquake source parameter determinations, the determination of earth structure using natural sources, and controlled-source seismology. The emphasis in each section is on a description of data, the principles behind the analysis techniques, and the assumptions and uncertainties in interpretation. Rather than focusing on future directions in seismology, the goal here is to summarize past and current practice as a companion to the review papers in this volume. Reliable earthquake hypocenters and focal mechanisms require seismograph locations with a broad distribution in azimuth and distance from the earthquakes; a recording within one focal depth of the epicenter provides excellent hypocentral depth control. For earthquakes of magnitude greater than 4.5, waveform modeling methods may be used to determine source parameters. The seismic moment tensor provides the most complete and accurate measure of earthquake source parameters, and offers a dynamic picture of the faulting process. Methods for determining the Earth's structure from natural sources exist for local, regional, and teleseismic sources. One-dimensional models of structure are obtained from body and surface waves using both forward and inverse modeling. -
Modelling Seismic Wave Propagation for Geophysical Imaging J
Modelling Seismic Wave Propagation for Geophysical Imaging J. Virieux, V. Etienne, V. Cruz-Atienza, R. Brossier, E. Chaljub, O. Coutant, S. Garambois, D. Mercerat, V. Prieux, S. Operto, et al. To cite this version: J. Virieux, V. Etienne, V. Cruz-Atienza, R. Brossier, E. Chaljub, et al.. Modelling Seismic Wave Propagation for Geophysical Imaging. Seismic Waves - Research and Analysis, Masaki Kanao, 253- 304, Chap.13, 2012, 978-953-307-944-8. hal-00682707 HAL Id: hal-00682707 https://hal.archives-ouvertes.fr/hal-00682707 Submitted on 5 Apr 2012 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 130 Modelling Seismic Wave Propagation for Geophysical Imaging Jean Virieux et al.1,* Vincent Etienne et al.2†and Victor Cruz-Atienza et al.3‡ 1ISTerre, Université Joseph Fourier, Grenoble 2GeoAzur, Centre National de la Recherche Scientifique, Institut de Recherche pour le développement 3Instituto de Geofisica, Departamento de Sismologia, Universidad Nacional Autónoma de México 1,2France 3Mexico 1. Introduction − The Earth is an heterogeneous complex media from -
Earthquake Location Accuracy
Theme IV - Understanding Seismicity Catalogs and their Problems Earthquake Location Accuracy 1 2 Stephan Husen • Jeanne L. Hardebeck 1. Swiss Seismological Service, ETH Zurich 2. United States Geological Survey How to cite this article: Husen, S., and J.L. Hardebeck (2010), Earthquake location accuracy, Community Online Resource for Statistical Seismicity Analysis, doi:10.5078/corssa-55815573. Available at http://www.corssa.org. Document Information: Issue date: 1 September 2010 Version: 1.0 2 www.corssa.org Contents 1 Motivation .................................................................................................................................................. 3 2 Location Techniques ................................................................................................................................... 4 3 Uncertainty and Artifacts .......................................................................................................................... 9 4 Choosing a Catalog, and What to Expect ................................................................................................ 25 5 Summary, Further Reading, Next Steps ................................................................................................... 30 Earthquake Location Accuracy 3 Abstract Earthquake location catalogs are not an exact representation of the true earthquake locations. They contain random error, for example from errors in the arrival time picks, as well as systematic biases. The most important source of systematic