Sample records for seismic interpretation abstracts

  1. Interpreting Abstract Interpretations in Membership Equational Logic

    NASA Technical Reports Server (NTRS)

    Fischer, Bernd; Rosu, Grigore

    2001-01-01

    We present a logical framework in which abstract interpretations can be naturally specified and then verified. Our approach is based on membership equational logic which extends equational logics by membership axioms, asserting that a term has a certain sort. We represent an abstract interpretation as a membership equational logic specification, usually as an overloaded order-sorted signature with membership axioms. It turns out that, for any term, its least sort over this specification corresponds to its most concrete abstract value. Maude implements membership equational logic and provides mechanisms to calculate the least sort of a term efficiently. We first show how Maude can be used to get prototyping of abstract interpretations "for free." Building on the meta-logic facilities of Maude, we further develop a tool that automatically checks and abstract interpretation against a set of user-defined properties. This can be used to select an appropriate abstract interpretation, to characterize the specified loss of information during abstraction, and to compare different abstractions with each other.

  2. Abstract Interpreters for Free

    NASA Astrophysics Data System (ADS)

    Might, Matthew

    In small-step abstract interpretations, the concrete and abstract semantics bear an uncanny resemblance. In this work, we present an analysis-design methodology that both explains and exploits that resemblance. Specifically, we present a two-step method to convert a small-step concrete semantics into a family of sound, computable abstract interpretations. The first step re-factors the concrete state-space to eliminate recursive structure; this refactoring of the state-space simultaneously determines a store-passing-style transformation on the underlying concrete semantics. The second step uses inference rules to generate an abstract state-space and a Galois connection simultaneously. The Galois connection allows the calculation of the "optimal" abstract interpretation. The two-step process is unambiguous, but nondeterministic: at each step, analysis designers face choices. Some of these choices ultimately influence properties such as flow-, field- and context-sensitivity. Thus, under the method, we can give the emergence of these properties a graph-theoretic characterization. To illustrate the method, we systematically abstract the continuation-passing style lambda calculus to arrive at two distinct families of analyses. The first is the well-known k-CFA family of analyses. The second consists of novel "environment-centric" abstract interpretations, none of which appear in the literature on static analysis of higher-order programs.

  3. Calibration method helps in seismic velocity interpretation

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

    Guzman, C.E.; Davenport, H.A.; Wilhelm, R.

    1997-11-03

    Acoustic velocities derived from seismic reflection data, when properly calibrated to subsurface measurements, help interpreters make pure velocity predictions. A method of calibrating seismic to measured velocities has improved interpretation of subsurface features in the Gulf of Mexico. In this method, the interpreter in essence creates a kind of gauge. Properly calibrated, the gauge enables the interpreter to match predicted velocities to velocities measured at wells. Slow-velocity zones are of special interest because they sometimes appear near hydrocarbon accumulations. Changes in velocity vary in strength with location; the structural picture is hidden unless the variations are accounted for by mappingmore » in depth instead of time. Preliminary observations suggest that the presence of hydrocarbons alters the lithology in the neighborhood of the trap; this hydrocarbon effect may be reflected in the rock velocity. The effect indicates a direct use of seismic velocity in exploration. This article uses the terms seismic velocity and seismic stacking velocity interchangeably. It uses ground velocity, checkshot average velocity, and well velocity interchangeably. Interval velocities are derived from seismic stacking velocities or well average velocities; they refer to velocities of subsurface intervals or zones. Interval travel time (ITT) is the reciprocal of interval velocity in microseconds per foot.« less

  4. Quantitative Seismic Interpretation: Applying Rock Physics Tools to Reduce Interpretation Risk

    NASA Astrophysics Data System (ADS)

    Sondergeld, Carl H.

    This book is divided into seven chapters that cover rock physics, statistical rock physics, seismic inversion techniques, case studies, and work flows. On balance, the emphasis is on rock physics. Included are 56 color figures that greatly help in the interpretation of more complicated plots and displays.The domain of rock physics falls between petrophysics and seismics. It is the basis for interpreting seismic observations and therefore is pivotal to the understanding of this book. The first two chapters are dedicated to this topic (109 pages).

  5. Structural interpretation of seismic data and inherent uncertainties

    NASA Astrophysics Data System (ADS)

    Bond, Clare

    2013-04-01

    Geoscience is perhaps unique in its reliance on incomplete datasets and building knowledge from their interpretation. This interpretation basis for the science is fundamental at all levels; from creation of a geological map to interpretation of remotely sensed data. To teach and understand better the uncertainties in dealing with incomplete data we need to understand the strategies individual practitioners deploy that make them effective interpreters. The nature of interpretation is such that the interpreter needs to use their cognitive ability in the analysis of the data to propose a sensible solution in their final output that is both consistent not only with the original data but also with other knowledge and understanding. In a series of experiments Bond et al. (2007, 2008, 2011, 2012) investigated the strategies and pitfalls of expert and non-expert interpretation of seismic images. These studies focused on large numbers of participants to provide a statistically sound basis for analysis of the results. The outcome of these experiments showed that a wide variety of conceptual models were applied to single seismic datasets. Highlighting not only spatial variations in fault placements, but whether interpreters thought they existed at all, or had the same sense of movement. Further, statistical analysis suggests that the strategies an interpreter employs are more important than expert knowledge per se in developing successful interpretations. Experts are successful because of their application of these techniques. In a new set of experiments a small number of experts are focused on to determine how they use their cognitive and reasoning skills, in the interpretation of 2D seismic profiles. Live video and practitioner commentary were used to track the evolving interpretation and to gain insight on their decision processes. The outputs of the study allow us to create an educational resource of expert interpretation through online video footage and commentary with

  6. Modelling Metamorphism by Abstract Interpretation

    NASA Astrophysics Data System (ADS)

    Dalla Preda, Mila; Giacobazzi, Roberto; Debray, Saumya; Coogan, Kevin; Townsend, Gregg M.

    Metamorphic malware apply semantics-preserving transformations to their own code in order to foil detection systems based on signature matching. In this paper we consider the problem of automatically extract metamorphic signatures from these malware. We introduce a semantics for self-modifying code, later called phase semantics, and prove its correctness by showing that it is an abstract interpretation of the standard trace semantics. Phase semantics precisely models the metamorphic code behavior by providing a set of traces of programs which correspond to the possible evolutions of the metamorphic code during execution. We show that metamorphic signatures can be automatically extracted by abstract interpretation of the phase semantics, and that regular metamorphism can be modelled as finite state automata abstraction of the phase semantics.

  7. What defines an Expert? - Uncertainty in the interpretation of seismic data

    NASA Astrophysics Data System (ADS)

    Bond, C. E.

    2008-12-01

    Studies focusing on the elicitation of information from experts are concentrated primarily in economics and world markets, medical practice and expert witness testimonies. Expert elicitation theory has been applied in the natural sciences, most notably in the prediction of fluid flow in hydrological studies. In the geological sciences expert elicitation has been limited to theoretical analysis with studies focusing on the elicitation element, gaining expert opinion rather than necessarily understanding the basis behind the expert view. In these cases experts are defined in a traditional sense, based for example on: standing in the field, no. of years of experience, no. of peer reviewed publications, the experts position in a company hierarchy or academia. Here traditional indicators of expertise have been compared for significance on affective seismic interpretation. Polytomous regression analysis has been used to assess the relative significance of length and type of experience on the outcome of a seismic interpretation exercise. Following the initial analysis the techniques used by participants to interpret the seismic image were added as additional variables to the analysis. Specific technical skills and techniques were found to be more important for the affective geological interpretation of seismic data than the traditional indicators of expertise. The results of a seismic interpretation exercise, the techniques used to interpret the seismic and the participant's prior experience have been combined and analysed to answer the question - who is and what defines an expert?

  8. On the Power of Abstract Interpretation

    NASA Technical Reports Server (NTRS)

    Reddy, Uday S.; Kamin, Samuel N.

    1991-01-01

    Increasingly sophisticated applications of static analysis place increased burden on the reliability of the analysis techniques. Often, the failure of the analysis technique to detect some information my mean that the time or space complexity of the generated code would be altered. Thus, it is important to precisely characterize the power of static analysis techniques. We follow the approach of Selur et. al. who studied the power of strictness analysis techniques. Their result can be summarized by saying 'strictness analysis is perfect up to variations in constants.' In other words, strictness analysis is as good as it could be, short of actually distinguishing between concrete values. We use this approach to characterize a broad class of analysis techniques based on abstract interpretation including, but not limited to, strictness analysis. For the first-order case, we consider abstract interpretations where the abstract domain for data values is totally ordered. This condition is satisfied by Mycroft's strictness analysis that of Sekar et. al. and Wadler's analysis of list-strictness. For such abstract interpretations, we show that the analysis is complete in the sense that, short of actually distinguishing between concrete values with the same abstraction, it gives the best possible information. We further generalize these results to typed lambda calculus with pairs and higher-order functions. Note that products and function spaces over totally ordered domains are not totally ordered. In fact, the notion of completeness used in the first-order case fails if product domains or function spaces are added. We formulate a weaker notion of completeness based on observability of values. Two values (including pairs and functions) are considered indistinguishable if their observable components are indistinguishable. We show that abstract interpretation of typed lambda calculus programs is complete up to this notion of indistinguishability. We use denotationally

  9. Accessing seismic data through geological interpretation: Challenges and solutions

    NASA Astrophysics Data System (ADS)

    Butler, R. W.; Clayton, S.; McCaffrey, B.

    2008-12-01

    Between them, the world's research programs, national institutions and corporations, especially oil and gas companies, have acquired substantial volumes of seismic reflection data. Although the vast majority are proprietary and confidential, significant data are released and available for research, including those in public data libraries. The challenge now is to maximise use of these data, by providing routes to seismic not simply on the basis of acquisition or processing attributes but via the geology they image. The Virtual Seismic Atlas (VSA: www.seismicatlas.org) meets this challenge by providing an independent, free-to-use community based internet resource that captures and shares the geological interpretation of seismic data globally. Images and associated documents are explicitly indexed by extensive metadata trees, using not only existing survey and geographical data but also the geology they portray. The solution uses a Documentum database interrogated through Endeca Guided Navigation, to search, discover and retrieve images. The VSA allows users to compare contrasting interpretations of clean data thereby exploring the ranges of uncertainty in the geometric interpretation of subsurface structure. The metadata structures can be used to link reports and published research together with other data types such as wells. And the VSA can link to existing data libraries. Searches can take different paths, revealing arrays of geological analogues, new datasets while providing entirely novel insights and genuine surprises. This can then drive new creative opportunities for research and training, and expose the contents of seismic data libraries to the world.

  10. Classical seismic sequence stratigraphic interpretation of intraslope basin fill: Deepwater Nigeria

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

    Duncan, E.A.

    Detailed interpretation of seismic facies patterns performed within the workstation environment provides an observation based methodology for constructing depositional models of turbidite and other reservoir bearing systems expected in deepwater Nigeria. The increased fidelity of the workstation allows greater detail and accuracy to be imposed onto depositional model construction by vastly improving the discrimination of depositional from structural seismic reflection geometries. In deepwater Nigeria interslope basins, depositional cyclicity is clearly indicated by vertical seismic facies successions in the same way as can be recognized in bed thickness trends from outcrop or well log data. The recognition of the seismic faciesmore » successions appears to break the stratigraphy into at least fourth and fifth order scale sequences. Highly {open_quotes}zoomed{close_quotes} instantaneous phase displays enhance the reflection character so that near outcrop scale (resolution less than 50 mters) interpretations of depositional facies can be made. Common seismic facies and geologic interpretation include: (1) low angle erosional surfaces as channel scour or mass wasting detachment; (2) low relief mounds, often in compensation cycle overlapping stacks reflecting compacted channelbelt fill; (3) unidirectional, low angle clinoform sets suggesting laterial accretion within a channel belt or possible contourite mounds; (4) abrupt, shingled blocks illustrating tilted fault blocks of small scale intraformation slumping; and (5) high reflection amplitude and continuous, parallel reflections of pelagic and hemipelagic condensed sections. There are other subtle seismic facies resolvable given the incraesed fidelity of the workstation interpretation. Mapping and translation of these geometries into more robust stratigraphic predictions should have positive impact on exploration and development success.« less

  11. Static Analysis Using Abstract Interpretation

    NASA Technical Reports Server (NTRS)

    Arthaud, Maxime

    2017-01-01

    Short presentation about static analysis and most particularly abstract interpretation. It starts with a brief explanation on why static analysis is used at NASA. Then, it describes the IKOS (Inference Kernel for Open Static Analyzers) tool chain. Results on NASA projects are shown. Several well known algorithms from the static analysis literature are then explained (such as pointer analyses, memory analyses, weak relational abstract domains, function summarization, etc.). It ends with interesting problems we encountered (such as C++ analysis with exception handling, or the detection of integer overflow).

  12. Automated Fault Interpretation and Extraction using Improved Supplementary Seismic Datasets

    NASA Astrophysics Data System (ADS)

    Bollmann, T. A.; Shank, R.

    2017-12-01

    During the interpretation of seismic volumes, it is necessary to interpret faults along with horizons of interest. With the improvement of technology, the interpretation of faults can be expedited with the aid of different algorithms that create supplementary seismic attributes, such as semblance and coherency. These products highlight discontinuities, but still need a large amount of human interaction to interpret faults and are plagued by noise and stratigraphic discontinuities. Hale (2013) presents a method to improve on these datasets by creating what is referred to as a Fault Likelihood volume. In general, these volumes contain less noise and do not emphasize stratigraphic features. Instead, planar features within a specified strike and dip range are highlighted. Once a satisfactory Fault Likelihood Volume is created, extraction of fault surfaces is much easier. The extracted fault surfaces are then exported to interpretation software for QC. Numerous software packages have implemented this methodology with varying results. After investigating these platforms, we developed a preferred Automated Fault Interpretation workflow.

  13. The Virtual Seismic Atlas Project: sharing the interpretation of seismic data

    NASA Astrophysics Data System (ADS)

    Butler, R.; Mortimer, E.; McCaffrey, B.; Stuart, G.; Sizer, M.; Clayton, S.

    2007-12-01

    Through the activities of academic research programs, national institutions and corporations, especially oil and gas companies, there is a substantial volume of seismic reflection data. Although the majority is proprietary and confidential, there are significant volumes of data that are potentially within the public domain and available for research. Yet the community is poorly connected to these data and consequently geological and other research using seismic reflection data is limited to very few groups of researchers. This is about to change. The Virtual Seismic Atlas (VSA) is generating an independent, free-to-use, community based internet resource that captures and shares the geological interpretation of seismic data globally. Images and associated documents are explicitly indexed using not only existing survey and geographical data but also on the geology they portray. By using "Guided Navigation" to search, discover and retrieve images, users are exposed to arrays of geological analogues that provide novel insights and opportunities for research and education. The VSA goes live, with evolving content and functionality, through 2008. There are opportunities for designed integration with other global data programs in the earth sciences.

  14. Fuzzy logic and image processing techniques for the interpretation of seismic data

    NASA Astrophysics Data System (ADS)

    Orozco-del-Castillo, M. G.; Ortiz-Alemán, C.; Urrutia-Fucugauchi, J.; Rodríguez-Castellanos, A.

    2011-06-01

    Since interpretation of seismic data is usually a tedious and repetitive task, the ability to do so automatically or semi-automatically has become an important objective of recent research. We believe that the vagueness and uncertainty in the interpretation process makes fuzzy logic an appropriate tool to deal with seismic data. In this work we developed a semi-automated fuzzy inference system to detect the internal architecture of a mass transport complex (MTC) in seismic images. We propose that the observed characteristics of a MTC can be expressed as fuzzy if-then rules consisting of linguistic values associated with fuzzy membership functions. The constructions of the fuzzy inference system and various image processing techniques are presented. We conclude that this is a well-suited problem for fuzzy logic since the application of the proposed methodology yields a semi-automatically interpreted MTC which closely resembles the MTC from expert manual interpretation.

  15. A bird's eye view: the cognitive strategies of experts interpreting seismic profiles

    NASA Astrophysics Data System (ADS)

    Bond, C. E.; Butler, R.

    2012-12-01

    Geoscience is perhaps unique in its reliance on incomplete datasets and building knowledge from their interpretation. This interpretation basis for the science is fundamental at all levels; from creation of a geological map to interpretation of remotely sensed data. To teach and understand better the uncertainties in dealing with incomplete data we need to understand the strategies individual practitioners deploy that make them effective interpreters. The nature of interpretation is such that the interpreter needs to use their cognitive ability in the analysis of the data to propose a sensible solution in their final output that is both consistent not only with the original data but also with other knowledge and understanding. In a series of experiments Bond et al. (2007, 2008, 2011, 2012) investigated the strategies and pitfalls of expert and non-expert interpretation of seismic images. These studies focused on large numbers of participants to provide a statistically sound basis for analysis of the results. The outcome of these experiments showed that techniques and strategies are more important than expert knowledge per se in developing successful interpretations. Experts are successful because of their application of these techniques. In a new set of experiments we have focused on a small number of experts to determine how they use their cognitive and reasoning skills, in the interpretation of 2D seismic profiles. Live video and practitioner commentary were used to track the evolving interpretation and to gain insight on their decision processes. The outputs of the study allow us to create an educational resource of expert interpretation through online video footage and commentary with associated further interpretation and analysis of the techniques and strategies employed. This resource will be of use to undergraduate, post-graduate, industry and academic professionals seeking to improve their seismic interpretation skills, develop reasoning strategies for

  16. Application of seismic interpretation in the development of Jerneh Field, Malay Basin

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

    Yusoff, Z.

    1994-07-01

    Development of the Jerneh gas field has been significantly aided by the use of 3-D and site survey seismic interpretations. The two aspects that have been of particular importance are identification of sea-floor and near-surface safety hazards for safe platform installation/development drilling and mapping of reservoirs/hydrocarbons within gas-productive sands of the Miocene groups B, D, and E. Choice of platform location as well as casing design require detailed analysis of sea-floor and near-surface safety hazards. At Jerneh, sea-floor pockmarks near-surface high amplitudes, distributary channels, and minor faults were recognized as potential operational safety hazards. The integration of conventional 3-D andmore » site survey seismic data enabled comprehensive understanding of the occurrence and distribution of potential hazards to platform installation and development well drilling. Three-dimensional seismic interpretation has been instrumental not only in the field structural definition but also in recognition of reservoir trends and hydrocarbon distribution. Additional gas reservoirs were identified by their DHI characteristics and subsequently confirmed by development wells. The innovative use of seismic attribute mapping techniques has been very important in defining both fluid and reservoir distribution in groups B and D. Integration of 3-D seismic data and well-log interpretations has helped in optimal field development, including the planning of well locations and drilling sequence.« less

  17. Information Leakage Analysis by Abstract Interpretation

    NASA Astrophysics Data System (ADS)

    Zanioli, Matteo; Cortesi, Agostino

    Protecting the confidentiality of information stored in a computer system or transmitted over a public network is a relevant problem in computer security. The approach of information flow analysis involves performing a static analysis of the program with the aim of proving that there will not be leaks of sensitive information. In this paper we propose a new domain that combines variable dependency analysis, based on propositional formulas, and variables' value analysis, based on polyhedra. The resulting analysis is strictly more accurate than the state of the art abstract interpretation based analyses for information leakage detection. Its modular construction allows to deal with the tradeoff between efficiency and accuracy by tuning the granularity of the abstraction and the complexity of the abstract operators.

  18. 3-D visualisation and interpretation of seismic attributes extracted from large 3-D seismic datasets: Subregional and prospect evaluation, deepwater Nigeria

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

    Sola, M.; Haakon Nordby, L.; Dailey, D.V.

    High resolution 3-D visualization of horizon interpretation and seismic attributes from large 3-D seismic surveys in deepwater Nigeria has greatly enhanced the exploration team`s ability to quickly recognize prospective segments of subregional and prospect specific scale areas. Integrated workstation generated structure, isopach and extracted horizon consistent, interval and windowed attributes are particularly useful in illustrating the complex structural and stratigraphical prospectivity of deepwater Nigeria. Large 3-D seismic volumes acquired over 750 square kilometers can be manipulated within the visualization system with attribute tracking capability that allows for real time data interrogation and interpretation. As in classical seismic stratigraphic studies, patternmore » recognition is fundamental to effective depositions facies interpretation and reservoir model construction. The 3-D perspective enhances the data interpretation through clear representation of relative scale, spatial distribution and magnitude of attributes. In deepwater Nigeria, many prospective traps rely on an interplay between syndepositional structure and slope turbidite depositional systems. Reservoir systems in many prospects appear to be dominated by unconfined to moderately focused slope feeder channel facies. These units have spatially complex facies architecture with feeder channel axes separated by extensive interchannel areas. Structural culminations generally have a history of initial compressional folding with late in extensional collapse and accommodation faulting. The resulting complex trap configurations often have stacked reservoirs over intervals as thick as 1500 meters. Exploration, appraisal and development scenarios in these settings can be optimized by taking full advantage of integrating high resolution 3-D visualization and seismic workstation interpretation.« less

  19. 3-D visualisation and interpretation of seismic attributes extracted from large 3-D seismic datasets: Subregional and prospect evaluation, deepwater Nigeria

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

    Sola, M.; Haakon Nordby, L.; Dailey, D.V.

    High resolution 3-D visualization of horizon interpretation and seismic attributes from large 3-D seismic surveys in deepwater Nigeria has greatly enhanced the exploration team's ability to quickly recognize prospective segments of subregional and prospect specific scale areas. Integrated workstation generated structure, isopach and extracted horizon consistent, interval and windowed attributes are particularly useful in illustrating the complex structural and stratigraphical prospectivity of deepwater Nigeria. Large 3-D seismic volumes acquired over 750 square kilometers can be manipulated within the visualization system with attribute tracking capability that allows for real time data interrogation and interpretation. As in classical seismic stratigraphic studies, patternmore » recognition is fundamental to effective depositions facies interpretation and reservoir model construction. The 3-D perspective enhances the data interpretation through clear representation of relative scale, spatial distribution and magnitude of attributes. In deepwater Nigeria, many prospective traps rely on an interplay between syndepositional structure and slope turbidite depositional systems. Reservoir systems in many prospects appear to be dominated by unconfined to moderately focused slope feeder channel facies. These units have spatially complex facies architecture with feeder channel axes separated by extensive interchannel areas. Structural culminations generally have a history of initial compressional folding with late in extensional collapse and accommodation faulting. The resulting complex trap configurations often have stacked reservoirs over intervals as thick as 1500 meters. Exploration, appraisal and development scenarios in these settings can be optimized by taking full advantage of integrating high resolution 3-D visualization and seismic workstation interpretation.« less

  20. Structural interpretation from horizontal seismic sections

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

    Brown, A.R.

    1983-03-01

    The interpreter of a 3D survey must use a data volume. Horizontal slices through a data volume, called Seiscrop sections, have unique properties and structural interpretation from them is fast, convenient, and effective. An event on a Seiscrop section displays local strike, a property which permits direct contouring of a structural surface without any timing and posting. The width of an event on a Seiscrop section is a composition of the frequency of the data and the structural dip. Event terminations indicate faults or other discontinuities when they are transverse to structural strike. Faults parallel to structural strike are muchmore » less evident on a single Seiscrop section but become apparent with the relative movement of events from section to section. In practical mapping, we normally contour one fault block before proceeding to the next with the correlation between them being established from the vertical sections. With dual polarity variable area displays, the interpreter can perceive five amplitude levels and normally picks the edge of a trough. With color amplitude Seiscrop sections, it is possible to pick on the crest of any event. With color phase sections the interpreter can pick at any arbitrary but consistent point on the seismic waveform. Subtle structural features are commonly revealed on horizontal sections which may never have been noticed if working from vertical sections alone.« less

  1. SEISVIZ3D: Stereoscopic system for the representation of seismic data - Interpretation and Immersion

    NASA Astrophysics Data System (ADS)

    von Hartmann, Hartwig; Rilling, Stefan; Bogen, Manfred; Thomas, Rüdiger

    2015-04-01

    The seismic method is a valuable tool for getting 3D-images from the subsurface. Seismic data acquisition today is not only a topic for oil and gas exploration but is used also for geothermal exploration, inspections of nuclear waste sites and for scientific investigations. The system presented in this contribution may also have an impact on the visualization of 3D-data of other geophysical methods. 3D-seismic data can be displayed in different ways to give a spatial impression of the subsurface.They are a combination of individual vertical cuts, possibly linked to a cubical portion of the data volume, and the stereoscopic view of the seismic data. By these methods, the spatial perception for the structures and thus of the processes in the subsurface should be increased. Stereoscopic techniques are e. g. implemented in the CAVE and the WALL, both of which require a lot of space and high technical effort. The aim of the interpretation system shown here is stereoscopic visualization of seismic data at the workplace, i.e. at the personal workstation and monitor. The system was developed with following criteria in mind: • Fast rendering of large amounts of data so that a continuous view of the data when changing the viewing angle and the data section is possible, • defining areas in stereoscopic view to translate the spatial impression directly into an interpretation, • the development of an appropriate user interface, including head-tracking, for handling the increased degrees of freedom, • the possibility of collaboration, i.e. teamwork and idea exchange with the simultaneous viewing of a scene at remote locations. The possibilities offered by the use of a stereoscopic system do not replace a conventional interpretation workflow. Rather they have to be implemented into it as an additional step. The amplitude distribution of the seismic data is a challenge for the stereoscopic display because the opacity level and the scaling and selection of the data have to

  2. Integrating sequence stratigraphy and rock-physics to interpret seismic amplitudes and predict reservoir quality

    NASA Astrophysics Data System (ADS)

    Dutta, Tanima

    This dissertation focuses on the link between seismic amplitudes and reservoir properties. Prediction of reservoir properties, such as sorting, sand/shale ratio, and cement-volume from seismic amplitudes improves by integrating knowledge from multiple disciplines. The key contribution of this dissertation is to improve the prediction of reservoir properties by integrating sequence stratigraphy and rock physics. Sequence stratigraphy has been successfully used for qualitative interpretation of seismic amplitudes to predict reservoir properties. Rock physics modeling allows quantitative interpretation of seismic amplitudes. However, often there is uncertainty about selecting geologically appropriate rock physics model and its input parameters, away from the wells. In the present dissertation, we exploit the predictive power of sequence stratigraphy to extract the spatial trends of sedimentological parameters that control seismic amplitudes. These spatial trends of sedimentological parameters can serve as valuable constraints in rock physics modeling, especially away from the wells. Consequently, rock physics modeling, integrated with the trends from sequence stratigraphy, become useful for interpreting observed seismic amplitudes away from the wells in terms of underlying sedimentological parameters. We illustrate this methodology using a comprehensive dataset from channelized turbidite systems, deposited in minibasin settings in the offshore Equatorial Guinea, West Africa. First, we present a practical recipe for using closed-form expressions of effective medium models to predict seismic velocities in unconsolidated sandstones. We use an effective medium model that combines perfectly rough and smooth grains (the extended Walton model), and use that model to derive coordination number, porosity, and pressure relations for P and S wave velocities from experimental data. Our recipe provides reasonable fits to other experimental and borehole data, and specifically

  3. Cordilleran front range structural features in northwest Montana interpreted from vintage seismic reflection data

    NASA Astrophysics Data System (ADS)

    Porter, Mason C.; Rutherford, Bradley S.; Speece, Marvin A.; Mosolf, Jesse G.

    2016-04-01

    Industry seismic reflection data spanning the Rocky Mountain Cordillera front ranges of northwest Montana were reprocessed and interpreted in this study. Five seismic profiles represent 160 km of deep reflection data collected in 1983 that span the eastern Purcell anticlinorium, Rocky Mountain Trench (RMT), Rocky Mountain Basal Décollement (RMBD), and Lewis thrust. The data were reprocessed using modern techniques including refraction statics, pre-stack time migration (PSTM), and pre- and post-stack depth migration. Results indicate the RMBD is 8-13 km below the Earth's surface and dip 3-10° west. Evidence for the autochthonous Mesoproterozoic Belt and basal Cambrian rocks beneath the RMBD is present in all of the profiles and appears to extend east of the RMT. The Lewis thrust was identified in the seismic profiles and appears to sole into the RMBD east of the RMT. The RMT fault system has a dip displacement of 3-4 km and forms a half graben filled with 1 km of unconsolidated Tertiary sedimentary deposits. The RMT and adjacent Flathead fault systems are interpreted to be structurally linked and may represent a synthetic, en echelon fault system.

  4. Seismic interpretation of the deep structure of the Wabash Valley Fault System

    USGS Publications Warehouse

    Bear, G.W.; Rupp, J.A.; Rudman, A.J.

    1997-01-01

    Interpretations of newly available seismic reflection profiles near the center of the Illinois Basin indicate that the Wabash Valley Fault System is rooted in a series of basement-penetrating faults. The fault system is composed predominantly of north-northeast-trending high-angle normal faults. The largest faults in the system bound the 22-km wide 40-km long Grayville Graben. Structure contour maps drawn on the base of the Mount Simon Sandstone (Cambrian System) and a deeper pre-Mount Simon horizon show dip-slip displacements totaling at least 600 meters across the New Harmony fault. In contrast to previous interpretations, the N-S extent of significant fault offsets is restricted to a region north of 38?? latitude and south of 38.35?? latitude. This suggests that the graben is not a NE extension of the structural complex composed of the Rough Creek Fault System and the Reelfoot Rift as previously interpreted. Structural complexity on the graben floor also decreases to the south. Structural trends north of 38?? latitude are offset laterally across several large faults, indicating strike-slip motions of 2 to 4 km. Some of the major faults are interpreted to penetrate to depths of 7 km or more. Correlation of these faults with steep potential field gradients suggests that the fault positions are controlled by major lithologic contacts within the basement and that the faults may extend into the depth range where earthquakes are generated, revealing a potential link between specific faults and recently observed low-level seismicity in the area.

  5. Preliminary interpretation of industry two-dimensional seismic data from Susitna Basin, south-central Alaska

    USGS Publications Warehouse

    Lewis, Kristen A.; Potter, Christopher J.; Shah, Anjana K.; Stanley, Richard G.; Haeussler, Peter J.; Saltus, Richard W.

    2015-07-30

    The eastern seismic lines show evidence of numerous short-wavelength antiforms that appear to correspond to a series of northeast-trending lineations observed in aeromagnetic data, which have been interpreted as being due to folding of Paleogene volcanic strata. The eastern side of the basin is also cut by a number of reverse faults and thrust faults, the majority of which strike north-south. The western side of the Susitna Basin is cut by a series of regional reverse faults and is characterized by synformal structures in two fault blocks between the Kahiltna River and Skwentna faults. These synforms are progressively deeper to the west in the footwalls of the east-vergent Skwentna and northeast-vergent Beluga Mountain reverse faults. Although the seismic data are limited to the south, we interpret a potential regional south-southeast-directed reverse fault striking east-northeast on the east side of the basin that may cross the entire southern portion of the basin.

  6. Kink-style detachment folding in Bachu fold belt of central Tarim Basin, China: geometry and seismic interpretation

    NASA Astrophysics Data System (ADS)

    Bo, Zhang; Jinjiang, Zhang; Shuyu, Yan; Jiang, Liu; Jinhai, Zhang; Zhongpei, Zhang

    2010-05-01

    The phenomenon of Kink banding is well known throughout the engineering and geophysical sciences. Associated with layered structures compressed in a layer-parallel direction, it arises for example in stratified geological systems under tectonic compression. Our work documented it is also possible to develop super large-scale kink-bands in sedimentary sequences. We interpret the Bachu fold uplift belt of the central Tarim basin in western China to be composed of detachment folds flanked by megascopic-scale kink-bands. Those previous principal fold models for the Bachu uplift belt incorporated components of large-scale thrust faulting, such as the imbricate fault-related fold model and the high-angle, reverse-faulted detachment fold model. Based on our observations in the outcrops and on the two-dimension seismic profiles, we interpret that first-order structures in the region are kink-band style detachment folds to accommodate regional shortening, and thrust faulting can be a second-order deformation style occurring on the limb of the detachment folds or at the cores of some folds to accommodate the further strain of these folds. The belt mainly consists of detachment folds overlying a ductile decollement layer. The crests of the detachment folds are bounded by large-scale kink-bands, which are zones of angularly folded strata. These low-signal-tonoise, low-reflectivity zones observed on seismic profiles across the Bachu belt are poorly imaged sections, which resulted from steeply dipping bedding in the kink-bands. The substantial width (beyond 200m) of these low-reflectivity zones, their sub-parallel edges in cross section, and their orientations at a high angle to layering between 50 and 60 degrees, as well as their conjugate geometry, support a kink-band interpretation. The kink-band interpretation model is based on the Maximum Effective Moment Criteria for continuous deformation, rather than Mohr-Column Criteria for brittle fracture. Seismic modeling is done to

  7. Enhanced Structural Interpretation Using Multitrace Seismic Attribute For Oligo-Miocene Target at Madura Strait Offshore

    NASA Astrophysics Data System (ADS)

    Pratama Wahyu Hidayat, Putra; Hary Murti, Antonius; Sudarmaji; Shirly, Agung; Tiofan, Bani; Damayanti, Shinta

    2018-03-01

    Geometry is an important parameter for the field of hydrocarbon exploration and exploitation, it has significant effect to the amount of resources or reserves, rock spreading, and risk analysis. The existence of geological structure or fault becomes one factor affecting geometry. This study is conducted as an effort to enhance seismic image quality in faults dominated area namely offshore Madura Strait. For the past 10 years, Oligo-Miocene carbonate rock has been slightly explored on Madura Strait area, the main reason because migration and trap geometry still became risks to be concern. This study tries to determine the boundary of each fault zone as subsurface image generated by converting seismic data into variance attribute. Variance attribute is a multitrace seismic attribute as the derivative result from amplitude seismic data. The result of this study shows variance section of Madura Strait area having zero (0) value for seismic continuity and one (1) value for discontinuity of seismic data. Variance section shows the boundary of RMKS fault zone with Kendeng zone distinctly. Geological structure and subsurface geometry for Oligo-Miocene carbonate rock could be identified perfectly using this method. Generally structure interpretation to identify the boundary of fault zones could be good determined by variance attribute.

  8. Seismics-electrics Joint Interpretation in a gypsiferous context.

    NASA Astrophysics Data System (ADS)

    Marzan, Ignacio; Marti, David; Lobo, Agustin; Alvarez-Marron, Joaquina; Carbonell, Ramon

    2016-04-01

    The main objective of this study is to improve the geophysical characterization resulting from a shallow 3D high resolution travel-time tomography survey (500x500m). This survey was acquired in Villar de Cañas (Cuenca, Spain) in late 2013 and early 2014. Lithology down to 150 m depth in this site is characterized by endorheic sediments, mainly siltstone and gypsum. After processing the tomography data, the velocity model showed a good correlation with geology models and borehole data except for the siltstone-gypsum transition. The model involves two lithological limits: the "transition layer - massive gypsum layer" (well resolved by a relatively high velocity contrast) and the "siltstone layer - transition layer" (constrained only in the central part of the model by a relatively low velocity contrast). As electrical resistivity is able to characterize shale-gypsum transitions, we complemented the seismic data with results from a collection of 2D ERT surveys, for which we build a new 3D grid with 2 parameters by node: velocity and resistivity. In order to derive a geological interpretation, we apply a statistical classification method (Linear Discriminant Analysis) to the new bi-parametric grid, using reference classes from well logs. This process results on a final 3D lithological model with less ambiguity and thus with a better definition of the two limits under discussion. Our study shows that the integration of seismic and electric methods significantly improves geological characterization in a gypsiferous context.

  9. Properties of an improved Gabor wavelet transform and its applications to seismic signal processing and interpretation

    NASA Astrophysics Data System (ADS)

    Ji, Zhan-Huai; Yan, Sheng-Gang

    2017-12-01

    This paper presents an analytical study of the complete transform of improved Gabor wavelets (IGWs), and discusses its application to the processing and interpretation of seismic signals. The complete Gabor wavelet transform has the following properties. First, unlike the conventional transform, the improved Gabor wavelet transform (IGWT) maps time domain signals to the time-frequency domain instead of the time-scale domain. Second, the IGW's dominant frequency is fixed, so the transform can perform signal frequency division, where the dominant frequency components of the extracted sub-band signal carry essentially the same information as the corresponding components of the original signal, and the subband signal bandwidth can be regulated effectively by the transform's resolution factor. Third, a time-frequency filter consisting of an IGWT and its inverse transform can accurately locate target areas in the time-frequency field and perform filtering in a given time-frequency range. The complete IGW transform's properties are investigated using simulation experiments and test cases, showing positive results for seismic signal processing and interpretation, such as enhancing seismic signal resolution, permitting signal frequency division, and allowing small faults to be identified.

  10. Erosional unconformity or non-deposition? An alternative interpretation of the Eocene seismic stratigraphy offshore Wilkes Land, East Antarctica

    NASA Astrophysics Data System (ADS)

    Sauermilch, Isabel; Whittaker, Joanne; Totterdell, Jennifer; Jokat, Wilfried

    2017-04-01

    The sedimentary stratigraphy along the conjugate Australian-Antarctic continental margins provide insights into their tectonic evolution as well as changes in paleoceanographic conditions in the Southern Ocean. A comprehensive network of multichannel seismic reflection data as well as geological information from drill cores have been used to interpret the stratigraphic evolution of these margins. However, a number of alternative seismic interpretations exist for the Antarctic side, particularly due to sparse drill core information. A prominent high-amplitude reflector observed along the margin, extending from the continental shelf to the foot-of-slope, is at the centre of debate. Recently, two major hiatuses (from 33.6 - 47.9 Ma and 51.06 - 51.9 Ma) were recovered by the IODP drill core U1356A offshore Wilkes Land and correlated to this prominent reflector. Previous seismic stratigraphic investigations interpreted this structure as an erosional unconformity and proposed different events as a possible cause for this formation, including first arrival of the continental glaciation at the coast at about 34 Ma, increase in spreading rate between Australia and Antarctica at about 45 Ma and drastic global sea level drop of 70 m at about 43 Ma. However, such a large-scale erosion must consequently lead to a re-deposition of a significantly large amount of sediment somewhere along the margins, but, to date, no such deposition is observed in the seismic reflection data. Here, we present an alternative seismo-stratigraphic interpretation based on correlation to the sedimentary structures along the Australian margin. We argue that the prominent unconformity is formed due to non-deposition of sediment between 47.8 and 33.6 Ma. The sedimentary units underlying this unconformity show strong similarities in structure, seismic characteristics and variation along the margin with sequences that are partly exposed to the seafloor at the foot of the Australian slope. On the Australian

  11. Geological and Seismic Data Mining For The Development of An Interpretation System Within The Alptransit Project

    NASA Astrophysics Data System (ADS)

    Klose, C. D.; Giese, R.; Löw, S.; Borm, G.

    Especially for deep underground excavations, the prediction of the locations of small- scale hazardous geotechnical structures is nearly impossible when exploration is re- stricted to surface based methods. Hence, for the AlpTransit base tunnels, exploration ahead has become an essential component of the excavation plan. The project de- scribed in this talk aims at improving the technology for the geological interpretation of reflection seismic data. The discovered geological-seismic relations will be used to develop an interpretation system based on artificial intelligence to predict hazardous geotechnical structures of the advancing tunnel face. This talk gives, at first, an overview about the data mining of geological and seismic properties of metamorphic rocks within the Penninic gneiss zone in Southern Switzer- land. The data results from measurements of a specific geophysical prediction system developed by the GFZ Potsdam, Germany, along the 2600 m long and 1400 m deep Faido access tunnel. The goal is to find those seismic features (i.e. compression and shear wave velocities, velocity ratios and velocity gradients) which show a significant relation to geological properties (i.e. fracturing and fabric features). The seismic properties were acquired from different tomograms, whereas the geolog- ical features derive from tunnel face maps. The features are statistically compared with the seismic rock properties taking into account the different methods used for the tunnel excavation (TBM and Drill/Blast). Fracturing and the mica content stay in a positive relation to the velocity values. Both, P- and S-wave velocities near the tunnel surface describe the petrology better, whereas in the interior of the rock mass they correlate to natural micro- and macro-scopic fractures surrounding tectonites, i.e. cataclasites. The latter lie outside of the excavation damage zone and the tunnel loos- ening zone. The shear wave velocities are better indicators for rock

  12. Seismic interpretation and thrust tectonics of the Amadeus Basin, central Australia, along the BMR regional seismic line

    NASA Astrophysics Data System (ADS)

    Shaw, Russell D.; Korsch, Russell J.; Wright, C.; Goleby, B. R.

    At the northern margin of the Amadeus Basin the monoclinal upturn (the MacDonnell Homocline) is interpreted to be the result of rotation and limited back-thrusting of the sedimentary sequence in front of a southerly-directed, imbricate basement thrust-wedge. This thrust complex is linked at depth to the crust-cutting Redbank Thrust Zone. In the northern part of the basin immediately to the south, regional seismic reflection profiling across the Missionary Plain shows a sub-horizontal, north-dipping, parautochthonous sedimentary sequence between about 8.5 km and 12.0 km thick. This sedimentary sequence shows upturning only at the northern and southern extremities, and represents an unusual, relatively undeformed region between converging thrust systems. In this intervening region, the crust appears to have been tilted downwards and northwards in response to the upthrusting to the north. Still farther to the south, the vertical uplift of the southern hanging wall of the Gardiner Thrust is about 6 km. Seismic reflection profiling in the region immediately south of the Gardiner Thrust indicates repetition of the sedimentary sequence. At the far end of the profile, in the Kernot Range, an imbricate thrust system fans ahead of a ramp-flat thrust pair. This thrust system (the Kernot Range Thrust System) occurs immediately north of an aeromagnetic domain boundary which marks the southern limit of a central ridge region characterized by thin Palaeozoic sedimentary cover and shallow depths to magnetic basement. A planar seismic event, imaged to a depth of at least 18 km, may correspond to the same boundary and is interpreted as a pre-basin Proterozoic thrust. Overall, the structure in the shallow sedimentary section in the central-southern region of the Amadeus Basin indicates that north-directed thrusting during the Dovonian-Carboniferous Alice Springs Orogeny was thin-skinned. During this orogeny an earlier thrust system, formed during the Petermann Ranges Orogeny and

  13. Integration of P- and SH-wave high-resolution seismic reflection and micro-gravity techniques to improve interpretation of shallow subsurface structure: New Madrid seismic zone

    USGS Publications Warehouse

    Bexfield, C.E.; McBride, J.H.; Pugin, Andre J.M.; Ravat, D.; Biswas, S.; Nelson, W.J.; Larson, T.H.; Sargent, S.L.; Fillerup, M.A.; Tingey, B.E.; Wald, L.; Northcott, M.L.; South, J.V.; Okure, M.S.; Chandler, M.R.

    2006-01-01

    Shallow high-resolution seismic reflection surveys have traditionally been restricted to either compressional (P) or horizontally polarized shear (SH) waves in order to produce 2-D images of subsurface structure. The northernmost Mississippi embayment and coincident New Madrid seismic zone (NMSZ) provide an ideal laboratory to study the experimental use of integrating P- and SH-wave seismic profiles, integrated, where practicable, with micro-gravity data. In this area, the relation between "deeper" deformation of Paleozoic bedrock associated with the formation of the Reelfoot rift and NMSZ seismicity and "shallower" deformation of overlying sediments has remained elusive, but could be revealed using integrated P- and SH-wave reflection. Surface expressions of deformation are almost non-existent in this region, which makes seismic reflection surveying the only means of detecting structures that are possibly pertinent to seismic hazard assessment. Since P- and SH-waves respond differently to the rock and fluid properties and travel at dissimilar speeds, the resulting seismic profiles provide complementary views of the subsurface based on different levels of resolution and imaging capability. P-wave profiles acquired in southwestern Illinois and western Kentucky (USA) detect faulting of deep, Paleozoic bedrock and Cretaceous reflectors while coincident SH-wave surveys show that this deformation propagates higher into overlying Tertiary and Quaternary strata. Forward modeling of micro-gravity data acquired along one of the seismic profiles further supports an interpretation of faulting of bedrock and Cretaceous strata. The integration of the two seismic and the micro-gravity methods therefore increases the scope for investigating the relation between the older and younger deformation in an area of critical seismic hazard. ?? 2006 Elsevier B.V. All rights reserved.

  14. Interpretation of shallow crustal structure of the Imperial Valley, California, from seismic reflection profiles

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

    Severson, L.K.

    1987-05-01

    Eight seismic reflection profiles (285 km total length) from the Imperial Valley, California, were provided to CALCRUST for reprocessing and interpretation. Two profiles were located along the western margin of the valley, five profiles were situated along the eastern margin and one traversed the deepest portion of the basin. These data reveal that the central basin contains a wedge of highly faulted sediments that thins to the east. Most of the faulting is strike-slip but there is evidence for block rotations on the scale of 5 to 10 kilometers within the Brawley Seismic Zone. These lines provide insight into themore » nature of the east and west edges of the Imperial Valley. The basement at the northwestern margin of the valley, to the north of the Superstition Hills, has been normal-faulted and blocks of basement material have ''calved'' into the trough. A blanket of sediments has been deposited on this margin. To the south of the Superstition Hills and Superstition Mountain, the top of the basement is a detachment surface that dips gently into the basin. This margin is also covered by a thick sequence sediments. The basement of the eastern margin consists of metamorphic rocks of the upper plate of the Chocolate Mountain Thrust system underlain by the Orocopia Schist. These rocks dip to the southeast and extend westward to the Sand Hills Fault but do not appear to cross it. Thus, the Sand Hills Fault is interpreted to be the southern extension of the San Andreas Fault. North of the Sand Hills Fault the East Highline Canal seismicity lineament is associated with a strike-slip fault and is probably linked to the Sand Hills Fault. Six geothermal areas crossed by these lines, in agreement with previous studies of geothermal reservoirs, are associated with ''faded'' zones, Bouguer gravity and heat flow maxima, and with higher seismic velocities than surrounding terranes.« less

  15. IKOS: A Framework for Static Analysis based on Abstract Interpretation (Tool Paper)

    NASA Technical Reports Server (NTRS)

    Brat, Guillaume P.; Laserna, Jorge A.; Shi, Nija; Venet, Arnaud Jean

    2014-01-01

    The RTCA standard (DO-178C) for developing avionic software and getting certification credits includes an extension (DO-333) that describes how developers can use static analysis in certification. In this paper, we give an overview of the IKOS static analysis framework that helps developing static analyses that are both precise and scalable. IKOS harnesses the power of Abstract Interpretation and makes it accessible to a larger class of static analysis developers by separating concerns such as code parsing, model development, abstract domain management, results management, and analysis strategy. The benefits of the approach is demonstrated by a buffer overflow analysis applied to flight control systems.

  16. Gas and seismicity within the Istanbul seismic gap.

    PubMed

    Géli, L; Henry, P; Grall, C; Tary, J-B; Lomax, A; Batsi, E; Riboulot, V; Cros, E; Gürbüz, C; Işık, S E; Sengör, A M C; Le Pichon, X; Ruffine, L; Dupré, S; Thomas, Y; Kalafat, D; Bayrakci, G; Coutellier, Q; Regnier, T; Westbrook, G; Saritas, H; Çifçi, G; Çağatay, M N; Özeren, M S; Görür, N; Tryon, M; Bohnhoff, M; Gasperini, L; Klingelhoefer, F; Scalabrin, C; Augustin, J-M; Embriaco, D; Marinaro, G; Frugoni, F; Monna, S; Etiope, G; Favali, P; Bécel, A

    2018-05-01

    Understanding micro-seismicity is a critical question for earthquake hazard assessment. Since the devastating earthquakes of Izmit and Duzce in 1999, the seismicity along the submerged section of North Anatolian Fault within the Sea of Marmara (comprising the "Istanbul seismic gap") has been extensively studied in order to infer its mechanical behaviour (creeping vs locked). So far, the seismicity has been interpreted only in terms of being tectonic-driven, although the Main Marmara Fault (MMF) is known to strike across multiple hydrocarbon gas sources. Here, we show that a large number of the aftershocks that followed the M 5.1 earthquake of July, 25 th 2011 in the western Sea of Marmara, occurred within a zone of gas overpressuring in the 1.5-5 km depth range, from where pressurized gas is expected to migrate along the MMF, up to the surface sediment layers. Hence, gas-related processes should also be considered for a complete interpretation of the micro-seismicity (~M < 3) within the Istanbul offshore domain.

  17. Interpretation for scales of measurement linking with abstract algebra.

    PubMed

    Sawamura, Jitsuki; Morishita, Shigeru; Ishigooka, Jun

    2014-01-01

    THE STEVENS CLASSIFICATION OF LEVELS OF MEASUREMENT INVOLVES FOUR TYPES OF SCALE: "Nominal", "Ordinal", "Interval" and "Ratio". This classification has been used widely in medical fields and has accomplished an important role in composition and interpretation of scale. With this classification, levels of measurements appear organized and validated. However, a group theory-like systematization beckons as an alternative because of its logical consistency and unexceptional applicability in the natural sciences but which may offer great advantages in clinical medicine. According to this viewpoint, the Stevens classification is reformulated within an abstract algebra-like scheme; 'Abelian modulo additive group' for "Ordinal scale" accompanied with 'zero', 'Abelian additive group' for "Interval scale", and 'field' for "Ratio scale". Furthermore, a vector-like display arranges a mixture of schemes describing the assessment of patient states. With this vector-like notation, data-mining and data-set combination is possible on a higher abstract structure level based upon a hierarchical-cluster form. Using simple examples, we show that operations acting on the corresponding mixed schemes of this display allow for a sophisticated means of classifying, updating, monitoring, and prognosis, where better data mining/data usage and efficacy is expected.

  18. New Elastic Moduli for Amphiboles and Feldspars: Impact on Interpretations of Seismic Velocities

    NASA Astrophysics Data System (ADS)

    Brown, J. M.; Angel, R. J.

    2016-12-01

    more sensitive to iron. Variations in Poisson's ratio (which depends on the ratio of isotropic compressional and shear wave velocities) associated with compositions within the amphiboles and the feldspars are larger than previously predicted. The extent of modifications to seismic interpretations is evaluated.

  19. Interpretation for scales of measurement linking with abstract algebra

    PubMed Central

    2014-01-01

    The Stevens classification of levels of measurement involves four types of scale: “Nominal”, “Ordinal”, “Interval” and “Ratio”. This classification has been used widely in medical fields and has accomplished an important role in composition and interpretation of scale. With this classification, levels of measurements appear organized and validated. However, a group theory-like systematization beckons as an alternative because of its logical consistency and unexceptional applicability in the natural sciences but which may offer great advantages in clinical medicine. According to this viewpoint, the Stevens classification is reformulated within an abstract algebra-like scheme; ‘Abelian modulo additive group’ for “Ordinal scale” accompanied with ‘zero’, ‘Abelian additive group’ for “Interval scale”, and ‘field’ for “Ratio scale”. Furthermore, a vector-like display arranges a mixture of schemes describing the assessment of patient states. With this vector-like notation, data-mining and data-set combination is possible on a higher abstract structure level based upon a hierarchical-cluster form. Using simple examples, we show that operations acting on the corresponding mixed schemes of this display allow for a sophisticated means of classifying, updating, monitoring, and prognosis, where better data mining/data usage and efficacy is expected. PMID:24987515

  20. Tutorial review of seismic surface waves' phenomenology

    NASA Astrophysics Data System (ADS)

    Levshin, A. L.; Barmin, M. P.; Ritzwoller, M. H.

    2018-03-01

    In recent years, surface wave seismology has become one of the leading directions in seismological investigations of the Earth's structure and seismic sources. Various applications cover a wide spectrum of goals, dealing with differences in sources of seismic excitation, penetration depths, frequency ranges, and interpretation techniques. Observed seismic data demonstrates the great variability of phenomenology which can produce difficulties in interpretation for beginners. This tutorial review is based on the many years' experience of authors in processing and interpretation of seismic surface wave observations and the lectures of one of the authors (ALL) at Workshops on Seismic Wave Excitation, Propagation and Interpretation held at the Abdus Salam International Center for Theoretical Physics (Trieste, Italy) in 1990-2012. We present some typical examples of wave patterns which could be encountered in different applications and which can serve as a guide to analysis of observed seismograms.

  1. 3D seismic data interpretation of Boonsville Field, Texas

    NASA Astrophysics Data System (ADS)

    Alhakeem, Aamer Ali

    The Boonsville field is one of the largest gas fields in the US located in the Fort Worth Basin, north central Texas. The highest potential reservoirs reside in the Bend Conglomerate deposited during the Pennsylvanian. The Boonsville data set is prepared by the Bureau of Economic Geology at the University of Texas, Austin, as part of the secondary gas recovery program. The Boonsville field seismic data set covers an area of 5.5 mi2. It includes 38 wells data. The Bend Conglomerate is deposited in fluvio-deltaic transaction. It is subdivided into many genetic sequences which include depositions of sandy conglomerate representing the potential reserves in the Boonsville field. The geologic structure of the Boonsville field subsurface are visualized by constructing structure maps of Caddo, Davis, Runaway, Beans Cr, Vineyard, and Wade. The mapping includes time structure, depth structure, horizon slice, velocity maps, and isopach maps. Many anticlines and folds are illustrated. Karst collapse features are indicated specially in the lower Atoka. Dipping direction of the Bend Conglomerate horizons are changing from dipping toward north at the top to dipping toward east at the bottom. Stratigraphic interpretation of the Runaway Formation and the Vineyard Formation using well logs and seismic data integration showed presence of fluvial dominated channels, point bars, and a mouth bar. RMS amplitude maps are generated and used as direct hydrocarbon indicator for the targeted formations. As a result, bright spots are indicated and used to identify potential reservoirs. Petrophysical analysis is conducted to obtain gross, net pay, NGR, water saturation, shale volume, porosity, and gas formation factor. Volumetric calculations estimated 989.44 MMSCF as the recoverable original gas in-place for a prospect in the Runaway and 3.32 BSCF for a prospect in the Vineyard Formation.

  2. Visualization of volumetric seismic data

    NASA Astrophysics Data System (ADS)

    Spickermann, Dela; Böttinger, Michael; Ashfaq Ahmed, Khawar; Gajewski, Dirk

    2015-04-01

    Mostly driven by demands of high quality subsurface imaging, highly specialized tools and methods have been developed to support the processing, visualization and interpretation of seismic data. 3D seismic data acquisition and 4D time-lapse seismic monitoring are well-established techniques in academia and industry, producing large amounts of data to be processed, visualized and interpreted. In this context, interactive 3D visualization methods proved to be valuable for the analysis of 3D seismic data cubes - especially for sedimentary environments with continuous horizons. In crystalline and hard rock environments, where hydraulic stimulation techniques may be applied to produce geothermal energy, interpretation of the seismic data is a more challenging problem. Instead of continuous reflection horizons, the imaging targets are often steep dipping faults, causing a lot of diffractions. Without further preprocessing these geological structures are often hidden behind the noise in the data. In this PICO presentation we will present a workflow consisting of data processing steps, which enhance the signal-to-noise ratio, followed by a visualization step based on the use the commercially available general purpose 3D visualization system Avizo. Specifically, we have used Avizo Earth, an extension to Avizo, which supports the import of seismic data in SEG-Y format and offers easy access to state-of-the-art 3D visualization methods at interactive frame rates, even for large seismic data cubes. In seismic interpretation using visualization, interactivity is a key requirement for understanding complex 3D structures. In order to enable an easy communication of the insights gained during the interactive visualization process, animations of the visualized data were created which support the spatial understanding of the data.

  3. Lithostratigraphic interpretation from joint analysis of seismic tomography and magnetotelluric resistivity models using self-organizing map techniques

    NASA Astrophysics Data System (ADS)

    Bauer, K.; Muñoz, G.; Moeck, I.

    2012-12-01

    The combined interpretation of different models as derived from seismic tomography and magnetotelluric (MT) inversion represents a more efficient approach to determine the lithology of the subsurface compared with the separate treatment of each discipline. Such models can be developed independently or by application of joint inversion strategies. After the step of model generation using different geophysical methodologies, a joint interpretation work flow includes the following steps: (1) adjustment of a joint earth model based on the adapted, identical model geometry for the different methods, (2) classification of the model components (e.g. model blocks described by a set of geophysical parameters), and (3) re-mapping of the classified rock types to visualise their distribution within the earth model, and petrophysical characterization and interpretation. One possible approach for the classification of multi-parameter models is based on statistical pattern recognition, where different models are combined and translated into probability density functions. Classes of rock types are identified in these methods as isolated clusters with high probability density function values. Such techniques are well-established for the analysis of two-parameter models. Alternatively we apply self-organizing map (SOM) techniques, which have no limitations in the number of parameters to be analysed in the joint interpretation. Our SOM work flow includes (1) generation of a joint earth model described by so-called data vectors, (2) unsupervised learning or training, (3) analysis of the feature map by adopting image processing techniques, and (4) application of the knowledge to derive a lithological model which is based on the different geophysical parameters. We show the usage of the SOM work flow for a synthetic and a real data case study. Both tests rely on three geophysical properties: P velocity and vertical velocity gradient from seismic tomography, and electrical resistivity

  4. Interpreting intraplate tectonics for seismic hazard: a UK historical perspective

    NASA Astrophysics Data System (ADS)

    Musson, R. M. W.

    2012-04-01

    It is notoriously difficult to construct seismic source models for probabilistic seismic hazard assessment in intraplate areas on the basis of geological information, and many practitioners have given up the task in favour of purely seismicity-based models. This risks losing potentially valuable information in regions where the earthquake catalogue is short compared to the seismic cycle. It is interesting to survey how attitudes to this issue have evolved over the past 30 years. This paper takes the UK as an example, and traces the evolution of seismic source models through generations of hazard studies. It is found that in the UK, while the earliest studies did not consider regional tectonics in any way, there has been a gradual evolution towards more tectonically based models. Experience in other countries, of course, may differ.

  5. Seismic Observations and Interpretation in NE China, Infrasound Observations and Interpretation in Utah

    DTIC Science & Technology

    2010-07-30

    from Xu et al., 2005). (b) Map of SMU-IGPCEA Huailai Seismic Network and seismicity ( open circles) for the time period of January 01, 2002 through...the Beijing-Huailai-Fengzhen (H20) refraction/ wide angle reflection profile (Zhu et al., 1997). Open circles are locations of two historical...historycatalog_query.jsp) and the China Seismograph Network ( CSN ) Catalog (http://210.72.96.165/wdcd/csn_catalog_p001.jsp) list a total of 323 earthquakes with magnitude

  6. Automatic Processing and Interpretation of Long Records of Endogenous Micro-Seismicity: the Case of the Super-Sauze Soft-Rock Landslide.

    NASA Astrophysics Data System (ADS)

    Provost, F.; Malet, J. P.; Hibert, C.; Doubre, C.

    2017-12-01

    The Super-Sauze landslide is a clay-rich landslide located the Southern French Alps. The landslide exhibits a complex pattern of deformation: a large number of rockfalls are observed in the 100 m height main scarp while the deformation of the upper part of the accumulated material is mainly affected by material shearing along stable in-situ crests. Several fissures are locally observed. The shallowest layer of the accumulated material tends to behave in a brittle manner but may undergo fluidization and/or rapid acceleration. Previous studies have demonstrated the presence of a rich endogenous micro-seismicity associated to the deformation of the landslide. However, the lack of long-term seismic records and suitable processing chains prevented a full interpretation of the links between the external forcings, the deformation and the recorded seismic signals. Since 2013, two permanent seismic arrays are installed in the upper part of the landslide. We here present the methodology adopted to process this dataset. The processing chain consists of a set of automated methods for automatic and robust detection, classification and location of the recorded seismicity. Thousands of events are detected and further automatically classified. The classification method is based on the description of the signal through attributes (e.g. waveform, spectral content properties). These attributes are used as inputs to classify the signal using a Random Forest machine-learning algorithm in four classes: endogenous micro-quakes, rockfalls, regional earthquakes and natural/anthropogenic noises. The endogenous landslide sources (i.e. micro-quake and rockfall) are further located. The location method is adapted to the type of event. The micro-quakes are located with a 3D velocity model derived from a seismic tomography campaign and an optimization of the first arrival picking with the inter-trace correlation of the P-wave arrivals. The rockfalls are located by optimizing the inter

  7. Preliminary Interpretations of Multi-Channel Seismic Reflection and Magnetic Data on North Anatolian Fault (NAF) in the Eastern Marmara Region, Turkey

    NASA Astrophysics Data System (ADS)

    Gözde Okut Toksoy, Nigar; Kurt, Hülya; İşseven, Turgay

    2017-04-01

    of Istanbul Technical University is used for processing. Proton magnetometer is used for measuring the magnetic field variations on the one of the profiles. Total magnetic field values are corrected using base readings from Bogazici University Kandilli Observatory, Iznik Earthquake Hazard Mitigation Center. Processed seismic and magnetic data are interpreted and compared to see effect of the NAF. Preliminary interpretations show vertical seismic discontinuities related to the fault figured out on the time-migrated seismic sections from surface to the about 1 s two-way travel time depth. Magnetic anomalies are also realized on the profile related to the NAF supporting the seismic data.

  8. Participation in the Apollo passive seismic experiment

    NASA Technical Reports Server (NTRS)

    Press, F.; Toksoez, M. N.; Dainty, A.

    1972-01-01

    Computer programs which were written to read digital tapes containing lunar seismic data were studied. Interpreting very early parts of the lunar seismogram as seismic body-wave phases enabled the determination of the structure of the outer part of the moon in the Fra Mauro region. The crust in the Fra Mauro region is 60 to 65 km-thick, overlaying a high velocity mantle. The crust is further divided into an upper part, 25 km thick, apparently made of material similar to the surficial basalts, and a lower part of seemingly different composition, possibly an anorthositic gabbro. The generation of the exceedingly long reverberating wave-train observed in lunar seismogram was also studied. This is believed to be due to an intense scattering layer with very high quality coefficient overlying a more homogeneous elastic medium. Titles and abstracts of related published papers are included.

  9. Structural interpretation and physical property estimates based on COAST 2012 seismic reflection profiles offshore central Washington, Cascadia subduction zone

    NASA Astrophysics Data System (ADS)

    Webb, S. I.; Tobin, H. J.; Everson, E. D.; Fortin, W.; Holbrook, W. S.; Kent, G.; Keranen, K. M.

    2014-12-01

    The Cascadia subduction zone has a history of large magnitude earthquakes, but a near-total lack of plate interface seismicity, making the updip limit of the seismogenic zone difficult to locate. In addition, the central Cascadia accretionary prism is characterized by an extremely low wedge taper angle, landward vergent initial thrusting, and a flat midslope terrace between the inner and outer wedges, unlike most other accretionary prisms (e.g. the Nankai Trough, Japan). The Cascadia Open Access Seismic Transect (COAST) lines were shot by R/V Marcus Langseth in July of 2012 off central Washington to image this subduction zone. Two trench-parallel and nine trench-perpendicular lines were collected. In this study, we present detailed seismic interpretation of both time- and depth-migrated stacked profiles, focused on elucidating the deposition and deformation of both pre- and syn-tectonic sediment in the trench and slope. Distribution and timing of sediments and their deformation is used to unravel the evolution of the wedge through time. Initially, interpretation of the time-sections is carried out to support the building of tomographic velocity models to aid in the pre-stack depth migration (PSDM) of selected lines. In turn, we use PSDM velocity models to estimate porosity and pore pressure conditions at the base of the wedge and across the basal plate interface décollement where possible, using established velocity-porosity transforms. Interpretation in this way incorporates both accurate structural relationships and robust porosity models to document wedge development and present-day stress state, in particular regions of potential overpressure. Results shed light on the origin and evolution of the mid-slope terrace and the low taper angle for the forearc wedge. This work may shed light ultimately on the position of the potential updip limit of the seismogenic zone beneath the wedge.

  10. Seismic stratigraphic interpretations suggest that sectors of the central and western Ross Sea were near or above sea level during earliest Oligocene time

    NASA Astrophysics Data System (ADS)

    Sorlien, C. C.; Sauli, C.; De Santis, L.; Luyendyk, B. P.; Wardell, N.; Davis, S. M.; Wilson, D. S.; Brazell, S.; Bartek, L., III; Bart, P. J.

    2016-12-01

    Most of West Antarctica has been interpreted as a high-elevation plateau that has subsided between about 100 Ma and present. Ross Sea was characterized by subaerial ridges and islands up to mid-Cenozoic time. It was in such an environment that Oligocene ice sheets and glaciers advanced and retreated within Ross Embayment. The extent to which Oligocene ice affected the embayment north of the current ice shelf has not been established, with either ice caps on islands, or broad glaciers affecting basins having been proposed. We used all available data from the Seismic Data Library System to interpret stratigraphic horizons through most of Ross Sea. A new 3D velocity model was constructed for the western 2/3 of Ross Sea. Stratigraphic age control was provided by deep scientific coring, including Deep Sea Drilling Program sites, the Cape Roberts Drilling Program, and published correlations to ANDRILL sites. The correlation with recent drill records and much additional seismic reflection data allowed a new interpretation of Ross Sea, which differs from the previous comprehensive seismic stratigraphic interpretation (ANTOSTRAT 1995). Sedimentary rocks of given ages are twice as deep within Terror Rift in westernmost Ross Sea in our interpretation. In contrast, acoustic basement is 1 km shallower in part of Central Trough. The 200 km-wide smooth acoustic basement on Central High eroded sub-aerially until it subsided differentially through sea level toward the centers of Cretaceous and Cenozoic rifts. If the subsiding basins were kept filled with sediment eroded by Oligocene ice sheets, then the age the strata aggrading above the planar rock platform date subsidence through sea level at each location. Using such an assumption, much of central and western Ross Sea was near or above sea level during earliest Oligocene time. These assumptions will be tested by backstripping and thermal subsidence models.

  11. Interpretation of a 3D Seismic-Reflection Volume in the Basin and Range, Hawthorne, Nevada

    NASA Astrophysics Data System (ADS)

    Louie, J. N.; Kell, A. M.; Pullammanappallil, S.; Oldow, J. S.; Sabin, A.; Lazaro, M.

    2009-12-01

    A collaborative effort by the Great Basin Center for Geothermal Energy at the University of Nevada, Reno, and Optim Inc. of Reno has interpreted a 3d seismic data set recorded by the U.S. Navy Geothermal Programs Office (GPO) at the Hawthorne Army Depot, Nevada. The 3d survey incorporated about 20 NNW-striking lines covering an area of approximately 3 by 10 km. The survey covered an alluvial area below the eastern flank of the Wassuk Range. In the reflection volume the most prominent events are interpreted to be the base of Quaternary alluvium, the Quaternary Wassuk Range-front normal fault zone, and sequences of intercalated Tertiary volcanic flows and sediments. Such a data set is rare in the Basin and Range. Our interpretation reveals structural and stratigraphic details that form a basis for rapid development of the geothermal-energy resources underlying the Depot. We interpret a map of the time-elevation of the Wassuk Range fault and its associated splays and basin-ward step faults. The range-front fault is the deepest, and its isochron map provides essentially a map of "economic basement" under the prospect area. There are three faults that are the most readily picked through vertical sections. The fault reflections show an uncertainty in the time-depth that we can interpret for them of 50 to 200 ms, due to the over-migrated appearance of the processing contractor’s prestack time-migrated data set. Proper assessment of velocities for mitigating the migration artifacts through prestack depth migration is not possible from this data set alone, as the offsets are not long enough for sufficiently deep velocity tomography. The three faults we interpreted appear as gradients in potential-field maps. In addition, the southern boundary of a major Tertiary graben may be seen within the volume as the northward termination of the strong reflections from older Tertiary volcanics. Using a transparent volume view across the survey gives a view of the volcanics in full

  12. Preliminary interpretation of high resolution 3D seismic data from offshore Mt. Etna, Italy

    NASA Astrophysics Data System (ADS)

    Gross, F.; Krastel, S.; Chiocci, F. L.; Ridente, D.; Cukur, D.; Bialas, J.; Papenberg, C. A.; Crutchley, G.; Koch, S.

    2013-12-01

    In order to gain knowledge about subsurface structures and its correlation to seafloor expressions, a hydro-acoustic dataset was collected during RV Meteor Cruise M86/2 (December 2011/January 2012) in Messina Straits and offshore Mt. Etna. Especially offshore Mt. Etna, the data reveals an obvious connection between subsurface structures and previously known morphological features at the sea floor. Therefore a high resolution 3D seismic dataset was acquired between Riposto Ridge and Catania Canyon close to the shore of eastern Sicily. The study area is characterized by a major structural high, which hosts several ridge-like features at the seafloor. These features are connected to a SW-NE trending fault system. The ridges are bended in their NE-SW direction and host major escarpments at the seafloor. Furthermore they are located directly next to a massive amphitheater structure offshore Mt. Etna with slope gradients of up to 35°, which is interpreted as remnants of a massive submarine mass wasting event off Sicily. The new 3D seismic dataset allows an in depth analysis of the ongoing deformation of the east flank of Mt. Etna.

  13. Trade-off of Elastic Structure and Q in Interpretations of Seismic Attenuation

    NASA Astrophysics Data System (ADS)

    Deng, Wubing; Morozov, Igor B.

    2017-10-01

    The quality factor Q is an important phenomenological parameter measured from seismic or laboratory seismic data and representing wave-energy dissipation rate. However, depending on the types of measurements and models or assumptions about the elastic structure, several types of Qs exist, such as intrinsic and scattering Qs, coda Q, and apparent Qs observed from wavefield fluctuations. We consider three general types of elastic structures that are commonly encountered in seismology: (1) shapes and dimensions of rock specimens in laboratory studies, (2) geometric spreading or scattering in body-, surface- and coda-wave studies, and (3) reflectivity on fine layering in reflection seismic studies. For each of these types, the measured Q strongly trades off with the (inherently limited) knowledge about the respective elastic structure. For the third of the above types, the trade-off is examined quantitatively in this paper. For a layered sequence of reflectors (e.g., an oil or gas reservoir or a hydrothermal zone), reflection amplitudes and phases vary with frequency, which is analogous to a reflection from a contrast in attenuation. We demonstrate a quantitative equivalence between phase-shifted reflections from anelastic zones and reflections from elastic layering. Reflections from the top of an elastic layer followed by weaker reflections from its bottom can appear as resulting from a low Q within or above this layer. This apparent Q can be frequency-independent or -dependent, according to the pattern of thin layering. Due to the layering, the interpreted Q can be positive or negative, and it can depend on source-receiver offsets. Therefore, estimating Q values from frequency-dependent or phase-shifted reflection amplitudes always requires additional geologic or rock-physics constraints, such as sparseness and/or randomness of reflectors, the absence of attenuation in certain layers, or specific physical mechanisms of attenuation. Similar conclusions about the

  14. Abstraction in perceptual symbol systems.

    PubMed Central

    Barsalou, Lawrence W

    2003-01-01

    After reviewing six senses of abstraction, this article focuses on abstractions that take the form of summary representations. Three central properties of these abstractions are established: ( i ) type-token interpretation; (ii) structured representation; and (iii) dynamic realization. Traditional theories of representation handle interpretation and structure well but are not sufficiently dynamical. Conversely, connectionist theories are exquisitely dynamic but have problems with structure. Perceptual symbol systems offer an approach that implements all three properties naturally. Within this framework, a loose collection of property and relation simulators develops to represent abstractions. Type-token interpretation results from binding a property simulator to a region of a perceived or simulated category member. Structured representation results from binding a configuration of property and relation simulators to multiple regions in an integrated manner. Dynamic realization results from applying different subsets of property and relation simulators to category members on different occasions. From this standpoint, there are no permanent or complete abstractions of a category in memory. Instead, abstraction is the skill to construct temporary online interpretations of a category's members. Although an infinite number of abstractions are possible, attractors develop for habitual approaches to interpretation. This approach provides new ways of thinking about abstraction phenomena in categorization, inference, background knowledge and learning. PMID:12903648

  15. Interpretation of a seismic refraction profile across the Roosevelt Hot Springs, Utah and vicinity

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

    Gertson, R.C.; Smith, R.B.

    1979-03-01

    In April 1977, a seismic refraction profile was recorded across the Milford Valley, the Roosevelt Hot Springs KGRA, and the northern Mineral Mountains in southwestern Utah. Seven shot points were used to provide multiple subsurface seismic refraction coverage along the 30 km east-west profile line. Since an inspection of power spectrums revealed large components of 60 Hz noise on some traces, computer routines were used to low-pass filter all seismograms. Amplitude information was utilized by normalizing all traces that recorded the same blast. Subsurface structural modeling was conducted by means of first arrival P-wave delay-time analysis and ray tracing. Herglotz-Wiechertmore » travel-time inversion was used for the velocity-depth distribution in the Mineral Mountains. The interpretation of the P-wave travel-times suggests that the Milford Valley fill consists of two units with a total thickness of at least 1.8 km. In the vicinity of the Roosevelt KGRA, a thin low velocity alluvial layer covers a basement igneous complex with a velocity of 5.2 km/s. Granite velocities between 3.3 km/s and 4.0 km/s were calculated from the travel-times in the Mineral Mountains.« less

  16. Combined interpretation of 3D seismic reflection attributes for geothermal exploration in the Polish Basin using self-organizing maps

    NASA Astrophysics Data System (ADS)

    Bauer, Klaus; Pussak, Marcin; Stiller, Manfred; Bujakowski, Wieslaw

    2014-05-01

    Self-organizing maps (SOM) are neural network techniques which can be used for the joint interpretation of multi-disciplinary data sets. In this investigation we apply SOM within a geothermal exploration project using 3D seismic reflection data. The study area is located in the central part of the Polish basin. Several sedimentary target horizons were identified at this location based on fluid flow rate measurements in the geothermal research well Kompina-2. The general objective is a seismic facies analysis and characterization of the major geothermal target reservoir. A 3D seismic reflection experiment with a sparse acquisition geometry was carried out around well Kompina-2. Conventional signal processing (amplitude corrections, filtering, spectral whitening, deconvolution, static corrections, muting) was followed by normal-moveout (NMO) stacking, and, alternatively, by common-reflection-surface (CRS) stacking. Different signal attributes were then derived from the stacked images including root-mean-square (RMS) amplitude, instantaneous frequency and coherency. Furthermore, spectral decomposition attributes were calculated based on the continuous wavelet transform. The resulting attribute maps along major target horizons appear noisy after the NMO stack and clearly structured after the CRS stack. Consequently, the following SOM-based multi-parameter signal attribute analysis was applied only to the CRS images. We applied our SOM work flow, which includes data preparation, unsupervised learning, segmentation of the trained SOM using image processing techniques, and final application of the learned knowledge. For the Lower Jurassic target horizon Ja1 we derived four different clusters with distinct seismic attribute signatures. As the most striking feature, a corridor parallel to a fault system was identified, which is characterized by decreased RMS amplitudes and low frequencies. In our interpretation we assume that this combination of signal properties can be

  17. High resolution seismic reflection survey in the Gulf of Pozzuoli, Naples, Italy. An example of preliminary interpretation of seismic profiles.

    NASA Astrophysics Data System (ADS)

    D'Aniello, Elena; di Fiore, Vincenzo; Sacchi, Marco; Rapolla, Antonio

    2010-05-01

    were recognized. The correspondence between magnetic structures, interpreted as volcanic bodies, and the faults NE-SW and NW-SE trending, supports the hypothesis that the magma rises along normal faults cutting the carbonate platform. We here present two significant seismic profiles: their interpretation reveals a complex stratigraphic and structural setting, dominated by the occurrence of volcanic bodies and siliciclastic depositional units, mostly deriving from the dismantling of the adjacent vents and volcaniclastic units. The results of this preliminary research include the recognition of volcanic features and structures not yet described in the literature that may represent a relevant contribute to the understanding of the Late Quaternary evolution of the Campi Flegrei area. References: Bruno P.P., Rapolla A., Di Fiore V., 2003. Structural setting of the Bay of Naples (Italy) seismic reflection data: implications for Campanian volcanism. Tectonophysics, 372, 193-213. Bruno P.P., 2004. Structure and evolution of the Bay of Pozzuoli (Italy) using marine seismic reflection data: implication for collapse of the Campi Flegrei caldera. Bull. Volcanol., 66, 342-355. Di Fiore V., D'Aniello E., Rapolla A., Sacchi M., Secomandi M., Spiess V., 2009. Multichannel seismic survey in coastal Campania area by two different resolution sources. EGU General Assembly 2009, vol.11. Sacchi M., Alessio G., Aquino I., Esposito E., Molisso F., Nappi R., Porfido S., Violante C., 2008. Risultati preliminari della campagna oceanografica CAFE_07 - Leg 3 nei Golfi di Napoli e Pozzuoli, Mar Tirreno Orientale. Quaderni di Geofisica, n. 64. Secomandi M., Paoletti V., Aiello G., Fedi M., Marsella E., Ruggieri S., D'Argenio B., Rapolla A., 2003. Analysis of the magnetic anomaly field of the volcanic district of the Bay of Naples, Italy. Marine Geophysical Researches. 24: 207-221.

  18. Breakup magmatism on the Vøring Margin, mid-Norway: New insight from interpretation of high-quality 2D and 3D seismic reflection data

    NASA Astrophysics Data System (ADS)

    Abdelmalak, M. M.; Planke, S.; Millett, J.; Jerram, D. A.; Maharjan, D.; Zastrozhnov, D.; Schmid, D. W.; Faleide, J. I.; Svensen, H.; Myklebust, R.

    2017-12-01

    The Vøring Margin offshore mid-Norway is a classic volcanic rifted margin, characterized by voluminous Paleogene igneous rocks present on both sides of the continent-ocean boundary. The margin displays (1) thickened transitional crust with a well-defined lower crustal high-velocity body and prominent deep crustal reflections, the so-called T-Reflection, (2) seaward dipping reflector (SDR) wedges and a prominent northeast-trending escarpment on the Vøring Marginal High, and (3) extensive sill complexes in the adjacent Cretaceous Vøring Basin. During the last decade, new 2D and 3D industry seismic data along with improved processing techniques, such as broadband processing and noise reduction processing sequences, have made it possible to image and map the breakup igneous complex in much greater detail than previously possible. Our interpretation includes a combination of (1) seismic horizon picking, (2) integrated seismic-gravity-magnetic (SGM) interpretation, (3) seismic volcanostratigraphy, and (4) igneous seismic geomorphology. The results are integrated with published wide-angle seismic data, re-analyzed borehole data including new geochronology, and new geodynamic modeling of the effects of magmatism on the thermal history and subsidence of the margin. The extensive sill complexes and associated hydrothermal vent complexes in the Vøring Basin have a Paleocene-Eocene boundary age based on high-precision U/Pb dating combined with seismic mapping constraints. On the marginal high, our results show a highly variable crustal structure, with a pre-breakup configuration consisting of large-scale structural highs and sedimentary basins. These structures were in-filled and covered by basalt flows and volcanogenic sediments during the early stages of continental breakup in the earliest Eocene. Subsequently, rift basins developed along the continent-ocean boundary and where infilled by up to ca. 6 km thick basalt sequences, currently imaged as SDRs fed by a dike swarm

  19. Induced Seismicity from different sources in Italy: how to interpret it?

    NASA Astrophysics Data System (ADS)

    Pastori, M.; De Gori, P.; Piccinini, D.; Bagh, S.; Improta, L.; Chiarabba, C.

    2015-12-01

    Typically the term "induced seismicity" is used to refer minor earthquakes and tremors caused by human activities that alter the stresses and strains on the Earth's crust. In the last years, the interest in the induced seismicity related to fluids (oil and gas, and geothermal resources) extraction or injection is increased, because it is believed to be responsible to enucleate earthquakes. Possible sources of induced seismicity are not only represented by the oil and gas production but also, i.e., by changes in the water level of artificial lakes. The aim of this work is to show results from two different sources, wastewater injection and changes in the water level of an artificial reservoir (Pertusillo lake), that can produce induced earthquakes observed in the Val d'Agri basin (Italy) and to compare them with variation in crustal elastic parameters. Val d'Agri basin in the Apennines extensional belt hosts the largest oilfield in onshore Europe and is bordered by NW-SE ­trending fault systems. Most of the recorded seismicity seems to be related to these structures. We correlated the seismicity rate, injection curves and changes in water levels with temporal variations of Vp/Vs and anisotropic parameters of the crustal reservoirs and in the nearby area. We analysed about 983 high-quality recordings occurred from 2002 to 2014 in Val d'Agri basin from temporary and permanent network held by INGV and ENI corporate. 3D high-precision locations and manual-revised P- and S-picking are used to estimate anisotropic parameters (delay time and fast direction polarization) and Vp/Vs ratio. Seismicity is mainly located in two areas: in the SW of the Pertusillo Lake, and near the Eni Oil field (SW and NE of the Val d'Agri basin respectively). Our correlations well recognize the seismicity diffusion process, caused by both water injection and water level changes; these findings could help to model the active and pre-existing faults failure behaviour.

  20. Annotated bibliography, seismicity of and near the island of Hawaii and seismic hazard analysis of the East Rift of Kilauea

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

    Klein, F.W.

    1994-03-28

    This bibliography is divided into the following four sections: Seismicity of Hawaii and Kilauea Volcano; Occurrence, locations and accelerations from large historical Hawaiian earthquakes; Seismic hazards of Hawaii; and Methods of seismic hazard analysis. It contains 62 references, most of which are accompanied by short abstracts.

  1. Seismic Monitoring for the United Arab Emirates

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

    Rodgers, A; Nakanishi, K

    2005-04-11

    There is potential for earthquakes in the United Arab Emirates and in the Zagros mountains to cause structural damage and pose a threat to safety of people. Damaging effects from earthquakes can be mitigated by knowledge of the location and size of earthquakes, effects on construction, and monitoring these effects over time. Although a general idea of seismicity in the UAE may be determined with data from global seismic networks, these global networks do not have the sensitivity to record smaller seismic events and do not have the necessary accuracy to locate the events. A National Seismic Monitoring Observatory ismore » needed for the UAE that consists of a modern seismic network and a multidisciplinary staff that can analyze and interpret the data from the network. A seismic network is essential to locate earthquakes, determine event magnitudes, identify active faults and measure ground motions from earthquakes. Such a network can provide the data necessary for a reliable seismic hazard assessment in the UAE. The National Seismic Monitoring Observatory would ideally be situated at a university that would provide access to the wide range of disciplines needed in operating the network and providing expertise in analysis and interpretation.« less

  2. Seismic expression of Red Fork channels in Major and Kay Counties, Oklahoma

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

    Hanoch, C.A.

    1987-08-01

    This paper investigates the application of regional seismic to exploration and development Red Fork sands of the Cherokee Group, in Major and Kay Counties, Oklahoma. A computer-aided exploration system (CAEX) was used to justify the subtle seismic expressions with the geological interpretation. Modeling shows that the low-velocity shales are the anomalous rock in the Cherokee package, which is most represented by siltstone and thin sands. Because the Red Fork channel sands were incised into or deposited with laterally time-equivalent siltstones, no strong reflection coefficient is associated with the top of the sands. The objective sands become a seismic anomaly onlymore » when they cut into and replace a low-velocity shale. This knowledge allows mapping the channel thickness by interpreting the shale thickness from seismic data. A group shoot line in Major County, Oklahoma, has been tied to the geologic control, and the channel thicknesses have been interpreted assuming a detectable vertical resolution of 10 ft. A personal computer-based geophysical work station is used to construct velocity logs representative of the geology to produce forward-modeled synthetic seismic sections, and to display, in color, the seismic trace attributes. These synthetic sections are used as tools to compare with and interpret the seismic line and to evaluate the interpretative value of lowest cost, lesser quality data versus reprocessing or new data acquisition.« less

  3. Investigating the complex structural integrity of the Zeit Bay Field, Gulf of Suez, Egypt, using interpretation of 3D seismic reflection data

    NASA Astrophysics Data System (ADS)

    Afife, M.; Salem, M.; Aziz, M. Abdel

    2017-07-01

    Zeit Bay Field is one of the most important oil-bearing fields in the Gulf of Suez, Egypt, producing oil from the fractured basement rocks. Due to the complex structural setting of the area and the classical exploration concept that was based mainly on 2D seismic survey data, the area suffered from limited hydrocarbon interest for several years. During this time, most of the drilled wells hit structural highs and resulted in several dry holes. The present study is based on the interpretation of more recently acquired 3D seismic survey data as, matched with the available well logs, used to understand the complex structural setting of the Zeit Bay Field and provide insight into the entrapment style of the implied hydrocarbons. Several selected seismic cross sections were constructed, to extract subsurface geologic information, using available seismic profiles and wells. In addition, structure contour maps (isochronous maps, converted to depth maps) were constructed for the peaks of the basement, Nubian Sandstone, Kareem and Belayim Formations. Folds (anticlines and synclines) and faults (dip-slip) are identified on these maps, both individually and in groups, giving rise to step-like belts, as well as graben and horst blocks.

  4. How a joint interpretation of seismic scattering, velocity, and attenuation models explains the nature of the Campi Flegrei (Italy).

    NASA Astrophysics Data System (ADS)

    Calo, M.; Tramelli, A.

    2017-12-01

    Seismic P and S velocity models (and their ratio Vp/Vs) help illuminating the geometrical structure of the bodies and give insight on the presence of water, molten or gas saturated regions. Seismic attenuation represents the anelastic behavior of the medium. Due to its dependence on temperature, fluid contents and cracks presence, this parameter is also largely used to characterize the structures of volcanoes and geothermal areas. Scattering attenuation is related, in the upper crust, to the amount, size and organization of the fractures giving complementary information on the state of the medium.Therefore a joint interpretation of these models provides an exhaustive view of the elastic parameters in volcanic regions. Campi Flegrei is an active Caldera marked by strong vertical deformations of the ground called bradyseisms and several models have been proposed to describe the nature and the geometry of the bodies responsible of the bradyseisms. Here we show Vp, Vp/Vs, Qp and scattering models carried out by applying an enhanced seismic tomography method that combines de double difference approach (Zhang and Thurber, 2003) and the Weigthed Average Method (Calò et al., 2009, Calò et al., 2011, 2013). The data used are the earthquakes recorded during the largest bradyseism crisis of the 80's. Our method allowed to image structures with linear dimension of 0.5-1.2km, resulting in an improvement of the resolving power at least two times of the other published models (e.g. Priolo et al., 2012). The joint interpretation of seismic models allowed to discern small anomalous bodies at shallow depth (0.5-2.0 km) marked by relatively low Vp, high Vp/Vs ratio and low Qp values associated with the presence of shallow geothermal water saturated reservoir from regions with low Vp, low Vp/Vs and low Qp related to the gas saturated part of the reservoir. At deeper depth (2-3.5 km) bodies with high Vp and Vp/Vs and low Qp are associated with magmatic intrusions. The Scattering

  5. Reevaluation of the Seismicity and seismic hazards of Northeastern Libya

    NASA Astrophysics Data System (ADS)

    Ben Suleman, abdunnur; Aousetta, Fawzi

    2014-05-01

    Libya, located at the northern margin of the African continent, underwent many episodes of orogenic activities. These episodes of orogenic activities affected and shaped the geological setting of the country. This study represents a detailed investigation that aims to focus on the seismicity and its implications on earthquake hazards of Northeastern Libya. At the end of year 2005 the Libyan National Seismological Network starts functioning with 15 stations. The Seismicity of the area under investigation was reevaluated using data recorded by the recently established network. The Al-Maraj earthquake occurred in May 22nd 2005was analyzed. This earthquake was located in a known seismically active area. This area was the sight of the well known 1963 earthquake that kills over 200 people. Earthquakes were plotted and resulting maps were interpreted and discussed. The level of seismic activity is higher in some areas, such as the city of Al-Maraj. The offshore areas north of Al-Maraj seem to have higher seismic activity. It is highly recommended that the recent earthquake activity is considered in the seismic hazard assessments for the northeastern part of Libya.

  6. Seismic refraction survey of the ANS preferred site

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

    Davis, R.K.; Hopkins, R.A.; Doll, W.E.

    1992-02-01

    Between September 19, 1991 and October 8, 1991 personnel from Martin Marietta Energy Systems, Inc. (Energy Systems), Automated Sciences Group, Inc., and Marrich, Inc. performed a seismic refraction survey at the Advanced Neutron Source (ANS) preferred site. The purpose of this survey was to provide estimates of top-of-rock topography, based on seismic velocities, and to delineate variations in rock and soil velocities. Forty-four seismic refraction spreads were shot to determine top-of-rock depths at 42 locations. Nine of the seismic spreads were shot with long offsets to provide 216 top-of-rock depths for 4 seismic refraction profiles. The refraction spread locations weremore » based on the grid for the ANS Phase I drilling program. Interpretation of the seismic refraction data supports the assumption that the top-of-rock surface generally follows the local topography. The shallow top-of-rock interface interpreted from the seismic refraction data is also supported by limited drill information at the site. Some zones of anomalous data are present that could be the result of locally variable weathering, a localized variation in shale content, or depth to top-of-rock greater than the site norm.« less

  7. A 3D joint interpretation of magnetotelluric and seismic tomographic models: The case of the volcanic island of Tenerife

    NASA Astrophysics Data System (ADS)

    García-Yeguas, Araceli; Ledo, Juanjo; Piña-Varas, Perla; Prudencio, Janire; Queralt, Pilar; Marcuello, Alex; Ibañez, Jesús M.; Benjumea, Beatriz; Sánchez-Alzola, Alberto; Pérez, Nemesio

    2017-12-01

    In this work we have done a 3D joint interpretation of magnetotelluric and seismic tomography models. Previously we have described different techniques to infer the inner structure of the Earth. We have focused on volcanic regions, specifically on Tenerife Island volcano (Canary Islands, Spain). In this area, magnetotelluric and seismic tomography studies have been done separately. The novelty of the present work is the combination of both techniques in Tenerife Island. For this aim we have applied Fuzzy Clusters Method at different depths obtaining several clusters or classes. From the results, a geothermal system has been inferred below Teide volcano, in the center of Tenerife Island. An edifice hydrothermally altered and full of fluids is situated below Teide, ending at 600 m below sea level. From this depth the resistivity and VP values increase downwards. We also observe a clay cap structure, a typical feature in geothermal systems related with low resistivity and low VP values.

  8. Hillslope characterization in terms of geophysical units based on the joint interpretation of electrical resistivity and seismic velocity data

    NASA Astrophysics Data System (ADS)

    Feskova, Tatiana; Dietrich, Peter

    2015-04-01

    Hydrological conditions in a catchment depend on many factors such as climatic, geological, geomorphological, biological and human, which interact with each other and influence water balance in a catchment. This interaction leads to the subordination in the landscape structure, namely the weak elements subordinate to the powerful elements. Thereby, geological and geomorphological factors play an essential role in catchment development and organization. A hillslope consequently can be allocated to one class of the representative units because the important flow processes run at the hillslope. Moreover, a hillslope can be subdivided into stratigraphic subsurface units and significant hillslope areas based on the lithological change of contrasting interfaces. The knowledge of subsurface structures is necessary to understand and predicate complex hydrological processes in a catchment. Geophysical techniques provide a good opportunity to explore the subsurface. A complete geophysical investigation of subsurface in a catchment with difficult environmental conditions never will be achieved because of large time effort in the field, equipment logistic, and ambiguity in the data interpretation. The case study demonstrates how a catchment can be investigated using geophysical methods in an effective manner in terms of characterization of representative units with respect to a functional role in the catchment. This case study aims to develop combined resistivity and seismic velocity hillslope subsurface models for the distinction of representative functional units. In order to identify the contrasting interfaces of the hillslope, to localize significant hillslope areas, and to address the ambiguity in the geophysical data interpretation, the case study combined resistivity surveys (vertical electrical soundings and electrical resistivity tomography) with refraction seismic method, and conducted these measurements at one single profile along the hillslope transect and

  9. Expected Seismicity and the Seismic Noise Environment of Europa

    NASA Astrophysics Data System (ADS)

    Panning, Mark P.; Stähler, Simon C.; Huang, Hsin-Hua; Vance, Steven D.; Kedar, Sharon; Tsai, Victor C.; Pike, William T.; Lorenz, Ralph D.

    2018-01-01

    Seismic data will be a vital geophysical constraint on internal structure of Europa if we land instruments on the surface. Quantifying expected seismic activity on Europa both in terms of large, recognizable signals and ambient background noise is important for understanding dynamics of the moon, as well as interpretation of potential future data. Seismic energy sources will likely include cracking in the ice shell and turbulent motion in the oceans. We define a range of models of seismic activity in Europa's ice shell by assuming each model follows a Gutenberg-Richter relationship with varying parameters. A range of cumulative seismic moment release between 1016 and 1018 Nm/yr is defined by scaling tidal dissipation energy to tectonic events on the Earth's moon. Random catalogs are generated and used to create synthetic continuous noise records through numerical wave propagation in thermodynamically self-consistent models of the interior structure of Europa. Spectral characteristics of the noise are calculated by determining probabilistic power spectral densities of the synthetic records. While the range of seismicity models predicts noise levels that vary by 80 dB, we show that most noise estimates are below the self-noise floor of high-frequency geophones but may be recorded by more sensitive instruments. The largest expected signals exceed background noise by ˜50 dB. Noise records may allow for constraints on interior structure through autocorrelation. Models of seismic noise generated by pressure variations at the base of the ice shell due to turbulent motions in the subsurface ocean may also generate observable seismic noise.

  10. Interactive web visualization tools to the results interpretation of a seismic risk study aimed at the emergency levels definition

    NASA Astrophysics Data System (ADS)

    Rivas-Medina, A.; Gutierrez, V.; Gaspar-Escribano, J. M.; Benito, B.

    2009-04-01

    Results of a seismic risk assessment study are often applied and interpreted by users unspecialised on the topic or lacking a scientific background. In this context, the availability of tools that help translating essentially scientific contents to broader audiences (such as decision makers or civil defence officials) as well as representing and managing results in a user-friendly fashion, are on indubitable value. On of such tools is the visualization tool VISOR-RISNA, a web tool developed within the RISNA project (financed by the Emergency Agency of Navarre, Spain) for regional seismic risk assessment of Navarre and the subsequent development of emergency plans. The RISNA study included seismic hazard evaluation, geotechnical characterization of soils, incorporation of site effects to expected ground motions, vulnerability distribution assessment and estimation of expected damage distributions for a 10% probability of exceedance in 50 years. The main goal of RISNA was the identification of higher risk area where focusing detailed, local-scale risk studies in the future and the corresponding urban emergency plans. A geographic information system was used to combine different information layers, generate tables of results and represent maps with partial and final results. The visualization tool VISOR-RISNA is intended to facilitate the interpretation and representation of the collection of results, with the ultimate purpose of defining actuation plans. A number of criteria for defining actuation priorities are proposed in this work. They are based on combinations of risk parameters resulting from the risk study (such as expected ground motion and damage and exposed population), as determined by risk assessment specialists. Although the values that these parameters take are a result of the risk study, their distribution in several classes depends on the intervals defined by decision takers or civil defense officials. These criteria provide a ranking of

  11. Apalachicola Bay interpreted seismic horizons and updated IRIS chirp seismic-reflection data

    USGS Publications Warehouse

    Cross, V.A.; Twichell, D.C.; Foster, D.S.; O'Brien, T.F.

    2012-01-01

    Apalachicola Bay and St. George Sound contain the largest oyster fishery in Florida, and the growth and distribution of the numerous oyster reefs here are the combined product of modern estuarine conditions and the late Holocene evolution of the bay. A suite of geophysical data and cores were collected during a cooperative study by the U.S. Geological Survey, the National Oceanic and Atmospheric Administration Coastal Services Center, and the Apalachicola National Estuarine Research Reserve to refine the geology of the bay floor as well as the bay's Holocene stratigraphy. Sidescan-sonar imagery, bathymetry, high-resolution seismic profiles, and cores show that oyster reefs occupy the crests of sandy shoals that range from 1 to 7 kilometers in length, while most of the remainder of the bay floor is covered by mud. The sandy shoals are the surficial expression of broader sand deposits associated with deltas that advanced southward into the bay between 6,400 and 4,400 years before present. The seismic and core data indicate that the extent of oyster reefs was greatest between 2,400 and 1,200 years before present and has decreased since then due to the continued input of mud to the bay by the Apalachicola River. The association of oyster reefs with the middle to late Holocene sandy delta deposits indicates that the present distribution of oyster beds is controlled in part by the geologic evolution of the estuary.

  12. Application of seismic-refraction techniques to hydrologic studies

    USGS Publications Warehouse

    Haeni, F.P.

    1988-01-01

    During the past 30 years, seismic-refraction methods have been used extensively in petroleum, mineral, and engineering investigations and to some extent for hydrologic applications. Recent advances in equipment, sound sources, and computer interpretation techniques make seismic refraction a highly effective and economical means of obtaining subsurface data in hydrologic studies. Aquifers that can be defined by one or more high-seismic-velocity surface, such as (1) alluvial or glacial deposits in consolidated rock valleys, (2) limestone or sandstone underlain by metamorphic or igneous rock, or (3) saturated unconsolidated deposits overlain by unsaturated unconsolidated deposits, are ideally suited for seismic-refraction methods. These methods allow economical collection of subsurface data, provide the basis for more efficient collection of data by test drilling or aquifer tests, and result in improved hydrologic studies. This manual briefly reviews the basics of seismic-refraction theory and principles. It emphasizes the use of these techniques in hydrologic investigations and describes the planning, equipment, field procedures, and interpretation techniques needed for this type of study. Further-more, examples of the use of seismic-refraction techniques in a wide variety of hydrologic studies are presented.

  13. Causality between expansion of seismic cloud and maximum magnitude of induced seismicity in geothermal field

    NASA Astrophysics Data System (ADS)

    Mukuhira, Yusuke; Asanuma, Hiroshi; Ito, Takatoshi; Häring, Markus

    2016-04-01

    Occurrence of induced seismicity with large magnitude is critical environmental issues associated with fluid injection for shale gas/oil extraction, waste water disposal, carbon capture and storage, and engineered geothermal systems (EGS). Studies for prediction of the hazardous seismicity and risk assessment of induced seismicity has been activated recently. Many of these studies are based on the seismological statistics and these models use the information of the occurrence time and event magnitude. We have originally developed physics based model named "possible seismic moment model" to evaluate seismic activity and assess seismic moment which can be ready to release. This model is totally based on microseismic information of occurrence time, hypocenter location and magnitude (seismic moment). This model assumes existence of representative parameter having physical meaning that release-able seismic moment per rock volume (seismic moment density) at given field. Seismic moment density is to be estimated from microseismic distribution and their seismic moment. In addition to this, stimulated rock volume is also inferred by progress of microseismic cloud at given time and this quantity can be interpreted as the rock volume which can release seismic energy due to weakening effect of normal stress by injected fluid. Product of these two parameters (equation (1)) provide possible seismic moment which can be released from current stimulated zone as a model output. Difference between output of this model and observed cumulative seismic moment corresponds the seismic moment which will be released in future, based on current stimulation conditions. This value can be translated into possible maximum magnitude of induced seismicity in future. As this way, possible seismic moment can be used to have feedback to hydraulic stimulation operation in real time as an index which can be interpreted easily and intuitively. Possible seismic moment is defined as equation (1), where D

  14. Effects of volcano topography on seismic broad-band waveforms

    NASA Astrophysics Data System (ADS)

    Neuberg, Jürgen; Pointer, Tim

    2000-10-01

    Volcano seismology often deals with rather shallow seismic sources and seismic stations deployed in their near field. The complex stratigraphy on volcanoes and near-field source effects have a strong impact on the seismic wavefield, complicating the interpretation techniques that are usually employed in earthquake seismology. In addition, as most volcanoes have a pronounced topography, the interference of the seismic wavefield with the stress-free surface results in severe waveform perturbations that affect seismic interpretation methods. In this study we deal predominantly with the surface effects, but take into account the impact of a typical volcano stratigraphy as well as near-field source effects. We derive a correction term for plane seismic waves and a plane-free surface such that for smooth topographies the effect of the free surface can be totally removed. Seismo-volcanic sources radiate energy in a broad frequency range with a correspondingly wide range of different Fresnel zones. A 2-D boundary element method is employed to study how the size of the Fresnel zone is dependent on source depth, dominant wavelength and topography in order to estimate the limits of the plane wave approximation. This approximation remains valid if the dominant wavelength does not exceed twice the source depth. Further aspects of this study concern particle motion analysis to locate point sources and the influence of the stratigraphy on particle motions. Furthermore, the deployment strategy of seismic instruments on volcanoes, as well as the direct interpretation of the broad-band waveforms in terms of pressure fluctuations in the volcanic plumbing system, are discussed.

  15. Spatial distance effects on incremental semantic interpretation of abstract sentences: evidence from eye tracking.

    PubMed

    Guerra, Ernesto; Knoeferle, Pia

    2014-12-01

    A large body of evidence has shown that visual context information can rapidly modulate language comprehension for concrete sentences and when it is mediated by a referential or a lexical-semantic link. What has not yet been examined is whether visual context can also modulate comprehension of abstract sentences incrementally when it is neither referenced by, nor lexically associated with, the sentence. Three eye-tracking reading experiments examined the effects of spatial distance between words (Experiment 1) and objects (Experiment 2 and 3) on participants' reading times for sentences that convey similarity or difference between two abstract nouns (e.g., 'Peace and war are certainly different...'). Before reading the sentence, participants inspected a visual context with two playing cards that moved either far apart or close together. In Experiment 1, the cards turned and showed the first two nouns of the sentence (e.g., 'peace', 'war'). In Experiments 2 and 3, they turned but remained blank. Participants' reading times at the adjective (Experiment 1: first-pass reading time; Experiment 2: total times) and at the second noun phrase (Experiment 3: first-pass times) were faster for sentences that expressed similarity when the preceding words/objects were close together (vs. far apart) and for sentences that expressed dissimilarity when the preceding words/objects were far apart (vs. close together). Thus, spatial distance between words or entirely unrelated objects can rapidly and incrementally modulate the semantic interpretation of abstract sentences. Copyright © 2014 Elsevier B.V. All rights reserved.

  16. Plate and Plume Flux: Constraints for paleomagnetic reference frames and interpretation of deep mantle seismic heterogeneity. (Invited)

    NASA Astrophysics Data System (ADS)

    Bunge, H.; Schuberth, B. S.; Shephard, G. E.; Müller, D.

    2010-12-01

    Plate and plume flow are dominant modes of mantle convection, as pointed out by Geoff Davies early on. Driven, respectively, from a cold upper and a hot lower thermal boundary layer these modes are now sufficiently well imaged by seismic tomographers to exploit the thermal boundary layer concept as an effective tool in exploring two long standing geodynamic problems. One relates to the choice of an absolute reference frame in plate tectonic reconstructions. Several absolute reference frames have been proposed over the last decade, including those based on hotspot tracks displaying age progression and assuming either fixity or motion, as well as palaeomagnetically-based reference frames, a subduction reference frame and hybrid versions. Each reference frame implies a particular history of the location of subduction zones through time and thus the evolution of mantle heterogeneity via mixing of subducted slab material in the mantle. Here we compare five alternative absolute plate motion models in terms of their consequences for deep mantle structure. Taking global paleo-plate boundaries and plate velocities back to 140 Ma derived from the new plate tectonic reconstruction software GPlates and assimilating them into vigorous 3-D spherical mantle circulation models, we infer geodynamic mantle heterogeneity and compare it to seismic tomography for each absolute rotation model. We also focus on the challenging problem of interpreting deep mantle seismic heterogeneity in terms of thermal and compositional variations. Using published thermodynamically self-consistent mantle mineralogy models in the pyrolite composition, we find strong plume flux from the CMB, with a high temperature contrast (on the order of 1000 K) across the lower thermal boundary layer is entirely sufficient to explain elastic heterogeneity in the deep mantle for a number of quantitative measures. A high excess temperatures of +1000--1500 K for plumes in the lowermost mantle is particularly important in

  17. Gabor Deconvolution as Preliminary Method to Reduce Pitfall in Deeper Target Seismic Data

    NASA Astrophysics Data System (ADS)

    Oktariena, M.; Triyoso, W.

    2018-03-01

    Anelastic attenuation process during seismic wave propagation is the trigger of seismic non-stationary characteristic. An absorption and a scattering of energy are causing the seismic energy loss as the depth increasing. A series of thin reservoir layers found in the study area is located within Talang Akar Fm. Level, showing an indication of interpretation pitfall due to attenuation effect commonly occurred in deeper level seismic data. Attenuation effect greatly influences the seismic images of deeper target level, creating pitfalls in several aspect. Seismic amplitude in deeper target level often could not represent its real subsurface character due to a low amplitude value or a chaotic event nearing the Basement. Frequency wise, the decaying could be seen as the frequency content diminishing in deeper target. Meanwhile, seismic amplitude is the simple tool to point out Direct Hydrocarbon Indicator (DHI) in preliminary Geophysical study before a further advanced interpretation method applied. A quick-look of Post-Stack Seismic Data shows the reservoir associated with a bright spot DHI while another bigger bright spot body detected in the North East area near the field edge. A horizon slice confirms a possibility that the other bright spot zone has smaller delineation; an interpretation pitfall commonly occurs in deeper level of seismic. We evaluates this pitfall by applying Gabor Deconvolution to address the attenuation problem. Gabor Deconvolution forms a Partition of Unity to factorize the trace into smaller convolution window that could be processed as stationary packets. Gabor Deconvolution estimates both the magnitudes of source signature alongside its attenuation function. The enhanced seismic shows a better imaging in the pitfall area that previously detected as a vast bright spot zone. When the enhanced seismic is used for further advanced reprocessing process, the Seismic Impedance and Vp/Vs Ratio slices show a better reservoir delineation, in which the

  18. Computer program modifications of Open-file report 82-1065; a comprehensive system for interpreting seismic-refraction and arrival-time data using interactive computer methods

    USGS Publications Warehouse

    Ackermann, Hans D.; Pankratz, Leroy W.; Dansereau, Danny A.

    1983-01-01

    The computer programs published in Open-File Report 82-1065, A comprehensive system for interpreting seismic-refraction arrival-time data using interactive computer methods (Ackermann, Pankratz, and Dansereau, 1982), have been modified to run on a mini-computer. The new version uses approximately 1/10 of the memory of the initial version, is more efficient and gives the same results.

  19. Improving Seismic Event Characterisation

    DTIC Science & Technology

    1996-07-22

    classificat i,; and further phase identification . 6.4.3 Seismic event interpretation The’ system of event processing is based on an assumption tree ...and is enhanced with usez by a network. 14, SUBJECT TERMSý 15. NUMBER OF PAGES seismic models, travel. timtes phase identification 16 PRICE CODE 17...hesimwinlia’ rati of t lieDl scisillograonis is 2/3 secondIs andI the receiver spaci mi is 1 /3 degreeus. ’lIi iiaiiiii iltdiwic’ ewe ii rayv-the~oret~icaIl

  20. Spots of Seismic Danger Extracted by Properties of Low-Frequency Seismic Noise

    NASA Astrophysics Data System (ADS)

    Lyubushin, Alexey

    2013-04-01

    region of Nankai Trough. The analysis of seismic noise after March 2011 indicates increasing of probability of the 2nd mega-earthquake starting from the middle of 2013 within the region of Nankai Trough which remains to be SSD. References 1. Lyubushin A. Multifractal Parameters of Low-Frequency Microseisms // V. de Rubeis et al. (eds.), Synchronization and Triggering: from Fracture to Earthquake Processes, GeoPlanet: Earth and Planetary Sciences 1, DOI 10.1007/978-3-642-12300-9_15, Springer-Verlag Berlin Heidelberg, 2010, 388p., Chapter 15, pp.253-272. http://www.springerlink.com/content/hj2l211577533261/ 2. Lyubushin A.A. Synchronization of multifractal parameters of regional and global low-frequency microseisms - European Geosciences Union General Assembly 2010, Vienna, 02-07 of May, 2010, Geophysical Research Abstracts, Vol. 12, EGU2010-696, 2010. http://meetingorganizer.copernicus.org/EGU2010/EGU2010-696.pdf 3. Lyubushin A.A. Synchronization phenomena of low-frequency microseisms. European Seismological Commission, 32nd General Assembly, September 06-10, 2010, Montpelier, France. Book of abstracts, p.124, session ES6. http://alexeylyubushin.narod.ru/ESC-2010_Book_of_abstracts.pdf 4. Lyubushin A.A. Seismic Catastrophe in Japan on March 11, 2011: Long-Term Prediction on the Basis of Low-Frequency Microseisms - Izvestiya, Atmospheric and Oceanic Physics, 2011, Vol. 46, No. 8, pp. 904-921. http://www.springerlink.com/content/kq53j2667024w715/ 5. Lyubushin, A. Prognostic properties of low-frequency seismic noise. Natural Science, 4, 659-666.doi: 10.4236/ns.2012.428087. http://www.scirp.org/journal/PaperInformation.aspx?paperID=21656

  1. Lithofacies and seismic-reflection interpretation of temperate glacimarine sedimentation in Tarr Inlet, Glacier Bay, Alaska

    USGS Publications Warehouse

    Cai, J.; Powell, R.D.; Cowan, E.A.; Carlson, P.R.

    1997-01-01

    High-resolution seismic-reflection profiles of sediment fill within Tart Inlet of Glacier Bay, Alaska, show seismic facies changes with increasing distance from the glacial termini. Five types of seismic facies are recognized from analysis of Huntec and minisparker records, and seven lithofacies are determined from detailed sedimentologic study of gravity-, vibro- and box-cores, and bottom grab samples. Lithofacies and seismic facies associations, and fjord-floor morphology allow us to divide the fjord into three sedimentary environments: ice-proximal, iceberg-zone and ice-distal. The ice-proximal environment, characterized by a morainal-bank depositional system, can be subdivided into bank-back, bank-core and bank-front subenvironments, each of which is characterized by a different depositional subsystem. A bank-back subsystem shows chaotic seismic facies with a mounded surface, which we infer consists mainly of unsorted diamicton and poorly sorted coarse-grained sediments. A bank-core depositional subsystem is a mixture of diamicton, rubble, gravel, sand and mud. Seismic-reflection records of this subsystem are characterized by chaotic seismic facies with abundant hyperbolic diffractions and a hummocky surface. A bank-front depositional subsystem consists of mainly stratified and massive sand, and is characterized by internal hummocky facies on seismic-reflection records with significant surface relief and sediment gravity flow channels. The depositional system formed in the iceberg-zone environment consists of rhythmically laminated mud interbedded with thin beds of weakly stratified diamicton and stratified or massive sand and silt. On seismic-reflection profiles, this depositional system is characterized by discontinuously stratified facies with multiple channels on the surface in the proximal zone and a single channel on the largely flat sediment surface in the distal zone. The depositional system formed in the ice-distal environment consists of interbedded

  2. Using geologic maps and seismic refraction in pavement-deflection analysis

    DOT National Transportation Integrated Search

    1999-10-01

    The researchers examined the relationship between three data types -- geologic maps, pavement deflection, and seismic refraction data -- from diverse geologic settings to determine whether geologic maps and seismic data might be used to interpret def...

  3. Quaternary tectonics from seismic interpretation and its potential relation with deep geothermal fluids in the Marche (Central Italy).

    NASA Astrophysics Data System (ADS)

    Chicco, Jessica; Invernizzi, Chiara; Pierantoni, Pietro Paolo; Costa, Mario

    2017-04-01

    Knowledge of the structural features is fundamental in evaluating geothermal exchange potential and in modelling geothermal systems. In particular, faults and fractures play an important role for the circulation of fluids in the crust, and structural setting can influence groundwater flow, its regime, chemistry and electrical conductivity. In this context, data coming from accurate studies of groundwater physical properties in the Marche region (Central Italy), concerning electrical conductivity above all, revealed some anomalies in several localities that could be ascribed to a strong structural control. Data acquisition and interpretation of some SW-NE seismic reflection profiles crossing the Apennine chain to the Adriatic sea and kindly provided by ENI S.p.A, highlight important deep Plio-Quaternary structures connected with minor surface ones and to hydrogeological conditions. Seismic profiles interpretation allowed to reconstruct the structural setting and to identify the recent evolution of the Apennine Marche sector in more detail with respect to what is already known. In fact, some high angle structures affecting the whole sedimentary sequence and routing at high depth were labelled. These are NW-SE sub-parallel transpressive structures bounded by SW and NE-dipping high-angle reverse faults reaching > 10 km depth (positive flower structures), and probably involving the upper crust basement. Three main alignments were identified from W to the coast line. In some cases, flower nucleation gives rise to the lifting and counter-clockwise rotation of the Pre-Pliocene substratum blocks, with the upwelling and outcropping of Upper Miocene (Messinian) evaporite deposits along the axial zone of the transpressive structural highs. Noting the analyses of groundwater properties coming from wells placed in proximity of these structures or located along the analysed seismic profiles, anomalies in electrical conductivity are relevant. The activity of the deep rooting

  4. Micropaleontology of selected wells and seismic shot holes, northern Alaska

    USGS Publications Warehouse

    Mickey, Michael B.; Haga, Hideyo; Bird, Kenneth J.

    2006-01-01

    This report provides micropaleontologic data (foraminifera, pollen, spores, and microplankton) and interpretations of the rocks penetrated by 49 wells and 3,134 seismic shot holes distributed among 73 seismic lines (figs. 1, 2; table 1). All shot holes and 30 wells are located within the National Petroleum Reserve in Alaska (NPRA); the remaining 19 wells are located adjacent to the NPRA. The biostratigraphic zonation scheme, stratigraphy, and geologic ages followed in this study are summarized in figure 3. This update brings paleontologic analyses performed at various times over several decades to a current, unified set of interpretations that benefit from the evolution of northern Alaska biostratigraphic understanding developed during the past 33-years by Mickey and Haga. For each well, paleontologic information includes microfossil distribution charts, data spreadsheets, diversity graphs, and interpretive reports describing age and environments of deposition. Three biostratigraphic well-correlation sections that relate Chukchi Sea wells to onshore northwestern NPRA wells are also included. For all analyzed seismic shot hole samples, foraminiferal age and environmental interpretations are provided; palynological interpretations are provided only for those shot hole samples collected and analyzed after 1976, a little less than half of the total number of samples.

  5. 3D Seismic Interpretation of a Plio-Pleistocene Mass Transport Deposit in the Deepwater Taranaki Basin of New Zealand

    NASA Astrophysics Data System (ADS)

    Rusconi, Francisco Jose

    A series of Plio-Pleistocene mass transport deposits (MTD) have been identified in the deepwater Taranaki Basin, in New Zealand, using the Romney 3D seismic survey, which covers an area of approximately 2000 km2. One of these MTDs has been chosen for description and interpretation based on high confidence mapping of its boundary surfaces. The deposit exhibits an array of interesting features similar to those documented by researchers elsewhere plus a unique basal feature unlike those previously observed. The basal shear surface exhibits erosional features such as grooves, "monkey fingers", and glide tracks. Internally, the MTD is typically characterized by low impedance, chaotic, semi-transparent reflectors surrounding isolated coherent packages of seismic facies interpreted as intact blocks rafted within the mass transport complex. Distally, the deposit presents outrunner blocks and pressure ridges. The new element described in this work consists of a composite feature that includes a protruding obstacle ("shield block") on the paleo-seafloor that acted as a barrier to subsequent flows as they advanced downslope. These blocks disrupt the incoming flow and result in elongate, downflow negative features ("erosional shadow scours"), which are then infilled by the mass transport deposit, and are preserved as elongate isochore thicks. Kinematic evidence provided by various structures suggests that the MTD flow direction was SE-NW toward bathyal depths. The features presented and the absence of extensional headwall structures, such as local arcuate glide planes and rotated slide blocks, suggest that this part of the deposit belongs to the translational to distal domain of the MTD, and its source area is expected to be somewhere toward the SE in a paleo continental slope.

  6. Seismic characteristics of central Brazil crust and upper mantle: A deep seismic refraction study

    USGS Publications Warehouse

    Soares, J.E.; Berrocal, J.; Fuck, R.A.; Mooney, W.D.; Ventura, D.B.R.

    2006-01-01

    A two-dimensional model of the Brazilian central crust and upper mantle was obtained from the traveltime interpretation of deep seismic refraction data from the Porangatu and Cavalcante lines, each approximately 300 km long. When the lines were deployed, they overlapped by 50 km, forming an E-W transect approximately 530 km long across the Tocantins Province and western Sa??o Francisco Craton. The Tocantins Province formed during the Neoproterozoic when the Sa??o Francisco, the Paranapanema, and the Amazon cratons collided, following the subduction of the former Goia??s ocean basin. Average crustal VP and VP/VS ratios, Moho topography, and lateral discontinuities within crustal layers suggest that the crust beneath central Brazil can be associated with major geological domains recognized at the surface. The Moho is an irregular interface, between 36 and 44 km deep, that shows evidences of first-order tectonic structures. The 8.05 and 8.23 km s-1 P wave velocities identify the upper mantle beneath the Porangatu and Cavalcante lines, respectively. The observed seismic features allow for the identification of (1) the crust has largely felsic composition in the studied region, (2) the absence of the mafic-ultramafic root beneath the Goia??s magmatic arc, and (3) block tectonics in the foreland fold-and-thrust belt of the northern Brasi??lia Belt during the Neoproterozoic. Seismic data also suggested that the Bouguer gravimetric discontinuities are mainly compensated by differences in mass distribution within the lithospheric mantle. Finally, the Goia??s-Tocantins seismic belt can be interpreted as a natural seismic alignment related to the Neoproterozoic mantle domain. Copyright 2006 by the American Geophysical Union.

  7. Seismic Fracture Characterization Methodologies for Enhanced Geothermal Systems

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

    Queen, John H.

    2016-05-09

    Executive Summary The overall objective of this work was the development of surface and borehole seismic methodologies using both compressional and shear waves for characterizing faults and fractures in Enhanced Geothermal Systems. We used both surface seismic and vertical seismic profile (VSP) methods. We adapted these methods to the unique conditions encountered in Enhanced Geothermal Systems (EGS) creation. These conditions include geological environments with volcanic cover, highly altered rocks, severe structure, extreme near surface velocity contrasts and lack of distinct velocity contrasts at depth. One of the objectives was the development of methods for identifying more appropriate seismic acquisition parametersmore » for overcoming problems associated with these geological factors. Because temperatures up to 300º C are often encountered in these systems, another objective was the testing of VSP borehole tools capable of operating at depths in excess of 1,000 m and at temperatures in excess of 200º C. A final objective was the development of new processing and interpretation techniques based on scattering and time-frequency analysis, as well as the application of modern seismic migration imaging algorithms to seismic data acquired over geothermal areas. The use of surface seismic reflection data at Brady's Hot Springs was found useful in building a geological model, but only when combined with other extensive geological and geophysical data. The use of fine source and geophone spacing was critical in producing useful images. The surface seismic reflection data gave no information about the internal structure (extent, thickness and filling) of faults and fractures, and modeling suggests that they are unlikely to do so. Time-frequency analysis was applied to these data, but was not found to be significantly useful in their interpretation. Modeling does indicate that VSP and other seismic methods with sensors located at depth in wells will be the most

  8. Interpretation of Microseismicity Observed From Surface and Borehole Seismic Arrays During Hydraulic Fracturing in Shale - Bedding Plane Slip Model

    NASA Astrophysics Data System (ADS)

    Stanek, F.; Jechumtalova, Z.; Eisner, L.

    2017-12-01

    We present a geomechanical model explaining microseismicity induced by hydraulic fracturing in shales developed from many datasets acquired with two most common types of seismic monitoring arrays, surface and dual-borehole arrays. The geomechanical model explains the observed source mechanisms and locations of induced events from two stimulated shale reservoirs. We observe shear dip-slip source mechanisms with nodal planes aligned with location trends. We show that such seismicity can be explained as a shearing along bedding planes caused by aseismic opening of vertical hydraulic fractures. The source mechanism inversion was applied only to selected high-quality events with sufficient signal-to-noise ratio. We inverted P- and P- and S-wave arrival amplitudes to full-moment tensor and decomposed it to shear, volumetric and compensated linear vector dipole components. We also tested an effect of noise presented in the data to evaluate reliability of non-shear components. The observed seismicity from both surface and downhole monitoring of shale stimulations is very similar. The locations of induced microseismic events are limited to narrow depth intervals and propagate along distinct trend(s) showing fracture propagation in direction of maximum horizontal stress from injection well(s). The source mechanisms have a small non-shear component which can be partly explained as an effect of noise in the data, i.e. events represent shearing on faults. We observe predominantly dip-slip events with a strike of the steeper (almost vertical) nodal plane parallel to the fracture propagation. Therefore the other possible nodal plane is almost horizontal. The rake angles of the observed mechanisms divide these dip-slips into two groups with opposite polarities. It means that we observe opposite movements on the nearly identically oriented faults. Realizing a typical structural weakness of shale in horizontal planes, we interpret observed microseismicity as a result of shearing

  9. Broadband seismic and acoustic observations of volcanic seismicity

    NASA Astrophysics Data System (ADS)

    Aster, R.; Lees, J.; Neuberg, J.

    2000-08-01

    It has been frequently noted (e.g. Aki, 1992) that volcanoes present some of the most difficult challenges in seismology due to a plethora of complex source and structural issues. The broadband seismo-acoustic study of active volcanoes is still in its adolescence, and the papers in this volume primarily describe first-order attempts to understand these signals and to build on a much longer history of short-period seismic observations and interpretations.

  10. Digital recovery, modification, and analysis of Tetra Tech seismic horizon mapping, National Petroleum Reserve Alaska (NPRA), northern Alaska

    USGS Publications Warehouse

    Saltus, R.W.; Kulander, Christopher S.; Potter, Christopher J.

    2002-01-01

    We have digitized, modified, and analyzed seismic interpretation maps of 12 subsurface stratigraphic horizons spanning portions of the National Petroleum Reserve in Alaska (NPRA). These original maps were prepared by Tetra Tech, Inc., based on about 15,000 miles of seismic data collected from 1974 to 1981. We have also digitized interpreted faults and seismic velocities from Tetra Tech maps. The seismic surfaces were digitized as two-way travel time horizons and converted to depth using Tetra Tech seismic velocities. The depth surfaces were then modified by long-wavelength corrections based on recent USGS seismic re-interpretation along regional seismic lines. We have developed and executed an algorithm to identify and calculate statistics on the area, volume, height, and depth of closed structures based on these seismic horizons. These closure statistics are tabulated and have been used as input to oil and gas assessment calculations for the region. Directories accompanying this report contain basic digitized data, processed data, maps, tabulations of closure statistics, and software relating to this project.

  11. Artificial neural systems for interpretation and inversion of seismic data

    NASA Astrophysics Data System (ADS)

    Calderon-Macias, Carlos

    The goal of this work is to investigate the feasibility of using neural network (NN) models for solving geophysical exploration problems. First, a feedforward neural network (FNN) is used to solve inverse problems. The operational characteristics of a FNN are primarily controlled by a set of weights and a nonlinear function that performs a mapping between two sets of data. In a process known as training, the FNN weights are iteratively adjusted to perform the mapping. After training, the computed weights encode important features of the data that enable one pattern to be distinguished from another. Synthetic data computed from an ensemble of earth models and the corresponding models provide the training data. Two training methods are studied: the backpropagation method which is a gradient scheme, and a global optimization method called very fast simulated annealing (VFSA). A trained network is then used to predict models from new data (e.g., data from a new location) in a one-step procedure. The application of this method to the problems of obtaining formation resistivities and layer thicknesses from resistivity sounding data and 1D velocity models from seismic data shows that trained FNNs produce reasonably accurate earth models when observed data are input to the FNNs. In a second application, a FNN is used for automating the NMO correction process of seismic reflection data. The task of the FNN is to map CMP data at control locations along a seismic line into subsurface velocities. The network is trained while the velocity analyses are performed at the control locations. Once trained, the computed weights are used as an operator that acts on the remaining CMP data as a velocity interpolator, resulting in a fast method for NMO correction. The second part of this dissertation describes the application of a Hopfield neural network (HNN) to the problems of deconvolution and multiple attenuation. In these applications, the unknown parameters (reflection coefficients

  12. Seismic modeling of Earth's 3D structure: Recent advancements

    NASA Astrophysics Data System (ADS)

    Ritsema, J.

    2008-12-01

    Global models of Earth's seismic structure continue to improve due to the growth of seismic data sets, implementation of advanced wave propagations theories, and increased computational power. In my presentation, I will summarize seismic tomography results from the past 5-10 years. I will compare the most recent P and S velocity models, discuss model resolution and model interpretation, and present an, admittedly biased, list of research directions required to develop the next generation 3D models.

  13. Seismic reflection data imaging and interpretation from Braniewo2014 experiment using additional wide-angle refraction and reflection and well-logs data

    NASA Astrophysics Data System (ADS)

    Trzeciak, Maciej; Majdański, Mariusz; Białas, Sebastian; Gaczyński, Edward; Maksym, Andrzej

    2015-04-01

    Braniewo2014 reflection and refraction experiment was realized in cooperation between Polish Oil and Gas Company (PGNiG) and the Institute of Geophysics (IGF), Polish Academy of Sciences, near the locality of Braniewo in northern Poland. PGNiG realized a 20-km-long reflection profile, using vibroseis and dynamite shooting; the aim of the reflection survey was to characterise Silurian shale gas reservoir. IGF deployed 59 seismic stations along this profile and registered additional full-spread wide-angle refraction and reflection data, with offsets up to 12 km; maximum offsets from the seismic reflection survey was 3 km. To improve the velocity information two velocity logs from near deep boreholes were used. The main goal of the joint reflection-refraction interpretation was to find relations between velocity field from reflection velocity analysis and refraction tomography, and to build a velocity model which would be consistent for both, reflection and refraction, datasets. In this paper we present imaging results and velocity models from Braniewo2014 experiment and the methodology we used.

  14. Amplitude interpretation and visualization of three-dimensional reflection data

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

    Enachescu, M.E.

    1994-07-01

    Digital recording and processing of modern three-dimensional surveys allow for relative good preservation and correct spatial positioning of seismic reflection amplitude. A four-dimensional seismic reflection field matrix R (x,y,t,A), which can be computer visualized (i.e., real-time interactively rendered, edited, and animated), is now available to the interpreter. The amplitude contains encoded geological information indirectly related to lithologies and reservoir properties. The magnitude of the amplitude depends not only on the acoustic impedance contrast across a boundary, but is also strongly affected by the shape of the reflective boundary. This allows the interpreter to image subtle tectonic and structural elements notmore » obvious on time-structure maps. The use of modern workstations allows for appropriate color coding of the total available amplitude range, routine on-screen time/amplitude extraction, and late display of horizon amplitude maps (horizon slices) or complex amplitude-structure spatial visualization. Stratigraphic, structural, tectonic, fluid distribution, and paleogeographic information are commonly obtained by displaying the amplitude variation A = A(x,y,t) associated with a particular reflective surface or seismic interval. As illustrated with several case histories, traditional structural and stratigraphic interpretation combined with a detailed amplitude study generally greatly enhance extraction of subsurface geological information from a reflection data volume. In the context of three-dimensional seismic surveys, the horizon amplitude map (horizon slice), amplitude attachment to structure and [open quotes]bright clouds[close quotes] displays are very powerful tools available to the interpreter.« less

  15. Low-angle normal faulting and isostatic response in the Gulf of Suez: Evidence from seismic interpretation and geometric reconstruction

    NASA Technical Reports Server (NTRS)

    Perry, S. K.; Schamel, S.

    1985-01-01

    Tectonic extension within continental crust creates a variety of major features best classed as extensional orogens. These features have come under increasing attention in recent years, with the welding of field observation and theoretical concepts. Most recent advances have come from the Basin and Range Province of the southwestern United States and from the North Sea. Application of these geometric and isostatic concepts, in combination with seismic interpretation, to the southern Gulf of Suez, an active extensional orogen, allows generation of detailed structural maps and geometrically balanced sections which suggest a regional structural model. Geometric models which should prove to be a valuable adjunct to numerical and thermal models for the rifting process are discussed.

  16. The interpretation of proverbs by elderly with high, medium and low educational level: Abstract reasoning as an aspect of executive functions

    PubMed Central

    Wachholz, Thalita Bianchi de Oliveira; Yassuda, Mônica Sanches

    2011-01-01

    It is now known that cognitive functions tend to decline with age. Executive functions (EF) are among the first abilities to decline with aging. A subcomponent of the EF is abstract reasoning. The Test of Proverbs is an instrument that can be used to evaluate the capacity of abstract reasoning. Objective To examine the association of performance in interpretation of proverbs, with education and with episodic memory and EF tasks. Methods A total of 67 individuals aged between 60 and 75 years were evaluated, and divided into three categories of education: 1-4 years, 5-8 years, and 9 or more years of schooling. The instruments used were a sociodemographic questionnaire (gender, age, marital status, education, income, previous occupation, current occupation and health perception), the Mini Mental State Examination, Brief Cognitive Screening Battery; Geriatric Depression Scale; Forward and Backward Digit Span (WAIS-III), and the Test of Proverbs. Results A high impact of education was seen on the interpretation of proverbs, with lower performance among the elderly with less education. A significant association between performance on the Test of Proverbs and scores on the MMSE, GDS, and verbal fluency tests was found. There was a modest association with incidental memory. Conclusions The capacity to interpret proverbs is strongly associated with education and with performance on other EF tasks. PMID:29213717

  17. Seismic facies analysis based on self-organizing map and empirical mode decomposition

    NASA Astrophysics Data System (ADS)

    Du, Hao-kun; Cao, Jun-xing; Xue, Ya-juan; Wang, Xing-jian

    2015-01-01

    Seismic facies analysis plays an important role in seismic interpretation and reservoir model building by offering an effective way to identify the changes in geofacies inter wells. The selections of input seismic attributes and their time window have an obvious effect on the validity of classification and require iterative experimentation and prior knowledge. In general, it is sensitive to noise when waveform serves as the input data to cluster analysis, especially with a narrow window. To conquer this limitation, the Empirical Mode Decomposition (EMD) method is introduced into waveform classification based on SOM. We first de-noise the seismic data using EMD and then cluster the data using 1D grid SOM. The main advantages of this method are resolution enhancement and noise reduction. 3D seismic data from the western Sichuan basin, China, are collected for validation. The application results show that seismic facies analysis can be improved and better help the interpretation. The powerful tolerance for noise makes the proposed method to be a better seismic facies analysis tool than classical 1D grid SOM method, especially for waveform cluster with a narrow window.

  18. CALIBRATION OF SEISMIC ATTRIBUTES FOR RESERVOIR CHARACTERIZATION

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

    Wayne D. Pennington; Horacio Acevedo; Aaron Green

    2002-10-01

    The project, ''Calibration of Seismic Attributes for Reservoir Calibration,'' is now complete. Our original proposed scope of work included detailed analysis of seismic and other data from two to three hydrocarbon fields; we have analyzed data from four fields at this level of detail, two additional fields with less detail, and one other 2D seismic line used for experimentation. We also included time-lapse seismic data with ocean-bottom cable recordings in addition to the originally proposed static field data. A large number of publications and presentations have resulted from this work, including several that are in final stages of preparation ormore » printing; one of these is a chapter on ''Reservoir Geophysics'' for the new Petroleum Engineering Handbook from the Society of Petroleum Engineers. Major results from this project include a new approach to evaluating seismic attributes in time-lapse monitoring studies, evaluation of pitfalls in the use of point-based measurements and facies classifications, novel applications of inversion results, improved methods of tying seismic data to the wellbore, and a comparison of methods used to detect pressure compartments. Some of the data sets used are in the public domain, allowing other investigators to test our techniques or to improve upon them using the same data. From the public-domain Stratton data set we have demonstrated that an apparent correlation between attributes derived along ''phantom'' horizons are artifacts of isopach changes; only if the interpreter understands that the interpretation is based on this correlation with bed thickening or thinning, can reliable interpretations of channel horizons and facies be made. From the public-domain Boonsville data set we developed techniques to use conventional seismic attributes, including seismic facies generated under various neural network procedures, to subdivide regional facies determined from logs into productive and non-productive subfacies, and we

  19. Calibration of Seismic Attributes for Reservoir Characterization

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

    Wayne D. Pennington

    2002-09-29

    The project, "Calibration of Seismic Attributes for Reservoir Characterization," is now complete. Our original proposed scope of work included detailed analysis of seismic and other data from two to three hydrocarbon fields; we have analyzed data from four fields at this level of detail, two additional fields with less detail, and one other 2D seismic line used for experimentation. We also included time-lapse seismic data with ocean-bottom cable recordings in addition to the originally proposed static field data. A large number of publications and presentations have resulted from this work, inlcuding several that are in final stages of preparation ormore » printing; one of these is a chapter on "Reservoir Geophysics" for the new Petroleum Engineering Handbook from the Society of Petroleum Engineers. Major results from this project include a new approach to evaluating seismic attributes in time-lapse monitoring studies, evaluation of pitfalls in the use of point-based measurements and facies classifications, novel applications of inversion results, improved methods of tying seismic data to the wellbore, and a comparison of methods used to detect pressure compartments. Some of the data sets used are in the public domain, allowing other investigators to test our techniques or to improve upon them using the same data. From the public-domain Stratton data set we have demonstrated that an apparent correlation between attributes derived along 'phantom' horizons are artifacts of isopach changes; only if the interpreter understands that the interpretation is based on this correlation with bed thickening or thinning, can reliable interpretations of channel horizons and facies be made. From the public-domain Boonsville data set we developed techniques to use conventional seismic attributes, including seismic facies generated under various neural network procedures, to subdivide regional facies determined from logs into productive and non-productive subfacies, and we

  20. Regional seismic lines reprocessed using post-stack processing techniques; National Petroleum Reserve, Alaska

    USGS Publications Warehouse

    Miller, John J.; Agena, W.F.; Lee, M.W.; Zihlman, F.N.; Grow, J.A.; Taylor, D.J.; Killgore, Michele; Oliver, H.L.

    2000-01-01

    This CD-ROM contains stacked, migrated, 2-Dimensional seismic reflection data and associated support information for 22 regional seismic lines (3,470 line-miles) recorded in the National Petroleum Reserve ? Alaska (NPRA) from 1974 through 1981. Together, these lines constitute about one-quarter of the seismic data collected as part of the Federal Government?s program to evaluate the petroleum potential of the Reserve. The regional lines, which form a grid covering the entire NPRA, were created by combining various individual lines recorded in different years using different recording parameters. These data were reprocessed by the USGS using modern, post-stack processing techniques, to create a data set suitable for interpretation on interactive seismic interpretation computer workstations. Reprocessing was done in support of ongoing petroleum resource studies by the USGS Energy Program. The CD-ROM contains the following files: 1) 22 files containing the digital seismic data in standard, SEG-Y format; 2) 1 file containing navigation data for the 22 lines in standard SEG-P1 format; 3) 22 small scale graphic images of each seismic line in Adobe Acrobat? PDF format; 4) a graphic image of the location map, generated from the navigation file, with hyperlinks to the graphic images of the seismic lines; 5) an ASCII text file with cross-reference information for relating the sequential trace numbers on each regional line to the line number and shotpoint number of the original component lines; and 6) an explanation of the processing used to create the final seismic sections (this document). The SEG-Y format seismic files and SEG-P1 format navigation file contain all the information necessary for loading the data onto a seismic interpretation workstation.

  1. Seismic data interpretation for hydrocarbon potential, for Safwa/Sabbar field, East Ghazalat onshore area, Abu Gharadig basin, Western Desert, Egypt

    NASA Astrophysics Data System (ADS)

    Hameed El Redini, Naser A.; Ali Bakr, Ali M.; Dahroug, Said M.

    2017-12-01

    Safwa/Sabbar oil field located in the East Ghazalat Concession in the proven and prolific Abu Gharadig basin, Western Desert, Egypt, and about 250 km to the southwest of Cairo, it's located in the vicinity of several producing oil fields ranging from small to large size hydrocarbon accumulation, adjacent to the NW-SE trending major Abu Gharadig fault which is throwing to the Southwest. All the geological, "structure and stratigraphic" elements, have been identified after interpreting the recent high quality 3D seismic survey for prospect generation, evaluation and their relation to the hydrocarbon exploration. Synthetic seismograms have been carried out for all available wells to tie horizons to seismic data and to define the lateral variation characters of the beds. The analysis has been done using the suitable seismic attributes to understand the characteristics of different types of the reservoir formations, type of trap system, identify channels and faults, and delineating the stratigraphic plays of good reservoirs such as Eocene Apollonia Limestone, AR "F", AR "G" members, Upper Bahariya, Jurassic Khatatba Sandstone, upper Safa and Lower Safa Sandstone. The top Cenomanian Bahariya level is the main oil reservoir in the Study area, which consist of Sandstone, Siltstone and Shale, the thickness is varying from 1 to 50 ft along the study area. In addition to Upper-Bahariya there are a good accessibility of hydrocarbon potential within the Jurassic Khatatba Sandstone and the Eocene Apollonia Limestone. More exploring of these reservoirs are important to increase productivity of Oil and/or Gas in the study area.

  2. A seismic reflection velocity study of a Mississippian mud-mound in the Illinois basin

    NASA Astrophysics Data System (ADS)

    Ranaweera, Chamila Kumari

    Two mud-mounds have been reported in the Ullin limestone near, but not in, the Aden oil field in Hamilton County, Illinois. One mud-mound is in the Broughton oil field of Hamilton County 25 miles to the south of Aden. The second mud-mound is in the Johnsonville oil field in Wayne County 20 miles to the north of Aden. Seismic reflection profiles were shot in 2012 adjacent to the Aden oil field to evaluate the oil prospects and to investigate the possibility of detecting Mississippian mud-mounds near the Aden field. A feature on one of the seismic profiles was interpreted to be a mud-mound or carbonate buildup. A well drilled at the location of this interpreted structure provided digital geophysical logs and geological logs used to refine the interpretation of the seismic profiles. Geological data from the new well at Aden, in the form of drill cuttings, have been used to essentially confirm the existence of a mud-mound in the Ullin limestone at a depth of 4300 feet. Geophysical well logs from the new well near Aden were used to create 1-D computer models and synthetic seismograms for comparison to the seismic data. The reflection seismic method is widely used to aid interpreting subsurface geology. Processing seismic data is an important step in the method as a properly processed seismic section can give a better image of the subsurface geology whereas a poorly processed section could mislead the interpretation. Seismic reflections will be more accurately depicted with careful determination of seismic velocities and by carefully choosing the processing steps and parameters. Various data processing steps have been applied and parameters refined to produce improved stacked seismic records. The resulting seismic records from the Aden field area indicate a seismic response similar to what is expected from a carbonate mud-mound. One-dimensional synthetic seismograms were created using the available sonic and density logs from the well drilled near the Aden seismic lines

  3. Seismicity in Azerbaijan and Adjacent Caspian Sea

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

    Panahi, Behrouz M.

    2006-03-23

    So far no general view on the geodynamic evolution of the Black Sea to the Caspian Sea region is elaborated. This is associated with the geological and structural complexities of the region revealed by geophysical, geochemical, petrologic, structural, and other studies. A clash of opinions on geodynamic conditions of the Caucasus region, sometimes mutually exclusive, can be explained by a simplified interpretation of the seismic data. In this paper I analyze available data on earthquake occurrences in Azerbaijan and the adjacent Caspian Sea region. The results of the analysis of macroseismic and instrumental data, seismic regime, and earthquake reoccurrence indicatemore » that a level of seismicity in the region is moderate, and seismic event are concentrated in the shallow part of the lithosphere. Seismicity is mostly intra-plate, and spatial distribution of earthquake epicenters does not correlate with the plate boundaries.« less

  4. Reflection imaging of the Moon's interior using deep-moonquake seismic interferometry

    NASA Astrophysics Data System (ADS)

    Nishitsuji, Yohei; Rowe, C. A.; Wapenaar, Kees; Draganov, Deyan

    2016-04-01

    The internal structure of the Moon has been investigated over many years using a variety of seismic methods, such as travel time analysis, receiver functions, and tomography. Here we propose to apply body-wave seismic interferometry to deep moonquakes in order to retrieve zero-offset reflection responses (and thus images) beneath the Apollo stations on the nearside of the Moon from virtual sources colocated with the stations. This method is called deep-moonquake seismic interferometry (DMSI). Our results show a laterally coherent acoustic boundary around 50 km depth beneath all four Apollo stations. We interpret this boundary as the lunar seismic Moho. This depth agrees with Japan Aerospace Exploration Agency's (JAXA) SELenological and Engineering Explorer (SELENE) result and previous travel time analysis at the Apollo 12/14 sites. The deeper part of the image we obtain from DMSI shows laterally incoherent structures. Such lateral inhomogeneity we interpret as representing a zone characterized by strong scattering and constant apparent seismic velocity at our resolution scale (0.2-2.0 Hz).

  5. Tomography & Geochemistry: Precision, Repeatability, Accuracy and Joint Interpretations

    NASA Astrophysics Data System (ADS)

    Foulger, G. R.; Panza, G. F.; Artemieva, I. M.; Bastow, I. D.; Cammarano, F.; Doglioni, C.; Evans, J. R.; Hamilton, W. B.; Julian, B. R.; Lustrino, M.; Thybo, H.; Yanovskaya, T. B.

    2015-12-01

    Seismic tomography can reveal the spatial seismic structure of the mantle, but has little ability to constrain composition, phase or temperature. In contrast, petrology and geochemistry can give insights into mantle composition, but have severely limited spatial control on magma sources. For these reasons, results from these three disciplines are often interpreted jointly. Nevertheless, the limitations of each method are often underestimated, and underlying assumptions de-emphasized. Examples of the limitations of seismic tomography include its ability to image in detail the three-dimensional structure of the mantle or to determine with certainty the strengths of anomalies. Despite this, published seismic anomaly strengths are often unjustifiably translated directly into physical parameters. Tomography yields seismological parameters such as wave speed and attenuation, not geological or thermal parameters. Much of the mantle is poorly sampled by seismic waves, and resolution- and error-assessment methods do not express the true uncertainties. These and other problems have become highlighted in recent years as a result of multiple tomography experiments performed by different research groups, in areas of particular interest e.g., Yellowstone. The repeatability of the results is often poorer than the calculated resolutions. The ability of geochemistry and petrology to identify magma sources and locations is typically overestimated. These methods have little ability to determine source depths. Models that assign geochemical signatures to specific layers in the mantle, including the transition zone, the lower mantle, and the core-mantle boundary, are based on speculative models that cannot be verified and for which viable, less-astonishing alternatives are available. Our knowledge is poor of the size, distribution and location of protoliths, and of metasomatism of magma sources, the nature of the partial-melting and melt-extraction process, the mixing of disparate

  6. Interpretation of reflection seismic data acquired for Knight Hawk Coal, LLC.

    DOT National Transportation Integrated Search

    2011-10-01

    The Missouri University of Science and Technology geophysical crew acquired approximately 3000 lineal feet of reflection seismic : data along five separate traverses (1-5) at the PEUG South mine site. The objective was to determine if any of the trav...

  7. Seismic modeling of complex stratified reservoirs

    NASA Astrophysics Data System (ADS)

    Lai, Hung-Liang

    Turbidite reservoirs in deep-water depositional systems, such as the oil fields in the offshore Gulf of Mexico and North Sea, are becoming an important exploration target in the petroleum industry. Accurate seismic reservoir characterization, however, is complicated by the heterogeneous of the sand and shale distribution and also by the lack of resolution when imaging thin channel deposits. Amplitude variation with offset (AVO) is a very important technique that is widely applied to locate hydrocarbons. Inaccurate estimates of seismic reflection amplitudes may result in misleading interpretations because of these problems in application to turbidite reservoirs. Therefore, an efficient, accurate, and robust method of modeling seismic responses for such complex reservoirs is crucial and necessary to reduce exploration risk. A fast and accurate approach generating synthetic seismograms for such reservoir models combines wavefront construction ray tracing with composite reflection coefficients in a hybrid modeling algorithm. The wavefront construction approach is a modern, fast implementation of ray tracing that I have extended to model quasi-shear wave propagation in anisotropic media. Composite reflection coefficients, which are computed using propagator matrix methods, provide the exact seismic reflection amplitude for a stratified reservoir model. This is a distinct improvement over conventional AVO analysis based on a model with only two homogeneous half spaces. I combine the two methods to compute synthetic seismograms for test models of turbidite reservoirs in the Ursa field, Gulf of Mexico, validating the new results against exact calculations using the discrete wavenumber method. The new method, however, can also be used to generate synthetic seismograms for the laterally heterogeneous, complex stratified reservoir models. The results show important frequency dependence that may be useful for exploration. Because turbidite channel systems often display complex

  8. 2D Seismic Reflection Data across Central Illinois

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

    Smith, Valerie; Leetaru, Hannes

    In a continuing collaboration with the Midwest Geologic Sequestration Consortium (MGSC) on the Evaluation of the Carbon Sequestration Potential of the Cambro-Ordovician Strata of the Illinois and Michigan Basins project, Schlumberger Carbon Services and WesternGeco acquired two-dimensional (2D) seismic data in the Illinois Basin. This work included the design, acquisition and processing of approximately 125 miles of (2D) seismic reflection surveys running west to east in the central Illinois Basin. Schlumberger Carbon Services and WesternGeco oversaw the management of the field operations (including a pre-shoot planning, mobilization, acquisition and de-mobilization of the field personnel and equipment), procurement of the necessarymore » permits to conduct the survey, post-shoot closure, processing of the raw data, and provided expert consultation as needed in the interpretation of the delivered product. Three 2D seismic lines were acquired across central Illinois during November and December 2010 and January 2011. Traversing the Illinois Basin, this 2D seismic survey was designed to image the stratigraphy of the Cambro-Ordovician sections and also to discern the basement topography. Prior to this survey, there were no regionally extensive 2D seismic data spanning this section of the Illinois Basin. Between the NW side of Morgan County and northwestern border of Douglas County, these seismic lines ran through very rural portions of the state. Starting in Morgan County, Line 101 was the longest at 93 miles in length and ended NE of Decatur, Illinois. Line 501 ran W-E from the Illinois Basin – Decatur Project (IBDP) site to northwestern Douglas County and was 25 miles in length. Line 601 was the shortest and ran N-S past the IBDP site and connected lines 101 and 501. All three lines are correlated to well logs at the IBDP site. Originally processed in 2011, the 2D seismic profiles exhibited a degradation of signal quality below ~400 millisecond (ms) which made

  9. On vertical seismic profile processing

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

    Tariel, P.; Michon, D.

    1984-10-01

    From the wealth of information which can be deduced from VSP, the information most directly comparable to well logs is considered: P-wave and S-wave interval velocity, acoustic impedance, and the velocity ratio ..gamma.. = V /SUB s/ /V /SUB p/ . This information not only allows better interpretation of surface seismic sections but also improves processing. For these results to be usable a number of precautions must be taken during acquisition and processing; the sampling in depth should be chosen in such a way that aliasing phenomena do not unnecessarily limit the spectra during the separation of upwards and downwardsmore » travelling waves. True amplitudes should be respected and checked by recording of signatures, and the interference of upwards and downwards travelling waves should be taken into account for the picking of first arrivals. The different steps in processing and the combination of results in the interpretation of surface seismic results are described with actual records.« less

  10. Reprocessing and Interpretation of Vintage Seismic Reflection Data: Evidence for the Tectonic History of the Rocky Mountain Trench, Northwest Montana.

    NASA Astrophysics Data System (ADS)

    Porter, M.; Speece, M. A.; Rutherford, B. S.; Constenius, K. N.

    2014-12-01

    In 1983 Techno, Inc. collected five seismic reflection profiles in the region between Whitefish, Montana and the United States-Canada border. The poulter method was used to gather four of these profiles and one profile was collected using a vibroseis source. We are currently reprocessing these data in order to construct a regional geological interpretation. The profiles cover a key position in the hinterland of the Cordillera in the lee of the Lewis thrust salient where the east-northeast verging Lewis thrust fault system translated (horizontal displacement >100 km) and inverted a thick, strong slab of primarily Belt-Purcell rocks out of a deep Precambrian depositional basin onto a cratonic platform. In this event, Belt-Purcell rocks were thrust over complexly imbricated Phanerozoic strata in the foreland. Late Mesozoic compressional deformation was followed by Cenozoic extensional collapse of the over-thickened Cordillera and subsequent basin and range style deformation that produced an array of northwest trending grabens. Three of the seismic profiles cross the Rocky Mountain Trench; the Trench is a linear structure of regional dimension that is an expression of the extensional fragmentation of the Cordillera. Strong reflections, interpreted as sills encased within Lower Belt rocks (encountered in the Arco-Marathon 1 Paul Gibbs borehole), outline the complexly folded and faulted structure of the eastern limb of the Purcell anticlinorium. East of the Rocky Mountain Trench stratified reflections within Belt rocks clearly outline the Wigwam Thrust. Beneath the Whitefish Range, an apparent inflection in the strongly reflective basal Cambrian veneer marks the westerly increase in dip of the Rocky Mountain Basal Detachment. The dip contrast between the foreland and hinterland might be a manifestation of the tectonic loading of the Belt basin margin and the loading might have localized extension across the Rocky Mountain Trench.

  11. Seismic moment tensor for anisotropic media: implication for Non-double-couple earthquakes

    NASA Astrophysics Data System (ADS)

    Cai, X.; Chen, X.; Chen, Y.; Cai, M.

    2008-12-01

    It is often found that the inversion results of seismic moment tensor from real seismic recorded data show the trace of seismic moment tensor M is not zero, a phenomenon called non-double-couple earthquake sources mechanism. Recently we have derived the analytical expressions of M in transversely isotropic media with the titled axis of symmetry and the results shows even only pure shear-motion of fault can lead to the implosive components determined by several combined anisotropic elastic constants. Many non-double-couple earthquakes from observations often appear in volcanic and geothermal areas (Julian, 1998), where there exist a mount of stress-aligned fluid-saturated parallel vertical micro-cracks identical to transversely isotropic media (Crampin, 2008), this stress-aligned crack will modify the seismic moment tensor. In another word, non-double-couple earthquakes don't mean to have a seismic failure movement perpendicular to the fault plane, while traditional research of seismic moment tensor focus on the case of isotropy, which cannot provide correct interpretation of seismic source mechanism. Reference: Julian, B.R., Miller, A.D. and Foulger, G.R., 1998. Non-double-couple earthquakes,1. Theory, Rev. Geophys., 36, 525¨C549. Crampin,S., Peacock,S., 2008, A review of the current understanding of seismic shear-wave splitting in the Earth's crust and common fallacies in interpretation, wave motion, 45,675-722

  12. A microseismic workflow for managing induced seismicity risk as CO 2 storage projects

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

    Matzel, E.; Morency, C.; Pyle, M.

    2015-10-27

    It is well established that fluid injection has the potential to induce earthquakes—from microseismicity to large, damaging events—by altering state-of-stress conditions in the subsurface. While induced seismicity has not been a major operational issue for carbon storage projects to date, a seismicity hazard exists and must be carefully addressed. Two essential components of effective seismic risk management are (1) sensitive microseismic monitoring and (2) robust data interpretation tools. This report describes a novel workflow, based on advanced processing algorithms applied to microseismic data, to help improve management of seismic risk. This workflow has three main goals: (1) to improve themore » resolution and reliability of passive seismic monitoring, (2) to extract additional, valuable information from continuous waveform data that is often ignored in standard processing, and (3) to minimize the turn-around time between data collection, interpretation, and decision-making. These three objectives can allow for a better-informed and rapid response to changing subsurface conditions.« less

  13. Poor boy 3D seismic effort yields South Central Kentucky discovery

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

    Hanratty, M.

    1996-11-04

    Clinton County, Ky., is on the eastern flank of the Cincinnati arch and the western edge of the Appalachian basin and the Pine Mountain overthrust. Clinton County has long been known for high volume fractured carbonate wells. The discovery of these fractured reservoir, unfortunately, has historically been serendipitous. The author currently uses 2D seismic and satellite imagery to design 3D high resolution seismic shoots. This method has proven to be the most efficient and is the core of his program. The paper describes exploration methods, seismic acquisition, well data base, and seismic interpretation.

  14. Mapping the megathrust beneath the northern Gulf of Alaska using wide-angle seismic reflection/refraction profiles

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

    Brocher, T.M.; Fuis, G.S.; Fisher, M.A.

    1993-04-01

    In the northern Gulf of Alaska and Prince William Sound, wide-angle seismic reflection/refraction profiling, earthquake studies, and laboratory measurements of physical properties are used to determine the geometry of the Prince William and Yakutat terranes, and the subducting Pacific plate. In this complex region, the Yakutat terrane is underthrust beneath the Prince William terrane, and both terranes are interpreted to be underlain by the Pacific plate. Wide-angle seismic reflection/refraction profiles recorded along 5 seismic lines are used to unravel this terrane geometry. Modeled velocities in the upper crust of the Prince William terrane (to 18-km depth) agree closely with laboratorymore » velocity measurements of Orca Group phyllites and quartzofeldspathic graywackes (the chief components of the Prince William terrane) to hydrostatic pressures as high as 600 MPa (6 KBAR). An interpretation consistent with these data extends the Prince William terrane to at least 18-km depth. A landward dipping reflection at depths of 16--24 km is interpreted as the base of the Prince William terrane. This reflector corresponds to the top of the Wadati-Benioff zone seismicity and is interpreted as the megathrust. Beneath this reflector is a 6.9-km/s refractor, that is strongly reflective and magnetic, and is interpreted to be gabbro in Eocene age oceanic crust of the underthrust Yakutat terrane. Both wide-angle seismic and magnetic anomaly data indicate that the Yakutat terrane has been underthrust beneath the Prince William terrane for at least a few hundred kilometers. Wide-angle seismic data are consistent with a 9 to 10[degree] landward dip of the subducting Pacific plate, distinctly different from the inferred average 3 to 4[degree] dip of the overlying 6.9-km/s refractor and Wadati-Benioff seismic zone. The preferred interpretation of the geophysical data is that one composite plate, composed of the Pacific and Yakutat plates, is subducting beneath southern Alaska.« less

  15. Fallon, Nevada FORGE Seismic Reflection Profiles

    DOE Data Explorer

    Blankenship, Doug; Faulds, James; Queen, John; Fortuna, Mark

    2018-02-01

    Newly reprocessed Naval Air Station Fallon (1994) seismic lines: pre-stack depth migrations, with interpretations to support the Fallon FORGE (Phase 2B) 3D Geologic model. Data along seven profiles (>100 km of total profile length) through and adjacent to the Fallon site were re-processed. The most up-to-date, industry-tested seismic processing techniques were utilized to improve the signal strength and coherency in the sedimentary, volcanic, and Mesozoic crystalline basement sections, in conjunction with fault diffractions in order to improve the identification and definition of faults within the study area.

  16. Interpretation of Late Cretaceous Volcanic Mounds and Surrounding Gulfian Series Formations Using 3D Seismic Data in Zavala County, Texas

    NASA Astrophysics Data System (ADS)

    Bennett, Laura Claire

    The Late Cretaceous Gulfian series is a prominent and important series across the State of Texas that has been extensively studied since the nineteenth century. It is composed of series of southeast-dipping shelf carbonates and clastics deposited on the northwest margin of the Gulf of Mexico Basin. In south Texas, the Gulfian series was deposited in the Rio Grande Embayment and Maverick Basin and is comprised of the Eagle Ford Group, Austin Group, Anacacho Limestone, San Miguel Formation, Olmos Formation, and Escondido Formation that crop out and continue basinward in the subsurface. Late Cretaceous volcanism formed volcanic mounds composed of altered palagonite tuff that are clustered into two fields, including the Uvalde Field centered in Zavala County. Using the Pedernales 3D seismic survey, located in east-central Zavala County, several volcanic mounds were identified and mapped without the use of well log data by identifying structures and characteristics associated with the volcanic mounds. Isolating these mounds through mapping enabled the mapping of the tops surrounding Gulfian formations, Lower Eagle Ford, Upper Eagle Ford, Austin, Anacacho, and San Miguel, for which time-structure, amplitude, similarity/coherency attribute, and isochron maps were generated. By using 3D seismic data, the volcanic mounds and their relation to surrounding rocks can be better interpreted.

  17. Concept Abstractness and the Representation of Noun-Noun Combinations

    ERIC Educational Resources Information Center

    Xu, Xu; Paulson, Lisa

    2013-01-01

    Research on noun-noun combinations has been largely focusing on concrete concepts. Three experiments examined the role of concept abstractness in the representation of noun-noun combinations. In Experiment 1, participants provided written interpretations for phrases constituted by nouns of varying degrees of abstractness. Interpretive focus (the…

  18. Seismic investigations in downtown Copenhagen, Denmark

    NASA Astrophysics Data System (ADS)

    Martinez, K.; Mendoza, J. A.; Olsen, H.

    2009-12-01

    Near surface geophysics are gaining widespread use in major infrastructure projects with respect to geotechnical and engineering applications. The development of data acquisition, processing tools and interpretation methods have optimized survey production, reduced logistics costs and increase results reliability of seismic surveys during the last decades. However, the use of geophysical methods under urban environments continues to face challenges due to multiple noise sources and obstacles inherent to cities. A seismic investigation was conducted in Copenhagen aiming to produce information needed for hydrological, geotechnical and groundwater modeling assessments related to the planned Cityringen underground metro project. The particular objectives were a) map variations in subsurface Quaternary and limestone properties b) to map for near surface structural features. The geological setting in the Copenhagen region is characterized by several interlaced layers of glacial till and meltwater sand deposits. These layers, which are found unevenly distributed throughout the city and present in varying thicknesses, overlie limestone of different generations. There are common occurrences of incised valley structures containing localized instances of weathered or fractured limestone. The surveys consisted of combined seismic reflection and refraction profiles accounting for approximately 13 km along sections of the projected metro line. The data acquisition was carried out using standard 192 channels arrays, receiver groups with 5 m spacing and a Vibroseis as a source at 5 m spacing. In order to improve the resolution of the data, 29 Walkaway-Vertical Seismic Profiles were performed at selected wells along the surface seismic lines. The refraction data was processed with travel-time tomography and the reflection data underwent standard interpretation. The refraction data inversion was performed twofold; a surface refraction alone and combined with the VSP data. Three

  19. Imaging the Crust in the Northern Sector of the 2009 L'Aquila Seismic Sequence through Oil Exploration Data Interpretation

    NASA Astrophysics Data System (ADS)

    Grazia Ciaccio, Maria; Improta, Luigi; Patacca, Etta; Scandone, Paolo; Villani, Fabio

    2010-05-01

    The 2009 L'Aquila seismic sequence activated a complex, about 40 km long, NW-trending and SW-dipping normal fault system, consisting of three main faults arranged in right-lateral en-echelon geometry. While the northern sector of the epicentral area was extensively investigated by oil companies, only a few scattered, poor-quality commercial seismic profiles are available in the central and southern sector. In this study we interpret subsurface commercial data from the northern sector, which is the area where is located the source of the strong Mw5.4 aftershock occurred on the 9th April 2009. Our primary goals are: (1) to define a reliable framework of the upper crust structure, (2) to investigate how the intense aftershock activity, the bulk of which is clustered in the 5-10 km depth range, relates to the Quaternary extensional faults present in the area. The investigated area lies between the western termination of the W-E trending Gran Sasso thrust system to the south, the SW-NE trending Mt. Sibillini thrust front (Ancona-Anzio Line Auctt.) to the north and west, and by the NNW-SSE trending, SW-dipping Mt. Gorzano normal fault to the east. In this area only middle-upper Miocene deposits are exposed (Laga Flysch and underlying Cerrogna Marl), but commercial wells have revealed the presence of a Triassic-Miocene sedimentary succession identical to the well known Umbria-Marche stratigraphic sequence. We have analyzed several confidential seismic reflection profiles, mostly provided by ENI oil company. Seismic lines are tied to two public wells, 5766 m and 2541 m deep. Quality of the reflection imaging is highly variable. A few good quality stack sections contain interpretable signal down to 4.5-5.5 s TWT, corresponding to depths exceeding 10-12 km and thus allowing crustal imaging at seismogenic depths. Key-reflectors for the interpretation correspond to: (1) the top of the Miocene Cerrogna marls, (2) the top of the Upper Albian-Oligocene Scaglia Group, (3) the

  20. Incorporating Cutting Edge Scientific Results from the Margins-Geoprisms Program into the Undergraduate Curriculum, Rupturing Continental Lithosphere Part I: Introducing Seismic Interpretation and Isostasy Principles Using Gulf of California Examples

    NASA Astrophysics Data System (ADS)

    Lamb, M. A.; Cashman, S. M.; Dorsey, R. J.; Bennett, S. E. K.; Loveless, J. P.; Goodliffe, A. M.

    2014-12-01

    The NSF-MARGINS Program funded a decade of research on continental margin processes. The NSF-GeoPRISMS Mini-lesson Project, funded by NSF-TUES, is designed to integrate the significant findings from the MARGINS program into open-source college-level curriculum. The Gulf of California (GOC) served as the focus site for the Rupturing Continental Lithosphere initiative, which addressed several scientific questions: What forces drive rift initiation, localization, propagation and evolution? How does deformation vary in time and space, and why? How does crust evolve, physically and chemically, as rifting proceeds to sea-floor spreading? What is the role of sedimentation and magmatism in continental extension? We developed two weeks of curriculum designed for an upper-division structural geology, tectonics or geophysics course. The curriculum includes lectures, labs, and in-class activities that can be used as a whole or individually. The first set of materials introduces the RCL initiative to students and has them analyze the bathymetry and oblique-rifting geometry of the GOC in an exercise using GeoMapApp. The second set of materials has two goals: (1) introduce students to fundamental concepts of interpreting seismic reflection data via lectures and in-class interpretation of strata, basement, and faults from recent GOC seismic data, and (2) encourage students to discover the structural geometry and rift evolution, including the east-to-west progression of faulting and transition from detachment to high-angle faulting in the northern GOC, and changes in deformation style from north to south. In the third set of materials, students investigate isostatic affects of sediment fill in GOC oblique rift basins. This activity consists of a problem set, introduced in a lecture, where students integrate their findings from the previous bathymetry- and seismic-interpretation exercises.

  1. Seismic Imaging and Characterization of Bright Spots in the West Bohemia Seismic Zone (Germany and Czech Republic)

    NASA Astrophysics Data System (ADS)

    Alexandrakis, C.; Schreiter, L.; Hlousek, F.; Jusri, T.; Buske, S.

    2017-12-01

    In crystalline environments, imaging faults, layer boundaries and small scale structures is challenging due to the complex geometry of the structures themselves and the influence of the hardrock environment on the seismic wavefield. Optimally designed active seismic surveys and careful processing can produce a clear image of the subsurface structures. However, if little is known about the local geology and tectonic state of the area, the imaged reflections can be difficult to interpret. This is the case in the West Bohemia Seismic Zone, located along the border of Germany and Czech Republic. This geodynamically active area is spotted with springs and gas vents, and frequently experiences low magnitude seismic swarms. The most active region is located in the Cheb basin and coincides with the junction of a northwest trending fault with a north-south trending shear zone, making for a structurally complex hardrock setting. In the early 1990s, two long-offset reflection seismic profiles were collected along the boundary of the Cheb basin: MVE-90 along the northern edge, and 9HR-91 in the east. These profiles were recently reprocessed using Kirchhoff PreStack Depth Migration, revealing high amplitude reflections, or bright spots, that correlate to nearby seismicity. Several studies have hypothesized that the 9HR-91 bright spots image a fluid trap, where mantle-sourced fluids accumulate, thereby facilitating slip on the faults and triggering the swarms. However, the exact nature of the bright spots remains an open question. They may be a change in lithology and/or porosity, an infilled vein or an impermeable fault. We aim to answer this question by first using Coherency-Based PreStack Depth Migration to produce detailed images of the bright spots. We then forward model the waveforms guided by the reflection coefficients in order to derive rock-physical parameters. Finally, the best-fitting models are interpreted in terms of their possible relationship to the West Bohemia

  2. Seismic Readings from the Deepest Borehole in the New Madrid Seismic Zone

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

    Woolery, Edward W; Wang, Zhenming; Sturchio, Neil C

    2006-03-01

    Since the 1980s, the research associated with the UK network has been primarily strong-motion seismology of engineering interest. Currently the University of Kentucky operates a strong-motion network of nine stations in the New Madrid Seismic Zone. A unique feature of the network is the inclusions of vertical strong-motion arrays, each with one or two downhole accelerometers. The deepest borehole array is 260 m below the surfaces at station VASA in Fulton County, Kentucky. A preliminary surface seismic refraction survey was conducted at the site before drilling the hole at VSAS (Woolery and Wang, 2002). The depth to the Paleozoic bedrockmore » at the site was estimated to be approximately 595 m, and the depth to the first very stiff layer (i.e. Porters Creek Clay) was found to be about 260 m. These depths and stratigraphic interpretation correlated well with a proprietary seismic reflection line and the Ken-Ten Oil Exploration No. 1 Sanger hole (Schwalb, 1969), as well as our experience in the area (Street et al., 1995; Woolery et al., 1999).« less

  3. Calibration of Seismic Attributes for Reservoir Characterization

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

    Pennington, Wayne D.; Acevedo, Horacio; Green, Aaron

    2002-01-29

    This project has completed the initially scheduled third year of the contract, and is beginning a fourth year, designed to expand upon the tech transfer aspects of the project. From the Stratton data set, demonstrated that an apparent correlation between attributes derived along `phantom' horizons are artifacts of isopach changes; only if the interpreter understands that the interpretation is based on this correlation with bed thickening or thinning, can reliable interpretations of channel horizons and facies be made. From the Boonsville data set , developed techniques to use conventional seismic attributes, including seismic facies generated under various neural network procedures,more » to subdivide regional facies determined from logs into productive and non-productive subfacies, and developed a method involving cross-correlation of seismic waveforms to provide a reliable map of the various facies present in the area. The Teal South data set provided a surprising set of data, leading us to develop a pressure-dependent velocity relationship and to conclude that nearby reservoirs are undergoing a pressure drop in response to the production of the main reservoir, implying that oil is being lost through their spill points, never to be produced. The Wamsutter data set led to the use of unconventional attributes including lateral incoherence and horizon-dependent impedance variations to indicate regions of former sand bars and current high pressure, respectively, and to evaluation of various upscaling routines.« less

  4. Using 3D visualization and seismic attributes to improve structural and stratigraphic resolution of reservoirs

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

    Kerr, J.; Jones, G.L.

    1996-01-01

    Recent advances in hardware and software have given the interpreter and engineer new ways to view 3D seismic data and well bore information. Recent papers have also highlighted the use of various statistics and seismic attributes. By combining new 3D rendering technologies with recent trends in seismic analysis, the interpreter can improve the structural and stratigraphic resolution of hydrocarbon reservoirs. This paper gives several examples using 3D visualization to better define both the structural and stratigraphic aspects of several different structural types from around the world. Statistics, 3D visualization techniques and rapid animation are used to show complex faulting andmore » detailed channel systems. These systems would be difficult to map using either 2D or 3D data with conventional interpretation techniques.« less

  5. Using 3D visualization and seismic attributes to improve structural and stratigraphic resolution of reservoirs

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

    Kerr, J.; Jones, G.L.

    1996-12-31

    Recent advances in hardware and software have given the interpreter and engineer new ways to view 3D seismic data and well bore information. Recent papers have also highlighted the use of various statistics and seismic attributes. By combining new 3D rendering technologies with recent trends in seismic analysis, the interpreter can improve the structural and stratigraphic resolution of hydrocarbon reservoirs. This paper gives several examples using 3D visualization to better define both the structural and stratigraphic aspects of several different structural types from around the world. Statistics, 3D visualization techniques and rapid animation are used to show complex faulting andmore » detailed channel systems. These systems would be difficult to map using either 2D or 3D data with conventional interpretation techniques.« less

  6. Analysis of some seismic expressions of Big Injun sandstone and its adjacent interval

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

    Xiangdong, Zou; Wilson, T.A.; Donaldson, A.C.

    1991-08-01

    The Big Injun sandstone is an important oil and gas reservoir in western West Virginia. The pre-Greenbrier unconformity has complicated correlations, and hydrocarbon explorationists commonly have misidentified the Big Injun in the absence of a regional stratigraphic study. Paleogeologic maps on this unconformity show the West Virginia dome, with the Price/Pocono units truncated resulting in pinch-outs of different sandstones against the overlying Big Lime (Greenbrier Limestone). Drillers have named the first sandstone below the Big Lime as Big Injun, and miscorrelated the real Big Injun with Squaw, upper Weir, and even the Berea sandstone. In this report, an 8-mi (13-km)more » seismic section extending from Kanawha to Clay counties was interpreted. The study area is near the pinch-out of the Big Injun sandstone. A stratigraphic cross section was constructed from gamma-ray logs for comparison with the seismic interpretation. The modeling and interpretation of the seismic section recognized the relief on the unconformity and the ability to determine facies changes, too. Both geophysical wireline and seismic data can be used for detailed stratigraphic analysis within the Granny Creek oil field of Clay and Roane countries.« less

  7. Seismic Response of the Greenland Ice-sheet over Several Melt Seasons near Draining Supraglacial Lakes

    NASA Astrophysics Data System (ADS)

    Carmichael, J. D.; Joughin, I. R.; Behn, M. D.; Das, S. B.; Lizarralde, D.

    2012-12-01

    We present seismic observations assembled from 3+ years of melt season measurements collected near seasonally-draining supraglacial lakes on the Greenland Ice-sheet (68.7311,-49.5925). On transient time scales (< 1 day), these data include a record of seismic response coincident with at least three documented lake drainage events. During a particular event, drainage is preceded by two hours of impulsive high-energy seismic signals, followed by the onset of continuous broadband signals (2-50Hz) that we interpret as surface-to-bed meltwater transfer. This drainage is followed additional transient icequakes similar in timing and energy to the precursory activity. Over a seasonal time scale (> 1 month), our data records a transition in seismicity between two distinct modes, with one mode characterized by relative quiescence, and the other mode characterized by uniform energy that is observed network-wide as a continuous, repetitive signal. The transition between modes is abrupt (~ 2 hours) and is observed using multiple seismic discriminants. We interpret this rapid transition as reflecting the evolution of the morphology of a basal drainage system as it responds to melt input. This interpretation is tested against additional geophysical observations that include temperature-based melt models, satellite imagery, and GPS measurements. Finally, we outline and advocate a routine for monitoring icesheet seismicity with a focus on distinguishing surface from basal sources.

  8. Combining mineral physics with seismic observations: What can we deduce about the thermochemical structure of the Earth's deep interior?

    NASA Astrophysics Data System (ADS)

    Cobden, L. J.

    2017-12-01

    Mineral physics provides the essential link between seismic observations of the Earth's interior, and laboratory (or computer-simulated) measurements of rock properties. In this presentation I will outline the procedure for quantitative conversion from thermochemical structure to seismic structure (and vice versa) using the latest datasets from seismology and mineralogy. I will show examples of how this method can allow us to infer major chemical and dynamic properties of the deep mantle. I will also indicate where uncertainties and limitations in the data require us to exercise caution, in order not to "over-interpret" seismic observations. Understanding and modelling these uncertainties serves as a useful guide for mineralogists to ascertain which mineral parameters are most useful in seismic interpretation, and enables seismologists to optimise their data assembly and inversions for quantitative interpretations.

  9. 1D Seismic reflection technique to increase depth information in surface seismic investigations

    NASA Astrophysics Data System (ADS)

    Camilletti, Stefano; Fiera, Francesco; Umberto Pacini, Lando; Perini, Massimiliano; Prosperi, Andrea

    2017-04-01

    1D seismic methods, such as MASW Re.Mi. and HVSR, have been extensively used in engineering investigations, bedrock research, Vs profile and to some extent for hydrologic applications, during the past 20 years. Recent advances in equipment, sound sources and computer interpretation techniques, make 1D seismic methods highly effective in shallow subsoil modeling. Classical 1D seismic surveys allows economical collection of subsurface data however they fail to return accurate information for depths greater than 50 meters. Using a particular acquisition technique it is possible to collect data that can be quickly processed through reflection technique in order to obtain more accurate velocity information in depth. Furthermore, data processing returns a narrow stratigraphic section, alongside the 1D velocity model, where lithological boundaries are represented. This work will show how collect a single-CMP to determine: (1) depth of bedrock; (2) gravel layers in clayey domains; (3) accurate Vs profile. Seismic traces was processed by means a new software developed in collaboration with SARA electronics instruments S.r.l company, Perugia - ITALY. This software has the great advantage of being able to be used directly in the field in order to reduce the times elapsing between acquisition and processing.

  10. Interferometric Seismic Sources on the Core Mantle Boundary Revealed by Seismic Coda Crosscorrelation

    NASA Astrophysics Data System (ADS)

    Pham, T. S.; Tkalcic, H.; Sambridge, M.

    2017-12-01

    The crosscorrelation of earthquake coda can be used to extract seismic body waves which are sensitive to deep Earth interior. The retrieved peaks in crosscorrelation of two seismic records are commonly interpreted as seismic phases that originate at a point source collocated with the first recorder (Huygens-Fresnel principle), reflected upward from prominent underground reflectors and reaching the second recorder. From the time shift of these peaks measured at different interstation distances, new travel time curves can be constructed. This study focuses on a previously unexplained interferometric phase (named temporarily a ghost or "G phase") observed in crosscorrelogram stack sections utilizing seismic coda. In particular, we deploy waveforms recorded by two regional seismic networks, one in Australia and another in Alaska. We show that the G phase cannot be explained by as a reflection. Moreover, we demonstrate that the G phase is explained through the principle of energy partitioning, and specifically, conversions from compressional to shear motions at the core-mantle boundary (CMB). This can be thought of in terms of a continuous distribution of Huygens sources across the CMB that are "activated" in long-range wavefield coda following significant earthquakes. The newly explained phase is renamed to cPS, to indicate a CMB origin and the P to S conversion. This mechanism explains a range of newly observed global interferometric phases that can be used in combination with existing phases to constrain Earth structure.

  11. Insights into crustal structure of the Eastern North American Margin from community multichannel seismic and potential field data

    NASA Astrophysics Data System (ADS)

    Davis, J. K.; Becel, A.; Shillington, D. J.; Buck, W. R.

    2017-12-01

    In the fall of 2014, the R/V Marcus Langseth collected gravity, magnetic, and reflection seismic data as part of the Eastern North American Margin Community Seismic Experiment. The dataset covers a 500 km wide section of the Mid-Atlantic passive margin offshore North Carolina, which formed after the Mesozoic breakup of the supercontinent Pangaea. Using these seismic and potential field data, we present observations and interpretations along two cross margin and one along-margin profiles. Analyses and interpretations are conducted using pre-stack depth migrated reflection seismic profiles in conjunction with forward modeling of shipboard gravity and magnetic anomalies. Preliminary interpretations of the data reveal variations in basement character and structure across the entire transition between continental and oceanic domains. These interpretations help provide insight into the origin and nature of the prominent East Coast and Blake Spur magnetic anomalies, as well as the Inner Magnetic Quiet Zone which occupies the domain between the anomalies. Collectively, these observations can aid in deciphering the rift-to-drift transition during the breakup of North America and West Africa and formation of the Central Atlantic.

  12. Seismic Search Engine: A distributed database for mining large scale seismic data

    NASA Astrophysics Data System (ADS)

    Liu, Y.; Vaidya, S.; Kuzma, H. A.

    2009-12-01

    The International Monitoring System (IMS) of the CTBTO collects terabytes worth of seismic measurements from many receiver stations situated around the earth with the goal of detecting underground nuclear testing events and distinguishing them from other benign, but more common events such as earthquakes and mine blasts. The International Data Center (IDC) processes and analyzes these measurements, as they are collected by the IMS, to summarize event detections in daily bulletins. Thereafter, the data measurements are archived into a large format database. Our proposed Seismic Search Engine (SSE) will facilitate a framework for data exploration of the seismic database as well as the development of seismic data mining algorithms. Analogous to GenBank, the annotated genetic sequence database maintained by NIH, through SSE, we intend to provide public access to seismic data and a set of processing and analysis tools, along with community-generated annotations and statistical models to help interpret the data. SSE will implement queries as user-defined functions composed from standard tools and models. Each query is compiled and executed over the database internally before reporting results back to the user. Since queries are expressed with standard tools and models, users can easily reproduce published results within this framework for peer-review and making metric comparisons. As an illustration, an example query is “what are the best receiver stations in East Asia for detecting events in the Middle East?” Evaluating this query involves listing all receiver stations in East Asia, characterizing known seismic events in that region, and constructing a profile for each receiver station to determine how effective its measurements are at predicting each event. The results of this query can be used to help prioritize how data is collected, identify defective instruments, and guide future sensor placements.

  13. A new moonquake catalog from Apollo 17 seismic data I: Lunar Seismic Profiling Experiment: Thermal moonquakes and implications for surface processes

    NASA Astrophysics Data System (ADS)

    Weber, R. C.; Dimech, J. L.; Phillips, D.; Molaro, J.; Schmerr, N. C.

    2017-12-01

    Apollo 17's Lunar Seismic Profiling Experiment's (LSPE) primary objective was to constrain the near-surface velocity structure at the landing site using active sources detected by a 100 m-wide triangular geophone array. The experiment was later operated in "listening mode," and early studies of these data revealed the presence of thermal moonquakes - short-duration seismic events associated with terminator crossings. However, the full data set has never been systematically analyzed for natural seismic signal content. In this study, we analyze 8 months of continuous LSPE data using an automated event detection technique that has previously successfully been applied to the Apollo 16 Passive Seismic Experiment data. We detected 50,000 thermal moonquakes from three distinct event templates, representing impulsive, intermediate, and emergent onset of seismic energy, which we interpret as reflecting their relative distance from the array. Impulsive events occur largely at sunrise, possibly representing the thermal "pinging" of the nearby lunar lander, while emergent events occur at sunset, possibly representing cracking or slumping in more distant surface rocks and regolith. Preliminary application of an iterative event location algorithm to a subset of the impulsive waveforms supports this interpretation. We also perform 3D modeling of the lunar surface to explore the relative contribution of the lander, known rocks and surrounding topography to the thermal state of the regolith in the vicinity of the Apollo 17 landing site over the course of the lunar diurnal cycle. Further development of both this model and the event location algorithm may permit definitive discrimination between different types of local diurnal events e.g. lander noise, thermally-induced rock breakdown, or fault creep on the nearby Lee-Lincoln scarp. These results could place important constraints on both the contribution of seismicity to regolith production, and the age of young lobate scarps.

  14. Integration of seismic interpretation and petrophysical studies on Hawaz Formation in J-field NC-186 concession, Northwest Murzuq basin, Libya

    NASA Astrophysics Data System (ADS)

    Mohamed, A. K.; Selim, E. I.; Kashlaf, A.

    2016-12-01

    This study has been carried out by the integration of seismic interpretations and the well-logging analysis of ten wells distributed in J-field of concession NC-186, Murzuq basin, Libya. Twenty (3D) seismic lines and ten wells have been analyzed. The results of this study indicated that, the main reservoir in this concession is Hawaz Formation. Hawaz has been split into 8 units with a subdivision of Hawaz H4 into three subunits with the objective of better characterization of the three general fine upward intervals. The lower interval of H4 zone presents the better reservoir properties. The depth of reflector H4 ranges from 4100 ft in the northwestern part of the study area and increases to 4600 ft in the southeastern part of the study area. In this study, the outline of the Hawaz paleohighs which is NC-186 Field ;J; is generally trending in the NW-SE direction. The well logging analysis particularly quick look interpretation indicates that Hawaz Formation in the studied wells is mainly oil-bearing with some water-bearing sand levels at the horizons from H4 to and H6 which are potentially the main reservoirs. The water bearing zones are beyond these horizons starting from the sub-horizon H6c and the oil water contact is probably at depth 4495 ft. The crossplot of porosity-saturation for H5 and H6b indicates firmly that these horizons are indeed at irreducible state and will produce mainly oil as indicated in J4-NC186 well, while the crossplot of H8 shows wide scattering of points which is the main characteristic for water producing horizon. The depth of Hawaz Formation H4 is more than 4160 ft in J4, J12 and J16 wells in the northwestern parts of this field and increases to 4400 in the central part of the concession at well J1.

  15. Two types of seismicity accompanying hydraulic fracturing in Harrison County, Ohio - implications for seismic hazard and seismogenic mechanism

    NASA Astrophysics Data System (ADS)

    Kozlowska, M.; Brudzinski, M.; Friberg, P. A.; Skoumal, R.; Baxter, N. D.; Currie, B.

    2017-12-01

    While induced seismicity in the United States has mainly been attributed to wastewater disposal, Eastern Ohio has provided cases of seismicity induced by both hydraulic fracturing (HF) and wastewater disposal. In this study, we investigate five cases of seismicity associated with HF in Harrison County, OH. Because of their temporal and spatial isolation from other injection activities, this provide an ideal setting for studying the relationships between high pressure injection and earthquakes. Our analysis reveals two distinct groups of seismicity. Deeper earthquakes occur in the Precambrian crystalline basement, reach larger magnitudes (M>2), have lower b-values (<1), and continue for weeks following stimulation shut down. Shallower earthquakes, on the other hand, occur in Paleozoic sedimentary rocks 400 m below HF, are limited to smaller magnitudes (M<1), have higher b-values (>1.5), and lack post-stimulation activity. We seek the physical explanation of observed difference in earthquakes character and hypothesize that the maturity of faults is the main factor determining sequences b-values. Based on published results of laboratory experiments and fault modeling, we interpret the deep seismicity as slip on more mature faults in the older crystalline rocks and the shallow seismicity as slip on immature faults in the younger, lower viscosity sedimentary rocks. This suggests that HF inducing seismicity on deeper, more mature faults poses higher seismic hazards. The analysis of water and gas production data from these wells suggests that wells inducing deeper seismicity produced more water than wells with shallow seismicity. This indicates more extensive hydrologic connections outside the target reservoir, which may explain why gas production drops more quickly for wells with deeper seismicity. Despite these indications that hydraulic pressure fluctuations induce seismicity, we also find only 2-3 hours between onset of stimulation of HF wells and seismicity that is

  16. Focusing patterns of seismicity with relocation and collapsing

    NASA Astrophysics Data System (ADS)

    Li, Ka Lok; Gudmundsson, Ólafur; Tryggvason, Ari; Bödvarsson, Reynir; Brandsdóttir, Bryndís

    2016-07-01

    Seismicity is generally concentrated on faults or in fault zones of varying, sometimes complex geometry. An earthquake catalog, compiled over time, contains useful information about this geometry, which can help understanding the tectonics of a region. Interpreting the geometrical distribution of events in a catalog is often complicated by the diffuseness of the earthquake locations. Here, we explore a number of strategies to reduce this diffuseness and hence simplify the seismicity pattern of an earthquake catalog. These strategies utilize information about event locations contained in their overall catalog distribution. They apply this distribution as an a priori constraint on relocations of the events, or as an attractor for each individual event in a collapsing scheme, and thereby focus the locations. The latter strategy is not a relocation strategy in a strict sense, although event foci are moved, because the movements are not driven by data misfit. Both strategies simplify the seismicity pattern of the catalog and may help to interpret it. A synthetic example and a real-data example from an aftershock sequence in south west Iceland are presented to demonstrate application of the strategies. Entropy is used to quantify their effect.

  17. Integrating long-offset transient electromagnetics (LOTEM) with seismics in an exploration environment

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

    Strack, K.M.; Vozoff, K.

    The applications of electromagnetics have increased in the past two decades because of an improved understanding of the methods, improves service availability, and the increased focus of exploration in the more complex reservoir characterization issues. For electromagnetic methods surface applications for hydrocarbon Exploration and Production are still a special case, while applications in borehole and airborne research and for engineering and environmental objectives are routine. In the past, electromagnetic techniques, in particular deep transient electromagnetics, made up a completely different discipline in geophysics, although many of the principles are similar to the seismic one. With an understanding of the specificmore » problems related to data processing initially and then acquisition, the inclusion of principles learned from seismics happened almost naturally. Initially, the data processing was very similar to seismic full-waveform processing. The hardware was also changed to include multichannel acquisition systems, and the field procedures became very similar to seismic surveying. As a consequence, the integration and synergism of the interpretation process is becoming almost automatic. The long-offset transient electromagnetic (LOTEM) technique will be summarized from the viewpoint of its similarity to seismics. The complete concept of the method will also be reviewed. An interpretation case history that integrates seismic and LOTEM from a hydrocarbon area in China clearly demonstrates the limitations and benefits of the method.« less

  18. Using seismic and tilt measurements simultaneously to forecast eruptions of silicic volcanoes

    NASA Astrophysics Data System (ADS)

    Neuberg, Jurgen; Collinson, Amy; Mothes, Patricia

    2016-04-01

    Independent interpretations of seismic swarms and tilt measurement on active silicic volcanoes have been successfully used to assess their eruption potential. Swarms of low-frequency seismic events have been associated with brittle failure or stick-slip motion of magma during ascent and have been used to estimate qualitatively the magma ascent rate which typically accelerates before lava dome collapses. Tilt signals are extremely sensitive indicators for volcano deformation and have been often modelled and interpreted as inflation or deflation of a shallow magma reservoir. Here we show that tilt in many cases does not represent inflation or deflation but is directly linked to magma ascent rate.This talk aims to combine these two independent observations, seismicity and deformation, to design and implement a forecasting tool that can be deployed in volcano observatories on an operational level.

  19. Analysis of the seismic activity associated with the 2010 eruption of Merapi Volcano, Java

    NASA Astrophysics Data System (ADS)

    Budi-Santoso, Agus; Lesage, Philippe; Dwiyono, Sapari; Sumarti, Sri; Subandriyo; Surono; Jousset, Philippe; Metaxian, Jean-Philippe

    2013-07-01

    The 2010 eruption of Merapi is the first large explosive eruption of the volcano that has been instrumentally observed. The main characteristics of the seismic activity during the pre-eruptive period and the crisis are presented and interpreted in this paper. The first seismic precursors were a series of four shallow swarms during the period between 12 and 4 months before the eruption. These swarms are interpreted as the result of perturbations of the hydrothermal system by increasing heat flow. Shorter-term and more continuous precursory seismic activity started about 6 weeks before the initial explosion on 26 October 2010. During this period, the rate of seismicity increased almost constantly yielding a cumulative seismic energy release for volcano-tectonic (VT) and multiphase events (MP) of 7.5 × 1010 J. This value is 3 times the maximum energy release preceding previous effusive eruptions of Merapi. The high level reached and the accelerated behavior of both the deformation of the summit and the seismic activity are distinct features of the 2010 eruption. The hypocenters of VT events in 2010 occur in two clusters at of 2.5 to 5 km and less than 1.5 km depths below the summit. An aseismic zone was detected at 1.5-2.5 km depth, consistent with studies of previous eruptions, and indicating that this is a robust feature of Merapi's subsurface structure. Our analysis suggests that the aseismic zone is a poorly consolidated layer of altered material within the volcano. Deep VT events occurred mainly before 17 October 2010; subsequent to that time shallow activity strongly increased. The deep seismic activity is interpreted as associated with the enlargement of a narrow conduit by an unusually large volume of rapidly ascending magma. The shallow seismicity is interpreted as recording the final magma ascent and the rupture of a summit-dome plug, which triggered the eruption on 26 October 2010. Hindsight forecasting of the occurrence time of the eruption is performed

  20. New Possibilities In Assessing Time-dependent Seismic Risk

    NASA Astrophysics Data System (ADS)

    Kossobokov, V.

    A novel understanding of seismic occurrence process in terms of dynamics of a hierar- chical system of blocks-and-faults implies the necessity of new approaches to seismic risk assessment, which would allow for evident heterogeneity of seismic distribution in space and time. Spatial, apparently fractal, patterns of seismic distribution should be treated appropriately in estimation of seismic hazard. Otherwise the result could be over- or underestimated significantly. The patterns are clearly associated with tec- tonic movement, which traces being accumulated in a time-scale of tens of thousand years or larger provide geographic, geologic, gravity, and magnetic evidence of inten- sity of driving forces, their directivity and dating. This, term-less, in a sense of hu- man life-time, evidence, both clear and masked, requires analysis that involves pattern recognition and interpretation before it is used in favor of a conclusion about present day seismic activity. Moreover, the existing reproducible intermediate-term medium- range earthquake prediction algorithms that have passed statistical significance testing in forward application complement a knowledgeable estimation of the temporal devi- ation of seismic hazard in a given area from a constant. Bringing together the two estimations and convolving them with a given distribution of valuables of different kinds, e.g. population, industry, economy, etc., finalizes an estimation of seismic risk distribution.

  1. Application of seismic-refraction techniques to hydrologic studies

    USGS Publications Warehouse

    Haeni, F.P.

    1986-01-01

    During the past 30 years, seismic-refraction methods have been used extensively in petroleum, mineral, and engineering investigations, and to some extent for hydrologic applications. Recent advances in equipment, sound sources, and computer interpretation techniques make seismic refraction a highly effective and economical means of obtaining subsurface data in hydrologic studies. Aquifers that can be defined by one or more high seismic-velocity surfaces, such as (1) alluvial or glacial deposits in consolidated rock valleys, (2) limestone or sandstone underlain by metamorphic or igneous rock, or (3) saturated unconsolidated deposits overlain by unsaturated unconsolidated deposits,are ideally suited for applying seismic-refraction methods. These methods allow the economical collection of subsurface data, provide the basis for more efficient collection of data by test drilling or aquifer tests, and result in improved hydrologic studies.This manual briefly reviews the basics of seismic-refraction theory and principles. It emphasizes the use of this technique in hydrologic investigations and describes the planning, equipment, field procedures, and intrepretation techniques needed for this type of study.Examples of the use of seismic-refraction techniques in a wide variety of hydrologic studies are presented.

  2. Micro-seismicity in the Gulf of Cadiz: Is there a link between micro-seismicity, high magnitude earthquakes and active faults?

    NASA Astrophysics Data System (ADS)

    Silva, Sónia; Terrinha, Pedro; Matias, Luis; Duarte, João C.; Roque, Cristina; Ranero, César R.; Geissler, Wolfram H.; Zitellini, Nevio

    2017-10-01

    The Gulf of Cadiz seismicity is characterized by persistent low to intermediate magnitude earthquakes, occasionally punctuated by high magnitude events such as the M 8.7 1755 Great Lisbon earthquake and the M = 7.9 event of February 28th, 1969. Micro-seismicity was recorded during 11 months by a temporary network of 25 ocean bottom seismometers (OBSs) in an area of high seismic activity, encompassing the potential source areas of the mentioned large magnitude earthquakes. We combined micro-seismicity analysis with processing and interpretation of deep crustal seismic reflection profiles and available refraction data to investigate the possible tectonic control of the seismicity in the Gulf of Cadiz area. Three controlling mechanisms are explored: i) active tectonic structures, ii) transitions between different lithospheric domains and inherited Mesozoic structures, and iii) fault weakening mechanisms. Our results show that micro-seismicity is mostly located in the upper mantle and is associated with tectonic inversion of extensional rift structures and to the transition between different lithospheric/rheological domains. Even though the crustal structure is well imaged in the seismic profiles and in the bathymetry, crustal faults show low to negligible seismic activity. A possible explanation for this is that the crustal thrusts are thin-skinned structures rooting in relatively shallow sub-horizontal décollements associated with (aseismic) serpentinization levels at the top of the lithospheric mantle. Therefore, co-seismic slip along crustal thrusts may only occur during large magnitude events, while for most of the inter-seismic cycle these thrusts remain locked, or slip aseismically. We further speculate that high magnitude earthquake's ruptures may only nucleate in the lithospheric mantle and then propagate into the crust across the serpentinized layers.

  3. 2D seismic interpretation and characterization of the Hauterivian-Early Barremian source rock in Al Baraka oil field, Komombo Basin, Upper Egypt

    NASA Astrophysics Data System (ADS)

    Ali, Moamen; Darwish, M.; Essa, Mahmoud A.; Abdelhady, A.

    2018-03-01

    Komombo Basin is located in Upper Egypt about 570 km southeast of Cairo; it is an asymmetrical half graben and the first oil producing basin in Upper Egypt. The Six Hills Formation is of Early Cretaceous age and subdivided into seven members from base to top (A-G); meanwhile the B member is of Hauterivian-Early Barremian and it is the only source rock of Komombo Basin. Therefore, a detailed study of the SR should be carried out, which includes the determination of the main structural elements, thickness, facies distribution and characterization of the B member SR which has not been conducted previously in the study area. Twenty 2D seismic lines were interpreted with three vertical seismic profiles (VSP) to construct the depth structure-tectonic map on the top of the B member and to highlight the major structural elements. The interpretation of depth structure contour map shows two main fault trends directed towards the NW-SE and NE to ENE directions. The NW-SE trend is the dominant one, creating a major half-graben system. Also the depth values range from -8400 ft at the depocenter in the eastern part to -4800 ft at the shoulder of the basin in the northwestern part of the study area. Meanwhile the Isopach contour map of the B member shows a variable thickness ranging between 300 ft to 750 ft. The facies model shows that the B member SR is composed mainly of shale with some sandstone streaks. The B member rock samples were collected from Al Baraka-1 and Al Baraka SE-1 in the eastern part of Komombo Basin. The results indicate that the organic matter content (TOC) has mainly good to very good (1-3.36 wt %), The B member samples have HI values in the range 157-365 (mg HC/g TOC) and dominated by Type II/III kerogen, and is thus considered to be oil-gas prone based on Rock-Eval pyrolysis, Tmax values between 442° and 456° C therefore interpreted to be mature for hydrocarbon generation. Based on the measured vitrinite equivalent reflectance values, the B member SR

  4. Using seismic derived lithology parameters for hydrocarbon indication

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

    Van Riel, P.; Sisk, M.

    1996-08-01

    The last two decades have shown a strong increase in the use of seismic amplitude information for direct hydrocarbon indication. However, working with seismic amplitudes (and seismic attributes) has several drawbacks: tuning effects must be handled; quantitative analysis is difficult because seismic amplitudes are not directly related to lithology; and seismic amplitudes are reflection events, making it is unclear if amplitude changes relate to lithology variations above or below the interface. These drawbacks are overcome by working directly on seismic derived lithology data, lithology being a layer property rather than an interface property. Technology to extract lithology from seismic datamore » has made great strides, and a large range of methods are now available to users including: (1) Bandlimited acoustic impedance (AI) inversion; (2) Reconstruction of the low AI frequencies from seismic velocities, from spatial well log interpolation, and using constrained sparse spike inversion techniques; (3) Full bandwidth reconstruction of multiple lithology properties (porosity, sand fraction, density etc.,) in time and depth using inverse modeling. For these technologies to be fully leveraged, accessibility by end users is critical. All these technologies are available as interactive 2D and 3D workstation applications, integrated with seismic interpretation functionality. Using field data examples, we will demonstrate the impact of these different approaches on deriving lithology, and in particular show how accuracy and resolution is increased as more geologic and well information is added.« less

  5. Multivariate Formation Pressure Prediction with Seismic-derived Petrophysical Properties from Prestack AVO inversion and Poststack Seismic Motion Inversion

    NASA Astrophysics Data System (ADS)

    Yu, H.; Gu, H.

    2017-12-01

    A novel multivariate seismic formation pressure prediction methodology is presented, which incorporates high-resolution seismic velocity data from prestack AVO inversion, and petrophysical data (porosity and shale volume) derived from poststack seismic motion inversion. In contrast to traditional seismic formation prediction methods, the proposed methodology is based on a multivariate pressure prediction model and utilizes a trace-by-trace multivariate regression analysis on seismic-derived petrophysical properties to calibrate model parameters in order to make accurate predictions with higher resolution in both vertical and lateral directions. With prestack time migration velocity as initial velocity model, an AVO inversion was first applied to prestack dataset to obtain high-resolution seismic velocity with higher frequency that is to be used as the velocity input for seismic pressure prediction, and the density dataset to calculate accurate Overburden Pressure (OBP). Seismic Motion Inversion (SMI) is an inversion technique based on Markov Chain Monte Carlo simulation. Both structural variability and similarity of seismic waveform are used to incorporate well log data to characterize the variability of the property to be obtained. In this research, porosity and shale volume are first interpreted on well logs, and then combined with poststack seismic data using SMI to build porosity and shale volume datasets for seismic pressure prediction. A multivariate effective stress model is used to convert velocity, porosity and shale volume datasets to effective stress. After a thorough study of the regional stratigraphic and sedimentary characteristics, a regional normally compacted interval model is built, and then the coefficients in the multivariate prediction model are determined in a trace-by-trace multivariate regression analysis on the petrophysical data. The coefficients are used to convert velocity, porosity and shale volume datasets to effective stress and then

  6. Interpretation of interseismic deformations and the seismic cycle associated with large subduction earthquakes

    NASA Astrophysics Data System (ADS)

    Trubienko, Olga; Fleitout, Luce; Garaud, Jean-Didier; Vigny, Christophe

    2013-03-01

    The deformations of the overriding and subducting plates during the seismic cycle associated with large subduction earthquakes are modelled using 2D and 3D finite element techniques. A particular emphasis is put on the interseismic velocities and on the impact of the rheology of the asthenosphere. The distance over which the seismic cycle perturbs significantly the velocities depends upon the ratio of the viscosity in the asthenosphere to the period of the seismic cycle and can reach several thousand km for rheological parameters deduced from the first years of deformation after the Aceh earthquake. For a same early postseismic velocity, a Burger rheology of the asthenosphere implies a smaller duration of the postseismic phase and thus smaller interseismic velocities than a Maxwell rheology. A low viscosity wedge (LVW) modifies very significantly the predicted horizontal and vertical motions in the near and middle fields. In particular, with a LVW, the peak in vertical velocity at the end of the cycle is predicted to be no longer above the deep end of the locked section of the fault but further away, above the continentward limit of the LVW. The lateral viscosity variations linked to the presence at depth of the subducting slab affect substantially the results. The north-south interseismic compression predicted by this preliminary 2D model over more than 1500 km within the Sunda block is in good agreement with the pre-2004 velocities with respect to South-China inferred from GPS observations in Thailand, Malaysia and Indonesia. In Japan, before the Tohoku earthquake, the eastern part of northern Honshu was subsiding while the western part was uplifting. This transition from subsidence to uplift so far away from the trench is well fitted by the predictions from our models involving a LVW. Most of the results obtained here in a 2D geometry are shown to provide a good estimate of the displacements for fault segments of finite lateral extent, with a 3D spherical

  7. A new interpretation of seismic tomography in the southern Dead Sea basin using neural network clustering techniques

    NASA Astrophysics Data System (ADS)

    Braeuer, Benjamin; Bauer, Klaus

    2015-11-01

    The Dead Sea is a prime location to study the structure and development of pull-apart basins. We analyzed tomographic models of Vp, Vs, and Vp/Vs using self-organizing map clustering techniques. The method allows us to identify major lithologies by their petrophysical signatures. Remapping the clusters into the subsurface reveals the distribution of basin sediments, prebasin sedimentary rocks, and crystalline basement. The Dead Sea basin shows an asymmetric structure with thickness variation from 5 km in the west to 13 km in the east. Most importantly, we identified a distinct, well-defined body under the eastern part of the basin down to 18 km depth. Considering its geometry and petrophysical signature, this unit is interpreted as a buried counterpart of the shallow prebasin sediments encountered outside of the basin and not as crystalline basement. The seismicity distribution supports our results, where events are concentrated along boundaries of the basin and the deep prebasin sedimentary body. Our results suggest that the Dead Sea basin is about 4 km deeper than assumed from previous studies.

  8. Evaluation and developmental studies of possible active seismic experiments during the post-Apollo period

    NASA Technical Reports Server (NTRS)

    Kovach, R. L.

    1974-01-01

    Seismic velocity studies pertinent to the lunar crust and mantle are briefly summarized. The compressional and shear wave velocities in loose aggregates are discussed along with the effects of temperature on seismic velocity in compacted powders. Abstracts of papers concerning the lunar structure are included.

  9. Estimation of bedrock depth using the horizontal‐to‐vertical (H/V) ambient‐noise seismic method

    USGS Publications Warehouse

    Lane, John W.; White, Eric A.; Steele, Gregory V.; Cannia, James C.

    2008-01-01

    Estimating sediment thickness and the geometry of the bedrock surface is a key component of many hydrogeologic studies. The horizontal‐to‐vertical (H/V) ambient‐noise seismic method is a novel, non‐invasive technique that can be used to rapidly estimate the depth to bedrock. The H/V method uses a single, broad‐band three‐component seismometer to record ambient seismic noise. The ratio of the averaged horizontal‐to‐vertical frequency spectrum is used to determine the fundamental site resonance frequency, which can be interpreted using regression equations to estimate sediment thickness and depth to bedrock. The U.S. Geological Survey used the H/V seismic method during fall 2007 at 11 sites in Cape Cod, Massachusetts, and 13 sites in eastern Nebraska. In Cape Cod, H/V measurements were acquired along a 60‐kilometer (km) transect between Chatham and Provincetown, where glacial sediments overlie metamorphic rock. In Nebraska, H/V measurements were acquired along approximately 11‐ and 14‐km transects near Firth and Oakland, respectively, where glacial sediments overlie weathered sedimentary rock. The ambient‐noise seismic data from Cape Cod produced clear, easily identified resonance frequency peaks. The interpreted depth and geometry of the bedrock surface correlate well with boring data and previously published seismic refraction surveys. Conversely, the ambient‐noise seismic data from eastern Nebraska produced subtle resonance frequency peaks, and correlation of the interpreted bedrock surface with bedrock depths from borings is poor, which may indicate a low acoustic impedance contrast between the weathered sedimentary rock and overlying sediments and/or the effect of wind noise on the seismic records. Our results indicate the H/V ambient‐noise seismic method can be used effectively to estimate the depth to rock where there is a significant acoustic impedance contrast between the sediments and underlying rock. However, effective use of

  10. Seismic stratigraphy of the Heuksan mud belt in the southeastern Yellow Sea, Korea

    NASA Astrophysics Data System (ADS)

    Lee, Gwang-Soo; Yoo, Dong Geun; Bae, Sung Ho; Min, Gun-Hong; Kim, Seong-Pil; Choi, Hunsoo

    2015-12-01

    To establish the seismic stratigraphy of the Heuksan mud belt (HMB) and reconstruct its depositional history, approximately 1,600 km of high-resolution seismic data were newly obtained using chirp acoustic sub-bottom profiler, sparker, and air-gun seismic systems. Based on seismic stratigraphic analysis, the HMB can be divided into three major seismic units (I, II, and III, from top to bottom) and four subunits (II-a, II-b, III-a, and III-b) overlying transgressive sands, pre-last glacial maximum (LGM) deposits, and the acoustic basement. Each unit and subunit show different seismic facies and geometry, being clearly separated from each other by bounding surfaces formed since the LGM. The spatial distribution, thicknesses and volumes of the seismic units were determined and plotted to document the sequential formation of the HMB. The correlation between deep drill core data (HMB-101, HMB-102, HMB-103, YSDP-101, and YSDP-102) and the seismic data suggests that subunits III-b and III-a were formed by the continuous accumulation of fine-grained sediment with partial sandy sediment in an estuarine/deltaic environment during the early to middle transgressive stage, accompanied by landward migration of the shoreline. Subunits II-b and II-a were probably formed by re-deposition of large volumes of sediment eroded from unit III during the middle transgressive to early highstand stage. Unit I is interpreted as the most recent mud deposit representing the highstand systems tract when sea-level rise terminated. The careful definition of seismic units and their interpretation proposed in this study, on the basis of the large and partly new seismic dataset covering the entire HMB together with deep drill core data, have been instrumental in reconstructing the depositional environment and formation mechanisms of the HMB.

  11. Integrated reservoir characterization for unconventional reservoirs using seismic, microseismic and well log data

    NASA Astrophysics Data System (ADS)

    Maity, Debotyam

    and spatial variability as a means to better understand the reservoir behavior. As part of this study, we have developed the following elements which are discussed in the subsequent chapters: 1. An integrated characterization framework for unconventional settings with adaptable workflows for all stages of data processing, interpretation and analysis. 2. A novel autopicking workflow for noisy passive seismic data used for improved accuracy in event picking as well as for improved velocity model building. 3. Improved passive seismic survey design optimization framework for better data collection and improved property estimation. 4. Extensive post-stack seismic attribute studies incorporating robust schemes applicable in complex reservoir settings. 5. Uncertainty quantification and analysis to better quantify property estimates over and above the qualitative interpretations made and to validate observations independently with quantified uncertainties to prevent erroneous interpretations. 6. Property mapping from microseismic data including stress and anisotropic weakness estimates for integrated reservoir characterization and analysis. 7. Integration of results (seismic, microseismic and well logs) from analysis of individual data sets for integrated interpretation using predefined integration framework and soft computing tools.

  12. A 3-D seismic investigation of the Ray gas storage reef, Macomb County, Michigan

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

    Schaefer, S.F.; Dixon, R.A.

    1994-08-01

    A 4.2 mi[sup 2] 3-D seismic survey was acquired over the Ray Niagaran reef gas storage field in southeast Michigan as part of a program to maximize storage capacity and gas deliverability of the storage reservoir. Goals of the survey were to (1) determine if additional storage capacity could be found either as extensions to the Ray reef or as undiscovered satellite reefs, (2) investigate the relationship between the main body and a low-relief gas well east of the reef, and (3) determine if seismic data can be used to quantify reservoir parameters to maximize the productive capacity of infillmore » wells. Interpretation of the 3-D seismic data resulted in a detailed image of the reef, using several interpretive techniques. A seismic reflection within the reef was correlated with a known porosity zone, and a possible relationship between porosity and seismic amplitude was investigated. A potential connection between the main reef and the low-relief gas well was identified. This project illustrates the economic value of investigating an existing storage reef with 3-D seismic data, and underscores the necessity of such a survey prior to developing a new storage reservoir.« less

  13. Visualising uncertainty: interpreting quantified geoscientific inversion outputs for a diverse user community.

    NASA Astrophysics Data System (ADS)

    Reading, A. M.; Morse, P. E.; Staal, T.

    2017-12-01

    Geoscientific inversion outputs, such as seismic tomography contour images, are finding increasing use amongst scientific user communities that have limited knowledge of the impact of output parameter uncertainty on subsequent interpretations made from such images. We make use of a newly written computer application which enables seismic tomography images to be displayed in a performant 3D graphics environment. This facilitates the mapping of colour scales to the human visual sensorium for the interactive interpretation of contoured inversion results incorporating parameter uncertainty. Two case examples of seismic tomography inversions or contoured compilations are compared from the southern hemisphere continents of Australia and Antarctica. The Australian example is based on the AuSREM contoured seismic wavespeed model while the Antarctic example is a valuable but less well constrained result. Through adjusting the multiple colour gradients, layer separations, opacity, illumination, shadowing and background effects, we can optimise the insights obtained from the 3D structure in the inversion compilation or result. Importantly, we can also limit the display to show information in a way that is mapped to the uncertainty in the 3D result. Through this practical application, we demonstrate that the uncertainty in the result can be handled through a well-posed mapping of the parameter values to displayed colours in the knowledge of what is perceived visually by a typical human. We found that this approach maximises the chance of a useful tectonic interpretation by a diverse scientific user community. In general, we develop the idea that quantified inversion uncertainty can be used to tailor the way that the output is presented to the analyst for scientific interpretation.

  14. Geological interpretation of combined Seabeam, Gloria and seismic data from Anegada Passage (Virgin Islands, north Caribbean)

    USGS Publications Warehouse

    Jany, I.; Scanlon, Kathryn M.; Mauffret, A.

    1990-01-01

    The Anegada Passage (sensu lato) includes several basins and ridges from Southeast of Puerto Rico to the corner of the Virgin Islands Platform. Seabeam (Seacarib I) and Gloria long-range sidescan sonar surveys were carried out in this area. These new data allow us to propose an interpretation of the Anegada Passage. Most of the features described are related to wrench faulting: (a) St Croix and Virgin Islands Basins are pull-apart basins created in a right-lateral strike-slip environment based on their rhomboidal shape and seismic data (e.g. the flower structure). These two pull-aparts are divided into two sub-basins by a curvilinear normal fault in the Virgin Islands Basin and a right-lateral strike-slip fault in the St Croix Basin. (b) Tortola Ridge and a 'dog's leg' shaped structure are inferred to be restraining bends between two right-lateral strike-slip faults. (c) We identified two ENE-WSW volcanic lineaments in the eastern area and one volcano lying between Virgin Islands and St Croix Basins. (d) As shown by the seismic activity main wrench motion occurs along the north slope of Virgin Islands Basin and through Anegada Passage. A branching of this main fault transmits the transtensional motion to St Croix Basin. A two-stage story is proposed for the creation of the basins. A first extensional event during Eocene(?)-Oligocene-lower Miocene time created Virgin Islands, St Croix Basins and the tilted blocks of St Croix Ridge. A second transtensional event from Pliocene to Recent gave the present day pattern to this area. However, the displacement along the strike-slip faults is no more than 15 km long. The proposed geodynamic model is based on the separation of the northeastern Caribbean boundary into two blocks. In the West, the indenter of Beata Ridge gives a northeastern motion to Hispaniola Block. In the East, as a result of Hispaniola Block's motion, the Puerto Rico-Virgin Islands Block could escape in an east-northeast direction. 

  15. Earthquake dynamics. Mapping pressurized volcanic fluids from induced crustal seismic velocity drops.

    PubMed

    Brenguier, F; Campillo, M; Takeda, T; Aoki, Y; Shapiro, N M; Briand, X; Emoto, K; Miyake, H

    2014-07-04

    Volcanic eruptions are caused by the release of pressure that has accumulated due to hot volcanic fluids at depth. Here, we show that the extent of the regions affected by pressurized fluids can be imaged through the measurement of their response to transient stress perturbations. We used records of seismic noise from the Japanese Hi-net seismic network to measure the crustal seismic velocity changes below volcanic regions caused by the 2011 moment magnitude (M(w)) 9.0 Tohoku-Oki earthquake. We interpret coseismic crustal seismic velocity reductions as related to the mechanical weakening of the pressurized crust by the dynamic stress associated with the seismic waves. We suggest, therefore, that mapping seismic velocity susceptibility to dynamic stress perturbations can be used for the imaging and characterization of volcanic systems. Copyright © 2014, American Association for the Advancement of Science.

  16. The shallow structure of Solfatara Volcano, Italy, revealed by dense, wide-aperture seismic profiling.

    PubMed

    Bruno, Pier Paolo G; Maraio, Stefano; Festa, Gaetano

    2017-12-12

    Two active-source, high-resolution seismic profiles were acquired in the Solfatara tuff cone in May and November 2014, with dense, wide-aperture arrays. Common Receiver Surface processing was crucial in improving signal-to-noise ratio and reflector continuity. These surveys provide, for the first time, high-resolution seismic images of the Solfatara crater, depicting a ~400 m deep asymmetrical crater filled by volcanoclastic sediments and rocks and carved within an overall non-reflective pre-eruptive basement showing features consistent with the emplacement of shallow intrusive bodies. Seismic reflection data were interpreted using the trace complex attributes and clearly display several steep and segmented collapse faults, generally having normal kinematics and dipping toward the crater centre. Fault/fracture planes are imaged as sudden amplitude drops that generate narrow low-similarity and high-dip attributes. Uprising fluids degassed by a magmatic source are the most probable cause of the small-scale amplitude reduction. Seismic data also support the interpretation of the shallow structure of the Solfatara crater as a maar. Our results provides a solid framework to constrain the near-surface geological interpretation of such a complex area, which improves our understanding of the temporal changes of the structure in relation with other geophysical and geochemical measurements.

  17. On the likelihood of post-perovskite near the core-mantle boundary: A statistical interpretation of seismic observations

    NASA Astrophysics Data System (ADS)

    Cobden, Laura; Mosca, Ilaria; Trampert, Jeannot; Ritsema, Jeroen

    2012-11-01

    Recent experimental studies indicate that perovskite, the dominant lower mantle mineral, undergoes a phase change to post-perovskite at high pressures. However, it has been unclear whether this transition occurs within the Earth's mantle, due to uncertainties in both the thermochemical state of the lowermost mantle and the pressure-temperature conditions of the phase boundary. In this study we compare the relative fit to global seismic data of mantle models which do and do not contain post-perovskite, following a statistical approach. Our data comprise more than 10,000 Pdiff and Sdiff travel-times, global in coverage, from which we extract the global distributions of dln VS and dln VP near the core-mantle boundary (CMB). These distributions are sensitive to the underlying lateral variations in mineralogy and temperature even after seismic uncertainties are taken into account, and are ideally suited for investigating the likelihood of the presence of post-perovskite. A post-perovskite-bearing CMB region provides a significantly closer fit to the seismic data than a post-perovskite-free CMB region on both a global and regional scale. These results complement previous local seismic reflection studies, which have shown a consistency between seismic observations and the physical properties of post-perovskite inside the deep Earth.

  18. Exploring seismicity using geomagnetic and gravity data - a case study for Bulgaria

    NASA Astrophysics Data System (ADS)

    Trifonova, P.; Simeonova, S.; Solakov, D.; Metodiev, M.

    2012-04-01

    Seismicity exploration certainly requires comprehensive analysis of location, orientation and length distribution of fault and block systems with a variety of geophysical methods. In the present research capability of geomagnetic and gravity anomalous field data are used for revealing of buried structures inside the earth's upper layers. Interpretation of gravity and magnetic data is well known and often applied to delineate various geological structures such as faults, flexures, thrusts, borders of dislocated blocks etc. which create significant rock density contrast in horizontal planes. Study area of the present research covers the territory of Bulgaria which is part of the active continental margin of the Eurasian plate. This region is a typical example of high seismic risk area. The epicentral map shows that seismicity in the region is not uniformly distributed in space. Therefore the seismicity is described in distributed geographical zones (seismic source zones). Each source zone is characterized by its specific tectonic, seismic, and geological particulars. From the analysis of the depth distribution it was recognized that the earthquakes in the region occurred in the Earth's crust. Hypocenters are mainly located in the upper crust, and only a few events are related to the lower crust. The maximum depth reached is about 50 km in southwestern Bulgaria; outside, the foci affect only the surficial 30-35 km. Maximum density of seismicity involves the layer between 5 and 25 km. This fact determines the capability of potential fields data to reveal crustal structures and to examine their parameters as possible seismic sources. Results showed that a number of geophysically interpreted structures coincide with observed on the surface dislocations and epicenter clusters (well illustrated in northern Bulgaria) which confirms the reliability of the applied methodology. The complicated situation in southern Bulgaria is demonstrated by mosaics structure of geomagnetic

  19. Study of iron deposit using seismic refraction and resistivity in Carajás Mineral Province, Brazil

    NASA Astrophysics Data System (ADS)

    Nogueira, Pedro Vencovsky; Rocha, Marcelo Peres; Borges, Welitom Rodrigues; Silva, Adalene Moreira; Assis, Luciano Mozer de

    2016-10-01

    This work comprises the acquisition, processing and interpretation of 2D seismic shallow refraction (P-wave) and resistivity profiles located in the iron ore deposit of N4WS, Carajás Mineral Province (CMP), northern Brazil. The geophysical methods were used to identify the boundaries of the iron ore deposit. Another objective was to evaluate the potentiality of these geophysical methods in that geological context. In order to validate the results, the geophysical lines were located to match a geological borehole line. For the seismic refraction, we used 120 channels, spaced by 10 m, in a line of 1190 m, with seven shot points. The resistivity method used in the acquisition was the electrical resistivity imaging, with pole-pole array, in order to reach greater depths. The resistivity line had a length of 1430 m, with 10 m spacing between electrodes. The seismic results produced a model with two distinct layers. Based on the velocities values, the first layer was interpreted as altered rocks, and the second layer as more preserved rocks. It was not possible to discriminate different lithologies with the seismic method inside each layer. From the resistivity results, a zone of higher resistivity (> 3937 Ω·m) was interpreted as iron ore, and a region of intermediate resistivity (from 816 to 2330 Ω·m) as altered rocks. These two regions represent the first seismic layer. On the second seismic layer, an area with intermediated resistivity values (from 483 to 2330 Ω·m) was interpreted as mafic rocks, and the area with lower resistivity (< 483 Ω·m) as jaspilite. Our results were compared with geological boreholes and show reasonable correlation, suggesting that the geophysical anomalies correspond to the main variations in composition and physical properties of rocks.

  20. The analysis and interpretation of very-long-period seismic signals on volcanoes

    NASA Astrophysics Data System (ADS)

    Sindija, Dinko; Neuberg, Jurgen; Smith, Patrick

    2017-04-01

    The study of very long period (VLP) seismic signals became possible with the widespread use of broadband instruments. VLP seismic signals are caused by transients of pressure in the volcanic edifice and have periods ranging from several seconds to several minutes. For the VLP events recorded in March 2012 and 2014 at Soufriere Hills Volcano, Montserrat, we model the ground displacement using several source time functions: a step function using Richards growth equation, Küpper wavelet, and a damped sine wave to which an instrument response is then applied. This way we get a synthetic velocity seismogram which is directly comparable to the data. After the full vector field of ground displacement is determined, we model the source mechanism to determine the relationship between the source mechanism and the observed VLP waveforms. Emphasis of the research is on how different VLP waveforms are related to the volcano environment and the instrumentation used and on the processing steps in this low frequency band to get most out of broadband instruments.

  1. Maturity of nearby faults influences seismic hazard from hydraulic fracturing.

    PubMed

    Kozłowska, Maria; Brudzinski, Michael R; Friberg, Paul; Skoumal, Robert J; Baxter, Nicholas D; Currie, Brian S

    2018-02-20

    Understanding the causes of human-induced earthquakes is paramount to reducing societal risk. We investigated five cases of seismicity associated with hydraulic fracturing (HF) in Ohio since 2013 that, because of their isolation from other injection activities, provide an ideal setting for studying the relations between high-pressure injection and earthquakes. Our analysis revealed two distinct groups: ( i ) deeper earthquakes in the Precambrian basement, with larger magnitudes (M > 2), b-values < 1, and many post-shut-in earthquakes, versus ( ii ) shallower earthquakes in Paleozoic rocks ∼400 m below HF, with smaller magnitudes (M < 1), b-values > 1.5, and few post-shut-in earthquakes. Based on geologic history, laboratory experiments, and fault modeling, we interpret the deep seismicity as slip on more mature faults in older crystalline rocks and the shallow seismicity as slip on immature faults in younger sedimentary rocks. This suggests that HF inducing deeper seismicity may pose higher seismic hazards. Wells inducing deeper seismicity produced more water than wells with shallow seismicity, indicating more extensive hydrologic connections outside the target formation, consistent with pore pressure diffusion influencing seismicity. However, for both groups, the 2 to 3 h between onset of HF and seismicity is too short for typical fluid pressure diffusion rates across distances of ∼1 km and argues for poroelastic stress transfer also having a primary influence on seismicity.

  2. Maturity of nearby faults influences seismic hazard from hydraulic fracturing

    NASA Astrophysics Data System (ADS)

    Kozłowska, Maria; Brudzinski, Michael R.; Friberg, Paul; Skoumal, Robert J.; Baxter, Nicholas D.; Currie, Brian S.

    2018-02-01

    Understanding the causes of human-induced earthquakes is paramount to reducing societal risk. We investigated five cases of seismicity associated with hydraulic fracturing (HF) in Ohio since 2013 that, because of their isolation from other injection activities, provide an ideal setting for studying the relations between high-pressure injection and earthquakes. Our analysis revealed two distinct groups: (i) deeper earthquakes in the Precambrian basement, with larger magnitudes (M > 2), b-values < 1, and many post–shut-in earthquakes, versus (ii) shallower earthquakes in Paleozoic rocks ˜400 m below HF, with smaller magnitudes (M < 1), b-values > 1.5, and few post–shut-in earthquakes. Based on geologic history, laboratory experiments, and fault modeling, we interpret the deep seismicity as slip on more mature faults in older crystalline rocks and the shallow seismicity as slip on immature faults in younger sedimentary rocks. This suggests that HF inducing deeper seismicity may pose higher seismic hazards. Wells inducing deeper seismicity produced more water than wells with shallow seismicity, indicating more extensive hydrologic connections outside the target formation, consistent with pore pressure diffusion influencing seismicity. However, for both groups, the 2 to 3 h between onset of HF and seismicity is too short for typical fluid pressure diffusion rates across distances of ˜1 km and argues for poroelastic stress transfer also having a primary influence on seismicity.

  3. Research on Influencing Factors and Generalized Power of Synthetic Artificial Seismic Wave

    NASA Astrophysics Data System (ADS)

    Jiang, Yanpei

    2018-05-01

    Start your abstract here… In this paper, according to the trigonometric series method, the author adopts different envelope functions and the acceleration design spectrum in Seismic Code For Urban Bridge Design to simulate the seismic acceleration time history which meets the engineering accuracy requirements by modifying and iterating the initial wave. Spectral analysis is carried out to find out the the distribution law of the changing frequencies of the energy of seismic time history and to determine the main factors that affect the acceleration amplitude spectrum and energy spectrum density. The generalized power formula of seismic time history is derived from the discrete energy integral formula and the author studied the changing characteristics of generalized power of the seismic time history under different envelop functions. Examples are analyzed to illustrate that generalized power can measure the seismic performance of bridges.

  4. Seismic activity offshore Martinique and Dominica islands (Central Lesser Antilles subduction zone) from temporary onshore and offshore seismic networks

    NASA Astrophysics Data System (ADS)

    Ruiz, M.; Galve, A.; Monfret, T.; Sapin, M.; Charvis, P.; Laigle, M.; Evain, M.; Hirn, A.; Flueh, E.; Gallart, J.; Diaz, J.; Lebrun, J. F.

    2013-09-01

    This work focuses on the analysis of a unique set of seismological data recorded by two temporary networks of seismometers deployed onshore and offshore in the Central Lesser Antilles Island Arc from Martinique to Guadeloupe islands. During the whole recording period, extending from January to the end of August 2007, more than 1300 local seismic events were detected in this area. A subset of 769 earthquakes was located precisely by using HypoEllipse. We also computed focal mechanisms using P-wave polarities of the best azimuthally constrained earthquakes. We detected earthquakes beneath the Caribbean forearc and in the Atlantic oceanic plate as well. At depth seismicity delineates the Wadati-Benioff Zone down to 170 km depth. The main seismic activity is concentrated in the lower crust and in the mantle wedge, close to the island arc beneath an inner forearc domain in comparison to an outer forearc domain where little seismicity is observed. We propose that the difference of the seismicity beneath the inner and the outer forearc is related to a difference of crustal structure between the inner forearc interpreted as a dense, thick and rigid crustal block and the lighter and more flexible outer forearc. Seismicity is enhanced beneath the inner forearc because it likely increases the vertical stress applied to the subducting plate.

  5. Is Seismically Determined Q an Intrinsic Material Property?

    NASA Astrophysics Data System (ADS)

    Langston, C. A.

    2003-12-01

    The seismic quality factor, Q, has a well-defined physical meaning as an intrinsic material property associated with a visco-elastic or a non-linear stress-strain constitutive relation for a material. Measurement of Q from seismic waves, however, involves interpreting seismic wave amplitude and phase as deviations from some ideal elastic wave propagation model. Thus, assumptions in the elastic wave propagation model become the basis for attributing anelastic properties to the earth continuum. Scientifically, the resulting Q model derived from seismic data is no more than a hypothesis that needs to be verified by other independent experiments concerning the continuum constitutive law and through careful examination of the truth of the assumptions in the wave propagation model. A case in point concerns the anelasticity of Mississippi embayment sediments in the central U.S. that has important implications for evaluation of earthquake strong ground motions. Previous body wave analyses using converted Sp phases have suggested that Qs is ~30 in the sediments based on simple ray theory assumptions. However, detailed modeling of 1D heterogeneity in the sediments shows that Qs cannot be resolved by the Sp data. An independent experiment concerning the amplitude decay of surface waves propagating in the sediments shows that Qs must be generally greater than 80 but is also subject to scattering attenuation. Apparent Q effects seen in direct P and S waves can also be produced by wave tunneling mechanisms in relatively simple 1D heterogeneity. Heterogeneity is a general geophysical attribute of the earth as shown by many high-resolution data sets and should be used as the first litmus test on assumptions made in seismic Q studies before a Q model can be interpreted as an intrinsic material property.

  6. Rhetorical Interpretation of Abstracts in Sci-Tech Theses Based on Burke's Identification Theory

    ERIC Educational Resources Information Center

    Zhong, Jihong

    2017-01-01

    Abstract of a thesis is the brief and accurate representation of the thesis, with the important function of persuading readers to read on the thesis. So how the writer constructs the abstract and wins readers' recognition is our main focus. On the basis of Burke's Identification Theory, this paper analyzed 10 abstracts from "Nature" from…

  7. Seismic detection of the summit magma complex of kilauea volcano, hawaii.

    PubMed

    Thurber, C H

    1984-01-13

    Application of simultaneous inversion of seismic P-wave arrival time data to the investigation of the crust beneath Kilauea Volcano yields a detailed picture of the volcano's heterogeneous structure. Zones of anomalously high seismic velocity are found associated with the volcano's rift zones. A low-velocity zone at shallow depth directly beneath the caldera coincides with an aseismic region interpreted as being the locus of Kilauea's summit magma complex.

  8. A seismic fault recognition method based on ant colony optimization

    NASA Astrophysics Data System (ADS)

    Chen, Lei; Xiao, Chuangbai; Li, Xueliang; Wang, Zhenli; Huo, Shoudong

    2018-05-01

    Fault recognition is an important section in seismic interpretation and there are many methods for this technology, but no one can recognize fault exactly enough. For this problem, we proposed a new fault recognition method based on ant colony optimization which can locate fault precisely and extract fault from the seismic section. Firstly, seismic horizons are extracted by the connected component labeling algorithm; secondly, the fault location are decided according to the horizontal endpoints of each horizon; thirdly, the whole seismic section is divided into several rectangular blocks and the top and bottom endpoints of each rectangular block are considered as the nest and food respectively for the ant colony optimization algorithm. Besides that, the positive section is taken as an actual three dimensional terrain by using the seismic amplitude as a height. After that, the optimal route from nest to food calculated by the ant colony in each block is judged as a fault. Finally, extensive comparative tests were performed on the real seismic data. Availability and advancement of the proposed method were validated by the experimental results.

  9. The New Italian Seismic Hazard Model

    NASA Astrophysics Data System (ADS)

    Marzocchi, W.; Meletti, C.; Albarello, D.; D'Amico, V.; Luzi, L.; Martinelli, F.; Pace, B.; Pignone, M.; Rovida, A.; Visini, F.

    2017-12-01

    In 2015 the Seismic Hazard Center (Centro Pericolosità Sismica - CPS) of the National Institute of Geophysics and Volcanology was commissioned of coordinating the national scientific community with the aim to elaborate a new reference seismic hazard model, mainly finalized to the update of seismic code. The CPS designed a roadmap for releasing within three years a significantly renewed PSHA model, with regard both to the updated input elements and to the strategies to be followed. The main requirements of the model were discussed in meetings with the experts on earthquake engineering that then will participate to the revision of the building code. The activities were organized in 6 tasks: program coordination, input data, seismicity models, ground motion predictive equations (GMPEs), computation and rendering, testing. The input data task has been selecting the most updated information about seismicity (historical and instrumental), seismogenic faults, and deformation (both from seismicity and geodetic data). The seismicity models have been elaborating in terms of classic source areas, fault sources and gridded seismicity based on different approaches. The GMPEs task has selected the most recent models accounting for their tectonic suitability and forecasting performance. The testing phase has been planned to design statistical procedures to test with the available data the whole seismic hazard models, and single components such as the seismicity models and the GMPEs. In this talk we show some preliminary results, summarize the overall strategy for building the new Italian PSHA model, and discuss in detail important novelties that we put forward. Specifically, we adopt a new formal probabilistic framework to interpret the outcomes of the model and to test it meaningfully; this requires a proper definition and characterization of both aleatory variability and epistemic uncertainty that we accomplish through an ensemble modeling strategy. We use a weighting scheme

  10. Reducing Abstraction in High School Computer Science Education: The Case of Definition, Implementation, and Use of Abstract Data Types

    ERIC Educational Resources Information Center

    Sakhnini, Victoria; Hazzan, Orit

    2008-01-01

    The research presented in this article deals with the difficulties and mental processes involved in the definition, implementation, and use of abstract data types encountered by 12th grade advanced-level computer science students. Research findings are interpreted within the theoretical framework of "reducing abstraction" [Hazzan 1999]. The…

  11. Seismic signatures of carbonate caves affected by near-surface absorptions

    NASA Astrophysics Data System (ADS)

    Rao, Ying; Wang, Yanghua

    2015-12-01

    The near-surface absorption within a low-velocity zone generally has an exponential attenuation effect on seismic waves. But how does this absorption affect seismic signatures of karstic caves in deep carbonate reservoirs? Seismic simulation and analysis reveals that, although this near-surface absorption attenuates the wave energy of a continuous reflection, it does not alter the basic kinematic shape of bead-string reflections, a special seismic characteristic associated with carbonate caves in the Tarim Basin, China. Therefore, the bead-strings in seismic profiles can be utilized, with a great certainty, for interpreting the existence of caves within the deep carbonate reservoirs and for evaluating their pore spaces. Nevertheless, the difference between the central frequency and the peak frequency is increased along with the increment in the absorption. While the wave energy of bead-string reflections remains strong, due to the interference of seismic multiples generated by big impedance contrast between the infill materials of a cave and the surrounding carbonate rocks, the central frequency is shifted linearly with respect to the near-surface absorption. These two features can be exploited simultaneously, for a stable attenuation analysis of field seismic data.

  12. Areal distribution of sedimentary facies determined from seismic facies analysis and models of modern depositional systems

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

    Seramur, K.C.; Powell, R.D.; Carpenter, P.J.

    1988-02-01

    Seismic facies analysis was applied to 3.5-kHz single-channel analog reflection profiles of the sediment fill within Muir Inlet, Glacier Bay, southeast Alaska. Nine sedimentary facies have been interpreted from seven seismic facies identified on the profiles. The interpretations are based on reflection characteristics and structural features of the seismic facies. The following reflection characteristics and structural features are used: reflector spacing, amplitude and continuity of reflections, internal reflection configurations, attitude of reflection terminations at a facies boundary, body geometry of a facies, and the architectural associations of seismic facies within each basin. The depositional systems are reconstructed by determining themore » paleotopography, bedding patterns, sedimentary facies, and modes of deposition within the basin. Muir Inlet is a recently deglaciated fjord for which successive glacier terminus positions and consequent rates of glacial retreat are known. In this environment the depositional processes and sediment characteristics vary with distance from a glacier terminus, such that during a retreat a record of these variations is preserved in the aggrading sediment fill. Sedimentary facies within the basins of lower Muir Inlet are correlated with observed depositional processes near the present glacier terminus in the upper inlet. The areal distribution of sedimentary facies within the basins is interpreted using the seismic facies architecture and inferences from known sediment characteristics proximal to present glacier termini.« less

  13. Low-frequency seismic events in a wider volcanological context

    NASA Astrophysics Data System (ADS)

    Neuberg, J. W.; Collombet, M.

    2006-12-01

    Low-frequency seismic events have been in the centre of attention for several years, particularly on volcanoes with highly viscous magmas. The ultimate aim is to detect changes in volcanic activity by identifying changes in the seismic behaviour in order to forecast an eruption, or in case of an ongoing eruption, forecast the short and longterm behaviour of the volcanic system. A major boost in recent years arose through several attempts of multi-parameter volcanic monitoring and modelling programs, which allowed multi-disciplinary groups of volcanologists to interpret seismic signals together with, e.g. ground deformation, stress field analysis and petrological information. This talk will give several examples of such multi-disciplinary projects, focussing on the joint modelling of seismic source processes for low-frequency events together with advanced magma flow models, and the signs of magma movement in the deformation and stress field at the surface.

  14. Seismic Risk Studies in the United States.

    ERIC Educational Resources Information Center

    Algermissen, S.T.

    A new seismic risk map of the United States is presented, along with strain release and maximum Modified Mercalli intesity maps of the country. Frequency of occurrence of damaging earthquakes was not considered in zone ratings, but included frequency studies may aid interpretation. Discussion of methods is included with review of calculations. (MH)

  15. A 3D seismic investigation of the Ray Gas Storage Reef in Macomb County, Michigan

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

    Schaefer, S.F.; Dixon, R.A.

    1995-09-01

    A 4.2 square mile 3D seismic survey was acquired over the Ray Niagaran Reef Gas Storage Field in southeast Michigan as part of a program to maximize storage capacity and gas deliverability of the field. Goals of the survey were: (1) to determine if additional storage capacity could be found, either as extensions to the main reef or as undiscovered satellite reefs, (2) to determine if 3D seismic data can be utilized to quantify reservoir parameters in order to maximize the productive capacity of infill wells, and (3) to investigate the relationship between the main reef body and a lowmore » relief/flow volume gas well east of the reef. Interpretation of the 3D seismic data resulted in a detailed image of the reef, using several interpretive techniques. A seismic reflection within the reef was correlated with a known porosity zone, and the relationship between porosity and seismic amplitude was investigated. A possible connection between the main reef and the low relief gas well was identified. This project illustrates the economic value of investigating an existing storage reef with 3D seismic data, and underscores the necessity of acquiring such a survey prior to developing a new storage reservoir.« less

  16. Why style matters - uncertainty and structural interpretation in thrust belts.

    NASA Astrophysics Data System (ADS)

    Butler, Rob; Bond, Clare; Watkins, Hannah

    2016-04-01

    Structural complexity together with challenging seismic imaging make for significant uncertainty in developing geometric interpretations of fold and thrust belts. Here we examine these issues and develop more realistic approaches to building interpretations. At all scales, the best tests of the internal consistency of individual interpretations come from structural restoration (section balancing), provided allowance is made for heterogeneity in stratigraphy and strain. However, many existing balancing approaches give misleading perceptions of interpretational risk - both on the scale of individual fold-thrust (trap) structures and in regional cross-sections. At the trap-scale, idealised models are widely cited - fault-bend-fold, fault-propagation folding and trishear. These make entirely arbitrary choices for fault localisation and layer-by-layer deformation: precise relationships between faults and fold geometry are generally invalidated by real-world conditions of stratigraphic variation and distributed strain. Furthermore, subsurface predictions made using these idealisations for hydrocarbon exploration commonly fail the test of drilling. Rarely acknowledged, the geometric reliability of seismic images depends on the assigned seismic velocity model, which in turn relies on geological interpretation. Thus iterative approaches are required between geology and geophysics. The portfolio of commonly cited outcrop analogues is strongly biased to examples that simply conform to idealised models - apparently abnormal structures are rarely described - or even photographed! Insight can come from gravity-driven deep-water fold-belts where part of the spectrum of fold-thrust complexity is resolved through seismic imaging. This imagery shows deformation complexity in fold forelimbs and backlimbs. However, the applicability of these, weakly lithified systems to well-lithified successions (e.g. carbonates) of many foreland thrust belts remains conjectural. Examples of

  17. Pennsylvanian Tyler stratigraphic seismic concepts

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

    Moore, C.E.; Archer, R.J.

    Recent drilling in the Rattler Butte area of central Montana has renewed interest in the Pennsylvanian Tyler Formation as a drilling objective. New production in this area, coupled with the surrounding well density, provides an ideal situation for further development of Tyler stratigraphic-seismic exploration concepts and methods. Both geologic and geophysical Tyler thickness maps have proven to be useful tools in delineating eroded Heath and subsequent lower Tyler deposition. Seismic modeling has revealed a series of possible Tyler-Heath erosional edge characteristics, providing another tool for Tyler-Heath boundary definition. In modeling specific seismic sand signatures, it was found that seismic charactermore » and amplitude are dependent upon both formation thickness and lithology. Detailed mapping of the study area also revealed a new environmental interpretation of the Tyler. Unlike the fluvial system to the north, the Tyler regime in the Rattler Butte area appears to have fluctuated among fluvial, deltaic, and marine systems. Two hydrocarbon occurrence patterns have been noted within the Tyler: (1) although reservoir quality sands are present throughout the Tyler, those within the lower Tyler are more likely to contain hydrocarbons, and (2) close proximity to the Tyler-Heath erosional edge increases the chances of discovering oil-filled Tyler sands. Combined use of these exploration tools should greatly enhance the chances for successful lower Tyler exploration.« less

  18. Saudi Arabian seismic-refraction profile: A traveltime interpretation of crustal and upper mantle structure

    USGS Publications Warehouse

    Mooney, W.D.; Gettings, M.E.; Blank, H.R.; Healy, J.H.

    1985-01-01

    The crustal and upper mantle compressional-wave velocity structure across the southwestern Arabian Shield has been investigated by a 1000-km-long seismic refraction profile. The profile begins in Mesozoic cover rocks near Riyadh on the Arabian Platform, trends southwesterly across three major Precambrian tectonic provinces, traverses Cenozoic rocks of the coastal plain near Jizan, and terminates at the outer edge of the Farasan Bank in the southern Red Sea. More than 500 surveyed recording sites were occupied, and six shot points were used, including one in the Red Sea. Two-dimensional ray-tracing techniques, used to analyze amplitude-normalized record sections indicate that the Arabian Shield is composed, to first order, of two layers, each about 20 km thick, with average velocities of about 6.3 km/s and 7.0 km/s, respectively. West of the Shield-Red Sea margin, the crust thins to a total thickness of less than 20 km, beyond which the Red Sea shelf and coastal plain are interpreted to be underlain by oceanic crust. A major crustal inhomogeneity at the northeast end of the profile probably represents the suture zone between two crustal blocks of different composition. Elsewhere along the profile, several high-velocity anomalies in the upper crust correlate with mapped gneiss domes, the most prominent of which is the Khamis Mushayt gneiss. Based on their velocities, these domes may constitute areas where lower crustal rocks have been raised some 20 km. Two intracrustal reflectors in the center of the Shield at 13 km depth probably represent the tops of mafic intrusives. The Mohorovic??ic?? discontinuity beneath the Shield varies from a depth of 43 km and mantle velocity of 8.2 km/s in the northeast to a depth of 38 km and mantle velocity of 8.0 km/s depth in the southwest near the Shield-Red Sea transition. Two velocity discontinuities occur in the upper mantle, at 59 and 70 km depth. The crustal and upper mantle velocity structure of the Arabian Shield is

  19. Structure of the Wagner Basin in the Northern Gulf of California From Interpretation of Seismic Reflexion Data

    NASA Astrophysics Data System (ADS)

    Gonzalez, M.; Aguilar, C.; Martin, A.

    2007-05-01

    The northern Gulf of California straddles the transition in the style of deformation along the Pacific-North America plate boundary, from distributed deformation in the Upper Delfin and Wagner basins to localized dextral shear along the Cerro Prieto transform fault. Processing and interpretation of industry seismic data adquired by Petroleos Mexicanos (PEMEX) allow us to map the main fault structures and depocenters in the Wagner basin and to unravel the way strain is transferred northward into the Cerro Prieto fault system. Seismic data records from 0.5 to 5 TWTT. Data stacking and time-migration were performed using semblance coefficient method. Subsidence in the Wagner basin is controlled by two large N-S trending sub-parallel faults that intersect the NNW-trending Cerro Prieto transform fault. The Wagner fault bounds the eastern margin of the basin for more than 75 km. This fault dips ~50° to the west (up to 2 seconds) with distinctive reflectors displaced more than 1 km across the fault zone. The strata define a fanning pattern towards the Wagner fault. Northward the Wagner fault intersects the Cerro Prieto fault at 130° on map view and one depocenter of the Wagner basin bends to the NW adjacent to the Cerro Prieto fault zone. The eastern boundary of the modern depocenter is the Consag fault, which extends over 100 km in a N-S direction with an average dip of ~50° (up to 2s) to the east. The northern segment of the Consag fault bends 25° and intersects the Cerro Prieto fault zone at an angle of 110° on map view. The acoustic basement was not imaged in the northwest, but the stratigraphic succession increases its thickness towards the depocenter of the Wagner basin. Another important structure is El Chinero fault, which runs parallel to the Consag fault along 60 km and possibly intersects the Cerro Prieto fault to the north beneath the delta of the Colorado River. El Chinero fault dips at low-angle (~30°) to the east and has a vertical offset of about 0

  20. Finite-Difference Modeling of Seismic Reflection Data in a Hard Rock Environment: An Example from the Mineralized Otago Schist, New Zealand

    NASA Astrophysics Data System (ADS)

    Leslie, A.; Gorman, A. R.

    2004-12-01

    The interpretation of seismic reflection data in non-sedimentary environments is problematic. In the Macraes Flat region near Dunedin (South Island, New Zealand), ongoing mining of mineralized schist has prompted the development of a seismic interpretation scheme that is capable of imaging a gold-bearing shear zone and associated mineralized structures accurately to the meter scale. The anisotropic and complex structural nature of this geological environment necessitates a cost-effective computer-based modeling technique that can provide information on the physical characteristics of the schist. Such a method has been tested on seismic data acquired in 1993 over a region that has since been excavated and logged. Correlation to measured structural data permits a direct comparison between the seismic data and the actual geology. Synthetic modeling utilizes a 2D visco-elastic finite difference routine to constrain the interpretation of observed seismic characteristics, including the velocity, anisotropy, and contrast, of the shear zone structures. Iterative refinements of the model result in a more representative synthetic model that most closely matches the seismic response. The comparison between the actual and synthetic seismic sections provides promising results that will be tested by new data acquisition over the summer of 2004/2005 to identify structures and zones of potential mineralization. As a downstream benefit, this research could also contribute to earthquake risk assessment analyses at active faults with similar characteristics.

  1. Updated Tomographic Seismic Imaging at Kilauea Volcano, Hawaii

    NASA Astrophysics Data System (ADS)

    Okubo, P.; Johnson, J.; Felts, E. S.; Flores, N.

    2013-12-01

    Improved and more detailed geophysical, geological, and geochemical observations and measurements at Kilauea, along with prolonged eruptions at its summit caldera and east rift zone, are encouraging more ambitious interpretation and modeling of volcanic processes over a range of temporal and spatial scales. We are updating three-dimensional models of seismic wave-speed distributions within Kilauea using local earthquake arrival time tomography to support waveform-based modeling of seismic source mechanisms. We start from a tomographic model derived from a combination of permanent seismic stations comprising the Hawaiian Volcano Observatory (HVO) seismographic network and a dense deployment of temporary stations in the Kilauea caldera region in 1996. Using P- and S-wave arrival times measured from the HVO network for local earthquakes from 1997 through 2012, we compute velocity models with the finite difference tomographic seismic imaging technique implemented by Benz and others (1996), and applied to numerous volcanoes including Kilauea. Particular impetus to our current modeling was derived from a focused effort to review seismicity occurring in Kilauea's summit caldera and adjoining regions in 2012. Our results reveal clear P-wave low-velocity features at and slightly below sea level beneath Kilauea's summit caldera, lying between Halemaumau Crater and the north-facing scarps that mark the southern caldera boundary. The results are also suggestive of changes in seismic velocity distributions between 1996 and 2012. One example of such a change is an apparent decrease in the size and southeastward extent, compared to the earlier model, of the low VP feature imaged with the more recent data. However, we recognize the distinct possibility that these changes are reflective of differences in earthquake and seismic station distributions in the respective datasets, and we need to further populate the more recent HVO seismicity catalogs to possibly address this concern

  2. Lithospheric Models of the Middle East to Improve Seismic Source Parameter Determination/Event Location Accuracy

    DTIC Science & Technology

    2012-09-01

    State Award Nos. DE-AC52-07NA27344/24.2.3.2 and DOS_SIAA-11-AVC/NMA-1 ABSTRACT The Middle East is a tectonically complex and seismically...active region. The ability to accurately locate earthquakes and other seismic events in this region is complicated by tectonics , the uneven...and seismic source parameters show that this activity comes from tectonic events. This work is informed by continuous or event-based regional

  3. Developing Creativity and Abstraction in Representing Data

    ERIC Educational Resources Information Center

    South, Andy

    2012-01-01

    Creating charts and graphs is all about visual abstraction: the process of representing aspects of data with imagery that can be interpreted by the reader. Children may need help making the link between the "real" and the image. This abstraction can be achieved using symbols, size, colour and position. Where the representation is close to what…

  4. Bed load transport and boundary roughness changes as competing causes of hysteresis in the relationship between river discharge and seismic amplitude recorded near a steep mountain stream

    NASA Astrophysics Data System (ADS)

    Roth, Danica L.; Finnegan, Noah J.; Brodsky, Emily E.; Rickenmann, Dieter; Turowski, Jens M.; Badoux, Alexandre; Gimbert, Florent

    2017-05-01

    Hysteresis in the relationship between bed load transport and river stage is a well-documented phenomenon with multiple known causes. Consequently, numerous studies have interpreted hysteresis in the relationship between seismic ground motion near rivers and some measure of flow strength (i.e., discharge or stage) as the signature of bed load transport. Here we test this hypothesis in the Erlenbach stream (Swiss Prealps) using a metric to quantitatively compare hysteresis in seismic data with hysteresis recorded by geophones attached beneath steel plates within the streambed, a well-calibrated proxy for direct sediment transport measurements. We find that while both the geophones and seismometers demonstrate hysteresis, the magnitude and direction of hysteresis are not significantly correlated between these data, indicating that the seismic signal at this site is primarily reflecting hysteresis in processes other than sediment transport. Seismic hysteresis also does not correlate significantly with the magnitude of sediment transport recorded by the geophones, contrary to previous studies' assumptions. We suggest that hydrologic sources and changes in water turbulence, for instance due to evolving boundary conditions at the bed, rather than changes in sediment transport rates, may sometimes contribute to or even dominate the hysteresis observed in seismic amplitudes near steep mountain rivers.<abstract type="synopsis">Plain Language SummaryAn increasing number of studies have recently observed changes in the amount of <span class="hlt">seismic</span> shaking (hysteresis) recorded near a river at a given discharge during floods. Most studies have assumed that this hysteresis was caused by changes in the amount of sediment being transported in the river and have therefore used the hysteresis to assess sediment transport rates and patterns. We examine concurrent <span class="hlt">seismic</span> and sediment transport data from a steep mountain stream in the Swiss Prealps and find that changes in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009PhDT.......237S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009PhDT.......237S"><span>Attenuation and velocity dispersion in the exploration <span class="hlt">seismic</span> frequency band</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Langqiu</p> <p></p> <p>In an anelastic medium, <span class="hlt">seismic</span> waves are distorted by attenuation and velocity dispersion, which depend on petrophysical properties of reservoir rocks. The effective attenuation and velocity dispersion is a combination of intrinsic attenuation and apparent attenuation due to scattering, transmission response, and data acquisition system. Velocity dispersion is usually neglected in <span class="hlt">seismic</span> data processing partly because of insufficient observations in the exploration <span class="hlt">seismic</span> frequency band. This thesis investigates the methods of measuring velocity dispersion in the exploration <span class="hlt">seismic</span> frequency band and <span class="hlt">interprets</span> the velocity dispersion data in terms of petrophysical properties. Broadband, uncorrelated vibrator data are suitable for measuring velocity dispersion in the exploration <span class="hlt">seismic</span> frequency band, and a broad bandwidth optimizes the observability of velocity dispersion. Four methods of measuring velocity dispersion in uncorrelated vibrator VSP data are investigated, which are the sliding window crosscorrelation (SWCC) method, the instantaneous phase method, the spectral decomposition method, and the cross spectrum method. Among them, the SWCC method is a new method and has satisfactory robustness, accuracy, and efficiency. Using the SWCC method, velocity dispersion is measured in the uncorrelated vibrator VSP data from three areas with different geological settings, i.e., Mallik gas hydrate zone, McArthur River uranium mines, and Outokumpu crystalline rocks. The observed velocity dispersion is fitted to a straight line with respect to log frequency for a constant (frequency-independent) Q value. This provides an alternative method for calculating Q. A constant Q value does not directly link to petrophysical properties. A modeling study is implemented for the Mallik and McArthur River data to <span class="hlt">interpret</span> the velocity dispersion observations in terms of petrophysical properties. The detailed multi-parameter petrophysical reservoir models are built according to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.728....1A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.728....1A"><span>Deep structure of the continental margin and basin off Greater Kabylia, Algeria - New insights from wide-angle <span class="hlt">seismic</span> data modeling and multichannel <span class="hlt">seismic</span> <span class="hlt">interpretation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aïdi, Chafik; Beslier, Marie-Odile; Yelles-Chaouche, Abdel Karim; Klingelhoefer, Frauke; Bracene, Rabah; Galve, Audrey; Bounif, Abdallah; Schenini, Laure; Hamai, Lamine; Schnurle, Philippe; Djellit, Hamou; Sage, Françoise; Charvis, Philippe; Déverchère, Jacques</p> <p>2018-03-01</p> <p>During the Algerian-French SPIRAL survey aimed at investigating the deep structure of the Algerian margin and basin, two coincident wide-angle and reflection <span class="hlt">seismic</span> profiles were acquired in central Algeria, offshore Greater Kabylia, together with gravimetric, bathymetric and magnetic data. This 260 km-long offshore-onshore profile spans the Balearic basin, the central Algerian margin and the Greater Kabylia block up to the southward limit of the internal zones onshore. Results are obtained from modeling and <span class="hlt">interpretation</span> of the combined data sets. The Algerian basin offshore Greater Kabylia is floored by a thin oceanic crust ( 4 km) with P-wave velocities ranging between 5.2 and 6.8 km/s. In the northern Hannibal High region, the atypical 3-layer crustal structure is <span class="hlt">interpreted</span> as volcanic products stacked over a thin crust similar to that bordering the margin and related to Miocene post-accretion volcanism. These results support a two-step back-arc opening of the west-Algerian basin, comprising oceanic crust accretion during the first southward stage, and a magmatic and probably tectonic reworking of this young oceanic basement during the second, westward, opening phase. The structure of the central Algerian margin is that of a narrow ( 70 km), magma-poor rifted margin, with a wider zone of distal thinned continental crust than on the other margin segments. There is no evidence for mantle exhumation in the sharp ocean-continent transition, but transcurrent movements during the second opening phase may have changed its initial geometry. The Plio-Quaternary inversion of the margin related to ongoing convergence between Africa and Eurasia is expressed by a blind thrust system under the margin rising toward the surface at the slope toe, and by an isostatic disequilibrium resulting from opposite flexures of two plates decoupled at the continental slope. This disequilibrium is likely responsible for the peculiar asymmetrical shape of the crustal neck that may thus</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SolE....7..685B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SolE....7..685B"><span>Characterization of a complex near-surface structure using well logging and passive <span class="hlt">seismic</span> measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benjumea, Beatriz; Macau, Albert; Gabàs, Anna; Figueras, Sara</p> <p>2016-04-01</p> <p>We combine geophysical well logging and passive <span class="hlt">seismic</span> measurements to characterize the near-surface geology of an area located in Hontomin, Burgos (Spain). This area has some near-surface challenges for a geophysical study. The irregular topography is characterized by limestone outcrops and unconsolidated sediments areas. Additionally, the near-surface geology includes an upper layer of pure limestones overlying marly limestones and marls (Upper Cretaceous). These materials lie on top of Low Cretaceous siliciclastic sediments (sandstones, clays, gravels). In any case, a layer with reduced velocity is expected. The geophysical data sets used in this study include sonic and gamma-ray logs at two boreholes and passive <span class="hlt">seismic</span> measurements: three arrays and 224 <span class="hlt">seismic</span> stations for applying the horizontal-to-vertical amplitude spectra ratio method (H/V). Well-logging data define two significant changes in the P-wave-velocity log within the Upper Cretaceous layer and one more at the Upper to Lower Cretaceous contact. This technique has also been used for refining the geological <span class="hlt">interpretation</span>. The passive <span class="hlt">seismic</span> measurements provide a map of sediment thickness with a maximum of around 40 m and shear-wave velocity profiles from the array technique. A comparison between <span class="hlt">seismic</span> velocity coming from well logging and array measurements defines the resolution limits of the passive <span class="hlt">seismic</span> techniques and helps it to be <span class="hlt">interpreted</span>. This study shows how these low-cost techniques can provide useful information about near-surface complexity that could be used for designing a geophysical field survey or for <span class="hlt">seismic</span> processing steps such as statics or imaging.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/869651','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/869651"><span><span class="hlt">Seismic</span> event classification system</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Dowla, Farid U.; Jarpe, Stephen P.; Maurer, William</p> <p>1994-01-01</p> <p>In the computer <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> data, the critical first step is to identify the general class of an unknown event. For example, the classification might be: teleseismic, regional, local, vehicular, or noise. Self-organizing neural networks (SONNs) can be used for classifying such events. Both Kohonen and Adaptive Resonance Theory (ART) SONNs are useful for this purpose. Given the detection of a <span class="hlt">seismic</span> event and the corresponding signal, computation is made of: the time-frequency distribution, its binary representation, and finally a shift-invariant representation, which is the magnitude of the two-dimensional Fourier transform (2-D FFT) of the binary time-frequency distribution. This pre-processed input is fed into the SONNs. These neural networks are able to group events that look similar. The ART SONN has an advantage in classifying the event because the types of cluster groups do not need to be pre-defined. The results from the SONNs together with an expert seismologist's classification are then used to derive event classification probabilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013CG.....59...60B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013CG.....59...60B"><span>Spatial pattern recognition of <span class="hlt">seismic</span> events in South West Colombia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benítez, Hernán D.; Flórez, Juan F.; Duque, Diana P.; Benavides, Alberto; Lucía Baquero, Olga; Quintero, Jiber</p> <p>2013-09-01</p> <p>Recognition of seismogenic zones in geographical regions supports <span class="hlt">seismic</span> hazard studies. This recognition is usually based on visual, qualitative and subjective analysis of data. Spatial pattern recognition provides a well founded means to obtain relevant information from large amounts of data. The purpose of this work is to identify and classify spatial patterns in instrumental data of the South West Colombian <span class="hlt">seismic</span> database. In this research, clustering tendency analysis validates whether <span class="hlt">seismic</span> database possesses a clustering structure. A non-supervised fuzzy clustering algorithm creates groups of <span class="hlt">seismic</span> events. Given the sensitivity of fuzzy clustering algorithms to centroid initial positions, we proposed a methodology to initialize centroids that generates stable partitions with respect to centroid initialization. As a result of this work, a public software tool provides the user with the routines developed for clustering methodology. The analysis of the seismogenic zones obtained reveals meaningful spatial patterns in South-West Colombia. The clustering analysis provides a quantitative location and dispersion of seismogenic zones that facilitates seismological <span class="hlt">interpretations</span> of <span class="hlt">seismic</span> activities in South West Colombia.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGP23C..04F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGP23C..04F"><span>Joint <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> tomography and new magnetotelluric results provide evidence for support of high topography in the Southern Rocky Mountains and High Plains of eastern Colorado, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feucht, D. W.; Sheehan, A. F.; Bedrosian, P.</p> <p>2015-12-01</p> <p>A recent magnetotelluric (MT) survey in central Colorado, USA, when <span class="hlt">interpreted</span> alongside existing <span class="hlt">seismic</span> tomography, reveals potential mechanisms of support for high topography both regionally and locally. Broadband and long period magnetotelluric data were collected at twenty-three sites along a 330 km E-W profile across the Southern Rocky Mountains and High Plains of central North America as part of the Deep RIFT Electrical Resistivity (DRIFTER) experiment. Remote-reference data processing yielded high quality MT data over a period range of 100 Hz to 10,000 seconds. A prominent feature of the regional geo-electric structure is the Denver Basin, which contains a thick package of highly conductive shales and porous sandstone aquifers. One-dimensional forward modeling was performed on stations within the Denver Basin to estimate depth to the base of this shallow conductor. Those estimates were then used to place a horizontal penalty cut in the model mesh of a regularized two-dimensional inversion. Two-dimensional modeling of the resistivity structure reveals two major anomalous regions in the lithosphere: 1) a high conductivity region in the crust under the tallest peaks of the Rocky Mountains and 2) a lateral step increase in lithospheric resistivity beneath the plains. The Rocky Mountain crustal anomaly coincides with low <span class="hlt">seismic</span> wave speeds and enhanced heat flow and is thus <span class="hlt">interpreted</span> as evidence of partial melt and/or high temperature fluids emplaced in the crust by tectonic activity along the Rio Grande Rift. The lateral variation in the mantle lithosphere, while co-located with a pronounced step increase in <span class="hlt">seismic</span> velocity, appears to be a gradational boundary in resistivity across eastern Colorado and could indicate a small degree of compositional modification at the edge of the North American craton. These inferred conductivity mechanisms, namely crustal melt and modification of mantle lithosphere, likely contribute to high topography locally in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSMNS32A..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSMNS32A..01M"><span><span class="hlt">Seismic</span> site survey investigations in urban environments: The case of the underground metro project in Copenhagen, Denmark.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martínez, K.; Mendoza, J. A.; Colberg-Larsen, J.; Ploug, C.</p> <p>2009-05-01</p> <p>Near surface geophysics applications are gaining more widespread use in geotechnical and engineering projects. The development of data acquisition, processing tools and <span class="hlt">interpretation</span> methods have optimized survey time, reduced logistics costs and increase results reliability of <span class="hlt">seismic</span> surveys during the last decades. However, the use of wide-scale geophysical methods under urban environments continues to face great challenges due to multiple noise sources and obstacles inherent to cities. A <span class="hlt">seismic</span> pre-investigation was conducted to investigate the feasibility of using <span class="hlt">seismic</span> methods to obtain information about the subsurface layer locations and media properties in Copenhagen. Such information is needed for hydrological, geotechnical and groundwater modeling related to the Cityringen underground metro project. The pre-investigation objectives were to validate methods in an urban environment and optimize field survey procedures, processing and <span class="hlt">interpretation</span> methods in urban settings in the event of further <span class="hlt">seismic</span> investigations. The geological setting at the survey site is characterized by several interlaced layers of clay, till and sand. These layers are found unevenly distributed throughout the city and present varying thickness, overlaying several different unit types of limestone at shallow depths. Specific results objectives were to map the bedrock surface, ascertain a structural geological framework and investigate bedrock media properties relevant to the construction design. The <span class="hlt">seismic</span> test consisted of a combined <span class="hlt">seismic</span> reflection and refraction analyses of a profile line conducted along an approximately 1400 m section in the northern part of Copenhagen, along the projected metro city line. The data acquisition was carried out using a 192 channels array, receiver groups with 5 m spacing and a Vibroseis as a source at 10 m spacing. Complementarily, six vertical <span class="hlt">seismic</span> profiles (VSP) were performed at boreholes located along the line. The reflection</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982cost.rept...43P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982cost.rept...43P"><span>Foraminiferal and <span class="hlt">seismic</span> stratigraphy, paleoenvironments and depositional cycles in the Georges Bank Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poag, C. W.</p> <p></p> <p>Biostratigraphic analyses of foraminiferal assemblages sampled from rotary cuttings taken at 10 ft to 90 ft intervals were used with <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> sequences to determine the presence of nonconformities and to establish a chronostratigraphic framework for COST G-1 and G-2 wells. The chronostratigraphic sequences were then used to calculate sediment accumulation rates. Lithostratigraphic and chronostratigraphic units were compared with those of the Scotian Basin of Canada, and correlations were established between the COST G-2 and the Shell Mohican L-100 wells. Paleoenvironmental analysis was based on the microfossil record of the G-1 and G-2 wells and on <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> facies along USGS multichannel line 19.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.8023T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.8023T"><span>Romanian Educational <span class="hlt">Seismic</span> Network Project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tataru, Dragos; Ionescu, Constantin; Zaharia, Bogdan; Grecu, Bogdan; Tibu, Speranta; Popa, Mihaela; Borleanu, Felix; Toma, Dragos; Brisan, Nicoleta; Georgescu, Emil-Sever; Dobre, Daniela; Dragomir, Claudiu-Sorin</p> <p>2013-04-01</p> <p>Romania is one of the most active <span class="hlt">seismic</span> countries in Europe, with more than 500 earthquakes occurring every year. The <span class="hlt">seismic</span> hazard of Romania is relatively high and thus understanding the earthquake phenomena and their effects at the earth surface represents an important step toward the education of population in earthquake affected regions of the country and aims to raise the awareness about the earthquake risk and possible mitigation actions. In this direction, the first national educational project in the field of seismology has recently started in Romania: the ROmanian EDUcational <span class="hlt">SEISmic</span> NETwork (ROEDUSEIS-NET) project. It involves four partners: the National Institute for Earth Physics as coordinator, the National Institute for Research and Development in Construction, Urban Planning and Sustainable Spatial Development " URBAN - INCERC" Bucharest, the Babeş-Bolyai University (Faculty of Environmental Sciences and Engineering) and the software firm "BETA Software". The project has many educational, scientific and social goals. The main educational objectives are: training students and teachers in the analysis and <span class="hlt">interpretation</span> of seismological data, preparing of several comprehensive educational materials, designing and testing didactic activities using informatics and web-oriented tools. The scientific objective is to introduce into schools the use of advanced instruments and experimental methods that are usually restricted to research laboratories, with the main product being the creation of an earthquake waveform archive. Thus a large amount of such data will be used by students and teachers for educational purposes. For the social objectives, the project represents an effective instrument for informing and creating an awareness of the <span class="hlt">seismic</span> risk, for experimentation into the efficacy of scientific communication, and for an increase in the direct involvement of schools and the general public. A network of nine <span class="hlt">seismic</span> stations with SEP seismometers</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..300a2065P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..300a2065P"><span><span class="hlt">Seismic</span> Evaluation of A Historical Structure In Kastamonu - Turkey</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pınar, USTA; Işıl ÇARHOĞLU, Asuman; EVCİ, Ahmet</p> <p>2018-01-01</p> <p>The Kastomonu province is a <span class="hlt">seismically</span> active zone. the city has many historical buildings made of stone-masonry. In case of any probable future earthquakes, existing buildings may suffer substantial or heavy damages. In the present study, one of the historical traditional house located in Kastamonu were structurally investigated through probabilistic <span class="hlt">seismic</span> risk assessment methodology. In the study, the building was modeled by using the Finite Element Modeling (FEM) software, SAP2000. Time history analyses were carried out using 10 different ground motion data on the FEM models. Displacements were <span class="hlt">interpreted</span>, and the results were displayed graphically and discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhDT........64Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT........64Z"><span><span class="hlt">Seismic</span> imaging and hydrogeologic characterization of the Potomac Formation in northern New Castle County, Delaware</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zullo, Claudia Cristina</p> <p></p> <p> short distances, contrary to correlations in previous studies that have indicated connection of sands at distances of at least 3 km. The results highlight the importance of integrating multiple sources of geologic information for the <span class="hlt">interpretation</span> of the stratigraphic architecture of non-marine sediments, and the value of roadway-based land-streamer <span class="hlt">seismic</span> data for the <span class="hlt">interpretation</span> of near-surface (less than 300-m-depth) aquifer sand characteristics in developed areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994Tectp.232..309L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994Tectp.232..309L"><span>The nature of crustal boundaries: combined <span class="hlt">interpretation</span> of wide-angle and normal-incidence <span class="hlt">seismic</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>Long, Roger E.; Matthews, Patricia A.; Graham, Daniel P.</p> <p>1994-04-01</p> <p>After a few seconds two-way traveltime, normal-incidence <span class="hlt">seismic</span> reflection sections are composed mainly of assemblages of short reflections. Very rarely are seen continuous reflections that might correspond to the Moho or a mid-crustal discontinuity. The inferred continuity of these boundaries has traditionally come from refraction seismology. There is now a body of high quality, coincident wide-angle and normal-incidence <span class="hlt">seismic</span> data that have been recorded with 50-100 m shot spacing and with high frequency sources (e.g. MOBIL, BABEL). The complexity and characteristics of the wide-angle arrivals seen on these data suggest that they do not originate from continuous boundaries. It is suggested that these arrivals are reflections from the same assemblage of short length reflectors that are responsible for normal-incidence reflections. <span class="hlt">Seismic</span> velocities below the middle crust may (1) change corresponding to normal-incidence reflectivity, or (2) generally increase with depth with localised sills or lens structures of different velocity accounting for the observed reflections. Wide-angle arrivals that have traditionally been identified as reflections from crustal boundaries (e.g. the mid-crust and Moho) and which were considered indicative of a sharp velocity discontinuity from continuous boundaries, may instead result from a concentration of lamellae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAG...136..298D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAG...136..298D"><span>Comparison between deterministic and statistical wavelet estimation methods through predictive deconvolution: <span class="hlt">Seismic</span> to well tie example from the North Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Macedo, Isadora A. S.; da Silva, Carolina B.; de Figueiredo, J. J. S.; Omoboya, Bode</p> <p>2017-01-01</p> <p>Wavelet estimation as well as <span class="hlt">seismic</span>-to-well tie procedures are at the core of every <span class="hlt">seismic</span> <span class="hlt">interpretation</span> workflow. In this paper we perform a comparative study of wavelet estimation methods for <span class="hlt">seismic</span>-to-well tie. Two approaches to wavelet estimation are discussed: a deterministic estimation, based on both <span class="hlt">seismic</span> and well log data, and a statistical estimation, based on predictive deconvolution and the classical assumptions of the convolutional model, which provides a minimum-phase wavelet. Our algorithms, for both wavelet estimation methods introduce a semi-automatic approach to determine the optimum parameters of deterministic wavelet estimation and statistical wavelet estimation and, further, to estimate the optimum <span class="hlt">seismic</span> wavelets by searching for the highest correlation coefficient between the recorded trace and the synthetic trace, when the time-depth relationship is accurate. Tests with numerical data show some qualitative conclusions, which are probably useful for <span class="hlt">seismic</span> inversion and <span class="hlt">interpretation</span> of field data, by comparing deterministic wavelet estimation and statistical wavelet estimation in detail, especially for field data example. The feasibility of this approach is verified on real <span class="hlt">seismic</span> and well data from Viking Graben field, North Sea, Norway. Our results also show the influence of the washout zones on well log data on the quality of the well to <span class="hlt">seismic</span> tie.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MsT..........7A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MsT..........7A"><span>3D <span class="hlt">seismic</span> attribute expressions of deep offshore Niger Delta</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anyiam, Uzonna Okenna</p> <p></p> <p>Structural and stratigraphic <span class="hlt">interpretation</span> of 3D <span class="hlt">seismic</span> data for reservoir characterization in an area affected by dense faulting, such as the Niger Delta, is typically difficult and strongly model driven because of problems with imaging. In the Freeman field, located about 120km offshore southwestern Niger Delta at about 1300m water depth, 3D <span class="hlt">seismic</span> attribute-based analogs, and structural and stratigraphic based geometric models are combined to help enhance and constrain the <span class="hlt">interpretation</span>. The objectives being to show how 3D <span class="hlt">seismic</span> attribute analysis enhances <span class="hlt">seismic</span> <span class="hlt">interpretation</span>, develop structural style and stratigraphic architecture models and identify trap mechanisms in the study area; with the main purpose of producing structural and stratigraphic framework analogs to aid exploration and production companies, as well as researchers in better understanding the structural style, stratigraphic framework and trap mechanism of the Miocene to Pliocene Agbada Formation reservoirs in the deep Offshore Niger Delta Basin. A multidisciplinary approach which involved analyses of calculated variance-based coherence cube, spectral decomposition box probe and root-mean-square amplitude attributes, sequence stratigraphy based well correlation, and structural modeling; were undertaken to achieve these objectives. Studies reveal a massive northwest-southeast trending shale cored detachment fold anticline, with associated normal faults; <span class="hlt">interpreted</span> to have been folded and faulted by localized compression resulting from a combination of differential loading on the deep-seated overpressured-ductile-undercompacted-marine Akata shale, and gravitational collapse of the Niger delta continental slope due to influx of sediments. Crestal extension resulting from this localized compression, is believed to have given rise to the synthetic, antithetic and newly observed crossing conjugate normal faults in the study area. This structure is unique to the existing types of principal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5572387-seismic-lateral-prediction-chalky-limestone-reservoirs-offshore-qatar','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5572387-seismic-lateral-prediction-chalky-limestone-reservoirs-offshore-qatar"><span><span class="hlt">Seismic</span> lateral prediction in chalky limestone reservoirs offshore Qatar</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>Rubbens, I.B.H.M.; Murat, R.C.; Vankeulen, J.</p> <p></p> <p>Following the discovery of non-structurally trapped oil accumulations in Cretaceous chalky reservoirs on the northern flank of the North Dome offshore QATAR, a <span class="hlt">seismic</span> lateral prediction study was carried out for QATAR GENERAL PETROLEUM CORPORATION (Offshore Operations). The objectives of this study were to assist in the appraisal of these oil accumulations by predicting their possible lateral extent and to investigate if the technique applied could be used as a basis for further exploration of similar oil prospects in the area. Wireline logs of eight wells and some 1000 km of high quality <span class="hlt">seismic</span> data were processed into acoustic impedancemore » (A.I.) logs and <span class="hlt">seismic</span> A.I. sections. Having obtained a satisfactory match of the A.I. well logs and the A.I. of the <span class="hlt">seismic</span> traces at the well locations, relationships were established by the use of well log data which allowed the <span class="hlt">interpretation</span> of the <span class="hlt">seismic</span> A.I. in terms of reservoir quality. Measurements of the relevant A.I. characteristics were then carried out by computer along all <span class="hlt">seismic</span> lines and porosity distribution maps prepared for some of the reservoirs. These maps, combined with detailed <span class="hlt">seismic</span> depth contour maps at reservoir tops, lead to definition of good reservoir development areas downdip from poor reservoir quality zones i.e. of the stratigraphic trap areas, and drilling locations could thus be proposed. The system remains to be adequately calibrated when core material becomes available in the area of study.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/5601','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/5601"><span><span class="hlt">Interpretation</span> of electrical resistivity data acquired at the Aurora plant site</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2008-02-01</p> <p>MST proposes to acquire high-resolution reflection <span class="hlt">seismic</span> data at the Knight Hawk Coal Company construction site. These geophysical data will be processed, analyzed and <span class="hlt">interpreted</span> with the objective of locating and mapping any subsurface voids that...</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_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" 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_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> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P33D2909N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P33D2909N"><span>High Resolution Vertical <span class="hlt">Seismic</span> Profile from the Chicxulub IODP/ICDP Expedition 364 Borehole: Wave Speeds and <span class="hlt">Seismic</span> Reflectivity.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nixon, C.; Kofman, R.; Schmitt, D. R.; Lofi, J.; Gulick, S. P. S.; Christeson, G. L.; Saustrup, S., Sr.; Morgan, J. V.</p> <p>2017-12-01</p> <p>We acquired a closely-spaced vertical <span class="hlt">seismic</span> profile (VSP) in the Chicxulub K-Pg Impact Crater drilling program borehole to calibrate the existing surface <span class="hlt">seismic</span> profiles and provide complementary measurements of in situ <span class="hlt">seismic</span> wave speeds. Downhole <span class="hlt">seismic</span> records were obtained at spacings ranging from 1.25 m to 5 m along the borehole from 47.5 m to 1325 mwsf (meters wireline below sea floor) (Fig 1a) using a Sercel SlimwaveTM geophone chain (University of Alberta). The <span class="hlt">seismic</span> source was a 30/30ci Sercel Mini GI airgun (University of Texas), fired a minimum of 5 times per station. <span class="hlt">Seismic</span> data processing used a combination of a commercial processing package (Schlumberger's VISTA) and MatlabTM codes. The VSP displays detailed reflectivity (Fig. 1a) with the strongest reflection seen at 600 mwsf (280 ms one-way time), geologically corresponding to the sharp contact between the post-impact sediments and the target peak ring rock, thus confirming the pre-drilling <span class="hlt">interpretations</span> of the <span class="hlt">seismic</span> profiles. A two-way time trace extracted from the separated up-going wavefield matches the major reflection both in travel time and character. In the granitic rocks that form the peak ring of the Chicxulub impact crater, we observe P-wave velocities of 4000-4500 m/s which are significantly less than the expected values of granitoids ( 6000 m/s) (Fig. 1b). The VSP measured wave speeds are confirmed against downhole sonic logging and in laboratory velocimetry measurements; these data provide additional evidence that the crustal material displaced by the impact experienced a significant amount of damage. Samples and data provided by IODP. Samples can be requested at http://web.iodp.tamu.edu/sdrm after 19 October 2017. Expedition 364 was jointly funded by ECORD, ICDP, and IODP with contributions and logistical support from the Yucatan State Government and UNAM. The downhole <span class="hlt">seismic</span> chain and wireline system is funded by grants to DRS from the Canada Foundation for Innovation and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JSG....74..185B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JSG....74..185B"><span>Uncertainty in structural <span class="hlt">interpretation</span>: Lessons to be learnt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bond, Clare E.</p> <p>2015-05-01</p> <p>Uncertainty in the <span class="hlt">interpretation</span> of geological data is an inherent element of geology. Datasets from different sources: remotely sensed <span class="hlt">seismic</span> imagery, field data and borehole data, are often combined and <span class="hlt">interpreted</span> to create a geological model of the sub-surface. The data have limited resolution and spatial distribution that results in uncertainty in the <span class="hlt">interpretation</span> of the data and in the subsequent geological model(s) created. Methods to determine the extent of <span class="hlt">interpretational</span> uncertainty of a dataset, how to capture and express that uncertainty, and consideration of uncertainties in terms of risk have been investigated. Here I review the work that has taken place and discuss best practice in accounting for uncertainties in structural <span class="hlt">interpretation</span> workflows. Barriers to best practice are reflected on, including the use of software packages for <span class="hlt">interpretation</span>. Experimental evidence suggests that minimising <span class="hlt">interpretation</span> error through the use of geological reasoning and rules can help decrease <span class="hlt">interpretation</span> uncertainty; through identification of inadmissible <span class="hlt">interpretations</span> and in highlighting areas of uncertainty. Understanding expert thought processes and reasoning, including the use of visuospatial skills, during <span class="hlt">interpretation</span> may aid in the identification of uncertainties, and in the education of new geoscientists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1000063','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1000063"><span>MEASUREMENT OF COMPRESSIONAL-WAVE <span class="hlt">SEISMIC</span> VELOCITIES IN 29 WELLS AT THE HANFORD SITE</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>PETERSON SW</p> <p>2010-10-08</p> <p>Check shot <span class="hlt">seismic</span> velocity surveys were collected in 100 B/C, 200 East, 200-PO-1 Operational Unit (OU), and the Gable Gap areas in order to provide time-depth correlation information to aid the <span class="hlt">interpretation</span> of existing <span class="hlt">seismic</span> reflection data acquired at the Hanford Site (Figure 1). This report details results from 5 wells surveyed in fiscal year (FY) 2008, 7 wells in FY 2009, and 17 wells in FY 2010 and provides summary compressional-wave <span class="hlt">seismic</span> velocity information to help guide future <span class="hlt">seismic</span> survey design as well as improve current <span class="hlt">interpretations</span> of the <span class="hlt">seismic</span> data (SSC 1979/1980; SGW-39675; SGW-43746). Augmenting the check shotmore » database are four surveys acquired in 2007 in support of the Bechtel National, Inc. Waste Treatment Plant construction design (PNNL-16559, PNNL-16652), and check shot surveys in three wells to support <span class="hlt">seismic</span> testing in the 200 West Area (Waddell et al., 1999). Additional sonic logging was conducted during the late 1970s and early 1980s as part of the Basalt Waste Isolation Program (BWIP) (SSC 1979/1980) and check shot/sonic surveys as part of the safety report for the Skagit/Hanford Nuclear project (RDH/10-AMCP-0164). Check shot surveys are used to obtain an in situ measure of compressional-wave <span class="hlt">seismic</span> velocity for sediment and rock in the vicinity of the well point, and provide the <span class="hlt">seismic</span>-wave travel time to geologic horizons of interest. The check shot method deploys a downhole <span class="hlt">seismic</span> receiver (geophone) to record the arrival of <span class="hlt">seismic</span> waves generated by a source at the ground surface. The travel time of the first arriving <span class="hlt">seismic</span>-wave is determined and used to create a time-depth function to correlate encountered geologic intervals with the <span class="hlt">seismic</span> data. This critical tie with the underlying geology improves the <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> reflection profile information. Fieldwork for this investigation was conducted by in house staff during the weeks of September 22, 2008 for 5 wells in the 200 East Area (Figure 2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8737O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8737O"><span>Paleobathymetric Reconstruction of Ross Sea: <span class="hlt">seismic</span> data processing and regional reflectors mapping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olivo, Elisabetta; De Santis, Laura; Wardell, Nigel; Geletti, Riccardo; Busetti, Martina; Sauli, Chiara; Bergamasco, Andrea; Colleoni, Florence; Vanzella, Walter; Sorlien, Christopher; Wilson, Doug; De Conto, Robert; Powell, Ross; Bart, Phil; Luyendyk, Bruce</p> <p>2017-04-01</p> <p>PURPOSE: New maps of some major unconformities of the Ross Sea have been reconstructed, by using <span class="hlt">seismic</span> data grids, combined with the acoustic velocities from previous works, from new and reprocessed <span class="hlt">seismic</span> profiles. This work is carried out with the support of PNRA and in the frame of the bilateral Italy-USA project GLAISS (Global Sea Level Rise & Antarctic Ice Sheet Stability predictions), funded by the Ministry of Foreign Affairs. Paleobathymetric maps of 30, 14 and 4 million years ago, three 'key moments' for the glacial history of the Antarctic Ice Sheet, coinciding with global climatic changes. The paleobathymetric maps will then be used for numeric simulations focused on the width and thickness of the Ross Sea Ice Sheet. PRELIMINARY RESULTS: The first step was to create TWT maps of three main unconformity (RSU6, RSU4, and RSU2) of Ross Sea, revisiting and updating the ANTOSTRAT maps, through the <span class="hlt">interpretation</span> of sedimentary bodies and erosional features, used to infer active or old processes along the slope, we identified the main <span class="hlt">seismic</span> unconformities. We used the HIS Kingdom academic license. The different groups contribution was on the analysis of the Eastern Ross Sea continental slope and rise (OGS), of the Central Basin (KOPRI) of the western and central Ross Sea (Univ. of Santa Barbara and OGS), where new drill sites and <span class="hlt">seismic</span> profiles were collected after the publication of the ANTOSTRAT maps. Than we joined our <span class="hlt">interpretation</span> with previous <span class="hlt">interpretations</span>. We examined previous processing of several <span class="hlt">seismic</span> lines and all the old acoustic velocity analysis. In addiction we reprocessed some lines in order to have a higher data coverage. Then, combining the TWT maps of the unconformity with the old and new speed data we created new depth maps of the study area. The new depth maps will then be used for reconstructing the paleobathymetry of the Ross Sea by applying backstripping technique.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29326978','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29326978"><span><span class="hlt">Seismic</span> signature of active intrusions in mountain chains.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Di Luccio, Francesca; Chiodini, Giovanni; Caliro, Stefano; Cardellini, Carlo; Convertito, Vincenzo; Pino, Nicola Alessandro; Tolomei, Cristiano; Ventura, Guido</p> <p>2018-01-01</p> <p>Intrusions are a ubiquitous component of mountain chains and testify to the emplacement of magma at depth. Understanding the emplacement and growth mechanisms of intrusions, such as diapiric or dike-like ascent, is critical to constrain the evolution and structure of the crust. Petrological and geological data allow us to reconstruct magma pathways and long-term magma differentiation and assembly processes. However, our ability to detect and reconstruct the short-term dynamics related to active intrusive episodes in mountain chains is embryonic, lacking recognized geophysical signals. We analyze an anomalously deep <span class="hlt">seismic</span> sequence (maximum magnitude 5) characterized by low-frequency bursts of earthquakes that occurred in 2013 in the Apennine chain in Italy. We provide <span class="hlt">seismic</span> evidences of fluid involvement in the earthquake nucleation process and identify a thermal anomaly in aquifers where CO 2 of magmatic origin dissolves. We show that the intrusion of dike-like bodies in mountain chains may trigger earthquakes with magnitudes that may be relevant to <span class="hlt">seismic</span> hazard assessment. These findings provide a new perspective on the emplacement mechanisms of intrusive bodies and the <span class="hlt">interpretation</span> of the <span class="hlt">seismicity</span> in mountain chains.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5756663','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5756663"><span><span class="hlt">Seismic</span> signature of active intrusions in mountain chains</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Di Luccio, Francesca; Chiodini, Giovanni; Caliro, Stefano; Cardellini, Carlo; Convertito, Vincenzo; Pino, Nicola Alessandro; Tolomei, Cristiano; Ventura, Guido</p> <p>2018-01-01</p> <p>Intrusions are a ubiquitous component of mountain chains and testify to the emplacement of magma at depth. Understanding the emplacement and growth mechanisms of intrusions, such as diapiric or dike-like ascent, is critical to constrain the evolution and structure of the crust. Petrological and geological data allow us to reconstruct magma pathways and long-term magma differentiation and assembly processes. However, our ability to detect and reconstruct the short-term dynamics related to active intrusive episodes in mountain chains is embryonic, lacking recognized geophysical signals. We analyze an anomalously deep <span class="hlt">seismic</span> sequence (maximum magnitude 5) characterized by low-frequency bursts of earthquakes that occurred in 2013 in the Apennine chain in Italy. We provide <span class="hlt">seismic</span> evidences of fluid involvement in the earthquake nucleation process and identify a thermal anomaly in aquifers where CO2 of magmatic origin dissolves. We show that the intrusion of dike-like bodies in mountain chains may trigger earthquakes with magnitudes that may be relevant to <span class="hlt">seismic</span> hazard assessment. These findings provide a new perspective on the emplacement mechanisms of intrusive bodies and the <span class="hlt">interpretation</span> of the <span class="hlt">seismicity</span> in mountain chains. PMID:29326978</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1817219G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1817219G"><span>Investigation of sea-level changes and shelf break prograding sequences during the Late Quaternary offshore of Kusadasi (West Anatolia) and surroundings by high resolution <span class="hlt">seismic</span> methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gurcay, Savas; Cifci, Gunay; Dondurur, Derman; Okay, Seda; Atgin, Orhan; Ozel, Ozkan; Mert Kucuk, Hilmi</p> <p>2016-04-01</p> <p>High Resolution multi-channel <span class="hlt">seismic</span> reflection and Chirp data were collected by K. Piri Reis, research vessel of Dokuz Eylül University, in the central Aegean coast of the West Anatolia by research cruises carried out in 2005 and 2008, respectively. Submarine stratigraphic and structural features of Sıǧacık Gulf, Kuşadası Gulf and surroundings were investigated under this survey. The data were processed and <span class="hlt">interpreted</span> in SeisLab, D.E.U. Marine Sciences and Technology <span class="hlt">seismic</span> laboratory. Thirteen distinct unconformities can be traced below the study area that separate thirteen progradational stacked paleo-delta sequences (Lob1-Lob13) on <span class="hlt">seismic</span> profiles following and cutting each other. As a result of comparison with the oxygen isotopic stages (δ18), these deltas (Lob1-L13) were <span class="hlt">interpreted</span> that they have been deposited during the sea-level lowstands within Pleistocene glacial stages. In the study area the basement surface which observed as the lowest unconformity surface of the <span class="hlt">seismic</span> sections was called 'Acoustic Basement'. This basement which traced approximately all of the <span class="hlt">seismic</span> sections has generally quite wavy surface and underlain the upper <span class="hlt">seismic</span> units. It was observed that these <span class="hlt">seismic</span> units which terminated their formation in Pleistocene (Lob1-Lob13) and Holocene period were cut and uplifted by acoustic basement, like an intrusion. These type deformations were <span class="hlt">interpreted</span> as a result of magmatic intrusion into these upper <span class="hlt">seismic</span> units occurred in Late Pleistocene and Holocene period. Tectonic and structural <span class="hlt">interpretation</span> was carried out to constitute the submarine active tectonic map of the study area by correlated active faults identified on <span class="hlt">seismic</span> sections. Submarine active tectonic map and, basement topography and sediment thickness map were correlated together to present the relationship between tectonic deformation and stratigraphy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMDI43B0355R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMDI43B0355R"><span>SplitRacer - a new Semi-Automatic Tool to Quantify And <span class="hlt">Interpret</span> Teleseismic Shear-Wave Splitting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reiss, M. C.; Rumpker, G.</p> <p>2017-12-01</p> <p>We have developed a semi-automatic, MATLAB-based GUI to combine standard seismological tasks such as the analysis and <span class="hlt">interpretation</span> of teleseismic shear-wave splitting. Shear-wave splitting analysis is widely used to infer <span class="hlt">seismic</span> anisotropy, which can be <span class="hlt">interpreted</span> in terms of lattice-preferred orientation of mantle minerals, shape-preferred orientation caused by fluid-filled cracks or alternating layers. <span class="hlt">Seismic</span> anisotropy provides a unique link between directly observable surface structures and the more elusive dynamic processes in the mantle below. Thus, resolving the <span class="hlt">seismic</span> anisotropy of the lithosphere/asthenosphere is of particular importance for geodynamic modeling and <span class="hlt">interpretations</span>. The increasing number of <span class="hlt">seismic</span> stations from temporary experiments and permanent installations creates a new basis for comprehensive studies of <span class="hlt">seismic</span> anisotropy world-wide. However, the increasingly large data sets pose new challenges for the rapid and reliably analysis of teleseismic waveforms and for the <span class="hlt">interpretation</span> of the measurements. Well-established routines and programs are available but are often impractical for analyzing large data sets from hundreds of stations. Additionally, shear wave splitting results are seldom evaluated using the same well-defined quality criteria which may complicate comparison with results from different studies. SplitRacer has been designed to overcome these challenges by incorporation of the following processing steps: i) downloading of waveform data from multiple stations in mseed-format using FDSNWS tools; ii) automated initial screening and categorizing of XKS-waveforms using a pre-set SNR-threshold; iii) particle-motion analysis of selected phases at longer periods to detect and correct for sensor misalignment; iv) splitting analysis of selected phases based on transverse-energy minimization for multiple, randomly-selected, relevant time windows; v) one and two-layer joint-splitting analysis for all phases at one station by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap2_Okubo.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap2_Okubo.pdf"><span>The evolution of <span class="hlt">seismic</span> monitoring systems at the Hawaiian Volcano Observatory: Chapter 2 in Characteristics of Hawaiian volcanoes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Okubo, Paul G.; Nakata, Jennifer S.; Koyanagi, Robert Y.; Poland, Michael P.; Takahashi, T. Jane; Landowski, Claire M.</p> <p>2014-01-01</p> <p>In the century since the Hawaiian Volcano Observatory (HVO) put its first seismographs into operation at the edge of Kīlauea Volcano’s summit caldera, <span class="hlt">seismic</span> monitoring at HVO (now administered by the U.S. Geological Survey [USGS]) has evolved considerably. The HVO <span class="hlt">seismic</span> network extends across the entire Island of Hawai‘i and is complemented by stations installed and operated by monitoring partners in both the USGS and the National Oceanic and Atmospheric Administration. The <span class="hlt">seismic</span> data stream that is available to HVO for its monitoring of volcanic and <span class="hlt">seismic</span> activity in Hawai‘i, therefore, is built from hundreds of data channels from a diverse collection of instruments that can accurately record the ground motions of earthquakes ranging in magnitude from <1 to ≥8. In this chapter we describe the growth of HVO’s <span class="hlt">seismic</span> monitoring systems throughout its first hundred years of operation. Although other references provide specific details of the changes in instrumentation and data handling over time, we recount here, in more general terms, the evolution of HVO’s <span class="hlt">seismic</span> network. We focus not only on equipment but also on <span class="hlt">interpretative</span> products and results that were enabled by the new instrumentation and by improvements in HVO’s <span class="hlt">seismic</span> monitoring, analytical, and <span class="hlt">interpretative</span> capabilities implemented during the past century. As HVO enters its next hundred years of seismological studies, it is well situated to further improve upon insights into <span class="hlt">seismic</span> and volcanic processes by using contemporary seismological tools.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...88a2001Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...88a2001Z"><span>Characterizing Geological Facies using <span class="hlt">Seismic</span> Waveform Classification in Sarawak Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zahraa, Afiqah; Zailani, Ahmad; Prasad Ghosh, Deva</p> <p>2017-10-01</p> <p>Numerous effort have been made to build relationship between geology and geophysics using different techniques throughout the years. The integration of these two most important data in oil and gas industry can be used to reduce uncertainty in exploration and production especially for reservoir productivity enhancement and stratigraphic identification. This paper is focusing on <span class="hlt">seismic</span> waveform classification to different classes using neural network and to link them according to the geological facies which are established using the knowledge on lithology and log motif of well data. <span class="hlt">Seismic</span> inversion is used as the input for the neural network to act as the direct lithology indicator reducing dependency on well calibration. The <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> facies classification map provides a better understanding towards the lithology distribution, depositional environment and help to identify significant reservoir rock</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ExG....48..430J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ExG....48..430J"><span>Improved reservoir characterisation using fuzzy logic platform: an integrated petrophysical, <span class="hlt">seismic</span> structural and poststack inversion study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jafri, Muhammad Kamran; Lashin, Aref; Ibrahim, El-Khedr Hassan; Hassanein, Kamal A.; Al Arifi, Nassir; Naeem, Muhammad</p> <p>2017-06-01</p> <p>There is a tendency for applying different integrated geophysical approaches for better hydrocarbon reservoir characterisation and <span class="hlt">interpretation</span>. In this study, petrophysical properties, <span class="hlt">seismic</span> structural and poststack <span class="hlt">seismic</span> inversion results are integrated using the fuzzy logic AND operator to characterise the Tensleep Sandstone Formation (TSF) at Powder River Basin (PRB), Wyoming, USA. TSF is deposited in a coastal plain setting during the Pennsylvanian era, and contains cross-bedded sandstone of Aeolian origin as a major lithology with alternative sabkha dolomite/carbonates. Wireline logging datasets from 17 wells are used for the detailed petrophysical evaluation. Three units of the TSF (A-sandstone, B-dolomite and B-sandstone) are targeted and their major rock properties estimated (i.e. shale/clay volume, Vsh; porosity, φEff permeability, K; fluid saturations, Sw and SH; and bulk volume water, BVW). The B-sandstone zone, with its petrophysical properties of 5-20% effective porosity, 0.10-250 mD permeability and hydrocarbon potential up to 72%, is considered the best reservoir zone among the three studied units. Distributions of the most important petrophysical parameters of the B-sandstone reservoir (Vsh, φEff, K, Sw) are generated as GIS thematic layers. The two-dimensional (2D) and three-dimensional (3D) <span class="hlt">seismic</span> structural <span class="hlt">interpretations</span> revealed that the hydrocarbons are entrapped in an anticlinal structure bounded with fault closures at the west of the study area. Poststack acoustic impedance (PSAI) inversion is performed on 3D <span class="hlt">seismic</span> data to extract the inverted acoustic impedance (AI) cube. Two attribute slices (inverted AI and <span class="hlt">seismic</span> amplitude) were extracted at the top of the B-sandstone unit as GIS thematic layers. The reservoir properties and inverted <span class="hlt">seismic</span> attributes were then integrated using fuzzy AND operator. Finally, a fuzzy reservoir quality map was produced, and a prospective reservoir area with best reservoir characteristics is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031184','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031184"><span>Lithology-derived structure classification from the joint <span class="hlt">interpretation</span> of magnetotelluric and <span class="hlt">seismic</span> models</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bedrosian, P.A.; Maercklin, N.; Weckmann, U.; Bartov, Y.; Ryberg, T.; Ritter, O.</p> <p>2007-01-01</p> <p>Magnetotelluric and <span class="hlt">seismic</span> methods provide complementary information about the resistivity and velocity structure of the subsurface on similar scales and resolutions. No global relation, however, exists between these parameters, and correlations are often valid for only a limited target area. Independently derived inverse models from these methods can be combined using a classification approach to map geologic structure. The method employed is based solely on the statistical correlation of physical properties in a joint parameter space and is independent of theoretical or empirical relations linking electrical and <span class="hlt">seismic</span> parameters. Regions of high correlation (classes) between resistivity and velocity can in turn be mapped back and re-examined in depth section. The spatial distribution of these classes, and the boundaries between them, provide structural information not evident in the individual models. This method is applied to a 10 km long profile crossing the Dead Sea Transform in Jordan. Several prominent classes are identified with specific lithologies in accordance with local geology. An abrupt change in lithology across the fault, together with vertical uplift of the basement suggest the fault is sub-vertical within the upper crust. ?? 2007 The Authors Journal compilation ?? 2007 RAS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/541188-avo-helps-seismic-imaging-deepwater-environments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/541188-avo-helps-seismic-imaging-deepwater-environments"><span>AVO helps <span class="hlt">seismic</span> imaging in deepwater environments</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>Skidmore, C.; Lindsay, R.O.; Ratcliff, D.</p> <p>1997-11-03</p> <p>Amplitude and frequency variations related to offset should be analyzed routinely during <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> data acquired in deepwater environments. Amplitude variation with offset (AVO) in three dimensions is the key exploration tool in deep waters of the Gulf of Mexico. But application of the tool requires special care. Three-dimensional AVO helps the <span class="hlt">interpreter</span> understand stratigraphy and the meaning of amplitude anomalies. Used in conjunction with well log data, it can help the <span class="hlt">interpreter</span> distinguish amplitudes related to the presence of hydrocarbons from those that result from, for example, rock-property changes within a non-hydrocarbon-bearing layer, such as a shale, ormore » residual gas (fizz water) in high-porosity sands. The paper discusses examples from the Gulf of Mexico, will control application, improving detail, and frequency-dependent analysis.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/1985/4107/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/1985/4107/report.pdf"><span><span class="hlt">Seismic</span>-refraction study of suspected drift-filled bedrock valleys in Ramsey County, Minnesota</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Woodward, D.G.</p> <p>1985-01-01</p> <p>A drift-filled bedrock valley was thought to incise the St. Peter aquifer to an altitude between 770 and 800 feet above sea level at the Koppers site. The <span class="hlt">interpretation</span> of a <span class="hlt">seismic</span> profile just east of the Koppers site is not conclusive, but suggests that a bedrock valley may be present near the middle of the line. The <span class="hlt">interpretation</span> of a second <span class="hlt">seismic</span> profile across the westward extension of the same suspected valley also is not conclusive, but suggests that a bedrock valley may be present at the north end of the line. The optimal field layout for each line at the site (longer shot offsets) could not be obtained because of limited space available in the densely developed residential neighborhoods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.S23B0159A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.S23B0159A"><span>Finite-Difference Numerical Simulation of <span class="hlt">Seismic</span> Gradiometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aldridge, D. F.; Symons, N. P.; Haney, M. M.</p> <p>2006-12-01</p> <p>We use the phrase <span class="hlt">seismic</span> gradiometry to refer to the developing research area involving measurement, modeling, analysis, and <span class="hlt">interpretation</span> of spatial derivatives (or differences) of a <span class="hlt">seismic</span> wavefield. In analogy with gradiometric methods used in gravity and magnetic exploration, <span class="hlt">seismic</span> gradiometry offers the potential for enhancing resolution, and revealing new (or hitherto obscure) information about the subsurface. For example, measurement of pressure and rotation enables the decomposition of recorded <span class="hlt">seismic</span> data into compressional (P) and shear (S) components. Additionally, a complete observation of the total <span class="hlt">seismic</span> wavefield at a single receiver (including both rectilinear and rotational motions) offers the possibility of inferring the type, speed, and direction of an incident <span class="hlt">seismic</span> wave. Spatially extended receiver arrays, conventionally used for such directional and phase speed determinations, may be dispensed with. <span class="hlt">Seismic</span> wave propagation algorithms based on the explicit, time-domain, finite-difference (FD) numerical method are well-suited for investigating gradiometric effects. We have implemented in our acoustic, elastic, and poroelastic algorithms a point receiver that records the 9 components of the particle velocity gradient tensor. Pressure and particle rotation are obtained by forming particular linear combinations of these tensor components, and integrating with respect to time. All algorithms entail 3D O(2,4) FD solutions of coupled, first- order systems of partial differential equations on uniformly-spaced staggered spatial and temporal grids. Numerical tests with a 1D model composed of homogeneous and isotropic elastic layers show isolation of P, SV, and SH phases recorded in a multiple borehole configuration, even in the case of interfering events. Synthetic traces recorded by geophones and rotation receivers in a shallow crosswell geometry with randomly heterogeneous poroelastic models also illustrate clear P (fast and slow) and S</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT........61F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT........61F"><span>Extracting physical parameters from marine <span class="hlt">seismic</span> data: New methods in <span class="hlt">seismic</span> oceanography and velocity inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fortin, Will F. J.</p> <p></p> <p>The utility and meaning of a geophysical dataset is dependent on good <span class="hlt">interpretation</span> informed by high-quality data, processing, and attribute examination via technical methodologies. Active source marine <span class="hlt">seismic</span> reflection data contains a great deal of information in the location, phase, and amplitude of both pre- and post-stack <span class="hlt">seismic</span> reflections. Using pre- and post-stack data, this work has extracted useful information from marine reflection <span class="hlt">seismic</span> data in novel ways in both the oceanic water column and the sub-seafloor geology. In chapter 1 we develop a new method for estimating oceanic turbulence from a <span class="hlt">seismic</span> image. This method is tested on synthetic <span class="hlt">seismic</span> data to show the method's ability to accurately recover both distribution and levels of turbulent diffusivity. Then we apply the method to real data offshore Costa Rica where we observe lee waves. Our results find elevated diffusivities near the seafloor as well as above the lee waves five times greater than surrounding waters and 50 times greater than open ocean diffusivities. Chapter 2 investigates subsurface geology in the Cascadia Subduction Zone and outlines a workflow for using pre-stack waveform inversion to produce highly detailed velocity models and <span class="hlt">seismic</span> images. Using a newly developed inversion code, we achieve better imaging results as compared to the product of a standard, user-intensive method for building a velocity model. Our results image the subduction interface ~30 km farther landward than previous work and better images faults and sedimentary structures above the oceanic plate as well as in the accretionary prism. The resultant velocity model is highly detailed, inverted every 6.25 m with ~20 m vertical resolution, and will be used to examine the role of fluids in the subduction system. These results help us to better understand the natural hazards risks associated with the Cascadia Subduction Zone. Chapter 3 returns to <span class="hlt">seismic</span> oceanography and examines the dynamics of nonlinear</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5948652','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5948652"><span>A Monolithic Electrochemical Micro <span class="hlt">Seismic</span> Sensor Capable of Monitoring Three-Dimensional Vibrations</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chen, Lianhong; Sun, Zhenyuan; Li, Guanglei; Chen, Deyong; Wang, Junbo</p> <p>2018-01-01</p> <p>A monolithic electrochemical micro <span class="hlt">seismic</span> sensor capable of monitoring three-axial vibrations was proposed in this paper. The proposed micro sensor mainly consisted of four sensing units interconnected within flow channels and by <span class="hlt">interpreting</span> the voltage outputs of the sensing units, vibrations with arbitrary directions can be quantified. The proposed <span class="hlt">seismic</span> sensors are fabricated based on MEMS technologies and characterized, which produced sensitivities along x, y, and z axes as 2473.2 ± 184.5 V/(m/s), 2261.7 ± 119.6 V/(m/s), and 3480.7 ± 417.2 V/(m/s) at 30 Hz. In addition, the vibrations in x-y, x-z, and y-z planes were applied to the developed <span class="hlt">seismic</span> sensors, leading to comparable monitoring results after decoupling calculations with the input velocities. Furthermore, the results have shown its feasibilities for <span class="hlt">seismic</span> data recording. PMID:29614720</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3888L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3888L"><span>Integrating Reflection <span class="hlt">Seismic</span>, Gravity and Magnetic Data to Reveal the Structure of Crystalline Basement: Implications for Understanding Rift Development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenhart, Antje; Jackson, Christopher A.-L.; Bell, Rebecca E.; Duffy, Oliver B.; Fossen, Haakon; Gawthorpe, Robert L.</p> <p>2016-04-01</p> <p>Numerous rifts form above crystalline basement containing pervasive faults and shear zones. However, the compositional and mechanical heterogeneity within crystalline basement and the geometry and kinematics of discrete and pervasive basement fabrics are poorly understood. Furthermore, the <span class="hlt">interpretation</span> of intra-crustal structures beneath sedimentary basins is often complicated by limitations in the depth of conventional <span class="hlt">seismic</span> imaging, the commonly acoustically transparent nature of basement, limited well penetrations, and complex overprinting of multiple tectonic events. Yet, a detailed knowledge of the structural and lithological complexity of crystalline basement rocks is crucial to improve our understanding of how rifts evolve. Potential field methods are a powerful but perhaps underutilised regional tool that can decrease <span class="hlt">interpretational</span> uncertainty based solely on <span class="hlt">seismic</span> reflection data. We use petrophysical data, high-resolution 3D reflection <span class="hlt">seismic</span> volumes, gridded gravity and magnetic data, and 2D gravity and magnetic modelling to constrain the structure of crystalline basement offshore western Norway. Intra-basement structures are well-imaged on <span class="hlt">seismic</span> data due to relatively shallow burial of the basement beneath a thin (<3.5 km) sedimentary cover. Variations in basement composition were <span class="hlt">interpreted</span> from detailed <span class="hlt">seismic</span> facies analysis and mapping of discrete intra-basement reflections. A variety of data filtering and isolation techniques were applied to the original gravity and magnetic data in order to enhance small-scale field variations, to accentuate formation boundaries and discrete linear trends, and to isolate shallow and deep crustal anomalies. In addition, 2D gravity and magnetic data modelling was used to verify the <span class="hlt">seismic</span> <span class="hlt">interpretation</span> and to further constrain the configuration of the upper and lower crust. Our analysis shows that the basement offshore western Norway is predominantly composed of Caledonian allochthonous nappes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....11276P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....11276P"><span>Variations of <span class="hlt">seismic</span> parameters during different activity levels of the Soufriere Hills Volcano, Montserrat</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Powell, T.; Neuberg, J.</p> <p>2003-04-01</p> <p>The low-frequency <span class="hlt">seismic</span> events on Montserrat are linked to conduit resonance and the pressurisation of the volcanic system. Analysis of these events tell us more about the behaviour of the volcanic system and provide a monitoring and <span class="hlt">interpretation</span> tool. We have written an Automated Event Classification Algorithm Program (AECAP), which finds and classifies <span class="hlt">seismic</span> events and calculates <span class="hlt">seismic</span> parameters such as energy, intermittency, peak frequency and event duration. Comparison of low-frequency energy with the tilt cycles in 1997 allows us to link pressurisation of the volcano with <span class="hlt">seismic</span> behaviour. An empirical relationship provides us with an estimate of pressurisation through released <span class="hlt">seismic</span> energy. During 1997, the activity of the volcano varied considerably. We compare <span class="hlt">seismic</span> parameters from quiet periods to those from active periods and investigate how the relationships between these parameters change. These changes are then used to constrain models of magmatic processes during different stages of volcanic activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26173557','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26173557"><span><span class="hlt">Seismic</span> footprints of shallow dyke propagation at Etna, Italy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Falsaperla, Susanna; Neri, Marco</p> <p>2015-07-15</p> <p>One of the key issues in forecasting volcanic eruptions is to detect signals that can track the propagation of dykes towards the surface. Continuous monitoring of active volcanoes helps significantly in achieving this goal. The <span class="hlt">seismic</span> data presented here are unique, as they document surface faulting processes close (tens to a few hundred meters) to their source, namely the dyke tip. They originated nearby - and under - a <span class="hlt">seismic</span> station that was subsequently destroyed by lava flows during eruptive activity at Etna volcano, Italy, in 2013. On February 20, a ~600 m-long and ~120 m wide NW-SE fracture field opened at an altitude between 2750 and 2900 m. The consequent rock dislocation caused the station to tilt and offset the <span class="hlt">seismic</span> signal temporarily. Data acquisition continued until the arrival of the lava flow that led to the breakdown of the transmission system. Shallow ground fracturing and repeated low-frequency oscillations occurred during two stages in which the <span class="hlt">seismic</span> signal underwent a maximum offset ~2.57 × 10(4) nm/s. Bridging instrumental recordings, fieldwork and conceptual modelling, these data are <span class="hlt">interpreted</span> as the <span class="hlt">seismic</span> footprints of a magmatic dyke intrusion that moved at speed ~0.02 m/s (first stage) and 0.46 m/s (second stage).</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('https://pubs.usgs.gov/of/2006/1231/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2006/1231/"><span>Hawaiian Volcano Observatory <span class="hlt">seismic</span> data, January to December 2005</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakata, Jennifer S.</p> <p>2006-01-01</p> <p>The Hawaiian Volcano Observatory (HVO) summary presents <span class="hlt">seismic</span> data gathered during the year. The <span class="hlt">seismic</span> summary is offered without <span class="hlt">interpretation</span> as a source of preliminary data. It is complete in the sense that most data for events of M-1.5 routinely gathered by the Observatory are included. The HVO summaries have been published in various forms since 1956. Summaries prior to 1974 were issued quarterly, but cost, convenience of preparation and distribution, and the large quantities of data dictated an annual publication beginning with Summary 74 for the year 1974. Summary 86 (the introduction of CUSP at HVO) includes a description of the <span class="hlt">seismic</span> instrumentation, calibration, and processing used in recent years. Beginning with 2004, summaries will simply be identified by the year, rather than Summary number. The present summary includes background information on the <span class="hlt">seismic</span> network and processing to allow use of the data and to provide an understanding of how they were gathered. A report by Klein and Koyanagi (1980) tabulates instrumentation, calibration, and recording history of each <span class="hlt">seismic</span> station in the network. It is designed as a reference for users of seismograms and phase data and includes and augments the information in the station table in this summary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1073/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1073/"><span>Hawaiian Volcano Observatory <span class="hlt">Seismic</span> Data, January to December 2006</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakata, Jennifer</p> <p>2007-01-01</p> <p>Introduction The Hawaiian Volcano Observatory (HVO) summary presents <span class="hlt">seismic</span> data gathered during the year. The <span class="hlt">seismic</span> summary is offered without <span class="hlt">interpretation</span> as a source of preliminary data. It is complete in the sense that most data for events of M>1.5 routinely gathered by the Observatory are included. The HVO summaries have been published in various forms since 1956. Summaries prior to 1974 were issued quarterly, but cost, convenience of preparation and distribution, and the large quantities of data dictated an annual publication beginning with Summary 74 for the year 1974. Summary 86 (the introduction of CUSP at HVO) includes a description of the <span class="hlt">seismic</span> instrumentation, calibration, and processing used in recent years. Beginning with 2004, summaries are simply identified by the year, rather than Summary number. The present summary includes background information on the <span class="hlt">seismic</span> network and processing to allow use of the data and to provide an understanding of how they were gathered. A report by Klein and Koyanagi (1980) tabulates instrumentation, calibration, and recording history of each <span class="hlt">seismic</span> station in the network. It is designed as a reference for users of seismograms and phase data and includes and augments the information in the station table in this summary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3443G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3443G"><span><span class="hlt">Seismic</span> properties of fluid bearing formations in magmatic geothermal systems: can we directly detect geothermal activity with <span class="hlt">seismic</span> methods?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grab, Melchior; Scott, Samuel; Quintal, Beatriz; Caspari, Eva; Maurer, Hansruedi; Greenhalgh, Stewart</p> <p>2016-04-01</p> <p><span class="hlt">Seismic</span> methods are amongst the most common techniques to explore the earth's subsurface. <span class="hlt">Seismic</span> properties such as velocities, impedance contrasts and attenuation enable the characterization of the rocks in a geothermal system. The most important goal of geothermal exploration, however, is to describe the enthalpy state of the pore fluids, which act as the main transport medium for the geothermal heat, and to detect permeable structures such as fracture networks, which control the movement of these pore fluids in the subsurface. Since the quantities measured with <span class="hlt">seismic</span> methods are only indirectly related with the fluid state and the rock permeability, the <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> datasets is difficult and usually delivers ambiguous results. To help overcome this problem, we use a numerical modeling tool that quantifies the <span class="hlt">seismic</span> properties of fractured rock formations that are typically found in magmatic geothermal systems. We incorporate the physics of the pore fluids, ranging from the liquid to the boiling and ultimately vapor state. Furthermore, we consider the hydromechanics of permeable structures at different scales from small cooling joints to large caldera faults as are known to be present in volcanic systems. Our modeling techniques simulate oscillatory compressibility and shear tests and yield the P- and S-wave velocities and attenuation factors of fluid saturated fractured rock volumes. To apply this modeling technique to realistic scenarios, numerous input parameters need to be indentified. The properties of the rock matrix and individual fractures were derived from extensive literature research including a large number of laboratory-based studies. The geometries of fracture networks were provided by structural geologists from their published studies of outcrops. Finally, the physical properties of the pore fluid, ranging from those at ambient pressures and temperatures up to the supercritical conditions, were taken from the fluid physics</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C32A..03B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C32A..03B"><span>Patterned basal <span class="hlt">seismicity</span> shows sub-ice stream bedforms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barcheck, C. G.; Tulaczyk, S. M.; Schwartz, S. Y.</p> <p>2017-12-01</p> <p>Patterns in <span class="hlt">seismicity</span> emanating from the bottom of fast-moving ice streams and glaciers may indicate localized patches of higher basal resistance— sometimes called 'sticky spots', or otherwise varying basal properties. These seismogenic basal areas resist an unknown portion of the total driving stress of the Whillans Ice Plain (WIP), in West Antarctica, but may play an important role in the WIP stick-slip cycle and ice stream slowdown. To better understand the mechanism and importance of basal <span class="hlt">seismicity</span> beneath the WIP, we analyze <span class="hlt">seismic</span> data collected by a small aperture (< 3km) network of 8 surface and 5 borehole seismometers installed in the main central sticky spot of the WIP. We use a network beamforming technique to detect and roughly locate thousands of small (magnitude < 0), local basal micro-earthquakes in Dec 2014, and we compare the resulting map of <span class="hlt">seismicity</span> to ice bottom depth measured by airborne radar. The number of basal earthquakes per area within the network is spatially heterogeneous, but a pattern of two 400m wide streaks of high <span class="hlt">seismicity</span> rates is evident, with >50-500 earthquakes detected per 50x50m grid cell in 2 weeks. These <span class="hlt">seismically</span> active streaks are elongated approximately in the ice flow direction with a spacing of 750m. Independent airborne radar measurements of ice bottom depth from Jan 2013 show a low-amplitude ( 5m) undulation in the basal topography superposed on a regional gradient in ice bottom depth. The flow-perpendicular wavelength of these low-amplitude undulations is comparable to the spacing of the high <span class="hlt">seismicity</span> bands, and the streaks of high <span class="hlt">seismicity</span> intersect local lows in the undulating basal topography. We <span class="hlt">interpret</span> these <span class="hlt">seismic</span> and radar observations as showing <span class="hlt">seismically</span> active sub-ice stream bedforms that are low amplitude and elongated in the direction of ice flow, comparable to the morphology of mega scale glacial lineations (MSGLs), with high basal <span class="hlt">seismicity</span> rates observed in the MSGL troughs</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5777S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5777S"><span>Field observations of Flood Basalt structure: Implications for offshore <span class="hlt">interpretation</span> and sub-volcanic investigation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Single, R.; Jerram, D.; Pearson, D.; Hobbs, R.</p> <p>2003-04-01</p> <p>Field investigations in Skye and Namibia have provided insight into structure and architecture of CFBs. The studies have been developed into lava sequence models in 3-D software GoCad. The understanding has been applied to <span class="hlt">interpretation</span> of lavas in the Faeroe-Shetland trough. Volcanics hinder petroleum exploration in this play due to their complex internal geometries and velocity structure. <span class="hlt">Seismic</span> resolution is poor beneath volcanics. Fieldwork has shown that lavas on Skye have developed from (olivine-phyric) compound basalts towards the base of the sequence, into more massive flows higher up the succession. Fieldwork in the Etendeka CFBs reveal a similar style of lava field development. The focus of the offshore study is through the area of the GFA-99 <span class="hlt">seismic</span> data. Detailed 3-D <span class="hlt">interpretation</span> over the central data area is 20x20km in dimensions. The lava sequence present may be sub-divided vertically and laterally into 4 zones between the following <span class="hlt">seismic</span> picks: Base basalt/sub-basalt sills, top compound lava-dominated series, top Middle Series, top hyaloclastites, top massive basalt. Within the lava sequence, the surfaces have rugose topographies. Lower zone lavas are characterised by discontinuous, indistinct reflectors. These are <span class="hlt">interpreted</span> to be sub-aerially effused basalts with compound-braided architecture. Middle Series basalts are considered to be a combination of compound lavas and more massive, tabular flows. Steeply dipping <span class="hlt">seismic</span> reflectors also form part of the Middle Series and are <span class="hlt">interpreted</span> as foreset-bedded hyaloclastites. The uppermost lavas have strong reflection characteristics and are laterally extensive. These are <span class="hlt">interpreted</span> to be massive tabular lavas covering an area >8.4 x10^3 km^2. Such flows exist in upper parts of CFB sequences as evidenced from fieldwork. Complex stacking arrangements of lavas seen in the field, and the complexities observed in <span class="hlt">seismic</span>, suggest that many factors need to be considered within CFBs for improved sub</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21380919','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21380919"><span>Determining the depositional pattern by resistivity-<span class="hlt">seismic</span> inversion for the aquifer system of Maira area, Pakistan.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Akhter, Gulraiz; Farid, Asim; Ahmad, Zulfiqar</p> <p>2012-01-01</p> <p>Velocity and density measured in a well are crucial for synthetic <span class="hlt">seismic</span> generation which is, in turn, a key to <span class="hlt">interpreting</span> real <span class="hlt">seismic</span> amplitude in terms of lithology, porosity and fluid content. Investigations made in the water wells usually consist of spontaneous potential, resistivity long and short normal, point resistivity and gamma ray logs. The sonic logs are not available because these are usually run in the wells drilled for hydrocarbons. To generate the synthetic seismograms, sonic and density logs are required, which are useful to precisely mark the lithology contacts and formation tops. An attempt has been made to <span class="hlt">interpret</span> the subsurface soil of the aquifer system by means of resistivity to <span class="hlt">seismic</span> inversion. For this purpose, resistivity logs and surface resistivity sounding were used and the resistivity logs were converted to sonic logs whereas surface resistivity sounding data transformed into <span class="hlt">seismic</span> curves. The converted sonic logs and the surface <span class="hlt">seismic</span> curves were then used to generate synthetic seismograms. With the utilization of these synthetic seismograms, pseudo-<span class="hlt">seismic</span> sections have been developed. Subsurface lithologies encountered in wells exhibit different velocities and densities. The reflection patterns were marked by using amplitude standout, character and coherence. These pseudo-<span class="hlt">seismic</span> sections were later tied to well synthetics and lithologs. In this way, a lithology section was created for the alluvial fill. The cross-section suggested that the eastern portion of the studied area mainly consisted of sandy fill and the western portion constituted clayey part. This can be attributed to the depositional environment by the Indus and the Kabul Rivers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNS31A1939B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNS31A1939B"><span>Instrument Correction and Dynamic Site Profile Validation at the Central United States <span class="hlt">Seismic</span> Observatory, New Madrid <span class="hlt">Seismic</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>Brengman, C.; Woolery, E. W.; Wang, Z.; Carpenter, S.</p> <p>2016-12-01</p> <p>The Central United States <span class="hlt">Seismic</span> Observatory (CUSSO) is a vertical <span class="hlt">seismic</span> array located in southwestern Kentucky within the New Madrid <span class="hlt">seismic</span> zone. It is intended to describe the effects of local geology, including thick sediment overburden, on <span class="hlt">seismic</span>-wave propagation, particularly strong-motion. The three-borehole array at CUSSO is composed of <span class="hlt">seismic</span> sensors placed on the surface, and in the bedrock at various depths within the 585 m thick sediment overburden. The array's deep borehole provided a unique opportunity in the northern Mississippi embayment for the direct geological description and geophysical measurement of the complete late Cretaceous-Quaternary sediment column. A seven layer, intra-sediment velocity model is <span class="hlt">interpreted</span> from the complex, inhomogeneous stratigraphy. The S- and P-wave sediment velocities range between 160 and 875 m/s and between 1000 and 2300 m/s, respectively, with bedrock velocities of 1452 and 3775 m/s, respectively. Cross-correlation and direct comparisons were used to filter out the instrument response and determine the instrument orientation, making CUSSO data ready for analysis, and making CUSSO a viable calibration site for other free-field sensors in the area. The corrected bedrock motions were numerically propagated through the CUSSO soil profile (transfer function) and compared, in terms of both peak acceleration and amplitude spectra, to the recorded surface observations. Initial observations reveal a complex spectral mix of amplification and de-amplification across the array, indicating the site effect in this deep sediment setting is not simply generated by the shallowest layers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6640467','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6640467"><span><span class="hlt">Seismic</span> event classification system</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Dowla, F.U.; Jarpe, S.P.; Maurer, W.</p> <p>1994-12-13</p> <p>In the computer <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> data, the critical first step is to identify the general class of an unknown event. For example, the classification might be: teleseismic, regional, local, vehicular, or noise. Self-organizing neural networks (SONNs) can be used for classifying such events. Both Kohonen and Adaptive Resonance Theory (ART) SONNs are useful for this purpose. Given the detection of a <span class="hlt">seismic</span> event and the corresponding signal, computation is made of: the time-frequency distribution, its binary representation, and finally a shift-invariant representation, which is the magnitude of the two-dimensional Fourier transform (2-D FFT) of the binary time-frequency distribution. This pre-processed input is fed into the SONNs. These neural networks are able to group events that look similar. The ART SONN has an advantage in classifying the event because the types of cluster groups do not need to be pre-defined. The results from the SONNs together with an expert seismologist's classification are then used to derive event classification probabilities. 21 figures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAESc.145...37Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAESc.145...37Z"><span><span class="hlt">Seismic</span> probing of continental subduction zones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Liang; Xu, Xiaobing; Malusà, Marco G.</p> <p>2017-09-01</p> <p>High-resolution images of Earth's interior provide pivotal information for the understanding of a range of geodynamic processes, including continental subduction and exhumation of ultrahigh-pressure (UHP) metamorphic rocks. Here we present a synthesis of available global <span class="hlt">seismic</span> observations on continental subduction zones, and selected examples of <span class="hlt">seismic</span> probing from the European Alps, the Himalaya-Tibet and the Qinling-Dabie orogenic belts. Our synthesis and examples show that slabs recognized beneath exhumed continental UHP terranes generally have shallow dip angles (<45°) at depths <100 km, to become much steeper at depths >100 km. Slabs underlined by a clear high velocity anomaly from Earth's surface to the mantle are generally Cenozoic in age. Some of these slabs are continuous, whereas other continental subduction zones are located above discontinuous high velocity anomalies possibly suggesting slab breakoff. The density of <span class="hlt">seismic</span> stations and the quality of recordings are of primary importance to get high-resolution images of the upper mantle to be used as a starting point to provide reliable geodynamic <span class="hlt">interpretations</span>. In some cases, areas previously indicated as possible site of slab breakoff, such as the European Alps, have been later proven to be located above a continuous slab by using higher quality travel time data from denser <span class="hlt">seismic</span> arrays. Discriminating between oceanic and continental slabs can be challenging, but valuable information can be provided by combining teleseismic tomography and receiver function analysis. The upper mantle beneath most continental UHP terranes generally shows complex <span class="hlt">seismic</span> anisotropy patterns that are potentially preserved even in pre-Cenozoic subduction zones. These patterns can be used to provide information on continental slabs that are no longer highlighted by a clear high-velocity anomaly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.3509M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.3509M"><span>Bayesian identification of multiple <span class="hlt">seismic</span> change points and varying <span class="hlt">seismic</span> rates caused by induced <span class="hlt">seismicity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montoya-Noguera, Silvana; Wang, Yu</p> <p>2017-04-01</p> <p>The Central and Eastern United States (CEUS) has experienced an abnormal increase in <span class="hlt">seismic</span> activity, which is believed to be related to anthropogenic activities. The U.S. Geological Survey has acknowledged this situation and developed the CEUS 2016 1 year <span class="hlt">seismic</span> hazard model using the catalog of 2015 by assuming stationary <span class="hlt">seismicity</span> in that period. However, due to the nonstationary nature of induced <span class="hlt">seismicity</span>, it is essential to identify change points for accurate probabilistic <span class="hlt">seismic</span> hazard analysis (PSHA). We present a Bayesian procedure to identify the most probable change points in <span class="hlt">seismicity</span> and define their respective <span class="hlt">seismic</span> rates. It uses prior distributions in agreement with conventional PSHA and updates them with recent data to identify <span class="hlt">seismicity</span> changes. It can determine the change points in a regional scale and may incorporate different types of information in an objective manner. It is first successfully tested with simulated data, and then it is used to evaluate Oklahoma's regional <span class="hlt">seismicity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2013/1141/pdf/ofr2013-1141.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2013/1141/pdf/ofr2013-1141.pdf"><span>Preliminary stratigraphic and hydrogeologic cross sections and <span class="hlt">seismic</span> profile of the Floridan aquifer system of Broward County, Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reese, Ronald S.; Cunningham, Kevin J.</p> <p>2013-01-01</p> <p>To help water-resource managers evaluate the Floridan aquifer system (FAS) as an alternative water supply, the U.S. Geological Survey initiated a study, in cooperation with the Broward County Environmental Protection and Growth Management Department, to refine the hydrogeologic framework of the FAS in the eastern part of Broward County. This report presents three preliminary cross sections illustrating stratigraphy and hydrogeology in eastern Broward County as well as an <span class="hlt">interpreted</span> <span class="hlt">seismic</span> profile along one of the cross sections. Marker horizons were identified using borehole geophysical data and were initially used to perform well-to-well correlation. Core sample data were integrated with the borehole geophysical data to support stratigraphic and hydrogeologic <span class="hlt">interpretations</span> of marker horizons. Stratigraphic and hydrogeologic units were correlated across the county using borehole geophysical data from multiple wells. <span class="hlt">Seismic</span>-reflection data were collected along the Hillsboro Canal. Borehole geophysical data were used to identify and correlate hydrogeologic units in the <span class="hlt">seismic</span>-reflection profile. Faults and collapse structures that intersect hydrogeologic units were also identified in the <span class="hlt">seismic</span> profile. The information provided in the cross sections and the <span class="hlt">seismic</span> profile is preliminary and subject to revision.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030022709','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030022709"><span>Foundations of the Bandera <span class="hlt">Abstraction</span> Tools</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hatcliff, John; Dwyer, Matthew B.; Pasareanu, Corina S.; Robby</p> <p>2003-01-01</p> <p>Current research is demonstrating that model-checking and other forms of automated finite-state verification can be effective for checking properties of software systems. Due to the exponential costs associated with model-checking, multiple forms of <span class="hlt">abstraction</span> are often necessary to obtain system models that are tractable for automated checking. The Bandera Tool Set provides multiple forms of automated support for compiling concurrent Java software systems to models that can be supplied to several different model-checking tools. In this paper, we describe the foundations of Bandera's data <span class="hlt">abstraction</span> mechanism which is used to reduce the cardinality (and the program's state-space) of data domains in software to be model-checked. From a technical standpoint, the form of data <span class="hlt">abstraction</span> used in Bandera is simple, and it is based on classical presentations of <span class="hlt">abstract</span> <span class="hlt">interpretation</span>. We describe the mechanisms that Bandera provides for declaring <span class="hlt">abstractions</span>, for attaching <span class="hlt">abstractions</span> to programs, and for generating <span class="hlt">abstracted</span> programs and properties. The contributions of this work are the design and implementation of various forms of tool support required for effective application of data <span class="hlt">abstraction</span> to software components written in a programming language like Java which has a rich set of linguistic features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28916778','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28916778"><span>Hydrogeochemical changes before and during the 2016 Amatrice-Norcia <span class="hlt">seismic</span> sequence (central Italy).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barberio, Marino Domenico; Barbieri, Maurizio; Billi, Andrea; Doglioni, Carlo; Petitta, Marco</p> <p>2017-09-15</p> <p><span class="hlt">Seismic</span> precursors are an as yet unattained frontier in earthquake studies. With the aim of making a step towards this frontier, we present a hydrogeochemical dataset associated with the 2016 Amatrice-Norcia <span class="hlt">seismic</span> sequence (central Apennines, Italy), developed from August 24 th , with an M w 6.0 event, and culminating on October 30 th , with an M w 6.5 mainshock. The <span class="hlt">seismic</span> sequence occurred during a seasonal depletion of hydrostructures, and the four strongest earthquakes (M w  ≥ 5.5) generated an abrupt uplift of the water level, recorded up to 100 km away from the mainshock area. Monitoring a set of selected springs in the central Apennines, a few hydrogeochemical anomalies were observed months before the onset of the <span class="hlt">seismic</span> swarm, including a variation of pH values and an increase of As, V, and Fe concentrations. Cr concentrations increased immediately after the onset of the <span class="hlt">seismic</span> sequence. On November 2016, these elements recovered to their usual low concentrations. We <span class="hlt">interpret</span> these geochemical anomalies as reliable <span class="hlt">seismic</span> precursors for a dilational tectonic setting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApGeo..14..258F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApGeo..14..258F"><span><span class="hlt">Seismic</span> wavefield modeling based on time-domain symplectic and Fourier finite-difference method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fang, Gang; Ba, Jing; Liu, Xin-xin; Zhu, Kun; Liu, Guo-Chang</p> <p>2017-06-01</p> <p><span class="hlt">Seismic</span> wavefield modeling is important for improving <span class="hlt">seismic</span> data processing and <span class="hlt">interpretation</span>. Calculations of wavefield propagation are sometimes not stable when forward modeling of <span class="hlt">seismic</span> wave uses large time steps for long times. Based on the Hamiltonian expression of the acoustic wave equation, we propose a structure-preserving method for <span class="hlt">seismic</span> wavefield modeling by applying the symplectic finite-difference method on time grids and the Fourier finite-difference method on space grids to solve the acoustic wave equation. The proposed method is called the symplectic Fourier finite-difference (symplectic FFD) method, and offers high computational accuracy and improves the computational stability. Using acoustic approximation, we extend the method to anisotropic media. We discuss the calculations in the symplectic FFD method for <span class="hlt">seismic</span> wavefield modeling of isotropic and anisotropic media, and use the BP salt model and BP TTI model to test the proposed method. The numerical examples suggest that the proposed method can be used in <span class="hlt">seismic</span> modeling of strongly variable velocities, offering high computational accuracy and low numerical dispersion. The symplectic FFD method overcomes the residual qSV wave of <span class="hlt">seismic</span> modeling in anisotropic media and maintains the stability of the wavefield propagation for large time steps.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH53B0148S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH53B0148S"><span>Submarine Landslide Hazards Offshore Southern Alaska: <span class="hlt">Seismic</span> Strengthening Versus Rapid Sedimentation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sawyer, D.; Reece, R.; Gulick, S. P. S.; Lenz, B. L.</p> <p>2017-12-01</p> <p>The southern Alaskan offshore margin is prone to submarine landslides and tsunami hazards due to <span class="hlt">seismically</span> active plate boundaries and extreme sedimentation rates from glacially enhanced mountain erosion. We examine the submarine landslide potential with new shear strength measurements acquired by Integrated Ocean Drilling Program Expedition 341 on the continental slope and Surveyor Fan. These data reveal lower than expected sediment strength. Contrary to other active margins where <span class="hlt">seismic</span> strengthening enhances slope stability, the high-sedimentation margin offshore southern Alaska behaves like a passive margin from a shear strength perspective. We <span class="hlt">interpret</span> that <span class="hlt">seismic</span> strengthening occurs but is offset by high sedimentation rates and overpressure within the slope and Surveyor Fan. This conclusion is supported because shear strength follows an expected active margin profile outside of the fan, where background sedimentation rates occur. More broadly, <span class="hlt">seismically</span> active margins with wet-based glaciers are susceptible to submarine landslide hazards because of the combination of high sedimentation rates and earthquake shaking</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5459C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5459C"><span>Ischia Island: Historical <span class="hlt">Seismicity</span> and Dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carlino, S.; Cubellis, E.; Iannuzzi, R.; Luongo, G.; Obrizzo, F.</p> <p>2003-04-01</p> <p>The <span class="hlt">seismic</span> energy release in volcanic areas is a complex process and the island of Ischia provides a significant scenario of historical <span class="hlt">seismicity</span>. This is characterized by the occurence of earthquakes with low energy and high intensity. Information on the <span class="hlt">seismicity</span> of the island spans about eight centuries, starting from 1228. With regard to effects, the most recent earthquake of 1883 is extensively documented both in the literature and unpublished sources. The earthquake caused 2333 deaths and the destruction of the historical and environmental heritage of some areas of the island. The most severe damage occurred in Casamicciola. This event, which was the first great catastrophe after the unification of Italy in the 1860s (Imax = XI degree MCS), represents an important date in the prevention of natural disasters, in that it was after this earthquake that the first <span class="hlt">Seismic</span> Safety Act in Italy was passed by which lower risk zones were identified for new settlements. Thanks to such detailed analysis, reliable modelling of the <span class="hlt">seismic</span> source was also obtained. The historical data onwards makes it possible to identify the area of the epicenter of all known earthquakes as the northern slope of Monte Epomeo, while analysis of the effects of earthquakes and the geological structures allows us to evaluate the stress fields that generate the earthquakes. In a volcanic area, <span class="hlt">interpretation</span> of the mechanisms of release and propagation of <span class="hlt">seismic</span> energy is made even more complex as the stress field that acts at a regional level is compounded by that generated from migration of magmatic masses towards the surface, as well as the rheologic properties of the rocks dependent on the high geothermic gradient. Such structural and dynamic conditions make the island of Ischia a <span class="hlt">seismic</span> area of considerable interest. It would appear necessary to evaluate the expected damage caused by a new event linked to the renewal of dynamics of the island, where high population density and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS.995a2105I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS.995a2105I"><span>Rippability Assessment of Weathered Sedimentary Rock Mass using <span class="hlt">Seismic</span> Refraction Methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ismail, M. A. M.; Kumar, N. S.; Abidin, M. H. Z.; Madun, A.</p> <p>2018-04-01</p> <p>Rippability or ease of excavation in sedimentary rocks is a significant aspect of the preliminary work of any civil engineering project. Rippability assessment was performed in this study to select an available ripping machine to rip off earth materials using the <span class="hlt">seismic</span> velocity chart provided by Caterpillar. The research area is located at the proposed construction site for the development of a water reservoir and related infrastructure in Kampus Pauh Putra, Universiti Malaysia Perlis. The research was aimed at obtaining <span class="hlt">seismic</span> velocity, P-wave (Vp) using a <span class="hlt">seismic</span> refraction method to produce a 2D tomography model. A 2D <span class="hlt">seismic</span> model was used to delineate the layers into the velocity profile. The conventional geotechnical method of using a borehole was integrated with the <span class="hlt">seismic</span> velocity method to provide appropriate correlation. The correlated data can be used to categorize machineries for excavation activities based on the available systematic analysis procedure to predict rock rippability. The <span class="hlt">seismic</span> velocity profile obtained was used to <span class="hlt">interpret</span> rock layers within the ranges labelled as rippable, marginal, and non-rippable. Based on the <span class="hlt">seismic</span> velocity method the site can be classified into loose sand stone to moderately weathered rock. Laboratory test results shows that the site’s rock material falls between low strength and high strength. Results suggest that Caterpillar’s smallest ripper, namely, D8R, can successfully excavate materials based on the test results integration from <span class="hlt">seismic</span> velocity method and laboratory test.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7271755-new-madrid-seismic-zone-recurrence-intervals','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7271755-new-madrid-seismic-zone-recurrence-intervals"><span>New Madrid <span class="hlt">seismic</span> zone recurrence intervals</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>Schweig, E.S.; Ellis, M.A.</p> <p>1993-03-01</p> <p>Frequency-magnitude relations in the New Madrid <span class="hlt">seismic</span> zone suggest that great earthquakes should occur every 700--1,200 yrs, implying relatively high strain rates. These estimates are supported by some geological and GPS results. Recurrence intervals of this order should have produced about 50 km of strike-slip offset since Miocene time. No subsurface evidence for such large displacements is known within the <span class="hlt">seismic</span> zone. Moreover, the irregular fault pattern forming a compressive step that one sees today is not compatible with large displacements. There are at least three possible <span class="hlt">interpretations</span> of the observations of short recurrence intervals and high strain rates, butmore » apparently youthful fault geometry and lack of major post-Miocene deformation. One is that the seismological and geodetic evidence are misleading. A second possibility is that activity in the region is cyclic. That is, the geological and geodetic observations that suggest relatively short recurrence intervals reflect a time of high, but geologically temporary, pore-fluid pressure. Zoback and Zoback have suggested such a model for intraplate <span class="hlt">seismicity</span> in general. Alternatively, the New Madrid <span class="hlt">seismic</span> zone is geologically young feature that has been active for only the last few tens of thousands of years. In support of this, observe an irregular fault geometry associated with a unstable compressive step, a series of en echelon and discontinuous lineaments that may define the position of a youthful linking fault, and the general absence of significant post-Eocene faulting or topography.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008GeoJI.173..642J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008GeoJI.173..642J"><span>2-D traveltime and waveform inversion for improved <span class="hlt">seismic</span> imaging: Naga Thrust and Fold Belt, India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jaiswal, Priyank; Zelt, Colin A.; Bally, Albert W.; Dasgupta, Rahul</p> <p>2008-05-01</p> <p>Exploration along the Naga Thrust and Fold Belt in the Assam province of Northeast India encounters geological as well as logistic challenges. Drilling for hydrocarbons, traditionally guided by surface manifestations of the Naga thrust fault, faces additional challenges in the northeast where the thrust fault gradually deepens leaving subtle surface expressions. In such an area, multichannel 2-D <span class="hlt">seismic</span> data were collected along a line perpendicular to the trend of the thrust belt. The data have a moderate signal-to-noise ratio and suffer from ground roll and other acquisition-related noise. In addition to data quality, the complex geology of the thrust belt limits the ability of conventional <span class="hlt">seismic</span> processing to yield a reliable velocity model which in turn leads to poor subsurface image. In this paper, we demonstrate the application of traveltime and waveform inversion as supplements to conventional <span class="hlt">seismic</span> imaging and <span class="hlt">interpretation</span> processes. Both traveltime and waveform inversion utilize the first arrivals that are typically discarded during conventional <span class="hlt">seismic</span> processing. As a first step, a smooth velocity model with long wavelength characteristics of the subsurface is estimated through inversion of the first-arrival traveltimes. This velocity model is then used to obtain a Kirchhoff pre-stack depth-migrated image which in turn is used for the <span class="hlt">interpretation</span> of the fault. Waveform inversion is applied to the central part of the <span class="hlt">seismic</span> line to a depth of ~1 km where the quality of the migrated image is poor. Waveform inversion is performed in the frequency domain over a series of iterations, proceeding from low to high frequency (11-19 Hz) using the velocity model from traveltime inversion as the starting model. In the end, the pre-stack depth-migrated image and the waveform inversion model are jointly <span class="hlt">interpreted</span>. This study demonstrates that a combination of traveltime and waveform inversion with Kirchhoff pre-stack depth migration is a promising approach</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ApGeo..12...79Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ApGeo..12...79Z"><span>Three-component <span class="hlt">seismic</span> data in thin interbedded reservoir exploration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Li-Yan; Wang, Yan-Chun; Pei, Jiang-Yun</p> <p>2015-03-01</p> <p>We present the first successful application of three-component <span class="hlt">seismic</span> data to thin interbedded reservoir characterization in the Daqing placanticline of the LMD oilfield. The oilfield has reached the final high water cut stage and the principal problem is how to recognize the boundaries of sand layers that are thicker than 2 m. Conventional <span class="hlt">interpretation</span> of single PP-wave <span class="hlt">seismic</span> data results in multiple solutions, whereas the introduction of PS-wave enhances the reliability of <span class="hlt">interpretation</span>. We analyze the gas reservoir characteristics by joint PP- and PS-waves, and use the amplitude and frequency decomposition attributes to delineate the gas reservoir boundaries because of the minimal effect of fluids on S-wave. We perform joint inversion of PP- and PS-waves to obtain V P/ V S, λρ, and µ ρ and map the lithology changes by using density, λρ, and µ ρ. The 3D-3C attribute λρ slices describe the sand layers distribution, while considering the well log data, and point to favorable region for tapping the remaining oil.</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('http://adsabs.harvard.edu/abs/2016AGUFM.S53E..04L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S53E..04L"><span><span class="hlt">Seismic</span> variability and structural controls on fluid migration in Northern Oklahoma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lambert, C.; Keranen, K. M.; Stevens, N. T.</p> <p>2016-12-01</p> <p>The broad region of <span class="hlt">seismicity</span> in northern Oklahoma encompasses distinct structural settings; notably, the area contains both high-length, high-offset faults bounding a major structural uplift (the Nemaha uplift), and also encompasses regions of distributed, low-length, low-offset faults on either side of the uplift. <span class="hlt">Seismicity</span> differs between these structural settings in mode of migration, rate, magnitude, and mechanism. Here we use our catalog from 2015-2016, acquired using a dense network of 55 temporary broadband seismometers, complemented by data from 40+ regional stations, including the IRIS Wavefields stations. We compare <span class="hlt">seismicity</span> between these structural settings using precise earthquake locations, focal mechanism solutions, and body-wave tomography. Within and along the dominant Nemaha uplift, earthquakes rarely occur on one of the primary uplift-bounding faults. Earthquakes instead occur within the uplift on isolated, discrete faults, and migrate gradually along these faults at 20-30 m/day. The regions peripheral to the uplift hosted the majority of earthquakes within the year, on multiple series of frequently unmapped, densely-spaced, subparallel faults. We did not detect a similar slow migration along these faults. Earthquakes instead occurred via progressive failure of individual segments along a fault, or jumped abruptly from one fault to another nearby. Mechanisms in both regions are dominantly strike-slip, with the <span class="hlt">interpreted</span> dominant fault plane orientation rotating from N100E in the Wavefields area (west of the uplift) to N50E (within the uplift). We <span class="hlt">interpret</span> that the distinct variation in <span class="hlt">seismicity</span> may result from the variation in fault density and length between the uplift and the surrounding regions. <span class="hlt">Seismic</span> velocity within the upper basement of the uplift is lower than the velocity on either side, possibly indicative of enhanced fracturing within the uplift, as seen in the Nemaha uplift to the north. The fracturing, along with the large</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNS13A0008T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNS13A0008T"><span><span class="hlt">Seismic</span> Imaging of a Prospective Geothermal Play, Using a Dense Geophone Array</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Trow, A.; Pankow, K. L.; Wannamaker, P. E.; Lin, F. C.; Ward, K. M.</p> <p>2017-12-01</p> <p>In the summer of 2016 a dense array of 48 Nodal <span class="hlt">Seismic</span> geophones was deployed near Beaver, Utah on the eastern flank of the Mineral Mountains. The array aperture was approximately 20 kilometers and recorded continuous <span class="hlt">seismic</span> data for 30 days. Geophones were centered on a previously known shallow (5km depth) magnetolluric (MT) low-resistivity body. This region of low resistivity was <span class="hlt">interpreted</span> to possibly contain hydrothermal/geothermal fluids and was targeted for further <span class="hlt">seismic</span> investigation. The <span class="hlt">seismic</span> array geometry was designed to optimize <span class="hlt">seismic</span> event detection for small (magnitude of completeness zero) earthquakes and to facilitate <span class="hlt">seismic</span> imaging at depths of 5 km and deeper. For the duration of the experiment, one ML 1 earthquake was detected underneath the array with 15 other earthquakes detected to the east and south in the more <span class="hlt">seismically</span> active Pavant Range. Different passive imaging techniques, including ambient noise and earthquake tomography are being explored in order to produce a <span class="hlt">seismic</span> velocity image. Understanding the subsurface, specifically the fracture network and fluid content of the bedrock is important for characterization of a geothermal prospect. If it is rich in fluids, it can be assumed that some fracture network is in place to accommodate such fluids. Both fractures and fluid content of the prospect will have an effect on the <span class="hlt">seismic</span> velocities in the basement structure. These properties can help determine the viability of a geothermal system for power production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997JGR...10218267H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997JGR...10218267H"><span>Origin and nature of crystal reflections: Results from integrated <span class="hlt">seismic</span> measurements at the KTB superdeep drilling site</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harjes, H.-P.; Bram, K.; Dürbaum, H.-J.; Gebrande, H.; Hirschmann, G.; Janik, M.; KlöCkner, M.; Lüschen, E.; Rabbel, W.; Simon, M.; Thomas, R.; Tormann, J.; Wenzel, F.</p> <p>1997-08-01</p> <p>For almost 10 years the KTB superdeep drilling project has offered an excellent field laboratory for adapting <span class="hlt">seismic</span> techniques to crystalline environments and for testing new ideas for <span class="hlt">interpreting</span> <span class="hlt">seismic</span> reflections in terms of lithological or textural properties of metamorphic rock units. The <span class="hlt">seismic</span> investigations culminated in a three-dimensional (3-D) reflection survey on a 19×19 km area with the drill site at its center. <span class="hlt">Interpretation</span> of these data resulted in a detailed, structural model of the German Continental Deep Drilling Program (KTB) location with dominant, steep faults in the upper crust. The 3-D reflection survey was part of a suite of <span class="hlt">seismic</span> experiments, ranging from wide-angle reflection and refraction profiles to standard vertical <span class="hlt">seismic</span> profiles (VSP) and more sophisticated surface-to-borehole observations. It was predicted that the drill bit would meet the most prominent, steeply dipping, crustal reflector at a depth of about 6500-7000 m, and indeed, the borehole penetrated a major fault zone in the depth interval between 6850 and 7300 m. This reflector offered the rare opportunity to relate logging results, reflective properties, and geology to observed and modeled data. Post-Variscan thrusting caused cataclastic deformation, with partial, strong alterations within a steeply dipping reverse fault zone. This process generated impedance contrasts within the fault zone on a lateral scale large enough to cause <span class="hlt">seismic</span> reflections. This was confirmed by borehole measurements along the whole 9.1 km deep KTB profile. The strongest, reflected signals originated from fluid-filled fractures and cataclastic fracture zones rather than from lithological boundaries (i.e., first-order discontinuities between different rock types) or from texture- and/or foliation-induced anisotropy. During the <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> data at KTB several lessons were learned: Conventional processing of two-dimensional (2-D) reflection data from a presite survey</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGP34A..02N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGP34A..02N"><span>Homogenization of Electromagnetic and <span class="hlt">Seismic</span> Wavefields for Joint Inverse Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Newman, G. A.; Commer, M.; Petrov, P.; Um, E. S.</p> <p>2011-12-01</p> <p>A significant obstacle in developing a robust joint imaging technology exploiting <span class="hlt">seismic</span> and electromagnetic (EM) wave fields is the resolution at which these different geophysical measurements sense the subsurface. Imaging of <span class="hlt">seismic</span> reflection data is an order of magnitude finer in resolution and scale compared to images produced with EM data. A consistent joint image of the subsurface geophysical attributes (velocity, electrical conductivity) requires/demands the different geophysical data types be similar in their resolution of the subsurface. The superior resolution of <span class="hlt">seismic</span> data results from the fact that the energy propagates as a wave, while propagation of EM energy is diffusive and attenuates with distance. On the other hand, the complexity of the <span class="hlt">seismic</span> wave field can be a significant problem due to high reflectivity of the subsurface and the generation of multiple scattering events. While <span class="hlt">seismic</span> wave fields have been very useful in mapping the subsurface for energy resources, too much scattering and too many reflections can lead to difficulties in imaging and <span class="hlt">interpreting</span> <span class="hlt">seismic</span> data. To overcome these obstacles a formulation for joint imaging of <span class="hlt">seismic</span> and EM wave fields is introduced, where each data type is matched in resolution. In order to accomplish this, <span class="hlt">seismic</span> data are first transformed into the Laplace-Fourier Domain, which changes the modeling of the <span class="hlt">seismic</span> wave field from wave propagation to diffusion. Though high frequency information (reflectivity) is lost with this transformation, several benefits follow: (1) <span class="hlt">seismic</span> and EM data can be easily matched in resolution, governed by the same physics of diffusion, (2) standard least squares inversion works well with diffusive type problems including both transformed <span class="hlt">seismic</span> and EM, (3) joint imaging of <span class="hlt">seismic</span> and EM data may produce better starting velocity models critical for successful reverse time migration or full waveform imaging of <span class="hlt">seismic</span> data (non transformed) and (4</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5955145-areal-distribution-sedimentary-facies-determined-from-seismic-facies-analysis-models-modern-depositional-systems','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5955145-areal-distribution-sedimentary-facies-determined-from-seismic-facies-analysis-models-modern-depositional-systems"><span>Areal distribution of sedimentary facies determined from <span class="hlt">seismic</span> facies analysis and models of modern depositional systems</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>Seramur, K.C.; Powell, R.D.; Carpenter, P.J.</p> <p>1988-01-01</p> <p><span class="hlt">Seismic</span> facies analysis was applied to 3.5-kHz single-channel analog reflection profiles of the sediment fill within Muir Inlet, Glacier Bay, southeast Alaska. Nine sedimentary facies have been <span class="hlt">interpreted</span> from seven <span class="hlt">seismic</span> facies identified on the profiles. The <span class="hlt">interpretations</span> are based on reflection characteristics and structural features of the <span class="hlt">seismic</span> facies. The following reflection characteristics and structural features are used: reflector spacing, amplitude and continuity of reflections, internal reflection configurations, attitude of reflection terminations at a facies boundary, body geometry of a facies, and the architectural associations of <span class="hlt">seismic</span> facies within each basin. The depositional systems are reconstructed by determining themore » paleotopography, bedding patterns, sedimentary facies, and modes of deposition within the basin. Muir Inlet is a recently deglaciated fjord for which successive glacier terminus positions and consequent rates of glacial retreat are known. In this environment the depositional processes and sediment characteristics vary with distance from a glacier terminus, such that during a retreat a record of these variations is preserved in the aggrading sediment fill. Sedimentary facies within the basins of lower Muir Inlet are correlated with observed depositional processes near the present glacier terminus in the upper inlet.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4319N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4319N"><span>How <span class="hlt">seismicity</span> and shear stress-generated tilt can indicate imminent explosions on Tungurahua</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neuberg, Jurgen; Mothes, Patricia; Collinson, Amy; Marsden, Luke</p> <p>2017-04-01</p> <p><span class="hlt">Seismic</span> swarms and tilt measurement on active silicic volcanoes have been successfully used to assess their eruption potential. Swarms of low-frequency <span class="hlt">seismic</span> events have been associated with brittle failure or stick-slip motion of magma during ascent and have been used to estimate qualitatively the magma ascent. Tilt signals are extremely sensitive indicators for volcano deformation and their <span class="hlt">interpretation</span> includes shear stress as a generating source as well as inflation or deflation of a shallow magma reservoir. Here we use data sets from different tiltmeters deployed on Tungurahua volcano, Ecuador, and contrast the two source models for different locations and time intervals. We analyse a simultaneously recorded <span class="hlt">seismic</span> data set and address the question of shear stress partitioning resulting in both the generation of tilt and low-frequency <span class="hlt">seismicity</span> in critical phases prior to Vulcanion explosions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18.1111G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18.1111G"><span>Variations in pockmark composition at the Vestnesa Ridge: Insights from marine controlled source electromagnetic and <span class="hlt">seismic</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>Goswami, Bedanta K.; Weitemeyer, Karen A.; Bünz, Stefan; Minshull, Timothy A.; Westbrook, Graham K.; Ker, Stephan; Sinha, Martin C.</p> <p>2017-03-01</p> <p>The Vestnesa Ridge marks the northern boundary of a known submarine gas hydrate province in the west Svalbard margin. Several seafloor pockmarks at the eastern segment of the ridge are sites of active methane venting. Until recently, <span class="hlt">seismic</span> reflection data were the main tool for imaging beneath the ridge. Coincident controlled source electromagnetic (CSEM), high-resolution two-dimensional (2-D) airgun, sweep frequency SYSIF, and three-dimensional (3-D) p-cable <span class="hlt">seismic</span> reflection data were acquired at the south-eastern part of the ridge between 2011 and 2013. The CSEM and <span class="hlt">seismic</span> data contain profiles across and along the ridge, passing several active and inactive pockmarks. Joint <span class="hlt">interpretation</span> of resistivity models obtained from CSEM and <span class="hlt">seismic</span> reflection data provides new information regarding the fluid composition beneath the pockmarks. There is considerable variation in transverse resistance and <span class="hlt">seismic</span> reflection characteristics of the gas hydrate stability zone (GHSZ) between the ridge flanks and chimneys beneath pockmarks. Layered <span class="hlt">seismic</span> reflectors on the flanks are associated with around 300 Ωm2 transverse resistance, whereas the <span class="hlt">seismic</span> reflectors within the chimneys exhibit amplitude blanking and chaotic patterns. The transverse resistance of the GHSZ within the chimneys vary between 400 and 1200 Ωm2. Variance attributes obtained from the 3-D p-cable data also highlight faults and chimneys, which coincide with the resistivity anomalies. Based on the joint data <span class="hlt">interpretation</span>, widespread gas hydrate presence is likely at the ridge, with both hydrates and free gas contained within the faults and chimneys. However, at the active chimneys the effect of gas likely dominates the resistive anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000Tectp.329..269B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000Tectp.329..269B"><span>Deep <span class="hlt">seismic</span> reflection evidence for ancient subduction and collision zones within the continental lithosphere of northwestern Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Balling, N.</p> <p>2000-12-01</p> <p>Deep <span class="hlt">seismic</span> profiling experiments in the region of NW Europe (including BABEL in the Gulf of Bothnia and the Baltic Sea, Mobil Search in the Skagerrak and MONA LISA in the North Sea) have demonstrated the existence of <span class="hlt">seismic</span> reflectors in the mantle lithosphere beneath the Baltic Shield, the Tornquist Zone and the North Sea basins. Different sets of reflectors are observed, notably dipping and sub-horizontal. Dipping, distinct reflectivity, which may be followed from Moho/Moho offsets into the deeper parts of the continental lithosphere, is of special interest because of its tectonic and geodynamic significance. Such reflectivity, observed in several places, dipping 15-35° and covering a depth range of 30-90 km, constrained by surface geological information and radiometric age data, is <span class="hlt">interpreted</span> to represent fossil, ancient subduction and collison zones. Subduction slabs with remnant oceanic basaltic crust transformed into eclogite is assumed, in particular, to generate deep <span class="hlt">seismic</span> reflectivity. Deep <span class="hlt">seismic</span> evidence is presented for subduction, crustal accretion and collision processes with inferred ages from 1.9 to 1.1 Ga from the main structural provinces within the Baltic Shield including Svecofennian, Transscandinavian Igneous Belt, Gothian and Sveconorwegian. Along the southwestern border of Baltica (in the southeastern North Sea) south-dipping crustal and sub-crustal reflectivity is observed down to a depth of about 90 km, close to the lithosphere-asthenosphere boundary. These structures are <span class="hlt">interpreted</span> to reveal a lithosphere-scale Caledonian (ca. 440 Ma) suture zone resulting from the closure of the Tornquist Sea/Thor Ocean and the amalgamation of Baltica and Eastern Avalonia. These results demonstrate that deep structures within the continental lithosphere, originating from early crust-forming plate tectonic processes, may survive for a very long time and form <span class="hlt">seismic</span> marker reflectivity of great value in geotectonic <span class="hlt">interpretation</span> and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT........97K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT........97K"><span>A study of the Herald-Phillipstown fault in the Wabash Valley using drillhole and 3-D <span class="hlt">seismic</span> reflection data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kroenke, Samantha E.</p> <p></p> <p>In June 2009, a 2.2 square mile 3-D high resolution <span class="hlt">seismic</span> reflection survey was shot in southeastern Illinois in the Phillipstown Consolidated oilfield. A well was drilled in the 3-D survey area to tie the <span class="hlt">seismic</span> to the geological data with a synthetic seismogram from the sonic log. The objectives of the 3-D <span class="hlt">seismic</span> survey were three-fold: (1) To image and <span class="hlt">interpret</span> faulting of the Herald-Phillipstown Fault using drillhole-based geological and <span class="hlt">seismic</span> cross-sections and structural contour maps created from the drillhole data and <span class="hlt">seismic</span> reflection data, (2) To test the effectiveness of imaging the faults by selected <span class="hlt">seismic</span> attributes, and (3) To compare spectral decomposition amplitude maps with an isochron map and an isopach map of a selected geologic interval (VTG interval). Drillhole and <span class="hlt">seismic</span> reflection data show that various formation offsets increase near the main Herald-Phillipstown fault, and that the fault and its large offset subsidiary faults penetrate the Precambrian crystalline basement. A broad, northeast-trending 10,000 feet wide graben is consistently observed in the drillhole data. Both shallow and deep formations in the geological cross-sections reveal small horst and graben features within the broad graben created possibly in response to fault reactivations. The HPF faults have been <span class="hlt">interpreted</span> as originally Precambrian age high-angle, normal faults reactivated with various amounts and types of offset. Evidence for strike-slip movement is also clear on several faults. Changes in the <span class="hlt">seismic</span> attribute values in the selected interval and along various time slices throughout the whole dataset correlate with the Herald-Phillipstown faults. Overall, <span class="hlt">seismic</span> attributes could provide a means of mapping large offset faults in areas with limited or absent drillhole data. Results of the spectral decomposition suggest that if the interval velocity is known for a particular formation or interval, high-resolution 3-D <span class="hlt">seismic</span> reflection surveys could</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MsT.........18G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MsT.........18G"><span>The Summerville Formation: Evidence for a sub-horizontal stratigraphic sequence below the post-rift unconformity in the Middleton Place Summerville <span class="hlt">Seismic</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>Getz, Joseph Edward</p> <p></p> <p>The Middleton Place Summerville <span class="hlt">Seismic</span> Zone (MPSSZ) near Summerville, South Carolina was the site of renewed extensive investigation, beginning in the 1970's, for the source of the 1886 Charleston earthquake. Reactivation of faults associated with a putative fault-bounded Triassic rift basin through analysis of <span class="hlt">seismic</span> reflection, <span class="hlt">seismic</span> refraction, and well data has since become the favored <span class="hlt">interpretation</span> for the source of MPSSZ <span class="hlt">seismicity</span>. Critical to this <span class="hlt">interpretation</span> is the association of continental redbed sedimentary rocks with Triassic basins identified throughout the North American Atlantic margin. Reanalysis of 18 <span class="hlt">seismic</span> reflection profiles and 25 <span class="hlt">seismic</span> refraction profiles within the MPSSZ suggests that the red beds found here are a thin, sub-horizontal, regionally extensive, generally unbroken subsurface stratigraphic sequence distinct from the sedimentary architecture observed in analog Triassic rift systems. In addition, this sequence appears to unconformably overly a structural depression (the Jedberg basin) previously <span class="hlt">interpreted</span> as a Triassic rift basin in the vicinity of the MPSSZ. In addition to the geometries observed on <span class="hlt">seismic</span> reflection profiles, <span class="hlt">seismic</span> refraction velocities ranging from 4.2 to 6.1 km/s can be correlated with (1) Jurassic basalt flows, (2) the newly proposed Summerville Formation, and (3) the Basement (B) sequences respectively. The current study maps the Summerville red bed section and its bounding reflectors. In addition to mapping the regional extent of the newly proposed Summerville Formation, refraction velocities and changes in reflection character, the lateral extent of the basalt flows can be changed to a more localized flow rather than a regionally extensive flow of which was previously thought. Reanalysis of data in the MPSSZ suggests that the area may not be part of the Triassic South Georgia Rift system due to the sub-horizontal geometry of the red bed reflections, the apparent lack of faulting, and their</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..132a2035P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..132a2035P"><span>Passive <span class="hlt">Seismic</span> for Hydrocarbon Indicator : Between Expectation and Reality</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pandito, Riky H. B.</p> <p>2018-03-01</p> <p>In between 5 – 10 years, in our country, passive <span class="hlt">seismic</span> method became more popular to finding hydrocarbon. Low price, nondestructive acquisition and easy to mobilization is the best reason for choose the method. But in the other part, some people are pessimistically to deal with the result. Instrument specification, data condition and processing methods is several points which influence characteristic and <span class="hlt">interpretation</span> passive <span class="hlt">seismic</span> result. In 2010 one prospect in East Java Basin has been measurement constist of 112 objective points and several calibration points. Data measurement results indicate a positive response. Furthermore, in 2013 exploration drliing conducted on the prospect. Drill steam test showes 22 MMCFD in objective zone, upper – late oligocene. In 2015, remeasurement taken in objective area and show consistent responses with previous measurement. Passive <span class="hlt">seismic</span> is unique method, sometimes will have difference results on dry, gas and oil area, in field production and also temporary suspend area with hidrocarbon content.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/924622','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/924622"><span>4-D High-Resolution <span class="hlt">Seismic</span> Reflection Monitoring of Miscible CO2 Injected into a Carbonate Reservoir</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>Richard D. Miller; Abdelmoneam E. Raef; Alan P. Byrnes</p> <p>2007-06-30</p> <p>The objective of this research project was to acquire, process, and <span class="hlt">interpret</span> multiple high-resolution 3-D compressional wave and 2-D, 2-C shear wave <span class="hlt">seismic</span> data in the hopes of observing changes in fluid characteristics in an oil field before, during, and after the miscible carbon dioxide (CO{sub 2}) flood that began around December 1, 2003, as part of the DOE-sponsored Class Revisit Project (DOE No.DE-AC26-00BC15124). Unique and key to this imaging activity is the high-resolution nature of the <span class="hlt">seismic</span> data, minimal deployment design, and the temporal sampling throughout the flood. The 900-m-deep test reservoir is located in central Kansas oomoldic limestonesmore » of the Lansing-Kansas City Group, deposited on a shallow marine shelf in Pennsylvanian time. After 30 months of <span class="hlt">seismic</span> monitoring, one baseline and eight monitor surveys clearly detected changes that appear consistent with movement of CO{sub 2} as modeled with fluid simulators and observed in production data. Attribute analysis was a very useful tool in enhancing changes in <span class="hlt">seismic</span> character present, but difficult to <span class="hlt">interpret</span> on time amplitude slices. Lessons learned from and tools/techniques developed during this project will allow high-resolution <span class="hlt">seismic</span> imaging to be routinely applied to many CO{sub 2} injection programs in a large percentage of shallow carbonate oil fields in the midcontinent.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S21A2148T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S21A2148T"><span><span class="hlt">Seismic</span> Sources for the Territory of Georgia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsereteli, N. S.; Varazanashvili, O.</p> <p>2011-12-01</p> <p> will be obtained on the bases of structural geology, parameters of <span class="hlt">seismicity</span> and seismotectonics. This last approach was used by us. For achievement of this purpose it was necessary to solve following problems: to calculate the parameters of seismotectonic deformation; to reveal regularities in character of earthquake fault plane solution; use obtained regularities to develop principles of an establishment of borders between various hierarchical and scale levels of <span class="hlt">seismic</span> deformations fields and to give their geological <span class="hlt">interpretation</span>; Three dimensional matching of active faults with real geometrical dimension and earthquake sources have been investigated. Finally each zone have been defined with the parameters: the geometry, the magnitude-frequency parameters, maximum magnitude, and depth distribution as well as modern dynamical characteristics widely used for complex processes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4502396','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4502396"><span><span class="hlt">Seismic</span> footprints of shallow dyke propagation at Etna, Italy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Falsaperla, Susanna; Neri, Marco</p> <p>2015-01-01</p> <p>One of the key issues in forecasting volcanic eruptions is to detect signals that can track the propagation of dykes towards the surface. Continuous monitoring of active volcanoes helps significantly in achieving this goal. The <span class="hlt">seismic</span> data presented here are unique, as they document surface faulting processes close (tens to a few hundred meters) to their source, namely the dyke tip. They originated nearby - and under - a <span class="hlt">seismic</span> station that was subsequently destroyed by lava flows during eruptive activity at Etna volcano, Italy, in 2013. On February 20, a ~600 m-long and ~120 m wide NW-SE fracture field opened at an altitude between 2750 and 2900 m. The consequent rock dislocation caused the station to tilt and offset the <span class="hlt">seismic</span> signal temporarily. Data acquisition continued until the arrival of the lava flow that led to the breakdown of the transmission system. Shallow ground fracturing and repeated low-frequency oscillations occurred during two stages in which the <span class="hlt">seismic</span> signal underwent a maximum offset ~2.57 × 104 nm/s. Bridging instrumental recordings, fieldwork and conceptual modelling, these data are <span class="hlt">interpreted</span> as the <span class="hlt">seismic</span> footprints of a magmatic dyke intrusion that moved at speed ~0.02 m/s (first stage) and 0.46 m/s (second stage). PMID:26173557</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2005/5048/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2005/5048/"><span>Well log analysis to assist the <span class="hlt">interpretation</span> of 3-D <span class="hlt">seismic</span> data at Milne Point, north slope of Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lee, Myung W.</p> <p>2005-01-01</p> <p>In order to assess the resource potential of gas hydrate deposits in the North Slope of Alaska, 3-D <span class="hlt">seismic</span> and well data at Milne Point were obtained from BP Exploration (Alaska), Inc. The well-log analysis has three primary purposes: (1) Estimate gas hydrate or gas saturations from the well logs; (2) predict P-wave velocity where there is no measured P-wave velocity in order to generate synthetic seismograms; and (3) edit P-wave velocities where degraded borehole conditions, such as washouts, affected the P-wave measurement significantly. Edited/predicted P-wave velocities were needed to map the gas-hydrate-bearing horizons in the complexly faulted upper part of 3-D <span class="hlt">seismic</span> volume. The estimated gas-hydrate/gas saturations from the well logs were used to relate to <span class="hlt">seismic</span> attributes in order to map regional distribution of gas hydrate inside the 3-D <span class="hlt">seismic</span> grid. The P-wave velocities were predicted using the modified Biot-Gassmann theory, herein referred to as BGTL, with gas-hydrate saturations estimated from the resistivity logs, porosity, and clay volume content. The effect of gas on velocities was modeled using the classical Biot-Gassman theory (BGT) with parameters estimated from BGTL.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMNS51A1966L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMNS51A1966L"><span><p>Joint Optimization of Vertical Component Gravity and <span class="hlt">Seismic</span> P-wave First Arrivals by Simulated Annealing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Louie, J. N.; Basler-Reeder, K.; Kent, G. M.; Pullammanappallil, S. K.</p> <p>2015-12-01</p> <p>Simultaneous joint <span class="hlt">seismic</span>-gravity optimization improves P-wave velocity models in areas with sharp lateral velocity contrasts. Optimization is achieved using simulated annealing, a metaheuristic global optimization algorithm that does not require an accurate initial model. Balancing the <span class="hlt">seismic</span>-gravity objective function is accomplished by a novel approach based on analysis of Pareto charts. Gravity modeling uses a newly developed convolution algorithm, while <span class="hlt">seismic</span> modeling utilizes the highly efficient Vidale eikonal equation traveltime generation technique. Synthetic tests show that joint optimization improves velocity model accuracy and provides velocity control below the deepest headwave raypath. Detailed first arrival picking followed by trial velocity modeling remediates inconsistent data. We use a set of highly refined first arrival picks to compare results of a convergent joint <span class="hlt">seismic</span>-gravity optimization to the Plotrefa™ and SeisOpt® Pro™ velocity modeling packages. Plotrefa™ uses a nonlinear least squares approach that is initial model dependent and produces shallow velocity artifacts. SeisOpt® Pro™ utilizes the simulated annealing algorithm and is limited to depths above the deepest raypath. Joint optimization increases the depth of constrained velocities, improving reflector coherency at depth. Kirchoff prestack depth migrations reveal that joint optimization ameliorates shallow velocity artifacts caused by limitations in refraction ray coverage. <span class="hlt">Seismic</span> and gravity data from the San Emidio Geothermal field of the northwest Basin and Range province demonstrate that joint optimization changes <span class="hlt">interpretation</span> outcomes. The prior shallow-valley <span class="hlt">interpretation</span> gives way to a deep valley model, while shallow antiformal reflectors that could have been <span class="hlt">interpreted</span> as antiformal folds are flattened. Furthermore, joint optimization provides a clearer image of the rangefront fault. This technique can readily be applied to existing datasets and could</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1713883M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1713883M"><span><span class="hlt">Seismic</span> evidence of Messinian salt in opposite margins of West Mediterranean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mocnik, Arianna; Camerlenghi, Angelo; Del Ben, Anna; Geletti, Riccardo; Wardell, Nigel; Zgur, Fabrizio</p> <p>2015-04-01</p> <p>The post drift Messinian Salinity Crisis (MSC) affected the whole Mediterranean basin, with deposition of evaporitic sequences in the deep basins, in the lower continental slopes, and in several shallower marginal basins; usually, in the continental margins, the MSC originated noticeable erosional truncations that locally cause important hiatuses in the pre-Messinian sequences, covered by the Plio-Quaternary sediments. In this work we focus on the MSC <span class="hlt">seismic</span> signature of two new <span class="hlt">seismic</span> datasets acquired in 2010 (West Sardinia offshore) and in 2012 (within the Eurofleet project SALTFLU in the South Balearic continental margin and the northern Algero abyssal plain). The "Messinian trilogy" recognized in the West-Mediterranean abyssal plain, is characterized by different <span class="hlt">seismic</span> facies: the Lower evaporite Unit (LU), the salt Mobile Unit (MU) and the Upper evaporite mainly gypsiferous Unit (UU). Both <span class="hlt">seismic</span> datasets show the presence of the Messinian trilogy also if the LU is not always clearly <span class="hlt">interpretable</span> due to the strong <span class="hlt">seismic</span> signal absorption by the halite layers; the salt thickness of the MU is similar in both the basins as also the thickness and stratigraphy of the UU. The Upper Unit (UU) is made up of a well reflecting package of about 10 reflectors, partially deformed by salt tectonic and characterized by a thin transparent layer that we <span class="hlt">interpreted</span> as salt sequence inner the shallower part of the UU. Below the stratified UU, the MU exhibits a transparent layer in the deep basin and also on the foot of the slope, where a negative reflector, related to the high interval velocity of salt, marks its base. The halokinetic processes are not homogeneously distributed in the region, forming a great number of diapirs on the foot of the slope (due to the pression of the slided sediments) and giant domes toward the deep basin (due to the higher thickness of the Plio-quaternary sediments). This distribution seems to be related to the amount of salt and of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017P%26SS..144...89M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017P%26SS..144...89M"><span>Probing the internal structure of the asteriod Didymoon with a passive <span class="hlt">seismic</span> investigation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murdoch, N.; Hempel, S.; Pou, L.; Cadu, A.; Garcia, R. F.; Mimoun, D.; Margerin, L.; Karatekin, O.</p> <p>2017-09-01</p> <p>Understanding the internal structure of an asteroid has important implications for <span class="hlt">interpreting</span> its evolutionary history, for understanding its continuing geological evolution, and also for asteroid deflection and in-situ space resource utilisation. Given the strong evidence that asteroids are <span class="hlt">seismically</span> active, an in-situ passive <span class="hlt">seismic</span> experiment could provide information about the asteroid surface and interior properties. Here, we discuss the natural <span class="hlt">seismic</span> activity that may be present on Didymoon, the secondary component of asteroid (65803) Didymos. Our analysis of the tidal stresses in Didymoon shows that tidal quakes are likely to occur if the secondary has an eccentric orbit. Failure occurs most easily at the asteroid poles and close to the surface for both homogeneous and layered internal structures. Simulations of <span class="hlt">seismic</span> wave propagation in Didymoon show that the <span class="hlt">seismic</span> moment of even small meteoroid impacts can generate clearly observable body and surface waves if the asteroid's internal structure is homogeneous. The presence of a regolith layer over a consolidated core can result in the <span class="hlt">seismic</span> energy becoming trapped in the regolith due to the strong impedance contrast at the regolith-core boundary. The inclusion of macro-porosity (voids) further complexifies the wavefield due to increased scattering. The most prominent <span class="hlt">seismic</span> waves are always found to be those traveling along the surface of the asteroid and those focusing in the antipodal point of the <span class="hlt">seismic</span> source. We find also that the waveforms and ground acceleration spectra allow discrimination between the different internal structure models. Although the science return of a passive <span class="hlt">seismic</span> experiment would be enhanced by having multiple <span class="hlt">seismic</span> stations, one single <span class="hlt">seismic</span> station can already vastly improve our knowledge about the <span class="hlt">seismic</span> environment and sub-surface structure of an asteroid. We describe several <span class="hlt">seismic</span> measurement techniques that could be applied in order to study the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NHESS..13.2717R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NHESS..13.2717R"><span>The role of GIS in urban <span class="hlt">seismic</span> risk studies: application to the city of Almería (southern Spain)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rivas-Medina, A.; Gaspar-Escribano, J. M.; Benito, B.; Bernabé, M. A.</p> <p>2013-11-01</p> <p>This work describes the structure and characteristics of the geographic information system (GIS) developed for the urban <span class="hlt">seismic</span> risk study of the city of Almería (southern Spain), identifying the stages in which the use of this tool proved to be very beneficial for adopting informed decisions throughout the execution of the work. After the completion of the regional emergency plans for <span class="hlt">seismic</span> risk in Spain and its subsequent approval by the National Civil Defence Commission, the municipalities that need to develop specific local <span class="hlt">seismic</span> risk plans have been identified. Hence, the next action is to develop urban <span class="hlt">seismic</span> risk analyses at a proper scale (Urban <span class="hlt">Seismic</span> Risk Evaluation - Risk-UR). For this evaluation, different factors influencing <span class="hlt">seismic</span> risk such as <span class="hlt">seismic</span> hazard, geotechnical soil characteristics, vulnerability of structures of the region, reparation costs of damaged buildings and exposed population are combined. All these variables are gathered and analysed within a GIS and subsequently used for <span class="hlt">seismic</span> risk estimation. The GIS constitutes a highly useful working tool because it facilitates data interoperability, making the great volume of information required and the numerous processes that take part in the calculations easier to handle, speeding up the analysis and the <span class="hlt">interpretation</span> and presentation of the results of the different working phases. The result of this study is based on a great set of variables that provide a comprehensive view of the urban <span class="hlt">seismic</span> risk, such as the damage distribution of buildings and dwellings of different typologies, the mean damage and the number of uninhabitable buildings for the expected <span class="hlt">seismic</span> motion, the number of dead and injured at different times of the day, the cost of reconstruction and repair of buildings, among others. These results are intended for <span class="hlt">interpretation</span> and decision making in emergency management by unspecialised users (Civil Defence technicians and managers).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S31A0794H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S31A0794H"><span><span class="hlt">Seismic</span> reflection response from cross-correlations of ambient vibrations on non-conventional hidrocarbon reservoir</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huerta, F. V.; Granados, I.; Aguirre, J.; Carrera, R. Á.</p> <p>2017-12-01</p> <p>Nowadays, in hydrocarbon industry, there is a need to optimize and reduce exploration costs in the different types of reservoirs, motivating the community specialized in the search and development of alternative exploration geophysical methods. This study show the reflection response obtained from a shale gas / oil deposit through the method of <span class="hlt">seismic</span> interferometry of ambient vibrations in combination with Wavelet analysis and conventional <span class="hlt">seismic</span> reflection techniques (CMP & NMO). The method is to generate <span class="hlt">seismic</span> responses from virtual sources through the process of cross-correlation of records of Ambient <span class="hlt">Seismic</span> Vibrations (ASV), collected in different receivers. The <span class="hlt">seismic</span> response obtained is <span class="hlt">interpreted</span> as the response that would be measured in one of the receivers considering a virtual source in the other. The acquisition of ASV records was performed in northern of Mexico through semi-rectangular arrays of multi-component geophones with instrumental response of 10 Hz. The in-line distance between geophones was 40 m while in cross-line was 280 m, the sampling used during the data collection was 2 ms and the total duration of the records was 6 hours. The results show the reflection response of two lines in the in-line direction and two in the cross-line direction for which the continuity of coherent events have been identified and <span class="hlt">interpreted</span> as reflectors. There is certainty that the events identified correspond to reflections because the time-frequency analysis performed with the Wavelet Transform has allowed to identify the frequency band in which there are body waves. On the other hand, the CMP and NMO techniques have allowed to emphasize and correct the reflection response obtained during the correlation processes in the frequency band of interest. The results of the processing and analysis of ASV records through the <span class="hlt">seismic</span> interferometry method have allowed us to see interesting results in light of the cross-correlation process in combination with</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('http://adsabs.harvard.edu/abs/2018E%26PSL.482..193N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.482..193N"><span>Understanding cyclic <span class="hlt">seismicity</span> and ground deformation patterns at volcanoes: Intriguing lessons from Tungurahua volcano, Ecuador</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neuberg, Jürgen W.; Collinson, Amy S. D.; Mothes, Patricia A.; Ruiz, Mario C.; Aguaiza, Santiago</p> <p>2018-01-01</p> <p>Cyclic <span class="hlt">seismicity</span> and ground deformation patterns are observed on many volcanoes worldwide where <span class="hlt">seismic</span> swarms and the tilt of the volcanic flanks provide sensitive tools to assess the state of volcanic activity. Ground deformation at active volcanoes is often <span class="hlt">interpreted</span> as pressure changes in a magmatic reservoir, and tilt is simply translated accordingly into inflation and deflation of such a reservoir. Tilt data recorded by an instrument in the summit area of Tungurahua volcano in Ecuador, however, show an intriguing and unexpected behaviour on several occasions: prior to a Vulcanian explosion when a pressurisation of the system would be expected, the tilt signal declines significantly, hence indicating depressurisation. At the same time, <span class="hlt">seismicity</span> increases drastically. Envisaging that such a pattern could carry the potential to forecast Vulcanian explosions on Tungurahua, we use numerical modelling and reproduce the observed tilt patterns in both space and time. We demonstrate that the tilt signal can be more easily explained as caused by shear stress due to viscous flow resistance, rather than by pressurisation of the magmatic plumbing system. In general, our numerical models prove that if magma shear viscosity and ascent rate are high enough, the resulting shear stress is sufficient to generate a tilt signal as observed on Tungurahua. Furthermore, we address the interdependence of tilt and <span class="hlt">seismicity</span> through shear stress partitioning and suggest that a joint <span class="hlt">interpretation</span> of tilt and <span class="hlt">seismicity</span> can shed new light on the eruption potential of silicic volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1811188C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1811188C"><span>Faults dominant structure? -<span class="hlt">Seismic</span> images of the subsurface structure for the Ilan geothermal field in Taiwan.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Yu-Chun; Shih, Ruey-Chyuan; Wang, Chien-Ying; Kuo, Hsuan-Yu; Chen, Wen-Shan</p> <p>2016-04-01</p> <p>A prototype deep geothermal power plant is to be constructed at the Ilan plain in northeastern Taiwan. The site will be chosen from one of the two potential areas, one in the west and the other in the eastern side of the plain. The triangle-shaped Ilan plane is bounded by two mountain ranges at the northwest and the south, with argillite and slate outcrops exposed, respectively. The Ilan plane is believed situating in a structure extending area at the southwestern end of the Okinawa Trough. Many studies about subsurface structure of the plain have been conducted for years. The results showed that the thickest sediments, around 900 m, is located at the eastern coast of the plain, at north of the largest river in the plain, the Lanyang river, and then became shallower to the edges of the plain. Since the plane is covered by thick sediments, formations and structures beneath the sediments are barely known. However, the observed high geothermal gradient and the abundant hot spring in the Ilan area indicate that this area is having a high potential of geothermal energy. In order to build up a conceptual model for tracing the possible paths of geothermal water and search for a suitable site for the geothermal well, we used the <span class="hlt">seismic</span> reflection method to delineate the subsurface structure. The <span class="hlt">seismic</span> profiles showed a clear unconformity separating the sediments and the metamorphic bedrock, and some events dipping to the east in the bedrock. <span class="hlt">Seismic</span> images above the unconformity are clear; however, <span class="hlt">seismic</span> signals in the metamorphic bedrock are sort of ambiguous. There were two models <span class="hlt">interpreted</span> by using around 10 <span class="hlt">seismic</span> images that collected by us in the past 3 years by using two mini-vibrators (EnviroVibe) and a 360-channel <span class="hlt">seismic</span> data acquisition system. In the first model, <span class="hlt">seismic</span> signals in the bedrock were <span class="hlt">interpreted</span> as layer boundaries, and a fractured metamorphic layer down the depth of 1200m was thought as the source of geothermal water reservoir. In the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/58925','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/58925"><span><span class="hlt">Interpretations</span> from multichannel <span class="hlt">seismic</span>-reflection profiles of the deep crust crossing South Carolina and Georgia from the Appalachian Mountains to the Atlantic Coast</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Behrendt, John C.</p> <p>1985-01-01</p> <p>The Appalachian décollement does not appear continuous from the Appalachian Mountains to the coast but rather appears to extend southeastward only to the Carolina slate belt. A series of reflections on lines S4, S6, and S8 and on the COCORP line is <span class="hlt">interpreted</span> as evidence of southeastward-dipping imbricate faults, from the Brevard fault on the northwest to beyond the Augusta fault, which marks the southeastern extent of the Eastern Piedmont fault zone. The Carolina slate belt is characterized on the four <span class="hlt">seismic</span> profiles by a complex series of diffractions and reflections extending from less than 1 s to 8 s. These arrivals are possibly the result of layering in the metasedimentary rocks complexly disrupted by the imbricate faults. A number of Triassic (?) basins are apparent in the reflection data for the rifted Charleston terrane identified from low-gradient magnetic anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2008/1261/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2008/1261/"><span>Hawaiian Volcano Observatory <span class="hlt">Seismic</span> Data, January to December 2007</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakata, Jennifer S.; Okubo, Paul G.</p> <p>2008-01-01</p> <p>The U.S. Geological Survey (USGS), Hawaiian Volcano Observatory (HVO) summary presents <span class="hlt">seismic</span> data gathered during the year. The <span class="hlt">seismic</span> summary is offered without <span class="hlt">interpretation</span> as a source of preliminary data and is complete in that most data for events of M=1.5 are included. All latitude and longitude references in this report are stated in Old Hawaiian Datum. The HVO summaries have been published in various forms since 1956. Summaries prior to 1974 were issued quarterly, but cost, convenience of preparation and distribution, and the large quantities of data necessitated an annual publication, beginning with Summary 74 for the year 1974. Beginning in 2004, summaries are simply identified by the year, rather than by summary number. Summaries originally issued as administrative reports were republished in 2007 as Open-File Reports. All the summaries since 1956 are listed at http://geopubs.wr.usgs.gov/ (last accessed September 30, 2008). In January 1986, HVO adopted CUSP (California Institute of Technology USGS <span class="hlt">Seismic</span> Processing). Summary 86 includes a description of the <span class="hlt">seismic</span> instrumentation, calibration, and processing used in recent years. The present summary includes background information about the <span class="hlt">seismic</span> network to provide the end user an understanding of the processing parameters and how the data were gathered. A report by Klein and Koyanagi (1980) tabulates instrumentation, calibration, and recording history of each <span class="hlt">seismic</span> station in the network. It is designed as a reference for users of seismograms and phase data and includes and augments the information in the station table in this summary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920001515','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920001515"><span>Martian <span class="hlt">seismicity</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Phillips, Roger J.; Grimm, Robert E.</p> <p>1991-01-01</p> <p>The design and ultimate success of network seismology experiments on Mars depends on the present level of Martian <span class="hlt">seismicity</span>. Volcanic and tectonic landforms observed from imaging experiments show that Mars must have been a <span class="hlt">seismically</span> active planet in the past and there is no reason to discount the notion that Mars is <span class="hlt">seismically</span> active today but at a lower level of activity. Models are explored for present day Mars <span class="hlt">seismicity</span>. Depending on the sensitivity and geometry of a <span class="hlt">seismic</span> network and the attenuation and scattering properties of the interior, it appears that a reasonable number of Martian <span class="hlt">seismic</span> events would be detected over the period of a decade. The thermoelastic cooling mechanism as estimated is surely a lower bound, and a more refined estimate would take into account specifically the regional cooling of Tharsis and lead to a higher frequency of <span class="hlt">seismic</span> events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRB..120.7749D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRB..120.7749D"><span><span class="hlt">Seismic</span> hydraulic fracture migration originated by successive deep magma pulses: The 2011-2013 <span class="hlt">seismic</span> series associated to the volcanic activity of El Hierro Island</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Díaz-Moreno, A.; Ibáñez, J. M.; De Angelis, S.; García-Yeguas, A.; Prudencio, J.; Morales, J.; Tuvè, T.; García, L.</p> <p>2015-11-01</p> <p>In this manuscript we present a new <span class="hlt">interpretation</span> of the <span class="hlt">seismic</span> series that accompanied eruptive activity off the coast of El Hierro, Canary Islands, during 2011-2013. We estimated temporal variations of the Gutenberg-Richter b value throughout the period of analysis, and performed high-precision relocations of the preeruptive and syneruptive <span class="hlt">seismicity</span> using a realistic 3-D velocity model. Our results suggest that eruptive activity and the accompanying <span class="hlt">seismicity</span> were caused by repeated injections of magma from the mantle into the lower crust. These magma pulses occurred within a small and well-defined volume resulting in the emplacement of fresh magma along the crust-mantle boundary underneath El Hierro. We analyzed the distribution of earthquake hypocenters in time and space in order to assess <span class="hlt">seismic</span> diffusivity in the lower crust. Our results suggest that very high earthquake rates underneath El Hierro represent the response of a stable lower crust to stress perturbations with pulsatory character, linked to the injection of magma from the mantle. Magma input from depth caused large stress perturbations to propagate into the lower crust generating energetic <span class="hlt">seismic</span> swarms. The absence of any preferential alignment in the spatial pattern of <span class="hlt">seismicity</span> reinforces our hypothesis that stress perturbation and related <span class="hlt">seismicity</span>, had diffusive character. We conclude that the temporal and spatial evolution of <span class="hlt">seismicity</span> was neither tracking the path of magma migration nor it defines the boundaries of magma storage volumes such as a midcrustal sill. Our conceptual model considers pulsatory magma injection from the upper mantle and its propagation along the Moho. We suggest, within this framework, that the spatial and temporal distributions of earthquake hypocenters reflect hydraulic fracturing processes associated with stress propagation due to magma movement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010LNCS.6355...27B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010LNCS.6355...27B"><span>Constraint-Based <span class="hlt">Abstract</span> Semantics for Temporal Logic: A Direct Approach to Design and Implementation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Banda, Gourinath; Gallagher, John P.</p> <p></p> <p><span class="hlt">interpretation</span> provides a practical approach to verifying properties of infinite-state systems. We apply the framework of <span class="hlt">abstract</span> <span class="hlt">interpretation</span> to derive an <span class="hlt">abstract</span> semantic function for the modal μ-calculus, which is the basis for <span class="hlt">abstract</span> model checking. The <span class="hlt">abstract</span> semantic function is constructed directly from the standard concrete semantics together with a Galois connection between the concrete state-space and an <span class="hlt">abstract</span> domain. There is no need for mixed or modal transition systems to <span class="hlt">abstract</span> arbitrary temporal properties, as in previous work in the area of <span class="hlt">abstract</span> model checking. Using the modal μ-calculus to implement CTL, the <span class="hlt">abstract</span> semantics gives an over-approximation of the set of states in which an arbitrary CTL formula holds. Then we show that this leads directly to an effective implementation of an <span class="hlt">abstract</span> model checking algorithm for CTL using <span class="hlt">abstract</span> domains based on linear constraints. The implementation of the <span class="hlt">abstract</span> semantic function makes use of an SMT solver. We describe an implemented system for proving properties of linear hybrid automata and give some experimental results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA260030','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA260030"><span>Test and Evaluation of Neural Network Applications for <span class="hlt">Seismic</span> Signal Discrimination</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1992-09-28</p> <p>IMS) for automated processing and <span class="hlt">interpretation</span> of regional <span class="hlt">seismic</span> data. Also reported is the result of a preliminary study on the application of...of analyst-verified events that were missed by the automated processing decreased by more than a factor of 2 (about 10 events/week). The second</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.8435S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.8435S"><span>Submarine landslide and tsunami hazards offshore southern Alaska: <span class="hlt">Seismic</span> strengthening versus rapid sedimentation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sawyer, Derek E.; Reece, Robert S.; Gulick, Sean P. S.; Lenz, Brandi L.</p> <p>2017-08-01</p> <p>The southern Alaskan offshore margin is prone to submarine landslides and tsunami hazards due to <span class="hlt">seismically</span> active plate boundaries and extreme sedimentation rates from glacially enhanced mountain erosion. We examine the submarine landslide potential with new shear strength measurements acquired by Integrated Ocean Drilling Program Expedition 341 on the continental slope and Surveyor Fan. These data reveal lower than expected sediment strength. Contrary to other active margins where <span class="hlt">seismic</span> strengthening enhances slope stability, the high-sedimentation margin offshore southern Alaska behaves like a passive margin from a shear strength perspective. We <span class="hlt">interpret</span> that <span class="hlt">seismic</span> strengthening occurs but is offset by high sedimentation rates and overpressure. This conclusion is supported by shear strength outside of the fan that follow an active margin trend. More broadly, <span class="hlt">seismically</span> active margins with wet-based glaciers are susceptible to submarine landslide hazards because of the combination of high sedimentation rates and earthquake shaking.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820004825','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820004825"><span>Synthesis of regional crust and upper-mantle structure from <span class="hlt">seismic</span> and gravity data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Alexander, S. S.; Lavin, P. M.</p> <p>1979-01-01</p> <p>Available <span class="hlt">seismic</span> and ground based gravity data are combined to infer the three dimensional crust and upper mantle structure in selected regions. This synthesis and <span class="hlt">interpretation</span> proceeds from large-scale average models suitable for early comparison with high-altitude satellite potential field data to more detailed delineation of structural boundaries and other variations that may be significant in natural resource assessment. <span class="hlt">Seismic</span> and ground based gravity data are the primary focal point, but other relevant information (e.g. magnetic field, heat flow, Landsat imagery, geodetic leveling, and natural resources maps) is used to constrain the structure inferred and to assist in defining structural domains and boundaries. The <span class="hlt">seismic</span> data consists of regional refraction lines, limited reflection coverage, surface wave dispersion, teleseismic P and S wave delay times, anelastic absorption, and regional <span class="hlt">seismicity</span> patterns. The gravity data base consists of available point gravity determinations for the areas considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.1536S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.1536S"><span><span class="hlt">Seismic</span> Ecology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seleznev, V. S.; Soloviev, V. M.; Emanov, A. F.</p> <p></p> <p>The paper is devoted to researches of influence of <span class="hlt">seismic</span> actions for industrial and civil buildings and people. The <span class="hlt">seismic</span> actions bring influence directly on the people (vibration actions, force shocks at earthquakes) or indirectly through various build- ings and the constructions and can be strong (be felt by people) and weak (be fixed by sensing devices). The great number of work is devoted to influence of violent <span class="hlt">seismic</span> actions (first of all of earthquakes) on people and various constructions. This work is devoted to study weak, but long <span class="hlt">seismic</span> actions on various buildings and people. There is a need to take into account <span class="hlt">seismic</span> oscillations, acting on the territory, at construction of various buildings on urbanized territories. Essential influence, except for violent earthquakes, man-caused <span class="hlt">seismic</span> actions: the explosions, <span class="hlt">seismic</span> noise, emitted by plant facilities and moving transport, radiation from high-rise buildings and constructions under action of a wind, etc. can exert. Materials on increase of man- caused <span class="hlt">seismicity</span> in a number of regions in Russia, which earlier were not <span class="hlt">seismic</span>, are presented in the paper. Along with maps of <span class="hlt">seismic</span> microzoning maps to be built indicating a variation of amplitude spectra of <span class="hlt">seismic</span> noise within day, months, years. The presence of an information about amplitudes and frequencies of oscillations from possible earthquakes and man-caused oscillations in concrete regions allows carry- ing out soundly designing and construction of industrial and civil housing projects. The construction of buildings even in not <span class="hlt">seismically</span> dangerous regions, which have one from resonance frequencies coincident on magnitude to frequency of oscillations, emitted in this place by man-caused objects, can end in failure of these buildings and heaviest consequences for the people. The practical examples of detail of engineering- seismological investigation of large industrial and civil housing projects of Siberia territory (hydro power</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035242','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035242"><span>Widespread <span class="hlt">seismicity</span> excitation throughout central Japan following the 2011 M=9.0 Tohoku earthquake and its <span class="hlt">interpretation</span> by Coulomb stress transfer</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, S.; Stein, R.S.; Lin, J.</p> <p>2011-01-01</p> <p>We report on a broad and unprecedented increase in <span class="hlt">seismicity</span> rate following the M=9.0 Tohoku mainshock for M ≥ 2 earthquakes over inland Japan, parts of the Japan Sea and Izu islands, at distances of up to 425 km from the locus of high (≥15 m) <span class="hlt">seismic</span> slip on the megathrust. Such an increase was not seen for the 2004 M=9.1 Sumatra or 2010 M=8.8 Chile earthquakes, but they lacked the <span class="hlt">seismic</span> networks necessary to detect such small events. Here we explore the possibility that the rate changes are the product of static Coulomb stress transfer to small faults. We use the nodal planes of M ≥ 3.5 earthquakes as proxies for such small active faults, and find that of fifteen regions averaging ~80 by 80 km in size, 11 show a positive association between calculated stress changes and the observed <span class="hlt">seismicity</span> rate change, 3 show a negative correlation, and for one the changes are too small to assess. This work demonstrates that <span class="hlt">seismicity</span> can turn on in the nominal stress shadow of a mainshock as long as small geometrically diverse active faults exist there, which is likely quite common.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1610481L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1610481L"><span><span class="hlt">Seismic</span> atlas of the "Messinian Salinity Crisis" markers in the Mediterranean and Black seas - Volume 2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lofi, Johanna</p> <p>2014-05-01</p> <p>The <span class="hlt">Seismic</span> atlas of the "Messinian Salinity Crisis" markers in the Mediterranean and Black seas - Volume 2 is a publication project in the framework of the study of the Messinian Salinity Crisis. It follows the publication of a first volume in 2011 (see Editors' websites: http://ccgm.free.fr & http://sgfr.free.fr) and aims to illustrate the <span class="hlt">seismic</span> characteristics of the MSC markers over news study areas. The Messinian Salinity Crisis is a huge outstanding succession of events that deeply modified the Mediterranean area within a short time span at the geological scale. In 2011, a <span class="hlt">seismic</span> atlas of the Messinian markers in the Mediterranean and Black seas has been published [1]. This collective work summarizes, in one publication with a common format, the most relevant <span class="hlt">seismic</span> features related to this exceptional event in the offshore domain. It also proposes a new global and consistent terminology for the MSC markers in the entire offshore Mediterranean area in order to avoid nomenclatural problems. Throughout 13 study areas, the <span class="hlt">seismic</span> facies, geometry and extend of the Messinian markers (bounding surfaces and depositional units) are described. The Atlas however does not provide a complete description of all what that is known about the MSC and about the geology of each study area. Accordingly, illustrations in the Atlas should be used for a global description of the offshore imprints of the MSC at a broad scale, or for local information or site-specific general <span class="hlt">interpretations</span>. <span class="hlt">Interpreted</span> <span class="hlt">seismic</span> data were carefully selected according to their quality, position and significance. Raw and <span class="hlt">interpreted</span> <span class="hlt">seismic</span> profiles are available on CD-Rom. Volume 2 is currently under preparation with the objectives : (1) to image the Messinian <span class="hlt">seismic</span> marker from margins and basins that have not been illustrated in the first volume and (2) to complete the extension map of the MSC markers in the offshore and onshore domains at the Mediterranean scale. As the first volume, Volume</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5455452-evaluation-seismic-reflection-data-davis-lavender-canyons-study-area-paradox-basin-utah-faults-folds-joints-collapse-structures','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5455452-evaluation-seismic-reflection-data-davis-lavender-canyons-study-area-paradox-basin-utah-faults-folds-joints-collapse-structures"><span>Evaluation of <span class="hlt">seismic</span> reflection data in the Davis and Lavender Canyons study area, Paradox Basin, Utah. [Faults, folds, joints, and collapse structures</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>Kitcho, C.A.; Wong, I.G.; Turcotte, F.T.</p> <p>1986-08-01</p> <p><span class="hlt">Seismic</span> reflection data purchased from petroleum industry brokers and acquired through group speculative surveys were <span class="hlt">interpreted</span> for information on the regional subsurface geologic structure and stratigraphy within and surrounding the Davis and Lavender Canyons study area in the Paradox Basin of southeastern Utah. Structures of interest were faults, folds, joints, and collapse structures related to salt dissolution. The <span class="hlt">seismic</span> reflection data were used to <span class="hlt">interpret</span> stratigraphy by identifying continuous and discontinuous reflectors on the <span class="hlt">seismic</span> profiles. Thickening and thinning of strata and possible areas of salt flowage or dissolution could be identified from the <span class="hlt">seismic</span> data. Identifiable reflectors included themore » tops of the Precambrian and Mississippian, a distinctive interbed close to the middle of the Pennsylvanian Paradox salt formation (probably the interval between Salt Cycles 10 and 13), and near the top of the Paradox salt. Of the 56 faults identified from the <span class="hlt">seismic</span> reflection <span class="hlt">interpretation</span>, 33 trend northwest, west-northwest, or west, and most affect only the deeper part of the stratigraphic section. These faults are part of the deep structural system found throughout the Paradox Basin, including the fold and fault belt in the northeast part of the basin. The faults bound basement Precambrian blocks that experienced minor activity during Mississippian and early Pennsylvanian deposition, and showed major displacement during early Paradox salt deposition as the Paradox Basin subsided. Based on the <span class="hlt">seismic</span> data, most of these faults appear to have an upward terminus between the top of the Mississippian and the salt interbed reflector.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S31E..08E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S31E..08E"><span>Rapid Non-Gaussian Uncertainty Quantification of <span class="hlt">Seismic</span> Velocity Models and Images</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ely, G.; Malcolm, A. E.; Poliannikov, O. V.</p> <p>2017-12-01</p> <p>Conventional <span class="hlt">seismic</span> imaging typically provides a single estimate of the subsurface without any error bounds. Noise in the observed raw traces as well as the uncertainty of the velocity model directly impact the uncertainty of the final <span class="hlt">seismic</span> image and its resulting <span class="hlt">interpretation</span>. We present a Bayesian inference framework to quantify uncertainty in both the velocity model and <span class="hlt">seismic</span> images, given noise statistics of the observed data.To estimate velocity model uncertainty, we combine the field expansion method, a fast frequency domain wave equation solver, with the adaptive Metropolis-Hastings algorithm. The speed of the field expansion method and its reduced parameterization allows us to perform the tens or hundreds of thousands of forward solves needed for non-parametric posterior estimations. We then migrate the observed data with the distribution of velocity models to generate uncertainty estimates of the resulting subsurface image. This procedure allows us to create both qualitative descriptions of <span class="hlt">seismic</span> image uncertainty and put error bounds on quantities of interest such as the dip angle of a subduction slab or thickness of a stratigraphic layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1175994','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1175994"><span>Frequency-dependent processing and <span class="hlt">interpretation</span> (FDPI) of <span class="hlt">seismic</span> data for identifying, imaging and monitoring fluid-saturated underground reservoirs</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Goloshubin, Gennady M.; Korneev, Valeri A.</p> <p>2006-11-14</p> <p>A method for identifying, imaging and monitoring dry or fluid-saturated underground reservoirs using <span class="hlt">seismic</span> waves reflected from target porous or fractured layers is set forth. <span class="hlt">Seismic</span> imaging the porous or fractured layer occurs by low pass filtering of the windowed reflections from the target porous or fractured layers leaving frequencies below low-most corner (or full width at half maximum) of a recorded frequency spectra. Additionally, the ratio of image amplitudes is shown to be approximately proportional to reservoir permeability, viscosity of fluid, and the fluid saturation of the porous or fractured layers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1007804','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1007804"><span>Frequency-dependent processing and <span class="hlt">interpretation</span> (FDPI) of <span class="hlt">seismic</span> data for identifying, imaging and monitoring fluid-saturated underground reservoirs</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Goloshubin, Gennady M.; Korneev, Valeri A.</p> <p>2005-09-06</p> <p>A method for identifying, imaging and monitoring dry or fluid-saturated underground reservoirs using <span class="hlt">seismic</span> waves reflected from target porous or fractured layers is set forth. <span class="hlt">Seismic</span> imaging the porous or fractured layer occurs by low pass filtering of the windowed reflections from the target porous or fractured layers leaving frequencies below low-most corner (or full width at half maximum) of a recorded frequency spectra. Additionally, the ratio of image amplitudes is shown to be approximately proportional to reservoir permeability, viscosity of fluid, and the fluid saturation of the porous or fractured layers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.S11B1713S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.S11B1713S"><span>Real Time <span class="hlt">Seismic</span> Prediction while Drilling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schilling, F. R.; Bohlen, T.; Edelmann, T.; Kassel, A.; Heim, A.; Gehring, M.; Lüth, S.; Giese, R.; Jaksch, K.; Rechlin, A.; Kopf, M.; Stahlmann, J.; Gattermann, J.; Bruns, B.</p> <p>2009-12-01</p> <p>Efficient and safe drilling is a prerequisite to enhance the mobility of people and goods, to improve the traffic as well as utility infrastructure of growing megacities, and to ensure the growing energy demand while building geothermal and in hydroelectric power plants. Construction within the underground is often building within the unknown. An enhanced risk potential for people and the underground building may arise if drilling enters fracture zones, karsts, brittle rocks, mixed solid and soft rocks, caves, or anthropogenic obstacles. Knowing about the material behavior ahead of the drilling allows reducing the risk during drilling and construction operation. In drilling operations direct observations from boreholes can be complemented with geophysical investigations. In this presentation we focus on “real time” <span class="hlt">seismic</span> prediction while drilling which is seen as a prerequisite while using geophysical methods in modern drilling operations. In solid rocks P- and S-wave velocity, refraction and reflection as well as <span class="hlt">seismic</span> wave attenuation can be used for the <span class="hlt">interpretation</span> of structures ahead of the drilling. An Integrated <span class="hlt">Seismic</span> Imaging System (ISIS) for exploration ahead of a construction is used, where a pneumatic hammer or a magnetostrictive vibration source generate repetitive signals behind the tunneling machine. Tube waves are generated which travel along the tunnel to the working face. There the tube waves are converted to mainly S- but also P-Waves which interact with the formation ahead of the heading face. The reflected or refracted waves travel back to the working front are converted back to tube waves and recorded using three-component geophones which are fit into the tips of anchor rods. In near real time, the ISIS software allows for an integrated 3D imaging and <span class="hlt">interpretation</span> of the observed data, geological and geotechnical parameters. Fracture zones, heterogeneities, and variations in the rock properties can be revealed during the drilling</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22177662','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22177662"><span>Visually defining and querying consistent multi-granular clinical temporal <span class="hlt">abstractions</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Combi, Carlo; Oliboni, Barbara</p> <p>2012-02-01</p> <p>The main goal of this work is to propose a framework for the visual specification and query of consistent multi-granular clinical temporal <span class="hlt">abstractions</span>. We focus on the issue of querying patient clinical information by visually defining and composing temporal <span class="hlt">abstractions</span>, i.e., high level patterns derived from several time-stamped raw data. In particular, we focus on the visual specification of consistent temporal <span class="hlt">abstractions</span> with different granularities and on the visual composition of different temporal <span class="hlt">abstractions</span> for querying clinical databases. Temporal <span class="hlt">abstractions</span> on clinical data provide a concise and high-level description of temporal raw data, and a suitable way to support decision making. Granularities define partitions on the time line and allow one to represent time and, thus, temporal clinical information at different levels of detail, according to the requirements coming from the represented clinical domain. The visual representation of temporal information has been considered since several years in clinical domains. Proposed visualization techniques must be easy and quick to understand, and could benefit from visual metaphors that do not lead to ambiguous <span class="hlt">interpretations</span>. Recently, physical metaphors such as strips, springs, weights, and wires have been proposed and evaluated on clinical users for the specification of temporal clinical <span class="hlt">abstractions</span>. Visual approaches to boolean queries have been considered in the last years and confirmed that the visual support to the specification of complex boolean queries is both an important and difficult research topic. We propose and describe a visual language for the definition of temporal <span class="hlt">abstractions</span> based on a set of intuitive metaphors (striped wall, plastered wall, brick wall), allowing the clinician to use different granularities. A new algorithm, underlying the visual language, allows the physician to specify only consistent <span class="hlt">abstractions</span>, i.e., <span class="hlt">abstractions</span> not containing contradictory conditions on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.1666C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.1666C"><span><span class="hlt">Seismic</span> anisotropy in the lower crust: The link between rock composition, microstructure, texture and <span class="hlt">seismic</span> properties.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Czaplinska, Daria; Piazolo, Sandra; Almqvist, Bjarne</p> <p>2015-04-01</p> <p> techniques, including Voigt, Reuss, Hill, geometric mean and self-consistent and Asymptotic Expansion Homogenization (AEH) methods. To test the advantages and disadvantages of the method, results are compared to measured geophysical properties of equivalent rocks. Such comparison, allows refinement of <span class="hlt">seismic</span> data <span class="hlt">interpretation</span> for mid to lower crustal rocks. References: Cook, A., Vel., S., Johnson, S.E., Gerbi, C., Song, W.J., 2013. Elastic and <span class="hlt">Seismic</span> Properties (ESP) Toolbox (beta version); http://umaine.edu/mecheng/faculty-and-staff/senthil-vel/software/ESP_Toolbox/</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('http://adsabs.harvard.edu/abs/2017SGeo...38..617A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SGeo...38..617A"><span>Geodynamic Evolution of Northeastern Tunisia During the Maastrichtian-Paleocene Time: Insights from Integrated <span class="hlt">Seismic</span> Stratigraphic Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abidi, Oussama; Inoubli, Mohamed Hédi; Sebei, Kawthar; Amiri, Adnen; Boussiga, Haifa; Nasr, Imen Hamdi; Salem, Abdelhamid Ben; Elabed, Mahmoud</p> <p>2017-05-01</p> <p>The Maastrichtian-Paleocene El Haria formation was studied and defined in Tunisia on the basis of outcrops and borehole data; few studies were interested in its three-dimensional extent. In this paper, the El Haria formation is reviewed in the context of a tectono-stratigraphic interval using an integrated <span class="hlt">seismic</span> stratigraphic analysis based on borehole lithology logs, electrical well logging, well shots, vertical <span class="hlt">seismic</span> profiles and post-stack surface data. <span class="hlt">Seismic</span> analysis benefits from appropriate calibration with borehole data, conventional <span class="hlt">interpretation</span>, velocity mapping, <span class="hlt">seismic</span> attributes and post-stack model-based inversion. The applied methodology proved to be powerful for charactering the marly Maastrichtian-Paleocene interval of the El Haria formation. Migrated <span class="hlt">seismic</span> sections together with borehole measurements are used to detail the three-dimensional changes in thickness, facies and depositional environment in the Cap Bon and Gulf of Hammamet regions during the Maastrichtian-Paleocene time. Furthermore, dating based on their microfossil content divulges local and multiple internal hiatuses within the El Haria formation which are related to the geodynamic evolution of the depositional floor since the Campanian stage. <span class="hlt">Interpreted</span> <span class="hlt">seismic</span> sections display concordance, unconformities, pinchouts, sedimentary gaps, incised valleys and syn-sedimentary normal faulting. Based on the <span class="hlt">seismic</span> reflection geometry and terminations, seven sequences are delineated. These sequences are related to base-level changes as the combination of depositional floor paleo-topography, tectonic forces, subsidence and the developed accommodation space. These factors controlled the occurrence of the various parts of the Maastrichtian-Paleocene interval. Detailed examinations of these deposits together with the analysis of the structural deformation at different time periods allowed us to obtain a better understanding of the sediment architecture in depth and the delineation of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017126','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017126"><span><span class="hlt">Seismic</span> images of the Brooks Range fold and thrust belt, Arctic Alaska, from an integrated <span class="hlt">seismic</span> reflection/refraction experiment</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Levander, A.; Fuis, G.S.; Wissinger, E.S.; Lutter, W.J.; Oldow, J.S.; Moore, Thomas E.</p> <p>1994-01-01</p> <p>We describe results of an integrated <span class="hlt">seismic</span> reflection/refraction experiment across the Brooks Range and flanking geologic provinces in Arctic Alaska. The <span class="hlt">seismic</span> acquisition was unusual in that reflection and refraction data were collected simultaneously with a 700 channel seismograph system deployed numerous times along a 315 km profile. Shot records show continuous Moho reflections from 0-180 km offset, as well as numerous upper- and mid-crustal wide-angle events. Single and low-fold near-vertical incidence common midpoint (CMP) reflection images show complex upper- and middle-crustal structure across the range from the unmetamorphosed Endicott Mountains allochthon (EMA) in the north, to the metamorphic belts in the south. Lower-crustal and Moho reflections are visible across the entire reflection profile. Travel-time inversion of PmP arrivals shows that the Moho, at 33 km depth beneath the North Slope foothills, deepens abruptly beneath the EMA to a maximum of 46 km, and then shallows southward to 35 km at the southern edge of the range. Two zones of upper- and middle-crustal reflections underlie the northern Brooks Range above ~ 12-15 km depth. The upper zone, <span class="hlt">interpreted</span> as the base of the EMA, lies at a maximum depth of 6 km and extends over 50 km from the range front to the north central Brooks Range where the base of the EMA outcrops above the metasedimentary rocks exposed in the Doonerak window. We <span class="hlt">interpret</span> the base of the lower zone, at ~ 12 km depth, to be from carbonate rocks above the master detachment upon which the Brooks Range formed. The <span class="hlt">seismic</span> data suggest that the master detachment is connected to the faults in the EMA by several ramps. In the highly metamorphosed terranes south of the Doonerak window, the CMP section shows numerous south-dipping events which we <span class="hlt">interpret</span> as a crustal scale duplex involving the Doonerak window rocks. The basal detachment reflections can be traced approximately 100 km, and dip southward from about 10-12 km</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030465','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030465"><span>Scattered surface wave energy in the <span class="hlt">seismic</span> coda</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zeng, Y.</p> <p>2006-01-01</p> <p>One of the many important contributions that Aki has made to seismology pertains to the origin of coda waves (Aki, 1969; Aki and Chouet, 1975). In this paper, I revisit Aki's original idea of the role of scattered surface waves in the <span class="hlt">seismic</span> coda. Based on the radiative transfer theory, I developed a new set of scattered wave energy equations by including scattered surface waves and body wave to surface wave scattering conversions. The work is an extended study of Zeng et al. (1991), Zeng (1993) and Sato (1994a) on multiple isotropic-scattering, and may shed new insight into the <span class="hlt">seismic</span> coda wave <span class="hlt">interpretation</span>. The scattering equations are solved numerically by first discretizing the model at regular grids and then solving the linear integral equations iteratively. The results show that scattered wave energy can be well approximated by body-wave to body wave scattering at earlier arrival times and short distances. At long distances from the source, scattered surface waves dominate scattered body waves at surface stations. Since surface waves are 2-D propagating waves, their scattered energies should in theory follow a common decay curve. The observed common decay trends on <span class="hlt">seismic</span> coda of local earthquake recordings particular at long lapse times suggest that perhaps later <span class="hlt">seismic</span> codas are dominated by scattered surface waves. When efficient body wave to surface wave conversion mechanisms are present in the shallow crustal layers, such as soft sediment layers, the scattered surface waves dominate the <span class="hlt">seismic</span> coda at even early arrival times for shallow sources and at later arrival times for deeper events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMIN51A1145M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMIN51A1145M"><span>The GEON Integrated Data Viewer (IDV) and IRIS DMC Services Illustrate CyberInfrastructure Support for <span class="hlt">Seismic</span> Data Visualization and <span class="hlt">Interpretation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meertens, C.; Wier, S.; Ahern, T.; Casey, R.; Weertman, B.; Laughbon, C.</p> <p>2008-12-01</p> <p>UNAVCO and the IRIS DMC are data service partners for <span class="hlt">seismic</span> visualization, particularly for hypocentral data and tomography. UNAVCO provides the GEON Integrated Data Viewer (IDV), an extension of the Unidata IDV, a free, interactive, research-level, software display and analysis tool for data in 3D (latitude, longitude, depth) and 4D (with time), located on or inside the Earth. The GEON IDV is designed to meet the challenge of investigating complex, multi-variate, time-varying, three- dimensional geoscience data in the context of new remote and shared data sources. The GEON IDV supports data access from data sources using HTTP and FTP servers, OPeNDAP servers, THREDDS catalogs, RSS feeds, and WMS (web map) servers. The IRIS DMC (Data Management System) has developed web services providing data for earthquake hypocentral data and <span class="hlt">seismic</span> tomography model grids. These services can be called by the GEON IDV to access data at IRIS without copying files. The IRIS Earthquake Browser (IEB) is a web-based query tool for hypocentral data. The IEB combines the DMC's large database of more than 1,900,000 earthquakes with the Google Maps web interface. With the IEB you can quickly find earthquakes in any region of the globe and then import this information into the GEON Integrated Data Viewer where the hypocenters may be visualized. You can select earthquakes by location region, time, depth, and magnitude. The IEB gives the IDV a URL to the selected data. The IDV then shows the data as maps or 3D displays, with interactive control of vertical scale, area, map projection, with symbol size and color control by magnitude or depth. The IDV can show progressive time animation of, for example, aftershocks filling a source region. The IRIS Tomoserver converts <span class="hlt">seismic</span> tomography model output grids to NetCDF for use in the IDV. The Tomoserver accepts a tomographic model file as input from a user and provides an equivalent NetCDF file as output. The service supports NA04, S3D, A1D and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018219','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018219"><span>Scaling of the critical slip distance for <span class="hlt">seismic</span> faulting with shear strain in fault zones</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Marone, Chris; Kilgore, Brian D.</p> <p>1993-01-01</p> <p>THEORETICAL and experimentally based laws for <span class="hlt">seismic</span> faulting contain a critical slip distance1-5, Dc, which is the slip over which strength breaks down during earthquake nucleation. On an earthquake-generating fault, this distance plays a key role in determining the rupture nucleation dimension6, the amount of premonitory and post-<span class="hlt">seismic</span> slip7-10, and the maximum <span class="hlt">seismic</span> ground acceleration1,11. In laboratory friction experiments, Dc has been related to the size of surface contact junctions2,5,12; thus, the discrepancy between laboratory measurements of Dc (??? 10-5 m) and values obtained from modelling earthquakes (??? 10-2 m) has been attributed to differences in roughness between laboratory surfaces and natural faults5. This <span class="hlt">interpretation</span> predicts a dependence of Dc on the particle size of fault gouge 2 (breccia and wear material) but not on shear strain. Here we present experimental results showing that Dc scales with shear strain in simulated fault gouge. Our data suggest a new physical <span class="hlt">interpretation</span> for the critical slip distance, in which Dc is controlled by the thickness of the zone of localized shear strain. As gouge zones of mature faults are commonly 102-103 m thick13-17, whereas laboratory gouge layers are 1-10 mm thick, our data offer an alternative <span class="hlt">interpretation</span> of the discrepancy between laboratory and field-based estimates of Dc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70134541','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70134541"><span><span class="hlt">Seismic</span> images of a tectonic subdivision of the Greenville Orogen beneath lakes Ontario and Erie</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Forsyth, D. A.; Milkereit, B.; Davidson, A.; Hanmer, S.; Hutchinson, Deborah R.; Hinze, W. J.; Mereu, R.F.</p> <p>1994-01-01</p> <p>New <span class="hlt">seismic</span> data from marine air-gun and Vibroseis profiles in Lake Ontario and Lake Erie provide images of subhorizontal Phanerozoic sediments underlain by a remarkable series of easterly dipping reflections that extends from the crystalline basement to the lower crust. These reflections are <span class="hlt">interpreted</span> as structural features of crustal-scale subdivisions within the Grenville Orogen. Broadly deformed, imbricated, and overlapping thrust sheets within the western Central Metasedimentary Belt are succeeded to the west by a complex zone of easterly dipping, apparent thrust faults that are <span class="hlt">interpreted</span> as a southwest subsurface extension of the boundary zone between the Central Metasedimentary Belt and the Central Gneiss Belt. The <span class="hlt">interpreted</span> Central Metasedimentary Belt boundary zone has a characteristic magnetic anomaly that provides a link from the adjacent ends of lakes Ontario and Erie to structures exposed 150 km to the north. Less reflective, west-dipping events are <span class="hlt">interpreted</span> as structures within the eastern Central Gneiss Belt. The <span class="hlt">seismic</span> <span class="hlt">interpretation</span> augments current tectonic models that suggest the exposed ductile structures formed at depth as a result of crustal shortening along northwest-verging thrust faults. Relatively shallow reflections across the boundary region suggest local, Late Proterozoic extensional troughs containing post-Grenville sediments, preserved possibly as a result of pre-Paleozoic reactivation of basement structures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14...40S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14...40S"><span>2D - 3D high resolution <span class="hlt">seismic</span> survey on the Sea of Marmara - Western High</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saritas, H.; Cifci, G.; Géli, L.; Thomas, Y.; Marsset, B.; Rochat, A.; Westbrook, G. K.; Ker, S.; Atgin, O.; Akhun ćoşkun, S. D.; Grall, C.; Henr, P.; Gürçay, S.; Okay, S.; ćoşkun, S.; Özkan, Ö.; Barın, B.</p> <p>2012-04-01</p> <p>In the Sea of Marmara the main strand of the NAF is made up of the Ganos (15km long), Central Marmara (150 km), and North Boundary (45 km) fault segment (Okay et al., 2000). The Central Marmara Fault crosses over The Western High which is located between Tekirdag and Central Marmara Basins. The Western High and Cinarcik Basin is one of the major regions of geological interest which is the area close to the NAF where evidence of gas hydrates and gas escapes have been observed during previous scientific cruises. To understand movement of the NAF and origin of the gas , collecting data was focused on these areas by the latter cruises. It started with TAMAM (Turkish-American Marmara Multichannel) cruise in July 2008 by R/V Koca Piri Reis which belongs to Dokuz Eylul University , and after that it continued with MARMESONET (Marmara Demonstration Mission Program supported by European Seafloor Observatory Network) in December 2009 by R/V Le Suroit which belongs to IFREMER. This cruise consisted of two leg; leg-1 was about collecting multibeam and AUV data, Leg-2 was about collecting High Resolution 3D <span class="hlt">Seismic</span> data. The last cruise PirMarmara was carried out in June 2010 by R/V Koca Piri Reis , its aim was that collecting 2D High Resolution <span class="hlt">Seismic</span> Data .These projects are grouped in ESONET MARMARA-DM Project. 3D <span class="hlt">seismic</span> data provide detailed information about fault distribution and subsurface structures. Computer-based <span class="hlt">interpretation</span> and display of 3D <span class="hlt">seismic</span> data allow for more thorough analysis than 2D <span class="hlt">seismic</span> data. The objectives of this survey are; find gas strata and gas hydrate formation location in the western high, geological description of this area, understand tectonical movement related to dextral strike slip North Anatolian fault, focus on the mud volcano in which close to NAF, find gas hydrate and origin of the existing gas , and location of the gas escaping, investigate the creation of the Marmara Sea concerning with Western High. Integrate good velocity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2010/1111/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2010/1111/"><span>High-resolution <span class="hlt">seismic</span>-reflection data offshore of Dana Point, southern California borderland</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sliter, Ray W.; Ryan, Holly F.; Triezenberg, Peter J.</p> <p>2010-01-01</p> <p>The U.S. Geological Survey collected high-resolution shallow <span class="hlt">seismic</span>-reflection profiles in September 2006 in the offshore area between Dana Point and San Mateo Point in southern Orange and northern San Diego Counties, California. Reflection profiles were located to image folds and reverse faults associated with the San Mateo fault zone and high-angle strike-slip faults near the shelf break (the Newport-Inglewood fault zone) and at the base of the slope. <span class="hlt">Interpretations</span> of these data were used to update the USGS Quaternary fault database and in shaking hazard models for the State of California developed by the Working Group for California Earthquake Probabilities. This cruise was funded by the U.S. Geological Survey Coastal and Marine Catastrophic Hazards project. <span class="hlt">Seismic</span>-reflection data were acquired aboard the R/V Sea Explorer, which is operated by the Ocean Institute at Dana Point. A SIG ELC820 minisparker <span class="hlt">seismic</span> source and a SIG single-channel streamer were used. More than 420 km of <span class="hlt">seismic</span>-reflection data were collected. This report includes maps of the <span class="hlt">seismic</span>-survey sections, linked to Google Earth? software, and digital data files showing images of each transect in SEG-Y, JPEG, and TIFF formats.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Tectp.609....9P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Tectp.609....9P"><span>100 years of <span class="hlt">seismic</span> research on the Moho</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prodehl, Claus; Kennett, Brian; Artemieva, Irina M.; Thybo, Hans</p> <p>2013-12-01</p> <p>The detection of a <span class="hlt">seismic</span> boundary, the “Moho”, between the outermost shell of the Earth, the Earth's crust, and the Earth's mantle by A. Mohorovičić was the consequence of increased insight into the propagation of <span class="hlt">seismic</span> waves caused by earthquakes. This short history of <span class="hlt">seismic</span> research on the Moho is primarily based on the comprehensive overview of the worldwide history of seismological studies of the Earth's crust using controlled sources from 1850 to 2005, by Prodehl and Mooney (2012). Though the art of applying explosions, so-called “artificial events”, as energy sources for studies of the uppermost crustal layers began in the early 1900s, its effective use for studying the entire crust only began at the end of World War II. From 1945 onwards, controlled-source seismology has been the major approach to study details of the crust and underlying crust-mantle boundary, the Moho. The subsequent description of history of controlled-source crustal seismology and its seminal results is subdivided into separate chapters for each decade, highlighting the major advances achieved during that decade in terms of data acquisition, processing technology, and <span class="hlt">interpretation</span> methods. Since the late 1980s, passive seismology using distant earthquakes has played an increasingly important role in studies of crustal structure. The receiver function technique exploiting conversions between P and SV waves at discontinuities in <span class="hlt">seismic</span> wavespeed below a <span class="hlt">seismic</span> station has been extensively applied to the increasing numbers of permanent and portable broad-band <span class="hlt">seismic</span> stations across the globe. Receiver function studies supplement controlled source work with improved geographic coverage and now make a significant contribution to knowledge of the nature of the crust and the depth to Moho.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.T43D2359U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.T43D2359U"><span>The relationship between <span class="hlt">seismic</span> velocity structure and the <span class="hlt">seismic</span> coupling in the Hyuga-nada region, southwest Japan, deduced from onshore and offshore <span class="hlt">seismic</span> observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Uehira, K.; Yakiwara, H.; Yamada, T.; Umakoshi, K.; Nakao, S.; Kobayashi, R.; Goto, K.; Miyamachi, H.; Mochizuki, K.; Nakahigashi, K.; Shinohara, M.; Kanazawa, T.; Hino, R.; Goda, M.; Shimizu, H.</p> <p>2011-12-01</p> <p>In Hyuga-nada region, the Philippine Sea (PHS) plate is subducting beneath the Eurasian (EU) plate (the southwest Japan arc) along the Nankai trough at a rate of about 5 cm per year. Big earthquakes (M7 class) have occurred in the north region from latitude 31.6 degrees north, but it has not occurred in the south region from latitude 31.6 degrees north. The largest earthquake ever recorded in Hyuga-nada region is the 1968 Hyuga-nada earthquake (Mw 7.5). And microseismicity varies spatially. There are non-<span class="hlt">seismic</span> slip events in Hyuga-nada region. For example, the after-slips associated with events for 19 October 1996 and 3 December 1996 were observed (Yagi et al., 2001), and in the same region, the slow-slip events were also observed by GPS measurements (GSI, 2011). We performed extraordinary <span class="hlt">seismic</span> observations for 75 days from April to July 2006, for 73 days from April to July 2008, and for 77 days from April to July 2009. About 25 pop-up type ocean-bottom seismometers were deployed above hypocentral region in Hyuga-nada using Nagasaki-maru. And three data loggers were deployed on land in order to compensate a regular <span class="hlt">seismic</span> network. We used these data and permanent stations for this analysis. In order to obtain precise hypocenter distribution, focal mechanisms, and a 3D <span class="hlt">seismic</span> velocity structure around the Hyuga-nada region, we used Double-Difference (DD) Tomography method developed by Zhang and Thurber (2003). In northern part of Hyuga-nada, Vp/Vs ratio is high along the upper part of PHS slab, and this layer is <span class="hlt">interpreted</span> as the subducting oceanic crust. On the other hand, Vp/Vs ratio is about 1.73 in southern part of Hyuga-nada, and this is <span class="hlt">interpreted</span> as the subducted Kyushu-Palau Ridge, old island arc, which is made by granitic rock. More over, there is a difference of Poisson's ratio at mantle wedge. This value is high (> 0.3) in northern part of Hyuga-nada. The high Poisson's mantle wedge is suggesting that the zone probably corresponds to a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U13B..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U13B..06G"><span>Quantifying uncertainties of <span class="hlt">seismic</span> Bayesian inversion of Northern Great Plains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gao, C.; Lekic, V.</p> <p>2017-12-01</p> <p>Elastic waves excited by earthquakes are the fundamental observations of the seismological studies. Seismologists measure information such as travel time, amplitude, and polarization to infer the properties of earthquake source, <span class="hlt">seismic</span> wave propagation, and subsurface structure. Across numerous applications, <span class="hlt">seismic</span> imaging has been able to take advantage of complimentary <span class="hlt">seismic</span> observables to constrain profiles and lateral variations of Earth's elastic properties. Moreover, <span class="hlt">seismic</span> imaging plays a unique role in multidisciplinary studies of geoscience by providing direct constraints on the unreachable interior of the Earth. Accurate quantification of uncertainties of inferences made from <span class="hlt">seismic</span> observations is of paramount importance for <span class="hlt">interpreting</span> <span class="hlt">seismic</span> images and testing geological hypotheses. However, such quantification remains challenging and subjective due to the non-linearity and non-uniqueness of geophysical inverse problem. In this project, we apply a reverse jump Markov chain Monte Carlo (rjMcMC) algorithm for a transdimensional Bayesian inversion of continental lithosphere structure. Such inversion allows us to quantify the uncertainties of inversion results by inverting for an ensemble solution. It also yields an adaptive parameterization that enables simultaneous inversion of different elastic properties without imposing strong prior information on the relationship between them. We present retrieved profiles of shear velocity (Vs) and radial anisotropy in Northern Great Plains using measurements from USArray stations. We use both <span class="hlt">seismic</span> surface wave dispersion and receiver function data due to their complementary constraints of lithosphere structure. Furthermore, we analyze the uncertainties of both individual and joint inversion of those two data types to quantify the benefit of doing joint inversion. As an application, we infer the variation of Moho depths and crustal layering across the northern Great Plains.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V23A0468D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V23A0468D"><span>InSAR Surface Deformation and Source Modelling at Semisopochnoi Island During the 2014 and 2015 <span class="hlt">Seismic</span> Swarms with Constraints from Geochemical and <span class="hlt">Seismic</span> Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DeGrandpre, K.; Pesicek, J. D.; Lu, Z.</p> <p>2017-12-01</p> <p>During the summer of 2014 and the early spring of 2015 two notable increases in <span class="hlt">seismic</span> activity at Semisopochnoi Island in the western Aleutian islands were recorded on AVO seismometers on Semisopochnoi and neighboring islands. These <span class="hlt">seismic</span> swarms did not lead to an eruption. This study employs interferometric synthetic aperture radar (InSAR) techniques using TerraSAR-X images in conjunction with more accurately relocating the recorded <span class="hlt">seismic</span> events through simultaneous inversion of event travel times and a three-dimensional velocity model using tomoDD. The InSAR images exhibit surprising coherence and an island wide spatial distribution of inflation that is then used in Mogi, Okada, spheroid, and ellipsoid source models in order to define the three-dimensional location and volume change required for a source at the volcano to produce the observed surface deformation. The tomoDD relocations provide a more accurate and realistic three-dimensional velocity model as well as a tighter clustering of events for both swarms that clearly outline a linear <span class="hlt">seismic</span> void within the larger group of shallow (<10 km) <span class="hlt">seismicity</span>. The source models are fit to this void and pressure estimates from geochemical analysis are used to verify the storage depth of magmas at Semisopochnoi. Comparisons of calculated source cavity, magma injection, and surface deformation volumes are made in order to assess the reality behind the various modelling estimates. Incorporating geochemical and <span class="hlt">seismic</span> data to provide constraints on surface deformation source inversions provides an interdisciplinary approach that can be used to make more accurate <span class="hlt">interpretations</span> of dynamic observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUSMNS21A..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUSMNS21A..07M"><span>Tunnel Detection Using <span class="hlt">Seismic</span> Methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, R.; Park, C. B.; Xia, J.; Ivanov, J.; Steeples, D. W.; Ryden, N.; Ballard, R. F.; Llopis, J. L.; Anderson, T. S.; Moran, M. L.; Ketcham, S. A.</p> <p>2006-05-01</p> <p> in Kansas and California. Clandestine tunnels used for illegal entry into the U.S. from Mexico were studied at two different sites along the southern border of California. All these studies represent the empirical basis for suggesting surface <span class="hlt">seismic</span> has a significant role to play in tunnel detection and that methods are under development and very nearly at hand that will provide an effective tool in appraising and maintaining parameter security. As broadband sources, gravity-coupled towed spreads, and automated analysis software continues to make advancements, so does the applicability of routine deployment of <span class="hlt">seismic</span> imaging systems that can be operated by technicians with <span class="hlt">interpretation</span> aids for nearly real-time target selection. Key to making these systems commercial is the development of enhanced imaging techniques in geologically noisy areas and highly variable surface terrain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MarGR.tmp...16M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MarGR.tmp...16M"><span>Equatorial Pacific gravity lineaments: <span class="hlt">interpretations</span> with basement topography along <span class="hlt">seismic</span> reflection lines</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mitchell, Neil C.; Davies, Huw</p> <p>2018-03-01</p> <p>The central equatorial Pacific is interesting for studying clues to upper mantle processes, as the region lacks complicating effects of continental remnants or major volcanic plateaus. In particular, the most recently produced maps of the free-air gravity field from satellite altimetry show in greater detail the previously reported lineaments west of the East Pacific Rise (EPR) that are aligned with plate motion over the mantle and originally suggested to have formed from mantle convection rolls. In contrast, the gravity field 600 km or farther west of the EPR reveals lineaments with varied orientations. Some are also parallel with plate motion over the mantle but others are sub-parallel with fracture zones or have other orientations. This region is covered by pelagic sediments reaching 500-600 m thickness so bathymetry is not so useful for seeking evidence for plate deformation across the lineaments. We instead use depth to basement from three <span class="hlt">seismic</span> reflection cruises. In some segments of these <span class="hlt">seismic</span> data crossing the lineaments, we find that the co-variation between gravity and basement depth is roughly compatible with typical densities of basement rocks (basalt, gabbro or mantle), as expected for some explanations for the lineaments (e.g., mantle convection rolls, viscous asthenospheric inter-fingering or extensional deformation). However, some other lineaments are associated with major changes in basement depth with only subtle changes in the gravity field, suggesting topography that is locally supported by varied crustal thickness. Overall, the multiple gravity lineament orientations suggest that they have multiple origins. In particular, we propose that a further asthenospheric inter-fingering instability mechanism could occur from pressure variations in the asthenosphere arising from regional topography and such a mechanism may explain some obliquely oriented gravity lineaments that have no other obvious origin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S33D2479T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S33D2479T"><span>Evaluating the Gutenberg-Richter Relationship for Induced <span class="hlt">Seismicity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tymchak, M. P.; Flewelling, S. A.</p> <p>2013-12-01</p> <p>Large volumes of flowback and produced water generated from hydraulic fracturing and oil and gas production have led to increased wastewater disposal through underground injection wells. Several recent studies have linked recently felt <span class="hlt">seismic</span> events to underground injection wells in Arkansas, Ohio, Texas and Oklahoma, among others. However, in some cases, such as in Oklahoma, there is a lack of consensus as to whether the earthquakes were the result of fluid injection (Keranan et al., 2013), natural tectonic processes (Oklahoma Geological Survey, 2013), or were related to remote events (van der Elst et al., 2013). Moreover, it is unclear why earthquakes have occurred near some injection wells but not others, with apparently similar geology, target reservoirs, and injection rates (e.g., Frohlich, 2012). In instances where injection occurred near a fault (e.g., Rangely, CO), the timing and distribution of <span class="hlt">seismic</span> events was well correlated to fluid volumes, and the interaction between injection and induced <span class="hlt">seismicity</span> was easily resolved. In other cases (e.g., Oklahoma, Texas), it appears more difficult to <span class="hlt">interpret</span> whether a particular injection well was related to observed <span class="hlt">seismic</span> events. Therefore, metrics are needed as diagnostic tools to help differentiate between natural and induced <span class="hlt">seismicity</span>. It has been well established that the frequency-magnitude distribution of earthquakes follows the Gutenberg-Richter distribution log N(M) = a - bM, where the slope (b-value) is typically near one. However, in some instances of deep fluid injection, b-values may vary, depending on specific injection activities, such as enhanced geothermal or hydraulic fracturing (Dinske and Shapiro, 2013). In some cases, b-values may vary during successive fracture stages of a single horizontal well (e.g., Williams and Calvarez, 2013), and <span class="hlt">seismicity</span> associated with hydraulic fracturing may deviate from the Gutenberg-Richter relationship altogether (Hurd and Zoback, 2012). We evaluate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMDI13C..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMDI13C..07M"><span>Extrinsic Versus Intrinsic <span class="hlt">Seismic</span> Anisotropy and Attenuation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montagner, J. P.; Ricard, Y. R.; Capdeville, Y.; Bodin, T.; Wang, N.</p> <p>2015-12-01</p> <p>The apparent large scale anisotropy is the mixing of intrinsic anisotropic minerals (LPO) and extrinsic anisotropy due to materials with fine layering, fluid inclusions, cracks (SPO) . The same issue arises for attenuation (with many different anelastic processes). The proportion of extrinsic and intrinsic anisotropy and attenuation in the Earth mantle is still an open question. The <span class="hlt">interpretation</span> of observations of <span class="hlt">seismic</span> anisotropy and attenuation is the subject of controversies and often contradictory according to their intrinsic or extrinsic nature. Fine layering is a good candidate for explaining at the same time a large part of observed radial anisotropy (Wang et al., Geophys. Res. Lett., 2013) and attenuation (Ricard et al., Earth Planet. Sci. Lett., 2014). A plausible model of mixing of materials in a chaotic convecting fluid creates a spectrum of heterogeneity varying like 1/k (k wavenumber of the heterogeneity). A body wave propagating in a finely layered medium will be scattered and its distorted waveform can be <span class="hlt">interpreted</span> as due to attenuation with a quality factor Q. We showed that, with the specific 1/k spectrum and only 6-9% RMS heterogeneity, the resulting apparent attenuation Q is frequency independent. Aggregates of randomly orientated anisotropic minerals are good candidates for giving rise to this extrinsic apparent attenuation. The relationship for a 1/k spectrum with apparent <span class="hlt">seismic</span> anisotropy is also explored.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S23A2235V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S23A2235V"><span>Analysis of marine multi-channel <span class="hlt">seismic</span> data using a 2D continuous wavelet transform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vuong, A. K.; Zhang, J.; Gibson, R. L.; Sager, W. W.</p> <p>2011-12-01</p> <p>Marine multi-channel <span class="hlt">seismic</span> (MCS) profiles provide important constraints on crustal structure beneath the sea floor. MCS data usually provide good images of the upper part of the oceanic crust, especially in sedimentary layers. In contrast, it is often difficult to <span class="hlt">interpret</span> deeper layers, especially those within the igneous basement, which is often nearly <span class="hlt">seismically</span> transparent. That difference in <span class="hlt">interpretability</span> occurs because sediments typically have continuous, well-layered and easily-traced structural features, whereas volcanic materials are characterized by smaller features with poorer lateral continuity and often with weak impedance contrasts. Since the basement tends to create weaker reflections, the signal-to-noise ratio decreases, creating additional difficulties that can be exacerbated by the presence of multiples generated by the sea floor and other sources of noise. However, it is still important to characterize the basement accurately to better understand oceanic crust formation and associated basaltic volcanism. We analyzed marine MCS data collected by R/V Marcus G. Langseth across the TAMU Massif of Shatsky Rise in the Northwest Pacific. The <span class="hlt">seismic</span> data from this experiment display the typical problems in imaging basement features. Therefore, we seek to facilitate <span class="hlt">interpretation</span> by applying 2-D continuous wavelet transforms to the data. Conventional Fourier methods transform 2-D <span class="hlt">seismic</span> data from space and time domains to wavenumber and frequency, but the results are global in that there is no knowledge of temporal or spatial variations in frequency or wavenumber content. In contrast, wavelet transforms provide estimates of the local frequency and wavenumber content of the <span class="hlt">seismic</span> image. The transform achieves this result by utilizing a localized, 2D wavelet function instead of the infinite sines and cosines applied in Fourier transforms. We utilize an anisotropic Mexican hat wavelet, where the horizontal and vertical scales are related to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/30560','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/30560"><span>Continuous <span class="hlt">seismic</span>-reflection survey defining shallow sedimentary layers in the Charlotte Harbor and Venice areas, southwest Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wolansky, R.M.; Haeni, F.P.; Sylvester, R.E.</p> <p>1983-01-01</p> <p>A continuous marine <span class="hlt">seismic</span>-reflection survey system was used to define the configuration of shallow sedimentary layers underlying the Charlotte Harbor and Venice areas, southwest Florida. <span class="hlt">Seismic</span> profiling was conducted over a distance of about 57 miles of Charlotte Harbor, the Peace and Myakka Rivers, and the Intracoastal Waterway near Venice using a high resolution energy source capable of penetrating 200 feet of sediments with a resolution of 1 to 3 feet. Five stratigraphic units defined from the <span class="hlt">seismic</span> records includes sediments to Holocene to early Miocene age. All <span class="hlt">seismic</span>-profile records are presented, along with geologic sections constructed from the records. <span class="hlt">Seismic</span> reflection amplitude, frequency, continuity, configuration, external form, and areal association were utilized to <span class="hlt">interpret</span> facies and depositional environments of the stratigraphic units. The despositional framework of the units ranges from shallow shelf to prograded slope. The stratigraphic units are correlated with the surficial aquifer and intermediate artesian aquifers, and permeable zones of the aquifers are related to the <span class="hlt">seismic</span> records. (USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNS31C..07D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNS31C..07D"><span>Imaging near surface mineral targets with ambient <span class="hlt">seismic</span> noise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dales, P.; Audet, P.; Olivier, G.</p> <p>2017-12-01</p> <p>To keep up with global metal and mineral demand, new ore-deposits have to be discovered on a regular basis. This task is becoming increasingly difficult, since easily accessible deposits have been exhausted to a large degree. The typical procedure for mineral exploration begins with geophysical surveys followed by a drilling program to investigate potential targets. Since the retrieved drill core samples are one-dimensional observations, the many holes needed to interpolate and <span class="hlt">interpret</span> potential deposits can lead to very high costs. To reduce the amount of drilling, active <span class="hlt">seismic</span> imaging is sometimes used as an intermediary, however the active sources (e.g. large vibrating trucks or explosive shots) are expensive and unsuitable for operation in remote or environmentally sensitive areas. In recent years, passive <span class="hlt">seismic</span> imaging using ambient noise has emerged as a novel, low-cost and environmentally sensitive approach for exploring the sub-surface. This technique dispels with active <span class="hlt">seismic</span> sources and instead uses ambient <span class="hlt">seismic</span> noise such as ocean waves, traffic or minor earthquakes. Unfortunately at this point, passive surveys are not capable of reaching the required resolution to image the vast majority of the ore-bodies that are being explored. In this presentation, we will show the results of an experiment where ambient <span class="hlt">seismic</span> noise recorded on 60 <span class="hlt">seismic</span> stations was used to image a near-mine target. The target consists of a known ore-body that has been partially exhausted by mining efforts roughly 100 years ago. The experiment examined whether ambient <span class="hlt">seismic</span> noise interferometry can be used to image the intact and exhausted ore deposit. A drilling campaign was also conducted near the target which offers the opportunity to compare the two methods. If the accuracy and resolution of passive <span class="hlt">seismic</span> imaging can be improved to that of active surveys (and beyond), this method could become an inexpensive intermediary step in the exploration process and result</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014334','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014334"><span>Precursory <span class="hlt">seismic</span> quiescence: A preliminary assessment of the hypothesis</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reasenberg, P.A.; Matthews, M.V.</p> <p>1988-01-01</p> <p>Numerous cases of precursory <span class="hlt">seismic</span> quiescence have been reported in recent years. Some investigators have <span class="hlt">interpreted</span> these observations as evidence that <span class="hlt">seismic</span> quiescence is a somewhat reliable precursor to moderate or large earthquakes. However, because failures of the pattern to predict earthquakes may not, in general, be reported, and because numerous earthquakes are not preceded by quiescence, the validity and reliability of the quiescence precursor have not been established. We have analyzed the <span class="hlt">seismicity</span> rate prior to, and in the source region of, 37 shallow earthquakes (M 5.3-7.0) in central California and Japan for patterns of rate fluctuation, especially precursory quiescence. Nonuniformity in rate for these pre-mainshock sequences is relatively high, and numerous intervals with significant (p<0.10) extrema in rate are observed in some of the sequences. In other sequences, however, the rate remains within normal limits up to the time of the mainshock. Overall, in terms of an observational basis for intermediate-term earthquake prediction, no evidence is found in the cases studied for a systematic, widespread or reliable pattern of quiescence prior to the mainshocks. In earthquake sequences comprising full <span class="hlt">seismic</span> cycles for 5 sets of (M 3.7-5.1) repeat earthquakes on the San Andreas fault near Bear Valley, California, the <span class="hlt">seismicity</span> rates are found to be uniform. A composite of the estimated rate fluctuations for the sequences, normalized to the length of the <span class="hlt">seismic</span> cycle, reveals a weak pattern of a low rate in the first third of the cycle, and a high rate in the last few months. While these observations are qualitative, they may represent weak expressions of physical processes occurring in the source region over the <span class="hlt">seismic</span> cycle. Re-examination of <span class="hlt">seismicity</span> rate fluctuations in volumes along the creeping section of the San Andreas fault specified by Wyss and Burford (1985) qualitatively confirms the existence of low-rate intervals in volumes 361</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/70191533','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191533"><span>Micro-<span class="hlt">seismicity</span> within the Coso Geothermal field, California, from 1996-2012</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kaven, Joern; Hickman, Stephen H.; Weber, Lisa C.</p> <p>2017-01-01</p> <p>We extend our previous catalog of <span class="hlt">seismicity</span> within the Coso Geothermal field by adding over two and a half years of additional data to prior results. In total, we locate over 16 years of <span class="hlt">seismicity</span> spanning from April 1996 to May of 2012 using a refined velocity model, apply it to all events and utilize differential travel times in relocations to improve the accuracy of event locations. The improved locations elucidate major structural features within the reservoir that we <span class="hlt">interpret</span> to be faults that contribute to heat and fluid flow within the reservoir. Much of the relocated <span class="hlt">seismicity</span> remains diffuse between these major structural features, suggesting that a large volume of accessible and distributed fracture porosity is maintained within the geothermal reservoir through ongoing brittle failure. We further track changes in b value and <span class="hlt">seismic</span> moment release within the reservoir as a whole through time. We find that b values decrease significantly during 2009 and 2010, coincident with the occurrence of a greater number of moderate magnitude earthquakes (3.0 ≤ ML < 4.5). Analysis of spatial variations in <span class="hlt">seismic</span> moment release between years reveals that localized <span class="hlt">seismicity</span> tends to spread from regions of high moment release into regions with previously low moment release, akin to aftershock sequences. These results indicate that the Coso reservoir is comprised of a network of fractures at a variety of spatial scales that evolves dynamically over time, with progressive changes in characteristics of microseismicity and inferred fractures and faults that are only evident from a long period of <span class="hlt">seismic</span> monitoring analyzed using self-consistent methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.4462B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.4462B"><span>Reassessment of the <span class="hlt">Seismicity</span> and <span class="hlt">seismic</span> hazards of Libya</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ben Suleman, A.; Elmeladi, A.</p> <p>2009-04-01</p> <p>The tectonic evolution of Libya, located at the northern extreme of the African continent, has yielded a complex crustal structure that is composed of a series of basins and uplifts. The present day deformation of Libya is the result of the Eurasia-Africa continental collision. At the end of the year 2005, The Libyan National Seismological Network was established to monitor local, regional and teleseismic activities, as well as to provide high quality data for research projects both locally and on the regional and global scale. This study aims to discuss the <span class="hlt">seismicity</span> of Libya by using the new data from the Libyan national seismological network and to focus on the <span class="hlt">seismic</span> hazards. At first glance the <span class="hlt">seismic</span> activity map shows dominant trends of <span class="hlt">seismicity</span> with most of the <span class="hlt">seismic</span> activity concentrated along the northern coastal areas. Four major <span class="hlt">seismic</span> trends were quite noticeable. A first trend is a NW-SE direction coinciding with the eastern boarder of the Hun Graben. A second trend is also a NW-SE direction in the offshore area and might be a continuation of this trend. The other two trends were located in the western Gulf of Sirt and Cyrenaica platform. The rest of <span class="hlt">seismicity</span> is diffuse either offshore or in land, with no good correlation with well-mapped faults. Detailed investigations of the Libyan <span class="hlt">seismicity</span> indicates that the Libya has experienced earthquakes of varying magnitudes and that there is definitely a certain amount of <span class="hlt">seismic</span> risk involved in engineering projects, particularly in the northern regions. Detailed investigation of the distribution of the Libyan earthquakes in space and time along with all other geological considerations suggested the classification of the country into four <span class="hlt">seismic</span> zones with the Hun graben zone being the most <span class="hlt">seismically</span> active zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910023539','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910023539"><span>The formal verification of generic <span class="hlt">interpreters</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Windley, P.; Levitt, K.; Cohen, G. C.</p> <p>1991-01-01</p> <p>The task assignment 3 of the design and validation of digital flight control systems suitable for fly-by-wire applications is studied. Task 3 is associated with formal verification of embedded systems. In particular, results are presented that provide a methodological approach to microprocessor verification. A hierarchical decomposition strategy for specifying microprocessors is also presented. A theory of generic <span class="hlt">interpreters</span> is presented that can be used to model microprocessor behavior. The generic <span class="hlt">interpreter</span> theory <span class="hlt">abstracts</span> away the details of instruction functionality, leaving a general model of what an <span class="hlt">interpreter</span> does.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNH11A1704S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNH11A1704S"><span>Retrieval of P wave Basin Response from Autocorrelation of <span class="hlt">Seismic</span> Noise-Jakarta, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saygin, E.; Cummins, P. R.; Lumley, D. E.</p> <p>2016-12-01</p> <p>Indonesia's capital city, Jakarta, is home to a very large (over 10 million), vulnerable population and is proximate to known active faults, as well as to the subduction of Australian plate, which has a megathrust at abut 300 km distance, as well as intraslab <span class="hlt">seismicity</span> extending to directly beneath the city. It is also located in a basin filled with a thick layer of unconsolidated and poorly consolidated sediment, which increases the <span class="hlt">seismic</span> hazard the city is facing. Therefore, the information on the <span class="hlt">seismic</span> velocity structure of the basin is crucial for increasing our knowledge of the <span class="hlt">seismic</span> risk. We undertook a passive deployment of broadband seismographs throughout the city over a 3-month interval in 2013-2014, recording ambient <span class="hlt">seismic</span> noise at over 90 sites for intervals of 1 month or more. Here we consider autocorrelations of the vertical component of the continuously recorded <span class="hlt">seismic</span> wavefield across this dense network to image the shallow P wave velocity structure of Jakarta, Indonesia. Unlike the surface wave Green's functions used in ambient noise tomography, the vertical-component autocorrelograms are dominated by body wave energy that is potentially sensitive to sharp velocity contrasts, which makes them useful in <span class="hlt">seismic</span> imaging. Results show autocorrelograms at different <span class="hlt">seismic</span> stations with travel time variations that largely reflect changes in sediment thickness across the basin. We also confirm the validity our <span class="hlt">interpretation</span> of the observed autocorrelation waveforms by conducting 2D finite difference full waveform numerical modeling for randomly distributed <span class="hlt">seismic</span> sources to retrieve the reflection response through autocorrelation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1412717C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1412717C"><span><span class="hlt">Seismic</span> monitoring at Deception Island volcano (Antarctica): Recent advances</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carmona, E.; Almendros, J.; Martín, R.; Cortés, G.; Alguacil, G.; Moreno, J.; Martín, B.; Martos, A.; Serrano, I.; Stich, D.; Ibáñez, J. M.</p> <p>2012-04-01</p> <p> at Deception Island since 2008. In the current survey we collaborate with the Spanish Army to add another permanent station that will be able to send to the IAG-UGR <span class="hlt">seismic</span> information about the activity of the volcano during the winter, using a communications satellite (SPAINSAT). These advances simplify the field work and the data acquisition procedures, and allow us to obtain high-quality <span class="hlt">seismic</span> data in real-time. These improvements have a very important significance for a better and faster <span class="hlt">interpretation</span> of the seismo-volcanic activity and assessment of the volcanic hazards at Deception Island volcano.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMOS52B..06Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMOS52B..06Z"><span><span class="hlt">Seismic</span> investigation of an ocean-continent transition zone in the northern South China Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, J.; Qiu, X.; Xu, H.; Zhan, W.; Sun, Z.</p> <p>2011-12-01</p> <p>Rifted continental margins and basins are mainly formed by the lithospheric extension. Thined lithosphere of passive continental margins results in decompression melt of magma and created oceanic crust and thined ocean-continent transition (OCT) zone. Two refraction profiles used ocean bottom seismometers deployed in the broad continental shelf and three multi-channel <span class="hlt">seismic</span> reflection lines in the northern South China Sea, acquired by the ship "Shiyan 2" of the South China Sea Institute of Oceanology, Chinese Academy of Sciences in 2010, are processed and <span class="hlt">interpreted</span> in this study. <span class="hlt">Seismic</span> reflection lines cut through the Dongsha rise, Zhu-1 and Zhu-2 depression within a Tertiary basin, Pear River Mouth basin (called as Zhujiangkou basin). These tectonic features are clear imaged in the <span class="hlt">seismic</span> reflection records. Numerous normal faults, cutted through the basement and related to the stretch of the northern South China Sea margin, are imaged and <span class="hlt">interpreted</span>. Reflection characteristics of the ocean-continent transition (OCT) zone are summaried and outlined. The COT zone is mainly divided into the northern syn-rift subsidence zone, central volcano or buried volcano uplift zone and tilt faulted block near the South Chia Sea basin. Compared to the previous <span class="hlt">seismic</span> reflection data and refraction velocity models, the segmentation range of the OCT zone is outlined, from width of about 225 km in the northeastern South China Sea , of 160 km in the central to of 110 km in the north-central South China Sea. Based on the epicenter distribution of sporadic and large than 6 magnitude earthquakes, it suggests the OCT zone in the northern South China Sea at present is still an active <span class="hlt">seismic</span> zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E3SWC..3503007W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E3SWC..3503007W"><span>Instantaneous Attributes Applied to Full Waveform Sonic Log and <span class="hlt">Seismic</span> Data in Integration of Elastic Properties of Shale Gas Formations in Poland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wawrzyniak-Guz, Kamila</p> <p>2018-03-01</p> <p><span class="hlt">Seismic</span> attributes calculated from full waveform sonic log were proposed as a method that may enhance the <span class="hlt">interpretation</span> the data acquired at log and <span class="hlt">seismic</span> scales. Though attributes calculated in the study were the mathematical transformations of amplitude, frequency, phase or time of the acoustic full waveforms and <span class="hlt">seismic</span> traces, they could be related to the geological factors and/or petrophysical properties of rock formations. Attributes calculated from acoustic full waveforms were combined with selected attributes obtained for <span class="hlt">seismic</span> traces recorded in the vicinity of the borehole and with petrophysical parameters. Such relations may be helpful in elastic and reservoir properties estimation over the area covered by the <span class="hlt">seismic</span> survey.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4783796-site-cavity-location-seismic-profiling-nevada-test-site','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/4783796-site-cavity-location-seismic-profiling-nevada-test-site"><span>ON-SITE CAVITY LOCATION-<span class="hlt">SEISMIC</span> PROFILING AT NEVADA TEST SITE</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>Forbes, C.B.; Peterson, R.A.; Heald, C.L.</p> <p>1961-10-25</p> <p>Experimental <span class="hlt">seismic</span> studies were conducted at the Nevada Test Site for the purpose of designing and evaluating the most promising <span class="hlt">seismic</span> techniques for on-site inspection. Post-explosion <span class="hlt">seismic</span> profiling was done in volcanic tuff in the vicinity of the Rainier and Blanca underground explosions. Pre-explosion <span class="hlt">seismic</span> profiling was done over granitic rock outcrops in the Climax Stock area, and over tuff at proposed location for Linen and Orchid. Near surface velocity profiling techniques based on measurements of <span class="hlt">seismic</span> time-distance curves gave evidence of disturbances in near surface rock velocities over the Rainier and Refer als0 to <span class="hlt">abstract</span> 30187. Blanca sites. Thesemore » disturbances appear to be related to near surface fracturing and spallation effects resulting from the reflection of the original intense compression wave pulse at the near surface as a tension pulse. Large tuned seismometer arrays were used for horizontal <span class="hlt">seismic</span> ranging in an attempt to record back-scattered'' or reflected <span class="hlt">seismic</span> waves from subsurface cavities or zones of rock fracturing around the underground explosions. Some possible <span class="hlt">seismic</span> events were recorded from the near vicinities of the Rainier and Blanca sites. However, many more similar events were recorded from numerous other locations, presumably originating from naturally occurring underground geological features. No means was found for discriminating between artificial and natural events recorded by horizontal <span class="hlt">seismic</span> ranging, and the results were, therefore, not immediately useful for inspection purposes. It is concluded that in some instances near surface velocity profiling methods may provide a useful tool in verifying the presence of spalled zones above underground nuclear explosion sites. In the case of horizontal <span class="hlt">seismic</span> ranging it appears that successful application would require development of satisfactory means for recognition of and discrimination against <span class="hlt">seismic</span> responses to naturally occurring geological</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912973B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912973B"><span>Advanced <span class="hlt">seismic</span> imaging of overdeepened alpine valleys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burschil, Thomas; Buness, Hermann; Tanner, David; Gabriel, Gerald; Krawczyk, Charlotte M.</p> <p>2017-04-01</p> <p> the <span class="hlt">interpretation</span>, two possible drilling sites are suggested for DOVE that will also prove the <span class="hlt">seismic</span> <span class="hlt">interpretation</span> and explain differences in P- and S-wave imaging. First results for the intermountain Lienz Basin are available from four parallel P-wave sections which show the asymmetric basin shape. The sedimentary base is well imaged down to ca. 0.6 km depth, and internal reflectors point to a diverse fill. Here, S-wave imaging produces less distinct sections and requires more sophisticated processing. In summary, P-wave imaging is suitable to map overdeepened structures in the Alps while S-wave imaging can contribute additional information.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T33D0765H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T33D0765H"><span>Detailed <span class="hlt">seismic</span> velocity structure of the ultra-slow spread crust at the Mid-Cayman Spreading Center from travel-time tomography and synthetic seismograms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harding, J.; Van Avendonk, H. J.; Hayman, N. W.; Grevemeyer, I.; Peirce, C.</p> <p>2017-12-01</p> <p>The Mid-Cayman Spreading Center (MCSC), an ultraslow-spreading center in the Caribbean Sea, has formed highly variable oceanic crust. Seafloor dredges have recovered extrusive basalts in the axial deeps as well as gabbro on bathymetric highs and exhumed mantle peridotite along the only 110 km MCSC. Wide-angle refraction data were collected with active-source ocean bottom seismometers in April, 2015, along lines parallel and across the MCSC. Travel-time tomography produces relatively smooth 2-D tomographic models of compressional wave velocity. These velocity models reveal large along- and across-axis variations in <span class="hlt">seismic</span> velocity, indicating possible changes in crustal thickness, composition, faulting, and magmatism. It is difficult, however, to differentiate between competing <span class="hlt">interpretations</span> of <span class="hlt">seismic</span> velocity using these tomographic models alone. For example, in some areas the <span class="hlt">seismic</span> velocities may be explained by either thin igneous crust or exhumed, serpentinized mantle. Distinguishing between these two <span class="hlt">interpretations</span> is important as we explore the relationships between magmatism, faulting, and hydrothermal venting at ultraslow-spreading centers. We therefore improved our constraints on the shallow <span class="hlt">seismic</span> velocity structure of the MCSC by modeling the amplitude of <span class="hlt">seismic</span> refractions in the wide-angle data set. Synthetic seismograms were calculated with a finite-difference method for a range of models with different vertical velocity gradients. Small-scale features in the velocity models, such as steep velocity gradients and Moho boundaries, were explored systematically to best fit the real data. With this approach, we have improved our understanding of the compressional velocity structure of the MCSC along with the geological <span class="hlt">interpretations</span> that are consistent with three <span class="hlt">seismic</span> refraction profiles. Line P01 shows a variation in the thinness of lower <span class="hlt">seismic</span> velocities along the axis, indicating two segment centers, while across-axis lines P02 and P03</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AcGeo..55..191P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AcGeo..55..191P"><span>Identification of <span class="hlt">seismic</span> anomalies caused by gas saturation on the basis of theoretical P and PS wavefield in the Carpathian Foredeep, SE Poland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pietsch, Kaja; Marzec, Paweł; Kobylarski, Marcin; Danek, Tomasz; Leśniak, Andrzej; Tatarata, Artur; Gruszczyk, Edward</p> <p>2007-06-01</p> <p>The thin-layer build of the Carpathian Foredeep Miocene formations and large petrophysical parameter variation cause <span class="hlt">seismic</span> images of gas-saturated zones to be ambiguous, and the location of prospection wells on the basis of anomalous <span class="hlt">seismic</span> record is risky. A method that assists reservoir <span class="hlt">interpretation</span> of standard recorded <span class="hlt">seismic</span> profiles (P waves) can be a converted wave recording (PS waves). This paper presents the results of application of a multicomponent <span class="hlt">seismic</span> survey for the reservoir <span class="hlt">interpretation</span> over the Chałupki Dębniańskie gas deposit, carried out for the first time in Poland by Geofizyka Kraków Ltd. for the Polish Oil and Gas Company. <span class="hlt">Seismic</span> modeling was applied as the basic research tool, using the SeisMod program based on the finite-difference solution of the acoustic wave equation and equations of motion. Seismogeological models for P waves were developed using Acoustic Logs; S-wave model (records only from part of the well) was developed on the basis of theoretical curves calculated by means of the Estymacja program calibrated with average S-velocities, calculated by correlation of recorded P and PS wavefields with 1D modeling. The conformity between theoretical and recorded wavefields makes it possible to apply the criteria established on the basis of modeling for reservoir <span class="hlt">interpretation</span>. Direct hydrocarbon indicators (bright spots, phase change, time sag) unambiguously identify gas-prone layers within the ChD-2 prospect. A partial range of the indicators observed in the SW part of the studied profile (bright spot that covers a single, anticlinally bent <span class="hlt">seismic</span> horizon) points to saturation of the horizon. The proposed location is confirmed by criteria determined for converted waves (continuous <span class="hlt">seismic</span> horizons with constant, high amplitude) despite poorer agreement between theoretical and recorded wavefields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6987349-merging-seismic-mt-garden-valley-nevada','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6987349-merging-seismic-mt-garden-valley-nevada"><span>Merging <span class="hlt">seismic</span> and MT in Garden Valley, Nevada</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>Telleen, K.E.</p> <p>1986-04-01</p> <p>In the northern part of Garden Valley, Nevada, a 1978 regional <span class="hlt">seismic</span> program encountered a large area of poor to no-reflection data. Surface geology suggested that a large high structure might underlie the valley floor, and that shallowly buried basalts were causing the poor data. The implied strongly layered structure of electrical resistivity - resistive basalt on conductive Tertiary clastics on resistive paleozoic carbonates - formed an ideal theater for the magnetotelluric method. In 1984, Conoco acquired 48 magnetotelluric sites on about a half-mile grid. These data supported the presence of a buried high block in the Paleozoic rocks andmore » allowed confident mapping of its outlines. In addition, the magnetotelluric survey showed a thin, shallowly buried resistor coextensive with the <span class="hlt">seismic</span> no-reflection area. In 1985, a high-effort repeat of the earlier no-reflection <span class="hlt">seismic</span> line confirmed the high block, improved the fault <span class="hlt">interpretation</span>, and provided weak guidance on the depth of the targeted Paleozoic rocks. Because Garden Valley's Paleozoic stratigraphy differs negligibly from that at nearby Grant Canyon field, the high block constitutes an attractive prospect - possibly the first one found in Nevada due largely to magnetotelluric surveying.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRB..121.6009K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRB..121.6009K"><span>Validating induced <span class="hlt">seismicity</span> forecast models—Induced <span class="hlt">Seismicity</span> Test Bench</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Király-Proag, Eszter; Zechar, J. Douglas; Gischig, Valentin; Wiemer, Stefan; Karvounis, Dimitrios; Doetsch, Joseph</p> <p>2016-08-01</p> <p>Induced earthquakes often accompany fluid injection, and the <span class="hlt">seismic</span> hazard they pose threatens various underground engineering projects. Models to monitor and control induced <span class="hlt">seismic</span> hazard with traffic light systems should be probabilistic, forward-looking, and updated as new data arrive. In this study, we propose an Induced <span class="hlt">Seismicity</span> Test Bench to test and rank such models; this test bench can be used for model development, model selection, and ensemble model building. We apply the test bench to data from the Basel 2006 and Soultz-sous-Forêts 2004 geothermal stimulation projects, and we assess forecasts from two models: Shapiro and Smoothed <span class="hlt">Seismicity</span> (SaSS) and Hydraulics and <span class="hlt">Seismics</span> (HySei). These models incorporate a different mix of physics-based elements and stochastic representation of the induced sequences. Our results show that neither model is fully superior to the other. Generally, HySei forecasts the <span class="hlt">seismicity</span> rate better after shut-in but is only mediocre at forecasting the spatial distribution. On the other hand, SaSS forecasts the spatial distribution better and gives better <span class="hlt">seismicity</span> rate estimates before shut-in. The shut-in phase is a difficult moment for both models in both reservoirs: the models tend to underpredict the <span class="hlt">seismicity</span> rate around, and shortly after, shut-in.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.S12B0609S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.S12B0609S"><span>Current <span class="hlt">Seismicity</span> in the Vicinity of Yucca Mountain, Nevada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, K.; von Seggern, D.; dePolo, D.</p> <p>2001-12-01</p> <p>The 1992 to 2000 earthquakes in the Southern Great Basin have been relocated in order to better recognize the active tectonic processes in the vicinity of Yucca Mountain. During this time period <span class="hlt">seismic</span> monitoring in the Southern Great Basin transitioned from a primarily single-component analog network to a 3-component digital network. Through the transition analog and digital networks were run in tandem. The station density over this period is as great as any prior recording period. The analog and digital networks were administered separately during the transition, and we have merged the phase data from the two operations. We performed relocations starting in October 1992, thus creating a hypocentral list for FY1993-FY2000. Aftershocks of the June 1992 M 5.6 Little Skull Mountain earthquake, located approximately 20 km southeast of Yucca Mountain, dominate the <span class="hlt">seismicity</span> in the Southern Great Basin from 1992-2000. After the Little Skull Mountain earthquake, there was a general increase in earthquake activity in southern NTS, principally associated with the Rock Valley fault zone. There was no corresponding increase in <span class="hlt">seismicity</span> west of Little Skull Mountain near the potential repository site. The distribution of high-quality earthquake locations generally reflects trends in Miocene tectonism. In particular, a general north-south trending gravity low, <span class="hlt">interpreted</span> by Carr (1984) as the Kawich-Greenwater Rift, is highlighted by the microseismicity in many areas. Locally small magnitude earthquakes tend to outline the 8-10 Ma Timber Mountain caldera in northern and central NTS. Although these structures do not generally correlate with Quaternary faults, the micro-earthquake activity may reflect zones of weakness within these older structures. A 100 km long, conspicuous, north-south trending <span class="hlt">seismic</span> zone, which shows no correlation with know Quaternary features, aligns along the steep gravity gradient bordering the western side of the Kawich-Greenwater gravity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033279','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033279"><span>Successful gas hydrate prospecting using 3D <span class="hlt">seismic</span> - A case study for the Mt. Elbert prospect, Milne Point, North Slope Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Inks, T.L.; Agena, W.F.</p> <p>2008-01-01</p> <p>In February 2007, the Mt. Elbert Prospect stratigraphic test well, Milne Point, North Slope Alaska encountered thick methane gas hydrate intervals, as predicted by 3D <span class="hlt">seismic</span> <span class="hlt">interpretation</span> and modeling. Methane gas hydrate-saturated sediment was found in two intervals, totaling more than 100 ft., identified and mapped based on <span class="hlt">seismic</span> character and wavelet modeling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1093N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1093N"><span>The Role of Faulting on the Growth of a Carbonate Platform: Evidence from 3D <span class="hlt">Seismic</span> Analysis and Section Restoration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nur Fathiyah Jamaludin, Siti; Pubellier, Manuel; Prasad Ghosh, Deva; Menier, David; Pierson, Bernard</p> <p>2014-05-01</p> <p>Tectonics in addition to other environmental factors impacts the growth of carbonate platforms and plays an important role in shaping the internal architecture of the platforms. Detailed of faults and fractures development and healing in carbonate environment have not been explored sufficiently. Using 3D <span class="hlt">seismic</span> and well data, we attempt to reconstruct the structural evolution of a Miocene carbonate platform in Central Luconia Province, offshore Malaysia. Luconia Province is located in the NW coast of Borneo and has become one of the largest carbonate factories in SE Asia. <span class="hlt">Seismic</span> <span class="hlt">interpretations</span> including <span class="hlt">seismic</span> attribute analysis are applied to the carbonate platform to discern its sedimentology and structural details. Detailed <span class="hlt">seismic</span> <span class="hlt">interpretations</span> highlight the relationships of carbonate deposition with syn-depositional faulting. Branching conjugate faults are common in this carbonate platform and have become a template for reef growth, attesting lateral facies changes within the carbonate environments. Structural restoration was then appropriately performed on the <span class="hlt">interpreted</span> <span class="hlt">seismic</span> sections based on sequential restoration techniques, and provided images different from those of horizon flattening methods. This permits us to compensate faults' displacement, remove recent sediment layers and finally restore the older rock units prior to the fault motions. It allows prediction of platform evolution as a response to faulting before and after carbonate deposition and also enhances the pitfalls of <span class="hlt">interpretation</span>. Once updated, the reconstructions allow unravelling of the un-seen geological features underneath the carbonate platform, such as paleo-structures and paleo-topography which in turn reflects the paleo-environment before deformations took place. Interestingly, sections balancing and restoration revealed the late-phase (Late Oligocene-Early Miocene) rifting of South China Sea, otherwise difficult to visualize on <span class="hlt">seismic</span> sections. Later it is shown that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JSeis..21..941K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JSeis..21..941K"><span><span class="hlt">Seismic</span> hazard estimation of northern Iran using smoothed <span class="hlt">seismicity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khoshnevis, Naeem; Taborda, Ricardo; Azizzadeh-Roodpish, Shima; Cramer, Chris H.</p> <p>2017-07-01</p> <p>This article presents a <span class="hlt">seismic</span> hazard assessment for northern Iran, where a smoothed <span class="hlt">seismicity</span> approach has been used in combination with an updated <span class="hlt">seismic</span> catalog and a ground motion prediction equation recently found to yield good fit with data. We evaluate the hazard over a geographical area including the <span class="hlt">seismic</span> zones of Azerbaijan, the Alborz Mountain Range, and Kopeh-Dagh, as well as parts of other neighboring <span class="hlt">seismic</span> zones that fall within our region of interest. In the chosen approach, <span class="hlt">seismic</span> events are not assigned to specific faults but assumed to be potential seismogenic sources distributed within regular grid cells. After performing the corresponding magnitude conversions, we decluster both historical and instrumental <span class="hlt">seismicity</span> catalogs to obtain earthquake rates based on the number of events within each cell, and smooth the results to account for the uncertainty in the spatial distribution of future earthquakes. <span class="hlt">Seismicity</span> parameters are computed for each <span class="hlt">seismic</span> zone separately, and for the entire region of interest as a single uniform seismotectonic region. In the analysis, we consider uncertainties in the ground motion prediction equation, the <span class="hlt">seismicity</span> parameters, and combine the resulting models using a logic tree. The results are presented in terms of expected peak ground acceleration (PGA) maps and hazard curves at selected locations, considering exceedance probabilities of 2 and 10% in 50 years for rock site conditions. According to our results, the highest levels of hazard are observed west of the North Tabriz and east of the North Alborz faults, where expected PGA values are between about 0.5 and 1 g for 10 and 2% probability of exceedance in 50 years, respectively. We analyze our results in light of similar estimates available in the literature and offer our perspective on the differences observed. We find our results to be helpful in understanding <span class="hlt">seismic</span> hazard for northern Iran, but recognize that additional efforts are necessary to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19730013015&hterms=mortar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmortar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19730013015&hterms=mortar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmortar"><span>Active <span class="hlt">seismic</span> experiment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kovach, R. L.; Watkins, J. S.; Talwani, P.</p> <p>1972-01-01</p> <p>The Apollo 16 active <span class="hlt">seismic</span> experiment (ASE) was designed to generate and monitor <span class="hlt">seismic</span> waves for the study of the lunar near-surface structure. Several <span class="hlt">seismic</span> energy sources are used: an astronaut-activated thumper device, a mortar package that contains rocket-launched grenades, and the impulse produced by the lunar module ascent. Analysis of some <span class="hlt">seismic</span> signals recorded by the ASE has provided data concerning the near-surface structure at the Descartes landing site. Two compressional <span class="hlt">seismic</span> velocities have so far been recognized in the <span class="hlt">seismic</span> data. The deployment of the ASE is described, and the significant results obtained are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023654','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023654"><span><span class="hlt">Seismic</span> reflection images of shallow faulting, northernmost Mississippi embayment, north of the New Madrid <span class="hlt">seismic</span> zone</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McBride, J.H.; Nelson, W.J.</p> <p>2001-01-01</p> <p>High-resolution <span class="hlt">seismic</span> reflection surveys document tectonic faults that displace Pleistocene and older strata just beyond the northeast termination of the New Madrid <span class="hlt">seismic</span> zone, at the northernmost extent of the Mississippi embayment. These faults, which are part of the Fluorspar Area fault complex in southeastern Illinois, are directly in line with the northeast-trending <span class="hlt">seismic</span> zone. The reflection data were acquired using an elastic weight-drop source recorded to 500 msec by a 48-geophone array (24-fold) with a 10-ft (??3.0m) station interval. Recognizable reflections were recorded to about 200 msec (100-150 m). The effects of multiple reflections, numerous diffractions, low apparent velocity (i.e., steeply dipping) noise, and the relatively low-frequency content of the recorded signal provided challenges for data processing and <span class="hlt">interpreting</span> subtle fault offsets. Data processing steps that were critical to the detection of faults included residual statics, post-stack migration, deconvolution, and noise-reduction filtering. <span class="hlt">Seismic</span> migration was crucial for detecting and mitigating complex fault-related diffraction patterns, which produced an apparent 'folding' of reflectors on unmigrated sections. Detected individual offsets of shallow reflectors range from 5 to 10 m for the top of Paleozoic bedrock and younger strata. The migrated sections generally indicate vertical to steeply dipping normal and reverse faults, which in places outline small horsts and/or grabens. Tilting or folding of stratal reflectors associated with faulting is also locally observed. At one site, the observed faulting is superimposed over a prominent antiformal structure, which may itself be a product of the Quaternary deformation that produced the steep normal and reverse faults. Our results suggest that faulting of the Paleozoic bedrock and younger sediments of the northern Mississippi embayment is more pervasive and less localized than previously thought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010066742','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010066742"><span>Theory <span class="hlt">Interpretations</span> in PVS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Owre, Sam; Shankar, Natarajan; Butler, Ricky W. (Technical Monitor)</p> <p>2001-01-01</p> <p>The purpose of this task was to provide a mechanism for theory <span class="hlt">interpretations</span> in a prototype verification system (PVS) so that it is possible to demonstrate the consistency of a theory by exhibiting an <span class="hlt">interpretation</span> that validates the axioms. The mechanization makes it possible to show that one collection of theories is correctly <span class="hlt">interpreted</span> by another collection of theories under a user-specified <span class="hlt">interpretation</span> for the uninterpreted types and constants. A theory instance is generated and imported, while the axiom instances are generated as proof obligations to ensure that the <span class="hlt">interpretation</span> is valid. <span class="hlt">Interpretations</span> can be used to show that an implementation is a correct refinement of a specification, that an axiomatically defined specification is consistent, or that a axiomatically defined specification captures its intended models. In addition, the theory parameter mechanism has been extended with a notion of theory as parameter so that a theory instance can be given as an actual parameter to an imported theory. Theory <span class="hlt">interpretations</span> can thus be used to refine an <span class="hlt">abstract</span> specification or to demonstrate the consistency of an axiomatic theory. In this report we describe the mechanism in detail. This extension is a part of PVS version 3.0, which will be publicly released in mid-2001.</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/70024624','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024624"><span><span class="hlt">Seismic</span> anisotropy and mantle creep in young orogens</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Meissner, R.; Mooney, W.D.; Artemieva, I.</p> <p>2002-01-01</p> <p><span class="hlt">Seismic</span> anisotropy provides evidence for the physical state and tectonic evolution of the lithosphere. We discuss the origin of anisotropy at various depths, and relate it to tectonic stress, geotherms and rheology. The anisotropy of the uppermost mantle is controlled by the orthorhombic mineral olivine, and may result from ductile deformation, dynamic recrystallization or annealing. Anisotropy beneath young orogens has been measured for the <span class="hlt">seismic</span> phase Pn that propagates in the uppermost mantle. This anisotropy is <span class="hlt">interpreted</span> as being caused by deformation during the most recent thermotectonic event, and thus provides information on the process of mountain building. Whereas tectonic stress and many structural features in the upper crust are usually orientated perpendicular to the structural axis of mountain belts, Pn anisotropy is aligned parallel to the structural axis. We <span class="hlt">interpret</span> this to indicate mountain-parallel ductile (i.e. creeping) deformation in the uppermost mantle that is a consequence of mountain-perpendicular compressive stresses. The preferred orientation of the fast axes of some anisotropic minerals, such as olivine, is known to be in the creep direction, a consequence of the anisotropy of strength and viscosity of orientated minerals. In order to explain the anisotropy of the mantle beneath young orogens we extend the concept of crustal 'escape' (or 'extrusion') tectonics to the uppermost mantle. We present rheological model calculations to support this hypothesis. Mountain-perpendicular horizontal stress (determined in the upper crust) and mountain-parallel <span class="hlt">seismic</span> anisotropy (in the uppermost mantle) require a zone of ductile decoupling in the middle or lower crust of young mountain belts. Examples for stress and mountain-parallel Pn anisotropy are given for Tibet, the Alpine chains, and young mountain ranges in the Americas. Finally, we suggest a simple model for initiating mountain parallel creep.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMDI43A2661L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMDI43A2661L"><span>A first step to compare geodynamical models and <span class="hlt">seismic</span> observations of the inner core</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lasbleis, M.; Waszek, L.; Day, E. A.</p> <p>2016-12-01</p> <p><span class="hlt">Seismic</span> observations have revealed a complex inner core, with lateral and radial heterogeneities at all observable scales. The dominant feature is the east-west hemispherical dichotomy in <span class="hlt">seismic</span> velocity and attenuation. Several geodynamical models have been proposed to explain the observed structure: convective instabilities, external forces, crystallisation processes or influence of outer core convection. However, <span class="hlt">interpreting</span> such geodynamical models in terms of the <span class="hlt">seismic</span> observations is difficult, and has been performed only for very specific models (Geballe 2013, Lincot 2014, 2016). Here, we propose a common framework to make such comparisons. We have developed a Python code that propagates <span class="hlt">seismic</span> ray paths through kinematic geodynamical models for the inner core, computing a synthetic <span class="hlt">seismic</span> data set that can be compared to <span class="hlt">seismic</span> observations. Following the method of Geballe 2013, we start with the simple model of translation. For this, the <span class="hlt">seismic</span> velocity is proposed to be function of the age or initial growth rate of the material (since there is no deformation included in our models); the assumption is reasonable when considering translation, growth and super rotation of the inner core. Using both artificial (random) <span class="hlt">seismic</span> ray data sets and a real inner core data set (from Waszek et al. 2011), we compare these different models. Our goal is to determine the model which best matches the <span class="hlt">seismic</span> observations. Preliminary results show that super rotation successfully creates an eastward shift in properties with depth, as has been observed <span class="hlt">seismically</span>. Neither the growth rate of inner core material nor the relationship between crystal size and <span class="hlt">seismic</span> velocity are well constrained. Consequently our method does not directly compute the <span class="hlt">seismic</span> travel times. Instead, here we use age, growth rate and other parameters as proxies for the <span class="hlt">seismic</span> properties, which represent a good first step to compare geodynamical and <span class="hlt">seismic</span> observations.Ultimately we aim</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNS31B0011L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNS31B0011L"><span>Time-lapse <span class="hlt">seismic</span> - repeatability versus usefulness and 2D versus 3D</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Landro, M.</p> <p>2017-12-01</p> <p>Time-lapse <span class="hlt">seismic</span> has developed rapidly over the past decades, especially for monitoring of oil and gas reservoirs and subsurface storage of CO2. I will review and discuss some of the critical enabling factors for the commercial success of this technology. It was early realized that how well we are able to repeat our <span class="hlt">seismic</span> experiment is crucial. However, it is always a question of detectability versus repeatability. For marine <span class="hlt">seismic</span>, there are several factors limiting the repeatability: Weather conditions, positioning of sources and receivers and so on. I will discuss recent improvements in both acquisition and processing methods over the last decade. It is well known that repeated 3D <span class="hlt">seismic</span> data is the most accurate tool for reservoir monitoring purposes. However, several examples show that 2D <span class="hlt">seismic</span> data may be used for monitoring purposes despite lower repeatability. I will use examples from an underground blow out in the North Sea, and repeated 2D <span class="hlt">seismic</span> lines acquired before and after the Tohoku earthquake in 2011 to illustrate this. A major challenge when using repeated 2D <span class="hlt">seismic</span> for subsurface monitoring purposes is the lack of 3D calibration points and significantly less amount of data. For marine <span class="hlt">seismic</span> acquisition, feathering issues and crossline dip effects become more critical compared to 3D <span class="hlt">seismic</span> acquisition. Furthermore, the uncertainties arising from a non-ideal 2D <span class="hlt">seismic</span> acquisition are hard to assess, since the 3D subsurface geometry has not been mapped. One way to shed more light on this challenge is to use 3D time lapse <span class="hlt">seismic</span> modeling testing various crossline dips or geometries. Other ways are to use alternative data sources, such as bathymetry, time lapse gravity or electromagnetic data. The end result for all time-lapse monitoring projects is an <span class="hlt">interpretation</span> associated with uncertainties, and for the 2D case these uncertainties are often large. The purpose of this talk is to discuss how to reduces and control these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23575672','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23575672"><span><span class="hlt">Seismic</span> detection of increased degassing before Kīlauea's 2008 summit explosion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Johnson, Jessica H; Poland, Michael P</p> <p>2013-01-01</p> <p>The 2008 explosion that started a new eruption at the summit of Kīlauea Volcano, Hawai'i, was not preceded by a dramatic increase in earthquakes nor inflation, but was associated with increases in SO2 emissions and <span class="hlt">seismic</span> tremor. Here we perform shear wave splitting analysis on local earthquakes spanning the onset of the eruption. Shear wave splitting measures <span class="hlt">seismic</span> anisotropy and is traditionally used to infer changes in crustal stress over time. We show that shear wave splitting may also vary due to changes in volcanic degassing. The orientation of fast shear waves at Kīlauea is usually controlled by structure, but in 2008 showed changes with increased SO2 emissions preceding the start of the summit eruption. This <span class="hlt">interpretation</span> for changing anisotropy is supported by corresponding decreases in Vp/Vs ratio. Our result demonstrates a novel method for detecting changes in gas flux using <span class="hlt">seismic</span> observations and provides a new tool for monitoring under-instrumented volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70047755','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70047755"><span><span class="hlt">Seismic</span> detection of increased degassing before Kīlauea's 2008 summit explosion</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, Jessica H.; Poland, Michael P.</p> <p>2013-01-01</p> <p>The 2008 explosion that started a new eruption at the summit of Kīlauea Volcano, Hawai‘i, was not preceded by a dramatic increase in earthquakes nor inflation, but was associated with increases in SO2 emissions and <span class="hlt">seismic</span> tremor. Here we perform shear wave splitting analysis on local earthquakes spanning the onset of the eruption. Shear wave splitting measures <span class="hlt">seismic</span> anisotropy and is traditionally used to infer changes in crustal stress over time. We show that shear wave splitting may also vary due to changes in volcanic degassing. The orientation of fast shear waves at Kīlauea is usually controlled by structure, but in 2008 showed changes with increased SO2 emissions preceding the start of the summit eruption. This <span class="hlt">interpretation</span> for changing anisotropy is supported by corresponding decreases in Vp/Vs ratio. Our result demonstrates a novel method for detecting changes in gas flux using <span class="hlt">seismic</span> observations and provides a new tool for monitoring under-instrumented volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1047/srp/srp031/of2007-1047srp031.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1047/srp/srp031/of2007-1047srp031.pdf"><span>Unconsolidated sediments at the bottom of Lake Vostok from <span class="hlt">seismic</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>Filina, I.; Lukin, V.; Masolov, V.; Blankenship, D.</p> <p>2007-01-01</p> <p><span class="hlt">Seismic</span> soundings of Lake Vostok have been performed by the Polar Marine Geological Research Expedition in collaboration with the Russian Antarctic Expedition since the early 1990s. The seismograms recorded show at least two relatively closely spaced reflections associated with the lake bottom. These were initially <span class="hlt">interpreted</span> as boundaries of a layer of unconsolidated sediments at the bottom of the lake. A more recent <span class="hlt">interpretation</span> suggests that the observed reflections are side echoes from the rough lake bottom, and that there are no unconsolidated sediments at the bottom of the lake. The major goal of this paper is to reveal the nature of those reflections by testing three hypotheses of their origin. The results show that some of the reflections, but not all of them, are consistent with the hypothesis of a non-flat lake bottom along the source-receiver line (2D case). The reflections were also evaluated as side echoes from an adjacent sloping interface, but these tests implied unreasonably steep slopes (at least 8 degrees) at the lake bottom. The hypothesis that is the most compatible with <span class="hlt">seismic</span> data is the presence of a widespread layer of unconsolidated sediments at the bottom of Lake Vostok. The modeling suggests the presence of a two hundred meter thick sedimentary layer with a <span class="hlt">seismic</span> velocity of 1700 -1900 m/sec in the southern and middle parts of the lake. The sedimentary layer thickens in the northern basin to ~350 m</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PApGe.tmp.1302L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PApGe.tmp.1302L"><span>Simulating <span class="hlt">Seismic</span> Wave Propagation in Viscoelastic Media with an Irregular Free Surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Xiaobo; Chen, Jingyi; Zhao, Zhencong; Lan, Haiqiang; Liu, Fuping</p> <p>2018-05-01</p> <p>In <span class="hlt">seismic</span> numerical simulations of wave propagation, it is very important for us to consider surface topography and attenuation, which both have large effects (e.g., wave diffractions, conversion, amplitude/phase change) on <span class="hlt">seismic</span> imaging and inversion. An irregular free surface provides significant information for <span class="hlt">interpreting</span> the characteristics of <span class="hlt">seismic</span> wave propagation in areas with rugged or rapidly varying topography, and viscoelastic media are a better representation of the earth's properties than acoustic/elastic media. In this study, we develop an approach for <span class="hlt">seismic</span> wavefield simulation in 2D viscoelastic isotropic media with an irregular free surface. Based on the boundary-conforming grid method, the 2D time-domain second-order viscoelastic isotropic equations and irregular free surface boundary conditions are transferred from a Cartesian coordinate system to a curvilinear coordinate system. Finite difference operators with second-order accuracy are applied to discretize the viscoelastic wave equations and the irregular free surface in the curvilinear coordinate system. In addition, we select the convolutional perfectly matched layer boundary condition in order to effectively suppress artificial reflections from the edges of the model. The snapshot and seismogram results from numerical tests show that our algorithm successfully simulates <span class="hlt">seismic</span> wavefields (e.g., P-wave, Rayleigh wave and converted waves) in viscoelastic isotropic media with an irregular free surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AcGeo.tmp...42B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AcGeo.tmp...42B"><span>Influence of <span class="hlt">seismic</span> diffraction for high-resolution imaging: applications in offshore Malaysia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bashir, Yasir; Ghosh, Deva Prasad; Sum, Chow Weng</p> <p>2018-04-01</p> <p>Small-scale geological discontinuities are not easy to detect and image in <span class="hlt">seismic</span> data, as these features represent themselves as diffracted rather than reflected waves. However, the combined reflected and diffracted image contains full wave information and is of great value to an <span class="hlt">interpreter</span>, for instance enabling the identification of faults, fractures, and surfaces in built-up carbonate. Although diffraction imaging has a resolution below the typical <span class="hlt">seismic</span> wavelength, if the wavelength is much smaller than the width of the discontinuity then interference effects can be ignored, as they would not play a role in generating the <span class="hlt">seismic</span> diffractions. In this paper, by means of synthetic examples and real data, the potential of diffraction separation for high-resolution <span class="hlt">seismic</span> imaging is revealed and choosing the best method for preserving diffraction are discussed. We illustrate the accuracy of separating diffractions using the plane-wave destruction (PWD) and dip frequency filtering (DFF) techniques on data from the Sarawak Basin, a carbonate field. PWD is able to preserve the diffraction more intelligently than DFF, which is proven in the results by the model and real data. The final results illustrate the effectiveness of diffraction separation and possible imaging for high-resolution <span class="hlt">seismic</span> data of small but significant geological features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S41C2199M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S41C2199M"><span>Investigation on the characteristics of <span class="hlt">seismic</span> events observed during stimulation of geothermal reservoirs at Basel, Switzerland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mukuhira, Y.; Asanuma, H.; Niitsuma, H.; Häring, M. O.</p> <p>2011-12-01</p> <p>Hydraulic stimulation is commonly used to develop engineered geothermal systems (EGS) and enhancement of oil recovery (EOR). Occurrence of <span class="hlt">seismic</span> events with larger magnitude has been highlighted as one of the practical and critical problems. Some <span class="hlt">seismic</span> events with moment magnitude (Mw) larger than 2.0 occurred during and after hydraulic stimulation in Basel, Switzerland, in 2006, and these large events led to the geothermal project discontinued. We defined the large event as <span class="hlt">seismic</span> events with Mw>2.0, and have investigated fundamental characteristics of them as summarized in Table 1. It has been revealed that the characteristics of the large events are dependent on hypocentral location and origin time. We also found most of the large events occurred from 2 types of fracture planes: 6 of 9large events had FPSs with N-S azimuth. Other 3 large events including the largest events had FPSs ESE-WNW azimuth, which can be <span class="hlt">interpreted</span> as "most slip-able" under stress state at Basel. The large events clearly followed "constant stress drop scaling law". We also estimated critical pore pressure for shear slip using Coulomb failure criterion, and have revealed that the critical pore pressure of the large events was relatively lower. Our result shows that the occurrences of the large events can not be simply <span class="hlt">interpreted</span> by previous experience on induced <span class="hlt">seismicity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S23A4476Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S23A4476Y"><span>Progressive <span class="hlt">Seismic</span> Failure, <span class="hlt">Seismic</span> Gap, and Great <span class="hlt">Seismic</span> Risk across the Densely Populated North China Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yin, A.; Yu, X.; Shen, Z.</p> <p>2014-12-01</p> <p>Although the <span class="hlt">seismically</span> active North China basin has the most complete written records of pre-instrumentation earthquakes in the world, this information has not been fully utilized for assessing potential earthquake hazards of this densely populated region that hosts ~200 million people. In this study, we use the historical records to document the earthquake migration pattern and the existence of a 180-km <span class="hlt">seismic</span> gap along the 600-km long right-slip Tangshan-Hejian-Cixian (THC) fault zone that cuts across the North China basin. The newly recognized <span class="hlt">seismic</span> gap, which is centered at Tianjin with a population of 11 million people and ~120 km from Beijing (22 million people) and Tangshan (7 million people), has not been ruptured in the past 1000 years by M≥6 earthquakes. The <span class="hlt">seismic</span> migration pattern in the past millennium suggests that the epicenters of major earthquakes have shifted towards this <span class="hlt">seismic</span> gap along the THC fault, which implies that the 180- km gap could be the site of the next great earthquake with M≈7.6 if it is ruptured by a single event. Alternatively, the <span class="hlt">seismic</span> gap may be explained by aseismic creeping or <span class="hlt">seismic</span> strain transfer between active faults.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1983/0390/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1983/0390/report.pdf"><span>Saudi Arabian <span class="hlt">seismic</span> deep-refraction profiles; final project report</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Healy, J.H.; Mooney, W.D.; Blank, H.R.; Gettings, M.E.; Kohler, W.M.; Lamson, R.J.; Leone, L.E.</p> <p>1983-01-01</p> <p>In February 1978 a <span class="hlt">seismic</span> deep-refraction profile was recorded by the U.S. Geological Survey along a 1000-km line across the Arabian Shield in western Saudi Arabia. The line begins in Mesozoic cover rocks near Riyadh on the Arabian Platform, leads southwesterly across three major Precambrian tectonic provinces, traverses Cenozoic rocks of the coastal plain near Jizan (Tihamat-Asir), and terminates at the outer edge of the Farasan Bank in the southern Red Sea. More than 500 surveyed recording sites were occupied, including 19 in the Farasan Islands. Six shot points were used: five on land, with most charges placed below the water table in drill holes, and one at sea, with charges placed on the sea floor and detonated from a ship. Slightly more than 61 metric tons of explosives were used in 19 discrete firings. <span class="hlt">Seismic</span> energy was recorded by 100 newly-developed portable <span class="hlt">seismic</span> stations deployed in approximately 200 km-long arrays for each firing. Each station consisted of a standard 2-Hz vertical component geophone coupled to a self-contained analog recording instrument equipped with a magnetic-tape cassette. In this final report, we fully document the field and data-processing procedures and present the final seismogram data set as both a digital magnetic tape and as record sections for each shot point. Record sections include a normalized set of seismograms, reduced at 6 km/s, and a true-amplitude set, reduced at 8 km/s, which have been adjusted for amplifier gain, individual shot size, and distance from the shot point. Appendices give recorder station and shot information, digital data set descriptions, computer program listings, arrival times used in the <span class="hlt">interpretation</span>, and a bibliography of reports published as a result of this project. We used two-dimensional ray-tracing techniques in the data analysis, and our <span class="hlt">interpretation</span> is based primarily on horizontally layered models. The Arabian Shield is composed, to first-order, of two layers, each about 20 km</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH21A0159M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH21A0159M"><span>Time-Independent Annual <span class="hlt">Seismic</span> Rates, Based on Faults and Smoothed <span class="hlt">Seismicity</span>, Computed for <span class="hlt">Seismic</span> Hazard Assessment in Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murru, M.; Falcone, G.; Taroni, M.; Console, R.</p> <p>2017-12-01</p> <p>In 2015 the Italian Department of Civil Protection, started a project for upgrading the official Italian <span class="hlt">seismic</span> hazard map (MPS04) inviting the Italian scientific community to participate in a joint effort for its realization. We participated providing spatially variable time-independent (Poisson) long-term annual occurrence rates of <span class="hlt">seismic</span> events on the entire Italian territory, considering cells of 0.1°x0.1° from M4.5 up to M8.1 for magnitude bin of 0.1 units. Our final model was composed by two different models, merged in one ensemble model, each one with the same weight: the first one was realized by a smoothed <span class="hlt">seismicity</span> approach, the second one using the seismogenic faults. The spatial smoothed <span class="hlt">seismicity</span> was obtained using the smoothing method introduced by Frankel (1995) applied to the historical and instrumental <span class="hlt">seismicity</span>. In this approach we adopted a tapered Gutenberg-Richter relation with a b-value fixed to 1 and a corner magnitude estimated with the bigger events in the catalogs. For each seismogenic fault provided by the Database of the Individual Seismogenic Sources (DISS), we computed the annual rate (for each cells of 0.1°x0.1°) for magnitude bin of 0.1 units, assuming that the <span class="hlt">seismic</span> moments of the earthquakes generated by each fault are distributed according to the same tapered Gutenberg-Richter relation of the smoothed <span class="hlt">seismicity</span> model. The annual rate for the final model was determined in the following way: if the cell falls within one of the <span class="hlt">seismic</span> sources, we merge the respective value of rate determined by the <span class="hlt">seismic</span> moments of the earthquakes generated by each fault and the value of the smoothed <span class="hlt">seismicity</span> model with the same weight; if instead the cells fall outside of any <span class="hlt">seismic</span> source we considered the rate obtained from the spatial smoothed <span class="hlt">seismicity</span>. Here we present the final results of our study to be used for the new Italian <span class="hlt">seismic</span> hazard map.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2009/1251/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2009/1251/"><span>Hawaiian Volcano Observatory <span class="hlt">Seismic</span> Data, January to December 2008</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakata, Jennifer S.; Okubo, Paul G.</p> <p>2009-01-01</p> <p>The U.S. Geological Survey (USGS), Hawaiian Volcano Observatory (HVO) summary presents <span class="hlt">seismic</span> data gathered during the year. The <span class="hlt">seismic</span> summary is offered without <span class="hlt">interpretation</span> as a source of preliminary data and is complete in that most data for events of M greater than 1.5 are included. All latitude and longitude references in this report are stated in Old Hawaiian Datum. The HVO summaries have been published in various forms since 1956. Summaries prior to 1974 were issued quarterly, but cost, convenience of preparation and distribution, and the large quantities of data necessitated an annual publication, beginning with Summary 74 for the year 1974. Beginning in 2004, summaries are simply identified by the year, rather than by summary number. Summaries originally issued as administrative reports were republished in 2007 as Open-File Reports. All the summaries since 1956 are listed at http://geopubs.wr.usgs.gov/ (last accessed 09/21/2009). In January 1986, HVO adopted CUSP (California Institute of Technology USGS <span class="hlt">Seismic</span> Processing). Summary 86 includes a description of the <span class="hlt">seismic</span> instrumentation, calibration, and processing used in recent years. The present summary includes background information about the <span class="hlt">seismic</span> network to provide the end user an understanding of the processing parameters and how the data were gathered. A report by Klein and Koyanagi (1980) tabulates instrumentation, calibration, and recording history of each <span class="hlt">seismic</span> station in the network. It is designed as a reference for users of seismograms and phase data and includes and augments the information in the station table in this summary. Figures 11-14 are maps showing computer-located hypocenters. The maps were generated using the Generic Mapping Tools (GMT http://gmt.soest.hawaii.edu/, last accessed 09/21/2009) in place of traditional Qplot maps.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.8497P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.8497P"><span>Ultrasonic laboratory measurements of the <span class="hlt">seismic</span> velocity changes due to CO2 injection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, K. G.; Choi, H.; Park, Y. C.; Hwang, S.</p> <p>2009-04-01</p> <p>Monitoring the behavior and movement of carbon dioxide (CO2) in the subsurface is a quite important in sequestration of CO2 in geological formation because such information provides a basis for demonstrating the safety of CO2 sequestration. Recent several applications in many commercial and pilot scale projects and researches show that 4D surface or borehole <span class="hlt">seismic</span> methods are among the most promising techniques for this purpose. However, such information <span class="hlt">interpreted</span> from the <span class="hlt">seismic</span> velocity changes can be quite subjective and qualitative without petrophysical characterization for the effect of CO2 saturation on the <span class="hlt">seismic</span> changes since <span class="hlt">seismic</span> wave velocity depends on various factors and parameters like mineralogical composition, hydrogeological factors, in-situ conditions. In this respect, we have developed an ultrasonic laboratory measurement system and have carried out measurements for a porous sandstone sample to characterize the effects of CO2 injection to <span class="hlt">seismic</span> velocity and amplitude. Measurements are done by ultrasonic piezoelectric transducer mounted on both ends of cylindrical core sample under various pressure, temperature, and saturation conditions. According to our fundamental experiments, injected CO2 introduces the decrease of <span class="hlt">seismic</span> velocity and amplitude. We identified that the velocity decreases about 6% or more until fully saturated by CO2, but the attenuation of <span class="hlt">seismic</span> amplitude is more drastically than the velocity decrease. We also identified that Vs/Vp or elastic modulus is more sensitive to CO2 saturation. We note that this means <span class="hlt">seismic</span> amplitude and elastic modulus change can be an alternative target anomaly of <span class="hlt">seismic</span> techniques in CO2 sequestration monitoring. Thus, we expect that we can estimate more quantitative petrophysical relationships between the changes of <span class="hlt">seismic</span> attributes and CO2 concentration, which can provide basic relation for the quantitative assessment of CO2 sequestration by further researches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T13H..02K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T13H..02K"><span>Deep <span class="hlt">seismic</span> exploration into the Arctic Lithosphere: Arctic-2012 Russian wide-angle <span class="hlt">seismic</span> experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kashubin, S.</p> <p>2013-12-01</p> <p>Integrated geological and geophysical studies of the Earth's crust and upper mantle (the Russian project 'Arctic-2012') were carried out in 2012 in the Mendeleev Rise, central Arctic. The set of studies included wide-angle <span class="hlt">seismic</span> observations along the line crossing the Mendeleev Rise in its southern part. The DSS <span class="hlt">seismic</span> survey was aimed at the determination of the Mendeleev Rise crust type. A high-power air gun (120 liters or 7320 cu.in) and ocean stations with multi-component recording (X, Y, Z geophone components and a hydrophone) were used for the DSS. The line was studied using a dense system of observation: bottom station spacing was from 10 to 20 km, excitation point spacing (<span class="hlt">seismic</span> traces interval) was 315 m. Observation data were obtained in 27 location points of bottom stations, the distance between the first and the last stations was 480 km, the length of the excitation line was 740 km. In DSS wave fields, in the first and later arrivals, there are refracted and reflected waves associated with boundaries in the sedimentary cover, with the top of the basement, and with boundaries in the consolidated crust, including its bottom (Moho discontinuity). The waves could be traced for offsets up to 170-240 km. The DSS line coincides with the near-vertical CMP line worked out with the use of a 4500-m-long <span class="hlt">seismic</span> streamer and with a 50 m shot point interval that allowed essential detalization of the upper part of the section and taking it into account in the construction of a deep crust model. The deep velocity model was constructed using ray-trace modeling of compressional, shear, and converted waves with the use of the SeisWide program. Estimates were obtained for Vp/Vs velocity ratios, which played an important role in determining the type of crust. The results of the <span class="hlt">interpretation</span> show that the Mendeleev Rise section corresponds to sections of a thin continental crust of shelf seas and a thinned continental crust of submarine ridges and rises.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026758','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026758"><span><span class="hlt">Interpretation</span> of the Seattle uplift, Washington, as a passive-roof duplex</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, T.M.; Blakely, R.J.; Wells, R.E.</p> <p>2004-01-01</p> <p>We <span class="hlt">interpret</span> <span class="hlt">seismic</span> lines and a wide variety of other geological and geophysical data to suggest that the Seattle uplift is a passive-roof duplex. A passive-roof duplex is bounded top and bottom by thrust faults with opposite senses of vergence that form a triangle zone at the leading edge of the advancing thrust sheet. In passive-roof duplexes the roof thrust slips only when the floor thrust ruptures. The Seattle fault is a south-dipping reverse fault forming the leading edge of the Seattle uplift, a 40-km-wide fold-and-thrust belt. The recently discovered, north-dipping Tacoma reverse fault is <span class="hlt">interpreted</span> as a back thrust on the trailing edge of the belt, making the belt doubly vergent. Floor thrusts in the Seattle and Tacoma fault zones, imaged as discontinuous reflections, are <span class="hlt">interpreted</span> as blind faults that flatten updip into bedding plane thrusts. Shallow monoclines in both the Seattle and Tacoma basins are <span class="hlt">interpreted</span> to overlie the leading edges of thrust-bounded wedge tips advancing into the basins. Across the Seattle uplift, <span class="hlt">seismic</span> lines image several shallow, short-wavelength folds exhibiting Quaternary or late Quaternary growth. From reflector truncation, several north-dipping thrust faults (splay thrusts) are inferred to core these shallow folds and to splay upward from a shallow roof thrust. Some of these shallow splay thrusts ruptured to the surface in the late Holocene. Ages from offset soils in trenches across the fault scarps and from abruptly raised shorelines indicate that the splay, roof, and floor thrusts of the Seattle and Tacoma faults ruptured about 1100 years ago.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tecto..36.3192D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tecto..36.3192D"><span><span class="hlt">Seismic</span> Signature of the Continental Crust: What Thermodynamics Says. An Example From the Italian Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Diaferia, G.; Cammarano, F.</p> <p>2017-12-01</p> <p>Unraveling the temperature distribution and composition of Earth's crust is key for understanding its origin, evolution, and mechanical behavior. Models of compressional (<fi>V</fi><fi>P</fi>) and shear wave (<fi>V</fi><fi>S</fi>) velocity are obtained from seismological studies and can be <span class="hlt">interpreted</span> in terms of temperature and composition, using relationship defined through laboratory experiments. These empirical evidences often do not properly account for the effects driven by temperature, pressure, water content, and phase change of minerals. In this study, we use thermodynamic modeling to properly investigate the role of these variables in affecting <span class="hlt">seismic</span> properties, as a tool to guide (joint) inversion and <span class="hlt">interpretation</span> of geophysical data. We find that mineralogical phase transitions can be more <span class="hlt">seismically</span> relevant than a change in chemical composition. In particular, the α-β quartz transition would cause a jump in acoustic impedance and <fi>V</fi><fi>P</fi>/<fi>V</fi><fi>S</fi> ratio >8%, occurring in the 15-25 km depth range, depending on the thermal gradient. Moreover, in the case of a cold lower crust, the consumption of plagioclase in favor of high-velocity minerals might represent another relevant <span class="hlt">seismic</span> discontinuity. Different chemical compositions proposed for the Italian crust would be <span class="hlt">seismically</span> indistinguishable, since they give overlapping <span class="hlt">seismic</span> properties. Values of <fi>V</fi><fi>S</fi> < 3.6 km s-1 would imply a strong contribution of sediments and/or partial melt. The <fi>V</fi><fi>S</fi>/density ratio shows a narrow variability, suggesting that densities at depth can be directly derived in first approximation from <fi>V</fi><fi>S</fi>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3316L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3316L"><span>Map of Pseudo-F-statistics of <span class="hlt">seismic</span> noise parameters as an indicator of current <span class="hlt">seismic</span> danger in Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lyubushin, Alexey</p> <p>2016-04-01</p> <p>The problem of estimate of current <span class="hlt">seismic</span> danger based on monitoring of <span class="hlt">seismic</span> noise properties from broadband <span class="hlt">seismic</span> network F-net in Japan (84 stations) is considered. Variations of the following <span class="hlt">seismic</span> noise parameters are analyzed: multifractal singularity spectrum support width, generalized Hurst exponent, minimum Hölder-Lipschitz exponent and minimum normalized entropy of squared orthogonal wavelet coefficients. These parameters are estimated within adjacent time windows of the length 1 day for <span class="hlt">seismic</span> noise waveforms from each station. Calculating daily median values of these parameters by all stations provides 4-dimensional time series which describes integral properties of the <span class="hlt">seismic</span> noise in the region covered by the network. Cluster analysis is applied to the sequence of clouds of 4-dimensional vectors within moving time window of the length 365 days with mutual shift 3 days starting from the beginning of 1997 up to the current time. The purpose of the cluster analysis is to find the best number of clusters (BNC) from probe numbers which are varying from 1 up to the maximum value 40. The BNC is found from the maximum of pseudo-F-statistics (PFS). A 2D map could be created which presents dependence of PFS on the tested probe number of clusters and the right-hand end of moving time window which is rather similar to usual spectral time-frequency diagrams. In the paper [1] it was shown that the BNC before Tohoku mega-earthquake on March 11, 2011, has strongly chaotic regime with jumps from minimum up to maximum values in the time interval 1 year before the event and this time intervals was characterized by high PFS values. The PFS-map is proposed as the method for extracting time intervals with high current <span class="hlt">seismic</span> danger. The next danger time interval after Tohoku mega-EQ began at the end of 2012 and was finished at the middle of 2013. Starting from middle of 2015 the high PFS values and chaotic regime of BNC variations were returned. This could be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1712654R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1712654R"><span>The Pollino <span class="hlt">Seismic</span> Sequence: Activated Graben Structures in a <span class="hlt">Seismic</span> Gap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rößler, Dirk; Passarelli, Luigi; Govoni, Aladino; Bindi, Dino; Cesca, Simone; Hainzl, Sebatian; Maccaferri, Francesco; Rivalta, Eleonora; Woith, Heiko; Dahm, Torsten</p> <p>2015-04-01</p> <p>The Mercure Basin (MB) and the Castrovillari Fault (CF) in the Pollino range (Southern Apennines, Italy) represent one of the most prominent <span class="hlt">seismic</span> gaps in the Italian <span class="hlt">seismic</span> catalogue, with no M>5.5 earthquakes during the last centuries. In historical times several swarm-like <span class="hlt">seismic</span> sequences occurred in the area including two intense swarms within the past two decades. The most energetic one started in 2010 and has been still active in 2014. The <span class="hlt">seismicity</span> culminated in autumn 2012 with a M=5 event on 25 October. The range hosts a number of opposing normal faults forming a graben-like structure. Their rheology and their interactions are unclear. Current debates include the potential of the MB and the CF to host large earthquakes and the style of deformation. Understanding the <span class="hlt">seismicity</span> and the behaviour of the faults is necessary to assess the tectonics and the <span class="hlt">seismic</span> hazard. The GFZ German Research Centre for Geosciences and INGV, Italy, have jointly monitored the ongoing <span class="hlt">seismicity</span> using a small-aperture <span class="hlt">seismic</span> array, integrated in a temporary <span class="hlt">seismic</span> network. Based on this installation, we located more than 16,000 local earthquakes that occurred between November 2012 and September 2014. Here we investigate quantitatively all the phases of the <span class="hlt">seismic</span> sequence starting from January 2010. Event locations along with moment tensor inversion constrain spatially the structures activated by the swarm and the migration pattern of the <span class="hlt">seismicity</span>. The <span class="hlt">seismicity</span> forms clusters concentrated within the southern part of the MB and along the Pollino Fault linking MB and CF. Most earthquakes are confined to the upper 10 km of the crust in an area of ~15x15 km2. However, sparse <span class="hlt">seismicity</span> at depths between 15 and 20 km and moderate <span class="hlt">seismicity</span> further north with deepening hypocenters also exist. In contrast, the CF appears aseismic; only the northern part has experienced micro-<span class="hlt">seismicity</span>. The spatial distribution is however more complex than the major tectonic structures</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2008/1197/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2008/1197/"><span>Structure of the San Bernardino Basin Along Two <span class="hlt">Seismic</span> Transects: Rialto-Colton Fault to the San Andreas Fault and Along the I-215 Freeway (I-10 to SR30)</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.; Steedman, C.E.</p> <p>2008-01-01</p> <p>In this report, we present <span class="hlt">seismic</span> data and acquisition parameters for two <span class="hlt">seismic</span> profiles acquired in the San Bernardino, California area in May and October 2003. We refer to these <span class="hlt">seismic</span> profiles as the San Bernardino Regional (SBR) and San Bernardino High-Resolution (SBHR) <span class="hlt">seismic</span> profiles. We present both un-<span class="hlt">interpreted</span> and <span class="hlt">interpreted</span> <span class="hlt">seismic</span> images so that the structure of the area can independently <span class="hlt">interpreted</span> by others. We explain the rationale for our <span class="hlt">interpretations</span> within the text of this report, and in addition, we provide a large body of supporting evidence. The SBR <span class="hlt">seismic</span> profile extended across the San Bernardino Basin approximately N30?E from the town of Colton to the town of Highland. The data were acquired at night when the signal-to-noise ratios were reasonably good, and for the larger shots, <span class="hlt">seismic</span> energy propagated across the ~20-km-long array. Tomographic velocity data are available to depths of about 4 km, and low-fold reflection data are available to depths in excess of 5 km. The SBR <span class="hlt">seismic</span> data reveal an asymmetric, fault-bound basin to about 5 km depth. The SBHR <span class="hlt">seismic</span> profile trended along the I-215 freeway from its intersection with the Santa Ana River to approximately State Road 30 in San Bernardino. <span class="hlt">Seismic</span> data acquired along the I-215 freeway provide detailed images, with CDP spacing of approximately 2.5 m along an approximately 8.2-km-long profile; shot and geophone spacing was 5 m. For logistical reasons, the high-resolution (SBHR) <span class="hlt">seismic</span> data were acquired during daylight hours on the shoulder of the I-215 freeway and within 5 to 10 m of high-traffic volumes, resulting in low signal-to-noise ratios. The limited offset at which refracted first-arrivals could be measured along the SBHR <span class="hlt">seismic</span> profile limited our measurements of tomographic refraction velocities to relatively shallow (< 150 m) depths. The SBHR reflection data reveal a basin with complex structural details within the upper kilometer. The two <span class="hlt">seismic</span> profiles</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('http://adsabs.harvard.edu/abs/2017AGUFM.S13B0667M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S13B0667M"><span>Analysis of Deep Long-Period Subglacial <span class="hlt">Seismicity</span> in Marie Byrd Land, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McMahon, N. D.; Aster, R. C.; Myers, E. K.; Lough, A. C.</p> <p>2017-12-01</p> <p>We utilize subspace detection methodology to extend the detection and analysis of deep, long-period <span class="hlt">seismic</span> activity associated with the subglacial and lower crust magmatic complex beneath the Executive Committee Range volcanoes of Marie Byrd Land (Lough et al., 2013). The Marie Byrd Land (MBL) volcanic province is a remote continental region that is almost completely covered by the West Antarctic Ice Sheet (WAIS). The southern extent of Marie Byrd Land lies within the West Antarctic Rift System (WARS), which includes the volcanic Executive Committee Range. Lough et al. noted that <span class="hlt">seismic</span> stations in the POLENET/ANET <span class="hlt">seismic</span> network detected two swarms of <span class="hlt">seismic</span> activity during 2010 and 2011. These events have been <span class="hlt">interpreted</span> as deep, long-period (DLP) earthquakes based on their depth (25-40 km), tectonic context, and low frequency spectra. The DLP events in MBL lie beneath an inferred volcanic edifice that is visible in ice penetrating radar images via subglacial topography and intraglacial ash deposits, and have been <span class="hlt">interpreted</span> as a present location of Moho-proximal magmatic activity. The magmatic swarm activity in MBL provides a promising target for advanced subspace detection, and for the temporal, spatial, and event size analysis of an extensive deep long period earthquake swarm using a remote and sparse seismographic network. We utilized a catalog of 1370 traditionally identified DLP events to construct subspace detectors for the nine nearest stations using two years of data spanning 2010-2011. Via subspace detection we increase the number of observable detections more than 70 times at the highest signal to noise station while decreasing the overall minimum magnitude of completeness. In addition to the two previously identified swarms during early 2010 and early 2011, we find sustained activity throughout the two years of study that includes several previously unidentified periods of heightened activity. These events have a very high Gutenberg-Richter b</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S23F..07H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S23F..07H"><span>Constitutive law for <span class="hlt">seismicity</span> rate based on rate and state friction: Dieterich 1994 revisited.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heimisson, E. R.; Segall, P.</p> <p>2017-12-01</p> <p>Dieterich [1994] derived a constitutive law for <span class="hlt">seismicity</span> rate based on rate and state friction, which has been applied widely to aftershocks, earthquake triggering, and induced <span class="hlt">seismicity</span> in various geological settings. Here, this influential work is revisited, and re-derived in a more straightforward manner. By virtue of this new derivation the model is generalized to include changes in effective normal stress associated with background <span class="hlt">seismicity</span>. Furthermore, the general case when <span class="hlt">seismicity</span> rate is not constant under constant stressing rate is formulated. The new derivation provides directly practical integral expressions for the cumulative number of events and rate of <span class="hlt">seismicity</span> for arbitrary stressing history. Arguably, the most prominent limitation of Dieterich's 1994 theory is the assumption that <span class="hlt">seismic</span> sources do not interact. Here we derive a constitutive relationship that considers source interactions between sub-volumes of the crust, where the stress in each sub-volume is assumed constant. Interactions are considered both under constant stressing rate conditions and for arbitrary stressing history. This theory can be used to model <span class="hlt">seismicity</span> rate due to stress changes or to estimate stress changes using observed <span class="hlt">seismicity</span> from triggered earthquake swarms where earthquake interactions and magnitudes are take into account. We identify special conditions under which influence of interactions cancel and the predictions reduces to those of Dieterich 1994. This remarkable result may explain the apparent success of the model when applied to observations of triggered <span class="hlt">seismicity</span>. This approach has application to understanding and modeling induced and triggered <span class="hlt">seismicity</span>, and the quantitative <span class="hlt">interpretation</span> of geodetic and <span class="hlt">seismic</span> data. It enables simultaneous modeling of geodetic and <span class="hlt">seismic</span> data in a self-consistent framework. To date physics-based modeling of <span class="hlt">seismicity</span> with or without geodetic data has been found to give insight into various processes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRA..12010754B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRA..12010754B"><span>Toward the azimuthal characteristics of ionospheric and <span class="hlt">seismic</span> effects of "Chelyabinsk" meteorite fall according to the data from coherent radar, GPS, and <span class="hlt">seismic</span> networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Berngardt, O. I.; Perevalova, N. P.; Dobrynina, A. A.; Kutelev, K. A.; Shestakov, N. V.; Bakhtiarov, V. F.; Kusonsky, O. A.; Zagretdinov, R. V.; Zherebtsov, G. A.</p> <p>2015-12-01</p> <p>We present the results of a study of the azimuthal characteristics of ionospheric and <span class="hlt">seismic</span> effects of the meteorite `Chelyabinsk,' based on the data from the network of GPS receivers, coherent decameter radar EKB, and network of <span class="hlt">seismic</span> stations, located near the meteorite fall trajectory. It is shown that 6-14 min after the bolide explosion, GPS network observed the cone-shaped wavefront of traveling ionospheric disturbances (TIDs) that is <span class="hlt">interpreted</span> as a ballistic acoustic wave. The typical TIDs propagation velocity were observed 661 ± 256 m/s, which corresponds to the expected acoustic wave speed for 240 km height. Fourteen minutes after the bolide explosion, at distances of 200 km, we observed the emergence and propagation of a TID with annular wavefront that is <span class="hlt">interpreted</span> as gravitational mode of internal atmospheric waves. The propagation velocity of this TID was 337 ± 89 m/s which corresponds to the propagation velocity of these waves in similar situations. At EKB radar, we observed TIDs in the sector of azimuthal angles close to the perpendicular to the meteorite trajectory. The observed TID velocity (400 m/s) and azimuthal properties correlate well with the model of ballistic wave propagating at 120-140 km altitude. It is shown that the azimuthal distribution of the amplitude of vertical <span class="hlt">seismic</span> oscillations with periods 3-60 s can be described qualitatively by the model of vertical strike-slip rupture, propagating at 1 km/s along the meteorite fall trajectory to distance of about 40 km. These parameters correspond to the direction and velocity of propagation of the ballistic wave peak by the ground. It is shown that the model of ballistic wave caused by supersonic motion and burning of the meteorite in the upper atmosphere can satisfactorily explain the various azimuthal ionospheric effects, observed by the coherent decameter radar EKB, GPS receivers network, and the azimuthal characteristics of <span class="hlt">seismic</span> waves at large distances.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033543','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033543"><span>Anatomy of the Chesapeake Bay impact structure revealed by <span class="hlt">seismic</span> imaging, Delmarva Peninsula, Virginia, 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>Catchings, R.D.; Powars, D.S.; Gohn, G.S.; Horton, J. Wright; Goldman, M.R.; Hole, J.A.</p> <p>2008-01-01</p> <p>A 30-km-long, radial <span class="hlt">seismic</span> reflection and refraction survey completed across the northern part of the late Eocene Chesapeake Bay impact structure (CBIS) on the Delmarva Peninsula, Virginia, USA, confirms that the CBIS is a complex central-peak crater. We used a tomographic P wave velocity model and low-fold reflection images, constrained by data from two deep boreholes located on the profile, to <span class="hlt">interpret</span> the structure and composition of the upper 5 km of crust. The <span class="hlt">seismic</span> images exhibit well-defined structural features, including (with increasing radial distance) a collapsed central uplift, a breccia-filled moat, and a collapsed transient-crater margin (which collectively constitute a ???40-km-wide collapsed transient crater), and a shallowly deformed annular trough. These <span class="hlt">seismic</span> images are the first to resolve the deep structure of the crater (>1 km) and the boundaries between the central uplift, moat, and annular trough. Several distinct <span class="hlt">seismic</span> signatures distinguish breccia units from each other and from more coherent crystalline rocks below the central uplift, moat, and annular trough. Within the moat, breccia extends to a minimum depth of 1.5 km or a maximum of 3.5 km, depending upon the <span class="hlt">interpretation</span> of the deepest layered materials. The images show ???350 to 500 m of postimpact sediments above the impactites. The imaged structure of the CBIS indicates a complex sequence of event during the cratering process that will provide new constraints for numerical modeling. Copyright 2008 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.S21A1684L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.S21A1684L"><span>Controlled Source 4D <span class="hlt">Seismic</span> Imaging</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Y.; Morency, C.; Tromp, J.</p> <p>2009-12-01</p> <p>Earth's material properties may change after significant tectonic events, e.g., volcanic eruptions, earthquake ruptures, landslides, and hydrocarbon migration. While many studies focus on how to <span class="hlt">interpret</span> observations in terms of changes in wavespeeds and attenuation, the oil industry is more interested in how we can identify and locate such temporal changes using <span class="hlt">seismic</span> waves generated by controlled sources. 4D <span class="hlt">seismic</span> analysis is indeed an important tool to monitor fluid movement in hydrocarbon reservoirs during production, improving fields management. Classic 4D <span class="hlt">seismic</span> imaging involves comparing images obtained from two subsequent <span class="hlt">seismic</span> surveys. Differences between the two images tell us where temporal changes occurred. However, when the temporal changes are small, it may be quite hard to reliably identify and characterize the differences between the two images. We propose to back-project residual seismograms between two subsequent surveys using adjoint methods, which results in images highlighting temporal changes. We use the SEG/EAGE salt dome model to illustrate our approach. In two subsequent surveys, the wavespeeds and density within a target region are changed, mimicking possible fluid migration. Due to changes in material properties induced by fluid migration, seismograms recorded in the two surveys differ. By back propagating these residuals, the adjoint images identify the location of the affected region. An important issue involves the nature of model. For instance, are we characterizing only changes in wavespeed, or do we also consider density and attenuation? How many model parameters characterize the model, e.g., is our model isotropic or anisotropic? Is acoustic wave propagation accurate enough or do we need to consider elastic or poroelastic effects? We will investigate how imaging strategies based upon acoustic, elastic and poroelastic simulations affect our imaging capabilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S13D4490N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S13D4490N"><span>Angola <span class="hlt">Seismicity</span> MAP</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neto, F. A. P.; Franca, G.</p> <p>2014-12-01</p> <p>The purpose of this job was to study and document the Angola natural <span class="hlt">seismicity</span>, establishment of the first database <span class="hlt">seismic</span> data to facilitate consultation and search for information on <span class="hlt">seismic</span> activity in the country. The study was conducted based on query reports produced by National Institute of Meteorology and Geophysics (INAMET) 1968 to 2014 with emphasis to the work presented by Moreira (1968), that defined six seismogenic zones from macro <span class="hlt">seismic</span> data, with highlighting is Zone of Sá da Bandeira (Lubango)-Chibemba-Oncócua-Iona. This is the most important of Angola <span class="hlt">seismic</span> zone, covering the epicentral Quihita and Iona regions, geologically characterized by transcontinental structure tectono-magmatic activation of the Mesozoic with the installation of a wide variety of intrusive rocks of ultrabasic-alkaline composition, basic and alkaline, kimberlites and carbonatites, strongly marked by intense tectonism, presenting with several faults and fractures (locally called corredor de Lucapa). The earthquake of May 9, 1948 reached intensity VI on the Mercalli-Sieberg scale (MCS) in the locality of Quihita, and <span class="hlt">seismic</span> active of Iona January 15, 1964, the main shock hit the grade VI-VII. Although not having significant <span class="hlt">seismicity</span> rate can not be neglected, the other five zone are: Cassongue-Ganda-Massano de Amorim; Lola-Quilengues-Caluquembe; Gago Coutinho-zone; Cuima-Cachingues-Cambândua; The Upper Zambezi zone. We also analyzed technical reports on the <span class="hlt">seismicity</span> of the middle Kwanza produced by Hidroproekt (GAMEK) region as well as international <span class="hlt">seismic</span> bulletins of the International Seismological Centre (ISC), United States Geological Survey (USGS), and these data served for instrumental location of the epicenters. All compiled information made possible the creation of the First datbase of <span class="hlt">seismic</span> data for Angola, preparing the map of <span class="hlt">seismicity</span> with the reconfirmation of the main <span class="hlt">seismic</span> zones defined by Moreira (1968) and the identification of a new <span class="hlt">seismic</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MsT..........3A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MsT..........3A"><span>3D Modeling and Characterization of Hydraulic Fracture Efficiency Integrated with 4D/9C Time-Lapse <span class="hlt">Seismic</span> <span class="hlt">Interpretations</span> in the Niobrara Formation, Wattenberg Field, Denver Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alfataierge, Ahmed</p> <p></p> <p> production), the variability in production performance within the Niobrara Shale wells is shown to significantly be affected by the lateral variability in reservoir quality, well and stage positioning relative to the target interval, and the relative completion efficiency. The variation in reservoir properties, faults, rock strength parameters, and in-situ stress conditions are shown to influence and control the hydraulic fracturing geometry and stimulation efficiency resulting in complex and isolated induced fracture geometries to form within the reservoir. This consequently impacts the effective drainage areas, production performance and recovery rates from inefficiently stimulated horizontal wells. The 3D simulation results coupled with the 4D <span class="hlt">seismic</span> <span class="hlt">interpretations</span> illustrate that there is still room for improvement to be made in optimizing well spacing and hydraulic fracturing efficiency within the Niobrara Formation. Integrated analysis show that the Niobrara reservoir is not uniformly stimulated. The vertical and lateral variability in rock properties control the hydraulic fracturing efficiency and geometry. Better production is also correlated to higher fracture conductivity. 4D <span class="hlt">seismic</span> <span class="hlt">interpretation</span> is also shown to be essential for the validation and calibration hydraulic fracture simulation models. The hydraulic fracture modeling also demonstrations that there is bypassed pay in the Niobrara B chalk resulting from initial Niobrara C chalk stimulation treatments. Forward modeling also shows that low pressure intervals within the Niobrara reservoir influence hydraulic fracturing and infill drilling during field development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JVGR...84..311B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JVGR...84..311B"><span><span class="hlt">Seismic</span> study of the Mesozoic carbonate basement around Mt. Somma Vesuvius, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bruno, Pier Paolo G.; Cippitelli, Giuseppe; Rapolla, Antonio</p> <p>1998-09-01</p> <p>Fifteen <span class="hlt">seismic</span> reflection lines from AGIP surveys, in and around the Campanian Plain and Mt. Somma-Vesuvius (south Italy) have been <span class="hlt">interpreted</span>. The attention has been focused to the horizon pertinent to the top of the Mesozoic carbonate sequence and the Quaternary faults dissecting it. As a matter of fact, both are very important elements for understanding the origin of the volcanic activity in the area, that often in the past, has been the topic of debates not supported by reliable data. In the study area, referring to the depth of the carbonate basement, comparison between the result achieved by the <span class="hlt">seismic</span> prospecting and previous gravity studies has been made. It shows coherence in some areas but large discrepancy within others. Near the town of S. Anastasia, the gravity and <span class="hlt">seismic</span> depth estimates differ as much as 1000 m or more. Furthermore, the <span class="hlt">seismic</span> data show that the source of the greatest volcanic eruption in the area (the so-called `Campanian Ignimbrite') is probably not located in the Acerra depression, as suggested by other authors. A main NE-SW fault directed toward Vesuvius, considered as playing a primary role on volcanogenetic processes and previously recognised only offshore by marine <span class="hlt">seismic</span> survey, has been now identified also inland using this new <span class="hlt">seismic</span> information. The results presented here strengthen the hypothesis that Mt. Vesuvius is located at the crossing point of two regional Quaternary sets of fault heading NW-SE and NE-SW.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.G33A0621C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.G33A0621C"><span><span class="hlt">Seismicity</span> and strain transients in the Gulf of Corinth (Greece)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Canitano, A.; Bernard, P.; Linde, A. T.; Sacks, S. I.; Boudin, F.</p> <p>2009-12-01</p> <p> 1/10 of a period for 10-40 hrs period range). This analysis allows us to estimate a transfert function for each forcing signal but the physical <span class="hlt">interpretation</span> of the sea-level function is still unclear. As the strainmeter is at 150m depth, below the shoreline, a sea water percolation on land would increase the effect of sea level fluctuation, and be more efficient at longer periods. This <span class="hlt">interpretation</span> allow us to study accurately this external perturbations and to remove them from the strain signal. The residual signal is 8 times smaller than the original strain signal for 10mn-1hr period (RMS=0,27.10-9 strain and no sea-level signal delay) and 4 times for 30-40hr (RMS=0,63.10-9 strain). This residual signals are studied in order to find slow transient signatures, especially during the reported <span class="hlt">seismic</span> swarms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011E%26PSL.307..147M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011E%26PSL.307..147M"><span>Revealing the deep structure and rupture plane of the 2010 Maule, Chile earthquake (Mw = 8.8) using wide angle <span class="hlt">seismic</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>Moscoso, Eduardo; Grevemeyer, Ingo; Contreras-Reyes, Eduardo; Flueh, Ernst R.; Dzierma, Yvonne; Rabbel, Wolfgang; Thorwart, Martin</p> <p>2011-07-01</p> <p>The 27 February, 2010 Maule earthquake (Mw = 8.8) ruptured ~ 400 km of the Nazca-South America plate boundary and caused hundreds of fatalities and billions of dollars in material losses. Here we present constraints on the fore-arc structure and subduction zone of the rupture area derived from <span class="hlt">seismic</span> refraction and wide-angle data. The results show a wedge shaped body ~ 40 km wide with typical sedimentary velocities <span class="hlt">interpreted</span> as a frontal accretionary prism (FAP). Landward of the imaged FAP, the velocity model shows an abrupt velocity-contrast, suggesting a lithological change which is <span class="hlt">interpreted</span> as the contact between the FAP and the paleo accretionary prism (backstop). The backstop location is coincident with the seaward limit of the aftershocks, defining the updip limit of the co-<span class="hlt">seismic</span> rupture and seismogenic zone. Furthermore, the seaward limit of the aftershocks coincides with the location of the shelf break in the entire earthquake rupture area (33°S-38.5°S), which is <span class="hlt">interpreted</span> as the location of the backstop along the margin. Published <span class="hlt">seismic</span> profiles at the northern and southern limit of the rupture area also show the presence of a strong horizontal velocity gradient <span class="hlt">seismic</span> backstop at a distance of ~ 30 km from the deformation front. The <span class="hlt">seismic</span> wide-angle reflections from the top of the subducting oceanic crust constrain the location of the plate boundary offshore, dipping at ~ 10°. The projection of the epicenter of the Maule earthquake onto our derived interplate boundary yielded a hypocenter around 20 km depth, this implies that this earthquake nucleated somewhere in the middle of the seismogenic zone, neither at its updip nor at its downdip limit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S51A2320F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S51A2320F"><span><span class="hlt">Seismic</span> Noise Analysis and Reduction through Utilization of Collocated <span class="hlt">Seismic</span> and Atmospheric Sensors at the GRO Chile <span class="hlt">Seismic</span> Network</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farrell, M. E.; Russo, R. M.</p> <p>2013-12-01</p> <p>The installation of Earthscope Transportable Array-style geophysical observatories in Chile expands open data <span class="hlt">seismic</span> recording capabilities in the southern hemisphere by nearly 30%, and has nearly tripled the number of <span class="hlt">seismic</span> stations providing freely-available data in southern South America. Through the use of collocated <span class="hlt">seismic</span> and atmospheric sensors at these stations we are able to analyze how local atmospheric conditions generate <span class="hlt">seismic</span> noise, which can degrade data in <span class="hlt">seismic</span> frequency bands at stations in the ';roaring forties' (S latitudes). <span class="hlt">Seismic</span> vaults that are climate-controlled and insulated from the local environment are now employed throughout the world in an attempt to isolate seismometers from as many noise sources as possible. However, this is an expensive solution that is neither practical nor possible for all <span class="hlt">seismic</span> deployments; and also, the increasing number and scope of temporary <span class="hlt">seismic</span> deployments has resulted in the collection and archiving of terabytes of <span class="hlt">seismic</span> data that is affected to some degree by natural <span class="hlt">seismic</span> noise sources such as wind and atmospheric pressure changes. Changing air pressure can result in a depression and subsequent rebound of Earth's surface - which generates low frequency noise in <span class="hlt">seismic</span> frequency bands - and even moderate winds can apply enough force to ground-coupled structures or to the surface above the seismometers themselves, resulting in significant noise. The 10 stations of the permanent Geophysical Reporting Observatories (GRO Chile), jointly installed during 2011-12 by IRIS and the Chilean Servicio Sismológico, include instrumentation in addition to the standard three <span class="hlt">seismic</span> components. These stations, spaced approximately 300 km apart along the length of the country, continuously record a variety of atmospheric data including infrasound, air pressure, wind speed, and wind direction. The collocated <span class="hlt">seismic</span> and atmospheric sensors at each station allow us to analyze both datasets together, to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1615502V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1615502V"><span>Non-stationary background intensity and Caribbean <span class="hlt">seismic</span> events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Valmy, Larissa; Vaillant, Jean</p> <p>2014-05-01</p> <p>We consider <span class="hlt">seismic</span> risk calculation based on models with non-stationary background intensity. The aim is to improve predictive strategies in the framework of <span class="hlt">seismic</span> risk assessment from models describing at best the <span class="hlt">seismic</span> activity in the Caribbean arc. Appropriate statistical methods are required for analyzing the volumes of data collected. The focus is on calculating earthquakes occurrences probability and analyzing spatiotemporal evolution of these probabilities. The main modeling tool is the point process theory in order to take into account past history prior to a given date. Thus, the <span class="hlt">seismic</span> event conditional intensity is expressed by means of the background intensity and the self exciting component. This intensity can be <span class="hlt">interpreted</span> as the expected event rate per time and / or surface unit. The most popular intensity model in seismology is the ETAS (Epidemic Type Aftershock Sequence) model introduced and then generalized by Ogata [2, 3]. We extended this model and performed a comparison of different probability density functions for the triggered event times [4]. We illustrate our model by considering the CDSA (Centre de Données Sismiques des Antilles) catalog [1] which contains more than 7000 <span class="hlt">seismic</span> events occurred in the Lesser Antilles arc. Statistical tools for testing the background intensity stationarity and for dynamical segmentation are presented. [1] Bengoubou-Valérius M., Bazin S., Bertil D., Beauducel F. and Bosson A. (2008). CDSA: a new seismological data center for the French Lesser Antilles, Seismol. Res. Lett., 79 (1), 90-102. [2] Ogata Y. (1998). Space-time point-process models for earthquake occurrences, Annals of the Institute of Statistical Mathematics, 50 (2), 379-402. [3] Ogata, Y. (2011). Significant improvements of the space-time ETAS model for forecasting of accurate baseline <span class="hlt">seismicity</span>, Earth, Planets and Space, 63 (3), 217-229. [4] Valmy L. and Vaillant J. (2013). Statistical models in seismology: Lesser Antilles arc case</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..596Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..596Z"><span>Building an educational <span class="hlt">seismic</span> network in Romanian schools</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zaharia, Bogdan; Tataru, Dragos; Grecu, Bogdan; Ionescu, Constantin; Bican-Brisan, Nicoleta; Neagoe, Cristian</p> <p>2014-05-01</p> <p>Understanding the earthquake phenomena and their effects is an important step toward the education of population and aims to raise the awareness about the earthquake risk and possible mitigation actions. In this sense, The Romanian Educational <span class="hlt">Seismic</span> Network project represents an efficient communication tool, allowing teaching and learning about the earthquakes and <span class="hlt">seismic</span> wave impact through experimental practices and educational activities. The <span class="hlt">seismic</span> network consist of nine SEP seismometers installed in high-schools from the most important <span class="hlt">seismic</span> areas (Vrancea, Banat, Făgăraş, Dobrogea), vulnerable cities (Bucharest, Iasi) or high populated places (Cluj, Sibiu, Timisoara, Zalău) and is coordinated by the National Institute of Earth Physics from Bucharest. Once installed, the <span class="hlt">seismic</span> network is the starting point of activities for students through an e-learning platform. Some objectives are aimed: - To train students and teachers how to make analysis and <span class="hlt">interpretation</span> of seismological data; - To make science more interesting for students; - To improve the participation rates in physical sciences for students; - To raise awareness of geoscience as a scientific discipline for pre-university students; - To promote the installation and effective use of educational seismographs and <span class="hlt">seismic</span> data; - To reinforce and develop relationships between participating schools and research institutes; - To create an earthquake database this will be used by students and teachers for educational purposes. Different types of practical activities using educational seismometer, designed by researchers for students, are described in educational materials and in the web platform project. Also we encourage the teachers from the participating schools to share their experiences and produce new didactic tools for the classroom. This collaborative work could illustrate the conjugated efforts of researchers and teachers for a better education and awareness of the risk culture</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMED43C0875C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMED43C0875C"><span>Interactive Visualizations of Complex <span class="hlt">Seismic</span> Data and Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chai, C.; Ammon, C. J.; Maceira, M.; Herrmann, R. B.</p> <p>2016-12-01</p> <p>The volume and complexity of <span class="hlt">seismic</span> data and models have increased dramatically thanks to dense <span class="hlt">seismic</span> station deployments and advances in data modeling and processing. <span class="hlt">Seismic</span> observations such as receiver functions and surface-wave dispersion are multidimensional: latitude, longitude, time, amplitude and latitude, longitude, period, and velocity. Three-dimensional <span class="hlt">seismic</span> velocity models are characterized with three spatial dimensions and one additional dimension for the speed. In these circumstances, exploring the data and models and assessing the data fits is a challenge. A few professional packages are available to visualize these complex data and models. However, most of these packages rely on expensive commercial software or require a substantial time investment to master, and even when that effort is complete, communicating the results to others remains a problem. A traditional approach during the model <span class="hlt">interpretation</span> stage is to examine data fits and model features using a large number of static displays. Publications include a few key slices or cross-sections of these high-dimensional data, but this prevents others from directly exploring the model and corresponding data fits. In this presentation, we share interactive visualization examples of complex <span class="hlt">seismic</span> data and models that are based on open-source tools and are easy to implement. Model and data are linked in an intuitive and informative web-browser based display that can be used to explore the model and the features in the data that influence various aspects of the model. We encode the model and data into HTML files and present high-dimensional information using two approaches. The first uses a Python package to pack both data and interactive plots in a single file. The second approach uses JavaScript, CSS, and HTML to build a dynamic webpage for <span class="hlt">seismic</span> data visualization. The tools have proven useful and led to deeper insight into 3D <span class="hlt">seismic</span> models and the data that were used to construct them</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUSM.S33B..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUSM.S33B..01M"><span>Integration of Well & Core Data of Carbonate Reservoirs with Surface <span class="hlt">Seismic</span> in Garraf Oil Field, Southern Iraq</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mhuder, J. J.; Muhlhl, A. A.; Basra Geologiests</p> <p>2013-05-01</p> <p>The Garraf Field is situated in Southern Iraq in Nasiriya area, is located in Mesopotamian basin. The carbonate facies are dominant in main reservoirs in Garraf field (Mishrif and Yammama Formations) which is Cretaceous in age. The structure of the reservoir in this field are low relief gentle anticlinal structure aligned in NW to SE direction, and No fault were observed and <span class="hlt">interpreted</span> in 3D <span class="hlt">seismic</span> section. 3D <span class="hlt">seismic</span> survey by Iraqi Oil Exploration Company No 2 was successfully conducted on the Garraf field at 2008-2009 using recording system SERCEL 408UL and Vibrators Nomad 65. Bin size: 25*25, Fold: 36, SP Interval: 50m, Lines Interval: 300m, 3 wells were drilled Ga (1, 2, 3) and it used for <span class="hlt">seismic</span> to well tie in Petrel. Data analysis was conducted for each reservoirs for Lithological and sedimentological studies were based on core and well data .The study showed That the Mishrif Formation deposited in a broad carbonate platform with shallowing upward regressive succession and The depositional environment is extending from outer marine to shallow middle-inner shelf settings with restricted lagoons as supported by the present of Miliolid fossils. The fragmented rudist biostromes accumulated in the middle shelf. No rudist reef is presence in the studied cores. While the Major sequences are micritic limestone of lagoonal and oolitic/peloidal grainstone sandy shoal separated by mudstone of Yamama formation. Sedimentation feature are seen on <span class="hlt">seismic</span> attributes and it is help for understanding of sedimentation environment and suitable structure <span class="hlt">interpretation</span>. There is good relationship between Acustic Impedance and porosity, Acustic Impedance reflects porosity or facies change of carbonate rather than fluid content. Data input used for 3D Modeling include 3D <span class="hlt">seismic</span> and AI data, petrophysical analysis, core and thin section description. 3D structure modeling were created base on the geophysical data <span class="hlt">interpretation</span> and Al analysis. Data analysis for Al data were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T13B0506W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T13B0506W"><span><span class="hlt">Seismic</span> and thermal structure of the crust and uppermost mantle beneath Antarctica from inversion of multiple <span class="hlt">seismic</span> datasets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wiens, D.; Shen, W.; Anandakrishnan, S.; Aster, R. C.; Gerstoft, P.; Bromirski, P. D.; Dalziel, I.; Hansen, S. E.; Heeszel, D.; Huerta, A. D.; Nyblade, A.; Stephen, R. A.; Wilson, T. J.; Winberry, J. P.; Stern, T. A.</p> <p>2017-12-01</p> <p>Since the last decade of the 20th century, over 200 broadband <span class="hlt">seismic</span> stations have been deployed across Antarctica (e.g., temporary networks such as TAMSEIS, AGAP/GAMSEIS, POLENET/ANET, TAMNNET and RIS/DRIS by U.S. geoscientists as well as stations deployed by Japan, Britain, China, Norway, and other countries). In this presentation, we discuss our recent efforts to build reference crustal and uppermost mantle shear velocity (Vs) and thermal models for continental Antarctica based on those <span class="hlt">seismic</span> arrays. By combing the high resolution Rayleigh wave dispersion maps derived from both ambient noise and teleseismic earthquakes, together with P receiver function waveforms, we develop a 3-D Vs model for the crust and uppermost mantle beneath Central and West Antarctica to a depth of 200 km. Additionally, using this 3-D <span class="hlt">seismic</span> model to constrain the crustal structure, we re-invert for the upper mantle thermal structure using the surface wave data within a thermodynamic framework and construct a 3-D thermal model for the Antarctic lithosphere. The final product, a high resolution thermal model together with associated uncertainty estimates from the Monte Carlo inversion, allows us to derive lithospheric thickness and surface heat flux maps for much of the continent. West Antarctica shows a much thinner lithosphere ( 50-90 km) than East Antarctica ( 130-230 km), with a sharp transition along the Transantarctic Mountains (TAM). A variety of geological features, including a slower/hotter but highly heterogeneous West Antarctica and a much faster/colder East Antarctic craton, are present in the 3-D <span class="hlt">seismic</span>/thermal models. Notably, slow <span class="hlt">seismic</span> velocities observed in the uppermost mantle beneath the southern TAM are <span class="hlt">interpreted</span> as a signature of lithospheric foundering and replacement with hot asthenosphere. The high resolution image of these features from the 3-D models helps further investigation of the dynamic state of Antarctica's lithosphere and underlying asthenosphere</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAG...143...31P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAG...143...31P"><span>Capabilities of <span class="hlt">seismic</span> and georadar 2D/3D imaging of shallow subsurface of transport route using the Seismobile system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pilecki, Zenon; Isakow, Zbigniew; Czarny, Rafał; Pilecka, Elżbieta; Harba, Paulina; Barnaś, Maciej</p> <p>2017-08-01</p> <p>In this work, the capabilities of the Seismobile system for shallow subsurface imaging of transport routes, such as roads, railways, and airport runways, in different geological conditions were presented. The Seismobile system combines the advantages of <span class="hlt">seismic</span> profiling using landstreamer and georadar (GPR) profiling. It consists of up to four <span class="hlt">seismic</span> measuring lines and carriage with a suspended GPR antenna. Shallow subsurface recognition may be achieved to a maximum width of 10.5 m for a distance of 3.5 m between the measurement lines. GPR measurement is performed in the axis of the construction. Seismobile allows the measurement time, labour and costs to be reduced due to easy technique of its installation, remote data transmission from geophones to accompanying measuring modules, automated location of the system based on GPS and a highly automated method of <span class="hlt">seismic</span> wave excitation. In this paper, the results of field tests carried out in different geological conditions were presented. The methodologies of acquisition, processing and <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> and GPR measurements were broadly described. Seismograms and its spectrum registered by Seismobile system were compared to the ones registered by Geode seismograph of Geometrix. <span class="hlt">Seismic</span> data processing and <span class="hlt">interpretation</span> software allows for the obtaining of 2D/3D models of P- and S-wave velocities. Combined <span class="hlt">seismic</span> and GPR results achieved sufficient imaging of shallow subsurface to a depth of over a dozen metres. The obtained geophysical information correlated with geological information from the boreholes with good quality. The results of performed tests proved the efficiency of the Seismobile system in <span class="hlt">seismic</span> and GPR imaging of a shallow subsurface of transport routes under compound conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E3SWC..3503003S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E3SWC..3503003S"><span><span class="hlt">Seismic</span> Linear Noise Attenuation with Use of Radial Transform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szymańska-Małysa, Żaneta</p> <p>2018-03-01</p> <p>One of the goals of <span class="hlt">seismic</span> data processing is to attenuate the recorded noise in order to enable correct <span class="hlt">interpretation</span> of the image. Radial transform has been used as a very effective tool in the attenuation of various types of linear noise, both numerical and real (such as ground roll, direct waves, head waves, guided waves etc). The result of transformation from offset - time (X - T) domain into apparent velocity - time (R - T) domain is frequency separation between reflections and linear events. In this article synthetic and real <span class="hlt">seismic</span> shot gathers were examined. One example was targeted at far offset area of dataset where reflections and noise had similar apparent velocities and frequency bands. Another example was a result of elastic modelling where linear artefacts were produced. Bandpass filtering and scaling operation executed in radial domain attenuated all discussed types of linear noise very effectively. After noise reduction all further processing steps reveal better results, especially velocity analysis, migration and stacking. In all presented cases signal-to-noise ratio was significantly increased and reflections covered previously by noise were revealed. Power spectra of filtered <span class="hlt">seismic</span> records preserved real dynamics of reflections.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JSAES..16..759B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JSAES..16..759B"><span>Crustal <span class="hlt">seismicity</span> in central Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barrientos, S.; Vera, E.; Alvarado, P.; Monfret, T.</p> <p>2004-06-01</p> <p>Both the genesis and rates of activity of shallow intraplate <span class="hlt">seismic</span> activity in central Chile are poorly understood, mainly because of the lack of association of <span class="hlt">seismicity</span> with recognizable fault features at the surface and a poor record of <span class="hlt">seismic</span> activity. The goal of this work is to detail the characteristics of <span class="hlt">seismicity</span> that takes place in the western flank of the Andes in central Chile. This region, located less than 100 km from Santiago, has been the site of earthquakes with magnitudes up to 6.9, including several 5+ magnitude shocks in recent years. Because most of the events lie outside the Central Chile <span class="hlt">Seismic</span> Network, at distances up to 60 km to the east, it is essential to have adequate knowledge of the velocity structure in the Andean region to produce the highest possible quality of epicentral locations. For this, a N-S refraction line, using mining blasts of the Disputada de Las Condes open pit mine, has been acquired. These blasts were detected and recorded as far as 180 km south of the mine. <span class="hlt">Interpretation</span> of the travel times indicates an upper crustal model consisting of three layers: 2.2-, 6.7-, and 6.1-km thick, overlying a half space; their associated P wave velocities are 4.75-5.0 (gradient), 5.8-6.0 (gradient), 6.2, and 6.6 km/s, respectively. Hypocentral relocation of earthquakes in 1986-2001, using the newly developed velocity model, reveals several regions of concentrated <span class="hlt">seismicity</span>. One clearly delineates the fault zone and extensions of the strike-slip earthquake that took place in September 1987 at the source of the Cachapoal River. Other regions of activity are near the San José volcano, the source of the Maipo River, and two previously recognized lineaments that correspond to the southern extension of the Pocuro fault and Olivares River. A temporary array of seismographs, installed in the high Maipo River (1996) and San José volcano (1997) regions, established the hypocentral location of events with errors of less than 1 km</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://woodshole.er.usgs.gov/pubs/of2007-1150/OFR2007-1150.pdf','USGSPUBS'); return false;" href="http://woodshole.er.usgs.gov/pubs/of2007-1150/OFR2007-1150.pdf"><span>Sidescan-sonar imagery, multibeam bathymetry, and surficial geologic <span class="hlt">interpretations</span> of the sea floor in Rhode Island Sound, off Sakonnet Point, Rhode Island</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McMullen, Katherine Y.; Poppe, Lawrence J.; Twomey, Erin R.; Danforth, William W.; Haupt, Todd A.; Crocker, James M.</p> <p>2007-01-01</p> <p>The U.S. Geological Survey (USGS) is working with the National Oceanic and Atmospheric Administration (NOAA) to <span class="hlt">interpret</span> the surficial geology in estuaries and sounds along the northeastern coast of the United States. This report <span class="hlt">interprets</span> the area covered by NOAA Survey H11320, about 72 km² of sea floor in eastern Rhode Island Sound (RIS), located about 8 km south of Sakonnet Point, Rhode Island (fig. 1). Previous work in RIS includes studies of both sea-floor processes and subsurface geologic framework. McMaster (1960) mapped surficial sediment samples in Narragansett Bay and RIS and McMaster and others (1968) conducted a <span class="hlt">seismic</span>-reflection survey in Block Island Sound and RIS. O'Hara and Oldale (1980) collected <span class="hlt">seismic</span>-reflection profiles, sidescan-sonar data, and vibracores in eastern RIS (fig. 2). They <span class="hlt">interpreted</span> the geologic history, assessed sand and gravel resources, and evaluated the mining impact of these resources. McMaster's (1960) <span class="hlt">interpretation</span> of the surficial sediment within this study area consisted of sand with several isolated areas of gravel. Several other sediment samples were previously obtained within the study area: three National Oceanographic Data Center (NODC) dredge samples from 1942 consisted of sand and one National Ocean Service (NOS) sample from 1939 was rocky (fig. 2; Poppe and others, 2003). The purpose of this report is to define the sea-floor morphology and sedimentary environments and <span class="hlt">interpret</span> processes occurring on the sea floor using sidescan-sonar imagery, multibeam bathymetry, and historic <span class="hlt">seismic</span>-reflection profiles.</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('https://pubs.er.usgs.gov/publication/70029916','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029916"><span>The Northern end of the Dead Sea Basin: Geometry from reflection <span class="hlt">seismic</span> evidence</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Al-Zoubi, A. S.; Heinrichs, T.; Qabbani, I.; ten Brink, Uri S.</p> <p>2007-01-01</p> <p>Recently released reflection <span class="hlt">seismic</span> lines from the Eastern side of the Jordan River north of the Dead Sea were <span class="hlt">interpreted</span> by using borehole data and incorporated with the previously published <span class="hlt">seismic</span> lines of the eastern side of the Jordan River. For the first time, the lines from the eastern side of the Jordan River were combined with the published reflection <span class="hlt">seismic</span> lines from the western side of the Jordan River. In the complete cross sections, the inner deep basin is strongly asymmetric toward the Jericho Fault supporting the <span class="hlt">interpretation</span> of this segment of the fault as the long-lived and presently active part of the Dead Sea Transform. There is no indication for a shift of the depocenter toward a hypothetical eastern major fault with time, as recently suggested. Rather, the north-eastern margin of the deep basin takes the form of a large flexure, modestly faulted. In the N-S-section along its depocenter, the floor of the basin at its northern end appears to deepen continuously by roughly 0.5??km over 10??km distance, without evidence of a transverse fault. The asymmetric and gently-dipping shape of the basin can be explained by models in which the basin is located outside the area of overlap between en-echelon strike-slip faults. ?? 2007 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018794','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018794"><span>Stress/strain changes and triggered <span class="hlt">seismicity</span> following the MW7.3 Landers, California, earthquake</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, J.</p> <p>1996-01-01</p> <p>Calculations of dynamic stresses and strains, constrained by broadband seismograms, are used to investigate their role in generating the remotely triggered <span class="hlt">seismicity</span> that followed the June 28, 1992, MW7.3 Landers, California earthquake. I compare straingrams and dynamic Coulomb failure functions calculated for the Landers earthquake at sites that did experience triggered <span class="hlt">seismicity</span> with those at sites that did not. Bounds on triggering thresholds are obtained from analysis of dynamic strain spectra calculated for the Landers and MW,6.1 Joshua Tree, California, earthquakes at various sites, combined with results of static strain investigations by others. I <span class="hlt">interpret</span> three principal results of this study with those of a companion study by Gomberg and Davis [this issue]. First, the dynamic elastic stress changes themselves cannot explain the spatial distribution of triggered <span class="hlt">seismicity</span>, particularly the lack of triggered activity along the San Andreas fault system. In addition to the requirement to exceed a Coulomb failure stress level, this result implies the need to invoke and satisfy the requirements of appropriate slip instability theory. Second, results of this study are consistent with the existence of frequency- or rate-dependent stress/strain triggering thresholds, inferred from the companion study and <span class="hlt">interpreted</span> in terms of earthquake initiation involving a competition of processes, one promoting failure and the other inhibiting it. Such competition is also part of relevant instability theories. Third, the triggering threshold must vary from site to site, suggesting that the potential for triggering strongly depends on site characteristics and response. The lack of triggering along the San Andreas fault system may be correlated with the advanced maturity of its fault gouge zone; the strains from the Landers earthquake were either insufficient to exceed its larger critical slip distance or some other critical failure parameter; or the faults failed stably as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1712236L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1712236L"><span>Preliminary <span class="hlt">seismic</span> characterization of parts of the island of Gotland in preparation for a potential CO2 storage test site</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lydersen, Ida; Sopher, Daniel; Juhlin, Christopher</p> <p>2015-04-01</p> <p>Geological storage of CO2 is one of the available options to reduce CO2-emissions from large point sources. Previous work in the Baltic Sea Basin has inferred a large storage potential in several stratigraphic units. The most promising of these is the Faludden sandstone, exhibiting favorable reservoir properties and forming a regional stratigraphic trap. A potential location for a pilot CO2 injection site, to explore the suitability of the Faludden reservoir is onshore Gotland, Sweden. In this study onshore and offshore data have been digitized and <span class="hlt">interpreted</span>, along with well data, to provide a detailed characterization of the Faludden reservoir below parts of Gotland. Maps and regional <span class="hlt">seismic</span> profiles describing the extent and top structure of the Faludden sandstone are presented. The study area covers large parts of the island of Gotland, and extends about 50-70km offshore. The <span class="hlt">seismic</span> data presented is part of a larger dataset acquired by Oljeprospektering AB (OPAB) between 1970 and 1990. The dataset is to this date largely unpublished, therefore re-processing and <span class="hlt">interpretation</span> of these data provide improved insight into the subsurface of the study area. Two longer <span class="hlt">seismic</span> profiles crossing Gotland ENE-WSW have been <span class="hlt">interpreted</span> to give a large scale, regional control of the Faludden sandstone. A relatively tight grid of land <span class="hlt">seismic</span> following the extent of the Faludden sandstone along the eastern coast to the southernmost point has been <span class="hlt">interpreted</span> to better understand the actual distribution and geometry of the Faludden sandstone beneath Gotland. The maps from this study help to identify the most suitable area for a potential test injection site for CO2-storage, and to further the geological understanding of the area in general.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6964389-impact-seismic-data-nigerian-national-petroleum-corporation-chevron-nigeria-limited-joint-venture-development-drilling-program','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6964389-impact-seismic-data-nigerian-national-petroleum-corporation-chevron-nigeria-limited-joint-venture-development-drilling-program"><span>Impact of 3-D <span class="hlt">seismic</span> data on the Nigerian National Petroleum Corporation/Chevron Nigeria Limited joint venture development drilling program</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>Quam, S.</p> <p></p> <p>The Nigerian National Petroleum Corporation/Chevron Nigeria Limited joint venture has been acquiring three-dimensional (3-D) <span class="hlt">seismic</span> data over its concessions since 1984. To date, 1700 km[sup 2] have been recorded and processed at a cumulative cost of US $39 million. During 1991 - 1992, 20 development wells were drilled based directly on new 3-D <span class="hlt">seismic</span> <span class="hlt">interpretations</span>. These wells have added 148 million bbl of oil in new recoverable reserves, and to date have added 37,000 bbl/day to the joint venture's production. In addition, the 3-D <span class="hlt">interpretations</span> have resulted in a sizable inventory of wells for future development drilling. The new 3-Dmore » <span class="hlt">interpretations</span> provided more accurate pictures of fault patterns, fluid contacts, channel trends, stratigraphic continuity, and velocity/amplitude anomalies. In addition, the 3-D data were invaluable in designing low risk, directional well trajectories to tap relatively thin oil legs under large gas caps. Wells often were programmed to hit several objectives at their respective gas/oil contacts, resulting in maximized net oil sand pays and reducing the risk of gas production. In order to do this, directional [open quotes]sharpshooting,[close quotes] accurate depth conversion of the <span class="hlt">seismic</span> time maps, was critical. By using the 3-D <span class="hlt">seismic</span>, checkshot, and sonic data to develop a variable velocity space, well-top prognoses within 50 ft at depths of 6,000-10,000 ft were possible, and were key to the success of the program. As the joint venture acreage becomes more mature, development wells will be drilled for smaller numbers of stacked objectives, and sometimes for single sands. Highly accurate 3-D <span class="hlt">interpretations</span> and depth conversions will become even more critical in order to tap thinner pay zones in a cost-effect manner.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ISPAr42.3..239C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ISPAr42.3..239C"><span>High Resolution SAR Imaging Employing Geometric Features for Extracting <span class="hlt">Seismic</span> Damage of Buildings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cui, L. P.; Wang, X. P.; Dou, A. X.; Ding, X.</p> <p>2018-04-01</p> <p>Synthetic Aperture Radar (SAR) image is relatively easy to acquire but difficult for <span class="hlt">interpretation</span>. This paper probes how to identify <span class="hlt">seismic</span> damage of building using geometric features of SAR. The SAR imaging geometric features of buildings, such as the high intensity layover, bright line induced by double bounce backscattering and dark shadow is analysed, and show obvious differences texture features of homogeneity, similarity and entropy in combinatorial imaging geometric regions between the un-collapsed and collapsed buildings in airborne SAR images acquired in Yushu city damaged by 2010 Ms7.1 Yushu, Qinghai, China earthquake, which implicates a potential capability to discriminate collapsed and un-collapsed buildings from SAR image. Study also shows that the proportion of highlight (layover & bright line) area (HA) is related to the <span class="hlt">seismic</span> damage degree, thus a SAR image damage index (SARDI), which related to the ratio of HA to the building occupation are of building in a street block (SA), is proposed. While HA is identified through feature extraction with high-pass and low-pass filtering of SAR image in frequency domain. A partial region with 58 natural street blocks in the Yushu City are selected as study area. Then according to the above method, HA is extracted, SARDI is then calculated and further classified into 3 classes. The results show effective through validation check with <span class="hlt">seismic</span> damage classes <span class="hlt">interpreted</span> artificially from post-earthquake airborne high resolution optical image, which shows total classification accuracy 89.3 %, Kappa coefficient 0.79 and identical to the practical <span class="hlt">seismic</span> damage distribution. The results are also compared and discussed with the building damage identified from SAR image available by other authors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017672','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017672"><span>Optimization of wide-angle <span class="hlt">seismic</span> signal-to-noise ratios and P-wave transmission in Kenya</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jacob, A.W.B.; Vees, R.; Braile, L.W.; Criley, E.</p> <p>1994-01-01</p> <p>In previous refraction and wide-angle reflection experiments in the Kenya Rift there were problems with poor signal-noise ratios which made good <span class="hlt">seismic</span> <span class="hlt">interpretation</span> difficult. Careful planning and preparation for KRISP 90 has substantially overcome these problems and produced excellent <span class="hlt">seismic</span> sections in a difficult environment. Noise levels were minimized by working, as far as possible, at times of the day when conditions were quiet, while source signals were optimized by using dispersed charges in water where it was available and waterfilled boreholes in most cases where it was not. <span class="hlt">Seismic</span> coupling at optimum depth in water has been found to be more than 100 times greater than it is in a borehole in dry loosely compacted material. Allowing for the source coupling, a very marked difference has been found between the observation ranges in the rift and those on the flanks, where the observation ranges are greater. These appear to indicate a significant difference in <span class="hlt">seismic</span> transmission through the two types of crust. ?? 1994.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....14000C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....14000C"><span>Modelling the time behaviour of a self-organized <span class="hlt">seismic</span> region: a cellular automaton with memory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cisternas, A.; Rivera, L.; Munoz, D.</p> <p>2003-04-01</p> <p>The range of a cumulative sequence of earthquake moments in a <span class="hlt">seismic</span> region varies according to Hurst's law, namely a power law in the length of the time window. The range allows for an estimation of Mmax in a <span class="hlt">seismic</span> zone. In the case of an independent process, the Hurst exponent H is 0.5. Memory implies 0.5<H<1, a persistent behaviour. We study the time process of the <span class="hlt">seismic</span> behaviour of a crustal model, by using a cellular automata depending of several parameters: rate of strain accumulation, maximum strength of the crust, mean time delay for recovering strength in a broken fault (memory), friction on the fault, etc. We investigate the effect of the change of these parameters on the resulting Hurst exponents, and make a physical <span class="hlt">interpretation</span> of the results. An application is made to the time evolution of <span class="hlt">seismicity</span> in the Betic Cordillera (Southern Spain), and in the Marmara Region (Turkey).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5679967-diapiric-origin-blytheville-pascola-arches-reelfoot-rift-east-central-united-states-relation-new-madrid-seismicity','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5679967-diapiric-origin-blytheville-pascola-arches-reelfoot-rift-east-central-united-states-relation-new-madrid-seismicity"><span>Diapiric origin of the Blytheville and Pascola arches in the Reelfoot rift, east-central United States: Relation to New Madrid <span class="hlt">seismicity</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>McKeown, F.A.; Diehl, S.F.; Glick, E.E.</p> <p>1990-11-01</p> <p>Most of the earthquakes in the New Madrid <span class="hlt">seismic</span> zone correlate spatially with the Blytheville arch and part of the Pascoal arch, which are <span class="hlt">interpreted</span> to be the same structure. Both arches may have formed by diapirism along the axis of the Reelfoot rift. <span class="hlt">Seismic</span>, geophysical, and drill-hole data indicate that the rocks in the arches are highly deformed and fractured and have gross lithologic properties that make them weaker than rocks adjacent to the arches. The weaker rocks are inferred to fail <span class="hlt">seismically</span> more readily than the stronger rocks adjacent to the arches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T42C..07G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T42C..07G"><span>Marine forearc tectonics in the unbroken segment of the Northern Chile <span class="hlt">seismic</span> gap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geersen, J.; Behrmann, J.; Ranero, C. R.; Klaucke, I.; Kopp, H.; Lange, D.; Barckhausen, U.; Reichert, C. J.; Diaz-Naveas, J.</p> <p>2016-12-01</p> <p>While clearly occurring within the well-defined Northern Chile <span class="hlt">seismic</span> gap, the 2014 Mw. 8.1 Iquique Earthquake only ruptured part of this gap, leaving large and possibly highly coupled areas untouched. These non-ruptured areas now may pose an elevated <span class="hlt">seismic</span> hazard due to the transfer of stresses resulting from the 2014 rupture. Here we use recently collected multibeam bathymetric data, covering 90% of the North Chilean marine forearc, in combination with unpublished <span class="hlt">seismic</span> reflection images to derive a tectonic map of the marine forearc in the unbroken segment of the <span class="hlt">seismic</span> gap. In the entire study area we find evidence for widespread normal faulting. Seaward dipping normal faults locally extend close to the deformation front at the deep-sea trench under 8 km of water. Similar normal faults on the lower slope are neither observed further north (2014 Iquique earthquake area) nor further south (2007 Tocopilla earthquake area). On the upper continental slope, some of the normal faults dip towards the continent, defining N-S trending ridges that can be traced over tens of kilometers. The spatial variations in normal faulting do not correlate with obvious changes in the structural and tectonic setting of the subduction zone (e.g. plate convergence rate and direction, trench sediment thickness, subducting plate roughness). Thus, the permanent deformation recorded in the spatial distribution of faults may hold crucial information about the long-term <span class="hlt">seismic</span> behavior of the Northern Chile <span class="hlt">seismic</span> gap over multiple earthquake cycles. Although the structural <span class="hlt">interpretations</span> cannot directly be translated into <span class="hlt">seismic</span> hazard, the tectonic map serves to better understand deformation in the marine forearc in relation to the <span class="hlt">seismic</span> cycle, historic <span class="hlt">seismicity</span>, and the spatial distribution of plate-coupling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1812319K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1812319K"><span>Evaluation of induced <span class="hlt">seismicity</span> forecast models in the Induced <span class="hlt">Seismicity</span> Test Bench</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Király, Eszter; Gischig, Valentin; Zechar, Jeremy; Doetsch, Joseph; Karvounis, Dimitrios; Wiemer, Stefan</p> <p>2016-04-01</p> <p>Induced earthquakes often accompany fluid injection, and the <span class="hlt">seismic</span> hazard they pose threatens various underground engineering projects. Models to monitor and control induced <span class="hlt">seismic</span> hazard with traffic light systems should be probabilistic, forward-looking, and updated as new data arrive. Here, we propose an Induced <span class="hlt">Seismicity</span> Test Bench to test and rank such models. We apply the test bench to data from the Basel 2006 and Soultz-sous-Forêts 2004 geothermal stimulation projects, and we assess forecasts from two models that incorporate a different mix of physical understanding and stochastic representation of the induced sequences: Shapiro in Space (SiS) and Hydraulics and <span class="hlt">Seismics</span> (HySei). SiS is based on three pillars: the <span class="hlt">seismicity</span> rate is computed with help of the seismogenic index and a simple exponential decay of the <span class="hlt">seismicity</span>; the magnitude distribution follows the Gutenberg-Richter relation; and <span class="hlt">seismicity</span> is distributed in space based on smoothing <span class="hlt">seismicity</span> during the learning period with 3D Gaussian kernels. The HySei model describes <span class="hlt">seismicity</span> triggered by pressure diffusion with irreversible permeability enhancement. Our results show that neither model is fully superior to the other. HySei forecasts the <span class="hlt">seismicity</span> rate well, but is only mediocre at forecasting the spatial distribution. On the other hand, SiS forecasts the spatial distribution well but not the <span class="hlt">seismicity</span> rate. The shut-in phase is a difficult moment for both models in both reservoirs: the models tend to underpredict the <span class="hlt">seismicity</span> rate around, and shortly after, shut-in. Ensemble models that combine HySei's rate forecast with SiS's spatial forecast outperform each individual model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/15003921','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/15003921"><span>Passive <span class="hlt">Seismic</span> Monitoring for Rockfall at Yucca Mountain: Concept Tests</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>Cheng, J; Twilley, K; Murvosh, H</p> <p>2003-03-03</p> <p>For the purpose of proof-testing a system intended to remotely monitor rockfall inside a potential radioactive waste repository at Yucca Mountain, a system of <span class="hlt">seismic</span> sub-arrays will be deployed and tested on the surface of the mountain. The goal is to identify and locate rockfall events remotely using automated data collecting and processing techniques. We install seismometers on the ground surface, generate <span class="hlt">seismic</span> energy to simulate rockfall in underground space beneath the array, and <span class="hlt">interpret</span> the surface response to discriminate and locate the event. Data will be analyzed using matched-field processing, a generalized beam forming method for localizing discrete signals.more » Software is being developed to facilitate the processing. To date, a three-component sub-array has been installed and successfully tested.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003CRGeo.335..319Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003CRGeo.335..319Z"><span>Interprétation hydrogéologique de l'aquifère des bassins sud-rifains (Maroc) : apport de la sismique réflexionHydrogeological <span class="hlt">interpretation</span> of the southern Rifean basins aquifer (Morocco): <span class="hlt">seismic</span> reflexion contribution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zouhri, Lahcen; Gorini, Christian; Lamouroux, Christian; Vachard, Daniel; Dakki, Mohammed</p> <p>2003-03-01</p> <p>The aquifer of the Rharb Basin is constituted by heterogeneous material. The <span class="hlt">seismic</span> reflexion <span class="hlt">interpretation</span> carried out in this area, highlighted a permeable device compartmentalized in raised and subsided blocks. Depressions identified in the northern and southernmost zones are characterized by Plio-Quaternary fillings that are favourable to the hydrogeological exploitation. Two mechanisms contribute to structure the Plio-Quaternary aquifer: the Hercynian reactivation in the southernmost part, and the gravitational mechanism of the Pre-Rifean nappe. The groundwater flow and the aquifer thickening are controlled by this reactivation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.T53C1453N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.T53C1453N"><span>Fracturing and Transformation Into Veins Beneath the Crustal Scale Brittle Ductile Transition - a Record of Co-<span class="hlt">seismic</span> Loading and Post-<span class="hlt">seismic</span> Relaxation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nüchter, J. A.; Stöckhert, B.</p> <p>2005-12-01</p> <p>Metamorphic rocks approaching the crustal scale brittle-ductile transition (BDT) during exhumation are expected to become increasingly affected by short term stress fluctuations related to <span class="hlt">seismic</span> activity in the overlying seismogenic layer (schizosphere), while still residing in a long-term viscous environment (plastosphere). The structural and microstructural record of quartz veins in low grade - high pressure metamorphic rocks from southern Evia, Greece, yields insight into the processes and conditions just beneath the long-term BDT at temperatures of about 300 to 350°C, which switches between brittle failure and viscous flow as a function of imposed stress or strain rate. The following features are characteristic: (1) The veins have formed from tensile fractures, with a typical length on the order of 10-1 to 101 m; (2) The veins are discordant with respect to foliation and all pre-existing structures, with a uniform orientation over more than 500 km2; (3) The veins show a low aspect ratio of about 10 to 100 and an irregular or characteristic flame shape, which requires distributed ductile deformation of the host rock; (4) Fabrics of the sealing vein quartz indicate that - at a time - the veins were wide open cavities; (5) The sealing quartz crystals reveal a broad spectrum of microstructural features indicative of crystal plastic deformation at high stress and temperatures of about 300 to 350°C. These features indicate that opening and sealing of the fractures commenced immediately after brittle failure, controlled by ductile deformation of the host rock. Vein-parallel shortening was generally less than about 2%. Crystals formed early during sealing were plastically deformed upon progressive deformation and opening of the vein. The structural and microstructural record is <span class="hlt">interpreted</span> as follows: Brittle failure is proposed to be a consequence of short term co-<span class="hlt">seismic</span> loading. Subsequent opening of the fracture and sealing to become a vein is <span class="hlt">interpreted</span> to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.S43D..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.S43D..06C"><span>An Improved Statistical Solution for Global <span class="hlt">Seismicity</span> by the HIST-ETAS Approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chu, A.; Ogata, Y.; Katsura, K.</p> <p>2010-12-01</p> <p>For long-term global <span class="hlt">seismic</span> model fitting, recent work by Chu et al. (2010) applied the spatial-temporal ETAS model (Ogata 1998) and analyzed global data partitioned into tectonic zones based on geophysical characteristics (Bird 2003), and it has shown tremendous improvements of model fitting compared with one overall global model. While the ordinary ETAS model assumes constant parameter values across the complete region analyzed, the hierarchical space-time ETAS model (HIST-ETAS, Ogata 2004) is a newly introduced approach by proposing regional distinctions of the parameters for more accurate <span class="hlt">seismic</span> prediction. As the HIST-ETAS model has been fit to regional data of Japan (Ogata 2010), our work applies the model to describe global <span class="hlt">seismicity</span>. Employing the Akaike's Bayesian Information Criterion (ABIC) as an assessment method, we compare the MLE results with zone divisions considered to results obtained by an overall global model. Location dependent parameters of the model and Gutenberg-Richter b-values are optimized, and seismological <span class="hlt">interpretations</span> are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T41C2909A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T41C2909A"><span>Mineral texture based <span class="hlt">seismic</span> properties of meta-sedimentary and meta-igneous rocks in the orogenic wedge of the Central Scandinavian Caledonides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Almqvist, B. S. G.; Czaplinska, D.; Piazolo, S.</p> <p>2015-12-01</p> <p>Progress in <span class="hlt">seismic</span> methods offers the possibility to visualize in ever greater detail the structure and composition of middle to lower continental crust. Ideally, the <span class="hlt">seismic</span> parameters, including compressional (Vp) and shear (Vs) wave velocities, anisotropy and Vp/Vs-ratio, allow the inference of detailed and quantitative information on the deformation conditions, chemical composition, temperature and the amount and geometry of fluids and melts in the crust. However, such inferences regarding the crust should be calibrated with known mineral and rock physical properties. <span class="hlt">Seismic</span> properties calculated from the crystallographic preferred orientation (CPO) and laboratory measurements on representative core material allow us to quantify the <span class="hlt">interpretations</span> from <span class="hlt">seismic</span> data. The challenge of such calibrations lies in the non-unique <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> data. A large catalogue of physical rock properties is therefore useful, with as many constraining geophysical parameters as possible (including anisotropy and Vp/Vs ratio). We present new CPO data and modelled <span class="hlt">seismic</span> properties for amphibolite and greenschist grade rocks representing the orogenic wedge in the Central Scandinavian Caledonides. Samples were collected from outcrops in the field and from a 2.5 km long drill core, which penetrated an amphibolite-grade allochthonous unit composed of meta-sedimentary and meta-igneous rocks, as well as mica and chlorite-rich mylonites. The textural data was acquired using large area electron backscatter diffraction (EBSD) maps, and the chemical composition of minerals obtained by energy dispersive x-ray (EDS). Based on the texture data, we compare and evaluate some of the existing methods to calculate texture-based <span class="hlt">seismic</span> properties of rocks. The suite of samples consists of weakly anisotropic rocks such as felsic gneiss and calc-silicates, and more anisotropic amphibolite, metagabbro, mica-schist. The newly acquired dataset provides a range of <span class="hlt">seismic</span> properties that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4020S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4020S"><span>First <span class="hlt">seismic</span> shear wave velocity profile of the lunar crust as extracted from the Apollo 17 active <span class="hlt">seismic</span> data by wavefield gradient analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sollberger, David; Schmelzbach, Cedric; Robertsson, Johan O. A.; Greenhalgh, Stewart A.; Nakamura, Yosio; Khan, Amir</p> <p>2016-04-01</p> <p>We present a new <span class="hlt">seismic</span> velocity model of the shallow lunar crust, including, for the first time, shear wave velocity information. So far, the shear wave velocity structure of the lunar near-surface was effectively unconstrained due to the complexity of lunar seismograms. Intense scattering and low attenuation in the lunar crust lead to characteristic long-duration reverberations on the seismograms. The reverberations obscure later arriving shear waves and mode conversions, rendering them impossible to identify and analyze. Additionally, only vertical component data were recorded during the Apollo active <span class="hlt">seismic</span> experiments, which further compromises the identification of shear waves. We applied a novel processing and analysis technique to the data of the Apollo 17 lunar <span class="hlt">seismic</span> profiling experiment (LSPE), which involved recording <span class="hlt">seismic</span> energy generated by several explosive packages on a small areal array of four vertical component geophones. Our approach is based on the analysis of the spatial gradients of the <span class="hlt">seismic</span> wavefield and yields key parameters such as apparent phase velocity and rotational ground motion as a function of time (depth), which cannot be obtained through conventional <span class="hlt">seismic</span> data analysis. These new observables significantly enhance the data for <span class="hlt">interpretation</span> of the recorded <span class="hlt">seismic</span> wavefield and allow, for example, for the identification of S wave arrivals based on their lower apparent phase velocities and distinct higher amount of generated rotational motion relative to compressional (P-) waves. Using our methodology, we successfully identified pure-mode and mode-converted refracted shear wave arrivals in the complex LSPE data and derived a P- and S-wave velocity model of the shallow lunar crust at the Apollo 17 landing site. The extracted elastic-parameter model supports the current understanding of the lunar near-surface structure, suggesting a thin layer of low-velocity lunar regolith overlying a heavily fractured crust of basaltic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUSM.S52A..07B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUSM.S52A..07B"><span><span class="hlt">Seismic</span> Catalogue and <span class="hlt">Seismic</span> Network in Haiti</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belizaire, D.; Benito, B.; Carreño, E.; Meneses, C.; Huerfano, V.; Polanco, E.; McCormack, D.</p> <p>2013-05-01</p> <p>The destructive earthquake occurred on January 10, 2010 in Haiti, highlighted the lack of preparedness of the country to address <span class="hlt">seismic</span> phenomena. At the moment of the earthquake, there was no <span class="hlt">seismic</span> network operating in the country, and only a partial control of the past <span class="hlt">seismicity</span> was possible, due to the absence of a national catalogue. After the 2010 earthquake, some advances began towards the installation of a national network and the elaboration of a <span class="hlt">seismic</span> catalogue providing the necessary input for <span class="hlt">seismic</span> Hazard Studies. This paper presents the state of the works carried out covering both aspects. First, a <span class="hlt">seismic</span> catalogue has been built, compiling data of historical and instrumental events occurred in the Hispaniola Island and surroundings, in the frame of the SISMO-HAITI project, supported by the Technical University of Madrid (UPM) and Developed in cooperation with the Observatoire National de l'Environnement et de la Vulnérabilité of Haiti (ONEV). Data from different agencies all over the world were gathered, being relevant the role of the Dominican Republic and Puerto Rico seismological services which provides local data of their national networks. Almost 30000 events recorded in the area from 1551 till 2011 were compiled in a first catalogue, among them 7700 events with Mw ranges between 4.0 and 8.3. Since different magnitude scale were given by the different agencies (Ms, mb, MD, ML), this first catalogue was affected by important heterogeneity in the size parameter. Then it was homogenized to moment magnitude Mw using the empirical equations developed by Bonzoni et al (2011) for the eastern Caribbean. At present, this is the most exhaustive catalogue of the country, although it is difficult to assess its degree of completeness. Regarding the <span class="hlt">seismic</span> network, 3 stations were installed just after the 2010 earthquake by the Canadian Government. The data were sent by telemetry thought the Canadian System CARINA. In 2012, the Spanish IGN together</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870052170&hterms=Ocean+Stratification&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DOcean%2BStratification','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870052170&hterms=Ocean+Stratification&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DOcean%2BStratification"><span>Why does near ridge extensional <span class="hlt">seismicity</span> occur primarily in the Indian Ocean?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stein, Seth; Cloetingh, Sierd; Wortel, Rinus; Wiens, Douglas A.</p> <p>1987-01-01</p> <p>It is argued that though thermoelastic stresses provide a low level background in all plates, the data favoring their contributing significantly to the stress field and <span class="hlt">seismicity</span> in the young oceanic lithosphere may be <span class="hlt">interpreted</span> in terms of stresses resulting from individual plate geometry and local boundary effects. The dramatic concentration of extensional <span class="hlt">seismicity</span> in the Central Indian Ocean region is shown to be consistent with finite element results for the intraplate stress incorporating the effects of the Himalayan collision and the various subduction zones. Most of the data for both ridge-parallel extension and depth stratification are provided by earthquakes in this area, and it is suggested that these effects may be due more to the regional stress.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5200654-seismic-definition-lower-cretaceous-delta-south-whale-subbasin-offshore-newfoundland','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5200654-seismic-definition-lower-cretaceous-delta-south-whale-subbasin-offshore-newfoundland"><span><span class="hlt">Seismic</span> definition of Lower Cretaceous delta, south Whale subbasin, offshore Newfoundland</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>Jayasinghe, N.R.; Stokes, R.E.</p> <p>1986-05-01</p> <p>Recognition of stratigraphic traps in areas where previous prospects were structural is a trend attributable partly to the availability of new, high-quality <span class="hlt">seismic</span> data. In the South Whale subbasin, offshore Newfoundland, Canada, such a change in exploration philosophy is presently being evaluated. Exploratory drilling offshore eastern Canada began in 1966 in the South Whale subbasin. By the end of 1973, 13 wells were drilled in this subbasin; however, lack of success discouraged further drilling. These wells evaluated large, salt-related structures, well defined by <span class="hlt">seismic</span> data. Although an adequate reservoir was encountered in a number of these wells, faulting associated withmore » halokinesis may have resulted in petroleum migration out of the reservoir. <span class="hlt">Interpretation</span> of recently acquired high-quality <span class="hlt">seismic</span> data indicate a delta in the Lower Cretaceous Missisauga Formation in the study area. <span class="hlt">Seismic</span> dip sections across the delta show a shingled progradation pattern suggesting a wave-dominated depositional environment. The delta comprises approximately 400 km/sup 2/, with closure in the eastern half. Data from wells in the area indicate that adequate source and sealing beds could be present. Furthermore, rocks of similar age in the nearby Avalon basin contain significant petroleum accumulations, the most notable being within the Hibernia oil field.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRB..123.1615H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRB..123.1615H"><span>Local <span class="hlt">Seismicity</span> of the Rainbow Massif on the Mid-Atlantic Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horning, G.; Sohn, R. A.; Canales, J. P.; Dunn, R. A.</p> <p>2018-02-01</p> <p>The Rainbow massif, an oceanic core complex located in a nontransform discontinuity on the Mid-Atlantic Ridge (36°N), is notable for hosting high-temperature hydrothermal discharge through ultramafic rocks. Here we report results from a 9 month microearthquake survey conducted with a network of 13 ocean bottom seismometers deployed on and around the Rainbow massif as part of the MARINER experiment in 2013-2014. High rates ( 300 per day) of low-magnitude (average ML 0.5) microearthquakes were detected beneath the massif. The hypocenters do not cluster along deeply penetrating fault surfaces and do not exhibit mainshock/aftershock sequences, supporting the hypothesis that the faulting associated with the exhumation of the massif is currently inactive. Instead, the hypocenters demarcate a diffuse zone of continuous, low-magnitude deformation at relatively shallow (< 3 km) depths beneath the massif, sandwiched in between the seafloor and <span class="hlt">seismic</span> reflectors <span class="hlt">interpreted</span> to be magmatic sills driving hydrothermal convection. Most of the <span class="hlt">seismicity</span> is located in regions where <span class="hlt">seismic</span> refraction data indicate serpentinized ultramafic host rock, and although the <span class="hlt">seismic</span> network we deployed was not capable of constraining the focal mechanism of most events, our analysis suggests that serpentinization may play an important role in microearthquake generation at the Rainbow massif.</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/2017AGUFM.S53E..06S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S53E..06S"><span>Modeling the effects of structure on <span class="hlt">seismic</span> anisotropy in the Chester gneiss dome, southeast Vermont</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saif, S.; Brownlee, S. J.</p> <p>2017-12-01</p> <p>Compositional and structural heterogeneity in the continental crust are factors that contribute to the complex expression of crustal <span class="hlt">seismic</span> anisotropy. Understanding deformation and flow in the crust using <span class="hlt">seismic</span> anisotropy has thus proven difficult. <span class="hlt">Seismic</span> anisotropy is affected by rock microstructure and mineralogy, and a number of studies have begun to characterize the full elastic tensors of crustal rocks in an attempt to increase our understanding of these intrinsic factors. However, there is still a large gap in length-scale between laboratory characterization on the scale of centimeters and <span class="hlt">seismic</span> wavelengths on the order of kilometers. To address this length-scale gap we are developing a 3D crustal model that will help us determine the effects of rotating laboratory-scale elastic tensors into field-scale structures. The Chester gneiss dome in southeast Vermont is our primary focus. The model combines over 2000 structural data points from field measurements and published USGS structural data with elastic tensors of Chester dome rocks derived from electron backscatter diffraction data. We created a uniformly spaced grid by averaging structural measurements together in equally spaced grid boxes. The surface measurements are then projected into the third dimension using existing subsurface <span class="hlt">interpretations</span>. A measured elastic tensor for the specific rock type is rotated according to its unique structural input at each point in the model. The goal is to use this model to generate artificial seismograms using existing numerical wave propagation codes. Once completed, the model input can be varied to examine the effects of different subsurface structure <span class="hlt">interpretations</span>, as well as heterogeneity in rock composition and elastic tensors. Our goal is to be able to make predictions for how specific structures will appear in <span class="hlt">seismic</span> data, and how that appearance changes with variations in rock composition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989PhDT.......188K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989PhDT.......188K"><span><span class="hlt">Seismic</span> and potential field studies over the East Midlands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kirk, Wayne John</p> <p></p> <p>A <span class="hlt">seismic</span> refraction profile was undertaken to investigate the source of an aeromagnetic anomaly located above the Widmerpool Gulf, East Midlands. Ten shots were fired into 51 stations at c. 1.5km spacing in a 70km profile during 41 days recording. The refraction data were processed using standard techniques to improve the data quality. A new filtering technique, known as Correlated Adaptive Noise Cancellation was tested on synthetic data and successfully applied to controlled source and quarry blast data. Study of strong motion data reveals that the previous method of site calibration is invalid. A new calibration technique, known as the Scaled Amplitude method is presented to provide safer charge size estimation. Raytrace modelling of the refraction data and two dimensional gravity <span class="hlt">interpretation</span> confirms the presence of the Widmerpool Gulf but no support is found for the postulated intrusion. Two dimensional magnetic <span class="hlt">interpretation</span> revealed that the aeromagnetic anomaly could be modelled with a Carboniferous igneous source. A Lower Palaeozoic refractor with a velocity of 6.0 km/s is identified at a maximum depth of c. 2.85km beneath the Widmerpool Gulf. Carboniferous and post-Carboniferous sediments within the gulf have velocities between 2.6-5.5 km/s with a strong vertical gradient. At the gulf margins, a refractor with a constant velocity of 5.2 km/s is identified as Dinantian limestone. A low velocity layer of proposed unaltered Lower Palaeozoics is identified beneath the limestone at the eastern edge of the Derbyshire Dome. The existence and areal extent of this layer are also determined from <span class="hlt">seismic</span> reflection data. Image analysis of potential field data, presents a model identifying 3 structural provinces, the Midlands Microcraton, the Welsh and English Caledonides and a central region of complex linears. This model is used to explain the distribution of basement rocks determined from <span class="hlt">seismic</span> and gravity profiles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014006','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014006"><span>A//r//m//s AND <span class="hlt">SEISMIC</span> SOURCE STUDIES.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hanks, T.C.; ,</p> <p>1984-01-01</p> <p>This paper briefly summarizes some recent developments in studies of <span class="hlt">seismic</span> source parameter estimation, emphasizing the essential similarities between mining-induced seismogenic-failure and naturally occurring, tectonically driven earthquakes. The root-mean-square acceleration, a//r//m//s, shows much promise as an observational measure of high-frequency ground motion; it is very stable observationally, is insensitive to radiation pattern, and can be related linearly to the dynamic stress differences arising in the faulting process. To <span class="hlt">interpret</span> a//r//m//s correctly, however, requires knowledge of f//m//a//x, the high-frequency band-limitation of the radiated field of earthquakes. As a practical matter, f//m//a//x can be due to any number of causes, but an essential ambiguity is whether or not f//m//a//x can arise from source properties alone. The interaction of the aftershocks of the Oroville, California, earthquake illustrates how a//r//m//s stress drops may be connected to detailed <span class="hlt">seismicity</span> patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V21D0649O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V21D0649O"><span>A Closer Look at Recent Deep Mauna Loa <span class="hlt">Seismicity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Okubo, P. G.; Wolfe, C. J.; Nakata, J. S.; Koyanagi, S. K.; Uribe, J. O.</p> <p>2005-12-01</p> <p>In 2002, Mauna Loa Volcano showed signs of reawakening, some 18 years since its last eruption in 1984. First, in April, a brief flurry of microearthquakes occurred at cataloged depths from 25 to 55 km beneath Mauna Loa's summit caldera. Then in May 2002, after the microearthquake swarm had ended, geodetic monitors across Mauna Loa's summit caldera registered a change, from line-length shortening to extension, <span class="hlt">interpreted</span> as reinflation of a magma body approximately 4 km beneath the volcano's summit. Accordingly, the Hawaiian Volcano Observatory issued advisories related to Mauna Loa's stirring. In July 2004, HVO began to record deep long-period (LP) earthquakes beneath Mauna Loa. Historically, <span class="hlt">interpretations</span> of such <span class="hlt">seismicity</span> patterns have associated LP source volumes with magma chambers and magma pathways. Over a few weeks, this <span class="hlt">seismicity</span> dramatically jumped to levels of several dozen per day. Between the months of July and December 2004, nearly 2000 Mauna Loa LPs were located between roughly 25 km and greater than 60 km depths by HVO <span class="hlt">seismic</span> analysts. In late December, these earthquakes rather abruptly ceased, and their levels have remained low ever since. We seek a more detailed understanding of how these earthquakes may factor into Mauna Loa's eruptive framework. Given that their first arrivals are typically emergent, hypocentral estimates using only P-wave first-arrival times of LP earthquakes are often marginally constrained. With such hypocentral estimates, it is difficult to establish clear relationships among the earthquake locations themselves, or between the earthquakes and other processes like crustal extension or magma accumulation or withdrawl. Building on earlier applications to deep earthquakes in Hawaii and LP earthquakes beneath Kilauea, we are reexamining this unprecedented Mauna Loa deep <span class="hlt">seismicity</span> with waveform correlation and precise earthquake relocation techniques. Work to date reveals that, although the waveform correlation coefficients</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoJI.209.1168D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoJI.209.1168D"><span><span class="hlt">Seismic</span> gradiometry using ambient <span class="hlt">seismic</span> noise in an anisotropic Earth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Ridder, S. A. L.; Curtis, A.</p> <p>2017-05-01</p> <p>We introduce a wavefield gradiometry technique to estimate both isotropic and anisotropic local medium characteristics from short recordings of <span class="hlt">seismic</span> signals by inverting a wave equation. The method exploits the information in the spatial gradients of a <span class="hlt">seismic</span> wavefield that are calculated using dense deployments of <span class="hlt">seismic</span> arrays. The application of the method uses the surface wave energy in the ambient <span class="hlt">seismic</span> field. To estimate isotropic and anisotropic medium properties we invert an elliptically anisotropic wave equation. The spatial derivatives of the recorded wavefield are evaluated by calculating finite differences over nearby recordings, which introduces a systematic anisotropic error. A two-step approach corrects this error: finite difference stencils are first calibrated, then the output of the wave-equation inversion is corrected using the linearized impulse response to the inverted velocity anomaly. We test the procedure on ambient <span class="hlt">seismic</span> noise recorded in a large and dense ocean bottom cable array installed over Ekofisk field. The estimated azimuthal anisotropy forms a circular geometry around the production-induced subsidence bowl. This conforms with results from studies employing controlled sources, and with interferometry correlating long records of <span class="hlt">seismic</span> noise. Yet in this example, the results were obtained using only a few minutes of ambient <span class="hlt">seismic</span> noise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1512375M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1512375M"><span>Monitoring induced <span class="hlt">seismicity</span> from underground gas storage: first steps in Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mucciarelli, Marco; Priolo, Enrico</p> <p>2013-04-01</p> <p>The supply of natural gas and its storage are focal points of the Italian politics of energy production and will have increasing importance in the coming years. About a dozen reservoirs are currently in use and fifteen are in development or awaiting approval. Some of these are found in the vicinity of geological structures that are <span class="hlt">seismically</span> active. The assessment of <span class="hlt">seismic</span> hazard (both for natural background and induced <span class="hlt">seismicity</span>) for a geological gas storage facility has a number of unconventional aspects that must be recognized and traced in a clear, ordered way and using guidelines and rules that leave less room as possible for <span class="hlt">interpretation</span> by the individual applicant / verification body. Similarly, for control and monitoring there are not clearly defined procedures or standard instrumentation, let alone tools for analysing and processing data. Finally, governmental organizations in charge of permission grants and operative control tend to have appropriate scientific knowledge only in certain areas and not in others (e.g. the <span class="hlt">seismic</span> one), and the establishment of an independent multidisciplinary inspection body appears desirable. The project StoHaz (https://sites.google.com/site/s2stohaz/home) aims to initiate a series of actions to overcome these deficiencies and allow to define procedures and standards for the <span class="hlt">seismic</span> hazard assessment and control of the activities of natural gas storage in underground reservoirs. OGS will take advantage of the experience gained with the design, installation and maintenance of the <span class="hlt">seismic</span> network monitoring the Collalto reservoir, at the moment the only example in Italy of a public research institution monitoring independently the activities of a private gas storage company.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.S34A..03A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.S34A..03A"><span>Adding <span class="hlt">seismic</span> broadband analysis to characterize Andean backarc <span class="hlt">seismicity</span> in Argentina</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alvarado, P.; Giuliano, A.; Beck, S.; Zandt, G.</p> <p>2007-05-01</p> <p>Characterization of the highly <span class="hlt">seismically</span> active Andean backarc is crucial for assessment of earthquake hazards in western Argentina. Moderate-to-large crustal earthquakes have caused several deaths, damage and drastic economic consequences in Argentinean history. We have studied the Andean backarc crust between 30°S and 36°S using <span class="hlt">seismic</span> broadband data available from a previous ("the CHARGE") IRIS-PASSCAL experiment. We collected more than 12 terabytes of continuous <span class="hlt">seismic</span> data from 22 broadband instruments deployed across Chile and Argentina during 1.5 years. Using free software we modeled full regional broadband waveforms and obtained <span class="hlt">seismic</span> moment tensor inversions of crustal earthquakes testing for the best focal depth for each event. We also mapped differences in the Andean backarc crustal structure and found a clear correlation with different types of crustal <span class="hlt">seismicity</span> (i.e. focal depths, focal mechanisms, magnitudes and frequencies of occurrence) and previously mapped terrane boundaries. We now plan to use the same methodology to study other regions in Argentina using near-real time broadband data available from the national <span class="hlt">seismic</span> (INPRES) network and global <span class="hlt">seismic</span> networks operating in the region. We will re-design the national <span class="hlt">seismic</span> network to optimize short-period and broadband <span class="hlt">seismic</span> station coverage for different network purposes. This work is an international effort that involves researchers and students from universities and national government agencies with the goal of providing more information about earthquake hazards in western Argentina.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...88a2006L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...88a2006L"><span>Improving Vintage <span class="hlt">Seismic</span> Data Quality through Implementation of Advance Processing Techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Latiff, A. H. Abdul; Boon Hong, P. G.; Jamaludin, S. N. F.</p> <p>2017-10-01</p> <p>It is essential in petroleum exploration to have high resolution subsurface images, both vertically and horizontally, in uncovering new geological and geophysical aspects of our subsurface. The lack of success may have been from the poor imaging quality which led to inaccurate analysis and <span class="hlt">interpretation</span>. In this work, we re-processed the existing <span class="hlt">seismic</span> dataset with an emphasis on two objectives. Firstly, to produce a better 3D <span class="hlt">seismic</span> data quality with full retention of relative amplitudes and significantly reduce <span class="hlt">seismic</span> and structural uncertainty. Secondly, to facilitate further prospect delineation through enhanced data resolution, fault definitions and events continuity, particularly in syn-rift section and basement cover contacts and in turn, better understand the geology of the subsurface especially in regard to the distribution of the fluvial and channel sands. By adding recent, state-of-the-art broadband processing techniques such as source and receiver de-ghosting, high density velocity analysis and shallow water de-multiple, the final results produced a better overall reflection detail and frequency in specific target zones, particularly in the deeper section.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAG...140..145R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAG...140..145R"><span>3D <span class="hlt">seismic</span> data de-noising and reconstruction using Multichannel Time Slice Singular Spectrum Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rekapalli, Rajesh; Tiwari, R. K.; Sen, Mrinal K.; Vedanti, Nimisha</p> <p>2017-05-01</p> <p>Noises and data gaps complicate the <span class="hlt">seismic</span> data processing and subsequently cause difficulties in the geological <span class="hlt">interpretation</span>. We discuss a recent development and application of the Multi-channel Time Slice Singular Spectrum Analysis (MTSSSA) for 3D <span class="hlt">seismic</span> data de-noising in time domain. In addition, L1 norm based simultaneous data gap filling of 3D <span class="hlt">seismic</span> data using MTSSSA also discussed. We discriminated the noises from single individual time slices of 3D volumes by analyzing Eigen triplets of the trajectory matrix. We first tested the efficacy of the method on 3D synthetic <span class="hlt">seismic</span> data contaminated with noise and then applied to the post stack <span class="hlt">seismic</span> reflection data acquired from the Sleipner CO2 storage site (pre and post CO2 injection) from Norway. Our analysis suggests that the MTSSSA algorithm is efficient to enhance the S/N for better identification of amplitude anomalies along with simultaneous data gap filling. The bright spots identified in the de-noised data indicate upward migration of CO2 towards the top of the Utsira formation. The reflections identified applying MTSSSA to pre and post injection data correlate well with the geology of the Southern Viking Graben (SVG).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNS23A0003R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNS23A0003R"><span>High-Resolution <span class="hlt">Seismic</span> Reflection Imaging of the Reelfoot Fault, New Madrid, Missouri</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rosandich, B.; Harris, J. B.; Woolery, E. W.</p> <p>2017-12-01</p> <p>Earthquakes in the Lower Mississippi Valley are mainly concentrated in the New Madrid <span class="hlt">Seismic</span> Zone and are associated with reactivated faults of the Reelfoot Rift. Determining the relationship between the seismogenic faults (in crystalline basement rocks) and deformation at the Earth's surface and in the shallow subsurface has remained an active research topic for decades. An integrated <span class="hlt">seismic</span> data set, including compressional (P-) wave and shear (S-) wave <span class="hlt">seismic</span> reflection profiles, was collected in New Madrid, Missouri, across the "New Madrid" segment of the Reelfoot Fault, whose most significant rupture produced the M 7.5, February 7, 1812, New Madrid earthquake. The <span class="hlt">seismic</span> reflection profiles (215 m long) were centered on the updip projection of the fault, which is associated with a surface drainage feature (Des Cyprie Slough) located at the base of a prominent east-facing escarpment. The <span class="hlt">seismic</span> reflection profiles were collected using 48-channel (P-wave) and 24-channel (S-wave) towable landsteamer acquisition equipment. <span class="hlt">Seismic</span> energy was generated by five vertical impacts of a 1.8-kg sledgehammer on a small aluminum plate for the P-wave data and five horizontal impacts of the sledgehammer on a 10-kg steel I-beam for the S-wave data. <span class="hlt">Interpretation</span> of the profiles shows a west-dipping reverse fault (Reelfoot Fault) that propagates upward from Paleozoic sedimentary rocks (>500 m deep) to near-surface Quaternary sediments (<10 m deep). The hanging wall of the fault is anticlinally folded, a structural setting almost identical to that imaged on the Kentucky Bend and Reelfoot Lake segments (of the Reelfoot Fault) to the south.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGP33B..06A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGP33B..06A"><span>Eastern boundary of the Siletz terrane in the Puget Lowland from gravity and magnetic modeling with implications for <span class="hlt">seismic</span> 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>Anderson, M. L.; Blakely, R. J.; Wells, R. E.; Dragovich, J.</p> <p>2011-12-01</p> <p>The forearc of the Cascadia subduction zone in coastal Oregon and Washington is largely composed of a 15-30 km-thick stack of basalt flows comprising the Crescent Formation (WA) and Siletz River Volcanics (OR), and collectively termed the Siletz terrane. We are developing 3-D structural maps of the Puget Lowland to distinguish older and currently active structures for <span class="hlt">seismic</span> hazard analysis. The boundaries of the Siletz terrane in particular may strongly influence crustal rheology and neotectonic structures of the region. Careful analysis of the areal extent of this terrane will also facilitate more accurate <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> data and gravity anomalies, which will help define the extent and shape of overlying basins. Absence of extensive outcrop in the Lowland and a widespread veneer of Quaternary deposits require extensive subsurface geophysical studies to establish Lowland-wide crustal structure. Previous studies have used active <span class="hlt">seismic</span> surveys and <span class="hlt">interpretation</span> of existing industry <span class="hlt">seismic</span> data, with several studies using gravity and magnetic data or passive-source tomography support. However, steeply dipping boundaries in the mid-crust are difficult targets for <span class="hlt">seismic</span> study. We need to independently discriminate between potential models established by <span class="hlt">seismic</span> data using gravity and magnetic datasets. In the Puget Lowland the Siletz is a region of high <span class="hlt">seismic</span> wave speed, density, and magnetic susceptibility, and therefore its mid-crustal boundaries are good targets for definition by gravity and magnetic data. We present <span class="hlt">interpretations</span> of gravity and magnetic anomalies for the Puget Lowland region that together establish the most likely position and structure of the Crescent Formation boundary in the mid-upper crust. Well-constrained physical properties of Crescent basalts inform our aeromagnetic map <span class="hlt">interpretation</span> and give us baseline values for constructing three two-dimensional models by simultaneous forward modeling of aeromagnetic and isostatic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.3554Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.3554Y"><span>Two-dimensional magnetotelluric inversion using reflection <span class="hlt">seismic</span> data as constraints and application in the COSC project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yan, Ping; Kalscheuer, Thomas; Hedin, Peter; Garcia Juanatey, Maria A.</p> <p>2017-04-01</p> <p>We present a novel 2-D magnetotelluric (MT) inversion scheme, in which the local weights of the regularizing smoothness constraints are based on the envelope attribute of a reflection <span class="hlt">seismic</span> image. The weights resemble those of a previously published <span class="hlt">seismic</span> modification of the minimum gradient support method. We measure the directional gradients of the <span class="hlt">seismic</span> envelope to modify the horizontal and vertical smoothness constraints separately. Successful application of the inversion to MT field data of the Collisional Orogeny in the Scandinavian Caledonides (COSC) project using the envelope attribute of the COSC reflection <span class="hlt">seismic</span> profile helped to reduce the uncertainty of the <span class="hlt">interpretation</span> of the main décollement by demonstrating that the associated alum shales may be much thinner than suggested by a previous inversion model. Thus, the new model supports the proposed location of a future borehole COSC-2 which is hoped to penetrate the main décollement and the underlying Precambrian basement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/environmental-geophysics/seismic-methods','PESTICIDES'); return false;" href="https://www.epa.gov/environmental-geophysics/seismic-methods"><span><span class="hlt">Seismic</span> Methods</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p><span class="hlt">Seismic</span> methods are the most commonly conducted geophysical surveys for engineering investigations. <span class="hlt">Seismic</span> refraction provides engineers and geologists with the most basic of geologic data via simple procedures with common equipment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2006/1059/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2006/1059/"><span>Geologic <span class="hlt">interpretation</span> and multibeam bathymetry of the sea floor in southeastern Long Island Sound</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Poppe, Lawrence J.; Ackerman, Seth D.; Doran, Elizabeth F.; Moser, Marc S.; Stewart, Helen F.; Forfinski, Nicholas A.; Gardner, Uther L.; Keene, Jennifer A.</p> <p>2006-01-01</p> <p>Digital terrain models (DTMs) produced from multibeam echosounder (MBES) bathymetric data provide valuable base maps for marine geological <span class="hlt">interpretations</span> (e.g. Todd and others, 1999; Mosher and Thomson, 2002; ten Brink and others, 2004; Poppe and others, 2006a,b). These maps help define the geological variability of the sea floor (one of the primary controls of benthic habitat diversity); improve our understanding of the processes that control the distribution and transport of bottom sediments, the distribution of benthic habitats and associated infaunal community structures; and provide a detailed framework for future research, monitoring, and management activities. The bathymetric survey <span class="hlt">interpreted</span> herein (National Oceanic and Atmospheric Administration (NOAA) survey H11255) covers roughly 95 km? of sea floor in southeastern Long Island Sound (fig. 1). This bathymetry has been examined in relation to <span class="hlt">seismic</span> reflection data collected concurrently, as well as archived <span class="hlt">seismic</span> profiles acquired as part of a long-standing geologic mapping partnership between the State of Connecticut and the U.S. Geological Survey (USGS). The objective of this work was to use these geophysical data sets to <span class="hlt">interpret</span> geomorphological attributes of the sea floor in terms of the Quaternary geologic history and modern sedimentary processes within Long Island Sound.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAG...148..201M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAG...148..201M"><span>Integrated <span class="hlt">interpretation</span> of geophysical data of the Paleozoic structure in the northwestern part of the Siljan Ring impact crater, central Sweden</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muhamad, Harbe; Juhlin, Christopher; Malehmir, Alireza; Sopher, Daniel</p> <p>2018-01-01</p> <p>The Siljan Ring impact structure is the largest known impact structure in Europe and is Late Devonian in age. It contains a central uplift that is about 20-30 km in diameter and is surrounded by a ring-shaped depression. The Siljan area is one of the few areas in Sweden where the Paleozoic sequence has not been completely eroded, making it an important location for investigation of the geological and tectonic history of Baltica during the Paleozoic. The Paleozoic strata in this area also provide insight into the complex deformation processes associated with the impact. In this study we focus on the northwestern part of the Siljan Ring, close to the town of Orsa, with the main objective of characterizing the subsurface Paleozoic succession and uppermost Precambrian crystalline rocks along a series of <span class="hlt">seismic</span> reflection profiles, some of which have not previously been published. We combine these <span class="hlt">seismic</span> data with gravity and magnetic data and <span class="hlt">seismic</span> traveltime tomography results to produce an integrated <span class="hlt">interpretation</span> of the subsurface in the area. Our <span class="hlt">interpretation</span> shows that the Paleozoic sequence in this area is of a relatively constant thickness, with a total thickness typically between 300 and 500 m. Faulting appears to be predominantly extensional, which we <span class="hlt">interpret</span> to have occurred during the modification stage of the impact. Furthermore, based on the geophysical data in this area, we <span class="hlt">interpret</span> that the impact related deformation to differ in magnitude and style from other parts of the Siljan Ring.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1041187','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1041187"><span>Central and Eastern United States (CEUS) <span class="hlt">Seismic</span> Source Characterization (SSC) for Nuclear Facilities Project</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>Kevin J. Coppersmith; Lawrence A. Salomone; Chris W. Fuller</p> <p>2012-01-31</p> <p>This report describes a new <span class="hlt">seismic</span> source characterization (SSC) model for the Central and Eastern United States (CEUS). It will replace the <span class="hlt">Seismic</span> Hazard Methodology for the Central and Eastern United States, EPRI Report NP-4726 (July 1986) and the <span class="hlt">Seismic</span> Hazard Characterization of 69 Nuclear Plant Sites East of the Rocky Mountains, Lawrence Livermore National Laboratory Model, (Bernreuter et al., 1989). The objective of the CEUS SSC Project is to develop a new <span class="hlt">seismic</span> source model for the CEUS using a Senior <span class="hlt">Seismic</span> Hazard Analysis Committee (SSHAC) Level 3 assessment process. The goal of the SSHAC process is to representmore » the center, body, and range of technically defensible <span class="hlt">interpretations</span> of the available data, models, and methods. Input to a probabilistic <span class="hlt">seismic</span> hazard analysis (PSHA) consists of both <span class="hlt">seismic</span> source characterization and ground motion characterization. These two components are used to calculate probabilistic hazard results (or <span class="hlt">seismic</span> hazard curves) at a particular site. This report provides a new <span class="hlt">seismic</span> source model. Results and Findings The product of this report is a regional CEUS SSC model. This model includes consideration of an updated database, full assessment and incorporation of uncertainties, and the range of diverse technical <span class="hlt">interpretations</span> from the larger technical community. The SSC model will be widely applicable to the entire CEUS, so this project uses a ground motion model that includes generic variations to allow for a range of representative site conditions (deep soil, shallow soil, hard rock). Hazard and sensitivity calculations were conducted at seven test sites representative of different CEUS hazard environments. Challenges and Objectives The regional CEUS SSC model will be of value to readers who are involved in PSHA work, and who wish to use an updated SSC model. This model is based on a comprehensive and traceable process, in accordance with SSHAC guidelines in NUREG/CR-6372, Recommendations for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ExG....49....1Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ExG....49....1Y"><span><span class="hlt">Seismic</span> imaging for an ocean drilling site survey and its verification in the Izu rear arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamashita, Mikiya; Takahashi, Narumi; Tamura, Yoshihiko; Miura, Seiichi; Kodaira, Shuichi</p> <p>2018-01-01</p> <p>To evaluate the crustal structure of a site proposed for International Ocean Discovery Program drilling, the Japan Agency for Marine-Earth Science and Technology carried out <span class="hlt">seismic</span> surveys in the Izu rear arc between 2006 and 2008, using research vessels Kaiyo and Kairei. High-resolution dense grid surveys, consisting of three kinds of reflection surveys, generated clear <span class="hlt">seismic</span> profiles, together with a <span class="hlt">seismic</span> velocity image obtained from a <span class="hlt">seismic</span> refraction survey. In this paper, we compare the <span class="hlt">seismic</span> profiles with the geological column obtained from the drilling. Five volcaniclastic sedimentary units were identified in <span class="hlt">seismic</span> reflection profiles above the 5 km/s and 6 km/s contours of P-wave velocity obtained from the velocity image from the <span class="hlt">seismic</span> refraction survey. However, some of the unit boundaries <span class="hlt">interpreted</span> from the <span class="hlt">seismic</span> images were not recognised in the drilling core, highlighting the difficulties of geological target identification in volcanic regions from <span class="hlt">seismic</span> images alone. The geological core derived from drilling consisted of seven lithological units (labelled I to VII). Units I to V were aged at 0-9 Ma, and units VI and VII, from 1320-1806.5 m below seafloor (mbsf) had ages from 9 to ~15 Ma. The strong heterogeneity of volcanic sediments beneath the drilling site U1437 was also identified from coherence, calculated using cross-spectral analysis between grid survey lines. Our results suggest that use of a dense grid configuration is important in site surveys for ocean drilling in volcanic rear-arc situations, in order to recognise heterogeneous crustal structure, such as sediments from different origins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033856','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033856"><span>Rock formation characterization for CO2-EOR and carbon geosequestration; 3D <span class="hlt">seismic</span> amplitude and coherency anomalies, Wellington Field, Kansas, 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>Ohl, D.; Raef, A.; Watnef, L.; Bhattacharya, S.</p> <p>2011-01-01</p> <p>In this paper, we present a workflow for a Mississipian carbonates characterization case-study integrating post-stack <span class="hlt">seismic</span> attributes, well-logs porosities, and <span class="hlt">seismic</span> modeling to explore relating changes in small-scale "lithofacies" properties and/or sub-<span class="hlt">seismic</span> resolution faulting to key amplitude and coherency 3D <span class="hlt">seismic</span> attributes. The main objective of this study is to put emphasis on reservoir characterization that is both optimized for and subsequently benefiting from pilot tertiary CO2-EOR in preparation for future carbon geosequestration in a depleting reservoir and a deep saline aquifer. The extracted 3D <span class="hlt">seismic</span> coherency attribute indicated anomalous features that can be <span class="hlt">interpreted</span> as a lithofacies change or a sub-<span class="hlt">seismic</span> resolution faulting. A 2D finite difference modeling has been undertaken to understand and potentially build discriminant attributes to map structural and/or lithofacies anomalies of interest especially when embarking upon CO2-EOR and/or carbon sequestration monitoring and management projects. ?? 2011 Society of Exploration Geophysicists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022988','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022988"><span>A <span class="hlt">seismic</span> hazard uncertainty analysis for the New Madrid <span class="hlt">seismic</span> zone</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cramer, C.H.</p> <p>2001-01-01</p> <p>A review of the scientific issues relevant to characterizing earthquake sources in the New Madrid <span class="hlt">seismic</span> zone has led to the development of a logic tree of possible alternative parameters. A variability analysis, using Monte Carlo sampling of this consensus logic tree, is presented and discussed. The analysis shows that for 2%-exceedence-in-50-year hazard, the best-estimate <span class="hlt">seismic</span> hazard map is similar to previously published <span class="hlt">seismic</span> hazard maps for the area. For peak ground acceleration (PGA) and spectral acceleration at 0.2 and 1.0 s (0.2 and 1.0 s Sa), the coefficient of variation (COV) representing the knowledge-based uncertainty in <span class="hlt">seismic</span> hazard can exceed 0.6 over the New Madrid <span class="hlt">seismic</span> zone and diminishes to about 0.1 away from areas of <span class="hlt">seismic</span> activity. Sensitivity analyses show that the largest contributor to PGA, 0.2 and 1.0 s Sa <span class="hlt">seismic</span> hazard variability is the uncertainty in the location of future 1811-1812 New Madrid sized earthquakes. This is followed by the variability due to the choice of ground motion attenuation relation, the magnitude for the 1811-1812 New Madrid earthquakes, and the recurrence interval for M>6.5 events. <span class="hlt">Seismic</span> hazard is not very sensitive to the variability in seismogenic width and length. Published by Elsevier Science B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1480056','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1480056"><span><span class="hlt">Interpreting</span> Hypernymic Propositions in an Online Medical Encyclopedia</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Fiszman, Marcelo; Rindflesch, Thomas C.; Kilicoglu, Halil</p> <p>2003-01-01</p> <p><span class="hlt">Interpretation</span> of semantic propositions from biomedical texts documents would provide valuable support to natural language processing (NLP) applications. We are developing a methodology to <span class="hlt">interpret</span> a kind of semantic proposition, the hypernymic proposition, in MEDLINE <span class="hlt">abstracts</span>. In this paper, we expanded the system to identify these structures in a different discourse domain: the Medical Encyclopedia from the National Library of Medicine’s MEDLINEplus® Website. PMID:14728345</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('https://www.ncbi.nlm.nih.gov/pubmed/14728345','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14728345"><span><span class="hlt">Interpreting</span> hypernymic propositions in an online medical encyclopedia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fiszman, Marcelo; Rindflesch, Thomas C; Kilicoglu, Halil</p> <p>2003-01-01</p> <p><span class="hlt">Interpretation</span> of semantic propositions from bio-medical texts documents would provide valuable support to natural language processing (NLP) applications. We are developing a methodology to <span class="hlt">interpret</span> a kind of semantic proposition, the hypernymic proposition, in MEDLINE <span class="hlt">abstracts</span>. In this paper, we expanded the system to identify these structures in a different discourse domain: the Medical Encyclopedia from the National Library of Medi-cine's MEDLINEplus Website.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860003409','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860003409"><span>Small-scale convection beneath the transverse ranges, California: Implications for <span class="hlt">interpretation</span> of gravity anomalies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Humphreys, E. D.; Hager, B. H.</p> <p>1985-01-01</p> <p>Tomographic inversion of upper mantle P wave velocity heterogeneities beneath southern California shows two prominent features: an east-west trending curtain of high velocity material (up to 3% fast) in the upper 250 km beneath the Transverse Ranges and a region of low velocity material (up to 4% slow) in the 100 km beneath the Salton Trough. These <span class="hlt">seismic</span> velocity anomalies were <span class="hlt">interpreted</span> as due to small scale convection in the mantle. Using this hypothesis and assuming that temperature and density anomalies are linearly related to <span class="hlt">seismic</span> velocity anomalies through standard coefficients of proportionality, leads to inferred variations of approx. + or - 300 C and approx. + or - 0.03 g/cc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JAG...103..221O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JAG...103..221O"><span>Rock formation characterization for carbon dioxide geosequestration: 3D <span class="hlt">seismic</span> amplitude and coherency anomalies, and <span class="hlt">seismic</span> petrophysical facies classification, Wellington and Anson-Bates Fields, Kansas, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ohl, Derek; Raef, Abdelmoneam</p> <p>2014-04-01</p> <p>Higher resolution rock formation characterization is of paramount priority, amid growing interest in injecting carbon dioxide, CO2, into subsurface rock formations of depeleting/depleted hydrocarbon reservoirs or saline aquifers in order to reduce emissions of greenhouse gases. In this paper, we present a case study for a Mississippian carbonate characterization integrating post-stack <span class="hlt">seismic</span> attributes, well log porosities, and <span class="hlt">seismic</span> petrophysical facies classification. We evaluated changes in petrophysical lithofacies and reveal structural facies-controls in the study area. Three cross-plot clusters in a plot of well log porosity and acoustic impedance corroborated a Neural Network petrophysical facies classification, which was based on training and validation utilizing three petrophysically-different wells and three volume <span class="hlt">seismic</span> attributes, extracted from a time window including the wavelet of the reservoir-top reflection. Reworked lithofacies along small-throw faults has been revealed based on comparing coherency and <span class="hlt">seismic</span> petrophysical facies. The main objective of this study is to put an emphasis on reservoir characterization that is both optimized for and subsequently benefiting from pilot tertiary CO2 carbon geosequestration in a depleting reservoir and also in the deeper saline aquifer of the Arbuckle Group, south central Kansas. The 3D <span class="hlt">seismic</span> coherency attribute, we calculated from a window embracing the Mississippian top reflection event, indicated anomalous features that can be <span class="hlt">interpreted</span> as a change in lithofacies or faulting effect. An Artificial Neural Network (ANN) lithofacies modeling has been used to better understand these subtle features, and also provide petrophysical classes, which will benefit flow-simulation modeling and/or time-lapse <span class="hlt">seismic</span> monitoring feasibility analysis. This paper emphasizes the need of paying greater attention to small-scale features when embarking upon characterization of a reservoir or saline-aquifer for CO2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024188','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024188"><span>High-resolution image of Calaveras fault <span class="hlt">seismicity</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>Schaff, D.P.; Bokelmann, G.H.R.; Beroza, G.C.; Waldhauser, F.; Ellsworth, W.L.</p> <p>2002-01-01</p> <p>By measuring relative earthquake arrival times using waveform cross correlation and locating earthquakes using the double difference technique, we are able to reduce hypocentral errors by 1 to 2 orders of magnitude over routine locations for nearly 8000 events along a 35-km section of the Calaveras Fault. This represents ~92% of all <span class="hlt">seismicity</span> since 1984 and includes the rupture zone of the M 6.2 1984 Morgan Hill, California, earthquake. The relocated <span class="hlt">seismicity</span> forms highly organized structures that were previously obscured by location errors. There are abundant repeating earthquake sequences as well as linear clusters of earthquakes. Large voids in <span class="hlt">seismicity</span> appear with dimensions of kilometers that have been aseismic over the 30-year time interval, suggesting that these portions of the fault are either locked or creeping. The area of greatest slip in the Morgan Hill main shock coincides with the most prominent of these voids, suggesting that this part of the fault may be locked between large earthquakes. We find that the Calaveras Fault at depth is extremely thin, with an average upper bound on fault zone width of 75 m. Given the location error, however, this width is not resolvably different from zero. The relocations reveal active secondary faults, which we use to solve for the stress field in the immediate vicinity of the Calaveras Fault. We find that the maximum compressive stress is at a high angle, only 13 from the fault normal, supporting previous <span class="hlt">interpretations</span> that this fault is weak.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRB..121.5838R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRB..121.5838R"><span><span class="hlt">Seismic</span> moulin tremor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roeoesli, Claudia; Walter, Fabian; Ampuero, Jean-Paul; Kissling, Edi</p> <p>2016-08-01</p> <p>Through glacial moulins, meltwater is routed from the glacier surface to its base. Moulins are a main feature feeding subglacial drainage systems and thus influencing basal motion and ice dynamics, but their geometry remains poorly known. Here we show that analysis of the <span class="hlt">seismic</span> wavefield generated by water falling into a moulin can help constrain its geometry. We present modeling results of hour-long seimic tremors emitted from a vertical moulin shaft, observed with a seismometer array installed at the surface of the Greenland Ice Sheet. The tremor was triggered when the moulin water level exceeded a certain height, which we associate with the threshold for the waterfall to hit directly the surface of the moulin water column. The amplitude of the tremor signal changed over each tremor episode, in close relation to the amount of inflowing water. The tremor spectrum features multiple prominent peaks, whose characteristic frequencies are distributed like the resonant modes of a semiopen organ pipe and were found to depend on the moulin water level, consistent with a source composed of resonant tube waves (water pressure waves coupled to elastic deformation of the moulin walls) along the water-filled moulin pipe. Analysis of surface particle motions lends further support to this <span class="hlt">interpretation</span>. The <span class="hlt">seismic</span> wavefield was modeled as a superposition of sustained wave radiation by pressure sources on the side walls and at the bottom of the moulin. The former was found to dominate the wave field at close distance and the latter at large distance to the moulin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18.2149V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18.2149V"><span><span class="hlt">Seismic</span> structure and segmentation of the axial valley of the Mid-Cayman Spreading Center</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Van Avendonk, Harm J. A.; Hayman, Nicholas W.; Harding, Jennifer L.; Grevemeyer, Ingo; Peirce, Christine; Dannowski, Anke</p> <p>2017-06-01</p> <p>We report the results of a two-dimensional tomographic inversion of marine <span class="hlt">seismic</span> refraction data from an array of ocean-bottom seismographs (OBSs), which produced an image of the crustal structure along the axial valley of the ultraslow spreading Mid-Cayman Spreading Center (MCSC). The <span class="hlt">seismic</span> velocity model shows variations in the thickness and properties of the young oceanic crust that are consistent with the existence of two magmatic-tectonic segments along the 110 km long spreading center. <span class="hlt">Seismic</span> wave speeds are consistent with exhumed mantle at the boundary between these two segments, but changes in the vertical gradient of <span class="hlt">seismic</span> velocity suggest that volcanic crust occupies most of the axial valley seafloor along the <span class="hlt">seismic</span> transect. The two spreading segments both have a low-velocity zone (LVZ) several kilometers beneath the seafloor, which may indicate the presence of shallow melt. However, the northern segment also has low <span class="hlt">seismic</span> velocities (3 km/s) in a thick upper crustal layer (1.5-2.0 km), which we <span class="hlt">interpret</span> as an extrusive volcanic section with high porosity and permeability. This segment hosts the Beebe vent field, the deepest known high-temperature black smoker hydrothermal vent system. In contrast, the southern spreading segment has <span class="hlt">seismic</span> velocities as high as 4.0 km/s near the seafloor. We suggest that the porosity and permeability of the volcanic crust in the southern segment are much lower, thus limiting deep seawater penetration and hydrothermal recharge. This may explain why no hydrothermal vent system has been found in the southern half of the MCSC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAESc.143..343P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAESc.143..343P"><span>Subsurface structural <span class="hlt">interpretation</span> by applying trishear algorithm: An example from the Lenghu5 fold-and-thrust belt, Qaidam Basin, Northern Tibetan Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pei, Yangwen; Paton, Douglas A.; Wu, Kongyou; Xie, Liujuan</p> <p>2017-08-01</p> <p>The application of trishear algorithm, in which deformation occurs in a triangle zone in front of a propagating fault tip, is often used to understand fault related folding. In comparison to kink-band methods, a key characteristic of trishear algorithm is that non-uniform deformation within the triangle zone allows the layer thickness and horizon length to change during deformation, which is commonly observed in natural structures. An example from the Lenghu5 fold-and-thrust belt (Qaidam Basin, Northern Tibetan Plateau) is <span class="hlt">interpreted</span> to help understand how to employ trishear forward modelling to improve the accuracy of <span class="hlt">seismic</span> <span class="hlt">interpretation</span>. High resolution fieldwork data, including high-angle dips, 'dragging structures', thinning hanging-wall and thickening footwall, are used to determined best-fit trishear model to explain the deformation happened to the Lenghu5 fold-and-thrust belt. We also consider the factors that increase the complexity of trishear models, including: (a) fault-dip changes and (b) pre-existing faults. We integrate fault dip change and pre-existing faults to predict subsurface structures that are apparently under <span class="hlt">seismic</span> resolution. The analogue analysis by trishear models indicates that the Lenghu5 fold-and-thrust belt is controlled by an upward-steepening reverse fault above a pre-existing opposite-thrusting fault in deeper subsurface. The validity of the trishear model is confirmed by the high accordance between the model and the high-resolution fieldwork. The validated trishear forward model provides geometric constraints to the faults and horizons in the <span class="hlt">seismic</span> section, e.g., fault cutoffs and fault tip position, faults' intersecting relationship and horizon/fault cross-cutting relationship. The subsurface prediction using trishear algorithm can significantly increase the accuracy of <span class="hlt">seismic</span> <span class="hlt">interpretation</span>, particularly in <span class="hlt">seismic</span> sections with low signal/noise ratio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S43F..08M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S43F..08M"><span>Using <span class="hlt">Seismic</span> Interferometry to Investigate <span class="hlt">Seismic</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>Matzel, E.; Morency, C.; Templeton, D. C.</p> <p>2017-12-01</p> <p><span class="hlt">Seismicity</span> provides a direct means of measuring the physical characteristics of active tectonic features such as fault zones. Hundreds of small earthquakes often occur along a fault during a <span class="hlt">seismic</span> swarm. This <span class="hlt">seismicity</span> helps define the tectonically active region. When processed using novel geophysical techniques, we can isolate the energy sensitive to the fault, itself. Here we focus on two methods of <span class="hlt">seismic</span> interferometry, ambient noise correlation (ANC) and the virtual seismometer method (VSM). ANC is based on the observation that the Earth's background noise includes coherent energy, which can be recovered by observing over long time periods and allowing the incoherent energy to cancel out. The cross correlation of ambient noise between a pair of stations results in a waveform that is identical to the seismogram that would result if an impulsive source located at one of the stations was recorded at the other, the Green function (GF). The calculation of the GF is often stable after a few weeks of continuous data correlation, any perturbations to the GF after that point are directly related to changes in the subsurface and can be used for 4D monitoring.VSM is a style of <span class="hlt">seismic</span> interferometry that provides fast, precise, high frequency estimates of the Green's function (GF) between earthquakes. VSM illuminates the subsurface precisely where the pressures are changing and has the potential to image the evolution of <span class="hlt">seismicity</span> over time, including changes in the style of faulting. With hundreds of earthquakes, we can calculate thousands of waveforms. At the same time, VSM collapses the computational domain, often by 2-3 orders of magnitude. This allows us to do high frequency 3D modeling in the fault region. Using data from a swarm of earthquakes near the Salton Sea, we demonstrate the power of these techniques, illustrating our ability to scale from the far field, where sources are well separated, to the near field where their locations fall within each other</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2004/1242/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2004/1242/"><span>Hawaiian volcano observatory summary 103; Part I, <span class="hlt">seismic</span> data, January to December 2003</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakata, Jennifer S.; Heliker, C.; Orr, T.; Hoblitt, R.</p> <p>2004-01-01</p> <p>The Hawaiian Volcano Observatory (HVO) summary presents <span class="hlt">seismic</span> data gathered during the year and a chronological narrative describing the volcanic events. The <span class="hlt">seismic</span> summary is offered without <span class="hlt">interpretation</span> as a source of preliminary data. It is complete in the sense that most data for events of M= 1.5 routinely gathered by the Observatory are included. The emphasis in collection of tilt and deformation data has shifted from quarterly measurements at a few water-tube tilt stations ('wet' tilt) to a larger number of continuously recording borehole tiltmeters, repeated measurements at numerous spirit-level tilt stations ('dry' tilt), and surveying of level and trilateration networks. Because of the large quantity of deformation data now gathered and differing schedules of data reduction, the <span class="hlt">seismic</span> and deformation summaries are published separately. The HVO summaries have been published in various forms since 1956. Summaries prior to 1974 were issued quarterly, but cost, convenience of preparation and distribution, and the large quantities of data dictated an annual publication beginning with Summary 74 for the year 1974. Summary 86 (the introduction of CUSP at HVO) includes a description of the <span class="hlt">seismic</span> instrumentation, calibration, and processing used in recent years. The present summary includes background information on the <span class="hlt">seismic</span> network and processing to allow use of the data and to provide an understanding of how they were gathered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2001/0332/pdf/of01-332.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2001/0332/pdf/of01-332.pdf"><span>Hawaiian Volcano Observatory summary 100; Part 1, <span class="hlt">seismic</span> data, January to December 2000</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakata, Jennifer S.</p> <p>2001-01-01</p> <p>The Hawaiian Volcano Observatory (HVO) summary presents <span class="hlt">seismic</span> data gathered during the year and a chronological narrative describing the volcanic events. The <span class="hlt">seismic</span> summary is offered without <span class="hlt">interpretation</span> as a source of preliminary data. It is complete in the sense that all data for events of M≥1.5 routinely gathered by the Observatory are included. The emphasis in collection of tilt and deformation data has shifted from quarterly measurements at a few water-tube tilt stations (“wet” tilt) to a larger number of continuously recording borehole tiltmeters, repeated measurements at numerous spirit-level tilt stations (“dry” tilt), and surveying of level and trilateration networks. Because of the large quantity of deformation data now gathered and differing schedules of data reduction, the <span class="hlt">seismic</span> and deformation summaries are published separately. The HVO summaries have been published in various forms since 1956. Summaries prior to 1974 were issued quarterly, but cost, convenience of preparation and distribution, and the large quantities of data dictated an annual publication beginning with Summary 74 for the year 1974. Summary 86 (the introduction of CUSP at HVO) includes a description of the <span class="hlt">seismic</span> instrumentation, calibration, and processing used in recent years. The present summary includes enough background information on the <span class="hlt">seismic</span> network and processing to allow use of the data and to provide an understanding of how they were gathered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2002/0157/pdf/of02-157.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2002/0157/pdf/of02-157.pdf"><span>Hawaiian Volcano Observatory summary 101: Part 1, <span class="hlt">seismic</span> data, January to December 2001</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nakata, Jennifer S.; Chronological summary by Heliker, C.</p> <p>2002-01-01</p> <p>The Hawaiian Volcano Observatory (HVO) summary presents <span class="hlt">seismic</span> data gathered during the year and a chronological narrative describing the volcanic events. The <span class="hlt">seismic</span> summary is offered without <span class="hlt">interpretation</span> as a source of preliminary data. It is complete in the sense that all data for events of M>1.5 routinely gathered by the Observatory are included. The emphasis in collection of tilt and deformation data has shifted from quarterly measurements at a few water-tube tilt stations ("wet" tilt) to a larger number of continuously recording borehole tiltmeters, repeated measurements at numerous spirit-level tilt stations ("dry" tilt), and surveying of level and trilateration networks. Because of the large quantity of deformation data now gathered and differing schedules of data reduction, the <span class="hlt">seismic</span> and deformation summaries are published separately. The HVO summaries have been published in various forms since 1956. Summaries prior to 1974 were issued quarterly, but cost, convenience of preparation and distribution, and the large quantities of data dictated an annual publication beginning with Summary 74 for the year 1974. Summary 86 (the introduction of CUSP at HVO) includes a description of the <span class="hlt">seismic</span> instrumentation, calibration, and processing used in recent years. The present summary includes enough background information on the <span class="hlt">seismic</span> network and processing to allow use of the data and to provide an understanding of how they were gathered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007SPIE.6562E..0RW','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007SPIE.6562E..0RW"><span>Acoustic/<span class="hlt">seismic</span> signal propagation and sensor performance modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, D. Keith; Marlin, David H.; Mackay, Sean</p> <p>2007-04-01</p> <p>Performance, optimal employment, and <span class="hlt">interpretation</span> of data from acoustic and <span class="hlt">seismic</span> sensors depend strongly and in complex ways on the environment in which they operate. Software tools for guiding non-expert users of acoustic and <span class="hlt">seismic</span> sensors are therefore much needed. However, such tools require that many individual components be constructed and correctly connected together. These components include the source signature and directionality, representation of the atmospheric and terrain environment, calculation of the signal propagation, characterization of the sensor response, and mimicking of the data processing at the sensor. Selection of an appropriate signal propagation model is particularly important, as there are significant trade-offs between output fidelity and computation speed. Attenuation of signal energy, random fading, and (for array systems) variations in wavefront angle-of-arrival should all be considered. Characterization of the complex operational environment is often the weak link in sensor modeling: important issues for acoustic and <span class="hlt">seismic</span> modeling activities include the temporal/spatial resolution of the atmospheric data, knowledge of the surface and subsurface terrain properties, and representation of ambient background noise and vibrations. Design of software tools that address these challenges is illustrated with two examples: a detailed target-to-sensor calculation application called the Sensor Performance Evaluator for Battlefield Environments (SPEBE) and a GIS-embedded approach called Battlefield Terrain Reasoning and Awareness (BTRA).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoJI.200.1172B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoJI.200.1172B"><span>Induced <span class="hlt">seismicity</span> constraints on subsurface geological structure, Paradox Valley, Colorado</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Block, Lisa V.; Wood, Christopher K.; Yeck, William L.; King, Vanessa M.</p> <p>2015-02-01</p> <p>Precise relative hypocentres of <span class="hlt">seismic</span> events induced by long-term fluid injection at the Paradox Valley Unit (PVU) brine disposal well provide constraints on the subsurface geological structure and compliment information available from deep <span class="hlt">seismic</span> reflection and well data. We use the 3-D spatial distribution of the hypocentres to refine the locations, strikes, and throws of subsurface faults interpre­ted previously from geophysical surveys and to infer the existence of previously unidentified subsurface faults. From distinct epicentre lineations and focal mechanism trends, we identify a set of conjugate fracture orientations consistent with shear-slip reactivation of late-Palaeozoic fractures over a widespread area, as well as an additional fracture orientation present only near the injection well. We propose simple Mohr-Coulomb fracture models to explain these observations. The observation that induced <span class="hlt">seismicity</span> preferentially occurs along one of the identified conjugate fracture orientations can be explained by a rotation in the direction of the regional maximum compressive stress from the time when the fractures were formed to the present. Shear slip along the third fracture orientation observed near the injection well is inconsistent with the current regional stress field and suggests a local rotation of the horizontal stresses. The detailed subsurface model produced by this analysis provides important insights for anticipating spatial patterns of future induced <span class="hlt">seismicity</span> and for evaluation of possible additional injection well sites that are likely to be <span class="hlt">seismically</span> and hydrologically isolated from the current well. In addition, the <span class="hlt">interpreted</span> fault patterns provide constraints for estimating the maximum magnitude earthquake that may be induced, and for building geomechanical models to simulate pore pressure diffusion, stress changes and earthquake triggering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814120S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814120S"><span><span class="hlt">Seismic</span> wave propagation through an extrusive basalt sequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sanford, Oliver; Hobbs, Richard; Brown, Richard; Schofield, Nick</p> <p>2016-04-01</p> <p>Layers of basalt flows within sedimentary successions (e.g. in the Faeroe-Shetland Basin) cause complex scattering and attenuation of <span class="hlt">seismic</span> waves during <span class="hlt">seismic</span> exploration surveys. Extrusive basaltic sequences are highly heterogeneous and contain strong impedance contrasts between higher velocity crystalline flow cores (˜6 km s-1) and the lower velocity fragmented and weathered flow crusts (3-4 km s-1). Typically, the refracted wave from the basaltic layer is used to build a velocity model by tomography. This velocity model is then used to aid processing of the reflection data where direct determination of velocity is ambiguous, or as a starting point for full waveform inversion, for example. The model may also be used as part of assessing drilling risk of potential wells, as it is believed to constrain the total thickness of the sequence. In heterogeneous media, where the scatter size is of the order of the <span class="hlt">seismic</span> wavelength or larger, scattering preferentially traps the <span class="hlt">seismic</span> energy in the low velocity regions. This causes a build-up of energy that is guided along the low velocity layers. This has implications for the <span class="hlt">interpretation</span> of the observed first arrival of the <span class="hlt">seismic</span> wave, which may be a biased towards the low velocity regions. This will then lead to an underestimate of the velocity structure and hence the thickness of the basalt, with implications for the drilling of wells hoping to penetrate through the base of the basalts in search of hydrocarbons. Using 2-D acoustic finite difference modelling of the guided wave through a simple layered basalt sequence, we consider the relative importance of different parameters of the basalt on the <span class="hlt">seismic</span> energy propagating through the layers. These include the proportion of high to low velocity material, the number of layers, their thickness and the roughness of the interfaces between the layers. We observe a non-linear relationship between the ratio of high to low velocity layers and the apparent velocity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/835546','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/835546"><span>NON-INVASIVE DETERMINATION OF THE LOCATION AND DISTRBUTION OF FREE-PHASE DENSE NONAQUEOUS PHASE LIQUIDS (DNAPL) BY <span class="hlt">SEISMIC</span> REFLECTION TECHNIQUES</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>Michael G. Waddell; William J. Domoracki; Jerome Eyer</p> <p>2003-01-01</p> <p>The Earth Sciences and Resources Institute, University of South Carolina is conducting a proof of concept study to determine the location and distribution of subsurface DNAPL carbon tetrachloride (CCl{sub 4}) contamination at the 216-Z-9 crib, 200 West area, DOE Hanford Site, Washington by use of two-dimensional high-resolution <span class="hlt">seismic</span> reflection surveys and borehole geophysical data. The study makes use of recent advances in <span class="hlt">seismic</span> reflection amplitude versus offset (AVO) technology to directly detect the presence of subsurface DNAPL. The techniques proposed are noninvasive means of site characterization and direct free-phase DNAPL detection. This final report covers the results of Tasks 1,more » 2, and 3. Task (1) contains site evaluation and <span class="hlt">seismic</span> modeling studies. The site evaluation consists of identifying and collecting preexisting geological and geophysical information regarding subsurface structure and the presence and quantity of DNAPL. The <span class="hlt">seismic</span> modeling studies were undertaken to determine the likelihood that an AVO response exists and its probable manifestation. Task (2) is the design and acquisition of 2-D <span class="hlt">seismic</span> reflection data to image areas of probable high concentration of DNAPL. Task (3) is the processing and <span class="hlt">interpretation</span> of the 2-D data. During the commission of these tasks four <span class="hlt">seismic</span> reflection profiles were collected. Subsurface velocity information was obtained by vertical <span class="hlt">seismic</span> profile surveys in three wells. The <span class="hlt">interpretation</span> of these data is in two parts. Part one is the construction and <span class="hlt">interpretation</span> of structural contour maps of the contact between the Hanford Fine unit and the underlying Plio/Pleistocene unit and of the contact between the Plio/Pleistocene unit and the underlying caliche layer. These two contacts were determined to be the most likely surfaces to contain the highest concentration CCl{sub 4}. Part two of the <span class="hlt">interpretation</span> uses the results of the AVO modeling to locate any <span class="hlt">seismic</span> amplitude anomalies that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991ESRv...31...11P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991ESRv...31...11P"><span>Geomorphology and <span class="hlt">seismic</span> risk</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panizza, Mario</p> <p>1991-07-01</p> <p>The author analyses the contributions provided by geomorphology in studies suited to the assessment of <span class="hlt">seismic</span> risk: this is defined as function of the <span class="hlt">seismic</span> hazard, of the <span class="hlt">seismic</span> susceptibility, and of the vulnerability. The geomorphological studies applicable to <span class="hlt">seismic</span> risk assessment can be divided into two sectors: (a) morpho-neotectonic investigations conducted to identify active tectonic structures; (b) geomorphological and morphometric analyses aimed at identifying the particular situations that amplify or reduce <span class="hlt">seismic</span> susceptibility. The morpho-neotectonic studies lead to the identification, selection and classification of the lineaments that can be linked with active tectonic structures. The most important geomorphological situations that can condition <span class="hlt">seismic</span> susceptibility are: slope angle, debris, morphology, degradational slopes, paleo-landslides and underground cavities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1862c0180H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1862c0180H"><span>Integrated <span class="hlt">seismic</span> stochastic inversion and multi-attributes to delineate reservoir distribution: Case study MZ fields, Central Sumatra Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haris, A.; Novriyani, M.; Suparno, S.; Hidayat, R.; Riyanto, A.</p> <p>2017-07-01</p> <p>This study presents the integration of <span class="hlt">seismic</span> stochastic inversion and multi-attributes for delineating the reservoir distribution in term of lithology and porosity in the formation within depth interval between the Top Sihapas and Top Pematang. The method that has been used is a stochastic inversion, which is integrated with multi-attribute <span class="hlt">seismic</span> by applying neural network Probabilistic Neural Network (PNN). Stochastic methods are used to predict the probability mapping sandstone as the result of impedance varied with 50 realizations that will produce a good probability. Analysis of Stochastic <span class="hlt">Seismic</span> Tnversion provides more <span class="hlt">interpretive</span> because it directly gives the value of the property. Our experiment shows that AT of stochastic inversion provides more diverse uncertainty so that the probability value will be close to the actual values. The produced AT is then used for an input of a multi-attribute analysis, which is used to predict the gamma ray, density and porosity logs. To obtain the number of attributes that are used, stepwise regression algorithm is applied. The results are attributes which are used in the process of PNN. This PNN method is chosen because it has the best correlation of others neural network method. Finally, we <span class="hlt">interpret</span> the product of the multi-attribute analysis are in the form of pseudo-gamma ray volume, density volume and volume of pseudo-porosity to delineate the reservoir distribution. Our <span class="hlt">interpretation</span> shows that the structural trap is identified in the southeastern part of study area, which is along the anticline.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MsT..........1V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MsT..........1V"><span>Near-Surface and High Resolution <span class="hlt">Seismic</span> Imaging of the Bennett Thrust Fault in the Indio Mountains of West Texas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vennemann, Alan</p> <p></p> <p>My research investigates the structure of the Indio Mountains in southwest Texas, 34 kilometers southwest of Van Horn, at the UTEP (University of Texas at El Paso) Field Station using newly acquired active-source <span class="hlt">seismic</span> data. The area is underlain by deformed Cretaceous sedimentary rocks that represent a transgressive sequence nearly 2 km in total stratigraphic thickness. The rocks were deposited in mid Cretaceous extensional basins and later contracted into fold-thrust structures during Laramide orogenesis. The stratigraphic sequence is an analog for similar areas that are ideal for pre-salt petroleum reservoirs, such as reservoirs off the coasts of Brazil and Angola (Li, 2014; Fox, 2016; Kattah, 2017). The 1-km-long 2-D shallow <span class="hlt">seismic</span> reflection survey that I planned and led during May 2016 was the first at the UTEP Field Station, providing critical subsurface information that was previously lacking. The data were processed with Landmark ProMAX <span class="hlt">seismic</span> processing software to create a <span class="hlt">seismic</span> reflection image of the Bennett Thrust Fault and additional imbricate faulting not expressed at the surface. Along the 1-km line, reflection data were recorded with 200 4.5 Hz geophones, using 100 150-gram explosive charges and 490 sledge-hammer blows for sources. A <span class="hlt">seismic</span> reflection profile was produced using the lower frequency explosive dataset, which was used in the identification of the Bennett Thrust Fault and additional faulting and folding in the subsurface. This dataset provides three possible <span class="hlt">interpretations</span> for the subsurface geometries of the faulting and folding present. However, producing a <span class="hlt">seismic</span> reflection image with the higher frequency sledge-hammer sourced dataset for <span class="hlt">interpretation</span> proved more challenging. While there are no petroleum plays in the Indio Mountains region, imaging and understanding subsurface structural and lithological geometries and how that geometry directs potential fluid flow has implications for other regions with petroleum plays.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.S52A..02P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.S52A..02P"><span><span class="hlt">Seismic</span> sequences in the Sombrero <span class="hlt">Seismic</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>Pulliam, J.; Huerfano, V. A.; ten Brink, U.; von Hillebrandt, C.</p> <p>2007-05-01</p> <p>The northeastern Caribbean, in the vicinity of Puerto Rico and the Virgin Islands, has a long and well-documented history of devastating earthquakes and tsunamis, including major events in 1670, 1787, 1867, 1916, 1918, and 1943. Recently, <span class="hlt">seismicity</span> has been concentrated to the north and west of the British Virgin Islands, in the region referred to as the Sombrero <span class="hlt">Seismic</span> Zone by the Puerto Rico <span class="hlt">Seismic</span> Network (PRSN). In the combined <span class="hlt">seismicity</span> catalog maintained by the PRSN, several hundred small to moderate magnitude events can be found in this region prior to 2006. However, beginning in 2006 and continuing to the present, the rate of <span class="hlt">seismicity</span> in the Sombrero suddenly increased, and a new locus of activity developed to the east of the previous location. Accurate estimates of <span class="hlt">seismic</span> hazard, and the tsunamigenic potential of <span class="hlt">seismic</span> events, depend on an accurate and comprehensive understanding of how strain is being accommodated in this corner region. Are faults locked and accumulating strain for release in a major event? Or is strain being released via slip over a diffuse system of faults? A careful analysis of <span class="hlt">seismicity</span> patterns in the Sombrero region has the potential to both identify faults and modes of failure, provided the aggregation scheme is tuned to properly identify related events. To this end, we experimented with a scheme to identify <span class="hlt">seismic</span> sequences based on physical and temporal proximity, under the assumptions that (a) events occur on related fault systems as stress is refocused by immediately previous events and (b) such 'stress waves' die out with time, so that two events that occur on the same system within a relatively short time window can be said to have a similar 'trigger' in ways that two nearby events that occurred years apart cannot. Patterns that emerge from the identification, temporal sequence, and refined locations of such sequences of events carry information about stress accommodation that is obscured by large clouds of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6635151-seismic-data-field-development-landslide-field-case-study','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6635151-seismic-data-field-development-landslide-field-case-study"><span>3-D <span class="hlt">seismic</span> data for field development: Landslide field case study</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>Raeuchle, S.K.; Carr, T.R.; Tucker, R.D.</p> <p>1990-05-01</p> <p>The Landslide field is located on the extreme southern flank of the San Joaquin basin, approximately 25 mi south of Bakersfield, California. The field, discovered in 1985, has produced in excess 9 million bbl of oil with an estimated ultimate recovery of more than 13 MMBO. The Miocene Stevens sands, which form the reservoir units at Landslide field, are <span class="hlt">interpreted</span> as a series of constructional submarine fan deposits. Deposition of the fans was controlled by paleotopography with an abrupt updip pinch-out of the sands to the southwest. The three-dimensional <span class="hlt">seismic</span> data over the field was used to locate the bottommore » hole of the landslide 22X-30 development well as close to this abrupt updip pinchout as possible in order to maximize oil recovery. A location was selected two traces (330 ft) from the updip pinch-out as mapped on the <span class="hlt">seismic</span> data. The well was successfully drilled during 1989, encountering 150 ft of net sand with initial production in excess of 1,500 bbl of oil/day. A pressure buildup test indicates the presence of a boundary approximately 200 ft from the well bore. This boundary is <span class="hlt">interpreted</span> as the updip pinchout of the Stevens sands against the paleohigh. Based on examination of changes in amplitude, the absence or presence of reservoir-quality sand can be mapped across the paleohighs. Application of three-dimensional <span class="hlt">seismic</span> data, integration with well data, and in particular reconstruction cuts tied closely to existing wells can be used to map the ultimate extent of the field and contribute to efficient development.« less</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://seismic.alaska.gov','SCIGOVWS'); return false;" href="http://seismic.alaska.gov"><span>Alaska <span class="hlt">Seismic</span> Hazards Safety Commission</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>State Employees ASHSC State of Alaska search Alaska <span class="hlt">Seismic</span> Hazards <em>Safety</em> Commission View of Anchorage and Commissions Alaska <span class="hlt">Seismic</span> Hazards <em>Safety</em> Commission (ASHSC) main contant Alaska <span class="hlt">Seismic</span> Hazards <em>Safety</em> Commission logo Alaska <span class="hlt">Seismic</span> Hazards <em>Safety</em> Commission (ASHSC) - Mission The Alaska <span class="hlt">Seismic</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1434051','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1434051"><span>Gas hydrate characterization from a 3D <span class="hlt">seismic</span> dataset in the deepwater eastern Gulf of Mexico</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>McConnell, Daniel; Haneberg, William C.</p> <p></p> <p><span class="hlt">Seismic</span> stratigraphic features are delineated using principal component analysis of the band limited data at potential gas hydrate sands, and compared and calibrated with spectral decomposition thickness to constrain thickness in the absence of well control. Layers in the abyssal fan sediments are thinner than can be resolved with 50 Hz <span class="hlt">seismic</span> and thus comprise composite thin-bed reflections. Amplitude vs frequency analysis are used to indicate gas and gas hydrate reflections. Synthetic <span class="hlt">seismic</span> wedge models show that with 50Hz <span class="hlt">seismic</span> data, a 40% saturation of a Plio Pleistocene GoM sand in the hydrate stability zone with no subjacent gas canmore » produce a phase change (negative to positive) with a strong correlation between amplitude and hydrate saturation. The synthetic <span class="hlt">seismic</span> response is more complicated if the gas hydrate filled sediments overlie gassy sediments. Hydrate (or gas) saturation in thin beds enhances the amplitude response and can be used to estimate saturation. Gas hydrate saturation from rock physics, amplitude, and frequency analysis is compared to saturation derived from inversion at several <span class="hlt">interpreted</span> gas hydrate accumulations in the eastern Gulf of Mexico.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012620','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012620"><span><span class="hlt">Seismic</span> gaps and source zones of recent large earthquakes in coastal Peru</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dewey, J.W.; Spence, W.</p> <p>1979-01-01</p> <p>The earthquakes of central coastal Peru occur principally in two distinct zones of shallow earthquake activity that are inland of and parallel to the axis of the Peru Trench. The interface-thrust (IT) zone includes the great thrust-fault earthquakes of 17 October 1966 and 3 October 1974. The coastal-plate interior (CPI) zone includes the great earthquake of 31 May 1970, and is located about 50 km inland of and 30 km deeper than the interface thrust zone. The occurrence of a large earthquake in one zone may not relieve elastic strain in the adjoining zone, thus complicating the application of the <span class="hlt">seismic</span> gap concept to central coastal Peru. However, recognition of two <span class="hlt">seismic</span> zones may facilitate detection of <span class="hlt">seismicity</span> precursory to a large earthquake in a given zone; removal of probable CPI-zone earthquakes from plots of <span class="hlt">seismicity</span> prior to the 1974 main shock dramatically emphasizes the high <span class="hlt">seismic</span> activity near the rupture zone of that earthquake in the five years preceding the main shock. Other conclusions on the <span class="hlt">seismicity</span> of coastal Peru that affect the application of the <span class="hlt">seismic</span> gap concept to this region are: (1) Aftershocks of the great earthquakes of 1966, 1970, and 1974 occurred in spatially separated clusters. Some clusters may represent distinct small source regions triggered by the main shock rather than delimiting the total extent of main-shock rupture. The uncertainty in the <span class="hlt">interpretation</span> of aftershock clusters results in corresponding uncertainties in estimates of stress drop and estimates of the dimensions of the <span class="hlt">seismic</span> gap that has been filled by a major earthquake. (2) Aftershocks of the great thrust-fault earthquakes of 1966 and 1974 generally did not extend seaward as far as the Peru Trench. (3) None of the three great earthquakes produced significant teleseismic activity in the following month in the source regions of the other two earthquakes. The earthquake hypocenters that form the basis of this study were relocated using station</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010PhDT........74T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010PhDT........74T"><span><span class="hlt">Seismic</span> investigation of the southern Rio Grande Rift</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thompson, Lennox E.</p> <p></p> <p>Competing models exist to explain what caused the Earth's crust to spread apart 29 million years ago to create a region known today as the Rio Grande Rift (RGR). The RGR extends from central Colorado through New Mexico to northern Mexico, near El Paso. The RGR has different geologic features that distinguish it from most other valleys (e.g., the RGR was not cut by a river nor does a river branch upstream). A growing body of evidence shows that geologic activity still occurs in the RGR, with a continuation of faulting, <span class="hlt">seismicity</span> and widening at a small rate of about 0.3 mm/yr (Woodward , 1977). We map of the <span class="hlt">seismic</span> velocity structure and crustal thickness using data from the Rio Grande Rift <span class="hlt">Seismic</span> TRAnsect (RISTRA) experiment and the EarthScope Transportable Array (USArray) dataset. In addition to the data we collected from the RISTRA experiment and USArray dataset, we also acquired receiver functions from the EarthScope Automatic Receiver Survey (EARS) website (http://www.earthscope.org/data) and waveform data from the Incorporated Research Institutes for Seismology (IRIS) Data Management Center (DMC). We requested seismograms from the IRIS DMC database where we acquired teleseismic events from Jan 2000 to Dec 2009. This includes 7,259 <span class="hlt">seismic</span> events with a minimum magnitude of 5.5 and 106,389 continuous waveforms. This data was preprocessed (merged, rotated) using a program called Standing Order of Data (SOD). The RISTRA experiment and the USArray were designed to image crust and mantle structures by computing receiver functions for all data in the Southern Rio Grande Rift (SRGR). We map the crustal thickness, <span class="hlt">seismic</span> velocity, and mantle structure for the sole purpose to better determine the nature of tectonic activity that is presently taking place and further investigate the regional extension of the Southern Rio Grande Rift (SRGR). Here we present preliminary results of the crustal and velocity structure using the kriging interpolation scheme seem stable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S23C4501S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S23C4501S"><span>Tectonic Inversion Along the Algerian and Ligurian Margins: On the Insight Provided By Latest <span class="hlt">Seismic</span> Processing Techniques Applied to Recent and Vintage 2D Offshore Multichannel <span class="hlt">Seismic</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>Schenini, L.; Beslier, M. O.; Sage, F.; Badji, R.; Galibert, P. Y.; Lepretre, A.; Dessa, J. X.; Aidi, C.; Watremez, L.</p> <p>2014-12-01</p> <p>Recent studies on the Algerian and the North-Ligurian margins in the Western Mediterranean have evidenced inversion-related superficial structures, such as folds and asymmetric sedimentary perched basins whose geometry hints at deep compressive structures dipping towards the continent. Deep <span class="hlt">seismic</span> imaging of these margins is difficult due to steep slope and superficial multiples, and, in the Mediterranean context, to the highly diffractive Messinian evaporitic series in the basin. During the Algerian-French SPIRAL survey (2009, R/V Atalante), 2D marine multi-channel <span class="hlt">seismic</span> (MCS) reflection data were collected along the Algerian Margin using a 4.5 km, 360 channel digital streamer and a 3040 cu. in. air-gun array. An advanced processing workflow has been laid out using Geocluster CGG software, which includes noise attenuation, 2D SRME multiple attenuation, surface consistent deconvolution, Kirchhoff pre-stack time migration. This processing produces satisfactory <span class="hlt">seismic</span> images of the whole sedimentary cover, and of southward dipping reflectors in the acoustic basement along the central part of the margin offshore Great Kabylia, that are <span class="hlt">interpreted</span> as inversion-related blind thrusts as part of flat-ramp systems. We applied this successful processing workflow to old 2D marine MCS data acquired on the North-Ligurian Margin (Malis survey, 1995, R/V Le Nadir), using a 2.5 km, 96 channel streamer and a 1140 cu. in. air-gun array. Particular attention was paid to multiple attenuation in adapting our workflow. The resulting reprocessed <span class="hlt">seismic</span> images, <span class="hlt">interpreted</span> with a coincident velocity model obtained by wide-angle data tomography, provide (1) enhanced imaging of the sedimentary cover down to the top of the acoustic basement, including the base of the Messinian evaporites and the sub-salt Miocene series, which appear to be tectonized as far as in the mid-basin, and (2) new evidence of deep crustal structures in the margin which the initial processing had failed to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUSMNS11A..05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUSMNS11A..05D"><span>Natural Gas Hydrates Estimation Using <span class="hlt">Seismic</span> Inversion and Rock Physics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dutta, N.; Dai, J.; Kleinberg, R.; Xu, H.</p> <p>2005-05-01</p> <p>Gas hydrate drilling worldwide indicates that the formation of gas hydrates in shallow sediments tends to increase P- and S-wave velocities of the hosting rocks. Rock physics models of gas hydrates provide the links between velocity anomalies and gas hydrate concentration. In this <span class="hlt">abstract</span>, we evaluate the numerical predictions of some of the major rock physics models of gas hydrates and validate those with well log data from the Mallik and Blake Ridge wells. We find that a model in which the gas hydrate is a part of the rock framework produces results that are consistent with well log data. To enhance the accuracy of <span class="hlt">seismic</span> estimation, we adopt a five-step, integrated workflow that enables us to identify and quantify gas hydrates in the deepwater Gulf of Mexico (GOM). It includes: 1) Reprocessing conventional 3D <span class="hlt">seismic</span> data at high resolution using an amplitude-preserving flow with prestack time migration, 2) A detailed stratigraphic evaluation to identify potential hydrate zones, 3) <span class="hlt">Seismic</span> attribute analysis to further delineate anomalous zones, 4) Full waveform prestack inversion to characterize acoustic properties of gas hydrates in 1D (Mallick, 1995; Mallick, 1999) and map in 3D using hybrid inversion techniques (Dutta, 2002; Mallick and Dutta, 2002), and 5) Quantitative estimation of gas hydrate saturation using rock property models. We illustrate the procedure using 3D <span class="hlt">seismic</span> data, and estimate gas hydrate saturation in the study area in the GOM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70191534','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191534"><span>Micro-<span class="hlt">seismicity</span> and <span class="hlt">seismic</span> moment release within the Coso Geothermal Field, 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>Kaven, Joern; Hickman, Stephen H.; Davatzes, Nicholas C.</p> <p>2014-01-01</p> <p>We relocate 16 years of <span class="hlt">seismicity</span> in the Coso Geothermal Field (CGF) using differential travel times and simultaneously invert for <span class="hlt">seismic</span> velocities to improve our knowledge of the subsurface geologic and hydrologic structure. We expand on our previous results by doubling the number of relocated events from April 1996 through May 2012 using a new field-wide 3-D velocity model. Relocated micro-<span class="hlt">seismicity</span> sharpens in many portions of the active geothermal reservoir, likely defining large-scale fault zones and fluid pressure compartment boundaries. However, a significant fraction of <span class="hlt">seismicity</span> remains diffuse and does not cluster into sharply defined structures, suggesting that permeability is maintained within the reservoir through distributed brittle failure. The <span class="hlt">seismic</span> velocity structure reveals heterogeneous distributions of compressional (Vp) and shear (Vs) wave speed, with Vs generally higher in the Main Field and East Flank and Vp remaining relatively uniform across the CGF, but with significant local variations. The Vp/Vs ratio appears to outline the two main producing compartments of the reservoir at depths below mean ground level of approximately 1 to 2.5 km, with a ridge of relatively high Vp/Vs separating the Main Field from the East Flank. Detailed analyses of spatial and temporal variations in earthquake relocations and cumulative <span class="hlt">seismic</span> moment release in the East Flank reveal three regions with persistently high rates of <span class="hlt">seismic</span> activity. Two of these regions exhibit sharp, stationary boundaries at the margins of the East Flank that likely represent barriers to fluid flow and advective heat transport. However, <span class="hlt">seismicity</span> and moment release in a third region at the northern end of the East Flank spread over time to form an elongated NE to SW structure, roughly parallel both to an elongated cluster of <span class="hlt">seismicity</span> at the southern end of the East Flank and to regional fault traces mapped at the surface. Our results indicate that high</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGE....15..164W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGE....15..164W"><span>An improved peak frequency shift method for Q estimation based on generalized <span class="hlt">seismic</span> wavelet function</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Qian; Gao, Jinghuai</p> <p>2018-02-01</p> <p>As a powerful tool for hydrocarbon detection and reservoir characterization, the quality factor, Q, provides useful information in <span class="hlt">seismic</span> data processing and <span class="hlt">interpretation</span>. In this paper, we propose a novel method for Q estimation. The generalized <span class="hlt">seismic</span> wavelet (GSW) function was introduced to fit the amplitude spectrum of <span class="hlt">seismic</span> waveforms with two parameters: fractional value and reference frequency. Then we derive an analytical relation between the GSW function and the Q factor of the medium. When a <span class="hlt">seismic</span> wave propagates through a viscoelastic medium, the GSW function can be employed to fit the amplitude spectrum of the source and attenuated wavelets, then the fractional values and reference frequencies can be evaluated numerically from the discrete Fourier spectrum. After calculating the peak frequency based on the obtained fractional value and reference frequency, the relationship between the GSW function and the Q factor can be built by the conventional peak frequency shift method. Synthetic tests indicate that our method can achieve higher accuracy and be more robust to random noise compared with existing methods. Furthermore, the proposed method is applicable to different types of source wavelet. Field data application also demonstrates the effectiveness of our method in <span class="hlt">seismic</span> attenuation and the potential in the reservoir characteristic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027524','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027524"><span>Delineation of tectonic provinces of New York state as a component of <span class="hlt">seismic</span>-hazard evaluation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fakundiny, R.H.</p> <p>2004-01-01</p> <p><span class="hlt">Seismic</span>-hazard evaluations in the eastern United States must be based on <span class="hlt">interpretations</span> of the composition and form of Proterozoic basement-rock terranes and overlying Paleozoic strata, and on factors that can cause relative movements among their units, rather than Phanerozoic orogenic structures, which may be independent of modern tectonics. The tectonic-province concept is a major part of both probabilistic and deterministic <span class="hlt">seismic</span>-hazard evaluations, yet those that have been proposed to date have not attempted to geographically correlate modern earthquakes with regional basement structure. Comparison of basement terrane (megablock) boundaries with the spatial pattern of modern <span class="hlt">seismicity</span> may lead to the mechanically sound definition of tectonic provinces, and thus, better <span class="hlt">seismic</span>-hazard evaluation capability than is currently available. Delineation of megablock boundaries will require research on the many factors that affect their structure and movement. This paper discusses and groups these factors into two broad categories-megablock tectonics in relation to <span class="hlt">seismicity</span> and regional horizontal-compressive stresses, with megablock tectonics divided into subcategories of basement, overlying strata, regional lineaments, basement tectonic terranes, earthquake epicenter distribution, and epeirogeny, and compressive stresses divided into pop-ups and the contemporary maximum horizontal-compressive stress field. A list presenting four to nine proposed research topics for each of these categories is given at the end.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AcGeo..64.1989J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AcGeo..64.1989J"><span>Various Approaches to Forward and Inverse Wide-Angle <span class="hlt">Seismic</span> Modelling Tested on Data from DOBRE-4 Experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Janik, Tomasz; Środa, Piotr; Czuba, Wojciech; Lysynchuk, Dmytro</p> <p>2016-12-01</p> <p>The <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> refraction and wide angle reflection data usually involves the creation of a velocity model based on an inverse or forward modelling of the travel times of crustal and mantle phases using the ray theory approach. The modelling codes differ in terms of model parameterization, data used for modelling, regularization of the result, etc. It is helpful to know the capabilities, advantages and limitations of the code used compared to others. This work compares some popular 2D <span class="hlt">seismic</span> modelling codes using the dataset collected along the <span class="hlt">seismic</span> wide-angle profile DOBRE-4, where quite peculiar/uncommon reflected phases were observed in the wavefield. The 505 km long profile was realized in southern Ukraine in 2009, using 13 shot points and 230 recording stations. Double PMP phases with a different reduced time (7.5-11 s) and a different apparent velocity, intersecting each other, are observed in the <span class="hlt">seismic</span> wavefield. This is the most striking feature of the data. They are <span class="hlt">interpreted</span> as reflections from strongly dipping Moho segments with an opposite dip. Two steps were used for the modelling. In the previous work by Starostenko et al. (2013), the trial-and-error forward model based on refracted and reflected phases (SEIS83 code) was published. The interesting feature is the high-amplitude (8-17 km) variability of the Moho depth in the form of downward and upward bends. This model is compared with results from other <span class="hlt">seismic</span> inversion methods: the first arrivals tomography package FAST based on first arrivals; the JIVE3D code, which can also use later refracted arrivals and reflections; and the forward and inversion code RAYINVR using both refracted and reflected phases. Modelling with all the codes tested showed substantial variability of the Moho depth along the DOBRE-4 profile. However, SEIS83 and RAYINVR packages seem to give the most coincident results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T13E..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T13E..03P"><span>Detailed imaging of the 2007 Pisco co-<span class="hlt">seismic</span> and post-<span class="hlt">seismic</span> deformation - implications on the seismogenic behavior of subduction megathrusts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perfettini, H.; Sladen, A.; Avouac, J.; Simons, M.; Nocquet, J.; Bondoux, F.; Kositsky, A.; Chlieh, M.; Tavera, H.; Audin, L.; Konca, A.; Fielding, E. J.; Farber, D.; Ortega, F. H.</p> <p>2009-12-01</p> <p>In the last couple of decades, advances in the analysis techniques and instrumentation have improved significantly our capability to document the different stages of the <span class="hlt">seismic</span> cycle, namely the co-, post- and inter-<span class="hlt">seismic</span> phases. To this respect, the Mw8.0 Pisco, Peru, earthquake of August 2007 is exemplary, with numerous data sets allowing to explore the details of each phase and study their relationship. We derive a kinematic model of the coseismic rupture from the joint non-linear inversion of teleseismic and six Interferometric Synthetic Aperture Radar (InSAR) images. Our preferred model indicates a remarkable anti-correlation between the co-<span class="hlt">seismic</span> slip distribution and the aftershock distribution determined from the Peruvian <span class="hlt">seismic</span> network. The proposed source model is compatible with regional run-up measurements and open-ocean tsunami records. In particular, the tsunami observations validate that the rupture did not extend to the trench, and confirm that the Pisco event is not a tsunami earthquake despite its low apparent rupture velocity (< 1.5 km/s). We favor the <span class="hlt">interpretation</span> that the earthquake consists of 2 subevents, each with a conventional rupture velocity (2-4 km/s). The delay between the 2 subevents might reflect the time for the second shock to nucleate or, alternatively, the time it took for afterslip to increase the stress level on the second asperity to a level necessary for static triggering. The source model predicts uplift offshore and subsidence onland with the pivot line following the changes in curvature of the coastline. This observation set the Pisco earthquake as one of the best examples of a link between the geomorphology of the coastline and the pattern of surface deformation induced by large interplate ruptures. The post-<span class="hlt">seismic</span> deformation following the mainshock is studied using a local network of continuous GPS stations and the PCAIM inversion method. The inversion indicates that the two patches of co-<span class="hlt">seismic</span> slip triggered</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981GeoRL...8.1129W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981GeoRL...8.1129W"><span>The excitation of long period <span class="hlt">seismic</span> waves by a source spanning a structural discontinuity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Woodhouse, J. H.</p> <p></p> <p>Simple theoretical results are obtained for the excitation of <span class="hlt">seismic</span> waves by an indigenous <span class="hlt">seismic</span> source in the case that the source volume is intersected by a structural discontinuity. In the long wavelength approximation the <span class="hlt">seismic</span> radiation is identical to that of a point source placed on one side of the discontinuity or of a different point source placed on the other side. The moment tensors of these two equivalent sources are related by a specific linear transformation and may differ appreciably both in magnitude and geometry. Either of these sources could be obtained by linear inversion of <span class="hlt">seismic</span> data but the physical <span class="hlt">interpretation</span> is more complicated than in the usual case. A source which involved no volume change would, for example, yield an isotropic component if, during inversion, it were assumed to lie on the wrong side of the discontinuity. The problem of determining the true moment tensor of the source is indeterminate unless further assumptions are made about the stress glut distribution; one way to resolve this indeterminancy is to assume proportionality between the integrated stress glut on each side of the discontinuity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000JAESc..18..441L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000JAESc..18..441L"><span>Quaternary <span class="hlt">seismic</span> stratigraphy and paleoenvironments on the continental shelf of the East China Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Zhen-Xia; Berne, Serge; Saito, Yoshiki; Lericolais, G.; Marsset, T.</p> <p>2000-08-01</p> <p>Paleoenvironments and stratigraphy have been <span class="hlt">interpreted</span> from 4380 km of <span class="hlt">seismic</span> profiling collected during a geological and geophysical cruise on the continental shelf of the East China Sea (ECS) undertaken in 1996. The geophysical data are correlated with a borehole situated on the outer shelf obtained by Shanghai Marine Geology Bureau, indicating that six <span class="hlt">seismic</span> units have been preserved since oxygen-isotope stage 6, including four regressive-transgressive cycles. <span class="hlt">Seismic</span> units U2, U3+U4+U5, U6, and U7 are <span class="hlt">interpreted</span> to correspond respectively to oxygen-isotope stages 1, 3, 5, and 6, implying that sediment partitioning and sequence architecture in the ECS have been controlled by glacio-eustasy and global climate changes. Alternating continental and marine strata corresponding to glaciation and interglaciation are well preserved on the outer shelf of the ECS. Most of the cold environment strata, which formed on the outer shelf during oxygen-isotope stages 2 and 4, are too thin to be recognized on SIG 600J because of resolution, but corresponding erosion surfaces exist. <span class="hlt">Seismic</span> unit U7 is widespread over the shelf, extending to the continental edge and showing little variation in thickness, as the regression was pronounced and lasted a long time. Thus, U7 can be used as a marker layer for correlation of Quaternary strata on the shelf of the ECS. Post-glacial transgression is obvious in the ECS. Marine strata with varied thickness were developed in the shallow sea of the inner shelf, thinning toward the outer shelf. The continental shelf of the ECS has been influenced by Pacific tide-wave systems for a long time, forming tidal sand-ridge sequences, developed during transgressions, corresponding to oxygen-isotope stages 7 (or 9), 5, 3 and 1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.7101B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.7101B"><span>Studying temporal velocity changes with ambient <span class="hlt">seismic</span> noise at Hawaiian volcanoes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ballmer, S.; Wolfe, C. J.; Okubo, P. G.; Haney, M. M.; Thurber, C. H.</p> <p>2012-04-01</p> <p>In order to understand the dynamics of volcanoes and to assess the associated hazards, the analysis of ambient <span class="hlt">seismic</span> noise - a continuous passive source - has been used for both imaging and monitoring temporal changes in <span class="hlt">seismic</span> velocity. Between pairs of <span class="hlt">seismic</span> stations, surface wave Green's functions can be retrieved from the background ocean-generated noise being sensitive to the shallow subsurface. Such Green's functions allow the measurement of very small temporal perturbations in <span class="hlt">seismic</span> velocity with a variety of applications. In particular, velocity decreases prior to some volcanic eruptions have been documented and motivate our present study. Here we perform ambient <span class="hlt">seismic</span> noise interferometry to study temporal changes in <span class="hlt">seismic</span> velocities within the shallow (<5km) subsurface of the Hawaiian volcanoes. Our study is the first to assess the potential for using ambient noise analyses as a tool for Hawaiian volcano monitoring. Five volcanoes comprise the island of Hawaii, of which two are active: Mauna Loa volcano, which last erupted in 1984, and Kilauea volcano, where the Pu'u'O'o-Kupaianaha eruption along the east rift zone has been ongoing since 1983. For our analysis, we use data from the USGS Hawaiian Volcano Observatory (HVO) <span class="hlt">seismic</span> network from 05/2007 to 12/2009. Our study period includes the Father's Day dike intrusion into Kilauea's east rift zone in mid-June 2007 as well as increased summit activity commencing in late 2007 and leading to several minor explosions in early 2008. These volcanic events are of interest for the study of potential associated <span class="hlt">seismic</span> velocity changes. However, we find that volcanic tremor complicates the measurement of velocity changes. Volcanic tremor is continuously present during most of our study period, and contaminates the recovered Green's functions for station pairs across the entire island. Initial results suggest that a careful quality assessment (i.e. visually inspecting the Green's functions and filtering</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S51D2721W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S51D2721W"><span>Monte Carlo Volcano <span class="hlt">Seismic</span> Moment Tensors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Waite, G. P.; Brill, K. A.; Lanza, F.</p> <p>2015-12-01</p> <p>Inverse modeling of volcano <span class="hlt">seismic</span> sources can provide insight into the geometry and dynamics of volcanic conduits. But given the logistical challenges of working on an active volcano, <span class="hlt">seismic</span> networks are typically deficient in spatial and temporal coverage; this potentially leads to large errors in source models. In addition, uncertainties in the centroid location and moment-tensor components, including volumetric components, are difficult to constrain from the linear inversion results, which leads to a poor understanding of the model space. In this study, we employ a nonlinear inversion using a Monte Carlo scheme with the objective of defining robustly resolved elements of model space. The model space is randomized by centroid location and moment tensor eigenvectors. Point sources densely sample the summit area and moment tensors are constrained to a randomly chosen geometry within the inversion; Green's functions for the random moment tensors are all calculated from modeled single forces, making the nonlinear inversion computationally reasonable. We apply this method to very-long-period (VLP) <span class="hlt">seismic</span> events that accompany minor eruptions at Fuego volcano, Guatemala. The library of single force Green's functions is computed with a 3D finite-difference modeling algorithm through a homogeneous velocity-density model that includes topography, for a 3D grid of nodes, spaced 40 m apart, within the summit region. The homogenous velocity and density model is justified by long wavelength of VLP data. The nonlinear inversion reveals well resolved model features and informs the <span class="hlt">interpretation</span> through a better understanding of the possible models. This approach can also be used to evaluate possible station geometries in order to optimize networks prior to deployment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Tectp.647..105M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Tectp.647..105M"><span><span class="hlt">Seismic</span> imaging of the geodynamic activity at the western Eger rift in central Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mullick, N.; Buske, S.; Hrubcova, P.; Ruzek, B.; Shapiro, S.; Wigger, P.; Fischer, T.</p> <p>2015-04-01</p> <p>The western Eger rift at the Czech-German border in central Europe is an important geodynamically active area within the European Cenzoic rift system (ECRS) in the forelands of the Alps. Along with two other active areas of the ECRS, the French Massif Central and the east and west Eifel volcanic fields, it is characterized by numerous CO2-rich fluid emission points and frequent micro-<span class="hlt">seismicity</span>. Existence of a plume(s) is indicated in the upper mantle which may be responsible for these observations. Here we reprocess a pre-existing deep <span class="hlt">seismic</span> reflection profile '9HR' and <span class="hlt">interpret</span> the subsurface structures as mapped by <span class="hlt">seismic</span> reflectivity with previous findings, mainly from seismological and geochemical studies, to investigate the geodynamic activity in the subsurface. We find prominent hints of pathways which may allow magmatic fluids originating in the upper mantle to rise through the crust and cause the observed fluid emanations and earthquake activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS.995a2107A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS.995a2107A"><span>Subsurface Characterization using Geophysical <span class="hlt">Seismic</span> Refraction Survey for Slope Stabilization Design with Soil Nailing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ashraf Mohamad Ismail, Mohd; Ng, Soon Min; Hazreek Zainal Abidin, Mohd; Madun, Aziman</p> <p>2018-04-01</p> <p>The application of geophysical <span class="hlt">seismic</span> refraction for slope stabilization design using soil nailing method was demonstrated in this study. The potential weak layer of the study area is first identify prior to determining the appropriate length and location of the soil nail. A total of 7 <span class="hlt">seismic</span> refraction survey lines were conducted at the study area with standard procedures. The refraction data were then analyzed by using the Pickwin and Plotrefa computer software package to obtain the <span class="hlt">seismic</span> velocity profiles distribution. These results were correlated with the complementary borehole data to <span class="hlt">interpret</span> the subsurface profile of the study area. It has been identified that layer 1 to 3 is the potential weak zone susceptible to slope failure. Hence, soil nails should be installed to transfer the tensile load from the less stable layer 3 to the more stable layer 4. The soil-nail interaction will provide a reinforcing action to the soil mass thereby increasing the stability of the slope.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S23B0790R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S23B0790R"><span>The Induced <span class="hlt">Seismicity</span> Roller Coaster: Up, and then Down, and then Up Again</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riffault, J.; Dempsey, D.</p> <p>2017-12-01</p> <p>Diverse industries from oil & gas, to geothermal and CO2 storage have triggered significant numbers of earthquakes in the last decade. There is broad agreement that the underlying cause is injection of large volumes of fluid and subsequent pressure rise in the disposal and connected formations. Thus, it stands to reason that reducing injection will have a flow-through effect on the <span class="hlt">seismicity</span>. For example, in an attempt to mitigate earthquakes in Oklahoma, a 40% injection rate reduction was enforced, resulting in a significant decrease in the <span class="hlt">seismicity</span> rate. Here, we show that, under certain conditions, cutting the injection rate leads to transients in the <span class="hlt">seismicity</span> rate that could mislead operators and regulators into a false sense of security. We used semi-analytic solutions of injection and fluid flow in a radial geometry coupled with a model that links the pressure rise with the rate of induced <span class="hlt">seismicity</span>. We find that cutting the injection rate causes complex pressure transients around the injection well: (i) initially, pressure will continue to increase; (ii), then, it reaches a peak and starts to decline; (iii) finally, the decline is reversed and pressure starts to increase again. Depending on the stress criticality of the system and the size of the injection rate cut, the outcome can be a short-term decrease, or even a total cessation, of the <span class="hlt">seismicity</span>. However, over the longer term, <span class="hlt">seismicity</span> will increase to a new steady-state (which is nevertheless lower than that preceding the rate cut.) Our results imply that it can be misleading to rely on observations of the <span class="hlt">seismicity</span> rate shortly after mitigation measures are implemented as an indicator of their efficacy. It is also possible to use this model to <span class="hlt">interpret</span> the results injection well step tests, with the aim of quantifying aspects of the crustal stress state.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T24B..08B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T24B..08B"><span>Characterizing the Inner Accretionary Prism of the Nankai Trough with 3D <span class="hlt">Seismic</span> and Logging While Drilling at IODP Site C0002</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boston, B.; Moore, G. F.; Jurado, M. J.; Sone, H.; Tobin, H. J.; Saffer, D. M.; Hirose, T.; Toczko, S.; Maeda, L.</p> <p>2014-12-01</p> <p>The deeper, inner parts of active accretionary prisms have been poorly studied due the lack of drilling data, low <span class="hlt">seismic</span> image quality and typically thick overlying sediments. Our project focuses on the interior of the Nankai Trough inner accretionary prism using deep scientific drilling and a 3D <span class="hlt">seismic</span> cube. International Ocean Discovery Program (IODP) Expedition 348 extended the existing riser hole to more than 3000 meters below seafloor (mbsf) at Site C0002. Logging while drilling (LWD) data included gamma ray, resistivity, resistivity image, and sonic logs. LWD analysis of the lower section revealed on the borehole images intense deformation characterized by steep bedding, faults and fractures. Bedding plane orientations were measured throughout, with minor gaps at heavily deformed zones disrupting the quality of the resistivity images. Bedding trends are predominantly steeply dipping (60-90°) to the NW. <span class="hlt">Interpretation</span> of fractures and faults in the image log revealed the existence of different sets of fractures and faults and variable fracture density, remarkably high at fault zones. Gamma ray, resistivity and sonic logs indicated generally homogenous lithology <span class="hlt">interpretation</span> along this section, consistent with the "silty-claystone" predominant lithologies described on cutting samples. Drops in sonic velocity were observed at the fault zones defined on borehole images. <span class="hlt">Seismic</span> reflection <span class="hlt">interpretation</span> of the deep faults in the inner prism is exceedingly difficult due to a strong seafloor multiple, high-angle bedding dips, and low frequency of the data. Structural reconstructions were employed to test whether folding of <span class="hlt">seismic</span> horizons in the overlying forearc basin could be from an <span class="hlt">interpreted</span> paleothrust within the inner prism. We used a trishear-based restoration to estimate fault slip on folded horizons landward of C0002. We estimate ~500 m of slip from a steeply dipping deep thrust within the last ~0.9 Ma. Folding is not found in the Kumano sediments</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSeis.tmp...48N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSeis.tmp...48N"><span>Angola <span class="hlt">seismicity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neto, Francisco António Pereira; França, George Sand; Condori, Cristobal; Sant'Anna Marotta, Giuliano; Chimpliganond, Cristiano Naibert</p> <p>2018-05-01</p> <p>This work describes the development of the Angolan earthquake catalog and <span class="hlt">seismicity</span> distribution in the Southwestern African Plate, in Angola. This region is one of the least <span class="hlt">seismically</span> active, even for stable continental regions (SCRs) in the world. The maximum known earthquake had a magnitude of 6.0 Ms, while events with magnitudes of 4.5 have return period of about 10 years. Events with magnitude 5 and above occur with return period of about 20 years. Five <span class="hlt">seismic</span> zones can be confirmed in Angola, within and along craton edges and in the sedimentary basins including offshore. Overall, the exposed cratonic regions tend to have more earthquakes compared to other regions such as sedimentary basins. Earthquakes tend to occur in Archaic rocks, especially inside preexisting weakness zones and in tectonic-magmatic reactivation zones of Mesozoic and Meso-Cenozoic, associated with the installation of a wide variety of intrusive rocks, strongly marked by intense tectonism. This fact can be explained by the models of preexisting weakness zones and stress concentration near intersecting structures. The Angolan passive margin is also a new region where <span class="hlt">seismic</span> activity occurs. Although clear differences are found between different areas along the passive margin, in the middle near Porto Amboim city, <span class="hlt">seismic</span> activity is more frequent compared with northwestern and southwestern regions.</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/2017AGUFMPA21C0353B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPA21C0353B"><span>Rescaled Range analysis of Induced <span class="hlt">Seismicity</span>: rapid classification of clusters in <span class="hlt">seismic</span> crisis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bejar-Pizarro, M.; Perez Lopez, R.; Benito-Parejo, M.; Guardiola-Albert, C.; Herraiz, M.</p> <p>2017-12-01</p> <p>Different underground fluid operations, mainly gas storing, fracking and water pumping, can trigger Induced <span class="hlt">Seismicity</span> (IS). This <span class="hlt">seismicity</span> is normally featured by small-sized earthquakes (M<2.5), although particular cases reach magnitude as great as 5. It has been up for debate whether earthquakes greater than 5 can be triggered by IS or this level of magnitude only corresponds to tectonic earthquakes caused by stress change. Whatever the case, the characterization of IS for <span class="hlt">seismic</span> clusters and <span class="hlt">seismic</span> series recorded close but not into the gas storage, is still under discussion. Time-series of earthquakes obey non-linear patterns where the Hurst exponent describes the persistency or anti-persistency of the sequence. Natural <span class="hlt">seismic</span> sequences have an H-exponent close to 0.7, which combined with the b-value time evolution during the time clusters, give us valuable information about the stationarity of the phenomena. Tectonic earthquakes consist in a main shock with a decay of time-occurrence of <span class="hlt">seismic</span> shocks obeying the Omori's empirical law. On the contrary, IS does not exhibit a main shock and the time occurrence depends on the injection operations instead of on the tectonic energy released. In this context, the H-exponent can give information about the origin of the sequence. In 2013, a <span class="hlt">seismic</span> crisis was declared from the Castor underground gas storing located off-shore in the Mediterranean Sea, close to the Northeastern Spanish cost. The greatest induced earthquake was 3.7. However, a 4.2 earthquake, probably of tectonic origin, occurred few days after the operations stopped. In this work, we have compared the H-exponent and the b-value time evolution according to the timeline of gas injection. Moreover, we have divided the <span class="hlt">seismic</span> sequence into two groups: (1) Induced <span class="hlt">Seismicity</span> and (2) Triggered <span class="hlt">Seismicity</span>. The rescaled range analysis allows the differentiation between natural and induced <span class="hlt">seismicity</span> and gives information about the persistency and long</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1313/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1313/report.pdf"><span>Studies related to the Charleston, South Carolina, earthquake of 1886; tectonics and <span class="hlt">seismicity</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>Gottfried, David; Annell, C.S.; Byerly, G.R.; Lanphere, Marvin A.; Phillips, Jeffrey D.; Gohn, Gregory S.; Houser, Brenda B.; Schneider, Ray R.; Ackermann, Hans D.; Yantis, B.R.; Costain, John K.; Schilt, F. Steve; Brown, Larry; Oliver, Jack E.; Kaufman, Sidney; Hamilton, Robert Morrison; Behrendt, John C.; Henry, V. James; Bayer, Kenneth C.; Daniels, David L.; Zietz, Isidore; Popenoe, Peter; Chowns, T.M.; Williams, C.T.; Dooley, Robert E.; Wampler, J.; Dillon, William P.; Klitgord, Kim D.; Paull, Charles K.; McGinnis, Lyle D.; Dewey, James W.; Tarr, Arthur C.; Rhea, Susan; Wentworth, Carl M.; Mergner-Keefer, Marcia; Bollinger, G.A.; Gohn, Gregory S.</p> <p>1983-01-01</p> <p>, at the present time, none of the young structures can be related unequivocally to the <span class="hlt">seismicity</span> because earthquake fault-plane solutions and hypocenter distributions do not agree with the locations and orientations of these structures. Therefore, a major emphasis of continuing USGS investigations near Charleston will be to identify additional faults, if any exist, to delineate fault movement histories, and to further refine earthquake locations, focal mechanisms, and related seismological <span class="hlt">interpretations</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ExG....48..272E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ExG....48..272E"><span>New comprehensive standard <span class="hlt">seismic</span> noise models and 3D <span class="hlt">seismic</span> noise variation for Morocco territory, North Africa, obtained using <span class="hlt">seismic</span> broadband stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>El Fellah, Younes; El-Aal, Abd El-Aziz Khairy Abd; Harnafi, Mimoun; Villaseñor, Antonio</p> <p>2017-05-01</p> <p>In the current work, we constructed new comprehensive standard <span class="hlt">seismic</span> noise models and 3D temporal-spatial <span class="hlt">seismic</span> noise level cubes for Morocco in north-west Africa to be used for seismological and engineering purposes. Indeed, the original global standard <span class="hlt">seismic</span> noise models published by Peterson (1993) and their following updates by Astiz and Creager (1995), Ekström (2001) and Berger et al. (2003) had no contributing <span class="hlt">seismic</span> stations deployed in North Africa. Consequently, this preliminary study was conducted to shed light on <span class="hlt">seismic</span> noise levels specific to north-west Africa. For this purpose, 23 broadband <span class="hlt">seismic</span> stations recently installed in different structural domains throughout Morocco are used to study the nature and characteristics of <span class="hlt">seismic</span> noise and to create <span class="hlt">seismic</span> noise models for Morocco. Continuous data recorded during 2009, 2010 and 2011 were processed and analysed to construct these new noise models and 3D noise levels from all stations. We compared the Peterson new high-noise model (NHNM) and low-noise model (NLNM) with the Moroccan high-noise model (MHNM) and low-noise model (MLNM). These new noise models are comparable to the United States Geological Survey (USGS) models in the short period band; however, in the period range 1.2 s to 1000 s for MLNM and 10 s to 1000 s for MHNM display significant variations. This variation is attributed to differences in the nature of <span class="hlt">seismic</span> noise sources that dominate Morocco in these period bands. The results of this study have a new perception about permanent <span class="hlt">seismic</span> noise models for this spectacular region and can be considered a significant contribution because it supplements the Peterson models and can also be used to site future permanent <span class="hlt">seismic</span> stations in Morocco.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70170508','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70170508"><span>Three-dimensional <span class="hlt">seismic</span> velocity structure of Mauna Loa and Kilauea volcanoes in Hawaii from local <span class="hlt">seismic</span> tomography</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, Guoqing; Shearer, Peter M.; Matoza, Robin S.; Okubo, Paul G.; Amelung, Falk</p> <p>2016-01-01</p> <p>We present a new three-dimensional <span class="hlt">seismic</span> velocity model of the crustal and upper mantle structure for Mauna Loa and Kilauea volcanoes in Hawaii. Our model is derived from the first-arrival times of the compressional and shear waves from about 53,000 events on and near the Island of Hawaii between 1992 and 2009 recorded by the Hawaiian Volcano Observatory stations. The Vp model generally agrees with previous studies, showing high-velocity anomalies near the calderas and rift zones and low-velocity anomalies in the fault systems. The most significant difference from previous models is in Vp/Vs structure. The high-Vp and high-Vp/Vs anomalies below Mauna Loa caldera are <span class="hlt">interpreted</span> as mafic magmatic cumulates. The observed low-Vp and high-Vp/Vs bodies in the Kaoiki <span class="hlt">seismic</span> zone between 5 and 15 km depth are attributed to the underlying volcaniclastic sediments. The high-Vp and moderate- to low-Vp/Vs anomalies beneath Kilauea caldera can be explained by a combination of different mafic compositions, likely to be olivine-rich gabbro and dunite. The systematically low-Vp and low-Vp/Vs bodies in the southeast flank of Kilauea may be caused by the presence of volatiles. Another difference between this study and previous ones is the improved Vp model resolution in deeper layers, owing to the inclusion of events with large epicentral distances. The new velocity model is used to relocate the <span class="hlt">seismicity</span> of Mauna Loa and Kilauea for improved absolute locations and ultimately to develop a high-precision earthquake catalog using waveform cross-correlation data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22391567-preliminary-results-characteristic-seismic-anisotropy-beneath-sunda-banda-subduction-collision-zone','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22391567-preliminary-results-characteristic-seismic-anisotropy-beneath-sunda-banda-subduction-collision-zone"><span>Preliminary results of characteristic <span class="hlt">seismic</span> anisotropy beneath Sunda-Banda subduction-collision zone</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>Wiyono, Samsul H., E-mail: samsul.wiyono@bmkg.go.id; Indonesia’s Agency for Meteorology Climatology and Geophysics, Jakarta 10610; Nugraha, Andri Dian, E-mail: nugraha@gf.itb.ac.id</p> <p>2015-04-24</p> <p>Determining of <span class="hlt">seismic</span> anisotropy allowed us for understanding the deformation processes that occured in the past and present. In this study, we performed shear wave splitting to characterize <span class="hlt">seismic</span> anisotropy beneath Sunda-Banda subduction-collision zone. For about 1,610 XKS waveforms from INATEWS-BMKG networks have been analyzed. From its measurements showed that fast polarization direction is consistent with trench-perpendicular orientation but several stations presented different orientation. We also compared between fast polarization direction with absolute plate motion in the no net rotation and hotspot frame. Its result showed that both absolute plate motion frame had strong correlation with fast polarization direction. Strongmore » correlation between the fast polarization direction and the absolute plate motion can be <span class="hlt">interpreted</span> as the possibility of dominant anisotropy is in the asthenosphere.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5286C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5286C"><span>GeoNetGIS: a Geodetic Network Geographical Information System to manage GPS networks in <span class="hlt">seismic</span> and volcanic areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cristofoletti, P.; Esposito, A.; Anzidei, M.</p> <p>2003-04-01</p> <p>This paper presents the methodologies and issues involved in the use of GIS techniques to manage geodetic information derived from networks in <span class="hlt">seismic</span> and volcanic areas. Organization and manipulation of different geodetical, geological and <span class="hlt">seismic</span> database, give us a new challenge in <span class="hlt">interpretation</span> of information that has several dimensions, including spatial and temporal variations, also the flexibility and brand range of tools available in GeoNetGIS, make it an attractive platform for earthquake risk assessment. During the last decade the use of geodetic networks based on the Global Positioning System, devoted to geophysical applications, especially for crustal deformation monitoring in <span class="hlt">seismic</span> and volcanic areas, increased dramatically. The large amount of data provided by these networks, combined with different and independent observations, such as epicentre distribution of recent and historical earthquakes, geological and structural data, photo <span class="hlt">interpretation</span> of aerial and satellite images, can aid for the detection and parameterization of seismogenic sources. In particular we applied our geodetic oriented GIS to a new GPS network recently set up and surveyed in the Central Apennine region: the CA-GeoNet. GeoNetGIS is designed to analyze in three and four dimensions GPS sources and to improve crustal deformation analysis and <span class="hlt">interpretation</span> related with tectonic structures and <span class="hlt">seismicity</span>. It manages many database (DBMS) consisting of different classes, such as Geodesy, Topography, <span class="hlt">Seismicity</span>, Geology, Geography and Raster Images, administrated according to Thematic Layers. GeoNetGIS represents a powerful research tool allowing to join the analysis of all data layers to integrate the different data base which aid for the identification of the activity of known faults or structures and suggesting the new evidences of active tectonics. A new approach to data integration given by GeoNetGIS capabilities, allow us to create and deliver a wide range of maps, digital</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028355','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028355"><span>Local thickening of the Cascadia forearc crust and the origin of <span class="hlt">seismic</span> reflectors in the uppermost mantle</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Calvert, A.J.; Ramachandran, K.; Kao, H.; Fisher, M.A.</p> <p>2006-01-01</p> <p><span class="hlt">Seismic</span> reflection profiles from three different surveys of the Cascadia forearc are <span class="hlt">interpreted</span> using P wave velocities and relocated hypocentres, which were both derived from the first arrival travel time inversion of wide-angle <span class="hlt">seismic</span> data and local earthquakes. The subduction decollement, which is characterized beneath the continental shelf by a reflection of 0.5 s duration, can be traced landward into a large duplex structure in the lower forearc crust near southern Vancouver Island. Beneath Vancouver Island, the roof thrust of the duplex is revealed by a 5–12 km thick zone, identified previously as the E reflectors, and the floor thrust is defined by a short duration reflection from a − 1. We suggest that these relatively low velocities indicate the presence of either crustal rocks from the oceanic plate that have been underplated to the continent or crustal rocks from the forearc that have been transported downward by subduction erosion. The absence of <span class="hlt">seismicity</span> from within the E reflectors implies that they are significantly weaker than the overlying crust, and the reflectors may be a zone of active ductile shear. In contrast, <span class="hlt">seismicity</span> in parts of the D reflectors can be <span class="hlt">interpreted</span> to mean that ductile shearing no longer occurs in the landward part of the duplex. Merging of the D and E reflectors at 42–46 km depth creates reflectivity in the uppermost mantle with a vertical thickness of at least 15 km. We suggest that pervasive reflectivity in the upper mantle elsewhere beneath Puget Sound and the Strait of Georgia arises from similar shear zones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21973353','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21973353"><span>Two applications of time reversal mirrors: <span class="hlt">seismic</span> radio and <span class="hlt">seismic</span> radar.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hanafy, Sherif M; Schuster, Gerard T</p> <p>2011-10-01</p> <p>Two <span class="hlt">seismic</span> applications of time reversal mirrors (TRMs) are introduced and tested with field experiments. The first one is sending, receiving, and decoding coded messages similar to a radio except <span class="hlt">seismic</span> waves are used. The second one is, similar to radar surveillance, detecting and tracking a moving object(s) in a remote area, including the determination of the objects speed of movement. Both applications require the prior recording of calibration Green's functions in the area of interest. This reference Green's function will be used as a codebook to decrypt the coded message in the first application and as a moving sensor for the second application. Field tests show that <span class="hlt">seismic</span> radar can detect the moving coordinates (x(t), y(t), z(t)) of a person running through a calibration site. This information also allows for a calculation of his velocity as a function of location. Results with the <span class="hlt">seismic</span> radio are successful in <span class="hlt">seismically</span> detecting and decoding coded pulses produced by a hammer. Both <span class="hlt">seismic</span> radio and radar are highly robust to signals in high noise environments due to the super-stacking property of TRMs. © 2011 Acoustical Society of America</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S31B2740C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S31B2740C"><span><span class="hlt">Seismicity</span> and source spectra analysis in Salton Sea Geothermal Field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cheng, Y.; Chen, X.</p> <p>2016-12-01</p> <p>The surge of "man-made" earthquakes in recent years has led to considerable concerns about the associated hazards. Improved monitoring of small earthquakes would significantly help understand such phenomena and the underlying physical mechanisms. In the Salton Sea Geothermal field in southern California, open access of a local borehole network provides a unique opportunity to better understand the <span class="hlt">seismicity</span> characteristics, the related earthquake hazards, and the relationship with the geothermal system, tectonic faulting and other physical conditions. We obtain high-resolution earthquake locations in the Salton Sea Geothermal Field, analyze characteristics of spatiotemporal isolated earthquake clusters, magnitude-frequency distributions and spatial variation of stress drops. The analysis reveals spatial coherent distributions of different types of clustering, b-value distributions, and stress drop distribution. The mixture type clusters (short-duration rapid bursts with high aftershock productivity) are predominately located within active geothermal field that correlate with high b-value, low stress drop microearthquake clouds, while regular aftershock sequences and swarms are distributed throughout the study area. The differences between earthquakes inside and outside of geothermal operation field suggest a possible way to distinguish directly induced <span class="hlt">seismicity</span> due to energy operation versus typical <span class="hlt">seismic</span> slip driven sequences. The spatial coherent b-value distribution enables in-situ estimation of probabilities for M≥3 earthquakes, and shows that the high large-magnitude-event (LME) probability zones with high stress drop are likely associated with tectonic faulting. The high stress drop in shallow (1-3 km) depth indicates the existence of active faults, while low stress drops near injection wells likely corresponds to the <span class="hlt">seismic</span> response to fluid injection. I <span class="hlt">interpret</span> the spatial variation of <span class="hlt">seismicity</span> and source characteristics as the result of fluid</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7660M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7660M"><span>New Insights on co-<span class="hlt">seismic</span> landslide clustering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meunier, Patrick; Marc, Odin; Hovius, Niels</p> <p>2015-04-01</p> <p>Earthquake-triggered landslides tend to cluster along topographic crests while rainfall-induced landslides should occur downslope preferentially, where pore pressure induced by groundwater flows is the highest [1]. Past studies on landslide clustering are all based on the analysis of complete dataset or subdataset of landslides associated with a given event (<span class="hlt">seismic</span> or climatic) as a whole. In this work, we document the spatial and temporal variations of the landslide position (on hillslopes) within the epicentral area of the 1994 Northridge, the 1999 Chichi, the 2004 Niigata, the 2008 Iwate and the 2008 Wenchuan earthquakes. We show that crest clustering is not systematic, non uniform in space and exhibit patterns that vary a lot from one case to another. These patterns are not easy to <span class="hlt">interpret</span> as they don't seem to be controlled by a single governing parameter but result from a complex interaction between local (hillslope length and gradient, lithology) and <span class="hlt">seismic</span> (distance to source, slope aspect, radiation pattern, coseismic uplift) parameters. [1] Meunier, P., Hovius, N., & Haines, J. A. (2008). Topographic site effects and the location of earthquake induced landslides. Earth and Planetary Science Letters, 275(3), 221-232</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/862663','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/862663"><span><span class="hlt">Seismic</span> intrusion detector system</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Hawk, Hervey L.; Hawley, James G.; Portlock, John M.; Scheibner, James E.</p> <p>1976-01-01</p> <p>A system for monitoring man-associated <span class="hlt">seismic</span> movements within a control area including a geophone for generating an electrical signal in response to <span class="hlt">seismic</span> movement, a bandpass amplifier and threshold detector for eliminating unwanted signals, pulse counting system for counting and storing the number of <span class="hlt">seismic</span> movements within the area, and a monitoring system operable on command having a variable frequency oscillator generating an audio frequency signal proportional to the number of said <span class="hlt">seismic</span> movements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175396','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175396"><span>Shallow repeating <span class="hlt">seismic</span> events under an alpine glacier at Mount Rainier, Washington, 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>Thelen, Weston A.; Allstadt, Kate E.; De Angelis, Silvio; Malone, Stephen D.; Moran, Seth C.; Vidale, John</p> <p>2013-01-01</p> <p>We observed several swarms of repeating low-frequency (1–5 Hz) <span class="hlt">seismic</span> events during a 3 week period in May–June 2010, near the summit of Mount Rainier, Washington, USA, that likely were a result of stick–slip motion at the base of alpine glaciers. The dominant set of repeating events ('multiplets') featured >4000 individual events and did not exhibit daytime variations in recurrence interval or amplitude. Volcanoes and glaciers around the world are known to produce <span class="hlt">seismic</span> signals with great variability in both frequency content and size. The low-frequency character and periodic recurrence of the Mount Rainier multiplets mimic long-period <span class="hlt">seismicity</span> often seen at volcanoes, particularly during periods of unrest. However, their near-surface location, lack of common spectral peaks across the recording network, rapid attenuation of amplitudes with distance, and temporal correlation with weather systems all indicate that ice-related source mechanisms are the most likely explanation. We <span class="hlt">interpret</span> the low-frequency character of these multiplets to be the result of trapping of <span class="hlt">seismic</span> energy under glacial ice as it propagates through the highly heterogeneous and attenuating volcanic material. The Mount Rainier multiplet sequences underscore the difficulties in differentiating low-frequency signals due to glacial processes from those caused by volcanic processes on glacier-clad volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSeis.tmp...40G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSeis.tmp...40G"><span>Regionalization and dependence of coda Q on frequency and lapse time in the <span class="hlt">seismically</span> active Peloritani region (northeastern Sicily, Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Giampiccolo, Elisabetta; Tuvè, Tiziana</p> <p>2018-05-01</p> <p>The Peloritani region is one of the most <span class="hlt">seismically</span> active regions in Italy and, consequently, the quantification of attenuation of the medium plays an important role for <span class="hlt">seismic</span> risk evaluation. Moreover, it is necessary for the prediction of earth ground motion and future <span class="hlt">seismic</span> source studies. An in depth analysis has been made here to understand the frequency and lapse time dependence of attenuation characteristics of the region by using the coda of local earthquakes. A regionalization is likewise performed in order to investigate the spatial variation of coda Q across the whole region. Finally, our results are jointly <span class="hlt">interpreted</span> with those obtained from recently published 3D velocity tomographies for further insights.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.5486B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.5486B"><span>Dike propagation energy balance from deformation modeling and <span class="hlt">seismic</span> release</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonaccorso, Alessandro; Aoki, Yosuke; Rivalta, Eleonora</p> <p>2017-06-01</p> <p>Magma is transported in the crust mainly by dike intrusions. In volcanic areas, dikes can ascend toward the free surface and also move by lateral propagation, eventually feeding flank eruptions. Understanding dike mechanics is a key to forecasting the expected propagation and associated hazard. Several studies have been conducted on dike mechanisms and propagation; however, a less in-depth investigated aspect is the relation between measured dike-induced deformation and the <span class="hlt">seismicity</span> released during its propagation. We individuated a simple x that can be used as a proxy of the expected mechanical energy released by a propagating dike and is related to its average thickness. For several intrusions around the world (Afar, Japan, and Mount Etna), we correlate such mechanical energy to the <span class="hlt">seismic</span> moment released by the induced earthquakes. We obtain an empirical law that quantifies the expected <span class="hlt">seismic</span> energy released before arrest. The proposed approach may be helpful to predict the total <span class="hlt">seismic</span> moment that will be released by an intrusion and thus to control the energy status during its propagation and the time of dike arrest.<<span class="hlt">abstract</span> type="synopsis"><title type="main">Plain Language SummaryDike propagation is a dominant mechanism for magma ascent, transport, and eruptions. Besides being an intriguing physical process, it has critical hazard implications. After the magma intrusion starts, it is difficult to predict when and where a specific horizontal dike is going to halt and what its final length will be. In our study, we singled an equation that can be used as a proxy of the expected mechanical energy to be released by the opening dike. We related this expected energy to the <span class="hlt">seismic</span> moment of several eruptive intrusions around the world (Afar region, Japanese volcanoes, and Mount Etna). The proposed novel approach is helpful to estimate the total <span class="hlt">seismic</span> moment to be released, therefore allowing potentially predicting when the dike will end its propagation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4811R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4811R"><span>Nature of the <span class="hlt">seismic</span> crust at the Aegir Ridge: A downward continuation approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rai, Abhishek; Breivik, Asbj|rn; Mjelde, Rolf; Hanan, Barry; Ito, Garrett; Sayit, Kaan; Howell, Sam; Vogt, Peter; Pedersen, Rolf-Birger</p> <p>2013-04-01</p> <p>The marine <span class="hlt">seismic</span> data are influenced by variations in the thickness and velocity of the water column which causes fluctuations in the arrival times of <span class="hlt">seismic</span> phases. Downward continuation of the ocean-bottom seismometer data are used to remove the contributions of the water column by bring the shot and receiver at a common datum such as the seafloor. Additionally, the downward continuation focus the <span class="hlt">seismic</span> energy and hence improves the resolution. We apply the downward continuation technique to analyze the OBS data collected along the eastern shoulder of the Aegir Ridge. The Aegir Ridge is an extinct spreading ridge in the North-East Atlantic ocean. Its proximity to the active Iceland hot-spot makes it important for understanding the process of hotspot-ridge interaction during the Oligocene. We present results of an OBS experiment, supported by single channel streamer, gravity and magnetic observations. Usable <span class="hlt">seismic</span> data from 20 OBSs distributed along ~550 km length of the profile reveal the variations in crustal thickness and <span class="hlt">seismic</span> velocities. Regional magnetic anomalies show a faster spreading rate towards the north and a slower spreading towards the southern end near the Iceland hotspot during the active period of the ridge. However, the observed and the predicted crustal thickness show an opposite trend. We <span class="hlt">interpret</span> this anti-correlation between the seafloor spreading rate and the crustal thickness as a result of the interaction between the Iceland hotspot and the Aegir Ridge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2948P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2948P"><span>Detection and <span class="hlt">interpretation</span> of seismoacoustic events at German infrasound stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pilger, Christoph; Koch, Karl; Ceranna, Lars</p> <p>2016-04-01</p> <p>Three infrasound arrays with collocated or nearby installed seismometers are operated by the Federal Institute for Geosciences and Natural Resources (BGR) as the German National Data Center (NDC) for the verification of the Comprehensive Nuclear-Test-Ban Treaty (CTBT). Infrasound generated by seismoacoustic events is routinely detected at these infrasound arrays, but air-to-ground coupled acoustic waves occasionally show up in seismometer recordings as well. Different natural and artificial sources like meteoroids as well as industrial and mining activity generate infrasonic signatures that are simultaneously detected at microbarometers and seismometers. Furthermore, many near-surface sources like earthquakes and explosions generate both <span class="hlt">seismic</span> and infrasonic waves that can be detected successively with both technologies. The combined <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> and acoustic signatures provides additional information about the origin time and location of remote infrasound events or about the characterization of <span class="hlt">seismic</span> events distinguishing man-made and natural origins. Furthermore, seismoacoustic studies help to improve the modelling of infrasound propagation and ducting in the atmosphere and allow quantifying the portion of energy coupled into ground and into air by seismoacoustic sources. An overview of different seismoacoustic sources and their detection by German infrasound stations as well as some conclusions on the benefit of a combined seismoacoustic analysis are presented within this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RMRE...51..893O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RMRE...51..893O"><span><span class="hlt">Seismic</span> Design of a Single Bored Tunnel: Longitudinal Deformations and <span class="hlt">Seismic</span> Joints</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oh, J.; Moon, T.</p> <p>2018-03-01</p> <p>The large diameter bored tunnel passing through rock and alluvial deposits subjected to <span class="hlt">seismic</span> loading is analyzed for estimating longitudinal deformations and member forces on the segmental tunnel liners. The project site has challenges including high hydrostatic pressure, variable ground profile and high <span class="hlt">seismic</span> loading. To ensure the safety of segmental tunnel liner from the <span class="hlt">seismic</span> demands, the performance-based two-level design earthquake approach, Functional Evaluation Earthquake and Safety Evaluation Earthquake, has been adopted. The longitudinal tunnel and ground response <span class="hlt">seismic</span> analyses are performed using a three-dimensional quasi-static linear elastic and nonlinear elastic discrete beam-spring elements to represent segmental liner and ground spring, respectively. Three components (longitudinal, transverse and vertical) of free-field ground displacement-time histories evaluated from site response analyses considering wave passage effects have been applied at the end support of the strain-compatible ground springs. The result of the longitudinal <span class="hlt">seismic</span> analyses suggests that <span class="hlt">seismic</span> joint for the mitigation measure requiring the design deflection capacity of 5-7.5 cm is to be furnished at the transition zone between hard and soft ground condition where the maximum member forces on the segmental liner (i.e., axial, shear forces and bending moments) are induced. The paper illustrates how detailed numerical analyses can be practically applied to evaluate the axial and curvature deformations along the tunnel alignment under difficult ground conditions and to provide the <span class="hlt">seismic</span> joints at proper locations to effectively reduce the <span class="hlt">seismic</span> demands below the allowable levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMED31B0858B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMED31B0858B"><span>The Effect of Regional Tectonics on Faults in Bonaire and the Bonaire Basin: A <span class="hlt">Seismic</span> Reflection Study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brandl, C.; Reece, R.; Bayer, J.; Bales, M. K.</p> <p>2016-12-01</p> <p>Bonaire is located on the Bonaire microplate between the Caribbean and South American plates, and is part of the Netherlands Leeward Antilles as well as the ABC Islands along with Aruba and Curacao. As the major tectonic plates move they stress the microplate, which causes deformation as faulting. This study utilizes legacy <span class="hlt">seismic</span> reflection data combined with a recent nearshore survey to study tectonic deformation in the basins surrounding Bonaire. Our legacy data covers a large portion of the ABC Islands; one dataset is a 1981 multichannel <span class="hlt">seismic</span> (MCS) WesternGeco survey and the other is a 1971 USGS survey that we converted from print to SEGY. The modern dataset (2013) is a high-resolution MCS survey acquired off the western coast of Bonaire. We will use the legacy datasets to validate previous <span class="hlt">interpretations</span> in the nearshore environment and extend these <span class="hlt">interpretations</span> to the deepwater basins. Faults influenced by regional tectonics are more evident in deepwater basins because of their lateral continuity, and offset of thick sedimentary strata. A recent study of nearshore Bonaire utilizing the high-resolution <span class="hlt">seismic</span> dataset <span class="hlt">interpreted</span> several NE-SW dipping normal faults, which may correspond to regional extension. However, the influence is not clear, perhaps due to a lack of data or the nearshore nature of the dataset. Analysis of the legacy datasets show several areas in the surrounding basins with faults dipping NE-SW. Further analysis may reinforce observations made in the nearshore environment. Studying the tectonics of Bonaire can provide insight about the evolution of the region and help better define the effect of regional tectonic forces on the microplate. This study also shows the benefit of legacy <span class="hlt">seismic</span> datasets that are publically available but stored as print or film in conjunction with modern data. They can provide value to a modern study by expanding the scope of available data as well as increasing the number of questions a study can</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70107484','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70107484"><span><span class="hlt">Seismicity</span> and <span class="hlt">seismic</span> structure at Okmok Volcano, Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ohlendorf, Summer J.; Thurber, Clifford H.; Pesicek, Jeremy D.; Prejean, Stephanie G.</p> <p>2014-01-01</p> <p>Okmok volcano is an active volcanic caldera located on the northeastern portion of Umnak Island in the Aleutian arc, with recent eruptions in 1997 and 2008. The Okmok area had ~900 locatable earthquakes between 2003 and June 2008, and an additional ~600 earthquakes from the beginning of the 2008 eruption to mid 2009, providing an adequate dataset for <span class="hlt">seismic</span> tomography. To image the <span class="hlt">seismic</span> velocity structure of Okmok, we apply waveform cross-correlation using bispectrum verification and double-difference tomography to a subset of these earthquakes. We also perform P-wave attenuation tomography using a spectral decay technique. We examine the spatio-temporal characteristics of <span class="hlt">seismicity</span> in the opening sequence of the 2008 eruption to investigate the path of magma migration during the establishment of a new eruptive vent. We also incorporate the new earthquake relocations and three-dimensional (3D) velocity model with first-motion polarities to compute focal mechanisms for selected events in the 2008 pre-eruptive and eruptive periods. Through these techniques we obtain precise relocations, a well-constrained 3D P-wave velocity model, and a marginally resolved S-wave velocity model. We image a main low Vp and Vs anomaly directly under the caldera consisting of a shallow zone at 0–2 km depth connected to a larger deeper zone that extends to about 6 km depth. We find that areas of low Qp are concentrated in the central to southwestern portion of the caldera and correspond fairly well with areas of low Vp. We <span class="hlt">interpret</span> the deeper part of the low velocity anomaly (4–6 km depth) beneath the caldera as a magma body. This is consistent with results from ambient noise tomography and suggests that previous estimates of depth to Okmok's magma chamber based only on geodetic data may be too shallow. The distribution of events preceding the 2008 eruption suggest that a combination of overpressure in the zone surrounding the magma chamber and the introduction of new material</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/872840','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/872840"><span>Method of migrating <span class="hlt">seismic</span> records</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Ober, Curtis C.; Romero, Louis A.; Ghiglia, Dennis C.</p> <p>2000-01-01</p> <p>The present invention provides a method of migrating <span class="hlt">seismic</span> records that retains the information in the <span class="hlt">seismic</span> records and allows migration with significant reductions in computing cost. The present invention comprises phase encoding <span class="hlt">seismic</span> records and combining the encoded <span class="hlt">seismic</span> records before migration. Phase encoding can minimize the effect of unwanted cross terms while still allowing significant reductions in the cost to migrate a number of <span class="hlt">seismic</span> records.</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('http://adsabs.harvard.edu/abs/2017AGUFM.S31A0802C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S31A0802C"><span>Observing Drought-Induced Groundwater Depletion in California with <span class="hlt">Seismic</span> Noise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clements, T.; Denolle, M.</p> <p>2017-12-01</p> <p>While heavy rainfall replenished reservoirs and snowpack recovered in winter 2016/2017, groundwater levels across much of California are still at or near all-time lows following one of the worst droughts in the state's history. Groundwater depletion in California has been studied extensively using GPS, InSAR, and GRACE. Here, we propose to monitor groundwater levels across California through measuring the temporal variation in <span class="hlt">seismic</span> velocity (dv/v) at a regional scale. In the last decade, dv/v has emerged as a technique to investigate near surface and surficial processes such as landslides, volcanic eruptions, and earthquakes. Toward predicting groundwater levels through real-time monitoring with <span class="hlt">seismic</span> noise, we investigate the relations between the dv/v time series and observed groundwater levels. 12 years (Jan 2006 - July 2017) of noise cross-correlation functions (CCF) are computed from continuous vertical component <span class="hlt">seismic</span> data recorded at 100+ sites across California. Velocity changes (dv/v) are obtained by inverting all daily CCFs to produce a dv/v time series for each station pair. Our preliminary results show a seasonal variation in dv/v along with a gradual increase in dv/v throughout the drought. We <span class="hlt">interpret</span> the increase in dv/v as a response to declining groundwater levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T11D..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T11D..05S"><span>Deep <span class="hlt">Seismic</span> Reflection Images of the Sumatra <span class="hlt">Seismic</span> and Aseismic Gaps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Singh, S. C.; Hananto, N. D.; Chauhan, A.; Carton, H. D.; Midenet, S.; Djajadihardja, Y.</p> <p>2009-12-01</p> <p>The Sumatra subduction zone is <span class="hlt">seismically</span> most active region on the Earth, and has been the site of three great earthquakes only in the last four years. The first of the series, the 2004 Boxing Day earthquake, broke 1300 km of the plate boundary and produced the devastating tsunami around the Indian Ocean. The second great earthquake occurred three months later in March 2005, about 150 km SE of the 2004 event. The Earth waited for three years, and then broke again in September 2007 at 1300 km SE of the 2004 event producing a twin earthquake of magnitudes of 8.5 and 7.9 at an interval of 12 hours, leaving a <span class="hlt">seismic</span> gap of about 600 km between the second and third earthquake, the Sumatra <span class="hlt">Seismic</span> Gap. Seismological and geodetic studies suggest that this gap is fully locked and may break any time. In order to study the <span class="hlt">seismic</span> and tsunami risk in this locked region, a deep <span class="hlt">seismic</span> reflection survey (Tsunami Investigation Deep Evaluation <span class="hlt">Seismic</span> -TIDES) was carried out in May 2009 using the CGGVeritas vessel Geowave Champion towing a 15 long streamer, the longest ever used during a <span class="hlt">seismic</span> survey, to image the nature of the subducting plate and associated features, including the seismogenic zone, from seafloor down to 50 km depth. A total of 1700 km of deep <span class="hlt">seismic</span> reflection data were acquired. Three dip lines traverse the Sumatra subduction zone; one going through the Sumatra <span class="hlt">Seismic</span> Gap, one crossing the region that broke during the 2007 great earthquake, and one going through the aseismic zone. These three dip profiles should provide insight about the locking mechanism and help us to understand why an earthquake occurs in one zone and not in aseismic zone. A strike-line was shot in the forearc basin connecting the locked zone with broken zone profiles, which should provide insight about barriers that might have stopped propagation of 2007 earthquake rupture further northward.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoJI.213.1113K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoJI.213.1113K"><span>The 2014, MW6.9 North Aegean earthquake: <span class="hlt">seismic</span> and geodetic evidence for coseismic slip on persistent asperities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konca, Ali Ozgun; Cetin, Seda; Karabulut, Hayrullah; Reilinger, Robert; Dogan, Ugur; Ergintav, Semih; Cakir, Ziyadin; Tari, Ergin</p> <p>2018-05-01</p> <p>We report that asperities with the highest coseismic slip in the 2014 MW6.9 North Aegean earthquake persisted through the interseismic, coseismic and immediate post-<span class="hlt">seismic</span> periods. We use GPS and <span class="hlt">seismic</span> data to obtain the source model of the 2014 earthquake, which is located on the western extension of the North Anatolian Fault (NAF). The earthquake ruptured a bilateral, 90 km strike-slip fault with three slip patches: one asperity located west of the hypocentre and two to the east with a rupture duration of 40 s. Relocated pre-earthquake <span class="hlt">seismicity</span> and aftershocks show that zones with significant coseismic slip were relatively quiet during both the 7 yr of interseismic and the 3-month aftershock periods, while the surrounding regions generated significant <span class="hlt">seismicity</span> during both the interseismic and post-<span class="hlt">seismic</span> periods. We <span class="hlt">interpret</span> the unusually long fault length and source duration, and distribution of pre- and post-main-shock <span class="hlt">seismicity</span> as evidence for a rupture of asperities that persisted through strain accumulation and coseismic strain release in a partially coupled fault zone. We further suggest that the association of <span class="hlt">seismicity</span> with fault creep may characterize the adjacent Izmit, Marmara Sea and Saros segments of the NAF. Similar behaviour has been reported for sections of the San Andreas Fault, and some large subduction zones, suggesting that the association of <span class="hlt">seismicity</span> with creeping fault segments and rapid relocking of asperities may characterize many large earthquake faults.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.T43B2223C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.T43B2223C"><span>South-Central Tibetan <span class="hlt">Seismicity</span> from HiCLIMB <span class="hlt">Seismic</span> Array Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carpenter, S.; Nabelek, J.; Braunmiller, J.</p> <p>2010-12-01</p> <p>The HiCLIMB broadband passive <span class="hlt">seismic</span> experiment (2002-2005) operated 233 sites along a 800-km long north-south array extending from the Himalayan foreland into the Central Tibetan Plateau and a flanking 350x350 km lateral array in southern Tibet and eastern Nepal. We use data from the experiment’s second phase (June 2004 to August 2005), when stations operated in Tibet, to locate earthquakes in south-central Tibet, a region with no permanent <span class="hlt">seismic</span> network where little is known about its <span class="hlt">seismicity</span>. We used the Antelope software for automatic detection and arrival time picking, event-arrival association and event location. Requiring a low detection and event association threshold initially resulted in ~110,000 declared events. The large database size rendered manual inspection unfeasible and we developed automated post-processing modules to weed out spurious detections and erroneous phase and event associations, which stemmed, e.g., from multiple coincident earthquakes within the array or misplaced <span class="hlt">seismicity</span> from the great 2004 Sumatra earthquake. The resulting database contains ~32,000 events within 5° distance from the closest station. We consider ~7,600 events defined by more than 30 P and S arrivals well located and discuss them here. <span class="hlt">Seismicity</span> in the subset correlates well with mapped faults and structures seen on satellite imagery attesting to high location quality. This is confirmed by non-systematic, kilometer-scale differences between automatic and manual locations for selected events. <span class="hlt">Seismicity</span> in south-central Tibet is intense north of the Yarlung-Tsangpo Suture. Almost 90% of events occurred in the Lhasa Terrane mainly along north-south trending rifts. Vigorous activity (>4,800 events) accompanied two M>6 earthquakes in the Payang Basin (84°E), ~100 km west of the linear array. The Tangra-Yum Co (86.5°E) and Pumqu-Xianza (88°E) rifts were very active (~1,000 events) without dominant main shocks indicating swarm like-behavior possibly related</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016211','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016211"><span><span class="hlt">Seismic</span>-wave attenuation associated with crustal faults in the New Madrid <span class="hlt">seismic</span> zone</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hamilton, R.M.; Mooney, W.D.</p> <p>1990-01-01</p> <p>The attenuation of upper crustal <span class="hlt">seismic</span> waves that are refracted with a velocity of about 6 kilometers per second varies greatly among profiles in the area of the New Madrid <span class="hlt">seismic</span> zone in the central Mississippi Valley. The waves that have the strongest attenuation pass through the <span class="hlt">seismic</span> trend along the axis of the Reelfoot rift in the area of the Blytheville arch. Defocusing of the waves in a low-velocity zone and/ or <span class="hlt">seismic</span> scattering and absorption could cause the attenuation; these effects are most likely associated with the highly deformed rocks along the arch. Consequently, strong <span class="hlt">seismic</span>-wave attenuation may be a useful criterion for identifying seismogenic fault zones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1713796J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1713796J"><span>Real-time monitoring of <span class="hlt">seismicity</span> and deformation during the Bárdarbunga rifting event and associated caldera subsidence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jónsdóttir, Kristín; Ófeigsson, Benedikt; Vogfjörd, Kristín; Roberts, Matthew; Barsotti, Sara; Gudmundsson, Gunnar; Hensch, Martin; Bergsson, Bergur; Kjartansson, vilhjálmur; Erlendsson, Pálmi; Friðriksdóttir, Hildur; Hreinsdóttir, Sigrún; Guðmundsson, Magnús; Sigmundsson, Freysteinn; Árnadóttir, Thóra; Heimisson, Elías; Hjorleifsdóttir, Vala; Soring, Jón; Björnsson, Bogi; Oddsson, Björn</p> <p>2015-04-01</p> <p>We present a monitoring overview of a rifting event and associated caldera subsidence in a glaciated environment during the Bárðarbunga volcanic crisis. Following a slight increase in <span class="hlt">seismicity</span> and a weak deformation signal, noticed a few months before the unrest by the SIL monitoring team, an intense <span class="hlt">seismic</span> swarm began in the subglacial Bárðarbunga caldera on August 16 2014. During the following two weeks, a dyke intruded into the crust beneath the Vatnajökull ice cap, propagating 48 km from the caldera to the east-north-east and north of the glacier where an effusive eruption started in Holuhraun. The eruption is still ongoing at the time of writing and has become the largest eruption in over 200 years in Iceland. The dyke propagation was episodic with a variable rate and on several occasions low frequency <span class="hlt">seismic</span> tremor was observed. Four ice cauldrons, manifestations of small subglacial eruptions, were detected. Soon after the swarm began the 7x11 km wide caldera started to subside and is still subsiding (although at slower rates) and has in total subsided over 60 meters. Unrest in subglacial volcanoes always calls for interdisciplinary efforts and teamwork plays a key role for efficient monitoring. Iceland has experienced six subglacial volcanic crises since modern digital monitoring started in the early 90s. With every crisis the monitoring capabilities, data <span class="hlt">interpretations</span>, communication and information dissemination procedures have improved. The Civil Protection calls for a board of experts and scientists (Civil Protection Science Board, CPSB) to share their knowledge and provide up-to-date information on the current status of the volcano, the relevant hazards and most likely scenarios. The evolution of the rifting was monitored in real-time by the joint <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> and cGPS data. The dyke propagation could be tracked and new, updated models of the dyke volume were presented at the CPSB meetings, often daily. In addition, deformation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70197722','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70197722"><span>Evolution of the 2015 Cotopaxi eruption revealed by combined geochemical & <span class="hlt">seismic</span> 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>Hidalgo, Silvana; Battaglia, Jean; Arellano, Santiago; Sierra, Daniel; Bernard, Benjamin; Parra, Rene; Kelly, Peter; Dinger, Florian; Barrington, Charlotte; Samaniego, Pablo</p> <p>2018-01-01</p> <p>Through integration of multiple data streams to monitor volcanic unrest scientists are able to make more robust eruption forecast and to obtain a more holistic <span class="hlt">interpretation</span> of volcanic systems. We examined gas emission and gas geochemistry, <span class="hlt">seismic</span> and petrologic data recorded during the 2015 unrest of Cotopaxi (Ecuador) in order to decipher the origin and temporal evolution of this eruption. Identification of families of similar <span class="hlt">seismic</span> events and the use of <span class="hlt">seismic</span> amplitude ratios reveals temporal changes in volcanic processes. SO2 (300 to 24000 t/d), BrO/SO2 (5-10 x10-5), SO2/HCl (5.8 ± 4.8 and 6.6 ± 3.0) and CO2/SO2 (0.6 to 2.1) measured throughout the eruption indicate a shallow magmatic source. Bulk ash and glass chemistry indicate a homogenous andesitic (SiO2 wt%=56.94 ± 0.25) magma having undergone extensive S-exsolution and degassing during ascent. These data lead us to <span class="hlt">interpret</span> this eruption as a magma intrusion and ascend to shallow levels. The intrusion progressively interacted with the hydrothermal system, boiled off water, and produced hydromagmatic explosions. A small volume of this intrusion continued to fragment and produced episodic ash emissions until it was sufficiently degassed and rheologically stiff. Based on the 470 kt of measured SO2 we estimate that ~ 65.3 x106 m3 of magma were required to supply the emitted gases. This volume exceeds the volume of erupted juvenile material by a factor of 50. This result emphasizes the importance of careful monitoring of Cotopaxi to identify the intrusion of a new batch of magma, which could rejuvenate the non-erupted material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033979','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033979"><span><span class="hlt">Seismic</span> hazard assessment: Issues and alternatives</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wang, Z.</p> <p>2011-01-01</p> <p><span class="hlt">Seismic</span> hazard and risk are two very important concepts in engineering design and other policy considerations. Although <span class="hlt">seismic</span> hazard and risk have often been used inter-changeably, they are fundamentally different. Furthermore, <span class="hlt">seismic</span> risk is more important in engineering design and other policy considerations. <span class="hlt">Seismic</span> hazard assessment is an effort by earth scientists to quantify <span class="hlt">seismic</span> hazard and its associated uncertainty in time and space and to provide <span class="hlt">seismic</span> hazard estimates for <span class="hlt">seismic</span> risk assessment and other applications. Although <span class="hlt">seismic</span> hazard assessment is more a scientific issue, it deserves special attention because of its significant implication to society. Two approaches, probabilistic <span class="hlt">seismic</span> hazard analysis (PSHA) and deterministic <span class="hlt">seismic</span> hazard analysis (DSHA), are commonly used for <span class="hlt">seismic</span> hazard assessment. Although PSHA has been pro-claimed as the best approach for <span class="hlt">seismic</span> hazard assessment, it is scientifically flawed (i.e., the physics and mathematics that PSHA is based on are not valid). Use of PSHA could lead to either unsafe or overly conservative engineering design or public policy, each of which has dire consequences to society. On the other hand, DSHA is a viable approach for <span class="hlt">seismic</span> hazard assessment even though it has been labeled as unreliable. The biggest drawback of DSHA is that the temporal characteristics (i.e., earthquake frequency of occurrence and the associated uncertainty) are often neglected. An alternative, <span class="hlt">seismic</span> hazard analysis (SHA), utilizes earthquake science and statistics directly and provides a <span class="hlt">seismic</span> hazard estimate that can be readily used for <span class="hlt">seismic</span> risk assessment and other applications. ?? 2010 Springer Basel AG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S54B..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S54B..02D"><span><span class="hlt">Seismic</span> and thermodynamics constraints on temperature and composition of the Italian crust.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Diaferia, G.; Cammarano, F.; Piana Agostinetti, N.; Gao, C.; Boschi, L.; Molinari, I.</p> <p>2017-12-01</p> <p>Describing the variation of temperature and composition within the crust is of key importance for the understanding of its formation, evolution and its volcano-tectonic processes. We combine different geophysical observations with information on material properties, contributing to improve our knowledge on the structure, chemical and thermal heterogeneity of the crust. We use thermodynamic modeling to assess the effects of temperature, pressure and water content on <span class="hlt">seismic</span> velocities. We find that i) temperature, rather than composition and water content, plays a major role in affecting <span class="hlt">seismic</span> properties of crustal rocks, ii) mineralogical phase transitions, such as the α-β quartz transition and the plagioclase breakdown, play an important role on <span class="hlt">seismic</span> observables, iii) the ratio between shear-wave velocity and density does not change appreciably in the crust, even as temperature and mineralogy are varied. Informed by these findings, we apply a trans-dimensional Montecarlo Markov-Chain inversion algorithm to jointly invert Rayleigh wave dispersion curves and receiver functions. Dispersion curves are derived from ambient-noise and provide a homogeneous coverage of the Italian Peninsula. More than 200 receiver functions are used with their error and correlation functions included during the inversion phase, to account for data uncertainty. The ensemble of <span class="hlt">seismic</span> models obtained through the joint inversion is analyzed and preliminary <span class="hlt">interpretations</span> based on petrological and thermodynamics constraints are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511011N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511011N"><span>Very-long-period <span class="hlt">seismic</span> signals - filling the gap between deformation and <span class="hlt">seismicity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neuberg, Jurgen; Smith, Paddy</p> <p>2013-04-01</p> <p>Good broadband <span class="hlt">seismic</span> sensors are capable to record <span class="hlt">seismic</span> transients with dominant wavelengths of several tens or even hundreds of seconds. This allows us to generate a multi-component record of <span class="hlt">seismic</span> volcanic events that are located in between the conventional high to low-frequency <span class="hlt">seismic</span> spectrum and deformation signals. With a much higher temporal resolution and accuracy than e.g. GPS records, these signals fill the gap between <span class="hlt">seismicity</span> and deformation studies. In this contribution we will review the non-trivial processing steps necessary to retrieve ground deformation from the original velocity seismogram and explore which role the resulting displacement signals have in the analysis of volcanic events. We use examples from Soufriere Hills volcano in Montserrat, West Indies, to discuss the benefits and shortcomings of such methods regarding new insights into volcanic processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.9113C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.9113C"><span>Crustal <span class="hlt">seismic</span> anisotropy and structure from textural and <span class="hlt">seismic</span> investigations in the Cycladic region, Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cossette, Élise; Schneider, David; Audet, Pascal; Grasemann, Bernhard</p> <p>2016-04-01</p> <p> studies, and reveal an intra-crustal discontinuity at depth varying from 3 to 11 km, mostly observed in the south-central Aegean. Harmonic decomposition of the receiver functions further indicates layering of both shallow and deep crustal anisotropy related to crustal structures. We model synthetic receiver functions based on constraints from the in situ rock properties that we measured using the EBSD technique. Our results indicate that the shallow upper crustal layer is characterized by metapelites with ~5% anisotropy, underlain by a 20 km thick and anisotropic layer of possible high-pressure rocks comprising blueschist and eclogite and/or restitic crust as a consequence of Miocene magmatism. <span class="hlt">Seismic</span> anisotropy models require a sub-vertical axis of hexagonal symmetry in the upper crust (i.e. radial anisotropy), consistent with in situ rock data. Finally, a thinned crust is likely caused by back-arc extension associated with elevated sub-crustal temperatures, in agreement with thermal isostasy models of back arcs. This study demonstrates the importance of integrating rock textural data with <span class="hlt">seismic</span> velocity profiles in the <span class="hlt">interpretation</span> of crustal architecture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.U54B..06P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.U54B..06P"><span><span class="hlt">Seismic</span> and Geodetic Monitoring of the Nicoya, Costa Rica, <span class="hlt">Seismic</span> Gap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Protti, M.; Gonzalez, V.; Schwartz, S.; Dixon, T.; Kato, T.; Kaneda, Y.; Simila, G.; Sampson, D.</p> <p>2007-05-01</p> <p>The Nicoya segment of the Middle America Trench has been recognized as a mature <span class="hlt">seismic</span> gap with potential to generate a large earthquake in the near future (it ruptured with large earthquakes in 1853, 1900 and 1950). Low level of background <span class="hlt">seismicity</span> and fast crustal deformation of the forearc are indicatives of strong coupling along the plate interface. Given its high <span class="hlt">seismic</span> potential, the available data and especially the fact that the Nicoya peninsula extends over large part of the rupture area, this gap was selected as one of the two sites for a MARGINS-SEIZE experiment. With the goal of documenting the evolution of loading and stress release along this <span class="hlt">seismic</span> gap, an international effort involving several institutions from Costa Rica, the United States and Japan is being carried out for over a decade in the region. This effort involves the installation of temporary and permanent <span class="hlt">seismic</span> and geodetic networks. The <span class="hlt">seismic</span> network includes short period, broad band and strong motion instruments. The <span class="hlt">seismic</span> monitoring has provided valuable information on the geometry and characteristics of the plate interface. The geodetic network includes temporary and permanent GPS stations as well as surface and borehole tiltmeters. The geodetic networks have helped quantify the extend and degree of coupling. A continuously recording, three- station GPS network on the Nicoya Peninsula, Costa Rica, recorded what we believe is the first slow slip event observed along the plate interface of the Costa Rica subduction zone. We will present results from these monitoring networks. Collaborative international efforts are focused on expanding these <span class="hlt">seismic</span> and geodetic networks to provide improved resolution of future creep events, to enhanced understanding of the mechanical behavior of the Nicoya subduction segment of the Middle American Trench and possibly capture the next large earthquake and its potential precursor deformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S41A2764I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S41A2764I"><span><span class="hlt">Seismic</span> Structure of Perth Basin (Australia) and surroundings from Passive <span class="hlt">Seismic</span> Deployments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Issa, N.; Saygin, E.; Lumley, D. E.; Hoskin, T. E.</p> <p>2016-12-01</p> <p>We image the subsurface structure of Perth Basin, Western Australia and surroundings by using ambient <span class="hlt">seismic</span> noise data from 14 <span class="hlt">seismic</span> stations recently deployed by University of Western Australia (UWA) and other available permanent stations from Geoscience Australia <span class="hlt">seismic</span> network and the Australian Seismometers in Schools program. Each of these 14 UWA <span class="hlt">seismic</span> stations comprises a broadband sensor and a high fidelity 3-component 10 Hz geophone, recording in tandem at 250 Hz and 1000 Hz. The other stations used in this study are equipped with short period and broadband sensors. In addition, one shallow borehole station is operated with eight 3 component geophones at depths of between 2 and 44 m. The network is deployed to characterize natural <span class="hlt">seismicity</span> in the basin and to try and identify any microseismic activity across Darling Fault Zone (DFZ), bounding the basin to the east. The DFZ stretches to approximately 1000 km north-south in Western Australia, and is one of the longest fault zones on the earth with a limited number of detected earthquakes. We use <span class="hlt">seismic</span> noise cross- and auto-correlation methods to map <span class="hlt">seismic</span> velocity perturbations across the basin and the transition from DFZ to the basin. Retrieved Green's functions are stable and show clear dispersed waveforms. Travel times of the surface wave Green's functions from noise cross-correlations are inverted with a two-step probabilistic framework to map the absolute shear wave velocities as a function of depth. The single station auto-correlations from the <span class="hlt">seismic</span> noise yields P wave reflectivity under each station, marking the major discontinuities. Resulting images show the shear velocity perturbations across the region. We also quantify the variation of ambient <span class="hlt">seismic</span> noise at different depths in the near surface using the geophones in the shallow borehole array.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005PhDT.......134P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005PhDT.......134P"><span>Tectonic and thermal history of the western Serrania del Interior foreland fold and thrust belt and Guarico Basin, north central Venezuela: Implications of new apatite fission track analysis and <span class="hlt">seismic</span> <span class="hlt">interpretation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perez de Armas, Jaime Gonzalo</p> <p></p> <p>Structural analysis, <span class="hlt">interpretation</span> of <span class="hlt">seismic</span> reflection lines, and apatite fission-track analysis in the Western Serrania del Interior fold and thrust belt and in the Guarico basin of north-central Venezuela indicate that the area underwent Mesozoic and Tertiary-to-Recent deformation. Mesozoic deformation, related to the breakup of Pangea, resulted in the formation of the Espino graben in the southernmost portion of the Guarico basin and in the formation of the Proto-Caribbean lithosphere between the diverging North and South American plates. The northern margin of Venezuela became a northward facing passive margin. Minor normal faults formed in the Guarico basin. The most intense deformation took place in the Neogene when the Leeward Antilles volcanic island arc collided obliquely with South America. The inception of the basal foredeep unconformity in the Late Eocene-Early Oligocene marks the formation of a perisutural basin on top of a buried graben system. It is coeval with minor extension and possible reactivation of Cretaceous normal faults in the Guarico basin. It marks the deepening of the foredeep. Cooling ages derived from apatite fission-tracks suggest that the obduction of the fold and thrust belt in the study area occurred in the Late Oligocene through the Middle Miocene. Field data and <span class="hlt">seismic</span> <span class="hlt">interpretations</span> suggest also that contractional deformation began during the Neogene, and specifically during the Miocene. The most surprising results of the detrital apatite fission-track study are the ages acquired in the sedimentary rocks of the easternmost part of the study area in the foreland fold and thrust belt. They indicate an Eocene thermal event. This event may be related to the Eocene NW-SE convergence of the North and South American plates that must have caused the Proto-Caribbean lithosphere to be shortened. This event is not related to the collision of the arc with South America, as the arc was far to the west during the Eocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S43C2877M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S43C2877M"><span>Tectonic history in the Fort Worth Basin, north Texas, derived from well-log integration with multiple 3D <span class="hlt">seismic</span> reflection surveys: implications for paleo and present-day <span class="hlt">seismicity</span> in the basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Magnani, M. B.; Hornbach, M. J.</p> <p>2016-12-01</p> <p>Oil and gas exploration and production in the Fort Worth Basin (FWB) in north Texas have accelerated in the last 10 years due to the success of unconventional gas production. Here, hydraulic fracturing wastewater is disposed via re-injection into deep wells that penetrate Ordovician carbonate formations. The rise in wastewater injection has coincided with a marked rise in earthquake rates, suggesting a causal relationship between industry practices and <span class="hlt">seismicity</span>. Most studies addressing this relationship in intraplate regions like the FWB focus on current <span class="hlt">seismicity</span>, which provides an a-posteriori assessment of the processes involved. 3D <span class="hlt">seismic</span> reflection data contribute complementary information on the existence, distribution, orientation and long-term deformation history of faults that can potentially become reactivated by the injection process. Here we present new insights into the tectonic evolution of faults in the FWB using multiple 3D <span class="hlt">seismic</span> reflection surveys in the basin, west of the Dallas Fort-Worth Metroplex, where high-volume wastewater injection wells have increased most significantly in number in the past few years. The datasets image with remarkable clarity the 3,300 m-thick sedimentary rocks of the basin, from the crystalline basement to the Cretaceous cover, with particular detail of the Paleozoic section. The data, <span class="hlt">interpreted</span> using coincident and nearby wells to correlate <span class="hlt">seismic</span> reflections with stratigraphic markers, allow us to identify faults, extract their orientation, length and displacements at several geologic time intervals, and therefore, reconstruct the long-term deformation history. Throughout the basin, the data show that all <span class="hlt">seismically</span> detectable faults were active during the Mississippian and Pennsylvanian, but that displacement amounts drop below data resolution ( 7 m) in the post-Pennsylvanian deposits. These results indicate that faults have been inactive for at least the past 300 Ma, until the recent 2008 surge in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918141K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918141K"><span>2D magnetotelluric inversion using reflection <span class="hlt">seismic</span> images as constraints and application in the COSC project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kalscheuer, Thomas; Yan, Ping; Hedin, Peter; Garcia Juanatey, Maria d. l. A.</p> <p>2017-04-01</p> <p>We introduce a new constrained 2D magnetotelluric (MT) inversion scheme, in which the local weights of the regularization operator with smoothness constraints are based directly on the envelope attribute of a reflection <span class="hlt">seismic</span> image. The weights resemble those of a previously published <span class="hlt">seismic</span> modification of the minimum gradient support method introducing a global stabilization parameter. We measure the directional gradients of the <span class="hlt">seismic</span> envelope to modify the horizontal and vertical smoothness constraints separately. An appropriate choice of the new stabilization parameter is based on a simple trial-and-error procedure. Our proposed constrained inversion scheme was easily implemented in an existing Gauss-Newton inversion package. From a theoretical perspective, we compare our new constrained inversion to similar constrained inversion methods, which are based on image theory and <span class="hlt">seismic</span> attributes. Successful application of the proposed inversion scheme to the MT field data of the Collisional Orogeny in the Scandinavian Caledonides (COSC) project using constraints from the envelope attribute of the COSC reflection <span class="hlt">seismic</span> profile (CSP) helped to reduce the uncertainty of the <span class="hlt">interpretation</span> of the main décollement. Thus, the new model gave support to the proposed location of a future borehole COSC-2 which is supposed to penetrate the main décollement and the underlying Precambrian basement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017451','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017451"><span>Reconciling deep <span class="hlt">seismic</span> refraction and reflection data from the grenvillian-appalachian boundary in western New England</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hughes, S.; Luetgert, J.H.; Christensen, N.I.</p> <p>1993-01-01</p> <p>The Grenvillian-Appalachian boundary is characterized by pervasive mylonitic deformation and retrograde alteration of a suite of imbricated allochthonous and parautochthonous gneisses that were thrust upon the Grenvillian continental margin during the lower Paleozoic. <span class="hlt">Seismic</span> reflection profiling across this structural boundary zone reveals prominent dipping reflectors <span class="hlt">interpreted</span> as overthrust basement slices (parautochthons) of the Green Mountain Anticlinorium. In contrast, a <span class="hlt">seismic</span> refraction study of the Grenvillian-Appalachian boundary reveals a sub-horizontally layered <span class="hlt">seismic</span> velocity model that is difficult to reconcile with the pronounced sub-vertical structures observed in the Green mountains. A suite of rock samples was collected from the Green Mountain Anticlinorium and measured at high pressures in the laboratory to determine the <span class="hlt">seismic</span> properties of these allochthonous and parautochthonous gneisses. The laboratory-measured <span class="hlt">seismic</span> velocities agree favorably with the modelled velocity structure across the Grenvillian-Appalachian boundary suggesting that the rock samples are reliable indicators of the rock mass as whole. Samples of the parautochthonous Grenvillian basement exposed in the Green Mountains have lower velocities, by about 0.5 km/s, than lithologically equivalent units exposed in the eastern Adirondack Highlands. Velocity reduction in the Green Mountain parautochthons can be accounted for by retrograde metamorphic alteration (hydration) of the paragneisses. <span class="hlt">Seismic</span> anisotropies, ranging from 2 to 12%, in the mylonitized Green Mountain paragneisses may also contribute to the observation of lower <span class="hlt">seismic</span> velocities, where the direction of ray propagation is normal to the foliation. The velocity properties of the Green Mountain paragneisses are thus insufficiently different from the mantling Appalachian allochthons to permit their resolution by the Ontario-New York-New England <span class="hlt">seismic</span> refraction profile. ?? 1993.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.T23A1999L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.T23A1999L"><span>Sunda-Banda Arc Transition: Marine Multichannel <span class="hlt">Seismic</span> Profiling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lueschen, E.; Mueller, C.; Kopp, H.; Djajadihardja, Y.; Ehrhardt, A.; Engels, M.; Lutz, R.; Planert, L.; Shulgin, A.; Working Group, S.</p> <p>2008-12-01</p> <p>After the Indian Ocean Mw 9.3 earthquake and tsunami on December 26, 2004, intensive research activities focussed on the Sunda Arc subduction system offshore Sumatra. For this area a broad database is now available <span class="hlt">interpreted</span> in terms of plate segmentation and outer arc high evolution. In contrast, the highly active easternmost part of this subduction system, as indicated by the south of Java Mw 7.7 earthquake and tsunami on July 17, 2006, has remained almost unexplored until recently. During RV SONNE cruise SO190 from October until December 2006 almost 5000 km of marine geophysical profiles have been acquired at the eastern Sunda Arc and the transition to the Banda Arc. The SINDBAD project (<span class="hlt">Seismic</span> and Geoacoustic Investigations along the Sunda-Banda Arc Transition) comprises 30-fold multichannel reflection <span class="hlt">seismics</span> with a 3-km streamer, wide-angle OBH/OBS refraction <span class="hlt">seismics</span> for deep velocity control (see poster of Shulgin et al. in this session), swath bathymetry, sediment echosounder, gravimetric and geomagnetic measurements. We present data and <span class="hlt">interpretations</span> of several 250-380 km long, prestack depth-migrated <span class="hlt">seismic</span> sections, perpendicular to the deformation front, based on velocity models from focussing analysis and inversion of OBH/OBS refraction data. We focus on the variability of the lower plate and the tectonic response of the overriding plate in terms of outer arc high formation and evolution, forearc basin development, accretion and erosion processes at the base of the overriding plate. The subducting Indo-Australian Plate is characterized by three segments: i) the Roo Rise with rough topography offshore eastern Java ii) the Argo Abyssal Plain with smooth oceanic crust offshore Bali, Lombok, and Sumbawa, and iii) the Scott Plateau with continental crust colliding with the Banda island arc. The forearc responds to differences in the incoming oceanic plate with the absence of a pronounced forearc basin offshore eastern Java and with development of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210022L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210022L"><span>Messinian <span class="hlt">seismic</span> Markers in the Western Tyrrhenian Sea: preliminary results from the "METYSS" Cruise (June 2009)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lofi, Johanna; Gaullier, Virginie; Sage, Françoise; Chanier, Franck; Deverchere, Jacques; Gorini, Christian; Maillard, Agnès.; Pascucci, Vincenzo; Sellier, Nicolas; Thinon, Isabelle</p> <p>2010-05-01</p> <p>, distribution) of the MSC markers that are similar to those observed in the deep Provençal basin and can thus be <span class="hlt">interpreted</span> in respect to the new nomenclature proposed by Lofi et al. (2010). Several erosion surfaces (MES, TES, BES) and depositional units (UU: Upper Unit; MU: Mobile Unit)are identified. Those two latter commonly form the two upper units of the Messinian trilogy observed in the deep western basin. Observations show that the spatial organization of the Messinian markers strongly varies according to their location on the different margin and basin segments. South-eastward, in the vicinity of the Cornaglia Seamount, salt tectonics appears surprisingly huge. Preliminary <span class="hlt">interpretation</span> suggests a syn-rift character for some of the Messinian deposits. Among other points, we expect from these data to better argue: 1) the paleogeography, paleo-depths, connections and evolution of the basin and sub-basins during the MSC; 2) The base-level dynamics and the modalities of salt precipitation during this event; 3) The interactions between crustal tectonics, salt tectonics and sedimentation in order to precise the relative vertical movements (tilting, subsidence, magmatism…) and geodynamical history of the different segments of the area since 6 Ma. Acknowledgments: This work is founded by "Actions Marges" and "Action Coordonnée Pré-Campagne" - INSU. References: Gaullier V., Lofi J., Sage F., Chanier F., Déverchère J., Dutreuil V., Gorini C., Loncke L., Maillard A., Pascucci V., Thinon I., Sellier N., Suc J.P., Clauzon G. and the METYSS Scientific Party, 2009. The Messinian event on the eastern Sardinian margin (Tyrrhenian sea) from <span class="hlt">seismic</span> study: new insights from the "METYSS" cruise. IAS2009, extended <span class="hlt">abstract</span>, in press. Hsu K.J., Cita M.B. and Ryan, W.B.F., 1973. The origin of the Mediterranean evaporites. Initial Reports of the Deep Sea Drilling Project, U.S. Government Printing Office, Washington, DC, 1203- 1231. Jolivet L., Augier R., Robin C., Suc J.-P. and Rouchy</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNS31A1927L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNS31A1927L"><span>Combined Application of Shallow <span class="hlt">Seismic</span> Reflection and High-resolution Refraction Exploration Approach to Active Fault Survey, Central Orogenic Belt, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, S.; Luo, D.; Yanlin, F.; Li, Y.</p> <p>2016-12-01</p> <p>Shallow <span class="hlt">Seismic</span> Reflection (SSR) is a major geophysical exploration method with its exploration depth range, high-resolution in urban active fault exploration. In this paper, we carried out (SSR) and High-resolution refraction (HRR) test in the Liangyun Basin to explore a buried fault. We used NZ distributed 64 channel <span class="hlt">seismic</span> instrument, 60HZ high sensitivity detector, Geode multi-channel portable acquisition system and hammer source. We selected single side hammer hit multiple overlay, 48 channels received and 12 times of coverage. As there are some coincidence measuring lines of SSR and HRR, we chose multi chase and encounter observation system. Based on the satellite positioning, we arranged 11 survey lines in our study area with total length for 8132 meters. GEOGIGA <span class="hlt">seismic</span> reflection data processing software was used to deal with the SSR data. After repeated tests from the aspects of single shot record compilation, interference wave pressing, static correction, velocity parameter extraction, dynamic correction, eventually got the shallow <span class="hlt">seismic</span> reflection profile images. Meanwhile, we used Canadian technology company good refraction and tomographic imaging software to deal with HRR <span class="hlt">seismic</span> data, which is based on nonlinear first arrival wave travel time tomography. Combined with drilling geological profiles, we explained 11 measured <span class="hlt">seismic</span> profiles. Results show 18 obvious fault feature breakpoints, including 4 normal faults of south-west, 7 reverse faults of south-west, one normal fault of north-east and 6 reverse faults of north-east. Breakpoints buried depth is 15-18 meters, and the inferred fault distance is 3-12 meters. Comprehensive analysis shows that the fault property is reverse fault with northeast incline section, and fewer branch normal faults presenting southwest incline section. Since good corresponding relationship between the <span class="hlt">seismic</span> <span class="hlt">interpretation</span> results, drilling data and SEM results on the property, occurrence, broken length of the fault</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/2017AGUFM.U23B..04G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U23B..04G"><span>Improvement of real-time <span class="hlt">seismic</span> magnitude estimation by combining <span class="hlt">seismic</span> and geodetic instrumentation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D.; Bock, Y.; Melgar, D.</p> <p>2017-12-01</p> <p>Rapid <span class="hlt">seismic</span> magnitude assessment is a top priority for earthquake and tsunami early warning systems. For the largest earthquakes, <span class="hlt">seismic</span> instrumentation tends to underestimate the magnitude, leading to an insufficient early warning, particularly in the case of tsunami evacuation orders. GPS instrumentation provides more accurate magnitude estimations using near-field stations, but isn't sensitive enough to detect the first <span class="hlt">seismic</span> wave arrivals, thereby limiting solution speed. By optimally combining collocated <span class="hlt">seismic</span> and GPS instruments, we demonstrate improved solution speed of earthquake magnitude for the largest <span class="hlt">seismic</span> events. We present a real-time implementation of magnitude-scaling relations that adapts to consider the length of the recording, reflecting the observed evolution of ground motion with time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S53E..05L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S53E..05L"><span>MSNoise: a Python Package for Monitoring <span class="hlt">Seismic</span> Velocity Changes using Ambient <span class="hlt">Seismic</span> Noise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lecocq, T.; Caudron, C.; Brenguier, F.</p> <p>2013-12-01</p> <p>Earthquakes occur every day all around the world and are recorded by thousands of <span class="hlt">seismic</span> stations. In between earthquakes, stations are recording "noise". In the last 10 years, the understanding of this noise and its potential usage have been increasing rapidly. The method, called "<span class="hlt">seismic</span> interferometry", uses the principle that <span class="hlt">seismic</span> waves travel between two recorders and are multiple-scattered in the medium. By cross-correlating the two records, one gets an information on the medium below/between the stations. The cross-correlation function (CCF) is a proxy to the Green Function of the medium. Recent developments of the technique have shown those CCF can be used to image the earth at depth (3D <span class="hlt">seismic</span> tomography) or study the medium changes with time. We present MSNoise, a complete software suite to compute relative <span class="hlt">seismic</span> velocity changes under a <span class="hlt">seismic</span> network, using ambient <span class="hlt">seismic</span> noise. The whole is written in Python, from the monitoring of data archives, to the production of high quality figures. All steps have been optimized to only compute the necessary steps and to use 'job'-based processing. We present a validation of the software on a dataset acquired during the UnderVolc[1] project on the Piton de la Fournaise Volcano, La Réunion Island, France, for which precursory relative changes of <span class="hlt">seismic</span> velocity are visible for three eruptions betwee 2009 and 2011.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMDI41A0332L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMDI41A0332L"><span><span class="hlt">Seismic</span> Attenuation in the African LLSVP Estimated from PcS Phases</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, C.; Grand, S.</p> <p>2017-12-01</p> <p><span class="hlt">Seismic</span> tomography has shown that the lowermost mantle beneath the south central Pacific and southern Africa are marked by broad regions with 3% slower shear velocity than normal. The structures have come to be known as large-low-shear-velocity provinces (LLSVPs). The cause of the <span class="hlt">seismic</span> anomalies associated with the LLSVPs is of great interest to geophysicists as they are related to the chemical, thermal, and dynamic structure of the mantle. Some have <span class="hlt">interpreted</span> the heterogeneity in the LLSVPs to be caused by purely thermal effects while others believe the LLSVPs are chemically distinct from normal mantle. <span class="hlt">Seismic</span> velocity variations alone cannot distinguish the thermal from chemical <span class="hlt">interpretations</span>. Anelastic structure, however, can help discriminate among models of the LLSVPs as intrinsic attenuation is much more sensitive to temperature than to chemical variations. In this study, we use PcS <span class="hlt">seismic</span> waves, from an earthquake located in the Scotia Arc, recorded by 50 broadband seismometers deployed in Southern Africa during the Kaapvaal experiment (1997-1999) to estimate Q in the African LLSVP. With increasing epicentral distances, the upward leg PcS waves in lower mantle sweep from normal mantle into the African LLSVP. We divided the PcS data into a group that sampled the LLSVP and another group that passed through normal lower mantle. We determined Δt* between these two groups by stacking spectra and using the spectral ratio method. The waves passing through the LLSVP are noticeably more attenuated than those outside. Taking Q values outside the LLSVP from different published 1D Q models (e.g. PREM [Dziewonski and Anderson, 1981]; QLM9 [Lawrence and Wysession, 2006a]; QHR12 [Hwang and Ritsema, 2011]), we estimate the corresponding average shear wave Q in the African LLSVP to be 127, 115, and 118, far lower than any published average Earth Q models for the lower mantle. Using a range of activation energies (E*), from 200 - 500 kJ/mol (Matas and Bukowinski</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/environmental-geophysics/seismic-reflection-methods','PESTICIDES'); return false;" href="https://www.epa.gov/environmental-geophysics/seismic-reflection-methods"><span><span class="hlt">Seismic</span> Reflection Methods</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p><span class="hlt">Seismic</span> methods are the most commonly conducted geophysical surveys for engineering investigations. <span class="hlt">Seismic</span> refraction provides engineers and geologists with the most basic of geologic data via simple procedures with common equipment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18667625','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18667625"><span>Discrepancies and rates of publication in orthopaedic sports medicine <span class="hlt">abstracts</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kleweno, Conor P; Bryant, Whitney K; Jacir, Albert M; Levine, William N; Ahmad, Christopher S</p> <p>2008-10-01</p> <p>Presentations of clinically relevant data at AOSSM national meetings are presented yearly and may influence clinical decision making. The incidence of presentations that do not subsequently get published is high, and the numbers of major and minor inconsistencies, once published, are also high. Systematic review. A database was created of all <span class="hlt">abstracts</span> presented at AOSSM meetings from 1999 to 2001 from official program books. To assess whether each <span class="hlt">abstract</span> had been followed by publication in a peer-reviewed journal, a PubMed search was conducted to include a 5-year follow-up for each conference. Minor inconsistencies included differences in title, authors, presentation of all outcomes, and authors' <span class="hlt">interpretation</span> of data. Major inconsistencies included discrepancies in study objective and/or hypothesis, study design, primary and secondary outcome measures, sample size, statistical analysis, results, and standard deviations/confidence intervals. Overall, 98 of the 165 <span class="hlt">abstracts</span> presented at AOSSM national meetings from 1999 to 2001 were published in a peer-reviewed journal within 5 years, a publication rate of 59.4%. The median time to publication for all articles was 21 (range, 1-60) months. The majority of articles (61) were published in the American Journal of Sports Medicine (62.2%). The median number of major and minor inconsistencies from <span class="hlt">abstract</span> to publication was 1 (range, 0-5) and 1 (range, 0-4), respectively. Sixty-two of the 98 published <span class="hlt">abstracts</span> (63%) had at least 1 major inconsistency, while 79 (81%) had at least 1 minor inconsistency. In 5 manuscripts (5%), the authors' <span class="hlt">interpretation</span> of the data had changed, and in 2 (2%), the change essentially invalidated the <span class="hlt">abstract</span>. A large number of scientific presentations do not get published in a peer-reviewed journal. In addition, those published have a significant number of changes that, in a small percentage of cases, alter the validity of the original presentation. Orthopaedic surgeons and other</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010GeoJI.183..339R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010GeoJI.183..339R"><span>High-resolution lithospheric imaging with <span class="hlt">seismic</span> interferometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ruigrok, Elmer; Campman, Xander; Draganov, Deyan; Wapenaar, Kees</p> <p>2010-10-01</p> <p>In recent years, there has been an increase in the deployment of relatively dense arrays of <span class="hlt">seismic</span> stations. The availability of spatially densely sampled global and regional <span class="hlt">seismic</span> data has stimulated the adoption of industry-style imaging algorithms applied to converted- and scattered-wave energy from distant earthquakes, leading to relatively high-resolution images of the lower crust and upper mantle. We use <span class="hlt">seismic</span> interferometry to extract reflection responses from the coda of transmitted energy from distant earthquakes. In theory, higher-resolution images can be obtained when migrating reflections obtained with <span class="hlt">seismic</span> interferometry rather than with conversions, traditionally used in lithospheric imaging methods. Moreover, reflection data allow the straightforward application of algorithms previously developed in exploration seismology. In particular, the availability of reflection data allows us to extract from it a velocity model using standard multichannel data-processing methods. However, the success of our approach relies mainly on a favourable distribution of earthquakes. In this paper, we investigate how the quality of the reflection response obtained with interferometry is influenced by the distribution of earthquakes and the complexity of the transmitted wavefields. Our analysis shows that a reasonable reflection response could be extracted if (1) the array is approximately aligned with an active zone of earthquakes, (2) different phase responses are used to gather adequate angular illumination of the array and (3) the illumination directions are properly accounted for during processing. We illustrate our analysis using a synthetic data set with similar illumination and source-side reverberation characteristics as field data recorded during the 2000-2001 Laramie broad-band experiment. Finally, we apply our method to the Laramie data, retrieving reflection data. We extract a 2-D velocity model from the reflections and use this model to migrate the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.S41B2446G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.S41B2446G"><span><span class="hlt">Seismic</span> databases of The Caucasus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gunia, I.; Sokhadze, G.; Mikava, D.; Tvaradze, N.; Godoladze, T.</p> <p>2012-12-01</p> <p>The Caucasus is one of the active segments of the Alpine-Himalayan collision belt. The region needs continues <span class="hlt">seismic</span> monitoring systems for better understanding of tectonic processes going in the region. <span class="hlt">Seismic</span> Monitoring Center of Georgia (Ilia State University) is operating the digital <span class="hlt">seismic</span> network of the country and is also collecting and exchanging data with neighboring countries. The main focus of our study was to create <span class="hlt">seismic</span> database which is well organized, easily reachable and is convenient for scientists to use. The seismological database includes the information about more than 100 000 earthquakes from the whole Caucasus. We have to mention that it includes data from analog and digital <span class="hlt">seismic</span> networks. The first analog <span class="hlt">seismic</span> station in Georgia was installed in 1899 in the Caucasus in Tbilisi city. The number of analog <span class="hlt">seismic</span> stations was increasing during next decades and in 1980s about 100 analog stations were operated all over the region. From 1992 due to political and economical situation the number of stations has been decreased and in 2002 just two analog equipments was operated. New digital <span class="hlt">seismic</span> network was developed in Georgia since 2003. The number of digital <span class="hlt">seismic</span> stations was increasing and in current days there are more than 25 digital stations operating in the country. The database includes the detailed information about all equipments installed on <span class="hlt">seismic</span> stations. Database is available online. That will make convenient interface for <span class="hlt">seismic</span> data exchange data between Caucasus neighboring countries. It also makes easier both the <span class="hlt">seismic</span> data processing and transferring them to the database and decreases the operator's mistakes during the routine work. The database was created using the followings: php, MySql, Javascript, Ajax, GMT, Gmap, Hypoinverse.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003GeoRL..30.2177Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003GeoRL..30.2177Y"><span>Co-<span class="hlt">seismic</span> slip, post-<span class="hlt">seismic</span> slip, and largest aftershock associated with the 1994 Sanriku-haruka-oki, Japan, earthquake</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yagi, Yuji; Kikuchi, Masayuki; Nishimura, Takuya</p> <p>2003-11-01</p> <p>We analyzed continuous GPS data to investigate the spatio-temporal distribution of co-<span class="hlt">seismic</span> slip, post-<span class="hlt">seismic</span> slip, and largest aftershock associated with the 1994 Sanriku-haruka-oki, Japan, earthquake (Mw = 7.7). To get better resolution for co-<span class="hlt">seismic</span> and post-<span class="hlt">seismic</span> slip distribution, we imposed a weak constraint as a priori information of the co-<span class="hlt">seismic</span> slip determined by <span class="hlt">seismic</span> wave analyses. We found that the post-<span class="hlt">seismic</span> slip during 100 days following the main-shock amount to as much moment release as the main-shock, and that the sites of co-<span class="hlt">seismic</span> slip and post-<span class="hlt">seismic</span> slip are partitioning on a plate boundary region in complimentary fashion. The major post-<span class="hlt">seismic</span> slip was triggered by the mainshock in western side of the co-<span class="hlt">seismic</span> slip, and the extent of the post-<span class="hlt">seismic</span> slip is almost unchanged with time. It rapidly developed a shear stress concentration ahead of the slip area, and triggered the largest aftershock.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=effects+AND+recycling&pg=4&id=ED166752','ERIC'); return false;" href="https://eric.ed.gov/?q=effects+AND+recycling&pg=4&id=ED166752"><span>Drama and Oral <span class="hlt">Interpretation</span>: <span class="hlt">Abstracts</span> of Doctoral Dissertations Published in "Dissertation <span class="hlt">Abstracts</span> International," July through December 1978 (Vol. 39 Nos. 1 through 6).</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>ERIC Clearinghouse on Reading and Communication Skills, Urbana, IL.</p> <p></p> <p>This collection of <span class="hlt">abstracts</span> is part of a continuing series providing information on recent doctoral dissertations. The 15 titles deal with the following topics: interpersonal conflict and the nonviolent peacemaking tradition; theatrical transactional analysis; recycling existing spaces for theatre use; the effect of theatre study on the…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.3160C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.3160C"><span><span class="hlt">Seismic</span> risk perception test</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crescimbene, Massimo; La Longa, Federica; Camassi, Romano; Pino, Nicola Alessandro</p> <p>2013-04-01</p> <p>The perception of risks involves the process of collecting, selecting and <span class="hlt">interpreting</span> signals about uncertain impacts of events, activities or technologies. In the natural sciences the term risk seems to be clearly defined, it means the probability distribution of adverse effects, but the everyday use of risk has different connotations (Renn, 2008). The two terms, hazards and risks, are often used interchangeably by the public. Knowledge, experience, values, attitudes and feelings all influence the thinking and judgement of people about the seriousness and acceptability of risks. Within the social sciences however the terminology of 'risk perception' has become the conventional standard (Slovic, 1987). The mental models and other psychological mechanisms which people use to judge risks (such as cognitive heuristics and risk images) are internalized through social and cultural learning and constantly moderated (reinforced, modified, amplified or attenuated) by media reports, peer influences and other communication processes (Morgan et al., 2001). Yet, a theory of risk perception that offers an integrative, as well as empirically valid, approach to understanding and explaining risk perception is still missing". To understand the perception of risk is necessary to consider several areas: social, psychological, cultural, and their interactions. Among the various research in an international context on the perception of natural hazards, it seemed promising the approach with the method of semantic differential (Osgood, C.E., Suci, G., & Tannenbaum, P. 1957, The measurement of meaning. Urbana, IL: University of Illinois Press). The test on <span class="hlt">seismic</span> risk perception has been constructed by the method of the semantic differential. To compare opposite adjectives or terms has been used a Likert's scale to seven point. The test consists of an informative part and six sections respectively dedicated to: hazard; vulnerability (home and workplace); exposed value (with reference to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMDI21A0391S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMDI21A0391S"><span>Small aperture <span class="hlt">seismic</span> arrays for studying planetary interiors and <span class="hlt">seismicity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmerr, N. C.; Lekic, V.; Fouch, M. J.; Panning, M. P.; Siegler, M.; Weber, R. C.</p> <p>2017-12-01</p> <p><span class="hlt">Seismic</span> arrays are a powerful tool for understanding the interior structure and <span class="hlt">seismicity</span> across objects in the Solar System. Given the operational constraints of ground-based lander investigations, a small aperture <span class="hlt">seismic</span> array can provide many of the benefits of a larger-scale network, but does not necessitate a global deployment of instrumentation. Here we define a small aperture array as a deployment of multiple seismometers, with a separation between instruments of 1-1000 meters. For example, small aperture <span class="hlt">seismic</span> arrays have been deployed on the Moon during the Apollo program, the Active <span class="hlt">Seismic</span> Experiments of Apollo 14 and 16, and the Lunar <span class="hlt">Seismic</span> Profiling Experiment deployed by the Apollo 17 astronauts. Both were high frequency geophone arrays with spacing of 50 meters that provided information on the layering and velocity structure of the uppermost kilometer of the lunar crust. Ideally such arrays would consist of instruments that are 3-axis short period or broadband seismometers. The instruments must have a sampling rate and frequency range sensitivity capable of distinguishing between waves arriving at each station in the array. Both terrestrial analogs and the data retrieved from the Apollo arrays demonstrate the efficacy of this approach. Future opportunities exist for deployment of <span class="hlt">seismic</span> arrays on Europa, asteroids, and other objects throughout the Solar System. Here we will present both observational data and 3-D synthetic modeling results that reveal the sensing requirements and the primary advantages of a small aperture <span class="hlt">seismic</span> array over single station approach. For example, at the smallest apertures of < 1 m, we constrain that sampling rates must exceed 500 Hz and instrument sensitivity must extend to 100 Hz or greater. Such advantages include the improved ability to resolve the location of the sources near the array through detection of backazimuth and differential timing between stations, determination of the small-scale structure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2000/ofr-00-460/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2000/ofr-00-460/"><span>Reprocessing of multi-channel <span class="hlt">seismic</span>-reflection data collected in the Beaufort Sea</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Agena, W.F.; Lee, Myung W.; Hart, P.E.</p> <p>2000-01-01</p> <p>Contained on this set of two CD-ROMs are stacked and migrated multi-channel <span class="hlt">seismic</span>-reflection data for 65 lines recorded in the Beaufort Sea by the United States Geological Survey in 1977. All data were reprocessed by the USGS using updated processing methods resulting in improved <span class="hlt">interpretability</span>. Each of the two CD-ROMs contains the following files: 1) 65 files containing the digital <span class="hlt">seismic</span> data in standard, SEG-Y format; 2) 1 file containing navigation data for the 65 lines in standard SEG-P1 format; 3) an ASCII text file with cross-reference information for relating the sequential trace numbers on each line to cdp numbers and shotpoint numbers; 4) 2 small scale graphic images (stacked and migrated) of a segment of line 722 in Adobe Acrobat (R) PDF format; 5) a graphic image of the location map, generated from the navigation file; 6) PlotSeis, an MS-DOS Application that allows PC users to interactively view the SEG-Y files; 7) a PlotSeis documentation file; and 8) an explanation of the processing used to create the final <span class="hlt">seismic</span> sections (this document).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70188674','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70188674"><span>The use of vertical <span class="hlt">seismic</span> profiles in <span class="hlt">seismic</span> investigations of the earth</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Balch, Alfred H.; Lee, M.W.; Miller, J.J.; Ryder, Robert T.</p> <p>1982-01-01</p> <p>During the past 8 years, the U.S. Geological Survey has conducted an extensive investigation on the use of vertical <span class="hlt">seismic</span> profiles (VSP) in a variety of <span class="hlt">seismic</span> exploration applications. <span class="hlt">Seismic</span> sources used were surface air guns, vibrators, explosives, marine air guns, and downhole air guns. Source offsets have ranged from 100 to 7800 ft. Well depths have been from 1200 to over 10,000 ft. We have found three specific ways in which VSPs can be applied to <span class="hlt">seismic</span> exploration. First, <span class="hlt">seismic</span> events observed at the surface of the ground can be traced, level by level, to their point of origin within the earth. Thus, one can tie a surface profile to a well log with an extraordinarily high degree of confidence. Second, one can establish the detectability of a target horizon, such as a porous zone. One can determine (either before or after surface profiling) whether or not a given horizon or layered sequence returns a detectable reflection to the surface. The amplitude and character of the reflection can also be observed. Third, acoustic properties of a stratigraphic sequence can be measured and sometimes correlated to important exploration parameters. For example, sometimes a relationship between apparent attenuation and sand percentage can be established. The technique shows additional promise of aiding surface exploration indirectly through studies of the evolution of the <span class="hlt">seismic</span> pulse, studies of ghosts and multiples, and studies of <span class="hlt">seismic</span> trace inversion techniques. Nearly all current <span class="hlt">seismic</span> data‐processing techniques are adaptable to the processing of VSP data, such as normal moveout (NMO) corrections, stacking, single‐and multiple‐channel filtering, deconvolution, and wavelet shaping.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5064A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5064A"><span>Structural model of the eastern Achara-Trialeti fold and thrust belt using <span class="hlt">seismic</span> reflection profiles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alania, Victor; Chabukiani, Alexander; Enukidze, Onise; Razmadze, Alexander; Sosson, Marc; Tsereteli, Nino; Varazanashvili, Otar</p> <p>2017-04-01</p> <p>Our study focused on the structural geometry at the eastern Achara-Trialeti fold and thrust belt (ATFTB) located at the retro-wedge of the Lesser Caucasus orogen (Alania et al., 2016a). Our <span class="hlt">interpretation</span> has integrated <span class="hlt">seismic</span> reflection profiles, several oil-wells, and the surface geology data to reveal structural characteristics of the eastern ATFTB. Fault-related folding theories were used to <span class="hlt">seismic</span> <span class="hlt">interpretation</span> (Shaw et al., 2004). <span class="hlt">Seismic</span> reflection data reveal the presence of basement structural wedge, south-vergent backthrust, north-vergent forethrust and some structural wedges (or duplex). The rocks are involved in the deformation range from Paleozoic basement rocks to Tertiary strata. Building of thick-skinned structures of eastern Achara-Trialeti was formed by basement wedges propagated from south to north along detachment horizons within the cover generating thin-skinned structures. The kinematic evolution of the south-vergent backthrust zone with respect to the northward propagating structural wedge (or duplexes). The main style of deformation within the backthrust belt is a series of fault-propagation folds. Frontal part of eastern ATFTB are represent by triangle zone (Alania et al., 2016b; Sosson et al., 2016). A detailed study was done for Tbilisi area: <span class="hlt">seismic</span> refection profiles, serial balanced cross-sections, and earthquakes reveal the presence of an active blind thrust fault beneath Tbilisi. 2 & 3-D structural models show that 2002 Mw 4.5 Tbilisi earthquake related to a north-vergent blind thrust. Empirical relations between blind fault rupture area and magnitude suggest that these fault segments could generate earthquakes of Mw 6.5. The growth fault-propagation fold has been observed near Tbilisi in the frontal part of eastern ATFTB. <span class="hlt">Seismic</span> reflection profile through Ormoiani syncline shows that south-vergent growth fault-propagation fold related to out-of-the-syncline thrust. The outcrop of fault-propagation fold shown the geometry of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUSMNS51A..02F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUSMNS51A..02F"><span>High Resolution Near Surface 3D <span class="hlt">Seismic</span> Experiments: A Carbonate Platform vs. a Siliciclastic Sequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Filippidou, N.; Drijkoningen, G.; Braaksma, H.; Verwer, K.; Kenter, J.</p> <p>2005-05-01</p> <p>, opposing to the predicted <span class="hlt">seismic</span> stratigraphy/geology of the area. The Llumajor Platform has been buried only a few meters at most, therefore primary and secondary porocity remains intact, creating a fractal like environment of scatterers and diffractors. We have <span class="hlt">interpreted</span> two possible reflections, the top of the reef and the water table; the former is nicely coupled with the VSP. The <span class="hlt">seismic</span> wave attenuation observed is believed to be predominantly due to the scattering effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN33A0106B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN33A0106B"><span>4-D Visualization of <span class="hlt">Seismic</span> and Geodetic Data of the Big Island of Hawai'i</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burstein, J. A.; Smith-Konter, B. R.; Aryal, A.</p> <p>2017-12-01</p> <p>For decades Hawai'i has served as a natural laboratory for studying complex interactions between magmatic and <span class="hlt">seismic</span> processes. Investigating characteristics of these processes, as well as the crustal response to major Hawaiian earthquakes, requires a synthesis of <span class="hlt">seismic</span> and geodetic data and models. Here, we present a 4-D visualization of the Big Island of Hawai'i that investigates geospatial and temporal relationships of <span class="hlt">seismicity</span>, <span class="hlt">seismic</span> velocity structure, and GPS crustal motions to known volcanic and <span class="hlt">seismically</span> active features. Using the QPS Fledermaus visualization package, we compile 90 m resolution topographic data from NASA's Shuttle Radar Topography Mission (SRTM) and 50 m resolution bathymetric data from the Hawaiian Mapping Research Group (HMRG) with a high-precision earthquake catalog of more than 130,000 events from 1992-2009 [Matoza et al., 2013] and a 3-D <span class="hlt">seismic</span> velocity model of Hawai'i [Lin et al., 2014] based on <span class="hlt">seismic</span> data from the Hawaiian Volcano Observatory (HVO). Long-term crustal motion vectors are integrated into the visualization from HVO GPS time-series data. These interactive data sets reveal well-defined <span class="hlt">seismic</span> structure near the summit areas of Mauna Loa and Kilauea volcanoes, where high Vp and high Vp/Vs anomalies at 5-12 km depth, as well as clusters of low magnitude (M < 3.5) <span class="hlt">seismicity</span>, are observed. These areas of high Vp and high Vp/Vs are <span class="hlt">interpreted</span> as mafic dike complexes and the surrounding <span class="hlt">seismic</span> clusters are associated with shallow magma processes. GPS data are also used to help identify <span class="hlt">seismic</span> clusters associated with the steady crustal detachment of the south flank of Kilauea's East Rift Zone. We also investigate the fault geometry of the 2006 M6.7 Kiholo Bay earthquake event by analyzing elastic dislocation deformation modeling results [Okada, 1985] and HVO GPS and <span class="hlt">seismic</span> data of this event. We demonstrate the 3-D fault mechanisms of the Kiholo Bay main shock as a combination of strike-slip and dip</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023086','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023086"><span>Geologic structures related to New Madrid earthquakes near Memphis, Tennessee, based on gravity and magnetic <span class="hlt">interpretations</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.; Stuart, W.D.; Talwani, P.</p> <p>2001-01-01</p> <p>New inversions of gravity and magnetic data in the region north of memphis. Tennessee, and south of latitude 36?? define boundaries of regional structures and igneous complexes in the upper crust. Microseismicity patterns near <span class="hlt">interpreted</span> boundaries suggest that igneous complexes influence the locations of microseismicity. A weak <span class="hlt">seismicity</span> cluster occurs near one intrusion (Covington pluton), at the intersection of the southwest margin of the Missouri batholith and the southeast margin of the Reelfoot rift. A narrow <span class="hlt">seismicity</span> trend along the Reelfoot rift axis becomes diffuse near a second intrusion (Osceola intrusive complex) and changes direction to an area along the northwest flank of the intrusion. The axial <span class="hlt">seismicity</span> trend also contains a tight cluster of earthquakes located just outside the Osceola intrusive complex. The mechanical explanation of the two <span class="hlt">seismicity</span> patterns is uncertain, but the first cluster may be caused by stress concentration due to the high elastic stiffness and strength of the Covington intrusion. The spatially changing <span class="hlt">seismicity</span> pattern near the Osceola complex may be caused by the preceding factors plus interaction with faulting along the rift axis. The axial <span class="hlt">seismicity</span> strand itself is one of several connected and interacting active strands that may produce stress concentrations at strand ends and junctions. The microseismicity clusters at the peripheries of the two intrusions lead us to conclude that these stress concentrations or stressed volumes may be locations of future moderate to large earthquakes near Memphis. Published by Elsevier Science B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S33A2745C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S33A2745C"><span><span class="hlt">Seismic</span> Characterization of the Jakarta Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cipta, A.; Saygin, E.; Cummins, P. R.; Masturyono, M.; Rudyanto, A.; Irsyam, M.</p> <p>2015-12-01</p> <p>Jakarta, Indonesia, is home to more than 10 million people. Many of these people live in <span class="hlt">seismically</span> non-resilient structures in an area that historical records suggest is prone to earthquake shaking. The city lies in a sedimentary basin composed of Quaternary alluvium that experiences rapid subsidence (26 cm/year) due to groundwater extraction. Forecasts of how much subsidence may occur in the future are dependent on the thickness of the basin. However, basin geometry and sediment thickness are poorly known. In term of <span class="hlt">seismic</span> hazard, thick loose sediment can lead to high amplification of <span class="hlt">seismic</span> waves, of the kind that led to widespread damage in Mexico city during the Michoacan Earthquake of 1985. In order to characterize basin structure, a temporary seismograph deployment was undertaken in Jakarta in Oct 2013- Jan 2014. A total of 96 <span class="hlt">seismic</span> instrument were deployed throughout Jakarta were deployed throughout Jakarta at 3-5 km spacing. Ambient noise tomography was applied to obtain models of the subsurface velocity structure. Important key, low velocity anomalies at short period (<8s) correspond to the main sedimentary sub-basins thought to be present based on geological <span class="hlt">interpretations</span> of shallow stratigraphy in the Jakarta Basin. The result shows that at a depth of 300 m, shear-wave velocity in the northern part (600 m/s) of the basin is lower than that in the southern part. The most prominent low velocity structure appears in the northwest of the basin, down to a depth of 800 m, with velocity as low as 1200 m/s. This very low velocity indicates the thickness of sediment and the variability of basin geometry. Waveform computation using SPECFEM2D shows that amplification due to basin geometry occurs at the basin edge and the thick sediment leads to amplification at the basin center. Computation also shows the longer shaking duration occurrs at the basin edge and center of the basin. The nest step will be validating the basin model using earthquake events</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JESS..126...83D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JESS..126...83D"><span><span class="hlt">Seismic</span> profile analysis of the Kangra and Dehradun re-entrant of NW Himalayan Foreland thrust belt, India: A new approach to delineate subsurface geometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dey, Joyjit; Perumal, R. Jayangonda; Sarkar, Subham; Bhowmik, Anamitra</p> <p>2017-08-01</p> <p>In the NW Sub-Himalayan frontal thrust belt in India, <span class="hlt">seismic</span> <span class="hlt">interpretation</span> of subsurface geometry of the Kangra and Dehradun re-entrant mismatch with the previously proposed models. These procedures lack direct quantitative measurement on the <span class="hlt">seismic</span> profile required for subsurface structural architecture. Here we use a predictive angular function for establishing quantitative geometric relationships between fault and fold shapes with `Distance-displacement method' (D-d method). It is a prognostic straightforward mechanism to probe the possible structural network from a <span class="hlt">seismic</span> profile. Two <span class="hlt">seismic</span> profiles Kangra-2 and Kangra-4 of Kangra re-entrant, Himachal Pradesh (India), are investigated for the fault-related folds associated with the Balh and Paror anticlines. For Paror anticline, the final cut-off angle β =35{°} was obtained by transforming the <span class="hlt">seismic</span> time profile into depth profile to corroborate the <span class="hlt">interpreted</span> structures. Also, the estimated shortening along the Jawalamukhi Thrust and Jhor Fault, lying between the Himalayan Frontal Thrust (HFT) and the Main Boundary Thrust (MBT) in the frontal fold-thrust belt, were found to be 6.06 and 0.25 km, respectively. Lastly, the geometric method of fold-fault relationship has been exercised to document the existence of a fault-bend fold above the Himalayan Frontal Thrust (HFT). Measurement of shortening along the fault plane is employed as an ancillary tool to prove the multi-bending geometry of the blind thrust of the Dehradun re-entrant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5996D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5996D"><span>New insights on the <span class="hlt">seismic</span> hazard in the Balkans inferred from GPS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>D'Agostino, Nicola; Métois, Marianne; Avallone, Antonio; Chamot-Rooke, Nicolas</p> <p>2014-05-01</p> <p>The Balkans region sits at the transition between stable Eurasia and highly straining continental Eastern Mediterranean, resulting in a widespread <span class="hlt">seismicity</span> and high <span class="hlt">seismic</span> hazard. Because of intensive human and economic development over the last decades, the vulnerability has increased in the region faster than the progress in <span class="hlt">seismic</span> hazard assessments. Opposite to the relatively good understanding of the <span class="hlt">seismicity</span> in plate boundaries contexts, the <span class="hlt">seismic</span> hazard is poorly known in the regions of distributed continental deformation like the Balkan region and is often underestimated (England and Jackson, 2011). Current <span class="hlt">seismic</span> hazard assessments are based on the historical and instrumental catalogues. However, the completeness interval of the historical data bases may be below the average recurrence of individual seismogenic structures. In addition, relatively sparse seismological networks in the region and limited cross-border <span class="hlt">seismic</span> data exchanges cast doubts in seismotectonic <span class="hlt">interpretation</span> and challenge our understanding of <span class="hlt">seismic</span> and geodynamic processes. This results in a inhomogeneous knowledge of the <span class="hlt">seismic</span> hazard of the region to date. Geodetic measurements have the capability to contribute to <span class="hlt">seismic</span> hazard by mapping the field of current active deformation and translating it into estimates of the seismogenic potential. With simple assumptions, measurements of crustal deformation can be translated in estimates of the average frequency and magnitude of the largest events and assessments of the aseismic deformation. GPS networks in the Balkans have been growing during the last few years mainly for civilian application (e.g. Cadastral plan, telecommunications), but opening new opportunities to quantify the present-day rates of crustal deformation. Here we present the initial results of GEOSAB (Geodetic Estimate of Strain Accumulation over Balkans), an AXA-Research-Fund supported project devoted to the estimation of crustal deformation and the</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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