Sample records for zone head waves

  1. Finite-frequency sensitivity kernels for head waves

    NASA Astrophysics Data System (ADS)

    Zhang, Zhigang; Shen, Yang; Zhao, Li

    2007-11-01

    Head waves are extremely important in determining the structure of the predominantly layered Earth. While several recent studies have shown the diffractive nature and the 3-D Fréchet kernels of finite-frequency turning waves, analogues of head waves in a continuous velocity structure, the finite-frequency effects and sensitivity kernels of head waves are yet to be carefully examined. We present the results of a numerical study focusing on the finite-frequency effects of head waves. Our model has a low-velocity layer over a high-velocity half-space and a cylindrical-shaped velocity perturbation placed beneath the interface at different locations. A 3-D finite-difference method is used to calculate synthetic waveforms. Traveltime and amplitude anomalies are measured by the cross-correlation of synthetic seismograms from models with and without the velocity perturbation and are compared to the 3-D sensitivity kernels constructed from full waveform simulations. The results show that the head wave arrival-time and amplitude are influenced by the velocity structure surrounding the ray path in a pattern that is consistent with the Fresnel zones. Unlike the `banana-doughnut' traveltime sensitivity kernels of turning waves, the traveltime sensitivity of the head wave along the ray path below the interface is weak, but non-zero. Below the ray path, the traveltime sensitivity reaches the maximum (absolute value) at a depth that depends on the wavelength and propagation distance. The sensitivity kernels vary with the vertical velocity gradient in the lower layer, but the variation is relatively small at short propagation distances when the vertical velocity gradient is within the range of the commonly accepted values. Finally, the depression or shoaling of the interface results in increased or decreased sensitivities, respectively, beneath the interface topography.

  2. Incorporating fault zone head wave and direct wave secondary arrival times into seismic tomography: Application at Parkfield, California

    NASA Astrophysics Data System (ADS)

    Bennington, N. L.; Thurber, C. H.; Zhang, H.; Peng, Z.; Zhao, P.

    2011-12-01

    Large crustal faults such as the San Andreas fault (SAF) often juxtapose rocks of significantly different elastic properties, resulting in well-defined bimaterial interfaces. A sharp material contrast across the fault interface is expected to generate fault zone head waves (FZHW's) that spend a large portion of their propagation paths refracting along the bimaterial interface (Ben-Zion 1989, 1990; Ben-Zion & Aki 1990). Because of this FZHW's provide a high-resolution tool for imaging the velocity contrast across the fault. Recently, Zhao et al. (2010) systematically analyzed large data sets of near-fault waveforms recorded by several permanent and temporary seismic networks along the Parkfield section of the SAF. The local-scale tomography study of Zhang et al. (2009) for a roughly 10 km3 volume centered on SAFOD and the more regional-scale study of Thurber et al. (2006) for a 130 km x 120 km x 20 km volume centered on the 2004 Parkfield earthquake rupture provide what are probably the best 3D images of the seismic velocity structure of the area. The former shows a low velocity zone associated with the SAF extending to significant depth, and both image the well-known velocity contrast across the fault. Seismic tomography generally uses just first P and/or S arrivals because of the relative simplicity of phase picking and ray tracing. Adding secondary arrivals such as FZHW's, however, can enhance the resolution of structure and strengthen constraints on earthquake locations and focal mechanisms. We present a model of 3D velocity structure for the Parkfield region that utilizes a combination of arrival times for FZHW's and the associated direct-wave secondary arrivals as well as existing P-wave arrival time data. The resulting image provides a higher-resolution model of the SAF at depth than previously published models. In addition, we plan to measure polarizations of the direct P and S waves and FZHW's and incorporate the data into our updated velocity tomography

  3. Automatic identification of fault zone head waves and direct P waves and its application in the Parkfield section of the San Andreas Fault, California

    NASA Astrophysics Data System (ADS)

    Li, Zefeng; Peng, Zhigang

    2016-06-01

    Fault zone head waves (FZHWs) are observed along major strike-slip faults and can provide high-resolution imaging of fault interface properties at seismogenic depth. In this paper, we present a new method to automatically detect FZHWs and pick direct P waves secondary arrivals (DWSAs). The algorithm identifies FZHWs by computing the amplitude ratios between the potential FZHWs and DSWAs. The polarities, polarizations and characteristic periods of FZHWs and DSWAs are then used to refine the picks or evaluate the pick quality. We apply the method to the Parkfield section of the San Andreas Fault where FZHWs have been identified before by manual picks. We compare results from automatically and manually picked arrivals and find general agreement between them. The obtained velocity contrast at Parkfield is generally 5-10 per cent near Middle Mountain while it decreases below 5 per cent near Gold Hill. We also find many FZHWs recorded by the stations within 1 km of the background seismicity (i.e. the Southwest Fracture Zone) that have not been reported before. These FZHWs could be generated within a relatively wide low velocity zone sandwiched between the fast Salinian block on the southwest side and the slow Franciscan Mélange on the northeast side. Station FROB on the southwest (fast) side also recorded a small portion of weak precursory signals before sharp P waves. However, the polarities of weak signals are consistent with the right-lateral strike-slip mechanisms, suggesting that they are unlikely genuine FZHW signals.

  4. Incorporating fault zone head wave and direct wave secondary arrival times into seismic tomography: Application at Parkfield, California

    NASA Astrophysics Data System (ADS)

    Bennington, Ninfa L.; Thurber, Clifford; Peng, Zhigang; Zhang, Haijiang; Zhao, Peng

    2013-03-01

    We present a three-dimensional (3D) P wave velocity (Vp) model of the Parkfield region that utilizes existing P wave arrival time data, including fault zone head waves (FZHWs), and data from direct wave secondary arrivals (DWSAs). The first-arrival and DWSA travel times are obtained as the global- and local-minimum travel time paths, respectively. The inclusion of FZHWs and DWSAs results in as much as a 5% and a 10% increase in the across-fault velocity contrast, respectively, for the Vp model at Parkfield relative to that of Thurber et al. [2006]. Viewed along strike, three pronounced velocity contrast regions are observed: a pair of strong positive velocity contrasts (SW fast), one NW of the 1966 Parkfield earthquake hypocenter and the other SE of the 2004 Parkfield earthquake hypocenter, and a strong negative velocity contrast (NE fast) between the two hypocenters. The negative velocity contrast partially to entirely encompasses peak coseismic slip estimated in several slip models for the 2004 earthquake, suggesting that the negative velocity contrast played a part in defining the rupture patch of the 2004 Parkfield earthquake. Following Ampuero and Ben-Zion (2008), the pattern of velocity contrasts is consistent with the observed bilateral rupture propagation for the 2004 Parkfield earthquake. Although the velocity contrasts also suggest bilateral rupture propagation for the 1966 Parkfield earthquake, the fault is creeping to the NW here, i.e., exhibiting velocity-strengthening behavior. Thus, it is not surprising that rupture propagated only SE during this event.

  5. Travelling and splitting of a wave of hedgehog expression involved in spider-head segmentation.

    PubMed

    Kanayama, Masaki; Akiyama-Oda, Yasuko; Nishimura, Osamu; Tarui, Hiroshi; Agata, Kiyokazu; Oda, Hiroki

    2011-10-11

    During development segmentation is a process that generates a spatial periodic pattern. Peak splitting of waves of gene expression is a mathematically predicted, simple strategy accounting for this type of process, but it has not been well characterized biologically. Here we show temporally repeated splitting of gene expression into stripes that is associated with head axis growth in the spider Achaearanea embryo. Preceding segmentation, a wave of hedgehog homologue gene expression is observed to travel posteriorly during development stage 6. This stripe, co-expressing an orthodenticle homologue, undergoes two cycles of splitting and shifting accompanied by convergent extension, serving as a generative zone for the head segments. The two orthodenticle and odd-paired homologues are identified as targets of Hedgehog signalling, and evidence suggests that their activities mediate feedback to maintain the head generative zone and to promote stripe splitting in this zone. We propose that the 'stripe-splitting' strategy employs genetic components shared with Drosophila blastoderm subdivision, which are required for participation in an autoregulatory signalling network.

  6. Head wave correlations in ambient noise.

    PubMed

    Gebbie, John; Siderius, Martin

    2016-07-01

    Ambient ocean noise is processed with a vertical line array to reveal coherent time-separated arrivals suggesting the presence of head wave multipath propagation. Head waves, which are critically propagating water waves created by seabed waves traveling parallel to the water-sediment interface, can propagate faster than water-only waves. Such eigenrays are much weaker than water-only eigenrays, and are often completely overshadowed by them. Surface-generated noise is different whereby it amplifies the coherence between head waves and critically propagating water-only waves, which is measured by cross-correlating critically steered beams. This phenomenon is demonstrated both experimentally and with a full wave simulation.

  7. Seismic Velocity Structure of the San Jacinto Fault Zone from Double-Difference Tomography and Expected Distribution of Head Waves

    NASA Astrophysics Data System (ADS)

    Allam, A. A.; Ben-Zion, Y.

    2010-12-01

    We present initial results of double-difference tomographic images for the velocity structure of the San Jacinto Fault Zone (SJFZ), and related 3D forward calculations of waves in the immediate vicinity of the SJFZ. We begin by discretizing the SJFZ region with a uniform grid spacing of 500 m, extending 140 km by 80 km and down to 25 km depth. We adopt the layered 1D model of Dreger & Helmberger (1993) as a starting model for this region, and invert for 3D distributions of VP and VS with the double-difference tomography of Zhang & Thurber (2003), which makes use of absolute event-station travel times as well as relative travel times for phases from nearby event pairs. Absolute arrival times of over 78,000 P- and S-wave phase picks generated by 1127 earthquakes and recorded at 70 stations near the SJFZ are used. Only data from events with Mw greater than 2.2 are used. Though ray coverage is limited at shallow depths, we obtain relatively high-resolution images from 4 to 13 km which show a clear contrast in velocity across the NW section of the SJFZ. To the SE, in the so-called trifurcation area, the structure is more complicated, though station coverage is poorest in this region. Using the obtained image, the current event locations, and the 3D finite-difference code of Olsen (1994), we estimate the likely distributions of fault zone head waves as a tool for future deployment of instrument. We plan to conduct further studies by including more travel time picks, including those from newly-deployed stations in the SJFZ area, in order to gain a more accurate image of the velocity structure.

  8. Short-crested waves in the surf zone

    NASA Astrophysics Data System (ADS)

    Wei, Zhangping; Dalrymple, Robert A.; Xu, Munan; Garnier, Roland; Derakhti, Morteza

    2017-05-01

    This study investigates short-crested waves in the surf zone by using the mesh-free Smoothed Particle Hydrodynamics model, GPUSPH. The short-crested waves are created by generating intersecting wave trains in a numerical wave basin with a beach. We first validate the numerical model for short-crested waves by comparison with large-scale laboratory measurements. Then short-crested wave breaking over a planar beach is studied comprehensively. We observe rip currents as discussed in Dalrymple (1975) and undertow created by synchronous intersecting waves. The wave breaking of the short-crested wavefield created by the nonlinear superposition of intersecting waves and wave-current interaction result in the formation of isolated breakers at the ends of breaking wave crests. Wave amplitude diffraction at these isolated breakers gives rise to an increase in the alongshore wave number in the inner surf zone. Moreover, 3-D vortices and multiple circulation cells with a rotation frequency much lower than the incident wave frequency are observed across the outer surf zone to the beach. Finally, we investigate vertical vorticity generation under short-crested wave breaking and find that breaking of short-crested waves generates vorticity as pointed out by Peregrine (1998). Vorticity generation is not only observed under short-crested waves with a limited number of wave components but also under directional wave spectra.

  9. The incorporation of fault zone head wave and direct wave secondary arrival times and arrival polarizations into seismic tomography: Application to the Parkfield, California area

    NASA Astrophysics Data System (ADS)

    Bennington, N. L.; Thurber, C. H.; Peng, Z.; Zhao, P.

    2012-12-01

    We present a 3D P-wave velocity (Vp) model of the Parkfield region that utilizes existing P-wave arrival time data, including fault zone head waves (FZHW), plus new data from direct wave secondary arrivals (DWSA). The first-arrival and DWSA travel times are obtained as the global and local minimum travel time paths, respectively. The inclusion of DWSA results in as much as a 10% increase in the across-fault velocity contrast for the Vp model at Parkfield relative to Thurber et al. (2006). Viewed along strike, three pronounced velocity contrast regions are observed: a pair of strong positive velocity contrasts (SW fast), one NW of the 1966 Parkfield hypocenter and the other SE of the 2004 Parkfield hypocenter, and a strong negative velocity contrast (NE fast) between the two hypocenters. The negative velocity contrast partially to entirely encompasses peak coseismic slip estimated in several slip models for the 2004 earthquake, suggesting that the negative velocity contrast played a part in defining the rupture patch of the 2004 Parkfield earthquake. We expand on this work by modifying our seismic tomography algorithm to incorporate arrival polarizations (azimuths). Synthetic tests will be presented to demonstrate the improvements in velocity structure when arrival polarizations are incorporated. These tests will compare the synthetic model recovered when FZHW/DWSA arrivals as well as existing P-wave arrival time data are inverted to that recovered with the same dataset with the inclusion of arrival polarizations. We plan to extend this work to carry out a full scale seismic tomography/relocation inversion at Parkfield, CA utilizing arrival polarizations from all first-P arrivals, and FZHW/DWSA arrivals as well as existing P-wave arrival time data. This effort requires the determination of polarization data for all P-waves and FZHW's at Parkfield. To this end, we use changes in the arrival azimuth from fault normal to source-receiver direction to identify FZHW and

  10. Extending RTM Imaging With a Focus on Head Waves

    NASA Astrophysics Data System (ADS)

    Holicki, Max; Drijkoningen, Guy

    2016-04-01

    Conventional industry seismic imaging predominantly focuses on pre-critical reflections, muting post-critical arrivals in the process. This standard approach neglects a lot of information present in the recorded wave field. This negligence has been partially remedied with the inclusion of head waves in more advanced imaging techniques, like Full Waveform Inversion (FWI). We would like to see post-critical information leave the realm of labour-intensive travel-time picking and tomographic inversion towards full migration to improve subsurface imaging and parameter estimation. We present a novel seismic imaging approach aimed at exploiting post-critical information, using the constant travel path for head-waves between shots. To this end, we propose to generalize conventional Reverse Time Migration (RTM) to scenarios where the sources for the forward and backward propagated wave-fields are not coinciding. RTM functions on the principle that backward propagated receiver data, due to a source at some locations, must overlap with the forward propagated source wave field, from the same source location, at subsurface scatterers. Where the wave-fields overlap in the subsurface there is a peak at the zero-lag cross-correlation, and this peak is used for the imaging. For the inclusion of head waves, we propose to relax the condition of coincident sources. This means that wave-fields, from non-coincident-sources, will not overlap properly in the subsurface anymore. We can make the wave-fields overlap in the subsurface again, by time shifting either the forward or backward propagated wave-fields until the wave-fields overlap. This is the same as imaging at non-zero cross-correlation lags, where the lag is the travel time difference between the two wave-fields for a given event. This allows us to steer which arrivals we would like to use for imaging. In the simplest case we could use Eikonal travel-times to generate our migration image, or we exclusively image the subsurface

  11. Fault-zone waves observed at the southern Joshua Tree earthquake rupture zone

    USGS Publications Warehouse

    Hough, S.E.; Ben-Zion, Y.; Leary, P.

    1994-01-01

    Waveform and spectral characteristics of several aftershocks of the M 6.1 22 April 1992 Joshua Tree earthquake recorded at stations just north of the Indio Hills in the Coachella Valley can be interpreted in terms of waves propagating within narrow, low-velocity, high-attenuation, vertical zones. Evidence for our interpretation consists of: (1) emergent P arrivals prior to and opposite in polarity to the impulsive direct phase; these arrivals can be modeled as headwaves indicative of a transfault velocity contrast; (2) spectral peaks in the S wave train that can be interpreted as internally reflected, low-velocity fault-zone wave energy; and (3) spatial selectivity of event-station pairs at which these data are observed, suggesting a long, narrow geologic structure. The observed waveforms are modeled using the analytical solution of Ben-Zion and Aki (1990) for a plane-parallel layered fault-zone structure. Synthetic waveform fits to the observed data indicate the presence of NS-trending vertical fault-zone layers characterized by a thickness of 50 to 100 m, a velocity decrease of 10 to 15% relative to the surrounding rock, and a P-wave quality factor in the range 25 to 50.

  12. Fault zone characterization using P- and S-waves

    NASA Astrophysics Data System (ADS)

    Wawerzinek, Britta; Buness, Hermann; Polom, Ulrich; Tanner, David C.; Thomas, Rüdiger

    2014-05-01

    Although deep fault zones have high potential for geothermal energy extraction, their real usability depends on complex lithological and tectonic factors. Therefore a detailed fault zone exploration using P- and S-wave reflection seismic data is required. P- and S-wave reflection seismic surveys were carried out along and across the eastern border of the Leinetal Graben in Lower Saxony, Germany, to analyse the structural setting, different reflection characteristics and possible anisotropic effects. In both directions the P-wave reflection seismic measurements show a detailed and complex structure. This structure was developed during several tectonic phases and comprises both steeply- and shallowly-dipping faults. In a profile perpendicular to the graben, a strong P-wave reflector is interpreted as shallowly west-dipping fault that is traceable from the surface down to 500 m depth. It is also detectable along the graben. In contrast, the S-waves show different reflection characteristics: There is no indication of the strong P-wave reflector in the S-wave reflection seismic measurements - neither across nor along the graben. Only diffuse S-wave reflections are observable in this region. Due to the higher resolution of S-waves in the near-surface area it is possible to map structures which cannot be detected in P-wave reflection seismic, e.g the thinning of the uppermost Jurassic layer towards the south. In the next step a petrophysical analysis will be conducted by using seismic FD modelling to a) determine the cause (lithological, structural, or a combination of both) of the different reflection characteristics of P- and S-waves, b) characterize the fault zone, as well as c) analyse the influence of different fault zone properties on the seismic wave field. This work is part of the gebo collaborative research programme which is funded by the 'Niedersächsisches Ministerium für Wissenschaft und Kultur' and Baker Hughes.

  13. Two-zone elastic-plastic single shock waves in solids.

    PubMed

    Zhakhovsky, Vasily V; Budzevich, Mikalai M; Inogamov, Nail A; Oleynik, Ivan I; White, Carter T

    2011-09-23

    By decoupling time and length scales in moving window molecular dynamics shock-wave simulations, a new regime of shock-wave propagation is uncovered characterized by a two-zone elastic-plastic shock-wave structure consisting of a leading elastic front followed by a plastic front, both moving with the same average speed and having a fixed net thickness that can extend to microns. The material in the elastic zone is in a metastable state that supports a pressure that can substantially exceed the critical pressure characteristic of the onset of the well-known split-elastic-plastic, two-wave propagation. The two-zone elastic-plastic wave is a general phenomenon observed in simulations of a broad class of crystalline materials and is within the reach of current experimental techniques.

  14. Assessment of renal injury with a clinical dual head lithotriptor delivering 240 shock waves per minute.

    PubMed

    Handa, Rajash K; McAteer, James A; Evan, Andrew P; Connors, Bret A; Pishchalnikov, Yuri A; Gao, Sujuan

    2009-02-01

    Lithotriptors with 2 treatment heads deliver shock waves along separate paths. Firing 1 head and then the other in alternating mode has been suggested as a strategy to treat stones twice as rapidly as with conventional shock wave lithotripsy. Because the shock wave rate is known to have a role in shock wave lithotripsy induced injury, and given that treatment using 2 separate shock wave sources exposes more renal tissue to shock wave energy than treatment with a conventional lithotriptor, we assessed renal trauma in pigs following treatment at rapid rate (240 shock waves per minute and 120 shock waves per minute per head) using a Duet lithotriptor (Direx Medical Systems, Petach Tikva, Israel) fired in alternating mode. Eight adult female pigs (Hardin Farms, Danville, Indiana) each were treated with sham shock wave lithotripsy or 2,400 shock waves delivered in alternating mode (1,200 shock waves per head, 120 shock waves per minute per head and 240 shock waves per minute overall at a power level of 10) to the lower renal pole. Renal functional parameters, including glomerular filtration rate and effective renal plasma flow, were determined before and 1 hour after shock wave lithotripsy. The kidneys were perfusion fixed in situ and the hemorrhagic lesion was quantified as a percent of functional renal volume. Shock wave treatment resulted in no significant change in renal function and the response was similar to the functional response seen in sham shock wave treated animals. In 6 pigs treated with alternating mode the renal lesion was small at a mean +/- SEM of 0.22% +/- 0.09% of functional renal volume. Kidney tissue and function were minimally affected by a clinical dose of shock waves delivered in alternating mode (120 shock waves per minute per head and 240 shock waves per minute overall) with a Duet lithotriptor. These observations decrease concern that dual head lithotripsy at a rapid rate is inherently dangerous.

  15. Slab anisotropy from subduction zone guided waves in Taiwan

    NASA Astrophysics Data System (ADS)

    Chen, K. H.; Tseng, Y. L.; Hu, J. C.

    2014-12-01

    Frozen-in anisotropic structure in the oceanic lithosphere and faulting/hydration in the upper layer of the slab are expected to play an important role in anisotropic signature of the subducted slab. Over the past several decades, despite the advances in characterizing anisotropy using shear wave splitting method and its developments, the character of slab anisotropy remains poorly understood. In this study we investigate the slab anisotropy using subduction zone guided waves characterized by long path length in the slab. In the southernmost Ryukyu subduction zone, seismic waves from events deeper than 100 km offshore northern Taiwan reveal wave guide behavior: (1) a low-frequency (< 1 Hz) first arrival recognized on vertical and radial components but not transverse component (2) large, sustained high-frequency (3-10 Hz) signal in P and S wave trains. The depth dependent high-frequency content (3-10Hz) confirms the association with a waveguide effect in the subducting slab rather than localized site amplification effects. Using the selected subduction zone guided wave events, we further analyzed the shear wave splitting for intermediate-depth earthquakes in different frequency bands, to provide the statistically meaningful shear wave splitting parameters. We determine shear wave splitting parameters from the 34 PSP guided events that are deeper than 100 km with ray path traveling along the subducted slab. From shear wave splitting analysis, the slab and crust effects reveal consistent polarization pattern of fast directions of EN-WS and delay time of 0.13 - 0.27 sec. This implies that slab anisotropy is stronger than the crust effect (<0.1 s) but weaker than the mantle wedge and sub-slab mantle effect (0.3-1.3 s) in Taiwan.

  16. Remote Sensing Characterization of Two-dimensional Wave Forcing in the Surf Zone

    NASA Astrophysics Data System (ADS)

    Carini, R. J.; Chickadel, C. C.; Jessup, A. T.

    2016-02-01

    In the surf zone, breaking waves drive longshore currents, transport sediment, shape bathymetry, and enhance air-sea gas and particle exchange. Furthermore, wave group forcing influences the generation and duration of rip currents. Wave breaking exhibits large gradients in space and time, making it challenging to measure in situ. Remote sensing technologies, specifically thermal infrared (IR) imagery, can provide detailed spatial and temporal measurements of wave breaking at the water surface. We construct two-dimensional maps of active wave breaking from IR imagery collected during the Surf Zone Optics Experiment in September 2010 at the US Army Corps of Engineers' Field Research Facility in Duck, NC. For each breaker identified in the camera's field of view, the crest-perpendicular length of the aerated breaking region (roller length) and wave direction are estimated and used to compute the wave energy dissipation rate. The resultant dissipation rate maps are analyzed over different time scales: peak wave period, infragravity wave period, and tidal wave period. For each time scale, spatial maps of wave breaking are used to characterize wave forcing in the surf zone for a variety of wave conditions. The following phenomena are examined: (1) wave dissipation rates over the bar (location of most intense breaking) have increased variance in infragravity wave frequencies, which are different from the peak frequency of the incoming wave field and different from the wave forcing variability at the shoreline, and (2) wave forcing has a wider spatial distribution during low tide than during high tide due to depth-limited breaking over the barred bathymetry. Future work will investigate the response of the variability in wave setup, longshore currents and rip currents, to the variability in wave forcing in the surf zone.

  17. Head-on collision between two dust acoustic solitary waves and study of rogue waves in multicomponent dusty plasma

    NASA Astrophysics Data System (ADS)

    Singh, Kuldeep; Kaur, Nimardeep; Saini, N. S.

    2017-06-01

    In this investigation, the study of head-on collision between two dust acoustic solitary waves (DASWs) and characteristics of rogue waves in a dusty plasma composed of dust fluid, kappa distributed ions, electrons, and positrons has been presented. Two Korteweg-de Vries equations are derived by employing the extended Poincaré-Lighthill-Kuo reductive perturbation method. The analytical phase shifts and trajectories after head-on collision of two DA solitary waves have been studied numerically. It is found that the presence of superthermal ions, electrons, as well as positrons; concentrations of electrons and positrons; and temperature of electrons and dust have an emphatic influence on the phase shifts after the head-on collision of two rarefactive DA solitary waves. The time evolution of two rarefactive DASWs has also been presented. Further, the generation of dust acoustic rogue waves (DARWs) has been studied in the framework of rational solution of nonlinear Schrödinger equation. The dependence of the rogue wave profile on the relevant physical parameters has been discussed in detail. It is emphasized that the real implementation of our present results may be of great importance in different regions of space and astrophysical environments, especially in the interstellar medium and Jupiter rings.

  18. Large sand waves in Navarinsky Canyon head, Bering Sea

    USGS Publications Warehouse

    Karl, Herman A.; Carlson, P.R.

    1982-01-01

    Sand waves are present in the heads of large submarine canyons in the northwestern Bering Sea. They vary in height between 2 to 15 m and have wavelengths of 600 m. They are not only expressed on the seafloor, but are also well defined in the subsurface and resemble enormous climbing bed forms. We conjecture that the sand waves originated during lower stands of sea level in the Pleistocene. Although we cannot explain the mechanics of formation of the sand waves, internal-wave generated currents are among four types of current that could account for these large structures. ?? 1982 A. M. Dowden, Inc.

  19. A numerical investigation of head waves and leaky modes in fluid- filled boreholes.

    USGS Publications Warehouse

    Paillet, Frederick L.; Cheng, C.H.

    1986-01-01

    Although synthetic borehole seismograms can be computed for a wide range of borehole conditions, the physical nature of shear and compressional head waves in fluid-filled boreholes is poorly understood. Presents a series of numerical experiments designed to explain the physical mechanisms controlling head-wave propagation in boreholes. These calculations demonstrate the existence of compressional normal modes equivalent to shear normal modes, or pseudo-Rayleigh waves, with sequential cutoff frequencies spaced between the cutoff frequencies for the shear normal modes.-from Authors

  20. Transient cnoidal waves explain the formation and geometry of fault damage zones

    NASA Astrophysics Data System (ADS)

    Veveakis, Manolis; Schrank, Christoph

    2017-04-01

    The spatial footprint of a brittle fault is usually dominated by a wide area of deformation bands and fractures surrounding a narrow, highly deformed fault core. This diffuse damage zone relates to the deformation history of a fault, including its seismicity, and has a significant impact on flow and mechanical properties of faulted rock. Here, we propose a new mechanical model for damage-zone formation. It builds on a novel mathematical theory postulating fundamental material instabilities in solids with internal mass transfer associated with volumetric deformation due to elastoviscoplastic p-waves termed cnoidal waves. We show that transient cnoidal waves triggered by fault slip events can explain the characteristic distribution and extent of deformation bands and fractures within natural fault damage zones. Our model suggests that an overpressure wave propagating away from the slipping fault and the material properties of the host rock control damage-zone geometry. Hence, cnoidal-wave theory may open a new chapter for predicting seismicity, material and geometrical properties as well as the location of brittle faults.

  1. Impacts of wave-induced circulation in the surf zone on wave setup

    NASA Astrophysics Data System (ADS)

    Guérin, Thomas; Bertin, Xavier; Coulombier, Thibault; de Bakker, Anouk

    2018-03-01

    Wave setup corresponds to the increase in mean water level along the coast associated with the breaking of short-waves and is of key importance for coastal dynamics, as it contributes to storm surges and the generation of undertows. Although overall well explained by the divergence of the momentum flux associated with short waves in the surf zone, several studies reported substantial underestimations along the coastline. This paper investigates the impacts of the wave-induced circulation that takes place in the surf zone on wave setup, based on the analysis of 3D modelling results. A 3D phase-averaged modelling system using a vortex force formalism is applied to hindcast an unpublished field experiment, carried out at a dissipative beach under moderate to very energetic wave conditions (Hm 0 = 6m at breaking and Tp = 22s). When using an adaptive wave breaking parameterisation based on the beach slope, model predictions for water levels, short waves and undertows improved by about 30%, with errors reducing to 0.10 m, 0.10 m and 0.09 m/s, respectively. The analysis of model results suggests a very limited impact of the vertical circulation on wave setup at this dissipative beach. When extending this analysis to idealized simulations for different beach slopes ranging from 0.01 to 0.05, it shows that the contribution of the vertical circulation (horizontal and vertical advection and vertical viscosity terms) becomes more and more relevant as the beach slope increases. In contrast, for a given beach slope, the wave height at the breaking point has a limited impact on the relative contribution of the vertical circulation on the wave setup. For a slope of 0.05, the contribution of the terms associated with the vertical circulation accounts for up to 17% (i.e. a 20% increase) of the total setup at the shoreline, which provides a new explanation for the underestimations reported in previously published studies.

  2. Pulse wave velocity in patients with severe head injury a pilot study.

    PubMed

    Shahsavari, S; McKelvey, T; Rydenhag, B; Ritzén, C Eriksson

    2010-01-01

    The study aimed to determine the potential of pulse wave velocity measurements to reflect changes in compliant cerebral arteries/arterioles in head injured patients. The approach utilizes the electrocardiogram and intracranial pressure signals to measure the wave transit time between heart and cranial cavity. Thirty five clinical records of nineteen head injured patients, with different levels of cerebrovascular pressure-reactivity response, were investigated through the study. Results were compared with magnitude of normalized transfer function at the fundamental cardiac frequency. In patients with intact cerebrovascular pressure-reactivity, magnitude of normalized transfer function at the fundamental cardiac component was found to be highly correlated with pulse wave transit time.

  3. Seismic-wave attenuation associated with crustal faults in the New Madrid seismic zone

    USGS Publications Warehouse

    Hamilton, R.M.; Mooney, W.D.

    1990-01-01

    The attenuation of upper crustal seismic waves that are refracted with a velocity of about 6 kilometers per second varies greatly among profiles in the area of the New Madrid seismic zone in the central Mississippi Valley. The waves that have the strongest attenuation pass through the seismic 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 seismic scattering and absorption could cause the attenuation; these effects are most likely associated with the highly deformed rocks along the arch. Consequently, strong seismic-wave attenuation may be a useful criterion for identifying seismogenic fault zones.

  4. Waves and mesoscale features in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Peng, Chih Y.

    1993-01-01

    Ocean-ice interaction processes in the Marginal Ice Zone (MIZ) by waves and mesoscale features, such as upwelling and eddies, are studied using ERS-1 Synthetic Aperture Radar (SAR) imagery and wave-ice interaction models. Satellite observations of mesoscale features can play a crucial role in ocean-ice interaction study.

  5. Fault-zone guided waves from explosions in the San Andreas fault at Parkfield and Cienega Valley, California

    USGS Publications Warehouse

    Li, Y.-G.; Ellsworth, W.L.; Thurber, C.H.; Malin, P.E.; Aki, K.

    1997-01-01

    Fault-zone guided waves were successfully excited by near-surface explosions in the San Andreas fault zone both at Parkfield and Cienega Valley, central California. The guided waves were observed on linear, three-component seismic arrays deployed across the fault trace. These waves were not excited by explosions located outside the fault zone. The amplitude spectra of guided waves show a maximum peak at 2 Hz at Parkfield and 3 Hz at Cienega Valley. The guided wave amplitude decays sharply with observation distance from the fault trace. The explosion-excited fault-zone guided waves are similar to those generated by earthquakes at Parkfield but have lower frequencies and travel more slowly. These observations suggest that the fault-zone wave guide has lower seismic velocities as it approaches the surface at Parkfield. We have modeled the waveforms as S waves trapped in a low-velocity wave guide sandwiched between high-velocity wall rocks, resulting in Love-type fault-zone guided waves. While the results are nonunique, the Parkfield data are adequately fit by a shallow wave guide 170 m wide with an S velocity 0.85 km/sec and an apparent Q ??? 30 to 40. At Cienega Valley, the fault-zone wave guide appears to be about 120 m wide with an S velocity 0.7 km/sec and a Q ??? 30.

  6. Large-scale bedforms induced by supercritical flows and wave-wave interference in the intertidal zone (Cap Ferret, France)

    NASA Astrophysics Data System (ADS)

    Vaucher, Romain; Pittet, Bernard; Humbert, Thomas; Ferry, Serge

    2017-11-01

    The Cap Ferret sand spit is situated along the wave-dominated, tidally modulated Atlantic coast of western France, characterized by a semidiurnal macrotidal range. It displays peculiar dome-like bedforms that can be observed at low tide across the intertidal zone. These bedforms exhibit a wavelength of ca. 1.2 m and an elevation of ca. 30 cm. They occur only when the incident wave heights reach 1.5-2 m. The internal stratifications are characterized by swaley-like, sub-planar, oblique-tangential, oblique-tabular, as well as hummocky-like stratifications. The tabular and tangential stratifications comprise prograding oblique sets (defined as foresets and backsets) that almost always show variations in their steepness. Downcutting into the bottomsets of the oblique-tangential stratifications is common. The sets of laminae observed in the bedforms share common characteristics with those formed by supercritical flows in flume experiments of earlier studies. These peculiar bedforms are observed at the surf-swash transition zone where the backwash flow reaches supercritical conditions. This type of flow can explain their internal architecture but not their general dome-like (three-dimensional) morphology. Wave-wave interference induced by the geomorphology (i.e. tidal channel) of the coastal environment is proposed as explanation for the localized formation of such bedforms. This study highlights that the combination of supercritical flows occurring in the surf-swash transition zone and wave-wave interferences can generate dome-like bedforms in intertidal zones.

  7. Large-scale bedforms induced by supercritical flows and wave-wave interference in the intertidal zone (Cap Ferret, France)

    NASA Astrophysics Data System (ADS)

    Vaucher, Romain; Pittet, Bernard; Humbert, Thomas; Ferry, Serge

    2018-06-01

    The Cap Ferret sand spit is situated along the wave-dominated, tidally modulated Atlantic coast of western France, characterized by a semidiurnal macrotidal range. It displays peculiar dome-like bedforms that can be observed at low tide across the intertidal zone. These bedforms exhibit a wavelength of ca. 1.2 m and an elevation of ca. 30 cm. They occur only when the incident wave heights reach 1.5-2 m. The internal stratifications are characterized by swaley-like, sub-planar, oblique-tangential, oblique-tabular, as well as hummocky-like stratifications. The tabular and tangential stratifications comprise prograding oblique sets (defined as foresets and backsets) that almost always show variations in their steepness. Downcutting into the bottomsets of the oblique-tangential stratifications is common. The sets of laminae observed in the bedforms share common characteristics with those formed by supercritical flows in flume experiments of earlier studies. These peculiar bedforms are observed at the surf-swash transition zone where the backwash flow reaches supercritical conditions. This type of flow can explain their internal architecture but not their general dome-like (three-dimensional) morphology. Wave-wave interference induced by the geomorphology (i.e. tidal channel) of the coastal environment is proposed as explanation for the localized formation of such bedforms. This study highlights that the combination of supercritical flows occurring in the surf-swash transition zone and wave-wave interferences can generate dome-like bedforms in intertidal zones.

  8. Quantitative analysis of seismic fault zone waves in the rupture zone of the 1992 Landers, California, earthquake: Evidence for a shallow trapping structure

    USGS Publications Warehouse

    Peng, Z.; Ben-Zion, Y.; Michael, A.J.; Zhu, L.

    2003-01-01

    We analyse quantitatively a waveform data set of 238 earthquakes recorded by a dense seismic array across and along the rupture zone of the 1992 Landers earthquake. A grid-search method with station delay corrections is used to locate events that do not have catalogue locations. The quality of fault zone trapped waves generated by each event is determined from the ratios of seismic energy in time windows corresponding to trapped waves and direct S waves at stations close to and off the fault zone. Approximately 70 per cent of the events with S-P times of less than 2 s, including many clearly off the fault, produce considerable trapped wave energy. This distribution is in marked contrast with previous claims that trapped waves are generated only by sources close to or inside the Landers rupture zone. The time difference between the S arrival and trapped waves group does not grow systematically with increasing hypocentral distance and depth. The dispersion measured from the trapped waves is weak. These results imply that the seismic trapping structure at the Landers rupture zone is shallow and does not extend continuously along-strike by more than a few kilometres. Synthetic waveform modelling indicates that the fault zone waveguide has depth of approximately 2-4 km, a width of approximately 200 m, an S-wave velocity reduction relative to the host rock of approximately 30-40 per cent and an S-wave attenuation coefficient of approximately 20-30. The fault zone waveguide north of the array appears to be shallower and weaker than that south of the array. The waveform modelling also indicates that the seismic trapping structure below the array is centred approximately 100 m east of the surface break.

  9. Wave Climate and Wave Mixing in the Marginal Ice Zones of Arctic Seas, Observations and Modelling

    DTIC Science & Technology

    2014-09-30

    At the same time, the PIs participate in Australian efforts of developing wave-ocean- ice coupled models for Antarctica . Specific new physics modules...Wave Mixing in the Marginal Ice Zones of Arctic Seas, Observations and Modelling Alexander V. Babanin Swinburne University of Technology, PO Box...operational forecast. Altimeter climatology and the wave models will be used to study the current and future wind/wave and ice trends. APPROACH

  10. Head-on collision of the second mode internal solitary waves

    NASA Astrophysics Data System (ADS)

    Terletska, Kateryna; Maderich, Vladimir; Jung, Kyung Tae

    2017-04-01

    Second mode internal waves are widespread in offshore areas, and they frequently follow the first mode internal waves on the oceanic shelf. Large amplitude internal solitary waves (ISW) of second mode containing trapped cores associated with closed streamlines can also transport plankton and nutrients. An interaction of ISWs with trapped cores takes place in a specific manner. It motivated us to carry out a computational study of head-on collision of ISWs of second mode propagating in a laboratory-scale numerical tank using the nonhydrostatic 3D numerical model based on the Navier-Stokes equations for a continuously stratified fluid. Three main classes of ISW of second mode propagating in the pycnocline layer of thickness h between homogeneous deep layers can be identified: (i) the weakly nonlinear waves; (ii) the stable strongly nonlinear waves with trapped cores; and (iii) the shear unstable strongly nonlinear waves (Maderich et al., 2015). Four interaction regimes for symmetric collision were separated from simulation results using this classification: (A) an almost elastic interaction of the weakly nonlinear waves; (B) a non-elastic interaction of waves with trapped cores when ISW amplitudes were close to critical non-dimensional amplitude a/h; (C) an almost elastic interaction of stable strongly nonlinear waves with trapped cores; (D) non-elastic interaction of the unstable strongly nonlinear waves. The unexpected result of simulation was that relative loss of energy due to the collision was maximal for regime B. New regime appeared when ISW of different amplitudes belonged to class (ii) collide. In result of interaction the exchange of mass between ISW occurred: the trapped core of smaller wave was entrained by core of larger ISW without mixing forming a new ISW of larger amplitude whereas in smaller ISW core of smaller wave totally substituted by fluid from larger wave. Overall, the wave characteristics induced by head-on collision agree well with the

  11. Wave effects on ocean-ice interaction in the marginal ice zone

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Hakkinen, Sirpa; Peng, Chih Y.

    1993-01-01

    The effects of wave train on ice-ocean interaction in the marginal ice zone are studied through numerical modeling. A coupled two-dimensional ice-ocean model has been developed to include wave effects and wind stress for the predictions of ice edge dynamics. The sea ice model is coupled to the reduced-gravity ocean model through interfacial stresses. The main dynamic balance in the ice momentum is between water-ice stress, wind stress, and wave radiation stresses. By considering the exchange of momentum between waves and ice pack through radiation stress for decaying waves, a parametric study of the effects of wave stress and wind stress on ice edge dynamics has been performed. The numerical results show significant effects from wave action. The ice edge is sharper, and ice edge meanders form in the marginal ice zone owing to forcing by wave action and refraction of swell system after a couple of days. Upwelling at the ice edge and eddy formation can be enhanced by the nonlinear effects of wave action; wave action sharpens the ice edge and can produce ice meandering, which enhances local Ekman pumping and pycnocline anomalies. The resulting ice concentration, pycnocline changes, and flow velocity field are shown to be consistent with previous observations.

  12. Experimental investigation of change of energy of infragavity waves in dependence on spectral characteristics of an irregular wind waves in coastal zone

    NASA Astrophysics Data System (ADS)

    Saprykina, Yana; Divinskii, Boris

    2013-04-01

    An infragravity waves are long waves with periods of 20 - 300 s. Most essential influence of infragarvity waves on dynamic processes is in a coastal zone, where its energy can exceed the energy of wind waves. From practical point of view, the infragravity waves are important, firstly, due to their influence on sand transport processes in a coastal zone. For example, interacting with group structure of wind waves the infragravity waves can define position of underwater bars on sandy coast. Secondly, they are responsible on formation of long waves in harbors. Main source of infragravity waves is wave group structure defined by sub-nonlinear interactions of wind waves (Longuet-Higgins, Stewart, 1962). These infragravity waves are bound with groups of wind waves and propagate with wave group velocity. Another type of infragravity waves are formed in a surf zone as a result of migration a wave breaking point (Symonds, et al., 1982). What from described above mechanisms of formation of infragravity waves prevails, till now it is unknown. It is also unknown how energy of infragravity waves depends on energy of input wind waves and how it changes during nonlinear wave transformation in coastal zone. In our work on the basis of the analysis of data of field experiment and numerical simulation a contribution of infragravity waves in total wave energy in depending on integral characteristics of an irregular wave field in the conditions of a real bathymetry was investigated. For analysis the data of field experiment "Shkorpilovtsy-2007" (Black sea) and data of numerical modeling of Boussinesq type equation with extended dispersion characteristics (Madsen et al., 1997) were used. It was revealed that infragravity waves in a coastal zone are defined mainly by local group structure of waves, which permanently changes due to nonlinearity, shoaling and breaking processes. Free infragravity waves appearing after wave breaking exist together with bound infragravity waves. There are

  13. Subduction zone guided waves in Northern Chile

    NASA Astrophysics Data System (ADS)

    Garth, Thomas; Rietbrock, Andreas

    2016-04-01

    Guided wave dispersion is observed in subduction zones as high frequency energy is retained and delayed by low velocity structure in the subducting slab, while lower frequency energy is able to travel at the faster velocities associated with the surrounding mantle material. As subduction zone guided waves spend longer interacting with the low velocity structure of the slab than any other seismic phase, they have a unique capability to resolve these low velocity structures. In Northern Chile, guided wave arrivals are clearly observed on two stations in the Chilean fore-arc on permanent stations of the IPOC network. High frequency (> 5 Hz) P-wave arrivals are delayed by approximately 2 seconds compared to the low frequency (< 2 Hz) P-wave arrivals. Full waveform finite difference modelling is used to test the low velocity slab structure that cause this P-wave dispersion. The synthetic waveforms produced by these models are compared to the recorded waveforms. Spectrograms are used to compare the relative arrival times of different frequencies, while the velocity spectra is used to constrain the relative amplitude of the arrivals. Constraining the waveform in these two ways means that the full waveform is also matched, and the low pass filtered observed and synthetic waveforms can be compared. A combined misfit between synthetic and observed waveforms is then calculated following Garth & Rietbrock (2014). Based on this misfit criterion we constrain the velocity model by using a grid search approach. Modelling the guided wave arrivals suggest that the observed dispersion cannot be solely accounted for by a single low velocity layer as suggested by previous guided wave studies. Including dipping low velocity normal fault structures in the synthetic model not only accounts for the observed strong P-wave coda, but also produces a clear first motion dispersion. We therefore propose that the lithospheric mantle of the subducting Nazca plate is highly hydrated at intermediate

  14. Seismic fault zone trapped noise

    NASA Astrophysics Data System (ADS)

    Hillers, G.; Campillo, M.; Ben-Zion, Y.; Roux, P.

    2014-07-01

    Systematic velocity contrasts across and within fault zones can lead to head and trapped waves that provide direct information on structural units that are important for many aspects of earthquake and fault mechanics. Here we construct trapped waves from the scattered seismic wavefield recorded by a fault zone array. The frequency-dependent interaction between the ambient wavefield and the fault zone environment is studied using properties of the noise correlation field. A critical frequency fc ≈ 0.5 Hz defines a threshold above which the in-fault scattered wavefield has increased isotropy and coherency compared to the ambient noise. The increased randomization of in-fault propagation directions produces a wavefield that is trapped in a waveguide/cavity-like structure associated with the low-velocity damage zone. Dense spatial sampling allows the resolution of a near-field focal spot, which emerges from the superposition of a collapsing, time reversed wavefront. The shape of the focal spot depends on local medium properties, and a focal spot-based fault normal distribution of wave speeds indicates a ˜50% velocity reduction consistent with estimates from a far-field travel time inversion. The arrival time pattern of a synthetic correlation field can be tuned to match properties of an observed pattern, providing a noise-based imaging tool that can complement analyses of trapped ballistic waves. The results can have wide applicability for investigating the internal properties of fault damage zones, because mechanisms controlling the emergence of trapped noise have less limitations compared to trapped ballistic waves.

  15. 77 FR 50062 - Safety Zone; Embry-Riddle Wings and Waves, Atlantic Ocean; Daytona Beach, FL

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-08-20

    ... 1625-AA00 Safety Zone; Embry-Riddle Wings and Waves, Atlantic Ocean; Daytona Beach, FL AGENCY: Coast...-Riddle Wings and Waves air show. The event is scheduled to take place from Thursday, October 11, 2012...: Sec. 165.T07-0653 Safety Zone; Embry Riddle Wings and Waves, Atlantic Ocean, Daytona Beach, FL. (a...

  16. Remote sensing of the correlation between breakpoint oscillations and infragravity waves in the surf and swash zone

    NASA Astrophysics Data System (ADS)

    Moura, T.; Baldock, T. E.

    2017-04-01

    A novel remote sensing methodology to determine the dominant infragravity mechanism in the inner surf and swash zone in the field is presented. Video observations of the breakpoint motion are correlated with the shoreline motion and inner surf zone water levels to determine the relationship between the time-varying breakpoint oscillations and the shoreline motion. The results of 13 field data sets collected from three different beaches indicate that, inside the surf zone, the dominance of bound wave or breakpoint forcing is strongly dependent on the surf zone width and the type of short wave breaking. Infragravity generation by bound wave release was stronger for conditions with relatively narrow surf zones and plunging waves; breakpoint forcing was dominant for wider surf zones and spilling breaker conditions.

  17. Computation of Acoustic Waves Through Sliding-Zone Interfaces Using an Euler/Navier-Stokes Code

    NASA Technical Reports Server (NTRS)

    Rumsey, Christopher L.

    1996-01-01

    The effect of a patched sliding-zone interface on the transmission of acoustic waves is examined for two- and three-dimensional model problems. A simple but general interpolation scheme at the patched boundary passes acoustic waves without distortion, provided that a sufficiently small time step is taken. A guideline is provided for the maximum permissible time step or zone speed that gives an acceptable error introduced by the sliding-zone interface.

  18. Wave attenuation in the marginal ice zone during LIMEX

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Vachon, Paris W.; Peng, Chih Y.; Bhogal, A. S.

    1992-01-01

    The effect of ice cover on ocean-wave attenuation is investigated for waves under flexure in the marginal ice zone (MIZ) with SAR image spectra and the results of models. Directional wavenumber spectra are taken from the SAR image data, and the wave-attenuation rate is evaluated with SAR image spectra and by means of the model by Liu and Mollo-Christensen (1988). Eddy viscosity is described by means of dimensional analysis as a function of ice roughness and wave-induced velocity, and comparisons are made with the remotely sensed data. The model corrects the open-water model by introducing the effects of a continuous ice sheet, and turbulent eddy viscosity is shown to depend on ice thickness, floe sizes, significant wave height, and wave period. SAR and wave-buoy data support the trends described in the model results, and a characteristic rollover is noted in the model and experimental wave-attenuation rates at high wavenumbers.

  19. Fault zone reverberations from cross-correlations of earthquake waveforms and seismic noise

    NASA Astrophysics Data System (ADS)

    Hillers, Gregor; Campillo, Michel

    2016-03-01

    Seismic wavefields interact with low-velocity fault damage zones. Waveforms of ballistic fault zone head waves, trapped waves, reflected waves and signatures of trapped noise can provide important information on structural and mechanical fault zone properties. Here we extend the class of observable fault zone waves and reconstruct in-fault reverberations or multiples in a strike-slip faulting environment. Manifestations of the reverberations are significant, consistent wave fronts in the coda of cross-correlation functions that are obtained from scattered earthquake waveforms and seismic noise recorded by a linear fault zone array. The physical reconstruction of Green's functions is evident from the high similarity between the signals obtained from the two different scattered wavefields. Modal partitioning of the reverberation wavefield can be tuned using different data normalization techniques. The results imply that fault zones create their own ambiance, and that the here reconstructed reverberations are a key seismic signature of wear zones. Using synthetic waveform modelling we show that reverberations can be used for the imaging of structural units by estimating the location, extend and magnitude of lateral velocity contrasts. The robust reconstruction of the reverberations from noise records suggests the possibility to resolve the response of the damage zone material to various external and internal loading mechanisms.

  20. Ocean Wave Energy Regimes of the Circumpolar Coastal Zones

    NASA Astrophysics Data System (ADS)

    Atkinson, D. E.

    2004-12-01

    Ocean wave activity is a major enviromental forcing agent of the ice-rich sediments that comprise large sections of the arctic coastal margins. While it is instructive to possess information about the wind regimes in these regions, direct application to geomorphological and engineering needs requires knowledge of the resultant wave-energy regimes. Wave energy information has been calculated at the regional scale using adjusted reanalysis model windfield data. Calculations at this scale are not designed to account for local-scale coastline/bathymetric irregularities and variability. Results will be presented for the circumpolar zones specified by the Arctic Coastal Dynamics Project.

  1. Modelling guided waves in the Alaskan-Aleutian subduction zone

    NASA Astrophysics Data System (ADS)

    Coulson, Sophie; Garth, Thomas; Reitbrock, Andreas

    2016-04-01

    Subduction zone guided wave arrivals from intermediate depth earthquakes (70-300 km depth) have a huge potential to tell us about the velocity structure of the subducting oceanic crust as it dehydrates at these depths. We see guided waves as the oceanic crust has a slower seismic velocity than the surrounding material, and so high frequency energy is retained and delayed in the crustal material. Lower frequency energy is not retained in this crustal waveguide and so travels at faster velocities of the surrounding material. This gives a unique observation at the surface with low frequency energy arriving before the higher frequencies. We constrain this guided wave dispersion by comparing the waveforms recorded in real subduction zones with simulated waveforms, produced using finite difference full waveform modelling techniques. This method has been used to show that hydrated minerals in the oceanic crust persist to much greater depths than accepted thermal petrological subduction zone models would suggest in Northern Japan (Garth & Rietbrock, 2014a), and South America (Garth & Rietbrock, in prep). These observations also suggest that the subducting oceanic mantle may be highly hydrated at intermediate depth by dipping normal faults (Garth & Rietbrock 2014b). We use this guided wave analysis technique to constrain the velocity structure of the down going ~45 Ma Pacific plate beneath Alaska. Dispersion analysis is primarily carried out on guided wave arrivals recorded on the Alaskan regional seismic network. Earthquake locations from global earthquake catalogues (ISC and PDE) and regional earthquake locations from the AEIC (Alaskan Earthquake Information Centre) catalogue are used to constrain the slab geometry and to identify potentially dispersive events. Dispersed arrivals are seen at stations close to the trench, with high frequency (>2 Hz) arrivals delayed by 2 - 4 seconds. This dispersion is analysed to constrain the velocity and width of the proposed waveguide

  2. Wave attenuation in the marginal ice zone during LIMEX

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Peng, Chih Y.; Vachon, Paris W.

    1991-01-01

    During LIMEX'87 and '89, the CCRS CV-580 aircraft collected SAR (synthetic aperture radar) data over the marginal ice zone off the coast of Newfoundland. Based upon the wavenumber spectra from SAR data, the wave attenuation rate is estimated and compared with a model. The model-data comparisons are reasonably good for the ice conditions during LIMEX (Labrador Ice Margin Experiment). Both model and SAR-derived wave attenuation rates show a roll-over at high wavenumbers.

  3. Effects of neurofeedback training on the brain wave of adults with forward head posture

    PubMed Central

    Oh, Hyun-Ju; Song, Gui-Bin

    2016-01-01

    [Purpose] The purpose of the present study was to examine the effects of neurofeedback training on electroencephalogram changes in the cervical spine in adults with forward head posture through x-ray. [Subjects and Methods] The subjects of the study were 40 college students with forward head posture, randomly divided into a neurofeedback training group (NFTG, n=20) and a control group (CG, n=20). The neurofeedback training group performed six sessions of pottery and archery games, each for two minutes, three times per week for four weeks, while using the neurofeedback system. [Results] There were significant effects within and between groups in terms of the Delta wave, the Theta wave, the Alpha wave, the Beta wave, or the sensory motor rhythm. Especially, the Delta wave, Beta wave, and the sensory motor rhythm were showed significant effects between the groups. [Conclusion] It is thought that neurofeedback training, a training approach to self-regulate brain waves, enhances concentration and relaxation without stress, as well as an increase in attention, memory, and verbal cognitive performance. Therefore an effective intervention method to improve neck pain and daily activities. PMID:27821966

  4. Effects of neurofeedback training on the brain wave of adults with forward head posture.

    PubMed

    Oh, Hyun-Ju; Song, Gui-Bin

    2016-10-01

    [Purpose] The purpose of the present study was to examine the effects of neurofeedback training on electroencephalogram changes in the cervical spine in adults with forward head posture through x-ray. [Subjects and Methods] The subjects of the study were 40 college students with forward head posture, randomly divided into a neurofeedback training group (NFTG, n=20) and a control group (CG, n=20). The neurofeedback training group performed six sessions of pottery and archery games, each for two minutes, three times per week for four weeks, while using the neurofeedback system. [Results] There were significant effects within and between groups in terms of the Delta wave, the Theta wave, the Alpha wave, the Beta wave, or the sensory motor rhythm. Especially, the Delta wave, Beta wave, and the sensory motor rhythm were showed significant effects between the groups. [Conclusion] It is thought that neurofeedback training, a training approach to self-regulate brain waves, enhances concentration and relaxation without stress, as well as an increase in attention, memory, and verbal cognitive performance. Therefore an effective intervention method to improve neck pain and daily activities.

  5. Head-on collision of normal shock waves with rigid porous materials

    NASA Astrophysics Data System (ADS)

    Levy, A.; Ben-Dor, G.; Skews, B. W.; Sorek, S.

    1993-08-01

    The head-on collision of a planar shock wave with a rigid porous material has been investigated experimentally in a 75 mm × 75 mm shock tube. The experimental study indicated that unlike the reflection from a flexible porous material (e.g., polyurethane foam) where the transmitted compression waves do not converge to a sharp shock wave, in the case of a rigid porous material (e.g., alumina) the transmitted compression waves do converge to a sharp shock wave, which decays as it propagates along the porous material. In addition to this major difference, many other differences were observed. They are outlined in the following sections. Based on these observations a suggestion modifying the phenomenology of the reflection/interaction process in the case a porous material with large permeability is proposed.

  6. Modeling Wave-Ice Interactions in the Marginal Ice Zone

    NASA Astrophysics Data System (ADS)

    Orzech, Mark; Shi, Fengyan; Bateman, Sam; Veeramony, Jay; Calantoni, Joe

    2015-04-01

    The small-scale (O(m)) interactions between waves and ice floes in the marginal ice zone (MIZ) are investigated with a coupled model system. Waves are simulated with the non-hydrostatic finite-volume model NHWAVE (Ma et al., 2012) and ice floes are represented as bonded collections of smaller particles with the discrete element system LIGGGHTS (Kloss et al., 2012). The physics of fluid and ice are recreated as authentically as possible, to allow the coupled system to supplement and/or substitute for more costly and demanding field experiments. The presentation will first describe the development and validation of the coupled system, then discuss the results of a series of virtual experiments in which ice floe and wave characteristics are varied to examine their effects on energy dissipation, MIZ floe size distribution, and ice pack retreat rates. Although Wadhams et al. (1986) suggest that only a small portion (roughly 10%) of wave energy entering the MIZ is reflected, dissipation mechanisms for the remaining energy have yet to be delineated or measured. The virtual experiments are designed to focus on specific properties and processes - such as floe size and shape, collision and fracturing events, and variations in wave climate - and measure their relative roles the transfer of energy and momentum from waves to ice. Questions to be examined include: How is energy dissipated by ice floe collisions, fracturing, and drag, and how significant is the wave attenuation associated with each process? Do specific wave/floe length scale ratios cause greater wave attenuation? How does ice material strength affect the rate of wave energy loss? The coupled system will ultimately be used to test and improve upon wave-ice parameterizations for large-scale climate models. References: >Kloss, C., C. Goniva, A. Hager, S. Amberger, and S. Pirker (2012). Models, algorithms and validation for opensource DEM and CFD-DEM. Progress in Computational Fluid Dynamics 12(2/3), 140-152. >Ma, G

  7. Numerical study of the impact response of woodpecker's head

    NASA Astrophysics Data System (ADS)

    Zhu, Zhao Dan; Ma, Guo Jun; Wu, Cheng Wei; Chen, Zhen

    2012-12-01

    Woodpecker can beat trees 20-25 times per second and lasts for several seconds, with a 1200 g deceleration, but it appears that they never get brain concussion. How does the stress wave propagate from the beak tip to brain and how does a woodpecker protect itself from brain damage? In this paper, we establish a finite element model of typical woodpecker head based on its X-ray tomography images and conduct the numerical analysis of the impact response of the woodpecker's head by using a viscoelasticity material model. Especially, the woodpecker head response to an impact speed of 7 m/s is investigated to explore the stress concentration zone and how the stress wave propagates in its head. The numerical results show that the stress wave in the head propagates from the upper beak to back skull and is reduced by the specific structure of hyoid and viscoelasticity of biomaterials. The maximum stresses in skull and brain are both below the safe level. The stress in skull almost disappears before the next impact. The stress in brain lasts for a little longer but shows smaller value with little variation. The stress is impossible to accumulate in the limited pecking time, so the brain damage can be avoided.

  8. Monochromatic body waves excited by great subduction zone earthquakes

    NASA Astrophysics Data System (ADS)

    Ihmlé, Pierre F.; Madariaga, Raúl

    Large quasi-monochromatic body waves were excited by the 1995 Chile Mw=8.1 and by the 1994 Kurile Mw=8.3 events. They are observed on vertical/radial component seismograms following the direct P and Pdiff arrivals, at all azimuths. We devise a slant stack algorithm to characterize the source of the oscillations. This technique aims at locating near-source isotropic scatterers using broadband data from global networks. For both events, we find that the oscillations emanate from the trench. We show that these monochromatic waves are due to localized oscillations of the water column. Their period corresponds to the gravest ID mode of a water layer for vertically traveling compressional waves. We suggest that these monochromatic body waves may yield additional constraints on the source process of great subduction zone earthquakes.

  9. The effect of gradational velocities and anisotropy on fault-zone trapped waves

    NASA Astrophysics Data System (ADS)

    Gulley, A. K.; Eccles, J. D.; Kaipio, J. P.; Malin, P. E.

    2017-08-01

    Synthetic fault-zone trapped wave (FZTW) dispersion curves and amplitude responses for FL (Love) and FR (Rayleigh) type phases are analysed in transversely isotropic 1-D elastic models. We explore the effects of velocity gradients, anisotropy, source location and mechanism. These experiments suggest: (i) A smooth exponentially decaying velocity model produces a significantly different dispersion curve to that of a three-layer model, with the main difference being that Airy phases are not produced. (ii) The FZTW dispersion and amplitude information of a waveguide with transverse-isotropy depends mostly on the Shear wave velocities in the direction parallel with the fault, particularly if the fault zone to country-rock velocity contrast is small. In this low velocity contrast situation, fully isotropic approximations to a transversely isotropic velocity model can be made. (iii) Fault-aligned fractures and/or bedding in the fault zone that cause transverse-isotropy enhance the amplitude and wave-train length of the FR type FZTW. (iv) Moving the source and/or receiver away from the fault zone removes the higher frequencies first, similar to attenuation. (v) In most physically realistic cases, the radial component of the FR type FZTW is significantly smaller in amplitude than the transverse.

  10. Untangling the Effect of Head Acceleration on Brain Responses to Blast Waves

    PubMed Central

    Mao, Haojie; Unnikrishnan, Ginu; Rakesh, Vineet; Reifman, Jaques

    2015-01-01

    Multiple injury-causing mechanisms, such as wave propagation, skull flexure, cavitation, and head acceleration, have been proposed to explain blast-induced traumatic brain injury (bTBI). An accurate, quantitative description of the individual contribution of each of these mechanisms may be necessary to develop preventive strategies against bTBI. However, to date, despite numerous experimental and computational studies of bTBI, this question remains elusive. In this study, using a two-dimensional (2D) rat head model, we quantified the contribution of head acceleration to the biomechanical response of brain tissues when exposed to blast waves in a shock tube. We compared brain pressure at the coup, middle, and contre-coup regions between a 2D rat head model capable of simulating all mechanisms (i.e., the all-effects model) and an acceleration-only model. From our simulations, we determined that head acceleration contributed 36–45% of the maximum brain pressure at the coup region, had a negligible effect on the pressure at the middle region, and was responsible for the low pressure at the contre-coup region. Our findings also demonstrate that the current practice of measuring rat brain pressures close to the center of the brain would record only two-thirds of the maximum pressure observed at the coup region. Therefore, to accurately capture the effects of acceleration in experiments, we recommend placing a pressure sensor near the coup region, especially when investigating the acceleration mechanism using different experimental setups. PMID:26458125

  11. The Consequences of Alfven Waves and Parallel Potential Drops in the Auroral Zone

    NASA Technical Reports Server (NTRS)

    Schriver, David

    2003-01-01

    The goal of this research is to examine the causes of field-aligned plasma acceleration in the auroral zone using satellite data and numerical simulations. A primary question to be addressed is what causes the field-aligned acceleration of electrons (leading to precipitation) and ions (leading to upwelling ions) in the auroral zone. Data from the Fast Auroral SnapshoT (FAST) and Polar satellites is used when the two satellites are in approximate magnetic conjunction and are in the auroral region. FAST is at relatively low altitudes and samples plasma in the midst of the auroral acceleration region while Polar is at much higher altitudes and can measure plasmas and waves propagating towards the Earth. Polar can determine the sources of energy streaming earthward from the magnetotail, either in the form of field-aligned currents, electromagnetic waves or kinetic particle energy, that ultimately leads to the acceleration of plasma in the auroral zone. After identifying and examining several events, numerical simulations are run that bridges the spatial region between the two satellites. The code is a one-dimensional, long system length particle in cell simulation that has been developed to model the auroral region. A main goal of this research project is to include Alfven waves in the simulation to examine how these waves can accelerate plasma in the auroral zone.

  12. P and S wave attenuation tomography of the Japan subduction zone

    NASA Astrophysics Data System (ADS)

    Wang, Zewei; Zhao, Dapeng; Liu, Xin; Chen, Chuanxu; Li, Xibing

    2017-04-01

    We determine the first high-resolution P and S wave attenuation (Q) tomography beneath the entire Japan Islands using a large number of high-quality t∗ data collected from P and S wave velocity spectra of 4222 local shallow and intermediate-depth earthquakes. The suboceanic earthquakes used in this study are relocated precisely using sP depth phases. Significant landward dipping high-Q zones are revealed clearly, which reflect the subducting Pacific slab beneath Hokkaido and Tohoku, and the subducting Philippine Sea (PHS) slab beneath SW Japan. Prominent low-Q zones are visible in the crust and mantle wedge beneath the active arc volcanoes in Hokkaido, Tohoku, and Kyushu, which reflect source zones of arc magmatism caused by fluids from the slab dehydration and corner flow in the mantle wedge. Our results also show that nonvolcanic low-frequency earthquakes (LFEs) in SW Japan mainly occur in the transition zone between a narrow low-Q belt and its adjacent high-Q zones right above the flat segment of the PHS slab. This feature suggests that the nonvolcanic LFEs are caused by not only fluid-affected slab interface but also specific conditions such as high pore pressure which is influenced by the overriding plate.

  13. Wave-Ice interaction in the Marginal Ice Zone: Toward a Wave-Ocean-Ice Coupled Modeling System

    DTIC Science & Technology

    2015-09-30

    MIZ using WW3 (3 frequency bins, ice retreat in August and ice advance in October); Blue (solid): Based on observations near Antarctica by Meylan...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Wave- Ice interaction in the Marginal Ice Zone: Toward a...Wave-Ocean- Ice Coupled Modeling System W. E. Rogers Naval Research Laboratory, Code 7322 Stennis Space Center, MS 39529 phone: (228) 688-4727

  14. Temporal variability in wind-wave climate and its validation with ESSO-NIOT wave atlas for the head Bay of Bengal

    NASA Astrophysics Data System (ADS)

    Patra, Anindita; Bhaskaran, Prasad K.

    2017-08-01

    The head Bay region bordering the northern Bay of Bengal is a densely populated area with a complex geomorphologic setting, and highly vulnerable to extreme water levels along with other factors like sea level rise and impact of tropical cyclones. The influence of climate change on wind-wave regime from this region of Bay of Bengal is not known well and that requires special attention, and there is a need to perform its long-term assessment for societal benefits. This study provides a comprehensive analysis on the temporal variability in domain averaged wind speed, significant wave height (SWH) utilizing satellite altimeter data (1992-2012) and mean wave period using ECMWF reanalysis products ERA-Interim (1992-2012) and ERA-20C (1992-2010) over this region. The SWH derived from WAVEWATCH III (WW3) model along with the ERA-Interim reanalysis supplements the observed variability in satellite altimeter observations. Further, the study performs an extensive error estimation of SWH and mean wave period with ESSO-NIOT wave atlas that shows a high degree of under-estimation in the wave atlas mean wave period. Annual mean and wind speed maxima from altimeter show an increasing trend, and to a lesser extent in the SWH. Interestingly, the estimated trend is higher for maxima compared to the mean conditions. Analysis of decadal variability exhibits an increased frequency of higher waves in the present decade compared to the past. Linear trend analysis show significant upswing in spatially averaged ERA-20C mean wave period, whereas the noticed variations are marginal in the ERA-Interim data. A separate trend analysis for the wind-seas, swell wave heights and period from ERA-20C decipher the fact that distant swells governs the local wind-wave climatology over the head Bay region, and over time the swell activity have increased in this region.

  15. TURBULENCE, TRANSPORT, AND WAVES IN OHMIC DEAD ZONES

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

    Gole, Daniel; Simon, Jacob B.; Armitage, Philip J.

    We use local numerical simulations to study a vertically stratified accretion disk with a resistive mid-plane that damps magnetohydrodynamic (MHD) turbulence. This is an idealized model for the dead zones that may be present at some radii in protoplanetary and dwarf novae disks. We vary the relative thickness of the dead and active zones to quantify how forced fluid motions in the dead zone change. We find that the residual Reynolds stress near the mid-plane decreases with increasing dead zone thickness, becoming negligible in cases where the active to dead mass ratio is less than a few percent. This impliesmore » that purely Ohmic dead zones would be vulnerable to episodic accretion outbursts via the mechanism of Martin and Lubow. We show that even thick dead zones support a large amount of kinetic energy, but this energy is largely in fluid motions that are inefficient at angular momentum transport. Confirming results from Oishi and Mac Low, the perturbed velocity field in the dead zone is dominated by an oscillatory, vertically extended circulation pattern with a low frequency compared to the orbital frequency. This disturbance has the properties predicted for the lowest order r mode in a hydrodynamic disk. We suggest that in a global disk similar excitations would lead to propagating waves, whose properties would vary with the thickness of the dead zone and the nature of the perturbations (isothermal or adiabatic). Flows with similar amplitudes would buckle settled particle layers and could reduce the efficiency of pebble accretion.« less

  16. Alongshore momentum transfer to the nearshore zone from energetic ocean waves generated by passing hurricanes

    NASA Astrophysics Data System (ADS)

    Mulligan, Ryan P.; Hanson, Jeffrey L.

    2016-06-01

    Wave and current measurements from a cross-shore array of nearshore sensors in Duck, NC, are used to elucidate the balance of alongshore momentum under energetic wave conditions with wide surf zones, generated by passing hurricanes that are close to and far from to the coast. The observations indicate that a distant storm (Hurricane Bill, 2009) with large waves has low variability in directional wave characteristics resulting in alongshore currents that are driven mainly by the changes in wave energy. A storm close to the coast (Hurricane Earl, 2010), with strong local wind stress and combined sea and swell components in wave energy spectra, has high variability in wave direction and wave period that influence wave breaking and nearshore circulation as the storm passes. During both large wave events, the horizontal current shear is strong and radiation stress gradients, bottom stress, wind stress, horizontal mixing, and cross-shore advection contribute to alongshore momentum at different spatial locations across the nearshore region. Horizontal mixing during Hurricane Earl, estimated from rotational velocities, was particularly strong suggesting that intense eddies were generated by the high horizontal shear from opposing wind-driven and wave-driven currents. The results provide insight into the cross-shore distribution of the alongshore current and the connection between flows inside and outside the surf zone during major storms, indicating that the current shear and mixing at the interface between the surf zone and shallow inner shelf is strongly dependent on the distance from the storm center to the coast.

  17. Finite-frequency wave propagation through outer rise fault zones and seismic measurements of upper mantle hydration

    USGS Publications Warehouse

    Miller, Nathaniel; Lizarralde, Daniel

    2016-01-01

    Effects of serpentine-filled fault zones on seismic wave propagation in the upper mantle at the outer rise of subduction zones are evaluated using acoustic wave propagation models. Modeled wave speeds depend on azimuth, with slowest speeds in the fault-normal direction. Propagation is fastest along faults, but, for fault widths on the order of the seismic wavelength, apparent wave speeds in this direction depend on frequency. For the 5–12 Hz Pn arrivals used in tomographic studies, joint-parallel wavefronts are slowed by joints. This delay can account for the slowing seen in tomographic images of the outer rise upper mantle. At the Middle America Trench, confining serpentine to fault zones, as opposed to a uniform distribution, reduces estimates of bulk upper mantle hydration from ~3.5 wt % to as low as 0.33 wt % H2O.

  18. Head orientation affects the intracranial pressure response resulting from shock wave loading in the rat.

    PubMed

    Dal Cengio Leonardi, Alessandra; Keane, Nickolas J; Bir, Cynthia A; Ryan, Anne G; Xu, Liaosa; Vandevord, Pamela J

    2012-10-11

    Since an increasing number of returning military personnel are presenting with neurological manifestations of traumatic brain injury (TBI), there has been a great focus on the effects resulting from blast exposure. It is paramount to resolve the physical mechanism by which the critical stress is being inflicted on brain tissue from blast wave encounters with the head. This study quantitatively measured the effect of head orientation on intracranial pressure (ICP) of rats exposed to a shock wave. Furthermore, the study examined how skull maturity affects ICP response of animals exposed to shock waves at various orientations. Results showed a significant increase in ICP values in larger rats at any orientation. Furthermore, when side-ICP values were compared to the other orientations, the peak pressures were significantly lower suggesting a relation between ICP and orientation of the head due to geometry of the skull and location of sutures. This finding accentuates the importance of skull dynamics in explaining possible injury mechanisms during blast. Also, the rate of pressure change was measured and indicated that the rate was significantly higher when the top of the head was facing the shock front. The results confirm that the biomechanical response of the superior rat skull is distinctive compared to other areas of the skull, suggesting a skull flexure mechanism. These results not only present insights into the mechanism of brain injury, but also provide information which can be used for designing more effective protective head gear. Copyright © 2012 Elsevier Ltd. All rights reserved.

  19. Quantifying Wave Breaking Shape and Type in the Surf-Zone Using LiDAR

    NASA Astrophysics Data System (ADS)

    Albright, A.; Brodie, K. L.; Hartzell, P. J.; Glennie, C. L.

    2017-12-01

    Waves change shape as they shoal and break across the surf-zone, ultimately dissipating and transferring their energy into turbulence by either spilling or plunging. This injection of turbulence and changes in wave shape can affect the direction of sediment transport at the seafloor, and ultimately lead to morphological evolution. Typical methods for collecting wave data in the surf-zone include in-situ pressure gauges, velocimeters, ultrasonic sensors, and video imagery. Drawbacks to these data collection methods are low spatial resolution of point measurements, reliance on linear theory to calculate sea-surface elevations, and intensive computations required to extract wave properties from stereo 2D imagery. As a result, few field measurements of the shapes of plunging and/or spilling breakers exist, and existing knowledge is confined to results of laboratory studies. We therefore examine the use of a multi-beam scanning Light Detection and Ranging (LiDAR) remote sensing instrument with the goal of classifying the breaking type of propagating waves in the surf-zone and quantitatively determining wave morphometric properties. Data were collected with a Velodyne HDL-32E LiDAR scanner (360° vertical field of view) mounted on an arm of the Coastal Research Amphibious Buggy (CRAB) at the U.S. Army Corps of Engineers Field Research Facility in Duck, North Carolina. Processed laser scan data are used to visualize the lifecycle of a wave (shoaling, breaking, broken) and identify wave types (spilling, plunging, non-breaking) as they pass beneath the scanner. For each rotation of the LiDAR scanner, the point cloud data are filtered, smoothed, and detrended in order to identify individual waves and measure their properties, such as speed, height, period, upward/downward slope, asymmetry, and skewness. The 3D nature of point cloud data is advantageous for research, because it enables viewing from any angle. In our analysis, plan views are used to separate individual waves

  20. 78 FR 42733 - Safety Zone; Cleveland Dragon Boat Festival and Head of the Cuyahoga, Cuyahoga River, Cleveland, OH

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-07-17

    ...-AA00 Safety Zone; Cleveland Dragon Boat Festival and Head of the Cuyahoga, Cuyahoga River, Cleveland... intended to restrict vessels from a portion of the Cuyahoga River during the Dragon Boat Festival and Head... over a decade and the Dragon Boat Festival for the last 7 years. In response to past years' events, the...

  1. Coupling of Waves, Turbulence and Thermodynamics Across the Marginal Ice Zone

    DTIC Science & Technology

    2015-09-30

    1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Coupling of Waves, Turbulence and Thermodynamics across...developing Thermodynamically Forced Marginal Ice Zone. Submitted to JGR. Heiles,A. S., NPS thesis, Sep. 2014 Schmidt, B. K., NPS thesis March 2012 Shaw

  2. Acute Appendicitis, Somatosensory Disturbances ("Head Zones"), and the Differential Diagnosis of Anterior Cutaneous Nerve Entrapment Syndrome (ACNES).

    PubMed

    Roumen, Rudi M H; Vening, Wouter; Wouda, Rosanne; Scheltinga, Marc M

    2017-06-01

    Anterior cutaneous nerve entrapment syndrome (ACNES) is a neuropathic abdominal wall pain syndrome typically characterized by locally altered skin sensations. On the other hand, visceral disease may also be associated with similar painful and altered skin sensations ("Head zones"). Aim of the study was to determine if patients with acute appendicitis demonstrated somatosensory disturbances in the corresponding right lower quadrant Head zone. The presence of somatosensory disturbances such as hyperalgesia, hypoesthesia, altered cool perception, or positive pinch test was determined in 100 patients before and after an appendectomy. Potential associations between altered skin sensations and various items including age, sex, history, body temperature, C-reactive protein (CRP), leukocyte count, and type of appendicopathy (normal, inflamed, necrotic, or perforated) were assessed. A total of 39 patients demonstrated at least one right lower abdominal quadrant skin somatosensory disturbance before the laparoscopic appendectomy. However, locoregional skin sensation normalized in all but 2 patients 2 weeks postoperatively. No differences were found concerning patient characteristics or type of appendicopathy between populations with or without altered lower abdominal skin sensations. A substantial portion of patients with acute appendicitis demonstrate right lower abdominal somatosensory disturbances that are similar as observed in acute ACNES. Both may be different sides of the same coin and are possibly expressions of segmental phenomena as described by Head. McBurney's point, a landmark area of maximum pain in acute appendicitis, is possibly a trigger point within a Head zone. Differentiating acute appendicitis from acute ACNES is extremely difficult, but imaging and observation may aid in the diagnostic process.

  3. Study of internal gravity waves in the meteor zone

    NASA Technical Reports Server (NTRS)

    Gavrilov, N. M.

    1987-01-01

    An important component of the dynamical regime of the atmosphere at heights near 100 km are internal gravity waves (IGW) with periods from about 5 min to about 17.5 hrs which propagate from the lower atmospheric layers and are generated in the uppermost region of the atmosphere. As IGW propagate upwards, their amplitudes increase and they have a considerable effect on upper atmospheric processes: (1) they provide heat flux divergences comparable with solar heating; (2) they influence the gaseous composition and produce wave variations of the concentrations of gaseous components and emissions of the upper atmosphere; and (3) they cause considerable acceleration of the mean stream. It was concluded that the periods, wavelengths, amplitudes and velocities of IGW propagation in the meteor zone are now measured quite reliably. However, for estimating the influence of IGW on the thermal regime and the circulation of the upper atmosphere these parameters are not as important as the values of wave fluxes of energy, heat, moment and mass.

  4. Shock Wave Technology and Application: An Update☆

    PubMed Central

    Rassweiler, Jens J.; Knoll, Thomas; Köhrmann, Kai-Uwe; McAteer, James A.; Lingeman, James E.; Cleveland, Robin O.; Bailey, Michael R.; Chaussy, Christian

    2012-01-01

    Context The introduction of new lithotripters has increased problems associated with shock wave application. Recent studies concerning mechanisms of stone disintegration, shock wave focusing, coupling, and application have appeared that may address some of these problems. Objective To present a consensus with respect to the physics and techniques used by urologists, physicists, and representatives of European lithotripter companies. Evidence acquisition We reviewed recent literature (PubMed, Embase, Medline) that focused on the physics of shock waves, theories of stone disintegration, and studies on optimising shock wave application. In addition, we used relevant information from a consensus meeting of the German Society of Shock Wave Lithotripsy. Evidence synthesis Besides established mechanisms describing initial fragmentation (tear and shear forces, spallation, cavitation, quasi-static squeezing), the model of dynamic squeezing offers new insight in stone comminution. Manufacturers have modified sources to either enlarge the focal zone or offer different focal sizes. The efficacy of extracorporeal shock wave lithotripsy (ESWL) can be increased by lowering the pulse rate to 60–80 shock waves/min and by ramping the shock wave energy. With the water cushion, the quality of coupling has become a critical factor that depends on the amount, viscosity, and temperature of the gel. Fluoroscopy time can be reduced by automated localisation or the use of optical and acoustic tracking systems. There is a trend towards larger focal zones and lower shock wave pressures. Conclusions New theories for stone disintegration favour the use of shock wave sources with larger focal zones. Use of slower pulse rates, ramping strategies, and adequate coupling of the shock wave head can significantly increase the efficacy and safety of ESWL. PMID:21354696

  5. Numerical modelling of wind effects on breaking waves in the surf zone

    NASA Astrophysics Data System (ADS)

    Xie, Zhihua

    2017-10-01

    Wind effects on periodic breaking waves in the surf zone have been investigated in this study using a two-phase flow model. The model solves the Reynolds-averaged Navier-Stokes equations with the k - 𝜖 turbulence model simultaneously for the flows both in the air and water. Both spilling and plunging breakers over a 1:35 sloping beach have been studied under the influence of wind, with a focus during wave breaking. Detailed information of the distribution of wave amplitudes and mean water level, wave-height-to-water-depth ratio, the water surface profiles, velocity, vorticity, and turbulence fields have been presented and discussed. The inclusion of wind alters the air flow structure above water waves, increases the generation of vorticity, and affects the wave shoaling, breaking, overturning, and splash-up processes. Wind increases the water particle velocities and causes water waves to break earlier and seaward, which agrees with the previous experiment.

  6. Propagation of arbitrary initial wave packets in a quantum parametric oscillator: Instability zones for higher order moments

    NASA Astrophysics Data System (ADS)

    Biswas, Subhadip; Chattopadhyay, Rohitashwa; Bhattacharjee, Jayanta K.

    2018-05-01

    We consider the dynamics of a particle in a parametric oscillator with a view to exploring any quantum feature of the initial wave packet that shows divergent (in time) behaviour for parameter values where the classical motion dynamics of the mean position is bounded. We use Ehrenfest's theorem to explore the dynamics of nth order moment which reduces exactly to a linear non autonomous differential equation of order n + 1. It is found that while the width and skewness of the packet is unbounded exactly in the zones where the classical motion is unbounded, the kurtosis of an initially non-gaussian wave packet can become infinitely large in certain additional zones. This implies that the shape of the wave packet can change drastically with time in these zones.

  7. Acoustic pressure waves induced in human heads by RF pulses from high-field MRI scanners.

    PubMed

    Lin, James C; Wang, Zhangwei

    2010-04-01

    The current evolution toward greater image resolution from magnetic resonance image (MRI) scanners has prompted the exploration of higher strength magnetic fields and use of higher levels of radio frequencies (RFs). Auditory perception of RF pulses by humans has been reported during MRI with head coils. It has shown that the mechanism of interaction for the auditory effect is caused by an RF pulse-induced thermoelastic pressure wave inside the head. We report a computational study of the intensity and frequency of thermoelastic pressure waves generated by RF pulses in the human head inside high-field MRI and clinical scanners. The U.S. Food and Drug Administration (U.S. FDA) guides limit the local specific absorption rate (SAR) in the body-including the head-to 8 W kg(-1). We present results as functions of SAR and show that for a given SAR the peak acoustic pressures generated in the anatomic head model were essentially the same at 64, 300, and 400 MHz (1.5, 7.0, and 9.4 T). Pressures generated in the anatomic head are comparable to the threshold pressure of 20 mPa for sound perception by humans at the cochlea for 4 W kg(-1). Moreover, results indicate that the peak acoustic pressure in the brain is only 2 to 3 times the auditory threshold at the U.S. FDA guideline of 8 W kg(-1). Even at a high SAR of 20 W kg(-1), where the acoustic pressure in the brain could be more than 7 times the auditory threshold, the sound pressure levels would not be more than 17 db above threshold of perception at the cochlea.

  8. Ultrasonic probing of the fracture process zone in rock using surface waves

    NASA Technical Reports Server (NTRS)

    Swanson, P. L.; Spetzler, H.

    1984-01-01

    A microcrack process zone is frequently suggested to accompany macrofractures in rock and play an important role in the resistance to fracture propagation. Attenuation of surface waves propagating through mode I fractures in wedge-loaded double-cantilever beam specimens of Westerly granite has been recorded in an attempt to characterize the structure of the fracture process zone. The ultrasonic measurements do not support the generally accepted model of a macroscopic fracture that incrementally propagates with the accompaniment of a cloud of microcracks. Instead, fractures in Westerly granite appear to form as gradually separating surfaces within a zone having a width of a few millimeters and a length of several tens of millimeters. A fracture process zone of this size would necessitate the use of meter-sized specimens in order for linear elastic fracture mechanics to be applicable.

  9. Modelling wave-induced sea ice break-up in the marginal ice zone

    NASA Astrophysics Data System (ADS)

    Montiel, F.; Squire, V. A.

    2017-10-01

    A model of ice floe break-up under ocean wave forcing in the marginal ice zone (MIZ) is proposed to investigate how floe size distribution (FSD) evolves under repeated wave break-up events. A three-dimensional linear model of ocean wave scattering by a finite array of compliant circular ice floes is coupled to a flexural failure model, which breaks a floe into two floes provided the two-dimensional stress field satisfies a break-up criterion. A closed-feedback loop algorithm is devised, which (i) solves the wave-scattering problem for a given FSD under time-harmonic plane wave forcing, (ii) computes the stress field in all the floes, (iii) fractures the floes satisfying the break-up criterion, and (iv) generates an updated FSD, initializing the geometry for the next iteration of the loop. The FSD after 50 break-up events is unimodal and near normal, or bimodal, suggesting waves alone do not govern the power law observed in some field studies. Multiple scattering is found to enhance break-up for long waves and thin ice, but to reduce break-up for short waves and thick ice. A break-up front marches forward in the latter regime, as wave-induced fracture weakens the ice cover, allowing waves to travel deeper into the MIZ.

  10. Subsurface fault damage zone of the 2014 Mw 6.0 South Napa, California, earthquake viewed from fault‐zone trapped waves

    USGS Publications Warehouse

    Li, Yong-Gang; Catchings, Rufus D.; Goldman, Mark R.

    2016-01-01

    The aftershocks of the 24 August 2014 Mw 6.0 South Napa earthquake generated prominent fault‐zone trapped waves (FZTWs) that were recorded on two 1.9‐km‐long seismic arrays deployed across the northern projection (array 1, A1) and the southern part (A2) of the surface rupture of the West Napa fault zone (WNFZ). We also observed FZTWs on an array (A3) deployed across the intersection of the Franklin and Southampton faults, which appear to be the southward continuations of the WNFZ. A1, A2, and A3 consisted of 20, 20, and 10 L28 (4.5 Hz) three‐component seismographs. We analyzed waveforms of FZTWs from 55 aftershocks in both time and frequency to characterize the fault damage zone associated with this Mw 6.0 earthquake. Post‐S coda durations of FZTWs increase with epicentral distances and focal depths from the recording arrays, suggesting a low‐velocity waveguide along the WNFZ to depths in excess of 5–7 km. Locations of the aftershocks showing FZTWs, combined with 3D finite‐difference simulations, suggest the subsurface rupture zone having an S‐wave speed reduction of ∼40%–50% between A1 and A2, coincident with the ∼14‐km‐long mapped surface rupture zone and at least an ∼500‐m‐wide deformation zone. The low‐velocity waveguide along the WNFZ extends further southward to at least A3, but with a more moderate‐velocity reduction of 30%–35% at ray depth. This last FZTW observation suggests continuity between the WNFZ and Franklin fault. The waveguide effect may have localized and amplified ground shaking along the WNFZ and the faults farther to the south (see a companion paper by Catchings et al., 2016).

  11. A shallow fault-zone structure illuminated by trapped waves in the Karadere-Duzce branch of the North Anatolian Fault, western Turkey

    USGS Publications Warehouse

    Ben-Zion, Y.; Peng, Z.; Okaya, D.; Seeber, L.; Armbruster, J.G.; Ozer, N.; Michael, A.J.; Baris, S.; Aktar, M.

    2003-01-01

    We discuss the subsurface structure of the Karadere-Duzce branch of the North Anatolian Fault based on analysis of a large seismic data set recorded by a local PASSCAL network in the 6 months following the Mw = 7.4 1999 Izmit earthquake. Seismograms observed at stations located in the immediate vicinity of the rupture zone show motion amplification and long-period oscillations in both P- and S-wave trains that do not exist in nearby off-fault stations. Examination of thousands of waveforms reveals that these characteristics are commonly generated by events that are well outside the fault zone. The anomalous features in fault-zone seismograms produced by events not necessarily in the fault may be referred to generally as fault-zone-related site effects. The oscillatory shear wave trains after the direct S arrival in these seismograms are analysed as trapped waves propagating in a low-velocity fault-zone layer. The time difference between the S arrival and trapped waves group does not grow systematically with increasing source-receiver separation along the fault. These observations imply that the trapping of seismic energy in the Karadere-Duzce rupture zone is generated by a shallow fault-zone layer. Traveltime analysis and synthetic waveform modelling indicate that the depth of the trapping structure is approximately 3-4 km. The synthetic waveform modelling indicates further that the shallow trapping structure has effective waveguide properties consisting of thickness of the order of 100 m, a velocity decrease relative to the surrounding rock of approximately 50 per cent and an S-wave quality factor of 10-15. The results are supported by large 2-D and 3-D parameter space studies and are compatible with recent analyses of trapped waves in a number of other faults and rupture zones. The inferred shallow trapping structure is likely to be a common structural element of fault zones and may correspond to the top part of a flower-type structure. The motion amplification

  12. Simplified method for the calculation of irregular waves in the coastal zone

    NASA Astrophysics Data System (ADS)

    Leont'ev, I. O.

    2011-04-01

    A method applicable for the estimation of the wave parameters along a set bottom profile is suggested. It takes into account the principal processes having an influence on the waves in the coastal zone: the transformation, refraction, bottom friction, and breaking. The ability to use a constant mean value of the friction coefficient under conditions of sandy shores is implied. The wave breaking is interpreted from the viewpoint of the concept of the limiting wave height at a given depth. The mean and root-mean-square wave heights are determined by the height distribution function, which transforms under the effect of the breaking. The verification of the method on the basis of the natural data shows that the calculation results reproduce the observed variations of the wave heights in a wide range of conditions, including profiles with underwater bars. The deviations from the calculated values mostly do not exceed 25%, and the mean square error is 11%. The method does not require a preliminary setting and can be implemented in the form of a relatively simple calculator accessible even for an inexperienced user.

  13. Stereo Refractive Imaging of Breaking Free-Surface Waves in the Surf Zone

    NASA Astrophysics Data System (ADS)

    Mandel, Tracy; Weitzman, Joel; Koseff, Jeffrey; Environmental Fluid Mechanics Laboratory Team

    2014-11-01

    Ocean waves drive the evolution of coastlines across the globe. Wave breaking suspends sediments, while wave run-up, run-down, and the undertow transport this sediment across the shore. Complex bathymetric features and natural biotic communities can influence all of these dynamics, and provide protection against erosion and flooding. However, our knowledge of the exact mechanisms by which this occurs, and how they can be modeled and parameterized, is limited. We have conducted a series of controlled laboratory experiments with the goal of elucidating these details. These have focused on quantifying the spatially-varying characteristics of breaking waves and developing more accurate techniques for measuring and predicting wave setup, setdown, and run-up. Using dynamic refraction stereo imaging, data on free-surface slope and height can be obtained over an entire plane. Wave evolution is thus obtained with high spatial precision. These surface features are compared with measures of instantaneous turbulence and mean currents within the water column. We then use this newly-developed ability to resolve three-dimensional surface features over a canopy of seagrass mimics, in order to validate theoretical formulations of wave-vegetation interactions in the surf zone.

  14. Wave-induced current considering wave-tide interaction in Haeundae

    NASA Astrophysics Data System (ADS)

    Lim, Hak Soo

    2017-04-01

    The Haeundae, located at the south eastern end of the Korean Peninsula, is a famous beach, which has an approximately 1.6 km long and 70 m wide coastline. The beach has been repeatedly eroded by the swell waves caused by typhoons in summer and high waves originating in the East Sea in winter. The Korean government conducted beach restoration projects including beach nourishment (620,000 m3) and construction of two submerged breakwaters near both ends of the beach. To prevent the beach erosion and to support the beach restoration project, the Korean government initiated a R&D project, the development of coastal erosion control technology since 2013. As a part of the project, we have been measuring waves and currents at a water depth of 22 m, 1.8 km away from the beach using an acoustic wave and current meter (AWAC) continuously for more than three years; we have also measured waves and currents intensively near the surf-zone in summer and winter. In this study, a numerical simulation using a wave and current coupled model (ROMS-SWAN) was conducted for determining the wave-induced current considering seasonal swell waves (Hs : 2.5 m, Tp: 12 s) and for better understanding of the coastal process near the surf-zone in Haeundae. By comparing the measured and simulated results, we found that cross-shore current during summer is mainly caused by the eddy produced by the wave-induced current near the beach, which in turn, is generated by the strong waves coming from the SSW and S directions. During other seasons, longshore wave-induced current is produced by the swell waves coming from the E and ESE directions. The longshore current heading west toward Dong-Back Island, west end of the beach, during all the seasons and eddy current toward Mipo-Port, east end of the beach, in summer which is well matched with the observed residual current. The wave-induced current with long-term measurement data is incorporated in simulation of sediment transport modeling for developing

  15. Thermal comfort zone of the hands, feet and head in males and females.

    PubMed

    Ciuha, Urša; Mekjavic, Igor B

    2017-10-01

    The present study compared the thermal comfort zones (TCZ) of the hands, feet and head in eight male and eight female participants, assessed with water-perfused segments (WPS). On separate occasions, and separated by a minimum of one day, participants were requested to regulate the temperature of three distal skin regions (hands, feet and head) within their TCZ. On each occasion they donned a specific water-perfused segment (WPS), either gloves, socks or hood for assessing the TCZ of the hands, feet and head, respectively. In the absence of regulation, the temperature of the water perfusing the WPS changed in a saw-tooth manner from 10 to 50°C; by depressing a switch and reversing the direction of the temperature at the limits of the TCZ, each participant defined the TCZ for each skin region investigated. The range of regulated temperatures (upper and lower limits of the TCZ) did not differ between studied skin regions or between genders. Participants however maintained higher head (35.7±0.4°C; p˂0.001) skin temperature (Tsk) compared to hands (34.5±0.8°C) and feet (33.8±1.1°C). When exposed to normothermic conditions, distal skin regions do not differ in ranges of temperatures, perceived as thermally comfortable. Copyright © 2017. Published by Elsevier Inc.

  16. Modelling wave-induced sea ice break-up in the marginal ice zone

    PubMed Central

    Squire, V. A.

    2017-01-01

    A model of ice floe break-up under ocean wave forcing in the marginal ice zone (MIZ) is proposed to investigate how floe size distribution (FSD) evolves under repeated wave break-up events. A three-dimensional linear model of ocean wave scattering by a finite array of compliant circular ice floes is coupled to a flexural failure model, which breaks a floe into two floes provided the two-dimensional stress field satisfies a break-up criterion. A closed-feedback loop algorithm is devised, which (i) solves the wave-scattering problem for a given FSD under time-harmonic plane wave forcing, (ii) computes the stress field in all the floes, (iii) fractures the floes satisfying the break-up criterion, and (iv) generates an updated FSD, initializing the geometry for the next iteration of the loop. The FSD after 50 break-up events is unimodal and near normal, or bimodal, suggesting waves alone do not govern the power law observed in some field studies. Multiple scattering is found to enhance break-up for long waves and thin ice, but to reduce break-up for short waves and thick ice. A break-up front marches forward in the latter regime, as wave-induced fracture weakens the ice cover, allowing waves to travel deeper into the MIZ. PMID:29118659

  17. Modelling wave-induced sea ice break-up in the marginal ice zone.

    PubMed

    Montiel, F; Squire, V A

    2017-10-01

    A model of ice floe break-up under ocean wave forcing in the marginal ice zone (MIZ) is proposed to investigate how floe size distribution (FSD) evolves under repeated wave break-up events. A three-dimensional linear model of ocean wave scattering by a finite array of compliant circular ice floes is coupled to a flexural failure model, which breaks a floe into two floes provided the two-dimensional stress field satisfies a break-up criterion. A closed-feedback loop algorithm is devised, which (i) solves the wave-scattering problem for a given FSD under time-harmonic plane wave forcing, (ii) computes the stress field in all the floes, (iii) fractures the floes satisfying the break-up criterion, and (iv) generates an updated FSD, initializing the geometry for the next iteration of the loop. The FSD after 50 break-up events is unimodal and near normal, or bimodal, suggesting waves alone do not govern the power law observed in some field studies. Multiple scattering is found to enhance break-up for long waves and thin ice, but to reduce break-up for short waves and thick ice. A break-up front marches forward in the latter regime, as wave-induced fracture weakens the ice cover, allowing waves to travel deeper into the MIZ.

  18. Head-on collision between positron acoustic waves in homogeneous and inhomogeneous plasmas

    NASA Astrophysics Data System (ADS)

    Alam, M. S.; Hafez, M. G.; Talukder, M. R.; Ali, M. Hossain

    2018-05-01

    The head-on collision between positron acoustic solitary waves (PASWs) as well as the production of rogue waves (RWs) in homogeneous and PASWs in inhomogeneous unmagnetized plasma systems are investigated deriving the nonlinear evolution equations. The plasmas are composed of immobile positive ions, mobile cold and hot positrons, and hot electrons, where the hot positrons and hot electrons are assumed to follow the Kappa distributions. The evolution equations are derived using the appropriate coordinate transformation and the reductive perturbation technique. The effects of concentrations, kappa parameters of hot electrons and positrons, and temperature ratios on the characteristics of PASWs and RWs are examined. It is found that the kappa parameters and temperature ratios significantly modify phase shifts after head-on collisions and RWs in homogeneous as well as PASWs in inhomogeneous plasmas. The amplitudes of the PASWs in inhomogeneous plasmas are diminished with increasing kappa parameters, concentration and temperature ratios. Further, the amplitudes of RWs are reduced with increasing charged particles concentration, while it enhances with increasing kappa- and temperature parameters. Besides, the compressive and rarefactive solitons are produced at critical densities from KdV equation for hot and cold positrons, while the compressive solitons are only produced from mKdV equation for both in homogeneous and inhomogeneous plasmas.

  19. Deep rock damage in the San Andreas Fault revealed by P- and S-type fault-zone-guided waves

    USGS Publications Warehouse

    Ellsworth, William L.; Malin, Peter E.

    2011-01-01

    Damage to fault-zone rocks during fault slip results in the formation of a channel of low seismic-wave velocities. Within such channels guided seismic waves, denoted by Fg, can propagate. Here we show with core samples, well logs and Fg-waves that such a channel is crossed by the SAFOD (San Andreas Fault Observatory at Depth) borehole at a depth of 2.7 km near Parkfield, California, USA. This laterally extensive channel extends downwards to at least half way through the seismogenic crust, more than about 7 km. The channel supports not only the previously recognized Love-type- (FL) and Rayleigh-type- (FR) guided waves, but also a new fault-guided wave, which we name FF. As recorded 2.7 km underground, FF is normally dispersed, ends in an Airy phase, and arrives between the P- and S-waves. Modelling shows that FF travels as a leaky mode within the core of the fault zone. Combined with the drill core samples, well logs and the two other types of guided waves, FF at SAFOD reveals a zone of profound, deep, rock damage. Originating from damage accumulated over the recent history of fault movement, we suggest it is maintained either by fracturing near the slip surface of earthquakes, such as the 1857 Fort Tejon M 7.9, or is an unexplained part of the fault-creep process known to be active at this site.

  20. Quantification of Surf Zone Bathymetry from Video Observations of Wave Breaking

    NASA Astrophysics Data System (ADS)

    Aarninkhof, S.; Ruessink, G.

    2002-12-01

    Cost-efficient methods to quantify surf zone bathymetry with high resolution in time and space would be of great value for coastal research and management. Automated video techniques provide the potential to do so. Time-averaged video observations of the nearshore zone show bright intensities at locations where waves preferentially break. Highly similar patterns are found from model simulations of depth-induced wave breaking, which show increasing rates of wave dissipation in shallow areas like sand bars. Thus, video observations of wave breaking - at least qualitatively - reflect sub-merged beach bathymetry. In search of the quantification of this relationship, we present a new model concept to map sub-merged beach bathymetry from time-averaged video images. This is achieved by matching model-predicted and video-observed rates of wave dissipation. First, time-averaged image intensities are sampled along a cross-shore array and interpreted in terms of a wave dissipation parameter. This involves a correction for the effect of persistent foam, which is visible at time-averaged video images but not predicted by common wave propagation models. The dissipation profiles thus obtained are used to update an initial beach bathymetry through optimisation of the match between measured and modelled rates of wave dissipation. The latter is done by raising the bottom elevation in areas where the measured dissipation rate exceeds the computed dissipation and vice versa. Since the model includes video data with high resolution in time (typically multiple images over a tidal cycle), it allows for virtually continous monitoring of surfzone bathymetry . Model tests against a synthetic data set of artificially generated wave dissipation profiles have shown the model's capability to accurately reconstruct beach bathymetry, over a wide range of morphological configurations. Maximum model deviations were found in the case of highly developed bar-trough systems (bar heights up to 4 m) and

  1. A study on the prenatal zone of ultrasonic guided waves in plates

    NASA Astrophysics Data System (ADS)

    Thomas, Tibin; Balasubramaniam, Krishnan

    2017-02-01

    Low frequency guided wave based inspection is an extensively used method for asset management with the advantage of wide area coverage from a single location at the cost of spatial resolution. With the advent of high frequency guided waves, short range inspections with high spatial resolution for monitoring corrosion under pipe supports and tank annular plates has gained widespread interest and acceptance. One of the major challenges in the application of high frequency guided waves in a short range inspection is to attain the desired modal displacements with respect to the application. In this paper, an investigation on the generation and formation of fundamental S0 mode is carried out through numerical simulation and experiments to establish a prenatal zone for guided waves. The effect of frequency, thickness of the plate and frequency-thickness (f*d) is studied. The investigation reveals the existence of a rudimentary form with similar modal features to the fully developed mode. This study helps in the design and development of a high frequency guided wave generator for particular applications which demands waves with very less sensitivity to the surface and loading during the initial phase which immediately evolves to a more sensitive wave towards the surface on propagation for the detection of shallow defects.

  2. Realistic numerical modelling of human head tissue exposure to electromagnetic waves from cellular phones

    NASA Astrophysics Data System (ADS)

    Scarella, Gilles; Clatz, Olivier; Lanteri, Stéphane; Beaume, Grégory; Oudot, Steve; Pons, Jean-Philippe; Piperno, Sergo; Joly, Patrick; Wiart, Joe

    2006-06-01

    The ever-rising diffusion of cellular phones has brought about an increased concern for the possible consequences of electromagnetic radiation on human health. Possible thermal effects have been investigated, via experimentation or simulation, by several research projects in the last decade. Concerning numerical modeling, the power absorption in a user's head is generally computed using discretized models built from clinical MRI data. The vast majority of such numerical studies have been conducted using Finite Differences Time Domain methods, although strong limitations of their accuracy are due to heterogeneity, poor definition of the detailed structures of head tissues (staircasing effects), etc. In order to propose numerical modeling using Finite Element or Discontinuous Galerkin Time Domain methods, reliable automated tools for the unstructured discretization of human heads are also needed. Results presented in this article aim at filling the gap between human head MRI images and the accurate numerical modeling of wave propagation in biological tissues and its thermal effects. To cite this article: G. Scarella et al., C. R. Physique 7 (2006).

  3. A unified spectral,parameterization for wave breaking: from the deep ocean to the surf zone

    NASA Astrophysics Data System (ADS)

    Filipot, J.

    2010-12-01

    A new wave-breaking dissipation parameterization designed for spectral wave models is presented. It combines wave breaking basic physical quantities, namely, the breaking probability and the dissipation rate per unit area. The energy lost by waves is fi[|#12#|]rst calculated in the physical space before being distributed over the relevant spectral components. This parameterization allows a seamless numerical model from the deep ocean into the surf zone. This transition from deep to shallow water is made possible by a dissipation rate per unit area of breaking waves that varies with the wave height, wavelength and water depth.The parameterization is further tested in the WAVEWATCH III TM code, from the global ocean to the beach scale. Model errors are smaller than with most specialized deep or shallow water parameterizations.

  4. The Sorong Fault Zone, Indonesia: Mapping a Fault Zone Offshore

    NASA Astrophysics Data System (ADS)

    Melia, S.; Hall, R.

    2017-12-01

    The Sorong Fault Zone is a left-lateral strike-slip fault zone in eastern Indonesia, extending westwards from the Bird's Head peninsula of West Papua towards Sulawesi. It is the result of interactions between the Pacific, Caroline, Philippine Sea, and Australian Plates and much of it is offshore. Previous research on the fault zone has been limited by the low resolution of available data offshore, leading to debates over the extent, location, and timing of movements, and the tectonic evolution of eastern Indonesia. Different studies have shown it north of the Sula Islands, truncated south of Halmahera, continuing to Sulawesi, or splaying into a horsetail fan of smaller faults. Recently acquired high resolution multibeam bathymetry of the seafloor (with a resolution of 15-25 meters), and 2D seismic lines, provide the opportunity to trace the fault offshore. The position of different strands can be identified. On land, SRTM topography shows that in the northern Bird's Head the fault zone is characterised by closely spaced E-W trending faults. NW of the Bird's Head offshore there is a fold and thrust belt which terminates some strands. To the west of the Bird's Head offshore the fault zone diverges into multiple strands trending ENE-WSW. Regions of Riedel shearing are evident west of the Bird's Head, indicating sinistral strike-slip motion. Further west, the ENE-WSW trending faults turn to an E-W trend and there are at least three fault zones situated immediately south of Halmahera, north of the Sula Islands, and between the islands of Sanana and Mangole where the fault system terminates in horsetail strands. South of the Sula islands some former normal faults at the continent-ocean boundary with the North Banda Sea are being reactivated as strike-slip faults. The fault zone does not currently reach Sulawesi. The new fault map differs from previous interpretations concerning the location, age and significance of different parts of the Sorong Fault Zone. Kinematic

  5. Imaging San Jacinto Fault damage zone structure using dense linear arrays: application of ambient noise tomography, Rayleigh wave ellipticity, and site amplification

    NASA Astrophysics Data System (ADS)

    Wang, Y.; Lin, F. C.; Allam, A. A.; Ben-Zion, Y.

    2017-12-01

    The San Jacinto fault is presently the most seismically active component of the San Andreas Transform system in Southern California. To study the damage zone structure, two dense linear geophone arrays (BS and RR) were deployed across the Clark segment of the San Jacinto Fault between Anza and Hemet during winter 2015 and Fall 2016, respectively. Both arrays were 2 km long with 20 m station spacing. Month-long three-component ambient seismic noise data were recorded and used to calculate multi-channel cross-correlation functions. All three-component noise records of each array were normalized simultaneously to retain relative amplitude information between different stations and different components. We observed clear Rayleigh waves and Love waves on the cross-correlations of both arrays at 0.3 - 1 s period. The phase travel times of the Rayleigh waves on both arrays were measured by frequency-time analysis (FTAN), and inverted for Rayleigh wave phase velocity profiles of the upper 500 m depth. For both arrays, we observe prominent asymmetric low velocity zones which narrow with depth. At the BS array near the Hemet Stepover, an approximately 250m wide slow zone is observed to be offset by 75m to the northeast of the surface fault trace. At the RR array near the Anza segment of the fault, a similar low velocity zone width and offset are observed, along with a 10% across-fault velocity contrast. Analyses of Rayleigh wave ellipticity (H/V ratio), Love wave phase travel times, and site amplification are in progress. By using multiple measurements from ambient noise cross-correlations, we can obtain strong constraints on the local damage zone structure of the San Jacinto Fault. The results contribute to improved understanding of rupture directivity, maximum earthquake magnitude and more generally seismic hazard associated with the San Jacinto fault zone.

  6. A note on specific variability of long surface gravity waves and drag coefficient in coastal upwelling zone

    NASA Astrophysics Data System (ADS)

    Krzyścin, Janusz

    1990-01-01

    In this paper we solve analytically wave kinematic equations and the wave energy transport equation, for basic long surface gravity wave in the coastal upwelling zone. Using Gent and Taylor's (1978) parameterization of drag coefficient (which includes interaction between long surface waves and the air flow) we find variability of this coefficient due to wave amplification and refraction caused by specific surface water current in the region. The drag coefficient grows towards the shore. The growth is faster for stronger current. When the angle between waves and the current is less than 90° the growth is mainly connected with the waves steepness, but when the angle is larger, it is caused by relative growth of the wave phase velocity.

  7. Propagation of acoustic-gravity waves in arctic zones with elastic ice-sheets

    NASA Astrophysics Data System (ADS)

    Kadri, Usama; Abdolali, Ali; Kirby, James T.

    2017-04-01

    We present an analytical solution of the boundary value problem of propagating acoustic-gravity waves generated in the ocean by earthquakes or ice-quakes in arctic zones. At the surface, we assume elastic ice-sheets of a variable thickness, and show that the propagating acoustic-gravity modes have different mode shape than originally derived by Ref. [1] for a rigid ice-sheet settings. Computationally, we couple the ice-sheet problem with the free surface model by Ref. [2] representing shrinking ice blocks in realistic sea state, where the randomly oriented ice-sheets cause inter modal transition at the edges and multidirectional reflections. We then derive a depth-integrated equation valid for spatially slowly varying thickness of ice-sheet and water depth. Surprisingly, and unlike the free-surface setting, here it is found that the higher acoustic-gravity modes exhibit a larger contribution. These modes travel at the speed of sound in water carrying information on their source, e.g. ice-sheet motion or submarine earthquake, providing various implications for ocean monitoring and detection of quakes. In addition, we found that the propagating acoustic-gravity modes can result in orbital displacements of fluid parcels sufficiently high that may contribute to deep ocean currents and circulation, as postulated by Refs. [1, 3]. References [1] U. Kadri, 2016. Generation of Hydroacoustic Waves by an Oscillating Ice Block in Arctic Zones. Advances in Acoustics and Vibration, 2016, Article ID 8076108, 7 pages http://dx.doi.org/10.1155/2016/8076108 [2] A. Abdolali, J. T. Kirby and G. Bellotti, 2015, Depth-integrated equation for hydro-acoustic waves with bottom damping, J. Fluid Mech., 766, R1 doi:10.1017/jfm.2015.37 [3] U. Kadri, 2014. Deep ocean water transportation by acoustic?gravity waves. J. Geophys. Res. Oceans, 119, doi:10.1002/ 2014JC010234

  8. A unified spectral parameterization for wave breaking: From the deep ocean to the surf zone

    NASA Astrophysics Data System (ADS)

    Filipot, J.-F.; Ardhuin, F.

    2012-11-01

    A new wave-breaking dissipation parameterization designed for phase-averaged spectral wave models is presented. It combines wave breaking basic physical quantities, namely, the breaking probability and the dissipation rate per unit area. The energy lost by waves is first explicitly calculated in physical space before being distributed over the relevant spectral components. The transition from deep to shallow water is made possible by using a dissipation rate per unit area of breaking waves that varies with the wave height, wavelength and water depth. This parameterization is implemented in the WAVEWATCH III modeling framework, which is applied to a wide range of conditions and scales, from the global ocean to the beach scale. Wave height, peak and mean periods, and spectral data are validated using in situ and remote sensing data. Model errors are comparable to those of other specialized deep or shallow water parameterizations. This work shows that it is possible to have a seamless parameterization from the deep ocean to the surf zone.

  9. Radar Remote Sensing of Waves and Currents in the Nearshore Zone

    DTIC Science & Technology

    2006-01-01

    and application of novel microwave, acoustic, and optical remote sensing techniques. The objectives of this effort are to determine the extent to which...Doppler radar techniques are useful for nearshore remote sensing applications. Of particular interest are estimates of surf zone location and extent...surface currents, waves, and bathymetry. To date, optical (video) techniques have been the primary remote sensing technology used for these applications. A key advantage of the radar is its all weather day-night operability.

  10. Shallow Vs Structure Accross Hayward Fault Zone Inferred from Multichannel Analysis of Surface Waves (MASW)

    NASA Astrophysics Data System (ADS)

    Chan, J. H.; Richardson, I. S.; Strayer, L. M.; Catchings, R.; McEvilly, A.; Goldman, M.; Criley, C.; Sickler, R. R.

    2017-12-01

    The Hayward Fault Zone (HFZ) includes the Hayward fault (HF), as well as several named and unnamed subparallel, subsidiary faults to the east, among them the Quaternary-active Chabot Fault (CF), the Miller Creek Fault (MCF), and a heretofore unnamed fault, the Redwood Thrust Fault (RTF). With an ≥M6.0 recurrence interval of 130 y for the HF and the last major earthquake in 1868, the HFZ is a major seismic hazard in the San Francisco Bay Area, exacerbated by the many unknown and potentially active secondary faults of the HFZ. In 2016, researchers from California State University, East Bay, working in concert with the United States Geological Survey conducted the East Bay Seismic Investigation (EBSI). We deployed 296 RefTek RT125 (Texan) seismographs along a 15-km-long linear seismic profile across the HF, extending from the bay in San Leandro to the hills in Castro Valley. Two-channel seismographs were deployed at 100 m intervals to record P- and S-waves, and additional single-channel seismographs were deployed at 20 m intervals where the seismic line crossed mapped faults. The active-source survey consisted of 16 buried explosive shots located at approximately 1-km intervals along the seismic line. We used the Multichannel Analysis of Surfaces Waves (MASW) method to develop 2-D shear-wave velocity models across the CF, MCF, and RTF. Preliminary MASW analysis show areas of anomalously low S-wave velocities , indicating zones of reduced shear modulus, coincident with these three mapped faults; additional velocity anomalies coincide with unmapped faults within the HFZ. Such compliant zones likely correspond to heavily fractured rock surrounding the faults, where the shear modulus is expected to be low compared to the undeformed host rock.

  11. Mass-energy and momentum extraction by gravitational wave emission in the merger of two colliding black holes: The non-head-on case

    NASA Astrophysics Data System (ADS)

    Aranha, R. F.; Soares, I. Damião; Tonini, E. V.

    2012-01-01

    We examine numerically the post-merger regime of two nonspining holes in non-head-on collisions in the realm of nonaxisymmetric Robinson-Trautman spacetimes. Characteristic initial data for the system are constructed and evolved via the Robinson-Trautman equation. The numerical integration is performed using a Galerkin spectral method which is sufficiently stable to reach the final configuration of the remnant black hole, when the gravitational wave emission ceases. The initial data contains three independent parameters, the ratio mass α of the individual colliding black holes, their initial premerger infalling velocity and the incidence angle of collision ρ0. The remnant black hole is characterized by its final boost parameter, rest mass and scattering angle. The motion of the remnant black hole is restricted to the plane determined by the directions of the two initial colliding black holes, characterizing a planar collision. The net momentum fluxes carried out by gravitational waves are confined to this plane. We evaluate the efficiency of mass-energy extraction, the total energy and momentum carried out by gravitational waves and the momentum distribution of the remnant black hole for a large domain of initial data parameters. Our analysis is based on the Bondi-Sachs four-momentum conservation laws. The process of mass-energy extraction is shown to be less efficient as the initial data departs from the head-on configuration. Head-on collisions (ρ0=0o) and orthogonal collisions (ρ0=90°) constitute, respectively, upper and lower bounds to the power emission and to the efficiency of mass-energy extraction. On the contrary, head-on collisions and orthogonal collisions constitute, respectively, lower and upper bounds for the momentum of the remnant. Distinct regimes of gravitational wave emission (bursts or quiescent emission) are characterized by the analysis of the time behavior of the gravitational wave power as a function of α. In particular, the net

  12. Regional P wave velocity structure of the Northern Cascadia Subduction Zone

    USGS Publications Warehouse

    Ramachandran, K.; Hyndman, R.D.; Brocher, T.M.

    2006-01-01

    This paper presents the first regional three-dimensional, P wave velocity model for the Northern Cascadia Subduction. Zone (SW British Columbia and NW Washington State) constructed through tomographic inversion of first-arrival traveltime data from active source experiments together with earthquake traveltime data recorded at permanent stations. The velocity model images the structure of the subducting Juan de Fuca plate, megathrust, and the fore-arc crust and upper mantle. Beneath southern Vancouver Island the megathrust above the Juan de Fuca plate is characterized by a broad zone (25-35 km depth) having relatively low velocities of 6.4-6.6 km/s. This relative low velocity zone coincides with the location of most of the episodic tremors recently mapped beneath Vancouver Island, and its low velocity may also partially reflect the presence of trapped fluids and sheared lower crustal rocks. The rocks of the Olympic Subduction Complex are inferred to deform aseismically as evidenced by the lack of earthquakes withi the low-velocity rocks. The fore-arc upper mantle beneath the Strait of Georgia and Puget Sound is characterized by velocities of 7.2-7.6 km/s. Such low velocities represent regional serpentinization of the upper fore-arc mantle and provide evidence for slab dewatering and densification. Tertiary sedimentary basins in the Strait of Georgia and Puget Lowland imaged by the velocity model lie above the inferred region of slab dewatering and densification and may therefore partly result from a higher rate of slab sinking. In contrast, sedimentary basins in the Strait of Juan de Fuca lie in a synclinal depression in the Crescent Terrane. The correlation of in-slab earthquake hypocenters M>4 with P wave velocities greater than 7.8 km/s at the hypocenters suggests that they originate near the oceanic Moho of the subducting Juan de Fuca plate. Copyright 2006 by the American Geophysical Union.

  13. Transverse ion energization and low-frequency plasma waves in the mid-altitude auroral zone - A case study

    NASA Technical Reports Server (NTRS)

    Peterson, W. K.; Shelley, E. G.; Boardsen, S. A.; Gurnett, D. A.; Ledley, B. G.; Sugiura, M.; Moore, T. E.

    1988-01-01

    Evidence of transverse ion energization at altitudes of several earth radii in the auroral zone was reexamined using several hundred hours of high-sensitivity and high-resolution plasma data obtained by the Dynamics Explorer 1 satellite. The data on particle environment encountered at midaltitudes in the auroral zone disclosed rapid variations in the values of total density, thermal structure, and composition of the plasma in the interval measured; the modes of low-frequency plasma waves also varied rapidly. It was not possible to unambiguously identify in these data particle and wave signature of local transverse ion energization; however, many intervals were found where local transverse ion heating was consistent with the observations.

  14. Wave-induced bedload transport - a study of the southern Baltic coastal zone

    NASA Astrophysics Data System (ADS)

    Dudkowska, Aleksandra; Gic-Grusza, Gabriela

    2017-03-01

    The wave-induced bedload transport and spatial distribution of its magnitude in the southern Baltic coastal zone of Poland are estimated. The vicinity of Lubiatowo was selected as a representative part of the Polish coast. It was assumed that transport is a function of shear stress; alternative approaches, based on force balances and discharge relationships, were not considered in the present study. Four models were studied and compared over a wide range of bottom shear stress and wind-wave conditions. The set of models comprises classic theories that assume a simplified influence of turbulence on sediment transport (e.g., advocated by authors such as Du Boys, Meyer-Peter and Müller, Ribberink, Engelund and Hansen). It is shown that these models allow to estimate transport comparable to measured values under similar environmental conditions. A united general model for bedload transport is proposed, and a set of maps of wave bedload transport for various wind conditions in the study area is presented.

  15. Complex permeability structure of a fault zone crosscutting a sequence of sandstones and shales and its influence on hydraulic head distribution

    NASA Astrophysics Data System (ADS)

    Cilona, A.; Aydin, A.; Hazelton, G.

    2013-12-01

    Characterization of the structural architecture of a 5 km-long, N40°E-striking fault zone provides new insights for the interpretation of hydraulic heads measured across and along the fault. Of interest is the contaminant transport across a portion of the Upper Cretaceous Chatsworth Formation, a 1400 m-thick turbidite sequence of sandstones and shales exposed in the Simi Hills, south California. Local bedding consistently dips about 20° to 30° to NW. Participating hydrogeologists monitor the local groundwater system by means of numerous boreholes used to define the 3D distribution of the groundwater table around the fault. Sixty hydraulic head measurements consistently show differences of 10s of meters, except for a small area. In this presentation, we propose a link between this distribution and the fault zone architecture. Despite an apparent linear morphological trend, the fault is made up of at least three distinct segments named here as northern, central and southern segments. Key aspects of the fault zone architecture have been delineated at two sites. The first is an outcrop of the central segment and the second is a borehole intersecting the northern segment at depth. The first site shows the fault zone juxtaposing sandstones against shales. Here the fault zone consists of a 13 meter-wide fault rock including a highly deformed sliver of sandstone on the northwestern side. In the sandstone, shear offset was resolved along N42°E striking and SE dipping fracture surfaces localized within a 40 cm thick strand. Here the central core of the fault zone is 8 m-wide and contains mostly shale characterized by highly diffuse deformation. It shows a complex texture overprinted by N30°E-striking carbonate veins. At the southeastern edge of the fault zone exposure, a shale unit dipping 50° NW towards the fault zone provides the key information that the shale unit was incorporated into the fault zone in a manner consistent with shale smearing. At the second site, a

  16. Subwavelength and directional control of flexural waves in zone-folding induced topological plates

    NASA Astrophysics Data System (ADS)

    Chaunsali, Rajesh; Chen, Chun-Wei; Yang, Jinkyu

    2018-02-01

    Inspired by the quantum spin Hall effect shown by topological insulators, we propose a plate structure that can be used to demonstrate the pseudospin Hall effect for flexural waves. The system consists of a thin plate with periodically arranged resonators mounted on its top surface. We extend a technique based on the plane-wave expansion method to identify a double Dirac cone emerging due to the zone-folding in frequency band structures. This particular design allows us to move the double Dirac cone to a lower frequency than the resonating frequency of local resonators. We then manipulate the pattern of local resonators to open subwavelength Bragg band gaps that are topologically distinct. Building on this method, we verify numerically that a waveguide at an interface between two topologically distinct resonating plate structures can be used for guiding low-frequency, spin-dependent one-way flexural waves along a desired path with bends.

  17. Wave evolution in the marginal ice zone - Model predictions and comparisons with on-site and remote data

    NASA Technical Reports Server (NTRS)

    Liu, A. K.; Holt, B.; Vachon, P. W.

    1989-01-01

    The ocean-wave dispersion relation and viscous attenuation by a sea ice cover were studied for waves in the marginal ice zone (MIZ). The Labrador ice margin experiment (Limex), conducted off the east coast of Newfoundland, Canada in March 1987, provided aircraft SAR, wave buoy, and ice property data. Based on the wave number spectrum from SAR data, the concurrent wave frequency spectrum from ocean buoy data, and accelerometer data on the ice during Limex '87, the dispersion relation has been derived and compared with the model. Accelerometers were deployed at the ice edge and into the ice pack. Data from the accelerometers were used to estimate wave energy attenuation rates and compared with the model. The model-data comparisons are reasonably good for the ice conditions observed during Limex' 87.

  18. Evidence of Enhanced Subrosion in a Fault Zone and Characterization of Hazard Zones with Elastic Parameters derived from SH-wave reflection Seismics and VSP

    NASA Astrophysics Data System (ADS)

    Wadas, S. H.; Tanner, D. C.; Tschache, S.; Polom, U.; Krawczyk, C. M.

    2017-12-01

    Subrosion, the dissolution of soluble rocks, e.g., sulfate, salt, or carbonate, requires unsaturated water and fluid pathways that enable the water to flow through the subsurface and generate cavities. Over time, different structures can occur that depend on, e.g., rock solubility, flow rate, and overburden type. The two main structures are sinkholes and depressions. To analyze the link between faults, groundwater flow, and soluble rocks, and to determine parameters that are useful to characterize hazard zones, several shear-wave (SH) reflection seismic profiles were surveyed in Thuringia in Germany, where Permian sulfate rocks and salt subcrop close to the surface. From the analysis of the seismic sections we conclude that areas affected by tectonic deformation phases are prone to enhanced subrosion. The deformation of fault blocks leads to the generation of a damage zone with a dense fracture network. This increases the rock permeability and thus serves as a fluid pathway for, e.g., artesian-confined groundwater. The more complex the fault geometry and the more interaction between faults, the more fractures are generated, e.g., in a strike slip-fault zone. The faults also act as barriers for horizontal groundwater flow perpendicular to the fault surfaces and as conduits for groundwater flow along the fault strike. In addition, seismic velocity anomalies and attenuation of seismic waves are observed. Low velocities <200 m/s and high attenuation may indicate areas affected by subrosion. Other parameters that characterize the underground stability are the shear modulus and the Vp/Vs ratio. The data revealed zones of low shear modulus <100 MPa and high Vp/Vs ratio >2.5, which probably indicate unstable areas due to subrosion. Structural analysis of S-wave seismics is a valuable tool to detect near-surface faults in order to determine whether or not an area is prone to subrosion. The recognition of even small fault blocks can help to better understand the hydrodynamic

  19. Low-grazing angle laser scans of foreshore topography, swash and inner surf-zone wave heights, and mean water level: validation and storm response

    NASA Astrophysics Data System (ADS)

    Brodie, K. L.; McNinch, J. E.; Forte, M.; Slocum, R.

    2010-12-01

    Accurately predicting beach evolution during storms requires models that correctly parameterize wave runup and inner surf-zone processes, the principle drivers of sediment exchange between the beach and surf-zone. Previous studies that aimed at measuring wave runup and swash zone water levels have been restricted to analyzing water-elevation time series of (1) the shoreward-most swash excursion using video imaging or near-bed resistance wires, or (2) the free water surface at a particular location on the foreshore using pressure sensors. These data are often compared with wave forcing parameters in deeper water as well as with beach topography observed at finite intervals throughout the time series to identify links between foreshore evolution, wave spectra, and water level variations. These approaches have lead to numerous parameterizations and empirical equations for wave runup but have difficulty providing adequate data to quantify and understand short-term spatial and temporal variations in foreshore evolution. As a result, modeling shoreline response and changes in sub-aerial beach volume during storms remains a substantial challenge. Here, we demonstrate a novel technique in which a terrestrial laser scanner is used to continuously measure beach and foreshore topography as well as water elevation (and wave height) in the swash and inner surf-zone during storms. The terrestrial laser scanner is mounted 2-m above the dune crest at the Field Research Facility in Duck, NC in line with cross-shore wave gauges located at 2-m, 3-m, 5-m, 6-m, and 8-m of water depth. The laser is automated to collect hourly, two-dimensional, 20-minute time series of data along a narrow swath in addition to an hourly three-dimensional laser scan of beach and dune topography +/- 250m alongshore from the laser. Low grazing-angle laser scans are found to reflect off of the surface of the water, providing spatially (e.g. dx <= 0.1 m) and temporally (e.g. dt = 3Hz) dense elevation data of

  20. Identification of the Low-velocity Zone Beneath the Northern Taiwan by the P-wave Delays Analysis

    NASA Astrophysics Data System (ADS)

    Chang, C. W.; Che-Min, L.

    2017-12-01

    Taipei City, the capital of Taiwan, located in northern Taiwan is near to the Tatun volcano group and the Shanchiao fault which is an active fault. This region is a complex tectonic environment. The Tatun volcano group is seen as a dormant volcano. Recently, the location of the magma reservoir of the Tatun volcano was discussed again. However, the volume and the location of the magma reservoir are still unclear. There are several seismic networks operated by different institutions around Taipei and Tatun volcano. In this study, we combined the data of these networks to analysis the P-wave arrival times for clarifying the magma reservoir. The events with hypocenters are deeper than 100 km and the local magnitude (ML) are larger than 4.0 were collected to analysis. Our results show that the stations could be separated into three groups by the slope of the P-wave arrival time. They are distributed at the western of the Basin edge, the Jin-Shan Plain areal and the Taipei Basin, respectively. When the epicenter distance of the different stations is the same, the P-wave arrival time of the stations on the west side of the basin edge will be 0.3 0.5 seconds later than that in the Taipei Basin, and the stations on the Jin-Shan Plain will be 0.1 0.4 seconds later than in the Taipei Basin. The slope of the P-wave arrival time in 3 groups is very different, indicating that the low-velocity zone is existed in shallow crustal beneath of these areas. However, the low-velocity zone can be connected to the magma reservoir of the Tatun volcano group or submarine volcano of Keelung Island or not? It can be discussed the correlation between the magma reservoir and the low-velocity zone by more events collected.

  1. Spatial characterization of innervation zones under electrically elicited M-wave.

    PubMed

    Zhang, C; Peng, Y; Li, S; Zhou, P; Munoz, A; Tang, D; Zhang, Y

    2016-08-01

    The three dimensional (3D) innervation zone (IZ) imaging approach (3DIZI) has been developed in our group to localize the IZ of a particular motor unit (MU) from its motor unit action potentials decomposed from high-density surface electromyography (EMG) recordings. In this study, the developed 3DIZI approach was combined with electrical stimulation to investigate global distributions of IZs in muscles from electrically elicited M-wave recordings. Electrical stimulations were applied to the musculocutaneous nerve to activate supramaximal muscle response of the biceps brachii in one healthy subject, and high-density (128 channels) surface EMG signals of the biceps brachii muscles were recorded. The 3DIZI approach was then employed to image the IZ distribution of IZs in the 3D space of the biceps brachii. The performance of the M-wave based 3DIZI approach was evaluated with different stimulation intensities. Results show that the reconstructed IZs under supramaximal stimulation are spatially distributed in the center region of muscle belly which is consistent with previous studies. With sub-maximal stimulation intensity, the imaged IZ centers became more proximally and deeply located. The proposed M-wave based 3DIZI approach demonstrated its capability of imaging global distribution of IZs in muscles, which provide valuable information for clinical applications such as guiding botulinum toxin injection in treating muscle spasticity.

  2. Incident wave, infragravity wave, and non-linear low-frequency bore evolution across fringing coral reefs

    NASA Astrophysics Data System (ADS)

    Storlazzi, C. D.; Griffioen, D.; Cheriton, O. M.

    2016-12-01

    Coral reefs have been shown to significantly attenuate incident wave energy and thus provide protection for 100s of millions of people globally. To better constrain wave dynamics and wave-driven water levels over fringing coral reefs, a 4-month deployment of wave and tide gauges was conducted across two shore-normal transects on Roi-Namur Island and two transects on Kwajalein Island in the Republic of the Marshall Islands. At all locations, although incident wave (periods <25 s) heights were an order of magnitude greater than infragravity wave (periods > 250 s) heights on the outer reef flat just inshore of the zone of wave breaking, the infragravity wave heights generally equaled the incident wave heights by the middle of the reef flat and exceeded the incident wave heights on the inner reef flat by the shoreline. The infragravity waves generally were asymmetric, positively skewed, bore-like forms with incident-band waves riding the infragravity wave crest at the head of the bore; these wave packets have similar structure to high-frequency internal waves on an internal wave bore. Bore height was shown to scale with water depth, offshore wave height, and offshore wave period. For a given tidal elevation, with increasing offshore wave heights, such bores occurred more frequently on the middle reef flat, whereas they occurred less frequently on the inner reef flat. Skewed, asymmetric waves are known to drive large gradients in velocity and shear stress that can transport material onshore. Thus, a better understanding of these low-frequency, energetic bores on reef flats is critical to forecasting how coral reef-lined coasts may respond to sea-level rise and climate change.

  3. Limited Retinacular Vessel Damage Does Not Compromise Femoral Head Perfusion During Hip Arthroscopy - Can the Vascular Safe Zone be Extended?

    PubMed Central

    Nawabi, Danyal H.; Bedi, Asheesh; Kelly, Bryan T.

    2015-01-01

    Objectives: The utilization of hip arthroscopy for FAI is on the rise. Hip arthroscopy has been shown to be safe to the blood supply of the femoral head when performing femoral osteochondroplasty. There are no reports of avascular necrosis of the femoral head after hip arthroscopy from cohort studies. Arthroscopic safe zones have been identified, based on femoral head vascularity studies, that extend from the lateral synovial fold anterior to 12 o clock to the medial synovial fold at 6 o clock. However, advances in technique have allowed for treatment of more extensile posterolateral cam deformities with both arthroscopic and open approaches, and may therefore place a portion of the retinacular vessels at risk for injury. The purpose of this study was to quantify the effect of an extended arthroscopic femoroplasty on femoral head vascularity. We hypothesized that limited retinacular vessel damage by extending a cam resection posterior to 12 o clock would not cause a significant reduction in femoral head perfusion. Methods: Ten fresh-frozen cadaveric specimens with an intact pelvis and bilateral femurs were used. The mean patient age was 66 years (range, 64-69). Each pelvis was randomized to either the Standard Resection (SR) or Wide Resection (WR) group. In the SR group, bone was resected with a motorized burr from the lateral synovial fold at 12 o clock to the medial synovial fold, at a depth of 10mm. In the WR group, bone was resected as in the SR group but was then extended posterolaterally to 11 o clock, damaging the intervening vessels. For each pelvis, one hip was the experimental side and the contralateral hip served as a matched control. Arteriotomy was performed and the medial femoral circumflex artery origin was cannulated. After unilateral arthroscopic resection, all specimens underwent a gadolinium-enhanced MRI with a validated, quantitative protocol. A CT scan was then performed to confirm the zones of osseous resection. Contrast enhancement on MRI was

  4. Small Effect of Hydration on Elastic Wave Velocities of Ringwoodite in Earth's Transition Zone

    NASA Astrophysics Data System (ADS)

    Schulze, K.; Marquardt, H.; Boffa Ballaran, T.; Kurnosov, A.; Kawazoe, T.; Koch-Müller, M.

    2017-12-01

    Ringwoodite can incorporate significant amounts of hydrogen as OH-defects into its crystal structure. The measurement of 1.4 wt.% H20 in a natural ringwoodite diamond inclusion (Pearson et al. 2014) showed that hydrous ringwoodite can exist in the Earth's mantle. Since ringwoodite is considered to be the major phase in the mantle between 520 and 660 km depth it likely plays an important role for Earth's deep water cycle and the mantle water budget. Previous experimental work has shown that hydration reduces seismic wave velocities in ringwoodite, motivating attempts to map the hydration state of the mantle using seismic wave speed variations as depicted by seismic tomography. However, large uncertainties on the actual effects at transition zone pressures and temperatures remain. A major difficulty is the comparability of studies with different experimental setups and pressure- and temperature conditions. Here, we present results from a comparative elasticity study designed to quantify the effects of hydration on the seismic wave velocities of ringwoodite in Earth's transition zone. Focused ion beam cut single-crystals of four samples of either Fo90 or Fo100 ringwoodite with hydration states between 0.21 - 1.71 wt.% H2O were loaded in the pressure chamber of one diamond-anvil cell to ensure identical experimental conditions. Single-crystal Brillouin Spectroscopy and X-ray diffraction measurements were performed at room temperature to a pressure of 22 GPa. Additional experiments at high pressure and temperatures up to 500 K were performed. Our data collected at low pressures show a significant reduction of elastic wave velocities with hydration, consistent with previous work. However, in contrast to previous inferences, our results indicate that pressure significantly reduces the effect of hydration. Based on the outcome of our work, the redution in aggregate velocities caused by 1 wt.% H2O becomes smaller than 1% in ringwoodite at pressures equivalent to the Earth

  5. Long Wave Runup in Asymmetric Bays and in Fjords With Two Separate Heads

    NASA Astrophysics Data System (ADS)

    Raz, Amir; Nicolsky, Dmitry; Rybkin, Alexei; Pelinovsky, Efim

    2018-03-01

    Modeling of tsunamis in glacial fjords prompts us to evaluate applicability of the cross-sectionally averaged nonlinear shallow water equations to model propagation and runup of long waves in asymmetrical bays and also in fjords with two heads. We utilize the Tuck-Hwang transformation, initially introduced for the plane beaches and currently generalized for bays with arbitrary cross section, to transform the nonlinear governing equations into a linear equation. The solution of the linearized equation describing the runup at the shore line is computed by taking into account the incident wave at the toe of the last sloping segment. We verify our predictions against direct numerical simulation of the 2-D shallow water equations and show that our solution is valid both for bays with an asymmetric L-shaped cross section, and for fjords with two heads—bays with a W-shaped cross section.

  6. Evidence for self-refraction in a convergence zone: NPE (Nonlinear progressive wave equation) model results

    NASA Technical Reports Server (NTRS)

    Mcdonald, B. Edward; Plante, Daniel R.

    1989-01-01

    The nonlinear progressive wave equation (NPE) model was developed by the Naval Ocean Research and Development Activity during 1982 to 1987 to study nonlinear effects in long range oceanic propagation of finite amplitude acoustic waves, including weak shocks. The NPE model was applied to propagation of a generic shock wave (initial condition provided by Sandia Division 1533) in a few illustrative environments. The following consequences of nonlinearity are seen by comparing linear and nonlinear NPE results: (1) a decrease in shock strength versus range (a well-known result of entropy increases at the shock front); (2) an increase in the convergence zone range; and (3) a vertical meandering of the energy path about the corresponding linear ray path. Items (2) and (3) are manifestations of self-refraction.

  7. Importance of Antecedent Beach and Surf-Zone Morphology to Wave Runup Predictions

    DTIC Science & Technology

    2016-10-01

    position on the dune, the laser reflects well off of the water surface when foam is present (blue dots, Figure 1B). Maximum range of measurement...depends upon the amount of breaking and foam present in the surf-zone at any given time, but rarely exceeds 150 m for this laser scanner. Drawbacks to...determined by reverse-shoaling data from the FRF’s 11 m Acoustic Wave and Current (AWAC) profiler to deep water values. Local water levels (tide and surge

  8. [Characteristics of Waves Generated Beneath the Solar Convection Zone by Penetrative Overshoot

    NASA Technical Reports Server (NTRS)

    Julien, Keith

    2000-01-01

    The goal of this project was to theoretically and numerically characterize the waves generated beneath the solar convection zone by penetrative overshoot. Three dimensional model simulations were designed to isolate the effects of rotation and shear. In order to overcome the numerically imposed limitations of finite Reynolds numbers (Re) below solar values, series of simulations were designed to elucidate the Reynolds-number dependence (hoped to exhibit mathematically simple scaling on Re) so that one could cautiously extrapolate to solar values.

  9. Anisotropy in subduction zones: Insights from new source side S wave splitting measurements from India

    NASA Astrophysics Data System (ADS)

    Roy, Sunil K.; Kumar, M. Ravi; Davuluri, Srinagesh

    2017-08-01

    This study presents 106 splitting and 40 null measurements of source side anisotropy in subduction zones, utilizing direct S waves registered at two stations sited on the Indian continent, which show null shear wave splitting measurements for SKS phases. Our results suggest that trench-parallel anisotropy is dominant beneath the Philippines, Mariana, Izu-Bonin, and edge of the Java slab, while plate motion-parallel anisotropy is observed beneath the Solomon, Aegean, Japan, and Java slabs. Results from Kuril and Aleutian regions reveal trench-oblique anisotropy. We chose to interpret these observations primarily in terms of mantle flow beneath a subduction zone. While the two-dimensional (2-D) slab entrained flow model offers a simple explanation for trench-normal fast polarization azimuths (FPA), the trench-parallel FPA can be reconciled by extension due to slab rollback. The model that invokes age of the subducting lithosphere can explain anisotropy in the subslab, derived from rays recorded at the updip stations. However, when downdip stations are used, contributions from the slab and supraslab need to be considered. In Japan, anisotropy in the subslab mantle shallower than 300 km might be associated with trench-parallel mantle flow resulting in the alignment of FPA in the same direction. Anisotropy in the deeper part, above the transition zone, is probably associated with 2-D flow resulting in trench-normal FPA. Anisotropy in the Mariana Trench might be associated with trench-parallel mantle flow in the supraslab region, with similar deformation in the upper mantle and the transition zone.

  10. Numerical modeling of nonlinear modulation of coda wave interferometry in a multiple scattering medium with the presence of a localized micro-cracked zone

    NASA Astrophysics Data System (ADS)

    Chen, Guangzhi; Pageot, Damien; Legland, Jean-Baptiste; Abraham, Odile; Chekroun, Mathieu; Tournat, Vincent

    2018-04-01

    The spectral element method is used to perform a parametric sensitivity study of the nonlinear coda wave interferometry (NCWI) method in a homogeneous sample with localized damage [1]. The influence of a strong pump wave on a localized nonlinear damage zone is modeled as modifications to the elastic properties of an effective damage zone (EDZ), depending on the pump wave amplitude. The local change of the elastic modulus and the attenuation coefficient have been shown to vary linearly with respect to the excitation amplitude of the pump wave as in previous experimental studies of Zhang et al. [2]. In this study, the boundary conditions of the cracks, i.e. clapping effects is taken into account in the modeling of the damaged zone. The EDZ is then modeled with random cracks of random orientations, new parametric studies are established to model the pump wave influence with two new parameters: the change of the crack length and the crack density. The numerical results reported constitute another step towards quantification and forecasting of the nonlinear acoustic response of a cracked material, which proves to be necessary for quantitative non-destructive evaluation.

  11. Wave propagation in the marginal ice zone - Model predictions and comparisons with buoy and synthetic aperture radar data

    NASA Technical Reports Server (NTRS)

    Liu, Antony K.; Holt, Benjamin; Vachon, Paris W.

    1991-01-01

    Ocean wave dispersion relation and viscous attenuation by a sea ice cover are studied for waves propagating into the marginal ice zone (MIZ). The Labrador ice margin experiment (LIMEX), conducted on the MIZ off the east coast of Newfoundland, Canada in March 1987, provided aircraft SAR imagery, ice property and wave buoy data. Wave energy attenuation rates are estimated from SAR data and the ice motion package data that were deployed at the ice edge and into the ice pack, and compared with a model. It is shown that the model data comparisons are quite good for the ice conditions observed during LIMEX 1987.

  12. Coherent Waves in Seismic Researches

    NASA Astrophysics Data System (ADS)

    Emanov, A.; Seleznev, V. S.

    2013-05-01

    Development of digital processing algorithms of seismic wave fields for the purpose of useful event picking to study environment and other objects is the basis for the establishment of new seismic techniques. In the submitted paper a fundamental property of seismic wave field coherence is used. The authors extended conception of coherence types of observed wave fields and devised a technique of coherent component selection from observed wave field. Time coherence and space coherence are widely known. In this paper conception "parameter coherence" has been added. The parameter by which wave field is coherent can be the most manifold. The reason is that the wave field is a multivariate process described by a set of parameters. Coherence in the first place means independence of linear connection in wave field of parameter. In seismic wave fields, recorded in confined space, in building-blocks and stratified mediums time coherent standing waves are formed. In prospecting seismology at observation systems with multiple overlapping head waves are coherent by parallel correlation course or, in other words, by one measurement on generalized plane of observation system. For detail prospecting seismology at observation systems with multiple overlapping on basis of coherence property by one measurement of area algorithms have been developed, permitting seismic records to be converted to head wave time sections which have neither reflected nor other types of waves. Conversion in time section is executed on any specified observation base. Energy storage of head waves relative to noise on basis of multiplicity of observation system is realized within area of head wave recording. Conversion on base below the area of wave tracking is performed with lack of signal/noise ratio relative to maximum of this ratio, fit to observation system. Construction of head wave time section and dynamic plots a basis of automatic processing have been developed, similar to CDP procedure in method of

  13. On the influence of reflection over a rhythmic swash zone on surf zone dynamics

    NASA Astrophysics Data System (ADS)

    Almar, Rafael; Nicolae Lerma, Alexandre; Castelle, Bruno; Scott, Timothy

    2018-05-01

    The reflection of incident gravity waves over an irregular swash zone morphology and the resulting influence on surf zone dynamics remains mostly unexplored. The wave-phase resolving SWASH model is applied to investigate this feedback using realistic low-tide terraced beach morphology with well-developed beach cusps. The rhythmic reflection generates a standing wave that mimics a subharmonic edge wave, from the superimposition of incident and two-dimensional reflected waves. This mechanism is enhanced by shore-normal, narrow-banded waves in both direction and frequency. Our study suggests that wave reflection over steep beaches could be a mechanism for the development of rhythmic morphological features such as beach cusps and rip currents.

  14. Mortality during a Large-Scale Heat Wave by Place, Demographic Group, Internal and External Causes of Death, and Building Climate Zone

    PubMed Central

    Joe, Lauren; Hoshiko, Sumi; Dobraca, Dina; Jackson, Rebecca; Smorodinsky, Svetlana; Smith, Daniel; Harnly, Martha

    2016-01-01

    Mortality increases during periods of elevated heat. Identification of vulnerable subgroups by demographics, causes of death, and geographic regions, including deaths occurring at home, is needed to inform public health prevention efforts. We calculated mortality relative risks (RRs) and excess deaths associated with a large-scale California heat wave in 2006, comparing deaths during the heat wave with reference days. For total (all-place) and at-home mortality, we examined risks by demographic factors, internal and external causes of death, and building climate zones. During the heat wave, 582 excess deaths occurred, a 5% increase over expected (RR = 1.05, 95% confidence interval (CI) 1.03–1.08). Sixty-six percent of excess deaths were at home (RR = 1.12, CI 1.07–1.16). Total mortality risk was higher among those aged 35–44 years than ≥65, and among Hispanics than whites. Deaths from external causes increased more sharply (RR = 1.18, CI 1.10–1.27) than from internal causes (RR = 1.04, CI 1.02–1.07). Geographically, risk varied by building climate zone; the highest risks of at-home death occurred in the northernmost coastal zone (RR = 1.58, CI 1.01–2.48) and the southernmost zone of California’s Central Valley (RR = 1.43, CI 1.21–1.68). Heat wave mortality risk varied across subpopulations, and some patterns of vulnerability differed from those previously identified. Public health efforts should also address at-home mortality, non-elderly adults, external causes, and at-risk geographic regions. PMID:27005646

  15. Mortality during a Large-Scale Heat Wave by Place, Demographic Group, Internal and External Causes of Death, and Building Climate Zone.

    PubMed

    Joe, Lauren; Hoshiko, Sumi; Dobraca, Dina; Jackson, Rebecca; Smorodinsky, Svetlana; Smith, Daniel; Harnly, Martha

    2016-03-09

    Mortality increases during periods of elevated heat. Identification of vulnerable subgroups by demographics, causes of death, and geographic regions, including deaths occurring at home, is needed to inform public health prevention efforts. We calculated mortality relative risks (RRs) and excess deaths associated with a large-scale California heat wave in 2006, comparing deaths during the heat wave with reference days. For total (all-place) and at-home mortality, we examined risks by demographic factors, internal and external causes of death, and building climate zones. During the heat wave, 582 excess deaths occurred, a 5% increase over expected (RR = 1.05, 95% confidence interval (CI) 1.03-1.08). Sixty-six percent of excess deaths were at home (RR = 1.12, CI 1.07-1.16). Total mortality risk was higher among those aged 35-44 years than ≥ 65, and among Hispanics than whites. Deaths from external causes increased more sharply (RR = 1.18, CI 1.10-1.27) than from internal causes (RR = 1.04, CI 1.02-1.07). Geographically, risk varied by building climate zone; the highest risks of at-home death occurred in the northernmost coastal zone (RR = 1.58, CI 1.01-2.48) and the southernmost zone of California's Central Valley (RR = 1.43, CI 1.21-1.68). Heat wave mortality risk varied across subpopulations, and some patterns of vulnerability differed from those previously identified. Public health efforts should also address at-home mortality, non-elderly adults, external causes, and at-risk geographic regions.

  16. Influence of gravity for optimal head positions in the treatment of head injury patients.

    PubMed

    Li, Xiaogai; von Holst, Hans; Kleiven, Svein

    2011-10-01

    Brain edema is a major neurological complication of traumatic brain injury (TBI), commonly including a pathologically increased intracranial pressure (ICP) associated with poor outcome. In this study, gravitational force is suggested to have a significant impact on the pressure of the edema zone in the brain tissue and the objective of the study was to investigate the significance of head position on edema at the posterior part of the brain using a finite element (FE) model. A detailed FE model including the meninges, brain tissue and a fully connected cerebrospinal fluid (CSF) system was used in this study. Brain tissue was modelled as a poroelastic material consisting of an elastic solid skeleton composed of neurons and neuroglia, permeated by interstitial fluid. The effect of head positions (supine and prone position) due to gravity was investigated for a localized brain edema at the posterior part of the brain. The water content increment at the edema zone remained nearly identical for both positions. However, the interstitial fluid pressure (IFP) inside the edema zone decreased around 15% by having the head in a prone position compared with a supine position. The decrease of IFP inside the edema zone by changing patient position from supine to prone has the potential to alleviate the damage to central nervous system nerves. These observations indicate that considering the patient's head position during intensive care and at rehabilitation might be of importance to the treatment of edematous regions in TBI patients.

  17. Making the most of CZ seismics: Improving shallow critical zone characterization using surface-wave analysis

    NASA Astrophysics Data System (ADS)

    Pasquet, S.; Wang, W.; Holbrook, W. S.; Bodet, L.; Carr, B.; Flinchum, B. A.

    2017-12-01

    Estimating porosity and saturation in the shallow subsurface over large lateral scales is vitally important for understanding the development and evolution of the Critical Zone (CZ). Because elastic properties (P- and S-wave velocities) are particularly sensitive to porosity and saturation, seismic methods (in combination with petrophysical models) are effective tools for mapping CZ architecture and processes. While many studies employ P-wave refraction methods, fewer use the surface waves that are typically also recorded in those same surveys. Here we show the value of exploiting surface waves to extract supplementary shear-wave velocity (Vs) information in the CZ. We use a new, user-friendly, open-source MATLAB-based package (SWIP) to invert surface-wave data and estimate lateral variations of Vs in the CZ. Results from synthetics show that this approach enables the resolution of physical property variations in the upper 10-15 m below the surface with lateral scales of about 5 m - a vast improvement compared to P-wave tomography alone. A field example at a Yellowstone hydrothermal system also demonstrates the benefits of including Vs in the petrophysical models to estimate not only porosity but also saturation, thus highlighting subsurface gas pathways. In light of these results, we strongly suggest that surface-wave analysis should become a standard approach in CZ seismic surveys.

  18. Real-time simulation of combined short-wave and long-wave infrared vision on a head-up display

    NASA Astrophysics Data System (ADS)

    Peinecke, Niklas; Schmerwitz, Sven

    2014-05-01

    Landing under adverse weather conditions can be challenging, even if the airfields are well known to the pilots. This is true for civil as well as military aviation. Within the scope of this paper we concentrate especially on fog conditions. The work has been conducted within the project ALICIA. ALICIA is a research and development project co-funded by European Commission under the Seventh Framework Programme. ALICIA aims at developing new and scalable cockpit applications which can extend operations of aircraft in degraded conditions: All Conditions Operations. One of the systems developed is a head-up display that can display a generated symbology together with a raster-mode infrared image. We will detail how we implemented a real-time enabled simulation of a combined short-wave and long-wave infrared image for landing. A major challenge was to integrate several already existing simulation solutions, e.g., for visual simulation and sensors with the required data-bases. For the simulations DLRs in-house sensor simulation framework F3S was used, together with a commercially available airport model that had to be heavily modified in order to provide realistic infrared data. Special effort was invested for a realistic impression of runway lighting under foggy conditions. We will present results and sketch further improvements for future simulations.

  19. Structure of the Cascadia Subduction Zone Imaged Using Surface Wave Tomography

    NASA Astrophysics Data System (ADS)

    Schaeffer, A. J.; Audet, P.

    2017-12-01

    Studies of the complete structure of the Cascadia subduction zone from the ridge to the arc have historically been limited by the lack of offshore ocean bottom seismograph (OBS) infrastructure. On land, numerous dense seismic deployments have illuminated detailed structures and dynamics associated with the interaction between the subducting oceanic plate and the overriding continental plate, including cycling of fluids, serpentinization of the overlying forearc mantle wedge, and the location of the upper surface of the Juan de Fuca plate as it subducts beneath the Pacific Northwest. In the last half-decade, the Cascadia Initiative (CI), along with Neptune (ONC) and several other OBS initiatives, have instrumented both the continental shelf and abyssal plains off shore of the Cascadia subduction zone, facilitating the construction of a complete picture of the subduction zone from ridge to trench and volcanic arc. In this study, we present a preliminary azimuthally anisotropic surface-wave phase-velocity based model of the complete system, capturing both the young, unaltered Juan de Fuca plate from the ridge, to its alteration as it enters the subduction zone, in addition to the overlying continent. This model is constructed from a combination of ambient noise cross-correlations and teleseismic two station interferometry, and combines together concurrently running offshore OBS and onshore stations. We furthermore perform a number of representative 1D depth inversions for shear velocity to categorize the pristine oceanic, subducted oceanic, and continental crust and lithospheric structure. In the future the dispersion dataset will be jointly inverted with receiver functions to constrain a 3D shear-velocity model of the complete region.

  20. Mapping Deep Low Velocity Zones in Alaskan Arctic Coastal Permafrost using Seismic Surface Waves

    NASA Astrophysics Data System (ADS)

    Dou, S.; Ajo Franklin, J. B.; Dreger, D. S.

    2012-12-01

    Surface Waves (MASW) suggests the existence of pronounced low shear wave velocity zones that span the depth range of 2 - 30 meters; this zone has shear velocity values comparable to partially thawed soils. Such features coincide with previous findings of very low electrical resistivity structure (as low as ~10 Ohm*m at some locations) from measurements obtained in the first NGEE-Arctic geophysical field campaign (conducted in the week of September 24 - October 1, 2011). These low shear velocity zones are likely representative of regions with high unfrozen water content and thus have important implications on the rate of microbial activity and the vulnerability of deep permafrost carbon pools. Analysis of this dataset required development of a novel inversion approach based on waveform inversion. The existence of multiple closely spaced Rayleigh wave modes made traditional inversion based on mode picking virtually impossible; As a result, we selected a direct misfit evaluation based on comparing dispersion images in the phase velocity/frequency domain. The misfit function was optimized using a global search algorithm, in this case Huyer and Neumaier's Multi Coordinate Search algorithm (MCS). This combination of MCS and waveform misfit allowed recovery of the low velocity region despite the existence of closely spaced modes.

  1. Linear excitation of the trapped waves by an incident wave

    NASA Astrophysics Data System (ADS)

    Postacioglu, Nazmi; Sinan Özeren, M.

    2016-04-01

    The excitation of the trapped waves by coastal events such as landslides has been extensively studied. The events in the open sea have in general larger magnitude. However the incident waves produced by these events in the open sea can only excite the the trapped waves through no linearity if the isobaths are straight lines that are in parallel with the coastline. We will show that the imperfections of the coastline can couple the incident and trapped waves using only linear processes. The Coriolis force is neglected in this work . Accordingly the trapped waves are consequence of uneven bathimetry. In the bathimetry we consider, the sea is divided into zones of constant depth and the boundaries between the zones are a family of hyperbolas. The boundary conditions between the zones will lead to an integral equation for the source distribution on the boundaries. The solution will contain both radiating and trapped waves. The trapped waves pose a serious threat for the coastal communities as they can travel long distances along the coastline without losing their energy through geometrical spreading.

  2. Anatomic fit of six different radial head plates: comparison of precontoured low-profile radial head plates.

    PubMed

    Burkhart, Klaus Josef; Nowak, Tobias E; Kim, Yoon-Joo; Rommens, Pol M; Müller, Lars P

    2011-04-01

    Bulky implants may lead to symptomatic soft tissue irritation after open reduction and internal fixation of radial head and neck fractures. The purpose of our study was to compare the anatomic fit of precontoured radial head plates. We stripped 22 embalmed human cadaveric radiuses of soft tissues. We investigated 6 radial head plates: (1) the Medartis radial head buttress plate (MBP), (2) the Medartis radial head rim plate (MRP), (3) the Synthes radial neck plate (SNP), (4) the Synthes radial head plate (SHP), (5) the Acumed radial head plate (AHP), and (6) the Wright radial head plate (WHP). Each plate was applied to each radial head at the place of best fit within the safe zone. We tested 4 parameters of anatomic fit: (1) plate-to-bone distance, (2) plate contact judged by 3 different observers, (3) pin-subchondral zone distance, and (4) plate-to-bone contact after adjustment of the plates. The MBP and MRP showed the lowest profile by objective measurements, the SNP and AHP had a moderate profile, and the SHP and WHP demonstrated the bulkiest profile. The subjective assessments also demonstrated the best fit for the MBP, a good fit for the SNP, a moderate fit for the MRP and AHP, and a poor fit for the SHP and WHP. The MBP, MRP, and AHP could always provide pin-subchondral zone contact, unlike the SHP, SNP, and WHP. After bending, significant improvement of plate-to-bone distance could only be seen for the MBP, MRP, and WHP. The ranking among plates remained the same except for the WHP, which showed a significantly lower plate-to-bone distance than the SHP. Currently available radial head implants are heterogeneous. The MBP and MRP showed the lowest profile and best anatomic fit. Owing to the complex radial head anatomy, to date there is no one radial head plate that perfectly fits all radial heads. Conformance of existing plates to the radial head and neck is not perfect. Careful plate selection and modification, when necessary, may minimize interference of this

  3. Photon migration through fetal head in utero using continuous wave, near infrared spectroscopy: development and evaluation of experimental and numerical models

    NASA Astrophysics Data System (ADS)

    Vishnoi, Gargi; Hielscher, Andreas H.; Ramanujam, Nirmala; Chance, Britton

    2000-04-01

    In this work experimental tissue phantoms and numerical models were developed to estimate photon migration through the fetal head in utero. The tissue phantoms incorporate a fetal head within an amniotic fluid sac surrounded by a maternal tissue layer. A continuous wave, dual-wavelength ((lambda) equals 760 and 850 nm) spectrometer was employed to make near-infrared measurements on the tissue phantoms for various source-detector separations, fetal-head positions, and fetal-head optical properties. In addition, numerical simulations of photon propagation were performed with finite-difference algorithms that provide solutions to the equation of radiative transfer as well as the diffusion equation. The simulations were compared with measurements on tissue phantoms to determine the best numerical model to describe photon migration through the fetal head in utero. Evaluation of the results indicates that tissue phantoms in which the contact between fetal head and uterine wall is uniform best simulates the fetal head in utero for near-term pregnancies. Furthermore, we found that maximum sensitivity to the head can be achieved if the source of the probe is positioned directly above the fetal head. By optimizing the source-detector separation, this signal originating from photons that have traveled through the fetal head can drastically be increased.

  4. Diffracted and head waves associated with waves on nonseparable surfaces

    NASA Technical Reports Server (NTRS)

    Barger, Raymond L.

    1992-01-01

    A theory is presented for computing waves radiated from waves on a smooth surface. With the assumption that attention of the surface wave is due only to radiation and not to dissipation in the surface material, the radiation coefficient is derived in terms of the attenuation factor. The excitation coefficient is determined by the reciprocity condition. Formulas for the shape and the spreading of the radiated wave are derived, and some sample calculations are presented. An investigation of resonant phase matching for nonseparable surfaces is presented with a sample calculation. A discussion of how such calculations might be related to resonant frequencies of nonseparable thin shell structures is included. A description is given of nonseparable surfaces that can be modeled in the vector that facilitates use of the appropriate formulas of differential geometry.

  5. Wave groupiness variations in the nearshore

    USGS Publications Warehouse

    List, J.H.

    1991-01-01

    This paper proposes a new definition of the groupiness factor, GF, based on the envelope of the incident-wave time series. It is shown that an envelope-based GF has several important advantages over the SIWEH-based groupiness factor, including objective criteria for determining the accuracy of the envelope function and well-defined numerical limits. Using this new GF, the variability of incident wave groupiness in the field is examined both temporally, in unbroken waves at a fixed location, and spatially, in a cross-shore array through the surf zone. Contrary to previous studies using the SIWEH-based GF, results suggest that incident wave groupiness may not be an independent parameter in unbroken waves; through a wide range of spectral shapes, from swell to storm waves, the groupiness did not vary significantly. As expected, the groupiness decreases rapidly as waves break through the surf zone, although significant wave height variability persists even through a saturated surf zone. The source of this inner surf zone groupiness is not identified; however, this observation implies that models of long wave generation must account for nonsteady radiation stress gradients landward of some narrow zone near the mean breakpoint. ?? 1991.

  6. Wave interference: mechanics of the standing wave component and the illusion of "which way" information

    NASA Astrophysics Data System (ADS)

    Hudgins, W. R.; Meulenberg, A.; Penland, R. F.

    2015-09-01

    Two adjacent coherent light beams, 180° out of phase and traveling on adjacent, parallel paths, remain visibly separated by the null (dark) zone from their mutual interference pattern as they merge. Each half of the pattern can be traced to one of the beams. Does such an experiment provide both "which way" and momentum knowledge? To answer this question, we demonstrate, by examining behavior of wave momentum and energy in a medium, that interfering waves interact. Central to the mechanism of interference is a standing wave component resulting from the combination of coherent waves. We show the mathematics for the formation of the standing wave component and for wave momentum involved in the waves' interaction. In water and in open coaxial cable, we observe that standing waves form cells bounded "reflection zones" where wave momentum from adjacent cells is reversed, confining oscillating energy to each cell. Applying principles observed in standing waves in media to the standing wave component of interfering light beams, we identify dark (null) regions to be the reflection zones. Each part of the interference pattern is affected by interactions between other parts, obscuring "which-way" information. We demonstrated physical interaction experimentally using two beams interfering slightly with one dark zone between them. Blocking one beam "downstream" from the interference region removed the null zone and allowed the remaining beam to evolve to a footprint of a single beam.

  7. Evolution of a Directional Wave Spectrum in a 3D Marginal Ice Zone with Random Floe Size Distribution

    NASA Astrophysics Data System (ADS)

    Montiel, F.; Squire, V. A.

    2013-12-01

    A new ocean wave/sea-ice interaction model is proposed that simulates how a directional wave spectrum evolves as it travels through a realistic marginal ice zone (MIZ), where wave/ice dynamics are entirely governed by coherent conservative wave scattering effects. Field experiments conducted by Wadhams et al. (1986) in the Greenland Sea generated important data on wave attenuation in the MIZ and, particularly, on whether the wave spectrum spreads directionally or collimates with distance from the ice edge. The data suggest that angular isotropy, arising from multiple scattering by ice floes, occurs close to the edge and thenceforth dominates wave propagation throughout the MIZ. Although several attempts have been made to replicate this finding theoretically, including by the use of numerical models, none have confronted this problem in a 3D MIZ with fully randomised floe distribution properties. We construct such a model by subdividing the discontinuous ice cover into adjacent infinite slabs of finite width parallel to the ice edge. Each slab contains an arbitrary (but finite) number of circular ice floes with randomly distributed properties. Ice floes are modeled as thin elastic plates with uniform thickness and finite draught. We consider a directional wave spectrum with harmonic time dependence incident on the MIZ from the open ocean, defined as a continuous superposition of plane waves traveling at different angles. The scattering problem within each slab is then solved using Graf's interaction theory for an arbitrary incident directional plane wave spectrum. Using an appropriate integral representation of the Hankel function of the first kind (see Cincotti et al., 1993), we map the outgoing circular wave field from each floe on the slab boundaries into a directional spectrum of plane waves, which characterizes the slab reflected and transmitted fields. Discretizing the angular spectrum, we can obtain a scattering matrix for each slab. Standard recursive

  8. Propagation of acoustic shock waves between parallel rigid boundaries and into shadow zones

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

    Desjouy, C., E-mail: cyril.desjouy@gmail.com; Ollivier, S.; Dragna, D.

    2015-10-28

    The study of acoustic shock propagation in complex environments is of great interest for urban acoustics, but also for source localization, an underlying problematic in military applications. To give a better understanding of the phenomenon taking place during the propagation of acoustic shocks, laboratory-scale experiments and numerical simulations were performed to study the propagation of weak shock waves between parallel rigid boundaries, and into shadow zones created by corners. In particular, this work focuses on the study of the local interactions taking place between incident, reflected, and diffracted waves according to the geometry in both regular or irregular – alsomore » called Von Neumann – regimes of reflection. In this latter case, an irregular reflection can lead to the formation of a Mach stem that can modify the spatial distribution of the acoustic pressure. Short duration acoustic shock waves were produced by a 20 kilovolts electric spark source and a schlieren optical method was used to visualize the incident shockfront and the reflection/diffraction patterns. Experimental results are compared to numerical simulations based on the high-order finite difference solution of the two dimensional Navier-Stokes equations.« less

  9. Constraining the hydration of the subducting Nazca plate beneath Northern Chile using subduction zone guided waves

    NASA Astrophysics Data System (ADS)

    Garth, Tom; Rietbrock, Andreas

    2017-09-01

    Guided wave dispersion is observed from earthquakes at 180-280 km depth recorded at stations in the fore-arc of Northern Chile, where the 44 Ma Nazca plate subducts beneath South America. Characteristic P-wave dispersion is observed at several stations in the Chilean fore-arc with high frequency energy (>5 Hz) arriving up to 3 s after low frequency (<2 Hz) arrivals. This dispersion has been attributed to low velocity structure within the subducting Nazca plate which acts as a waveguide, retaining and delaying high frequency energy. Full waveform modelling shows that the single LVL proposed by previous studies does not produce the first motion dispersion observed at multiple stations, or the extended P-wave coda observed in arrivals from intermediate depth events within the Nazca plate. These signals can however be accurately accounted for if dipping low velocity fault zones are included within the subducting lithospheric mantle. A grid search over possible LVL and faults zone parameters (width, velocity contrast and separation distance) was carried out to constrain the best fitting model parameters. Our results imply that fault zone structures of 0.5-1.0 km thickness, and 5-10 km spacing, consistent with observations at the outer rise are present within the subducted slab at intermediate depths. We propose that these low velocity fault zone structures represent the hydrated structure within the lithospheric mantle. They may be formed initially by normal faults at the outer rise, which act as a pathway for fluids to penetrate the deeper slab due to the bending and unbending stresses within the subducting plate. Our observations suggest that the lithospheric mantle is 5-15% serpentinised, and therefore may transport approximately 13-42 Tg/Myr of water per meter of arc. The guided wave observations also suggest that a thin LVL (∼1 km thick) interpreted as un-eclogitised subducted oceanic crust persists to depths of at least 220 km. Comparison of the inferred seismic

  10. Quantitative analysis of seismic trapped waves in the rupture zone of the Landers, 1992, California earthquake: Evidence for a shallow trapping structure

    NASA Astrophysics Data System (ADS)

    Peng, Z.; Ben-Zion, Y.; Michael, A. J.; Zhu, L.

    2002-12-01

    Waveform modeling of seismic fault zone (FZ) trapped waves has been claimed to provide a high resolution imaging of FZ structure at seismogenic depth. We analyze quantitatively a waveform data set generated by 238 Landers aftershocks recorded by a portable seismic array (Lee, 1999). The array consists of 33 three-component L-22 seismometers, 22 of which on a line crossing the surface rupture zone of the mainshock. A subset of 93 aftershocks were also recorded by the Southern California Seismic Network, while the other events were recorded only by the FZ array. We locate the latter subset of events with a "grid-search relocation method" using accurately picked P and S arrival times, a half-space velocity model, and back-azimuth adjustment to correct the effect of low velocity FZ material on phase arrivals. Next we determine the quality of FZ trapped wave generation from the ratio of trapped waves to S-wave energy for stations relatively close to and far from the FZ. Energy ratios exceeding 4, between 2 and 4, and less than 2, are assigned quality A, B, and C of trapped wave generation. We find that about 70% of nearby events with S-P time less than 2 sec, including many clearly off the fault, generate FZ trapped waves with quality A or B. This distribution is in marked contrast with previous claims that trapped waves at Landers are generated only by sources close to or inside the fault zone (Li et al., 1994, 2000). The existence of trapped waves due to sources outside the Landers rupture zone indicates that the generating structure is shallow, as demonstrated in recent 3D calculations of wave propagation in irregular FZ structures (Fohrmann et al., 2002). The time difference between the S arrivals and trapped wave group does not grow systematically with increasing source-receiver distance along the fault, in agreement with the above conclusion. The dispersion of trapped waves at Landers is rather weak, again suggesting a short propagation distance inside the low

  11. Physical linkages between an offshore canyon and surf zone morphologic change

    NASA Astrophysics Data System (ADS)

    Hansen, Jeff E.; Raubenheimer, Britt; Elgar, Steve; List, Jeffrey H.; Lippmann, Thomas C.

    2017-04-01

    The causes of surf zone morphologic changes observed along a sandy beach onshore of a submarine canyon were investigated using field observations and a numerical model (Delft3D/SWAN). Numerically simulated morphologic changes using four different sediment transport formulae reproduce the temporal and spatial patterns of net cross-shore integrated (between 0 and 6.5 m water depths) accretion and erosion observed in a ˜300 m alongshore region, a few hundred meters from the canyon head. The observations and simulations indicate that the accretion or erosion results from converging or diverging alongshore currents driven primarily by breaking waves and alongshore pressure gradients. The location of convergence or divergence depends on the direction of the offshore waves that refract over the canyon, suggesting that bathymetric features on the inner shelf can have first-order effects on short-term nearshore morphologic change.

  12. Gas exchange in the ice zone: the role of small waves and big animals

    NASA Astrophysics Data System (ADS)

    Loose, B.; Takahashi, A.; Bigdeli, A.

    2016-12-01

    The balance of air-sea gas exchange and net biological carbon fixation determine the transport and transformation of carbon dioxide and methane in the ocean. Air-sea gas exchange is mostly driven by upper ocean physics, but biology can also play a role. In the open ocean, gas exchange increases proportionate to the square of wind speed. When sea ice is present, this dependence breaks down in part because breaking waves and air bubble entrainment are damped out by interactions between sea ice and the wave field. At the same time, sea ice motions, formation, melt, and even sea ice-associated organisms can act to introduce turbulence and air bubbles into the upper ocean, thereby enhancing air-sea gas exchange. We take advantage of the knowledge advances of upper ocean physics including bubble dynamics to formulate a model for air-sea gas exchange in the sea ice zone. Here, we use the model to examine the role of small-scale waves and diving animals that trap air for insulation, including penguins, seals and polar bears. We compare these processes to existing parameterizations of wave and bubble dynamics in the open ocean, to observe how sea ice both mitigates and locally enhances air-sea gas transfer.

  13. Wave Dissipation over Nearshore Beach Morphology: Insights from High-Resolution LIDAR Observations and the SWASH Wave Model

    NASA Astrophysics Data System (ADS)

    Mulligan, R. P.; Gomes, E.; McNinch, J.; Brodie, K. L.

    2016-02-01

    Numerical modelling of the nearshore zone can be computationally intensive due to the complexity of wave breaking, and the need for high temporal and spatial resolution. In this study we apply the SWASH non-hydrostatic wave-flow model that phase-resolves the free surface and fluid motions in the water column at high resolution. The model is forced using observed directional energy spectra, and results are compared to wave observations during moderate storm events. Observations are collected outside the surf zone using acoustic wave and currents sensors, and inside the surf zone over a 100 m transect using high-resolution LIDAR measurements of the sea surface from a sensor mounted on a tower on the beach dune at the Field Research Facility in Duck, NC. The model is applied to four cases with different wave conditions and bathymetry, and used to predict the spatial variability in wave breaking, and correlation between energy dissipation and morphologic features. Model results compare well with observations of spectral evolution outside the surf zone, and with the remotely sensed observations of wave transformation inside the surf zone. The results indicate the importance of nearshore bars, rip-channels, and larger features (major scour depression under the pier following large waves from Hurricane Irene) on the location of wave breaking and alongshore variability in wave energy dissipation.

  14. Acoustic Gravity Waves Generated by an Oscillating Ice Sheet in Arctic Zone

    NASA Astrophysics Data System (ADS)

    Abdolali, A.; Kadri, U.; Kirby, J. T., Jr.

    2016-12-01

    ., 2015, Depth-integrated equation for hydro-acoustic waves with bottom damping, Journal of Fluid Mechanics, 766, R1 doi:10.1017/jfm.2015.37 Kadri, U., 2016, Generation of Hydroacoustic Waves by an Oscillating Ice Block in Arctic Zones, Advances in Acoustics and Vibration. 2016. doi:10.1155/2016/8076108

  15. Comparison of tracer methods to quantify hydrodynamic exchange within the hyporheic zone

    NASA Astrophysics Data System (ADS)

    Engelhardt, I.; Piepenbrink, M.; Trauth, N.; Stadler, S.; Kludt, C.; Schulz, M.; Schüth, C.; Ternes, T. A.

    2011-03-01

    SummaryHydrodynamic exchange between surface-water and groundwater was studied at a river located within the Rhine Valley in Germany. Piezometric pressure heads and environmental tracers such as temperature, stable isotopes, chloride, X-ray contrast media, and artificial sweetener were investigated within the hyporheic zone and river water plume. Vertical profiles of environmental tracers were collected using multi-level wells within the neutral up-gradient zone, beneath the river bed, and within the horizontal proximal and distal down-gradient zone. Infiltration velocities were calculated from pressure heads, temperature fluctuations and gradients. The amount of river water within groundwater was estimated from vertical profiles of chloride, stable isotopes, and persistent pharmaceuticals. Profiles of stable isotopes and chloride reveal the existence of down-welling within the shallow hyporheic zone that is generated by river bed irregularities. Due to down-welling an above-average migration of river water into the hyporheic zone establishes even under upward hydraulic pressure gradients. The investigated environmental tracers could not distinctively display short-time-infiltration velocities representative for flood waves, while average infiltration velocities calculated over several months are uniform displayed. Based on vertical temperature profiles the down-gradient migration of the river water plume could be observed even after long periods of effluent conditions and over a distance of 200 m from the river bank. X-ray contrast media and artificial sweeteners were observed in high concentrations within the proximal zone, but were not detected at a distance of 200 m from the river bank. Using temperature as environmental tracer within the hyporheic zone may result in overestimating the migration of pollutants within the river water plume as the process of natural attenuation will be neglected. Furthermore, temperature was not able to display the effect of down

  16. Scenario based tsunami wave height estimation towards hazard evaluation for the Hellenic coastline and examples of extreme inundation zones in South Aegean

    NASA Astrophysics Data System (ADS)

    Melis, Nikolaos S.; Barberopoulou, Aggeliki; Frentzos, Elias; Krassanakis, Vassilios

    2016-04-01

    A scenario based methodology for tsunami hazard assessment is used, by incorporating earthquake sources with the potential to produce extreme tsunamis (measured through their capacity to cause maximum wave height and inundation extent). In the present study we follow a two phase approach. In the first phase, existing earthquake hazard zoning in the greater Aegean region is used to derive representative maximum expected earthquake magnitude events, with realistic seismotectonic source characteristics, and of greatest tsunamigenic potential within each zone. By stacking the scenario produced maximum wave heights a global maximum map is constructed for the entire Hellenic coastline, corresponding to all expected extreme offshore earthquake sources. Further evaluation of the produced coastline categories based on the maximum expected wave heights emphasizes the tsunami hazard in selected coastal zones with important functions (i.e. touristic crowded zones, industrial zones, airports, power plants etc). Owing to its proximity to the Hellenic Arc, many urban centres and being a popular tourist destination, Crete Island and the South Aegean region are given a top priority to define extreme inundation zoning. In the second phase, a set of four large coastal cities (Kalamata, Chania, Heraklion and Rethymno), important for tsunami hazard, due i.e. to the crowded beaches during the summer season or industrial facilities, are explored towards preparedness and resilience for tsunami hazard in Greece. To simulate tsunamis in the Aegean region (generation, propagation and runup) the MOST - ComMIT NOAA code was used. High resolution DEMs for bathymetry and topography were joined via an interface, specifically developed for the inundation maps in this study and with similar products in mind. For the examples explored in the present study, we used 5m resolution for the topography and 30m resolution for the bathymetry, respectively. Although this study can be considered as

  17. 46 CFR 76.23-5 - Zoning.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Manual Sprinkling System, Details § 76.23-5 Zoning. (a) Separate zones may be used for each deck, and on any particular... that the end sprinkler heads of both adjoining zones will cover the identical area. Table 76.23-5(b...

  18. 46 CFR 76.23-5 - Zoning.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Manual Sprinkling System, Details § 76.23-5 Zoning. (a) Separate zones may be used for each deck, and on any particular... that the end sprinkler heads of both adjoining zones will cover the identical area. Table 76.23-5(b...

  19. 46 CFR 76.23-5 - Zoning.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Manual Sprinkling System, Details § 76.23-5 Zoning. (a) Separate zones may be used for each deck, and on any particular... that the end sprinkler heads of both adjoining zones will cover the identical area. Table 76.23-5(b...

  20. 46 CFR 76.23-5 - Zoning.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Manual Sprinkling System, Details § 76.23-5 Zoning. (a) Separate zones may be used for each deck, and on any particular... that the end sprinkler heads of both adjoining zones will cover the identical area. Table 76.23-5(b...

  1. 46 CFR 76.23-5 - Zoning.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Manual Sprinkling System, Details § 76.23-5 Zoning. (a) Separate zones may be used for each deck, and on any particular... that the end sprinkler heads of both adjoining zones will cover the identical area. Table 76.23-5(b...

  2. Brain Response to Primary Blast Wave Using Validated Finite Element Models of Human Head and Advanced Combat Helmet

    PubMed Central

    Zhang, Liying; Makwana, Rahul; Sharma, Sumit

    2013-01-01

    Blast-induced traumatic brain injury has emerged as a “signature injury” in combat casualty care. Present combat helmets are designed primarily to protect against ballistic and blunt impacts, but the current issue with helmets is protection concerning blasts. In order to delineate the blast wave attenuating capability of the Advanced Combat Helmet (ACH), a finite element (FE) study was undertaken to evaluate the head response against blast loadings with and without helmet using a partially validated FE model of the human head and ACH. Four levels of overpressures (0.27–0.66 MPa) from the Bowen’s lung iso-damage threshold curves were used to simulate blast insults. Effectiveness of the helmet with respect to head orientation was also investigated. The resulting biomechanical responses of the brain to blast threats were compared for human head with and without the helmet. For all Bowen’s cases, the peak intracranial pressures (ICP) in the head ranged from 0.68 to 1.8 MPa in the coup cortical region. ACH was found to mitigate ICP in the head by 10–35%. Helmeted head resulted in 30% lower average peak brain strains and product of strain and strain rate. Among three blast loading directions with ACH, highest reduction in peak ICP (44%) was due to backward blasts whereas the lowest reduction in peak ICP and brain strains was due to forward blast (27%). The biomechanical responses of a human head to primary blast insult exhibited directional sensitivity owing to the different geometry contours and coverage of the helmet construction and asymmetric anatomy of the head. Thus, direction-specific tolerances are needed in helmet design in order to offer omni-directional protection for the human head. The blasts of varying peak overpressures and durations that are believed to produce the same level of lung injury produce different levels of mechanical responses in the brain, and hence “iso-damage” curves for brain injury are likely different than the Bowen

  3. Development of groundwater vulnerability zones in a data-scarce eogenetic karst area using Head-Guided Zonation and particle-tracking simulation methods.

    PubMed

    Klaas, Dua K S Y; Imteaz, Monzur Alam; Arulrajah, Arul

    2017-10-01

    Delineation of groundwater vulnerability zones based on a valid groundwater model is crucial towards an accurate design of management strategies. However, limited data often restrain the development of a robust groundwater model. This study presents a methodology to develop groundwater vulnerability zones in a data-scarce area. The Head-Guided Zonation (HGZ) method was applied on the recharge area of Oemau Spring in Rote Island, Indonesia, which is under potential risk of contamination from rapid land use changes. In this method the model domain is divided into zones of piecewise constant into which the values of subsurface properties are assigned in the parameterisation step. Using reverse particle-tracking simulation on the calibrated and validated groundwater model, the simulation results (travel time and pathline trajectory) were combined with the potential groundwater contamination risk from human activities (land use type and current practice) to develop three vulnerability zones. The corresponding preventive management strategies were proposed to protect the spring from contamination and to ensure provision of safe and good quality water from the spring. Copyright © 2017 Elsevier Ltd. All rights reserved.

  4. High accuracy binary black hole simulations with an extended wave zone

    NASA Astrophysics Data System (ADS)

    Pollney, Denis; Reisswig, Christian; Schnetter, Erik; Dorband, Nils; Diener, Peter

    2011-02-01

    We present results from a new code for binary black hole evolutions using the moving-puncture approach, implementing finite differences in generalized coordinates, and allowing the spacetime to be covered with multiple communicating nonsingular coordinate patches. Here we consider a regular Cartesian near-zone, with adapted spherical grids covering the wave zone. The efficiencies resulting from the use of adapted coordinates allow us to maintain sufficient grid resolution to an artificial outer boundary location which is causally disconnected from the measurement. For the well-studied test case of the inspiral of an equal-mass nonspinning binary (evolved for more than 8 orbits before merger), we determine the phase and amplitude to numerical accuracies better than 0.010% and 0.090% during inspiral, respectively, and 0.003% and 0.153% during merger. The waveforms, including the resolved higher harmonics, are convergent and can be consistently extrapolated to r→∞ throughout the simulation, including the merger and ringdown. Ringdown frequencies for these modes (to (ℓ,m)=(6,6)) match perturbative calculations to within 0.01%, providing a strong confirmation that the remnant settles to a Kerr black hole with irreducible mass Mirr=0.884355±20×10-6 and spin Sf/Mf2=0.686923±10×10-6.

  5. Dependence of shear wave seismoelectrics on soil textures: a numerical study in the vadose zone

    NASA Astrophysics Data System (ADS)

    Zyserman, F. I.; Monachesi, L. B.; Jouniaux, L.

    2017-02-01

    In this work, we study seismoelectric conversions generated in the vadose zone, when this region is traversed by a pure SH wave. We assume that the soil is a 1-D partially saturated lossy porous medium and we use the van Genuchten's constitutive model to describe the water saturation profile. Correspondingly, we extend Pride's formulation to deal with partially saturated media. In order to evaluate the influence of different soil textures we perform a numerical analysis considering, among other relevant properties, the electrokinetic coupling, coseismic responses and interface responses (IRs). We propose new analytical transfer functions for the electric and magnetic field as a function of the water saturation, modifying those of Bordes et al. and Garambois & Dietrich, respectively. Further, we introduce two substantially different saturation-dependent functions into the electrokinetic (EK) coupling linking the poroelastic and the electromagnetic wave equations. The numerical results show that the electric field IRs markedly depend on the soil texture and the chosen EK coupling model, and are several orders of magnitude stronger than the electric field coseismic ones. We also found that the IRs of the water table for the silty and clayey soils are stronger than those for the sandy soils, assuming a non-monotonous saturation dependence of the EK coupling, which takes into account the charged air-water interface. These IRs have been interpreted as the result of the jump in the viscous electric current density at the water table. The amplitude of the IR is obtained using a plane SH wave, neglecting both the spherical spreading and the restriction of its origin to the first Fresnel zone, effects that could lower the predicted values. However, we made an estimation of the expected electric field IR amplitudes detectable in the field by means of the analytical transfer functions, accounting for spherical spreading of the SH seismic waves. This prediction yields a value

  6. Tribocorrosion: Ceramic and Oxidized Zirconium vs Cobalt-Chromium Heads in Total Hip Arthroplasty.

    PubMed

    Tan, Sok Chuen; Lau, Adrian C K; Del Balso, Christopher; Howard, James L; Lanting, Brent A; Teeter, Matthew G

    2016-09-01

    This matched-cohort study aims to compare tribocorrosion between matched ceramic and cobalt-chromium femoral head trunnions and between matched Oxinium and cobalt-chromium femoral head trunnions. Secondary objectives were to investigate whether taper design, depth of trunnion, implantation time, age, body mass index, and gender have an effect on fretting and corrosion. All hip prostheses retrieved between 1999 and 2015 at one center were reviewed, giving a total of 52 ceramic heads. These were matched to a cobalt-chromium cohort according to taper design, head size, neck length, and implantation time. The trunnions were examined by 2 observers using a 4-point scoring technique and scored in 3 zones: apex, middle, and base. The observers were blinded to clinical and manufacturing data where possible. A separate matched-cohort analysis was performed between 8 Oxinium heads and 8 cobalt-chromium heads, which were similarly scored. Ceramic head trunnions demonstrated a lower median fretting and corrosion score at the base zone (P < .001), middle zone (P < .001), and in the combined score (P < .001). Taper design had a significant effect on fretting and corrosion in the apex zone (P = .04) of the ceramic group, as well as the cobalt-chromium group (P = .03). Between Oxinium heads and cobalt-chromium heads, there was no significant difference in the fretting and corrosion score across all 3 zones (base: P = .22; middle: P = .92; and apex: P = .71) and for the combined score (P = .67). This study shows that ceramic head confers an advantage in trunnion fretting and corrosion. Taper design and implantation time were also significant factors for fretting and corrosion. Copyright © 2016 Elsevier Inc. All rights reserved.

  7. Oblique muscle surgery for treatment of nystagmus with head tilt.

    PubMed

    Lueder, Gregg T; Galli, Marlo

    2012-08-01

    Patients with nystagmus may adopt an abnormal head posture if they have a null zone in eccentric gaze. These patients uncommonly present with torticollis due to a null zone when the head is tilted. We describe the results of surgery on the oblique muscles to improve the abnormal head posture in this condition. This was a retrospective review of patients who had head tilts due to null zones of nystagmus. Surgery consisted of an anterior 50% tenectomy of the superior oblique tendon on one side and recession of the inferior oblique muscle to a position 6 mm posterior to the insertion of the inferior rectus muscle on the contralateral side. The patients' clinical histories and outcomes were reviewed. Six patients underwent the procedure. Of these, four had infantile nystagmus syndrome and two were born prematurely and had histories of intraventricular hemorrhages. Five of the patients had previous Kestenbaum surgery that corrected the horizontal component of their abnormal head postures. Age at time of surgery for the head tilt ranged from 3 to 13 years. Postoperative follow-up ranged from 1.5 to 3 years. The preoperative head tilts ranged from 25° to 45° (mean, 39°). The postoperative improvement ranged from 20° to 40° (mean, 28°). One of the patients with a history of intraventricular hemorrhage required additional surgery for strabismus unrelated to nystagmus. Anterior tenectomy of the superior oblique tendon combined with contralateral recession of the inferior oblique muscle improved head tilts related to a null zone of nystagmus. Copyright © 2012 American Association for Pediatric Ophthalmology and Strabismus. Published by Mosby, Inc. All rights reserved.

  8. Features of HF Radio Wave Attenuation in the Midlatitude Ionosphere Near the Skip Zone Boundary

    NASA Astrophysics Data System (ADS)

    Denisenko, P. F.; Skazik, A. I.

    2017-06-01

    We briefly describe the history of studying the decameter radio wave attenuation by different methods in the midlatitude ionosphere. A new method of estimating the attenuation of HF radio waves in the ionospheric F region near the skip zone boundary is presented. This method is based on an analysis of the time structure of the interference field generated by highly stable monochromatic X-mode radio waves at the observation point. The main parameter is the effective electron collision frequency νeff, which allows for all energy losses in the form of equivalent heat loss. The frequency νeff is estimated by matching the assumed (model) and the experimentally observed structures. Model calculations are performed using the geometrical-optics approximation. The spatial attenuation caused by the influence of the medium-scale traveling ionospheric disturbances is taken into account. Spherical shape of the ionosphere and the Earth's magnetic field are roughly allowed for. The results of recording of the level of signals from the RWM (Moscow) station at a frequency of 9.996 MHz at point Rostov are used.

  9. 2D shear-wave ultrasound elastography (SWE) evaluation of ablation zone following radiofrequency ablation of liver lesions: is it more accurate?

    PubMed Central

    Bo, Xiao W; Li, Xiao L; Guo, Le H; Li, Dan D; Liu, Bo J; Wang, Dan; He, Ya P; Xu, Xiao H

    2016-01-01

    Objective: To evaluate the usefulness of two-dimensional quantitative ultrasound shear-wave elastography (2D-SWE) [i.e. virtual touch imaging quantification (VTIQ)] in assessing the ablation zone after radiofrequency ablation (RFA) for ex vivo swine livers. Methods: RFA was performed in 10 pieces of fresh ex vivo swine livers with a T20 electrode needle and 20-W output power. Conventional ultrasound, conventional strain elastography (SE) and VTIQ were performed to depict the ablation zone 0 min, 10 min, 30 min and 60 min after ablation. On VTIQ, the ablation zones were evaluated qualitatively by evaluating the shear-wave velocity (SWV) map and quantitatively by measuring the SWV. The ultrasound, SE and VTIQ results were compared against gross pathological and histopathological specimens. Results: VTIQ SWV maps gave more details about the ablation zone, the central necrotic zone appeared as red, lateral necrotic zone as green and transitional zone as light green, from inner to exterior, while the peripheral unablated liver appeared as blue. Conventional ultrasound and SE, however, only marginally depicted the whole ablation zone. The volumes of the whole ablation zone (central necrotic zone + lateral necrotic zone + transitional zone) and necrotic zone (central necrotic zone + lateral necrotic zone) measured by VTIQ showed excellent correlation (r = 0.915, p < 0.001, and 0.856, p = 0.002, respectively) with those by gross pathological specimen, whereas both conventional ultrasound and SE underestimated the volume of the whole ablation zone. The SWV values of the central necrotic zone, lateral necrotic zone, transitional zone and unablated liver parenchyma were 7.54–8.03 m s−1, 5.13–5.28 m s−1, 3.31–3.53 m s−1 and 2.11–2.21 m s−1, respectively (p < 0.001 for all the comparisons). The SWV value for each ablation zone did not change significantly at different observation times within an hour after RFA

  10. The Effects Of Tides And Waves On Water-Table Elevations In Coastal Zones

    NASA Astrophysics Data System (ADS)

    Turner, Ian L.; Coates, Bruce P.; Acworth, R. Ian

    1996-02-01

    A resurgence of interest in the literature about coastal zones has highlighted the fact that ocean processes can have a significant influence on unconfined coastal aquifers, resulting in a net super-elevation of the water table at the land-ocean boundary to groundwater discharge. This theoretical and experimental notion appears to be less well recognized in the field of groundwater investigation, where it is more usual to assume that the coastal boundary is equivalent to mean sea level. Coastal over-height is due to the ability of a sloping beach face to `fill' (vertical infiltration) at a greater rate than it can `drain' (horizontal seepage). The results of a three-month monitoring of the groundwater profile within a narrow coastal aquifer at New South Wales, Australia, confirms the significance of tide and wave processes to groundwater elevation. The mean height of the water table on the upper beach face was about 1.2 m above mean sea level, rising to 2.0 m during a period of coincident spring tides, storm waves, and rainfall. This elevation was sufficient to temporarily reverse the direction of groundwater flow. Fourier analysis and cross-correlation are used to help distinguish the role of tides in maintaining groundwater super-elevation from the role of storm waves in further raising the coastal water table for periods of two to three days. The results of a simple numerical simulation demonstrate that estimated rates of groundwater discharge at the study site were halved when the effect of tides and waves was incorporated in the definition of the ocean boundary.

  11. Refracted arrival waves in a zone of silence from a finite thickness mixing layer.

    PubMed

    Suzuki, Takao; Lele, Sanjiva K

    2002-02-01

    Refracted arrival waves which propagate in the zone of silence of a finite thickness mixing layer are analyzed using geometrical acoustics in two dimensions. Here, two simplifying assumptions are made: (i) the mean flow field is transversely sheared, and (ii) the mean velocity and temperature profiles approach the free-stream conditions exponentially. Under these assumptions, ray trajectories are analytically solved, and a formula for acoustic pressure amplitude in the far field is derived in the high-frequency limit. This formula is compared with the existing theory based on a vortex sheet corresponding to the low-frequency limit. The analysis covers the dependence on the Mach number as well as on the temperature ratio. The results show that both limits have some qualitative similarities, but the amplitude in the zone of silence at high frequencies is proportional to omega(-1/2), while that at low frequencies is proportional to omega(-3/2), omega being the angular frequency of the source.

  12. Modeling Water Waves with Smoothed Particle Hydrodynamics

    DTIC Science & Technology

    2013-09-30

    SPH Model for Water Waves and Other Free Surface Flows ...Lagrangian nature of SPH allows the modeling of wave breaking, surf zones, ship waves, and wave-structure interaction, where the free surface becomes...proving to be a competent modeling scheme for free surface flows in three dimensions including the complex flows of the surf zone. As the GPU

  13. Role of helmet in the mechanics of shock wave propagation under blast loading conditions.

    PubMed

    Ganpule, S; Gu, L; Alai, A; Chandra, N

    2012-01-01

    The effectiveness of helmets in extenuating the primary shock waves generated by the explosions of improvised explosive devices is not clearly understood. In this work, the role of helmet on the overpressurisation and impulse experienced by the head were examined. The shock wave-head interactions were studied under three different cases: (i) unprotected head, (ii) head with helmet but with varying head-helmet gaps and (iii) head covered with helmet and tightly fitting foam pads. The intensification effect was discussed by examining the shock wave flow pattern and verified with experiments. A helmet with a better protection against shock wave is suggested.

  14. Implementation of the vortex force formalism in the coupled ocean-atmosphere-wave-sediment transport (COAWST) modeling system for inner shelf and surf zone applications

    NASA Astrophysics Data System (ADS)

    Kumar, Nirnimesh; Voulgaris, George; Warner, John C.; Olabarrieta, Maitane

    The coupled ocean-atmosphere-wave-sediment transport modeling system (COAWST) enables simulations that integrate oceanic, atmospheric, wave and morphological processes in the coastal ocean. Within the modeling system, the three-dimensional ocean circulation module (ROMS) is coupled with the wave generation and propagation model (SWAN) to allow full integration of the effect of waves on circulation and vice versa. The existing wave-current coupling component utilizes a depth dependent radiation stress approach. In here we present a new approach that uses the vortex force formalism. The formulation adopted and the various parameterizations used in the model as well as their numerical implementation are presented in detail. The performance of the new system is examined through the presentation of four test cases. These include obliquely incident waves on a synthetic planar beach and a natural barred beach (DUCK' 94); normal incident waves on a nearshore barred morphology with rip channels; and wave-induced mean flows outside the surf zone at the Martha's Vineyard Coastal Observatory (MVCO). Model results from the planar beach case show good agreement with depth-averaged analytical solutions and with theoretical flow structures. Simulation results for the DUCK' 94 experiment agree closely with measured profiles of cross-shore and longshore velocity data from Garcez Faria et al. (1998, 2000). Diagnostic simulations showed that the nonlinear processes of wave roller generation and wave-induced mixing are important for the accurate simulation of surf zone flows. It is further recommended that a more realistic approach for determining the contribution of wave rollers and breaking induced turbulent mixing can be formulated using non-dimensional parameters which are functions of local wave parameters and the beach slope. Dominant terms in the cross-shore momentum balance are found to be the quasi-static pressure gradient and breaking acceleration. In the alongshore direction

  15. Fault Zone Imaging from Correlations of Aftershock Waveforms

    NASA Astrophysics Data System (ADS)

    Hillers, Gregor; Campillo, Michel

    2018-03-01

    We image an active fault zone environment using cross correlations of 154 15 s long 1992 Landers earthquake aftershock seismograms recorded along a line array. A group velocity and phase velocity dispersion analysis of the reconstructed Rayleigh waves and Love waves yields shear wave velocity images of the top 100 m along the 800 m long array that consists of 22 three component stations. Estimates of the position, width, and seismic velocity of a low-velocity zone are in good agreement with the findings of previous fault zone trapped waves studies. Our preferred solution indicates the zone is offset from the surface break to the east, 100-200 m wide, and characterized by a 30% velocity reduction. Imaging in the 2-6 Hz range resolves further a high-velocity body of similar width to the west of the fault break. Symmetry and shape of zero-lag correlation fields or focal spots indicate a frequency and position dependent wavefield composition. At frequencies greater than 4 Hz surface wave propagation dominates, whereas at lower frequencies the correlation field also exhibits signatures of body waves that likely interact with the high-velocity zone. The polarization and late arrival times of coherent wavefronts observed above the low-velocity zone indicate reflections associated with velocity contrasts in the fault zone environment. Our study highlights the utility of the high-frequency correlation wavefield obtained from records of local and regional seismicity. The approach does not depend on knowledge of earthquake source parameters, which suggests the method can return images quickly during aftershock campaigns to guide network updates for optimal coverage of interesting geological features.

  16. Wave-Ice Interaction and the Marginal Ice Zone

    DTIC Science & Technology

    2013-09-30

    concept, using a high-quality attitude and heading reference system ( AHRS ) together with an accurate twin-antennae GPS compass. The instruments logged...the AHRS parameters at 50Hz, together with GPS-derived fixes, heading (accurate to better than 1o) and velocities at 10Hz. The 30MB hourly files

  17. High-resolution imaging of the low velocity layer in Alaskan subduction zone with scattered waves and interferometry

    NASA Astrophysics Data System (ADS)

    Kim, D.; Keranen, K. M.; Abers, G. A.; Kim, Y.; Li, J.; Shillington, D. J.; Brown, L. D.

    2017-12-01

    The physical factors that control the rupture process of great earthquakes at convergent plate boundaries remain incompletely understood. While recent developments in imaging using the teleseismic wavefield have led to marked advances at wavelengths of a couple kilometers to tens of kilometers, higher resolution imaging of the rupture zone would improve the resolution of imaging and thus provide improved parameter estimation, as the teleseismic wavefield is fundamentally limited by its low frequency content. This study compares and evaluates two seismic imaging techniques using the high-frequency signals from teleseismic coda versus earthquake scattered waves to image the subducting Yakutat oceanic plateau in the Alaska subduction zone. We use earthquakes recorded by the MOOS PASSCAL broadband deployment in southern Alaska. In our first method, we select local earthquakes that lie directly beneath and laterally near the recording array for imaging, and extract body wave information via a simple autocorrelation and stacking. Profiles analogous to seismic reflection profile are constructed using the near-vertically travelling waves. In our second method, we compute teleseismic receiver functions within the 0.02-1.0 Hz frequency band. Both results image interfaces that we associate with the subducting oceanic plate in Alaska-Aleutian system, with greater resolution than commonly used methods with teleseismic sources. Structural details from our results can further our understanding of the conditions and materials that characterize the subduction megathrusts, and the techniques can be employed in other regions along the Alaska-Aleutian system and at other convergent margins with suitable seismic arrays.

  18. 46 CFR 76.25-5 - Zoning.

    Code of Federal Regulations, 2014 CFR

    2014-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Automatic Sprinkling System, Details § 76.25-5 Zoning. (a) The automatic sprinkling system shall be divided into separate... more than 250 sprinkler heads. (c) The sprinkling zone may cover more than one deck, in which case, the...

  19. 46 CFR 76.25-5 - Zoning.

    Code of Federal Regulations, 2013 CFR

    2013-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Automatic Sprinkling System, Details § 76.25-5 Zoning. (a) The automatic sprinkling system shall be divided into separate... more than 250 sprinkler heads. (c) The sprinkling zone may cover more than one deck, in which case, the...

  20. 46 CFR 76.25-5 - Zoning.

    Code of Federal Regulations, 2010 CFR

    2010-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Automatic Sprinkling System, Details § 76.25-5 Zoning. (a) The automatic sprinkling system shall be divided into separate... more than 250 sprinkler heads. (c) The sprinkling zone may cover more than one deck, in which case, the...

  1. 46 CFR 76.25-5 - Zoning.

    Code of Federal Regulations, 2012 CFR

    2012-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Automatic Sprinkling System, Details § 76.25-5 Zoning. (a) The automatic sprinkling system shall be divided into separate... more than 250 sprinkler heads. (c) The sprinkling zone may cover more than one deck, in which case, the...

  2. 46 CFR 76.25-5 - Zoning.

    Code of Federal Regulations, 2011 CFR

    2011-10-01

    ..., DEPARTMENT OF HOMELAND SECURITY (CONTINUED) PASSENGER VESSELS FIRE PROTECTION EQUIPMENT Automatic Sprinkling System, Details § 76.25-5 Zoning. (a) The automatic sprinkling system shall be divided into separate... more than 250 sprinkler heads. (c) The sprinkling zone may cover more than one deck, in which case, the...

  3. Diffusion in coastal and harbour zones, effects of Waves,Wind and Currents

    NASA Astrophysics Data System (ADS)

    Diez, M.; Redondo, J. M.

    2009-04-01

    As there are multiple processes at different scales that produce turbulent mixing in the ocean, thus giving a large variation of horizontal eddy diffusivities, we use a direct method to evaluate the influence of different ambient parameters such as wave height and wind on coastal dispersion. Measurements of the diffusivity are made by digital processing of images taken from from video recordings of the sea surface near the coast. The use of image analysis allows to estimate both spatial and temporal characteristics of wave fields, surface circulation and mixing in the surf zone, near Wave breakers and inside Harbours. The study of near-shore dispersion [1], with the added complexity of the interaction between wave fields, longshore currents, turbulence and beach morphology, needs detailed measurements of simple mixing processes to compare the respective influences of forcings at different scales. The measurements include simultaneous time series of waves, currents, wind velocities from the studied area. Cuantitative information from the video images is accomplished using the DigImage video processing system [3], and a frame grabber. The video may be controlled by the computer, allowing, remote control of the processing. Spectral analysis on the images has also used n order to estimate dominant wave periods as well as the dispersion relations of dominant instabilities. The measurements presented here consist mostly on the comarison of difussion coeficients measured by evaluating the spread of blobs of dye (milk) as well as by measuring the separation between different buoys released at the same time. We have used a techniques, developed by Bahia(1997), Diez(1998) and Bezerra(2000)[1-3] to study turbulent diffusion by means of digital processing of images taken from remote sensing and video recordings of the sea surface. The use of image analysis allows to measure variations of several decades in horizontal diffusivity values, the comparison of the diffusivities

  4. 77 FR 31493 - Safety Zones; Fourth of July Fireworks Displays Within the Captain of the Port Charleston Zone, SC

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-05-29

    ... temporary safety zones during Fourth of July Fireworks Displays on certain navigable waterways in Hilton... below. 1. Hilton Head Island, South Carolina. All waters within a 500 yard radius around the barge from... each safety zone. All coordinates are North American Datum 1983. [[Page 31496

  5. Estimating the sound speed of a shallow-water marine sediment from the head wave excited by a low-flying helicopter.

    PubMed

    Bevans, Dieter A; Buckingham, Michael J

    2017-10-01

    The frequency bandwidth of the sound from a light helicopter, such as a Robinson R44, extends from about 13 Hz to 2.5 kHz. As such, the R44 has potential as a low-frequency sound source in underwater acoustics applications. To explore this idea, an experiment was conducted in shallow water off the coast of southern California in which a horizontal line of hydrophones detected the sound of an R44 hovering in an end-fire position relative to the array. Some of the helicopter sound interacted with seabed to excite the head wave in the water column. A theoretical analysis of the sound field in the water column generated by a stationary airborne source leads to an expression for the two-point horizontal coherence function of the head wave, which, apart from frequency, depends only on the sensor separation and the sediment sound speed. By matching the zero crossings of the measured and theoretical horizontal coherence functions, the sound speed in the sediment was recovered and found to take a value of 1682.42 ± 16.20 m/s. This is consistent with the sediment type at the experiment site, which is known from a previous survey to be a fine to very-fine sand.

  6. Implementation of the vortex force formalism in the coupled ocean-atmosphere-wave-sediment transport (COAWST) modeling system for inner shelf and surf zone applications

    USGS Publications Warehouse

    Kumar, Nirnimesh; Voulgaris, George; Warner, John C.; Olabarrieta, Maitane

    2012-01-01

    Model results from the planar beach case show good agreement with depth-averaged analytical solutions and with theoretical flow structures. Simulation results for the DUCK' 94 experiment agree closely with measured profiles of cross-shore and longshore velocity data from and . Diagnostic simulations showed that the nonlinear processes of wave roller generation and wave-induced mixing are important for the accurate simulation of surf zone flows. It is further recommended that a more realistic approach for determining the contribution of wave rollers and breaking induced turbulent mixing can be formulated using non-dimensional parameters which are functions of local wave parameters and the beach slope. Dominant terms in the cross-shore momentum balance are found to be the quasi-static pressure gradient and breaking acceleration. In the alongshore direction, bottom stress, breaking acceleration, horizontal advection and horizontal vortex forces dominate the momentum balance. The simulation results for the bar/rip channel morphology case clearly show the ability of the modeling system to reproduce horizontal and vertical circulation patterns similar to those found in laboratory studies and to numerical simulations using the radiation stress representation. The vortex force term is found to be more important at locations where strong flow vorticity interacts with the wave-induced Stokes flow field. Outside the surf zone, the three-dimensional model simulations of wave-induced flows for non-breaking waves closely agree with flow observations from MVCO, with the vertical structure of the simulated flow varying as a function of the vertical viscosity as demonstrated by Lentz et al. (2008).

  7. Shear-wave splitting in Quaternary sediments: Neotectonic implications in the central New Madrid seismic zone

    USGS Publications Warehouse

    Harris, J.B.

    1996-01-01

    Determining the extent and location of surface/near-surface structural deformation in the New Madrid seismic zone (NMSZ) is very important for evaluating earthquake hazards. A shallow shear-wave splitting experiment, located near the crest of the Lake County uplift (LCU) in the central NMSZ, shows the presence of near-surface azimuthal anisotropy believed to be associated with neotectonic deformation. A shallow fourcomponent data set, recorded using a hammer and mass source, displayed abundant shallow reflection energy on records made with orthogonal source-receiver orientations, an indicator of shear-wave splitting. Following rotation of the data matrix by 40??, the S1 and S2 sections (principal components of the data matrix) were aligned with the natural coordinate system at orientations of N35??W and N55??E, respectively. A dynamic mis-tie of 8 ms at a two-way traveltime of 375 ms produced an average azimuthal anisotropy of ???2% between the target reflector (top of Quaternary gravel at a depth of 35 m) and the surface. Based on the shear-wave polarization data, two explanations for the azimuthal anisotropy in the study area are (1) fractures/cracks aligned in response to near-surface tensional stress produced by uplift of the LCU, and (2) faults/fractures oriented parallel to the Kentucky Bend scarp, a recently identified surface deformation feature believed to be associated with contemporary seismicity in the central NMSZ. In addition to increased seismic resolution by the use of shear-wave methods in unconsolidated, water-saturated sediments, measurement of near-surface directional polarizations, produced by shear-wave splitting, may provide valuable information for identifying neotectonic deformation and evaluating associated earthquake hazards.

  8. Planktonic Subsidies to Surf-Zone and Intertidal Communities

    NASA Astrophysics Data System (ADS)

    Morgan, Steven G.; Shanks, Alan L.; MacMahan, Jamie H.; Reniers, Ad J. H. M.; Feddersen, Falk

    2018-01-01

    Plankton are transported onshore, providing subsidies of food and new recruits to surf-zone and intertidal communities. The transport of plankton to the surf zone is influenced by wind, wave, and tidal forcing, and whether they enter the surf zone depends on alongshore variation in surf-zone hydrodynamics caused by the interaction of breaking waves with coastal morphology. Areas with gently sloping shores and wide surf zones typically have orders-of-magnitude-higher concentrations of plankton in the surf zone and dense larval settlement in intertidal communities because of the presence of bathymetric rip currents, which are absent in areas with steep shores and narrow surf zones. These striking differences in subsidies have profound consequences; areas with greater subsidies support more productive surf-zone communities and possibly more productive rocky intertidal communities. Recognition of the importance of spatial subsidies for rocky community dynamics has recently advanced ecological theory, and incorporating surf-zone hydrodynamics would be an especially fruitful line of investigation.

  9. On the interaction of small-scale linear waves with nonlinear solitary waves

    NASA Astrophysics Data System (ADS)

    Xu, Chengzhu; Stastna, Marek

    2017-04-01

    In the study of environmental and geophysical fluid flows, linear wave theory is well developed and its application has been considered for phenomena of various length and time scales. However, due to the nonlinear nature of fluid flows, in many cases results predicted by linear theory do not agree with observations. One of such cases is internal wave dynamics. While small-amplitude wave motion may be approximated by linear theory, large amplitude waves tend to be solitary-like. In some cases, when the wave is highly nonlinear, even weakly nonlinear theories fail to predict the wave properties correctly. We study the interaction of small-scale linear waves with nonlinear solitary waves using highly accurate pseudo spectral simulations that begin with a fully nonlinear solitary wave and a train of small-amplitude waves initialized from linear waves. The solitary wave then interacts with the linear waves through either an overtaking collision or a head-on collision. During the collision, there is a net energy transfer from the linear wave train to the solitary wave, resulting in an increase in the kinetic energy carried by the solitary wave and a phase shift of the solitary wave with respect to a freely propagating solitary wave. At the same time the linear waves are greatly reduced in amplitude. The percentage of energy transferred depends primarily on the wavelength of the linear waves. We found that after one full collision cycle, the longest waves may retain as much as 90% of the kinetic energy they had initially, while the shortest waves lose almost all of their initial energy. We also found that a head-on collision is more efficient in destroying the linear waves than an overtaking collision. On the other hand, the initial amplitude of the linear waves has very little impact on the percentage of energy that can be transferred to the solitary wave. Because of the nonlinearity of the solitary wave, these results provide us some insight into wave-mean flow

  10. Mapping of Crustal Anisotropy in the New Madrid Seismic Zone with Shear Wave Splitting

    NASA Astrophysics Data System (ADS)

    Martin, P.; Arroucau, P.; Vlahovic, G.

    2013-12-01

    Crustal anisotropy in the New Madrid seismic zone (NMSZ) is investigated by analyzing shear wave splitting measurements from local earthquake data. For the initial data set, the Center for Earthquake Research and Information (CERI) provided over 3000 events, along with 900 seismograms recorded by the Portable Array for Numerical Data Acquisition (PANDA) network. Data reduction led to a final data set of 168 and 43 useable events from the CERI and PANDA data, respectively. From this, 186 pairs of measurements were produced from the CERI data set as well as 49 from the PANDA data set, by means of the automated shear wave splitting measurement program MFAST. Results from this study identified two dominant fast polarization directions, striking NE-SW and WNW-ESE. These are interpreted to be due to stress aligned microcracks in the upper crust. The NE-SW polarization direction is consistent with the maximum horizontal stress orientation of the region and has previously been observed in the NMSZ, while the WNW-ESE polarization direction has not. Path normalized time delays from this study range from 1-33 ms/km for the CERI network data, and 2-31 ms/km for the PANDA data, giving a range of estimated differential shear wave anisotropy between 1% and 8%, with the majority of large path normalized time delays (>20 ms/km) located along the Reelfoot fault segment. The estimated differential shear wave anisotropy values from this study are higher than those previously determined in the region, and are attributed to high crack densities and high pore fluid pressures, which agree with previous results from local earthquake tomography and microseismic swarm analysis in the NMSZ.

  11. An Asymptotic and Stochastic Theory for the Effects of Surface Gravity Waves on Currents and Infragravity Waves

    NASA Astrophysics Data System (ADS)

    McWilliams, J. C.; Lane, E.; Melville, K.; Restrepo, J.; Sullivan, P.

    2004-12-01

    Oceanic surface gravity waves are approximately irrotational, weakly nonlinear, and conservative, and they have a much shorter time scale than oceanic currents and longer waves (e.g., infragravity waves) --- except where the primary surface waves break. This provides a framework for an asymptotic theory, based on separation of time (and space) scales, of wave-averaged effects associated with the conservative primary wave dynamics combined with a stochastic representation of the momentum transfer and induced mixing associated with non-conservative wave breaking. Such a theory requires only modest information about the primary wave field from measurements or operational model forecasts and thus avoids the enormous burden of calculating the waves on their intrinsically small space and time scales. For the conservative effects, the result is a vortex force associated with the primary wave's Stokes drift; a wave-averaged Bernoulli head and sea-level set-up; and an incremental material advection by the Stokes drift. This can be compared to the "radiation stress" formalism of Longuet-Higgins, Stewart, and Hasselmann; it is shown to be a preferable representation since the radiation stress is trivial at its apparent leading order. For the non-conservative breaking effects, a population of stochastic impulses is added to the current and infragravity momentum equations with distribution functions taken from measurements. In offshore wind-wave equilibria, these impulses replace the conventional surface wind stress and cause significant differences in the surface boundary layer currents and entrainment rate, particularly when acting in combination with the conservative vortex force. In the surf zone, where breaking associated with shoaling removes nearly all of the primary wave momentum and energy, the stochastic forcing plays an analogous role as the widely used nearshore radiation stress parameterizations. This talk describes the theoretical framework and presents some

  12. Near surface structure of the North Anatolian Fault Zone near 30°E from Rayleigh and Love wave tomography using ambient seismic noise.

    NASA Astrophysics Data System (ADS)

    Taylor, G.; Rost, S.; Houseman, G. A.; Hillers, G.

    2017-12-01

    By utilising short period surface waves present in the noise field, we can construct images of shallow structure in the Earth's upper crust: a depth-range that is usually poorly resolved in earthquake tomography. Here, we use data from a dense seismic array (Dense Array for Northern Anatolia - DANA) deployed across the North Anatolian Fault Zone (NAFZ) in the source region of the 1999 magnitude 7.6 Izmit earthquake in western Turkey. The NAFZ is a major strike-slip system that extends 1200 km across northern Turkey and continues to pose a high level of seismic hazard, in particular to the mega-city of Istanbul. We obtain maps of group velocity variation using surface wave tomography applied to short period (1- 6 s) Rayleigh and Love waves to construct high-resolution images of SV and SH-wave velocity in the upper 5 km of a 70 km x 35 km region centred on the eastern end of the fault segment that ruptured in the 1999 Izmit earthquake. The average Rayleigh wave group velocities in the region vary between 1.8 km/s at 1.5 s period, to 2.2 km/s at 6 s period. The NAFZ bifurcates into northern and southern strands in this region; both are active but only the northern strand ruptured in the 1999 event. The signatures of both the northern and southern branches of the NAFZ are clearly associated with strong gradients in seismic velocity that also denote the boundaries of major tectonic units. This observation implies that the fault zone exploits the pre-existing structure of the Intra-Pontide suture zone. To the north of the NAFZ, we observe low S-wave velocities ( 2.0 km/s) associated with the unconsolidated sediments of the Adapazari basin, and blocks of weathered terrigenous clastic sediments. To the south of the northern branch of the NAFZ in the Armutlu block, we detect higher velocities ( 2.9 km/s) associated with a shallow crystalline basement, in particular a block of metamorphosed schists and marbles that bound the northern branch of the NAFZ.

  13. Hydraulic head applications of flow logs in the study of heterogeneous aquifers

    USGS Publications Warehouse

    Paillet, Frederick L.

    2001-01-01

    Permeability profiles derived from high-resolution flow logs in heterogeneous aquifers provide a limited sample of the most permeable beds or fractures determining the hydraulic properties of those aquifers. This paper demonstrates that flow logs can also be used to infer the large-scale properties of aquifers surrounding boreholes. The analysis is based on the interpretation of the hydraulic head values estimated from the flow log analysis. Pairs of quasi-steady flow profiles obtained under ambient conditions and while either pumping or injecting are used to estimate the hydraulic head in each water-producing zone. Although the analysis yields localized estimates of transmissivity for a few water-producing zones, the hydraulic head estimates apply to the farfield aquifers to which these zones are connected. The hydraulic head data are combined with information from other sources to identify the large-scale structure of heterogeneous aquifers. More complicated cross-borehole flow experiments are used to characterize the pattern of connection between large-scale aquifer units inferred from the hydraulic head estimates. The interpretation of hydraulic heads in situ under steady and transient conditions is illustrated by several case studies, including an example with heterogeneous permeable beds in an unconsolidated aquifer, and four examples with heterogeneous distributions of bedding planes and/or fractures in bedrock aquifers.

  14. Modeling ocean wave propagation under sea ice covers

    NASA Astrophysics Data System (ADS)

    Zhao, Xin; Shen, Hayley H.; Cheng, Sukun

    2015-02-01

    Operational ocean wave models need to work globally, yet current ocean wave models can only treat ice-covered regions crudely. The purpose of this paper is to provide a brief overview of ice effects on wave propagation and different research methodology used in studying these effects. Based on its proximity to land or sea, sea ice can be classified as: landfast ice zone, shear zone, and the marginal ice zone. All ice covers attenuate wave energy. Only long swells can penetrate deep into an ice cover. Being closest to open water, wave propagation in the marginal ice zone is the most complex to model. The physical appearance of sea ice in the marginal ice zone varies. Grease ice, pancake ice, brash ice, floe aggregates, and continuous ice sheet may be found in this zone at different times and locations. These types of ice are formed under different thermal-mechanical forcing. There are three classic models that describe wave propagation through an idealized ice cover: mass loading, thin elastic plate, and viscous layer models. From physical arguments we may conjecture that mass loading model is suitable for disjoint aggregates of ice floes much smaller than the wavelength, thin elastic plate model is suitable for a continuous ice sheet, and the viscous layer model is suitable for grease ice. For different sea ice types we may need different wave ice interaction models. A recently proposed viscoelastic model is able to synthesize all three classic models into one. Under suitable limiting conditions it converges to the three previous models. The complete theoretical framework for evaluating wave propagation through various ice covers need to be implemented in the operational ocean wave models. In this review, we introduce the sea ice types, previous wave ice interaction models, wave attenuation mechanisms, the methods to calculate wave reflection and transmission between different ice covers, and the effect of ice floe breaking on shaping the sea ice morphology

  15. On the Navier Stokes equations simulation of the head-on collision between two surface solitary waves

    NASA Astrophysics Data System (ADS)

    Lubin, Pierre; Vincent, Stéphane; Caltagirone, Jean-Paul

    2005-04-01

    The scope of this Note is to show the results obtained for simulating the two-dimensional head-on collision of two solitary waves by solving the Navier-Stokes equations in air and water. The work is dedicated to the numerical investigation of the hydrodynamics associated to this highly nonlinear flow configuration, the first numerical results being analyzed. The original numerical model is proved to be efficient and accurate in predicting the main features described in experiments found in the literature. This Note also outlines the interest of this configuration to be considered as a test-case for numerical models dedicated to computational fluid mechanics. To cite this article: P. Lubin et al., C. R. Mecanique 333 (2005).

  16. Seismic‐wave attenuation determined from tectonic tremor in multiple subduction zones

    USGS Publications Warehouse

    Yabe, Suguru; Baltay, Annemarie S.; Ide, Satoshi; Beroza, Gregory C.

    2014-01-01

    Tectonic tremor provides a new source of observations that can be used to constrain the seismic attenuation parameter for ground‐motion prediction and hazard mapping. Traditionally, recorded earthquakes of magnitude ∼3–8 are used to develop ground‐motion prediction equations; however, typical earthquake records may be sparse in areas of high hazard. In this study, we constrain the distance decay of seismic waves using measurements of the amplitude decay of tectonic tremor, which is plentiful in some regions. Tectonic tremor occurs in the frequency band of interest for ground‐motion prediction (i.e., ∼2–8  Hz) and is located on the subducting plate interface, at the lower boundary of where future large earthquakes are expected. We empirically fit the distance decay of peak ground velocity from tremor to determine the attenuation parameter in four subduction zones: Nankai, Japan; Cascadia, United States–Canada; Jalisco, Mexico; and southern Chile. With the large amount of data available from tremor, we show that in the upper plate, the lower crust is less attenuating than the upper crust. We apply the same analysis to intraslab events in Nankai and show the possibility that waves traveling from deeper intraslab events experience more attenuation than those from the shallower tremor due to ray paths that pass through the subducting and highly attenuating oceanic crust. This suggests that high pore‐fluid pressure is present in the tremor source region. These differences imply that the attenuation parameter determined from intraslab earthquakes may underestimate ground motion for future large earthquakes on the plate interface.

  17. Automatic Calibration Method for Driver’s Head Orientation in Natural Driving Environment

    PubMed Central

    Fu, Xianping; Guan, Xiao; Peli, Eli; Liu, Hongbo; Luo, Gang

    2013-01-01

    Gaze tracking is crucial for studying driver’s attention, detecting fatigue, and improving driver assistance systems, but it is difficult in natural driving environments due to nonuniform and highly variable illumination and large head movements. Traditional calibrations that require subjects to follow calibrators are very cumbersome to be implemented in daily driving situations. A new automatic calibration method, based on a single camera for determining the head orientation and which utilizes the side mirrors, the rear-view mirror, the instrument board, and different zones in the windshield as calibration points, is presented in this paper. Supported by a self-learning algorithm, the system tracks the head and categorizes the head pose in 12 gaze zones based on facial features. The particle filter is used to estimate the head pose to obtain an accurate gaze zone by updating the calibration parameters. Experimental results show that, after several hours of driving, the automatic calibration method without driver’s corporation can achieve the same accuracy as a manual calibration method. The mean error of estimated eye gazes was less than 5°in day and night driving. PMID:24639620

  18. Surface Wave Dynamics in the Coastal Zone

    DTIC Science & Technology

    2014-09-30

    also collected from the Duck measurement site, operated by the USACE Field Research Facility at Duck , North Carolina. The collection and validation...similar analysis for 10 storm periods using wave data collected at Duck , North Carolina. The preparations consist of creating a dedicated unstructured...validated in the Southern North Sea and Duck validation studies. The shallow water source terms for wave breaking and triad interactions are being

  19. Photon migration through fetal head in utero using continuous wave, near infrared spectroscopy: clinical and experimental model studies

    NASA Astrophysics Data System (ADS)

    Ramanujam, Nirmala; Vishnoi, Gargi; Hielscher, Andreas H.; Rode, Martha; Forouzan, Iraj; Chance, Britton

    2000-04-01

    Near infrared (NIR) measurements were made from the maternal abdomen (clinical studies) and laboratory tissue phantoms (experimental studies) to gain insight into photon migration through the fetal head in utero. Specifically, a continuous wave spectrometer was modified and employed to make NIR measurements at 760 and 850 nm, at a large (10 cm) and small (2.5/4 cm) source-detector separation, simultaneously, on the maternal abdomen, directly above the fetal head. A total of 19 patients were evaluated, whose average gestational age and fetal head depth, were 37 weeks +/- 3 and 2.25 cm +/- 0.7, respectively. At the large source-detector separation, the photons are expected to migrate through both the underlying maternal and fetal tissues before being detected at the surface, while at the short source-detector separation, the photons are expected to migrate primarily through the superficial maternal tissues before being detected. Second, similar NIR measurements were made on laboratory tissue phantoms, with variable optical properties and physical geometries. The variable optical properties were obtained using different concentrations of India ink and Intralipid in water, while the variable physical geometries were realized by employing glass containers of different shapes and sizes. Third, the NIR measurements, which were made on the laboratory tissue phantoms, were compared to the NIR measurements made on the maternal abdomen to determine which tissue phantom best simulates the photon migration path through the fetal head in utero. The results of the comparison were used to provide insight into the optical properties and physical geometry of the maternal and fetal tissues in the photon migration path.

  20. Turbidity Current Head Mixing

    NASA Astrophysics Data System (ADS)

    Hernandez, David; Sanchez, Miguel Angel; Medina, Pablo

    2010-05-01

    A laboratory experimental set - up for studying the behaviour of sediment in presence of a turbulent field with zero mean flow is compared with the behaviour of turbidity currents [1] . Particular interest is shown on the initiation of sediment motion and in the sediment lift - off. The behaviour of the turbidity current in a flat ground is compared with the zero mean flow oscilating grid generated turbulence as when wave flow lifts off suspended sediments [2,3]. Some examples of the results obtained with this set-up relating the height of the head of the turbidity current to the equilibrium level of stirred lutoclines are shown. A turbulent velocity u' lower than that estimated by the Shield diagram is required to start sediment motion. The minimum u' required to start sediment lift - off, is a function of sediment size, cohesivity and resting time. The lutocline height depends on u', and the vorticity at the lutocline seems constant for a fixed sediment size [1,3]. Combining grid stirring and turbidty current head shapes analyzed by means of advanced image analysis, sediment vertical fluxes and settling speeds can be measured [4,5]. [1] D. Hernandez Turbulent structure of turbidity currents and sediment transport Ms Thesis ETSECCPB, UPC. Barcelona 2009. [2] A. Sánchez-Arcilla; A. Rodríguez; J.C. Santás; J.M. Redondo; V. Gracia; R. K'Osyan; S. Kuznetsov; C. Mösso. Delta'96 Surf-zone and nearshore measurements at the Ebro Delta. A: International Conference on Coastal Research through large Scale Experiments (Coastal Dynamics '97). University of Plymouth, 1997, p. 186-187. [3] P. Medina, M. A. Sánchez and J. M. Redondo. Grid stirred turbulence: applications to the initiation of sediment motion and lift-off studies Physics and Chemistry of the Earth, Part B: Hydrology, Oceans and Atmosphere. 26, Issue 4, 2001, Pages 299-304 [4] M.O. Bezerra, M. Diez, C. Medeiros, A. Rodriguez, E. Bahia., A. Sanchez-Arcilla and J.M. Redondo. Study on the influence of waves on

  1. Observations of storm morphodynamics using Coastal Lidar and Radar Imaging System (CLARIS): Importance of wave refraction and dissipation over complex surf-zone morphology at a shoreline erosional hotspot

    NASA Astrophysics Data System (ADS)

    Brodie, Katherine L.

    Elevated water levels and large waves during storms cause beach erosion, overwash, and coastal flooding, particularly along barrier island coastlines. While predictions of storm tracks have greatly improved over the last decade, predictions of maximum water levels and variations in the extent of damage along a coastline need improvement. In particular, physics based models still cannot explain why some regions along a relatively straight coastline may experience significant erosion and overwash during a storm, while nearby locations remain seemingly unchanged. Correct predictions of both the timing of erosion and variations in the magnitude of erosion along the coast will be useful to both emergency managers and homeowners preparing for an approaching storm. Unfortunately, research on the impact of a storm to the beach has mainly been derived from "pre" and "post" storm surveys of beach topography and nearshore bathymetry during calm conditions. This has created a lack of data during storms from which to ground-truth model predictions and test hypotheses that explain variations in erosion along a coastline. We have developed Coastal Lidar and Radar Imaging System (CLARIS), a mobile system that combines a terrestrial scanning laser and an X-band marine radar system using precise motion and location information. CLARIS can operate during storms, measuring beach topography, nearshore bathymetry (from radar-derived wave speed measurements), surf-zone wave parameters, and maximum water levels remotely. In this dissertation, we present details on the development, design, and testing of CLARIS and then use CLARIS to observe a 10 km section of coastline in Kitty Hawk and Kill Devil Hills on the Outer Banks of North Carolina every 12 hours during a Nor'Easter (peak wave height in 8 m of water depth = 3.4 m). High decadal rates of shoreline change as well as heightened erosion during storms have previously been documented to occur within the field site. In addition, complex

  2. An empirical method to estimate shear wave velocity of soils in the New Madrid seismic zone

    USGS Publications Warehouse

    Wei, B.-Z.; Pezeshk, S.; Chang, T.-S.; Hall, K.H.; Liu, Huaibao P.

    1996-01-01

    In this study, a set of charts are developed to estimate shear wave velocity of soils in the New Madrid seismic zone (NMSZ), using the standard penetration test (SPT) N values and soil depths. Laboratory dynamic test results of soil samples collected from the NMSZ showed that the shear wave velocity of soils is related to the void ratio and the effective confining pressure applied to the soils. The void ratio of soils can be estimated from the SPT N values and the effective confining pressure depends on the depth of soils. Therefore, the shear wave velocity of soils can be estimated from the SPT N value and the soil depth. To make the methodology practical, two corrections should be made. One is that field SPT N values of soils must be adjusted to an unified SPT N??? value to account the effects of overburden pressure and equipment. The second is that the effect of water table to effective overburden pressure of soils must be considered. To verify the methodology, shear wave velocities of five sites in the NMSZ are estimated and compared with those obtained from field measurements. The comparison shows that our approach and the field tests are consistent with an error of less than of 15%. Thus, the method developed in this study is useful for dynamic study and practical designs in the NMSZ region. Copyright ?? 1996 Elsevier Science Limited.

  3. Remote sensing of the marginal ice zone during Marginal Ice Zone Experiment (MIZEX) 83

    NASA Technical Reports Server (NTRS)

    Shuchman, R. A.; Campbell, W. J.; Burns, B. A.; Ellingsen, E.; Farrelly, B. A.; Gloersen, P.; Grenfell, T. C.; Hollinger, J.; Horn, D.; Johannessen, J. A.

    1984-01-01

    The remote sensing techniques utilized in the Marginal Ice Zone Experiment (MIZEX) to study the physical characteristics and geophysical processes of the Fram Strait Region of the Greenland Sea are described. The studies, which utilized satellites, aircraft, helicopters, and ship and ground-based remote sensors, focused on the use of microwave remote sensors. Results indicate that remote sensors can provide marginal ice zone characteristics which include ice edge and ice boundary locations, ice types and concentration, ice deformation, ice kinematics, gravity waves and swell (in the water and the ice), location of internal wave fields, location of eddies and current boundaries, surface currents and sea surface winds.

  4. Teleseismic P and S wave attenuation constraints on temperature and melt of the upper mantle in the Alaska Subduction Zone.

    NASA Astrophysics Data System (ADS)

    Soto Castaneda, R. A.; Abers, G. A.; Eilon, Z.; Christensen, D. H.

    2017-12-01

    Recent broadband deployments in Alaska provide an excellent opportunity to advance our understanding of the Alaska-Aleutians subduction system, with implications for subduction processes worldwide. Seismic attenuation, measured from teleseismic body waves, provides a strong constraint on thermal structure as well as an indirect indication of ground shaking expected from large intermediate-depth earthquakes. We measure P and S wave attenuation from pairwise amplitude and phase spectral ratios for teleseisms recorded at 204 Transportable Array, Alaska Regional, and Alaska Volcano Observatory, SALMON (Southern Alaska Lithosphere & Mantle Observation Network) and WVLF (Wrangell Volcanics & subducting Lithosphere Fate) stations in central Alaska. The spectral ratios are inverted in a least squares sense for differential t* (path-averaged attenuation operator) and travel time anomalies at every station. Our preliminary results indicate a zone of low attenuation across the forearc and strong attenuation beneath arc and backarc in the Cook Inlet-Kenai region where the Aleutian-Yakutat slab subducts, similar to other subduction zones. This attenuation differential is observed in both the volcanic Cook Inlet segment and amagmatic Denali segments of the Aleutian subduction zone. By comparison, preliminary results for the Wrangell-St. Elias region past the eastern edge of the Aleutian slab show strong attenuation beneath the Wrangell Volcanic Field, as well as much further south than in the Cook Inlet-Kenai region. This pattern of attenuation seems to indicate a short slab fragment in the east of the subduction zone, though the picture is complex. Results also suggest the slab may focus or transmit energy with minimal attenuation, adding to the complexity. To image the critical transition between the Alaska-Aleutian slab and the region to its east, we plan to incorporate new broadband data from the WVLF array, an ongoing deployment of 37 PASSCAL instruments installed in 2016

  5. Continuity of the West Napa–Franklin fault zone inferred from guided waves generated by earthquakes following the 24 August 2014 Mw 6.0 South Napa earthquake

    USGS Publications Warehouse

    Catchings, Rufus D.; Goldman, Mark R.; Li, Yong-Gang; Chan, Joanne

    2016-01-01

    We measure peak ground velocities from fault‐zone guided waves (FZGWs), generated by on‐fault earthquakes associated with the 24 August 2014 Mw 6.0 South Napa earthquake. The data were recorded on three arrays deployed across north and south of the 2014 surface rupture. The observed FZGWs indicate that the West Napa fault zone (WNFZ) and the Franklin fault (FF) are continuous in the subsurface for at least 75 km. Previously published potential‐field data indicate that the WNFZ extends northward to the Maacama fault (MF), and previous geologic mapping indicates that the FF extends southward to the Calaveras fault (CF); this suggests a total length of at least 110 km for the WNFZ–FF. Because the WNFZ–FF appears contiguous with the MF and CF, these faults apparently form a continuous Calaveras–Franklin–WNFZ–Maacama (CFWM) fault that is second only in length (∼300  km) to the San Andreas fault in the San Francisco Bay area. The long distances over which we observe FZGWs, coupled with their high amplitudes (2–10 times the S waves) suggest that strong shaking from large earthquakes on any part of the CFWM fault may cause far‐field amplified fault‐zone shaking. We interpret guided waves and seismicity cross sections to indicate multiple upper crustal splays of the WNFZ–FF, including a northward extension of the Southhampton fault, which may cause strong shaking in the Napa Valley and the Vallejo area. Based on travel times from each earthquake to each recording array, we estimate average P‐, S‐, and guided‐wave velocities within the WNFZ–FF (4.8–5.7, 2.2–3.2, and 1.1–2.8  km/s, respectively), with FZGW velocities ranging from 58% to 93% of the average S‐wave velocities.

  6. Comparison of different assimilation methodologies of groundwater levels to improve predictions of root zone soil moisture with an integrated terrestrial system model

    NASA Astrophysics Data System (ADS)

    Zhang, Hongjuan; Kurtz, Wolfgang; Kollet, Stefan; Vereecken, Harry; Franssen, Harrie-Jan Hendricks

    2018-01-01

    The linkage between root zone soil moisture and groundwater is either neglected or simplified in most land surface models. The fully-coupled subsurface-land surface model TerrSysMP including variably saturated groundwater dynamics is used in this work. We test and compare five data assimilation methodologies for assimilating groundwater level data via the ensemble Kalman filter (EnKF) to improve root zone soil moisture estimation with TerrSysMP. Groundwater level data are assimilated in the form of pressure head or soil moisture (set equal to porosity in the saturated zone) to update state vectors. In the five assimilation methodologies, the state vector contains either (i) pressure head, or (ii) log-transformed pressure head, or (iii) soil moisture, or (iv) pressure head for the saturated zone only, or (v) a combination of pressure head and soil moisture, pressure head for the saturated zone and soil moisture for the unsaturated zone. These methodologies are evaluated in synthetic experiments which are performed for different climate conditions, soil types and plant functional types to simulate various root zone soil moisture distributions and groundwater levels. The results demonstrate that EnKF cannot properly handle strongly skewed pressure distributions which are caused by extreme negative pressure heads in the unsaturated zone during dry periods. This problem can only be alleviated by methodology (iii), (iv) and (v). The last approach gives the best results and avoids unphysical updates related to strongly skewed pressure heads in the unsaturated zone. If groundwater level data are assimilated by methodology (iii), EnKF fails to update the state vector containing the soil moisture values if for (almost) all the realizations the observation does not bring significant new information. Synthetic experiments for the joint assimilation of groundwater levels and surface soil moisture support methodology (v) and show great potential for improving the representation

  7. Suitability of temperature, hydraulic heads, and acesulfame to quantify wastewater-related fluxes in the hyporheic and riparian zone

    NASA Astrophysics Data System (ADS)

    Engelhardt, Irina; Prommer, Henning; Moore, Catherine; Schulz, Manoj; Schüth, Christoph; Ternes, Thomas A.

    2013-01-01

    Groundwater and surface water are in many cases closely linked components of the water cycle with respect to both quantity and quality. Bank filtrates may eventually be impacted by the infiltration of wastewater-derived micropollutants from surface waters. Artificial sweeteners such as acesulfame have recently been reported as a novel class of potentially valuable tracers to study the fate of wastewater-derived substances in groundwater and, in particular, to determine the (bio)degradability of micropollutants. In this paper, a model-based analysis of a field experiment within the hyporheic and riparian zone of a highly polluted German stream was performed to assess the physical and chemical behavior of the artificial sweetener acesulfame. In the first part of this study, a reliable flow and transport model was established by jointly using hydraulic heads, temperatures, and acesulfame concentrations as inverse model calibration constraints. The analysis confirmed the conservative behavior of acesulfame and, therefore, its usability as an indicator of sewage flux provenance. However, a comparison of the appropriateness of hydraulic head, temperature, and acesulfame concentrations revealed that the characterization of the surface water-groundwater flux data indicated diurnal temperature fluctuations are the best indicator in terms of characterizing the flow and transport behavior in the groundwater system.

  8. Smart optical writing head design for laser-based manufacturing

    NASA Astrophysics Data System (ADS)

    Amin, M. Junaid; Riza, Nabeel A.

    2014-03-01

    Proposed is a smart optical writing head design suitable for high precision industrial laser based machining and manufacturing applications. The design uses an Electronically Controlled Variable Focus Lens (ECVFL) which enables the highest achievable spatial resolution of writing head spot sizes for axial target distances reaching 8 meters. A proof-of-concept experiment is conducted using a visible wavelength laser with a collimated beam that is coupled to beam conditioning optics which includes an electromagnetically actuated deformable membrane liquid ECVFL cascaded with a bias convex lens of fixed focal length. Electronic tuning and control of the ECVFL keeps the laser writing head far-field spot beam radii under 1 mm that is demonstrated over a target range of 20 cm to 800 cm. Applications for the proposed writing head design, which can accommodate both continuous wave and pulsed wave sources, include laser machining, high precision industrial molding of components, as well as materials processing requiring material sensitive optical power density control.

  9. Borehole geophysical, fluid, and hydraulic properties within and surrounding the freshwater/saline-water transition zone, San Antonio segment of the Edwards aquifer, south-central Texas, 2010-11

    USGS Publications Warehouse

    Thomas, Jonathan V.; Stanton, Gregory P.; Lambert, Rebecca B.

    2012-01-01

    Although analyses of daily mean equivalent freshwater heads for the East Uvalde transect indicated that the gradient across the freshwater/saline-water interface varied between into and out of the freshwater zone, the data indicate that there was a slightly longer period during which the gradient was out of the freshwater zone. Analyses of all daily mean equivalent freshwater heads for the Tri-County transect indicated that the lateral-head gradients across the freshwater/saline-water interface were typically mixed (not indicative of flow into or out of freshwater zone). Assessment of the daily mean equivalent freshwater heads indicated that, although the lateral-head gradient at the Kyle transect varied between into and out of the freshwater zone, the lateral-head gradient was typically from the transition zone into the freshwater zone.

  10. ON HYDRODYNAMIC MOTIONS IN DEAD ZONES

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

    Oishi, Jeffrey S.; Mac Low, Mordecai-Mark, E-mail: jsoishi@astro.berkeley.ed, E-mail: mordecai@amnh.or

    We investigate fluid motions near the midplane of vertically stratified accretion disks with highly resistive midplanes. In such disks, the magnetorotational instability drives turbulence in thin layers surrounding a resistive, stable dead zone. The turbulent layers in turn drive motions in the dead zone. We examine the properties of these motions using three-dimensional, stratified, local, shearing-box, non-ideal, magnetohydrodynamical simulations. Although the turbulence in the active zones provides a source of vorticity to the midplane, no evidence for coherent vortices is found in our simulations. It appears that this is because of strong vertical oscillations in the dead zone. By analyzingmore » time series of azimuthally averaged flow quantities, we identify an axisymmetric wave mode particular to models with dead zones. This mode is reduced in amplitude, but not suppressed entirely, by changing the equation of state from isothermal to ideal. These waves are too low frequency to affect sedimentation of dust to the midplane, but may have significance for the gravitational stability of the resulting midplane dust layers.« less

  11. Lidar Observations of Wave Shape

    NASA Astrophysics Data System (ADS)

    Brodie, K. L.; Raubenheimer, B.; Spore, N.; Gorrell, L.; Slocum, R. K.; Elgar, S.

    2016-02-01

    As waves propagate across the inner-surf zone, through a shorebreak, to the swash, their shapes can evolve rapidly, particularly if there are large changes in water depth over a wavelength. As wave shapes evolve, the time history of near-bed wave-orbital velocities also changes. Asymmetrical near-bed velocities result in preferential directions for sediment transport, and spatial variations in asymmetries can lead to morphological evolution. Thus, understanding and predicting wave shapes in the inner-surf and swash zones is important to improving sediment transport predictions. Here, rapid changes in wave shape, quantified by 3rd moments (skewness and asymmetry) of the sea-surface elevation time series, were observed on a sandy Atlantic Ocean beach near Duck, NC using terrestrial lidar scanners that measure the elevation of the water surface along a narrow cross-shore transect with high spatial [O(1 cm)] and temporal [O(0.5 s)] resolution. The terrestrial lidar scanners were mounted on a tower on the beach dune (about 8 m above the water surface) and on an 8-m tall amphibious tripod [the Coastal Research Amphibious Buggy (CRAB)]. Observations with the dune lidar are used to investigate how bulk wave shape parameters such as wave skewness and asymmetry, and the ratio of wave height to water depth (gamma) vary with beach slope, tide level, and offshore wave conditions. Observations with the lidar mounted on the CRAB are used to investigate the evolution of individual waves propagating across the surf zone and shorebreak to the swash. For example, preliminary observations from the CRAB include a wave that appeared to shoal and then "pitch" backwards immediately prior to breaking and running up the beach. Funded by the USACE Coastal Field Data Collection Program, ASD(R&E), and ONR.

  12. Damping Effect of an Unsaturated-Saturated System on Tempospatial Variations of Pressure Head and Specific Flux

    NASA Astrophysics Data System (ADS)

    Yang, C.; Zhang, Y. K.; Liang, X.

    2014-12-01

    Damping effect of an unsaturated-saturated system on tempospatialvariations of pressurehead and specificflux was investigated. The variance and covariance of both pressure head and specific flux in such a system due to a white noise infiltration were obtained by solving the moment equations of water flow in the system and verified with Monte Carlo simulations. It was found that both the pressure head and specific flux in this case are temporally non-stationary. The variance is zero at early time due to a deterministic initial condition used, then increases with time, and approaches anasymptotic limit at late time.Both pressure head and specific flux arealso non-stationary in space since the variance decreases from source to sink. The unsaturated-saturated systembehavesasa noise filterand it damps both the pressure head and specific flux, i.e., reduces their variations and enhances their correlation. The effect is stronger in upper unsaturated zone than in lower unsaturated zone and saturated zone. As a noise filter, the unsaturated-saturated system is mainly a low pass filter, filtering out the high frequency components in the time series of hydrological variables. The damping effect is much stronger in the saturated zone than in the saturated zone.

  13. Landslide stability: Role of rainfall-induced, laterally propagating, pore-pressure waves

    USGS Publications Warehouse

    Priest, G.R.; Schulz, W.H.; Ellis, W.L.; Allan, J.A.; Niem, A.R.; Niem, W.A.

    2011-01-01

    The Johnson Creek Landslide is a translational slide in seaward-dipping Miocene siltstone and sandstone (Astoria Formation) and an overlying Quaternary marine terrace deposit. The basal slide plane slopes sub-parallel to the dip of the Miocene rocks, except beneath the back-tilted toe block, where it slopes inland. Rainfall events raise pore-water pressure in the basal shear zone in the form of pulses of water pressure traveling laterally from the headwall graben down the axis of the slide at rates of 1-6 m/hr. Infiltration of meteoric water and vertical pressure transmission through the unsaturated zone has been measured at ~50 mm/hr. Infiltration and vertical pressure transmission were too slow to directly raise head at the basal shear zone prior to landslide movement. Only at the headwall graben was the saturated zone shallow enough for rainfall events to trigger lateral pulses of water pressure through the saturated zone. When pressure levels in the basal shear zone exceeded thresholds defined in this paper, the slide began slow, creeping movement as an intact block. As pressures exceeded thresholds for movement in more of the slide mass, movement accelerated, and differential displacement between internal slide blocks became more pronounced. Rainfall-induced pore-pressure waves are probably a common landslide trigger wherever effective hydraulic conductivity is high and the saturated zone is located near the surface in some part of a slide. An ancillary finding is apparently greater accuracy of grouted piezometers relative to those in sand packs for measurement of pore pressures at the installed depth.

  14. Does littoral sand bypass the head of Mugu Submarine Canyon? - a modeling study

    USGS Publications Warehouse

    Xu, Jingping; Elias, Edwin; Kinsman, Nicole; Wang, Ping; Rosati, Julie D.; Roberts, Tiffany M.

    2011-01-01

    A newly developed sand-tracer code for the process-based model Delft3D (Deltares, The Netherlands) was used to simulate the littoral transport near the head of the Mugu Submarine Canyon in California, USA. For westerly swells, which account for more than 90% of the wave conditions in the region, the sand tracers in the downcoast littoral drift were unable to bypass the canyon head. A flow convergence near the upcoast rim of the canyon intercepts the tracers and moves them either offshore onto the shelf just west of the canyon rim (low wave height conditions) or into the canyon head (storm wave conditions). This finding supports the notion that Mugu Canyon is the true terminus of the Santa Barbara Littoral Cell.

  15. Probing the critical zone using passive- and active-source estimates of subsurface shear-wave velocities

    NASA Astrophysics Data System (ADS)

    Callahan, R. P.; Taylor, N. J.; Pasquet, S.; Dueker, K. G.; Riebe, C. S.; Holbrook, W. S.

    2016-12-01

    Geophysical imaging is rapidly becoming popular for quantifying subsurface critical zone (CZ) architecture. However, a diverse array of measurements and measurement techniques are available, raising the question of which are appropriate for specific study goals. Here we compare two techniques for measuring S-wave velocities (Vs) in the near surface. The first approach quantifies Vs in three dimensions using a passive source and an iterative residual least-squares tomographic inversion. The second approach uses a more traditional active-source seismic survey to quantify Vs in two dimensions via a Monte Carlo surface-wave dispersion inversion. Our analysis focuses on three 0.01 km2 study plots on weathered granitic bedrock in the Southern Sierra Critical Zone Observatory. Preliminary results indicate that depth-averaged velocities from the two methods agree over the scales of resolution of the techniques. While the passive- and active-source techniques both quantify Vs, each method has distinct advantages and disadvantages during data acquisition and analysis. The passive-source method has the advantage of generating a three dimensional distribution of subsurface Vs structure across a broad area. Because this method relies on the ambient seismic field as a source, which varies unpredictably across space and time, data quality and depth of investigation are outside the control of the user. Meanwhile, traditional active-source surveys can be designed around a desired depth of investigation. However, they only generate a two dimensional image of Vs structure. Whereas traditional active-source surveys can be inverted quickly on a personal computer in the field, passive source surveys require significantly more computations, and are best conducted in a high-performance computing environment. We use data from our study sites to compare these methods across different scales and to explore how these methods can be used to better understand subsurface CZ architecture.

  16. Progressive addition spectacle lenses: Design preferences and head movements while reading

    NASA Astrophysics Data System (ADS)

    Preston, Julie Lynn

    In a subjective preference study, two key progressive addition lens parameters, near zone width and corridor length, were varied in a double-masked, randomized, clinical trial of 49 patients. Each subject received a complete eye examination and a new frame. Each wore 6 pairs of lenses for one week at a time and completed questionnaires relating to vision, adaptation, and satisfaction. The preferred lens was identified from the three near zone width lenses and from the three corridor length lenses. Patient characteristics were analyzed for their effect on design preference. Satisfaction ratings following a brief experience with each design were compared to ratings after one week of wear in order to ascertain the predictability of initial impressions. One lens design appeared twice in the preference trial, providing an assessment of the repeatability of the rating instrument. The lens design with the widest near zone was rated significantly lower than the other near zone width designs for nearly every question relating to vision, adaptation, and satisfaction. This lens was also least preferred of all the designs. Preferences for corridor length were evenly distributed among the three designs. Of patient characteristics, years of progressive addition lens wear and gender significantly affected design preference in this population. Initial impressions were not predictive of satisfaction after a week of wear. The rating instrument was judged to have low repeatability. In the head movement portion of the study, 18 participants from the preference study wore the three near zone width designs while reading three paragraphs of varying print size. From a 20 second recording for each of three different paragraphs with each lens, measures of head rotation and posture were collected. The amplitude of head rotation was significantly affected by print size but not by lens design. The effective zone widths on the lenses scanned by the eyes and the locations of the reading levels

  17. Velocity Memory Effect for polarized gravitational waves

    NASA Astrophysics Data System (ADS)

    Zhang, P.-M.; Duval, C.; Gibbons, G. W.; Horvathy, P. A.

    2018-05-01

    Circularly polarized gravitational sandwich waves exhibit, as do their linearly polarized counterparts, the Velocity Memory Effect: freely falling test particles in the flat after-zone fly apart along straight lines with constant velocity. In the inside zone their trajectories combine oscillatory and rotational motions in a complicated way. For circularly polarized periodic gravitational waves some trajectories remain bounded, while others spiral outward. These waves admit an additional "screw" isometry beyond the usual five. The consequences of this extra symmetry are explored.

  18. ROSSBY WAVE INSTABILITY AT DEAD ZONE BOUNDARIES IN THREE-DIMENSIONAL RESISTIVE MAGNETOHYDRODYNAMICAL GLOBAL MODELS OF PROTOPLANETARY DISKS

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

    Lyra, Wladimir; Mac Low, Mordecai-Mark, E-mail: wlyra@jpl.nasa.gov, E-mail: mordecai@amnh.org

    It has been suggested that the transition between magnetorotationally active and dead zones in protoplanetary disks should be prone to the excitation of vortices via Rossby wave instability (RWI). However, the only numerical evidence for this has come from alpha disk models, where the magnetic field evolution is not followed, and the effect of turbulence is parameterized by Laplacian viscosity. We aim to establish the phenomenology of the flow in the transition in three-dimensional resistive-magnetohydrodynamical models. We model the transition by a sharp jump in resistivity, as expected in the inner dead zone boundary, using the PENCIL CODE to simulatemore » the flow. We find that vortices are readily excited in the dead side of the transition. We measure the mass accretion rate finding similar levels of Reynolds stress at the dead and active zones, at the {alpha} Almost-Equal-To 10{sup -2} level. The vortex sits in a pressure maximum and does not migrate, surviving until the end of the simulation. A pressure maximum in the active zone also triggers the RWI. The magnetized vortex that results should be disrupted by parasitical magneto-elliptic instabilities, yet it subsists in high resolution. This suggests that either the parasitic modes are still numerically damped or that the RWI supplies vorticity faster than they can destroy it. We conclude that the resistive transition between the active and dead zones in the inner regions of protoplanetary disks, if sharp enough, can indeed excite vortices via RWI. Our results lend credence to previous works that relied on the alpha-disk approximation, and caution against the use of overly reduced azimuthal coverage on modeling this transition.« less

  19. Interactive navigation system for shock wave applications.

    PubMed

    Hagelauer, U; Russo, S; Gigliotti, S; de Durante, C; Corrado, E M

    2001-01-01

    The latest generation of shock wave lithotripters, with therapy heads mounted on articulated arms, have found widespread application in the treatment of orthopedic diseases. Currently, integration of an ultrasound probe in the therapy head is the dominant modality for positioning the shock wave focus on the treatment area. For orthopedic applications, however, X-ray imaging is often preferred. This article describes a new method to locate the therapy head of a lithotripter. In the first step, the surgeon positions the tissue to be treated at the isocenter of a C-arc. This is achieved using AP and 30-degree lateral projections, with corresponding horizontal and vertical movements of the patient under fluoroscopic guidance. These movements register the anatomic location in the coordinate system of the C-arc. In the second step, the therapy head is navigated to align the shock wave focus with the isocenter. Position data are reported from an optical tracker mounted on the X-ray system, which tracks an array of infrared LEDs on the therapy head. The accuracy of the tracking system was determined on a test bench, and was calculated to be 1.55 mm (RMS) for an angular movement of +/-15 degrees around a calibrated position. Free-hand navigation and precise alignment are performed with a single virtual reality display. The display is calculated by a computer system in real time, and uses graphical symbols to represent the shock wave path and isocenter. In an interactive process, the physician observes the display while navigating the therapy head towards the isocenter. Precise alignment is achieved by displaying an enlarged view of the intersecting graphical symbols. Results from the first tests on 100 patients demonstrate the feasibility of this approach in a clinical environment. Copyright 2001 Wiley-Liss, Inc.

  20. Evolution of Spiral and Scroll Waves of Excitation in a Mathematical Model of Ischaemic Border Zone

    PubMed Central

    Biktashev, Vadim N.; Biktasheva, Irina V.; Sarvazyan, Narine A.

    2011-01-01

    Abnormal electrical activity from the boundaries of ischemic cardiac tissue is recognized as one of the major causes in generation of ischemia-reperfusion arrhythmias. Here we present theoretical analysis of the waves of electrical activity that can rise on the boundary of cardiac cell network upon its recovery from ischaemia-like conditions. The main factors included in our analysis are macroscopic gradients of the cell-to-cell coupling and cell excitability and microscopic heterogeneity of individual cells. The interplay between these factors allows one to explain how spirals form, drift together with the moving boundary, get transiently pinned to local inhomogeneities, and finally penetrate into the bulk of the well-coupled tissue where they reach macroscopic scale. The asymptotic theory of the drift of spiral and scroll waves based on response functions provides explanation of the drifts involved in this mechanism, with the exception of effects due to the discreteness of cardiac tissue. In particular, this asymptotic theory allows an extrapolation of 2D events into 3D, which has shown that cells within the border zone can give rise to 3D analogues of spirals, the scroll waves. When and if such scroll waves escape into a better coupled tissue, they are likely to collapse due to the positive filament tension. However, our simulations have shown that such collapse of newly generated scrolls is not inevitable and that under certain conditions filament tension becomes negative, leading to scroll filaments to expand and multiply leading to a fibrillation-like state within small areas of cardiac tissue. PMID:21935402

  1. On the physics of waves in the solar atmosphere: Wave heating and wind acceleration

    NASA Technical Reports Server (NTRS)

    Musielak, Z. E.

    1994-01-01

    This paper presents work performed on the generation and physics of acoustic waves in the solar atmosphere. The investigators have incorporated spatial and temporal turbulent energy spectra in a newly corrected version of the Lighthill-Stein theory of acoustic wave generation in order to calculate the acoustic wave energy fluxes generated in the solar convective zone. The investigators have also revised and improved the treatment of the generation of magnetic flux tube waves, which can carry energy along the tubes far away from the region of their origin, and have calculated the tube wave energy fluxes for the sun. They also examine the transfer of the wave energy originated in the solar convective zone to the outer atmospheric layers through computation of wave propagation and dissipation in highly nonhomogeneous solar atmosphere. These waves may efficiently heat the solar atmosphere and the heating will be especially significant in the chromospheric network. It is also shown that the role played by Alfven waves in solar wind acceleration and coronal hole heating is dominant. The second part of the project concerned investigation of wave propagation in highly inhomogeneous stellar atmospheres using an approach based on an analytic tool developed by Musielak, Fontenla, and Moore. In addition, a new technique based on Dirac equations has been developed to investigate coupling between different MHD waves propagating in stratified stellar atmospheres.

  2. Imaging the mantle tranzition zone beneath the South American platform using P- and S-wave receiver functions

    NASA Astrophysics Data System (ADS)

    Bianchi, M.; Heit, B.; Yuan, X.; Assumpcao, M.; Kind, R.

    2009-04-01

    results observed are: 1) A clear cratonic signature, consisting of higher wave velocities for the mantle under the cratons and normal (410km and 660km) depths for the discontinuities 2) Strong presence of the Nazca subducted plate near 410 and 660 km discontinuities under the Southern part of the Parana basin 3) Lack of variation in the Transition Zone thickness and in the mantle velocities due to the presence of the possible plume proposed in 1995 by Vandecar at the Northern Parana basin region and 4) A possible transition zone thinning near the Matiqueira complex, at the Ribeira fold beld, near the Atlantic passive margin.

  3. Between tide and wave marks: a unifying model of physical zonation on littoral shores

    PubMed Central

    Bird, Christopher E.; Franklin, Erik C.; Smith, Celia M.

    2013-01-01

    The effects of tides on littoral marine habitats are so ubiquitous that shorelines are commonly described as ‘intertidal’, whereas waves are considered a secondary factor that simply modifies the intertidal habitat. However mean significant wave height exceeds tidal range at many locations worldwide. Here we construct a simple sinusoidal model of coastal water level based on both tidal range and wave height. From the patterns of emergence and submergence predicted by the model, we derive four vertical shoreline benchmarks which bracket up to three novel, spatially distinct, and physically defined zones. The (1) emergent tidal zone is characterized by tidally driven emergence in air; the (2) wave zone is characterized by constant (not periodic) wave wash; and the (3) submergent tidal zone is characterized by tidally driven submergence. The decoupling of tidally driven emergence and submergence made possible by wave action is a critical prediction of the model. On wave-dominated shores (wave height ≫ tidal range), all three zones are predicted to exist separately, but on tide-dominated shores (tidal range ≫ wave height) the wave zone is absent and the emergent and submergent tidal zones overlap substantially, forming the traditional “intertidal zone”. We conclude by incorporating time and space in the model to illustrate variability in the physical conditions and zonation on littoral shores. The wave:tide physical zonation model is a unifying framework that can facilitate our understanding of physical conditions on littoral shores whether tropical or temperate, marine or lentic. PMID:24109544

  4. Observations of wave-induced pore pressure gradients and bed level response on a surf zone sandbar

    NASA Astrophysics Data System (ADS)

    Anderson, Dylan; Cox, Dan; Mieras, Ryan; Puleo, Jack A.; Hsu, Tian-Jian

    2017-06-01

    Horizontal and vertical pressure gradients may be important physical mechanisms contributing to onshore sediment transport beneath steep, near-breaking waves in the surf zone. A barred beach was constructed in a large-scale laboratory wave flume with a fixed profile containing a mobile sediment layer on the crest of the sandbar. Horizontal and vertical pore pressure gradients were obtained by finite differences of measurements from an array of pressure transducers buried within the upper several centimeters of the bed. Colocated observations of erosion depth were made during asymmetric wave trials with wave heights between 0.10 and 0.98 m, consistently resulting in onshore sheet flow sediment transport. The pore pressure gradient vector within the bed exhibited temporal rotations during each wave cycle, directed predominantly upward under the trough and then rapidly rotating onshore and downward as the wavefront passed. The magnitude of the pore pressure gradient during each phase of rotation was correlated with local wave steepness and relative depth. Momentary bed failures as deep as 20 grain diameters were coincident with sharp increases in the onshore-directed pore pressure gradients, but occurred at horizontal pressure gradients less than theoretical critical values for initiation of the motion for compact beds. An expression combining the effects of both horizontal and vertical pore pressure gradients with bed shear stress and soil stability is used to determine that failure of the bed is initiated at nonnegligible values of both forces.Plain Language SummaryThe pressure gradient present within the seabed beneath breaking <span class="hlt">waves</span> may be an important physical mechanism transporting sediment. A large-scale laboratory was used to replicate realistic surfzone conditions in controlled tests, allowing for horizontal and vertical pressure gradient magnitudes and the resulting sediment bed response to be observed with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.G31A1046S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.G31A1046S"><span>Seafloor Geodesy usi­ng <span class="hlt">Wave</span> Gliders to study Earthquake and Tsunami Hazards at Subduction <span class="hlt">Zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sathiakumar, S.; Barbot, S.; Hill, E.; Peng, D.; Zerucha, J.; Suhaimee, S.; Chia, G.; Salamena, G. G.; Syahailatua, A.</p> <p>2016-12-01</p> <p>Land-based GNSS networks are now in place to monitor most subduction <span class="hlt">zones</span> of the world. These provide valuable information about the amount of­ geodetic strain accumulated in the region, which in turn gives insight into the seismic potential. However, it is usually impossible to resolve activity on the megathrust near the trench using land-based GNSS data alone, given typical signal-to-noise ratios. Ship-based seafloor geodesy is being used today to fill this observation gap. However, surveys using ships are very expensive, tedious and impractical due to the large areas to be covered. Instead of discrete missions using ships, continuous monitoring of the seafloor using autonomous marine robots would aid in understanding the tectonic setting of the seafloor better at a potentially lower cost, as well as help in designing better warning systems. Thus, we are developing seafloor geodesy capabilities using <span class="hlt">Wave</span> Gliders, a new class of <span class="hlt">wave</span>-propelled, persistent marine autonomous vehicle using a combination of acoustic and GNSS technologies. We use GNSS/INS to position the platform, and acoustic ranging to locate the seafloor. The GNSS/INS system to be integrated with the <span class="hlt">Wave</span> Gliders has stringent requirements of low power, light weight, and high accuracy. All these factors are equally important due to limited power and space in the <span class="hlt">Wave</span> Gliders and the need for highly accurate and precise measurements. With this hardware setup, a limiting factor is the accuracy of measurement of the sound velocity in the water column. We plan to obtain precise positioning of seafloor by exploring a measurement setup that minimizes uncertainties in sound velocity. This will be achieved by making fine-resolution measurements of the two-way travel time of the acoustic <span class="hlt">waves</span> underwater using the <span class="hlt">Wave</span> Gliders, and performing statistical signal processing on this data to obtain more reliable sound velocity measurement. This enhanced seafloor geodetic technique using <span class="hlt">Wave</span> Gliders should</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940031888','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940031888"><span>On the physics of <span class="hlt">waves</span> in the solar atmosphere: <span class="hlt">Wave</span> heating and wind acceleration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Musielak, Z. E.</p> <p>1993-01-01</p> <p>This paper presents work performed on the generation and physics of acoustic <span class="hlt">waves</span> in the solar atmosphere. The investigators have incorporated spatial and temporal turbulent energy spectra in a newly corrected version of the Lighthill-Stein theory of acoustic <span class="hlt">wave</span> generation in order to calculate the acoustic <span class="hlt">wave</span> energy fluxes generated in the solar convective <span class="hlt">zone</span>. The investigators have also revised and improved the treatment of the generation of magnetic flux tube <span class="hlt">waves</span>, which can carry energy along the tubes far away from the region of their origin, and have calculated the tube energy fluxes for the sun. They also examine the transfer of the <span class="hlt">wave</span> energy originated in the solar convective <span class="hlt">zone</span> to the outer atmospheric layers through computation of <span class="hlt">wave</span> propagation and dissipation in highly nonhomogeneous solar atmosphere. These <span class="hlt">waves</span> may efficiently heat the solar atmosphere and the heating will be especially significant in the chromospheric network. It is also shown that the role played by Alfven <span class="hlt">waves</span> in solar wind acceleration and coronal hole heating is dominant. The second part of the project concerned investigation of <span class="hlt">wave</span> propagation in highly inhomogeneous stellar atmospheres using an approach based on an analytic tool developed by Musielak, Fontenla, and Moore. In addition, a new technique based on Dirac equations has been developed to investigate coupling between different MHD <span class="hlt">waves</span> propagating in stratified stellar atmospheres.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.3737H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.3737H"><span>Observations and Simulations of the Impact of <span class="hlt">Wave</span>-Current Interaction on <span class="hlt">Wave</span> Direction in the Surf <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hopkins, Julia; Elgar, Steve; Raubenheimer, Britt</p> <p>2017-04-01</p> <p>Accurately characterizing the interaction of <span class="hlt">waves</span> and currents can improve predictions of <span class="hlt">wave</span> propagation and subsequent sediment transport in the nearshore. Along the southern shoreline of Martha's Vineyard, MA, <span class="hlt">waves</span> propagate across strong tidal currents as they shoal, providing an ideal environment for investigating <span class="hlt">wave</span>-current interaction. <span class="hlt">Wave</span> directions and mean currents observed for two 1-month-long periods in 7- and 2-m water depths along 11 km of the Martha's Vineyard shoreline have strong tidal modulations. <span class="hlt">Wave</span> directions shift by as much as 70 degrees over a tidal cycle in 7 m depth, and by as much as 25 degrees in 2 m depth. The magnitude of the tidal modulations in the <span class="hlt">wave</span> field decreases alongshore to the west, consistent with the observed decrease in tidal currents from 2.1 to 0.2 m/s. The observations are reproduced accurately by a numerical model (SWAN and Deflt3D-FLOW) that simulates <span class="hlt">waves</span> and currents over the observed bathymetry. Model simulations with and without <span class="hlt">wave</span>-current interaction and tidal depth changes demonstrate that the observed tidal modulations of the <span class="hlt">wave</span> field primarily are caused by <span class="hlt">wave</span>-current interaction and not by tidal changes to water depths over the nearby complex shoals. Sediment transport estimates from simulated <span class="hlt">wave</span> conditions using a range of tidal currents and offshore <span class="hlt">wave</span> fields indicate that the modulation of the <span class="hlt">wave</span> field at Martha's Vineyard can impact the direction of <span class="hlt">wave</span>-induced alongshore sediment transport, sometimes driving transport opposing the direction of the offshore incident <span class="hlt">wave</span> field. As such, the observations and model simulations suggest the importance of <span class="hlt">wave</span>-current interaction to tidally averaged transport in mixed-energy <span class="hlt">wave</span>-and-current nearshore environments. Supported by ASD(R&E), NSF, NOAA (Sea Grant), and ONR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911079J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911079J"><span>Shoreline-crossing shear-velocity structure of the Juan de Fuca plate and Cascadia subduction <span class="hlt">zone</span> from surface <span class="hlt">waves</span> and receiver functions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Janiszewski, Helen; Gaherty, James; Abers, Geoffrey; Gao, Haiying</p> <p>2017-04-01</p> <p>The Cascadia subduction <span class="hlt">zone</span> (CSZ) is the site of the onshore-offshore Cascadia Initiative, which deployed seismometers extending from the Juan de Fuca ridge to the subduction <span class="hlt">zone</span> and onshore beyond the volcanic arc. This array allows the unique opportunity to seismically image the evolution and along-strike variation of the crust and mantle of the entire CSZ. We compare teleseismic receiver functions, ambient-noise Rayleigh-<span class="hlt">wave</span> phase velocities in the 10-20 s period band, and earthquake-source Rayleigh-<span class="hlt">wave</span> phase velocities from 20-100 s, to determine shear-velocity structure in the upper 200 km. Receiver functions from both onshore and shallow-water offshore sites provide constraints on crustal and plate interface structure. Spectral-domain fitting of ambient-noise empirical Green's functions constrains shear velocity of the crust and shallow mantle. An automated multi-channel cross-correlation analysis of teleseismic Rayleigh <span class="hlt">waves</span> provides deeper lithosphere and asthenosphere constraints. The amphibious nature of the array means it is essential to examine the effect of noise variability on data quality. Ocean bottom seismometers (OBS) are affected by tilt and compliance noise. Removal of this noise from the vertical components of the OBS is essential for the teleseismic Rayleigh <span class="hlt">waves</span>; this stabilizes the output phase velocity maps particularly along the coastline where observations are predominately from shallow water OBS. Our noise-corrected phase velocity maps reflect major structures and tectonic transitions including the transition from high-velocity oceanic lithosphere to low-velocity continental lithosphere, high velocities associated with the subducting slab, and low velocities beneath the ridge and arc. We interpret the resulting shear-velocity model in the context of temperature and compositional variation in the incoming plate and along the strike of the CSZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T31D2944J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T31D2944J"><span>Shoreline-Crossing Shear-Velocity Structure of the Juan de Fuca Plate and Cascadia Subduction <span class="hlt">Zone</span> from Surface <span class="hlt">Waves</span> and Receiver Functions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Janiszewski, H. A.; Gaherty, J. B.; Abers, G. A.; Gao, H.</p> <p>2016-12-01</p> <p>The Cascadia subduction <span class="hlt">zone</span> (CSZ) is the site of the onshore-offshore Cascadia Initiative, which deployed seismometers extending from the Juan de Fuca ridge to the subduction <span class="hlt">zone</span> and onshore beyond the volcanic arc. This array allows the unique opportunity to seismically image the evolution and along-strike variation of the crust and mantle of the entire CSZ. We compare teleseismic receiver functions, ambient-noise Rayleigh-<span class="hlt">wave</span> phase velocities in the 10-20 s period band, and earthquake-source Rayleigh-<span class="hlt">wave</span> phase velocities from 20-100 s, to determine shear-velocity structure in the upper 200 km. Receiver functions from both onshore and shallow-water offshore sites provide constraints on crustal and plate interface structure. Spectral-domain fitting of ambient-noise empirical Green's functions constrains shear velocity of the crust and shallow mantle. An automated multi-channel cross-correlation analysis of teleseismic Rayleigh <span class="hlt">waves</span> provides deeper lithosphere and asthenosphere constraints. The amphibious nature of the array means it is essential to examine the effect of noise variability on data quality. Ocean bottom seismometers (OBS) are affected by tilt and compliance noise. Removal of this noise from the vertical components of the OBS is essential for the teleseismic Rayleigh <span class="hlt">waves</span>; this stabilizes the output phase velocity maps particularly along the coastline where observations are predominately from shallow water OBS. Our noise-corrected phase velocity maps reflect major structures and tectonic transitions including the transition from high-velocity oceanic lithosphere to low-velocity continental lithosphere, high velocities associated with the subducting slab, and low velocities beneath the ridge and arc. We interpret the resulting shear-velocity model in the context of temperature and compositional variation in the incoming plate and along the strike of the CSZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..171a2065D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..171a2065D"><span>Investigation of the effect of a bend in a transfer line that separates a pulse tube cold <span class="hlt">head</span> and a pressure <span class="hlt">wave</span> generator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dev, A. A.; Atrey, M. D.; Vanapalli, S.</p> <p>2017-02-01</p> <p>A transfer line between a pulse tube cold <span class="hlt">head</span> and a pressure <span class="hlt">wave</span> generator is usually required to isolate the cold <span class="hlt">head</span> from the vibrations of the compressor. Although it is a common practice to use a thin and narrow straight tube, a bent tube would allow design flexibility and easy mounting of the cold <span class="hlt">head</span>, such as in a split Stirling type pulse tube cryocooler. In this paper, we report a preliminary investigation on the effect of the bending of the tube on the flow transfer characteristics. A numerical study using commercial computational fluid dynamics model is performed to gain insight into the flow characteristics in the bent tube. Oscillating flow experiments are performed with a straight and a bent tube at a filling pressure of 15 bar and an operating frequency of 40, 50 and 60 Hz. The data and the corresponding numerical simulations point to the hypothesis that the secondary flow in the bent tube causes a decrease in flow at a fixed pressure amplitude.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010fgcn.conf...11R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010fgcn.conf...11R"><span>An Efficient Method for Detecting Misbehaving <span class="hlt">Zone</span> Manager in MANET</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rafsanjani, Marjan Kuchaki; Pakzad, Farzaneh; Asadinia, Sanaz</p> <p></p> <p>In recent years, one of the wireless technologies increased tremendously is mobile ad hoc networks (MANETs) in which mobile nodes organize themselves without the help of any predefined infrastructure. MANETs are highly vulnerable to attack due to the open medium, dynamically changing network topology, cooperative algorithms, lack of centralized monitoring, management point and lack of a clear defense line. In this paper, we report our progress in developing intrusion detection (ID) capabilities for MANET. In our proposed scheme, the network with distributed hierarchical architecture is partitioned into <span class="hlt">zones</span>, so that in each of them there is one <span class="hlt">zone</span> manager. The <span class="hlt">zone</span> manager is responsible for monitoring the cluster <span class="hlt">heads</span> in its <span class="hlt">zone</span> and cluster <span class="hlt">heads</span> are in charge of monitoring their members. However, the most important problem is how the trustworthiness of the <span class="hlt">zone</span> manager can be recognized. So, we propose a scheme in which "honest neighbors" of <span class="hlt">zone</span> manager specify the validation of their <span class="hlt">zone</span> manager. These honest neighbors prevent false accusations and also allow manager if it is wrongly misbehaving. However, if the manger repeats its misbehavior, then it will lose its management degree. Therefore, our scheme will be improved intrusion detection and also provide a more reliable network.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6883T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6883T"><span>Upper crustal structure of the North Anatolian Fault <span class="hlt">Zone</span> from ambient seismic noise Rayleigh and Love <span class="hlt">wave</span> tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Taylor, George; Rost, Sebastian; Houseman, Gregory; Hillers, Gregor</p> <p>2017-04-01</p> <p>By utilising short period surface <span class="hlt">waves</span> present in the noise field, we can construct images of shallow structure in the Earth's upper crust: a region that is usually poorly resolved in earthquake tomography. Here, we use data from a dense seismic array (Dense Array for Northern Anatolia - DANA) deployed across the North Anatolian Fault <span class="hlt">Zone</span> (NAFZ) in the region of the 1999 magnitude 7.6 Izmit earthquake in western Turkey. The NAFZ is a major strike-slip system that extends ˜1200 km across northern Turkey and continues to pose a high level of seismic hazard, in particular to the mega-city of Istanbul. We obtain maps of group velocity variation using surface <span class="hlt">wave</span> tomography applied to short period (1- 6 s) Rayleigh and Love <span class="hlt">waves</span> to construct high-resolution images of the upper 5 km of a 70 km x 35 km region centred on the eastern end of the fault segment that ruptured in the 1999 Izmit earthquake. The average Rayleigh <span class="hlt">wave</span> group velocities in the region vary between 1.8 km/s at 1.5 s period, to 2.2 km/s at 6 s period. The NAFZ bifurcates into northern and southern strands in this region; both are active but only the northern strand moved in the 1999 event. The signatures of both the northern and southern branches of the NAFZ are clearly associated with strong gradients in surface <span class="hlt">wave</span> group velocity. To the north of the NAFZ, we observe low Rayleigh <span class="hlt">wave</span> group velocities ( 1.2 km/s) associated with the unconsolidated sediments of the Adapazari basin, and blocks of weathered terrigenous clastic sediments. To the south of the northern branch of the NAFZ, we detect high velocities ( 2.5 km/s) associated with a shallow crystalline basement, in particular a block of metamorphosed schists and marbles that bound the northern branch of the NAFZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25096095','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25096095"><span>Reconstructing surface <span class="hlt">wave</span> profiles from reflected acoustic pulses using multiple receivers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Walstead, Sean P; Deane, Grant B</p> <p>2014-08-01</p> <p>Surface <span class="hlt">wave</span> shapes are determined by analyzing underwater reflected acoustic signals collected at multiple receivers. The transmitted signals are of nominal frequency 300 kHz and are reflected off surface gravity <span class="hlt">waves</span> that are paddle-generated in a <span class="hlt">wave</span> tank. An inverse processing algorithm reconstructs 50 surface <span class="hlt">wave</span> shapes over a length span of 2.10 m. The inverse scheme uses a broadband forward scattering model based on Kirchhoff's diffraction formula to determine <span class="hlt">wave</span> shapes. The surface reconstruction algorithm is self-starting in that source and receiver geometry and initial estimates of <span class="hlt">wave</span> shape are determined from the same acoustic signals used in the inverse processing. A high speed camera provides ground-truth measurements of the surface <span class="hlt">wave</span> field for comparison with the acoustically derived surface <span class="hlt">waves</span>. Within Fresnel <span class="hlt">zone</span> regions the statistical confidence of the inversely optimized surface profile exceeds that of the camera profile. Reconstructed surfaces are accurate to a resolution of about a quarter-wavelength of the acoustic pulse only within Fresnel <span class="hlt">zones</span> associated with each source and receiver pair. Multiple isolated Fresnel <span class="hlt">zones</span> from multiple receivers extend the spatial extent of accurate surface reconstruction while overlapping Fresnel <span class="hlt">zones</span> increase confidence in the optimized profiles there.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GMS...216..121M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GMS...216..121M"><span>Relationship between Alfvén <span class="hlt">Wave</span> and Quasi-Static Acceleration in Earth's Auroral <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mottez, Fabrice</p> <p>2016-02-01</p> <p>There are two main categories of acceleration processes in the Earth's auroral <span class="hlt">zone</span>: those based on quasi-static structures, and those based on Alfvén <span class="hlt">wave</span> (AW). AWs play a nonnegligible role in the global energy budget of the plasma surrounding the Earth because they participate in auroral acceleration, and because auroral acceleration conveys a large portion of the energy flux across the magnetosphere. Acceleration events by double layers (DLs) and by AW have mostly been investigated separately, but many studies cited in this chapter show that they are not independent: these processes can occur simultaneously, and one process can be the cause of the other. The quasi-simultaneous occurrences of acceleration by AW and by quasi-static structures have been observed predominantly at the polar cap boundary of auroral arc systems, where often new bright arcs develop or intensify.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028283','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028283"><span>The Olmsted fault <span class="hlt">zone</span>, southernmost Illinois: A key to understanding seismic hazard in the northern new Madrid seismic <span class="hlt">zone</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>Bexfield, C.E.; McBride, J.H.; Pugin, Andre J.M.; Nelson, W.J.; Larson, T.H.; Sargent, S.L.</p> <p>2005-01-01</p> <p>Geological deformation in the northern New Madrid seismic <span class="hlt">zone</span>, near Olmsted, Illinois (USA), is analyzed using integrated compressional-<span class="hlt">wave</span> (P) and horizontally polarized-<span class="hlt">wave</span> (SH) seismic reflection and regional and dedicated borehole information. Seismic hazards are of special concern because of strategic facilities (e.g., lock and dam sites and chemical plants on the Ohio River near its confluence with the Mississippi River) and because of alluvial soils subject to high amplification of earthquake shock. We use an integrated approach starting with lower resolution, but deeper penetration, P-<span class="hlt">wave</span> reflection profiles to identify displacement of Paleozoic bedrock. Higher resolution, but shallower penetration, SH-<span class="hlt">wave</span> images show deformation that has propagated upward from bedrock faults into Pleistocene loess. We have mapped an intricate <span class="hlt">zone</span> more than 8 km wide of high-angle faults in Mississippi embayment sediments localized over Paleozoic bedrock faults that trend north to northeast, parallel to the Ohio River. These faults align with the pattern of epicenters in the New Madrid seismic <span class="hlt">zone</span>. Normal and reverse offsets along with positive flower structures imply a component of strike-slip; the current stress regime favors right-lateral slip on northeast-trending faults. The largest fault, the Olmsted fault, underwent principal displacement near the end of the Cretaceous Period 65 to 70 million years ago. Strata of this age (dated via fossil pollen) thicken greatly on the downthrown side of the Olmsted fault into a locally subsiding basin. Small offsets of Tertiary and Quaternary strata are evident on high-resolution SH-<span class="hlt">wave</span> seismic profiles. Our results imply recent reactivation and possible future seismic activity in a critical area of the New Madrid seismic <span class="hlt">zone</span>. This integrated approach provides a strategy for evaluating shallow seismic hazard-related targets for engineering concerns. ?? 2005 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29732525','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29732525"><span>An efficient use of mixing model for computing the effective dielectric and thermal properties of the human <span class="hlt">head</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mishra, Varsha; Puthucheri, Smitha; Singh, Dharmendra</p> <p>2018-05-07</p> <p>As a preventive measure against the electromagnetic (EM) <span class="hlt">wave</span> exposure to human body, EM radiation regulatory authorities such as ICNIRP and FCC defined the value of specific absorption rate (SAR) for the human <span class="hlt">head</span> during EM <span class="hlt">wave</span> exposure from mobile phone. SAR quantifies the absorption of EM <span class="hlt">waves</span> in the human body and it mainly depends on the dielectric properties (ε', σ) of the corresponding tissues. The <span class="hlt">head</span> part of the human body is more susceptible to EM <span class="hlt">wave</span> exposure due to the usage of mobile phones. The human <span class="hlt">head</span> is a complex structure made up of multiple tissues with intermixing of many layers; thus, the accurate measurement of permittivity (ε') and conductivity (σ) of the tissues of the human <span class="hlt">head</span> is still a challenge. For computing the SAR, researchers are using multilayer model, which has some challenges for defining the boundary for layers. Therefore, in this paper, an attempt has been made to propose a method to compute effective complex permittivity of the human <span class="hlt">head</span> in the range of 0.3 to 3.0 GHz by applying De-Loor mixing model. Similarly, for defining the thermal effect in the tissue, thermal properties of the human <span class="hlt">head</span> have also been computed using the De-Loor mixing method. The effective dielectric and thermal properties of equivalent human <span class="hlt">head</span> model are compared with the IEEE Std. 1528. Graphical abstract ᅟ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S42B..03E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S42B..03E"><span>Remote Love <span class="hlt">Wave</span> Triggering of Tremor in the Nankai Subduction <span class="hlt">Zone</span>: New Observations and Dynamic Stress Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Enescu, B.; Chao, K.; Obara, K.; Peng, Z.; Matsuzawa, T.; Yagi, Y.</p> <p>2013-12-01</p> <p>The triggering of deep non-volcanic tremor (NVT) in the Nankai region, southwest Japan, by the surface <span class="hlt">waves</span> of several large teleseismic earthquakes has been well documented (e.g., Miyazawa & Mori, 2005). These previous studies report that the Nankai NVT is primarily triggered by the passage of Rayleigh <span class="hlt">waves</span> from the teleseismic events (e.g., Miyazawa & Brodsky, 2008). The relative lack of Love <span class="hlt">wave</span> triggering in Nankai would be, however, an exception to the general observation that triggered tremor shows a positive correlation with the triggering potential, defined using the Coulomb failure criteria (Hill, 2012). To clarify the Nankai NVT triggering mechanism, we have systematically searched for triggered tremor due to large teleseismic events (Mw ≥ 7.5) occurred from 2001 to 2012. Our present analysis focuses on western Shikoku, where triggered NVT has been previously reported (e.g., Miyazawa & Mori, 2006). From a total of 55 teleseismic events, 18 show associated triggered NVT. Our analysis presents clear evidence of triggered NVT that correlates well with the passage of Love <span class="hlt">waves</span>. The most outstanding example is that of the 2012 M8.6 Sumatra earthquake, a strike-slip event characterized by relatively large amplitude Love <span class="hlt">waves</span>. The incoming surface <span class="hlt">waves</span> from this earthquake are almost strike-parallel to the Nankai subduction <span class="hlt">zone</span>, which corresponds to a higher Love <span class="hlt">wave</span> triggering potential (Hill, 2012). The 2001 M7.8 Kunlun, the 2003 M8.3 Tokachi-oki, the 2004 M9.2 & 2007 M8.5 Sumatra, the 2006 M8.3 Kuril-Islands and the 2008 M7.9 Wenchuan earthquakes show as well Love-<span class="hlt">wave</span> associated NVT triggering. In most of these cases the tremor is initiated by the incoming, faster-traveling Love <span class="hlt">waves</span> and continues during the latter, larger-amplitude Rayleigh <span class="hlt">waves</span>. We are also conducting dynamic stress modeling to better understand the triggering mechanism of tremor. Our approach builds up on the methods of Gonzalez-Huizar & Velasco (2011) and Obara (2012). In the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000GeoRL..27..827O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000GeoRL..27..827O"><span>Mantle transition <span class="hlt">zone</span> structure beneath Tanzania, east Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Owens, Thomas J.; Nyblade, Andrew A.; Gurrola, Harold; Langston, Charles A.</p> <p>2000-03-01</p> <p>We apply a three-dimensional stacking method to receiver functions from the Tanzania Broadband Seismic Experiment to determine relative variations in the thickness of the mantle transition <span class="hlt">zone</span> beneath Tanzania. The transition <span class="hlt">zone</span> under the Eastern rift is 30-40 km thinner than under areas of the Tanzania Craton in the interior of the East African Plateau unaffected by rift faulting. The region of transition <span class="hlt">zone</span> thinning under the Eastern rift is several hundred kilometers wide and coincides with a 2-3% reduction in S <span class="hlt">wave</span> velocities. The thinning of the transition <span class="hlt">zone</span>, as well as the reduction in S <span class="hlt">wave</span> velocities, can be attributed to a 200-300°K increase in temperature. This thermal anomaly at >400 km depth beneath the Eastern rift cannot be easily explained by passive rifting and but is consistent with a plume origin for the Cenozoic rifting, volcanism and plateau uplift in East Africa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T51C2936G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T51C2936G"><span>Inferences of Complex Anisotropic Layering and Mantle Flow Beneath the Malawi Rift <span class="hlt">Zone</span> from Shear-<span class="hlt">Wave</span> Splitting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gao, S. S.; Reed, C. A.; Yu, Y.; Liu, K. H.; Chindandali, P. R. N.; Mdala, H. S.; Massinque, B.; Mutamina, D. M.</p> <p>2016-12-01</p> <p>Measuring the magnitude and orientation of seismic anisotropy beneath actively extending rift <span class="hlt">zones</span> provides invaluable estimates of the influence of numerous geodynamic parameters upon their evolution. In order to infer the character and origin of extensional forces acting upon the Malawi Rift <span class="hlt">Zone</span> (MRZ) and Luangwa Rift <span class="hlt">Zone</span> (LRZ) of southern Africa, we installed 33 Seismic Arrays For African Rift Initiation (SAFARI) three-component broadband seismic stations in Malawi, Mozambique, and Zambia between 2012-2014. Shear-<span class="hlt">wave</span> splitting parameters, including the fast-component polarization orientation and the splitting time, are extracted from 142 events recorded during that time period for a total of 642 well-defined PKS, SKKS, and SKS phase measurements. Polarizations trend NE-SW along the western flank of the LRZ, whereupon they demonstrate an abrupt shift to N-S within the rift valley and the eastern flank. SWS orientations shift increasingly counterclockwise toward the east until, at 33°E, they shift from WNW-ESE to ENE-WSW, suggesting a systematic change in dominant mantle fabric orientation. The resulting fast orientations demonstrate remarkable variability within the MRZ, with E-W measurements in the north rotating counterclockwise toward the south to N-S within the southernmost MRZ. Measurements revert to E-W and NE-SW orientations toward the east in Mozambique, suggesting the presence of complex two-layer anisotropy. Azimuthal variations of SWS parameters recorded by stations within the central MRZ exhibit excellent 90° periodicity, further suggesting complex anisotropic layering. Lateral variation of measurements between the northern and southern MRZ imply the modulation of the mantle flow system beneath the active rift <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JGR...104.7329I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JGR...104.7329I"><span>Excitation of high-frequency surface <span class="hlt">waves</span> with long duration in the Valley of Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iida, Masahiro</p> <p>1999-04-01</p> <p>During the 1985 Michoacan earthquake (Ms = 8.1), large-amplitude seismograms with extremely long duration were recorded in the lake bed <span class="hlt">zone</span> of Mexico City. We interpret high-frequency seismic <span class="hlt">wave</span> fields in the three geotechnical <span class="hlt">zones</span> (the hill, the transition, and the lake bed <span class="hlt">zones</span>) in the Valley of Mexico on the basis of a systematic analysis for borehole strong motion recordings. We make identification of <span class="hlt">wave</span> types for real seismograms. First, amplitude ratios between surface and underground seismograms indicate that predominant periods of the surface seismograms are largely controlled by the <span class="hlt">wave</span> field incident into surficial layers in the Valley of Mexico. We interpret recorded surface <span class="hlt">waves</span> as fundamental-mode Love <span class="hlt">waves</span> excited in the Mexican Volcanic Belt by calculating theoretical amplification for different-scale structures. Second, according to a cross-correlation analysis, the hill and transition seismograms are mostly surface <span class="hlt">waves</span>. In the lake bed <span class="hlt">zone</span>, while early portions are noisy body <span class="hlt">waves</span>, late portions are mostly surface <span class="hlt">waves</span>. Third, using two kinds of surface arrays with different station intervals, we investigate high-frequency surface-<span class="hlt">wave</span> propagation in the lake bed <span class="hlt">zone</span>. The <span class="hlt">wave</span> propagation is very complicated, depending upon the time section and the frequency band. Finally, on the basis of a statistical time series model with an information criterion, we separate S- and surface-<span class="hlt">wave</span> portions from lake bed seismograms. Surface <span class="hlt">waves</span> are dominant and are recognized even in the early time section. Thus high-frequency surface <span class="hlt">waves</span> with long duration in the Valley of Mexico are excited by the Mexican Volcanic Belt.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OGeo....9...37S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OGeo....9...37S"><span>Coda <span class="hlt">Wave</span> Attenuation Characteristics for North Anatolian Fault <span class="hlt">Zone</span>, Turkey</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sertcelik, Fadime; Guleroglu, Mehmet</p> <p>2017-10-01</p> <p>North Anatolian Fault <span class="hlt">Zone</span>, on which large earthquakes have occurred in the past, migrates regularly from east to west, and it is one of the most active faults in the world. The purpose of this study is to estimate the coda <span class="hlt">wave</span> quality factor (Qc) for each of the five sub regionsthat were determined according to the fault rupture of these large earthquakes and along the fault. 978 records have been analyzed for 1.5, 3, 6, 9, 12 and 18 Hz frequencies by Single Backscattering Method. Along the fault, the variations in the Qc with lapse time are determined via, Qc = (136±25)f(0.96±0.027), Qc = (208±22)f(0.85±0.02) Qc = (307±28)f(0.72±0.025) at 20, 30, 40 sec lapse times, respectively. The estimated average frequency-dependence quality factor for all lapse time are; Qc(f) = (189±26)f(0.86±0.02) for Karliova-Tokat region; Qc(f) = (216±19)f(0.76±0.018) for Tokat-Çorum region; Qc(f) = (232±18)f(0.76±0.019) for Çorum-Adapazari region; Qc(f) = (280±28)f(0.79±0.021) for Adapazari-Yalova region; Qc(f) = (252±26)f(0.81±0.022) for Yalova-Gulf of Saros region. The coda <span class="hlt">wave</span> quality factor at all the lapse times and frequencies is Qc(f) = (206±15)f(0.85±0.012) in the study area. The most change of Qc with lapse time is determined at Yalova-Saros region. The result may be related to heterogeneity degree of rapidly decreases towards the deep crust like compared to the other sub region. Moreover, the highest Qc is calculated between Adapazari - Yalova. It was interpreted as a result of seismic energy released by 1999 Kocaeli Earthquake. Besides, it couldn't be established a causal relationship between the regional variation of Qc with frequency and lapse time associated to migration of the big earthquakes. These results have been interpreted as the attenuation mechanism is affected by both regional heterogeneity and consist of a single or multi strands of the fault structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22271317-zoned-near-zero-refractive-index-fishnet-lens-antenna-steering-millimeter-waves','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22271317-zoned-near-zero-refractive-index-fishnet-lens-antenna-steering-millimeter-waves"><span><span class="hlt">Zoned</span> near-zero refractive index fishnet lens antenna: Steering millimeter <span class="hlt">waves</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>Pacheco-Peña, V., E-mail: victor.pacheco@unavarra.es; Orazbayev, B., E-mail: b.orazbayev@unavarra.es; Beaskoetxea, U., E-mail: unai.beaskoetxea@unavarra.es</p> <p>2014-03-28</p> <p>A <span class="hlt">zoned</span> fishnet metamaterial lens is designed, fabricated, and experimentally demonstrated at millimeter wavelengths to work as a negative near-zero refractive index lens suitable for compact lens antenna configurations. At the design frequency f = 56.7 GHz (λ{sub 0} = 5.29 mm), the <span class="hlt">zoned</span> fishnet metamaterial lens, designed to have a focal length FL = 9λ{sub 0}, exhibits a refractive index n = −0.25. The focusing performance of the diffractive optical element is briefly compared with that of a non-<span class="hlt">zoned</span> fishnet metamaterial lens and an isotropic homogeneous <span class="hlt">zoned</span> lens made of a material with the same refractive index. Experimental and numerically-computed radiation diagrams of the fabricated <span class="hlt">zoned</span> lens are presentedmore » and compared in detail with that of a simulated non-<span class="hlt">zoned</span> lens. Simulation and experimental results are in good agreement, demonstrating an enhancement generated by the <span class="hlt">zoned</span> lens of 10.7 dB, corresponding to a gain of 12.26 dB. Moreover, beam steering capability of the structure by shifting the feeder on the xz-plane is demonstrated.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870040136&hterms=midi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmidi','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870040136&hterms=midi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmidi"><span>Nonlinear density <span class="hlt">waves</span> in planetary rings</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borderies, Nicole; Goldreich, Peter; Tremaine, Scott</p> <p>1986-01-01</p> <p>The steady-state structure of planetary rings in the presence of density <span class="hlt">waves</span> at the Lindblad resonances of a satellite is indicated. The study is based on the dispersion relation and damping rate for nonlinear density <span class="hlt">waves</span>, derived by Shu et al. (1985) and by Borderies, Goldreich, and Tremaine (1985). It is shown that strong density <span class="hlt">waves</span> lead to an enhancement of the background surface density in the <span class="hlt">wave</span> <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3666475','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3666475"><span>Short-term effectiveness of bi-phase oscillatory <span class="hlt">waves</span> versus hyperthermia for isolated long <span class="hlt">head</span> biceps tendinopathy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Oliva, Francesco; Via, Alessio Giai; Rossi, Silvio</p> <p>2011-01-01</p> <p>Summary Introduction: Long <span class="hlt">head</span> biceps (LHB) tendinopathy is a common cause of anterior shoulder pain. Isolated LHB pathology is most common among younger people who practise overhead sports. The authors conducted a short-term prospective randomised study to test the effectiveness of two different methods for the treatment of isolated LHB tendinopathy: biphasic oscillatory <span class="hlt">waves</span> and hyperthermia. Study design: The study is a prospective randomised study (Level II). Material and methods: The authors identified 20 patients who had clinical and ultrasound (US) evidence of LHB tendinopathy. No patient was a high-level athlete. The patients were randomly assigned to two groups. Group A (10 patients) was treated with bi-phasic oscillatory <span class="hlt">waves</span>, while Group B received hyperthermia. During the treatment period, no other electromedical therapy, injections with corticosteroids, oral analgesics or nonsteroidal anti-inflammatory drugs were allowed. All the patients were assessed at baseline (T0), immediately after the end of the treatment period (T1) and 6 months after the end of treatment (T2) using a visual analogic scale (VAS) and Constant-Murley Score (CMS). Furthermore, all patients underwent US examinations at T0 and at T1. All the US examinations were performed by the same radiologist. Results: The VAS scores showed a highly statistically significant reduction of pain at T1 both in Group A (65%; p=0,004) and in Group B (50%; p=0,0002). The CMS also showed a statistically significant improvement between the pre-intervention, the post-treatment and the short-term follow-up in both groups. In addition, the peritendinous fluid evident on US examination at T0 was no longer present in all cases at T1. Conclusion: These findings suggest that both bi-phasic oscillatory <span class="hlt">waves</span> and hyperthermia are able to relieve pain in patients with isolated LHB tendinopathy. This is a Class II level of evidence. PMID:23738257</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5126218-morphology-auroral-zone-radio-wave-scintillation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5126218-morphology-auroral-zone-radio-wave-scintillation"><span>Morphology of auroral <span class="hlt">zone</span> radio <span class="hlt">wave</span> scintillation</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>Rino, C.L.; Matthews, S.J.</p> <p>1980-08-01</p> <p>This paper describes the morphology of midnight sector and morning sector auroral <span class="hlt">zone</span> scintillation observations made over a two-year period using the Wideband satelite, which is in a sun-synchronous, low-altitude orbit. No definitive seasonal variation was found. The nighttime data showed the highest scintillation ocurrence levels, but significant amounts of morning scintillation were observed. For the most part the scintillation activity followed the general pattern of local magnetic activity. The most prominent feature in the nightime data is a localized amplitude and phase scintillation enhancement at the point where the propagation vector lies within an L shell. A geometrical effectmore » due to a dynamic slab of sheetlike structures in the F region is hypothesized as the source of his enhancement. The data have been sorted by magnetic activity, proximity to local midnight, and season. The general features of the data are in agreement with the accepted morphology of auroral <span class="hlt">zone</span> scintillation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMDI51C0333H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMDI51C0333H"><span>Teleseismic P-<span class="hlt">wave</span> tomography of the Sunda-Banda Arc subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harris, C. W.; Miller, M. S.; Widiyantoro, S.; Supendi, P.; O'Driscoll, L.; Roosmawati, N.; Porritt, R.</p> <p>2017-12-01</p> <p>The Sunda-Banda Arc is the site of multiple ongoing tectonic deformation processes and is perhaps the best example of the transition from subduction of oceanic lithosphere to an active arc-continent collision. Investigating the mantle structure that has resulted from the collision of continental Australia, as well as the concurrent phenomena of continental subduction, slab-rollback, lithospheric tearing, and subduction polarity reversal is possible through seismic tomography. While both regional scale and global tomographic models have previously been constructed to study the tectonics this region, here we use 250 seismic stations that span the length of this convergent margin to invert for P-<span class="hlt">wave</span> velocity perturbations in the upper mantle. We combine data from a temporary deployment of 30 broadband instruments as part of the NSF-funded Banda Arc Project, along with data from permanent broadband stations maintained by the Meteorological, Climatological, and Geophysical Agency of Indonesia (BMKG) to image mantle structure, in particular the subducted Indo-Australian plate. The BMKG dataset spans 2009-2017 and includes >200 broadband seismometers. The Banda Arc array (network YS) adds coverage and resolution to southeastern Indonesia and Timor-Leste, where few permanent seismometers are located but the Australian continent-Banda Arc collision is most advanced. The preliminary model was computed using 50,000 teleseismic P-<span class="hlt">wave</span> travel-time residuals and 3D finite frequency sensitivity kernels. Results from the inversion of the combined dataset are presented as well as resolution tests to assess the quality of the model. The velocity model shows an arcuate Sunda-Banda slab with morphological changes along strike that correlate with the tectonic collision. The model also features the double-sided Molucca Sea slab and regions of high velocity below the bottom of the transition <span class="hlt">zone</span>. The resolution added by the targeted USC deployment is clear when comparing models that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011SPIE.8205E..1LX','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011SPIE.8205E..1LX"><span>Study on compensation algorithm of <span class="hlt">head</span> skew in hard disk drives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, Yong; Ge, Xiaoyu; Sun, Jingna; Wang, Xiaoyan</p> <p>2011-10-01</p> <p>In hard disk drives (HDDs), <span class="hlt">head</span> skew among multiple <span class="hlt">heads</span> is pre-calibrated during manufacturing process. In real applications with high capacity of storage, the <span class="hlt">head</span> stack may be tilted due to environmental change, resulting in additional <span class="hlt">head</span> skew errors from outer diameter (OD) to inner diameter (ID). In case these errors are below the preset threshold for power on recalibration, the current strategy may not be aware, and drive performance under severe environment will be degraded. In this paper, in-the-field compensation of small DC <span class="hlt">head</span> skew variation across stroke is proposed, where a <span class="hlt">zone</span> table has been equipped. Test results demonstrating its effectiveness to reduce observer error and to enhance drive performance via accurate prediction of DC <span class="hlt">head</span> skew are provided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE24A1441S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE24A1441S"><span>Ice Floe Breaking in Contemporary Third Generation Operational <span class="hlt">Wave</span> Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sévigny, C.; Baudry, J.; Gauthier, J. C.; Dumont, D.</p> <p>2016-02-01</p> <p>The dynamical <span class="hlt">zone</span> observed at the edge of the consolidated ice area where are found the <span class="hlt">wave</span>-fractured floes (i.e. marginal ice <span class="hlt">zone</span> or MIZ) has become an important topic in ocean modeling. As both operational and climate ocean models now seek to reproduce the complex atmosphere-ice-ocean system with realistic coupling processes, many theoretical and numerical studies have focused on understanding and modeling this <span class="hlt">zone</span>. Few attempts have been made to embed <span class="hlt">wave</span>-ice interactions specific to the MIZ within a two-dimensional model, giving the possibility to calculate both the attenuation of surface <span class="hlt">waves</span> by sea ice and the concomitant breaking of the sea ice-cover into smaller floes. One of the first challenges consists in improving the parameterization of <span class="hlt">wave</span>-ice dynamics in contemporary third generation operational <span class="hlt">wave</span> models. A simple <span class="hlt">waves</span>-in-ice model (WIM) similar to the one proposed by Williams et al. (2013a,b) was implemented in WAVEWATCH III. This WIM considers ice floes as floating elastic plates and predicts the dimensionless attenuation coefficient by the use of a lookup-table-based, <span class="hlt">wave</span> scattering scheme. As in Dumont et al. (2011), the different frequencies are treated individually and floe breaking occurs for a particular frequency when the expected <span class="hlt">wave</span> amplitude exceeds the allowed strain amplitude, which considers ice floes properties and wavelength in ice field. The model is here further refined and tested in idealized two-dimensional cases, giving preliminary results of the performance and sensitivity of the parameterization to initial <span class="hlt">wave</span> and ice conditions. The effects of the <span class="hlt">wave</span>-ice coupling over the incident <span class="hlt">wave</span> spectrum are analyzed as well as the resulting floe size distribution. The model gives prognostic values of the lateral extent of the marginal ice <span class="hlt">zone</span> with maximum ice floe diameter that progressively increases with distance from the ice edge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920024703','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920024703"><span>On the physics of <span class="hlt">waves</span> in the solar atmosphere: <span class="hlt">Wave</span> heating and wind acceleration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Musielak, Z. E.</p> <p>1992-01-01</p> <p>In the area of solar physics, new calculations of the acoustic <span class="hlt">wave</span> energy fluxes generated in the solar convective <span class="hlt">zone</span> was performed. The original theory developed was corrected by including a new frequency factor describing temporal variations of the turbulent energy spectrum. We have modified the original Stein code by including this new frequency factor, and tested the code extensively. Another possible source of the mechanical energy generated in the solar convective <span class="hlt">zone</span> is the excitation of magnetic flux tube <span class="hlt">waves</span> which can carry energy along the tubes far away from the region. The problem as to how efficiently those <span class="hlt">waves</span> are generated in the Sun was recently solved. The propagation of nonlinear magnetic tube <span class="hlt">waves</span> in the solar atmosphere was calculated, and mode coupling, shock formation, and heating of the local medium was studied. The <span class="hlt">wave</span> trapping problems and evaluation of critical frequencies for <span class="hlt">wave</span> reflection in the solar atmosphere was studied. It was shown that the role played by Alfven <span class="hlt">waves</span> in the wind accelerations and the coronal hole heating is dominant. Presently, we are performing calculations of <span class="hlt">wave</span> energy fluxes generated in late-type dwarf stars and studying physical processes responsible for the heating of stellar chromospheres and coronae. In the area of physics of <span class="hlt">waves</span>, a new analytical approach for studying linear Alfven <span class="hlt">waves</span> in smoothly nonuniform media was recently developed. This approach is presently being extended to study the propagation of linear and nonlinear magnetohydrodynamic (MHD) <span class="hlt">waves</span> in stratified, nonisothermal and solar atmosphere. The Lighthill theory of sound generation to nonisothermal media (with a special temperature distribution) was extended. Energy cascade by nonlinear MHD <span class="hlt">waves</span> and possible chaos driven by these <span class="hlt">waves</span> are presently considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMOS13D1224Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMOS13D1224Y"><span>Observation of <span class="hlt">wave</span> celerity evolution in the nearshore using digital video imagery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yoo, J.; Fritz, H. M.; Haas, K. A.; Work, P. A.; Barnes, C. F.; Cho, Y.</p> <p>2008-12-01</p> <p>Celerity of incident <span class="hlt">waves</span> in the nearshore is observed from oblique video imagery collected at Myrtle Beach, S.C.. The video camera covers the field view of length scales O(100) m. Celerity of <span class="hlt">waves</span> propagating in shallow water including the surf <span class="hlt">zone</span> is estimated by applying advanced image processing and analysis methods to the individual video images sampled at 3 Hz. Original image sequences are processed through video image frame differencing, directional low-pass image filtering to reduce the noise arising from foam in the surf <span class="hlt">zone</span>. The breaking <span class="hlt">wave</span> celerity is computed along a cross-shore transect from the <span class="hlt">wave</span> crest tracks extracted by a Radon transform-based line detection method. The observed celerity from the nearshore video imagery is larger than the linear <span class="hlt">wave</span> celerity computed from the measured water depths over the entire surf <span class="hlt">zone</span>. Compared to the nonlinear shallow water <span class="hlt">wave</span> equation (NSWE)-based celerity computed using the measured depths and <span class="hlt">wave</span> heights, in general, the video-based celerity shows good agreements over the surf <span class="hlt">zone</span> except the regions across the incipient <span class="hlt">wave</span> breaking locations. In the regions across the breaker points, the observed <span class="hlt">wave</span> celerity is even larger than the NSWE-based celerity due to the transition of <span class="hlt">wave</span> crest shapes. The observed celerity using the video imagery can be used to monitor the nearshore geometry through depth inversion based on the nonlinear <span class="hlt">wave</span> celerity theories. For this purpose, the exceeding celerity across the breaker points needs to be corrected accordingly compared to a nonlinear <span class="hlt">wave</span> celerity theory applied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNS23A0013L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNS23A0013L"><span>Sonic logging for detecting the excavation disturbed and fracture <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, Y. C.; Chang, Y. F.; Liu, J. W.; Tseng, C. W.</p> <p>2017-12-01</p> <p>This study presents a new sonic logging method to detect the excavation disturbed <span class="hlt">zone</span> (EDZ) and fracture <span class="hlt">zones</span> in a tunnel. The EDZ is a weak rock <span class="hlt">zone</span> where its properties and conditions have been changed by excavation, which results such as fracturing, stress redistribution and desaturation in this <span class="hlt">zone</span>. Thus, the EDZ is considered as a physically less stable and could form a continuous and high-permeable pathway for groundwater flow. Since EDZ and fracture <span class="hlt">zone</span> have the potential of affecting the safety of the underground openings and repository performance, many studies were conducted to characterize the EDZ and fracture <span class="hlt">zone</span> by different methods, such as the rock mass displacements and strain measurements, seismic refraction survey, seismic tomography and hydraulic test, etc. In this study, we designed a new sonic logging method to explore the EDZ and fracture <span class="hlt">zone</span> in a tunnel at eastern Taiwan. A high power and high frequency sonic system was set up which includes a two hydrophones pitch-catch technique with a common-offset immersed in water-filled uncased wells and producing a 20 KHz sound to scan the well rock. Four dominant sonic events were observed in the measurements, they are refracted P- and S-<span class="hlt">wave</span> along the well rock, direct water <span class="hlt">wave</span> and the reverberation in the well water. Thus the measured P- and S-<span class="hlt">wave</span> velocities, the signal-to-noise ratio of the refraction and the amplitudes of reverberation along the well rock were used as indexes to determine the EDZ and fracture <span class="hlt">zone</span>. Comparing these indexes with core samples shows that significant changes in the indexes are consistent with the EDZ and fracture <span class="hlt">zone</span>. Thus, the EDZ and fracture <span class="hlt">zone</span> can be detected by this new sonic method conclusively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022359','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022359"><span>Fracture process <span class="hlt">zone</span> in granite</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zang, A.; Wagner, F.C.; Stanchits, S.; Janssen, C.; Dresen, G.</p> <p>2000-01-01</p> <p>In uniaxial compression tests performed on Aue granite cores (diameter 50 mm, length 100 mm), a steel loading plate was used to induce the formation of a discrete shear fracture. A <span class="hlt">zone</span> of distributed microcracks surrounds the tip of the propagating fracture. This process <span class="hlt">zone</span> is imaged by locating acoustic emission events using 12 piezoceramic sensors attached to the samples. Propagation velocity of the process <span class="hlt">zone</span> is varied by using the rate of acoustic emissions to control the applied axial force. The resulting velocities range from 2 mm/s in displacement-controlled tests to 2 ??m/s in tests controlled by acoustic emission rate. <span class="hlt">Wave</span> velocities and amplitudes are monitored during fault formation. P <span class="hlt">waves</span> transmitted through the approaching process <span class="hlt">zone</span> show a drop in amplitude of 26 dB, and ultrasonic velocities are reduced by 10%. The width of the process <span class="hlt">zone</span> is ???9 times the grain diameter inferred from acoustic data but is only 2 times the grain size from optical crack inspection. The process <span class="hlt">zone</span> of fast propagating fractures is wider than for slow ones. The density of microcracks and acoustic emissions increases approaching the main fracture. Shear displacement scales linearly with fracture length. Fault plane solutions from acoustic events show similar orientation of nodal planes on both sides of the shear fracture. The ratio of the process <span class="hlt">zone</span> width to the fault length in Aue granite ranges from 0.01 to 0.1 inferred from crack data and acoustic emissions, respectively. The fracture surface energy is estimated from microstructure analysis to be ???2 J. A lower bound estimate for the energy dissipated by acoustic events is 0.1 J. Copyright 2000 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15933416','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15933416"><span>Shock <span class="hlt">wave</span> treatment in medicine.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shrivastava, S K; Kailash</p> <p>2005-03-01</p> <p>Extracorporeal shock <span class="hlt">wave</span> therapy in orthopedics and traumatology is still a young therapy method. Since the last few years the development of shock <span class="hlt">wave</span> therapy has progressed rapidly. Shock <span class="hlt">waves</span> have changed the treatment of urolithiasis substantially. Today shock <span class="hlt">waves</span> are the first choice to treat kidney and urethral stones. Urology has long been the only medical field for shock <span class="hlt">waves</span> in medicine. Meanwhile shock <span class="hlt">waves</span> have been used in orthopedics and traumatology to treat insertion tendinitis, avascular necrosis of the <span class="hlt">head</span> of femur and other necrotic bone alterations. Another field of shock <span class="hlt">wave</span> application is the treatment of tendons, ligaments and bones on horses in veterinary medicine. In the present paper we discuss the basic theory and application of shock <span class="hlt">waves</span> and its history in medicine. The idea behind using shock <span class="hlt">wave</span> therapy for orthopedic diseases is the stimulation of healing in tendons, surrounding tissue and bones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910048402&hterms=fast+memory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dfast%2Bmemory','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910048402&hterms=fast+memory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dfast%2Bmemory"><span><span class="hlt">Wave</span>-particle interactions on the FAST satellite</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Temerin, M. A.; Carlson, C. W.; Cattell, C. A.; Ergun, R. E.; Mcfadden, J. P.</p> <p>1990-01-01</p> <p>NASA's Fast Auroral Snapshot, or 'FAST' satellite, scheduled for launch in 1993, will investigate the plasma physics of the low altitude auroral <span class="hlt">zone</span> from a 3500-km apogee polar orbit. FAST will give attention to <span class="hlt">wave</span>, double-layer, and soliton production processes due to electrons and ions, as well as to <span class="hlt">wave-wave</span> interactions, and the acceleration of electrons and ions by <span class="hlt">waves</span> and electric fields. FAST will employ an intelligent data-handling system capacle of data acquisition at rates of up to 1 Mb/sec, in addition to a 1-Gbit solid-state memory. The data need be gathered for only a few minutes during passes through the auroral <span class="hlt">zone</span>, since the most interesting auroral phenomena occur in such narrow regions as auroral arcs, electrostatic shocks, and superthermal electron bursts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810943H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810943H"><span>Impacts of <span class="hlt">wave</span> energy conversion devices on local <span class="hlt">wave</span> climate: observations and modelling from the Perth <span class="hlt">Wave</span> Energy Project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoeke, Ron; Hemer, Mark; Contardo, Stephanie; Symonds, Graham; Mcinnes, Kathy</p> <p>2016-04-01</p> <p>As demonstrated by the Australian <span class="hlt">Wave</span> Energy Atlas (AWavEA), the southern and western margins of the country possess considerable <span class="hlt">wave</span> energy resources. The Australia Government has made notable investments in pre-commercial <span class="hlt">wave</span> energy developments in these areas, however little is known about how this technology may impact local <span class="hlt">wave</span> climate and subsequently affect neighbouring coastal environments, e.g. altering sediment transport, causing shoreline erosion or accretion. In this study, a network of in-situ <span class="hlt">wave</span> measurement devices have been deployed surrounding the 3 <span class="hlt">wave</span> energy converters of the Carnegie <span class="hlt">Wave</span> Energy Limited's Perth <span class="hlt">Wave</span> Energy Project. This data is being used to develop, calibrate and validate numerical simulations of the project site. Early stage results will be presented and potential simulation strategies for scaling-up the findings to larger arrays of <span class="hlt">wave</span> energy converters will be discussed. The intended project outcomes are to establish <span class="hlt">zones</span> of impact defined in terms of changes in local <span class="hlt">wave</span> energy spectra and to initiate best practice guidelines for the establishment of <span class="hlt">wave</span> energy conversion sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994nasa.reptR....P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994nasa.reptR....P"><span>Method for cancelling expansion <span class="hlt">waves</span> in a <span class="hlt">wave</span> rotor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paxson, Daniel E.</p> <p>1994-03-01</p> <p>A <span class="hlt">wave</span> rotor system includes a <span class="hlt">wave</span> rotor coupled to first and second end plates. Special ports are provided, one in each of the first and second end plates, to cancel expansion <span class="hlt">waves</span> generated by the release of working fluid from the <span class="hlt">wave</span> rotor. One of the expansion <span class="hlt">waves</span> is reflected in the <span class="hlt">wave</span> rotor from a reflecting portion, and provided to the special port in the second end plate. Fluid present at the special port in the second end plate has a stagnation pressure and mass flow which is substantially the same as that of the cells of the <span class="hlt">wave</span> rotor communicating with such special port. This allows for cancellation of the expansion <span class="hlt">wave</span> generated by the release of working fluid from the <span class="hlt">wave</span> rotor. The special port in the second end plate has a first end corresponding substantially to the <span class="hlt">head</span> of the expansion <span class="hlt">wave</span>, and a second end corresponding substantially to the tail of the expansion <span class="hlt">wave</span>. Also, the special port is configured to continually change along the circumference of the second end plate to affect expansion <span class="hlt">wave</span> cancellation. An expansion <span class="hlt">wave</span> generated by a second release of working fluid from the <span class="hlt">wave</span> rotor is cancelled in a similar manner to that described above using a special port in the first end plate. Preferably the cycle of operation of the <span class="hlt">wave</span> rotor system is designed so that the stagnation pressure and mass flow of the fluid present at the special ports is the same so that the special ports may be connected by a common duct.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SPIE.9281E..1UH','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SPIE.9281E..1UH"><span>Research on the magnetorheological finishing (MRF) technology with dual polishing <span class="hlt">heads</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Wen; Zhang, Yunfei; He, Jianguo; Zheng, Yongcheng; Luo, Qing; Hou, Jing; Yuan, Zhigang</p> <p>2014-08-01</p> <p>Magnetorheological finishing (MRF) is a key polishing technique capable of rapidly converging to the required surface figure. Due to the deficiency of general one-polishing-<span class="hlt">head</span> MRF technology, a dual polishing <span class="hlt">heads</span> MRF technology was studied and a dual polishing <span class="hlt">heads</span> MRF machine with 8 axes was developed. The machine has the ability to manufacture large aperture optics with high figure accuracy. The large polishing <span class="hlt">head</span> is suitable for polishing large aperture optics, controlling large spatial length's <span class="hlt">wave</span> structures, correcting low-medium frequency errors with high removal rates. While the small polishing <span class="hlt">head</span> has more advantages in manufacturing small aperture optics, controlling small spatial wavelength's <span class="hlt">wave</span> structures, correcting mid-high frequency and removing nanoscale materials. Material removal characteristic and figure correction ability for each of large and small polishing <span class="hlt">head</span> was studied. Each of two polishing <span class="hlt">heads</span> respectively acquired stable and valid polishing removal function and ultra-precision flat sample. After a single polishing iteration using small polishing <span class="hlt">head</span>, the figure error in 45mm diameter of a 50 mm diameter plano optics was significantly improved from 0.21λ to 0.08λ by PV (RMS 0.053λ to 0.015λ). After three polishing iterations using large polishing <span class="hlt">head</span> , the figure error in 410mm×410mm of a 430mm×430mm large plano optics was significantly improved from 0.40λ to 0.10λ by PV (RMS 0.068λ to 0.013λ) .This results show that the dual polishing <span class="hlt">heads</span> MRF machine not only have good material removal stability, but also excellent figure correction capability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.2424C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.2424C"><span>Abyssal Upwelling in Mid-Ocean Ridge Fracture <span class="hlt">Zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clément, Louis; Thurnherr, Andreas M.</p> <p>2018-03-01</p> <p>Turbulence in the abyssal ocean plays a fundamental role in the climate system by sustaining the deepest branch of the overturning circulation. Over the western flank of the Mid-Atlantic Ridge in the South Atlantic, previously observed bottom-intensified and tidally modulated mixing of abyssal waters appears to imply a counterintuitive densification of deep and bottom waters. Here we show that inside fracture <span class="hlt">zones</span>, however, turbulence is elevated away from the seafloor because of intensified downward propagating near-inertial <span class="hlt">wave</span> energy, which decays below a subinertial shear maximum. Ray-tracing simulations predict a decay of <span class="hlt">wave</span> energy subsequent to <span class="hlt">wave</span>-mean flow interactions. The hypothesized <span class="hlt">wave</span>-mean flow interactions drive a deep flow toward lighter densities of up to 0.6 Sv over the mid-ocean ridge flank in the Brazil Basin, and the same process may also cause upwelling of abyssal waters in other ocean basins with mid-ocean ridges with fracture <span class="hlt">zones</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23345257','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23345257"><span>Biomechanical responses of a pig <span class="hlt">head</span> under blast loading: a computational simulation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhu, Feng; Skelton, Paul; Chou, Cliff C; Mao, Haojie; Yang, King H; King, Albert I</p> <p>2013-03-01</p> <p>A series of computational studies were performed to investigate the biomechanical responses of the pig <span class="hlt">head</span> under a specific shock tube environment. A finite element model of the <span class="hlt">head</span> of a 50-kg Yorkshire pig was developed with sufficient details, based on the Lagrangian formulation, and a shock tube model was developed using the multimaterial arbitrary Lagrangian-Eulerian (MMALE) approach. These two models were integrated and a fluid/solid coupling algorithm was used to simulate the interaction of the shock <span class="hlt">wave</span> with the pig's <span class="hlt">head</span>. The finite element model-predicted incident and intracranial pressure traces were in reasonable agreement with those obtained experimentally. Using the verified numerical model of the shock tube and pig <span class="hlt">head</span>, further investigations were carried out to study the spatial and temporal distributions of pressure, shear stress, and principal strain within the <span class="hlt">head</span>. Pressure enhancement was found in the skull, which is believed to be caused by shock <span class="hlt">wave</span> reflection at the interface of the materials with distinct <span class="hlt">wave</span> impedances. Brain tissue has a shock attenuation effect and larger pressures were observed in the frontal and occipital regions, suggesting a greater possibility of coup and contrecoup contusion. Shear stresses in the brain and deflection in the skull remained at a low level. Higher principal strains were observed in the brain near the foramen magnum, suggesting that there is a greater chance of cellular or vascular injuries in the brainstem region. Copyright © 2012 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27165895','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27165895"><span>Plateau <span class="hlt">Waves</span> of Intracranial Pressure and Multimodal Brain Monitoring.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dias, Celeste; Maia, Isabel; Cerejo, Antonio; Smielewski, Peter; Paiva, José-Artur; Czosnyka, Marek</p> <p>2016-01-01</p> <p>The aim of this study was to describe multimodal brain monitoring characteristics during plateau <span class="hlt">waves</span> of intracranial pressure (ICP) in patients with <span class="hlt">head</span> injury, using ICM+ software for continuous recording. Plateau <span class="hlt">waves</span> consist of an abrupt elevation of ICP above 40 mmHg for 5-20 min. This is a prospective observational study of patients with <span class="hlt">head</span> injury who were admitted to a neurocritical care unit and who developed plateau <span class="hlt">waves</span>. We analyzed 59 plateau <span class="hlt">waves</span> that occurred in 8 of 18 patients (44 %). At the top of plateau <span class="hlt">waves</span> arterial blood pressure remained almost constant, but cerebral perfusion pressure, cerebral blood flow, brain tissue oxygenation, and cerebral oximetry decreased. After plateau <span class="hlt">waves</span>, patients with a previously better autoregulation status developed hyperemia, demonstrated by an increase in cerebral blood flow and brain oxygenation. Pressure and oxygen cerebrovascular reactivity indexes (pressure reactivity index and ORxshort) increased significantly during the plateau <span class="hlt">wave</span> as a sign of disruption of autoregulation. Bedside multimodal brain monitoring is important to characterize increases in ICP and give differential diagnoses of plateau <span class="hlt">waves</span>, as management of this phenomenon differs from that of regular ICP.</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/2015AGUFMNH23A1870J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMNH23A1870J"><span>Sensitivity of Tsunami <span class="hlt">Waves</span> and Coastal Inundation/Runup to Seabed Displacement Models: Application to the Cascadia Subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jalali Farahani, R.; Fitzenz, D. D.; Nyst, M.</p> <p>2015-12-01</p> <p>Major components of tsunami hazard modeling include earthquake source characterization, seabed displacement, <span class="hlt">wave</span> propagation, and coastal inundation/run-up. Accurate modeling of these components is essential to identify the disaster risk exposures effectively, which would be crucial for insurance industry as well as policy makers to have tsunami resistant design of structures and evacuation planning (FEMA, 2008). In this study, the sensitivity and variability of tsunami coastal inundation due to Cascadia megathrust subduction earthquake are studied by considering the different approaches for seabed displacement model. The first approach is the analytical expressions that were proposed by Okada (1985, 1992) for the surface displacements and strains of rectangular sources. The second approach was introduced by Meade (2006) who introduced analytical solutions for calculating displacements, strains, and stresses on triangular sources. In this study, the seabed displacement using triangular representation of geometrically complex fault surfaces is compared with the Okada rectangular representations for the Cascadia subduction <span class="hlt">zone</span>. In the triangular dislocation algorithm, the displacement is calculated using superposition of two angular dislocations for each of the three triangle legs. The triangular elements could give a better and gap-free representation of the fault surfaces. In addition, the rectangular representation gives large unphysical vertical displacement along the shallow-depth fault edge that generates unrealistic short-wavelength <span class="hlt">waves</span>. To study the impact of these two different algorithms on the final tsunami inundation, the initial tsunami <span class="hlt">wave</span> as well as <span class="hlt">wave</span> propagation and the coastal inundation are simulated. To model the propagation of tsunami <span class="hlt">waves</span> and coastal inundation, 2D shallow water equations are modeled using the seabed displacement as the initial condition for the numerical model. Tsunami numerical simulation has been performed on high</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23996897','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23996897"><span>Computational modeling of human <span class="hlt">head</span> under blast in confined and open spaces: primary blast injury.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rezaei, A; Salimi Jazi, M; Karami, G</p> <p>2014-01-01</p> <p>In this paper, a computational modeling for biomechanical analysis of primary blast injuries is presented. The responses of the brain in terms of mechanical parameters under different blast spaces including open, semi-confined, and confined environments are studied. In the study, the effect of direct and indirect blast <span class="hlt">waves</span> from the neighboring walls in the confined environments will be taken into consideration. A 50th percentile finite element <span class="hlt">head</span> model is exposed to blast <span class="hlt">waves</span> of different intensities. In the open space, the <span class="hlt">head</span> experiences a sudden intracranial pressure (ICP) change, which vanishes in a matter of a few milliseconds. The situation is similar in semi-confined space, but in the confined space, the reflections from the walls will create a number of subsequent peaks in ICP with a longer duration. The analysis procedure is based on a simultaneous interaction simulation of the deformable <span class="hlt">head</span> and its components with the blast <span class="hlt">wave</span> propagations. It is concluded that compared with the open and semi-confined space settings, the walls in the confined space scenario enhance the risk of primary blast injuries considerably because of indirect blast <span class="hlt">waves</span> transferring a larger amount of damaging energy to the <span class="hlt">head</span>. Copyright © 2013 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://pubs.water.usgs.gov/wri984091','USGSPUBS'); return false;" href="http://pubs.water.usgs.gov/wri984091"><span>Transmissivity and water quality of water-producing <span class="hlt">zones</span> in the intermediate aquifer system, Sarasota 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>Knochenmus, L.A.; Bowman, Geronia</p> <p>1998-01-01</p> <p>The intermediate aquifer system is an important water source in Sarasota County, Florida, because the quality of water in it is usually better than that in the underlying Upper Floridan aquifer. The intermediate aquifer system consists of a group of up to three water-producing <span class="hlt">zones</span> separated by less-permeable units that restrict the vertical movement of ground water between <span class="hlt">zones</span>. The diverse lithology, that makes up the intermediate aquifer system, reflects the variety of depositional environments that occurred during the late Oligocene and Miocene epochs. Slight changes in the depositional environment resulted in aquifer heterogeneity, creating both localized connection between water-producing <span class="hlt">zones</span> and abrupt culmination of water-producing <span class="hlt">zones</span> that are not well documented. Aquifer heterogeneity results in vertical and areal variability in hydraulic and water-quality properties. The uppermost water-producing <span class="hlt">zone</span> is designated producing <span class="hlt">zone</span> 1 but is not extensively used because of its limited production capability and limited areal extent. The second water-producing <span class="hlt">zone</span> is designated producing <span class="hlt">zone</span> 2, and most of the domestic- and irrigation-supply wells in the area are open to this <span class="hlt">zone</span>. Additionally, producing <span class="hlt">zone</span> 2 is utilized for public supply in southern coastal areas of Sarasota County. Producing <span class="hlt">zone</span> 3 is the lowermost and most productive water-producing <span class="hlt">zone</span> in the intermediate aquifer system. Public-supply well fields serving the cities of Sarasota and Venice, as well as the Plantation and Mabry Carlton Reserve well fields, utilize producing <span class="hlt">zone</span> 3. <span class="hlt">Heads</span> within the intermediate aquifer system generally increase with aquifer depth. However, localized <span class="hlt">head</span>-gradient reversals occur in the study area, coinciding with sites of intense ground-water withdrawals. <span class="hlt">Heads</span> in producing <span class="hlt">zones</span> 1, 2, and 3 range from 1 to 23, 0.2 to 34, and 7 to 42 feet above sea level, respectively. Generally, an upward <span class="hlt">head</span> gradient exists between producing <span class="hlt">zones</span> 3 and 2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770023763','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770023763"><span>Coastal <span class="hlt">wave</span> measurements during passage of tropical storm Amy</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Morris, W. D.</p> <p>1977-01-01</p> <p>Aerial photographic and laser profilometer data of <span class="hlt">waves</span> generated by tropical storm Amy are presented. The data mission consisted primarily of two legs, one in the direction of the wind <span class="hlt">waves</span>, and the second along the direction of swell propagation, using Jennette's Pier at Nags <span class="hlt">Head</span>, North Carolina, as a focal point. At flight time, Amy's center was 512 nmi from shore and had maximum winds of 60 knots. The storm's history is presented, along with a satellite photograph, showing the extent of the storm on the day of the flight. Flight ground tracks are presented along with sample aerial photographs of the <span class="hlt">wave</span> conditions showing approximate wavelength and direction. Sample <span class="hlt">wave</span> energy spectra are presented both from the laser profilometer onboard the aircraft, and from the Corps of Engineers Research Center (CERC) shore gauge at Nags <span class="hlt">Head</span>, North Carolina.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26674675','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26674675"><span>Effects of Focused Extracorporeal Shock <span class="hlt">Waves</span> on Bone Marrow Mesenchymal Stem Cells in Patients with Avascular Necrosis of the Femoral <span class="hlt">Head</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhai, Lei; Sun, Nan; Zhang, Bo; Liu, Shui-Tao; Zhao, Zhe; Jin, Hai-Chao; Ma, Xin-Long; Xing, Geng-Yan</p> <p>2016-03-01</p> <p>To observe the effect of extracorporeal shock <span class="hlt">waves</span> (ESWs) on bone marrow mesenchymal stem cells (MSCs) in patients with avascular necrosis of the femoral <span class="hlt">head</span>, we collected bone marrow donated by patients and then cultivated and passaged MSCs in vitro using density gradient centrifugation combined with adherence screening methods. The P3 generation MSCs were divided into the ESW group and the control group. The cell counting kit for MSCs detected some proliferation differences. Cytochemistry, alkaline phosphatase staining and Alizarin red staining were used to determine alkaline phosphatase content. Simultaneously, real-time polymerase factor α1, osteocalcin and peroxisome proliferator-activated receptor γ. Together, the results of our study first indicate that moderate ESW intensity, which is instrumental in enhancing MSC proliferation, inducing conversion of MSCs into osteoblasts, and inhibiting differentiation of MSCs into adipocytes from MSCs, is one of the effective mechanisms for treating avascular necrosis of the femoral <span class="hlt">head</span>. Copyright © 2016 World Federation for Ultrasound in Medicine & Biology. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S41E..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S41E..01M"><span>Imaging the Alaskan subduction <span class="hlt">zone</span> with joint inversion of ambient noise and teleseismic surface <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin-Short, R.; Allen, R. M.; Porritt, R.</p> <p>2017-12-01</p> <p>Alaska consists of a complex arrangement of terranes of various geological affinities, mostof which have been accreted to the margin of North America over the last 200Myr. Today,the southern margin of Alaska is a site of active subduction, displaying a myriad ofenigmatic tectonic features. These include transition from compressional to strike-slipdominated deformation, accretion of the over-thickened Yakutat terrane, termination ofAleutian arc magnetism and the Wrangell Volcanic Field, whose magma source remainsdebated. The ongoing deployment of Transportable Array (TA) seismometers across Alaskaprovides an unprecedented opportunity to image these features in detail and learn moreabout the tectonic history of the region. Here we present a three dimensional model ofshear <span class="hlt">wave</span> (Vsv) velocity beneath Alaska constructed using joint inversion of phasevelocity maps derived from ambient noise and teleseismic surface <span class="hlt">wave</span> tomography. Thismodel possesses good resolution from the upper crust to about 150km depth, thuscomplementing recent body <span class="hlt">wave</span> models of the region, which lack resolution above 100km.In the upper crust, we are able to distinguish major sedimentary basins and the cores ofmountain belts. At mid-crustal depths, we see a sharp velocity contrast across the Denalifault, suggesting that it marks a significant step in crustal thickness. In the mantle wedgeabove the subducting Yakutat terrane we observe a high velocity anomaly that may berelated to paucity of volcanism in this region. At greater depths, we image the subductingPacific-Yakutat slab as an elongate, high velocity anomaly that terminates abruptly at 145ºW, slightly further east than suggested by the Wadati-Benioff <span class="hlt">zone</span> alone. There is alarge, low velocity anomaly beneath the Wrangell Volcanic Field, hinting that magmatismhere may be related to mantle upwelling around the slab edge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/182705-hydrodynamic-force-characteristics-slender-cylinders-splash-zone','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/182705-hydrodynamic-force-characteristics-slender-cylinders-splash-zone"><span>Hydrodynamic force characteristics of slender cylinders in the splash <span class="hlt">zone</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>Haritos, N.; Daliri, M.R.</p> <p>1995-12-31</p> <p>This paper presents results from a pilot experimental program of research being performed on segmented vertical surface-piercing cylinders in the Department of Civil and Environmental Engineering at The University of Melbourne. The primary aim of this investigation is to determine the influence of the splash <span class="hlt">zone</span> on the hydrodynamic force characteristics of such cylinders to <span class="hlt">wave</span> loading in the Morison regime. This influence is assessed from a comparison of the observed force characteristics of instrumented segments located in the splash <span class="hlt">zone</span> with the corresponding results obtained from similarly instrumented segments located in the fully submerged <span class="hlt">zone</span> and from those obtainedmore » for the cylinder as a whole via measurements of the cylinder tip restraint force. Results to hand for uni-directional regular <span class="hlt">waves</span> suggest that there appears to be a mild frequency dependence in the inertia force coefficient in the splash <span class="hlt">zone</span> which only marginally exceeds the corresponding values observed for a submerged segment immediately below this <span class="hlt">zone</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/449664-hydrodynamic-force-characteristics-splash-zone','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/449664-hydrodynamic-force-characteristics-splash-zone"><span>Hydrodynamic force characteristics in the splash <span class="hlt">zone</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>Daliri, M.R.; Haritos, N.</p> <p>1996-12-31</p> <p>A comprehensive experimental study concerned with the hydrodynamic force characteristics of both rigid and compliant surface piercing cylinders, with a major focus on the local nature of these characteristics as realized in the splash <span class="hlt">zone</span> and in the fully submerged <span class="hlt">zone</span> immediately below this region, has been in progress at the University of Melbourne for the last three years. This paper concentrates on a portion of this study associated with uni-directional regular <span class="hlt">wave</span> inputs with <span class="hlt">wave</span> steepness (H/{lambda}) in the range 0.0005--0.1580 and Keulegan-Carpenter (KC) numbers in the range 2--15 which encompasses inertia force dominant (KC<5) to drag force significantmore » conditions (5« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013695','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013695"><span><span class="hlt">Wave</span> Climate and <span class="hlt">Wave</span> Mixing in the Marginal Ice <span class="hlt">Zones</span> of Arctic Seas, Observations and Modelling</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>ababanin.com/ LONG-TERM GOALS The long-term goals of the present project are two: wind/<span class="hlt">wave</span> climatology for the Arctic Seas, and their current...OBJECTIVES The wind/<span class="hlt">wave</span> climatology for the Arctic Seas will be developed based on altimeter observations. It will have a major scientific and...applied significance as presently there is no reference climatology for this region of the ocean available. The new versions of <span class="hlt">wave</span> models for the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E3SWC..3804017G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E3SWC..3804017G"><span>Modeling and Simulation of Hydropower Station Diversion System's characteristic line method by introducing water <span class="hlt">head</span> to flow feedback</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guangwen, Xu; Xi, Li; Ze, Yao</p> <p>2018-06-01</p> <p>To solve the damping problem of water hammer <span class="hlt">wave</span> in the modeling method of water diversion system of hydropower station, this paper introduces the feedback regulation technology from <span class="hlt">head</span> to flow, that is: A fixed water <span class="hlt">head</span> is taken out for flow feedback, and the following conclusions are obtained through modeling and simulation. Adjusting the feedback coefficient F of the water <span class="hlt">head</span> to the flow rate can change the damping characteristic of the system, which can simulate the attenuation process of the water shock <span class="hlt">wave</span> in the true water diversion pipeline. Even if a small feedback coefficient is introduced, the damping effect of the system is very obvious, but it has little effect on the amplitude of the first water shock <span class="hlt">wave</span> after the transition process. Therefore, it is feasible and reasonable to introduce water <span class="hlt">head</span> to flow rate feedback coefficient F in hydraulic turbine diversion system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28011730','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28011730"><span>Arrestant Effect of Human Scalp Components on <span class="hlt">Head</span> Louse (Phthiraptera: Pediculidae) Behavior.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ortega-Insaurralde, Isabel; Ceferino Toloza, Ariel; Gonzalez-Audino, Paola; Inés Picollo, María</p> <p>2017-03-01</p> <p>Relevant evidence has shown that parasites process host-related information using chemical, visual, tactile, or auditory cues. However, the cues that are involved in the host-parasite interaction between Pediculus humanus capitis (De Geer 1767) and humans have not been identified yet. In this work, we studied the effect of human scalp components on the behavior of adult <span class="hlt">head</span> lice. Filter paper segments were rubbed on volunteers' scalps and then placed in the experimental arena, where adult <span class="hlt">head</span> lice were individually tested. The movement of the insects was recorded for each arena using the software EthoVision. Average movement parameters were calculated for the treatments in the bioassays such as total distance, velocity, number of times a <span class="hlt">head</span> louse crossed between <span class="hlt">zones</span> of the arena, and time in each <span class="hlt">zone</span> of the arena. We found that scalp components induced <span class="hlt">head</span> lice to decrease average locomotor activity and to remain arrested on the treated paper. The effect of the ageing of human scalp samples in the response of <span class="hlt">head</span> lice was not statistically significant (i.e., human scalp samples of 4, 18, 40, and 60 h of ageing did not elicit a significant change in <span class="hlt">head</span> louse behavior). When we analyzed the effect of the sex in the response of <span class="hlt">head</span> lice to human scalp samples, males demonstrated significant differences. Our results showed for the first time the effect of host components conditioning <span class="hlt">head</span> lice behavior. We discuss the role of these components in the dynamic of <span class="hlt">head</span> lice infestation. © The Authors 2016. Published by Oxford University Press on behalf of Entomological Society of America. All rights reserved. For Permissions, please email: journals.permissions@oup.com.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170000975&hterms=climate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dclimate','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170000975&hterms=climate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dclimate"><span>Tropical <span class="hlt">Waves</span> and the Quasi-Biennial Oscillation in a 7-km Global Climate Simulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Holt, Laura A.; Alexander, M. Joan; Coy, Lawrence; Molod, Andrea; Putman, William; Pawson, Steven</p> <p>2016-01-01</p> <p>This study investigates tropical <span class="hlt">waves</span> and their role in driving a quasi-biennial oscillation (QBO)-like signal in stratospheric winds in a global 7-km-horizontal-resolution atmospheric general circulation model. The Nature Run (NR) is a 2-year global mesoscale simulation of the Goddard Earth Observing System Model, version 5 (GEOS-5). In the tropics, there is evidence that the NR supports a broad range of convectively generated <span class="hlt">waves</span>. The NR precipitation spectrum resembles the observed spectrum in many aspects, including the preference for westward-propagating <span class="hlt">waves</span>. However, even with very high horizontal resolution and a healthy population of resolved <span class="hlt">waves</span>, the zonal force provided by the resolved <span class="hlt">waves</span> is still too low in the QBO region and parameterized gravity <span class="hlt">wave</span> drag is the main driver of the NR QBO-like oscillation (NRQBO). The authors suggest that causes include coarse vertical resolution and excessive dissipation. Nevertheless, the very-high-resolution NR provides an opportunity to analyze the resolved <span class="hlt">wave</span> forcing of the NR-QBO. In agreement with previous studies, large-scale Kelvin and small-scale <span class="hlt">waves</span> contribute to the NRQBO driving in eastward shear <span class="hlt">zones</span> and small-scale <span class="hlt">waves</span> dominate the NR-QBO driving in westward shear <span class="hlt">zones</span>. <span class="hlt">Waves</span> with zonal wavelength,1000 km account for up to half of the small-scale (,3300 km) resolved <span class="hlt">wave</span> forcing in eastward shear <span class="hlt">zones</span> and up to 70% of the small-scale resolved <span class="hlt">wave</span> forcing in westward shear <span class="hlt">zones</span> of the NR-QBO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1615997L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1615997L"><span>Analysis of X-band radar images for the detection of the reflected and diffracted <span class="hlt">waves</span> in coastal <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ludeno, Giovanni; Natale, Antonio; Soldovieri, Francesco; Vicinanza, Diego; Serafino, Francesco</p> <p>2014-05-01</p> <p>The observation of nearshore <span class="hlt">waves</span> and the knowledge of the sea state parameters can play a crucial role for the safety of harbors and ocean engineering. In the last two decades, different algorithms for the estimation of sea state parameters, surface currents and bathymetry from X-band radar data have been developed and validated [1, 2]. The retrieval of ocean <span class="hlt">wave</span> parameters such as significant height, period, direction and wavelength of the dominant <span class="hlt">wave</span> is based on the spectral analysis of data sequences collected by nautical X-band radars [3]. In particular, the reconstruction of the <span class="hlt">wave</span> motion is carried out through the inversion procedure explained in [1-3], which exploits the dispersion relationship to define a band pass filter used to separate the energy associated with the ocean <span class="hlt">waves</span> from the background noise. It is worth to note that the shape of such a band pass filter depends upon the value of both the surface currents and bathymetry; in our reconstruction algorithm these parameters are estimated through the (Normalized Scalar Product) procedure [1], which outperforms other existing methods (e.g., the Least Squares) [4]. From the reconstructed <span class="hlt">wave</span> elevation sequences we can get the directional spectrum that provides useful information (i.e., wavelength, period, direction and amplitude) relevant to the main <span class="hlt">waves</span> contributing to the <span class="hlt">wave</span> motion. Of course, in coastal <span class="hlt">zones</span> a number of diffraction and reflection phenomena can be observed, due to sea-<span class="hlt">waves</span> impinging obstacles as jetties, breakwaters and boats. In the present paper we want to show the capability to detect reflected and diffracted sea-<span class="hlt">waves</span> offered by the processing of X-band radar data. Further details relevant to the obtained results will be provided in the full paper and at the conference time. References [1] F. Serafino, C. Lugni, F. Soldovieri, "A novel strategy for the surface current determination from marine X-Band radar data", IEEE Geosci. and Remote Sensing Letters, vol. 7, no</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3288437','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3288437"><span><span class="hlt">Head</span> direction cells in the postsubiculum do not show replay of prior waking sequences during sleep</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Brandon, Mark P.; Bogaard, Andrew; Andrews, Chris M.; Hasselmo, Michael E.</p> <p>2011-01-01</p> <p>During slow-<span class="hlt">wave</span> sleep and REM sleep, hippocampal place cells in the rat show replay of sequences previously observed during waking. We tested the hypothesis from computational modelling that the temporal structure of REM sleep replay could arise from an interplay of place cells with <span class="hlt">head</span> direction cells in the postsubiculum. Physiological single-unit recording was performed simultaneously from five or more <span class="hlt">head</span> direction or place by <span class="hlt">head</span> direction cells in the postsubiculum during running on a circular track allowing sampling of a full range of <span class="hlt">head</span> directions, and during sleep periods before and after running on the circular track. Data analysis compared the spiking activity during individual REM periods with waking as in previous analysis procedures for REM sleep. We also used a new procedure comparing groups of similar runs during waking with REM sleep periods. There was no consistent evidence for a statistically significant correlation of the temporal structure of spiking during REM sleep with spiking during waking running periods. Thus, the spiking activity of <span class="hlt">head</span> direction cells during REM sleep does not show replay of <span class="hlt">head</span> direction cell activity occurring during a previous waking period of running on the task. In addition, we compared the spiking of postsubiculum neurons during hippocampal sharp <span class="hlt">wave</span> ripple events. We show that <span class="hlt">head</span> direction cells are not activated during sharp <span class="hlt">wave</span> ripples, while neurons responsive to place in the postsubiculum show reliable spiking at ripple events. PMID:21509854</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21129403','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21129403"><span>Relationship between orientation to a blast and pressure <span class="hlt">wave</span> propagation inside the rat brain.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chavko, Mikulas; Watanabe, Tomas; Adeeb, Saleena; Lankasky, Jason; Ahlers, Stephen T; McCarron, Richard M</p> <p>2011-01-30</p> <p>Exposure to a blast <span class="hlt">wave</span> generated during an explosion may result in brain damage and related neurological impairments. Several mechanisms by which the primary blast <span class="hlt">wave</span> can damage the brain have been proposed, including: (1) a direct effect of the shock <span class="hlt">wave</span> on the brain causing tissue damage by skull flexure and propagation of stress and shear forces; and (2) an indirect transfer of kinetic energy from the blast, through large blood vessels and cerebrospinal fluid (CSF), to the central nervous system. To address a basic question related to the mechanisms of blast brain injury, pressure was measured inside the brains of rats exposed to a low level of blast (~35kPa), while positioned in three different orientations with respect to the primary blast <span class="hlt">wave</span>; <span class="hlt">head</span> facing blast, right side exposed to blast and <span class="hlt">head</span> facing away from blast. Data show different patterns and durations of the pressure traces inside the brain, depending on the rat orientation to blast. Frontal exposures (<span class="hlt">head</span> facing blast) resulted in pressure traces of higher amplitude and longer duration, suggesting direct transmission and reflection of the pressure inside the brain (dynamic pressure transfer). The pattern of the pressure <span class="hlt">wave</span> inside the brain in the <span class="hlt">head</span> facing away from blast exposures assumes contribution of the static pressure, similar to hydrodynamic pressure to the pressure <span class="hlt">wave</span> inside the brain. Published by Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25108178','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25108178"><span>Numerical study of <span class="hlt">wave</span> effects on groundwater flow and solute transport in a laboratory beach.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Geng, Xiaolong; Boufadel, Michel C; Xia, Yuqiang; Li, Hailong; Zhao, Lin; Jackson, Nancy L; Miller, Richard S</p> <p>2014-09-01</p> <p>A numerical study was undertaken to investigate the effects of <span class="hlt">waves</span> on groundwater flow and associated inland-released solute transport based on tracer experiments in a laboratory beach. The MARUN model was used to simulate the density-dependent groundwater flow and subsurface solute transport in the saturated and unsaturated regions of the beach subjected to <span class="hlt">waves</span>. The Computational Fluid Dynamics (CFD) software, Fluent, was used to simulate <span class="hlt">waves</span>, which were the seaward boundary condition for MARUN. A no-<span class="hlt">wave</span> case was also simulated for comparison. Simulation results matched the observed water table and concentration at numerous locations. The results revealed that <span class="hlt">waves</span> generated seawater-groundwater circulations in the swash and surf <span class="hlt">zones</span> of the beach, which induced a large seawater-groundwater exchange across the beach face. In comparison to the no-<span class="hlt">wave</span> case, <span class="hlt">waves</span> significantly increased the residence time and spreading of inland-applied solutes in the beach. <span class="hlt">Waves</span> also altered solute pathways and shifted the solute discharge <span class="hlt">zone</span> further seaward. Residence Time Maps (RTM) revealed that the <span class="hlt">wave</span>-induced residence time of the inland-applied solutes was largest near the solute exit <span class="hlt">zone</span> to the sea. Sensitivity analyses suggested that the change in the permeability in the beach altered solute transport properties in a nonlinear way. Due to the slow movement of solutes in the unsaturated <span class="hlt">zone</span>, the mass of the solute in the unsaturated <span class="hlt">zone</span>, which reached up to 10% of the total mass in some cases, constituted a continuous slow release of solutes to the saturated <span class="hlt">zone</span> of the beach. This means of control was not addressed in prior studies. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026667','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026667"><span>Shear <span class="hlt">wave</span> velocity variation across the Taupo Volcanic <span class="hlt">Zone</span>, New Zealand, from receiver function inversion</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bannister, S.; Bryan, C.J.; Bibby, H.M.</p> <p>2004-01-01</p> <p>The Taupo Volcanic <span class="hlt">Zone</span> (TVZ), New Zealand is a region characterized by very high magma eruption rates and extremely high heat flow, which is manifest in high-temperature geothermal waters. The shear <span class="hlt">wave</span> velocity structure across the region is inferred using non-linear inversion of receiver functions, which were derived from teleseismic earthquake data. Results from the non-linear inversion, and from forward synthetic modelling, indicate low S velocities at ???6- 16 km depth near the Rotorua and Reporoa calderas. We infer these low-velocity layers to represent the presence of high-level bodies of partial melt associated with the volcanism. Receiver functions at other stations are complicated by reverberations associated with near-surface sedimentary layers. The receiver function data also indicate that the Moho lies between 25 and 30 km, deeper than the 15 ?? 2 km depth previously inferred for the crust-mantle boundary beneath the TVZ. ?? 2004 RAS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.894a2072P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.894a2072P"><span>Effect of <span class="hlt">wave</span> action on near-well <span class="hlt">zone</span> cleaning</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pen'kovskii, V. I.; Korsakova, N. K.</p> <p>2017-10-01</p> <p>Drilling filtrate invasion into the producing formation and native water accumulating of the near-well <span class="hlt">zone</span> in well operation reduce the well productivity. As a result of that, depending on characteristic capillary pressure scale and differential pressure drawdown, oil production rate may become lower than expected one. In this paper, it is considered the hysteresis effects of capillary pressure after reversion of displacement. As applied to laboratory experiment conditions, the solution of problem of oil flow in formation model with a pressure drop on the model sides harmonically varied with time is presented. It was estimated a range of fluid vibration effective action on the near-well <span class="hlt">zone</span> cleaning from capillary locking water. The plant simulating extraction of oil from formation using widely practised sucker-rod pump has been created. Formation model is presented as a slot filled with broken glass between two plates. In the process, natural oil and sodium chloride solution were used as working fluids. The experiments qualitatively confirm a positive effect of jack pumps on the near-well <span class="hlt">zone</span> cleaning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.3799M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.3799M"><span>Rip currents and alongshore flows in single channels dredged in the surf <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moulton, Melissa; Elgar, Steve; Raubenheimer, Britt; Warner, John C.; Kumar, Nirnimesh</p> <p>2017-05-01</p> <p>To investigate the dynamics of flows near nonuniform bathymetry, single channels (on average 30 m wide and 1.5 m deep) were dredged across the surf <span class="hlt">zone</span> at five different times, and the subsequent evolution of currents and morphology was observed for a range of <span class="hlt">wave</span> and tidal conditions. In addition, circulation was simulated with the numerical modeling system COAWST, initialized with the observed incident <span class="hlt">waves</span> and channel bathymetry, and with an extended set of <span class="hlt">wave</span> conditions and channel geometries. The simulated flows are consistent with alongshore flows and rip-current circulation patterns observed in the surf <span class="hlt">zone</span>. Near the offshore-directed flows that develop in the channel, the dominant terms in modeled momentum balances are <span class="hlt">wave</span>-breaking accelerations, pressure gradients, advection, and the vortex force. The balances vary spatially, and are sensitive to <span class="hlt">wave</span> conditions and the channel geometry. The observed and modeled maximum offshore-directed flow speeds are correlated with a parameter based on the alongshore gradient in breaking-<span class="hlt">wave</span>-driven-setup across the nonuniform bathymetry (a function of <span class="hlt">wave</span> height and angle, water depths in the channel and on the sandbar, and a breaking threshold) and the breaking-<span class="hlt">wave</span>-driven alongshore flow speed. The offshore-directed flow speed increases with dissipation on the bar and reaches a maximum (when the surf <span class="hlt">zone</span> is saturated) set by the vertical scale of the bathymetric variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189256','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189256"><span>Rip currents and alongshore flows in single channels dredged in the surf <span class="hlt">zone</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>Moulton, Melissa; Elgar, Steve; Raubenheimer, Britt; Warner, John C.; Kumar, Nirnimesh</p> <p>2017-01-01</p> <p>To investigate the dynamics of flows near nonuniform bathymetry, single channels (on average 30 m wide and 1.5 m deep) were dredged across the surf <span class="hlt">zone</span> at five different times, and the subsequent evolution of currents and morphology was observed for a range of <span class="hlt">wave</span> and tidal conditions. In addition, circulation was simulated with the numerical modeling system COAWST, initialized with the observed incident <span class="hlt">waves</span> and channel bathymetry, and with an extended set of <span class="hlt">wave</span> conditions and channel geometries. The simulated flows are consistent with alongshore flows and rip-current circulation patterns observed in the surf <span class="hlt">zone</span>. Near the offshore-directed flows that develop in the channel, the dominant terms in modeled momentum balances are <span class="hlt">wave</span>-breaking accelerations, pressure gradients, advection, and the vortex force. The balances vary spatially, and are sensitive to <span class="hlt">wave</span> conditions and the channel geometry. The observed and modeled maximum offshore-directed flow speeds are correlated with a parameter based on the alongshore gradient in breaking-<span class="hlt">wave</span>-driven-setup across the nonuniform bathymetry (a function of <span class="hlt">wave</span> height and angle, water depths in the channel and on the sandbar, and a breaking threshold) and the breaking-<span class="hlt">wave</span>-driven alongshore flow speed. The offshore-directed flow speed increases with dissipation on the bar and reaches a maximum (when the surf <span class="hlt">zone</span> is saturated) set by the vertical scale of the bathymetric variability.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26736500','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26736500"><span><span class="hlt">Head</span> ballistocardiogram based on wireless multi-location sensors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Onizuka, Kohei; Sodini, Charles G</p> <p>2015-08-01</p> <p>Recently a wearable BCG monitoring technique based on an accelerometer worn at the ear was demonstrated to replace a conventional bulky BCG acquisition system. In this work, a multi-location wireless vital signs monitor was developed, and at least two common acceleration vectors correlating to sitting-BCG were found in the supine position by using <span class="hlt">head</span> PPG signal as a reference for eight healthy human subjects. The <span class="hlt">head</span> side amplitude in the supine position is roughly proportional to the sitting amplitude that is in turn proportional to the stroke volume. Signal processing techniques to identify J-<span class="hlt">waves</span> in a subject having small amplitude was also developed based on the two common vectors at the <span class="hlt">head</span> side and top.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22492847-spin-wave-driven-high-speed-domain-wall-motions-soft-magnetic-nanotubes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22492847-spin-wave-driven-high-speed-domain-wall-motions-soft-magnetic-nanotubes"><span>Spin-<span class="hlt">wave</span>-driven high-speed domain-wall motions in soft magnetic nanotubes</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>Yang, Jaehak; Yoo, Myoung-Woo; Kim, Sang-Koog, E-mail: sangkoog@snu.ac.kr</p> <p></p> <p>We report on a micromagnetic simulation study of interactions between propagating spin <span class="hlt">waves</span> and a <span class="hlt">head-to-head</span> domain wall in geometrically confined magnetic nanotubes. We found that incident spin <span class="hlt">waves</span> of specific frequencies can lead to sufficiently high-speed (on the order of a few hundreds of m/s or higher) domain-wall motions in the same direction as that of the incident spin-<span class="hlt">waves</span>. The domain-wall motions and their speed vary remarkably with the frequency and the amplitude of the incident spin-<span class="hlt">waves</span>. High-speed domain-wall motions originate from the transfer torque of spin <span class="hlt">waves</span>' linear momentum to the domain wall, through the partial or completemore » reflection of the incident spin <span class="hlt">waves</span> from the domain wall. This work provides a fundamental understanding of the interaction of the spin <span class="hlt">waves</span> with a domain wall in the magnetic nanotubes as well as a route to all-magnetic control of domain-wall motions in the magnetic nanoelements.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22114667','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22114667"><span>New mechanism of spiral <span class="hlt">wave</span> initiation in a reaction-diffusion-mechanics system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Weise, Louis D; Panfilov, Alexander V</p> <p>2011-01-01</p> <p>Spiral <span class="hlt">wave</span> initiation in the heart muscle is a mechanism for the onset of dangerous cardiac arrhythmias. A standard protocol for spiral <span class="hlt">wave</span> initiation is the application of a stimulus in the refractory tail of a propagating excitation <span class="hlt">wave</span>, a region that we call the "classical vulnerable <span class="hlt">zone</span>." Previous studies of vulnerability to spiral <span class="hlt">wave</span> initiation did not take the influence of deformation into account, which has been shown to have a substantial effect on the excitation process of cardiomyocytes via the mechano-electrical feedback phenomenon. In this work we study the effect of deformation on the vulnerability of excitable media in a discrete reaction-diffusion-mechanics (dRDM) model. The dRDM model combines FitzHugh-Nagumo type equations for cardiac excitation with a discrete mechanical description of a finite-elastic isotropic material (Seth material) to model cardiac excitation-contraction coupling and stretch activated depolarizing current. We show that deformation alters the "classical," and forms a new vulnerable <span class="hlt">zone</span> at longer coupling intervals. This mechanically caused vulnerable <span class="hlt">zone</span> results in a new mechanism of spiral <span class="hlt">wave</span> initiation, where unidirectional conduction block and rotation directions of the consequently initiated spiral <span class="hlt">waves</span> are opposite compared to the mechanism of spiral <span class="hlt">wave</span> initiation due to the "classical vulnerable <span class="hlt">zone</span>." We show that this new mechanism of spiral <span class="hlt">wave</span> initiation can naturally occur in situations that involve <span class="hlt">wave</span> fronts with curvature, and discuss its relation to supernormal excitability of cardiac tissue. The concept of mechanically induced vulnerability may lead to a better understanding about the onset of dangerous heart arrhythmias via mechano-electrical feedback.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23909919','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23909919"><span>A new zonation algorithm with parameter estimation using hydraulic <span class="hlt">head</span> and subsidence observations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Meijing; Burbey, Thomas J; Nunes, Vitor Dos Santos; Borggaard, Jeff</p> <p>2014-01-01</p> <p>Parameter estimation codes such as UCODE_2005 are becoming well-known tools in groundwater modeling investigations. These programs estimate important parameter values such as transmissivity (T) and aquifer storage values (Sa ) from known observations of hydraulic <span class="hlt">head</span>, flow, or other physical quantities. One drawback inherent in these codes is that the parameter <span class="hlt">zones</span> must be specified by the user. However, such knowledge is often unknown even if a detailed hydrogeological description is available. To overcome this deficiency, we present a discrete adjoint algorithm for identifying suitable zonations from hydraulic <span class="hlt">head</span> and subsidence measurements, which are highly sensitive to both elastic (Sske) and inelastic (Sskv) skeletal specific storage coefficients. With the advent of interferometric synthetic aperture radar (InSAR), distributed spatial and temporal subsidence measurements can be obtained. A synthetic conceptual model containing seven transmissivity <span class="hlt">zones</span>, one aquifer storage <span class="hlt">zone</span> and three interbed <span class="hlt">zones</span> for elastic and inelastic storage coefficients were developed to simulate drawdown and subsidence in an aquifer interbedded with clay that exhibits delayed drainage. Simulated delayed land subsidence and groundwater <span class="hlt">head</span> data are assumed to be the observed measurements, to which the discrete adjoint algorithm is called to create approximate spatial zonations of T, Sske , and Sskv . UCODE-2005 is then used to obtain the final optimal parameter values. Calibration results indicate that the estimated zonations calculated from the discrete adjoint algorithm closely approximate the true parameter zonations. This automation algorithm reduces the bias established by the initial distribution of <span class="hlt">zones</span> and provides a robust parameter zonation distribution. © 2013, National Ground Water Association.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24072460','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24072460"><span>Pressures, flow, and brain oxygenation during plateau <span class="hlt">waves</span> of intracranial pressure.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dias, Celeste; Maia, Isabel; Cerejo, António; Varsos, Georgios; Smielewski, Peter; Paiva, José-Artur; Czosnyka, Marek</p> <p>2014-08-01</p> <p>Plateau <span class="hlt">waves</span> are common in traumatic brain injury. They constitute abrupt increases of intracranial pressure (ICP) above 40 mmHg associated with a decrease in cerebral perfusion pressure (CPP). The aim of this study was to describe plateau <span class="hlt">waves</span> characteristics with multimodal brain monitoring in <span class="hlt">head</span> injured patients admitted in neurocritical care. Prospective observational study in 18 multiple trauma patients with <span class="hlt">head</span> injury admitted to Neurocritical Care Unit of Hospital Sao Joao in Porto. Multimodal systemic and brain monitoring of primary variables [heart rate, arterial blood pressure, ICP, CPP, pulse amplitude, end tidal CO₂, brain temperature, brain tissue oxygenation pressure, cerebral oximetry (CO) with transcutaneous near-infrared spectroscopy and cerebral blood flow (CBF)] and secondary variables related to cerebral compensatory reserve and cerebrovascular reactivity were supported by dedicated software ICM+ ( www.neurosurg.cam.ac.uk/icmplus) . The compiled data were analyzed in patients who developed plateau <span class="hlt">waves</span>. In this study we identified 59 plateau <span class="hlt">waves</span> that occurred in 44% of the patients (8/18). During plateau <span class="hlt">waves</span> CBF, cerebrovascular resistance, CO, and brain tissue oxygenation decreased. The duration and magnitude of plateau <span class="hlt">waves</span> were greater in patients with working cerebrovascular reactivity. After the end of plateau <span class="hlt">wave</span>, a hyperemic response was recorded in 64% of cases with increase in CBF and brain oxygenation. The magnitude of hyperemia was associated with better autoregulation status and low oxygenation levels at baseline. Multimodal brain monitoring facilitates identification and understanding of intrinsic vascular brain phenomenon, such as plateau <span class="hlt">waves</span>, and may help the adequate management of acute <span class="hlt">head</span> injury at bed side.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010026442','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010026442"><span>Idealized Simulations of the Effects of Amazon Convection and Baroclinic <span class="hlt">Waves</span> on the South Atlantic Convergence <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ferreira, Rosana Nieto; Suarez, Max J.; Nigam, Sumant; Einaudi, Franco (Technical Monitor)</p> <p>2001-01-01</p> <p>The South Atlantic Convergence <span class="hlt">Zone</span> (SACZ) is a NW-SE oriented, stationary region of enhanced convergence and convection that extends southeastward from the ITCZ convection anchored over the Amazon region. On daily satellite images each SACZ episode is seen as a progression of one or several midlatitude cold fronts that intrude into the subtropics and tropics, becoming stationary over southeastern Brazil for a few days. Previous studies have shown that while Amazon convection plays a fundamental role in the formation of the SACZ, Atlantic sea surface temperatures and the Andes Mountains play a relatively minor role in the strength and location of the SACZ. The role of interactions between Amazon convection and midlatitude baroclinic <span class="hlt">waves</span> in establishing the origin, position, and maintenance of the SACZ is studied here using idealized dry, multilayer global model simulations that do not include the effects of topography. The model simulations produce SACZ-like regions of low-level convergence in the presence of Amazon convection embedded in a mean-flow that contains propagating baroclinic <span class="hlt">waves</span>. The results of these simulations indicate that Amazon convection plays two fundamental roles in the formation and location of the SACZ. First, it produces a NW-SE oriented region of low-level convergence to the SE of Amazon convection. Second, it produces a storm-track region and accompanying stronger midlatitude baroclinic <span class="hlt">waves</span> in the region of the SACZ. It is suggested that in the presence of moist effects, the 'seedling' SACZ regions produced in these simulations can be enhanced to produce the observed SACZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA437351','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA437351"><span>Evaluation of Acoustic Propagation Paths into the Human <span class="hlt">Head</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2005-07-25</p> <p>paths. A 3D finite-element solid mesh was constructed using a digital image database of an adult male <span class="hlt">head</span>. Finite-element analysis was used to model the...air-borne sound pressure amplitude) via the alternate propagation paths. A 3D finite-element solid mesh was constructed using a digital image database ... database of an adult male <span class="hlt">head</span> Coupled acoustic-mechanical finite-element analysis (FEA) was used to model the <span class="hlt">wave</span> propagation through the fluid-solid</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29433003','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29433003"><span>Mixing of ultrasonic Lamb <span class="hlt">waves</span> in thin plates with quadratic nonlinearity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Feilong; Zhao, Youxuan; Cao, Peng; Hu, Ning</p> <p>2018-07-01</p> <p>This paper investigates the propagation of Lamb <span class="hlt">waves</span> in thin plates with quadratic nonlinearity by one-way mixing method using numerical simulations. It is shown that an A 0 -mode <span class="hlt">wave</span> can be generated by a pair of S 0 and A 0 mode <span class="hlt">waves</span> only when mixing condition is satisfied, and mixing <span class="hlt">wave</span> signals are capable of locating the damage <span class="hlt">zone</span>. Additionally, it is manifested that the acoustic nonlinear parameter increases linearly with quadratic nonlinearity but monotonously with the size of mixing <span class="hlt">zone</span>. Furthermore, because of frequency deviation, the waveform of the mixing <span class="hlt">wave</span> changes significantly from a regular diamond shape to toneburst trains. Copyright © 2018 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1377063','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1377063"><span>Assimilation of <span class="hlt">Wave</span> Imaging Radar Observations for Real-time <span class="hlt">Wave-by-Wave</span> Forecasting</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>Simpson, Alexandra; Haller, Merrick; Walker, David</p> <p></p> <p> of forecasting in real-time, as the GPU-based <span class="hlt">wave</span> model backbone was very computationally efficient. The data assimilation algorithm was developed on a polar grid domain in order to match the sampling characteristics of the observation system (<span class="hlt">wave</span> imaging marine radar). For verification purposes, a substantial set of synthetic <span class="hlt">wave</span> data (i.e. forward runs of the <span class="hlt">wave</span> model) were generated to be used as ground truth for comparison to the reconstructions and forecasts produced by Wavecast. For these synthetic cases, Wavecast demonstrated very good accuracy, for example, typical forecast correlation coefficients were between 0.84-0.95 when compared to the input data. Dependencies on shadowing, observational noise, and forecast horizon were also identified. During the second year of the project, a short field deployment was conducted in order to assess forecast accuracy under field conditions. For this, a radar was installed on a fishing vessel and observations were collected at the South Energy Test Site (SETS) off the coast of Newport, OR. At the SETS site, simultaneous in situ <span class="hlt">wave</span> observations were also available owing to an ongoing field project funded separately. Unfortunately, the position and <span class="hlt">heading</span> information that was available for the fishing vessel were not of sufficient accuracy in order to validate the forecast in a phase-resolving sense. Instead, a spectral comparison was made between the Wavecast forecast and the data from the in situ <span class="hlt">wave</span> buoy. Although the <span class="hlt">wave</span> and wind conditions during the field test were complex, the comparison showed a promising reconstruction of the <span class="hlt">wave</span> spectral shape, where both peaks in the bimodal spectrum were represented. However, the total reconstructed spectral energy (across all directions and frequencies) was limited to 44% of the observed spectrum. Overall, <span class="hlt">wave-by-wave</span> forecasting using a data assimilation approach based on <span class="hlt">wave</span> imaging radar observations and a physics-based <span class="hlt">wave</span> model shows promise for short</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSV...414..259S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSV...414..259S"><span>Analytical solution for the transient <span class="hlt">wave</span> propagation of a buried cylindrical P-<span class="hlt">wave</span> line source in a semi-infinite elastic medium with a fluid surface layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shan, Zhendong; Ling, Daosheng</p> <p>2018-02-01</p> <p>This article develops an analytical solution for the transient <span class="hlt">wave</span> propagation of a cylindrical P-<span class="hlt">wave</span> line source in a semi-infinite elastic solid with a fluid layer. The analytical solution is presented in a simple closed form in which each term represents a transient physical <span class="hlt">wave</span>. The Scholte equation is derived, through which the Scholte <span class="hlt">wave</span> velocity can be determined. The Scholte <span class="hlt">wave</span> is the <span class="hlt">wave</span> that propagates along the interface between the fluid and solid. To develop the analytical solution, the <span class="hlt">wave</span> fields in the fluid and solid are defined, their analytical solutions in the Laplace domain are derived using the boundary and interface conditions, and the solutions are then decomposed into series form according to the power series expansion method. Each item of the series solution has a clear physical meaning and represents a transient <span class="hlt">wave</span> path. Finally, by applying Cagniard's method and the convolution theorem, the analytical solutions are transformed into the time domain. Numerical examples are provided to illustrate some interesting features in the fluid layer, the interface and the semi-infinite solid. When the P-<span class="hlt">wave</span> velocity in the fluid is higher than that in the solid, two <span class="hlt">head</span> <span class="hlt">waves</span> in the solid, one <span class="hlt">head</span> <span class="hlt">wave</span> in the fluid and a Scholte <span class="hlt">wave</span> at the interface are observed for the cylindrical P-<span class="hlt">wave</span> line source.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H13H1488M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H13H1488M"><span>Freshwater-Brine Mixing <span class="hlt">Zone</span> Hydrodynamics in Salt Flats (Salar de Atacama)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marazuela, M. A.; Vázquez-Suñé, E.; Custodio, E.; Palma, T.; García-Gil, A.</p> <p>2017-12-01</p> <p>The increase in the demand of strategic minerals for the development of medicines and batteries require detailed knowledge of the salt flats freshwater-brine interface to make its exploitation efficient. The interface <span class="hlt">zone</span> is the result of a physical balance between the recharged and evaporated water. The sharp interface approach assumes the immiscibility of the fluids and thus neglects the mixing between them. As a consequence, for miscible fluids it is more accurate and often needed to use the mixing <span class="hlt">zone</span> concept, which results from the dynamic equilibrium of flowing freshwater and brine. In this study, we consider two and three-dimensional scale approaches for the management of the mixing <span class="hlt">zone</span>. The two-dimensional approach is used to understand the dynamics and the characteristics of the salt flat mixing <span class="hlt">zone</span>, especially in the Salar de Atacama (Atacama salt flat) case. By making use of this model we analyze and quantify the effects of the aquitards on the mixing <span class="hlt">zone</span> geometry. However, the understanding of the complex physical processes occurring in the salt flats and the management of these environments requires the adoption of three-dimensional regional scale numerical models. The models that take into account the effects of variable density represent the best management tool, but they require large computational resources, especially in the three-dimensional case. In order to avoid these computational limitations in the modeling of salt flats and their valuable ecosystems, we propose a three-step methodology, consisting of: (1) collection, validation and interpretation of the hydrogeochemical data, (2) identification and three-dimensional mapping of the mixing <span class="hlt">zone</span> on the land surface and in depth, and (3) application of a water <span class="hlt">head</span> correction to the freshwater and mixed water <span class="hlt">heads</span> in order to compensate the density variations and to transform them to brine water <span class="hlt">heads</span>. Finally, an evaluation of the sensibility of the mixing <span class="hlt">zone</span> to anthropogenic and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090002661','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090002661"><span>Tape Placement <span class="hlt">Head</span> for Applying Thermoplastic Tape to an Object</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cope, Ralph D. (Inventor); Funck, Steve B. (Inventor); Gruber, Mark B. (Inventor); Lamontia, Mark A. (Inventor); Johnson, Anthony D. (Inventor)</p> <p>2008-01-01</p> <p>A tape placement <span class="hlt">head</span> for applying thermoplastic tape to an object includes a heated feeder which guides the tape/tow to a heated <span class="hlt">zone</span>. The heated <span class="hlt">zone</span> has a line compactor having a single row of at least one movable heated member. An area compactor is located in the heated <span class="hlt">zone</span> downstream from the line compactor. The area compactor includes a plurality of rows of movable feet which are extendable toward the tape/tow different distances with respect to each other to conform to the shape of the object. A shim is located between the heated compactors and the tape/tow. A chilled compactor is in a chilled <span class="hlt">zone</span> downstream from the heated <span class="hlt">zone</span>. The chilled <span class="hlt">zone</span> includes a line chilled compactor and an area chilled compactor. A chilled shim is mounted between the chilled compactor and the tape/tow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23306446','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23306446"><span>Position control of desiccation cracks by memory effect and Faraday <span class="hlt">waves</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nakayama, Hiroshi; Matsuo, Yousuke; Takeshi, Ooshida; Nakahara, Akio</p> <p>2013-01-01</p> <p>Pattern formation of desiccation cracks on a layer of a calcium carbonate paste is studied experimentally. This paste is known to exhibit a memory effect, which means that a short-time application of horizontal vibration to the fresh paste predetermines the direction of the cracks that are formed after the paste is dried. While the position of the cracks (as opposed to their direction) is still stochastic in the case of horizontal vibration, the present work reports that their positioning is also controllable, at least to some extent, by applying vertical vibration to the paste and imprinting the pattern of Faraday <span class="hlt">waves</span>, thus breaking the translational symmetry of the system. The experiments show that the cracks tend to appear in the node <span class="hlt">zones</span> of the Faraday <span class="hlt">waves</span>: in the case of stripe-patterned Faraday <span class="hlt">waves</span>, the cracks are formed twice more frequently in the node <span class="hlt">zones</span> than in the anti-node <span class="hlt">zones</span>, presumably due to the localized horizontal motion. As a result of this preference of the cracks to the node <span class="hlt">zones</span>, the memory of the square lattice pattern of Faraday <span class="hlt">waves</span> makes the cracks run in the oblique direction differing by 45 degrees from the intuitive lattice direction of the Faraday <span class="hlt">waves</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016LatJP..53c..22B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016LatJP..53c..22B"><span><span class="hlt">Wave</span> Energy Potential in the Latvian EEZ</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beriņš, J.; Beriņš, J.; Kalnačs, J.; Kalnačs, A.</p> <p>2016-06-01</p> <p>The present article deals with one of the alternative forms of energy - sea <span class="hlt">wave</span> energy potential in the Latvian Exclusice Economic <span class="hlt">Zone</span> (EEZ). Results have been achieved using a new method - VEVPP. Calculations have been performed using the data on <span class="hlt">wave</span> parameters over the past five years (2010-2014). We have also considered <span class="hlt">wave</span> energy potential in the Gulf of Riga. The conclusions have been drawn on the recommended methodology for the sea <span class="hlt">wave</span> potential and power calculations for <span class="hlt">wave</span>-power plant pre-design stage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRB..123.2410G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRB..123.2410G"><span>The Origin and Mantle Dynamics of Quaternary Intraplate Volcanism in Northeast China From Joint Inversion of Surface <span class="hlt">Wave</span> and Body <span class="hlt">Wave</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Zhen; Wang, Kai; Yang, Yingjie; Tang, Youcai; John Chen, Y.; Hung, Shu-Huei</p> <p>2018-03-01</p> <p>We present a 3-D model of NE China by joint inversion of body and surface <span class="hlt">waves</span>. The joint inversion significantly improves the resolution at shallow depths compared with body <span class="hlt">wave</span> tomography alone and provides seismic evidence for the origin of Quaternary volcanism in NE China. Our model reveals that the mantle upwelling beneath the Changbaishan volcano originates from the transition <span class="hlt">zone</span> and extends up to 60 km, and spreads at the base of the lithosphere with the upwelling <span class="hlt">head</span> 5 times wider than the raising tail in the lower upper mantle. However, low velocities beneath the Halaha and Abaga volcanoes in the Xingmeng belt are confined to depths shallower than 150 km, suggesting that magmatism in the Xingmeng belt is more likely caused by localized asthenospheric upwelling at shallow depths rather than from the common deep source. A small-scale sublithospheric mantle convection may control the spatial and temporal distribution of Quaternary magmatism in NE China; that is, the upwelling beneath the Changbaishan volcano triggers the downwelling beneath the southern Songliao basin, where the high velocity imaged extends to 300 km. The downwelling may further induce localized upwelling in the surrounding areas, such as the Halaha and Abaga volcanoes. Thanks to the joint constraints from both surface and body <span class="hlt">waves</span>, we can estimate the dimension of the convection cell. The convection cell is located between 42°N and 45°N, spreads around 500 km in the W-E direction measured from the distance between centers of downwelling and upwelling, and extends to 300 km vertically.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSMG54B2040R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSMG54B2040R"><span>The Effect of Vegetation on Sea-Swell <span class="hlt">Waves</span>, Infragravity <span class="hlt">Waves</span> and <span class="hlt">Wave</span>-Induced Setup</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roelvink, J. A.; van Rooijen, A.; McCall, R. T.; Van Dongeren, A.; Reniers, A.; van Thiel de Vries, J.</p> <p>2016-02-01</p> <p>Aquatic vegetation in the coastal <span class="hlt">zone</span> (e.g. mangrove trees) attenuates <span class="hlt">wave</span> energy and thereby reduces flood risk along many shorelines worldwide. However, in addition to the attenuation of incident-band (sea-swell) <span class="hlt">waves</span>, vegetation may also affect infragravity-band (IG) <span class="hlt">waves</span> and the <span class="hlt">wave</span>-induced water level setup (in short: <span class="hlt">wave</span> setup). Currently, knowledge on the effect of vegetation on IG <span class="hlt">waves</span> and <span class="hlt">wave</span> setup is lacking, while they are they are key parameters for coastal risk assessment. In this study, the process-based storm impact model XBeach was extended with formulations for attenuation of sea-swell and IG <span class="hlt">waves</span> as well as the effect on the <span class="hlt">wave</span> setup, in two modes: the sea-swell <span class="hlt">wave</span> phase-resolving (non-hydrostatic) and the phase-averaged (surfbeat) mode. In surfbeat mode a <span class="hlt">wave</span> shape model was implemented to estimate the <span class="hlt">wave</span> phase and to capture the intra-<span class="hlt">wave</span> scale effect of emergent vegetation and nonlinear <span class="hlt">waves</span> on the <span class="hlt">wave</span> setup. Both modeling modes were validated using data from two flume experiments and show good skill in computing the attenuation of both sea-swell and IG <span class="hlt">waves</span> as well as the effect on the <span class="hlt">wave</span>-induced water level setup. In surfbeat mode, the prediction of nearshore mean water levels greatly improved when using the <span class="hlt">wave</span> shape model, while in non-hydrostatic mode this effect is directly accounted for. Subsequently, the model was used to study the influence of the bottom profile slope and the location of the vegetation field on the computed <span class="hlt">wave</span> setup with and without vegetation. It was found that the reduction is <span class="hlt">wave</span> setup is strongly related to the location of vegetation relative to the <span class="hlt">wave</span> breaking point, and that the <span class="hlt">wave</span> setup is lower for milder slopes. The extended version of XBeach developed within this study can be used to study the nearshore hydrodynamics on coasts fronted by vegetation such as mangroves. It can also serve as tool for storm impact studies on coasts with aquatic vegetation, and can help to quantify the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NHESS..17.2335W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NHESS..17.2335W"><span>Structural analysis of S-<span class="hlt">wave</span> seismics around an urban sinkhole: evidence of enhanced dissolution in a strike-slip fault <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wadas, Sonja H.; Tanner, David C.; Polom, Ulrich; Krawczyk, Charlotte M.</p> <p>2017-12-01</p> <p>In November 2010, a large sinkhole opened up in the urban area of Schmalkalden, Germany. To determine the key factors which benefited the development of this collapse structure and therefore the dissolution, we carried out several shear-<span class="hlt">wave</span> reflection-seismic profiles around the sinkhole. In the seismic sections we see evidence of the Mesozoic tectonic movement in the form of a NW-SE striking, dextral strike-slip fault, known as the Heßleser Fault, which faulted and fractured the subsurface below the town. The strike-slip faulting created a <span class="hlt">zone</span> of small blocks ( < 100 m in size), around which steep-dipping normal faults, reverse faults and a dense fracture network serve as fluid pathways for the artesian-confined groundwater. The faults also acted as barriers for horizontal groundwater flow perpendicular to the fault planes. Instead groundwater flows along the faults which serve as conduits and forms cavities in the Permian deposits below ca. 60 m depth. Mass movements and the resulting cavities lead to the formation of sinkholes and dissolution-induced depressions. Since the processes are still ongoing, the occurrence of a new sinkhole cannot be ruled out. This case study demonstrates how S-<span class="hlt">wave</span> seismics can characterize a sinkhole and, together with geological information, can be used to study the processes that result in sinkhole formation, such as a near-surface fault <span class="hlt">zone</span> located in soluble rocks. The more complex the fault geometry and interaction between faults, the more prone an area is to sinkhole occurrence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S12A..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S12A..07C"><span>Shear-<span class="hlt">wave</span> Velocity Structure and Inter-Seismic Strain Accumulation in the Up-Dip Region of the Cascadia Subduction <span class="hlt">Zone</span>: Similarities to Tohoku?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Collins, J. A.; McGuire, J. J.; Wei, M.</p> <p>2013-12-01</p> <p>The up-dip region of subduction <span class="hlt">zone</span> thrusts is difficult to study using land-based seismic and geodetic networks, yet documenting its ability to store and release elastic strain is critical for understanding the mechanics of great subduction earthquakes and tsunami generation. The 2011 Tohoku earthquake produced extremely large slip in the shallowest portion of the subduction <span class="hlt">zone</span> beneath a region of the fore-arc that is comprised of extremely low-velocity, unconsolidated sediments [Tsuru et al. JGR 2012]. The influence of the sediment material properties on the co-seismic slip distribution and tsunami generation can be considerable through both the effects on the dynamic wavefield during the rupture [Kozdon and Dunham, BSSA 2012] and potentially the build up of strain during the inter-seismic period. As part of the 2010-2011 SeaJade experiment [Scherwath et al, EOS 2011], we deployed 10 ocean bottom seismographs (OBS) on the continental slope offshore of Vancouver Island in the region of the NEPTUNE Canada observatory. One goal of the experiment is to measure the shear modulus of the sediments lying above the subducting plate using the seafloor compliance technique. Using seafloor acceleration measured by broadband seismometer and seafloor pressure measured by Differential Pressure Gauge (DPG), we estimate the compliance spectrum in the infra-gravity <span class="hlt">wave</span> band (~0.002-0.04 Hz) at 9 sites following the methodology of Crawford et al. [JGR, 1991]. We calibrated DPG sensitivities using laboratory measurements and by comparing teleseismic Rayleigh arrivals recorded on the seismometer and DPG channels [Webb, pers. comm]. We correct the vertical-component seismometer data for tilt using the procedure of Crawford and Webb [BSSA, 2000], Corrections for the gravitational attraction of the surface gravity <span class="hlt">waves</span> [Crawford et al., JGR, 1998] are important at frequencies of 0.003-0.006 Hz only. Typically, the coherences are high (>0.7) in the 0.006 to 0.03 Hz range. We invert</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993nasa.reptQR...P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993nasa.reptQR...P"><span>System and method for cancelling expansion <span class="hlt">waves</span> in a <span class="hlt">wave</span> rotor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paxson, Daniel E.</p> <p>1993-12-01</p> <p>A <span class="hlt">wave</span> rotor system that is comprised of a <span class="hlt">wave</span> rotor coupled to first and second plates is described. Special ports are provided, one in each of the first and second end plates, to cancel expansion <span class="hlt">waves</span> generated by the release of working fluid from the <span class="hlt">wave</span> rotor. One of the expansion <span class="hlt">waves</span> is reflected in the <span class="hlt">wave</span> rotor from a reflecting portion and provided to the special port in the second end plate. Fluid present at the special port in the second end plate has a stagnation pressure and mass flow which is the same as that of the cells of the <span class="hlt">wave</span> rotor communicating with such special port. This allows for cancellation of the expansion <span class="hlt">wave</span> generated by the release of working fluid from the <span class="hlt">wave</span> rotor. The special port in the second end plate has a first end corresponding to the <span class="hlt">head</span> of the expansion <span class="hlt">wave</span> and a second end corresponding to the tail of the expansion <span class="hlt">wave</span>. Also, the special port is configured to continually change along the circumference of the second end plate to affect expansion <span class="hlt">wave</span> cancellation. An expansion <span class="hlt">wave</span> generated by a second release of working fluid from the <span class="hlt">wave</span> rotor is cancelled in a similar manner to that described above using a special port in the first end plate. The cycle of operation of the <span class="hlt">wave</span> rotor system is designed so that the stagnation pressure and mass flow of the fluid present at the special ports is the same so that the special ports may be connected by a common duct.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T51A2859G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T51A2859G"><span>Seismic Evidence of A Widely Distributed West Napa Fault <span class="hlt">Zone</span>, Hendry Winery, Napa, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldman, M.; Catchings, R.; Chan, J. H.; Criley, C.</p> <p>2015-12-01</p> <p>Following the 24 August 2014 Mw 6.0 South Napa earthquake, surface rupture was mapped along the West Napa Fault <span class="hlt">Zone</span> (WNFZ) for a distance of ~ 14 km and locally within <span class="hlt">zones</span> up to ~ 2 km wide. Near the northern end of the surface rupture, however, several strands coalesced to form a narrow, ~100-m-wide <span class="hlt">zone</span> of surface rupture. To determine the location, width, and shallow (upper few hundred meters) geometry of the fault <span class="hlt">zone</span>, we acquired an active-source seismic survey across the northern surface rupture in February 2015. We acquired both P- and S-<span class="hlt">wave</span> data, from which we developed reflection images and tomographic images of Vp, Vs, Vp/Vs, and Poisson's ratio of the upper 100 m. We also used small explosive charges within surface ruptures located ~600 m north of our seismic array to record fault-<span class="hlt">zone</span> guided <span class="hlt">waves</span>. Our data indicate that at the latitude of the Hendry Winery, the WNFZ is characterized by at least five fault traces that are spaced 60 to 200 m apart. <span class="hlt">Zones</span> of low-Vs, low-Vp/Vs, and disrupted reflectors highlight the fault traces on the tomography and reflection images. On peak-ground-velocity (PGV) plots, the most pronounced high-amplitude guided-<span class="hlt">wave</span> seismic energy coincides precisely with the mapped surface ruptures, and the guided <span class="hlt">waves</span> also show discrete high PGV <span class="hlt">zones</span> associated with unmapped fault traces east of the surface ruptures. Although the surface ruptures of the WNFZ were observed only over a 100-m-wide <span class="hlt">zone</span> at the Hendry Winery, our data indicate that the fault <span class="hlt">zone</span> is at least 400 m wide, which is probably a minimum width given the 400-m length of our seismic profile. Slip on the WNFZ is generally considered to be low relative to most other Bay Area faults, but we suggest that the West Napa Fault is a <span class="hlt">zone</span> of widely distributed shear, and to fully account for the total slip on the WNFZ, slip on all traces of this wide fault <span class="hlt">zone</span> must be considered.</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/2017AGUFMEP41E..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP41E..04B"><span>Numerical Modeling of Scour at the <span class="hlt">Head</span> of a Vertical-Wall Breakwater in <span class="hlt">Waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baykal, C.; Balcı, H. B.; Sumer, B. M.; Fuhrman, D. R.</p> <p>2017-12-01</p> <p>This study presents a 3D numerical modeling study on the flow and scour at the <span class="hlt">head</span> of a vertical-wall breakwater in regular <span class="hlt">waves</span>. The numerical model utilized in the study is based on that given by Jacobsen (2011). The present model has been applied successfully to the scour and backfilling beneath submarine pipelines by Fuhrman et al. (2014), and around a vertical cylindrical pile mounted on a horizontal plane sediment bed by Baykal et al. (2015, 2017). The model is composed of two main modules. The first module is the hydrodynamic model where Reynolds Averaged Navier Stokes (RANS) equations are solved with a k-ω turbulence closure. The second module is the morphologic model which comprises five sub-modules, namely; bed load, suspended load, sand slide, bed evolution and 3D mesh motion. The model is constructed in open-source CFD toolbox OpenFOAM. In this study, the model is applied to experimental data sets of Sumer and Fredsoe (1997) on the scour around a vertical-wall breakwater with a circular round <span class="hlt">head</span>. Here, it is given the preliminary results of bed evolution of Test-8 of Sumer and Fredsoe (1997) in which a vertical-wall breakwater <span class="hlt">head</span> with a width of B=140 mm is subjected to oscillatory flow with Tw=2.0 s and maximum orbital velocity at the bed Um=22cm/s, resulting in a Keulegan-Carpenter number, KC=3.14, close to KC experienced in real-life situations (KC = O(1)). The grain size is d=0.17 mm. The Shields parameter in the test case is given as θc=0.11, larger than the critical value for the initiation of motion implying that the scour is in the live-bed regime. The computational domain used in the simulations has the following dimensions: Length, l=40B, Width, w=20B, and Height, h=2B. The total number of cells is O(105) in the simulations. The scoured bed profile computed at the end of 3 periods of oscillatory flow of Test-8 is given in the figure below. The color scale in the figure is given for the ratio of bed elevation to the width of breakwater</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.T32A..03M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.T32A..03M"><span>Mantle Structure Beneath East Africa and Zambia from Body <span class="hlt">Wave</span> Tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mulibo, G.; Nyblade, A.; Tugume, F.</p> <p>2011-12-01</p> <p>In this study, P and S travel time residuals from teleseismic earthquakes recorded on over 60 temporary AfricaArray seismic stations deployed in Uganda, Kenya, Tanzania and Zambia between 2007 and 2011 are being inverted, together with travel time residuals from previous deployments, for a 3D image of mantle <span class="hlt">wave</span> speeds variations extending to a depth of 1200 km. Preliminary results show that at depths of 200 km of less, low <span class="hlt">wave</span> speed anomalies are well developed beneath the Eastern and Western Branches of the East African Rift System. At deep depths, the low <span class="hlt">wave</span> speed anomalies focus under the center and southern part of the East African Plateau and extend into the transition <span class="hlt">zone</span>. At transition <span class="hlt">zone</span> depths and within the top part of the lower mantle, the low <span class="hlt">wave</span> speed anomaly shifts to the southwest beneath Zambia, indicating that the low <span class="hlt">wave</span> speed anomaly is continuous across the transition <span class="hlt">zone</span> and that it extends into the lower mantle. This result suggests that the upper mantle low <span class="hlt">wave</span> speed anomaly beneath East Africa is connected to the African superplume anomaly in the lower mantle beneath southern Africa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T11D2645H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T11D2645H"><span>Widespread imaging of the lower crust, Moho, and upper mantle from Rayleigh <span class="hlt">waves</span>: A comparison of the Cascadia and Aleutian-Alaska subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haney, M. M.; Tsai, V. C.; Ward, K. M.</p> <p>2016-12-01</p> <p>Recently, Haney and Tsai (2015) developed a new approach to Rayleigh-<span class="hlt">wave</span> inversion based on assumptions that are similar to those used in the formulation of the Dix equation in reflection seismology. Here we apply the Dix technique to Rayleigh-<span class="hlt">wave</span> phase-velocity maps by Ekstrom (2013) and Ward (2015) of the contiguous US and Alaska, respectively, at periods between 12 and 45 s. We refine the initial Dix result with subsequent nonlinear inversion to estimate Moho depth together with shear-<span class="hlt">wave</span> velocity of the lower crust and upper mantle. In the contiguous US, the Moho we image agrees well with recent receiver function studies. There is an apparent deepening of the Moho to the west of the Cascades volcanic chain that we interpret as the waveguide interface transitioning to the slab due to the continental Moho becoming transparent above the mantle forearc. This feature abruptly terminates at the southern extent of the Cascadia subduction <span class="hlt">zone</span>. We compare the depths of this "apparent Moho" with published estimates of the depth to the Juan de Fuca Plate since, owing to the paucity of tectonic earthquakes, the Slab1.0 model is not defined in Cascadia. Our result in Alaska is the first regional Moho map derived explicitly from seismic <span class="hlt">waves</span>. We find that crustal thickness is generally correlated with topography, with thicker crust beneath mountain ranges in southern Alaska. North of the Denali Fault, the Moho is smoother than to the south and located at typical depths of 30-35 km. There are also indications that the waveguide interface we solve for beneath Prince William Sound is actually the subducting slab instead of the continental Moho. The slab structure beneath Prince William Sound extends further east than the Pacific slab represented in the Slab1.0 model. Using the limited number of broadband seismometers in the Aleutian Islands, we obtain preliminary estimates for the crustal structure beneath the western portion of the Aleutian-Alaska subduction <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29394948','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29394948"><span>High-energy extracorporeal shock <span class="hlt">wave</span> therapy for nontraumatic osteonecrosis of the femoral <span class="hlt">head</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Kai; Mao, Yuanqing; Qu, Xinhua; Dai, Kerong; Jia, Qingwei; Zhu, Zhenan; Yan, Mengning</p> <p>2018-02-02</p> <p>Nontraumatic osteonecrosis of the femoral <span class="hlt">head</span> (ONFH) is treated with a series of methods. High-energy extracorporeal shock <span class="hlt">wave</span> therapy (ESWT) is an option with promising mid-term outcomes. The objective of this study was to determine the long-term outcomes of ESWT for ONFH. Fifty-three hips in 39 consecutive patients were treated with ESWT in our hospital between January 2005 and July 2006. Forty-four hips in 31 patients with stage I-III nontraumatic ONFH, according to the Association Research Circulation Osseous (ARCO) system, were reviewed in the current retrospective study. The visual analog pain scale (VAS), Harris hip score, radiography, and magnetic resonance imaging were used to estimate treatment results. The progression of ONFH was evaluated by imaging examination and clinical outcomes. The results were classified as clinical success (no progression of hip symptoms) and imaging success (no progression of stage or substage on radiography and MRI). The mean follow-up duration was 130.6 months (range, 121 to 138 months). The mean VAS decreased from 3.8 before ESWT to 2.2 points at the 10-year follow-up (p < 0.001). The mean Harris hip score improved from 77.4 before ESWT to 86.9 points at the 10-year follow-up. The clinical success rates were 87.5% in ARCO stage I patients, 71.4% in ARCO stage II patients, and 75.0% in ARCO stage III patients. Imaging success was observed in all stage I hips, 64.3% of stage II hips, and 12.5% of stage III hips. Seventeen hips showed progression of the ARCO stage/substage on imaging examination. Eight hips showed femoral <span class="hlt">head</span> collapse at the 10-year follow-up. Four hips in ARCO stage III and one hip in ARCO stage II were treated with total hip arthroplasty during the follow-up. Three were performed 1 year after ESWT, one at 2 years, and one at 5 years. The results of the current study indicated that ESWT is an effective treatment method for nontraumatic ONFH, resulting in pain relief and function restoration</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1039876','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1039876"><span>Predicting DNAPL Source <span class="hlt">Zone</span> and Plume Response Using Site-Measured Characteristics</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-05-19</p> <p>FINAL REPORT Predicting DNAPL Source <span class="hlt">Zone</span> and Plume Response Using Site- Measured Characteristics SERDP Project ER-1613 MAY 2017...Final Report 3. DATES COVERED (From - To) 2007 - 2017 4. TITLE AND SUBTITLE PREDICTING DNAPL SOURCE <span class="hlt">ZONE</span> AND PLUME RESPONSE USING SITE- MEASURED ...historical record of concentration and <span class="hlt">head</span> measurements , particularly in the near-source region. For each site considered, currently available data</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JFM...529..279S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JFM...529..279S"><span>Kinematics and depth-integrated terms in surf <span class="hlt">zone</span> <span class="hlt">waves</span> from laboratory measurement</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stansby, Peter K.; Feng, Tong</p> <p>2005-04-01</p> <p>Kinematics of nominally periodic surf <span class="hlt">zone</span> <span class="hlt">waves</span> have been measured in the laboratory using LDA (laser Doppler anemometry), above trough level as well as below, for weakly plunging breakers transforming into bores in shallower water. The aim was to determine, through phase- or ensemble-averaging, periodic flow structures in a two-dimensional vertical plane, from large-scale down to small-scale vortical structures. Coherent multiple vortical structures were evident at the initiation of breaking, becoming elongated along the surface during bore propagation. The initial region is likely to become more extensive as <span class="hlt">waves</span> become more strongly plunging and could explain the difference in turbulence characteristics between plunging and spilling breakers observed elsewhere. Comparison of vorticity magnitudes with hydraulic-jump measurements showed some similarities during the initial stages of breaking, but these quickly grew less as breaking progressed into shallower water. Period-averaged kinematics and vorticity were also obtained showing shoreward mass transport above trough level and undertow below, with a thick layer of vorticity at trough level and a thin layer of vorticity of opposite rotation at the bed. There were also concentrated regions of mean vorticity near the end of the plunging region. Residual turbulence of relatively high frequency was presented as Reynolds stresses, showing marked anisotrophy. Dynamic pressure (pressure minus its hydrostatic component) was determined from the kinematics. The magnitudes of different effects were evaluated through the depth-integrated Reynolds-averaged Navier-Stokes (RANS) equations, which may be reduced to nine terms (the standard inviscid terms of the shallow-water equations conserving mass and momentum with hydrostatic pressure, and six additional terms), assuming that the complex, often aerated, free surface is treated as a simple interface. All terms were evaluated, assuming that a space/time transformation was</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDD34006K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDD34006K"><span>Influence of Internal <span class="hlt">Waves</span> on Transport by a Gravity Current</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koseff, Jeffrey; Hogg, Charlie; Ouillon, Raphael; Ouellette, Nicholas; Meiburg, Eckart</p> <p>2017-11-01</p> <p>Gravity currents moving along the continental slope can be influenced by internal <span class="hlt">waves</span> shoaling on the slope resulting in mixing between the gravity current and the ambient fluid. Whilst some observations of the potential influence of internal <span class="hlt">waves</span> on gravity currents have been made, the process has not been studied systematically. We present laboratory experiments, and some initial numerical simulations, in which a gravity current descends down a sloped boundary through a pycnocline at the same time as an internal <span class="hlt">wave</span> at the pycnocline shoals on the slope. Measurements of the downslope mass flux of the gravity current fluid in cases with different amplitudes of the incident internal <span class="hlt">wave</span> will be discussed. For the parameter regime considered, the mass flux in the <span class="hlt">head</span> of the gravity current was found to reduce with increasingly larger incident amplitude <span class="hlt">waves</span>. This reduction was effectively caused by a ``decapitation'' process whereby the breaking internal <span class="hlt">wave</span> captures and moves fluid from the <span class="hlt">head</span> of the gravity current back up the slope. The significance of the impact of the internal <span class="hlt">waves</span> on gravity current transport, strongly suggests that the local internal <span class="hlt">wave</span> climate may need to be considered when calculating gravity current transport. The Bob and Norma Street Environmental Fluid Mechanics Laboratory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714375A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714375A"><span>Laboratory modeling of edge <span class="hlt">wave</span> generation over a plane beach by breaking <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abcha, Nizar; Ezersky, Alexander; Pelinovsky, Efim</p> <p>2015-04-01</p> <p>Edge <span class="hlt">waves</span> play an important role in coastal hydrodynamics: in sediment transport, in formation of coastline structure and coastal bottom topography. Investigation of physical mechanisms leading to the edge <span class="hlt">waves</span> generation allows us to determine their effect on the characteristics of spatially periodic patterns like crescent submarine bars and cusps observed in the coastal <span class="hlt">zone</span>. In the present paper we investigate parametric excitation of edge <span class="hlt">wave</span> with frequency two times less than the frequency of surface <span class="hlt">wave</span> propagating perpendicular to the beach. Such mechanism of edge <span class="hlt">wave</span> generation has been studied previously in a large number of papers using the assumption of non-breaking <span class="hlt">waves</span>. This assumption was used in theoretical calculations and such conditions were created in laboratory experiments. In the natural conditions, the <span class="hlt">wave</span> breaking is typical when edge <span class="hlt">waves</span> are generated at sea beach. We study features of such processes in laboratory experiments. Experiments were performed in the <span class="hlt">wave</span> flume of the Laboratory of Continental and Coast Morphodynamics (M2C), Caen. The flume is equipment with a <span class="hlt">wave</span> maker controlled by computer. To model a plane beach, a PVC plate is placed at small angle to the horizontal bottom. Several resistive probes were used to measure characteristics of <span class="hlt">waves</span>: one of them was used to measure free surface displacement near the <span class="hlt">wave</span> maker and two probes were glued on the inclined plate. These probes allowed us to measure run-up due to parametrically excited edge <span class="hlt">waves</span>. Run-up height is determined by processing a movie shot by high-speed camera. Sub-harmonic generation of standing edge <span class="hlt">waves</span> is observed for definite control parameters: edge <span class="hlt">waves</span> represent themselves a spatial mode with wavelength equal to double width of the flume; the frequency of edge <span class="hlt">wave</span> is equal to half of surface <span class="hlt">wave</span> frequency. Appearance of sub-harmonic mode instability is studied using probes and movie processing. The dependence of edge <span class="hlt">wave</span> exponential</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S41C0813D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S41C0813D"><span>Seismic <span class="hlt">Wave</span> Velocity in the Subducted Oceanic Crust from Autocorrelation of Tectonic Tremor Signals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ducellier, A.; Creager, K.</p> <p>2017-12-01</p> <p>Hydration and dehydration of minerals in subduction <span class="hlt">zones</span> play a key role in the geodynamic processes that generate seismicity and that allow tectonic plates to subduct. Detecting the presence of water in the subducted plate is thus crucial to better understand the seismogenesis and the consequent seismic hazard. A landward dipping, low velocity layer has been detected in most subduction <span class="hlt">zones</span>. In Cascadia, this low velocity <span class="hlt">zone</span> is characterized by a low S-<span class="hlt">wave</span> velocity and a very high Poisson's ratio, which has been interpreted as high pore-fluid pressure in the upper half part of the subducted oceanic crust. Most previous studies were based on seismic reflection imaging, receiver function analysis, or body <span class="hlt">wave</span> tomography, with seismic sources located far from the low velocity <span class="hlt">zone</span>. In contrast, the sources of the tectonic tremors generated during Episodic Tremor and Slip (ETS) events are located on the plate boundary. As the sources of the tremors are much closer to the low velocity <span class="hlt">zone</span>, seismic <span class="hlt">waves</span> recorded during ETS events should illuminate the area with greater precision. Most methods to detect and locate tectonic tremors and low-frequency earthquakes are based on the cross correlation of seismic signals; either signals at the same station for different events, or the same event at different stations. We use the autocorrelation of the seismic signal recorded by eight arrays of stations, located in the Olympic Peninsula, Washington. Each tremor, assumed to be on the plate boundary, generates a direct <span class="hlt">wave</span> and reflected and converted <span class="hlt">waves</span> from both the strong shear-<span class="hlt">wave</span> velocity contrast in the mid-oceanic crust, and from the Moho of the subducted oceanic crust. The time lag between the arrivals of these different <span class="hlt">waves</span> at a seismic station corresponds to a peak of amplitude on the autocorrelation signals. Using the time lags observed for different locations of the tremor source, we intend to invert for the seismic <span class="hlt">wave</span> velocity of the subducted oceanic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wsp/2331/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wsp/2331/report.pdf"><span>Simulation of saltwater movement in the Floridan aquifer system, Hilton <span class="hlt">Head</span> Island, South Carolina</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bush, Peter W.</p> <p>1988-01-01</p> <p>Freshwater to supply Hilton <span class="hlt">Head</span> Island, S.C., is obtained from the upper permeable <span class="hlt">zone</span> of the Upper Floridan aquifer. Long-term pumping at Savannah, Ga., and the steadily increasing pumping on Hilton <span class="hlt">Head</span> Island, have lowered Upper Floridan <span class="hlt">heads</span> near the center of the island from about 10 feet above sea level to about 6 to 7 feet below sea level. The seaward hydraulic gradient that existed before pumping began has been reversed, thus increasing the potential for saltwater intrusion. Simulations of predevelopment, recent, and future ground-water flow in the Floridan aquifer system beneath the north end of Hilton <span class="hlt">Head</span> Island and Port Royal Sound are presented. A finite-element model for fluid-density-dependent ground-water flow and solute transport was used in cross section. The general configuration of the simulated predevelopment flowfield is typical of a coastal aquifer having a seaward gradient in the freshwater. The freshwater flows toward Port Royal Sound over an intruding wedge of saltwater. The simulated flowfield at the end of 1983 shows that ground water in the Floridan aquifer system beneath most of Hilton <span class="hlt">Head</span> Island has reversed its predevelopment direction and is moving toward Savannah. The distribution of chloride concentrations, based on simulation at the end of 1983, is about the same as the predevelopment distribution of chloride concentrations obtained from simulation. Results of two 50-year simulations from 1983 to 2034 suggest that there will be no significant threat of saltwater intrusion into the upper permeable <span class="hlt">zone</span> of the Upper Floridan aquifer if <span class="hlt">heads</span> on Hilton <span class="hlt">Head</span> Island remain at current levels for the next 45 to 50 years. However, if <span class="hlt">head</span> decline continues at the historical rate, any flow that presently occurs from the north end of the island toward Port Royal Sound will cease, allowing lateral intrusion of saltwater to proceed. Even under these conditions, chloride concentrations in the upper permeable <span class="hlt">zone</span> of the Upper Floridan</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015987','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015987"><span>Acceleration spectra for subduction <span class="hlt">zone</span> earthquakes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Boatwright, J.; Choy, G.L.</p> <p>1989-01-01</p> <p>We estimate the source spectra of shallow earthquakes from digital recordings of teleseismic P <span class="hlt">wave</span> groups, that is, P+pP+sP, by making frequency dependent corrections for the attenuation and for the interference of the free surface. The correction for the interference of the free surface assumes that the earthquake radiates energy from a range of depths. We apply this spectral analysis to a set of 12 subduction <span class="hlt">zone</span> earthquakes which range in size from Ms = 6.2 to 8.1, obtaining corrected P <span class="hlt">wave</span> acceleration spectra on the frequency band from 0.01 to 2.0 Hz. Seismic moment estimates from surface <span class="hlt">waves</span> and normal modes are used to extend these P <span class="hlt">wave</span> spectra to the frequency band from 0.001 to 0.01 Hz. The acceleration spectra of large subduction <span class="hlt">zone</span> earthquakes, that is, earthquakes whose seismic moments are greater than 1027 dyn cm, exhibit intermediate slopes where u(w)???w5/4 for frequencies from 0.005 to 0.05 Hz. For these earthquakes, spectral shape appears to be a discontinuous function of seismic moment. Using reasonable assumptions for the phase characteristics, we transform the spectral shape observed for large earthquakes into the time domain to fit Ekstrom's (1987) moment rate functions for the Ms=8.1 Michoacan earthquake of September 19, 1985, and the Ms=7.6 Michoacan aftershock of September 21, 1985. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850021594','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850021594"><span>Turbulence and <span class="hlt">wave</span> particle interactions in solar-terrestrial plasmas</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dulk, G. A.; Goldman, M. V.; Toomre, J.</p> <p>1985-01-01</p> <p>Activities in the following study areas are reported: (1) particle and <span class="hlt">wave</span> processes in solar flares; (2) solar convection <span class="hlt">zone</span> turbulence; and (3) solar radiation emission. To investigate the amplification of cyclotron maser radiation in solar flares, a radio frequency. (RF) heating model was developed for the corona surrounding the energy release site. Then nonlinear simulations of compressible convection display prominent penetration by plumes into regions of stable stratification at the base of the solar convection <span class="hlt">zone</span>, leading to the excitation of internal gravity <span class="hlt">waves</span> there. Lastly, linear saturation of electron-beam-driven Langmuir <span class="hlt">waves</span> by ambient density fluctuations, nonlinear saturation by strong turbulence processes, and radiation emission mechanisms are examined. An additional section discusses solar magnetic fields and hydromagnetic <span class="hlt">waves</span> in inhomogeneous media, and the effect of magnetic fields on stellar oscillation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70135102','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70135102"><span>Vertical structure of mean cross-shore currents across a barred surf <span class="hlt">zone</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>Haines, John W.; Sallenger, Asbury H.</p> <p>1994-01-01</p> <p>Mean cross-shore currents observed across a barred surf <span class="hlt">zone</span> are compared to model predictions. The model is based on a simplified momentum balance with a turbulent boundary layer at the bed. Turbulent exchange is parameterized by an eddy viscosity formulation, with the eddy viscosity Aυ independent of time and the vertical coordinate. Mean currents result from gradients due to <span class="hlt">wave</span> breaking and shoaling, and the presence of a mean setup of the free surface. Descriptions of the <span class="hlt">wave</span> field are provided by the <span class="hlt">wave</span> transformation model of Thornton and Guza [1983]. The <span class="hlt">wave</span> transformation model adequately reproduces the observed <span class="hlt">wave</span> heights across the surf <span class="hlt">zone</span>. The mean current model successfully reproduces the observed cross-shore flows. Both observations and predictions show predominantly offshore flow with onshore flow restricted to a relatively thin surface layer. Successful application of the mean flow model requires an eddy viscosity which varies horizontally across the surf <span class="hlt">zone</span>. Attempts are made to parameterize this variation with some success. The data does not discriminate between alternative parameterizations proposed. The overall variability in eddy viscosity suggested by the model fitting should be resolvable by field measurements of the turbulent stresses. Consistent shortcomings of the parameterizations, and the overall modeling effort, suggest avenues for further development and data collection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4526238','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4526238"><span>Analysis of Rapid Multi-Focal <span class="hlt">Zone</span> ARFI Imaging</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rosenzweig, Stephen; Palmeri, Mark; Nightingale, Kathryn</p> <p>2015-01-01</p> <p>Acoustic radiation force impulse (ARFI) imaging has shown promise for visualizing structure and pathology within multiple organs; however, because the contrast depends on the push beam excitation width, image quality suffers outside of the region of excitation. Multi-focal <span class="hlt">zone</span> ARFI imaging has previously been used to extend the region of excitation (ROE), but the increased acquisition duration and acoustic exposure have limited its utility. Supersonic shear <span class="hlt">wave</span> imaging has previously demonstrated that through technological improvements in ultrasound scanners and power supplies, it is possible to rapidly push at multiple locations prior to tracking displacements, facilitating extended depth of field shear <span class="hlt">wave</span> sources. Similarly, ARFI imaging can utilize these same radiation force excitations to achieve tight pushing beams with a large depth of field. Finite element method simulations and experimental data are presented demonstrating that single- and rapid multi-focal <span class="hlt">zone</span> ARFI have comparable image quality (less than 20% loss in contrast), but the multi-focal <span class="hlt">zone</span> approach has an extended axial region of excitation. Additionally, as compared to single push sequences, the rapid multi-focal <span class="hlt">zone</span> acquisitions improve the contrast to noise ratio by up to 40% in an example 4 mm diameter lesion. PMID:25643078</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19495329','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19495329"><span>Analysis of <span class="hlt">wave</span> propagation in a two-dimensional photonic crystal with negative index of refraction: plane <span class="hlt">wave</span> decomposition of the Bloch modes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martínez, Alejandro; Míguez, Hernán; Sánchez-Dehesa, José; Martí, Javier</p> <p>2005-05-30</p> <p>This work presents a comprehensive analysis of electromagnetic <span class="hlt">wave</span> propagation inside a two-dimensional photonic crystal in a spectral region in which the crystal behaves as an effective medium to which a negative effective index of refraction can be associated. It is obtained that the main plane <span class="hlt">wave</span> component of the Bloch mode that propagates inside the photonic crystal has its <span class="hlt">wave</span> vector k' out of the first Brillouin <span class="hlt">zone</span> and it is parallel to the Poynting vector ( S' ? k'> 0 ), so light propagation in these composites is different from that reported for left-handed materials despite the fact that negative refraction can take place at the interface between air and both kinds of composites. However, <span class="hlt">wave</span> coupling at the interfaces is well explained using the reduced <span class="hlt">wave</span> vector ( k' ) in the first Brillouin <span class="hlt">zone</span>, which is opposed to the energy flow, and agrees well with previous works dealing with negative refraction in photonic crystals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/6183206','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/6183206"><span>Experimental high-velocity missile <span class="hlt">head</span> injury.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Allen, I V; Scott, R; Tanner, J A</p> <p>1982-09-01</p> <p>A standardized experimental high-velocity penetrating <span class="hlt">head</span>-injury model has been produced in which pathological lesions were observed, not only in the wound track but at sites more remote from the track in the hypothalamus, brain stem and cerebellum. Diffuse subarachnoid haemorrhage was common and intraventricular haemorrhage was a constant feature. Other constant histological abnormalities were:L 1. Perivascular "ring' haemorrhages. 2. Perivascular haemorrhage with a surrounding <span class="hlt">zone</span> of decreased staining intensity. 3. Perivascular increased staining intensity. 4. Areas of decreased staining intensity apparently dissociated from areas of haemorrhage. The pathogenesis of the perivascular lesions is discussed and preliminary studies suggest that these may be the site of early oedema. The implications of this experiment for military surgery and for ballistic protection of the <span class="hlt">head</span> are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=304418','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=304418"><span><span class="hlt">Wave</span> energy and intertidal productivity</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Leigh, Egbert G.; Paine, Robert T.; Quinn, James F.; Suchanek, Thomas H.</p> <p>1987-01-01</p> <p>In the northeastern Pacific, intertidal <span class="hlt">zones</span> of the most <span class="hlt">wave</span>-beaten shores receive more energy from breaking <span class="hlt">waves</span> than from the sun. Despite severe mortality from winter storms, communities at some <span class="hlt">wave</span>-beaten sites produce an extraordinary quantity of dry matter per unit area of shore per year. At <span class="hlt">wave</span>-beaten sites of Tatoosh Island, WA, sea palms, Postelsia palmaeformis, can produce > 10 kg of dry matter, or 1.5 × 108 J, per m2 in a good year. Extraordinarily productive organisms such as Postelsia are restricted to <span class="hlt">wave</span>-beaten sites. Intertidal organisms cannot transform <span class="hlt">wave</span> energy into chemical energy, as photosynthetic plants transform solar energy, nor can intertidal organisms “harness” <span class="hlt">wave</span> energy. Nonetheless, <span class="hlt">wave</span> energy enhances the productivity of intertidal organisms. On exposed shores, <span class="hlt">waves</span> increase the capacity of resident algae to acquire nutrients and use sunlight, augment the competitive ability of productive organisms, and protect intertidal residents by knocking away their enemies or preventing them from feeding. PMID:16593813</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AcAau.135..114S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AcAau.135..114S"><span>Detonation onset following shock <span class="hlt">wave</span> focusing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smirnov, N. N.; Penyazkov, O. G.; Sevrouk, K. L.; Nikitin, V. F.; Stamov, L. I.; Tyurenkova, V. V.</p> <p>2017-06-01</p> <p>The aim of the present paper is to study detonation initiation due to focusing of a shock <span class="hlt">wave</span> reflected inside a cone. Both numerical and experimental investigations were conducted. Comparison of results made it possible to validate the developed 3-d transient mathematical model of chemically reacting gas mixture flows incorporating hydrogen - air mixtures. The results of theoretical and numerical experiments made it possible improving kinetic schemes and turbulence models. Several different flow scenarios were detected in reflection of shock <span class="hlt">waves</span> all being dependent on incident shock <span class="hlt">wave</span> intensity: reflecting of shock <span class="hlt">wave</span> with lagging behind combustion <span class="hlt">zone</span>, formation of detonation <span class="hlt">wave</span> in reflection and focusing, and intermediate transient regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034824','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034824"><span>Shallow seismic structure of Kunlun fault <span class="hlt">zone</span> in northern Tibetan Plateau, China: Implications for the 2001 M s8.1 Kunlun 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>Wang, Chun-Yong; Mooney, W.D.; Ding, Z.; Yang, J.; Yao, Z.; Lou, H.</p> <p>2009-01-01</p> <p>The shallow seismic velocity structure of the Kunlun fault <span class="hlt">zone</span> (KLFZ) was jointly deduced from seismic refraction profiling and the records of trapped <span class="hlt">waves</span> that were excited by five explosions. The data were collected after the 2001 Kunlun M s8.1 earthquake in the northern Tibetan Plateau. Seismic phases for the in-line record sections (26 records up to a distance of 15 km) along the fault <span class="hlt">zone</span> were analysed, and 1-D P- and S-<span class="hlt">wave</span> velocity models of shallow crust within the fault <span class="hlt">zone</span> were determined by using the seismic refraction method. Sixteen seismic stations were deployed along the off-line profile perpendicular to the fault <span class="hlt">zone</span>. Fault-<span class="hlt">zone</span> trapped <span class="hlt">waves</span> appear clearly on the record sections, which were simulated with a 3-D finite difference algorithm. Quantitative analysis of the correlation coefficients of the synthetic and observed trapped waveforms indicates that the Kunlun fault-<span class="hlt">zone</span> width is 300 m, and S-<span class="hlt">wave</span> quality factor Q within the fault <span class="hlt">zone</span> is 15. Significantly, S-<span class="hlt">wave</span> velocities within the fault <span class="hlt">zone</span> are reduced by 30-45 per cent from surrounding rocks to a depth of at least 1-2 km, while P-<span class="hlt">wave</span> velocities are reduced by 7-20 per cent. A fault-<span class="hlt">zone</span> with such P- and S-low velocities is an indication of high fluid pressure because Vs is affected more than Vp. The low-velocity and low-Q <span class="hlt">zone</span> in the KLFZ model is the effect of multiple ruptures along the fault trace of the 2001 M s8.1 Kunlun earthquake. ?? 2009 The Authors Journal compilation ?? 2009 RAS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.712..623N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.712..623N"><span>Attenuation of Lg <span class="hlt">waves</span> in the New Madrid seismic <span class="hlt">zone</span> of the central United States using the coda normalization method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nazemi, Nima; Pezeshk, Shahram; Sedaghati, Farhad</p> <p>2017-08-01</p> <p>Unique properties of coda <span class="hlt">waves</span> are employed to evaluate the frequency dependent quality factor of Lg <span class="hlt">waves</span> using the coda normalization method in the New Madrid seismic <span class="hlt">zone</span> of the central United States. Instrument and site responses are eliminated and source functions are isolated to construct the inversion problem. For this purpose, we used 121 seismograms from 37 events with moment magnitudes, M, ranging from 2.5 to 5.2 and hypocentral distances from 120 to 440 km recorded by 11 broadband stations. A singular value decomposition (SVD) algorithm is used to extract Q values from the data, while the geometric spreading exponent is assumed to be a constant. Inversion results are then fitted with a power law equation from 3 to 12 Hz to derive the frequency dependent quality factor function. The final results of the analysis are QVLg (f) = (410 ± 38) f0.49 ± 0.05 for the vertical component and QHLg (f) = (390 ± 26) f0.56 ± 0.04 for the horizontal component, where the term after ± sign represents one standard error. For stations within the Mississippi embayment with an average sediment depth of 1 km around the Memphis metropolitan area, estimation of quality factor using the coda normalization method is not well-constrained at low frequencies (f < 3 Hz). There may be several reasons contributing to this issue, such as low frequency surface <span class="hlt">wave</span> contamination, site effects, or even a change in coda <span class="hlt">wave</span> scattering regime which can exacerbate the scatter of the data.</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('http://adsabs.harvard.edu/abs/2001AGUSM...S32A05P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUSM...S32A05P"><span>Receiver Functions From Regional and Near-Teleseismic P <span class="hlt">Waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, J.; Levin, V.</p> <p>2001-05-01</p> <p>P <span class="hlt">waves</span> from regional-distance earthquakes are complex and reverberatory, as would be expected from a combination of <span class="hlt">head</span> <span class="hlt">waves</span>, post-critical crustal reflections and shallow-incident P from the upper mantle. Although developed to analyze steeply-incident teleseismic P <span class="hlt">waves</span>, receiver function analysis can also retrieve information about crustal structure from regional and near-teleseismic P. Using a new method to estimate receiver functions, based on multiple-taper spectral analysis, regional-distance RFs for GSN stations RAYN and ANTO show broad agreement with teleseismic RFs. At RAYN the moveout of the Moho-converted Ps phase, relative to direct P, follows well the predictions of the IASP91 earth model. The Moho-converted Ps phase shows complexity associated with the transition-<span class="hlt">zone</span> triplication near Δ =20o and constant delay (zero moveout) as Δ -> 0, consistent with conversion from Pn. Similar behavior is seen for ANTO for events that arrive from the west. For eastern backazimuths the ANTO RFs show features whose moveout is negative as Δ -> 0. This moveout is poorly fit by reverberations in flat layers or by direct scattering from a dipping interface, but is consistent with a topographic scatterer 20--30 km eastward of the ANTO site. Regional receiver functions may therefore be useful in judging whether teleseismic RFs at a particular station are suitable candidates for a 1-D velocity structure inversion. Synthetic seismograms of regional P phases, computed with a locked-mode reflectivity approach, confirm broad features of the RAYN and ANTO regional receiver functions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvF...2e3201M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvF...2e3201M"><span>Propagation of gaseous detonation <span class="hlt">waves</span> in a spatially inhomogeneous reactive medium</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mi, XiaoCheng; Higgins, Andrew J.; Ng, Hoi Dick; Kiyanda, Charles B.; Nikiforakis, Nikolaos</p> <p>2017-05-01</p> <p>Detonation propagation in a compressible medium wherein the energy release has been made spatially inhomogeneous is examined via numerical simulation. The inhomogeneity is introduced via step functions in the reaction progress variable, with the local value of energy release correspondingly increased so as to maintain the same average energy density in the medium and thus a constant Chapman-Jouguet (CJ) detonation velocity. A one-step Arrhenius rate governs the rate of energy release in the reactive <span class="hlt">zones</span>. The resulting dynamics of a detonation propagating in such systems with one-dimensional layers and two-dimensional squares are simulated using a Godunov-type finite-volume scheme. The resulting <span class="hlt">wave</span> dynamics are analyzed by computing the average <span class="hlt">wave</span> velocity and one-dimensional averaged <span class="hlt">wave</span> structure. In the case of sufficiently inhomogeneous media wherein the spacing between reactive <span class="hlt">zones</span> is greater than the inherent reaction <span class="hlt">zone</span> length, average <span class="hlt">wave</span> speeds significantly greater than the corresponding CJ speed of the homogenized medium are obtained. If the shock transit time between reactive <span class="hlt">zones</span> is less than the reaction time scale, then the classical CJ detonation velocity is recovered. The spatiotemporal averaged structure of the <span class="hlt">waves</span> in these systems is analyzed via a Favre-averaging technique, with terms associated with the thermal and mechanical fluctuations being explicitly computed. The analysis of the averaged <span class="hlt">wave</span> structure identifies the super-CJ detonations as weak detonations owing to the existence of mechanical nonequilibrium at the effective sonic point embedded within the <span class="hlt">wave</span> structure. The correspondence of the super-CJ behavior identified in this study with real detonation phenomena that may be observed in experiments is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P33D2902F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P33D2902F"><span>Imaging the Chicxulub central crater <span class="hlt">zone</span> from large scale seismic acoustic <span class="hlt">wave</span> propagation and gravity modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fucugauchi, J. U.; Ortiz-Aleman, C.; Martin, R.</p> <p>2017-12-01</p> <p>Large complex craters are characterized by central uplifts that represent large-scale differential movement of deep basement from the transient cavity. Here we investigate the central sector of the large multiring Chicxulub crater, which has been surveyed by an array of marine, aerial and land-borne geophysical methods. Despite high contrasts in physical properties,contrasting results for the central uplift have been obtained, with seismic reflection surveys showing lack of resolution in the central <span class="hlt">zone</span>. We develop an integrated seismic and gravity model for the main structural elements, imaging the central basement uplift and melt and breccia units. The 3-D velocity model built from interpolation of seismic data is validated using perfectly matched layer seismic acoustic <span class="hlt">wave</span> propagation modeling, optimized at grazing incidence using shift in the frequency domain. Modeling shows significant lack of illumination in the central sector, masking presence of the central uplift. Seismic energy remains trapped in an upper low velocity <span class="hlt">zone</span> corresponding to the sedimentary infill, melt/breccias and surrounding faulted blocks. After conversion of seismic velocities into a volume of density values, we use massive parallel forward gravity modeling to constrain the size and shape of the central uplift that lies at 4.5 km depth, providing a high-resolution image of crater structure.The Bouguer anomaly and gravity response of modeled units show asymmetries, corresponding to the crater structure and distribution of post-impact carbonates, breccias, melt and target sediments</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112t4101J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112t4101J"><span>Sharp acoustic vortex focusing by Fresnel-spiral <span class="hlt">zone</span> plates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiménez, Noé; Romero-García, Vicent; García-Raffi, Luis M.; Camarena, Francisco; Staliunas, Kestutis</p> <p>2018-05-01</p> <p>We report the optimal focusing of acoustic vortex beams by using flat lenses based on a Fresnel-spiral diffraction grating. The flat lenses are designed by spiral-shaped Fresnel <span class="hlt">zone</span> plates composed of one or several arms. The constructive and destructive interferences of the diffracted <span class="hlt">waves</span> by the spiral grating result in sharp acoustic vortex beams, following the focal laws obtained in analogy with the Fresnel <span class="hlt">zone</span> plate lenses. In addition, we show that the number of arms determines the topological charge of the vortex, allowing the precise manipulation of the acoustic <span class="hlt">wave</span> field by flat lenses. The experimental results in the ultrasonic regime show excellent agreement with the theory and full-<span class="hlt">wave</span> numerical simulations. A comparison with beam focusing by Archimedean spirals also showing vortex focusing is given. The results of this work may have potential applications for particle trapping, ultrasound therapy, imaging, or underwater acoustic transmitters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=348052','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=348052"><span>High-frequency surface <span class="hlt">waves</span> method for agricultural applications</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>A high-frequency surface <span class="hlt">wave</span> method has been recently developed to explore shallow soil in the vadose <span class="hlt">zone</span> for agricultural applications. This method is a modification from the conventional multichannel analysis of surface <span class="hlt">wave</span> (MASW) method that explores near surface soil properties from a couple ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMOS31A1982F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS31A1982F"><span>Effects of beach morphology and <span class="hlt">waves</span> on onshore larval transport</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fujimura, A.; Reniers, A.; Paris, C. B.; Shanks, A.; MacMahan, J.; Morgan, S.</p> <p>2015-12-01</p> <p>Larvae of intertidal species grow offshore, and migrate back to the shore when they are ready to settle on their adult substrates. In order to reach the habitat, they must cross the surf <span class="hlt">zone</span>, which is characterized as a semi-permeable barrier. This is accomplished through physical forcing (i.e., <span class="hlt">waves</span> and current) as well as their own behavior. Two possible scenarios of onshore larval transport are proposed: Negatively buoyant larvae stay in the bottom boundary layer because of turbulence-dependent sinking behavior, and are carried toward the shore by streaming of the bottom boundary layer; positively buoyant larvae move to the shore during onshore wind events, and sink to the bottom once they encounter high turbulence (i.e., surf <span class="hlt">zone</span> edge), where they are carried by the bottom current toward the shore (Fujimura et al. 2014). Our biophysical Lagrangian particle tracking model helps to explain how beach morphology and <span class="hlt">wave</span> conditions affect larval distribution patterns and abundance. Model results and field observations show that larval abundance in the surf <span class="hlt">zone</span> is higher at mildly sloped, rip-channeled beaches than at steep pocket beaches. Beach attributes are broken up to examine which and how beach configuration factors affect larval abundance. Modeling with alongshore uniform beaches with variable slopes reveal that larval populations in the surf <span class="hlt">zone</span> are negatively correlated with beach steepness. Alongshore variability enhances onshore larval transport because of increased cross-shore water exchange by rip currents. <span class="hlt">Wave</span> groups produce transient rip currents and enhance cross-shore exchange. Effects of other <span class="hlt">wave</span> components, such as <span class="hlt">wave</span> height and breaking <span class="hlt">wave</span> rollers are also considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PApGe.tmp.1306W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PApGe.tmp.1306W"><span>Joint Inversion of 1-D Magnetotelluric and Surface-<span class="hlt">Wave</span> Dispersion Data with an Improved Multi-Objective Genetic Algorithm and Application to the Data of the Longmenshan Fault <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Pingping; Tan, Handong; Peng, Miao; Ma, Huan; Wang, Mao</p> <p>2018-05-01</p> <p>Magnetotellurics and seismic surface <span class="hlt">waves</span> are two prominent geophysical methods for deep underground exploration. Joint inversion of these two datasets can help enhance the accuracy of inversion. In this paper, we describe a method for developing an improved multi-objective genetic algorithm (NSGA-SBX) and applying it to two numerical tests to verify the advantages of the algorithm. Our findings show that joint inversion with the NSGA-SBX method can improve the inversion results by strengthening structural coupling when the discontinuities of the electrical and velocity models are consistent, and in case of inconsistent discontinuities between these models, joint inversion can retain the advantages of individual inversions. By applying the algorithm to four detection points along the Longmenshan fault <span class="hlt">zone</span>, we observe several features. The Sichuan Basin demonstrates low S-<span class="hlt">wave</span> velocity and high conductivity in the shallow crust probably due to thick sedimentary layers. The eastern margin of the Tibetan Plateau shows high velocity and high resistivity in the shallow crust, while two low velocity layers and a high conductivity layer are observed in the middle lower crust, probably indicating the mid-crustal channel flow. Along the Longmenshan fault <span class="hlt">zone</span>, a high conductivity layer from 8 to 20 km is observed beneath the northern segment and decreases with depth beneath the middle segment, which might be caused by the elevated fluid content of the fault <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920054208&hterms=acoustic+interior&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dacoustic%2Binterior','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920054208&hterms=acoustic+interior&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dacoustic%2Binterior"><span>Study of intensification <span class="hlt">zones</span> in a rectangular acoustic cavity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Peretti, Linda F.; Dowell, Earl H.</p> <p>1992-01-01</p> <p>The interior acoustic field of a rectangular acoustic cavity, which is excited by the structural vibration of one of its walls, or a portion of the wall, has been studied. Particularly, the spatial variations of sound pressure levels from the peak levels at the boundaries (intensification <span class="hlt">zones</span>) to the uniform interior are considered. Analytical expressions, which describe the intensification <span class="hlt">zones</span>, are obtained using the methodology of asymptotic modal analysis. These results agree well with results computed by a discrete summation over all of the modes. The intensification <span class="hlt">zones</span> were also modeled as a set of oblique <span class="hlt">waves</span> incident upon a surface. The result for a rigid surface agrees with the asymptotic modal analysis result. In the presence of an absorptive surface, the character of the intensification <span class="hlt">zone</span> is dramatically changed. The behavior of the acoustic field near an absorptive wall is described by an expression containing the rigid wall result plus additional terms containing impedance information. The important parameter in the intensification <span class="hlt">zone</span> analysis is the bandwidth to center frequency ratio. The effect of bandwidth is separated from that of center frequency by expanding the expression about the center frequency <span class="hlt">wave</span> number. The contribution from the bandwidth is second order in bandwidth to center frequency ratio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA557148','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA557148"><span>Modeling Water <span class="hlt">Waves</span> with Smoothed Particle Hydrodynamics</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2011-09-30</p> <p>Lagrangian nature of SPH allows the modeling of <span class="hlt">wave</span> breaking, surf <span class="hlt">zones</span>, ship <span class="hlt">waves</span>, and <span class="hlt">wave</span>-structure interaction, where the free surface becomes...particle detection--To study free surface flows and analyze their complex deformations, we need to know which particles are located on the free surface ...Hydrodynamics is proving to be a competent modeling scheme for free surface flows in two and three dimensions. As the GPU hardware improves, it is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51E0541H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51E0541H"><span>S-<span class="hlt">wave</span> tomography of the Cascadia Subduction <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hawley, W. B.; Allen, R. M.</p> <p>2017-12-01</p> <p>We present an S-<span class="hlt">wave</span> tomographic model of the Pacific Northwestern United States using regional seismic arrays, including the amphibious Cascadia Initiative. Offshore, our model shows a rapid transition from slow velocities beneath the ridge to fast velocities under the central Juan de Fuca plate, as seen in previous studies of the region (c.f., Bell et al., 2016; Byrnes et al., 2017). Our model also shows an elongated low-velocity feature beneath the hinge of the Juan de Fuca slab, similar to that observed in a P-<span class="hlt">wave</span> study (Hawley et al., 2016). The addition of offshore data also allows us to investigate along-strike variations in the structure of the subducting slab. Of particular note is a `gap' in the high velocity slab between 44N and 46N, beginning around 100km depth. There exist a number of explanations for this section of lower velocities, ranging from a change in minerology along strike, to a true tear in the subducting slab.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020017455&hterms=ultrasound&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dultrasound','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020017455&hterms=ultrasound&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dultrasound"><span>Measurement of Transcranial Distance During <span class="hlt">Head</span>-Down Tilt Using Ultrasound</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Torikoshi, Shigeyo; Ballard, R. E.; Watenpaugh, D. E.; Murthy, G.; Bowley, S.; Yost, W. T.; Hargens, Alan R.</p> <p>1995-01-01</p> <p>Exposure to microgravity probably elevates blood pressure and flow in the <span class="hlt">head</span> which may increase intracranial volume (ICV) and pressure (ICP). Due to the slightly compliant nature of the cranium, any increase of ICP will increase ICV and transcranial distance. We used a noninvasive ultrasound technique to measure transcranial distance (frontal to occipital) during <span class="hlt">head</span>-down tilt. Seven subjects (ages 26-53) underwent the following tilt angles: 90 deg. upright, 30 deg., 0 deg., -6 deg., -10 deg., -6 deg., 0 deg., 30 deg., and 90 deg. Each angle was maintained for 1 min. Ultrasound <span class="hlt">wave</span> frequency was collected continuously and transcranial distance was calculated (Delta(x) = x(Delta)f/f, where x is path length and f is frequency of the <span class="hlt">wave</span>) for each tilt angle. Frequency decreased from 503.687 kHz (90 deg. upright) to 502.619 kHz (-10 deg.). These frequencies translated to an increased transcranial distance of 0.403 mm. Although our data suggest a significant increase in transcranial distance during <span class="hlt">head</span>-down tilt, this apparent increase may result, in part, from <span class="hlt">head</span>-down tilt-induced subcutaneous edema or cutaneous blood volume elevation. In three subjects, when the above protocol was repeated with an ace bandage wrapped around the <span class="hlt">head</span> to minimize such edema, the increased transcranial distance from 90 deg. to -10 deg. was reduced by 0.174 mm. Further development of the technique to quantify bone-to-bone expansion unconfounded by cutaneous fluid is necessary. Therefore, this ultrasound technique may provide measurements of changes in cranial dimensions during microgravity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA102666','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA102666"><span>Transformation of <span class="hlt">Waves</span> Across the Surf <span class="hlt">Zone</span>.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1981-03-01</p> <p>Kuo is more realis- tic but still results in a sharp cut-off of the distribution at the breaking heights. 5. Goda Distribution Goda (1975) derived a...J.I., "Probabilities of Breaking <span class="hlt">Wave</span> Characteris- tics ," Proc. 12th Coastal Engineering Conf., pp. 399- 412, 1970. Chakrabarty, S.K. and R.P. Cooley...Spring, MD 20910 21. Director 2 Instituto Oceanografico de la Armada Guayaquil, Ecuador 22. Director de Educacion de la Armada Comandancia General de</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981InJEE..61..169R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981InJEE..61..169R"><span>Hydroelectric power from ocean <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raghavendran, K.</p> <p>1981-02-01</p> <p>This paper describes a system which converts the variable energy of ocean <span class="hlt">waves</span> into a steady supply of energy in a conventional form. The system consists of a set of floats and Persian wheels located off-shore and a storage reservoir on the shore. The floats oscillate vertically as the <span class="hlt">waves</span> pass below them and turn their respective Persian wheels which lift sea water to a height and deliver to the reservoir through an interconnecting pipeline. The <span class="hlt">head</span> of water in the reservoir operates a hydraulic turbine which in turn works a generator to supply electricity. Due to the recurrent <span class="hlt">wave</span> action, water is maintained at the optimum level in the reservoir to ensure continuous power supply.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51E0525C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51E0525C"><span>Update on GPS-Acoustics Measurements on the Continental Slope of the Cascadia Subduction <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chadwell, C. D.</p> <p>2017-12-01</p> <p>Land-based GPS measurements suggest the megathrust is locked offshore along the Cascadia Subduction <span class="hlt">Zone</span>. However, land-based data alone lack geometric resolution to constrain the how the slip is distributed. GPS-Acoustic measurements can provide these constraints, but using traditional GPS-Acoustic approaches employing a ship is costly. <span class="hlt">Wave</span> Gliders, a <span class="hlt">wave</span>- and solar-powered, remotely-piloted sea surface platform, provide a low cost method for collecting GPS-A data. We have adapted GPS-Acoustic technology to the <span class="hlt">Wave</span> Glider and in 2016 began annual measurements at three sites in the Cascadia Subduction <span class="hlt">Zone</span> (CSZ). Here, we review positioning results collected during summer 2017 at two sites on the continental slope of the Cascadia Subduction <span class="hlt">Zone</span>: One site is approximately 45 NM offshore central Oregon and the other approximately 50 NM offshore central Washington State. A third site is approximately 90 NM offshore central Oregon on the incoming Juan de Fuca plate. We will report on initial results of the GPS-A data collection and operational experiences of the missions in 2016 and 2017. <span class="hlt">Wave</span> Glider based GPS-A measurement have the potential to significantly increase the number and frequency of measurements of strain accumulation in Cascadia Subduction <span class="hlt">Zone</span> and elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSeis..22..455P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSeis..22..455P"><span>Near-source attenuation of high-frequency body <span class="hlt">waves</span> beneath the New Madrid Seismic <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pezeshk, Shahram; Sedaghati, Farhad; Nazemi, Nima</p> <p>2018-03-01</p> <p>Attenuation characteristics in the New Madrid Seismic <span class="hlt">Zone</span> (NMSZ) are estimated from 157 local seismograph recordings out of 46 earthquakes of 2.6 ≤ M ≤ 4.1 with hypocentral distances up to 60 km and focal depths down to 25 km. Digital waveform seismograms were obtained from local earthquakes in the NMSZ recorded by the Center for Earthquake Research and Information (CERI) at the University of Memphis. Using the coda normalization method, we tried to determine Q values and geometrical spreading exponents at 13 center frequencies. The scatter of the data and trade-off between the geometrical spreading and the quality factor did not allow us to simultaneously derive both these parameters from inversion. Assuming 1/ R 1.0 as the geometrical spreading function in the NMSZ, the Q P and Q S estimates increase with increasing frequency from 354 and 426 at 4 Hz to 729 and 1091 at 24 Hz, respectively. Fitting a power law equation to the Q estimates, we found the attenuation models for the P <span class="hlt">waves</span> and S <span class="hlt">waves</span> in the frequency range of 4 to 24 Hz as Q P = (115.80 ± 1.36) f (0.495 ± 0.129) and Q S = (161.34 ± 1.73) f (0.613 ± 0.067), respectively. We did not consider Q estimates from the coda normalization method for frequencies less than 4 Hz in the regression analysis since the decay of coda amplitude was not observed at most bandpass filtered seismograms for these frequencies. Q S/ Q P > 1, for 4 ≤ f ≤ 24 Hz as well as strong intrinsic attenuation, suggest that the crust beneath the NMSZ is partially fluid-saturated. Further, high scattering attenuation indicates the presence of a high level of small-scale heterogeneities inside the crust in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AIPC..845.1026T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AIPC..845.1026T"><span>Detonation Reaction <span class="hlt">Zones</span> in Condensed Explosives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tarver, Craig M.</p> <p>2006-07-01</p> <p>Experimental measurements using nanosecond time resolved embedded gauges and laser interferometric techniques, combined with Non-Equilibrium Zeldovich - von Neumann - Doling (NEZND) theory and Ignition and Growth reactive flow hydrodynamic modeling, have revealed the average pressure/particle velocity states attained in reaction <span class="hlt">zones</span> of self-sustaining detonation <span class="hlt">waves</span> in several solid and liquid explosives. The time durations of these reaction <span class="hlt">zone</span> processes are discussed for explosives based on pentaerythritol tetranitrate (PETN), nitromethane, octahydro-1,3,5,7-tetranitro-1,3,5,7-tetrazocine (HMX), triaminitrinitrobenzene(TATB) and trinitrotoluene (TNT).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4310549','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4310549"><span>A hybrid <span class="hlt">zone</span> revisited: molecular and morphological analysis of the maintenance, movement, and evolution of a Great Plains avian (Cardinalidae: Pheucticus) hybrid <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>METTLER, R. D.; SPELLMAN, G. M.</p> <p>2014-01-01</p> <p>Black-<span class="hlt">headed</span> Grosbeaks (Pheucticus melanocephalus) and Rose-breasted Grosbeaks (Pheucticus ludovicianus) are passerine bird species known to hybridize in the Great Plains of North America. Both extrinsic (environmental) and intrinsic factors (pre- and postzygotic reproductive isolation) have been credited for the generation and maintenance of the grosbeak hybrid <span class="hlt">zone</span>, but little is known about the genetic characteristics of this hybrid <span class="hlt">zone</span>. To investigate the stability and extent of the grosbeak hybrid <span class="hlt">zone</span>, we constructed clines from both molecular sequence data (mtDNA, 3 autosomal intron loci, and 1 Z-linked locus) and morphological data (morphometric analyses and hybrid index scores) to determined <span class="hlt">zone</span> center and width. Hybrid <span class="hlt">zone</span> center and width were also determined for samples collected across the <span class="hlt">zone</span> 40 years ago from morphological data. The present and past clines were compared and provided support for stability in hybrid <span class="hlt">zone</span> location and width, and the evolutionary implications of this are discussed. Three models of hybrid <span class="hlt">zone</span> maintenance were investigated to consider the influence of intrinsic and extrinsic factors on this <span class="hlt">zone</span>. Our results suggest low hybrid frequencies, a stable <span class="hlt">zone</span> location and narrow width, and reduced hybrid fitness over the past 40 years best categorize the grosbeak hybrid <span class="hlt">zone</span> as a tension <span class="hlt">zone</span>. PMID:19619198</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7975H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7975H"><span>Experimental study on <span class="hlt">waves</span> propagation over a coarse-grained sloping beach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hsu, Tai-Wen; Lai, Jian-Wu</p> <p>2013-04-01</p> <p>This study investigates velocity fields of <span class="hlt">wave</span> propagation over a coarse-grained sloping beach using laboratory experiments. The experiment was conducted in a <span class="hlt">wave</span> flume of 25 m long, 0.5 m wide and 0.6 m high in which a coarse-grained sloping 1:5 beach was placed with two layers ball. The glass ball is D=7.9 cm and the center to center distance of each ball is 8.0 cm. The test section for observing <span class="hlt">wave</span> and flow fields is located at the middle part of the flume. A piston type <span class="hlt">wave</span> maker driven by an electromechanical hydraulic serve system is installed at the end of the flume. The intrinsic permeability Kp and turbulent drag coefficient Cf were obtained from steady flow water-<span class="hlt">head</span> experiments. The flow velocity was measured by the particle image velocimeter (PIV) and digital image process (DIP) techniques. Eleven fields of view (FOVS) were integrated into a complete representation including the outer, surf and swash <span class="hlt">zone</span>. Details of the definition sketch of the coarse-grained sloping beach model as well as experimental setup are referred to Lai et al. (2008). A high resolution of CCD camera was used to capture the images which was calibrated by the direct linear transform (DCT) algorithm proposed by Abed El-Aziz and Kar-Ara (1971). The water surface between the interface of air and water at each time step are calculated by Otsu' (1978) detect algorithm. The comparison shows that the water surface elevation observed by integrated image agrees well with that of Otsu' detection results. For the flow field measurement, each image pair was cross correlated with 32X32 pixel inter rogation window and a half overlap between adjacent windows. The repeatability and synchronization are the key elements for both <span class="hlt">wave</span> motion and PIV technique. The <span class="hlt">wave</span> profiles and flow field were compared during several <span class="hlt">wave</span> periods to ensure that they can be reproduced by the present system. The water depth is kept as a constant of h=32 cm. The incident <span class="hlt">wave</span> conditions are set to be <span class="hlt">wave</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSEC14C0991M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSEC14C0991M"><span>Sheet flow measurements on a surf-<span class="hlt">zone</span> sandbar under shoaling and breaking <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mieras, R.; Puleo, J. A.; Cox, D. T.; Anderson, D. L.; Kim, Y.; Hsu, T. J.</p> <p>2016-02-01</p> <p>A large-scale experiment to quantify sheet flow processes over a sandbar under varying levels of <span class="hlt">wave</span> steepness was conducted in the <span class="hlt">wave</span> flume at Oregon State University's O.H. Hinsdale <span class="hlt">Wave</span> Research Laboratory. A fixed profile was constructed with concrete slabs anchored to the flume side walls, with the exception of the sandbar crest, where a steel pit was installed and filled with well-sorted sediment (d50 0.17 mm). This hybrid approach allowed for the isolation of small-scale bed response to large-scale <span class="hlt">wave</span> forcing over the sandbar, where an array of sensors was positioned to measure hydrodynamic forcing and sediment response. Near-bed (< 3 cm above the bed) velocities were estimated using Nortek Vectrino-II profiling velocimeters, while sheet layer sediment concentration profiles (volumetric concentrations > 0.08 m3/m3) were approximated using Conductivity Concentration Profilers. Test conditions consisted of a regular <span class="hlt">wave</span> train with incident <span class="hlt">wave</span> heights for individual runs ranging from 0.4 m to 0.6 m and incident <span class="hlt">wave</span> periods from 5 s to 9 s, encompassing a variety of skewed and asymmetric <span class="hlt">wave</span> shapes across the shoaling and breaking regimes. Ensemble-averaged sediment concentration profiles exhibit considerable variation across the different conditions. The largest variation in sheet layer thickness occurs beneath the <span class="hlt">wave</span> crest, ranging from 30 grain diameters for 5 sec, 0.4 m <span class="hlt">waves</span>, up to 80 grain diameters for 7 sec, 0.6 m <span class="hlt">waves</span>. Furthermore, the initiation and duration of sheet flow relative to the <span class="hlt">wave</span> period differs for each condition set. It is likely that more than one mechanism plays a role in determining the aforementioned sheet layer characteristics. In the present work, we focus on the relative magnitude and phase of the near-bed flow acceleration and shear stress in determining the characteristics of the sheet layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013702','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013702"><span><span class="hlt">Wave</span> Processes in Arctic Seas, Observed from TerraSAR-X</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>in order to improve <span class="hlt">wave</span> models as well as ice models applicable to a changing Arctic <span class="hlt">wave</span>/ and ice climate . This includes observation and...fields retrieved from the TS-X image swaths. 4. “<span class="hlt">Wave</span> Climate and <span class="hlt">Wave</span> Mixing in the Marginal Ice <span class="hlt">Zones</span> of Arctic Seas, Observations and Modelling”, by...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. “<span class="hlt">Wave</span> Processes in Arctic Seas, Observed from TerraSAR-X</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/70039999','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70039999"><span>Demography and movement patterns of leopard sharks (Triakis semifasciata) aggregating near the <span class="hlt">head</span> of a submarine canyon along the open coast of southern California, 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>Nosal, D.C.; Cartamil, D.C.; Long, J.W.; Luhrmann, M.; Wegner, N.C.; Graham, J.B.</p> <p>2013-01-01</p> <p>The demography, spatial distribution, and movement patterns of leopard sharks (Triakis semifasciata) aggregating near the <span class="hlt">head</span> of a submarine canyon in La Jolla, California, USA, were investigated to resolve the causal explanations for this and similar shark aggregations. All sharks sampled from the aggregation site (n=140) were sexually mature and 97.1 % were female. Aerial photographs taken during tethered balloon surveys revealed high densities of milling sharks of up to 5470 sharks ha-1. Eight sharks were each tagged with a continuous acoustic transmitter and manually tracked without interruption for up to 48 h. Sharks exhibited strong site-fidelity and were generally confined to a divergence (shadow) <span class="hlt">zone</span> of low <span class="hlt">wave</span> energy, which results from <span class="hlt">wave</span> refraction over the steep bathymetric contours of the submarine canyon. Within this divergence <span class="hlt">zone</span>, the movements of sharks were strongly localized over the seismically active Rose Canyon Fault. Tracked sharks spent most of their time in shallow water (≤2 m for 71.0 % and ≤10 m for 95.9 % of time), with some dispersing to deeper (max: 53.9 m) and cooler (min: 12.7 °C) water after sunset, subsequently returning by sunrise. These findings suggest multiple functions of this aggregation and that the mechanism controlling its formation, maintenance, and dissolution is complex and rooted in the sharks' variable response to numerous confounding environmental factors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED582429.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED582429.pdf"><span>From Innovation Schools to an Innovation <span class="hlt">Zone</span> in Denver, Colorado</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>Iyengar, Nithin; Lewis-LaMonica, Kate; Perigo, Mike</p> <p>2017-01-01</p> <p>This article is part of a Bridgespan Group research project that focuses on a new <span class="hlt">wave</span> of district-led "innovation <span class="hlt">zones</span>" that holds promise to overcome the challenges of turning around failing schools and deliver significant improvements in student outcomes. This new <span class="hlt">wave</span> provides a subset of district schools with control over staffing,…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhyD..241.1567E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhyD..241.1567E"><span>Refraction of dispersive shock <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>El, G. A.; Khodorovskii, V. V.; Leszczyszyn, A. M.</p> <p>2012-09-01</p> <p>We study a dispersive counterpart of the classical gas dynamics problem of the interaction of a shock <span class="hlt">wave</span> with a counter-propagating simple rarefaction <span class="hlt">wave</span>, often referred to as the shock <span class="hlt">wave</span> refraction. The refraction of a one-dimensional dispersive shock <span class="hlt">wave</span> (DSW) due to its <span class="hlt">head</span>-on collision with the centred rarefaction <span class="hlt">wave</span> (RW) is considered in the framework of the defocusing nonlinear Schrödinger (NLS) equation. For the integrable cubic nonlinearity case we present a full asymptotic description of the DSW refraction by constructing appropriate exact solutions of the Whitham modulation equations in Riemann invariants. For the NLS equation with saturable nonlinearity, whose modulation system does not possess Riemann invariants, we take advantage of the recently developed method for the DSW description in non-integrable dispersive systems to obtain main physical parameters of the DSW refraction. The key features of the DSW-RW interaction predicted by our modulation theory analysis are confirmed by direct numerical solutions of the full dispersive problem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/8936','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/8936"><span>Effect of knots on stress <span class="hlt">waves</span> in lumber</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>C.C. Gerhards</p> <p>1982-01-01</p> <p>An impact stress <span class="hlt">wave</span> was induced in the end of 2 by 6 lumber containing knots. Rather than a normal, perpendicular-to-the-axis profile in transiting by a knot, the stress <span class="hlt">wave</span> tended to Iead in <span class="hlt">zones</span> of clear wood in the direction of the slope of grain or slope of the annual rings and to lag behind the knot. Of three methods evaluated to time the stress <span class="hlt">wave</span>, the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17885225','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17885225"><span>Extracorporeal shock <span class="hlt">wave</span> therapy in treatment of delayed bone-tendon healing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Lin; Qin, Ling; Lu, Hong-bin; Cheung, Wing-hoi; Yang, Hu; Wong, Wan-nar; Chan, Kai-ming; Leung, Kwok-sui</p> <p>2008-02-01</p> <p>Extracorporeal shock <span class="hlt">wave</span> therapy is indicated for treatment of chronic injuries of soft tissues and delayed fracture healing and nonunion. No investigation has been conducted to study the effect of shock <span class="hlt">wave</span> on delayed healing at the bone-tendon junction. Shock <span class="hlt">wave</span> promotes osteogenesis, regeneration of fibrocartilage <span class="hlt">zone</span>, and remodeling of healing tissue in delayed healing of bone-tendon junction surgical repair. Controlled laboratory study. Twenty-eight mature rabbits were used for establishing a delayed healing model at the patella-patellar tendon complex after partial patellectomy and then divided into control and shock <span class="hlt">wave</span> groups. In the shock <span class="hlt">wave</span> group, a single shock <span class="hlt">wave</span> treatment was given at week 6 postoperatively to the patella-patellar tendon healing complex. Seven samples were harvested at week 8 and 7 samples at week 12 for radiologic, densitometric, histologic, and mechanical evaluations. Radiographic measurements showed 293.4% and 185.8% more new bone formation at the patella-patellar tendon healing junction in the shock <span class="hlt">wave</span> group at weeks 8 and 12, respectively. Significantly better bone mineral status was found in the week 12 shock <span class="hlt">wave</span> group. Histologically, the shock <span class="hlt">wave</span> group showed more advanced remodeling in terms of better alignment of collagen fibers and thicker and more mature regenerated fibrocartilage <span class="hlt">zone</span> at both weeks 8 and 12. Mechanical testing showed 167.7% and 145.1% higher tensile load and strength in the shock <span class="hlt">wave</span> group at week 8 and week 12, respectively, compared with controls. Extracorporeal shock <span class="hlt">wave</span> promotes osteogenesis, regeneration of fibrocartilage <span class="hlt">zone</span>, and remodeling in the delayed bone-to-tendon healing junction in rabbits. These results provide a foundation for future clinical studies toward establishment of clinical indication for treatment of delayed bone-to-tendon junction healing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H23D1691S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H23D1691S"><span>Mixing-dependent Reactions in the Hyporheic <span class="hlt">Zone</span>: Laboratory and Numerical Experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santizo, K. Y.; Eastes, L. A.; Hester, E. T.; Widdowson, M.</p> <p>2017-12-01</p> <p>The hyporheic <span class="hlt">zone</span> is the surface water-groundwater interface surrounding the river's perimeter. Prior research demonstrates the ability of the hyporheic <span class="hlt">zone</span> to attenuate pollutants when surface water cycles through reactive sediments (non-mixing-dependent reactions). However, the colocation of both surface and ground water within hyporheic sediments also allows mixing-dependent reactions that require mixing of reactants from these two water sources. Recent modeling studies show these mixing <span class="hlt">zones</span> can be small under steady state homogeneous conditions, but do not validate those results in the laboratory or explore the range of hydrological characteristics that control the extent of mixing. Our objective was to simulate the mixing <span class="hlt">zone</span>, quantify its thickness, and probe its hydrological controls using a "mix" of laboratory and numerical experiments. For the lab experiments, a hyporheic <span class="hlt">zone</span> was simulated in a sand mesocosm, and a mixing-dependent abiotic reaction of sodium sulfite and dissolved oxygen was induced. Oxygen concentration response and oxygen consumption were visualized via planar optodes. Sulfate production by the mixing-dependent reaction was measured by fluid samples and a spectrophometer. Key hydrologic controls varied in the mesocosm included <span class="hlt">head</span> gradient driving hyporheic exchange and hydraulic conductivity/heterogeneity. Results show a clear mixing area, sulfate production, and oxygen gradient. Mixing <span class="hlt">zone</span> length (hyporheic flow cell size) and thickness both increase with the driving <span class="hlt">head</span> gradient. For the numerical experiments, transient surface water boundary conditions were implemented together with heterogeneity of hydraulic conductivity. Results indicate that both fluctuating boundary conditions and heterogeneity increase mixing-dependent reaction. The hyporheic <span class="hlt">zone</span> is deemed an attenuation hotspot by multiple studies, but here we demonstrate its potential for mixing-dependent reactions and the influence of important hydrological</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.S41C1927M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.S41C1927M"><span>A surface <span class="hlt">wave</span> reflector in Southwestern Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mak, S.; Koketsu, K.; Miyake, H.; Obara, K.; Sekine, S.</p> <p>2009-12-01</p> <p>Surface <span class="hlt">waves</span> at short periods (<35s) are affected severely by heterogeneities in the crust and the uppermost mantle. When the scale of heterogeneity is sufficiently large, its effect can be studied in a deterministic way using conventional concepts of reflection and refraction. A well-known example is surface <span class="hlt">wave</span> refraction at continental margin. We present a case study to investigate the composition of surface <span class="hlt">wave</span> coda in a deterministic approach. A long duration of surface <span class="hlt">wave</span> coda with a predominant period of 20s is observed during various strong earthquakes around Japan. The coda shows an unambiguous propagation direction, implying a deterministic nature. Beamforming and particle motion analysis suggest that the surface <span class="hlt">wave</span> later arrivals could be explained by Love <span class="hlt">wave</span> reflections by a point reflector located at offshore southeast to Kyushu. The reflection demonstrates a seemingly incidence-independent favorable azimuth in emitting strength. In additional to beamforming, we use a new regional crustal velocity model to perform a grid-search ray-tracing with the assumption of point reflector to further constrain to location of coda generation. Because strong velocity anomalies exist near the <span class="hlt">zone</span> of interest, we decide to use a network shortest-path ray-tracing method, instead of analytical methods like shooting and bending, to avoid the problems like convergence, shadow <span class="hlt">zone</span>, and smooth model assumption. Two geological features are found to be related to the formation of the coda. The primary one is the intersection between the Kyushu-Palau Ridge and the Nankai Trough at offshore southeast to Kyushu (hereafter referred as "KPR-NT"), which may act as a point reflector. There is a strong Love <span class="hlt">wave</span> phase velocity anomaly at KPR-NT but not other parts of the ridge, implying that topography is irrelevant. Rayleigh <span class="hlt">wave</span> phase velocity does not experience a strong anomaly there, which is consistent to the absence of Rayleigh <span class="hlt">wave</span> reflections implied by the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005ASAJ..117.2369H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005ASAJ..117.2369H"><span>Extracorporeal shock <span class="hlt">wave</span> therapy in orthopedics, basic research, and clinical implications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hausdorf, Joerg; Jansson, Volkmar; Maier, Markus; Delius, Michael</p> <p>2005-04-01</p> <p>The molecular events following shock <span class="hlt">wave</span> treatment of bone are widely unknown. Nevertheless patients with osteonecrosis and non unions are already treated partly successful with shock <span class="hlt">waves</span>. Concerning the first indication, the question of the permeation of the shock <span class="hlt">wave</span> into the bone was addressed. Therefore shockwaves were applied to porcine femoral <span class="hlt">heads</span> and the intraosseous pressure was measured. A linear correlation of the pressure to the intraosseous distance was found. Approximately 50% of the pressure are still measurable 10 mm inside the femoral <span class="hlt">head</span>. These findings should encourage continued shock <span class="hlt">wave</span> research on this indication. Concerning the second indication (non union), osteoblasts were subjected to 250 or 500 shock <span class="hlt">waves</span> at 25 kV. After 24, 48, and 72 h the levels of the bone and vascular growth factors bFGF, TGFbeta1, and VEGF were examined. After 24 h there was a significant increase in bFGF levels (p<0.05) with significant correlation (p<0.05) to the number of impulses. TGFbeta1, and VEGF showed no significant changes. This may be one piece in the cascade of new bone formation following shock <span class="hlt">wave</span> treatment and may lead to a more specific application of shock <span class="hlt">waves</span> in orthopedic surgery.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA12404.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA12404.html"><span>El Niño Surges; Warm Kelvin <span class="hlt">Wave</span> <span class="hlt">Headed</span> for South America</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2009-12-17</p> <p>The most recent sea-level height data from the NASA/European Ocean Surface Topography Mission/Jason-2 oceanography satellite show the continued eastward progression of a strong <span class="hlt">wave</span> of warm water, known as a Kelvin <span class="hlt">wave</span>, now approaching South America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.3287V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.3287V"><span>Large-scale laboratory study of breaking <span class="hlt">wave</span> hydrodynamics over a fixed bar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van der A, Dominic A.; van der Zanden, Joep; O'Donoghue, Tom; Hurther, David; Cáceres, Iván.; McLelland, Stuart J.; Ribberink, Jan S.</p> <p>2017-04-01</p> <p>A large-scale <span class="hlt">wave</span> flume experiment has been carried out involving a T = 4 s regular <span class="hlt">wave</span> with H = 0.85 m <span class="hlt">wave</span> height plunging over a fixed barred beach profile. Velocity profiles were measured at 12 locations along the breaker bar using LDA and ADV. A strong undertow is generated reaching magnitudes of 0.8 m/s on the shoreward side of the breaker bar. A circulation pattern occurs between the breaking area and the inner surf <span class="hlt">zone</span>. Time-averaged turbulent kinetic energy (TKE) is largest in the breaking area on the shoreward side of the bar where the plunging jet penetrates the water column. At this location, and on the bar crest, TKE generated at the water surface in the breaking process reaches the bottom boundary layer. In the breaking area, TKE does not reduce to zero within a <span class="hlt">wave</span> cycle which leads to a high level of "residual" turbulence and therefore lower temporal variation in TKE compared to previous studies of breaking <span class="hlt">waves</span> on plane beach slopes. It is argued that this residual turbulence results from the breaker bar-trough geometry, which enables larger length scales and time scales of breaking-generated vortices and which enhances turbulence production within the water column compared to plane beaches. Transport of TKE is dominated by the undertow-related flux, whereas the <span class="hlt">wave</span>-related and turbulent fluxes are approximately an order of magnitude smaller. Turbulence production and dissipation are largest in the breaker <span class="hlt">zone</span> and of similar magnitude, but in the shoaling <span class="hlt">zone</span> and inner surf <span class="hlt">zone</span> production is negligible and dissipation dominates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25748583','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25748583"><span>Field observation of morpho-dynamic processes during storms at a Pacific beach, Japan: role of long-period <span class="hlt">waves</span> in storm-induced berm erosion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mizuguchi, Masaru; Seki, Katsumi</p> <p>2015-01-01</p> <p>Many ultrasonic <span class="hlt">wave</span> gages were placed with a small spacing across the swash <span class="hlt">zone</span> to monitor either sand level or water level. Continuous monitoring conducted for a few years enabled the collection of data on the change in <span class="hlt">wave</span> properties as well as swash-<span class="hlt">zone</span> profiles. Data sets including two cases of large-scale berm erosion were analyzed. The results showed that 1) shoreline erosion started when high <span class="hlt">waves</span> with significant power in long-period (1 to 2 min.) <span class="hlt">waves</span> reached the top of a well-developed berm with the help of rising tide; 2) the beach in the swash <span class="hlt">zone</span> was eroded with higher elevation being more depressed, while the bottom elevation just outside the swash <span class="hlt">zone</span> remained almost unchanged; and 3) erosion stopped in a few hours after the berm was completely eroded or the swash-<span class="hlt">zone</span> slope became uniformly mild. These findings strongly suggest that long <span class="hlt">waves</span> play a dominant role in the swash-<span class="hlt">zone</span> dynamics associated with these erosional events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19750048814&hterms=liquid+soap&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dliquid%2Bsoap','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19750048814&hterms=liquid+soap&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dliquid%2Bsoap"><span>Studies of rotating liquid floating <span class="hlt">zones</span> on Skylab IV</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carruthers, J. R.; Gibson, E. G.; Klett, M. G.; Facemire, B. R.</p> <p>1975-01-01</p> <p>Liquid <span class="hlt">zones</span> of water, soap solution and soap foam were deployed between two aligned circular disks which were free to rotate about the <span class="hlt">zone</span> axis in the microgravity environment of Skylab IV. Such a configuration is of interest in the containerless handling of melts for possible future space processing crystal growth experiments. Three basic types of <span class="hlt">zone</span> surface deformation and instability were observed for these rotational conditions; axisymmetric shape changes under single disk rotation, nonaxisymmetric, whirling, C-modes for long <span class="hlt">zones</span> with equal rotation of both disks, and capillary <span class="hlt">wave</span> phenomena for short <span class="hlt">zones</span> with equal rotation of both disks. The sources of these instabilities and the conditions promoting them are analyzed in detail from video tape recordings of the Skylab experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GeoRL..39.2310C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GeoRL..39.2310C"><span>Shear <span class="hlt">wave</span> reflectivity imaging of the Nazca-South America subduction <span class="hlt">zone</span>: Stagnant slab in the mantle transition <span class="hlt">zone</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Contenti, Sean; Gu, Yu Jeffrey; Ökeler, Ahmet; Sacchi, Mauricio D.</p> <p>2012-01-01</p> <p>In this study we utilize over 5000 SS waveforms to investigate the high-resolution mantle reflectivity structure down to 1200 km beneath the South American convergent margin. Our results indicate that the dynamics of the Nazca subduction are more complex than previously suggested. The 410- and 660-km seismic discontinuities beneath the Pacific Ocean and Amazonian Shield exhibit limited lateral depth variations, but their depths vary substantially in the vicinity of the subducting Nazca plate. The reflection amplitude of the 410-km discontinuity is greatly diminished in a ˜1300-km wide region in the back-arc of the subducting plate, which is likely associated with a compositional heterogeneity on top of the upper mantle transition <span class="hlt">zone</span>. The underlying 660-km discontinuity is strongly depressed, showing localized depth and amplitude variations both within and to the east of the Wadati-Benioff <span class="hlt">zone</span>. The width of this anomalous <span class="hlt">zone</span> (˜1000 km) far exceeds that of the high-velocity slab structure and suggesting significant slab deformation within the transition <span class="hlt">zone</span>. The shape of the 660-km discontinuity and the presence of lower mantle reflectivity imply both stagnation and penetration are possible as the descending Nazca slab impinges upon the base of the upper mantle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29695807','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29695807"><span>Radiating pattern of surge-current-induced THz light in near-field and far-field <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Han, J W; Choi, Y G; Lee, J S</p> <p>2018-04-25</p> <p>We generate the THz <span class="hlt">wave</span> on the surface of an unbiased GaAs crystal by illuminating femtosecond laser pulses with a 45° incidence angle, and investigate its propagation properties comprehensively both in a near-field and in a far-field <span class="hlt">zone</span> by performing a knife-edge scan measurement. In the near-field <span class="hlt">zone</span>, i.e. 540 μm away from the generation point, we found that the beam simply takes a Gaussian shape of which width follows well a behavior predicted by a paraxial <span class="hlt">wave</span> equation. In the far-field <span class="hlt">zone</span>, on the other hand, it takes a highly anisotropic shape; whereas the beam profile maintains a Gaussian shape along the normal to the plane of incidence, it takes satellite peak structures along the direction in parallel to the plane of incidence. From the comparison with simulation results obtained by using a dipole radiation model, we demonstrated that this irregular beam pattern is attributed to the combined effect of the position-dependent phase retardation of the THz <span class="hlt">waves</span> and the diffraction-limited size of the initial beam which lead to the interference of the <span class="hlt">waves</span> in the far-field <span class="hlt">zone</span>. Also, we found that this consideration accounting for a crossover of THz beam profile to the anisotropic non-Gaussian beam in the far-field <span class="hlt">zone</span> can be applied for a comprehensive understanding of several other THz beam profiles obtained previously in different configurations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA455449','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA455449"><span>Longshore Sediment Transport Rate Calculated Incorporating <span class="hlt">Wave</span> Orbital Velocity Fluctuations</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-09-01</p> <p>distribution of longshore sediment transport in the surf <span class="hlt">zone</span> is necessary in the design and planning of groins, jetties, weirs and pipeline landfalls...transported by any current. Breaker height is defined as the vertical distance between the <span class="hlt">wave</span> crest and the preceding <span class="hlt">wave</span> trough at incipient...terminology; spilling breakers occur if the <span class="hlt">wave</span> crest becomes unstable and flows down the front face of the <span class="hlt">wave</span> producing a foamy water surface; plunging</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS21D..07G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS21D..07G"><span>HB06 : Field Validation of Realtime Predictions of Surfzone <span class="hlt">Waves</span> and Currents</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guza, R. T.; O'Reilly, W. C.; Feddersen, F.</p> <p>2006-12-01</p> <p>California shorelines can be contaminated by the discharge of polluted streams and rivers onto the beach face or into the surf <span class="hlt">zone</span>. Management decisions (for example, beach closures) can be assisted by accurate characterization of the <span class="hlt">waves</span> and currents that transport and mix these pollutants. A real-time, operational <span class="hlt">waves</span> and alongshore current model, developed for a 5 km alongshore reach at Huntington Beach (http://cdip.ucsd.edu/hb06/), will be tested for a month during Fall 2006 as part of the HB06 field experiment. The model has two components: prediction of incident <span class="hlt">waves</span> immediately seaward of the surf <span class="hlt">zone</span>, and the transformation of breaking <span class="hlt">waves</span> across the surf <span class="hlt">zone</span>. The California Safe Boating Network Model (O'Reilly et al., California World Ocean Conference, 2006) is used to estimate incident <span class="hlt">wave</span> properties. This regional <span class="hlt">wave</span> model accounts for blocking and refraction by offshore islands and shoals, and variation of the shoreline orientation. At Huntington Beach, the network model uses four buoys exposed to the deep ocean to estimate swell, and four nearby buoys to estimate locally generated seas. The model predictions will be compared with directional <span class="hlt">wave</span> buoy observations in 22 m depth, 1 km from the shore. The computationally fast model for surfzone <span class="hlt">waves</span> and breaking-<span class="hlt">wave</span> driven alongshore currents, appropriate for random <span class="hlt">waves</span> on beaches with simple bathymetry, is based on concepts developed and tested by Ed Thornton and his colleagues over the last 30 years. Modeled alongshore currents at Huntington Beach, with incident <span class="hlt">waves</span> predicted by the Network model, will be compared with <span class="hlt">waves</span> and currents observed during HB06 along a transect extending from 4 m depth to the shoreline. Support from the California Coastal Conservancy, NOAA, and ONR is gratefully acknowledged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28952806','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28952806"><span><span class="hlt">Head-To-Head</span> Comparison Between High- and Standard-b-Value DWI for Detecting Prostate Cancer: A Systematic Review and Meta-Analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Woo, Sungmin; Suh, Chong Hyun; Kim, Sang Youn; Cho, Jeong Yeon; Kim, Seung Hyup</p> <p>2018-01-01</p> <p>The purpose of this study was to perform a <span class="hlt">head-to-head</span> comparison between high-b-value (> 1000 s/mm 2 ) and standard-b-value (800-1000 s/mm 2 ) DWI regarding diagnostic performance in the detection of prostate cancer. The MEDLINE and EMBASE databases were searched up to April 1, 2017. The analysis included diagnostic accuracy studies in which high- and standard-b-value DWI were used for prostate cancer detection with histopathologic examination as the reference standard. Methodologic quality was assessed with the revised Quality Assessment of Diagnostic Accuracy Studies tool. Sensitivity and specificity of all studies were calculated and were pooled and plotted in a hierarchic summary ROC plot. Meta-regression and multiple-subgroup analyses were performed to compare the diagnostic performances of high- and standard-b-value DWI. Eleven studies (789 patients) were included. High-b-value DWI had greater pooled sensitivity (0.80 [95% CI, 0.70-0.87]) (p = 0.03) and specificity (0.92 [95% CI, 0.87-0.95]) (p = 0.01) than standard-b-value DWI (sensitivity, 0.78 [95% CI, 0.66-0.86]); specificity, 0.87 [95% CI, 0.77-0.93] (p < 0.01). Multiple-subgroup analyses showed that specificity was consistently higher for high- than for standard-b-value DWI (p ≤ 0.05). Sensitivity was significantly higher for high- than for standard-b-value DWI only in the following subgroups: peripheral <span class="hlt">zone</span> only, transition <span class="hlt">zone</span> only, multiparametric protocol (DWI and T2-weighted imaging), visual assessment of DW images, and per-lesion analysis (p ≤ 0.04). In a <span class="hlt">head-to-head</span> comparison, high-b-value DWI had significantly better sensitivity and specificity for detection of prostate cancer than did standard-b-value DWI. Multiple-subgroup analyses showed that specificity was consistently superior for high-b-value DWI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19780067007&hterms=tornado&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtornado','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780067007&hterms=tornado&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtornado"><span>Observation of gravity <span class="hlt">waves</span> during the extreme tornado outbreak of 3 April 1974</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hung, R. J.; Phan, T.; Smith, R. E.</p> <p>1978-01-01</p> <p>A continuous <span class="hlt">wave</span>-spectrum high-frequency radiowave Doppler sounder array was used to observe upper-atmospheric disturbances during an extreme tornado outbreak. The observations indicated that gravity <span class="hlt">waves</span> with two harmonic <span class="hlt">wave</span> periods were detected at the F-region ionospheric height. Using a group ray path computational technique, the observed gravity <span class="hlt">waves</span> were traced in order to locate potential sources. The signals were apparently excited 1-3 hours before tornado touchdown. Reverse ray tracing indicated that the <span class="hlt">wave</span> source was located at the aurora <span class="hlt">zone</span> with a Kp index of 6 at the time of <span class="hlt">wave</span> excitation. The summation of the 24-hour Kp index for the day was 36. The results agree with existing theories (Testud, 1970; Titheridge, 1971; Kato, 1976) for the excitation of large-scale traveling ionospheric disturbances associated with geomagnetic activity in the aurora <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S21E..06Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S21E..06Z"><span>Joint Inversion of Body-<span class="hlt">Wave</span> Arrival Times and Surface-<span class="hlt">Wave</span> Dispersion Data in the Wavelet Domain Constrained by Sparsity Regularization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, H.; Fang, H.; Yao, H.; Maceira, M.; van der Hilst, R. D.</p> <p>2014-12-01</p> <p>Recently, Zhang et al. (2014, Pure and Appiled Geophysics) have developed a joint inversion code incorporating body-<span class="hlt">wave</span> arrival times and surface-<span class="hlt">wave</span> dispersion data. The joint inversion code was based on the regional-scale version of the double-difference tomography algorithm tomoDD. The surface-<span class="hlt">wave</span> inversion part uses the propagator matrix solver in the algorithm DISPER80 (Saito, 1988) for forward calculation of dispersion curves from layered velocity models and the related sensitivities. The application of the joint inversion code to the SAFOD site in central California shows that the fault structure is better imaged in the new model, which is able to fit both the body-<span class="hlt">wave</span> and surface-<span class="hlt">wave</span> observations adequately. Here we present a new joint inversion method that solves the model in the wavelet domain constrained by sparsity regularization. Compared to the previous method, it has the following advantages: (1) The method is both data- and model-adaptive. For the velocity model, it can be represented by different wavelet coefficients at different scales, which are generally sparse. By constraining the model wavelet coefficients to be sparse, the inversion in the wavelet domain can inherently adapt to the data distribution so that the model has higher spatial resolution in the good data coverage <span class="hlt">zone</span>. Fang and Zhang (2014, Geophysical Journal International) have showed the superior performance of the wavelet-based double-difference seismic tomography method compared to the conventional method. (2) For the surface <span class="hlt">wave</span> inversion, the joint inversion code takes advantage of the recent development of direct inversion of surface <span class="hlt">wave</span> dispersion data for 3-D variations of shear <span class="hlt">wave</span> velocity without the intermediate step of phase or group velocity maps (Fang et al., 2014, Geophysical Journal International). A fast marching method is used to compute, at each period, surface <span class="hlt">wave</span> traveltimes and ray paths between sources and receivers. We will test the new joint</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24597153','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24597153"><span>Risk factors for closed-<span class="hlt">head</span> injuries during military airborne operations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Knapik, Joseph J; Steelman, Ryan; Hoedebecke, Kyle; Klug, Kevin L; Rankin, Shawn; Proctor, Stanley; Graham, Bria; Jones, Bruce H</p> <p>2014-02-01</p> <p>One of the more serious adverse outcomes of military airborne operations is closed-<span class="hlt">head</span> injuries. This investigation examined risk factors for closed-<span class="hlt">head</span> injuries in an Army airborne infantry unit. Closed-<span class="hlt">head</span> injuries were defined as energy exchanges in which the <span class="hlt">head</span> contacted the ground or an object and the soldier sought medical care for external trauma, headache, loss of consciousness, or altered mental state. Injury data were obtained by investigators in the drop <span class="hlt">zone</span> and diagnoses were confirmed by a physician. Operational data on potential injury risk factors were obtained from routine reports published by the infantry unit. Weather data were obtained using a pocket weather tracker. There were 96,132 jumps resulting in 310 closed-<span class="hlt">head</span> injuries for a crude incidence of 3.22/1000 jumps. In 98% of known cases the injury was associated with parachute landings. Multivariate logistic regression revealed that independent risk factors for closed-<span class="hlt">head</span> injuries included night jumps, combat loads, higher wind speeds, higher temperatures, enlisted rank, and entanglements. This study identifies the current incidence and extrinsic risk factors for closed-<span class="hlt">head</span> injuries during military airborne operations. Although it is necessary to conduct airborne training under realistic conditions, trainers and commanders should be aware of these risks and plan airborne operations accordingly.</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://www.dtic.mil/docs/citations/ADA623542','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA623542"><span>Introduction to Phase-Resolving <span class="hlt">Wave</span> Modeling with FUNWAVE</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-07-01</p> <p>Boussinesq <span class="hlt">wave</span> models have become a useful tool for modeling surface <span class="hlt">wave</span> transformation from deep water to the swash <span class="hlt">zone</span>, as well as <span class="hlt">wave</span>-induced...overlapping area of ghost cells, three rows deep , as required by the fourth-order MUSCL-TVD scheme. The MPI with nonblocking communication was used to...implemented ERDC/CHL CHETN-I-87 July 2015 12 SPONGE LAYER SPONGE_ON Sponge_west_width Sponge_east_width Sponge_south_width</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JSeis..17.1321T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JSeis..17.1321T"><span>Crustal thickness variations in the Zagros continental collision <span class="hlt">zone</span> (Iran) from joint inversion of receiver functions and surface <span class="hlt">wave</span> dispersion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tatar, M.; Nasrabadi, A.</p> <p>2013-10-01</p> <p>Variations in crustal thickness in the Zagros determined by joint inversion of P <span class="hlt">wave</span> receiver functions (RFs) and Rayleigh <span class="hlt">wave</span> group and phase velocity dispersion. The time domain iterative deconvolution procedure was employed to compute RFs from teleseismic recordings at seven broadband stations of INSN network. Rayleigh <span class="hlt">wave</span> phase velocity dispersion curves were estimated employing two-station method. Fundamental mode Rayleigh <span class="hlt">wave</span> group velocities for each station is taken from a regional scale surface <span class="hlt">wave</span> tomographic imaging. The main variations in crustal thickness that we observe are between stations located in the Zagros fold and thrust belt with those located in the Sanandaj-Sirjan <span class="hlt">zone</span> (SSZ) and Urumieh-Dokhtar magmatic assemblage (UDMA). Our results indicate that the average crustal thickness beneath the Zagros Mountain Range varies from ˜46 km in Western and Central Zagros beneath SHGR and GHIR up to ˜50 km beneath BNDS located in easternmost of the Zagros. Toward NE, we observe an increase in Moho depth where it reaches ˜58 km beneath SNGE located in the SSZ. Average crustal thickness also varies beneath the UDMA from ˜50 km in western parts below ASAO to ˜58 in central parts below NASN. The observed variation along the SSZ and UDMA may be associated to ongoing slab steepening or break off in the NW Zagros, comparing under thrusting of the Arabian plate beneath Central Zagros. The results show that in Central Iran, the crustal thickness decrease again to ˜47 km below KRBR. There is not a significant crustal thickness difference along the Zagros fold and thrust belt. We found the same crystalline crust of ˜34 km thick beneath the different parts of the Zagros fold and thrust belt. The similarity of crustal structure suggests that the crust of the Zagros fold and thrust belt was uniform before subsidence and deposition of the sediments. Our results confirm that the shortening of the western and eastern parts of the Zagros basement is small and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ShWav..27..919S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ShWav..27..919S"><span>Correlative analysis of <span class="hlt">head</span> kinematics and brain's tissue response: a computational approach toward understanding the mechanisms of blast TBI</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sarvghad-Moghaddam, H.; Rezaei, A.; Ziejewski, M.; Karami, G.</p> <p>2017-11-01</p> <p>Upon impingement of blast <span class="hlt">waves</span> on the <span class="hlt">head</span>, stress <span class="hlt">waves</span> generated at the interface of the skull are transferred into the cranium and the brain tissue and may cause mild to severe blast traumatic brain injury. The intensity of the shock front, defined by the blast overpressure (BoP), that is, the blast-induced peak static overpressure, significantly affects <span class="hlt">head</span> kinematics as well as the tissue responses of the brain. While evaluation of global linear and rotational accelerations may be feasible, an experimental determination of dynamic responses of the brain in terms of intracranial pressure (ICP), maximum shear stress (MSS), and maximum principal strain (MPS) is almost impossible. The main objective of this study is to investigate possible correlations between <span class="hlt">head</span> accelerations and the brain's ICP, MSS, and MPS. To this end, three different blasts were simulated by modeling the detonation of 70, 200, and 500 g of TNT at a fixed distance from the <span class="hlt">head</span>, corresponding to peak BoPs of 0.52, 1.2, and 2 MPa, respectively. A nonlinear multi-material finite element algorithm was implemented in the LS-DYNA explicit solver. Fluid-solid interaction between the blast <span class="hlt">waves</span> and <span class="hlt">head</span> was modeled using a penalty-based method. Strong correlations were found between the brain's dynamic responses and both global linear and rotational accelerations at different blast intensities (R^{2 }≥98%), implying that global kinematic parameters of the <span class="hlt">head</span> might be strong predictors of brain tissue biomechanical parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RSPTA.37670094K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RSPTA.37670094K"><span>Existence and amplitude bounds for irrotational water <span class="hlt">waves</span> in finite depth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kogelbauer, Florian</p> <p>2017-12-01</p> <p>We prove the existence of solutions to the irrotational water-<span class="hlt">wave</span> problem in finite depth and derive an explicit upper bound on the amplitude of the nonlinear solutions in terms of the wavenumber, the total hydraulic <span class="hlt">head</span>, the <span class="hlt">wave</span> speed and the relative mass flux. Our approach relies upon a reformulation of the water-<span class="hlt">wave</span> problem as a one-dimensional pseudo-differential equation and the Newton-Kantorovich iteration for Banach spaces. This article is part of the theme issue 'Nonlinear water <span class="hlt">waves</span>'.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMDI41B4336N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMDI41B4336N"><span>Evidence from P-<span class="hlt">wave</span> receiver functions for lower mantle plumes and mantle transition <span class="hlt">zone</span> water beneath West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nyblade, A.; Emry, E.; Juliá, J.; Anandakrishnan, S.; Aster, R. C.; Wiens, D. A.; Huerta, A. D.; Wilson, T. J.</p> <p>2014-12-01</p> <p>West Antarctica has experienced abundant Cenozoic volcanism, and it is suspected that the region is influenced by upwelling thermal plumes from the lower mantle; however this has not yet been verified, because seismic tomography results are not well resolved at mantle transition <span class="hlt">zone</span> (MTZ) depths. We use P-<span class="hlt">wave</span> receiver functions (PRFs) from the 2007-2013 Antarctic POLENET array to explore the characteristics of the MTZ throughout Marie Byrd Land and the West Antarctic Rift System. We obtained over 8000 high-quality PRFs for earthquakes occurring at 30-90° with Mb>5.5 using a time-domain iterative deconvolution method filtered with a Gaussian-width of 0.5 and 1.0, corresponding to frequencies less than ~0.24 Hz and ~0.48 Hz, respectively. We stack P receiver functions as single-station and by common conversion point and migrate them to depth using the ak135 1-d velocity model. Results suggest that the thickness of the MTZ varies throughout the region with thinning beneath the Ruppert Coast of Marie Byrd Land and beneath the Bentley Subglacial Trench and Whitmore Mountains. We identify the 520' discontinuity throughout much of West Antarctica; the discontinuity is most prominent beneath the Bentley Subglacial Trench and Whitmore Mountains. Additionally, prominent negative peaks are detected above the transition <span class="hlt">zone</span> beneath much of West Antarctica and may be evidence for water-induced partial melt above the MTZ. We propose that the MTZ beneath West Antarctica is hotter than average in some regions, possibly due to material upwelling from the lower mantle. Furthermore, we propose that the transition <span class="hlt">zone</span> is water-rich and that upward migration of hydrated material results in formation of a partial melt layer above the MTZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17829212','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17829212"><span>Simulation of tsunamis from great earthquakes on the cascadia subduction <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ng, M K; Leblond, P H; Murty, T S</p> <p>1990-11-30</p> <p>Large earthquakes occur episodically in the Cascadia subduction <span class="hlt">zone</span>. A numerical model has been used to simulate and assess the hazards of a tsunami generated by a hypothetical earthquake of magnitude 8.5 associated with rupture of the northern sections of the subduction <span class="hlt">zone</span>. <span class="hlt">Wave</span> amplitudes on the outer coast are closely related to the magnitude of sea-bottom displacement (5.0 meters). Some amplification, up to a factor of 3, may occur in some coastal embayments. <span class="hlt">Wave</span> amplitudes in the protected waters of Puget Sound and the Strait of Georgia are predicted to be only about one fifth of those estmated on the outer coast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EPJST.185...81S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EPJST.185...81S"><span>Rogue <span class="hlt">waves</span> in shallow water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soomere, T.</p> <p>2010-07-01</p> <p>Most of the processes resulting in the formation of unexpectedly high surface <span class="hlt">waves</span> in deep water (such as dispersive and geometrical focusing, interactions with currents and internal <span class="hlt">waves</span>, reflection from caustic areas, etc.) are active also in shallow areas. Only the mechanism of modulational instability is not active in finite depth conditions. Instead, <span class="hlt">wave</span> amplification along certain coastal profiles and the drastic dependence of the run-up height on the incident <span class="hlt">wave</span> shape may substantially contribute to the formation of rogue <span class="hlt">waves</span> in the nearshore. A unique source of long-living rogue <span class="hlt">waves</span> (that has no analogues in the deep ocean) is the nonlinear interaction of obliquely propagating solitary shallow-water <span class="hlt">waves</span> and an equivalent mechanism of Mach reflection of <span class="hlt">waves</span> from the coast. The characteristic features of these processes are (i) extreme amplification of the steepness of the <span class="hlt">wave</span> fronts, (ii) change in the orientation of the largest <span class="hlt">wave</span> crests compared with that of the counterparts and (iii) rapid displacement of the location of the extreme <span class="hlt">wave</span> humps along the crests of the interacting <span class="hlt">waves</span>. The presence of coasts raises a number of related questions such as the possibility of conversion of rogue <span class="hlt">waves</span> into sneaker <span class="hlt">waves</span> with extremely high run-up. Also, the reaction of bottom sediments and the entire coastal <span class="hlt">zone</span> to the rogue <span class="hlt">waves</span> may be drastic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMDI31B2185B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMDI31B2185B"><span>Global Transition <span class="hlt">Zone</span> Anisotropy and Consequences for Mantle Flow and Earth's Deep Water Cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beghein, C.; Yuan, K.</p> <p>2011-12-01</p> <p>The transition <span class="hlt">zone</span> has long been at the center of the debate between multi- and single-layered convection models that directly relate to heat transport and chemical mixing throughout the mantle. It has also been suggested that the transition <span class="hlt">zone</span> is a reservoir that collects water transported by subduction of the lithosphere into the mantle. Since water lowers mantle minerals density and viscosity, thereby modifying their rheology and melting behavior, it likely affects global mantle dynamics and the history of plate tectonics. Constraining mantle flow is therefore important for our understanding of Earth's thermochemical evolution and deep water cycle. Because it can result from deformation by dislocation creep during convection, seismic anisotropy can help us model mantle flow. It is relatively well constrained in the uppermost mantle, but its presence in the transition <span class="hlt">zone</span> is still debated. Its detection below 250 km depth has been challenging to date because of the poor vertical resolution of commonly used datasets. In this study, we used global Love <span class="hlt">wave</span> overtone phase velocity maps, which are sensitive to structure down to much larger depths than fundamental modes alone, and have greater depth resolution than shear <span class="hlt">wave</span>-splitting data. This enabled us to obtain a first 3-D model of azimuthal anisotropy for the upper 800km of the mantle. We inverted the 2Ψ terms of anisotropic phase velocity maps [Visser, et al., 2008] for the first five Love <span class="hlt">wave</span> overtones between 35s and 174s period. The resulting model shows that the average anisotropy amplitude for vertically polarized shear <span class="hlt">waves</span> displays two main stable peaks: one in the uppermost mantle and, most remarkably, one in the lower transition <span class="hlt">zone</span>. F-tests showed that the presence of 2Ψ anisotropy in the transition <span class="hlt">zone</span> is required to improve the third, fourth, and fifth overtones fit. Because of parameter trade-offs, however, we cannot exclude that the anisotropy is located in the upper transition <span class="hlt">zone</span> as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017743','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017743"><span>Detection of and response to a probable volcanogenic T-<span class="hlt">wave</span> event swarm on the western Blanco Transform Fault <span class="hlt">Zone</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>Dziak, R.P.; Fox, C.G.; Embley, R.W.; Lupton, J.E.; Johnson, G.C.; Chadwick, W.W.; Koski, R.A.</p> <p>1996-01-01</p> <p>The East Blanco Depression (EBD), a pull-apart basin within the western Blanco Transform Fault <span class="hlt">Zone</span> (BTFZ), was the site of an intense earthquake T-<span class="hlt">wave</span> swarm that began at 1317Z on January 9, 1994. Although tectonically generated earthquakes occur frequently along the BTFZ, this swarm was unusual in that it was preceded and accompanied by periodic, low-frequency, long-duration acoustic signals, that originated from near the swarm epicenters. These tremor-like signals were very similar in character to acoustic energy produced by a shallow-submarine eruption near Socorro Island, a seamount several hundred km west of Baja, California. The ???69 earthquakes and ???400 tremor-like events at the EBD occurred sporadically, with two periods of peak activity occurring between January 5-16 and 27-31. The swarm-like character of the earthquakes and the similarity of the tremor activity to the Socorro eruption indicated that the EBD was undergoing an intrusion or eruption episode. On January 27, six CTD/rosette casts were conducted at the site. Water samples from two of the stations yielded anomalous 3He concentrations, with maxima at ???2800 m depth over the main basin. In June 1994 two camera tows within the basin yielded evidence of pillow-lava volcanism and hydrothermal deposits, but no conclusive evidence of a recent seafloor eruption. In September 1994, deployments of the U.S. Navy's Advanced Tethered Vehicle resulted in the discovery of an active hydrothermal mound on the flanks of a pillow-lava volcano. The hydrothermal mound consists of Fe-rich hydrothermal precipitate and bacterial mats. Temperatures to 60??C were measured 30 cm below the surface. This is the first discovery of active hydrothermal vents along an oceanic fracture <span class="hlt">zone</span>. Although no conclusive evidence of volcanic activity associated with the T-<span class="hlt">wave</span> event swarm was found during these response efforts, the EBD has been the site of recent seafloor eruptions. Copyright 1996 by the American Geophysical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMSA...16..159B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMSA...16..159B"><span>Optimization of bottom-hinged flap-type <span class="hlt">wave</span> energy converter for a specific <span class="hlt">wave</span> rose</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Behzad, Hamed; Panahi, Roozbeh</p> <p>2017-06-01</p> <p>In this paper, we conducted a numerical analysis on the bottom-hinged flap-type <span class="hlt">Wave</span> Energy Convertor (WEC). The basic model, implemented through the study using ANSYS-AQWA, has been validated by a three-dimensional physical model of a pitching vertical cylinder. Then, a systematic parametric assessment has been performed on stiffness, damping, and WEC direction against an incoming <span class="hlt">wave</span> rose, resulting in an optimized flap-type WEC for a specific spot in the Persian Gulf. Here, stiffness is tuned to have a near-resonance condition considering the <span class="hlt">wave</span> rose, while damping is modified to capture the highest energy for each device direction. Moreover, such sets of specifications have been checked at different directions to present the best combination of stiffness, damping, and device <span class="hlt">heading</span>. It has been shown that for a real condition, including different <span class="hlt">wave</span> heights, periods, and directions, it is very important to implement the methodology introduced here to guarantee device performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoJI.210..931R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoJI.210..931R"><span>Subsurface images of the Eastern Rift, Africa, from the joint inversion of body <span class="hlt">waves</span>, surface <span class="hlt">waves</span> and gravity: investigating the role of fluids in early-stage continental rifting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roecker, S.; Ebinger, C.; Tiberi, C.; Mulibo, G.; Ferdinand-Wambura, R.; Mtelela, K.; Kianji, G.; Muzuka, A.; Gautier, S.; Albaric, J.; Peyrat, S.</p> <p>2017-08-01</p> <p>The Eastern Rift System (ERS) of northern Tanzania and southern Kenya, where a cratonic lithosphere is in the early stages of rifting, offers an ideal venue for investigating the roles of magma and other fluids in such an environment. To illuminate these roles, we jointly invert arrival times of locally recorded P and S body <span class="hlt">waves</span>, phase delays of ambient noise generated Rayleigh <span class="hlt">waves</span> and Bouguer anomalies from gravity observations to generate a 3-D image of P and S <span class="hlt">wave</span> speeds in the upper 25 km of the crust. While joint inversion of gravity and arrival times requires a relationship between density and <span class="hlt">wave</span> speeds, the improvement in resolution obtained by the combination of these disparate data sets serves to further constrain models, and reduce uncertainties. The most significant features in the 3-D model are (1) P and S <span class="hlt">wave</span> speeds that are 10-15 per cent lower beneath the rift <span class="hlt">zone</span> than in the surrounding regions, (2) a relatively high <span class="hlt">wave</span> speed tabular feature located along the western edge of the Natron and Manyara rifts, and (3) low (∼1.71) values of Vp/Vs throughout the upper crust, with the lowest ratios along the boundaries of the rift <span class="hlt">zones</span>. The low P and S <span class="hlt">wave</span> speeds at mid-crustal levels beneath the rift valley are an expected consequence of active volcanism, and the tabular, high-<span class="hlt">wave</span> speed feature is interpreted to be an uplifted footwall at the western edge of the rift. Given the high levels of CO2 outgassing observed at the surface along border fault <span class="hlt">zones</span>, and the sensitivity of Vp/Vs to pore-fluid compressibility, we infer that the low Vp/Vs values in and around the rift <span class="hlt">zone</span> are caused by the volcanic plumbing in the upper crust being suffused by a gaseous CO2 froth on top of a deeper, crystalline mush. The repository for molten rock is likely located in the lower crust and upper mantle, where the Vp/Vs ratios are significantly higher.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED031623.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED031623.pdf"><span>Educational Interests of Disadvantaged and Non-Disadvantaged Iowa Household <span class="hlt">Heads</span>.</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>Arendt, Donald Philip</p> <p></p> <p>A study was made of 538 disadvantaged and 247 non-disadvantaged household <span class="hlt">heads</span> in Iowa -- their occupation, training desired, material possessions, membership and participation. The sample included 643 males and 142 females and was distributed in <span class="hlt">zones</span> from open country to large urban areas. According to the prescribed criteria 14% of the…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1224043-directly-imaging-steeply-dipping-fault-zones-geothermal-fields-multicomponent-seismic-data','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1224043-directly-imaging-steeply-dipping-fault-zones-geothermal-fields-multicomponent-seismic-data"><span>Directly imaging steeply-dipping fault <span class="hlt">zones</span> in geothermal fields with multicomponent seismic data</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Chen, Ting; Huang, Lianjie</p> <p>2015-07-30</p> <p>For characterizing geothermal systems, it is important to have clear images of steeply-dipping fault <span class="hlt">zones</span> because they may confine the boundaries of geothermal reservoirs and influence hydrothermal flow. Elastic reverse-time migration (ERTM) is the most promising tool for subsurface imaging with multicomponent seismic data. However, conventional ERTM usually generates significant artifacts caused by the cross correlation of undesired wavefields and the polarity reversal of shear <span class="hlt">waves</span>. In addition, it is difficult for conventional ERTM to directly image steeply-dipping fault <span class="hlt">zones</span>. We develop a new ERTM imaging method in this paper to reduce these artifacts and directly image steeply-dipping fault <span class="hlt">zones</span>.more » In our new ERTM method, forward-propagated source wavefields and backward-propagated receiver wavefields are decomposed into compressional (P) and shear (S) components. Furthermore, each component of these wavefields is separated into left- and right-going, or downgoing and upgoing <span class="hlt">waves</span>. The cross correlation imaging condition is applied to the separated wavefields along opposite propagation directions. For converted <span class="hlt">waves</span> (P-to-S or S-to-P), the polarity correction is applied to the separated wavefields based on the analysis of Poynting vectors. Numerical imaging examples of synthetic seismic data demonstrate that our new ERTM method produces high-resolution images of steeply-dipping fault <span class="hlt">zones</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-09-06/pdf/2012-21921.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-09-06/pdf/2012-21921.pdf"><span>77 FR 54813 - Safety <span class="hlt">Zone</span>; <span class="hlt">Head</span> of the Cuyahoga, U.S. Rowing Masters <span class="hlt">Head</span> Race National Championship, and...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-09-06</p> <p>... Dragon Boat Festival, Cuyahoga River, Cleveland, OH AGENCY: Coast Guard, DHS. ACTION: Temporary final... Dragon Boat Festival. This safety <span class="hlt">zone</span> is necessary to protect spectators, participants, and vessels from... conjunction with the HOTC, the Cleveland Dragon Boat Festival will take place just north of the Detroit...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/1994/4012/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/1994/4012/report.pdf"><span>Description and application of capture <span class="hlt">zone</span> delineation for a wellfield at Hilton <span class="hlt">Head</span> Island, South Carolina</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Landmeyer, J.E.</p> <p>1994-01-01</p> <p>Ground-water capture <span class="hlt">zone</span> boundaries for individual pumped wells in a confined aquffer were delineated by using groundwater models. Both analytical and numerical (semi-analytical) models that more accurately represent the $round-water-flow system were used. All models delineated 2-dimensional boundaries (capture <span class="hlt">zones</span>) that represent the areal extent of groundwater contribution to a pumped well. The resultant capture <span class="hlt">zones</span> were evaluated on the basis of the ability of each model to realistically rapresent the part of the ground-water-flow system that contributed water to the pumped wells. Analytical models used were based on a fixed radius approach, and induded; an arbitrary radius model, a calculated fixed radius model based on the volumetric-flow equation with a time-of-travel criterion, and a calculated fixed radius model derived from modification of the Theis model with a drawdown criterion. Numerical models used induded the 2-dimensional, finite-difference models RESSQC and MWCAP. The arbitrary radius and Theis analytical models delineated capture <span class="hlt">zone</span> boundaries that compared least favorably with capture <span class="hlt">zones</span> delineated using the volumetric-flow analytical model and both numerical models. The numerical models produced more hydrologically reasonable capture <span class="hlt">zones</span> (that were oriented parallel to the regional flow direction) than the volumetric-flow equation. The RESSQC numerical model computed more hydrologically realistic capture <span class="hlt">zones</span> than the MWCAP numerical model by accounting for changes in the shape of capture <span class="hlt">zones</span> caused by multiple-well interference. The capture <span class="hlt">zone</span> boundaries generated by using both analytical and numerical models indicated that the curnmtly used 100-foot radius of protection around a wellhead in South Carolina is an underestimate of the extent of ground-water capture for pumped wetis in this particular wellfield in the Upper Floridan aquifer. The arbitrary fixed radius of 100 feet was shown to underestimate the upgradient</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900002426','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900002426"><span><span class="hlt">Wave</span> combustors for trans-atmospheric vehicles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Menees, Gene P.; Adelman, Henry G.; Cambier, Jean-Luc; Bowles, Jeffrey V.</p> <p>1989-01-01</p> <p>The <span class="hlt">Wave</span> Combustor is an airbreathing hypersonic propulsion system which utilizes shock and detonation <span class="hlt">waves</span> to enhance fuel-air mixing and combustion in supersonic flow. In this concept, an oblique shock <span class="hlt">wave</span> in the combustor can act as a flameholder by increasing the pressure and temperature of the air-fuel mixture and thereby decreasing the ignition delay. If the oblique shock is sufficiently strong, then the combustion front and the shock <span class="hlt">wave</span> can couple into a detonation <span class="hlt">wave</span>. In this case, combustion occurs almost instantaneously in a thin <span class="hlt">zone</span> behind the <span class="hlt">wave</span> front. The result is a shorter, lighter engine compared to the scramjet. This engine, which is called the Oblique Detonation <span class="hlt">Wave</span> Engine (ODWE), can then be utilized to provide a smaller, lighter vehicle or to provide a higher payload capability for a given vehicle weight. An analysis of the performance of a conceptual trans-atmospheric vehicle powered by an ODWE is given here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JNEng..14c6011Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JNEng..14c6011Z"><span>Imaging three-dimensional innervation <span class="hlt">zone</span> distribution in muscles from M-<span class="hlt">wave</span> recordings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Chuan; Peng, Yun; Liu, Yang; Li, Sheng; Zhou, Ping; Zev Rymer, William; Zhang, Yingchun</p> <p>2017-06-01</p> <p>Objective. To localize neuromuscular junctions in skeletal muscles in vivo which is of great importance in understanding, diagnosing and managing of neuromuscular disorders. Approach. A three-dimensional global innervation <span class="hlt">zone</span> imaging technique was developed to characterize the global distribution of innervation <span class="hlt">zones</span>, as an indication of the location and features of neuromuscular junctions, using electrically evoked high-density surface electromyogram recordings. Main results. The performance of the technique was evaluated in the biceps brachii of six intact human subjects. The geometric centers of the distributions of the reconstructed innervation <span class="hlt">zones</span> were determined with a mean distance of 9.4  ±  1.4 cm from the reference plane, situated at the medial epicondyle of the humerus. A mean depth was calculated as 1.5  ±  0.3 cm from the geometric centers to the closed points over the skin. The results are consistent with those reported in previous histology studies. It was also found that the volumes and distributions of the reconstructed innervation <span class="hlt">zones</span> changed as the stimulation intensities increased until the supramaximal muscle response was achieved. Significance. Results have demonstrated the high performance of the proposed imaging technique in noninvasively imaging global distributions of the innervation <span class="hlt">zones</span> in the three-dimensional muscle space in vivo, and the feasibility of its clinical applications, such as guiding botulinum toxin injections in spasticity management, or in early diagnosis of neurodegenerative progression of amyotrophic lateral sclerosis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960002674','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960002674"><span>Augmented shock <span class="hlt">wave</span> fracture/severance of materials</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schimmel, Morry L. (Inventor); Bement, Laurence J. (Inventor)</p> <p>1995-01-01</p> <p>The present invention related generally to severing materials, and more particularly to severing or weakening materials through explosively induced, augmented shock <span class="hlt">waves</span>. Explosive cords are placed in grooves on the upper surface of the material to be severed or weakened. The explosive cords are initiated simultaneously to introduce explosive shock <span class="hlt">waves</span> into the material. These shock <span class="hlt">waves</span> progress toward the centerline between the explosive cords and the lower surface of the material. Intersecting and reflected <span class="hlt">waves</span> produce a rarefaction <span class="hlt">zone</span> on the centerline to fail the material in tension. A groove may also be cut in the lower surface of the material to aid in severing or weakening the material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27067470','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27067470"><span>Trunnionosis: Does <span class="hlt">Head</span> Size Affect Fretting and Corrosion in Total Hip Arthroplasty?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Del Balso, Christopher; Teeter, Matthew G; Tan, Sok Chuen; Howard, James L; Lanting, Brent A</p> <p>2016-10-01</p> <p>Wear and tribocorrosion at the modular <span class="hlt">head</span>-neck taper interface may be a cause of failure in metal-on-polyethylene total hip arthroplasty (THA). The present investigation endeavored to elucidate the effect of femoral <span class="hlt">head</span> diameter on fretting and corrosion in retrieved <span class="hlt">head</span>-neck tapers. A retrieval analysis of THA prostheses in vivo for a minimum of 1 year was performed. Twenty-three femoral <span class="hlt">heads</span> of 32-mm diameter were matched with 28-mm <span class="hlt">heads</span> based on time in vivo and <span class="hlt">head</span> length (-3 mm to +8 mm). All included implants featured a single taper design from a single manufacturer. Fretting and corrosion damage scoring was performed for each implant under stereomicroscopic visualization. <span class="hlt">Head</span> diameter was observed to affect fretting (P = .01), with 32-mm femoral <span class="hlt">heads</span> exhibiting greater total fretting scores than 28-mm <span class="hlt">heads</span>. Fretting damage was greatest (P = .01) in the central concentric <span class="hlt">zone</span> of the femoral <span class="hlt">head</span> bore tapers, regardless of <span class="hlt">head</span> diameter, length, or stem offset. No significant effect on total corrosion scores was observed for any <span class="hlt">head</span> or stem variable. Retrieved implant total corrosion scores were positively correlated (ρ = 0.51, P < .001) with implantation time. Increased femoral <span class="hlt">head</span> diameter in THA may produce greater fretting damage owing to and increased <span class="hlt">head</span>-neck moment arm. There is no associated increase in corrosion with 28-mm and 32-mm <span class="hlt">heads</span> of this taper design. The longer a THA prosthesis is implanted, the greater the risk of damage due to corrosion. Copyright © 2016 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S31B4391P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S31B4391P"><span>High-Resolution 3D P-<span class="hlt">Wave</span> Velocity Model in the Trans-European Suture <span class="hlt">Zone</span> 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>Polkowski, M.; Grad, M.; Ostaficzuk, S.</p> <p>2014-12-01</p> <p>Poland is located on conjunction of major European tectonic units - the Precambrian East European Craton and the Paleozoic Platform of Central and Western Europe. This conjunction is known as Trans-European Suture <span class="hlt">Zone</span> (TESZ). Geological and seismic structure under area of Poland is well studied by over one hundred thousand boreholes, over thirty deep seismic refraction and wide angle reflection profiles and other methods: vertical seismic profiling, magnetic, gravity, magnetotelluric, thermal. Compilation of these studies allows creation of detailed, high-resolution 3D P-<span class="hlt">wave</span> velocity model for entire Earth's crust in the area of Poland. Model provides detailed six layer sediments (Tertiary and Quaternary, Cretaceous, Jurassic, Triassic, Permian, old Paleozoic), consolidated / crystalline crust and uppermost mantle. Continental suturing is a fundamental part of the plate tectonic cycle, and knowing its detailed structure allows understanding plate tectonic cycle. We present a set of crustal cross sections through the TESZ, illustrating differentiation in the structure between Precambrian and Wariscan Europe. National Science Centre Poland provided financial support for this work by NCN grant DEC- 2011/02/A/ST10/00284.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006PhFl...18e7106C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006PhFl...18e7106C"><span>Solitary water <span class="hlt">wave</span> interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Craig, W.; Guyenne, P.; Hammack, J.; Henderson, D.; Sulem, C.</p> <p>2006-05-01</p> <p>This article concerns the pairwise nonlinear interaction of solitary <span class="hlt">waves</span> in the free surface of a body of water lying over a horizontal bottom. Unlike solitary <span class="hlt">waves</span> in many completely integrable model systems, solitary <span class="hlt">waves</span> for the full Euler equations do not collide elastically; after interactions, there is a nonzero residual <span class="hlt">wave</span> that trails the post-collision solitary <span class="hlt">waves</span>. In this report on new numerical and experimental studies of such solitary <span class="hlt">wave</span> interactions, we verify that this is the case, both in <span class="hlt">head</span>-on collisions (the counterpropagating case) and overtaking collisions (the copropagating case), quantifying the degree to which interactions are inelastic. In the situation in which two identical solitary <span class="hlt">waves</span> undergo a <span class="hlt">head</span>-on collision, we compare the asymptotic predictions of Su and Mirie [J. Fluid Mech. 98, 509 (1980)] and Byatt-Smith [J. Fluid Mech. 49, 625 (1971)], the wavetank experiments of Maxworthy [J. Fluid Mech. 76, 177 (1976)], and the numerical results of Cooker, Weidman, and Bale [J. Fluid Mech. 342, 141 (1997)] with independent numerical simulations, in which we quantify the phase change, the run-up, and the form of the residual <span class="hlt">wave</span> and its Fourier signature in both small- and large-amplitude interactions. This updates the prior numerical observations of inelastic interactions in Fenton and Rienecker [J. Fluid Mech. 118, 411 (1982)]. In the case of two nonidentical solitary <span class="hlt">waves</span>, our precision wavetank experiments are compared with numerical simulations, again observing the run-up, phase lag, and generation of a residual from the interaction. Considering overtaking solitary <span class="hlt">wave</span> interactions, we compare our experimental observations, numerical simulations, and the asymptotic predictions of Zou and Su [Phys. Fluids 29, 2113 (1986)], and again we quantify the inelastic residual after collisions in the simulations. Geometrically, our numerical simulations of overtaking interactions fit into the three categories of Korteweg-deVries two</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28964966','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28964966"><span>Ambient temperature and added heat <span class="hlt">wave</span> effects on hospitalizations in California from 1999 to 2009.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sherbakov, Toki; Malig, Brian; Guirguis, Kristen; Gershunov, Alexander; Basu, Rupa</p> <p>2018-01-01</p> <p>Investigators have examined how heat <span class="hlt">waves</span> or incremental changes in temperature affect health outcomes, but few have examined both simultaneously. We utilized distributed lag nonlinear models (DLNM) to explore temperature associations and evaluate possible added heat <span class="hlt">wave</span> effects on hospitalizations in 16 climate <span class="hlt">zones</span> throughout California from May through October 1999-2009. We define heat <span class="hlt">waves</span> as a period when daily mean temperatures were above the <span class="hlt">zone</span>- and month-specific 95th percentile for at least two consecutive days. DLNMs were used to estimate climate <span class="hlt">zone</span>-specific non-linear temperature and heat <span class="hlt">wave</span> effects, which were then combined using random effects meta-analysis to produce an overall estimate for each. With higher temperatures, admissions for acute renal failure, appendicitis, dehydration, ischemic stroke, mental health, non-infectious enteritis, and primary diabetes were significantly increased, with added effects from heat <span class="hlt">waves</span> observed for acute renal failure and dehydration. Higher temperatures also predicted statistically significant decreases in hypertension admissions, respiratory admissions, and respiratory diseases with secondary diagnoses of diabetes, though heat <span class="hlt">waves</span> independently predicted an added increase in risk for both respiratory types. Our findings provide evidence that both heat <span class="hlt">wave</span> and temperature exposures can exert effects independently. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMOS13D1226C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMOS13D1226C"><span>Infragravity <span class="hlt">wave</span> generation and dynamics over a mild slope beach : Experiments and numerical computations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cienfuegos, R.; Duarte, L.; Hernandez, E.</p> <p>2008-12-01</p> <p>Charasteristic frequencies of gravity <span class="hlt">waves</span> generated by wind and propagating towards the coast are usually comprised between 0.05Hz and 1Hz. Nevertheless, lower frequecy <span class="hlt">waves</span>, in the range of 0.001Hz and 0.05Hz, have been observed in the nearshore <span class="hlt">zone</span>. Those long <span class="hlt">waves</span>, termed as infragravity <span class="hlt">waves</span>, are generated by complex nonlinear mechanisms affecting the propagation of irregular <span class="hlt">waves</span> up to the coast. The groupiness of an incident random <span class="hlt">wave</span> field may be responsible for producing a slow modulation of the mean water surface thus generating bound long <span class="hlt">waves</span> travelling at the group speed. Similarly, a quasi- periodic oscillation of the break-point location, will be accompained by a slow modulation of set-up/set-down in the surf <span class="hlt">zone</span> and generation and release of long <span class="hlt">waves</span>. If the primary structure of the carrying incident gravity <span class="hlt">waves</span> is destroyed (e.g. by breaking), forced long <span class="hlt">waves</span> can be freely released and even reflected at the coast. Infragravity <span class="hlt">waves</span> can affect port operation through resonating conditions, or strongly affect sediment transport and beach morphodynamics. In the present study we investigate infragravity <span class="hlt">wave</span> generation mechanisms both, from experiments and numerical computations. Measurements were conducted at the 70-meter long <span class="hlt">wave</span> tank, located at the Instituto Nacional de Hidraulica (Chile), prepared with a beach of very mild slope of 1/80 in order to produce large surf <span class="hlt">zone</span> extensions. A random JONSWAP type <span class="hlt">wave</span> field (h0=0.52m, fp=0.25Hz, Hmo=0.17m) was generated by a piston <span class="hlt">wave</span>-maker and measurements of the free surface displacements were performed all over its length at high spatial resolution (0.2m to 1m). Velocity profiles were also measured at four verticals inside the surf <span class="hlt">zone</span> using an ADV. Correlation maps of <span class="hlt">wave</span> group envelopes and infragravity <span class="hlt">waves</span> are computed in order to identify long <span class="hlt">wave</span> generation and dynamics in the experimental set-up. It appears that both mechanisms (groupiness and break-point oscillation) are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S31B4390C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S31B4390C"><span>Using P-<span class="hlt">wave</span> Triplications to Constrain the Mantle Transition <span class="hlt">Zone</span> beneath Central Iranian Plateau and Surrounding Area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chi, H. C.; Tseng, T. L.</p> <p>2014-12-01</p> <p>The Iranian Plateau is a tectonically complex region resulting from the continental collision between the African and Eurasian plates. The convergence of the two continents created the Zagros Mountains, the high topography southwest of Iran, and active seismicity along the Zagros-Bitlis suture. Tomographic studies in Iran reveal low seismic speeds and high attenuation of Sn <span class="hlt">wave</span> in the uppermost mantle beneath the Iranian Plateau relative to adjacent regions. The deeper structure, however, remains curiously inconclusive. By contrast, a prominent fast seismic anomaly is found under central Tibet near depth of 600 km in the mantle transition <span class="hlt">zone</span> (TZ), and it is speculated to be the remnant of lithosphere detached during the continental collision. We conduct a comparative study that utilizes triplicate arrivals of high-resolution P waveforms to investigate the velocity structure of mantle beneath the central Iranian Plateau and surroundings. Due to the abrupt increase in seismic <span class="hlt">wave</span> speeds and density across the 410- and 660-km discontinuities, seismic <span class="hlt">waves</span> at epicentral distances of 15-30 degrees would form multiple arrivals and the relative times and amplitudes between them are most sensitive to the variations in seismic speeds near the TZ. We combine several broadband arrays to construct 8 seismic profiles, each about 800 km long, that mainly sample the TZ under central Iranian Plateau, Turan shield and part of South Caspian basin. Move-outs between arrivals are clear in the profiles. Relative timings suggest a slightly smaller 660-km contrast under stable Turan shield. In the next stage, it is necessary to model waveforms after the source effect being removed properly. Our preliminary tests show that the F-K method can efficiently calculate the synthetic seismograms. We will determine the 1D velocity model for each sampled sector by minimizing the overall misfits between observed and predicted waveforms. The lateral variations may be further explored by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11988935','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11988935"><span>Biomechanical changes in the <span class="hlt">head</span> associated with penetrating injuries of the maxilla and mandible: an experimental investigation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tan, Yinghui; Zhou, Shuxia; Jiang, Hetian</p> <p>2002-05-01</p> <p>In this experiment, we studied the craniocerebral injury that occurs due to the transmission of forces when maxillofacial gunshot wounds are sustained by the facial bones and cranium. Forty fresh pigs' <span class="hlt">heads</span> were wounded by one of the following methods: steel spheres weighing 1.03 g at an impact velocity of 1,400 m/s, steel spheres weighing 1.03 g at an impact velocity of 800 m/s, M193 military bullets, or M56 military bullets. Pressure <span class="hlt">waves</span> in the brain, acceleration of the <span class="hlt">head</span>, and stress changes in the facial bones and cranium at the moment of the impact were recorded by pressure and acceleration transducers and strain gauges and were statistically compared. Some obvious differences between the mechanical values obtained from high-and low-velocity missile wounds were found. A negative relationship between the peak value of the pressure <span class="hlt">wave</span> in the brain and the distance from the point of impact to the transducer was obtained. The acceleration of the <span class="hlt">head</span> in the direction of the ballistic path was the strongest in absolute value. There were differences in the stress values between the mandible and the temporal bone. Acceleration of the <span class="hlt">head</span>, pressure <span class="hlt">wave</span> changes in the brain, and injury from bony stress conduction all play important roles in associated craniocerebral damage after maxillofacial firearm wounds. Copyright 2002 American Association of Oral and Maxillofacial Surgeons</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMNG14A..07L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMNG14A..07L"><span>Understanding exchanges across turbulent/stratified <span class="hlt">zones</span> interfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Le Bars, M.; Ribeiro, A.; Le Gal, P.; Aurnou, J. M.</p> <p>2013-12-01</p> <p>In many geophysical and astrophysical situations, a turbulent fluid layer is separated from a stably stratified one by a relatively sharp but deformable interface. Examples include the convective and radiative <span class="hlt">zones</span> in stars, the atmospheric convective layer and overlying stratosphere, the Earth's outer core... While motions in the stratified layer are often neglected, it actually supports oscillatory motions called gravito-inertial <span class="hlt">waves</span> (GIW) excited by Reynolds stresses, entropy fluctuations and interface deformations associated with the turbulence. Besides their direct observation as for instance in asteroseismology, GIW transport energy, carry momentum, break, mix... and are thus essential for accurate models of global climate and solar or core dynamics. Global integrated models including length scales and time scales spanning many orders of magnitude are required to fully address motions in turbulent and stratified <span class="hlt">zones</span> and to understand the details of the highly non-linear couplings between rotation, meridional circulation, turbulence and <span class="hlt">waves</span>: this is clearly very challenging from both analytical and numerical points of view. Here, we present results from two complementary laboratory experiments using water as a working fluid and salt or temperature to control the buoyancy effects, allowing to address the whole range of relevant physical issues in simplified models. In the first set-up, we take benefit from the unusual property of water that its density has a maximum value near 4oC to study its convective and oscillatory motions in a tank with a bottom boundary at about 0oC and a hotter upper surface. High precision local measurements of temperature fluctuations are performed simultaneously in the convective and stratified <span class="hlt">zones</span> to produce the corresponding power density spectrum and probability density function. In the second set-up, a turbulent jet generated by injection of water impinges upon the interface between a uniform density layer and a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70180070','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70180070"><span>A method and example of seismically imaging near‐surface fault <span class="hlt">zones</span> in geologically complex areas using Vp, Vs, and their ratios</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Catchings, Rufus D.; Rymer, Michael J.; Goldman, Mark R.; Sickler, Robert R.; Criley, Coyn J.</p> <p>2014-01-01</p> <p>The determination of near‐surface (vadose <span class="hlt">zone</span> and slightly below) fault locations and geometries is important because assessment of ground rupture, strong shaking, geologic slip rates, and rupture histories occurs at shallow depths. However, seismic imaging of fault <span class="hlt">zones</span> at shallow depths can be difficult due to near‐surface complexities, such as weathering, groundwater saturation, massive (nonlayered) rocks, and vertically layered strata. Combined P‐ and S‐<span class="hlt">wave</span> seismic‐refraction tomography data can overcome many of the near‐surface, fault‐<span class="hlt">zone</span> seismic‐imaging problems because of differences in the responses of elastic (bulk and shear) moduli of P and S <span class="hlt">waves</span> to shallow‐depth, fault‐<span class="hlt">zone</span> properties. We show that high‐resolution refraction tomography images of P‐ to S‐<span class="hlt">wave</span> velocity ratios (VP/VS) can reliably identify near‐surface faults. We demonstrate this method using tomography images of the San Andreas fault (SAF) surface‐rupture <span class="hlt">zone</span> associated with the 18 April 1906 ∼M 7.9 San Francisco earthquake on the San Francisco peninsula in California. There, the SAF cuts through Franciscan mélange, which consists of an incoherent assemblage of greywacke, chert, greenstone, and serpentinite. A near‐vertical <span class="hlt">zone</span> (∼75° northeast dip) of high P‐<span class="hlt">wave</span> velocities (up to 3000  m/s), low S‐<span class="hlt">wave</span> velocities (∼150–600  m/s), high VP/VS ratios (4–8.8), and high Poisson’s ratios (0.44–0.49) characterizes the main surface‐rupture <span class="hlt">zone</span> to a depth of about 20 m and is consistent with nearby trench observations. We suggest that the combined VP/VSimaging approach can reliably identify most near‐surface fault <span class="hlt">zones</span> in locations where many other seismic methods cannot be applied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAESc.159...60L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAESc.159...60L"><span>Transdimensional inversion of scattered body <span class="hlt">waves</span> for 1D S-<span class="hlt">wave</span> velocity structure - Application to the Tengchong volcanic area, Southwestern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Mengkui; Zhang, Shuangxi; Bodin, Thomas; Lin, Xu; Wu, Tengfei</p> <p>2018-06-01</p> <p>Inversion of receiver functions is commonly used to recover the S-<span class="hlt">wave</span> velocity structure beneath seismic stations. Traditional approaches are based on deconvolved waveforms, where the horizontal component of P-<span class="hlt">wave</span> seismograms is deconvolved by the vertical component. Deconvolution of noisy seismograms is a numerically unstable process that needs to be stabilized by regularization parameters. This biases noise statistics, making it difficult to estimate uncertainties in observed receiver functions for Bayesian inference. This study proposes a method to directly invert observed radial waveforms and to better account for data noise in a Bayesian formulation. We illustrate its feasibility with two synthetic tests having different types of noises added to seismograms. Then, a real site application is performed to obtain the 1-D S-<span class="hlt">wave</span> velocity structure beneath a seismic station located in the Tengchong volcanic area, Southwestern China. Surface <span class="hlt">wave</span> dispersion measurements spanning periods from 8 to 65 s are jointly inverted with P waveforms. The results show a complex S-<span class="hlt">wave</span> velocity structure, as two low velocity <span class="hlt">zones</span> are observed in the crust and uppermost mantle, suggesting the existence of magma chambers, or <span class="hlt">zones</span> of partial melt. The upper magma chambers may be the heart source that cause the thermal activity on the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/nj0005.photos.106820p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/nj0005.photos.106820p/"><span>11. DETAIL OF TERRACOTTA DECORATION, SHOWING SCROLL CONSOLE, <span class="hlt">WAVE</span> ORNAMENT, ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>11. DETAIL OF TERRACOTTA DECORATION, SHOWING SCROLL CONSOLE, <span class="hlt">WAVE</span> ORNAMENT, EGG-AND-DART, NYMPH <span class="hlt">HEADS</span> AND FOLIATE PATTERN AROUND WINDOWS - City Hall, Atlantic & Tennessee Avenues, Atlantic City, Atlantic County, NJ</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70160542','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70160542"><span>Non-linear resonant coupling of tsunami edge <span class="hlt">waves</span> using stochastic earthquake source 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>Geist, Eric L.</p> <p>2016-01-01</p> <p>Non-linear resonant coupling of edge <span class="hlt">waves</span> can occur with tsunamis generated by large-magnitude subduction <span class="hlt">zone</span> earthquakes. Earthquake rupture <span class="hlt">zones</span> that straddle beneath the coastline of continental margins are particularly efficient at generating tsunami edge <span class="hlt">waves</span>. Using a stochastic model for earthquake slip, it is shown that a wide range of edge-<span class="hlt">wave</span> modes and wavenumbers can be excited, depending on the variability of slip. If two modes are present that satisfy resonance conditions, then a third mode can gradually increase in amplitude over time, even if the earthquake did not originally excite that edge-<span class="hlt">wave</span> mode. These three edge <span class="hlt">waves</span> form a resonant triad that can cause unexpected variations in tsunami amplitude long after the first arrival. An M ∼ 9, 1100 km-long continental subduction <span class="hlt">zone</span> earthquake is considered as a test case. For the least-variable slip examined involving a Gaussian random variable, the dominant resonant triad includes a high-amplitude fundamental mode <span class="hlt">wave</span> with wavenumber associated with the along-strike dimension of rupture. The two other <span class="hlt">waves</span> that make up this triad include subharmonic <span class="hlt">waves</span>, one of fundamental mode and the other of mode 2 or 3. For the most variable slip examined involving a Cauchy-distributed random variable, the dominant triads involve higher wavenumbers and modes because subevents, rather than the overall rupture dimension, control the excitation of edge <span class="hlt">waves</span>. Calculation of the resonant period for energy transfer determines which cases resonant coupling may be instrumentally observed. For low-mode triads, the maximum transfer of energy occurs approximately 20–30 <span class="hlt">wave</span> periods after the first arrival and thus may be observed prior to the tsunami coda being completely attenuated. Therefore, under certain circumstances the necessary ingredients for resonant coupling of tsunami edge <span class="hlt">waves</span> exist, indicating that resonant triads may be observable and implicated in late, large-amplitude tsunami arrivals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028356','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028356"><span>Integration of P- and SH-<span class="hlt">wave</span> high-resolution seismic reflection and micro-gravity techniques to improve interpretation of shallow subsurface structure: New Madrid seismic <span class="hlt">zone</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>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.</p> <p>2006-01-01</p> <p>Shallow high-resolution seismic reflection surveys have traditionally been restricted to either compressional (P) or horizontally polarized shear (SH) <span class="hlt">waves</span> in order to produce 2-D images of subsurface structure. The northernmost Mississippi embayment and coincident New Madrid seismic <span class="hlt">zone</span> (NMSZ) provide an ideal laboratory to study the experimental use of integrating P- and SH-<span class="hlt">wave</span> 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-<span class="hlt">wave</span> 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-<span class="hlt">waves</span> 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-<span class="hlt">wave</span> profiles acquired in southwestern Illinois and western Kentucky (USA) detect faulting of deep, Paleozoic bedrock and Cretaceous reflectors while coincident SH-<span class="hlt">wave</span> 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H31E0661N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H31E0661N"><span>A Novel Application of the Multichannel Analysis of Surface <span class="hlt">Waves</span> (MASW) Method for Estimating the Critical <span class="hlt">Zone</span> Thicknes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nelson, S.; Yaede, J.; McBride, J. H.; Park, C.; Turnbull, S. J.; Tingey, D. G.</p> <p>2014-12-01</p> <p>MASW approaches are suitable for the accurate measurement of variably thick weathering profiles by producing shear-<span class="hlt">wave</span> (Vs) profiles. The critical <span class="hlt">zone</span> (CZ) base is usually a transitional boundary, which is captured by MASW but not by conventional seismic reflection techniques. Modified MASW methods were used in Hawaii, USA to extend the investigative depth of saprolite (kaolin clays, Fe-oxides) thickness calibrated against wells with geologic logs. Active-source ± passive dispersion curves produced improved low-frequency fundamental modes by combining records with varying source-receiver offsets, enabling the generation of Vs profiles to >50 m depth. The top of unaltered bedrock occurs at a Vs of >~500 m/s. Intra-saprolite high Vs <span class="hlt">zones</span> probably represent aa flow interiors with fewer primary discontinuities (vesicles and fractures), therefore imparting higher secondary stiffness than altered pahoehoe and pyroclastic material. The MASW approach permits measuring CZ thicknesses at discrete locations rapidly, inexpensively, and without drilling. For example, employed on slopes of the Koolau Volcano (neither aggrading nor degrading), the downward rate of advance of the weathering front of the CZ varies from 0.02 to 0.03 mm/yr in wet and ~0.01 mm/yr in dry areas. This compares well with recent work based on solute mass fluxes averaged over large areas. MASW can be deployed in a variety of settings where rapid estimation of the CZ thickness at particular locations is desired.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950008656','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950008656"><span>On the physics of <span class="hlt">waves</span> in the solar atmosphere: <span class="hlt">Wave</span> heating and wind acceleration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Musielak, Z. E.</p> <p>1994-01-01</p> <p>New calculations of the acoustic <span class="hlt">wave</span> energy fluxes generated in the solar convective <span class="hlt">zone</span> have been performed. The treatment of convective turbulence in the sun and solar-like stars, in particular, the precise nature of the turbulent power spectrum has been recognized as one of the most important issues in the <span class="hlt">wave</span> generation problem. Several different functional forms for spatial and temporal spectra have been considered in the literature and differences between the energy fluxes obtained for different forms often exceed two orders of magnitude. The basic criterion for choosing the appropriate spectrum was the maximal efficiency of the <span class="hlt">wave</span> generation. We have used a different approach based on physical and empirical arguments as well as on some results from numerical simulation of turbulent convection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/29718','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/29718"><span>Investigation of truck mounted attenuator (TMA) crashes in work <span class="hlt">zones</span> in Virginia.</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>2015-10-01</p> <p>Truck mounted attenuators (TMAs) are deployed on shadow vehicles in work <span class="hlt">zones</span> to mitigate the effects of errant : vehicles that strike the shadow vehicle, either by smoothly decelerating the vehicle to a stop when hit <span class="hlt">head</span>-on or by redirecting : the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11347686','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11347686"><span><span class="hlt">Heading</span> and <span class="hlt">head</span> injuries in soccer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kirkendall, D T; Jordan, S E; Garrett, W E</p> <p>2001-01-01</p> <p>In the world of sports, soccer is unique because of the purposeful use of the unprotected <span class="hlt">head</span> for controlling and advancing the ball. This skill obviously places the player at risk of <span class="hlt">head</span> injury and the game does carry some risk. <span class="hlt">Head</span> injury can be a result of contact of the <span class="hlt">head</span> with another <span class="hlt">head</span> (or other body parts), ground, goal post, other unknown objects or even the ball. Such impacts can lead to contusions, fractures, eye injuries, concussions or even, in rare cases, death. Coaches, players, parents and physicians are rightly concerned about the risk of <span class="hlt">head</span> injury in soccer. Current research shows that selected soccer players have some degree of cognitive dysfunction. It is important to determine the reasons behind such deficits. Purposeful <span class="hlt">heading</span> has been blamed, but a closer look at the studies that focus on <span class="hlt">heading</span> has revealed methodological concerns that question the validity of blaming purposeful <span class="hlt">heading</span> of the ball. The player's history and age (did they play when the ball was leather and could absorb significant amounts of water), alcohol intake, drug intake, learning disabilities, concussion definition and control group use/composition are all factors that cloud the ability to blame purposeful <span class="hlt">heading</span>. What does seem clear is that a player's history of concussive episodes is a more likely explanation for cognitive deficits. While it is likely that the subconcussive impact of purposeful <span class="hlt">heading</span> is a doubtful factor in the noted deficits, it is unknown whether multiple subconcussive impacts might have some lingering effects. In addition, it is unknown whether the noted deficits have any affect on daily life. Proper instruction in the technique is critical because if the ball contacts an unprepared <span class="hlt">head</span> (as in accidental <span class="hlt">head</span>-ball contacts), the potential for serious injury is possible. To further our understanding of the relationship of <span class="hlt">heading</span>, <span class="hlt">head</span> injury and cognitive deficits, we need to: learn more about the actual impact of a ball on the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011APS..DFD.E3007D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011APS..DFD.E3007D"><span>Large-<span class="hlt">wave</span> simulation of spilling breaking and undertow current over constant slope beach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dimas, Athanassios; Kolokythas, Gerasimos; Dimakopoulos, Aggelos</p> <p>2011-11-01</p> <p>The three-dimensional, free-surface flow, developing by the propagation of nonlinear breaking <span class="hlt">waves</span> over a constant slope bed, is numerically simulated. The main objective is to investigate the effect of spilling breaking on the characteristics of the induced undertow current by performing large-<span class="hlt">wave</span> simulations (LWS) based on the numerical solution of the Navier-Stokes equations subject to the fully nonlinear free-surface boundary conditions and the appropriate bottom, inflow and outflow boundary conditions. The equations are properly transformed so that the computational domain becomes time-independent. In the present study, the case of incoming <span class="hlt">waves</span> with wavelength to inflow depth ratio λ/ d ~ 6.6 and <span class="hlt">wave</span> steepness H/ λ ~0.025, over bed of slope tan β = 1/35, is investigated. The LWS predicts satisfactorily breaking parameters - height and depth - and <span class="hlt">wave</span> dissipation in the surf <span class="hlt">zone</span>, in comparison to experimental data. In the corresponding LES, breaking height and depth are smaller and <span class="hlt">wave</span> dissipation in the surf <span class="hlt">zone</span> is weaker. For the undertow current, it is found that it is induced by the breaking process at the free surface, while its strength is controlled by the bed shear stress. Finally, the amplitude of the bed shear stress increases substantially in the breaking <span class="hlt">zone</span>, becoming up to six times larger than the respective amplitude at the outer region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T31E2970Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T31E2970Z"><span>Mapping seismic azimuthal anisotropy of the Japan subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, D.; Liu, X.</p> <p>2016-12-01</p> <p>We present 3-D images of azimuthal anisotropy tomography of the crust and upper mantle of the Japan subduction <span class="hlt">zone</span>, which are determined using a large number of high-quality P- and S-<span class="hlt">wave</span> arrival-time data of local earthquakes and teleseismic events recorded by the dense seismic networks on the Japan Islands. A tomographic method for P-<span class="hlt">wave</span> velocity azimuthal anisotropy is modified and extended to invert S-<span class="hlt">wave</span> travel times for 3-D S-<span class="hlt">wave</span> velocity azimuthal anisotropy. A joint inversion of the P and S <span class="hlt">wave</span> data is conducted to constrain the 3-D azimuthal anisotropy of the Japan subduction <span class="hlt">zone</span>. Main findings of this work are summarized as follows. (1) The high-velocity subducting Pacific and Philippine Sea (PHS) slabs exhibit trench-parallel fast-velocity directions (FVDs), which may reflect frozen-in lattice-preferred orientation of aligned anisotropic minerals formed at the mid-ocean ridge as well as shape-preferred orientation such as normal faults produced at the outer-rise area near the trench axis. (2) Significant trench-normal FVDs are revealed in the mantle wedge, which reflects corner flow in the mantle wedge due to the active subduction and dehydration of the oceanic plates. (3) Obvious toroidal FVDs and low-velocity anomalies exist in and around a window (hole) in the aseismic PHS slab beneath Southwest Japan, which may reflect a toroidal mantle flow pattern resulting from hot and wet mantle upwelling caused by the joint effects of deep dehydration of the Pacific slab and the convective circulation process in the mantle wedge above the Pacific slab. (4) Significant low-velocity anomalies with trench-normal FVDs exist in the mantle below the Pacific slab beneath Northeast Japan, which may reflect a subducting oceanic asthenosphere affected by hot mantle upwelling from the deeper mantle. ReferencesLiu, X., D. Zhao (2016) Seismic velocity azimuthal anisotropy of the Japan subduction <span class="hlt">zone</span>: Constraints from P and S <span class="hlt">wave</span> traveltimes. J. Geophys. Res. 121, doi</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E.555E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E.555E"><span>Long-Term Observation of Small and Medium-Scale Gravity <span class="hlt">Waves</span> over the Brazilian Equatorial Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Essien, Patrick; Buriti, Ricardo; Wrasse, Cristiano M.; Medeiros, Amauri; Paulino, Igo; Takahashi, Hisao; Campos, Jose Andre</p> <p>2016-07-01</p> <p>This paper reports the long term observations of small and medium-scale gravity <span class="hlt">waves</span> over Brazilian equatorial region. Coordinated optical and radio measurements were made from OLAP at Sao Joao do Cariri (7.400S, 36.500W) to investigate the occurrences and properties and to characterize the regional mesospheric gravity <span class="hlt">wave</span> field. All-sky imager measurements were made from the site. for almost 11 consecutive years (September 2000 to November 2010). Most of the <span class="hlt">waves</span> propagated were characterized as small-scale gravity. The characteristics of the two <span class="hlt">waves</span> events agreed well with previous gravity <span class="hlt">wave</span> studies from Brazil and other sites. However, significant differences in the <span class="hlt">wave</span> propagation <span class="hlt">headings</span> indicate dissimilar source regions. The observed medium-scale gravity <span class="hlt">wave</span> events constitute an important new dataset to study their mesospheric properties at equatorial latitudes. These data exhibited similar propagation <span class="hlt">headings</span> to the short period events, suggesting they originated from the same source regions. It was also observed that some of the medium-scale were capable of propagating into the lower thermosphere where they may have acted directly as seeds for the Rayleigh-Taylor instability development. The <span class="hlt">wave</span> events were primarily generated by meteorological processes since there was no correlation between the evolution of the <span class="hlt">wave</span> events and solar cycle F10.7.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6285T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6285T"><span>Rayleigh-<span class="hlt">Wave</span> Group-Velocity Tomography of Saudi Arabia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tang, Zheng; Mai, P. Martin; Chang, Sung-Joon; Zahran, Hani</p> <p>2017-04-01</p> <p>We use surface-<span class="hlt">wave</span> tomography to investigate the lithospheric structure of the Arabian plate, which is traditionally divided into the Arabian shield in the west and the Arabian platform in the east. The Arabian shield is a complicated mélange of crustal material, composed of several Proterozoic terrains separated by ophiolite-bearing suture <span class="hlt">zones</span> and dotted by outcropping Cenozoic volcanic rocks. The Arabian platform is primarily covered by very thick Paleozoic, Mesozoic and Cenozoic sediments. We develop high-resolution tomographic images from fundamental-mode Rayleigh-<span class="hlt">wave</span> group-velocities across Saudi Arabia, utilizing the teleseismic data recorded by the permanent Saudi National Seismic Network (SNSN). Our study extends previous efforts on surface <span class="hlt">wave</span> work by increasing ray path density and improving spatial resolution. Good quality dispersion measurements for roughly 3000 Rayleigh-<span class="hlt">wave</span> paths have been obtained and utilized for the group-velocity tomography. We have applied the Fast Marching Surface Tomography (FMST) scheme of Rawlinson (2005) to obtain Rayleigh-<span class="hlt">wave</span> group-velocity images for periods from 8 s to 40 s on a 0.8° 0.8° grid and at resolutions approaching 2.5° based on the checkerboard tests. Our results indicate that short-period group-velocity maps (8-15 s) correlate well with surface geology, with slow velocities delineating the main sedimentary features including the Arabian platform, the Persian Gulf and Mesopotamia. For longer periods (20-40 s), the velocity contrast is due to the differences in crustal thickness and subduction/collision <span class="hlt">zones</span>. The lower velocities are sensitive to the thicker continental crust beneath the eastern Arabia and the subduction/collision <span class="hlt">zones</span> between the Arabian and Eurasian plate, while the higher velocities in the west infer mantle velocity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25493863','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25493863"><span>Multicomponent long-<span class="hlt">wave-short-wave</span> resonance interaction system: Bright solitons, energy-sharing collisions, and resonant solitons.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sakkaravarthi, K; Kanna, T; Vijayajayanthi, M; Lakshmanan, M</p> <p>2014-11-01</p> <p>We consider a general multicomponent (2+1)-dimensional long-<span class="hlt">wave-short-wave</span> resonance interaction (LSRI) system with arbitrary nonlinearity coefficients, which describes the nonlinear resonance interaction of multiple short <span class="hlt">waves</span> with a long <span class="hlt">wave</span> in two spatial dimensions. The general multicomponent LSRI system is shown to be integrable by performing the Painlevé analysis. Then we construct the exact bright multisoliton solutions by applying the Hirota's bilinearization method and study the propagation and collision dynamics of bright solitons in detail. Particularly, we investigate the <span class="hlt">head</span>-on and overtaking collisions of bright solitons and explore two types of energy-sharing collisions as well as standard elastic collision. We have also corroborated the obtained analytical one-soliton solution by direct numerical simulation. Also, we discuss the formation and dynamics of resonant solitons. Interestingly, we demonstrate the formation of resonant solitons admitting breather-like (localized periodic pulse train) structure and also large amplitude localized structures akin to rogue <span class="hlt">waves</span> coexisting with solitons. For completeness, we have also obtained dark one- and two-soliton solutions and studied their dynamics briefly.</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('https://www.ncbi.nlm.nih.gov/pubmed/12460476','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12460476"><span>Mantle shear-<span class="hlt">wave</span> tomography and the fate of subducted slabs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Grand, Steven P</p> <p>2002-11-15</p> <p>A new seismic model of the three-dimensional variation in shear velocity throughout the Earth's mantle is presented. The model is derived entirely from shear bodywave travel times. Multibounce shear <span class="hlt">waves</span>, core-reflected <span class="hlt">waves</span> and SKS and SKKS <span class="hlt">waves</span> that travel through the core are used in the analysis. A unique aspect of the dataset used in this study is the use of bodywaves that turn at shallow depths in the mantle, some of which are triplicated. The new model is compared with other global shear models. Although competing models show significant variations, several large-scale structures are common to most of the models. The high-velocity anomalies are mostly associated with subduction <span class="hlt">zones</span>. In some regions the anomalies only extend into the shallow lower mantle, whereas in other regions tabular high-velocity structures seem to extend to the deepest mantle. The base of the mantle shows long-wavelength high-velocity <span class="hlt">zones</span> also associated with subduction <span class="hlt">zones</span>. The heterogeneity seen in global tomography models is difficult to interpret in terms of mantle flow due to variations in structure from one subduction <span class="hlt">zone</span> to another. The simplest interpretation of the seismic images is that slabs in general penetrate to the deepest mantle, although the flow is likely to be sporadic. The interruption in slab sinking is likely to be associated with the 660 km discontinuity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B21A0007J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B21A0007J"><span>Elastic <span class="hlt">Wave</span> Imaging of in-Situ Bio-Alterations in a Contaminated Aquifer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jaiswal, P.; Raj, R.; Atekwana, E. A.; Briand, B.; Alam, I.</p> <p>2014-12-01</p> <p>We present a pioneering report on the utility of seismic methods in imaging bio-induced elastic property changes within a contaminated aquifer. To understand physical properties of contaminated soil, we acquired 48 meters long multichannel seismic profile over the Norman landfill leachate plume in Norman Oklahoma, USA. We estimated both the P- and S- <span class="hlt">wave</span> velocities respectively using full-waveform inversion of the transmission and the ground-roll coda. The resulting S-<span class="hlt">wave</span> model showed distinct velocity anomaly (~10% over background) within the water table fluctuation <span class="hlt">zone</span> bounded by the historical minimum and maximum groundwater table. In comparison, the P-<span class="hlt">wave</span> velocity anomaly within the same <span class="hlt">zone</span> was negligible. The Environmental Scanning Electron Microscope (ESEM) images of samples from a core located along the seismic profile clearly shows presence of biofilms in the water table fluctuation <span class="hlt">zone</span> and their absence both above and below the fluctuation <span class="hlt">zone</span>. Elemental chemistry further indicates that the sediment composition throughout the core is fairly constant. We conclude that the velocity anomaly in S-<span class="hlt">wave</span> is due to biofilms. As a next step, we develop mechanistic modeling to gain insights into the petro-physical behavior of biofilm-bearing sediments. Preliminary results suggest that a plausible model could be biofilms acting as contact cement between sediment grains. The biofilm cement can be placed in two ways - (i) superficial non-contact deposition on sediment grains, and (ii) deposition at grain contacts. Both models explain P- and S- <span class="hlt">wave</span> velocity structure at reasonable (~5-10%) biofilm saturation and are equivocally supported by the ESEM images. Ongoing attenuation modeling from full-waveform inversion and its mechanistic realization, may be able to further discriminate between the two cement models. Our study strongly suggests that as opposed to the traditional P-<span class="hlt">wave</span> seismic, S-<span class="hlt">wave</span> acquisition and imaging can be a more powerful tool for in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.2293B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.2293B"><span><span class="hlt">Wave</span> Attenuation and Gas Exchange Velocity in Marginal Sea Ice <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bigdeli, A.; Hara, T.; Loose, B.; Nguyen, A. T.</p> <p>2018-03-01</p> <p>The gas transfer velocity in marginal sea ice <span class="hlt">zones</span> exerts a strong control on the input of anthropogenic gases into the ocean interior. In this study, a sea state-dependent gas exchange parametric model is developed based on the turbulent kinetic energy dissipation rate. The model is tuned to match the conventional gas exchange parametrization in fetch-unlimited, fully developed seas. Next, fetch limitation is introduced in the model and results are compared to fetch limited experiments in lakes, showing that the model captures the effects of finite fetch on gas exchange with good fidelity. Having validated the results in fetch limited waters such as lakes, the model is next applied in sea ice <span class="hlt">zones</span> using an empirical relation between the sea ice cover and the effective fetch, while accounting for the sea ice motion effect that is unique to sea ice <span class="hlt">zones</span>. The model results compare favorably with the available field measurements. Applying this parametric model to a regional Arctic numerical model, it is shown that, under the present conditions, gas flux into the Arctic Ocean may be overestimated by 10% if a conventional parameterization is used.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GGG....16.2949C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GGG....16.2949C"><span>Multiple mantle upwellings in the transition <span class="hlt">zone</span> beneath the northern East-African Rift system from relative P-<span class="hlt">wave</span> travel-time tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Civiero, Chiara; Hammond, James O. S.; Goes, Saskia; Fishwick, Stewart; Ahmed, Abdulhakim; Ayele, Atalay; Doubre, Cecile; Goitom, Berhe; Keir, Derek; Kendall, J.-Michael; Leroy, Sylvie; Ogubazghi, Ghebrebrhan; Rümpker, Georg; Stuart, Graham W.</p> <p>2015-09-01</p> <p>Mantle plumes and consequent plate extension have been invoked as the likely cause of East African Rift volcanism. However, the nature of mantle upwelling is debated, with proposed configurations ranging from a single broad plume connected to the large low-shear-velocity province beneath Southern Africa, the so-called African Superplume, to multiple lower-mantle sources along the rift. We present a new P-<span class="hlt">wave</span> travel-time tomography model below the northern East-African, Red Sea, and Gulf of Aden rifts and surrounding areas. Data are from stations that span an area from Madagascar to Saudi Arabia. The aperture of the integrated data set allows us to image structures of ˜100 km length-scale down to depths of 700-800 km beneath the study region. Our images provide evidence of two clusters of low-velocity structures consisting of features with diameter of 100-200 km that extend through the transition <span class="hlt">zone</span>, the first beneath Afar and a second just west of the Main Ethiopian Rift, a region with off-rift volcanism. Considering seismic sensitivity to temperature, we interpret these features as upwellings with excess temperatures of 100 ± 50 K. The scale of the upwellings is smaller than expected for lower mantle plume sources. This, together with the change in pattern of the low-velocity anomalies across the base of the transition <span class="hlt">zone</span>, suggests that ponding or flow of deep-plume material below the transition <span class="hlt">zone</span> may be spawning these upper mantle upwellings. This article was corrected on 28 SEP 2015. See the end of the full text for details.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhRvL.109d6801A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhRvL.109d6801A"><span>Phonon Self-Energy Corrections to Nonzero <span class="hlt">Wave</span>-Vector Phonon Modes in Single-Layer Graphene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Araujo, P. T.; Mafra, D. L.; Sato, K.; Saito, R.; Kong, J.; Dresselhaus, M. S.</p> <p>2012-07-01</p> <p>Phonon self-energy corrections have mostly been studied theoretically and experimentally for phonon modes with <span class="hlt">zone</span>-center (q=0) <span class="hlt">wave</span> vectors. Here, gate-modulated Raman scattering is used to study phonons of a single layer of graphene originating from a double-resonant Raman process with q≠0. The observed phonon renormalization effects are different from what is observed for the <span class="hlt">zone</span>-center q=0 case. To explain our experimental findings, we explored the phonon self-energy for the phonons with nonzero <span class="hlt">wave</span> vectors (q≠0) in single-layer graphene in which the frequencies and decay widths are expected to behave oppositely to the behavior observed in the corresponding <span class="hlt">zone</span>-center q=0 processes. Within this framework, we resolve the identification of the phonon modes contributing to the G⋆ Raman feature at 2450cm-1 to include the iTO+LA combination modes with q≠0 and also the 2iTO overtone modes with q=0, showing both to be associated with <span class="hlt">wave</span> vectors near the high symmetry point K in the Brillouin <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28005956','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28005956"><span>The Intelligent Control System and Experiments for an Unmanned <span class="hlt">Wave</span> Glider.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liao, Yulei; Wang, Leifeng; Li, Yiming; Li, Ye; Jiang, Quanquan</p> <p>2016-01-01</p> <p>The control system designing of Unmanned <span class="hlt">Wave</span> Glider (UWG) is challenging since the control system is weak maneuvering, large time-lag and large disturbance, which is difficult to establish accurate mathematical model. Meanwhile, to complete marine environment monitoring in long time scale and large spatial scale autonomously, UWG asks high requirements of intelligence and reliability. This paper focuses on the "Ocean Rambler" UWG. First, the intelligent control system architecture is designed based on the cerebrum basic function combination <span class="hlt">zone</span> theory and hierarchic control method. The hardware and software designing of the embedded motion control system are mainly discussed. A motion control system based on rational behavior model of four layers is proposed. Then, combining with the line-of sight method(LOS), a self-adapting PID guidance law is proposed to compensate the steady state error in path following of UWG caused by marine environment disturbance especially current. Based on S-surface control method, an improved S-surface <span class="hlt">heading</span> controller is proposed to solve the <span class="hlt">heading</span> control problem of the weak maneuvering carrier under large disturbance. Finally, the simulation experiments were carried out and the UWG completed autonomous path following and marine environment monitoring in sea trials. The simulation experiments and sea trial results prove that the proposed intelligent control system, guidance law, controller have favorable control performance, and the feasibility and reliability of the designed intelligent control system of UWG are verified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5179121','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5179121"><span>The Intelligent Control System and Experiments for an Unmanned <span class="hlt">Wave</span> Glider</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Liao, Yulei; Wang, Leifeng; Li, Yiming; Li, Ye; Jiang, Quanquan</p> <p>2016-01-01</p> <p>The control system designing of Unmanned <span class="hlt">Wave</span> Glider (UWG) is challenging since the control system is weak maneuvering, large time-lag and large disturbance, which is difficult to establish accurate mathematical model. Meanwhile, to complete marine environment monitoring in long time scale and large spatial scale autonomously, UWG asks high requirements of intelligence and reliability. This paper focuses on the “Ocean Rambler” UWG. First, the intelligent control system architecture is designed based on the cerebrum basic function combination <span class="hlt">zone</span> theory and hierarchic control method. The hardware and software designing of the embedded motion control system are mainly discussed. A motion control system based on rational behavior model of four layers is proposed. Then, combining with the line-of sight method(LOS), a self-adapting PID guidance law is proposed to compensate the steady state error in path following of UWG caused by marine environment disturbance especially current. Based on S-surface control method, an improved S-surface <span class="hlt">heading</span> controller is proposed to solve the <span class="hlt">heading</span> control problem of the weak maneuvering carrier under large disturbance. Finally, the simulation experiments were carried out and the UWG completed autonomous path following and marine environment monitoring in sea trials. The simulation experiments and sea trial results prove that the proposed intelligent control system, guidance law, controller have favorable control performance, and the feasibility and reliability of the designed intelligent control system of UWG are verified. PMID:28005956</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24684377','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24684377"><span>The effects of exposure in sandy beach surf <span class="hlt">zones</span> on larval fishes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pattrick, P; Strydom, N A</p> <p>2014-05-01</p> <p>The influence of wind and <span class="hlt">wave</span> exposure on larval fish assemblages within a large bay system was investigated. Larval fishes were sampled from two areas with vastly different exposure to <span class="hlt">waves</span> and wind, namely the windward and leeward sectors of Algoa Bay. In total, 5702 larval fishes were collected using a modified larval seine. Of these, 4391 were collected in the leeward and 1311 in the windward sector of the bay, representing a total of 23 families and 57 species. Dominant fish families included Clinidae, Engraulidae, Kyphosidae, Mugilidae, Soleidae and Sparidae, similar to the situation elsewhere, highlighting continuity in the composition of larval fish assemblages and the utilization of surf <span class="hlt">zones</span> by a specific group of larval fishes. Nineteen estuary-associated marine species occurred within the surf <span class="hlt">zones</span> of Algoa Bay and dominated catches (86·7%) in terms of abundance. Postflexion larvae comprised > 80% of the catch, indicating the importance of the seemingly inhospitable surf <span class="hlt">zone</span> environment for the early life stages of many fish species. The greatest species diversity was observed within the windward sector of the bay. Distance-based linear modelling identified <span class="hlt">wave</span> period as the environmental variable explaining the largest proportion of the significant variation in the larval fish assemblage. The physical disturbance generated by breaking <span class="hlt">waves</span> could create a suitable environment for fish larvae, sheltered from predators and with an abundance of food resources. © 2014 The Fisheries Society of the British Isles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027765','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027765"><span>Numerical study of electromagnetic <span class="hlt">waves</span> generated by a prototype dielectric logging tool</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ellefsen, K.J.; Abraham, J.D.; Wright, D.L.; Mazzella, A.T.</p> <p>2004-01-01</p> <p>To understand the electromagnetic <span class="hlt">waves</span> generated by a prototype dielectric logging tool, a numerical study was conducted using both the finite-difference, time-domain method and a frequency-wavenumber method. When the propagation velocity in the borehole was greater than that in the formation (e.g., an air-filled borehole in the unsaturated <span class="hlt">zone</span>), only a guided <span class="hlt">wave</span> propagated along the borehole. As the frequency decreased, both the phase and the group velocities of the guided <span class="hlt">wave</span> asymptotically approached the phase velocity of a plane <span class="hlt">wave</span> in the formation. The guided <span class="hlt">wave</span> radiated electromagnetic energy into the formation, causing its amplitude to decrease. When the propagation velocity in the borehole was less than that in the formation (e.g., a water-filled borehole in the saturated <span class="hlt">zone</span>), both a refracted <span class="hlt">wave</span> and a guided <span class="hlt">wave</span> propagated along the borehole. The velocity of the refracted <span class="hlt">wave</span> equaled the phase velocity of a plane <span class="hlt">wave</span> in the formation, and the refracted <span class="hlt">wave</span> preceded the guided <span class="hlt">wave</span>. As the frequency decreased, both the phase and the group velocities of the guided <span class="hlt">wave</span> asymptotically approached the phase velocity of a plane <span class="hlt">wave</span> in the formation. The guided <span class="hlt">wave</span> did not radiate electromagnetic energy into the formation. To analyze traces recorded by the prototype tool during laboratory tests, they were compared to traces calculated with the finite-difference method. The first parts of both the recorded and the calculated traces were similar, indicating that guided and refracted <span class="hlt">waves</span> indeed propagated along the prototype tool. ?? 2004 Society of Exploration Geophysicists. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014OcMod..83...26L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014OcMod..83...26L"><span>Integration of coastal inundation modeling from storm tides to individual <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Ning; Roeber, Volker; Yamazaki, Yoshiki; Heitmann, Troy W.; Bai, Yefei; Cheung, Kwok Fai</p> <p>2014-11-01</p> <p>Modeling of storm-induced coastal inundation has primarily focused on the surge generated by atmospheric pressure and surface winds with phase-averaged effects of the <span class="hlt">waves</span> as setup. Through an interoperable model package, we investigate the role of phase-resolving <span class="hlt">wave</span> processes in simulation of coastal flood hazards. A spectral ocean <span class="hlt">wave</span> model describes generation and propagation of storm <span class="hlt">waves</span> from deep to intermediate water, while a non-hydrostatic storm-tide model has the option to couple with a spectral coastal <span class="hlt">wave</span> model for computation of phase-averaged processes in a near-shore region. The ocean <span class="hlt">wave</span> and storm-tide models can alternatively provide the <span class="hlt">wave</span> spectrum and the surface elevation as the boundary and initial conditions for a nested Boussinesq model. Additional surface-gradient terms in the Boussinesq equations maintain the quasi-steady, non-uniform storm tide for modeling of phase-resolving surf and swash-<span class="hlt">zone</span> processes as well as combined tide, surge, and <span class="hlt">wave</span> inundation. The two nesting schemes are demonstrated through a case study of Hurricane Iniki, which made landfall on the Hawaiian Island of Kauai in 1992. With input from a parametric hurricane model and global reanalysis and tidal datasets, the two approaches produce comparable significant <span class="hlt">wave</span> heights and phase-averaged surface elevations in the surf <span class="hlt">zone</span>. The nesting of the Boussinesq model provides a seamless approach to augment the inundation due to the individual <span class="hlt">waves</span> in matching the recorded debris line along the coast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.8695M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.8695M"><span>Formation of the chemical composition of water in channel <span class="hlt">head</span> in postglacial areas (West Pomerania, Poland)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mazurek, Małgorzata; Kruszyk, Robert; Szpikowska, Grażyna</p> <p>2016-04-01</p> <p>The channel <span class="hlt">head</span> is a <span class="hlt">zone</span> of hydrological changes determining the hydrochemical features of water in the final stage of groundwater flow and the start of the surface cycle. The chemistry of water flowing out of a channel <span class="hlt">head</span> reflects not only the characteristics of groundwater feeding the <span class="hlt">zone</span>, but also changes it undergoes in this area during the organisation of channel flow. Groundwater interacts with surface water in the hyporheic <span class="hlt">zone</span> where water from different environments is mixed and exchanged due to high hydraulic and chemical gradients. The goal of this study was to assess spatial differences in the concentrations of nutrients and compounds produced by chemical weathering in a channel <span class="hlt">head</span> and to establish the role of the hyporheic <span class="hlt">zone</span> in the transformation of the chemical composition of groundwater supplying a 1st-order stream. The research area was the channel <span class="hlt">head</span> Żarnowo, located on the southern slope of the upper Parsęta valley. Three hydrochemical mappings were conducted in the headwater alcove consisting of three parts developed in a glaciofluvial plain and an erosional-accumulative alluvial terrace. Water was sampled in places of groundwater outflow in the footslope <span class="hlt">zone</span> (9 sites), the hyporheic <span class="hlt">zone</span> (14 sites), and outflows in the individual alcove parts and the rivulet they formed (5 sites). Water temperature, pH, and electrical conductivity were measured in the field. Concentrations of K, Ca, Mg, Na, Fe, Mn, HCO3, Cl, NO3, PO4, SO4 and SiO2 were determined in the laboratory. The chemical composition of ground- and surface water shows the concentration of geogenic components like K, Ca, Mg, Na, HCO3, and SiO2 to be an effect of chemical weathering and the leaching of its products taking place in a zero-discharge catchment. Those ions display little spatial variability and a stability of concentration in individual measurement periods, while the greatest disproportions in their concentrations among the alcove parts were recorded for Cl, NO3</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70013147','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70013147"><span>ON PREDICTING INFRAGRAVITY ENERGY IN THE SURF <span class="hlt">ZONE</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>Sallenger,, Asbury H.; Holman, Robert A.; Edge, Billy L.</p> <p>1985-01-01</p> <p>Flow data were obtained in the surf <span class="hlt">zone</span> across a barred profile during a storm. RMS cross-shore velocities due to <span class="hlt">waves</span> in the intragravity band (<span class="hlt">wave</span> periods greater than 20 s) had maxima in excess of 0. 5 m/s over the bar crest. For comparison to measured spectra, synthetic spectra of cross-shore flow were computed using measured nearshore profiles. The structure, in the infragravity band, of these synthetic spectra corresponded reasonably well with the structure of the measured spectra. Total variances of measured cross-shore flow within the infragravity band were nondimensionalized by dividing by total infragravity variances of synthetic spectra. These nondimensional variances were independent of distance offshore and increased with the square of the breaker height. Thus, cross-shore flow due to infragravity <span class="hlt">waves</span> can be estimated with knowledge of the nearshore profile and incident <span class="hlt">wave</span> conditions. Refs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23407781','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23407781"><span>Characterization of the <span class="hlt">head</span>-twitch response induced by hallucinogens in mice: detection of the behavior based on the dynamics of <span class="hlt">head</span> movement.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Halberstadt, Adam L; Geyer, Mark A</p> <p>2013-06-01</p> <p>The <span class="hlt">head</span>-twitch response (HTR) is a rapid side-to-side rotational <span class="hlt">head</span> movement that occurs in rats and mice after administration of serotonergic hallucinogens and other 5-HT2A agonists. The HTR is widely used as a behavioral assay for 5-HT2A activation and to probe for interactions between the 5-HT2A receptor and other transmitter systems. High-speed video recordings were used to analyze the <span class="hlt">head</span> movement that occurs during <span class="hlt">head</span> twitches in C57BL/6J mice. Experiments were also conducted in C57BL/6J mice to determine whether a <span class="hlt">head</span>-mounted magnet and a magnetometer coil could be used to detect the HTR induced by serotonergic hallucinations based on the dynamics of the response. <span class="hlt">Head</span> movement during the HTR was highly rhythmic and occurred within a specific frequency range (mean <span class="hlt">head</span> movement frequency of 90.3 Hz). <span class="hlt">Head</span> twitches produced <span class="hlt">wave</span>-like oscillations of magnetometer coil voltage that matched the frequency of <span class="hlt">head</span> movement during the response. The magnetometer coil detected the HTR induced by the serotonergic hallucinogens 2,5-dimethoxy-4-iodoamphetamine (DOI; 0.25, 0.5, and 1.0 mg/kg, i.p.) and lysergic acid diethylamide (LSD; 0.05, 0.1, 0.2, and 0.4 mg/kg, i.p.) with extremely high sensitivity and specificity. Magnetometer coil recordings demonstrated that the non-hallucinogenic compounds (+)-amphetamine (2.5 and 5.0 mg/kg, i.p.) and lisuride (0.8, 1.6, and 3.2 mg/kg, i.p.) did not induce the HTR. These studies confirm that a magnetometer coil can be used to detect the HTR induced by hallucinogens. The use of magnetometer-based HTR detection provides a high-throughput, semi-automated assay for this behavior, and offers several advantages over traditional assessment methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996JPhD...29..369B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996JPhD...29..369B"><span>Pulsed discharges produced by high-power surface <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Böhle, A.; Ivanov, O.; Kolisko, A.; Kortshagen, U.; Schlüter, H.; Vikharev, A.</p> <p>1996-02-01</p> <p>The mechanisms of the ionization front advance in surface-<span class="hlt">wave</span>-produced discharges are investigated using two experimental set-ups. The high-power surface <span class="hlt">waves</span> are excited in a 3 cm wavelength band by a surfaguide and a novel type of launcher (an E-plane junction). The ionization front velocity of the surface <span class="hlt">wave</span> is measured for a wide range of gas pressures, incident microwave power and initial pre-ionization. The experimental results are compared with theoretical ones based on three different models. The comparison between theory and experiment allows one to suggest a new interpretation of the ionization front's advance. The ionization front velocity is determined by a breakdown <span class="hlt">wave</span> or an ionization <span class="hlt">wave</span> in the electric field of a high-power surface <span class="hlt">wave</span> in the <span class="hlt">zone</span> near the ionization front.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027083','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027083"><span>Delineation of a collapse feature in a noisy environment using a multichannel surface <span class="hlt">wave</span> technique</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Xia, J.; Chen, C.; Li, P.H.; Lewis, M.J.</p> <p>2004-01-01</p> <p>A collapse developed at Calvert Cliffs Nuclear Power Plant, Maryland, in early 2001. The location of the collapse was over a groundwater drainage system pipe buried at an elevation of +0??9 m (reference is to Chesapeake Bay level). The cause of the collapse was a subsurface drain pipe that collapsed because of saltwater corrosion of the corrugated metal pipe. The inflow/outflow of sea water and groundwater flow caused soil to be removed from the area where the pipe collapsed. To prevent damage to nearby structures, the collapse was quickly filled with uncompacted sand and gravel (???36000 kg). However, the plant had an immediate need to determine whether more underground voids existed. A high-frequency multichannel surface-<span class="hlt">wave</span> survey technique was conducted to define the <span class="hlt">zone</span> affected by the collapse. Although the surface-<span class="hlt">wave</span> survey at Calvert Cliffs Nuclear Power Plant was conducted at a noise level 50-100 times higher than the normal environment for a shallow seismic survey, the shear (S)-<span class="hlt">wave</span> velocity field calculated from surface-<span class="hlt">wave</span> data delineated a possible <span class="hlt">zone</span> affected by the collapse. The S-<span class="hlt">wave</span> velocity field showed chimney-shaped low-velocity anomalies that were directly related to the collapse. Based on S-<span class="hlt">wave</span> velocity field maps, a potential <span class="hlt">zone</span> affected by the collapse was tentatively defined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26010363','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26010363"><span>The vertical monitor position for presbyopic computer users with progressive lenses: how to reach clear vision and comfortable <span class="hlt">head</span> posture.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Weidling, Patrick; Jaschinski, Wolfgang</p> <p>2015-01-01</p> <p>When presbyopic employees are wearing general-purpose progressive lenses, they have clear vision only with a lower gaze inclination to the computer monitor, given the <span class="hlt">head</span> assumes a comfortable inclination. Therefore, in the present intervention field study the monitor position was lowered, also with the aim to reduce musculoskeletal symptoms. A comparison group comprised users of lenses that do not restrict the field of clear vision. The lower monitor positions led the participants to lower their <span class="hlt">head</span> inclination, which was linearly associated with a significant reduction in musculoskeletal symptoms. However, for progressive lenses a lower <span class="hlt">head</span> inclination means a lower <span class="hlt">zone</span> of clear vision, so that clear vision of the complete monitor was not achieved, rather the monitor should have been placed even lower. The procedures of this study may be useful for optimising the individual monitor position depending on the comfortable <span class="hlt">head</span> and gaze inclination and the vertical <span class="hlt">zone</span> of clear vision of progressive lenses. For users of general-purpose progressive lenses, it is suggested that low monitor positions allow for clear vision at the monitor and for a physiologically favourable <span class="hlt">head</span> inclination. Employees may improve their workplace using a flyer providing ergonomic-optometric information.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MSPE...24..247B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MSPE...24..247B"><span>Determination of the <span class="hlt">Zone</span> Endangered by Methane Explosion in Goaf with Caving of Longwalls Ventilated on "Y" System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brodny, Jarosław; Tutak, Magdalena</p> <p>2016-12-01</p> <p>One of the most dangerous and most commonly present risks in hard coal mines is methane hazard. During exploitation by longwall system with caving, methane is emitted to mine <span class="hlt">heading</span> from the mined coal and coal left in a pile. A large amount of methane also flows from neighboring seams through cracks and fissures formed in rock mass. In a case of accumulation of explosive methane concentration in goaf <span class="hlt">zone</span> and with appropriate oxygen concentration and occurrence of initials (e.g. spark or endogenous fire), it may come to the explosion of this gas. In the paper there are presented results of numerical analysis of mixture of air and methane streams flow through the real <span class="hlt">heading</span> system of a mine, characterized by high methane hazard. The aim of the studies was to analyze the ventilation system of considered <span class="hlt">heading</span> system and determination of braking <span class="hlt">zones</span> in goaf <span class="hlt">zone</span>, in which dangerous and explosive concertation of methane can occur with sufficient oxygen concentration equal to at least 12%. Determination of position of these <span class="hlt">zones</span> is necessary for the selection of appropriate parameters of the ventilation system to ensure safety of the crew. Analysis of the scale of methane hazard allows to select such a ventilation system of exploitation and neighboring <span class="hlt">headings</span> that ensures chemical composition of mining atmosphere required by regulation, and required efficiency of methane drainage. The obtained results clearly show that numerical methods, combined with the results of tests in real conditions can be successfully used for the analysis of variants of processes related to ventilation of underground mining, and also in the analysis of emergency states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JHyd..561..223M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JHyd..561..223M"><span>3D mapping, hydrodynamics and modelling of the freshwater-brine mixing <span class="hlt">zone</span> in salt flats similar to the Salar de Atacama (Chile)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marazuela, M. A.; Vázquez-Suñé, E.; Custodio, E.; Palma, T.; García-Gil, A.; Ayora, C.</p> <p>2018-06-01</p> <p>Salt flat brines are a major source of minerals and especially lithium. Moreover, valuable wetlands with delicate ecologies are also commonly present at the margins of salt flats. Therefore, the efficient and sustainable exploitation of the brines they contain requires detailed knowledge about the hydrogeology of the system. A critical issue is the freshwater-brine mixing <span class="hlt">zone</span>, which develops as a result of the mass balance between the recharged freshwater and the evaporating brine. The complex processes occurring in salt flats require a three-dimensional (3D) approach to assess the mixing <span class="hlt">zone</span> geometry. In this study, a 3D map of the mixing <span class="hlt">zone</span> in a salt flat is presented, using the Salar de Atacama as an example. This mapping procedure is proposed as the basis of computationally efficient three-dimensional numerical models, provided that the hydraulic <span class="hlt">heads</span> of freshwater and mixed waters are corrected based on their density variations to convert them into brine <span class="hlt">heads</span>. After this correction, the locations of lagoons and wetlands that are characteristic of the marginal <span class="hlt">zones</span> of the salt flats coincide with the regional minimum water (brine) <span class="hlt">heads</span>. The different morphologies of the mixing <span class="hlt">zone</span> resulting from this 3D mapping have been interpreted using a two-dimensional (2D) flow and transport numerical model of an idealized cross-section of the mixing <span class="hlt">zone</span>. The result of the model shows a slope of the mixing <span class="hlt">zone</span> that is similar to that obtained by 3D mapping and lower than in previous models. To explain this geometry, the 2D model was used to evaluate the effects of heterogeneity in the mixing <span class="hlt">zone</span> geometry. The higher the permeability of the upper aquifer is, the lower the slope and the shallower the mixing <span class="hlt">zone</span> become. This occurs because most of the freshwater lateral recharge flows through the upper aquifer due to its much higher transmissivity, thus reducing the freshwater <span class="hlt">head</span>. The presence of a few meters of highly permeable materials in the upper part of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.T41E..05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.T41E..05D"><span>Geometry and velocity structure of the northern Costa Rica seismogenic <span class="hlt">zone</span> from 3D local earthquake tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deshon, H. R.; Schwartz, S. Y.; Newman, A. V.; Dorman, L. M.; Protti, M.; Gonzalez, V.</p> <p>2003-12-01</p> <p>We present results of a 3D local earthquake tomography study of the Middle America Trench seismogenic <span class="hlt">zone</span> in northern Costa Rica. Local earthquake tomography can provide constraints on the updip, downdip, and lateral variability of seismicity and P- and S-<span class="hlt">wave</span> velocities; these constraints may in turn provide information on compositional and/or mechanical variability along the seismogenic <span class="hlt">zone</span>. We use arrival time data recorded by the Nicoya Peninsula seismic array, part of the Costa Rica seismogenic <span class="hlt">zone</span> experiment (CRSEIZE), a collaborative effort undertaken to better understand seismogenic behavior at the Costa Rica subduction <span class="hlt">zone</span> using data from land and ocean bottom seismic arrays, oceanic fluid flux meters, and GPS receivers. We invert ˜10,000 P-<span class="hlt">wave</span> and S-<span class="hlt">wave</span> arrival times from 475 well-recorded local earthquakes (GAP < 180° , >8 P-<span class="hlt">wave</span> arrivals) to solve for the best-fitting 1D P- and S-<span class="hlt">wave</span> velocity models, station corrections, and hypocenters using the algorithm VELEST. These 1D velocity models are used as a starting models for 3D simultaneous inversion using the algorithm SIMULPS14. Preliminary P-<span class="hlt">wave</span> inversions contain a positive velocity anomaly dipping beneath the Nicoya Peninsula, interpreted as the subducting Cocos Plate. Earthquakes occur in a narrow band along the slab-continent interface and are consistent with the results of Newman et al. (2002). The updip limit of seismicity occurs ˜5 km deeper and 5-10 km landward in the northern vs. the southern Nicoya Peninsula, and this shift spatially correlates to the change from Cocos-Nazca to East Pacific Rise derived oceanic plate. P-<span class="hlt">wave</span> velocities in the upper 5-10 km of the model are consistent with the geology of the Nicoya Peninsula. We will correlate relocated microseismicity to previously noted variability in oceanic plate morphology, heat flow, fluid flow, and thermal structure and compare the resulting P- and S-<span class="hlt">wave</span> velocity models to wide-angle refraction models and hypothesized mantle</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JGRB..114.4403H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JGRB..114.4403H"><span>Can compliant fault <span class="hlt">zones</span> be used to measure absolute stresses in the upper crust?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hearn, E. H.; Fialko, Y.</p> <p>2009-04-01</p> <p>Geodetic and seismic observations reveal long-lived <span class="hlt">zones</span> with reduced elastic moduli along active crustal faults. These fault <span class="hlt">zones</span> localize strain from nearby earthquakes, consistent with the response of a compliant, elastic layer. Fault <span class="hlt">zone</span> trapped <span class="hlt">wave</span> studies documented a small reduction in P and S <span class="hlt">wave</span> velocities along the Johnson Valley Fault caused by the 1999 Hector Mine earthquake. This reduction presumably perturbed a permanent compliant structure associated with the fault. The inferred changes in the fault <span class="hlt">zone</span> compliance may produce a measurable deformation in response to background (tectonic) stresses. This deformation should have the same sense as the background stress, rather than the coseismic stress change. Here we investigate how the observed deformation of compliant <span class="hlt">zones</span> in the Mojave Desert can be used to constrain the fault <span class="hlt">zone</span> structure and stresses in the upper crust. We find that gravitational contraction of the coseismically softened <span class="hlt">zones</span> should cause centimeters of coseismic subsidence of both the compliant <span class="hlt">zones</span> and the surrounding region, unless the compliant fault <span class="hlt">zones</span> are shallow and narrow, or essentially incompressible. We prefer the latter interpretation because profiles of line of sight displacements across compliant <span class="hlt">zones</span> cannot be fit by a narrow, shallow compliant <span class="hlt">zone</span>. Strain of the Camp Rock and Pinto Mountain fault <span class="hlt">zones</span> during the Hector Mine and Landers earthquakes suggests that background deviatoric stresses are broadly consistent with Mohr-Coulomb theory in the Mojave upper crust (with μ ≥ 0.7). Large uncertainties in Mojave compliant <span class="hlt">zone</span> properties and geometry preclude more precise estimates of crustal stresses in this region. With improved imaging of the geometry and elastic properties of compliant <span class="hlt">zones</span>, and with precise measurements of their strain in response to future earthquakes, the modeling approach we describe here may eventually provide robust estimates of absolute crustal stress.</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://ntrs.nasa.gov/search.jsp?R=20010059296&hterms=components+medium+environment&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcomponents%2Bmedium%2Benvironment','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010059296&hterms=components+medium+environment&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcomponents%2Bmedium%2Benvironment"><span>Diffusion Driven Combustion <span class="hlt">Waves</span> in Porous Media</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aldushin, A. P.; Matkowsky, B. J.</p> <p>2000-01-01</p> <p>Filtration of gas containing oxidizer, to the reaction <span class="hlt">zone</span> in a porous medium, due, e.g., to a buoyancy force or to an external pressure gradient, leads to the propagation of Filtration combustion (FC) <span class="hlt">waves</span>. The exothermic reaction occurs between the fuel component of the solid matrix and the oxidizer. In this paper, we analyze the ability of a reaction <span class="hlt">wave</span> to propagate in a porous medium without the aid of filtration. We find that one possible mechanism of propagation is that the <span class="hlt">wave</span> is driven by diffusion of oxidizer from the environment. The solution of the combustion problem describing diffusion driven <span class="hlt">waves</span> is similar to the solution of the Stefan problem describing the propagation of phase transition <span class="hlt">waves</span>, in that the temperature on the interface between the burned and unburned regions is constant, the combustion <span class="hlt">wave</span> is described by a similarity solution which is a function of the similarity variable x/square root of(t) and the <span class="hlt">wave</span> velocity decays as 1/square root of(t). The difference between the two problems is that in the combustion problem the temperature is not prescribed, but rather, is determined as part of the solution. We will show that the length of samples in which such self-sustained combustion <span class="hlt">waves</span> can occur, must exceed a critical value which strongly depends on the combustion temperature T(sub b). Smaller values of T(sub b) require longer sample lengths for diffusion driven combustion <span class="hlt">waves</span> to exist. Because of their relatively small velocity, diffusion driven <span class="hlt">waves</span> are considered to be relevant for the case of low heat losses, which occur for large diameter samples or in microgravity conditions, Another possible mechanism of porous medium combustion describes <span class="hlt">waves</span> which propagate by consuming the oxidizer initially stored in the pores of the sample. This occurs for abnormally high pressure and gas density. In this case, uniformly propagating planar <span class="hlt">waves</span>, which are kinetically controlled, can propagate, Diffusion of oxidizer decreases</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMEP53D1009M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMEP53D1009M"><span>Modification of the Undertow and Turbulence by Submerged Vegetation in a Laboratory Surf <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mandel, T.; Suckale, J.; Marras, S.; Maldonado, S.; Koseff, J. R.</p> <p>2016-12-01</p> <p>Breaking <span class="hlt">waves</span> in the surf <span class="hlt">zone</span> are a dominant factor shaping the evolution of our coastlines. The turbulence generated by <span class="hlt">wave</span> breaking causes sediment resuspension, while <span class="hlt">wave</span> runup, rundown, and the undertow transport this sediment along and across the shore (Longo et al., 2002). Coastal hazard models must now address the added complications of climate change, including sea level rise, stronger storm events, and ecosystem degradation (Arkema et al., 2013). A robust theoretical understanding of surf <span class="hlt">zone</span> dynamics is therefore imperative to considering the magnitude and implications of these potential changes. However, little work has been done to extend our current theoretical understanding to realistic beach faces, with aquatic vegetation, reefs, and other roughness elements that might mitigate scour and sedimentation. Clarifying these relationships will help scientists and policy-makers decide where to focus ecosystem restoration and preservation efforts, in order to maximize their protective benefits to infrastructure and economic activity on the coast. In order to evaluate the role of vegetation in coastal protection, we conducted a series of experiments in an idealized laboratory surf <span class="hlt">zone</span>. We examine the impact of submerged model vegetation on the undertow profile, <span class="hlt">wave</span> orbital velocities, turbulent kinetic energy, and <span class="hlt">wave</span>-induced stresses, and compare these results to theoretical formulations that model these quantities. We find that vegetation reduces the <span class="hlt">wave</span> energy available to be converted to turbulent kinetic energy during breaking, indicating a mechanism to mitigate suspension of sediment. Vegetation also reduces the magnitude of the undertow, likely reducing transport of sediment offshore. These results suggest that vegetation provides significant protective benefits for coastal communities at risk from erosion beyond its well-characterized ability to attenuate <span class="hlt">wave</span> height, and motivate further work to incorporate these effects into models of near</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24006887','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24006887"><span>Simple estimate of entrainment rate of pollutants from a coastal discharge into the surf <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wong, Simon H C; Monismith, Stephen G; Boehm, Alexandria B</p> <p>2013-10-15</p> <p>Microbial pollutants from coastal discharges can increase illness risks for swimmers and cause beach advisories. There is presently no predictive model for estimating the entrainment of pollution from coastal discharges into the surf <span class="hlt">zone</span>. We present a novel, quantitative framework for estimating surf <span class="hlt">zone</span> entrainment of pollution at a <span class="hlt">wave</span>-dominant open beach. Using physical arguments, we identify a dimensionless parameter equal to the quotient of the surf <span class="hlt">zone</span> width l(sz) and the cross-flow length scale of the discharge la = M(j) (1/2)/U(sz), where M(j) is the discharge's momentum flux and U(sz) is a representative alongshore velocity in the surf <span class="hlt">zone</span>. We conducted numerical modeling of a nonbuoyant discharge at an alongshore uniform beach with constant slope using a <span class="hlt">wave</span>-resolving hydrodynamic model. Using results from 144 numerical experiments we develop an empirical relationship between the surf <span class="hlt">zone</span> entrainment rate α and l(sz)/(la). The empirical relationship can reasonably explain seven measurements of surf <span class="hlt">zone</span> entrainment at three diverse coastal discharges. This predictive relationship can be a useful tool in coastal water quality management and can be used to develop predictive beach water quality models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S43B2819W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S43B2819W"><span>Complex Modeling of the Seismic Structure of the Trans-European Suture <span class="hlt">Zone</span>'s Margin from Receiver Function Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilde-Piorko, M.; Chrapkiewicz, K.; Lepore, S.; Polkowski, M.; Grad, M.</p> <p>2016-12-01</p> <p>The Trans-European Suture <span class="hlt">Zone</span> (TESZ) is one of the most prominent suture <span class="hlt">zones</span> in Europe separating the young Paleozoic Platform from the much older Precambrian East European Craton. The data recorded by "13 BB Star" broadband seismic stations (Grad et al., 2015) are analyzed to investigate the crustal and upper mantle structure of the margin of the Trans-European Suture <span class="hlt">Zone</span> (TESZ) in northern Poland. Receiver function (RF) locally provides the signature of sharp seismic discontinuities and information about the shear <span class="hlt">wave</span> (S-<span class="hlt">wave</span>) velocity distribution beneath the seismic station. Recorded seismograms are rotated from ZNE to LQT system with method using the properties of RF (Wilde-Piórko, 2015). Different techniques of receiver function interpretation are applied, including 1-D inversion of RF, 1-D forward modeling of RF, 2.5D forward modeling of RF, 1-D join inversion of RF and dispersion curves of surface <span class="hlt">wave</span>, to find the best S-<span class="hlt">wave</span> velocity model of the TESZ margin. A high-resolution 3D P-<span class="hlt">wave</span> velocity model in the area of Poland (Grad et al. 2016) are used as a starting model. National Science Centre Poland provided financial support for this work by NCN grant DEC-2011/02/A/ST10/00284.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016HydJ...24..439B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016HydJ...24..439B"><span>The puzzle of high <span class="hlt">heads</span> beneath the West Cumbrian coast, UK: a possible solution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Black, John H.; Barker, John A.</p> <p>2016-03-01</p> <p>A region of high <span class="hlt">heads</span> within the Borrowdale Volcanic Group (BVG; a fractured crystalline rock) beneath the coastal plain of West Cumbria, England (UK), is identified as a possible relic left over by the Late Devensian ice sheet. It was found during investigations in the 1990s. Contemporary modelling work failed to produce a satisfactory explanation of the high <span class="hlt">heads</span> compatible with the `cold recharge' isotopic signature of the groundwater. This study has reassessed the original hydraulic testing results. By plotting density-adjusted <span class="hlt">heads</span> versus their depth below the water table in the immediate vicinity of the borehole in which they were measured, a depth profile resembling a `<span class="hlt">wave</span>' was revealed with a peak value located at 1,100 m depth. The possibility that this <span class="hlt">wave</span> represents relic <span class="hlt">heads</span> from the last major ice sheet has been assessed using one-dimensional mathematical analysis based on a poroelastic approach. It is found that a wet-based ice sheet above the West Cumbrian coast was probably thick enough and sufficiently long-lasting to leave such relic <span class="hlt">heads</span> providing that the hydraulic diffusivity of the BVG is in the order of 10-6 m s-1. Initial assessment 20 years ago of the long-interval slug tests suggested that such low values are not likely. More recent interpretation argues for such low values of hydraulic diffusivity. It is concluded that ice sheet recharge is the most likely cause of the raised <span class="hlt">heads</span>, that the BVG contains significant patches of very low conductivity rock, and that long-interval single-hole tests should be avoided in fractured crystalline rock.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12657590','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12657590"><span>Dynamic interactions of eye and <span class="hlt">head</span> movements when reading with single-vision and progressive lenses in a simulated computer-based environment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Han, Ying; Ciuffreda, Kenneth J; Selenow, Arkady; Ali, Steven R</p> <p>2003-04-01</p> <p>To assess dynamic interactions of eye and <span class="hlt">head</span> movements during return-sweep saccades (RSS) when reading with single-vision (SVL) versus progressive-addition (PAL) lenses in a simulated computer-based business environment. Horizontal eye and <span class="hlt">head</span> movements were recorded objectively and simultaneously at a rate of 60 Hz during reading of single-page (SP; 14 degrees horizontal [H]) and double-page (DP; 37 degrees H) formats at 60 cm with binocular viewing. Subjects included 11 individuals with normal presbyopic vision aged 45 to 71 years selected by convenience sampling from a clinic population. Reading was performed with three types of spectacle lenses with a different clear near field of view (FOV): a SVL (60 degrees H clear FOV), a PAL-I with a relatively wide intermediate <span class="hlt">zone</span> (7.85 mm; 18 degrees H clear FOV), and a PAL-II with a relatively narrow intermediate <span class="hlt">zone</span> (5.60 mm; 13 degrees H clear FOV). Eye movements were initiated before <span class="hlt">head</span> movements in the SP condition, and the reverse was found in the DP condition, with all three lens types. Duration of eye movements increased as the <span class="hlt">zone</span> of clear vision decreased in the SP condition, and they were longer with the PALs than with the SVL in the DP condition. Gaze stabilization occurred later with the PALs than with the SVL in both the SP and DP conditions. The duration of <span class="hlt">head</span> movements was longer with the PAL-II than with the SVL in both the SP and DP conditions. Eye movement peak velocity was greater with the SVL than the PALs in the DP condition. Eye movement and <span class="hlt">head</span> movement strategies and timing were contingent on viewing conditions. The longer eye movement duration and gaze-stabilization times suggested that additional eye movements were needed to locate the clear-vision <span class="hlt">zone</span> and commence reading after the RSS. <span class="hlt">Head</span> movements with PALs for the SP condition were similarly optically induced. These eye movement and <span class="hlt">head</span> movement results may contribute to the reduced reading rate and related symptoms reported</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27022200','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27022200"><span>Parent Involvement in <span class="hlt">Head</span> Start and Children's Development: Indirect Effects Through Parenting.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ansari, Arya; Gershoff, Elizabeth</p> <p>2016-04-01</p> <p>The authors examined the extent to which parent involvement in <span class="hlt">Head</span> Start programs predicted changes in both parent and child outcomes over time, using a nationally representative sample of 1,020 three-year-old children over 3 <span class="hlt">waves</span> of the Family and Child Experiences Survey. Center policies that promote involvement predicted greater parent involvement, and parents who were more involved in <span class="hlt">Head</span> Start centers demonstrated increased cognitive stimulation and decreased spanking and controlling behaviors. In turn, these changes in parenting behaviors were associated with gains in children's academic and behavioral skills. These findings suggest that <span class="hlt">Head</span> Start programs should do even more to facilitate parent involvement because it can serve as an important means for promoting both parent and child outcomes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29491336','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29491336"><span>[Dropped <span class="hlt">head</span> syndrome as first manifestation of primary hyperparathyroid myopathy].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ota, Kiyobumi; Koseki, Sayo; Ikegami, Kenji; Onishi, Iichiroh; Tomimitsu, Hiyoryuki; Shintani, Shuzo</p> <p>2018-03-28</p> <p>75 years old woman presented with 6-month history of progressive dropped <span class="hlt">head</span> syndrome. Neurological examination revealed moderate weakness of flexor and extensor of neck and mild weakness of proximal appendicular muscles with normal deep tendon reflexes. The needle electromyography showed short duration and low amplitude motor unit potential. No fibrillation potentials or positive sharp <span class="hlt">waves</span> were seen. Biopsy of deltoid muscle was normal. Laboratory studies showed elevated levels of serum calcium (11.8 mg/dl, upper limit of normal 10.1) and intact parathyroid hormone (104 pg/ml, upper limit of normal 65), and decreased level of serum phosphorus (2.3 mg/dl, lower limit of normal 2.7). Ultrasonography and enhanced computed tomography revealed a parathyroid tumor. The tumor was removed surgically. Pathological examination proved tumor to be parathyroid adenoma. Dropped <span class="hlt">head</span> and weakness of muscles were dramatically improved within a week after the operation. Although hyperparathyroidism is a rare cause of dropped <span class="hlt">head</span> syndrome, neurologists must recognize hyperparathyroidism as a treatable cause of dropped <span class="hlt">head</span> syndrome.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T11F..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T11F..01B"><span>Multi-Scale Structure and Earthquake Properties in the San Jacinto Fault <span class="hlt">Zone</span> Area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ben-Zion, Y.</p> <p>2014-12-01</p> <p>I review multi-scale multi-signal seismological results on structure and earthquake properties within and around the San Jacinto Fault <span class="hlt">Zone</span> (SJFZ) in southern California. The results are based on data of the southern California and ANZA networks covering scales from a few km to over 100 km, additional near-fault seismometers and linear arrays with instrument spacing 25-50 m that cross the SJFZ at several locations, and a dense rectangular array with >1100 vertical-component nodes separated by 10-30 m centered on the fault. The structural studies utilize earthquake data to image the seismogenic sections and ambient noise to image the shallower structures. The earthquake studies use waveform inversions and additional time domain and spectral methods. We observe pronounced damage regions with low seismic velocities and anomalous Vp/Vs ratios around the fault, and clear velocity contrasts across various sections. The damage <span class="hlt">zones</span> and velocity contrasts produce fault <span class="hlt">zone</span> trapped and <span class="hlt">head</span> <span class="hlt">waves</span> at various locations, along with time delays, anisotropy and other signals. The damage <span class="hlt">zones</span> follow a flower-shape with depth; in places with velocity contrast they are offset to the stiffer side at depth as expected for bimaterial ruptures with persistent propagation direction. Analysis of PGV and PGA indicates clear persistent directivity at given fault sections and overall motion amplification within several km around the fault. Clear temporal changes of velocities, probably involving primarily the shallow material, are observed in response to seasonal, earthquake and other loadings. Full source tensor properties of M>4 earthquakes in the complex trifurcation area include statistically-robust small isotropic component, likely reflecting dynamic generation of rock damage in the source volumes. The dense fault <span class="hlt">zone</span> instruments record seismic "noise" at frequencies >200 Hz that can be used for imaging and monitoring the shallow material with high space and time details, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMMR13A2268J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMMR13A2268J"><span>Physical properties of fault <span class="hlt">zone</span> rocks from SAFOD: Tying logging data to high-pressure measurements on drill core</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeppson, T.; Tobin, H. J.</p> <p>2013-12-01</p> <p>In the summer of 2005, Phase 2 of the San Andreas Fault Observatory at Depth (SAFOD) borehole was completed and logged with wireline tools including a dipole sonic tool to measure P- and S-<span class="hlt">wave</span> velocities. A <span class="hlt">zone</span> of anomalously low velocity was detected from 3150 to 3414 m measured depth (MD), corresponding with the subsurface location of the San Andreas Fault <span class="hlt">Zone</span> (SAFZ). This low velocity <span class="hlt">zone</span> is 5-30% slower than the surrounding host rock. Within this broad low-velocity <span class="hlt">zone</span>, several slip surfaces were identified as well as two actively deforming shear <span class="hlt">zones</span>: the southwest deformation <span class="hlt">zone</span> (SDZ) and the central deformation <span class="hlt">zone</span> (CDZ), located at 3192 and 3302 m MD, respectively. The SAFZ had also previously been identified as a low velocity <span class="hlt">zone</span> in seismic velocity inversion models. The anomalously low velocity was hypothesized to result from either (a) brittle deformation in the damage <span class="hlt">zone</span> of the fault, (b) high fluid pressures with in the fault <span class="hlt">zone</span>, or (c) lithological variation, or a combination of the above. We measured P- and S-<span class="hlt">wave</span> velocities at ultrasonic frequencies on saturated 2.5 cm diameter core plug samples taken from SAFOD core obtained in 2007 from within the low velocity <span class="hlt">zone</span>. The resulting values fall into two distinct groups: foliated fault gouge and non-gouge. Samples of the foliated fault gouge have P-<span class="hlt">wave</span> velocities between 2.3-3.5 km/s while non-gouge samples lie between 4.1-5.4 km/s over a range of effective pressures from 5-70 MPa. There is a good correlation between the log measurements and laboratory values of P-and S <span class="hlt">wave</span> velocity at in situ pressure conditions especially for the foliated fault gouge. For non-gouge samples the laboratory values are approximately 0.08-0.73 km/s faster than the log values. This difference places the non-gouge velocities within the Great Valley siltstone velocity range, as measured by logs and ultrasonic measurements performed on outcrop samples. As a high fluid pressure <span class="hlt">zone</span> was not encountered during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25395458','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25395458"><span>Wnt/β-catenin signaling integrates patterning and metabolism of the insect growth <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Oberhofer, Georg; Grossmann, Daniela; Siemanowski, Janna L; Beissbarth, Tim; Bucher, Gregor</p> <p>2014-12-01</p> <p>Wnt/β-catenin and hedgehog (Hh) signaling are essential for transmitting signals across cell membranes in animal embryos. Early patterning of the principal insect model, Drosophila melanogaster, occurs in the syncytial blastoderm, where diffusion of transcription factors obviates the need for signaling pathways. However, in the cellularized growth <span class="hlt">zone</span> of typical short germ insect embryos, signaling pathways are predicted to play a more fundamental role. Indeed, the Wnt/β-catenin pathway is required for posterior elongation in most arthropods, although which target genes are activated in this context remains elusive. Here, we use the short germ beetle Tribolium castaneum to investigate two Wnt and Hh signaling centers located in the <span class="hlt">head</span> anlagen and in the growth <span class="hlt">zone</span> of early embryos. We find that Wnt/β-catenin signaling acts upstream of Hh in the growth <span class="hlt">zone</span>, whereas the opposite interaction occurs in the <span class="hlt">head</span>. We determine the target gene sets of the Wnt/β-catenin and Hh pathways and find that the growth <span class="hlt">zone</span> signaling center activates a much greater number of genes and that the Wnt and Hh target gene sets are essentially non-overlapping. The Wnt pathway activates key genes of all three germ layers, including pair-rule genes, and Tc-caudal and Tc-twist. Furthermore, the Wnt pathway is required for hindgut development and we identify Tc-senseless as a novel hindgut patterning gene required in the early growth <span class="hlt">zone</span>. At the same time, Wnt acts on growth <span class="hlt">zone</span> metabolism and cell division, thereby integrating growth with patterning. Posterior Hh signaling activates several genes potentially involved in a proteinase cascade of unknown function. © 2014. Published by The Company of Biologists Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4299277','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4299277"><span>Wnt/β-catenin signaling integrates patterning and metabolism of the insect growth <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Oberhofer, Georg; Grossmann, Daniela; Siemanowski, Janna L.; Beissbarth, Tim; Bucher, Gregor</p> <p>2014-01-01</p> <p>Wnt/β-catenin and hedgehog (Hh) signaling are essential for transmitting signals across cell membranes in animal embryos. Early patterning of the principal insect model, Drosophila melanogaster, occurs in the syncytial blastoderm, where diffusion of transcription factors obviates the need for signaling pathways. However, in the cellularized growth <span class="hlt">zone</span> of typical short germ insect embryos, signaling pathways are predicted to play a more fundamental role. Indeed, the Wnt/β-catenin pathway is required for posterior elongation in most arthropods, although which target genes are activated in this context remains elusive. Here, we use the short germ beetle Tribolium castaneum to investigate two Wnt and Hh signaling centers located in the <span class="hlt">head</span> anlagen and in the growth <span class="hlt">zone</span> of early embryos. We find that Wnt/β-catenin signaling acts upstream of Hh in the growth <span class="hlt">zone</span>, whereas the opposite interaction occurs in the <span class="hlt">head</span>. We determine the target gene sets of the Wnt/β-catenin and Hh pathways and find that the growth <span class="hlt">zone</span> signaling center activates a much greater number of genes and that the Wnt and Hh target gene sets are essentially non-overlapping. The Wnt pathway activates key genes of all three germ layers, including pair-rule genes, and Tc-caudal and Tc-twist. Furthermore, the Wnt pathway is required for hindgut development and we identify Tc-senseless as a novel hindgut patterning gene required in the early growth <span class="hlt">zone</span>. At the same time, Wnt acts on growth <span class="hlt">zone</span> metabolism and cell division, thereby integrating growth with patterning. Posterior Hh signaling activates several genes potentially involved in a proteinase cascade of unknown function. PMID:25395458</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020700','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020700"><span>Evidence of shallow fault <span class="hlt">zone</span> strengthening after the 1992 M7.5 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>Li, Y.-G.; Vidale, J.E.; Aki, K.; Xu, Fei; Burdette, T.</p> <p>1998-01-01</p> <p>Repeated seismic surveys of the Landers, California, fault <span class="hlt">zone</span> that ruptured in the magnitude (M) 7.5 earthquake of 1992 reveal an increase in seismic velocity with time. P, S, and fault <span class="hlt">zone</span> trapped <span class="hlt">waves</span> were excited by near-surface explosions in two locations in 1994 and 1996, and were recorded on two linear, three-component seismic arrays deployed across the Johnson Valley fault trace. The travel times of P and S <span class="hlt">waves</span> for identical shot-receiver pairs decreased by 0.5 to 1.5 percent from 1994 to 1996, with the larger changes at stations located within the fault <span class="hlt">zone</span>. These observations indicate that the shallow Johnson Valley fault is strengthening after the main shock, most likely because of closure of cracks that were opened by the 1992 earthquake. The increase in velocity is consistent with the prevalence of dry over wet cracks and with a reduction in the apparent crack density near the fault <span class="hlt">zone</span> by approximately 1.0 percent from 1994 to 1996.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AcAau..91..166C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AcAau..91..166C"><span>Impaired T-<span class="hlt">wave</span> amplitude adaptation to heart-rate induced by cardiac deconditioning after 5-days of <span class="hlt">head</span>-down bed-rest</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caiani, Enrico G.; Pellegrini, Alessandro; Bolea, Juan; Sotaquira, Miguel; Almeida, Rute; Vaïda, Pierre</p> <p>2013-10-01</p> <p>The study of QT/RR relationship is important for the clinical evaluation of possible risk of acquired or congenital ventricular tachyarrhythmias. In the hypothesis that microgravity exposure could induce changes in the repolarization mechanisms, our aim was to test if a short 5-days strict 6° <span class="hlt">head</span>-down bed-rest (HDBR) could induce alterations in the QT/RR relationship and spatial repolarization heterogeneity. Twenty-two healthy men (mean age 31±6) were enrolled as part of the European Space Agency HDBR studies. High fidelity (1000 Hz) 24 h Holter ECG (12-leads, Mortara Instrument) was acquired before (PRE), the last day of HDBR (HDT5), and four days after its conclusion (POST). The night period (23:00-06:30) was selected for analysis. X, Y, Z leads were derived and the vectorcardiogram computed. Selective beat averaging was used to obtain averages of P-QRS-T complexes preceded by the same RR (10 ms bin amplitude, in the range 900-1200 ms). For each averaged waveform (i.e., one for each bin), T-<span class="hlt">wave</span> maximum amplitude (Tmax), T-<span class="hlt">wave</span> area (Tarea), RTapex, RTend, ventricular gradient (VG) magnitude and spatial QRS-T angle were computed. Non-parametric Friedman test was applied. Compared to PRE, at HDT5 both RTapex and RTend resulted shortened (-4%), with a decrease in T-<span class="hlt">wave</span> amplitude (-8%) and area (-13%). VG was diminished by 10%, and QRS-T angle increased by 14°. At POST, QT duration and area parameters, as well as QRS-T angle were restored while Tmax resulted larger than PRE (+5%) and VG was still decreased by 3%. Also, a marked loss in strength of the linear regression with RR was found at HDT5 in Tmax and Tarea, that could represent a new dynamic marker of increased risk for life-threatening arrhythmias. Despite the short-term HDBR, ventricular repolarization during the night period was affected. This should be taken into account in astronauts for risk assessment during space flight.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15920988','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15920988"><span>Modelling the vestibular <span class="hlt">head</span> tilt response.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Heibert, D; Lithgow, B</p> <p>2005-03-01</p> <p>This paper attempts to verify the existence of potentially diagnostically significant periodic signals thought to exist in recordings of neural activity originating from the vestibular nerve, following a single tilt of the <span class="hlt">head</span>. It then attempts to find the physiological basis of this signal, in particular focusing on the mechanical response of the vestibular system. Simple mechanical models of the semi circular canals having angular velocities applied to them were looked at. A simple single canal model was simulated using CFX software. Finally, a simple model of all three canals with elastic duct walls and a moving cupula was constructed. Pressure <span class="hlt">waves</span> within the canals were simulated using water hammer or pressure transient theory. In particular, it was investigated whether pressure <span class="hlt">waves</span> within the utricle following a square pulse angular velocity applied to the canal(s) may be responsible for quasi-periodic oscillatory signals. The simulations showed that there are no pressure <span class="hlt">waves</span> resonating within the canals following a square pulse angular velocity applied to the canal(s). The results show that the oscillatory signals are most likely not mechanical in origin. It was concluded that further investigation is required.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3866102','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3866102"><span>Characterization of the <span class="hlt">head</span>-twitch response induced by hallucinogens in mice: detection of the behavior based on the dynamics of <span class="hlt">head</span> movement</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Halberstadt, Adam L.; Geyer, Mark A.</p> <p>2013-01-01</p> <p>Rationale The <span class="hlt">head</span>-twitch response (HTR) is a rapid side-to-side rotational <span class="hlt">head</span> movement that occurs in rats and mice after administration of serotonergic hallucinogens and other 5-HT2A agonists. The HTR is widely used as a behavioral assay for 5-HT2A activation and to probe for interactions between the 5-HT2A receptor and other transmitter systems. Objective High-speed video recordings were used to analyze the <span class="hlt">head</span> movement that occurs during <span class="hlt">head</span> twitches in C57BL/6J mice. Experiments were also conducted in C57BL/6J mice to determine whether a <span class="hlt">head</span>-mounted magnet and a magnetometer coil could be used to detect the HTR induced by serotonergic hallucinations based on the dynamics of the response. Results <span class="hlt">Head</span> movement during the HTR was highly rhythmic and occurred within a specific frequency range (mean reciprocation frequency of 90.3 Hz). <span class="hlt">Head</span> twitches produced <span class="hlt">wave</span>-like oscillations of magnetometer coil voltage that matched the frequency of <span class="hlt">head</span> movement during the response. The magnetometer coil detected the HTR induced by the serotonergic hallucinogens 2,5-dimethoxy-4-iodoamphetamine (DOI; 0.25, 0.5, and 1.0 mg/kg, IP) and lysergic acid diethylamide (LSD; 0.05, 0.1, 0.2, and 0.4 mg/kg, IP) with extremely high sensitivity and specificity. Magnetometer coil recordings demonstrated that the non-hallucinogenic compounds (+)-amphetamine (2.5 and 5.0 mg/kg, IP) and lisuride (0.8, 1.6, and 3.2 mg/kg, IP) did not induce the HTR. Conclusions These studies confirm that a magnetometer coil can be used to detect the HTR induced by hallucinogens. The use of magnetometer-based HTR detection provides a high-throughput, semi-automated assay for this behavior, and offers several advantages over traditional assessment methods. PMID:23407781</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAP...123b4904V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAP...123b4904V"><span>Nonlinear mechanisms of two-dimensional <span class="hlt">wave-wave</span> transformations in the initially coupled acoustic structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vorotnikov, K.; Starosvetsky, Y.</p> <p>2018-01-01</p> <p>The present study concerns two-dimensional nonlinear mechanisms of bidirectional and unidirectional channeling of longitudinal and shear <span class="hlt">waves</span> emerging in the locally resonant acoustic structure. The system under consideration comprises an oscillatory chain of the axially coupled masses. Each mass of the chain is subject to the local linear potential along the lateral direction and incorporates the lightweight internal rotator. In the present work, we demonstrate the emergence of special resonant regimes of complete bi- and unidirectional transitions between the longitudinal and the shear <span class="hlt">waves</span> of the locally resonant chain. These regimes are manifested by the two-dimensional energy channeling between the longitudinal and the shear traveling <span class="hlt">waves</span> in the recurrent as well as the irreversible fashion. We show that the spatial control of the two dimensional energy flow between the longitudinal and the shear <span class="hlt">waves</span> is solely governed by the motion of the internal rotators. Nonlinear analysis of the regimes of a bidirectional <span class="hlt">wave</span> channeling unveils their global bifurcation structure and predicts the <span class="hlt">zones</span> of their spontaneous transitions from a complete bi-directional <span class="hlt">wave</span> channeling to the one-directional entrapment. An additional regime of a complete irreversible resonant transformation of the longitudinal <span class="hlt">wave</span> into a shear <span class="hlt">wave</span> is analyzed in the study. The intrinsic mechanism governing the unidirectional <span class="hlt">wave</span> reorientation is described analytically. The results of the analysis of both mechanisms are substantiated by the numerical simulations of the full model and are found to be in a good agreement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17..463T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..463T"><span>Classification of regimes of internal solitary <span class="hlt">waves</span> transformation over a shelf-slope topography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Terletska, Kateryna; Maderich, Vladimir; Talipova, Tatiana; Brovchenko, Igor; Jung, Kyung Tae</p> <p>2015-04-01</p> <p> depression may be converted to <span class="hlt">wave</span> of elevation at the 'turning point' (h2 = h1) as they propagate from deep water onto a shallow shelf. Thus intersecting surfaces f1 and f2 divide three-dimensional diagram into four <span class="hlt">zones</span>. <span class="hlt">Zone</span> I located above two surfaces and corresponds to the non breaking regime. <span class="hlt">Zone</span> II lies above 'breaking' surfaces but below the surface of changing polarity and corresponds to regime of changing polarity without breaking. <span class="hlt">Zone</span> III lies above surface of changing polarity but below 'breaking' surfaces and corresponds to regime of <span class="hlt">wave</span> breaking without changing polarity. <span class="hlt">Zone</span> IV that located below two surfaces and corresponds to the regime of <span class="hlt">wave</span> breaking with changing polarity. Regimes predicted by diagram agree with results of numerical modelling, laboratory and observation data. Based on the proposed diagram the regions in α, β, γ space with a high energy dissipation of ISW passed over the shelf-slope topography are distinguished. References Talipova T., Terletska K., Maderich V, Brovchenko I., Jung K.T., Pelinovsky E. and Grimshaw R. 2013. Internal solitary <span class="hlt">wave</span> transformation over the bottom step: loss of energy. Phys. Fluids, 25, 032110 Vlasenko V., Hutter K. 2002. Numerical Experiments on the Breaking of Solitary Internal <span class="hlt">Waves</span> over a Slope-Shelf Topography. J. Phys. Oceanogr., 32 (6), 1779-1793</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22391502-prediction-subsurface-fracture-mining-zone-papua-using-passive-seismic-tomography-based-fresnel-zone','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22391502-prediction-subsurface-fracture-mining-zone-papua-using-passive-seismic-tomography-based-fresnel-zone"><span>Prediction of subsurface fracture in mining <span class="hlt">zone</span> of Papua using passive seismic tomography based on Fresnel <span class="hlt">zone</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>Setiadi, Herlan; Nurhandoko, Bagus Endar B.; Wely, Woen</p> <p></p> <p>Fracture prediction in a block cave of underground mine is very important to monitor the structure of the fracture that can be harmful to the mining activities. Many methods can be used to obtain such information, such as TDR (Time Domain Relectometry) and open hole. Both of them have limitations in range measurement. Passive seismic tomography is one of the subsurface imaging method. It has advantage in terms of measurements, cost, and rich of rock physical information. This passive seismic tomography studies using Fresnel <span class="hlt">zone</span> to model the wavepath by using frequency parameter. Fresnel <span class="hlt">zone</span> was developed by Nurhandoko inmore » 2000. The result of this study is tomography of P and S <span class="hlt">wave</span> velocity which can predict position of fracture. The study also attempted to use sum of the wavefronts to obtain position and time of seismic event occurence. Fresnel <span class="hlt">zone</span> tomography and the summation wavefront can predict location of geological structure of mine area as well.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29615415','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29615415"><span>Exposure of zebra mussels to extracorporeal shock <span class="hlt">waves</span> demonstrates formation of new mineralized tissue inside and outside the focus <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sternecker, Katharina; Geist, Juergen; Beggel, Sebastian; Dietz-Laursonn, Kristin; de la Fuente, Matias; Frank, Hans-Georg; Furia, John P; Milz, Stefan; Schmitz, Christoph</p> <p>2018-04-03</p> <p>The success rate of extracorporeal shock <span class="hlt">wave</span> therapy (ESWT) for fracture nonunions in human medicine (i.e., radiographic union at six months after ESWT) is only approximately 75%. Detailed knowledge regarding the underlying mechanisms that induce bio-calcification after ESWT is limited. We analyzed the biological response within mineralized tissue of a new invertebrate model organism, the zebra mussel Dreissena polymorpha , after exposure with extracorporeal shock <span class="hlt">waves</span> (ESWs). Mussels were exposed to ESWs with positive energy density of 0.4 mJ/mm 2 (A) or were sham exposed (B). Detection of newly calcified tissue was performed by exposing the mussels to fluorescent markers. Two weeks later, the A-mussels showed a higher mean fluorescence signal intensity within the shell <span class="hlt">zone</span> than the B-mussels (p<0.05). Acoustic measurements revealed that the increased mean fluorescence signal intensity within the shell of the A-mussels was independent of the size and position of the focal point of the ESWs. These data demonstrate that induction of bio-calcification after ESWT may not be restricted to the region of direct energy transfer of ESWs into calcified tissue. The results of the present study are of relevance for better understanding of the molecular and cellular mechanisms that induce formation of new mineralized tissue after ESWT. © 2018. Published by The Company of Biologists Ltd.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GGG....15.1419S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GGG....15.1419S"><span>Nonlinear attenuation of S-<span class="hlt">waves</span> and Love <span class="hlt">waves</span> within ambient rock</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sleep, Norman H.; Erickson, Brittany A.</p> <p>2014-04-01</p> <p>obtain scaling relationships for nonlinear attenuation of S-<span class="hlt">waves</span> and Love <span class="hlt">waves</span> within sedimentary basins to assist numerical modeling. These relationships constrain the past peak ground velocity (PGV) of strong 3-4 s Love <span class="hlt">waves</span> from San Andreas events within Greater Los Angeles, as well as the maximum PGV of future <span class="hlt">waves</span> that can propagate without strong nonlinear attenuation. During each event, the shaking episode cracks the stiff, shallow rock. Over multiple events, this repeated damage in the upper few hundred meters leads to self-organization of the shear modulus. Dynamic strain is PGV divided by phase velocity, and dynamic stress is strain times the shear modulus. The frictional yield stress is proportional to depth times the effective coefficient of friction. At the eventual quasi-steady self-organized state, the shear modulus increases linearly with depth allowing inference of past typical PGV where rock over the damaged depth range barely reaches frictional failure. Still greater future PGV would cause frictional failure throughout the damaged <span class="hlt">zone</span>, nonlinearly attenuating the <span class="hlt">wave</span>. Assuming self-organization has taken place, estimated maximum past PGV within Greater Los Angeles Basins is 0.4-2.6 m s-1. The upper part of this range includes regions of accumulating sediments with low S-<span class="hlt">wave</span> velocity that may have not yet compacted, rather than having been damaged by strong shaking. Published numerical models indicate that strong Love <span class="hlt">waves</span> from the San Andreas Fault pass through Whittier Narrows. Within this corridor, deep drawdown of the water table from its currently shallow and preindustrial levels would nearly double PGV of Love <span class="hlt">waves</span> reaching Downtown Los Angeles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870011448','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870011448"><span>Alfven-<span class="hlt">wave</span> dissipation: A support mechanism for quiescent prominences</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jensen, Eberhart</p> <p>1986-01-01</p> <p>High resolution filtergrams or spectrograms of the main body of quiescent prominences often show a very vivid dynamical picture that cannot be reconciled with static models. Even if large differences exist between individual prominences in this respect, at least parts of the prominence are usually found to be in a 'choppy', turbulent state. Evidence for systematic flows are found in local regions in the prominence and also in the transition <span class="hlt">zone</span> in the surroundings. These two regions are probably decoupled magnetically. Alfven <span class="hlt">waves</span> are generally believed to be responsible for the heating in the upper chromosphere and corona (Hollweg 1986). Since evidence for the presence of Alfven-<span class="hlt">waves</span> has also been found in the solar wind field, it is highly probable that such <span class="hlt">waves</span> are generated in the convection <span class="hlt">zone</span> of the sun and propagated outwards in the solar atmosphere wherever a proper magnetic field is present to carry the <span class="hlt">waves</span>. The most basic magnetic formations in the solar atmosphere are simple loops. They occur all over the solar surface and cover a large range of magnetic field strengths. Loops with the strongest magnetic fields are found in active regions. It is to be expected that the Alfven-<span class="hlt">wave</span> flux which is channelled into the loops from below, could show considerable variation both with heliocentric latitude, with time and locally between neighbouring loops. What happens when a magnetic loop is exposed to the appropriate Alfven-<span class="hlt">wave</span> flux required to heat the upper solar atmosphere is examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA524474','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA524474"><span>Seismic Tomography of the Arabian-Eurasian Collision <span class="hlt">Zone</span> and Surrounding Areas</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-05-20</p> <p><span class="hlt">zone</span>. The crustal models correlate well with geologic and tectonic features. The upper mantle tomograms show the images of the subducted Neotethys...We first obtain Pn and Sn velocities using local and regional arrival time data. Second, we obtain the 3-D crustal P and S velocity models...teleseismic tomography provides a high-resolution, 3-D P-<span class="hlt">wave</span> velocity model for the crust, upper mantle, and the transition <span class="hlt">zone</span>. The crustal models</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930052418&hterms=dynamo&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Ddynamo','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930052418&hterms=dynamo&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Ddynamo"><span>A solar dynamo surface <span class="hlt">wave</span> at the interface between convection and nonuniform rotation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parker, E. N.</p> <p>1993-01-01</p> <p>A simple dynamo surface <span class="hlt">wave</span> is presented to illustrate the basic principles of a dynamo operating in the thin layer of shear and suppressed eddy diffusion beneath the cyclonic convection in the convection <span class="hlt">zone</span> of the sun. It is shown that the restriction of the shear delta(Omega)/delta(r) to a region below the convective <span class="hlt">zone</span> provides the basic mode with a greatly reduced turbulent diffusion coefficient in the region of strong azimuthal field. The dynamo takes on the character of a surface <span class="hlt">wave</span> tied to the lower surface z = 0 of the convective <span class="hlt">zone</span>. There is a substantial body of evidence suggesting a fibril state for the principal flux bundles beneath the surface of the sun, with fundamental implications for the solar dynamo.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51E0540J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51E0540J"><span>Amphibious Shear Velocity Structure of the Cascadia Subduction <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Janiszewski, H. A.; Gaherty, J. B.; Abers, G. A.; Gao, H.</p> <p>2017-12-01</p> <p>The amphibious Cascadia Initiative crosses the coastline of the Cascadia subduction <span class="hlt">zone</span> (CSZ) deploying seismometers from the Juan de Fuca ridge offshore to beyond the volcanic arc onshore. This allows unprecedented seismic imaging of the CSZ, enabling examination of both the evolution of the Juan de Fuca plate prior to and during subduction as well as the along strike variability of the subduction system. Here we present new results from an amphibious shear velocity model for the crust and upper mantle across the Cascadia subduction <span class="hlt">zone</span>. The primary data used in this inversion are surface-<span class="hlt">wave</span> phase velocities derived from ambient-noise Rayleigh-<span class="hlt">wave</span> data in the 10 - 20 s period band, and teleseismic earthquake Rayleigh <span class="hlt">wave</span> phase velocities in the 20 - 160 s period band. Phase velocity maps from these data reflect major tectonic structures including the transition from oceanic to continental lithosphere, Juan de Fuca lithosphere that is faster than observations in the Pacific for oceanic crust of its age, slow velocities associated with the accretionary prism, the front of the fast subducting slab, and the Cascades volcanic arc which is associated with slower velocities in the south than in the north. Crustal structures are constrained by receiver functions in the offshore forearc and onshore regions, and by active source constraints on the Juan de Fuca plate prior to subduction. The shear-<span class="hlt">wave</span> velocities are interpreted in their relationships to temperature, presence of melt or hydrous alteration, and compositional variation of the CSZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.H21D0860C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.H21D0860C"><span>Finite Element Modeling of Transient <span class="hlt">Head</span> Field Associated with Partially Penetrating, Slug Tests in a Heterogeneous Aquifer with Low Permeability, Stratigraphic <span class="hlt">Zones</span> and Faults</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cheng, J.; Johnson, B.; Everett, M.</p> <p>2003-12-01</p> <p>Preliminary field work shows slug interference tests using an array of multilevel active and monitoring wells have potential of permitting enhanced aquifer characterization. Analysis of these test data, however, ultimately will rely on numerical geophysical inverse models. In order to gain insight as well as to provide synthetic data sets, we use a 3-D finite element analysis (code:FEHM-LANL) to explore the effect of idealized, low permeability, stratigraphical and structural (faults) heterogeneities on the transient <span class="hlt">head</span> field associated with a slug test in a packer-isolated interval of an open borehole. The borehole and packers are modeled explicitly; wellbore storage is selected to match values of field tests. The homogeneous model exhibits excellent agreement with that of the semi-analytical model of Liu and Butler (1995). Models are axisymmetric with a centrally located slugged interval within a homogenous, isotropic, confined aquifer with embedded, horizontal or vertical <span class="hlt">zones</span> of lower permeability that represent low permeability strata or faults, respectively. Either one or two horizontal layers are located opposite the borehole packers, which is a common situation at the field site; layer thickness (0.15-0.75 m), permeability contrast (up to 4 orders of magnitude contrast) and lateral continuity of layers are varied between models. The effect of a "hole" in a layer also is assessed. Fault models explore effects of thickness (0.05-0.75 m) and permeability contrast as well as additional effects associated with the offset of low permeability strata. Results of models are represented most clearly by contour maps of time of arrival and normalized amplitude of peak <span class="hlt">head</span> perturbation, but transient <span class="hlt">head</span> histories at selected locations provide additional insight. Synthesis of the models is on-going but a few points can be made at present. Spatial patterns are distinctive and allow easy discrimination between stratigraphic and structural impedance features. Time</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175912','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175912"><span>Near-surface versus fault <span class="hlt">zone</span> damage following the 1999 Chi-Chi earthquake: Observation and simulation of repeating earthquakes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Chen, Kate Huihsuan; Furumura, Takashi; Rubinstein, Justin L.</p> <p>2015-01-01</p> <p>We observe crustal damage and its subsequent recovery caused by the 1999 M7.6 Chi-Chi earthquake in central Taiwan. Analysis of repeating earthquakes in Hualien region, ~70 km east of the Chi-Chi earthquake, shows a remarkable change in <span class="hlt">wave</span> propagation beginning in the year 2000, revealing damage within the fault <span class="hlt">zone</span> and distributed across the near surface. We use moving window cross correlation to identify a dramatic decrease in the waveform similarity and delays in the S <span class="hlt">wave</span> coda. The maximum delay is up to 59 ms, corresponding to a 7.6% velocity decrease averaged over the <span class="hlt">wave</span> propagation path. The waveform changes on either side of the fault are distinct. They occur in different parts of the waveforms, affect different frequencies, and the size of the velocity reductions is different. Using a finite difference method, we simulate the effect of postseismic changes in the wavefield by introducing S <span class="hlt">wave</span> velocity anomaly in the fault <span class="hlt">zone</span> and near the surface. The models that best fit the observations point to pervasive damage in the near surface and deep, along-fault damage at the time of the Chi-Chi earthquake. The footwall stations show the combined effect of near-surface and the fault <span class="hlt">zone</span> damage, where the velocity reduction (2–7%) is twofold to threefold greater than the fault <span class="hlt">zone</span> damage observed in the hanging wall stations. The physical models obtained here allow us to monitor the temporal evolution and recovering process of the Chi-Chi fault <span class="hlt">zone</span> damage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMDI31B2633P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMDI31B2633P"><span>Slab geometry of the South American margin from joint inversion of body <span class="hlt">waves</span> and surface <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Porritt, R. W.; Ward, K. M.; Porter, R. C.; Portner, D. E.; Lynner, C.; Beck, S. L.; Zandt, G.</p> <p>2016-12-01</p> <p>The western margin of South America is a long subduction <span class="hlt">zone</span> with a complex, highly three -dimensional geometry. The first order structure of the slab has previously been inferred from seismicity patterns and locations of volcanoes, but confirmation of the slab geometry by seismic imaging for the entire margin has been limited by either shallow, lithospheric scale models or broader, upper mantle images, often defined on a limited spatial footprint. Here, we present new teleseismic tomographic SV seismic models of the upper mantle from 10°S to 40°S along the South American subduction <span class="hlt">zone</span> with resolution to a depth of 1000 km as inferred from checkerboard tests. In regions near the Peru Bolivia border (12°S to 18°S) and near central Chile and western Argentina (29.5°S to 33°S) we jointly invert the multi-band direct S and SKS relative delay times with Rayleigh <span class="hlt">wave</span> phase velocities from ambient noise and teleseismic surface <span class="hlt">wave</span> tomography. This self-consistent model provides information from the upper crust to below the mantle transition <span class="hlt">zone</span> along the western margin in these two regions. This consistency allows tracing the slab from the South American coastline to the sub-transition <span class="hlt">zone</span> upper mantle. From this model we image several features, but most notable is a significant eastward step near the southern edge of the margin (24°-30° S). West of this step, a large high shear velocity body is imaged in the base of and below the transition <span class="hlt">zone</span>. We suggest this may be a stagnant slab, which is descending into the lower mantle now that it is no longer attached to the surface. This suggests a new component to the subduction history of western South America when an older slab lead the convergence before anchoring in the transition <span class="hlt">zone</span>, breaking off from the surface, and being overtaken by the modern, actively subducting slab now located further east.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S21E..02Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S21E..02Z"><span>Joint Inversion of Body-<span class="hlt">Wave</span> Arrival Times and Surface-<span class="hlt">Wave</span> Dispersion Data for Three-Dimensional Seismic Velocity Structure Around SAFOD</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, H.; Thurber, C. H.; Maceira, M.; Roux, P.</p> <p>2013-12-01</p> <p>The crust around the San Andreas Fault Observatory at depth (SAFOD) has been the subject of many geophysical studies aimed at characterizing in detail the fault <span class="hlt">zone</span> structure and elucidating the lithologies and physical properties of the surrounding rocks. Seismic methods in particular have revealed the complex two-dimensional (2D) and three-dimensional (3D) structure of the crustal volume around SAFOD and the strong velocity reduction in the fault damage <span class="hlt">zone</span>. In this study we conduct a joint inversion using body-<span class="hlt">wave</span> arrival times and surface-<span class="hlt">wave</span> dispersion data to image the P-and S-<span class="hlt">wave</span> velocity structure of the upper crust surrounding SAFOD. The two data types have complementary strengths - the body-<span class="hlt">wave</span> data have good resolution at depth, albeit only where there are crossing rays between sources and receivers, whereas the surface <span class="hlt">waves</span> have very good near-surface resolution and are not dependent on the earthquake source distribution because they are derived from ambient noise. The body-<span class="hlt">wave</span> data are from local earthquakes and explosions, comprising the dataset analyzed by Zhang et al. (2009). The surface-<span class="hlt">wave</span> data are for Love <span class="hlt">waves</span> from ambient noise correlations, and are from Roux et al. (2011). The joint inversion code is based on the regional-scale version of the double-difference (DD) tomography algorithm tomoDD. The surface-<span class="hlt">wave</span> inversion code that is integrated into the joint inversion algorithm is from Maceira and Ammon (2009). The propagator matrix solver in the algorithm DISPER80 (Saito, 1988) is used for the forward calculation of dispersion curves from layered velocity models. We examined how the structural models vary as we vary the relative weighting of the fit to the two data sets and in comparison to the previous separate inversion results. The joint inversion with the 'optimal' weighting shows more clearly the U-shaped local structure from the Buzzard Canyon Fault on the west side of SAF to the Gold Hill Fault on the east side.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900030386&hterms=Scramjet+powered+vehicles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DScramjet%2Bpowered%2Bvehicles.','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900030386&hterms=Scramjet+powered+vehicles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DScramjet%2Bpowered%2Bvehicles."><span><span class="hlt">Wave</span> combustors for trans-atmospheric vehicles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Menees, Gene P.; Bowles, Jeffrey V.; Adelman, Henry G.; Cambier, Jean-Luc</p> <p>1989-01-01</p> <p>A performance analysis is given of a conceptual transatmospheric vehicle (TAV). The TAV is powered by a an oblique detonation <span class="hlt">wave</span> engine (ODWE). The ODWE is an airbreathing hypersonic propulsion system which utilizes shock and detonation <span class="hlt">waves</span> to enhance fuel-air mixing and combustion in supersonic flow. In this <span class="hlt">wave</span> combustor concept, an oblique shock <span class="hlt">wave</span> in the combustor can act as a flameholder by increasing the pressure and temperature of the air-fuel mixture, thereby decreasing the ignition delay. If the oblique shock is sufficiently strong, then the combustion front and the shock <span class="hlt">wave</span> can couple into a detonation <span class="hlt">wave</span>. In this case, combustion occurs almost instantaneously in a thin <span class="hlt">zone</span> behind the <span class="hlt">wave</span> front. The result is a shorter lighter engine compared to the scramjet. The ODWE-powered hypersonic vehicle performance is compared to that of a scramjet-powered vehicle. Among the results outlined, it is found that the ODWE trades a better engine performance above Mach 15 for a lower performance below Mach 15. The overall higher performance of the ODWE results in a 51,000-lb weight savings and a higher payload weight fraction of approximately 12 percent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS11A1248G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS11A1248G"><span>Non-Hydrostatic Modelling of <span class="hlt">Waves</span> and Currents over Subtle Bathymetric Features</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gomes, E.; Mulligan, R. P.; McNinch, J.</p> <p>2014-12-01</p> <p>Localized areas with high rates of shoreline erosion on beaches, referred to as erosional hotspots, can occur near clusters of relict shore-oblique sandbars. <span class="hlt">Wave</span> transformation and <span class="hlt">wave</span>-driven currents over these morphological features could provide an understanding of the hydrodynamic-morphologic coupling mechanism that connects them to the occurrence of erosional hotspots. To investigate this, we use the non-hydrostatic SWASH model that phase-resolves the free surface and fluid motions throughout the water column, allowing for high resolution of <span class="hlt">wave</span> propagation and breaking processes. In this study we apply a coupled system of nested models including SWAN over a large domain of the North Carolina shelf with smaller nested SWASH domains in areas of interest to determine the hydrodynamic processes occurring over shore oblique bars. In this presentation we focus on a high resolution grid (10 vertical layers, 10 m horizontal resolution) applied to the Duck region with model validation from acoustic <span class="hlt">wave</span> and current data, and observations from the Coastal Lidar And Radar Imaging System (CLARIS). By altering the bathymetry input for each model run based on bathymetric surveys and comparing the predicted and observed <span class="hlt">wave</span> heights and current profiles, the effects of subtle bathymetric perturbations have on <span class="hlt">wave</span> refraction, <span class="hlt">wave</span> breaking, surf <span class="hlt">zone</span> currents and vorticity are investigated. The ability to predict <span class="hlt">wave</span> breaking and hydrodynamics with a non-hydrostatic model may improve our understanding of surf <span class="hlt">zone</span> dynamics in relation to morphologic conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24281430','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24281430"><span>Morphology of seahorse <span class="hlt">head</span> hydrodynamically aids in capture of evasive prey.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gemmell, Brad J; Sheng, Jian; Buskey, Edward J</p> <p>2013-01-01</p> <p>Syngnathid fish (seahorses, pipefish and sea dragons) are slow swimmers yet capture evasive prey (copepods) using a technique known as the 'pivot' feeding, which involves rapid movement to overcome prey escape capabilities. However, this feeding mode functions only at short range and requires approaching very closely to hydrodynamically sensitive prey without triggering an escape. Here we investigate the role of <span class="hlt">head</span> morphology on prey capture using holographic and particle image velocimetry (PIV). We show that <span class="hlt">head</span> morphology functions to create a reduced fluid deformation <span class="hlt">zone</span>, minimizing hydrodynamic disturbance where feeding strikes occur (above the end of the snout), and permits syngnathid fish to approach highly sensitive copepod prey (Acartia tonsa) undetected. The results explain how these animals can successfully employ short range 'pivot' feeding effectively on evasive prey. The need to approach prey with stealth may have selected for a <span class="hlt">head</span> shape that produces lower deformation rates than other fish.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030062110','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030062110"><span>A Self-Consistent Model of the Interacting Ring Current Ions and Electromagnetic Ion Cyclotron <span class="hlt">Waves</span>, Initial Results: <span class="hlt">Waves</span> and Precipitating Fluxes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Khazanov, G. V.; Gamayunov, K. V.; Jordanova, V. K.; Krivorutsky, E. N.</p> <p>2002-01-01</p> <p>Initial results from a newly developed model of the interacting ring current ions and ion cyclotron <span class="hlt">waves</span> are presented. The model is based on the system of two kinetic equations: one equation describes the ring current ion dynamics, and another equation describes <span class="hlt">wave</span> evolution. The system gives a self-consistent description of the ring current ions and ion cyclotron <span class="hlt">waves</span> in a quasilinear approach. These equations for the ion phase space distribution function and for the <span class="hlt">wave</span> power spectral density were solved on aglobal magnetospheric scale undernonsteady state conditions during the 2-5 May 1998 storm. The structure and dynamics of the ring current proton precipitating flux regions and the ion cyclotron <span class="hlt">wave</span>-active <span class="hlt">zones</span> during extreme geomagnetic disturbances on 4 May 1998 are presented and discussed in detail.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JMagR.210..126M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JMagR.210..126M"><span>Continuous-<span class="hlt">wave</span> EPR at 275 GHz: Application to high-spin Fe 3+ systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mathies, G.; Blok, H.; Disselhorst, J. A. J. M.; Gast, P.; van der Meer, H.; Miedema, D. M.; Almeida, R. M.; Moura, J. J. G.; Hagen, W. R.; Groenen, E. J. J.</p> <p>2011-05-01</p> <p>The 275 GHz electron-paramagnetic-resonance spectrometer we reported on in 2004 has been equipped with a new probe <span class="hlt">head</span>, which contains a cavity especially designed for operation in continuous-<span class="hlt">wave</span> mode. The sensitivity and signal stability that is achieved with this new probe <span class="hlt">head</span> is illustrated with 275 GHz continuous-<span class="hlt">wave</span> spectra of a 1 mM frozen solution of the complex Fe(III)-ethylenediamine tetra-acetic acid and of 10 mM frozen solutions of the protein rubredoxin, which contains Fe 3+ in its active site, from three different organisms. The high quality of the spectra of the rubredoxins allows the determination of the zero-field-splitting parameters with an accuracy of 0.5 GHz. The success of our approach results partially from the enhanced absolute sensitivity, which can be reached using a single-mode cavity. At least as important is the signal stability that we were able to achieve with the new probe <span class="hlt">head</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70185376','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70185376"><span>Characterization of a high-transmissivity <span class="hlt">zone</span> by well test analysis: Steady state case</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tiedeman, Claire; Hsieh, Paul A.; Christian, Sarah B.</p> <p>1995-01-01</p> <p>A method is developed to analyze steady horizontal flow to a well pumped from a confined aquifer composed of two homogeneous <span class="hlt">zones</span> with contrasting transmissivities. <span class="hlt">Zone</span> 1 is laterally unbounded and encloses <span class="hlt">zone</span> 2, which is elliptical in shape and is several orders of magnitude more transmissive than <span class="hlt">zone</span> 1. The solution for <span class="hlt">head</span> is obtained by the boundary integral equation method. Nonlinear least squares regression is used to estimate the model parameters, which include the transmissivity of <span class="hlt">zone</span> 1, and the location, size, and orientation of <span class="hlt">zone</span> 2. The method is applied to a hypothetical aquifer where <span class="hlt">zone</span> 2 is a long and narrow <span class="hlt">zone</span> of vertical fractures. Synthetic data are generated from three different well patterns, representing different areal coverage and proximity to the fracture <span class="hlt">zone</span>. When <span class="hlt">zone</span> 1 of the hypothetical aquifer is homogeneous, the method correctly estimates all model parameters. When <span class="hlt">zone</span> 1 is a randomly heterogeneous transmissivity field, some parameter estimates, especially the length of <span class="hlt">zone</span> 2, become highly uncertain. To reduce uncertainty, the pumped well should be close to the fracture <span class="hlt">zone</span>, and surrounding observation wells should cover an area similar in dimension to the length of the fracture <span class="hlt">zone</span>. Some prior knowledge of the fracture <span class="hlt">zone</span>, such as that gained from a surface geophysical survey, would greatly aid in designing the well test.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15014496','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15014496"><span>Seismic reflection imaging of two megathrust shear <span class="hlt">zones</span> in the northern Cascadia subduction <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Calvert, Andrew J</p> <p>2004-03-11</p> <p>At convergent continental margins, the relative motion between the subducting oceanic plate and the overriding continent is usually accommodated by movement along a single, thin interface known as a megathrust. Great thrust earthquakes occur on the shallow part of this interface where the two plates are locked together. Earthquakes of lower magnitude occur within the underlying oceanic plate, and have been linked to geochemical dehydration reactions caused by the plate's descent. Here I present deep seismic reflection data from the northern Cascadia subduction <span class="hlt">zone</span> that show that the inter-plate boundary is up to 16 km thick and comprises two megathrust shear <span class="hlt">zones</span> that bound a >5-km-thick, approximately 110-km-wide region of imbricated crustal rocks. Earthquakes within the subducting plate occur predominantly in two geographic bands where the dip of the plate is inferred to increase as it is forced around the edges of the imbricated inter-plate boundary <span class="hlt">zone</span>. This implies that seismicity in the subducting slab is controlled primarily by deformation in the upper part of the plate. Slip on the shallower megathrust shear <span class="hlt">zone</span>, which may occur by aseismic slow slip, will transport crustal rocks into the upper mantle above the subducting oceanic plate and may, in part, provide an explanation for the unusually low seismic <span class="hlt">wave</span> speeds that are observed there.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008SPIE.6937E..3CP','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008SPIE.6937E..3CP"><span><span class="hlt">Head</span> related transfer functions measurement and processing for the purpose of creating a spatial sound environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pec, Michał; Bujacz, Michał; Strumiłło, Paweł</p> <p>2008-01-01</p> <p>The use of <span class="hlt">Head</span> Related Transfer Functions (HRTFs) in audio processing is a popular method of obtaining spatialized sound. HRTFs describe disturbances caused in the sound <span class="hlt">wave</span> by the human body, especially by <span class="hlt">head</span> and the ear pinnae. Since these shapes are unique, HRTFs differ greatly from person to person. For this reason measurement of personalized HRTFs is justified. Measured HRTFs also need further processing to be utilized in a system producing spatialized sound. This paper describes a system designed for efficient collecting of <span class="hlt">Head</span> Related Transfer Functions as well as the measurement, interpolation and verification procedures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070013788&hterms=distribution+normal&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddistribution%2Bnormal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070013788&hterms=distribution+normal&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddistribution%2Bnormal"><span>Effect of EMIC <span class="hlt">Wave</span> Normal Angle Distribution on Relativistic Electron Scattering</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gamayunov, K. V.; Khazanov, G. V.</p> <p>2006-01-01</p> <p>The flux level of outer-<span class="hlt">zone</span> relativistic electrons (above 1 MeV) is extremely variable during geomagnetic storms, and controlled by a competition between acceleration and loss. Precipitation of these electrons due to resonant pitch-angle scattering by electromagnetic ion cyclotron (EMIC) <span class="hlt">waves</span> is considered one of the major loss mechanisms. This mechanism was suggested in early theoretical studies more than three decades ago. However, direct experimental evidence of the <span class="hlt">wave</span> role in relativistic electrons precipitation is difficult to obtain because of lack of concurrent measurements of precipitating electrons at low altitudes and the <span class="hlt">waves</span> in a magnetically conjugate equatorial region. Recently, the data from balloon-borne X-ray instruments provided indirect but strong evidence on an efficiency of the EMIC <span class="hlt">wave</span> induced loss for the outer-<span class="hlt">zone</span> relativistic electrons. These observations stimulated theoretical studies that, particularly, demonstrated that EMIC <span class="hlt">wave</span> induced pitch-angle diffusion of MeV electrons can operate in the strong diffusion limit and this mechanism can compete with relativistic electron depletion caused by the Dst effect during the initial and main phases of storm. Although an effectiveness of relativistic electron scattering by EMIC <span class="hlt">waves</span> depends strongly on the <span class="hlt">wave</span> spectral properties, the most favorable assumptions regarding <span class="hlt">wave</span> characteristics has been made in all previous theoretical studies. Particularly, only quasi field-aligned EMIC <span class="hlt">waves</span> have been considered as a driver for relativistic electron loss. At the same time, there is growing experimental and theoretical evidence that these <span class="hlt">waves</span> can be highly oblique; EMIC <span class="hlt">wave</span> energy can occupy not only the region of generation, i.e. the region of small <span class="hlt">wave</span> normal angles, but also the entire <span class="hlt">wave</span> normal angle region, and even only the region near 90 degrees. The latter can dramatically change he effectiveness of relativistic electron scattering by EMIC <span class="hlt">waves</span>. In the present study, we</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4807601','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4807601"><span>Parent Involvement in <span class="hlt">Head</span> Start and Children’s Development: Indirect Effects Through Parenting</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ansari, Arya; Gershoff, Elizabeth</p> <p>2015-01-01</p> <p>The authors examined the extent to which parent involvement in <span class="hlt">Head</span> Start programs predicted changes in both parent and child outcomes over time, using a nationally representative sample of 1,020 three-year-old children over 3 <span class="hlt">waves</span> of the Family and Child Experiences Survey. Center policies that promote involvement predicted greater parent involvement, and parents who were more involved in <span class="hlt">Head</span> Start centers demonstrated increased cognitive stimulation and decreased spanking and controlling behaviors. In turn, these changes in parenting behaviors were associated with gains in children’s academic and behavioral skills. These findings suggest that <span class="hlt">Head</span> Start programs should do even more to facilitate parent involvement because it can serve as an important means for promoting both parent and child outcomes. PMID:27022200</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V11B0578W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V11B0578W"><span>Crustal P-<span class="hlt">Wave</span> Speed Structure Under Mount St. Helens From Local Earthquake Tomography</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.; Moran, S. C.</p> <p>2006-12-01</p> <p>We used local earthquake data to model the P-<span class="hlt">wave</span> speed structure of Mount St. Helens with the aim of improving our understanding of the active magmatic system. Our study used new data recorded by a dense array of 19 broadband seismographs that were deployed during the current eruption together with permanent network data recorded since the May 18, 1980 eruption. Most earthquakes around Mount St. Helens during the last 25 years were clustered in a narrow vertical column beneath the volcano from the surface to a depth of about 10 km. Earthquakes also occurred in a well-defined <span class="hlt">zone</span> extending to the NNW from the volcano known as the St. Helens Seismic <span class="hlt">Zone</span> (SHZ). During the current eruption, earthquakes have been confined to within 3 km of the surface beneath the crater floor. These earthquakes apparently radiate little shear-<span class="hlt">wave</span> energy and the shear arrivals are usually contaminated by surface <span class="hlt">waves</span>. Thus, we focused on developing an improved P- <span class="hlt">wave</span> speed model. We used two data sources: (1) the short-period, vertical-component Pacific Northwest Seismograph Network and (2) new data recorded on a temporary array between June 2005 and February 2006. We first solved for a minimum one-dimensional model, incorporating the Moho depth found during an earlier wide-aperture refraction study. The three-dimensional model was solved simultaneously with hypocenter locations using the computer code SIMULPS14, extended for full three-dimensional ray shooting. We modified the code to force raypaths to remain below the ground surface. We began with large grid spacing and progressed to smaller grid spacing where the earthquakes and stations were denser. In this way we achieve a 40 km by 40 km regional model as well as a 10 km by 10 km fine-scale model directly beneath Mount St. Helens. The large-scale model is consistent with mapped geology and other geophysical data in the vicinity of Mount St. Helens. For example, there is a <span class="hlt">zone</span> of relatively low velocities (-2% to -5% lower</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/2002ASAJ..112R2363W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002ASAJ..112R2363W"><span>Study on ambient noise generated from breaking <span class="hlt">waves</span> simulated by a <span class="hlt">wave</span> maker in a tank</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wei, Ruey-Chang; Chan, Hsiang-Chih</p> <p>2002-11-01</p> <p>This paper studies ambient noise in the surf <span class="hlt">zone</span> that was simulated by a piston-type <span class="hlt">wave</span> maker in a tank. The experiment analyzed the bubbles of a breaking <span class="hlt">wave</span> by using a hydrophone to receive the acoustic signal, and the images of bubbles were recorded by a digital video camera to observe the distribution of the bubbles. The slope of the simulated seabed is 1:5, and the dimensions of the water tank are 35 m x1 m x1.2 m. The studied parameters of ambient noise generated by breaking <span class="hlt">wave</span> bubbles were <span class="hlt">wave</span> height, period, and water depth. Short-time Fourier transform was applied to obtain the acoustic spectrum of bubbles, MATLAB programs were used to calculate mean sound pressure level, and determine the number of bubbles. Bubbles with resonant frequency from 0.5 to 10 kHz were studied, counted from peaks in the spectrum. The number of bubbles generated by breaking <span class="hlt">waves</span> could be estimated by the bubbles energy distributions. The sound pressure level of ambient noise was highly related to the <span class="hlt">wave</span> height and period, with correlation coefficient 0.7.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.2205R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.2205R"><span>Current-induced dissipation in spectral <span class="hlt">wave</span> models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rapizo, H.; Babanin, A. V.; Provis, D.; Rogers, W. E.</p> <p>2017-03-01</p> <p>Despite many recent developments of the parameterization for <span class="hlt">wave</span> dissipation in spectral models, it is evident that when <span class="hlt">waves</span> propagate onto strong adverse currents the rate of energy dissipation is not properly estimated. The issue of current-induced dissipation is studied through a comprehensive data set in the tidal inlet of Port Phillip <span class="hlt">Heads</span>, Australia. The <span class="hlt">wave</span> parameters analyzed are significantly modulated by the tidal currents. <span class="hlt">Wave</span> height in conditions of opposing currents (ebb tide) can reach twice the offshore value, whereas during coflowing currents (flood), it can be reduced to half. The wind-<span class="hlt">wave</span> model SWAN is able to reproduce the tide-induced modulation of <span class="hlt">waves</span> and the results show that the variation of currents is the dominant factor in modifying the <span class="hlt">wave</span> field. In stationary simulations, the model provides an accurate representation of <span class="hlt">wave</span> height for slack and flood tides. During ebb tides, <span class="hlt">wave</span> energy is highly overestimated over the opposing current jet. None of the four parameterizations for <span class="hlt">wave</span> dissipation tested performs satisfactorily. A modification to enhance dissipation as a function of the local currents is proposed. It consists of the addition of a factor that represents current-induced <span class="hlt">wave</span> steepening and it is scaled by the ratio of spectral energy to the threshold breaking level. The new term asymptotes to the original form as the current in the <span class="hlt">wave</span> direction tends to zero. The proposed modification considerably improves <span class="hlt">wave</span> height and mean period in conditions of adverse currents, whereas the good model performance in coflowing currents is unaltered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013726','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013726"><span>An Integrative <span class="hlt">Wave</span> Model for the Marginal Ice <span class="hlt">Zone</span> Based on a Rheological Parameterization</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>2015) Characterizing the behavior of gravity <span class="hlt">wave</span> propagation into a floating or submerged viscous layer , 2015 AGU Joint Assembly Meeting, May 3–7...are the PI and a PhD student. Task 1: Use an analytical method to determine the propagation of <span class="hlt">waves</span> through a floating viscoelastic mat for a wide...and Ben Holt. 2 Task 3: Assemble all existing laboratory and field data of <span class="hlt">wave</span> propagation in ice covers. Task 4: Determine if all existing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PEPI..250....1S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PEPI..250....1S"><span>Significant seismic anisotropy beneath southern Tibet inferred from splitting of direct S-<span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Singh, Arun; Eken, Tuna; Mohanty, Debasis D.; Saikia, Dipankar; Singh, Chandrani; Ravi Kumar, M.</p> <p>2016-01-01</p> <p>This study presents a total of 12008 shear <span class="hlt">wave</span> splitting measurements obtained using the reference-station technique applied to direct S-<span class="hlt">waves</span> from 106 earthquakes recorded at 143 seismic stations of the Hi-CLIMB seismic network. The results reveal significant anisotropy in regions of southern Tibet where null or negligible anisotropy has been hitherto reported from SK(K)S measurements. While the individual fast polarization direction (FPD) at each station are found to be consistent, the splitting time delays (TDs) exhibit deviations particularly at stations located south of the Indus-Tsangpo Suture <span class="hlt">Zone</span>. The fast polarization directions (FPDs) are oriented (a) NE-SW to E-W to the south of the Indus-Tsangpo Suture <span class="hlt">Zone</span> (b) NE-SW to ENE-SSW between Bangong-Nujiang Suture <span class="hlt">Zone</span> and the Indus-Tsangpo Suture <span class="hlt">Zone</span> (ITSZ) and (c) E-W to the extreme north of the profile. The splitting time delays (δt) vary between 0.45 and 1.3 s south of the ITSZ (<30°N latitude), while they range from 0.9 to 1.4 s north of it. The overall trends are similar to SKS/SKKS results. However, the differences may be due to the not so near vertical paths of direct S <span class="hlt">waves</span> which may sample the anisotropy in a different way in comparison to SKS <span class="hlt">waves</span>, or insufficient number of SKS observations. The significant anisotropy (∼ 0.8 s) observed beneath Himalaya reveals a complex deformation pattern in the region and can be best explained by the combined effects of deformation related to shear at the base of the lithosphere and subduction related flows with possible contributions from the crust. Additional measurements obtained using direct S-<span class="hlt">waves</span> provide new constraints in regions with complex anisotropy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830056111&hterms=Solar+system+facts&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DSolar%2Bsystem%2Bfacts','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830056111&hterms=Solar+system+facts&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DSolar%2Bsystem%2Bfacts"><span>On the large-scale dynamics of rapidly rotating convection <span class="hlt">zones</span>. [in solar and stellar interiors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Durney, B. R.</p> <p>1983-01-01</p> <p>The fact that the values of the eight basic <span class="hlt">waves</span> present in turbulent flows in the presence of rotation prohibit a tilt of eddy towards the axis of rotation is incorporated into a formalism for rapidly rotating convection <span class="hlt">zones</span>. Equations for turbulent velocities are defined in a rotating coordinate system, assuming that gravity and grad delta T act in a radial direction. An expression is derived for the lifetime of a basic <span class="hlt">wave</span> and then for the average velocity vector. A real convective eddy is formulated and the <span class="hlt">wave</span> vectors are calculated. The velocity amplitude and the stress tensor amplitude are integrated over the eddy domain. Applied to the solar convective <span class="hlt">zone</span>, it is found that the convective cells are aligned along the axis of rotation at the poles and at the equator, a model that conflicts with nonrotating mixng length theory predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4226S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4226S"><span>Research Centre for the Study of the Rogue <span class="hlt">Waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shamin, Roman</p> <p>2013-04-01</p> <p>In 2012, in Sakhalin (Russia) was established Research Center for the Study of the Rogue <span class="hlt">Waves</span>. This center unites many known scientists, who study rogue <span class="hlt">waves</span>. The center is founded by the following scientific organizations: - The Institute of Marine Geology and Geophysics of FEB RAS - The Far Eastern Federal University - Special Research Bureau for Automation of Marine Researches of FEB RAS - The Institute of Applied Physics of RAS - Shirshov Institute of Oceanology of RAS <span class="hlt">Heads</span> this center Dr. Roman V. Shamin (Russia). Topics projects: - Probability of emergence of rogue <span class="hlt">waves</span> - Finding of the sites of the Ocean most dangerous from the point of view of rogue <span class="hlt">waves</span> - Assessment of risk of dangerous impact of rogue <span class="hlt">waves</span> - and many others... Our Center is open for new participants from all countries. Our Centre have web-site: roguewaves.ru For contacts: center@roguewaves.ru (Dr. Roman Shamin)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=330304','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=330304"><span>Self-adaptive method for high frequency multi-channel analysis of surface <span class="hlt">wave</span> method</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>When the high frequency multi-channel analysis of surface <span class="hlt">waves</span> (MASW) method is conducted to explore soil properties in the vadose <span class="hlt">zone</span>, existing rules for selecting the near offset and spread lengths cannot satisfy the requirements of planar dominant Rayleigh <span class="hlt">waves</span> for all frequencies of interest ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006ShWav..16....1B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006ShWav..16....1B"><span>Shock <span class="hlt">wave</span> attenuation by grids and orifice plates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Britan, A.; Igra, O.; Ben-Dor, G.; Shapiro, H.</p> <p>2006-11-01</p> <p>The interaction of weak shock <span class="hlt">waves</span> with porous barriers of different geometries and porosities is examined. Installing a barrier inside the shock tube test section will cause the development of the following <span class="hlt">wave</span> pattern upon a <span class="hlt">head</span>-on collision between the incident shock <span class="hlt">wave</span> and the barrier: a reflected shock from the barrier and a transmitted shock propagating towards the shock tube end wall. Once the transmitted shock <span class="hlt">wave</span> reaches the end wall it is reflected back towards the barrier. This is the beginning of multiple reflections between the barrier and the end wall. This full cycle of shock reflections/interactions resulting from the incident shock <span class="hlt">wave</span> collision with the barrier can be studied in a single shock tube test. A one-dimensional (1D), inviscid flow model was proposed for simulating the flow resulting from the initial collision of the incident shock <span class="hlt">wave</span> with the barrier. Fairly good agreement is found between experimental findings and simulations based on a 1D flow model. Based on obtained numerical and experimental findings an optimal design procedure for shock <span class="hlt">wave</span> attenuator is suggested. The suggested attenuator may ensure the safety of the shelter’s ventilation systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997JAP....81.7193T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997JAP....81.7193T"><span>Detonation <span class="hlt">waves</span> in pentaerythritol tetranitrate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tarver, Craig M.; Breithaupt, R. Don; Kury, John W.</p> <p>1997-06-01</p> <p>Fabry-Perot laser interferometry was used to obtain nanosecond time resolved particle velocity histories of the free surfaces of tantalum discs accelerated by detonating pentaerythritol tetranitrate (PETN) charges and of the interfaces between PETN detonation products and lithium fluoride crystals. The experimental records were compared to particle velocity histories calculated using very finely <span class="hlt">zoned</span> meshes of the exact dimensions with the DYNA2D hydrodynamic code. The duration of the PETN detonation reaction <span class="hlt">zone</span> was demonstrated to be less than the 5 ns initial resolution of the Fabry-Perot technique, because the experimental records were accurately calculated using an instantaneous chemical reaction, the Chapman-Jouguet (C-J) model of detonation, and the reaction product Jones-Wilkins-Lee (JWL) equation of state for PETN detonation products previously determined by supracompression (overdriven detonation) studies. Some of the PETN charges were pressed to densities approaching the crystal density and exhibited the phenomenon of superdetonation. An ignition and growth Zeldovich-von Neumann-Doring (ZND) reactive flow model was developed to explain these experimental records and the results of previous PETN shock initiation experiments on single crystals of PETN. Good agreement was obtained for the induction time delays preceding chemical reaction, the run distances at which the initial shock <span class="hlt">waves</span> were overtaken by the detonation <span class="hlt">waves</span> in the compressed PETN, and the measured particle velocity histories produced by the overdriven detonation <span class="hlt">waves</span> before they could relax to steady state C-J velocity and pressure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20165113','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20165113"><span>Three-dimensional imaging from a unidirectional hologram: wide-viewing-<span class="hlt">zone</span> projection type.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Okoshi, T; Oshima, K</p> <p>1976-04-01</p> <p>In ordinary holography reconstructing a virtual image, the hologram must be wider than either the visual field or the viewing <span class="hlt">zone</span>. In this paper, an economical method of recording a wide-viewing-<span class="hlt">zone</span> wide-visual-field 3-D holographic image is proposed. In this method, many mirrors are used to collect object <span class="hlt">waves</span> onto a small hologram. In the reconstruction, a real image from the hologram is projected onto a horizontally direction-selective stereoscreen through the same mirrors. In the experiment, satisfactory 3-D images have been observed from a wide viewing <span class="hlt">zone</span>. The optimum design and information reduction techniques are also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.723..223D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.723..223D"><span>Strength of plate coupling in the southern Ryukyu subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Doo, Wen-Bin; Lo, Chung-Liang; Wu, Wen-Nan; Lin, Jing-Yi; Hsu, Shu-Kun; Huang, Yin-Sheng; Wang, Hsueh-Fen</p> <p>2018-01-01</p> <p>Understanding the strength of a plate coupling is critical for assessing potential seismic and tsunamic hazards in subduction <span class="hlt">zones</span>. The interaction between an overriding plate and the associated subducting plate can be used to evaluate the strength of plate coupling by examining the mantle lithospheric buoyancy. Here, we calculate the mantle lithosphere buoyancy across the northern portion of the southern Ryukyu subduction <span class="hlt">zone</span> based on gravity modeling with the constraints from a newly derived P-<span class="hlt">wave</span> seismic velocity model. The result indicates that the strength of the plate coupling in the study area is relatively strong, which is consistent with previous observations in the southernmost Ryukyu subduction <span class="hlt">zone</span>. Because few large earthquakes (Mw > 7) have occurred in the southern Ryukyu subduction <span class="hlt">zone</span>, a large amount of energy is locked and accumulated by plate coupling, that could be released in the near future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013CEJPh..11..760R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013CEJPh..11..760R"><span>Analysis of two colliding fractionally damped spherical shells in modelling blunt human <span class="hlt">head</span> impacts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rossikhin, Yury A.; Shitikova, Marina V.</p> <p>2013-06-01</p> <p>The collision of two elastic or viscoelastic spherical shells is investigated as a model for the dynamic response of a human <span class="hlt">head</span> impacted by another <span class="hlt">head</span> or by some spherical object. Determination of the impact force that is actually being transmitted to bone will require the model for the shock interaction of the impactor and human <span class="hlt">head</span>. This model is indended to be used in simulating crash scenarios in frontal impacts, and provide an effective tool to estimate the severity of effect on the human <span class="hlt">head</span> and to estimate brain injury risks. The model developed here suggests that after the moment of impact quasi-longitudinal and quasi-transverse shock <span class="hlt">waves</span> are generated, which then propagate along the spherical shells. The solution behind the <span class="hlt">wave</span> fronts is constructed with the help of the theory of discontinuities. It is assumed that the viscoelastic features of the shells are exhibited only in the contact domain, while the remaining parts retain their elastic properties. In this case, the contact spot is assumed to be a plane disk with constant radius, and the viscoelastic features of the shells are described by the fractional derivative standard linear solid model. In the case under consideration, the governing differential equations are solved analytically by the Laplace transform technique. It is shown that the fractional parameter of the fractional derivative model plays very important role, since its variation allows one to take into account the age-related changes in the mechanical properties of bone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011ECSS...95..349H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011ECSS...95..349H"><span>The use of remote sensing and linear <span class="hlt">wave</span> theory to model local <span class="hlt">wave</span> energy around Alphonse Atoll, Seychelles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hamylton, S.</p> <p>2011-12-01</p> <p>This paper demonstrates a practical step-wise method for modelling <span class="hlt">wave</span> energy at the landscape scale using GIS and remote sensing techniques at Alphonse Atoll, Seychelles. Inputs are a map of the benthic surface (seabed) cover, a detailed bathymetric model derived from remotely sensed Compact Airborne Spectrographic Imager (CASI) data and information on regional <span class="hlt">wave</span> heights. Incident energy at the reef crest around the atoll perimeter is calculated as a function of its deepwater value with <span class="hlt">wave</span> parameters (significant <span class="hlt">wave</span> height and period) hindcast in the offshore <span class="hlt">zone</span> using the <span class="hlt">Wave</span>Watch III application developed by the National Oceanographic and Atmospheric Administration. Energy modifications are calculated at constant intervals as <span class="hlt">waves</span> transform over the forereef platform along a series of reef profile transects running into the atoll centre. Factors for shoaling, refraction and frictional attenuation are calculated at each interval for given changes in bathymetry and benthic coverage type and a nominal reduction in absolute energy is incorporated at the reef crest to account for <span class="hlt">wave</span> breaking. Overall energy estimates are derived for a period of 5 years and related to spatial patterning of reef flat surface cover (sand and seagrass patches).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001SPIE.4361....1R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001SPIE.4361....1R"><span>Multispectral image-fused <span class="hlt">head</span>-tracked vision system (HTVS) for driving applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reese, Colin E.; Bender, Edward J.</p> <p>2001-08-01</p> <p>Current military thermal driver vision systems consist of a single Long <span class="hlt">Wave</span> Infrared (LWIR) sensor mounted on a manually operated gimbal, which is normally locked forward during driving. The sensor video imagery is presented on a large area flat panel display for direct view. The Night Vision and Electronics Sensors Directorate and Kaiser Electronics are cooperatively working to develop a driver's <span class="hlt">Head</span> Tracked Vision System (HTVS) which directs dual waveband sensors in a more natural <span class="hlt">head</span>-slewed imaging mode. The HTVS consists of LWIR and image intensified sensors, a high-speed gimbal, a <span class="hlt">head</span> mounted display, and a <span class="hlt">head</span> tracker. The first prototype systems have been delivered and have undergone preliminary field trials to characterize the operational benefits of a <span class="hlt">head</span> tracked sensor system for tactical military ground applications. This investigation will address the advantages of <span class="hlt">head</span> tracked vs. fixed sensor systems regarding peripheral sightings of threats, road hazards, and nearby vehicles. An additional thrust will investigate the degree to which additive (A+B) fusion of LWIR and image intensified sensors enhances overall driving performance. Typically, LWIR sensors are better for detecting threats, while image intensified sensors provide more natural scene cues, such as shadows and texture. This investigation will examine the degree to which the fusion of these two sensors enhances the driver's overall situational awareness.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160011505','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160011505"><span>Beam <span class="hlt">Wave</span> Considerations for Optical Link Budget Calculations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Manning, Robert M.</p> <p>2016-01-01</p> <p>The bounded beam <span class="hlt">wave</span> nature of electromagnetic radiation emanating from a finite size aperture is considered for diffraction-based link power budget calculations for an optical communications system. Unlike at radio frequency wavelengths, diffraction effects are very important at optical wavelengths. In the general case, the situation cannot be modeled by supposing isotropic radiating antennas and employing the concept of effective isotropic radiated power. It is shown here, however, that these considerations are no more difficult to treat than spherical-<span class="hlt">wave</span> isotopic based calculations. From first principles, a general expression governing the power transfer for a collimated beam <span class="hlt">wave</span> is derived and from this are defined the three regions of near-field, first Fresnel <span class="hlt">zone</span>, and far-field behavior. Corresponding equations for the power transfer are given for each region. It is shown that although the well-known linear expressions for power transfer in the far-field hold for all distances between source and receiver in the radio frequency case, nonlinear behavior within the first Fresnel <span class="hlt">zone</span> must be accounted for in the optical case at 1550 nm with typical aperture sizes at source/receiver separations less that 100 km.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19740045030&hterms=Venkataraman&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DVenkataraman','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19740045030&hterms=Venkataraman&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DVenkataraman"><span>Alfven <span class="hlt">waves</span> associated with long cylindrical satellites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Venkataraman, N. S.; Gustafson, W. A.</p> <p>1973-01-01</p> <p>The Alfven <span class="hlt">wave</span> excited by a long cylindrical satellite moving with a constant velocity at an angle relative to a uniform magnetic field has been calculated. Assuming a plasma with infinite conductivity, the linearized momentum equation and Maxwell's equations are applied to a cylindrical satellite carrying a variable current. The induced magnetic field is determined, and it is shown that the Alfven disturbance <span class="hlt">zone</span> is of limited extent, depending on the satellite shape. The <span class="hlt">wave</span> drag coefficient is calculated and shown to be small compared to the induction drag coefficient at all altitudes considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ThApC.129..341O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ThApC.129..341O"><span>On validation of the rain climatic <span class="hlt">zone</span> designations for Nigeria</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Obiyemi, O. O.; Ibiyemi, T. S.; Ojo, J. S.</p> <p>2017-07-01</p> <p>In this paper, validation of rain climatic <span class="hlt">zone</span> classifications for Nigeria is presented based on global radio-climatic models by the International Telecommunication Union-Radiocommunication (ITU-R) and Crane. Rain rate estimates deduced from several ground-based measurements and those earlier estimated from the precipitation index on the Tropical Rain Measurement Mission (TRMM) were employed for the validation exercise. Although earlier classifications indicated that Nigeria falls into <span class="hlt">zones</span> P, Q, N, and K for the ITU-R designations, and <span class="hlt">zones</span> E and H for Crane's climatic <span class="hlt">zone</span> designations, the results however confirmed that the rain climatic <span class="hlt">zones</span> across Nigeria can only be classified into four, namely P, Q, M, and N for the ITU-R designations, while the designations by Crane exhibited only three <span class="hlt">zones</span>, namely E, G, and H. The ITU-R classification was found to be more suitable for planning microwave and millimeter <span class="hlt">wave</span> links across Nigeria. The research outcomes are vital in boosting the confidence level of system designers in using the ITU-R designations as presented in the map developed for the rain <span class="hlt">zone</span> designations for estimating the attenuation induced by rain along satellite and terrestrial microwave links over Nigeria.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PEPI..261..141C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PEPI..261..141C"><span>Investigation of mantle kinematics beneath the Hellenic-subduction <span class="hlt">zone</span> with teleseismic direct shear <span class="hlt">waves</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Confal, Judith M.; Eken, Tuna; Tilmann, Frederik; Yolsal-Çevikbilen, Seda; Çubuk-Sabuncu, Yeşim; Saygin, Erdinc; Taymaz, Tuncay</p> <p>2016-12-01</p> <p>The subduction and roll-back of the African plate beneath the Eurasian plate along the arcuate Hellenic trench is the dominant geodynamic process in the Aegean and western Anatolia. Mantle flow and lithospheric kinematics in this region can potentially be understood better by mapping seismic anisotropy. This study uses direct shear-<span class="hlt">wave</span> splitting measurements based on the Reference Station Technique in the southern Aegean Sea to reveal seismic anisotropy in the mantle. The technique overcomes possible contamination from source-side anisotropy on direct S-<span class="hlt">wave</span> signals recorded at a station pair by maximizing the correlation between the seismic traces at reference and target stations after correcting the reference stations for known receiver-side anisotropy and the target stations for arbitrary splitting parameters probed via a grid search. We obtained splitting parameters at 35 stations with good-quality S-<span class="hlt">wave</span> signals extracted from 81 teleseismic events. Employing direct S-<span class="hlt">waves</span> enabled more stable and reliable splitting measurements than previously possible, based on sparse SKS data at temporary stations, with one to five events for local SKS studies, compared with an average of 12 events for each station in this study. The fast polarization directions mostly show NNE-SSW orientation with splitting time delays between 1.15 s and 1.62 s. Two stations in the west close to the Hellenic Trench and one in the east show N-S oriented fast polarizations. In the back-arc region three stations exhibit NE-SW orientation. The overall fast polarization variations tend to be similar to those obtained from previous SKS splitting studies in the region but indicate a more consistent pattern, most likely due to the usage of a larger number of individual observations in direct S-<span class="hlt">wave</span> derived splitting measurements. Splitting analysis on direct shear <span class="hlt">waves</span> typically resulted in larger split time delays compared to previous studies, possibly because S-<span class="hlt">waves</span> travel along a longer path</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRA..122.5431L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRA..122.5431L"><span>Roles of whistler mode <span class="hlt">waves</span> and magnetosonic <span class="hlt">waves</span> in changing the outer radiation belt and the slot region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, L. Y.; Yu, J.; Cao, J. B.; Yang, J. Y.; Li, X.; Baker, D. N.; Reeves, G. D.; Spence, H.</p> <p>2017-05-01</p> <p>Using the Van Allen Probe long-term (2013-2015) observations and quasi-linear simulations of <span class="hlt">wave</span>-particle interactions, we examine the combined or competing effects of whistler mode <span class="hlt">waves</span> (chorus or hiss) and magnetosonic (MS) <span class="hlt">waves</span> on energetic (<0.5 MeV) and relativistic (>0.5 MeV) electrons inside and outside the plasmasphere. Although whistler mode chorus <span class="hlt">waves</span> and MS <span class="hlt">waves</span> can singly or jointly accelerate electrons from the hundreds of keV energy to the MeV energy in the low-density trough, most of the relativistic electron enhancement events are best correlated with the chorus <span class="hlt">wave</span> emissions outside the plasmapause. Inside the plasmasphere, intense plasmaspheric hiss can cause the net loss of relativistic electrons via persistent pitch angle scattering, regardless of whether MS <span class="hlt">waves</span> were present or not. The intense hiss <span class="hlt">waves</span> not only create the energy-dependent electron slot region but also remove a lot of the outer radiation belt electrons when the expanding dayside plasmasphere frequently covers the outer <span class="hlt">zone</span>. Since whistler mode <span class="hlt">waves</span> (chorus or hiss) can resonate with more electrons than MS <span class="hlt">waves</span>, they play dominant roles in changing the outer radiation belt and the slot region. However, MS <span class="hlt">waves</span> can accelerate the energetic electrons below 400 keV and weaken their loss inside the plasmapause. Thus, MS <span class="hlt">waves</span> and plasmaspheric hiss generate different competing effects on energetic and relativistic electrons in the high-density plasmasphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014009','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014009"><span>High-frequency sediment-level oscillations in the swash <span class="hlt">zone</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>Sallenger, A.H.; Richmond, B.M.</p> <p>1984-01-01</p> <p>Sediment-level oscillations with heights of about 6 cm and shore-normal lengths of order 10 m have been measured in the swash <span class="hlt">zone</span> of a high-energy, coarse-sand beach. Crests of oscillations were shore parallel and continuous alongshore. The oscillations were of such low steepness (height-to-length ratio approximately 0.006) that they were difficult to detect visually. The period of oscillation ranged between 6 and 15 min and decreased landward across the swash <span class="hlt">zone</span>. The sediment-level oscillations were progressive landward with an average migration rate in the middle to upper swash <span class="hlt">zone</span> of 0.8 m min-1. Migration was caused mostly by erosion on the seaward flank of the crest of an oscillation during a period of net seaward sediment transport. Thus, the observed migration was a form migration landward rather than a migration involving net landward sediment transport. The observed sediment-level oscillations were different than sand <span class="hlt">waves</span> or other swash-<span class="hlt">zone</span> bedforms previously described. ?? 1984.</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/2008JAP...104d3506B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JAP...104d3506B"><span>Lamb <span class="hlt">waves</span> in phononic crystal slabs with square or rectangular symmetries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brunet, Thomas; Vasseur, Jérôme; Bonello, Bernard; Djafari-Rouhani, Bahram; Hladky-Hennion, Anne-Christine</p> <p>2008-08-01</p> <p>We report on both numerical and experimental results showing the occurrence of band gaps for Lamb <span class="hlt">waves</span> propagating in phononic crystal plates. The structures are made of centered rectangular and square arrays of holes drilled in a silicon plate. A supercell plane <span class="hlt">wave</span> expansion method is used to calculate the band structures and to predict the position and the magnitude of the gaps. The band structures of phononic crystal slabs are then measured using a laser ultrasonic technique. Lamb <span class="hlt">waves</span> in the megahertz range and with <span class="hlt">wave</span> vectors ranging over more than the first two reduced Brillouin <span class="hlt">zones</span> are investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AcMSn..29..494X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AcMSn..29..494X"><span>Numerical study on <span class="hlt">wave</span> loads and motions of two ships advancing in <span class="hlt">waves</span> by using three-dimensional translating-pulsating source</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Yong; Dong, Wen-Cai</p> <p>2013-08-01</p> <p>A frequency domain analysis method based on the three-dimensional translating-pulsating (3DTP) source Green function is developed to investigate <span class="hlt">wave</span> loads and free motions of two ships advancing on parallel course in <span class="hlt">waves</span>. Two experiments are carried out respectively to measure the <span class="hlt">wave</span> loads and the freemotions for a pair of side-byside arranged ship models advancing with an identical speed in <span class="hlt">head</span> regular <span class="hlt">waves</span>. For comparison, each model is also tested alone. Predictions obtained by the present solution are found in favorable agreement with the model tests and are more accurate than the traditional method based on the three dimensional pulsating (3DP) source Green function. Numerical resonances and peak shift can be found in the 3DP predictions, which result from the <span class="hlt">wave</span> energy trapped in the gap between two ships and the extremely inhomogeneous <span class="hlt">wave</span> load distribution on each hull. However, they can be eliminated by 3DTP, in which the speed affects the free surface and most of the <span class="hlt">wave</span> energy can be escaped from the gap. Both the experiment and the present prediction show that hydrodynamic interaction effects on <span class="hlt">wave</span> loads and free motions are significant. The present solver may serve as a validated tool to predict <span class="hlt">wave</span> loads and motions of two vessels under replenishment at sea, and may help to evaluate the hydrodynamic interaction effects on the ships safety in replenishment operation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS41C0628H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS41C0628H"><span>Remote Sensing Characteristics of <span class="hlt">Wave</span> Breaking Rollers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haller, M. C.; Catalan, P.</p> <p>2006-12-01</p> <p>The <span class="hlt">wave</span> roller has a primary influence on the balances of mass and momentum in the surf <span class="hlt">zone</span> (e.g. Svendsen, 1984; Dally and Brown, 1995; Ruessink et al., 2001). In addition, the roller area and its angle of inclination on the <span class="hlt">wave</span> front are important quantities governing the dissipation rates in breaking <span class="hlt">waves</span> (e.g Madsen et al., 1997). Yet, there have been very few measurements published of individual breaking <span class="hlt">wave</span> roller geometries in shallow water. A number of investigators have focused on observations of the initial jet-like motion at the onset of breaking before the establishment of the <span class="hlt">wave</span> roller (e.g. Basco, 1985; Jansen, 1986), while Govender et al. (2002) provide observations of <span class="hlt">wave</span> roller vertical cross-sections and angles of inclination for a pair of laboratory <span class="hlt">wave</span> conditions. Nonetheless, presently very little is known about the growth, evolution, and decay of this aerated region of white water as it propagates through the surf <span class="hlt">zone</span>; mostly due to the inherent difficulties in making the relevant observations. The present work is focused on analyzing observations of the time and space scales of individual shallow water breaking <span class="hlt">wave</span> rollers as derived from remote sensing systems. Using a high-resolution video system in a large-scale laboratory facility, we have obtained detailed measurements of the growth and evolution of the <span class="hlt">wave</span> breaking roller. In addition, by synchronizing the remote video with in-situ <span class="hlt">wave</span> gages, we are able to directly relate the video intensity signal to the underlying <span class="hlt">wave</span> shape. Results indicate that the horizontal length scale of breaking <span class="hlt">wave</span> rollers differs significantly from the previous observations of Duncan (1981), which has been a traditional basis for roller model parameterizations. The overall approach to the video analysis is new in the sense that we concentrate on individual breaking <span class="hlt">waves</span>, as opposed to the more commonly used time-exposure technique. In addition, a new parameter of interest, denoted Imax, is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA578392','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA578392"><span>Comparison of a Physical and Numerical Mobile-Bed Model of Beach and T-<span class="hlt">Head</span> Groin Interaction</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2011-05-01</p> <p>Hydraulic Centre’s Large Area Basin (LAB), utilizing a set of moveable <span class="hlt">wave</span> generators capable of providing long-crested <span class="hlt">waves</span> to match a variety...was conducted manually from a bridge as shown in Figure 4. The location of the transect (Profile 2) is shown in Figure 2. Planform morphology was...4. Physical model oblique view showing profile measurement location and bridge . 2617 The T-<span class="hlt">head</span> groins and the shore-normal breakwater trunk at the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1053271','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1053271"><span>Small-Scale Surf <span class="hlt">Zone</span> Geometric Roughness</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-12-01</p> <p>and an image of the tie points can be seen (Figure 6). 23 Figure 6. Screen Shot of Alignment Process On the left side is the workspace which...rest of the points, producing the 3D surface. 24 Figure 7. Screen Shot of Dense Cloud Process On the left side is the workspace which...maximum 200 words) Measurements of small-scale (O(mm)) geometric roughness (kf) associated with breaking <span class="hlt">wave</span> foam were obtained within the surf <span class="hlt">zone</span> on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ShWav..28...19O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ShWav..28...19O"><span>The multi-modal responses of a physical <span class="hlt">head</span> model subjected to various blast exposure conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ouellet, S.; Philippens, M.</p> <p>2018-01-01</p> <p>The local and global biomechanical response of the body to a blast <span class="hlt">wave</span> is the first step of a sequence that leads to the development of stresses and strains which can exceed the tolerance of brain tissue. These stresses and strains may then lead to neuro-physical changes in the brain and contribute to initiate a cascade of events leading to injury. The specific biomechanical pathways by which the blast energy is transmitted through the <span class="hlt">head</span> structure are, however, not clearly understood. Multiple transmission mechanisms have been proposed to explain the generation of brain stresses following the impingement of a blast <span class="hlt">wave</span> on the <span class="hlt">head</span>. With the use of a physical <span class="hlt">head</span> model, the work presented here aims at demonstrating that the proposed transmission mechanisms are not mutually exclusive. They are part of a continuum of <span class="hlt">head</span> responses where, depending on the exposure conditions, a given mechanism may or may not dominate. This article presents the joint analysis of previous blast test results generated with the brain injury protection evaluation device (BIPED) headform under four significantly different exposure conditions. The focus of the analysis is to demonstrate how the nature of the recorded response is highly dependent on the exposure characteristics and consequently, on the method used to reproduce blast exposure in a laboratory environment. The timing and magnitude of the variations in intra-cranial pressures (ICP) were analysed relative to the external pressure field in order to better understand the <span class="hlt">wave</span> dynamics occurring within the brain structure of the headform. ICP waveforms were also analysed in terms of their energy spectral density to better identify the energy partitioning between the different modes of response. It is shown that the BIPED response is multi-modal and that the energy partitioning between its different modes of response is greatly influenced by exposure characteristics such as external peak overpressure, impulse, blast <span class="hlt">wave</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006ChPhy..15.1149X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006ChPhy..15.1149X"><span><span class="hlt">Head</span>-on collision of ring dark solitons in Bose Einstein condensates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, Ju-Kui; Peng, Ping</p> <p>2006-06-01</p> <p>The ring dark solitons and their <span class="hlt">head</span>-on collisions in a Bose-Einstein condensates with thin disc-shaped potential are studied. It is shown that the system admits a solution with two concentric ring solitons, one moving inwards and the other moving outwards, which in small-amplitude limit, are described by the two cylindrical KdV equations in the respective reference frames. By using the extended Poincaré-Lighthill-Kuo perturbation method, the analytical phase shifts following the <span class="hlt">head</span>-on collisions between two ring dark solitary <span class="hlt">waves</span> are derived. It is shown that the phase shifts decrease with the radial coordinate r according to the r-1/3 law and depend on the initial soliton amplitude and radius.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22368483','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22368483"><span>A magnetic flux leakage and magnetostrictive guided <span class="hlt">wave</span> hybrid transducer for detecting bridge cables.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xu, Jiang; Wu, Xinjun; Cheng, Cheng; Ben, Anran</p> <p>2012-01-01</p> <p>Condition assessment of cables has gained considerable attention for the bridge safety. A magnetic flux leakage and magnetostrictive guided <span class="hlt">wave</span> hybrid transducer is provided to inspect bridge cables. The similarities and differences between the two methods are investigated. The hybrid transducer for bridge cables consists of an aluminum framework, climbing modules, embedded magnetizers and a ribbon coil. The static axial magnetic field provided by the magnetizers meets the needs of the magnetic flux leakage testing and the magnetostrictive guided <span class="hlt">wave</span> testing. The magnetizers also provide the attraction for the climbing modules. In the magnetic flux leakage testing for the free length of cable, the coil induces the axial leakage magnetic field. In the magnetostrictive guided <span class="hlt">wave</span> testing for the anchorage <span class="hlt">zone</span>, the coil provides a pulse high power variational magnetic field for generating guided <span class="hlt">waves</span>; the coil induces the magnetic field variation for receiving guided <span class="hlt">waves</span>. The experimental results show that the transducer with the corresponding inspection system could be applied to detect the broken wires in the free length and in the anchorage <span class="hlt">zone</span> of bridge cables.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3279227','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3279227"><span>A Magnetic Flux Leakage and Magnetostrictive Guided <span class="hlt">Wave</span> Hybrid Transducer for Detecting Bridge Cables</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Xu, Jiang; Wu, Xinjun; Cheng, Cheng; Ben, Anran</p> <p>2012-01-01</p> <p>Condition assessment of cables has gained considerable attention for the bridge safety. A magnetic flux leakage and magnetostrictive guided <span class="hlt">wave</span> hybrid transducer is provided to inspect bridge cables. The similarities and differences between the two methods are investigated. The hybrid transducer for bridge cables consists of an aluminum framework, climbing modules, embedded magnetizers and a ribbon coil. The static axial magnetic field provided by the magnetizers meets the needs of the magnetic flux leakage testing and the magnetostrictive guided <span class="hlt">wave</span> testing. The magnetizers also provide the attraction for the climbing modules. In the magnetic flux leakage testing for the free length of cable, the coil induces the axial leakage magnetic field. In the magnetostrictive guided <span class="hlt">wave</span> testing for the anchorage <span class="hlt">zone</span>, the coil provides a pulse high power variational magnetic field for generating guided <span class="hlt">waves</span>; the coil induces the magnetic field variation for receiving guided <span class="hlt">waves</span>. The experimental results show that the transducer with the corresponding inspection system could be applied to detect the broken wires in the free length and in the anchorage <span class="hlt">zone</span> of bridge cables. PMID:22368483</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.S34C..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.S34C..04H"><span>Mojave Compliant <span class="hlt">Zone</span> Structure and Properties: Constraints from InSAR and Mechanical Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hearn, E. H.; Fialko, Y.; Finzi, Y.</p> <p>2007-12-01</p> <p>Long-lived <span class="hlt">zones</span> with significantly lower elastic strength than their surroundings are associated with active Mojave faults (e.g., Li et al., 1999; Fialko et al., 2002, 2004). In an earthquake these weak features concentrate strain, causing them to show up as anomalous, short length-scale features in SAR interferograms (Fialko et al., 2002). Fault-<span class="hlt">zone</span> trapped <span class="hlt">wave</span> studies indicate that the 1999 Hector Mine earthquake caused a small reduction in P- and S-<span class="hlt">wave</span> velocities in a compliant <span class="hlt">zone</span> along the Landers earthquake rupture (Vidale and Li, 2003). This suggests that coseismic strain concentration, and the resulting damage, in the compliant <span class="hlt">zone</span> caused a further reduction in its elastic strength. Even a small coseismic strength drop should make a compliant <span class="hlt">zone</span> (CZ) deform, in response to the total (not just the coseismic) stress. The strain should be in the sense which is compatible with the orientations and values of the region's principal stresses. However, as indicated by Fialko and co-workers (2002, 2004), the sense of coseismic strain of Mojave compliant <span class="hlt">zones</span> was consistent with coseismic stress change, not the regional (background) stress. Here we use finite-element models to investigate how InSAR measurements of Mojave compliant <span class="hlt">zone</span> coseismic strain places limits on their dimensions and on upper crustal stresses. We find that unless the CZ is shallow, narrow, and has a high Poisson's ratio (e.g., 0.4), CZ contraction under lithostatic stress overshadows deformation due to deviatoric background stress or coseismic stress change. We present ranges of CZ dimensions which are compatible with the observed surface deformation and address how these dimensions compare with new results from damage-controlled fault evolution models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820033934&hterms=Gaze+nystagmus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DGaze%2Bnystagmus','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820033934&hterms=Gaze+nystagmus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DGaze%2Bnystagmus"><span>Active <span class="hlt">head</span> rotations and eye-<span class="hlt">head</span> coordination</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zangemeister, W. H.; Stark, L.</p> <p>1981-01-01</p> <p>It is pointed out that <span class="hlt">head</span> movements play an important role in gaze. The interaction between eye and <span class="hlt">head</span> movements involves both their shared role in directing gaze and the compensatory vestibular ocular reflex. The dynamics of <span class="hlt">head</span> trajectories are discussed, taking into account the use of parameterization to obtain the peak velocity, peak accelerations, the times of these extrema, and the duration of the movement. Attention is given to the main sequence, neck muscle EMG and details of the <span class="hlt">head</span>-movement trajectory, types of <span class="hlt">head</span> model accelerations, the latency of eye and <span class="hlt">head</span> movement in coordinated gaze, gaze latency as a function of various factors, and coordinated gaze types. Clinical examples of gaze-plane analysis are considered along with the instantaneous change of compensatory eye movement (CEM) gain, and aspects of variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AdWR..110...59O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AdWR..110...59O"><span>Vortex-induced suspension of sediment in the surf <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Otsuka, Junichi; Saruwatari, Ayumi; Watanabe, Yasunori</p> <p>2017-12-01</p> <p>A major mechanism of sediment suspension by organized vortices produced under violent breaking <span class="hlt">waves</span> in the surf <span class="hlt">zone</span> was identified through physical and computational experiments. Counter-rotating flows within obliquely descending eddies produced between adjacent primary roller vortices induce transverse convergent near-bed flows, driving bed load transport to form regular patterns of transverse depositions. The deposited sediment is then rapidly ejected by upward carrier flows induced between the vortices. This mechanism of vortex-induced suspension is supported by experimental evidence that coherent sediment clouds are ejected where the obliquely descending eddies reach the sea bed after the breaking <span class="hlt">wave</span> front has passed. In addition to the effects of settling and turbulent diffusion caused by breaking <span class="hlt">waves</span>, the effect of the vortex-induced flows was incorporated into a suspension model on the basis of vorticity dynamics and parametric characteristics of transverse flows in breaking <span class="hlt">waves</span>. The model proposed here reasonably predicts an exponential attenuation of the measured sediment concentration due to violent plunging <span class="hlt">waves</span> and significantly improves the underprediction of the concentration produced by previous models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22251975-magnetosonic-waves-interactions-spin-degenerate-quantum-plasma','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22251975-magnetosonic-waves-interactions-spin-degenerate-quantum-plasma"><span>Magnetosonic <span class="hlt">waves</span> interactions in a spin-1/2 degenerate quantum plasma</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>Li, Sheng-Chang, E-mail: lsc1128lsc@126.com; Han, Jiu-Ning</p> <p>2014-03-15</p> <p>We investigate the magnetosonic <span class="hlt">waves</span> and their interactions in a spin-1/2 degenerate quantum plasma. With the help of the extended Poincaré-Lighthill-Kuo perturbation method, we derive two Korteweg-de Vries-Burgers equations to describe the magnetosonic <span class="hlt">waves</span>. The parameter region where exists magnetosonic <span class="hlt">waves</span> and the phase diagram of the compressive and rarefactive solitary <span class="hlt">waves</span> with different plasma parameters are shown. We further explore the effects of quantum diffraction, quantum statistics, and electron spin magnetization on the <span class="hlt">head</span>-on collisions of magnetosonic solitary <span class="hlt">waves</span>. We obtain the collision-induced phase shifts (trajectory changes) analytically. Both for the compressive and rarefactive solitary <span class="hlt">waves</span>, it is foundmore » that the collisions only lead to negative phase shifts. Our present study should be useful to understand the collective phenomena related to the magnetosonic <span class="hlt">wave</span> collisions in degenerate plasmas like those in the outer shell of massive white dwarfs as well as to the potential applications of plasmas.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJST.226.1867M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJST.226.1867M"><span>Multiple scroll <span class="hlt">wave</span> chimera states</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maistrenko, Volodymyr; Sudakov, Oleksandr; Osiv, Oleksiy; Maistrenko, Yuri</p> <p>2017-06-01</p> <p>We report the appearance of three-dimensional (3D) multiheaded chimera states that display cascades of self-organized spatiotemporal patterns of coexisting coherence and incoherence. We demonstrate that the number of incoherent chimera domains can grow additively under appropriate variations of the system parameters generating thereby <span class="hlt">head</span>-adding cascades of the scroll <span class="hlt">wave</span> chimeras. The phenomenon is derived for the Kuramoto model of N 3 identical phase oscillators placed in the unit 3D cube with periodic boundary conditions, parameters being the coupling radius r and phase lag α. To obtain the multiheaded chimeras, we perform the so-called `cloning procedure' as follows: choose a sample single-<span class="hlt">headed</span> 3D chimera state, make appropriate scale transformation, and put some number of copies of them into the unit cube. After that, start numerical simulations with slightly perturbed initial conditions and continue them for a sufficiently long time to confirm or reject the state existence and stability. In this way it is found, that multiple scroll <span class="hlt">wave</span> chimeras including those with incoherent rolls, Hopf links and trefoil knots admit this sort of multiheaded regeneration. On the other hand, multiple 3D chimeras without spiral rotations, like coherent and incoherent balls, tubes, crosses, and layers appear to be unstable and are destroyed rather fast even for arbitrarily small initial perturbations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRF..123...97P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRF..123...97P"><span>The Role of Bed Roughness in <span class="hlt">Wave</span> Transformation Across Sloping Rock Shore Platforms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poate, Tim; Masselink, Gerd; Austin, Martin J.; Dickson, Mark; McCall, Robert</p> <p>2018-01-01</p> <p>We present for the first time observations and model simulations of <span class="hlt">wave</span> transformation across sloping (Type A) rock shore platforms. Pressure measurements of the water surface elevation using up to 15 sensors across five rock platforms with contrasting roughness, gradient, and <span class="hlt">wave</span> climate represent the most extensive collected, both in terms of the range of environmental conditions, and the temporal and spatial resolution. Platforms are shown to dissipate both incident and infragravity <span class="hlt">wave</span> energy as skewness and asymmetry develop and, in line with previous studies, surf <span class="hlt">zone</span> <span class="hlt">wave</span> heights are saturated and strongly tidally modulated. Overall, the observed properties of the <span class="hlt">waves</span> and formulations derived from sandy beaches do not highlight any systematic interplatform variation, in spite of significant differences in platform roughness, suggesting that friction can be neglected when studying short <span class="hlt">wave</span> transformation. Optimization of a numerical <span class="hlt">wave</span> transformation model shows that the <span class="hlt">wave</span> breaker criterion falls between the range of values reported for flat sandy beaches and those of steep coral fore reefs. However, the optimized drag coefficient shows significant scatter for the roughest sites and an alternative empirical drag model, based on the platform roughness, does not improve model performance. Thus, model results indicate that the parameterization of frictional drag using the bottom roughness length-scale may be inappropriate for the roughest platforms. Based on these results, we examine the balance of <span class="hlt">wave</span> breaking to frictional dissipation for rock platforms and find that friction is only significant for very rough, flat platforms during small <span class="hlt">wave</span> conditions outside the surf <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032322','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032322"><span><span class="hlt">Wave</span>-current interaction in Willapa Bay</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Olabarrieta, Maitane; Warner, John C.; Kumar, Nirnimesh</p> <p>2011-01-01</p> <p>This paper describes the importance of <span class="hlt">wave</span>-current interaction in an inlet-estuary system. The three-dimensional, fully coupled, Coupled Ocean-Atmosphere-<span class="hlt">Wave</span>-Sediment Transport (COAWST) modeling system was applied in Willapa Bay (Washington State) from 22 to 29 October 1998 that included a large storm event. To represent the interaction between <span class="hlt">waves</span> and currents, the vortex-force method was used. Model results were compared with water elevations, currents, and <span class="hlt">wave</span> measurements obtained by the U.S. Army Corp of Engineers. In general, a good agreement between field data and computed results was achieved, although some discrepancies were also observed in regard to <span class="hlt">wave</span> peak directions in the most upstream station. Several numerical experiments that considered different forcing terms were run in order to identify the effects of each wind, tide, and <span class="hlt">wave</span>-current interaction process. Comparison of the horizontal momentum balances results identified that <span class="hlt">wave</span>-breaking-induced acceleration is one of the leading terms in the inlet area. The enhancement of the apparent bed roughness caused by <span class="hlt">waves</span> also affected the values and distribution of the bottom shear stress. The pressure gradient showed significant changes with respect to the pure tidal case. During storm conditions the momentum balance in the inlet shares the characteristics of tidal-dominated and <span class="hlt">wave</span>-dominated surf <span class="hlt">zone</span> environments. The changes in the momentum balance caused by <span class="hlt">waves</span> were manifested both in water level and current variations. The most relevant effect on hydrodynamics was a <span class="hlt">wave</span>-induced setup in the inner part of the estuary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29031310','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29031310"><span>In a bad place: Carers of patients with <span class="hlt">head</span> and neck cancer experiences of travelling for cancer treatment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Balfe, Myles; Keohane, Kieran; O' Brien, Katie; Gooberman-Hill, Rachael; Maguire, Rebecca; Hanly, Paul; O' Sullivan, Eleanor; Sharp, Linda</p> <p>2017-10-01</p> <p>To explore the effect that treatment-related commuting has on carers of patients with <span class="hlt">head</span> and neck cancer. Semi-structured interviews, thematically analysed, with 31 carers. Treatment-related commuting had a considerable impact on carers of patients with <span class="hlt">head</span> and neck cancer, both in practical terms (economic costs, disruption) and also in psychological terms. Many carers of patients with <span class="hlt">head</span> and neck cancer described becoming distressed by their commute. Some carers from large urban cities appeared to have hidden commuting burdens. Some carers respond to commuting stress by '<span class="hlt">zoning</span> out' or becoming 'like zombies'. Treatment-related travel for <span class="hlt">head</span> and neck cancer can have significant practical and psychological impacts. Health professionals should be aware of the impacts that commuting can have on <span class="hlt">head</span> and neck caregivers. Health services may be able to take practical steps, such as providing subsidized parking, to address <span class="hlt">head</span> and neck carergivers' difficulties. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SPIE10599E..07J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10599E..07J"><span>Neutral axis determination of full size concrete structures using coda <span class="hlt">wave</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>Jiang, Hanwan; Zhan, Hanyu; Zhuang, Chenxu; Jiang, Ruinian</p> <p>2018-03-01</p> <p>Coda <span class="hlt">waves</span> experiencing multiple scattering behaviors are sensitive to weak changes occurring in media. In this paper, a typical four-point bending test with varied external loads is conducted on a 30-meter T-beam that is removed from a bridge after being in service for 15 years, and the coda <span class="hlt">wave</span> signals are collected with a couple of sources-receivers pairs. Then the observed coda <span class="hlt">waves</span> at different loads are compared to calculate their relative velocity variations, which are utilized as the parameter to distinct the compression and tensile <span class="hlt">zones</span> as well as determine the neutral axis position. Without any prior knowledge of the concrete beam, the estimated axis position agrees well with the associated strain gage measurement results, and the <span class="hlt">zones</span> bearing stress and tension behaviors are indicated. The presented work offers significant potential for Non-Destructive Testing and Evaluation of full-size concrete structures in future work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMSM11B2157R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMSM11B2157R"><span>Ground Signatures of EMIC <span class="hlt">Waves</span> obtained From a 3D Global <span class="hlt">Wave</span> Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rankin, R.; Sydorenko, D.; Zong, Q.; Zhang, L.</p> <p>2016-12-01</p> <p>EMIC <span class="hlt">waves</span> generated in the inner magnetosphere are important drivers of radiation belt particle loss. Van Allen Probes and ground observations of EMIC <span class="hlt">waves</span> suggest that localized magnetospheric sources inject <span class="hlt">waves</span> that are guided along geomagnetic field lines and then reflected and refracted in the low altitude magnetosphere [Kim, E.-H., and J. R. Johnson (2016), Geophys. Res. Lett., 43, 13-21, doi:10.1002/2015GL066978] before entering the ionosphere. The <span class="hlt">waves</span> then spread horizontally within the F-region waveguide and propagate to the ground. To understand the observed properties of EMIC <span class="hlt">waves</span>, a global 3D model of ULF <span class="hlt">waves</span> in Earth's magnetosphere, ionosphere, and neutral atmosphere has been developed. The simulation domain extends from Earth's surface to a spherical boundary a few tens of thousands of km in radius. The model uses spherical coordinates and incorporates an overset Yin-Yang grid that eliminates the singularity at the polar axis and improves uniformity of the grid in the polar areas [Kageyama, A., and T. Sato (2004), Geochem. Geophys. Geosyst., 5, Q09005, doi:10.1029/2004GC000734]. The geomagnetic field in the model is general, but is dipole in this study. The plasma is described as a set of electron and multiple species ion conducting fluids. Realistic 3D density profiles of various ion species as well as thermospheric parameters are provided by the Canadian Ionosphere Atmosphere Model (C-IAM) [Martynenko O.V. et al. (2014), J. Atmos. Solar-Terr. Phys., 120, 51-61, doi:10.1016/j.jastp.2014.08.014]. The global ULF <span class="hlt">wave</span> model is applied to study propagation of EMIC <span class="hlt">waves</span> excited in the equatorial plane near L=7. <span class="hlt">Wave</span> propagation along field lines, reflection and refraction in the <span class="hlt">zone</span> of critical frequencies, and further propagation through the ionosphere to the ground are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED558558.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED558558.pdf"><span>Toddlers in Early <span class="hlt">Head</span> Start: A Portrait of 2-Year-Olds, Their Families, and the Programs Serving Them. Volume 1: Age 2 Report. OPRE Report 2015-10</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>Vogel, Cheri A.; Caronongan, Pia; Thomas, Jaime; Bandel, Eileen; Xue, Yange; Henke, Juliette; Aikens, Nikki; Boller, Kimberly; Murphy, Lauren</p> <p>2015-01-01</p> <p>The Early <span class="hlt">Head</span> Start Family and Child Experiences Survey (Baby FACES) is a descriptive study of Early <span class="hlt">Head</span> Start programs designed to inform policy and practice at both national and local levels. Baby FACES follows two cohorts of children through their time in Early <span class="hlt">Head</span> Start, starting in 2009, the first <span class="hlt">wave</span> of data collection. The Newborn…</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/2017PhPl...24a3518N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhPl...24a3518N"><span>Correlation of <span class="hlt">wave</span> propagation modes in helicon plasma with source tube lengths</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niu, Chen; Zhao, Gao; Wang, Yu; Liu, Zhongwei; Chen, Qiang</p> <p>2017-01-01</p> <p>Helicon <span class="hlt">wave</span> plasma demonstrates lots of advantages in high coupling efficiency, high density, and low magnetic field. However, the helicon <span class="hlt">wave</span> plasma still meets challenges in applications of material deposition, surface treatment, and electromagnetic thrusters owing to the changeable coupled efficiency and the remarkable non-uniformity. In this paper, we explore the <span class="hlt">wave</span> propagation characterization by the B-dot probe in various lengths of source tubes. We find that in a long source tube the standing <span class="hlt">wave</span> appears under the antenna <span class="hlt">zone</span>, while the traveling <span class="hlt">wave</span> is formed out of the antenna region. The apparent modulation of <span class="hlt">wave</span> amplitude is formed in upstream rather than in downstream of the antenna. In a short source tube, however, there is only standing <span class="hlt">wave</span> propagation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2445T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2445T"><span>Fan-<span class="hlt">head</span> shear rupture mechanism as a source of off-fault tensile cracking</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tarasov, Boris</p> <p>2016-04-01</p> <p>This presentation discusses the role of a recently identified fan-<span class="hlt">head</span> shear rupture mechanism [1] in the creation of off-fault tensile cracks observed in earthquake laboratory experiments conducted on brittle photoelastic specimens [2,3]. According to the fan-mechanism the shear rupture propagation is associated with consecutive creation of small slabs in the fracture tip which, due to rotation caused by shear displacement of the fracture interfaces, form a fan-structure representing the fracture <span class="hlt">head</span>. The fan-<span class="hlt">head</span> combines such unique features as: extremely low shear resistance (below the frictional strength) and self-sustaining tensile stress intensification along one side of the interface. The variation of tensile stress within the fan-<span class="hlt">head</span> <span class="hlt">zone</span> is like this: it increases with distance from the fracture tip up to a maximum value and then decreases. For the initial formation of the fan-<span class="hlt">head</span> high local stresses corresponding to the fracture strength should be applied in a small area, however after completions of the fan-<span class="hlt">head</span> it can propagate dynamically through the material at low shear stresses (even below the frictional strength). The fan-mechanism allows explaining all unique features associated with the off-fault cracking process observed in photoelastic experiments [2,3]. In these experiments spontaneous shear ruptures were nucleated in a bonded, precut, inclined and pre-stressed interface by producing a local pressure pulse in a small area. Isochromatic fringe patterns around a shear rupture propagating along bonded interface indicate the following features of the off-fault tensile crack development: tensile cracks nucleate and grow periodically along one side of the interface at a roughly constant angle (about 80 degrees) relative to the shear rupture interface; the tensile crack nucleation takes place some distance behind the rupture tip; with distance from the point of nucleation tensile cracks grow up to a certain length within the rupture <span class="hlt">head</span> <span class="hlt">zone</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S44A..01A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S44A..01A"><span>numerical broadband modelling of ocean <span class="hlt">waves</span>, from 1 to 300 s: implications for seismic <span class="hlt">wave</span> sources and <span class="hlt">wave</span> climate studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ardhuin, F.; Stutzmann, E.; Gualtieri, L.</p> <p>2014-12-01</p> <p>Ocean <span class="hlt">waves</span> provide most of the energy that feeds the continuous vertical oscillations of the solid Earth. Three period bands are usually identified. The hum contains periods longer than 30 s, and the primary and secondary peaks are usually centered around 15 and 5 s, respectively. Motions in all three bands are recorded everywhere on our planet and can provide information on both the solid Earth structure and the ocean <span class="hlt">wave</span> climate over the past century. Here we describe recent efforts to extend the range of validity of ocean <span class="hlt">wave</span> models to cover periods from 1 to 300 s (Ardhuin et al., Ocean Modelling 2014), and the resulting public database of ocean <span class="hlt">wave</span> spectra (http://tinyurl.com/iowagaftp/HINDCAST/ ). We particularly discuss the sources of uncertainty for building a numerical model of acoustic and seismic noise on this knowledge of ocean <span class="hlt">wave</span> spectra. For acoustic periods shorter than 3 seconds, the main uncertainties are the directional distributions of <span class="hlt">wave</span> energy (Ardhuin et al., J. Acoust. Soc. Amer. 2013). For intermediate periods (3 to 25 s), the propagation properties of seismic <span class="hlt">waves</span> are probably the main source of error when producing synthetic spectra of Rayleigh <span class="hlt">waves</span> (Ardhuin et al. JGR 2011, Stutzmann et al. GJI 2012). For the longer periods (25 to 300 s), the poor knowledge of the bottom topography details may be the limiting factor for estimating hum spectra or inverting hum measurements in properties of the infragravity <span class="hlt">wave</span> field. All in all, the space and time variability of recorded seismic and acoustic spectra is generally well reproduced in the band 3 to 300 s, and work on shorter periods is under way. This direct model can be used to search for missing noise sources, such as <span class="hlt">wave</span> scattering in the marginal ice <span class="hlt">zone</span>, find events relevant for solid earth studies (e.g. Obrebski et al. JGR 2013) or invert <span class="hlt">wave</span> climate properties from microseismic records. The figure shows measured spectra of the vertical ground acceleration, and modeled</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JSV...339...65M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JSV...339...65M"><span><span class="hlt">Head</span>-mounted active noise control system with virtual sensing technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miyazaki, Nobuhiro; Kajikawa, Yoshinobu</p> <p>2015-03-01</p> <p>In this paper, we apply a virtual sensing technique to a <span class="hlt">head</span>-mounted active noise control (ANC) system we have already proposed. The proposed ANC system can reduce narrowband noise while improving the noise reduction ability at the desired locations. A <span class="hlt">head</span>-mounted ANC system based on an adaptive feedback structure can reduce noise with periodicity or narrowband components. However, since quiet <span class="hlt">zones</span> are formed only at the locations of error microphones, an adequate noise reduction cannot be achieved at the locations where error microphones cannot be placed such as near the eardrums. A solution to this problem is to apply a virtual sensing technique. A virtual sensing ANC system can achieve higher noise reduction at the desired locations by measuring the system models from physical sensors to virtual sensors, which will be used in the online operation of the virtual sensing ANC algorithm. Hence, we attempt to achieve the maximum noise reduction near the eardrums by applying the virtual sensing technique to the <span class="hlt">head</span>-mounted ANC system. However, it is impossible to place the microphone near the eardrums. Therefore, the system models from physical sensors to virtual sensors are estimated using the <span class="hlt">Head</span> And Torso Simulator (HATS) instead of human ears. Some simulation, experimental, and subjective assessment results demonstrate that the <span class="hlt">head</span>-mounted ANC system with virtual sensing is superior to that without virtual sensing in terms of the noise reduction ability at the desired locations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC43F1129C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC43F1129C"><span>More Intense Mega Heat <span class="hlt">Waves</span> in the Warmer World</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Choi, G.; Robinson, D. A.</p> <p>2017-12-01</p> <p>In this study, changes in the occurrences of heat <span class="hlt">waves</span> on the globe since the mid- 20th century and the synoptic characteristics of mega heat <span class="hlt">waves</span> at regional scales in the warmer climate are examined. The NCEP-NCAR reanalysis surface data show that there have been no obvious linear changes in the heat <span class="hlt">wave</span> frequencies at the continental scales since the mid-20th century, but amplified interdecadal variations led to unprecedented intense heat <span class="hlt">waves</span> in the recent decades at the regional scales. Such mega heat <span class="hlt">waves</span> have been more frequently observed in the poleward subtropical climate belts as well as in the interior region of continents. According to the analyses of upper tropospheric data, the occurrences of more intense mega heat <span class="hlt">waves</span> since the late 20th century may be associated with the expansion of subtropical high pressures. These results suggest that populous cities near the subtropical climate <span class="hlt">zones</span> should provide proactive mega heat <span class="hlt">wave</span> warning systems for residents due to their vulnerability to the sudden attack of human lives harvest by mega heat <span class="hlt">waves</span> in the warmer 21st century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120010521','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120010521"><span>New Gravity <span class="hlt">Wave</span> Treatments for GISS Climate Models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Geller, Marvin A.; Zhou, Tiehan; Ruedy, Reto; Aleinov, Igor; Nazarenko, Larissa; Tausnev, Nikolai L.; Sun, Shan; Kelley, Maxwell; Cheng, Ye</p> <p>2011-01-01</p> <p>Previous versions of GISS climate models have either used formulations of Rayleigh drag to represent unresolved gravity <span class="hlt">wave</span> interactions with the model-resolved flow or have included a rather complicated treatment of unresolved gravity <span class="hlt">waves</span> that, while being climate interactive, involved the specification of a relatively large number of parameters that were not well constrained by observations and also was computationally very expensive. Here, the authors introduce a relatively simple and computationally efficient specification of unresolved orographic and nonorographic gravity <span class="hlt">waves</span> and their interaction with the resolved flow. Comparisons of the GISS model winds and temperatures with no gravity <span class="hlt">wave</span> parameterization; with only orographic gravity <span class="hlt">wave</span> parameterization; and with both orographic and nonorographic gravity <span class="hlt">wave</span> parameterizations are shown to illustrate how the zonal mean winds and temperatures converge toward observations. The authors also show that the specifications of orographic and nonorographic gravity <span class="hlt">waves</span> must be different in the Northern and Southern Hemispheres. Then results are presented where the nonorographic gravity <span class="hlt">wave</span> sources are specified to represent sources from convection in the intertropical convergence <span class="hlt">zone</span> and spontaneous emission from jet imbalances. Finally, a strategy to include these effects in a climate-dependent manner is suggested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100032912','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100032912"><span>New Gravity <span class="hlt">Wave</span> Treatments for GISS Climate Models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Geller, Marvin A.; Zhou, Tiehan; Ruedy, Reto; Aleinov, Igor; Nazarenko, Larissa; Tausnev, Nikolai L.; Sun, Shan; Kelley, Maxwell; Cheng, Ye</p> <p>2010-01-01</p> <p>Previous versions of GISS climate models have either used formulations of Rayleigh drag to represent unresolved gravity <span class="hlt">wave</span> interactions with the model resolved flow or have included a rather complicated treatment of unresolved gravity <span class="hlt">waves</span> that, while being climate interactive, involved the specification of a relatively large number of parameters that were not well constrained by observations and also was computationally very expensive. Here, we introduce a relatively simple and computationally efficient specification of unresolved orographic and non-orographic gravity <span class="hlt">waves</span> and their interaction with the resolved flow. We show comparisons of the GISS model winds and temperatures with no gravity <span class="hlt">wave</span> parametrization; with only orographic gravity <span class="hlt">wave</span> parameterization; and with both orographic and non-orographic gravity <span class="hlt">wave</span> parameterizations to illustrate how the zonal mean winds and temperatures converge toward observations. We also show that the specifications of orographic and nonorographic gravity <span class="hlt">waves</span> must be different in the Northern and Southern Hemispheres. We then show results where the non-orographic gravity <span class="hlt">wave</span> sources are specified to represent sources from convection in the Intertropical Convergence <span class="hlt">Zone</span> and spontaneous emission from jet imbalances. Finally, we suggest a strategy to include these effects in a climate dependent manner.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28371495','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28371495"><span>Safe <span class="hlt">Zone</span> of Posterior Screw Insertion for Talar Neck Fractures on 3-Dimensional Reconstruction Model.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wu, Jian-Qun; Ma, Sheng-Hui; Liu, Song; Qin, Cheng-He; Jin, Dan; Yu, Bin</p> <p>2017-02-01</p> <p>To investigate the optimal posterior screw placement and the geometry of safe <span class="hlt">zones</span> for screw insertion in the talar neck. Computed tomography data for 15 normal feet were imported into Mimics 10.01 software for 3-dimensional reconstruction; 4.0-mm-diameter screws were simulated from the lateral tubercle of the posterior process of the talus to the talar <span class="hlt">head</span>. The range of screw paths trajectories and screw lengths at nine locations that did not breach the cortex of the talus were evaluated. In addition, the farthest (point a) and nearest point (point b) of the safe <span class="hlt">zone</span> to the subtalar joint at each location, the anteversion angle (angle A), which is parallel to the sagittal plane, and the horizontal angle (angle B), which is perpendicular to the sagittal plane, were measured. The safe <span class="hlt">zone</span> was mainly between the 30% location and the 60% location; the width of each safe <span class="hlt">zone</span> was 13.6° ± 1.4°; the maximum height of each safe <span class="hlt">zone</span> was 7.8° ± 1.2°. The height of the safe <span class="hlt">zone</span> was lowest at the 30% location (4.5°) and highest at the 50% location (7.3°). The mixed safe <span class="hlt">zone</span> of all tali was between the 50% location and the 60% location. When a screw was inserted at point a, the safe entry distance (screw length) ranged from 48.8 to 49.5 mm, and when inserted to point b, the distance ranged from 48.2 to 48.9 mm. And inserting a 48.7 mm screw, 5.6° laterally and 7.4° superiorly, from the lateral tubercle of the posterior process of the talus towards the talar <span class="hlt">head</span> is safest. The safe <span class="hlt">zone</span> of posterior screw fixation have been defined applying to most talus, assuming the fractures are well reduced, this may strengthen the stability, shorten the operation time and reduce the incidence of surgical complications. © 2017 Chinese Orthopaedic Association and John Wiley & Sons Australia, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/503590-detonation-waves-pentaerythritol-tetranitrate','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/503590-detonation-waves-pentaerythritol-tetranitrate"><span>Detonation <span class="hlt">waves</span> in pentaerythritol tetranitrate</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>Tarver, C.M.; Breithaupt, R.D.; Kury, J.W.</p> <p>1997-06-01</p> <p>Fabry{endash}Perot laser interferometry was used to obtain nanosecond time resolved particle velocity histories of the free surfaces of tantalum discs accelerated by detonating pentaerythritol tetranitrate (PETN) charges and of the interfaces between PETN detonation products and lithium fluoride crystals. The experimental records were compared to particle velocity histories calculated using very finely <span class="hlt">zoned</span> meshes of the exact dimensions with the DYNA2D hydrodynamic code. The duration of the PETN detonation reaction <span class="hlt">zone</span> was demonstrated to be less than the 5 ns initial resolution of the Fabry{endash}Perot technique, because the experimental records were accurately calculated using an instantaneous chemical reaction, the Chapman{endash}Jouguetmore » (C-J) model of detonation, and the reaction product Jones{endash}Wilkins{endash}Lee (JWL) equation of state for PETN detonation products previously determined by supracompression (overdriven detonation) studies. Some of the PETN charges were pressed to densities approaching the crystal density and exhibited the phenomenon of superdetonation. An ignition and growth Zeldovich{endash}von Neumann{endash}Doring (ZND) reactive flow model was developed to explain these experimental records and the results of previous PETN shock initiation experiments on single crystals of PETN. Good agreement was obtained for the induction time delays preceding chemical reaction, the run distances at which the initial shock <span class="hlt">waves</span> were overtaken by the detonation <span class="hlt">waves</span> in the compressed PETN, and the measured particle velocity histories produced by the overdriven detonation <span class="hlt">waves</span> before they could relax to steady state C-J velocity and pressure. {copyright} {ital 1997 American Institute of Physics.}« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..133a2019S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..133a2019S"><span>Assessment of <span class="hlt">wave</span> energy potential along the south coast of Java Island</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Song, Qingyang; Mayerle, Roberto</p> <p>2018-04-01</p> <p>The south coast of Java Island has a great potential for <span class="hlt">wave</span> energy. A long-term analysis of a 10-year <span class="hlt">wave</span> dataset obtained from the ERA-Interim database is performed for preliminary <span class="hlt">wave</span> energy assessment in this area, and it was seen that the annual median power is expected to exceed 20kW/m along the coast. A coastal <span class="hlt">wave</span> model with an unstructured grid was run to reveal the <span class="hlt">wave</span> conditions and to assess the <span class="hlt">wave</span> energy potential along the coast in detail. The effect of swells and local wind on the <span class="hlt">wave</span> conditions is investigated. Annual median <span class="hlt">wave</span> power, water depth and distance from the coast are selected as criteria for the identification of suitable locations for <span class="hlt">wave</span> energy conversion. Two <span class="hlt">zones</span> within the study area emerge to be suitable for <span class="hlt">wave</span> energy extraction. Swells from the southwest turned out to be the major source of <span class="hlt">wave</span> energy and highest monthly median <span class="hlt">wave</span> power reached about 33kW/m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA482228','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA482228"><span>Evaluation of Two Numerical <span class="hlt">Wave</span> Models with Inlet Physical Model</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2005-07-01</p> <p>GHOST in inlets and near structures compared slightly better with measurements. DOI: 10.1061/~ASCE!0733-950X~2005!131:4~149! CE Database subject <span class="hlt">headings</span>...full directional spectrum. GHOST represents <span class="hlt">wave</span> diffraction by implementing a formulation of the Eikonal equation ~Rivero et al. 1997a, b!, whereas</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28818943','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28818943"><span><span class="hlt">Zones</span>, spots, and planetary-scale <span class="hlt">waves</span> beating in brown dwarf atmospheres.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Apai, D; Karalidi, T; Marley, M S; Yang, H; Flateau, D; Metchev, S; Cowan, N B; Buenzli, E; Burgasser, A J; Radigan, J; Artigau, E; Lowrance, P</p> <p>2017-08-18</p> <p>Brown dwarfs are massive analogs of extrasolar giant planets and may host types of atmospheric circulation not seen in the solar system. We analyzed a long-term Spitzer Space Telescope infrared monitoring campaign of brown dwarfs to constrain cloud cover variations over a total of 192 rotations. The infrared brightness evolution is dominated by beat patterns caused by planetary-scale <span class="hlt">wave</span> pairs and by a small number of bright spots. The beating <span class="hlt">waves</span> have similar amplitudes but slightly different apparent periods because of differing velocities or directions. The power spectrum of intermediate-temperature brown dwarfs resembles that of Neptune, indicating the presence of zonal temperature and wind speed variations. Our findings explain three previously puzzling behaviors seen in brown dwarf brightness variations. Copyright © 2017 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHI54A1849O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHI54A1849O"><span>Development of a <span class="hlt">wave</span>-induced forcing threshold for nearshore impact of <span class="hlt">Wave</span> Energy Converter arrays</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Dea, A.; Haller, M. C.; Ozkan-Haller, H. T.</p> <p>2016-02-01</p> <p><span class="hlt">Wave</span>-induced forcing is a function of spatial gradients in the <span class="hlt">wave</span> radiation stresses and is the main driver of alongshore currents, rip currents, and nearshore sediment transport. The installation of nearshore <span class="hlt">Wave</span> Energy Converter (WEC) arrays may cause significant changes in the surf <span class="hlt">zone</span> radiation stresses and could therefore impact nearshore littoral processes. In the first part of this study, a new threshold for nearshore hydrodynamic impact due to the presence of WEC devices is established based on changes in the alongshore radiation stress gradients shoreward of WEC arrays. The threshold is defined based on the relationship between nearshore radiation stresses and alongshore currents as observed in field data. Next, we perform a parametric study of the nearshore impact of WEC arrays using the SWAN <span class="hlt">wave</span> model. Trials are conducted on an idealized, alongshore-uniform beach with a range of WEC array configurations, locations, and incident <span class="hlt">wave</span> conditions, and conditions that generate radiation stress gradients above the impact threshold are identified. Finally, the same methodology is applied to two <span class="hlt">wave</span> energy test sites off the coast of Newport, OR with more complicated bathymetries. Although the trends at the field sites are similar to those seen in the parametric study, the location and extent of the changes in the alongshore radiation stress gradients appear to be heavily influenced by the local bathymetry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27847717','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27847717"><span>Effectiveness of Lower Energy Density Extracorporeal Shock <span class="hlt">Wave</span> Therapy in the Early Stage of Avascular Necrosis of the Femoral <span class="hlt">Head</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Han, Yong; Lee, June-Kyung; Lee, Bong-Yeon; Kee, Hoi-Sung; Jung, Kwang-Ik; Yoon, Seo-Ra</p> <p>2016-10-01</p> <p>To evaluate the effectiveness of lower energy flux density (EFD) extracorporeal shock <span class="hlt">wave</span> therapy (ESWT) in the early stage of avascular necrosis (AVN) of the femoral <span class="hlt">head</span>. Nineteen patients and 30 hips were enrolled. All subjects received 4 weekly sessions of ESWT, at different energy levels; group A (n=15; 1,000 shocks/session, EFD per shock 0.12 mJ/mm 2 ) and group B (n=15; 1,000 shocks/session, EFD per shock 0.32 mJ/mm 2 ). We measured pain by using the visual analog scale (VAS), and disability by using the Harris hip score, Hip dysfunction and Osteoarthritis Outcome Score (HOOS), and the Western Ontario and McMaster University Osteoarthritis Index (WOMAC). To determine the effect of the lower EFD ESWT, we assessed the VAS, Harris hip score, HOOS, WOMAC of the subjects before and at 1, 3, and 6 months. In both groups, the VAS, Harris hip score, HOOS, and WOMAC scores improved over time (p<0.05). Lower EFD ESWT may be an effective method to improve the function and to relieve pain in the early stage of AVN.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018025','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018025"><span><span class="hlt">Wave</span> climate and nearshore lakebed response, Illinois Beach State Park, Lake Michigan</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Booth, J.S.</p> <p>1994-01-01</p> <p>Only under these major storm conditions is there a realistic potential for <span class="hlt">wave</span>-lakebed interaction (and associated wind-driven currents) to cause a significant net modification to the outer nearshore lakebed which, in turn, may promulgate change in the inner nearshore (surf) <span class="hlt">zone</span>. Analysis of bathymetric and sediment grain-size data, used in conjuction with published <span class="hlt">wave</span> hindcast data, <span class="hlt">wave</span> propagation modeling, and previous studies in the area, indicates that this potential occurs, most likely, on a scale of years. -from Author</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29661716','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29661716"><span>Small cell lymphocytic variant of marginal <span class="hlt">zone</span> lymphoma: A distinct form of marginal <span class="hlt">zone</span> lymphoma derived from naïve B cells as a cutaneous counterpart to the naïve marginal <span class="hlt">zone</span> lymphoma of splenic origin.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Magro, Cynthia M; Olson, Luke C</p> <p>2018-02-21</p> <p>Primary cutaneous marginal <span class="hlt">zone</span> lymphoma most commonly represents an indolent form of cutaneous B cell lymphoma. However, epidermotropic marginal <span class="hlt">zone</span> lymphoma, blastic marginal <span class="hlt">zone</span> lymphoma and B cell dominant variants without isotype switching can be associated with extracutaneous dissemination. The presumptive cell of origin is a post germinal center B cell with plasmacytic features. In the extracutaneous setting, however, a naïve B cell origin has been proposed for a subset of marginal <span class="hlt">zone</span> lymphomas, notably splenic marginal <span class="hlt">zone</span> lymphoma. The author encountered 11 cases of atypical lymphocytic infiltration of the skin primarily occurring in older individuals with an upper arm and <span class="hlt">head</span> and neck localization; there was a reproducible pattern of diffuse and nodular infiltration by small monomorphic-appearing B cells. Phenotypically, the infiltrate was one predominated by B cells exhibiting CD23 and IgD positivity without immunoreactivity for CD38 and there were either no plasma cells or only a few without light chain restriction. In cases presenting with a solitary lesion complete excision and/or radiation led to successful disease remission in all cases without recurrence or metastatic disease. Of three cases with multiple initial lesions, evidence of extracutaneous disease was seen in two cases and recurrence occurred in one case. No patients have died of lymphoma. Longer term follows up and additional cases are needed to determine if this subset of marginal <span class="hlt">zone</span> lymphoma is associated with a worse prognosis. Copyright © 2018. Published by Elsevier Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://medlineplus.gov/ency/article/000840.htm','NIH-MEDLINEPLUS'); return false;" href="https://medlineplus.gov/ency/article/000840.htm"><span><span class="hlt">Head</span> lice</span></a></p> <p><a target="_blank" href="http://medlineplus.gov/">MedlinePlus</a></p> <p></p> <p></p> <p>Pediculosis capitis - <span class="hlt">head</span> lice ... <span class="hlt">Head</span> lice infect hair on the <span class="hlt">head</span>. Tiny eggs on the hair look like flakes of dandruff . However, ... flaking off the scalp, they stay in place. <span class="hlt">Head</span> lice can live up to 30 days on a ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JMSA...11..437S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JMSA...11..437S"><span>Two dimensional fully nonlinear numerical <span class="hlt">wave</span> tank based on the BEM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Zhe; Pang, Yongjie; Li, Hongwei</p> <p>2012-12-01</p> <p>The development of a two dimensional numerical <span class="hlt">wave</span> tank (NWT) with a rocker or piston type wavemaker based on the high order boundary element method (BEM) and mixed Eulerian-Lagrangian (MEL) is examined. The cauchy principle value (CPV) integral is calculated by a special Gauss type quadrature and a change of variable. In addition the explicit truncated Taylor expansion formula is employed in the time-stepping process. A modified double nodes method is assumed to tackle the corner problem, as well as the damping <span class="hlt">zone</span> technique is used to absorb the propagation of the free surface <span class="hlt">wave</span> at the end of the tank. A variety of <span class="hlt">waves</span> are generated by the NWT, for example; a monochromatic <span class="hlt">wave</span>, solitary <span class="hlt">wave</span> and irregular <span class="hlt">wave</span>. The results confirm the NWT model is efficient and stable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70010915','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70010915"><span>Large sand <span class="hlt">waves</span> on the Atlantic Outer Continental Shelf around Wilmington Canyon, off Eastern United States</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Knebel, H.J.; Folger, D.W.</p> <p>1976-01-01</p> <p>New seismic-reflection data show that large sand <span class="hlt">waves</span> near the <span class="hlt">head</span> of Wilmington Canyon on the Atlantic Outer Continental Shelf have a spacing of 100-650 m and a relief of 2-9 m. The bedforms trend northwest and are asymmetrical, the steeper slopes being toward the south or west. Vibracore sediments indicate that the <span class="hlt">waves</span> apparently have formed on a substrate of relict nearshore sediments. Although the age of the original bedforms is unknown, the asymmetry is consistent with the dominant westerly to southerly drift in this area which has been determined by other methods; the asymmetry, therefore, is probably modern. Observations in the sand-<span class="hlt">wave</span> area from a submersible during August 1975, revealed weak bottom currents, sediment bioturbation, unrippled microtopography, and lack of scour. Thus, the asymmetry may be maintained by periodic water motion, possibly associated with storms or perhaps with flow in the canyon <span class="hlt">head</span>. ?? 1976.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22356686-magnetoacoustic-waves-propagating-along-dense-slab-harris-current-sheet-wavelet-spectra','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22356686-magnetoacoustic-waves-propagating-along-dense-slab-harris-current-sheet-wavelet-spectra"><span>Magnetoacoustic <span class="hlt">waves</span> propagating along a dense slab and Harris current sheet and their wavelet spectra</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>Mészárosová, Hana; Karlický, Marian; Jelínek, Petr</p> <p></p> <p>Currently, there is a common endeavor to detect magnetoacoustic <span class="hlt">waves</span> in solar flares. This paper contributes to this topic using an approach of numerical simulations. We studied a spatial and temporal evolution of impulsively generated fast and slow magnetoacoustic <span class="hlt">waves</span> propagating along the dense slab and Harris current sheet using two-dimensional magnetohydrodynamic numerical models. <span class="hlt">Wave</span> signals computed in numerical models were used for computations of the temporal and spatial wavelet spectra for their possible comparison with those obtained from observations. It is shown that these wavelet spectra allow us to estimate basic parameters of waveguides and perturbations. It was foundmore » that the wavelet spectra of <span class="hlt">waves</span> in the dense slab and current sheet differ in additional wavelet components that appear in association with the main tadpole structure. These additional components are new details in the wavelet spectrum of the signal. While in the dense slab this additional component is always delayed after the tadpole <span class="hlt">head</span>, in the current sheet this component always precedes the tadpole <span class="hlt">head</span>. It could help distinguish a type of the waveguide in observed data. We present a technique based on wavelets that separates <span class="hlt">wave</span> structures according to their spatial scales. This technique shows not only how to separate the magnetoacoustic <span class="hlt">waves</span> and waveguide structure in observed data, where the waveguide structure is not known, but also how propagating magnetoacoustic <span class="hlt">waves</span> would appear in observations with limited spatial resolutions. The possibilities detecting these <span class="hlt">waves</span> in observed data are mentioned.« 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_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. Their policies may differ from this site.</div> </div><!-- container --> <footer><a id="backToTop" href="#top"> </a><nav><a id="backToTop" href="#top"> </a><ul class="links"><a id="backToTop" href="#top"> </a><li><a id="backToTop" href="#top"></a><a href="/sitemap.html">Site Map</a></li> <li><a href="/members/index.html">Members Only</a></li> <li><a href="/website-policies.html">Website Policies</a></li> <li><a href="https://doe.responsibledisclosure.com/hc/en-us" target="_blank">Vulnerability Disclosure Program</a></li> <li><a href="/contact.html">Contact Us</a></li> </ul> <div class="small">Science.gov is maintained by the U.S. Department of Energy's <a href="https://www.osti.gov/" target="_blank">Office of Scientific and Technical Information</a>, in partnership with <a href="https://www.cendi.gov/" target="_blank">CENDI</a>.</div> </nav> </footer> <script type="text/javascript"><!-- // var lastDiv = ""; function showDiv(divName) { // hide last div if (lastDiv) { document.getElementById(lastDiv).className = "hiddenDiv"; } //if value of the box is not nothing and an object with that name exists, then change the class if (divName && document.getElementById(divName)) { document.getElementById(divName).className = "visibleDiv"; lastDiv = divName; } } //--> </script> <script> /** * Function that tracks a click on an outbound link in Google Analytics. * This function takes a valid URL string as an argument, and uses that URL string * as the event label. */ var trackOutboundLink = function(url,collectionCode) { try { h = window.open(url); setTimeout(function() { ga('send', 'event', 'topic-page-click-through', collectionCode, url); }, 1000); } catch(err){} }; </script> <!-- Google Analytics --> <script> (function(i,s,o,g,r,a,m){i['GoogleAnalyticsObject']=r;i[r]=i[r]||function(){ (i[r].q=i[r].q||[]).push(arguments)},i[r].l=1*new Date();a=s.createElement(o), m=s.getElementsByTagName(o)[0];a.async=1;a.src=g;m.parentNode.insertBefore(a,m) })(window,document,'script','//www.google-analytics.com/analytics.js','ga'); ga('create', 'UA-1122789-34', 'auto'); ga('send', 'pageview'); </script> <!-- End Google Analytics --> <script> showDiv('page_1') </script> </body> </html>