Search results for "SEISMOLOGY"

showing 10 items of 301 documents

The role of slabs and oceanic plate geometry in the net rotation of the lithosphere, trench motions, and slab return flow

2012

[1] Absolute plate motion models with respect to a deep mantle reference frame (e.g., hot spots) typically contain some net rotation (NR) of the lithosphere. Global mantle flow models for the present-day plate setting reproduce similarly oriented NRs but with amplitudes significantly smaller than those found in some high NR Pacific hot spot reference frames. It is therefore important to understand the mechanisms of NR excitation, which we attempt here with two-dimensional cylindrical models of an idealized Pacific domain. We study the influence of slab properties, oceanic ridge position, continental keels, and a weak asthenospheric layer on NR and trench migration. Fast slab return flow dev…

Slab suctiongeographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesMid-ocean ridgeGeophysics010502 geochemistry & geophysics01 natural sciencesMantle (geology)Geophysics13. Climate actionGeochemistry and PetrologyLithosphereOceanic crustTrenchSlab windowSlabSeismologyGeology0105 earth and related environmental sciencesGeochemistry, Geophysics, Geosystems
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The polarimetric and helioseismic imager on solar orbiter

2020

This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the Sun from outside the Sun-Earth line. It is the key instrument meant to address the top-level science question: How does the solar dynamo work and drive connections between the Sun and the heliosphere? SO/PHI will also play an important role in answering the other top-level science questions of Solar Orbiter, as well as hosting the potential of a rich return in further science. SO/PHI measures the Zeeman effect and the Doppler shift in the FeI 617.3nm spectral line. To this end, the instrument carries out narrow-band imaging…

Solar Telescope010504 meteorology & atmospheric sciencesphotosphere [Sun]FiltegramsHighly elliptical orbitFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionTelescopeOrbiterPhotospherelaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHelioseismologySolar dynamo010303 astronomy & astrophysicsSun: magnetic fieldsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesSun: helioseismologyPhysics[PHYS]Physics [physics]PhotosphereEllipsometrypolarimeters [Instrumentation]Spacecraftbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyinstrumentation: polarimetersSun: photosphereHeliosismologiaAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiestechniques: polarimetricmagnetic fields [Sun]Space and Planetary Sciencetechniques: imaging spectroscopyAstrophysics of Galaxies (astro-ph.GA)Physics::Space PhysicsHelioseismologyAstrophysics::Earth and Planetary AstrophysicsbusinessAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HeliosphereEl·lipsometria
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Resonant origin for density fluctuations deep within the Sun: helioseismology and magneto-gravity waves

2003

We analyze helioseismic waves near the solar equator in the presence of magnetic fields deep within the solar radiative zone. We find that reasonable magnetic fields can significantly alter the shapes of the wave profiles for helioseismic g-modes. They can do so because the existence of density gradients allows g-modes to resonantly excite Alfven waves, causing mode energy to be funnelled along magnetic field lines, away from the solar equatorial plane. The resulting wave forms show comparatively sharp spikes in the density profile at radii where these resonances take place. We estimate how big these waves might be in the Sun, and perform a first search for observable consequences. We find …

Solar neutrinoFOS: Physical sciencesAstrophysicsAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHelioseismology010303 astronomy & astrophysicsSolar equatorPhysics010308 nuclear & particles physicsGravitational waveAstrophysics (astro-ph)FísicaAstronomy and AstrophysicsObservableRadiation zoneMagnetic fieldHigh Energy Physics - PhenomenologyAmplitude13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary Astrophysics
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Southern-Tyrrhenian seismicity in space-time-magnitude domain

2006

An analysis is conducted on a catalogue containing more than 2000 seismic events
 occurred in the southern Tyrrhenian Sea between 1988 and October 2002, as an attempt
 to characterise the main seismogenetic processes active in the area in space, time and magnitude domain by means of the parameters of phenomenological laws.
 
 We chose to adopt simple phenomenological models, since the low number of data did
 not allow to use more complex laws.
 
 The two main seismogenetic volumes present in the area were considered for the purpose
 of this work. The first includes a nearly homogeneous distribution of hypocentres in a
 NW steeply dipping layer as far as a…

Southern-Tyrrhenian SeaPlane (geometry)Space timelcsh:QC801-809Magnitude (mathematics)Southern-Tyrrhenian Sea statistical models aftershock sequences background seismicitystatistical modelslcsh:QC851-999Induced seismicityHomogeneous distributionDomain (mathematical analysis)lcsh:Geophysics. Cosmic physicsGeophysicsaftershock sequencesLithosphereSlablcsh:Meteorology. ClimatologySeismologyGeologybackground seismicity.Annals of Geophysics
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ETAS Space time modelling of Chile induced seismicity using covariates.

2021

<p>Chilean seismic activity is among the strongest ones in the world. As already shown in previous papers, seismic activity can be usefully described by a space-time branching process, like the ETAS (Epidemic Type Aftershock Sequences) model, which is a semiparametric model with a large time scale component for the background seismicity and a small time scale component for the induced seismicity. The large-scale component intensity function  is usually estimated by  nonparametric techniques, specifically in our paper we used the Forward Likelihood Predictive approach (FLP); the induced seismicity is modelled with a parametric space-time function. In c…

Space timeCovariateseismicityInduced seismicitySeismologyGeology
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Local Spatial Log-Gaussian Cox Processes for seismic data

2022

AbstractIn this paper, we propose the use of advanced and flexible statistical models to describe the spatial displacement of earthquake data. The paper aims to account for the external geological information in the description of complex seismic point processes, through the estimation of models with space varying parameters. A local version of the Log-Gaussian Cox processes (LGCP) is introduced and applied for the first time, exploiting the inferential tools in Baddeley (Spat Stat 22:261–295, 2017), estimating the model by the local Palm likelihood. We provide methods and approaches accounting for the interaction among points, typically described by LGCP models through the estimation of th…

Statistics and ProbabilityEconomics and Econometricsspatial point processeApplied MathematicsModeling and SimulationLog-Gaussian Cox procelocal composite likelihoodPalm likelihoodseismologySettore SECS-S/01 - StatisticaSocial Sciences (miscellaneous)Analysis
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Forward likelihood-based predictive approach for space-time point processes

2011

Dealing with data from a space–time point process, the estimation of the conditional intensity function is a crucial issue even if a complete definition of a parametric model is not available. In particular, in case of exploratory contexts or if we want to assess the adequacy of a specific parametric model, some kind of nonparametric estimation procedure could be useful. Often, for these purposes kernel estimators are used and the estimation of the intensity function depends on the estimation of bandwidth parameters. In some fields, like for instance the seismological one, predictive properties of the estimated intensity function are pursued. Since a direct ML approach cannot be used, we pr…

Statistics and ProbabilityMathematical optimizationEcological ModelingSpace timespace–time point processesBandwidth (signal processing)Nonparametric statisticsEstimatorStatistical seismologynonparametric estimationPoint processParametric modellikelihood functionSettore SECS-S/01 - StatisticaLikelihood functionpredictive propertieMathematicsEnvironmetrics
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Quartz-strain-rate-metry (QSR), an efficient tool to quantify strain localization in the continental crust

2015

Strain (chemistry)RheologyContinental crustStrain rateShear zonePetrologyQuartzGeologySeismology
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Lattice-particle simulation of stress patterns in a Rwenzori-type rift transfer zone

2011

Abstract A new 3D spring lattice computer model has been developed and used to calculate the stress-field in the vicinity of a rift transfer zone. The numerical setup is based on the Rwenzori block, a transfer zone in the Western Branch of the East African Rift Valley. The study has two closely related, yet independent aims: primarily to gain insight into the pattern and the causes of the stress field in the Rwenzori area. The second aim is the evaluation of the model itself, based on a comparison of the model results with local geological structures. The simulations calculate the stress in the brittle part of the crust, at the topographic surface and at a depth of 10 km. The model does the…

Stress (mechanics)Stress fieldBrittlenessRiftLithosphereLattice (order)East African RiftGeologyCrustGeologySeismologyEarth-Surface ProcessesJournal of African Earth Sciences
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Seismic moment tensors and regional stress in the area of the December 2013–January 2014, Matese earthquake sequence (Italy)

2014

Abstract The main goal of this study is to provide moment tensor solutions for small and moderate earthquakes of the Matese seismic sequence in southern Italy for the period of December 2013–January 2014. We estimate the focal mechanisms of 31 earthquakes with local magnitudes related to the Matese earthquake seismic sequence (December 2013–January 2014) in Southern-Central Italy which are recorded by the broadband stations of the Italian National Seismic Network and the Mediterranean Very Broadband Seismographic Network (MedNet) run by the Istituto Nazionale di Geofisica e Vulcanologia (INGV). The solutions show that normal faulting is the prevailing style of seismic deformation in agreeme…

Stress (mechanics)TectonicsSequence (geology)GeophysicsDeformation (mechanics)Moment tensorSeismic momentStress inversionSeismologyGeologyEarth-Surface ProcessesJournal of Geodynamics
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