Search results for "Gravimeter"

showing 4 items of 4 documents

Tidal gravity observations at Mt. Etna and Stromboli: Results concerning the modeled and observed tidal factors

2009

Continuous gravity observations performed in the last few years, both at Mt. Etna and Stromboli, have prompted the need to improve the tidal analysis in order to acquire the best corrected data for the detection of volcano related signals. On Mt. Etna, the sites are very close to each other and the expected tidal factor differences are negligible. It is thus useful to unify the tidal analysis results of the different data sets in a unique tidal model. This tidal model, which can be independently confirmed by a modeling of the tidal parameters based on the elastic response of the Earth to tidal forces and the computation of the ocean tides effects on gravity, is very useful for the precise t…

Gravity (chemistry)geographygeography.geographical_feature_categorylcsh:QC801-809Astrophysics::Cosmology and Extragalactic AstrophysicsGeophysicslcsh:QC851-999GeodesyPhysics::GeophysicsTidal gravity modelslcsh:Geophysics. Cosmic physicsGeophysicsTidal ModelVolcanoTidal loadingTidal forceOcean tidelcsh:Meteorology. ClimatologyAstrophysics::Earth and Planetary AstrophysicsSensitivity (control systems)Tidal gravity models - Mt.Etna - La Coste and Romberg gravimeters - tidal loadingAstrophysics::Galaxy AstrophysicsGeology
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A network of superconducting gravimeters as a detector of matter with feeble nongravitational coupling

2020

Abstract Hidden matter that interacts only gravitationally would oscillate at characteristic frequencies when trapped inside of Earth. For small oscillations near the center of the Earth, these frequencies are around 300 μHz. Additionally, signatures at higher harmonics would appear because of the non-uniformity of Earth’s density. In this work, we use data from a global network of gravimeters of the International Geodynamics and Earth Tide Service (IGETS) to look for these hypothetical trapped objects. We find no evidence for such objects with masses on the order of 1014 kg or greater with an oscillation amplitude of 0.1 re. It may be possible to improve the sensitivity of the search by s…

Physics010308 nuclear & particles physicsGravimeter530 PhysicsInner coreAstronomyEarth tideGeodynamics530 Physik01 natural sciencesAtomic and Molecular Physics and OpticsPhysics::GeophysicsCoupling (physics)Orders of magnitude (time)HarmonicsPhysics::Space Physics0103 physical sciencesAstrophysics::Earth and Planetary Astrophysics010306 general physicsNoise (radio)
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Properties of the Binary Neutron Star Merger GW170817

2019

On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. In this work, we improve initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data. We extend the range of gravitational-wave frequencies considered down to 23 Hz, compared to 30 Hz in the initial analysis. We also compare results inferred using several signal models, which ar…

AstrofísicaGravitacióneutron star: binaryAstronomyGeneral Physics and AstronomyBinary numberAstrophysicsELECTROMAGNETIC COUNTERPARTspin01 natural sciencesGeneral Relativity and Quantum CosmologyGRAVITATIONAL-WAVESlocalization010305 fluids & plasmasGravitational wave detectorsEQUATIONenergy: densityLIGOGEO600QCastro-ph.HESettore FIS/01PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSSettore FIS/05PhysicsEquations of stateGravitational effectsGravitational-wave signalsDeformability parameterAmplitudePhysical SciencesPhysical effectsINSPIRALING COMPACT BINARIES[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Spectral energy densityAstrophysics - High Energy Astrophysical PhenomenaPARAMETER-ESTIMATIONBinary neutron starsdata analysis methodgr-qcQC1-999Physics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesBayesianGravimeterselectromagnetic field: productionPhysics and Astronomy (all)galaxy: binary0103 physical sciencesddc:530SDG 7 - Affordable and Clean Energy010306 general physicsgravitational radiation: frequencySTFCAstrophysics::Galaxy Astrophysicsequation of stateLIGHT CURVESEquation of stateScience & Technology/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energySpinsgravitational radiationRCUKSpectral densityKILONOVATRANSIENTSbinary: compactStarsGEO600GalaxyLIGOgravitational radiation detectorNeutron starVIRGOPhysics and Astronomygravitational radiation: emissionRADIATIONBayesian AnalysisDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Balances for Special Applications

2014

Some special applications and the corresponding balances are described in detail: laboratory balances, micro balances vacuum balances, thermo balances, magnetic suspension balances, oscillators, metrological comparators, tensiometer, suspended particles and elementary charge, mass analyser, density determination, particle analysis, magnetic susceptibility, post office and coin scales, body scales, and gravimeter. Vacuum equipment for balances, thermogravimetry, sorptometry, hygrometry, and moisture determination, gravimetric measurement of reaction kinetics, surface tension, ion traps, pyknometry, dust and particle concentration, grain size analysis are described. Gravimetric measurement of…

Surface tensionTensiometer (soil science)Materials scienceMoistureGravimeterAnalyserParticle-size distributionGravimetric analysisParticleMechanics
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