Search results for "Geophysics"

showing 10 items of 2645 documents

Correlation dimension and affinity of AE data and bicolored noise

1993

This paper is concerned with the general question of the dynamics of the magnetosphere. In general, to solve the dynamics of the magnetosphere one has to solve magnetohydrodynamic equations with some appropriate set of boundary conditions. This results in a very complex solution, which gives indications of being chaotic. The question of the chaotic nature of the magnetospheric dynamics has been addressed by various authors by looking at the correlation dimension of the auroral electrojet index. There has been disagreement on the outcome of such experiments, so the authors report on a detailed analysis of the auroral electrojet index time series. They find a correlation dimension of 3.4. For…

PhysicsCorrelation dimensionSeries (mathematics)ChaoticElectrojetMagnetosphereTheoretical physicsGeophysicsFractalColors of noisePhysics::Space PhysicsSubstormGeneral Earth and Planetary SciencesStatistical physicsGeophysical Research Letters
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THEORETISCHE UNTERSUCHUNG UBER DIE MEHRFACHAUFSTELLUNG VON GEOPHONEN*

1958

The receiving of seismic waves by multiple geophones (geophone-group) is described by a system of coupled differential equations considering only effective resistances. For so-called symmetrical connections of the geophone-group which are used in practice nearly in all cases, a method can be given for solving this system of differential equations. The solutions so derived are valid for seismic waves of any shape. The calculation takes into account the coupling of the geophones as well as the building-up transient oscillations. A suitable measure of superposition is defined, based on the energy transferred during the receiving of the seismic waves. By this means effects similar to interferen…

PhysicsCoupling (physics)Superposition principleGeophysicsGeochemistry and PetrologyMathematical analysisGeophoneTransient (oscillation)Interference (wave propagation)Measure (mathematics)Energy (signal processing)Seismic wavePhysics::GeophysicsGeophysical Prospecting
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A coupled-map model for the magnetotail current sheet

1999

A magnetic field model of the magnetotail current sheet in the form of a coupled-map lattice (CML) is presented. It is a continuously driven and based on the MHD diffusion equation. Solar wind vBs data (solar wind speed multiplied by the southward component of IMF) are used for driving the model, and it is shown to exhibit perturbations (avalanches) with power-law scalings in their distributions of duration and size. Such distributions may indicate self-organized critical (SOC) behavior. Furthermore, it is shown that the power spectra of the model outputs are of bicolor power-law form with different slopes for high and low frequencies. The model parameters determine the frequency of the bre…

PhysicsDiffusion equationSpectral densityGeophysicsPower lawSpectral lineComputational physicsMagnetic fieldCurrent sheetSolar windGeophysicsPhysics::Space PhysicsGeneral Earth and Planetary SciencesMagnetohydrodynamicsGeophysical Research Letters
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Energy oscillations and a possible route to chaos in a modified Riga dynamo

2010

Starting from the present version of the Riga dynamo experiment with its rotating magnetic eigenfield dominated by a single frequency we ask for those modifications of this set-up that would allow for a non-trivial magnetic field behaviour in the saturation regime. Assuming an increased ratio of azimuthal to axial flow velocity, we obtain energy oscillations with a frequency below the eigenfrequency of the magnetic field. These new oscillations are identified as magneto-inertial waves that result from a slight imbalance of Lorentz and inertial forces. Increasing the azimuthal velocity further, or increasing the total magnetic Reynolds number, we find transitions to a chaotic behaviour of th…

PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Lorentz transformationChaoticFluid Dynamics (physics.flu-dyn)Magnetic Reynolds numberFOS: Physical sciencesAstronomy and AstrophysicsPhysics - Fluid DynamicsPhysics - Plasma PhysicsMagnetic fieldGeophysics (physics.geo-ph)Plasma Physics (physics.plasm-ph)Physics::Fluid DynamicsPhysics - Geophysicssymbols.namesakeAxial compressorSpace and Planetary ScienceQuantum electrodynamicsFictitious forcesymbolsSaturation (magnetic)DynamoAstrophysics - Earth and Planetary Astrophysics
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Sensitivity on earth core and mantle densities using atmospheric neutrinos

2009

11 pages, 11 figures.-- ISI article identifier:000267776100008 .-- ArXiv pre-print avaible at: http://arxiv.org/abs/0904.0796

PhysicsEarth and Planetary Astrophysics (astro-ph.EP)business.industrysolar and atmospheric neutrinosNeutrino telescopeFísicaFOS: Physical sciencesAstronomy and AstrophysicsGeophysicsMantle (geology)Physics::GeophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorNondestructive testingUnderwaterNeutrinoAtmospheric neutrinobusinessAstrophysics - Earth and Planetary Astrophysicsneutrino detectors
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Influence of electromagnetic boundary conditions onto the onset of dynamo action in laboratory experiments

2009

We study the onset of dynamo action of the Riga and Karlsruhe experiments with the addition of an external wall, the electro-magnetic properties of which being different from those of the fluid in motion. We consider a wall of different thickness, conductivity and permeability. We also consider the case of a ferro-fluid in motion.

PhysicsFerrofluid[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Mechanics of the fluids [physics.class-ph][SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]Fluid Dynamics (physics.flu-dyn)FOS: Physical sciences[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Physics - Fluid DynamicsConductivity01 natural sciences010305 fluids & plasmas[SPI.MECA.MEFL]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Fluids mechanics [physics.class-ph]Physics::GeophysicsGeophysics (physics.geo-ph)Physics - GeophysicsPhysics::Fluid DynamicsClassical mechanicsPermeability (electromagnetism)0103 physical sciencesBoundary value problem[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph]010306 general physicsDynamo
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Nonlinear energy dissipation in a cellular automaton magnetotail field model

1999

A magnetic field model of the magnetotail current sheet based on cellular automaton (CA) is presented. The present isotropic model is a continuously driven, two-dimensional running CA. The model has a physical interpretation in terms of magnetohydrodynamic (MHD) equations, and features self-organized critical (SOC) behavior with power-law scalings both in durations and sizes of instabilities (avalanches). The model has nonlinear energy dissipation, and shows avalanches with and without an external trigger. Thus the model reproduces some of the statistical features recently observed in the magnetotail.

PhysicsField (physics)MechanicsDissipationCellular automatonMagnetic fieldNonlinear systemCurrent sheetGeophysicsClassical mechanicsPhysics::Space PhysicsGeneral Earth and Planetary SciencesMagnetohydrodynamic driveMagnetohydrodynamicsGeophysical Research Letters
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Measurement of fission products β decay properties using a total absorption spectrometer

2013

In a nuclear reactor, the decay of fission fragments is at the origin of decay heat and antineutrino flux. These quantities are not well known while they are very important for reactor safety and for our understanding of neutrino physics. One reason for the discrepancies observed in the estimation of the decay heat and antineutrinos flux coming from reactors could be linked with the Pandemonium effect. New measurements have been performed at the JYFL facility of Jyvaskyla with a Total Absorption Spectrometer (TAS) in order to circumvent this effect. An overview of the TAS technique and first results from the 2009 measurement campaign will be presented. © Owned by the authors, published by E…

PhysicsFission productsta114SpectrometerFissionPhysicsQC1-999Pandemonium effectParticle detectorPhysics::GeophysicsNuclear physicsHigh Energy Physics::ExperimentNeutrinoDecay heatNuclear ExperimentRadioactive decayEPJ Web of Conferences
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How singular are black hole interiors?

1991

Abstract Ori has recently shown that an astronaut approaching the inner horizon of a black hole is not necessarily torn apart by tidal forces. This raises anew the possibility of astronavigation through black holes, perhaps to other universes. We re-examine this question in the light of hypotheses about probable conditions in the black hole core.

PhysicsGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaWhite holeHorizonGeneral Physics and AstronomyAstrophysicsFuzzballPhysics::GeophysicsBlack holeGeneral Relativity and Quantum Cosmologyde Sitter–Schwarzschild metricNonsingular black hole modelsTidal forcePhysics Letters A
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The Emission of Terrestrial Gamma Ray Flashes From Encountering Streamer Coronae Associated to the Breakdown of Lightning Leaders

2020

Terrestrial gamma‐ray flashes (TGFs) are beams of high‐energy photons associated to lightning. These photons are the bremsstrahlung of energetic electrons whose origin is currently explained by two mechanisms: energizing electrons in weak, but large‐scale thundercloud fields or the acceleration of low‐energy electrons in strong, but localized fields of lightning leaders. Contemporary measurements by the Atmosphere‐Space Interactions Monitor suggest that the production of TGFs is related to the leader step and associated streamer coronae when upwards moving intracloud lightning illuminates. Based on these observations, we apply a particle‐in‐cell Monte Carlo code tracing electrons in the sup…

PhysicsGeophysics010504 meteorology & atmospheric sciences0103 physical sciencesMonte Carlo methodGamma rayGeneral Earth and Planetary SciencesStreamer coronaAstrophysics010306 general physics01 natural sciencesLightning0105 earth and related environmental sciencesGeophysical Research Letters
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