Search results for "Geophysic"

showing 10 items of 2684 documents

Determination of sea surface temperature at large observation angles using an angular and emissivity-dependent split-window equation

2007

Abstract This paper proposes an angular and emissivity-dependent split-window equation that permits the determination of the sea surface temperature (SST) to a reasonable level of accuracy for any observation angle, including large viewing angles at the image edges of satellite sensors with wide swaths. This is the case of the MODIS radiometer both on EOS Terra/Aqua platforms, with observation angles of up to 65° at the surface, for which the split-window equation has been developed in this study. The algorithm takes into account the angular dependence of both the atmospheric correction (due to the increase of the atmospheric optical path with angle) and the emissivity correction (since sea…

PhysicsBrightnessRadiometerAtmospheric correctionSoil ScienceGeologyPhysics::GeophysicsSea surface temperatureEmissivityRadiometrySatelliteBlack-body radiationComputers in Earth SciencesPhysics::Atmospheric and Oceanic PhysicsRemote sensingRemote Sensing of Environment
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Messungen der Himmelsstrahlung und deren Polarisationsgrad während der Sonnenfinsternis am 15.2.1961 in Viareggio (Italien)

1961

On the occasion of the total solar eclipse in Viareggio (Italy) measurements of intensity of sky radiation and polarization have been carried out at 90 degrees vertical distance from the sun. UV-, green- and red-filters have been used. The results showed a diminution of the intensity during the eclipse of about 3 powers of ten. The sky brightness in the point 90 degrees distant during the total eclipse was similar to the brightness when sun is 7 degrees below the horizon. About one minute before the total eclipse the degree of polarization diminuished to zero. — Furthermore photos of nearly the total sky were made using two cameras with wide angle lenses.

PhysicsBrightnessbusiness.industrySolar eclipsemedia_common.quotation_subjectDiffuse sky radiationVertical distanceAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsPolarization (waves)GeophysicsOpticsGeochemistry and PetrologySkyAstrophysics::Solar and Stellar AstrophysicsDegree of polarizationAstrophysics::Earth and Planetary AstrophysicsbusinessAstrophysics::Galaxy Astrophysicsmedia_commonGeofisica Pura e Applicata
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Digital rock physics, chemistry, and biology: challenges and prospects of pore-scale modelling approach

2021

Abstract Conventional and unconventional hydrocarbon rocks have complicated pore structures with heterogeneities distributed over various length scales (from nanometre to centimetre or even larger scales). Effective characterization of the properties of such rocks based on their digital twins is a challenging task. Digital rock physics (DRP) can be used to quantify the structural and morphological parameters of rocks directly and predict flow transport properties at the pore scale. Digital rock chemistry (DRC) or biology (DRB) applies when the changes in pore structures are due to interaction with solutes or microbial activities. Fluid–rock interactions or microbial activities complicate fl…

PhysicsChemistryFlow (psychology)Direct numerical simulation010501 environmental sciencesBiology010502 geochemistry & geophysics01 natural sciencesPollutionCharacterization (materials science)Permeability (earth sciences)Geochemistry and PetrologyVoid (composites)Fluid dynamicsEnvironmental ChemistryPorosityBiological system0105 earth and related environmental sciencesNetwork modelApplied Geochemistry
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Instabilities in a staircase stratified shear flow

2017

We study stratified shear flow instability where the density profile takes the form of a staircase of interfaces separating uniform layers. Internal gravity waves riding on density interfaces can r...

PhysicsComputational MechanicsAstronomy and Astrophysics02 engineering and technology01 natural sciencesInstability010305 fluids & plasmasPhysics::Fluid DynamicsInternal gravity wave020303 mechanical engineering & transportsGeophysicsClassical mechanics0203 mechanical engineeringGeochemistry and PetrologyMechanics of Materials0103 physical sciencesShear flowGeophysical & Astrophysical Fluid Dynamics
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Self-similarity and scaling of thermal shock fractures

2013

The problem of crack pattern formation due to thermal shock loading at the surface of half-space is solved numerically using two-dimensional boundary element method. The results of numerical simulations with 100-200 random simultaneously growing and interacting cracks are used to obtain scaling relations for crack length and spacing. The numerical results predict that such process of pattern formation with quasi-static crack growth is not stable and at some point the excess energy leads to unstable propagation of one of the longest crack. The onset of instability has also been determined from numerical results.

PhysicsCondensed Matter - Materials ScienceThermal shockSelf-similaritySurface PropertiesTemperatureMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesPattern formationMechanicsCondensed Matter - Soft Condensed MatterHalf-spacePhysics::Classical PhysicsInstabilityPhysics::GeophysicsCondensed Matter::Materials ScienceSoft Condensed Matter (cond-mat.soft)Stress MechanicalScalingBoundary element methodQuasistatic processMechanical PhenomenaPhysical Review E
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Illustration of microphysical processes in Amazonian deep convective clouds in the gamma phase space: introduction and potential applications

2017

Abstract. The behavior of tropical clouds remains a major open scientific question, resulting in poor representation by models. One challenge is to realistically reproduce cloud droplet size distributions (DSDs) and their evolution over time and space. Many applications, not limited to models, use the gamma function to represent DSDs. However, even though the statistical characteristics of the gamma parameters have been widely studied, there is almost no study dedicated to understanding the phase space of this function and the associated physics. This phase space can be defined by the three parameters that define the DSD intercept, shape, and curvature. Gamma phase space may provide a commo…

PhysicsConvectionAtmospheric Science010504 meteorology & atmospheric sciencesMicrophysicsSpacetimeMeteorologybusiness.industryCloud computingFunction (mathematics)010502 geochemistry & geophysicsCurvature01 natural sciencesMETEOROLOGIA FÍSICAlcsh:QC1-999lcsh:Chemistrylcsh:QD1-99913. Climate actionPhase spaceddc:550Statistical physicsbusinessRepresentation (mathematics)lcsh:Physics0105 earth and related environmental sciences
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A Non-normal-Mode Marginal State of Convection in a Porous Rectangle

2019

Author's accepted manuscript (postprint). This is a post-peer-review, pre-copyedit version of an article published in Transport in Porous Media. The final authenticated version is available online at: http://dx.doi.org/10.1007/s11242-019-01263-5. The fourth-order Darcy–Bénard eigenvalue problem for onset of thermal convection in a 2D rectangular porous box is investigated. The conventional type of solution has normal-mode dependency in at least one of the two spatial directions. The present eigenfunctions are of non-normal-mode type in both the horizontal and the vertical direction. A numerical solution is found by the finite element method, since no analytical method is known for this non-…

PhysicsConvectionConvective heat transferGeneral Chemical Engineering0208 environmental biotechnologyBoundary (topology)02 engineering and technologyMechanics010502 geochemistry & geophysicsVDP::Matematikk og Naturvitenskap: 400::Matematikk: 41001 natural sciencesCatalysisFinite element method020801 environmental engineeringHeat fluxNormal modeThermalRectangle0105 earth and related environmental sciencesTransport in Porous Media
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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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