Search results for "Physics - Geophysics"

showing 10 items of 26 documents

Smap-based retrieval of vegetation opacity and albedo

2020

Over land the vegetation canopy affects the microwave brightness temperature by emission, scattering and attenuation of surface soil emission. The questions addressed in this study are: 1) what is the transparency of the vegetation canopy for different biomes around the Globe at the low-frequency L-band?, 2) what is the seasonal amplitude of vegetation microwave optical depth for different biomes?, 3) what is the effective scattering at this frequency for different vegetation types?, 4) what is the impact of imprecise characterization of vegetation microwave properties on retrieval of soil surface conditions? These questions are addressed based on the recently completed one full annual cycl…

010504 meteorology & atmospheric sciencesBiome0211 other engineering and technologiesFOS: Physical sciences02 engineering and technology15. Life on landAlbedoAnnual cycle01 natural sciencesGeophysics (physics.geo-ph)Physics - GeophysicsMicrowave imaging13. Climate actionBrightness temperaturemedicineEnvironmental sciencemedicine.symptomVegetation (pathology)Water contentOptical depth021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensing2017 IEEE International Geoscience and Remote Sensing Symposium (IGARSS)
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GIGJ: a crustal gravity model of the Guangdong Province for predicting the geoneutrino signal at the JUNO experiment

2019

Gravimetric methods are expected to play a decisive role in geophysical modeling of the regional crustal structure applied to geoneutrino studies. GIGJ (GOCE Inversion for Geoneutrinos at JUNO) is a 3D numerical model constituted by ~46 x 10$^{3}$ voxels of 50 x 50 x 0.1 km, built by inverting gravimetric data over the 6{\deg} x 4{\deg} area centered at the Jiangmen Underground Neutrino Observatory (JUNO) experiment, currently under construction in the Guangdong Province (China). The a-priori modeling is based on the adoption of deep seismic sounding profiles, receiver functions, teleseismic P-wave velocity models and Moho depth maps, according to their own accuracy and spatial resolution. …

010504 meteorology & atmospheric sciencesGeoneutrinogeophysical uncertaintieInverse transform samplingFOS: Physical sciences01 natural sciencesBayesian methodUpper middle and lower crustStandard deviationNOSouth China BlockmiddlePhysics - GeophysicsMonte Carlo stochastic optimizationGOCE data gravimetric inversionGeophysical uncertaintiesGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Bayesian method; geophysical uncertainties; GOCE data gravimetric inversion; Monte Carlo stochastic optimization; South China Block; upper middle and lower crustImage resolution0105 earth and related environmental sciencesSubdivisionJiangmen Underground Neutrino Observatoryupper and middle and lower crustbusiness.industrySettore FIS/01 - Fisica SperimentaleCrustupperGeodesy[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Geophysics (physics.geo-ph)and lower crustDepth soundingGeophysics13. Climate actionSpace and Planetary SciencebusinessGeologyBayesian method geophysical uncertainties GOCE data gravimetric inversion Monte Carlo stochastic optimization South China Blockupper and middle and lower crust
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Growth of stylolite teeth patterns depending on normal stress and finite compaction

2007

Abstract Stylolites are spectacular rough dissolution surfaces that are found in many rock types. They are formed during a slow irreversible deformation in sedimentary rocks and therefore participate to the dissipation of tectonic stresses in the Earth's upper crust. Despite many studies, their genesis is still debated, particularly the time scales of their formation and the relationship between this time and their morphology. We developed a new discrete simulation technique to explore the dynamic growth of the stylolite roughness, starting from an initially flat dissolution surface. We demonstrate that the typical steep stylolite teeth geometry can accurately be modelled and reproduce natu…

010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph][SDE.MCG]Environmental Sciences/Global ChangesCompactionFOS: Physical sciencesMineralogyGeometry[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Surface finish010502 geochemistry & geophysics01 natural sciencesPhysics::GeophysicsPhysics - GeophysicsStress (mechanics)Geochemistry and Petrology[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistryEarth and Planetary Sciences (miscellaneous)Scaling0105 earth and related environmental sciencesElastic energyDissipation[SDE.MCG.CPE]Environmental Sciences/Global Changes/domain_sde.mcg.cpeGeophysics (physics.geo-ph)GeophysicsAmplitudeSpace and Planetary ScienceStyloliteGeologyEarth and Planetary Science Letters
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Are oxygen isotope fractionation factors between calcite and water derived from speleothems systematically biased due to prior calcite precipitation …

2021

Abstract The equilibrium oxygen isotope fractionation factor between calcite and water (18αcalcite/H2O) is an important quantity in stable isotope geochemistry and allows in principle to infer temperature variations from carbonate δ18O if carbonate formation occurred in thermodynamic equilibrium. For this reason, many studies intended to determine the value of the oxygen isotope fractionation factor between calcite and water (18αcalcite/H2O) for a wide range of temperatures using modern cave calcite and the corresponding cave drip water or ancient speleothem carbonate and fluid inclusion samples. However, the picture that emerges from all of these studies indicates that speleothem calcite i…

Calcitegeographygeography.geographical_feature_categoryStalactite010504 meteorology & atmospheric sciencesChemistryFOS: Physical sciencesSpeleothemMineralogyStalagmite010502 geochemistry & geophysics01 natural sciencesIsotopes of oxygenGeophysics (physics.geo-ph)Physics - Geophysicschemistry.chemical_compoundCaveGeochemistry and PetrologyIsotope geochemistryCarbonate0105 earth and related environmental sciences
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Recent progress on the characterization of the high-pressure behaviour of AVO4 orthovanadates

2018

AVO4 vanadates are materials of technological importance due to their variety of functional properties. They have applications as scintillators, thermophosphors, photocatalysts, cathodoluminescence, and laser-host materials. Studies at HP-HT are helpful for understanding the physical properties of the solid state, in special, the phase behavior of AVO4 materials. For instance, they have contributed to understand the macroscopic properties of vanadates in terms of microscopic mechanisms. A great progress has been made in the last decade towards the study of the pressure-effects on the structural, vibrational, and electronic properties of AVO4 compounds. Thanks to the combination of experimen…

Condensed Matter - Materials ScienceMaterials scienceFuture studiesResearch groupsSolid-stateMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesNanotechnologyPhysics - Applied PhysicsApplied Physics (physics.app-ph)02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesGeophysics (physics.geo-ph)Characterization (materials science)Physics - GeophysicsHigh pressure0103 physical sciencesGeneral Materials Science010306 general physics0210 nano-technologyElectronic propertiesProgress in Materials Science
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Effects of high-pressure on the structural, vibrational, and electronic properties of monazite-type PbCrO4

2012

We have performed an experimental study of the crystal structure, lattice dynamics, and optical properties of PbCrO 4 (the mineral crocoite) at ambient and high pressures. In particular, the crystal structure, Raman-active phonons, and electronic band gap have been accurately determined. X-ray-diffraction, Raman, and optical absorption experiments have allowed us also to completely characterize two pressure-induced structural phase transitions. The first transition is from a monoclinic structure to another monoclinic structure. It maintains the symmetry of the crystal but has important consequences in the physical properties; among others, a band-gap collapse is induced. The second one invo…

CrocoiteZirconMaterials scienceOrthophosphatesFOS: Physical sciencesElectronic structureCrystal structureType (model theory)CrystalPhysics - Geophysicssymbols.namesakeCrocoitePhysics - Chemical PhysicsCrystalChemical Physics (physics.chem-ph)Condensed Matter - Materials ScienceCondensed matter physicsMetalTemperatureMaterials Science (cond-mat.mtrl-sci)SpectraCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsGeophysics (physics.geo-ph)FISICA APLICADAX-ray crystallographyTransitionsymbolsRaman spectroscopySrCrO4Monoclinic crystal system
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High-pressure structural investigation of several zircon-type orthovanadates

2009

Room temperature angle-dispersive x-ray diffraction measurements on zircon-type EuVO4, LuVO4, and ScVO4 were performed up to 27 GPa. In the three compounds we found evidence of a pressure-induced structural phase transformation from zircon to a scheelite-type structure. The onset of the transition is near 8 GPa, but the transition is sluggish and the low- and high-pressure phases coexist in a pressure range of about 10 GPa. In EuVO4 and LuVO4 a second transition to a M-fergusonite-type phase was found near 21 GPa. The equations of state for the zircon and scheelite phases are also determined. Among the three studied compounds, we found that ScVO4 is less compressible than EuVO4 and LuVO4, b…

DiffractionStructural phaseCondensed Matter - Materials ScienceMaterials sciencebusiness.industryMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesType (model theory)Condensed Matter PhysicsElectronic Optical and Magnetic MaterialsGeophysics (physics.geo-ph)Pressure rangePhysics - Geophysicschemistry.chemical_compoundCrystallographyOpticschemistryHigh pressureScheelitePhase (matter)businessZircon
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Infrasonic, Acoustic and Seismic Waves Produced by the Axion Quark Nuggets

2022

We advocate an idea that the Axion Quark Nuggets (AQN) hitting the Earth can be detected by analysing the infrasound, acoustic and seismic waves which always accompany the AQN's passage in the atmosphere and underground. Our estimates for the infrasonic frequency $\nu\simeq 5$ ~Hz and overpressure $\delta p\sim 0.3 ~$Pa for relatively large size dark matter (DM) nuggets suggest that sensitivity of presently available instruments is already sufficient to detect very intense (but very rare) events today with existing technology. A study of much more frequent but less intense events requires a new type of instruments. We propose a detection strategy for a systematic study to search for such re…

Earth and Planetary Astrophysics (astro-ph.EP)570Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)General MathematicsFOS: Physical sciencesGeophysics (physics.geo-ph)Physics - GeophysicsHigh Energy Physics - PhenomenologyPhysics - Atmospheric and Oceanic PhysicsHigh Energy Physics - Phenomenology (hep-ph)Chemistry (miscellaneous)ddc:570Atmospheric and Oceanic Physics (physics.ao-ph)Computer Science (miscellaneous)dark matter; axion; quark nuggetsAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics - Earth and Planetary AstrophysicsSymmetry
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Nonlinear PCA for Spatio-Temporal Analysis of Earth Observation Data

2020

Remote sensing observations, products, and simulations are fundamental sources of information to monitor our planet and its climate variability. Uncovering the main modes of spatial and temporal variability in Earth data is essential to analyze and understand the underlying physical dynamics and processes driving the Earth System. Dimensionality reduction methods can work with spatio-temporal data sets and decompose the information efficiently. Principal component analysis (PCA), also known as empirical orthogonal functions (EOFs) in geophysics, has been traditionally used to analyze climatic data. However, when nonlinear feature relations are present, PCA/EOF fails. In this article, we pro…

Earth observationComputer scienceFeature extraction0211 other engineering and technologiesFOS: Physical sciencesEmpirical orthogonal functions02 engineering and technologyKernel principal component analysisPhysics::GeophysicsData cubePhysics - GeophysicsKernel (linear algebra)symbols.namesakeElectrical and Electronic EngineeringPhysics::Atmospheric and Oceanic Physics021101 geological & geomatics engineeringDimensionality reductionHilbert spaceComputational Physics (physics.comp-ph)Geophysics (physics.geo-ph)Data setPhysics - Atmospheric and Oceanic Physics13. Climate actionKernel (statistics)Atmospheric and Oceanic Physics (physics.ao-ph)Principal component analysissymbolsGeneral Earth and Planetary SciencesSpatial variabilityAlgorithmPhysics - Computational Physics
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Magnetic field dynamos and magnetically triggered flow instabilities

2017

The project A2 of the LIMTECH Alliance aimed at a better understanding of those magnetohydrodynamic instabilities that are relevant for the generation and the action of cosmic magnetic fields. These comprise the hydromagnetic dynamo effect and various magnetically triggered flow instabilities, such as the magnetorotational instability and the Tayler instability. The project was intended to support the experimental capabilities to become available in the framework of the DREsden Sodium facility for DYNamo and thermohydraulic studies (DRESDYN). An associated starting grant was focused on the dimensioning of a liquid metal experiment on the newly found magnetic destabilization of rotating flow…

F300FOS: Physical sciencesF5007. Clean energy01 natural sciencesInstability010305 fluids & plasmasPhysics - GeophysicsMagnetorotational instability0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic drive[NLIN]Nonlinear Sciences [physics]010306 general physicsPhysics[PHYS]Physics [physics]Fluid Dynamics (physics.flu-dyn)MechanicsPhysics - Fluid Dynamics[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Magnetic fieldGeophysics (physics.geo-ph)Shear (sheet metal)Flow (mathematics)Dynamo theory[NLIN.NLIN-CD]Nonlinear Sciences [physics]/Chaotic Dynamics [nlin.CD][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Dynamo
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