Search results for "waves"

showing 10 items of 1766 documents

PHYSICS-based retrieval of scattering albedo and vegetation optical depth using multi-sensor data integration

2017

Vegetation optical depth and scattering albedo are crucial parameters within the widely used τ-ω model for passive microwave remote sensing of vegetation and soil. A multi-sensor data integration approach using ICESat lidar vegetation heights and SMAP radar as well as radiometer data enables a direct retrieval of the two parameters on a physics-derived basis. The crucial step within the retrieval methodology is the calculus of the vegetation scattering coefficient KS, where one exact and three approximated solutions are provided. It is shown that, when using the assumption of a randomly oriented volume, the backscatter measurements of the radar provide a sufficient first order estimate and …

010504 meteorology & atmospheric sciencesScattering albedo0208 environmental biotechnologyradiometry02 engineering and technologyretrieval methodologycomputer.software_genre01 natural scienceslaw.inventionlawremote sensing by radarRadaractive-passive microwavesPhysics::Atmospheric and Oceanic PhysicsIndexespassive microwave remote sensingRemote sensingremote sensing by laser beamGeographyLidaroptical radarcrucial parametersmedicine.symptomvegetation scattering coefficientData integrationBackscattervegetation mappingta1171τ-ω modelsoilPhysics::GeophysicsICESat lidar vegetation heightsvegetationmedicineVegetation optical depthbackscatter0105 earth and related environmental sciencesRemote sensingsensor fusionRadiometerScatteringnovel multisensor approachSMAPAlbedoMulti-sensor020801 environmental engineeringradiometer dataVegetation (pathology)multisensor data integration approachcomputerICESatalbedo
researchProduct

Slow-Mode Magnetoacoustic Waves in Coronal Loops

2021

Rapidly decaying long-period oscillations often occur in hot coronal loops of active regions associated with small (or micro-) flares. This kind of wave activity was first discovered with the SOHO/SUMER spectrometer from Doppler velocity measurements of hot emission lines, thus also often called "SUMER" oscillations. They were mainly interpreted as global (or fundamental mode) standing slow magnetoacoustic waves. In addition, increasing evidence has suggested that the decaying harmonic type of pulsations detected in light curves of solar and stellar flares are likely caused by standing slow-mode waves. The study of slow magnetoacoustic waves in coronal loops has become a topic of particular…

010504 meteorology & atmospheric sciencesSolar activityFOS: Physical sciencesSolar corona01 natural sciencesStanding wave0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesCoronal seismologyPhysicsOscillationOscillations and wavesAstronomy and AstrophysicsCoronal loopLight curveThermal conductionCoronal loopsComputational physicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamics
researchProduct

Eustasy and sea water Sr composition: application to high-resolution Sr-isotope stratigraphy of Miocene shallow-water carbonates

2007

Oceanic 87 Sr/ 86 Sr-isotope ratios are strongly influenced by rates of silicate weathering and therefore linked not only to glaciation but also to sea-level change. The present study combines analysis of sequence stratigraphy and basin architecture with Sr-isotope stratigraphy in Miocene shallow-water sediments in southern Portugal and Crete (Greece). The common method is to use smoothed global sea water Sr-isotope reference curves but here a different approach is chosen. Instead, measured Sr-isotope curves are correlated with unsmoothed reference curves by identification of similar fluctuations in the order of several 100 kyr. Transgressive intervals are characterized by increasing Sr-iso…

010504 meteorology & atmospheric sciencesStratigraphy550 - Earth sciencesGeologyWeathering010502 geochemistry & geophysics01 natural sciencesSilicateWaves and shallow waterPaleontologychemistry.chemical_compoundStratigraphychemistry13. Climate actionDeglaciationSequence stratigraphySedimentary rock14. Life underwaterChronostratigraphyGeology0105 earth and related environmental sciencesSedimentology
researchProduct

The tsunami phenomenon

2017

Abstract With human activity increasingly concentrating on coasts, tsunamis (from Japanese tsu = harbour, nami = wave) are a major natural hazard to today’s society. Stimulated by disastrous tsunami impacts in recent years, for instance in south-east Asia (2004) or in Japan (2011), tsunami science has significantly flourished, which has brought great advances in hazard assessment and mitigation plans. Based on tsunami research of the last decades, this paper provides a thorough treatise on the tsunami phenomenon from a geoscientific point of view. Starting with the wave features, tsunamis are introduced as long shallow water waves or wave trains crossing entire oceans without major energy l…

010504 meteorology & atmospheric sciencesSubmarineGeologyAquatic ScienceHazard analysis010502 geochemistry & geophysics01 natural sciencesWaves and shallow waterOceanographyWave shoalingNatural hazardSubmarine pipelineSedimentary rockTsunami earthquakeGeologySeismology0105 earth and related environmental sciencesProgress in Oceanography
researchProduct

Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test

2018

Context. The determination from coronagraphic observations of physical parameters of the plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our understanding of the origin and evolution of these phenomena. Aims. The aim of this work is to perform the first ever numerical simulations of a CME as it will be observed by future two-channel (visible light VL and UV Ly-α) coronagraphs, such as the Metis instrument on-board ESA-Solar Orbiter mission, or any other future coronagraphs with the same spectral band-passes. These simulations are then used to test and optimize the plasma diagnostic techniques to be applied to future observations of CMEs. Methods. The CME diagno…

010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)Plasma parametersT-NDASContext (language use)Astrophysics01 natural sciencessymbols.namesakeMethods: data analysis0103 physical sciencesRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]numerical [Methods]Methods: numericalAstronomy and AstrophysicsPlasmaSun: UV radiationPolarization (waves)coronal mass ejections (CMEs) [Sun]Computational physicsQC PhysicsPlasmasSpace and Planetary SciencePhysics::Space PhysicssymbolsMagnetohydrodynamicsDoppler effectAstronomy & Astrophysics
researchProduct

Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations

2021

Gravitational waves provide a unique and powerful opportunity to constrain the dynamics in the interior of proto-neutron stars during core collapse supernovae. Convective motions play an important role in generating neutron stars magnetic fields, which could explain magnetar formation in the presence of fast rotation. We compute the gravitational wave emission from proto-neutron star convection and its associated dynamo, by post-processing three-dimensional MHD simulations of a model restricted to the convective zone in the anelastic approximation. We consider two different proto-neutron star structures representative of early times (with a convective layer) and late times (when the star is…

010504 meteorology & atmospheric sciencesdimension: 3neutron star: magnetic fieldtorusAstrophysicsMagnetar01 natural sciencesrotationstarstrong fieldMagnetarsAstrophysics::Solar and Stellar Astrophysicsgravitational radiation: spectrumgravitational radiation: signatureSupernova core collapse010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMethods numerical[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]formationscalingSupernovaAmplitudeAstrophysics - Solar and Stellar AstrophysicsConvection zoneAstrophysics - High Energy Astrophysical PhenomenaDynamosupernova: collapseprotoneutron starFOS: Physical sciencesConvectionsymmetry: axialGravitational waves0103 physical sciencesstructurenumerical calculationsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesGravitational waveAstronomy and AstrophysicsmagnetarNeutron star13. Climate actionSpace and Planetary Scienceefficiencygravitational radiation: emissionMagnetohydrodynamics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph][PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
researchProduct

Insolation cycles as a major control equatorial Indian Ocean primary production

1997

Analysis of a continuous sedimentary record taken in the Maldives indicates that strong primary production fluctuations (70 to 390 grams of carbon per square meter per year) have occurred in the equatorial Indian Ocean during the past 910,000 years. The record of primary production is coherent and in phase with the February equatorial insolation, whereas it shows diverse phase behavior with δ 18 O, depending on the orbital frequency (eccentricity, obliquity, or precession) examined. These observations imply a direct control of productivity in the equatorial oceanic system by insolation. In the equatorial Indian Ocean, productivity is driven by the wind intensity of westerlies, which is rel…

010504 meteorology & atmospheric sciencesδ18Omedia_common.quotation_subject[SDU.STU]Sciences of the Universe [physics]/Earth SciencesForcing (mathematics)010502 geochemistry & geophysics01 natural sciencesPhysics::Geophysics100000-year problem14. Life underwaterEccentricity (behavior)Physics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesmedia_common[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereMultidisciplinaryEquatorial wavesWesterliesOceanographyProductivity (ecology)13. Climate action[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyClimatologyPhysics::Space PhysicsPrecessionAstrophysics::Earth and Planetary Astrophysics[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/PaleontologyGeology
researchProduct

Climatic fluctuations and seasonality during the Late Jurassic (Oxfordian–Early Kimmeridgian) inferred from delta18O of Paris Basin oyster shells.

2008

10 pages; International audience; Oxygen isotope data from biostratigraphically well-dated oyster shells from the Late Jurassic of the eastern Paris Basin are used to reconstruct the thermal evolution of western Tethyan surface waters during the Early Oxfordian–Early Kimmeridgian interval. Seventy eight oyster shells were carefully screened for potential diagenetic alteration using cathodoluminescence microscopy. Isotope analyses were performed on nonluminescent parts of shells (n=264). Intra-shell δ18O variability was estimated by microsampling along a transect perpendicular to the growth lines of the largest oyster shell. The sinusoidal distribution of the δ18O values along this transect …

010506 paleontologyOysterδ18O[SDE.MCG]Environmental Sciences/Global ChangesJurassic010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesIsotopes of oxygenPaleontologycarbonateGeochemistry and Petrology[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistrybiology.animalParis BasinEarth and Planetary Sciences (miscellaneous)medicinepaleotemperatureBathymetry14. Life underwaterTransect0105 earth and related environmental sciences[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontologybiologyoxygen isotopesSeasonalitymedicine.disease[ SDU.STU.GC ] Sciences of the Universe [physics]/Earth Sciences/GeochemistryDiagenesisWaves and shallow water[ SDE.MCG ] Environmental Sciences/Global ChangesGeophysicsOceanography13. Climate actionSpace and Planetary Science[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphyoysters[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/PaleontologyGeology
researchProduct

Mn/Ca in shells of Arctica islandica (Baltic Sea) – A potential proxy for ocean hypoxia?

2021

Oxygen depletion threatens an increasing number of shallow water environments, specifically habitats below the seasonal halocline in coastal settings of the Baltic Sea. To understand the natural variations of dissolved oxygen levels on seasonal and inter-annual time-scales prior to the instrumental era, high-resolution archives are urgently required. The present study evaluates the potential use of Mn/Ca values in shells of the bivalve, Arctica islandica to infer concentrations of past dissolved oxygen concentrations. This study is based on laser ablation – inductively coupled plasma – mass spectrometry (LA-ICP-MS) data of six contemporaneous specimens and demonstrates that background varia…

0106 biological sciences010504 meteorology & atmospheric sciencesbiology010604 marine biology & hydrobiologyHaloclineHypoxia (environmental)Aquatic ScienceOceanographybiology.organism_classification01 natural sciencesWaves and shallow waterOceanographyWater columnBaltic seaSclerochronologyEnvironmental science14. Life underwaterInductively coupled plasmaArctica islandica0105 earth and related environmental sciences
researchProduct

Epifaunal and infaunal responses to submarine mine tailings in a Norwegian fjord.

2019

Abstract Disposal of mine tailings in marine shallow water ecosystems represents an environmental challenge, and the present paper reports results from a field study in Fraenfjorden, Norway, which is subject to such disposal. Structural and functional responses of benthic infauna and epifauna were investigated along a gradient from heavy tailings deposition to reference conditions. The tailings clearly impacted the faunal composition, with lowered species number close to the outfall. Total abundance of infauna increased in the most impacted area due to dominance of opportunistic species, whereas the epifauna was reduced and represented by a few scattered specimens only. In the most impacted…

0106 biological sciencesAquatic OrganismsGeologic SedimentsIndustrial WasteFjord010501 environmental sciencesAquatic ScienceOceanography01 natural sciencesMiningDominance (ecology)AnimalsEcosystemEcosystem0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryEcologyNorway010604 marine biology & hydrobiologyOutfallSmotheringPollutionTailingsWaves and shallow waterBenthic zoneEnvironmental scienceEstuariesWater Pollutants ChemicalEnvironmental MonitoringMarine pollution bulletin
researchProduct