Search results for "C [PolyI]"

showing 10 items of 30703 documents

Environmental and biological factors are joint drivers of mercury biomagnification in subarctic lake food webs along a climate and productivity gradi…

2021

Subarctic lakes are getting warmer and more productive due to the joint effects of climate change and intensive land-use practices (e.g. forest clear-cutting and peatland ditching), processes that potentially increase leaching of peat- and soil-stored mercury into lake ecosystems. We sampled biotic communities from primary producers (algae) to top consumers (piscivorous fish), in 19 subarctic lakes situated on a latitudinal (69.0-66.5 degrees N), climatic (+3.2 degrees C temperature and +30% precipitation from north to south) and catchment land-use (pristine to intensive forestry areas) gradient. We first tested how the joint effects of climate and productivity influence mercury biomagnific…

010504 meteorology & atmospheric sciencesBiomagnificationTROPHIC POSITIONmaankäyttö010501 environmental sciencesMETHYLMERCURY01 natural sciencesFood chainBiological FactorsONTARIO LAKESCHAIN STRUCTUREClimate changeympäristömyrkytWaste Management and DisposalLand-useApex predatorTrophic levelkalatStable isotopes2. Zero hungerFRESH-WATEREcologyFishesvesiekosysteemitBIOACCUMULATIONselkärangattomatPollutionSubarctic climateclimate changeProductivity (ecology)Environmental MonitoringFood chain lengthEnvironmental EngineeringFood Chainelohopeachemistry.chemical_elementstable isotopeskasautuminenWHITEFISHland-useEnvironmental ChemistryAnimalsravintoketjutEcosystem1172 Environmental sciences0105 earth and related environmental sciencesfishfood chain lengthLake ecosystemMercury15. Life on landilmastonmuutoksetCHARR SALVELINUS-ALPINUSinvertebratesInvertebratesMercury (element)LakesFishchemistryisotooppianalyysi13. Climate actionEnvironmental scienceMARINEWater Pollutants Chemical
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High-resolution stimulated Raman spectroscopy and analysis of the nu2, nu5 and 2 nu6 bands of 34SF6

2006

9 p.Special Issue: Nineteenth Colloquium on High Resolution Molecular Spectroscopy, Salamanca 11–16 September 2005

010504 meteorology & atmospheric sciencesBiophysicsAnalytical chemistryHigh resolution01 natural sciencesPreliminary analysisREGIONsymbols.namesakeMOLECULES0103 physical sciencesMoleculeStimulated ramanPhysical and Theoretical ChemistrySpectroscopyMolecular BiologyNU(3) BANDEMISSIONS0105 earth and related environmental sciences[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]SPECTRUM010304 chemical physicsChemistryCOMBINATION BANDCondensed Matter Physics3. Good healthOctahedron[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]NON-CO2 GREENHOUSE GASESsymbolsRaman spectroscopySF6
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Controlled time integration for the numerical simulation of meteor radar reflections

2016

We model meteoroids entering the Earth[U+05F3]s atmosphere as objects surrounded by non-magnetized plasma, and consider efficient numerical simulation of radar reflections from meteors in the time domain. Instead of the widely used finite difference time domain method (FDTD), we use more generalized finite differences by applying the discrete exterior calculus (DEC) and non-uniform leapfrog-style time discretization. The computational domain is presented by convex polyhedral elements. The convergence of the time integration is accelerated by the exact controllability method. The numerical experiments show that our code is efficiently parallelized. The DEC approach is compared to the volume …

010504 meteorology & atmospheric sciencesComputer scienceMETEORPLASMATIC OBJECTSRADAR REFLECTIONS01 natural sciencesplasmatic objectslaw.inventionINTEGRAL EQUATIONSlawRadar010303 astronomy & astrophysicsSpectroscopyEARTH ATMOSPHEREvolume integral equationRadiationPLASMANUMERICAL MODELSMathematical analysisFinite differenceNUMERICAL METHODMETEORSAtomic and Molecular Physics and OpticsCALCULATIONSControllabilityDISCRETE EXTERIOR CALCULUSAstrophysics::Earth and Planetary AstrophysicsMAGNETOPLASMADiscretizationRADAR REFLECTIONTIME DOMAIN ANALYSISVOLUME INTEGRAL EQUATIONdiscrete exterior calculusELECTROMAGNETIC SCATTERINGOpticsFINITE DIFFERENCE TIME DOMAIN METHOD0103 physical sciencesSCATTERINGTime domainmeteorsNUMERICAL METHODS0105 earth and related environmental sciencesta113ta114Computer simulationbusiness.industryta111Finite-difference time-domain methodRADARDiscrete exterior calculuselectromagnetic scatteringradar reflectionsELECTROMAGNETIC METHODmeteoritbusinessJournal of Quantitative Spectroscopy and Radiative Transfer
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The Influence of Crystal Size Distributions on the Rheology of Magmas: New Insights From Analog Experiments

2017

This study examines the influence of particle size distributions on the rheology of particle suspensions by using analogue experiments with spherical glass beads in silicone oil as magma equivalent. The analyses of 274 individual particle-bearing suspensions of varying modality (uni-, bi- tri- and tetramodality), as well as of polymodal suspensions with specific defined skewness and variance, are the first data set of its kind and provide important insights in the relationship between the solid particles of a suspension and its rheological behaviour. Since the relationship between the rheology of particle bearing suspensions and its maximum packing fraction ϕm is well established by several…

010504 meteorology & atmospheric sciencesDispersityMineralogyThermodynamics010502 geochemistry & geophysicsAtomic packing factor01 natural sciencesViscosityGeophysicsRheologyGeochemistry and PetrologyParticle-size distributionParticleParticle sizeSuspension (vehicle)Geology0105 earth and related environmental sciencesGeochemistry, Geophysics, Geosystems
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Ocean Acidification and the End-Permian Mass Extinction: To What Extent does Evidence Support Hypothesis?

2012

International audience; Ocean acidification in modern oceans is linked to rapid increase in atmospheric CO 2 , raising concern about marine diversity, food security and ecosystem services. Proxy evidence for acidification during past crises may help predict future change, but three issues limit confidence of comparisons between modern and ancient ocean acidification, illustrated from the end-Permian extinction, 252 million years ago: (1) problems with evidence for ocean acidification preserved in sedimentary rocks, where proposed marine dissolution surfaces may be subaerial. Sedimentary evidence that the extinction was partly due to ocean acidification is therefore inconclusive; (2) Fossils…

010504 meteorology & atmospheric sciencesEffects of global warming on oceansocean acidification010502 geochemistry & geophysics01 natural sciencesEcosystem services14. Life underwaterPermian–Triassic extinction event0105 earth and related environmental sciences[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/PaleontologyHigh rateend-Permian extinctionocean acidification; end-Permian extinction; microbialite; ocean buffer; stylolitestylolitelcsh:QE1-996.5fungiBiotaOcean acidificationlcsh:GeologyOceanographymicrobialite13. Climate actionSubaerialGeneral Earth and Planetary SciencesSedimentary rock[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/Paleontologyocean bufferGeologygeographic locations
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Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: Magnetic Channelling

2016

Dense plasma fragments were observed to fall back on the solar surface by the Solar Dynamics Observatory after an eruption on 7 June 2011, producing strong EUV brightenings. Previous studies investigated impacts in regions of weak magnetic field. Here we model the $\sim~300$ km/s impact of fragments channelled by the magnetic field close to active regions. In the observations, the magnetic channel brightens before the fragment impact. We use a 3D-MHD model of spherical blobs downfalling in a magnetized atmosphere. The blob parameters are constrained from the observation. We run numerical simulations with different ambient density and magnetic field intensity. We compare the model emission i…

010504 meteorology & atmospheric sciencesField (physics)FOS: Physical sciencesAstrophysics01 natural sciencesAtmosphereSettore FIS/05 - Astronomia E AstrofisicaSun: activity0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetic pressureSun: magnetic field010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSun: coronaAstronomy and AstrophysicsSun: UV radiation Supporting material: animationPlasmaCoronal loopAstronomy and AstrophysicRam pressureMagnetic fieldStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space Physics
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Geophysical prospection of the Roman city of Pollentia, Alcúdia (Mallorca, Balearic Islands, Spain)

2016

Abstract We present the results of the geophysical investigation carried out in the Roman city of Pollentia, in the island of Mallorca. The ancient city was identified in the 19th century. Old and new archaeological excavations have helped to uncover a residential area, a theatre, the forum, several necropolises and other remains of the city, but a large unexplored area has still to be investigated. For instance, the limits of the ancient town and the presence of harbour structures are still unknown. The geophysical survey has covered an area of more than 20.000 m2 by integrating magnetic, electromagnetic, electrical and ground penetrating radar (GPR) methods. Many unseen archaeological fea…

010504 meteorology & atmospheric sciencesGPRMagneticgovernment.political_district010502 geochemistry & geophysics01 natural sciencesSettore GEO/11 - Geofisica ApplicataElectrical resistivity tomographyElectrical resistivity tomographyArchaeological prospection0105 earth and related environmental sciencescomputer.programming_languagegeographyBalearic islandsgeography.geographical_feature_categoryEM surveyExcavationcomputer.file_formatArchaeologyResidential areaGeophysicsPollentiaGeophysical survey (archaeology)VRMLHarbourGround-penetrating radargovernmentArchaeological prospection; Electrical resistivity tomography; EM survey; GPR; Magnetic; Pollentia; GeophysicscomputerJournal of Applied Geophysics
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Rare earths behaviour during the deposition of volcanic sublimates

2017

Abstract In this study, the REE distribution between volcanic fluids and related solids in fumaroles with temperatures ranging from approximately 100 to 421 °C was investigated in different geological scenarios. The treatment of geochemical REE data was carried out by calculating the REE enrichment factors (EF REE ) relative to the volcanic host rocks in studied sites under the assumption that the REE transport takes place as silicate aerosol in volcanic fluids. Shale-normalised REE concentrations in these fluids have been assessed to investigate whether the REE transport as aqueous complexes in water-saturated volcanic gas is reasonable. The REE behaviour in alkaline condensates according …

010504 meteorology & atmospheric sciencesGeochemistryVolcanic condensatesSublimate010502 geochemistry & geophysicsVolcanic condensate01 natural sciencesAnthropogenic pollutionchemistry.chemical_compoundGd anomalyGeochemistry and PetrologySublimatesGeophysic0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryVolcanic islandsREESilicateFumaroleAerosolGeophysicsDeposition (aerosol physics)chemistryVolcanoVolcanic island[SDU]Sciences of the Universe [physics]Geology
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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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IceCube Search for High-Energy Neutrino Emission from TeV Pulsar Wind Nebulae

2020

Pulsar wind nebulae (PWNe) are the main gamma-ray emitters in the Galactic plane. They are diffuse nebulae that emit nonthermal radiation. Pulsar winds, relativistic magnetized outflows from the central star, shocked in the ambient medium produce a multiwavelength emission from the radio through gamma-rays. Although the leptonic scenario is able to explain most PWNe emission, a hadronic contribution cannot be excluded. A possible hadronic contribution to the high-energy gamma-ray emission inevitably leads to the production of neutrinos. Using 9.5 yr of all-sky IceCube data, we report results from a stacking analysis to search for neutrino emission from 35 PWNe that are high-energy gamma-ray…

010504 meteorology & atmospheric sciencesHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaNeutrino astronomy; High energy astrophysicsFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyPulsar0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstronomy and AstrophysicsGalactic planeCOSMIC-RAYSCRAB-NEBULACrab NebulaPhysics and AstronomyNeutrino astronomy13. Climate actionSpace and Planetary ScienceGALACTIC SOURCESDISCOVERYPhysique des particules élémentairesHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsGAMMA-RAY EMISSIONLepton
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