Search results for "Lean"

showing 10 items of 3611 documents

Modelling the Effects of Climate Change on the Supply of Inorganic Nitrogen

2009

Human-induced changes in the nitrogen cycle due to the increased use of artificial fertilisers, the cultivation of nitrogen-fixing crops and atmospheric deposition have made nitrogen pollution to surface waters a long-standing cause for concern. In Europe, legislation has been introduced to minimise the risk of water quality degradation from excessive nitrogen inputs e.g., the European Union Nitrates Directive (EU, 1991), Drinking Water Directive (EU, 1998) and Water Framework Directive (EU, 2000). Coastal regions in particular have been an important focus, since coastal eutrophication has been attributed to increased fluxes of nitrogen from the landscape (Howarth et al., 1996; Boesch et al…

010504 meteorology & atmospheric sciencesEcology0207 environmental engineering02 engineering and technology15. Life on land01 natural sciences6. Clean waterMacrophyteWater Framework Directive13. Climate actionEnvironmental protectionNutrient pollutionDrinking water directiveEnvironmental sciencemedia_common.cataloged_instance14. Life underwaterWater qualityEuropean union020701 environmental engineeringEutrophicationNitrogen cycle0105 earth and related environmental sciencesmedia_common
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Increase inabovegroundfreshlitterquantityover-stimulatessoil respiration inatemperatedeciduousforest

2010

In the context of climate change, the amount of carbon allocated to soil, particularly fresh litter, is predicted to increase with terrestrial ecosystem productivity, and may alter soil carbon storage capacities. In this study we performed a 1-year litter-manipulation experiment to examine how soil CO2 efflux was altered by the amount of fresh litter. Three treatments were applied: litter exclusion (E), control (C, natural amount: 486 g m −2 ) and litter addition (A, twice the natural amount: 972 g m −2

010504 meteorology & atmospheric sciencesEcologyEcologySoil biologySoil Science04 agricultural and veterinary sciencesSoil carbon15. Life on landPlant litter01 natural sciencesAgricultural and Biological Sciences (miscellaneous)6. Clean water[ SDE ] Environmental SciencesSoil respirationAgronomy13. Climate actionSoil water[SDE]Environmental Sciences040103 agronomy & agricultureLitter0401 agriculture forestry and fisheriesEnvironmental scienceTerrestrial ecosystemEcosystem0105 earth and related environmental sciences
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Environmental change during the Early Cretaceous in the Purbeck-type Durlston Bay section (Dorset, Southern England): a biomarker approach.

2007

20 pages; International audience; The Purbeck-type section (Durlston Bay, Dorset, UK) exhibits littoral lagoonal to lacustrine facies. It shows a gradual climatic/environmental change from semi-arid conditions associated with evaporites at the Jurassic–Cretaceous transition, to a more humid climate at the end of the Berriasian. Though generally organic-poor (total organic carbon, TOC, <1.3%), the Durlston Bay section shows an organic-rich episode (TOC up to 8.5%) located at the transition from evaporitic to more humid facies. A biomarker study was performed in order to determine the origin of the organic matter (OM) in the section and see if changes in organic sources accompanied the genera…

010504 meteorology & atmospheric sciencesEnvironmental change[SDE.MCG]Environmental Sciences/Global ChangesBotryococcus010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciences[ SDE.MCG.CPE ] Environmental Sciences/Global Changes/domain_sde.mcg.cpeBottom waterSteranechemistry.chemical_compoundGeochemistry and Petrology[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry0105 earth and related environmental sciencesTotal organic carbonbiologyEcology15. Life on landbiology.organism_classification[SDE.MCG.CPE]Environmental Sciences/Global Changes/domain_sde.mcg.cpe[ SDU.STU.GC ] Sciences of the Universe [physics]/Earth Sciences/Geochemistry6. Clean waterCretaceousPalynofacies[ SDE.MCG ] Environmental Sciences/Global Changeschemistry13. Climate action[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyBayGeology
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Impact of basin burial and exhumation on Jurassic carbonates diagenesis on both sides of a thick clay barrier (Paris Basin, NE France).

2014

27 pages; International audience; Several diagenetic models have been proposed for Middle and Upper Jurassic carbonates of the eastern Paris Basin. The paragenetic sequences are compared in both aquifers to propose a diagenetic model for the Middle and Late Jurassic deposits as a whole. Petrographic (optical and cathodoluminescence microscopy), structural (fracture orientations) and geochemical (δ18O, δ13C, REE) studies were conducted to characterize diagenetic cements, with a focus on blocky calcite cements, and their connection with fracturation events. Four generations of blocky calcite (Cal1-Cal4) are identified. Cal1 and Cal2 are widespread in the dominantly grain-supported facies of t…

010504 meteorology & atmospheric sciencesEvaporiteCarbonateStratigraphyGeochemistryJurassic[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy010502 geochemistry & geophysicsOceanography01 natural sciencesDiagenesisPetrographyOxygen and carbon isotopesPaleontologychemistry.chemical_compoundParis Basin[ SDU.STU.MI ] Sciences of the Universe [physics]/Earth Sciences/MineralogyRare earth elements0105 earth and related environmental sciencesCalciteGeologyCementation (geology)6. Clean waterCretaceousDiagenesisGeophysicschemistry[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyFaciesEconomic GeologyPaleogeneGeology[SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
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A giant exoplanet orbiting a very-low-mass star challenges planet formation models

2019

Surveys have shown that super-Earth and Neptune-mass exoplanets are more frequent than gas giants around low-mass stars, as predicted by the core accretion theory of planet formation. We report the discovery of a giant planet around the very-low-mass star GJ 3512, as determined by optical and near-infrared radial-velocity observations. The planet has a minimum mass of 0.46 Jupiter masses, very high for such a small host star, and an eccentric 204-day orbit. Dynamical models show that the high eccentricity is most likely due to planet-planet interactions. We use simulations to demonstrate that the GJ 3512 planetary system challenges generally accepted formation theories, and that it puts con…

010504 meteorology & atmospheric sciencesGas giant530 PhysicsFOS: Physical sciencesMinimum massAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSettore FIS/05 - Astronomia e AstrofisicaPlanet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsMultidisciplinary520 AstronomyGiant planetAstronomyPlanetary system620 EngineeringAccretion (astrophysics)ExoplanetOrbitAstrophysics - Solar and Stellar Astrophysics13. Climate actionAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Earth and Planetary AstrophysicsScience
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Reactive transport modelling of carbonate cementation in a deep saline aquifer, the Middle Jurassic Oolithe Blanche Formation, Paris Basin, France.

2016

10 pages; International audience; The Oolithe Blanche Formation (Bathonian, Middle Jurassic) is one of the deep saline aquifers of the Paris Basin in France. The spatial distribution of its reservoir properties (porosity, permeability, tortuosity, etc.) is now better known with relatively homogeneous properties, except for some levels in the central part of the basin, where permeability exhibits higher values. This spatial distribution has been correlated with diagenetic events (variability of cementation) and palaeo-fluid flow circulation phases leading to variable cementation. In this paper, numerical simulations of reactive transport are performed. They provide a preliminary quantitative…

010504 meteorology & atmospheric sciencesGeochemistryPalaeo-circulationsCarbonatesEarth and Planetary Sciences(all)Structural basin010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesPermeabilityDiagenesischemistry.chemical_compoundNumerical simulationsGeomorphology0105 earth and related environmental sciencesGlobal and Planetary ChangeHydrogeologyGroundwater rechargeCementation (geology)6. Clean waterDiagenesisPermeability (earth sciences)chemistry[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyMeteoric waterGeneral Earth and Planetary SciencesCarbonatePorosityGeology
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Targeted delivery of hydrogen for the bioremediation of aquifers contaminated by dissolved chlorinated compounds.

2019

Dihydrogen (H2) gas injection is a promising option to enhance the reductive biodehalogenation of contaminants in groundwater. However, it is challenging to ensure its targeted delivery at the right places in plumes, and for the long times required for bioremediation. In this paper, the ability of surfactant foam to retain H2 in the saturated zone and to enhance its release in the dissolved form was compared to traditional biosparging. H2 gas was injected, either alone, or as foam, in a 2D saturated cell packed with glass beads. This cell was continuously flushed with deoxygenated water to mimic aquifer circulation, and H2 was studied both in terms of gas distribution in the cell and dissol…

010504 meteorology & atmospheric sciencesGroundwater flowHalogenationHealth Toxicology and MutagenesisGroundwater remediationAquifer010501 environmental sciencesToxicology01 natural sciencesDiffusionSurface-Active AgentsBioremediationDissolutionGroundwaterComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryChemistryWaterGeneral MedicinePollution6. Clean waterPlumeBiodegradation Environmental13. Climate actionReagentEnvironmental chemistry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]GroundwaterWater Pollutants ChemicalHydrogenEnvironmental pollution (Barking, Essex : 1987)
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2021

Abstract Contaminated soils are lands in Europe deemed less favourable for conventional agriculture. To overcome the problem of their poor fertility, bio-fertilization could be a promising approach. Soil inoculation with a choice of biological species (e.g. earthworm, mycorrhizal fungi, diazotroph bacteria) can be performed in order to improve soil properties and promote nutrients recycling. However, questions arise concerning the dynamics of the contaminants in an inoculated soil. The aim of this study was to highlight the soil-plant-earthworm interactions in the case of a slightly contaminated soil. For this purpose, a pot experiment in controlled conditions was carried out during 2 month…

010504 meteorology & atmospheric sciencesHealth Toxicology and MutagenesisBiomass010501 environmental sciencesToxicologycomplex mixtures01 natural sciencesNutrient0105 earth and related environmental sciences2. Zero hungerbiologyChemistryEarthwormTrace elementfood and beveragesGeneral Medicine15. Life on landbiology.organism_classificationPollutionSoil contamination6. Clean waterBioavailability13. Climate actionEnvironmental chemistryBioaccumulationSoil waterEnvironmental Pollution
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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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Applications of a new set of methane line parameters to the modeling of Titan's spectrum in the 1.58 μm window

2012

International audience; In this paper we apply a recently released set of methane line parameters (Wang et al., 2011) to the modeling of Titan spectra in the 1.58 mu m window at both low and high spectral resolution. We first compare the methane absorption based on this new set of methane data to that calculated from the methane absorption coefficients derived in situ from DISR/Huygens (Tomasko et al., 2008a; Karkoschka and Tomasko, 2010) and from the band models of Irwin et al. (2006) and Karkoschka and Tomasko (2010). The Irwin et al. (2006) band model clearly underestimates the absorption in the window at temperature-pressure conditions representative of Titan's troposphere, while the Ka…

010504 meteorology & atmospheric sciencesInfraredCASSINI VIMSHUYGENS PROBEMONODEUTERATED METHANEAtmospheric sciences01 natural sciences7. Clean energyMethaneSpectral lineTropospherechemistry.chemical_compoundsymbols.namesake0103 physical sciencesSpectral resolutionSpectroscopy010303 astronomy & astrophysicsCLOUD STRUCTURE0105 earth and related environmental sciencesPhysics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Astronomy and Astrophysics9500 CM(-1)SPECTROSCOPIC DATABASEM TRANSPARENCY WINDOWComputational physicsAerosolchemistry[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]TEMPERATURE-DEPENDENCE13. Climate actionSpace and Planetary SciencesymbolsSHIFT COEFFICIENTSOUTER SOLAR-SYSTEMTitan (rocket family)
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