Search results for "Climate Action"

showing 10 items of 2410 documents

Towards a framework for assessment and management of cumulative human impacts on marine food webs

2015

Effective ecosystem-based management requires understanding ecosystem responses to multiple human threats, rather than focusing on single threats. To understand ecosystem responses to anthropogenic threats holistically, it is necessary to know how threats affect different components within ecosystems and ultimately alter ecosystem functioning. We used a case study of a Mediterranean seagrass (Posidonia oceanica) food web and expert knowledge elicitation in an application of the initial steps of a framework for assessment of cumulative human impacts on food webs. We produced a conceptual seagrass food web model, determined the main trophic relationships, identified the main threats to the fo…

seagrassBiodiversity & Conservationvulnerability05 Environmental SciencesVulnerabilityTHREATSExpert knowledge elicitationFood chainecosystem-based managementconservation actions ecosystem-based management expert knowledge elicitation multiple threats seagrass vulnerabilityECOSYSTEM-BASED MANAGEMENTWater Pollution ChemicalZoologíaComputingMilieux_MISCELLANEOUSTrophic levelelicitationAlismatalesAcciones de conservaciónbiologyEcologymultiple threatsSeagraEnvironmental resource managementconservation actionsobtencion de conocimiento de expertosEcosystem-based managementFood webacciones de conservaciónSeagrassobtención de conocimiento de expertosBiodiversity ConservationConservation actionAlismatidaeKnow-howLife Sciences & Biomedicineacciones de conservacionAmenazas múltiplesMultiple threatSettore BIO/07 - EcologiaConservation of Natural ResourcesFood ChainFisheriesEnvironmental Sciences & EcologyManejo con base en los ecosistemasamenazas múltiplesPastos marinosexpert knowledgeOCEANexpert knowledge elicitationMediterranean SeaHumansEcosystemObtención de conocimiento de expertos14. Life underwaterEcology Evolution Behavior and SystematicsNature and Landscape ConservationScience & Technologybusiness.industrymanejo con base en los ecosistemasvulnerabilidadpastos marinos15. Life on land06 Biological Sciencesbiology.organism_classification13. Climate actionamenazas multiples07 Agricultural And Veterinary Sciences[SDE.BE]Environmental Sciences/Biodiversity and EcologybusinessVulnerabilidadEnvironmental Sciences
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Fate of organic pollutants after sewage sludge spreading on agricultural soils: a 30-years field-scale recording

2006

Le DOI mentionné dans l'article 10.2166/WPT.2007.008 ne fonctionne pas; International audience; Toxic organic compounds, such as the surfactants linear alkylbenzene sulfonates (LAS) and nonylphenol polyethoxylates (NPE), Polycyclic aromatic hydrocarbons (PAH) and residues derived from plastics (PAE-phthalates) end up in sewage sludge. In order to evaluate and quantify the potential environmental risks associated with the xenobiotic introduction into biological life cycle, the EU BIOWASTE project (QLK5-CT-2002-01138) devotes one task to the study of the fate of xenobiotic in a sandy soil after sludge spreading on a 30-year field-scale record experiment. Experimental maize crop fields from Bo…

sludge disposalLinear alkylbenzene[SDE.MCG]Environmental Sciences/Global Changesxenobiotic010501 environmental sciences[SDV.SA.SDS]Life Sciences [q-bio]/Agricultural sciences/Soil study01 natural sciencesbiodegradationchemistry.chemical_compoundDry weight[SDU.STU.HY]Sciences of the Universe [physics]/Earth Sciences/Hydrology0105 earth and related environmental sciencesWater Science and Technology2. Zero hungerPollutantphthalates04 agricultural and veterinary sciencesPAHBiodegradationCOMPOSE TOXIQUE ORGANIQUE6. Clean waterNonylphenolLASchemistry13. Climate actionlong term effectEnvironmental chemistrySoil water[SDU.STU.HY] Sciences of the Universe [physics]/Earth Sciences/Hydrology040103 agronomy & agriculture0401 agriculture forestry and fisheriesEnvironmental scienceXenobioticSludgeNPEbound residues
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On-Orbit Degradation of Solar Instruments

2013

International audience; We present the lessons learned about the degradation observed in several space solar missions, based on contributions at the Workshop about On-Orbit Degradation of Solar and Space Weather Instruments that took place at the Solar Terrestrial Centre of Excellence (Royal Observatory of Belgium) in Brussels on 3 May 2012. The aim of this workshop was to open discussions related to the degradation observed in Sun-observing instruments exposed to the effects of the space environment. This article summarizes the various lessons learned and offers recommendations to reduce or correct expected degradation with the goal of increasing the useful lifespan of future and ongoing s…

solar instruments[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010504 meteorology & atmospheric sciencesFOS: Physical sciencesSolar missionSpace weatherSpace (commercial competition)7. Clean energy01 natural sciencesSpace explorationDegradationContaminationObservatory0103 physical sciencesAerospace engineeringInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesbusiness.industryAstronomy and Astrophysicscon- taminationcalibrationspace environment[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceOrbit (dynamics)Environmental scienceAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSpace environmentDegradation (telecommunications)SOLAR PHYSICS
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Total absorption γ -ray spectroscopy of niobium isomers

2019

15 pags. 17 figs., 5 tabs.

spektroskopiaNiobiumchemistry.chemical_element[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Structure7. Clean energy01 natural sciences0103 physical sciencesDecay heat010306 general physicsSpectroscopyAbsorption (electromagnetic radiation)Nuclear ExperimentPhysicsZirconiumSpectrometer010308 nuclear & particles physicsPandemonium effectPenning trapnuclear structure and decayschemistry13. Climate actionFísica nuclearbeta decayAtomic physicsisomer decaysydinfysiikka
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Urban Heat Island Monitoring and Impacts on Citizen's General Health Status in Isfahan Metropolis: A Remote Sensing and Field Survey Approach.

2020

Urban heat islands (UHIs) are one of the urban management challenges, especially in metropolises, which can affect citizens’ health and well-being. This study used a combination of remote sensing techniques with field survey to investigate systematically the effects of UHI on citizens’ health in Isfahan metropolis, Iran. For this purpose, the land surface temperature (LST) over a three-year period was monitored by Landsat-8 satellite imagery based on the split window algorithm. Then, the areas where UHI and urban cold island (UCI) phenomena occurred were identified and a general health questionnaire-28 (GHQ-28) was applied to evaluate the health status of 800 citizens in terms o…

split window algorithm010504 meteorology & atmospheric sciencesLand surface temperatureScienceQgeneral health questionnaire-28land surface temperatureurban heat island010501 environmental sciencesField survey01 natural sciencesGeography13. Climate actionRemote sensing (archaeology)Social function11. SustainabilityGeneral Earth and Planetary Sciencesurban heat island; land surface temperature; split window algorithm; general health questionnaire-28; Isfahan metropolisGeneral healthUrban heat islandIsfahan metropolisUrban management0105 earth and related environmental sciencesSocial functioningRemote sensingRemote sensing
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The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

2007

(abridged:) The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus star formation region, using the XMM-Newton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association. Many targets are also studied in the optical, and high-resolution X-ray grating spectroscopy has been obtained for selected bright sources. The X-ray spectra have been coherently analyzed with two different thermal models (2-component thermal model, and a continuous emission measure distribution model). We present ov…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaBrown dwarfFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Observatory0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsstars : formationStar formationMolecular cloudAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion (astrophysics)Starsgravitational waves13. Climate actionSpace and Planetary ScienceX-rays : star
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Spectral properties of X-ray bright variable sources in the Taurus Molecular Cloud

2006

We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), in order to characterize the variations with time of their coronal properties and to derive informations on the X-ray emitting structures. We performed time-resolved spectroscopy of the EPIC PN and MOS spectra of the XEST sources, using a model with one or two thermal components, and we used the time evolution of the temperatures and emission measures during the decay phase of flares to derive the size of the flaring loops. The light curves of the selected sources show different types of variability: flares, long-lasting decay or rise through the whole observation, sl…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-rays : starsFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciences7. Clean energySpectral linelaw.inventionlaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectroscopy010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsMolecular cloudAstrophysics (astro-ph)Astronomy and Astrophysicsstars : late-typeRadiusPlasmaLight curve13. Climate actionSpace and Planetary Sciencestars : coronaeFlare
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Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452

2012

International audience; Context. Be stars are rapidly rotating stars with a circumstellar decretion disk. They usually undergo pressure and/or gravity pulsation modes excited by the κ-mechanism, i.e. an effect of the opacity of iron-peak elements in the envelope of the star. In the Milky Way, p-modes are observed in stars that are hotter than or equal to the B3 spectral type, while g-modes are observed at the B2 spectral type and cooler. Aims. We observed a B0IVe star, HD 51452, with the high-precision, high-cadence photometric CoRoT satellite and high-resolution, ground-based HARPS and SOPHIE spectrographs to study its pulsations in great detail. We also used the lower resolution spectra a…

starsBe -stars010504 meteorology & atmospheric sciencesBe starK-type main-sequence staroscillations -starsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsrotation01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsStellar structureindividual010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences[PHYS]Physics [physics]PhysicsASTROFÍSICA ESTELARStellar rotationFlare starAstronomyAstronomy and AstrophysicsLight curveESPECTROSCOPIAHD 51452 -starsStarsT Tauri star13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsemission-line[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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Chemical Cartography with APOGEE: Multi-element Abundance Ratios

2019

We map the trends of elemental abundance ratios across the Galactic disk, spanning R = 3-15 kpc and midplane distance |Z|= 0-2 kpc, for 15 elements in a sample of 20,485 stars measured by the SDSS/APOGEE survey (O, Na, Mg, Al, Si, P, S, K, Ca, V, Cr, Mn, Fe, Co, Ni). Adopting Mg rather than Fe as our reference element, and separating stars into two populations based on [Fe/Mg], we find that the median trends of [X/Mg] vs. [Mg/H] in each population are nearly independent of location in the Galaxy. The full multi-element cartography can be summarized by combining these nearly universal median sequences with our measured metallicity distribution functions and the relative proportions of the lo…

stars: abundances010504 meteorology & atmospheric sciencesMilky WayMetallicityPopulationFOS: Physical sciences01 natural sciencesGalaxy: diskStellar nucleosynthesisNucleosynthesis0103 physical scienceseducation010303 astronomy & astrophysicsnuclear reactions0105 earth and related environmental sciencesPhysicseducation.field_of_studyabundancesnucleosynthesisAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxySupernova13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesSupernova nucleosynthesis[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]CartographyThe Astrophysical Journal
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The Gaia-ESO Survey: impact of extra mixing on C and N abundances of giant stars

2018

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical elements C and N at their surface. The surface abundances of these chemical species are well-known to change in stars during their evolution on the red giant branch after the first dredge-up episod, as a result of extra-mixing phenomena. We investigate the effects of thermohaline mixing on C and N abundances using the first comparison between the GES [C/N] determinations with simulations of the observed fields using a model of stellar population synthesis. We explore the effects of thermohaline mixing on the chemic…

stars: abundances010504 meteorology & atmospheric sciencesStellar populationMetallicityFOS: Physical sciencesabundances ; stars: evolution ; galaxy: stellar content ; galaxy: abundances ; astrophysics - solar and stellar astrophysics [stars]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomi astrofysik och kosmologi0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsstellar content [Galaxy]Astronomy Astrophysics and Cosmologystars: evolution14. Life underwater010303 astronomy & astrophysicsStellar evolutionSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsGalaxy: stellar contentabundances [Galaxy]Astronomy and AstrophysicsGiant starRed-giant branchabundances [stars]StarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceGlobular clusterevolution [stars]Galaxy: abundancesAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Open cluster
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