Search results for "Mission"

showing 10 items of 5334 documents

The WISE 2000 and 2001 Field Experiments in Support of the SMOS Mission:Sea Surface L-Band Brightness Temperature Observations and Their Application …

2004

Camps, Adriano ... et al.-- 20 pages, 16 figures, 3 tables

010504 meteorology & atmospheric sciences0211 other engineering and technologiesWind02 engineering and technologySea stateAtmospheric sciences01 natural sciencesOceanographic techniquesWind waveSurface roughnessEmissivitySeawater14. Life underwaterElectrical and Electronic EngineeringRadiometry[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environment021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingPhysics[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereRadiometerFoamsOcean wavesRemote sensingSea surface temperature13. Climate actionBrightness temperatureGeneral Earth and Planetary SciencesSMOS MissionSignificant wave height
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The global forest above-ground biomass pool for 2010 estimated from high-resolution satellite observations

2021

Funding Information: We are thankful to the GlobBiomass project team and Frank Martin Seifert (ESA) for valuable suggestions and stimulating scientific discussions. We are thankful to Takeo Tadono (JAXA EORC), Masato Hayashi, (JAXA EORC), Kazufumi Kobayashi (RESTEC), Åke Rosenqvist (soloEO), and Josef Kellndorfer (EBD) for support with the use and interpretation of the ALOS PALSAR mosaics. Support by the CCI Land Cover project team, in particular Sophie Bontemps (UCL), is greatly acknowledged. The help from Martin Jung (MPI-BGC) in feature selection and Ulrich Weber (MPI-BGC) for data processing for the GSV-to-AGB conversions is greatly acknowledged. Forest inventory data for the validation…

010504 meteorology & atmospheric sciencesALOS PALSAR0211 other engineering and technologies02 engineering and technology01 natural sciencesLaboratory of Geo-information Science and Remote SensingSDG 13 - Climate ActionGE1-350BiomassEMISSIONSSDG 15 - Life on LandQE1-996.5GROWING STOCK VOLUMETaigaGeologyPE&RCPlant Production SystemsMAPbiomaCARBON-CYCLECrop and Weed EcologySynthetic aperture radarPhysical geographyRETRIEVALUNITED-STATESEarth and Planetary Sciences(all)Synthetic aperture radarSubtropicsSpatial distributionEnvironmental scienceCarbon cycletropicsTemperate climateBOREAL FORESTSMANAGEMENTLife ScienceSpatial ecologySpatial distributionLaboratorium voor Geo-informatiekunde en Remote Sensing021101 geological & geomatics engineering0105 earth and related environmental sciencesForest inventoryRadarTemperate climateEnvironmental sciencesSatelliteEarth and Environmental SciencesDENSITYPlantaardige ProductiesystemenSpatial ecologyEnvironmental scienceGeneral Earth and Planetary SciencescavelabPhysical geographyForest inventory
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Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

2021

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsEP/ T017325/101 natural sciencesrotationGeneral Relativity and Quantum CosmologyPSR J0537−6910neutron starsLuminosityGravitatational Waves PSR J0537−6910 LIGO VirgoHISTORYLIGOSupernova remnantneutron star010303 astronomy & astrophysicsgravitational waveQCQBpulsarPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/03N157BPhysics/dk/atira/pure/sustainabledevelopmentgoals/partnershipsGravitational waves neutron stars pulsarEPSRCPhysical Sciencesmoment: multipole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodPSR J0537-6910Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsEphemeris1ST SEARCHGravitational wavesX-raySDG 17 - Partnerships for the GoalsPulsar0103 physical sciences/dk/atira/pure/subjectarea/asjc/1900/1912X-ray: emissiongravitational waves; pulsars; PSR J0537-6910; neutron starsSTFCAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyNeutron Star Interior Composition ExplorerR-MODEGravitational waveVirgopulsar: rotationRCUKAstronomy and AstrophysicsLIGONeutron starVIRGOSUPERNOVA REMNANTSpace and Planetary Sciencegravitational radiation: emissionpulsars/dk/atira/pure/subjectarea/asjc/3100/3103Gravitatational Waves[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Gravitational-wave Detection and Parameter Estimation for Accreting Black-hole Binaries and Their Electromagnetic Counterpart

2020

We study the impact of gas accretion on the orbital evolution of black-hole binaries initially at large separation in the band of the planned Laser Interferometer Space Antenna (LISA). We focus on two sources: (i)~stellar-origin black-hole binaries~(SOBHBs) that can migrate from the LISA band to the band of ground-based gravitational-wave observatories within weeks/months; and (ii) intermediate-mass black-hole binaries~(IMBHBs) in the LISA band only. Because of the large number of observable gravitational-wave cycles, the phase evolution of these systems needs to be modeled to great accuracy to avoid biasing the estimation of the source parameters. Accretion affects the gravitational-wave p…

010504 meteorology & atmospheric sciencesAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)Observableastro-ph.HE; astro-ph.HE; General Relativity and Quantum Cosmologygas: accretionblack holes gravitational wavesobservatoryInterferometrygravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenainterferometermedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgravitational radiation: direct detectionelectromagnetic field: productionGeneral Relativity and Quantum Cosmologybinary: coalescencestatistical analysisSettore FIS/05 - Astronomia e Astrofisicagravitation: weak field0103 physical sciencesnumerical calculationsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLISAGravitational wavegravitational radiationOrder (ring theory)black hole: accretionAstronomy and Astrophysicsblack holesgravitational radiation detectorRedshiftBlack holeblack hole: binarySpace and Planetary ScienceSkygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-ray: detectorThe Astrophysical Journal
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IGR J17329-2731: The birth of a symbiotic X-ray binary

2018

We report on the results of the multiwavelength campaign carried out after the discovery of the INTEGRAL transient IGR J17329-2731. The optical data collected with the SOAR telescope allowed us to identify the donor star in this system as a late M giant at a distance of 2.7$^{+3.4}_{-1.2}$ kpc. The data collected quasi-simultaneously with XMM-Newton and NuSTAR showed the presence of a modulation with a period of 6680$\pm$3 s in the X-ray light curves of the source. This unveils that the compact object hosted in this system is a slowly rotating neutron star. The broadband X-ray spectrum showed the presence of a strong absorption ($\gg$10$^{23}$ cm$^{-2}$) and prominent emission lines at 6.4 …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesFluxAstrophysicsCompact star01 natural sciencesSpectral linelaw.inventionTelescopeSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsAstronomy and AstrophysicLight curveX-rays: binarieNeutron starX-rays: individuals: IGR J17329-273113. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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Study of a sample of faint Be stars in the exofield of CoRoT

2013

International audience; Context. Be stars are probably the most rapid rotators among stars in the main sequence (MS) and, as such, are excellent candidates to study the incidence of the rotation on the characteristics of their non-radial pulsations, as well as on their internal structure. Pulsations are also thought to be possible mechanisms that help the mass ejection needed to build up the circumstellar disks of Be stars.Aims. The purpose of this paper is to identify a number of faint Be stars observed with the CoRoT satellite and to determine their fundamental parameters, which will enable us to study their pulsation properties as a function of the location in the HR diagram and to searc…

010504 meteorology & atmospheric sciencesBe starHertzsprung–Russell diagramK-type main-sequence starstars: emission-lineAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineBlue stragglersymbols.namesakestars: rotation0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AstronomyBeAstronomy and Astrophysicsstars: early-typeHerbig Ae/Be starT Tauri starStars[SDU]Sciences of the Universe [physics]Space and Planetary Sciencesymbolsstars: fundamental parametersstars: oscillationsAstrophysics::Earth and Planetary Astrophysicsbinaries: spectroscopicAstronomy & Astrophysics
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Developing an indicator-modelling approach to forecast changes in nitrogen critical load exceedance across Europe arising from agricultural reform

2011

International audience; Atmospheric nitrogen (N) deposition above the critical load causes eutrophication with adverse impacts on biodiversity. Average Accumulated critical load Exceedance (AAE) is a measure of the amount of critical load exceedance and the area of habitat which is affected, and has been adopted in Europe as a pressure indicator for biodiversity. In Europe, AAE is calculated by the Coordination Centre for Effects (CCE) of the United Nations Economic Commission for Europe based on modelled nitrogen deposition and country-level reporting of critical load thresholds and ecosystem area. Due to differences in country-level reporting, AAE values for semi-natural habitats may show…

010504 meteorology & atmospheric sciencesBiodiversityGeneral Decision Sciences010501 environmental sciences01 natural sciencesAMMONIA EMISSIONEnvironmental protectionEcosystemEcology Evolution Behavior and Systematics0105 earth and related environmental sciences2. Zero hungerCritical loadNITROGEN DEPOSITIONEcologyEMISSION D'AMONIAQUEbusiness.industry15. Life on landDeposition (aerosol physics)Habitat13. Climate actionAgricultureEUTROPHICATIONSpatial ecologyEnvironmental scienceBIODIVERSITYCAP REFORM[SDE.BE]Environmental Sciences/Biodiversity and EcologyEutrophicationbusiness
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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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Hydrothermal pressure-temperature control on CO2 emissions and seismicity at Campi Flegrei (Italy)

2021

Fluids supplied by stored magma at depth are causal factors of volcanic unrest, as they can cause pressurization/heating of hydrothermal systems. However, evidence for links between hydrothermal pressurization, CO2 emission and volcano seismicity have remained elusive. Here, we use recent (2010−2020) observations at Campi Flegrei caldera (CFc) to show hydrothermal pressure, gas emission and seismicity at CFc share common source areas and well-matching temporal evolutions. We interpret the recent escalation in seismicity and surface gas emissions as caused by pressure-temperature increase at the top of a vertically elongated (0.3–2 km deep) gas front. Using mass (steam) balance consideration…

010504 meteorology & atmospheric sciencesCampi Flegrei mantle geochemistry CO2 emission Fumarole compositions Hydrothermal systems Volcanic unrest Volcano seismicityInduced seismicity010502 geochemistry & geophysics01 natural sciencesHydrothermal circulationHydrothermal systemsCabin pressurizationGeochemistry and PetrologyCalderaPetrologyFumarole compositions0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryVolcanic unrest; Hydrothermal systems; Campi Flegrei; Fumarole compositions; CO2 emission; Volcano seismicityFront (oceanography)Volcano seismicityGeophysicsVolcanoVolume (thermodynamics)Volcanic unrestCO2 emissionMagmaCampi FlegreiGeology
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Relations between Air Quality and Covid-19 Lockdown Measures in Valencia, Spain

2021

The set of measures to contain the diffusion of COVID-19 instituted by the European governments gave an unparalleled opportunity to improve our understanding of the transport and industrial sectors’ contribution to urban air pollution. The purpose of this study was to assess the impacts of the lockdown measures on air quality and pollutant emissions in Valencia, Spain. For this reason, we determined if there was a significant difference in the concentration levels of different particulate matter (PM) sizes, PM10, PM2.5, and NOx, NO2, NO, and O3, between the period of restrictions in 2020 and the same period in 2019. Our findings indicated that PM pollutant levels during the lockdown period…

010504 meteorology & atmospheric sciencesCoronavirus disease 2019 (COVID-19)Pollutant emissionsHealth Toxicology and Mutagenesisair pollutionAir pollutionlcsh:Medicine010501 environmental sciencesmedicine.disease_cause01 natural sciencesArticleToxicologylockdownmedicineHumansValenciaAir quality index0105 earth and related environmental sciencesPollutantbiologyparticulate matter (pm)Significant differencelcsh:RPublic Health Environmental and Occupational HealthParticulatesbiology.organism_classificationnitrogen oxidesozoneSpainCommunicable Disease ControlEnvironmental scienceParticulate MatterCovid-19Environmental MonitoringInternational Journal of Environmental Research and Public Health
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