Search results for "clean energy"

showing 10 items of 2594 documents

The making of the New European Wind Atlas - Part 1: Model sensitivity

2020

This is the first of two papers that document the creation of the New European Wind Atlas (NEWA). It describes the sensitivity analysis and evaluation procedures that formed the basis for choosing the final setup of the mesoscale model simulations of the wind atlas. The suitable combination of model setup and parameterizations, bound by practical constraints, was found for simulating the climatology of the wind field at turbine-relevant heights with the Weather Research and Forecasting (WRF) model. Initial WRF model sensitivity experiments compared the wind climate generated by using two commonly used planetary boundary layer schemes and were carried out over several regions in Europe. They…

010504 meteorology & atmospheric sciencesMeteorologyPlanetary boundary layer010505 oceanography020209 energylcsh:QE1-996.5Mesoscale meteorologyFísica atmosférica02 engineering and technology01 natural sciences7. Clean energyWind speedlcsh:GeologyBoundary layerRoughness length/dk/atira/pure/sustainabledevelopmentgoals/climate_action13. Climate actionWeather Research and Forecasting ModelWind resource assessmentWind atlasSDG 13 - Climate Action0202 electrical engineering electronic engineering information engineeringEnvironmental science0105 earth and related environmental sciences
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The high overtone and combination levels of SF6 revisited at Doppler-limited resolution: A global effective rovibrational model for highly excited vi…

2017

Abstract Sulfur hexafluoride is an important prototypal molecule for modeling highly excited vibrational energy flow and multi quanta absorption processes in hexafluoride molecules of technological importance. It is also a strong greenhouse gas of anthropogenic origin. This heavy species, however, features many hot bands at room temperature (at which only 30% of the molecules lie in the ground vibrational state), especially those originating from the lowest, v 6 =1 vibrational state. Using a cryogenic long path cell with variable optical path length and temperatures regulated between 120 and 163 K, coupled to Synchrotron Radiation and a high resolution interferometer, Doppler-limited spectr…

010504 meteorology & atmospheric sciencesOvertoneInfrared spectroscopylow temperature01 natural sciences7. Clean energyHot bandSpectral linechemistry.chemical_compoundHexafluorideFar infraredhot bandRotation-vibration spectroscopy of SF 60103 physical sciencesSpectroscopy0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Radiation[ PHYS ] Physics [physics]010304 chemical physicsRotational–vibrational spectroscopyAtomic and Molecular Physics and Opticschemistry13. Climate actiongreenhouse gasExcited stateinfrared absorptionAtomic physicstensorial formalismLong path cell
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Photoreduction of gaseous oxidized mercury changes global atmospheric mercury speciation, transport and deposition

2018

9 pags, 8 figs. -- Correction autor: https://doi.org/10.1038/s41467-022-28455-w http://hdl.handle.net/10261/268181

010504 meteorology & atmospheric sciencesScienceGeneral Physics and Astronomychemistry.chemical_elementAtmospheric mercury010501 environmental sciences01 natural sciences7. Clean energyArticleGeneral Biochemistry Genetics and Molecular Biology14. Life underwaterlcsh:Science0105 earth and related environmental sciencesMultidisciplinaryChemistryAquatic ecosystemQPhotodissociationGeneral ChemistryMercury (element)Earth surface[SDU]Sciences of the Universe [physics]13. Climate actionEnvironmental chemistrySoil waterlcsh:Q
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A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation

2011

The dwarf planet Eris is a trans-Neptunian object with an orbital eccentricity of 0.44, an inclination of 44 degrees and a surface composition very similar to that of Pluto. It resides at present at 95.7 astronomical units (1ĝ€‰au is the Earth-Sun distance) from Earth, near its aphelion and more than three times farther than Pluto. Owing to this great distance, measuring its size or detecting a putative atmosphere is difficult. Here we report the observation of a multi-chord stellar occultation by Eris on 6 November 2010 ut. The event is consistent with a spherical shape for Eris, with radius 1,163±6 kilometres, density 2.52±0.05 grams per cm 3 and a high visible geometric albedo,. No nitro…

010504 meteorology & atmospheric sciences[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]Ciencias FísicasAstronomical unitDwarf planet[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]Orbital eccentricityAstrophysicsno utilizado01 natural sciences7. Clean energyOccultationdwarf planetAtmosphere0103 physical sciencesTrans-Neptunian object010303 astronomy & astrophysicsEris0105 earth and related environmental sciencesPhysicsMultidisciplinarybiologyPlutoAstronomybiology.organism_classificationPlutoAstronomíaEris13. Climate actionCIENCIAS NATURALES Y EXACTASalbedo
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Models and data analysis tools for the Solar Orbiter mission

2020

All authors: Rouillard, A. P.; Pinto, R. F.; Vourlidas, A.; De Groof, A.; Thompson, W. T.; Bemporad, A.; Dolei, S.; Indurain, M.; Buchlin, E.; Sasso, C.; Spadaro, D.; Dalmasse, K.; Hirzberger, J.; Zouganelis, I.; Strugarek, A.; Brun, A. S.; Alexandre, M.; Berghmans, D.; Raouafi, N. E.; Wiegelmann, T.; Pagano, P.; Arge, C. N.; Nieves-Chinchilla, T.; Lavarra, M.; Poirier, N.; Amari, T.; Aran, A.; Andretta, V.; Antonucci, E.; Anastasiadis, A.; Auchère, F.; Bellot Rubio, L.; Nicula, B.; Bonnin, X.; Bouchemit, M.; Budnik, E.; Caminade, S.; Cecconi, B.; Carlyle, J.; Cernuda, I.; Davila, J. M.; Etesi, L.; Espinosa Lara, F.; Fedorov, A.; Fineschi, S.; Fludra, A.; Génot, V.; Georgoulis, M. K.; Gilbe…

010504 meteorology & atmospheric sciencescorona [Sun]Solar windAstrophysics[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]7. Clean energy01 natural scienceslaw.inventionData acquisitionlawCoronal mass ejectiongeneral [Sun]QB AstronomyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSun: magnetic fieldsQCComputingMilieux_MISCELLANEOUSQBPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]3rd-DASenergetic particlesSolar windCORONAL MASS EJECTIONSnumerical modelingmagnetic fields [Sun]solar windPhysics::Space PhysicsSystems engineeringAstrophysics::Earth and Planetary Astrophysicsatmosphere [Sun]fundamental parameters [Sun]Sun: generalFORCE-FREE FIELDSun: fundamental parametersSolar radiusContext (language use)STREAMER STRUCTUREOrbiter0103 physical sciencesOPTIMIZATION APPROACH[SDU.ASTR.SR] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]POLARIZATION MEASUREMENTSSun: Solar wind3-DIMENSIONAL STRUCTURE0105 earth and related environmental sciencesSpacecraftbusiness.industrySun: corona[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]solar coronaMAGNETIC-FLUX ROPESAstronomy and AstrophysicsSHOCKS DRIVEN115 Astronomy Space scienceSPECTRAL-LINESQC Physics13. Climate actionSpace and Planetary SciencebusinessHeliosphereSun: atmosphereELECTRON-DENSITY
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First M87 Event Horizon Telescope Results. I. the Shadow of the Supermassive Black Hole

2019

When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon. To image and study this phenomenon, we have assembled the Event Horizon Telescope, a global very long baseline interferometry array observing at a wavelength of 1.3 mm. This allows us to reconstruct event-horizon-scale images of the supermassive black hole candidate in the center of the giant elliptical galaxy M87. We have resolved the central compact radio source as an asymmetric bright emission ring with a diameter of 42 ± 3 μas, which is circular and encompasses a central depression in brightness with a flux rati…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonAstronomyblack hole physicsjets [galaxies]galaxies: individualAstrophysicshigh-resolution7. Clean energy01 natural sciencesPhoton sphereGeneral Relativity and Quantum Cosmologyaccretionsagittarius-a-asterisk010303 astronomy & astrophysicsgalactic-centerHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsradio-sourcesaccretion disksGalactic Centergrmhd simulations3. Good healthenergy-distributionsactive [galaxies]AnatomyAstrophysics - High Energy Astrophysical PhenomenaActive galactic nucleusAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgalaxies: individual: M87galaxies: individual (M87)Cell and Developmental BiologyGeneral Relativity and Quantum Cosmology0103 physical sciences(M87)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeghz vlbi observationsfaraday-rotationAstronomy and Astrophysicsgalaxies: jetsAstrophysics - Astrophysics of GalaxiesBlack holeRotating black holeSpace and Planetary SciencegravitationAstrophysics of Galaxies (astro-ph.GA)advection-dominated accretion[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]ionized-gas
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First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole

2019

We present measurements of the properties of the central radio source in M87 using Event Horizon Telescope data obtained during the 2017 campaign. We develop and fit geometric crescent models (asymmetric rings with interior brightness depressions) using two independent sampling algorithms that consider distinct representations of the visibility data. We show that the crescent family of models is statistically preferred over other comparably complex geometric models that we explore. We calibrate the geometric model parameters using general relativistic magnetohydrodynamic (GRMHD) models of the emission region and estimate physical properties of the source. We further fit images generated fro…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonGeneral relativityAstronomyAstrophysics::High Energy Astrophysical Phenomenablack hole physicsFOS: Physical sciencesgalaxies: individualAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)GravitationGeneral Relativity and Quantum Cosmology0103 physical sciences(M87)010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsEvent Horizon TelescopeHigh Energy Astrophysical Phenomena (astro-ph.HE)high angular resolution [techniques]techniques: high angular resolutionAstronomy and Astrophysicsblack hole physicAstrophysics - Astrophysics of GalaxiesGalaxyinterferometric [techniques]Black holeRotating black holeSpace and Planetary Sciencegravitationtechniques: interferometricAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaSchwarzschild radius
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High-resolution spectroscopy and analysis of the V2 + V3 combination band of SF6 in a supersonic jet expansion

2013

International audience; Sulphur hexafluoride is a very strong greenhouse gas whose concentration is increasing in the atmosphere. It is detected through infrared absorption spectroscopy in the strong ν3 fundamental region. Due to the existence of low-lying vibrational states of this molecule, however, many hot bands arise at room temperature and those are still not known. We present here a contribution to the elucidation of this hot band structure, by analysing the ν2 + ν3 combination band. We use a supersonic jet expansion high-resolution spectrum at a rotational temperature of ca. 25 K that was recorded thanks to the Jet-AILES setup at the Source Optimisée de Lumière d'Energie Intermédiai…

010504 meteorology & atmospheric sciencessupersonic jet expansionBiophysicsInfrared spectroscopy7. Clean energy01 natural sciencesHot bandlaw.inventionsymbols.namesake[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]law0103 physical sciencesSupersonic speedPhysical and Theoretical ChemistrySpectroscopy[ PHYS.PHYS.PHYS-ATM-PH ] Physics [physics]/Physics [physics]/Atomic and Molecular Clusters [physics.atm-clus]Molecular BiologyComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciences[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]010304 chemical physicssulphur hexafluorideChemistry[PHYS.PHYS.PHYS-ATM-PH]Physics [physics]/Physics [physics]/Atomic and Molecular Clusters [physics.atm-clus]Rotational temperatureRotational–vibrational spectroscopyCondensed Matter PhysicsSynchrotron[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]13. Climate actiongreenhouse gassymbolsinfrared absorption[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physicsHamiltonian (quantum mechanics)tensorial formalism
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Bioconversion of amino acids into flavouring alcohols and esters by Erwinia carotovora subsp. atroseptica

1991

International audience; Erwinia carotovora subsp. atroseptica produced flavour compounds when infecting endives (Cichorium intybus). These compounds were identified as esters and branched-chain alcohols.They were produced from amino acids and some of them such as methionol, methionol acetate, isobutanol, isobutyl acetate, beta-phenyl ethanol and tryptophol were produced with good yields.

0106 biological sciencesBioconversionErwinia01 natural sciences7. Clean energyApplied Microbiology and Biotechnology03 medical and health scienceschemistry.chemical_compoundBiotransformation010608 biotechnologyCichoriumTryptopholOrganic chemistry[SDV.MP] Life Sciences [q-bio]/Microbiology and Parasitology030304 developmental biologychemistry.chemical_classification0303 health sciencesIsobutyl acetatebiologyIsobutanolfood and beveragesGeneral Medicinebiology.organism_classification3. Good healthAmino acid[SDV.MP]Life Sciences [q-bio]/Microbiology and ParasitologychemistryBiotechnology
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Towards food, feed and energy crops mitigating climate change

2011

Agriculture is an important source of anthropogenic emissions of the greenhouse gases (GHG), methane (CH 4 ) and nitrous oxide (N 2 O), and crops can affect the microbial processes controlling these emissions in many ways. Here, we summarize the current knowledge of plant–microbe interactions in relation to the CH 4 and N 2 O budgets and show how this is promoting new generations of crop cultivars that have the potential to mitigate GHG emissions for future agricultural use. The possibility of breeding low GHG-emitting cultivars is a paradigm shift towards sustainable agriculture that balances climate change and food and bioenergy security.

0106 biological sciencesCrops AgriculturalConservation of Natural ResourcesClimate ChangePlant ExudatesNitrous OxideClimate changePlant ScienceBiology7. Clean energy01 natural scienceskyoto protocolnitrogenCarbon CycleSoilBioenergyemission in agricultureSustainable agriculture[SDV.BV]Life Sciences [q-bio]/Vegetal BiologySoil Microbiology2. Zero hungerFood securityBacteriabusiness.industryAgroforestrymicrobial processmethanen2o04 agricultural and veterinary sciences15. Life on landNitrogen Cycleghg emissionEnergy crop13. Climate actionAgriculturegreenhouse gasGreenhouse gasWetlandsSustainabilityRhizosphere040103 agronomy & agriculture0401 agriculture forestry and fisheriesbusiness010606 plant biology & botany
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