Search results for "clean energy"

showing 10 items of 2594 documents

Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign

2021

Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; …

Accretion010504 meteorology & atmospheric sciencesAstronomyFluxAstrophysics7. Clean energy01 natural sciencesActive galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; Accretion; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HERadio coreAccretion (meteorology)PhysicsAstrophysical black holes520 Astronomie und zugeordnete WissenschaftenActive galactic nuclei ; Radio cores ; Low-luminosity ; active galactic nuclei ; High energy astrophysics ; Astrophysical black holes ; AccretionAstrophysical black holeLow-luminosity active galactic nucleiastro-ph.COAstrophysics - High Energy Astrophysical PhenomenaAccretion; Active galactic nuclei; Astrophysical black holes; High energy astrophysics; Low-luminosity active galactic nuclei; Radio coresHigh energy astrophysicsRadio coresAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusHigh-energy astronomyastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesF500Astrophysics::Cosmology and Extragalactic AstrophysicsHigh energy astrophysic0103 physical sciencesVery-long-baseline interferometryddc:530Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeActive galactic nucleiAstronomy and Astrophysics530 PhysikAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ddc:520Active galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; AccretionHESS - Abteilung Hinton[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon

2021

Full list of authors: Akiyama, Kazunori; Algaba, Juan Carlos; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barrett, John; Benson, Bradford A.; Bintley, Dan; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chan, Chi-kwan; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Chesler, Paul M.; Cho, Ilje; Christian, Pierre; Conway, John E.…

AccretionKinoAstrophysics - astrophysics of galaxiesAstrophysics::High Energy Astrophysical PhenomenaAstronomy19641347FOS: Physical sciences479Astrophysics::Cosmology and Extragalactic AstrophysicsF500870126101 natural sciences7. Clean energyAstrophysics - high energy astrophysical phenomena994MagnetohydrodynamicsRelativistic jets 14 162 479 870 886 994 1964 1261 1278 1335 1347 13900103 physical sciencesJetsPolarimetryRadiative transferPlasma astrophysicsRadio jets010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics162High Energy Astrophysical Phenomena (astro-ph.HE)Physics1278Event horizons1335010308 nuclear & particles physicsBlack holesChatterjee14886Astronomy and AstrophysicsCreative commons139013. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Magnetic fieldsKerr black holesFish <Actinopterygii>Relativistic jetsHumanities
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Developments towards in-gas-jet laser spectroscopy studies of actinium isotopes at LISOL

2015

To study exotic nuclides at the borders of stability with laser ionization and spectroscopy techniques, highest efficiencies in combination with a high spectral resolution are required. These usually opposing requirements are reconciled by applying the in-gas-laser ionization and spectroscopy (IGLIS) technique in the supersonic gas jet produced by a de Laval nozzle installed at the exit of the stopping gas cell. Carrying out laser ionization in the low-temperature and low density supersonic gas jet eliminates pressure broadening, which will significantly improve the spectral resolution. This article presents the required modifications at the Leuven Isotope Separator On-Line (LISOL) facility…

ActiniumNuclear and High Energy PhysicsRocket engine nozzleSeparator (oil production)chemistry.chemical_elementactinium[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesResonance ionization spectroscopylaw.inventionAtmospheric-pressure laser ionizationlawIonization0103 physical sciencesPhysics::Atomic Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsSpectroscopyInstrumentationGas jetJet (fluid)ta114010308 nuclear & particles physicsChemistrygas cellLaserActiniumresonance ionization spectroscopygas jetAtomic physicsGas cellNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Coupling hydrodynamics and radiation calculations for star-jet interactions in active galactic nuclei

2016

Context. Stars and their winds can contribute to the non-thermal emission in extragalactic jets. Because of the complexity of jet-star interactions, the properties of the resulting emission are closely linked to those of the emitting flows. Aims. We simulate the interaction between a stellar wind and a relativistic extragalactic jet and use the hydrodynamic results to compute the non-thermal emission under different conditions. Methods. We performed relativistic axisymmetric hydrodynamical simulations of a relativistic jet interacting with a supersonic, non-relativistic stellar wind. We computed the corresponding streamlines out of the simulation results and calculated the injection, evolut…

Active galactic nucleusElectromagnetic spectrumAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsElectronAstrophysicsRadiation7. Clean energy01 natural sciencessymbols.namesake0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHidrodinàmica010308 nuclear & particles physicsAstronomy and AstrophysicsStarsEstelsMagnetic fieldParticle accelerationStars13. Climate actionSpace and Planetary ScienceHydrodynamicssymbolsDoppler effectAstronomy &amp; Astrophysics
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Long-term monitoring of mrk 501 for its very high energy γ emission and a flare in 2011 october

2012

"As one of the brightest active blazars in both X-ray and very high energy γ -ray bands, Mrk 501, is very useful for" "physics associated with jets from active galactic nuclei. The ARGO-YBJ experiment has monitored Mrk 501 for γ - rays above 0.3 TeV since 2007 November. The largest flare since 2005 was observed from 2011 October and lasted until about 2012 April. In this paper, a detailed analysis of this event is reported. During the brightest γ -ray flaring episodes from 2011 October 17 to November 22, an excess of the event rate over 6σ is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the γ -ray flux above 1 TeV by a factor of 6.6 ± 2.2 from its steady…

Active galactic nucleusactive" ["galaxies]Astrophysics::High Energy Astrophysical PhenomenaFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSpectral linelaw.inventionlaw0103 physical sciencesBlazar010303 astronomy & astrophysicsPhysicsindividual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermal [BL Lacertae objects]" "general" ["gamma rays]010308 nuclear & particles physicsBL Lacertae objects: individual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermalSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsQuasarGalaxyindividual (Markarian 501)" ["BL Lacertae objects]13. Climate actionSpace and Planetary ScienceSpectral energy distributionFlare
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Variability in energy expenditure is much greater in males than females

2022

In mammals, trait variation is often reported to be greater among males than females. However, to date, mainly only morphological traits have been studied. Energy expenditure represents the metabolic costs of multiple physical, physiological, and behavioral traits. Energy expenditure could exhibit particularly high greater male variation through a cumulative effect if those traits mostly exhibit greater male variation, or a lack of greater male variation if many of them do not. Sex differences in energy expenditure variation have been little explored. We analyzed a large database on energy expenditure in adult humans (1494 males and 3108 females) to investigate whether humans have evolved s…

AdultMaleAgingDlwDLWArticleAffordable and Clean EnergyEnergeticsBehavioral and Social ScienceAnimalsHumansObesityEcology Evolution Behavior and SystematicsAgedMammalsSex CharacteristicsEvolutionary BiologyReproductionVDP::Matematikk og Naturvitenskap: 400Activity3141 Health care scienceArchaeologyAnthropologyBody CompositionFemaleTrait variabilityEnergy MetabolismBiological sex
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Sleep quality does not mediate the negative effects of chronodisruption on body composition and metabolic syndrome in healthcare workers in Ecuador

2020

Abstract Background and aims The objective of the present work was to determine to what extent sleep quality may mediate the association between chronodisruption (CD) and metabolic syndrome (MS), and between CD and body composition (BC). Methodology Cross-sectional study which included 300 adult health workers, 150 of whom were night shift workers and thereby exposed to CD. Diagnosis of MS was made based on Adult Treatment Panel III criteria. Sleep quality was measured using the Pittsburgh Sleep Quality Index. Body mass index (BMI), fat mass percentage, and visceral fat percentage were measured as indicators of body composition (BC). Data were analyzed using logistic, linear regression and …

AdultMaleHealth PersonnelEndocrinology Diabetes and MetabolismPhysiologyChronobiology DisordersFat massShift workPittsburgh Sleep Quality Index03 medical and health sciences0302 clinical medicineSDG 3 - Good Health and Well-beingWork Schedule ToleranceDiabetes mellitusHealth careInternal MedicinemedicineHumans030212 general & internal medicineSDG 7 - Affordable and Clean EnergyExerciseChronobiology PhenomenaMetabolic SyndromeSleep qualitybusiness.industryGeneral MedicineMiddle Agedmedicine.disease030210 environmental & occupational healthCross-Sectional StudiesBody CompositionFemaleEcuadorMetabolic syndromeEnergy IntakeSleepbusinessBody mass indexDiabetes and Metabolic Syndrome: Clinical Research and Reviews
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Adopting magnetocaloric heat pumping and refrigeration for electrical vehicle

2017

International audience; Refrigeration process is based on conventional gas compression and expansion techniques. However, this technique has numerous disadvantages since it generates greenhouse gas and is partly responsible for global warming. This paper exposes analternative method: magnetocaloric refrigeration that presents the advantage to combine high-energy efficiency and respect of theenvironment. Magnetic heat pumping and cooling is compared to conventional method applied on vehicle air conditioning system.Simulation results are used to demonstrate the approach.

Alternative methodsbusiness.industry020209 energy[SPI.NRJ]Engineering Sciences [physics]/Electric powerProcess (computing)Refrigeration02 engineering and technology7. Clean energyAutomotive engineering[SPI.AUTO]Engineering Sciences [physics]/Automatic13. Climate actionAir conditioningHeat pumpingGreenhouse gas0202 electrical engineering electronic engineering information engineeringMagnetic refrigeration[PHYS.MECA.THER]Physics [physics]/Mechanics [physics]/Thermics [physics.class-ph]Environmental science[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph]businessGas compressor
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Nontemplate Synthesis of CH3NH3PbBr3 Perovskite Nanoparticles

2014

To date, there is no example in the literature of free, nanometer-sized, organolead halide CH3NH3PbBr3 perovskites. We report here the preparation of 6 nm-sized nanoparticles of this type by a simple and fast method based on the use of an ammonium bromide with a medium-sized chain that keeps the nanoparticles dispersed in a wide range of organic solvents. These nanoparticles can be maintained stable in the solid state as well as in concentrated solutions for more than three months, without requiring a mesoporous material. This makes it possible to prepare homogeneous thin films of these nanoparticles by spin-coating on a quartz substrate. Both the colloidal solution and the thin film emit l…

Ammonium bromideInorganic chemistryNanoparticleHalideINGENIERÍAS Y TECNOLOGÍAS7. Clean energyBiochemistryCatalysischemistry.chemical_compoundColloidColloid and Surface ChemistryNanoparticle//purl.org/becyt/ford/2.10 [https]Thin filmFilmPerovskite (structure)NanotecnologíaColloidal DispersionGeneral ChemistryHybrid PerovskiteNano-materialeschemistryChemical engineering//purl.org/becyt/ford/2 [https]Mesoporous materialVisible spectrum
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Reversible Photodoping of TiO2 Nanoparticles for Photochromic Applications

2018

Financial support from the Estonian Research Council (IUT2-25, IUT2-26, and PUTJD680) is gratefully acknowledged. This work was supported by the Academy of Finland (decision numbers 141481 and 286713) and by the EU through the European Regional Development Fund (Center of Excellence for Zero Energy and Resource Efficient Smart Buildings and Districts-ZEBE, 2014-2020.4.01.15-0016). Work is supported by the Latvian Academy of Sciences in the framework of FLPP (Plasmonic oxide quantum dots for energy saving smart windows, lzp-2018/1-0187).

AnataseMaterials scienceGeneral Chemical EngineeringTio2 nanoparticlesPhysics::Optics02 engineering and technologyGeneral ChemistryCondensed Matter::Mesoscopic Systems and Quantum Hall Effect010402 general chemistry021001 nanoscience & nanotechnologyPhotochemistry01 natural sciences7. Clean energy0104 chemical sciencesCondensed Matter::Materials SciencePhotochromismQuantum dot:NATURAL SCIENCES:Physics [Research Subject Categories]Physics::Atomic and Molecular ClustersMaterials Chemistry0210 nano-technologyChemistry of Materials
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