Search results for "Solar"

showing 10 items of 2301 documents

Computational engineering to enhance the photovoltaic by end‐capped and bridging core alterations: Empowering the future with solar energy through sy…

2021

Core (optical fiber)Materials scienceBridging (networking)business.industryPhotovoltaic systemComputational Science and EngineeringPhysical and Theoretical ChemistryCondensed Matter PhysicsSolar energybusinessEngineering physicsAtomic and Molecular Physics and OpticsInternational Journal of Quantum Chemistry
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Nickel-Indium Sulphide Core-Shell Nonostructures Obtained by Spray-ILGAR Deposition

2013

Ni nanowires (NWs) of different lengths were fabricated by pulsed potentiostatic deposition within pores of polycarbonate membranes. After template dissolution, substrates underwent sequential Spray-ILGAR® depositions of thin indium sulphide films. The effect of deposition temperature was also investigated. For low number of deposition cycles, results showed complete and uniform covering of metal over the entire length of NWs, with formation of Ni - In2S3 core-shell structures. However, with increasing number of deposition cycles films became uneven and crusty, especially at higher temperatures, owing to the simultaneous formation of nickel sulfide. This drawback was almost eliminated doubl…

Core-shell nanostructures electrodeposition solar cells nanowiresSettore ING-IND/23 - Chimica Fisica Applicata
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THE MISSING LINK: MERGING NEUTRON STARS NATURALLY PRODUCE JET-LIKE STRUCTURES AND CAN POWER SHORT GAMMA-RAY BURSTS

2011

Short Gamma-Ray Bursts (SGRBs) are among the most luminous explosions in the universe, releasing in less than one second the energy emitted by our Galaxy over one year. Despite decades of observations, the nature of their "central-engine" remains unknown. Considering a binary of magnetized neutron stars and solving Einstein equations, we show that their merger results in a rapidly spinning black hole surrounded by a hot and highly magnetized torus. Lasting over 35 ms and much longer than previous simulations, our study reveals that magnetohydrodynamical instabilities amplify an initially turbulent magnetic field of ~ 10^{12} G to produce an ordered poloidal field of ~ 10^{15} G along the bl…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBinary numberGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesmagnetohydrodynamics binary neutron stars gravitational waves010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsTorusGalaxyMagnetic fieldBlack holeNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstAstrophysics - Cosmology and Nongalactic AstrophysicsThe Astrophysical Journal
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MIUSCAT: extended MILES spectral coverage. I. Stellar populations synthesis models

2012

We extend the spectral range of our stellar population synthesis models based on the MILES and CaT empirical stellar spectral libraries. For this purpose we combine these two libraries with the Indo-U.S. to construct composite stellar spectra to feed our models. The spectral energy distributions (SEDs) computed with these models and the originally published models are combined to construct composite SEDs for single-age, single-metallicity stellar populations (SSPs) covering the range 3465 - 9469\AA at moderately high, and uniform, resolution (FWHM=2.51\AA). The colours derived from these SSP SEDs provide good fits to Galactic globular cluster data. We find that the colours involving redder …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::Solar and Stellar AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Euclid Preparation. XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3

2021

Stanford, S. A., et al.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Calibration (statistics)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsColor space217101 natural sciencesCosmologyLarge-scale structure010309 optics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]galaxy spectroscopySettore FIS/05 - Astronomia e AstrofisicaSpitzer Space Telescope0103 physical sciencesDISTRIBUTIONSAstrophysics::Solar and Stellar AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PHOTOMETRIC REDSHIFTS010303 astronomy & astrophysicsWeak gravitational lensingAstrophysics::Galaxy AstrophysicsPhysicsHardware_MEMORYSTRUCTURESAstrophysics::Instrumentation and Methods for AstrophysicsEuclidAstronomy and AstrophysicsRedshiftGalaxyCosmologySpace and Planetary ScienceGalaxy spectroscopyDark energyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Probing long-range leptonic forces with solar and reactor neutrinos

2006

In this work we study the phenomenological consequences of the existence of long-range forces coupled to lepton flavour numbers in solar neutrino oscillations. We study electronic forces mediated by scalar, vector or tensor neutral bosons and analyze their effect on the propagation of solar neutrinos as a function of the force strength and range. Under the assumption of one mass scale dominance, we perform a global analysis of solar and KamLAND neutrino data which depends on the two standard oscillation parameters, \Delta m^2_{21} and \tan^2\theta_{12}, the force coupling constant, its range and, for the case of scalar-mediated interactions, on the neutrino mass scale as well. We find that,…

Coupling constantPhysicsParticle physics010308 nuclear & particles physicsOscillationSolar neutrinoHigh Energy Physics::PhenomenologyScalar (mathematics)FOS: Physical sciencesAstronomy and Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentTensorNeutrino010306 general physicsLeptonBosonJournal of Cosmology and Astroparticle Physics
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CIGS THIN FILM BY ONE-STEP ELECTRODEPOSITION FOR SOLAR CELLS

2013

In this work, we present a cost-effective technique to produce CIGS thin films for solar cells by means of a single-step electrodeposition. In fact, electrodeposition is known as an easy technique for building low cost materials for photovoltaic device processing. Morphological, structural and optical characterization of these films has been performed.

Cu(InGa)Se2(CIGS)Settore ING-IND/23 - Chimica Fisica ApplicataOne-step electrodepositionCIGS solar cellThin-film solar cellSettore ING-INF/01 - Elettronica
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Electrochemical and chemical synthesis of CIS/Zn(S,O,OH) for thin film solar cells

2014

In this work, we are reporting results on the electrodeposition of the CuInSe2 thin films on molybdenum thin foil substrates. We have used an aqueous non-buffered electrolyte and a careful choice of deposition parameters to ensure a good quality and composition of the deposited films. In addition, CdS was replaced in the buffer layer with a wider bandgap Zn(S,O,OH) film obtained by chemical bath deposition. The deposited films were annealed in inert atmosphere at different temperatures. The influence of annealing temperature on the properties of the films is briefly discussed. Films were also characterized by photoelectrochemical and I-V measurements. Structural characterization was carried…

CuInSe2ElectrodepositionSolar CellThin FilmMo foil
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ALTERNATIVES TO METHYL BROMIDE IN STRAWBERRY CULTIVATION

2009

Cultural controlBiocidechemistry.chemical_compound13-DichloropropenechemistryAgronomyBromideChloropicrinSoil solarizationHorticultureChemical controlActa Horticulturae
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Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations

2019

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting constraints on its progenitor system (Dimitriadis et al. 2018, Shappee et al. 2018b). Here, we present extensive optical, ultraviolet, and near-infrared photometry, as well as dense sampling of optical spectra, for this object. SN 2018oh is relatively normal in its photometric evolution, with a rise time of 18.3$\pm$0.3 days and $\Delta$m$_{15}(B)=0.96\pm$0.03 mag, but it seems to have bluer $B - V$ colors. We construct the "uvoir" bolometric light curve hav…

DATA RELEASEULTRAVIOLETFACTORY OBSERVATIONSFOS: Physical sciencesAstrophysicsType (model theory)medicine.disease_causeSN 2011FE01 natural sciencesLuminosityPhotometry (optics)individual (SN 2018oh) [supernovae]supernovae: generalCIRCUMSTELLAR MATERIAL0103 physical sciencesmedicineSPECTRAAbsorption (logic)Ejecta010303 astronomy & astrophysicssupernovae: individualQCSolar and Stellar Astrophysics (astro-ph.SR)QBLIGHT CURVESHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHIGH-VELOCITY FEATURES010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveSupernovaAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceIMPROVED DISTANCESWHITE-DWARF MODELSAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [supernovae]Ultraviolet
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