Search results for "solar [matter]"

showing 10 items of 1254 documents

A procedure to calculate the I–V characteristics of thin-film photovoltaic modules using an explicit rational form

2015

Abstract Accurate models of the electrical behaviour of photovoltaic modules are effective tools for system design. One or two diode equivalent circuits have been widely used even though some mathematical difficulties were found dealing with implicit equations. In this paper, a new model based on a simple rational function, which does not contain any implicit exponential form, is presented. The model was conceived in order to be used with thin-film photovoltaic modules, whose current–voltage curves are characterised by very smooth shapes. The parameters of the model are evaluated by means of the derivatives of the issued characteristics in the short circuit and open circuit points at standa…

Amorphous siliconEngineeringSettore ING-IND/11 - Fisica Tecnica AmbientaleMaximum power principlebusiness.industryMechanical EngineeringPhotovoltaic systemThin-film photovoltaic modules five-parameter modelfI–V characteristics solar energyBuilding and ConstructionRational functionManagement Monitoring Policy and LawTopologySolar irradiancechemistry.chemical_compoundGeneral EnergychemistryElectronic engineeringEquivalent circuitSystems designbusinessShort circuit
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A procedure to evaluate the seven parameters of the two-diode model for photovoltaic modules

2019

Abstract The paper presents an analytical procedure to calculate the seven parameters of the two-diode model of photovoltaic (PV) panels for any value of the solar irradiance and cell temperature. Six parameters (the photocurrent, the diode reverse saturation currents, the quality factor of the first diode and the series and shunt resistances), are evaluated by solving the equations related to the properties of the main points of the current-voltage (I-V) characteristics. The further information, necessary to calculate the entire set of seven truly independent parameters, is based on two conditions that have to be simultaneously satisfied: 1) the exclusion of negative values of the model pa…

Amorphous siliconI-V characteristic020209 energySeven-parameter equivalent modelTwo-diode model02 engineering and technologyTopologySolar irradianceMonocrystalline siliconchemistry.chemical_compoundSolar energy0202 electrical engineering electronic engineering information engineering0601 history and archaeologyDiodeMathematicsPhotocurrent060102 archaeologyRenewable Energy Sustainability and the Environmentbusiness.industryPhotovoltaic systemPV panel06 humanities and the artsSolar energyCopper indium gallium selenide solar cellschemistrybusinessRenewable Energy
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An accurate one-diode model suited to represent the current-voltage characteristics of crystalline and thin-film photovoltaic modules

2020

Abstract In this paper a new one-diode model, conceived in order to be used to represent the current-voltage curves of both crystalline and thin-film photovoltaic modules, is presented. The model parameters are calculated from the information contained in the datasheets issued by manufactures by means of simple iterative procedures that do not require the assumption of simplifying hypotheses. Some innovative relations describing the dependence of the parameters from the solar irradiance and cell temperature are adopted in order to permit the model to reliably simulate the electrical behaviour of photovoltaic devices operating in real conditions. The ability of the model to calculate the cur…

Amorphous siliconMaterials scienceSettore ING-IND/11 - Fisica Tecnica Ambientale060102 archaeologyMaximum power principleRenewable Energy Sustainability and the Environment020209 energyPhotovoltaic systemMechanical engineering06 humanities and the arts02 engineering and technologySolar irradianceCopper indium gallium selenide solar cellsPower (physics)Monocrystalline siliconThin-film photovoltaic modules One-diode model Five-parameter model I-V characteristics Solar energychemistry.chemical_compoundchemistry0202 electrical engineering electronic engineering information engineering0601 history and archaeologyDiode
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Three-dimensional photonic crystal intermediate reflectors for enhanced light-trapping in tandem solar cells

2011

A three-dimensional photonic crystal intermediate reflector for enhanced light trapping in tandem solar cells is presented. The intermediate reflector consists of a transparent and conductive ZnO:Al inverted opal sandwiched in between the top amorphous silicon and bottom microcrystalline silicon cell.

Amorphous siliconPhotonsSiliconMaterials scienceLightTandembusiness.industryMechanical EngineeringTrappingchemistry.chemical_compoundchemistryMechanics of MaterialsSolar EnergyOptoelectronicsGeneral Materials ScienceZinc OxideCrystallizationbusinessAluminumPhotonic crystal
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Optical and ultraviolet pulsed emission from an accreting millisecond pulsar

2021

Ambrosino, F., et al.

Angular momentum010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosityNeutron starsSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsAccretion (astrophysics)Particle accelerationNeutron starAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity

2014

According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumstellar disks which they interact with through accretion of mass. The accretion builds up the star to its final mass and is also believed to power the mass outflows, which may in turn have a significant role in removing the excess angular momentum from the star-disk system. Although the process of mass accretion is a critical aspect of star formation, some of its mechanisms are still to be fully understood. On the other hand, strong flaring activity is a common feature of young stellar objects (YSOs). In the Sun, such events give rise to perturbations of the interplanetary medium. Similar but mo…

Angular momentumMHDStars: flareAstrophysics::High Energy Astrophysical PhenomenaYoung stellar objectFOS: Physical sciencesInterplanetary mediumAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAcoustics and UltrasonicAccretion accretion diskIntermediate polarAstrophysics::Solar and Stellar AstrophysicsX-rays: starSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsNuclear and High Energy PhysicGeneral Environmental SciencePhysicsRadiationStar formationAstronomyAccretion (astrophysics)StarsAstrophysics - Solar and Stellar Astrophysicslcsh:TA1-2040Space and Planetary ScienceStars: circumstellar matterGeneral Earth and Planetary SciencesCircumstellar dustAstrophysics::Earth and Planetary Astrophysicslcsh:Engineering (General). Civil engineering (General)Stars: pre-main-sequenceActa Polytechnica CTU Proceedings
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A stellar flare-coronal mass ejection event revealed by X-ray plasma motions

2019

Coronal mass ejections (CMEs), often associated with flares, are the most powerful magnetic phenomena occurring on the Sun. Stars show magnetic activity levels up to 10^4 times higher, and CME effects on stellar physics and circumstellar environments are predicted to be significant. However, stellar CMEs remain observationally unexplored. Using time-resolved high-resolution X-ray spectroscopy of a stellar flare on the active star HR 9024 observed with Chandra/HETGS, we distinctly detected Doppler shifts in S XVI, Si XIV, and Mg XII lines that indicate upward and downward motions of hot plasmas (~10-25 MK) within the flaring loop, with velocity v~100-400 km/s, in agreement with a model of fl…

Angular momentumX-ray Astronomy010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaStars: flareFOS: Physical sciencesAstrophysicsKinetic energy01 natural scienceslaw.inventionSpitzer Space Telescopelaw0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsStars: coronae010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsStarsAstrophysics - Solar and Stellar AstrophysicsStellar physicsPhysics::Space PhysicsStars: CMEAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFlare
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Evolutionary paths of binaries with a neutron star - I. The case of SAX J1808.4 - 3658

2018

The evolutionary status of the low mass X-ray binary SAX J1808.4-3658 is simulated by following the binary evolution of its possible progenitor system through mass transfer, starting at a period of $\sim$6.6 hr. The evolution includes angular momentum losses via magnetic braking and gravitational radiation. It also takes into account the effects of illumination of the donor by both the X-ray emission and the spin down luminosity of the pulsar. The system goes through stages of mass transfer and stages during which it is detached, where only the rotationally powered pulsar irradiates the donor. We show that the pulsar irradiation is a necessary ingredient to reach SAX J1808.4-3658 orbital pe…

Angular momentumastro-ph.SRAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesLuminosityPulsars: individual: SAX J1808.4Settore FIS/05 - Astronomia E AstrofisicaPulsarBinaries: closeMass transfer0103 physical sciencesBinaries: generalStars: low-maAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)3658 -X-rays: binarieHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HE010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsAstronomy and AstrophysicOrbital periodNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaLow Mass
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Modeling And Measurements Of The Arc Plasma In A Mixture Of Gases

2006

Radial distributions of Ar mass fractions and temperatures in plasmas produced in a wall-stabilized arc have been calculated. Modeling have been performed for many different mixtures of Ar+N2 and three different arc currents. The obtained results show that the radial distributions of Ar mass fractions strongly depend on the chemical composition of the plasma. In plasmas containing large amount of Ar the distributions have local minima at the arc axis (in high temperature plasma regions), whereas in plasmas consisting mainly of nitrogen the distributions reveal maxima on the discharge axis. Those features seem to be connected with the dissociation of the nitrogen.

ArgonPlasma cleaningchemistry.chemical_elementPlasmaDissociation (chemistry)chemistryPhysics::Plasma PhysicsPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsPlasma diagnosticsElectric currentAtomic physicsChemical compositionMass fractionAIP Conference Proceedings
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Temperature dependence of the rate constant of hydrogen isotope interactions with a lithium capillary-porous system under reactor irradiation

2013

Abstract Experiments with a sample of a lithium capillary-porous system (CPS) were performed at the reactor IVG-1.M of the Institute of Atomic Energy NNC RK to study the effects of neutron irradiation on the parameters of hydrogen isotope interactions with a lithium CPS. The absorption technique was used during the experiments, and this technique allowed the temperature dependences of the hydrogen isotope interaction rate constants with the lithium CPS to be obtained under various reactor powers. The obtained dependencies were used to determine the main interaction parameters: the activation energies and the pre-exponents of the Arrhenius dependence of the hydrogen interaction rate constant…

Arrhenius equationMaterials scienceHydrogenCapillary actionMechanical EngineeringDivertortechnology industry and agricultureAnalytical chemistrychemistry.chemical_elementcomplex mixturessymbols.namesakeReaction rate constantNuclear Energy and EngineeringchemistrysymbolsAstrophysics::Solar and Stellar AstrophysicsComputer Science::Programming LanguagesGeneral Materials ScienceLithiumPhysics::Atomic PhysicsIrradiationAbsorption (chemistry)Civil and Structural EngineeringFusion Engineering and Design
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