Search results for " Solar"

showing 10 items of 958 documents

Empowering Photovoltaics with Smart Light Management Technologies

2021

The daily Sun supplies the continents of the Earth with four times more energy than humanity consumes in a year. This enormous potential of solar energy to generate clean energy is therefore driving great efforts to replace conventional and unsustainable fossil fuel consumption that damages our climate and our environment. Solar photovoltaic (PV) is emerging as the fastest growing renewable energy technology in the world, yet its share to the electricity production currently is less than 3%. While coal and gas remain key to electricity production, the climate crisis demands a fast transition to a carbon-neutral energy system. In the year 2019, the PV industry produced solar panels with a ca…

Solar energyLight-trappingFlexible PVDielectric structureTandem solar cellsDiffractive structureThin-film PVPhotovoltaicPlasmonic
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Exergetic and exergoeconomic analysis of a renewable polygeneration system serving a small isolated community

2014

A great interest has been arising in the last decade for the sustainable supply of energy and fresh water, also due to the rapidly growing demand from developing countries. Facing this demand by traditional technologies and fossil energy sources implies evident difficulties and risks, because of the scarcity and high cost of fuels and their relevant environmental impact in terms of local pollution and global warming emissions. Then, the efforts of researchers have been focusing on alternative solutions, either based on the use of renewable energy sources and on innovative plant schemes for the combined and efficient production of several energy and material flows. In this paper an innovativ…

Solar heating and cooling PVT solar desalination MED exergy analysis exergoeconomicsSettore ING-IND/10 - Fisica Tecnica Industriale
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A novel solar trigeneration system integrating Photovoltaic/Thermal collectors and seawater desalination: dynamic simulation and economic assessment

2013

This paper investigates the integration of renewable energy sources and water systems, presenting a novel solar system producing simultaneously: electrical energy, thermal energy, cooling energy and domestic water. The polygeneration system under analysis includes photovoltaic/thermal solar collectors (PVT), a multi-effect distillation (MED) system for seawater desalination, a single-stage LiBr-H2O absorption chiller and additional components, such as storage tanks, auxiliary heaters and balance of plant devices. The PVT produces simultaneously electrical energy and thermal energy, at a maximum temperature of about 100 °C. The electrical energy is delivered to the grid, whereas the thermal …

Solar heating and cooling PVT solar desalination MEDSettore ING-IND/10 - Fisica Tecnica Industriale
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Sphinx measurements of the 2009 solar minimum x-ray emission

2012

The SphinX X-ray spectrophotometer on the CORONAS-PHOTON spacecraft measured soft X-ray emission in the 1-15 keV energy range during the deep solar minimum of 2009 with a sensitivity much greater than GOES. Several intervals are identified when the X-ray flux was exceptionally low, and the flux and solar X-ray luminosity are estimated. Spectral fits to the emission at these times give temperatures of 1.7-1.9 MK and emission measures between 4 x 10^47 cm^-3 and 1.1 x 10^48 cm^-3. Comparing SphinX emission with that from the Hinode X-ray Telescope, we deduce that most of the emission is from general coronal structures rather than confined features like bright points. For one of 27 intervals o…

Solar minimumAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionLuminosityTelescopeSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesROSATAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsRange (particle radiation)Spacecraft010308 nuclear & particles physicsbusiness.industryX-rayAstronomy and Astrophysicsactivity Sun: corona Sun: X-rays gamma rays [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSun: activity Sun: corona Sun: X-rays gamma raysbusiness
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Acid versus base peptization of mesoporous nanocrystalline TiO2 films: functional studies in dye sensitized solar cells

2005

We report an analysis of the influence of acid/base conditions employed in the synthesis of TiO2 nanoparticles upon the performance of dye sensitised photoelectrochemical solar cells fabricated from these particles. The functional properties of the TiO2 nanoparticles in these devices are investigated by potential step chronoamperometry, transient laser spectroscopy, and photovoltaic device characterisation. We find that base peptization conditions employed in the sol–gel fabrication of the TiO2 nanoparticles result in a reduction in film electron density under negative applied bias, correlated with slower interfacial recombination losses and a higher device open circuit voltage.

Solution of Schrödinger equation for a step potentialDye-sensitized solar cellMaterials scienceFabricationChemical engineeringOpen-circuit voltageInorganic chemistryMaterials ChemistryGeneral ChemistryChronoamperometryPeptizationMesoporous materialNanocrystalline materialJournal of Materials Chemistry
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Sensitizer exchange dynamics in air and solvent filled semiconductor nanocavities

2010

Multiple dye binding sites and their exchange in equilibrium in air and solvent filled sensitized titanium oxide nanocavities were identified by 2DIR spectroscopy. Binding geometry and flexibility may influence electron injection efficiency of solar cells.

SolventSolar cell efficiencySemiconductorMaterials scienceOrganic solar cellChemical engineeringbusiness.industryQuantum dotAnalytical chemistryInfrared spectroscopyThin filmbusinessTitanium oxideInternational Conference on Ultrafast Phenomena
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PV effect of fullerene/poly(3-hexylthiophene) blend sensitized by phthalocyanine having infrared absorption CT band

2008

An attempt was made to extend the photosensitivity spectral range of fullerene/poly(3-hexylthiophene) blend to NIR region by adding extra electron donor — hydroxygallium phthalocyanine (GaOHPc) with a strong and wide intermolecular charge transfer (CT) band around 830 nm. Multilayer cells of ITO/PEDOT: PSS/6 GaOHPc/P3HT: C61(CO2Et)2 have been prepared by spin coating with vacuum evaporated Al or In top electrodes. Significant photosensitivity of the cells was in 370–900 nm spectral range. However charge carrier photogeneration efficiency was 3 times higher for illumination in P3HT absorption band as compared with the GaOHPc CT band at 830 nm. But when GaOHPc was mixed in the blend forming P…

Spin coatingMaterials sciencebusiness.industryPhotochemistryPolymer solar cellchemistry.chemical_compoundPhotosensitivityPEDOT:PSSchemistryAbsorption bandPhthalocyanineOptoelectronicsQuantum efficiencyCharge carrierbusiness
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The effect of ISM absorption on stellar activity measurements and its relevance for exoplanet studies

2017

Past UV and optical observations of stars hosting hot Jupiters have shown that some of these stars present an anomalously low chromospheric activity, significantly below the basal level. For WASP-13, observations have shown that the apparent lack of activity is possibly caused by absorption from the intervening ISM. Inspired by this result, we study the effect of ISM absorption on activity measurements (S and logR'$_{\rm HK}$ indices) for main-sequence late-type stars. To this end, we employ synthetic stellar photospheric spectra combined with varying amounts of chromospheric emission and ISM absorption. We present the effect of ISM absorption on activity measurements by varying several ins…

Stars: activity010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsStars: late-typeAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linePlanets and satellites: general0103 physical sciencesHot JupiterAstrophysics::Solar and Stellar AstrophysicsAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesISM: generalPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Astronomy and AstrophysicsExoplanetStars: chromospheresStarsActivity measurementsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceStars: activity; Stars: chromospheres; Stars: late-type; ISM: general; Planets and satellites: generalAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Earth and Planetary Astrophysics
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Correcting the effect of stellar spots on ARIEL transmission spectra – II. The limb-darkening effect

2021

This paper is part of an effort to correct the transmission spectra of a transiting planet orbiting an active star. In Paper I (Cracchiolo et al. 2020) we have demonstrated a methodology to minimize the potential bias induced by unocculted star spots on the transmission spectrum, assuming a spot model parameterized by filling factor and temperature. In this work we introduce the limb darkening effect, therefore the position of the spot in the stellar disk and the impact parameter of the transiting planet now play a key role. The method is tested on simulations of planetary transits of three representative kinds of planetary systems, at ARIEL resolution. We find that a realistic treatment of…

Stars: activityFOS: Physical sciencesTechniques: spectroscopicAstrophysicsF.2.2; I.2.701 natural sciencesSpectral lineSettore FIS/05 - Astronomia E AstrofisicaPlanet0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Earth and Planetary Astrophysics (astro-ph.EP)PhysicsPlanets and satellites: atmosphere010308 nuclear & particles physicsFilling factorI.2.7StarspotAstronomy and AstrophysicsPlanetary systemStarspotsAstrophysics - Solar and Stellar AstrophysicsTransmission (telecommunications)Space and Planetary ScienceLimb darkeningAstrophysics::Earth and Planetary AstrophysicsF.2.2Impact parameterAstrophysics - Instrumentation and Methods for AstrophysicsTechniques: photometricAstrophysics - Earth and Planetary AstrophysicsMonthly Notices of the Royal Astronomical Society
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The GAPS programme at TNG

2020

Understanding stellar activity in M dwarfs is fundamental to improving our knowledge of the physics of stellar atmospheres and for planet search programmes. High levels of stellar activity (also with flare events) can cause additional variations in the stellar emission that contaminate the signal induced by a planet and that need to be corrected. The study of activity indicators in active stars can improve our capability of modelling this signal. Our aim is to understand the behaviour of stellar chromospheres of M stars, studying the more sensitive chromospheric activity indicators, characterising their variability and on finding the correlations among these indicators to obtain information…

Stars: activityPhysicsStars: flareStellar atmosphereFOS: Physical sciencesBalmer seriesAstronomy and AstrophysicsContext (language use)AstrophysicsStars: chromospheresSpectral linelaw.inventionStarssymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePlanetlawsymbolsSolar and Stellar Astrophysics (astro-ph.SR)FlareLine (formation)Astronomy & Astrophysics
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