Search results for " Solar"

showing 10 items of 958 documents

3D Order for Improved Organic Solar Cells Effiency

2010

naonoscience solar cells organic electronicsSettore CHIM/02 - Chimica Fisica
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Solar neutrino spectroscopy in Borexino

2018

International audience; In more than ten years of operation, Borexino has performed a precision measurement of the solar neutrino spectrum, resolving almost all spectral components originating from the proton-proton fusion chain. The presentation will review the results recently released for the second data taking phase 2012–2016 during which the detector excelled by its unprecedentedly low background levels. New results on the rate of pp, 7Be, pep and 8B neutrinos as well as their implications for solar neutrino oscillations and metallicity are discussed.

neutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoMetallicityNuclear physicsbackground: lowneutrino: spectrum[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino oscillationSpectroscopyBorexinoPhysicsProton–proton chain reactionpp-chainp p: fusionprecision measurementDetector* Automatic Keywords *13. Climate actionsolar neutrinosspectralHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae

2021

The eventual detection of gravitational waves from core-collapse supernovae (CCSN) will help improve our current understanding of the explosion mechanism of massive stars. The stochastic nature of the late post-bounce gravitational wave signal due to the non-linear dynamics of the matter involved and the large number of degrees of freedom of the phenomenon make the source parameter inference problem very challenging. In this paper we take a step towards that goal and present a parameter estimation approach which is based on the gravitational waves associated with oscillations of proto-neutron stars (PNS). Numerical simulations of CCSN have shown that buoyancy-driven g-modes are responsible …

noiseGravitational-wave observatorygravitational radiation: stochasticAstrophysics::High Energy Astrophysical Phenomenaprotoneutron starDegrees of freedom (physics and chemistry)FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyEinstein Telescopeeffect: nonlinearsupernova0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGOnumerical calculations010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)equation of statePhysicsSolar massmass: solarEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationoscillationgravitational radiation detectorLIGOgravitation: collapsedetector: sensitivitystar: massiveSupernovaStarswave: modelVIRGO13. Climate actiongravitational radiation: emission[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]galaxyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics and astroparticle physics
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Diurnal Cycle Relationships between Passive Fluorescence, PRI and NPQ of Vegetation in a Controlled Stress Experiment

2017

In order to estimate vegetation photosynthesis from remote sensing observations; some critical parameters need to be quantified. From all absorbed light; the plant needs to release any excess that is not used for photosynthesis; by non-photochemical quenching; by fluorescence emission and unregulated thermal dissipation. Non-photochemical quenching (NPQ) processes are controlled photoprotective mechanisms which; once activated; strongly control the dynamics of photochemical efficiency. With illumination conditions increasing and decreasing during a diurnal cycle; photoprotection mechanisms needs to change accordingly. The goal of this work is to quantify dynamic NPQ; measured from active fl…

non-photochemical energy dissipation0106 biological sciencesPhotoinhibition010504 meteorology & atmospheric sciencesSciencedroughtsolar-induced fluorescence (SIF)PhotosynthesisPhotochemical Reflectance IndexAtmospheric sciencesFLuorescence EXplorer01 natural sciencesstressDiurnal cycle0105 earth and related environmental sciencesRemote sensingphotosynthesisQuenching (fluorescence)Chemistry(FLEX)Qdrought; stress; non-photochemical energy dissipation; solar-induced fluorescence (SIF); photosynthesis; non-photochemical quenching (NPQ); Photochemical Reflectance Index (PRI); FLuorescence EXplorer; (FLEX)15. Life on landFluorescencePhotochemical Reflectance Index (PRI)non-photochemical quenching (NPQ)Photosynthetically active radiationPhotoprotectionGeneral Earth and Planetary Sciences010606 plant biology & botanyRemote Sensing; Volume 9; Issue 8; Pages: 770
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The Gaia-ESO Survey: The inner disk, intermediate-age open cluster Trumpler 23

2017

Full list of authors: Overbeek, J. C.; Friel, E. D.; Donati, P.; Smiljanic, R.; Jacobson, H. R.; Hatzidimitriou, D.; Held, E. V.; Magrini, L.; Bragaglia, A.; Randich, S.; Vallenari, A.; Cantat-Gaudin, T.; Tautvaišienė, G.; Jiménez-Esteban, F.; Frasca, A.; Geisler, D.; Villanova, S.; Tang, B.; Muñoz, C.; Marconi, G. Carraro, G.; San Roman, I.; Drazdauskas, A.; Ženovienė, R.; Gilmore, G.; Jeffries, R. D.; Flaccomio, E.; Pancino, E.; Bayo, A.; Costado, M. T.; Damiani, F.; Jofré, P.; Monaco, L.; Prisinzano, L.; Sousa, S. G.; Zaggia, S.

open clusters and associations: individual: Trumpler 23stars: abundancesMetallicityFOS: Physical sciencesGalaxy: abundances; Galaxy: disk; Galaxy: formation; Open clusters and associations: individual: Trumpler 23; Stars: abundances; Astronomy and Astrophysics; Space and Planetary ScienceAstrophysics01 natural sciencesGalaxy: diskPhotometry (optics)0103 physical sciencesGalaxy formation and evolutionDisc010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QBPhysics010308 nuclear & particles physicsabundances [Galaxy]Astronomy and AstrophysicsGalactic planeAstrophysics - Astrophysics of GalaxiesRadial velocityStarsindividual: Trumpler 23 [Open clusters and associations]Astrophysics - Solar and Stellar Astrophysicsformation [Galaxy]Space and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)abundances [Stars]Galaxy: abundancesdisk [Galaxy]Open cluster
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Donor-π-acceptors containing the 10-(1,3-dithiol-2-ylidene)anthracene unit for dye-sensitized solar cells

2012

Two donor-acceptor molecular tweezers incorporating the 10-(1,3-dithiol-2-ylidene)anthracene unit as donor group and two cyanoacrylic units as accepting/anchoring groups are reported as metal-free sensitizers for dye-sensitized solar cells. By changing the phenyl spacer with 3,4-ethylenedioxythiophene (EDOT) units, the absorption spectrum of the sensitizer is red-shifted with a corresponding increase in the molar absorptivity. Density functional calculations confirmed the intramolecular charge-transfer nature of the lowest-energy absorption bands. The new dyes are highly distorted from planarity and are bound to the TiO(2) surface through the two anchoring groups in a unidentate binding for…

optical propertiesAbsorption spectroscopypigments010402 general chemistryPhotochemistrydyes01 natural sciences7. Clean energyCatalysischemistry.chemical_compound[CHIM]Chemical SciencesComputingMilieux_MISCELLANEOUSAnthracene010405 organic chemistryOrganic ChemistryDithiolGeneral ChemistryMolar absorptivity0104 chemical sciencesDye-sensitized solar cellchemistryIntramolecular forcesensitizerssolar cellsAbsorption (chemistry)absorptionMolecular tweezers
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The Relation between Photoconductivity Threshold and Open-Circuit Voltage in Organic Solar Cells

2022

Financial support provided by Scientific Research Project for Students and Young Researchers No. SJZ/2020/08 implemented at the Institute of Solid State Physics, University of Latvia is greatly acknowledged. Institute of Solid State Physics, University of Latvia as the Centre of Excellence has received funding from the European Union’s Horizon 2020 Framework Programme H2020-WIDESPREAD-01-2016-2017-TeamingPhase2 under grant agreement No. 739508, project CAMART².

organic materialsopen-circuit voltagedirect charge transferphotoconductivity:NATURAL SCIENCES::Physics [Research Subject Categories]organic solar cellsenergy levels
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Fabrication and characterization of Donor/Acceptor heterojunction organic solar cells

2018

Results of initial development of organic solar cells having the Donor/Acceptor heterojunction structure with and without an exciton blocking layer are reported. Characterization is carried out in AM1.0 condition with 100 mW/cm2 incident optical power density. The best device has the exciton blocking layer and exhibits an open circuit voltage VOC = 0.43 V, a short circuit current density JSC = 2.35 mA/cm2 with a fill factor FF ≈ 50%, an external quantum efficiency (electrons/s over incident photons/s) EQE ≈ 5% and a power conversion efficiency of about 0.5%.

organic photovoltaicexciton blocking layerdonor/acceptor heterojuntionOrganic solar cell
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STUDIES OF VARIABILITY IN PROTO-PLANETARY NEBULAE. II. LIGHT AND VELOCITY CURVE ANALYSES OF IRAS 22272+5435 AND 22223+4327

2013

We have carried out a detailed observational study of the light, color, and velocity variations of two bright, carbon-rich proto-planetary nebulae, IRAS 22223+4327 and 22272+5435. The light curves are based upon our observations from 1994 to 2011, together with published data by Arkhipova and collaborators. They each display four significant periods, with primary periods for IRAS 22223+4327 and 22272+5435 being 90 and 132 days, respectively. For each of them, the ratio of secondary to primary period is 0.95, a value much different from that found in Cepheids, but which may be characteristic of post-asymptotic giant branch (AGB) stars. Fewer significant periods are found in the smaller radia…

oscillations [stars]Cepheid variableFOS: Physical sciencesAstrophysics01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsgeneral [planetary nebulae]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsGalaxy rotation curvePhysicsNebula010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveAGB and post-AGB [stars]Planetary nebulaRadial velocityStarsAmplitudeAstrophysics - Solar and Stellar Astrophysicsvariables: general [stars]Space and Planetary Scienceindividual (IRAS 22223+4327 IRAS 22272+5435) [stars]Astrophysics::Earth and Planetary AstrophysicsThe Astrophysical Journal
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Butlletí de problemes energia solar fotovoltaica

2019

Aquest document ha rebut l'ajut del Servei de Política Lingüística de la Universitat de València per a la correcció de materials docents en valencià. En aquest document es presenta el procediment de dimensionament d'una instal.lació solar fotovoltaica autònoma, així com el plantetjament de diversos problemes-exercicis de dimensionament d'aquest tipus d'instal.lacions.

panell solarinstal.lació solar autònomaUNESCO::CIENCIAS TECNOLÓGICASbateria
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