Search results for "Solar"

showing 10 items of 2301 documents

The assessment of the reliability of an innovative 3rd generation solar cell integrated with “thermal belt” glass block

2017

Glass block is a building product widely used for the construction of translucent building façades and roofs. The need to adapt the product to the regulations in the field of energy saving and environmental sustainability has led to the design of innovative configurations, through the integration of different sub-components. These ones are able to improve its energy performance by means of the integration of a“thermal belt”, cold glued to the glass shells, which constitute the traditional glass block, and 3rd generation solar cells. This paper reports the first results of the experimental program designed to assess some durability components: inherent and critical reliability. <div id="g…

lcsh:Architectural engineering. Structural engineering of buildingsComplementary and alternative medicinelcsh:TH845-895Settore ICAR/10 - Architettura TecnicaPharmaceutical SciencePharmacology (medical)Glass-block Durability Reliability Accelerated aging Dye-sensitized solar cellTema
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Determining the infrared radiative effects of Saharan dust: a radiative transfer modelling study based on vertically resolved measurements at Lampedu…

2018

Detailed measurements of radiation, atmospheric and aerosol properties were carried out in summer 2013 during the Aerosol Direct Radiative Impact on the regional climate in the MEDiterranean region (ADRIMED) campaign in the framework of the Chemistry-Aerosol Mediterranean Experiment (ChArMEx) experiment. This study focusses on the characterization of infrared (IR) optical properties and direct radiative effects of mineral dust, based on three vertical profiles of atmospheric and aerosol properties and IR broadband and narrowband radiation from airborne measurements, made in conjunction with radiosonde and ground-based observations at Lampedusa, in the central Mediterranean. Satellite IR spe…

lcsh:Chemistrylcsh:QD1-999Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Earth and Planetary AstrophysicsPhysics::Atmospheric and Oceanic PhysicsAstrophysics::Galaxy Astrophysicslcsh:Physicslcsh:QC1-999Atmospheric Chemistry and Physics
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Temperature variability in the Iberian Range since 1602 inferred from tree-ring records

2017

Abstract. Tree rings are an important proxy to understand the natural drivers of climate variability in the Mediterranean Basin and hence to improve future climate scenarios in a vulnerable region. Here, we compile 316 tree-ring width series from 11 conifer sites in the western Iberian Range. We apply a new standardization method based on the trunk basal area instead of the tree cambial age to develop a regional chronology which preserves high- to low-frequency variability. A new reconstruction for the 1602–2012 period correlates at −0.78 with observational September temperatures with a cumulative mean of the 21 previous months over the 1945–2012 calibration period. The new IR2Tmax reconstr…

lcsh:GE1-350Global and Planetary Changegeographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesStratigraphyLaglcsh:Environmental protectionPaleontology010502 geochemistry & geophysicsSolar irradiance01 natural sciencesMediterranean BasinBasal areaVolcanolcsh:Environmental pollutionPeninsulaClimatologylcsh:TD172-193.5Dendrochronologylcsh:TD169-171.8Geologylcsh:Environmental sciences0105 earth and related environmental sciencesChronology
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A study of solar panel efficiency in Latvian climate conditions

2020

With solar panels increasingly used in nearly zero energy building solutions it is important to clarify if the panels can achieve the efficiency indicators specified by their producers in real operation conditions. To determine the efficiency of poly- and monocrystalline panels depending on their spatial orientation and the seasons a set of test panels was installed in 2018 in Riga, Latvia for long-term monitoring of the amount of generated power and produced energy. Here we summarize the results of the first year of monitoring. Data indicate that orientation has high significance, very small amounts of energy are generated in autumn/winter and that there is a good correspondence of the act…

lcsh:GE1-350Zero-energy buildingMeteorology020209 energyCloud coverLatvian02 engineering and technologylanguage.human_languageSolar cell efficiency020401 chemical engineering0202 electrical engineering electronic engineering information engineeringlanguageEnvironmental scienceProduction (economics)0204 chemical engineeringlcsh:Environmental sciencesE3S Web of Conferences
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Seasonal Modulation of the $^7$Be Solar Neutrino Rate in Borexino

2017

We detected the seasonal modulation of the $^7$Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, and phase of the observed time evolution of the signal are consistent with its solar origin, and the absence of an annual modulation is rejected at 99.99\% C.L. The data are analyzed using three methods: the sinusoidal fit, the Lomb-Scargle and the Empirical Mode Decomposition techniques, which all yield results in excellent agreement.

liquid scintillators detectorsPhysics - Instrumentation and Detectorsexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinolow background detectorsSolar neutrinos01 natural sciencesflux: time dependenceneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Liquid scintillators detectors; Low background detectors; Neutrino oscillations; Solar neutrinos; Astronomy and Astrophysics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Borexinoneutrino: interactionMSW effectPhysicsNeutrino oscillationsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)neutrino electron: elastic scatteringmodulationAmplitudeModulationsolar neutrinosBorexinoNeutrinoLiquid scintillators detectorFLUXLow background detectordata analysis methodNeutrino oscillationFOS: Physical sciencesSolar neutrinoNuclear physicsTIME-SERIES ANALYSIS[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Low background detectorsLiquid scintillators detectorsSEARCH0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SPACED DATA010306 general physicsNeutrino oscillationbackground: radioactivityneutrino oscillations010308 nuclear & particles physicsAstronomy and AstrophysicsEMPIRICAL MODE DECOMPOSITIONberylliumGran SassoHigh Energy Physics::Experimentneutrino: oscillationEvent (particle physics)experimental results
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Precision 71Ga – 71Ge mass-difference measurement

2016

The 71Ga(νe, e−) 71Ge reaction Q value has been measured with the JYFLTRAP mass spectrometer at the IGISOL facility of the University of Jyv¨askyl¨a to Q = 232.443(93) keV. This value agrees with previous measurements, though it features a much higher accuracy. The Q value is being discussed in the context of the solar neutrino capture rate in 71Ga. peerReviewed

mass measurementsQ value for solar-neutrino capture rates
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Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006

2018

We present ~400ks NuSTAR observations of the northeast (NE) and southwest (SW) non-thermal limbs of the Galactic SNR SN1006. We discovered three sources with X-ray emission detected at >50keV. Two of them are identified as background AGN. We extract the NuSTAR spectra from a few regions along the non-thermal limbs and jointly analyze them with the XMM-Newton spectra and the radio data. The broad-band radio/X-ray spectra can be well described with a synchrotron emission model from a single population of CR electrons with a power law energy distribution and an exponential cutoff. The power law index of the electron particle distribution function (PDF) is ~1.88-1.95 for both the NE and SW l…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryPower lawSpectral linecosmic rays0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumeducation010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonISM: supernova remnantsacceleration of particlesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_study010308 nuclear & particles physicsAstronomy and Astrophysicsshock wavesAstronomy and Astrophysicradiation mechanisms: non-thermalX-rays: ISMMagnetic fieldSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Lepton
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Discovery of slow X-ray pulsations in the high-mass X-ray binary 4U 2206+54

2008

Context. The source 4U 2206+54 is one of the most enigmatic high-mass X-ray binaries. In spite of intensive searches, X-ray pul- sations have not been detected in the time range 10−3–103 s. A cyclotron line at ∼30 keV has been suggested by various authors but never detected with significance. The stellar wind of the optical companion is abnormally slow. The orbital period, initially reported to be 9.6 days, disappeared and a new periodicity of 19.25 days emerged. Aims. The main objective of our RXTE monitoring of 4U 2206+54 is to study the X-ray orbital variability of the spectral and timing parameters. The new long and uninterrupted RXTE observations allow us to search for long (∼1 h) puls…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenapulsars : general [Stars]X-ray binaryFOS: Physical sciencesOrbital eccentricityAstrophysicsAstrophysicsStars : early-type; Stars : emission-line Be; Stars : binaries : close; X-rays : binaries; Stars : pulsars : generalLuminosityearly-type [Stars]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos XAstrophysics::Solar and Stellar AstrophysicsEccentricity (behavior)binaries : close [Stars]media_commonLine (formation)PhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsOrbital periodLight curveNeutron starSpace and Planetary Scienceemission-line Be [Stars]binaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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Lyman break and ultraviolet-selected galaxies at z ̃ 1-I. Stellar populations from the ALHAMBRA survey

2013

We take advantage of the exceptional photometric coverage provided by the combination of GALEX data in the ultraviolet (UV) and the ALHAMBRA survey in the optical and near-infrared to analyse the physical properties of a sample of 1225 GALEX-selected Lyman break galaxies (LBGs) at 0.8 ≲ z ≲ 1.2 that are located in the COSMOS field. This is the largest sample of LBGs studied in this redshift range to date. According to a spectral energy distribution (SED) fitting with synthetic stellar population templates, we find that LBGs at z ̃ 1 are mostly young galaxies with a median age of 341 Myr and have intermediate dust attenuation, (Es(B - V)) ̃ 0.20. Owing to the selection criterion, LBGs at z ̃…

media_common.quotation_subjectLibrary scienceAstrophysics::Cosmology and Extragalactic Astrophysicsstar formation [Galaxies]high-redshift [Galaxies]ExcellenceAstrophysics::Solar and Stellar Astrophysicsobservations [Cosmology]Astrophysics::Galaxy Astrophysicsmedia_commonPhysicsGalaxies: star formationphotometry [Galaxies]Cosmology: observationsGalaxies: high-redshiftAstronomyGalaxies: evolutionAstronomy and AstrophysicsGalaxies: photometryevolution [Galaxies]Galaxygalaxies [Ultraviolet]Space and Planetary ScienceUltraviolet: galaxiesAstrophysics::Earth and Planetary AstrophysicsAdministration (government)
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The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS+)

2014

The VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+) is surveying the southern Milky Way in u, g, r, i and Halpha at 1 arcsec angular resolution. Its footprint spans the Galactic latitude range -5 < b < +5 at all longitudes south of the celestial equator. Extensions around the Galactic Centre to Galactic latitudes +/-10 bring in much of the Galactic Bulge. This ESO public survey, begun on 28th December 2011, reaches down to 20th magnitude (10-sigma) and will provide single-epoch digital optical photometry for around 300 million stars. The observing strategy and data pipelining is described, and an appraisal of the segmented narrowband Halpha filter in us…

media_common.quotation_subjectMilky WayAstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energyPhotometry (optics)BulgeQB460Astrophysics::Solar and Stellar AstrophysicsQCAstrophysics::Galaxy Astrophysicsmedia_commonQBPhysicsCelestial equatorWhite dwarfAstronomyAstronomy and AstrophysicsGalactic planeAstrophysics - Astrophysics of GalaxiesStars13. Climate actionSpace and Planetary ScienceSkyAstrophysics of Galaxies (astro-ph.GA)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics::Earth and Planetary Astrophysics
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