Search results for " sky"

showing 10 items of 52 documents

Scaling laws in the distribution of galaxies

2004

Research done during the previous century established our Standard Cosmological Model. There are many details still to be filled in, but few would seriously doubt the basic premise. Past surveys have revealed that the large-scale distribution of galaxies in the Universe is far from random: it is highly structured over a vast range of scales. To describe cosmic structures, we need to build mathematically quantifiable descriptions of structure. Identifying where scaling laws apply and the nature of those scaling laws is an important part of understanding which physical mechanisms have been responsible for the organization of clusters, superclusters of galaxies and the voids between them. Find…

PhysicsStructure (mathematical logic)EXTRA-GALACTIC NEBULAEMICROWAVE BACKGROUND-RADIATIONCOSMIC cancer databaseCold dark matterAstrophysics (astro-ph)Cosmic microwave backgroundCAMPANAS REDSHIFT SURVEY2-POINT CORRELATION-FUNCTIONFOS: Physical sciencesGeneral Physics and AstronomyAstrophysicsN-BODY SIMULATIONSAstrophysicsPOINT CORRELATION-FUNCTIONSGalaxyCOLD DARK-MATTERFractalPROBE WMAP OBSERVATIONSDIGITAL SKY SURVEYPEAK-PATCH PICTUREStatistical physicsScalingGalaxy clusterReviews of Modern Physics
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Influence of Multiple Scattering of the Intensity and Polarization of Diffuse Sky Radiation

1964

A physical explanation of the intensity and polarization of diffusion skylight in the plane of the sun’s vertical is attempted by an approximation method which takes into account the effects of multiple scattering. Various model atmospheres are considered. The scattered radiation field is assumed to be composed of (1) the scattered radiation due to the molecular atmosphere resulting from all orders of scattering; (2) the scattered radiation due to the turbid atmosphere including primary scattering only; and (3) the scattered radiation due to the turbid atmosphere resulting from secondary and higher-order scattering. The contribution due to the first term can be computed from the tables appl…

Physicsbusiness.industryScatteringForward scatterMaterials Science (miscellaneous)Diffuse sky radiationPolarization (waves)Industrial and Manufacturing EngineeringLight scatteringsymbols.namesakeOpticssymbolsDegree of polarizationScattering theoryBusiness and International ManagementRayleigh scatteringbusinessApplied Optics
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Una linea che taglia il cielo. Carlo Scarpa a Palermo

2018

La tesi principale di questo scritto prende spunto da una la lezione itinerante dal titolo: Uno sguardo sulle mani. Carlo Scarpa a palazzo Abatellis passando dallo Steri. Questa ha fornito l’opportunità di far emergere un monito non scontato, da tenere non solo in mente, nel rapporto fra la realtà delle mani e i manufatti architettonici realizzati da Carlo Scarpa a Palermo. In senso oggettivo è un rimando agli spazi che generano di volta in volta l’idea di una strategia dei percorsi? Come cambia lo spazio di relazione in una logica dell’interconnessione? Il saggio cerca una possibile risposta a queste domande e ragionando sulla strategia dei percorsi studiati da Scarpa nei due interventi re…

Settore ICAR/14 - Composizione Architettonica E Urbanapath strategy sky visual relationships
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Vicarious calibration of MERIS over dark waters in the near infrared

2005

Abstract We propose to evaluate the calibration of MERIS (MEdium Resolution Imaging Spectrometer) over dark waters in the near infrared. We work with 5 months of data, from July to November 2003, over five world sites: Venice and Lampedusa in Italy, El Arenosillo in Spain, MOBY/Lanai and CalCOFI/San Nicolas in the United States. The sites are all equipped with a CIMEL station that forms part of the AERONET network. The basic idea is to associate CIMEL sky radiance measurements with MERIS level-1b data in a twin geometry which corresponds to the same scattering angle. This vicarious calibration relies on an accurate description of the atmospheric scattering based on the CIMEL measurements. A…

Spectrometermedia_common.quotation_subjectNear-infrared spectroscopyImaging spectrometerDiffuse sky radiationSoil ScienceGeologyAERONET[SDE.MCG] Environmental Sciences/Global Changes[ SDE.MCG ] Environmental Sciences/Global Changes[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/ClimatologySkyCalibrationRadianceEnvironmental scienceComputers in Earth Sciences[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyRemote sensingmedia_common
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Direct assessment of the sensitivity drift of SQM sensors installed outdoors

2021

Long-term monitoring of the evolution of the artificial night sky brightness is a key tool for developing science-informed public policies and assessing the efficacy of light pollution mitigation measures. Detecting the underlying artificial brightness trend is a challenging task, since the typical night sky brightness signal shows a large variability with characteristic time scales ranging from seconds to years. In order to effectively isolate the weak signature of the effect of interest, determining the potential long term drifts of the radiance sensing systems is crucial. If these drifts can be adequately characterized, the raw measurements could be easily corrected for them and transfor…

TC203-380BrightnessMonitoring010504 meteorology & atmospheric sciencesFotometriaNight skyLight pollutionFOS: Physical sciences01 natural sciencesPhotometryPhotometry (optics)0103 physical sciencesRadiació -- MesuramentRadiometry010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Lighting0105 earth and related environmental sciencesRemote sensing:Desenvolupament humà i sostenible [Àrees temàtiques de la UPC]Harbors and coast protective works. Coastal engineering. LighthousesEnllumenatContaminació lumínicaDetectorsustainable lighting light pollution monitoring radiometry photometryRangingQC350-467Optics. LightLight pollution13. Climate actionSustainable lightingRadianceRadiation -- MeasurementEnvironmental scienceRadiometryAstrophysics - Instrumentation and Methods for Astrophysics
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The starry sky, a territorial commons?

2021

International audience; Flagstaff, Arizona, United States, April 15, 1958: the city council adopts the ordinance n°440 which aims at “preventing a rapid deterioration of the visibility of the starry sky”. This regulation results from the mobilization of the Lowell Observatory astronomers against certain public lighting devices. Through this political act, the elected officials place their city at the epicenter of an emergent international movement: the ‘Dark-sky movement’. The first replica of this movement is felt in 1972 in Tucson, Arizona. From a discomfort perceived by astronomers from the Lowell and Kitt Peak observatories, the idea of ‘light pollution’ emerges and begins to spread thr…

[SHS.ARCHI]Humanities and Social Sciences/Architecture space management[SHS.GEO] Humanities and Social Sciences/Geography[SDE.MCG]Environmental Sciences/Global Changeslight pollution[SHS.GEO]Humanities and Social Sciences/Geography[SDE.ES]Environmental Sciences/Environmental and Society[SDE.BE] Environmental Sciences/Biodiversity and Ecologydark ecological network[SDE.MCG] Environmental Sciences/Global ChangesALAN[SHS.ENVIR] Humanities and Social Sciences/Environmental studiesdarkness[SHS.ENVIR]Humanities and Social Sciences/Environmental studiesstarry sky[SDE.ES] Environmental Sciences/Environmental and Society[SHS.ARCHI] Humanities and Social Sciences/Architecture space management[SDE.BE]Environmental Sciences/Biodiversity and Ecologydarkness preservationterritorialization process
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Spectral calibration of hyperspectral imagery using atmospheric absorption features

2006

One of the initial steps in the preprocessing of remote sensing data is the atmospheric correction of the at-sensor radiance images, i.e., radiances recorded at the sensor aperture. Apart from the accuracy in the estimation of the concentrations of the main atmospheric species, the retrieved surface reflectance is also influenced by the spectral calibration of the sensor, especially in those wavelengths mostly affected by gaseous absorptions. In particular, errors in the surface reflectance appear when a systematic shift in the nominal channel positions occurs. A method to assess the spectral calibration of hyperspectral imaging spectrometers from the acquired imagery is presented in this p…

atmospheric absorptionMaterials sciencebusiness.industryhyperspectral sensorMaterials Science (miscellaneous)Diffuse sky radiationAtmospheric correctionHyperspectral imaging550 - Earth sciencesIndustrial and Manufacturing EngineeringOpticsspectral calibrationFull spectral imagingRadianceRadiative transferBusiness and International ManagementbusinessRadiometric calibrationWater vaporRemote sensing
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Parental Teaching of Reading and Spelling Across the Transition From Kindergarten to Grade 1

2021

We investigated the longitudinal links between parental teaching of reading and spelling and children’s word reading and spelling skills. Data of 244 Lithuanian parent–child dyads were analyzed, who were followed across three time points: end of kindergarten (T1; Mage = 6.88; 116 girls), beginning of Grade 1 (T2), and end of Grade 1 (T3). The children’s word reading and spelling skills were tested, and the parents answered questionnaires on the frequency with which they taught their children reading and spelling. Overall, the results showed that the parents were responsive to their children’s skill levels across the domains of reading and spelling and across time (i.e., the transition from …

educationalakoululaisetPedagogika / PedagogylukeminenkotiympäristövanhemmatLietuva (Lithuania)Skaitymasesikouluikäisetteaching of reading ; teaching of spelling ; home literacy ; parents ; reading ; spellingŠeima / FamilylukutaitokirjoitustaitoRašyba. Skyryba. Ortografija / Spelling. Punctation. Orthographypsychological phenomena and processesGeneral PsychologykirjoittaminenFrontiers in Psychology
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B–T phase diagram of Pd/Fe/Ir(111) computed with parallel tempering Monte Carlo

2017

We use an atomistic spin model derived from density functional theory calculations for the ultra-thin film Pd/Fe/Ir(111) to show that temperature induces coexisting non-zero skyrmion and antiskyrmion densities. We apply the parallel tempering Monte Carlo method in order to reliably compute thermodynamical quantities and the B-T phase diagram in the presence of frustrated exchange interactions. We evaluate the critical temperatures using the topological susceptibility. We show that the critical temperatures depend on the magnetic field in contrast to previous work. In total, we identify five phases: spin spiral, skyrmion lattice, ferromagnetic phase, intermediate region with finite topologic…

frustration of magnetic exchangemagnetic skyrmionsMonte Carlo methodthermodynamic studyFOS: Physical sciencesGeneral Physics and Astronomy02 engineering and technology53001 natural sciences7. Clean energyMonte Carlo simulationsPhase (matter)0103 physical sciencesSpin model010306 general physicsTopological quantum numberPhase diagramPhysicsCondensed Matter - Materials ScienceCondensed matter physicsSkyrmionMaterials Science (cond-mat.mtrl-sci)021001 nanoscience & nanotechnologyCondensed Matter::Strongly Correlated ElectronsDensity functional theoryParallel tempering0210 nano-technologyNew Journal of Physics
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Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations

2018

Context. Asymmetries in atomic hydrogen (HI) in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project has demonstrated that isolated galaxies show the lowest level of asymmetry in their HI integrated profiles compared to even field galaxies, yet some present significant asymmetries. CIG 96 (NGC 864) is a representative case reaching a 16% level. Aims. Our aim is to investigate the HI asymmetries of the spiral galaxy CIG 96 and what processes have triggered the star-forming regions observed in the XUV pseudo-ring. Methods. We performed deep optical observations at CAHA1.23m, CAHA2.2m and V…

galaxies: spiralHIERARCHICAL SATELLITE ACCRETIONmedia_common.quotation_subjectFOS: Physical sciencesAstrophysicsI.01 natural sciences7. Clean energyAsymmetryAMIGA SAMPLElaw.inventionTelescopelaw0103 physical scienceskinematics and dynamics [galaxies]DARK-MATTER SUBSTRUCTURESurface brightness010303 astronomy & astrophysicsStellar evolutionComputingMilieux_MISCELLANEOUSevolution [galaxies]galaxies: kinematics and dynamicsLOPSIDED SPIRAL GALAXIESmedia_commonindividual: NGC 864 [galaxies]Physicsradio lines: galaxiesSpiral galaxy010308 nuclear & particles physicsgalaxies: individual: NGC864Astronomy and AstrophysicsDISK GALAXIESAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Galaxygalaxies [radio lines]RINGSTIDAL STREAMspiral [galaxies][SDU]Sciences of the Universe [physics]Space and Planetary ScienceGASAstrophysics of Galaxies (astro-ph.GA)structure [galaxies]galaxies: structureDIGITAL SKY SURVEYCirrusGalaxies: Individual: NGC 864galaxies: evolutionAstronomy & astrophysics
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