Search results for "Resolution"

showing 10 items of 1928 documents

Validation of a mapping and prediction model for human fasciolosis transmission in Andean very high altitude endemic areas using remote sensing data.

2001

The present paper aims to validate the usefulness of the Normalized Difference Vegetation Index (NDVI) obtained by satellite remote sensing for the development of local maps of risk and for prediction of human fasciolosis in the Northern Bolivian Altiplano. The endemic area, which is located at very high altitudes (3800-4100 m) between Lake Titicaca and the valley of the city of La Paz, presents the highest prevalences and intensities of fasciolosis known in humans. NDVI images of 1.1 km resolution from the Advanced Very High Resolution Radiometer (AVHRR) sensor on board the National Oceanic and Atmospheric Administration (NOAA) series of environmental satellites appear to provide adequate …

BoliviaFascioliasisGeographic information systemAdvanced very-high-resolution radiometerVeterinary (miscellaneous)Normalized Difference Vegetation IndexRisk FactorsmedicinePrevalenceHumansFasciolosisbusiness.industryAltitudeEffects of high altitude on humansmedicine.diseaseSatellite CommunicationsField (geography)Infectious DiseasesGeographyRemote sensing (archaeology)Insect ScienceLinear ModelsParasitologySatellitebusinessCartographyActa tropica
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High-resolution Fourier transform infrared spectroscopy and analysis of the ν3 fundamental band of P4

1999

Abstract We present the first high-resolution infrared absorption study of the ν 3 fundamental of white phosphorus, P 4 . This spectrum has been analyzed using the STDS (Spherical Top Data System) software. The band center lies at 466.286 cm −1 . With the approximation ( Bζ ) 3 =− B 0 /2, we found that the ground-state bond length is r 0 =219.58 pm. This value is consistent with that of ab initio studies reported previously but significantly different from a value obtained from a Raman study.

Bond lengthsymbols.namesakeChemistryAnalytical chemistryAb initiosymbolsGeneral Physics and AstronomyInfrared spectroscopyHigh resolutionPhysical and Theoretical ChemistryFourier transform infrared spectroscopyRaman spectroscopyFourier transform spectroscopyChemical Physics Letters
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Oscillatory integrals and fractal dimension

2021

Theory of singularities has been closely related with the study of oscillatory integrals. More precisely, the study of critical points is closely related to the study of asymptotic of oscillatory integrals. In our work we investigate the fractal properties of a geometrical representation of oscillatory integrals. We are motivated by a geometrical representation of Fresnel integrals by a spiral called the clothoid, and the idea to produce a classification of singularities using fractal dimension. Fresnel integrals are a well known class of oscillatory integrals. We consider oscillatory integral $$ I(\tau)=\int_{; ; \mathbb{; ; R}; ; ^n}; ; e^{; ; i\tau f(x)}; ; \phi(x) dx, $$ for large value…

Box dimensionGeneral Mathematics010102 general mathematicsMathematical analysisPhase (waves)Resolution of singularitiesOscillatory integral ; Box dimension ; Minkowski content ; Critical points ; Newton diagramCritical points01 natural sciencesFractal dimensionCritical point (mathematics)Oscillatory integralAmplitudeDimension (vector space)Mathematics - Classical Analysis and ODEsMinkowski contentClassical Analysis and ODEs (math.CA)FOS: Mathematics0101 mathematicsMinkowski contentOscillatory integralNewton diagram[MATH]Mathematics [math]fractal dimension; box dimension; oscillatory integrals; theory of singularitiesMathematics
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A method to reduce the FP/imm number through CC and MLO views comparison in mammographic images

2008

In this paper we propose a method to reduce the FP/imm number through CC and MLO mammographic views comparison of the same patient. The proposed solution uses the symmetry properties of the breast to compute a geometric transformation that permits to represent the two images in comparable coordinates systems. Through this method, potential pathological ROIs of one of the projections are correlated with the ROIs in the second view. To show the effectiveness of the result we apply the method on a dataset composed of 112 couples of pathological images. Experiments shows that method enables a reduction by up to 700/0 of the FP/imm number detected after the classification step

Breast tissueData setbusiness.industryPathological imageGeometric transformationPattern recognitionSymmetry propertiesReduction (complexity)CorrelationMedical imagingMedicineArtificial intelligenceNuclear medicinebusinessGeometric transformationImage resolutionTransformation geometryMammographicMammographic image2008 IEEE Nuclear Science Symposium Conference Record
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ARES I: WASP-76 b, A Tale of Two HST Spectra

2020

We analyse the transmission and emission spectra of the ultra-hot Jupiter WASP-76b, observed with the G141 grism of the Hubble Space Telescope's Wide Field Camera 3 (WFC3). We reduce and fit the raw data for each observation using the open-source software Iraclis before performing a fully Bayesian retrieval using the publicly available analysis suite TauRex 3. Previous studies of the WFC3 transmission spectra of WASP-76 b found hints of titanium oxide (TiO) and vanadium oxide (VO) or non-grey clouds. Accounting for a fainter stellar companion to WASP-76, we reanalyse this data and show that removing the effects of this background star changes the slope of the spectrum, resulting in these vi…

Brightness010504 meteorology & atmospheric sciencesExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope; Astrophysics - Earth and Planetary AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstronomy & AstrophysicsExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope01 natural sciencesSpectral lineAtmosphereJupiterHAT-P-7B0103 physical sciencesHubble Space TelescopeAstrophysics::Solar and Stellar AstrophysicsEmission spectrumMOLECULAR LINE LISTS010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHOTPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Science & TechnologyAstronomy and AstrophysicsATMOSPHEREGIANT EXOPLANETGrismRESOLUTIONTransmission (telecommunications)Exoplanet atmospheric composition13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Physical SciencesINFERENCEAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Wide Field Camera 3STARSExoplanet atmospheresAstrophysics - Earth and Planetary Astrophysics
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First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

2019

We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ~40 μas, consistent with the size and shape of the lensed photon orbit encircling the "shadow" of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others' work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to av…

Brightness010504 meteorology & atmospheric sciencesgalaxies: jetAstronomyblack hole physicsFOS: Physical sciencesgalaxies: individualtechniques: image processingAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciencesSynthetic dataGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)0103 physical sciencesimage processing [Techniques]010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesEvent Horizon TelescopePhysicsGround truthSupermassive black holetechniques: high angular resolutionAstronomy and AstrophysicsBlack hole physicsgalaxies: jetsindividual (M87) [Galaxies]Astrophysics - Astrophysics of Galaxiesblack hole physic3. Good healthOrbitInterferometryhigh angular resolution [Techniques]Space and Planetary Sciencetechniques: interferometricAstrophysics of Galaxies (astro-ph.GA)interferometric [Techniques]jets [Galaxies]Deconvolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for Astrophysics
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Imation of land surface emissivity differences in the split-window channels of AVHRR

1994

Abstract A method for estimating the difference between the channel emissivities in NOAA-AVHRR Channels 4 and 5 is proposed and applied to a data set from the HAPEX-MOBILHY experiment. The method is based on the separation between the atmospheric and emissivity effects in the brightness temperature difference measured with AVHRR Channels 4 and 5. Atmospheric profiles coincident to the satellite overpass and a radiative transfer model are required to estimate the atmospheric correction for brightness temperatures. With this procedure, the emissivity difference Δe is obtained at the satellite spatial and spectral resolution, which has a great interest for correcting thermal images with the sp…

BrightnessAtmospheric correctionSoil ScienceGeologyAtmospheric radiative transfer codesCoincidentBrightness temperatureEmissivityAstrophysics::Solar and Stellar AstrophysicsEnvironmental scienceSatelliteComputers in Earth SciencesSpectral resolutionPhysics::Atmospheric and Oceanic PhysicsRemote sensingRemote Sensing of Environment
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Microwave and optical data fusion for global mapping of soil moisture at high resolution

2018

After more than 8 years in orbit the Soil Moisture and Ocean Salinity (SMOS) satellite is still in good health and several algorithms for improving its spatial resolution have been proposed and validated in a variety of catchments. However, none of them has yet been applied at the global scale. In this article we present: i) a review of the latest SMOS-BEC downscaling algorithm, which allows for its global application using an adaptive moving window and ii) a thorough validation of the resulting maps over two in-situ networks: REMEDHUS in Spain and OzNet in Australia. The proposed algorithm combines SMOS brightness temperatures (at ~40 km spatial resolution), and MODIS-derived Land Surface …

BrightnessTeledetecció010504 meteorology & atmospheric sciences0211 other engineering and technologies02 engineering and technology01 natural sciences:Enginyeria agroalimentària::Ciències de la terra i de la vida::Edafologia [Àrees temàtiques de la UPC]In-situ stationsDownscalingImage resolutionWater content021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingAdaptive moving windowRemote sensing:Enginyeria de la telecomunicació::Radiocomunicació i exploració electromagnètica::Teledetecció [Àrees temàtiques de la UPC]Orbit (dynamics)Environmental scienceERA5SatelliteSoil moistureSòls -- HumitatScale (map)MicrowaveDownscalingSMOS
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Atmospheric dust, early cases, and localized meningitis epidemics in the African meningitis belt: an analysis using high spatial resolution data.

2018

8 pages; International audience; Background : Bacterial meningitis causes a high burden of disease in the African meningitis belt, with regular seasonal hyperendemicity and sporadic short, but intense, localized epidemics during the late dry season occurring at a small spatial scale [i.e., below the district level, in individual health centers (HCs)]. In addition, epidemic waves with larger geographic extent occur every 7–10 y. Although atmospheric dust load is thought to be an essential factor for hyperendemicity, its role for localized epidemics remains hypothetic.Objectives : Our goal was to evaluate the association of localized meningitis epidemics in HC catchment areas with the dust lo…

Burden of disease010504 meteorology & atmospheric sciencesHealth Toxicology and MutagenesisMeningitis Meningococcal01 natural sciences03 medical and health sciences0302 clinical medicine[SDV.MHEP.MI]Life Sciences [q-bio]/Human health and pathology/Infectious diseasesEnvironmental healthBurkina FasoHigh spatial resolutionmedicineHumans030212 general & internal medicineEpidemics0105 earth and related environmental sciencesIncidence (epidemiology)IncidenceResearchPublic Health Environmental and Occupational HealthDustAtmospheric dustmedicine.disease3. Good healthGeography[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyBacterial meningitis[SDV.SPEE]Life Sciences [q-bio]/Santé publique et épidémiologieSeasonsAfrican meningitis beltMeningitis
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MILES extended: Stellar population synthesis models from the optical to the infrared

2016

We present the first single-burst stellar population models which covers the optical and the infrared wavelength range between 3500 and 50000 Angstrom and which are exclusively based on empirical stellar spectra. To obtain these joint models, we combined the extended MILES models in the optical with our new infrared models that are based on the IRTF (Infrared Telescope Facility) library. The latter are available only for a limited range in terms of both age and metallicity. Our combined single-burst stellar population models were calculated for ages larger than 1 Gyr, for metallicities between [Fe/H] = -0.40 and 0.26, for initial mass functions of various types and slopes, and on the basis …

CAII TRIPLETStellar populationInfraredMetallicityINITIAL MASS FUNCTIONBROWN DWARFSInfrared telescopeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomical spectroscopyinfrared: galaxiesATMOSPHERIC PARAMETERS0103 physical sciencesRange (statistics)Astrophysics::Solar and Stellar Astrophysics2.5 MU-MGIANT BRANCH STARS010303 astronomy & astrophysicsinfrared: starsEMPIRICAL CALIBRATIONAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsNear-infrared spectroscopyHIGH-SPECTRAL-RESOLUTIONAstronomy and AstrophysicsEVOLUTIONARY SYNTHESISAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)NEWTON-TELESCOPE LIBRARYgalaxies: stellar contentAstrophysics::Earth and Planetary Astrophysics
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