Search results for "Fitting method"

showing 10 items of 21 documents

Compensation of Oxygen Transmittance Effects for Proximal Sensing Retrieval of Canopy–Leaving Sun–Induced Chlorophyll Fluorescence

2018

Estimates of Sun–Induced vegetation chlorophyll Fluorescence (SIF) using remote sensing techniques are commonly determined by exploiting solar and/or telluric absorption features. When SIF is retrieved in the strong oxygen (O 2 ) absorption features, atmospheric effects must always be compensated. Whereas correction of atmospheric effects is a standard airborne or satellite data processing step, there is no consensus regarding whether it is required for SIF proximal–sensing measurements nor what is the best strategy to be followed. Thus, by using simulated data, this work provides a comprehensive analysis about how atmospheric effects impact SIF estimations on proximal sensing, regarding: (…

1171 GeosciencesFLUXspectral fitting method (SFM)AIRBORNE010504 meteorology & atmospheric sciencesScience0211 other engineering and technologiesFlux02 engineering and technologyfraunhofer line discriminator (FLD)Surface pressure01 natural sciencesO2 transmittanceAtmospheric radiative transfer codesatmospheric pressureFIELD SPECTROSCOPYTransmittanceAstrophysics::Solar and Stellar AstrophysicsSPACESpectral resolutionAbsorption (electromagnetic radiation)021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingproximal sensing4112 Forestrysun-induced chlorophyll fluorescence (SIF)Atmospheric pressureSTRESS DETECTIONPHOTOSYNTHESISQAtmospheric correctionO-2 transmittanceair temperatureREFLECTANCEsun–induced chlorophyll fluorescence (SIF)Physics::Space Physicssun–induced chlorophyll fluorescence (SIF); proximal sensing; O<sub>2</sub> transmittance; fraunhofer line discriminator (FLD); spectral fitting method (SFM); air temperature; atmospheric pressureLUMINESCENCEGeneral Earth and Planetary SciencesEnvironmental scienceABSORPTION-BANDSAstrophysics::Earth and Planetary AstrophysicsVEGETATIONRemote Sensing
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FPGA implementation of a deep learning algorithm for real-time signal reconstruction in particle detectors under high pile-up conditions

2019

The analog signals generated in the read-out electronics of particle detectors are shaped prior to the digitization in order to improve the signal to noise ratio (SNR). The real amplitude of the analog signal is then obtained using digital filters, which provides information about the energy deposited in the detector. The classical digital filters have a good performance in ideal situations with Gaussian electronic noise and no pulse shape distortion. However, high-energy particle colliders, such as the Large Hadron Collider (LHC) at CERN, can produce multiple simultaneous events, which produce signal pileup. The performance of classical digital filters deteriorates in these conditions sinc…

Calibration and fitting methods010308 nuclear & particles physicsSignal reconstructionComputer scienceCluster findingDetectorTime signal01 natural sciencesSignal030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineSignal-to-noise ratioAnalog signalPattern recognitionData processing methods0103 physical sciencesSimulation methods and programsInstrumentationDigital filterAlgorithmMathematical PhysicsEnergy (signal processing)Journal of Instrumentation
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Performance of Spectral Fitting Methods for vegetation fluorescence quantification

2010

The Fraunhofer Line Discriminator (FLD) principle has long been considered as the reference method to quantify solar-induced chlorophyll fluorescence (F) from passive remote sensing measurements. Recently, alternative retrieval algorithms based on the spectral fitting of hyperspectral radiance observations, Spectral Fitting Methods (SFMs), have been proposed. The aim of this manuscript is to investigate the performance of such algorithms and to provide relevant information regarding their use. FLD and SFMs were used to estimate F starting from Top Of Canopy (TOC) fluxes at very high spectral resolution (0.12 nm) and sampling interval (0.1 nm), exploiting the O2-B (687.0 nm) and O2-A (760.6 …

DiscriminatorreflectanceHyperspectral remote sensingSolar-induced chlorophyll fluorescenceMETIS-304492Soil Science550 - Earth sciencesFraunhofer Line Discriminatorin-vivoNoise (electronics)Spectral lineRadiative transfer simulationLaboratory of Geo-information Science and Remote SensingSampling (signal processing)luminescenceLaboratorium voor Geo-informatiekunde en Remote Sensinginduced chlorophyll fluorescenceComputers in Earth SciencesSpectral resolutionMathematicsRemote sensingcanopymodelphotosynthesisscatteringairborneHyperspectral imagingGeologySpectral Fitting MethodPE&RCAGR/14 - PEDOLOGIASpectroradiometerspectroradiometerRadianceREMOTE SENSING OF ENVIRONMENT
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Interpretation of Ocular Melanin Drug Binding Assays. Alternatives to the Model of Multiple Classes of Independent Sites

2016

Melanin has a high binding affinity for a wide range of drugs. The determination of the melanin binding capacity and its binding affinity are important, e.g., in the determination of the ocular drug distribution, the prediction of drug effects in the eye, and the trans-scleral drug delivery. The binding parameters estimated from a given data set vary significantly when using different isotherms or different nonlinear fitting methods. In this work, the commonly used bi-Langmuir isotherm, which assumes two classes of independent sites, is confronted with the Sips isotherm. Direct, log-log, and Scatchard plots are used, and the interpretation of the binding curves in the latter is critically a…

Drugmedia_common.quotation_subjectBinding energyPharmaceutical Science02 engineering and technology010402 general chemistryBioinformatics01 natural sciencesInterpretation (model theory)MelaninGoodness of fitMelanin bindingFitting methodsDrug Discoverymedia_commonMelaninsScatchard plotChemistrytechnology industry and agricultureChloroquineModels Theoretical021001 nanoscience & nanotechnology0104 chemical sciencesKineticsBiophysicsMolecular Medicine0210 nano-technologyMetoprololMolecular Pharmaceutics
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A Convolutional Neural Network based Cascade Reconstruction for the IceCube Neutrino Observatory

2021

Continued improvements on existing reconstruction methods are vital to the success of high-energy physics experiments, such as the IceCube Neutrino Observatory. In IceCube, further challenges arise as the detector is situated at the geographic South Pole where computational resources are limited. However, to perform real-time analyses and to issue alerts to telescopes around the world, powerful and fast reconstruction methods are desired. Deep neural networks can be extremely powerful, and their usage is computationally inexpensive once the networks are trained. These characteristics make a deep learning-based approach an excellent candidate for the application in IceCube. A reconstruction …

FOS: Computer and information sciencesComputer Science - Machine LearningAstrophysics::High Energy Astrophysical Phenomenacs.LGData analysisFOS: Physical sciencesFitting methods01 natural sciencesConvolutional neural networkCalibration; Cluster finding; Data analysis; Fitting methods; Neutrino detectors; Pattern recognitionHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryMachine Learning (cs.LG)High Energy Physics - Experiment (hep-ex)Pattern recognition0103 physical sciencesNeutrino detectors010303 astronomy & astrophysicsInstrumentationMathematical Physics010308 nuclear & particles physicsbusiness.industryhep-exDeep learningCluster findingDetectorNeutrino detectorComputer engineeringOrders of magnitude (time)13. Climate actionCascadeCalibrationPattern recognition (psychology)Artificial intelligencebusiness
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Exploring the spatial relationship between airborne-derived red and far-red sun-induced fluorescence and process-based GPP estimates in a forest ecos…

2019

International audience; Terrestrial gross primary productivity (GPP) plays an essential role in the global carbon cycle, but the quantification of the spatial and temporal variations in photosynthesis is still largely uncertain. Our work aimed to investigate the potential of remote sensing to provide new insights into plant photosynthesis at a fine spatial resolution. This goal was achieved by exploiting high-resolution images acquired with the FLuorescence EXplorer (FLEX) airborne demonstrator HyPlant. The sensor was flown over a mixed forest, and the images collected were elaborated to obtain two independent indicators of plant photosynthesis. First, maps of sun-induced chlorophyll fluore…

Forest ecosystems[SDV.SA]Life Sciences [q-bio]/Agricultural sciences010504 meteorology & atmospheric sciencesFIS/06 - FISICA PER IL SISTEMA TERRA E PER IL MEZZO CIRCUMTERRESTRE0208 environmental biotechnologyGEO/04 - GEOGRAFIA FISICA E GEOMORFOLOGIASpectral fitting methodSoil Science02 engineering and technology01 natural sciencesArticleCarbon cycleGEO/11 - GEOFISICA APPLICATAAtmospheric radiative transfer codesAirborne spectroscopyForest ecologySun-induced chlorophyll fluorescenceddc:550LUEEcosystemAPARSun-induced chlorophyll fluorescenceSpectral fitting methodPlant traitsINFORMGPPAPARLUEBESSForest ecosystemsHyPlantAirborne spectroscopyComputers in Earth SciencesChlorophyll fluorescenceBESS0105 earth and related environmental sciencesRemote sensingPlant traitsINFORMGEO/12 - OCEANOGRAFIA E FISICA DELL'ATMOSFERAGeology15. Life on land020801 environmental engineeringSpatial heterogeneityGEO/10 - GEOFISICA DELLA TERRA SOLIDA13. Climate actionHyPlantEnvironmental scienceSpatial variabilityGPPScale (map)
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Precision luminosity measurements at LHCb

2014

Measuring cross-sections at the LHC requires the luminosity to be determined accurately at each centre-of-mass energy $\sqrt{s}$. In this paper results are reported from the luminosity calibrations carried out at the LHC interaction point 8 with the LHCb detector for $\sqrt{s}$ = 2.76, 7 and 8 TeV (proton-proton collisions) and for $\sqrt{s_{NN}}$ = 5 TeV (proton-lead collisions). Both the "van der Meer scan" and "beam-gas imaging" luminosity calibration methods were employed. It is observed that the beam density profile cannot always be described by a function that is factorizable in the two transverse coordinates. The introduction of a two-dimensional description of the beams improves sig…

Instrumentation for particle accelerators and storage rings - high energy (linear acceleratorsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)cluster finding[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment06.20.fbInstrumentationMathematical PhysicsQCPhysicsLuminosity (scattering theory)Large Hadron ColliderPattern recognition cluster finding calibration and fitting methodssynchrotrons)DetectorPattern recognition cluster finding calibration and fitting methodsComputer interfacecalibration and fitting methodsFísica nuclearTracking and position-sensitive detectorLHCParticle Physics - ExperimentParticle physics29.40.GxPattern recognition cluster finding calibration and fitting methods; Instrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsLHCb - Abteilung HofmannPattern recognition cluster finding calibration and fitting methodInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons)NOConsistency (statistics)Pattern recognitionCalibrationSDG 7 - Affordable and Clean EnergyInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons)/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyInteraction pointStandards and calibrationFunction (mathematics)29.50.+vLHCbInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons); Pattern recognition cluster finding calibration and fitting methods; Instrumentation; Mathematical PhysicsTEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons); Pattern recognition cluster finding calibration and fitting methodsEnergy (signal processing)
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Initial results of NEXT-DEMO, a large-scale prototype of the NEXT-100 experiment

2013

NEXT-DEMO is a large-scale prototype of the NEXT-100 detector, an electroluminescent time projection chamber that will search for the neutrinoless double beta decay of Xe-136 using 100-150 kg of enriched xenon gas. NEXT-DEMO was built to prove the expected performance of NEXT-100, namely, energy resolution better than 1% FWHM at 2.5MeV and event topological reconstruction. In this paper we describe the prototype and its initial results. A resolution of 1.75% FWHM at 511 keV (which extrapolates to 0.8% FWHM at 2.5 MeV) was obtained at 10 bar pressure using a gamma-ray calibration source. Also, a basic study of the event topology along the longitudinal coordinate is presented, proving that it…

MECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhysics - Instrumentation and DetectorsBar (music)Isòtops radioactius -- DesintegracióTime projection chambersPattern recognition SystemsFOS: Physical scienceschemistry.chemical_elementElectron7. Clean energy01 natural sciencesNuclear physicsTECNOLOGIA ELECTRONICAXenonCambres d'ionitzacióCluster analysisDouble beta decayPattern recognition0103 physical sciencesCalibrationReconeixement de formes (Informàtica)Calibratge010306 general physicsInstrumentationMathematical PhysicsRadioisotopes -- DecayPhysicsCalibration and fitting methodsTime projection chamber010308 nuclear & particles physicsDetectorCluster findingFísicaInstrumentation and Detectors (physics.ins-det)Double-beta decay detectorsAnàlisi de conglomeratschemistryCalibrationEvent (particle physics)Ionization Chambers
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Operation and first results of the NEXT-DEMO prototype using a silicon photomultiplier tracking array

2013

NEXT-DEMO is a high-pressure xenon gas TPC which acts as a technological test-bed and demonstrator for the NEXT-100 neutrinoless double beta decay experiment. In its current configuration the apparatus fully implements the NEXT-100 design concept. This is an asymmetric TPC, with an energy plane made of photomultipliers and a tracking plane made of silicon photomultipliers (SiPM) coated with TPB. The detector in this new configuration has been used to reconstruct the characteristic signature of electrons in dense gas, demonstrating the ability to identify the MIP and "blob" regions. Moreover, the SiPM tracking plane allows for the definition of a large fiducial region in which an excellent e…

PhotomultiplierMECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhysics - Instrumentation and DetectorsPhysical measurementsParticle tracking detectors (Gaseous detectors)Time projection chambersPattern recognition SystemsFísica -- Mesuramentschemistry.chemical_elementFOS: Physical sciencesTracking (particle physics)01 natural sciences7. Clean energyTECNOLOGIA ELECTRONICAXenonSilicon photomultiplierOpticsCluster analysisDouble beta decayPattern recognition0103 physical sciencesCalibrationReconeixement de formes (Informàtica)Calibratge010306 general physicsInstrumentationImage resolutionMathematical PhysicsDetectors de radiacióPhysicsCalibration and fitting methods010308 nuclear & particles physicsbusiness.industryDetectorCluster findingFísicaInstrumentation and Detectors (physics.ins-det)Double-beta decay detectorsAnàlisi de conglomeratschemistryNuclear countersCalibrationbusiness
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Extraction of the Muon Signals Recorded with the Surface Detector of the Pierre Auger Observatory Using Recurrent Neural Networks

2021

The Pierre Auger Observatory, at present the largest cosmic-ray observatory ever built, is instrumented with a ground array of 1600 water-Cherenkov detectors, known as the Surface Detector (SD). The SD samples the secondary particle content (mostly photons, electrons, positrons and muons) of extensive air showers initiated by cosmic rays with energies ranging from $10^{17}~$eV up to more than $10^{20}~$eV. Measuring the independent contribution of the muon component to the total registered signal is crucial to enhance the capability of the Observatory to estimate the mass of the cosmic rays on an event-by-event basis. However, with the current design of the SD, it is difficult to straightfo…

PhotonPhysics::Instrumentation and DetectorsAstronomyElectron01 natural sciencesHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)mass [cosmic radiation]surface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]photon: cosmic radiationInstrumentationMathematical PhysicsPhysicsAGASAPhysicsSettore FIS/01 - Fisica SperimentaleDetectorcosmic radiation [photon]Astrophysics::Instrumentation and Methods for AstrophysicsMonte Carlo [numerical calculations]electromagnetic [showers]Augerobservatorycosmic radiation [electron]Analysis and statistical methodsnumerical calculations: Monte CarloAnalysis and statistical methodperformancepositron: cosmic radiationatmosphere [showers]Cherenkov detectordata analysis methodAnalysis and statistical methods; Calibration and fitting methods; Cherenkov detectors; Cluster finding; Large detector systems for particle and astroparticle physics; Pattern recognitionCherenkov counter: waterairneural networkAstrophysics::High Energy Astrophysical Phenomena610FOS: Physical sciencesCosmic raycosmic radiation [positron]cosmic radiation: massCalibration and fitting methodNuclear physicsstatistical analysisPattern recognition0103 physical sciencesshowers: electromagneticddc:530ddc:610High Energy Physics010306 general physicsZenithPierre Auger ObservatoryCalibration and fitting methodscosmic radiation [muon]Muonshowers: atmosphere010308 nuclear & particles physicsdetector: surfacehep-exLarge detector systems for particle and astroparticle physicswater [Cherenkov counter]Cherenkov detectorsCluster findingelectron: cosmic radiationRecurrent neural networkmuon: cosmic radiationLarge detector systems for particle and astroparticle physicExperimental High Energy PhysicsHigh Energy Physics::ExperimentRAIOS CÓSMICOSexperimental results
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