Search results for "Spectral line"

showing 10 items of 1453 documents

Line parameters and shapes of high clusters: R-branch of the nu3 band of CH4 in He mixtures

2002

International audience; The IR absorption spectra of CH4 in pure gas and in mixture with helium were studied in the region of nu3 band at higher J line clusters R(17)-R(22). The frequencies and intensities of rotation-vibration lines were estimated from the experimental spectra at Doppler shape conditions. The line frequencies and intensities were calculated and used for the attribution of overlapped lines in clusters. The calculated line intensities are close to the experimental values. The calculated frequency structure of the higher J manifolds are somewhat wider than the observed one. The shapes of helium-broadened line clusters were compared with those calculated accounting for line mi…

010504 meteorology & atmospheric sciences[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]chemistry.chemical_elementSemiclassical physics01 natural sciencesSpectral linesymbols.namesakeLine parameters[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesRelaxation matrixSpectroscopyMixing (physics)Helium0105 earth and related environmental sciencesLine (formation)PhysicsRadiationIr absorption010304 chemical physicsVibration-rotation spectraLine mixingAtomic and Molecular Physics and OpticschemistrysymbolsAtomic physicsDoppler effectMethane
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A new method for the identification of archaeological soils by their spectral signatures in the vis-NIR region

2020

Abstract This paper introduces a statistical method to identify spectral signatures of buried archaeological remains and distinguish them from spectra of the background soil in the visible to near infrared region. The proposed method is based on the Principal Component Analysis (PCA). The difference between an archaeological spectrum and non-archaeological soil spectra is quantified by a so-called R value. R values larger than 1 indicate that the spectrum represents an archaeological material. The method is successfully applied to samples from five study sites in Italy and Hungary with special conditions. The reflection spectra are taken in a time-efficient way with a field spectrometer. Th…

010506 paleontologyArcheologySpectral signature060102 archaeologySpectrometerNear-infrared spectroscopy06 humanities and the artsCC01 natural sciencesArchaeologyField (geography)Spectral linePrincipal component analysisReflection (physics)0601 history and archaeologySpectral resolutionGeology0105 earth and related environmental sciencesJournal of Archaeological Science: Reports
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Chlorophyll fluorescence emission spectrum inside a leaf

2008

International audience; Chlorophyll a fluorescence can be used as an early stress indicator. Fluorescence is also connected to photosynthesis so it can be proposed for global monitoring of vegetation status from a satellite platform. Nevertheless, the correct interpretation of fluorescence requires accurate physical models. The spectral shape of the leaf fluorescence free of any re-absorption effect plays a key role in the models and is difficult to measure. We present a vegetation fluorescence emission spectrum free of re-absorption based on a combination of measurements and modelling. The suggested spectrum takes into account the photosystem I and II spectra and their relative contributio…

0106 biological sciencesChlorophyllChlorophyll aSpectral shape analysisI REACTION CENTERSSPINACH THYLAKOID MEMBRANES[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]PHOTOSYNTHETIC MEMBRANEPhotosystem I01 natural sciencesSpectral lineHIGHER-PLANTSPROTEIN COMPLEXES03 medical and health scienceschemistry.chemical_compoundmedicineEmission spectrumPhysical and Theoretical ChemistryChlorophyll fluorescenceLIGHT-HARVESTING COMPLEX030304 developmental biologyRemote sensing0303 health sciencesPhotosystem I Protein Complex[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Photosystem II Protein Complexfood and beveragesFluorescencePlant LeavesSpectrometry FluorescenceROOM-TEMPERATUREchemistryPHOTOSYSTEM-I[SDU]Sciences of the Universe [physics]Espectroscòpia de fluorescènciaARABIDOPSIS-THALIANAmedicine.symptomVegetation (pathology)ENERGY-TRANSFER010606 plant biology & botany
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Leaf-Level Spectral Fluorescence Measurements : Comparing Methodologies for Broadleaves and Needles

2019

Successful measurements of chlorophyll fluorescence (ChlF) spectral properties (typically in the wavelength range of 650–850 nm) across plant species, environmental conditions, and stress levels are a first step towards establishing a quantitative link between solar-induced chlorophyll fluorescence (SIF), which can only be measured at discrete ChlF spectral bands, and photosynthetic functionality. Despite its importance and significance, the various methodologies for the estimation of leaf-level ChlF spectral properties have not yet been compared, especially when applied to leaves with complex morphology, such as needles. Here we present, to the best of our knowledge, a first comparison of …

0106 biological sciencesCorrection methodMaterials science010504 meteorology & atmospheric sciencesSciencesun-induced fluorescenceAnalytical chemistryleaf morphology01 natural sciencesSpectral lineFluoWatlingonberryLEAVESChlorophyll fluorescence0105 earth and related environmental sciences4112 Forestryphotosynthesischlorophyll fluorescencesilver birchQSpectral propertiesSpectral bandsOPTICAL-PROPERTIESA FLUORESCENCECANOPY-LEVELFluorescencebaseline correctionRATIO F690/F730Integrating sphereLIGHTPHOTOSYSTEM-IPlant speciesScots pineINDUCED CHLOROPHYLL FLUORESCENCEMINIMIZING MEASUREMENT UNCERTAINTIESREVISED MEASUREMENT METHODOLOGYGeneral Earth and Planetary Sciencesbaseline correction; chlorophyll fluorescence; FluoWat; leaf morphology; lingonberry; photosynthesis; Scots pine; silver birch; sun-induced fluorescence010606 plant biology & botany
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Assessment of UV Biological Spectral Weighting Functions for Phenolic Metabolites and Growth Responses in Silver Birch Seedlings

2009

In research concerning stratospheric ozone depletion, action spectra are used as biological spectral weighting functions (BSWFs) for describing the effects of UV radiation on plant responses. Our aim was to evaluate the appropriateness of six frequently used BSWFs that differ in effectiveness with increasing wavelength. The evaluation of action spectra was based on calculating the effective UV radiation doses according to 1-2) two formulations of the generalized plant action spectrum, 3) a spectrum for ultraviolet induced erythema in human skin, 4) a spectrum for the accumulation of a flavonol in Mesembryanthemum crystallinum, 5) a spectrum for DNA damage in alfalfa seedlings and 6) the pla…

0106 biological sciencesOzoneUltraviolet Raysmedicine.disease_cause01 natural sciencesBiochemistrySpectral line03 medical and health scienceschemistry.chemical_compoundOzoneFlavonolsPhenolsBotanymedicineFood sciencePhysical and Theoretical ChemistryBetula030304 developmental biologyAction spectrumchemistry.chemical_classification0303 health sciencesbiologyMesembryanthemum crystallinumDose-Response Relationship RadiationGeneral Medicinebiology.organism_classificationOzone depletionchemistrySeedlings13. Climate actionChlorophyllUltraviolet010606 plant biology & botanyPhotochemistry and Photobiology
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Full spectra coloration and condition-dependent signaling in a skin-based carotenoid sexual ornament

2020

AbstractCarotenoid-based traits commonly act as condition-dependent signals of quality to both males and females. Such colors are typically quantified using summary metrics (e.g., redness) derived by partitioning measured reflectance spectra into blocks. However, perceived coloration is a product of the whole spectrum. Recently, new methods have quantified a range of environmental factors and their impact on reflection data at narrow wavebands across the whole spectrum. Using this approach, we modeled the reflectance of red integumentary eye combs displayed by male black grouse (Lyrurus tetrix) as a function of ornament size and variables related to male quality. We investigated the strengt…

0106 biological scienceschemistry.chemical_classificationC300 ZoologybiologyC182 EvolutionC120 Behavioural BiologyBlack grousebiology.organism_classification010603 evolutionary biology01 natural sciencesReflectivitySpectral line010605 ornithologychemistryAnimal Science and ZoologyBiological systemCarotenoidCondition dependentEcology Evolution Behavior and SystematicsBehavioral Ecology
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Multiplicity dependence of the average transverse momentum in pp, p–Pb, and Pb–Pb collisions at the LHC

2013

The average transverse momentum $\langle p_{\rm T}\rangle$ versus the charged-particle multiplicity $N_{\rm ch}$ was measured in p-Pb collisions at a collision energy per nucleon-nucleon pair $\sqrt{s_{\rm NN}}=5.02$ TeV and in pp collisions at collision energies of $\sqrt{s}=0.9$, 2.76, and 7 TeV in the kinematic range $0.15<p_{\rm T}<10.0$ GeV/$c$ and $|\eta|<0.3$ with the ALICE apparatus at the LHC. These data are compared to results in Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76$ TeV at similar charged-particle multiplicities. In pp and p-Pb collisions, a strong increase of $\langle p_{\rm T}\rangle$ with $N_{\rm ch}$ is observed, which is much stronger than that measured in Pb-Pb colli…

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Multiplicity dependencePROTON-PROTON COLLISIONSPb-Pbpp01 natural sciencesSpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEMultiplicity dependence; transverse momentum; pp; p–Pb; and Pb–Pb collisionsPions[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]multiplicityNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentALICE experiment; Transverse momentum and particle multiplicity; p-p; p-Pb and Pb-Pb collisionsPhysicsLarge Hadron ColliderPhysicsand Pb–Pb collisionsSpectraCharged particleheavy ion:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]PRIRODNE ZNANOSTI. Fizika.:Nuclear and elementary particle physics: 431 [VDP]CHARGED-PARTICLESRoot-S=0.9Transverse momentum7 TEVParticle Physics - ExperimentParticle physicsNuclear and High Energy Physicsp–PbAstrophysics::High Energy Astrophysical PhenomenaVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431FOS: Physical sciencestransverse momentum[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]p-pNuclear physicsPion0103 physical sciencesNuclear Physics - ExperimentTransverse momentum and particle multiplicity010306 general physicsLONG-RANGEp-PbVDP::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431ta114010308 nuclear & particles physicsPROTON-PROTON COLLISIONS; CHARGED-PARTICLES; 7 TEV; ANGULAR-CORRELATIONS; LONG-RANGEHigh Energy Physics::Phenomenology:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]ALICE experimentKaonsMultiplicity (mathematics)Collisionmultiplicity; transverse momentum; pp; p-Pb; Pb-Pb; heavy ion; ALICENATURAL SCIENCES. Physics.ANGULAR-CORRELATIONSHeavy ionHigh Energy Physics::ExperimentPROTON-PROTON COLLISIONS; CHARGED-PARTICLES; 7 TEV; ANGULAR-CORRELATIONS; LONG-RANGE; ROOT-S=0.9; MODEL; SPECTRA; PIONS; KAONSModelp-Pb and Pb-Pb collisions
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Energy dependence of the transverse momentum distributions of charged particles in pp collisions measured by ALICE

2013

Differential cross sections of charged particles in inelastic pp collisions as a function of $p_{\rm T}$ have been measured at $\sqrt{s}=$ 0.9, 2.76 and 7 TeV at the LHC. The $p_{\rm T}$ spectra are compared to NLO-pQCD calculations. Though the differential cross section for an individual $\sqrt{s}$ cannot be described by NLO-pQCD, the relative increase of cross section with $\sqrt{s}$ is in agreement with NLO-pQCD. Based on these measurements and observations, procedures are discussed to construct pp reference spectra at $\sqrt{s} =$ 2.76 and 5.02 TeV up to $p_{\rm T}$ = 50 GeV/$c$ as required for the calculation of the nuclear modification factor in nucleus-nucleus and proton-nucleus coll…

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Physics and Astronomy (miscellaneous)heavy ion collisionsNuclear Theory01 natural sciences7. Clean energySpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)pp collisionALICEpp collisions; transverse momentum; ALICE[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)transverse momentum distributionNuclear ExperimentNuclear ExperimentPhysicsLarge Hadron Collidertransverse momentum; pp; ALICE; charged particlesPhysicsCharged particle3. Good health:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]:Nuclear and elementary particle physics: 431 [VDP]Transverse momentumLhcDiffractionpp collisionsParticle Physics - ExperimentRegular Article - Experimental PhysicsVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431particle productionFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]transverse momentumtransverse momentum distribution; PP COLLISIONSNuclear physicsRoot-S(Nn)=2.76 TevCross section (physics)0103 physical sciencesNuclear Physics - ExperimentPb-Pb Collisions010306 general physicsEngineering (miscellaneous)SuppressionALICE experiment; particle production; heavy ion collisionsVDP::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTransverse momentum distributions:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]ALICE experimentFunction (mathematics)Proton-Proton Collisionsp-p collisionHigh Energy Physics::ExperimentALICE (propellant)Energy (signal processing)
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

2009

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming ντ may interact in the Earth's crust and produce a τ lepton by means of charged-current interactions. The τ lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by τ decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is de…

ACTIVE GALACTIC NUCLEIASTROPHYSICS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsActive galactic nucleusPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayPROPAGATIONAstrophysics7. Clean energy01 natural sciencesLeptonSpectral lineSettore FIS/04 - Fisica Nucleare e SubnucleareAugerSEARCHTau neutrino0103 physical sciencesTau neutrinoOSCILLATIONS010306 general physicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSPierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaultrahigh energy cosmic rays ; tau neutrinos ; Pierre Auger ObservatoryDiffuse fluxPierre Auger ObservatoryPERFORMANCECOSMIC-RAYScosmic radiation13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaLeptonPhysical Review D
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H-He collision-induced satellite in the Lyman alpha profile of DBA white dwarf stars

2020

The spectra of helium-dominated white dwarf stars with hydrogen in their atmosphere present a distinctive broad feature centered around 1160~\AA\/ in the blue wing of the Lyman-$\alpha$ line. It is extremely apparent in WD 1425+540 recently observed with HST COS. With new theoretical line profiles based on ab initio atomic interaction potentials we show that this feature is a signature of a collision-induced satellite due to an asymptotically forbidden transition. This quasi-molecular spectral satellite is crucial to understanding the asymmetrical shape of Lyman-$\alpha$ seen in this and other white dwarf spectra. Our previous work predicting this absorption feature was limited by molecular…

ATOMIC DATALINE: PROFILEAb initiochemistry.chemical_elementBASIS-SETLINEEXCITED-STATEAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linePhysics - Atomic PhysicsWHITE DWARF0103 physical sciencesRadiative transferABSORPTIONAstrophysics::Solar and Stellar AstrophysicsAB-INITIO CALCULATIONPhysics::Atomic PhysicsELECTRONIC-TRANSITION MOMENT010306 general physicsSTARS: ATMOSPHERE010303 astronomy & astrophysicsHeliumLine (formation)POTENTIAL-ENERGY CURVEPhysics[PHYS]Physics [physics]BALMER-ALPHAWhite dwarfAstronomy and AstrophysicsMOLECULAR DATAPotential energyDipolechemistryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceATOMIC PROCESSSHAPE[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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