Search results for " Resolution"

showing 10 items of 1159 documents

On the high resolution spectroscopy and intramolecular potential function of SO2

2009

Abstract Two weak stretching bands, ν 1  + 3 ν 3 and 3 ν 1  +  ν 3 , of the sulfur dioxide molecule have been recorded at high resolution and analyzed for the first time with using a Fourier transform Bruker IFS-120 HR interferometer. About 1000 transitions with J max .  = 51, K a max . = 16 , and 900 transitions with J max .  = 53, K a max . = 16 have been assigned to the bands ν 1  + 3 ν 3 and 3 ν 1  +  ν 3 , respectively. Analysis of the recorded spectra was made using the model of isolated vibrational states. Parameters obtained from the fit reproduce the initial experimental ro-vibrational energies with the rms deviation of 0.0006 and 0.0012 cm −1 for the bands, 3 ν 1  +  ν 3 and ν 1  …

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Analytical chemistryHigh resolution02 engineering and technology01 natural sciencesSpectral linesymbols.namesakeNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]High-resolution spectra0103 physical sciencesMoleculePhysical and Theoretical ChemistrySpectroscopySpectroscopyPhysics010304 chemical physicsPotential functionFunction (mathematics)Spectroscopic parameters021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsInterferometryFourier transformSulfur dioxideIntramolecular forcesymbols0210 nano-technology
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High resolution study of the six lowest doubly excited vibrational states of PH2D

2005

Abstract The five lowest doubly excited deformational vibrational bands ν 4  +  ν 6 , 2 ν 6 , ν 3  +  ν 4 , ν 3  +  ν 6 , and 2 ν 3 of PH 2 D have been recorded for the first time using a Bruker 120 HR interferometer with a resolution 0.0033 cm −1 and analysed. Some transitions belonging to a very weak band 2 ν 4 have been also assigned. From the fit 24 and 86, respectively, diagonal and resonance interaction parameters were obtained which reproduce 1089 upper energy levels obtained from more than 4600 assigned transitions with the rms deviation of 0.00059 cm −1 .

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]InfraredHigh resolution010402 general chemistry01 natural sciencesNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesVibrational bandsHigh resolutionPhysical and Theoretical ChemistryInfrared spectrumSpectroscopy[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Physics010304 chemical physicsResolution (electron density)ResonanceSpectroscopic parametersPH2D moleculeAtomic and Molecular Physics and Optics0104 chemical sciences[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]FTIRExcited stateAtomic physics
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Analysis of highly excited 'hot' bands in the SO2 molecule: ν2 + 3ν3 - ν2 and 2ν1 + ν2 + ν3 - ν2

2010

International audience; We set up a variational procedure of assignments of transitions and we applied it to the analysis very weak 'hot' bands, v(2) + 3v(3) - v(2) and 2v(1) + v(2) + v(3) - v(2), of the SO2 molecule. As the first step of the study, the 'cold' bands, 3v(3) and 2v(1) + v(3), are re-analysed and transitions belonging to those bands are assigned up to the values of quantum numbers J(max.) = 60, K-a(max.) = 19, and J(max.) = 69, K-a(max.) = 20 for the bands 3v(3) and 2v(1) + v(3), respectively. After 'cleaning' the experimental spectrum from transitions belonging to the 3v(3) and 2v(1) + v(3) bands, a variational procedure was used that allowed us to assign 230 and 115 transiti…

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]high-resolution spectraHIGH-RESOLUTION ANALYSISBiophysics02 engineering and technology01 natural sciences[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesMoleculespectroscopic parametersHigh resolution spectraPhysical and Theoretical ChemistrySpectroscopyLASER SPECTROSCOPYMolecular BiologyHigh resolution analysis010304 chemical physicsChemistryCOMBINATION BAND021001 nanoscience & nanotechnologyCondensed Matter PhysicsQuantum numberNU-3 BANDINTENSITIESSULFUR-DIOXIDEExcited stateLINE POSITIONSVIBRATIONAL-STATESsulphur dioxideEQUILIBRIUM ROTATIONAL-CONSTANTSAtomic physics0210 nano-technologySUBMILLIMETER-WAVE SPECTRUM
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Identifying clouds over the Pierre Auger Observatory using infrared satellite data

2013

We describe a new method of identifying night-time clouds over the Pierre Auger Observatory using infrared data from the Imager instruments on the GOES-12 and GOES-13 satellites. We compare cloud. identifications resulting from our method to those obtained by the Central Laser Facility of the Auger Observatory. Using our new method we can now develop cloud probability maps for the 3000 km(2) of the Pierre Auger Observatory twice per hour with a spatial resolution of similar to 2.4 km by similar to 5.5 km. Our method could also be applied to monitor cloud cover for other ground-based observatories and for space-based observatories. (C) 2013 Elsevier B.V. All rights reserved.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Atmospheric MonitoringSatellitesInfraredAstronomyCloud coverFOS: Physical sciencesAtmospheric monitoring01 natural sciencesCiencias de la Tierra y relacionadas con el Medio AmbienteAuger//purl.org/becyt/ford/1 [https]//purl.org/becyt/ford/1.5 [https]ObservatoryClouds0103 physical sciencesExtensive air showers010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Image resolutionCiencias ExactasPhysicsPierre Auger ObservatoryUHE Cosmic Rays atmosphere010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomyPierre Auger ObservatoryAstronomy and AstrophysicsUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]INFRAVERMELHOExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGPierre Auger observatoryultra-high energy cosmic rays; Pierre Auger Observatory; extensive air showers; atmospheric monitoring; clouds; satellitesFísica nuclearSatelliteCentral Laser FacilityExtensive Air ShowersAstrophysics - Instrumentation and Methods for AstrophysicsMeteorología y Ciencias AtmosféricasSYSTEMCIENCIAS NATURALES Y EXACTASAstroparticle Physics
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LOFT: the Large Observatory For X-ray Timing

2012

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is currently planned for between 2022 and 2024. LOFT is designed to exploit the diagnostics of rapid X-ray flux and spectral variability that directly probe the motion of matter down to distances very close to black holes and neutron stars, as well as the physical state of ultra-dense matter. These primary science goals will be addressed by a payload composed of a Large Area Detector (LAD) and a Wide Field Monitor (WFM). The LAD is a collimated (<1 degree field of view) experiment operating in the energy range 2-50 keV,…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]VisionX-ray timingAstronomySPIE ProceedingsObservatoriesX-ray timing X-ray spectroscopy X-ray imaging compact objectsSilicon Drift ChambersFOS: Physical sciencesddc:500.2X-ray missionsSpace (mathematics)Astrophysics01 natural sciences7. Clean energySettore FIS/05 - Astronomia E AstrofisicaX-rays0103 physical sciencesElectronicOptical and Magnetic MaterialsInstrumentation (computer programming)Electrical and Electronic EngineeringAerospace engineeringDiagnosticsCompact objects010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsSpatial resolutionsezeleSensors010308 nuclear & particles physicsbusiness.industryApplied MathematicsX-ray imagingSilicon Drift ChamberComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicsCompact objects; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineering[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]X-ray spectroscopySilicon Drift Chambers; X-ray missionsInstrumentation and Methods for AstrophysicsAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Infrared Spectroscopy of Ruthenium Tetroxide and High-resolution analysis of the v3 band

2015

International audience

[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th][PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th][PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]Isotopic shiftRuthenium TetroxideHigh resolution FTIR spectroscopy[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]ComputingMilieux_MISCELLANEOUSSimulation
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On-line measurements of RuO$_4$ during a PWR severe accident

2015

International audience; After the Fukushima accident, it became essential to have a way to monitor in real time the evolution of a nuclear reactor during a severe accident, in order to react efficiently and minimize the industrial, ecological and health consequences of the accident. Among gaseous fission products, the tetroxide of ruthenium RuO$_4$ is of prime importance since it has a significant radiological impact. Ruthenium is a low volatile fission product but in case of the rupture of the lower head by the molten corium, the air entering into the vessel oxidizes Ru into gaseous RuO$_4$, which is not trapped by the Filtered Containment Venting Systems. To monitor the presence of RuO$_4…

[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th][PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th][PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]TetroxideHigh resolution FTIR spectroscopyFission product[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Severe accidentRuthenium
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Spatio-Temporal Beam Mapping for Studying Nonlinear Dynamics in Graded Index Multimode Fiber

2020

We experimentally demonstrate high-resolution mapping of the spatio-temporal dynamics of the beam cleaning process in graded index multimode fibers. This high-resolution characterization reveals the time-dependent nature of the beam self-cleaning process.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics]optical fibersOptical fiberMaterials scienceKerr effect02 engineering and technology01 natural scienceslaw.invention010309 opticssymbols.namesakeOpticsKerr effectlaw0103 physical sciencesComputingMilieux_MISCELLANEOUS[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Multi-mode optical fiberbusiness.industry021001 nanoscience & nanotechnologyCharacterization (materials science)beam cleaningNonlinear systembeam cleaning; optical fibers; Kerr effectTemporal resolutionsymbolsPhysics::Accelerator Physics0210 nano-technologybusinessRaman scatteringBeam (structure)
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High resolution study of the SO2 infrared spectra: calculation scheme for assignment of transitions in very weak ro-vibrational bands.

2009

[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph][ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]High ResolutionMolecular Spectra[PHYS.QPHY] Physics [physics]/Quantum Physics [quant-ph]
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Mapping intra-plot topsoil diversity of Burgundy vineyards (Aloxe- Corton, France) from very high spatial resolution (VHSR) images

2012

International audience; In this work, we present a method based on very high spatial resolution (VHSR) aerial images acquired in the visible domain and that map soil surface diversity at the hillslope scale with a spatial resolution of a few centimeters. This method combines aerial VHSR image classification with local soil sampling. Principal component analysis (PCA) and non-supervised classification was performed on image characteristics to define soil surface characteristic classes (SSC). Then soil surface mapping was combined with soil surface descriptions and soil profiles to define soil types by physical and chemical characteristics.

[SDE] Environmental Sciences[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistory[SDE.ES]Environmental Sciences/Environmental and Societysoil surface characteristics[ SDE ] Environmental SciencesvineyardsSoil mapping[ SHS.ARCHEO ] Humanities and Social Sciences/Archaeology and Prehistory[SDE]Environmental Sciencesunmanned aerial vehicle[SDE.ES] Environmental Sciences/Environmental and Societyvery high spatial resolution[ SDE.ES ] Environmental Sciences/Environmental and Society
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