Search results for "Instrumentation"

showing 10 items of 4914 documents

Intercomparison of spectroradiometers and Sun photometers for the determination of the aerosol optical depth during the VELETA-2002 field campaign

2006

In July 2002 the VELETA-2002 field campaign was held in Sierra Nevada (Granada) in the south of Spain. The main objectives of this field campaign were the study of the influence of elevation and atmospheric aerosols on measured UV radiation. In the first stage of the field campaign, a common calibration and intercomparison between Licor-1800 spectroradiometers and Cimel-318 Sun photometers was performed in order to assess the quality of the measurements from the whole campaign. The intercomparison of the Licor spectroradiometers showed, for both direct and global irradiances, that when the comparisons were restricted to the visible part of the spectrum the deviations were within the instrum…

Atmospheric ScienceMeteorologyInstrumentationIrradianceRadiometersSoil ScienceAeronetNetworkAODAquatic ScienceOceanographyUV radiationlaw.inventionAbsorptionGeochemistry and PetrologylawEarth and Planetary Sciences (miscellaneous)CalibrationUrbanDirect solar irradianceField campaignEarth-Surface ProcessesWater Science and TechnologyRemote sensingSpectroradiometersEcologyElevationPaleontologyForestryPhotometerSize distributionAerosolBandGeophysicsSpectroradiometerSpace and Planetary ScienceCalibrationEnvironmental scienceSun photometersModel
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Comparison of Different Techniques for the Measurement of Precipitation in Tropical Montane Rain Forest Regions

2007

Abstract Characteristics of different precipitation measurements in a tropical mountain valley in southern Ecuador are compared in this study to determine potential errors. The instruments are used for different ecological purposes like erosion studies, through fall measurements, investigation of atmospheric chemistry, and modeling of area rainfall distribution. Five recording devices (two precipitation radars, an electro-optical present weather sensor, and two tipping buckets) and three totaling gauges were operated in parallel at a designated site. Data were taken between 1998 and 2003 with different temporal resolution and different operational periods. The general agreement between the …

Atmospheric ScienceMeteorologyRemote sensing (archaeology)InstrumentationTemporal resolutionAtmospheric chemistryErosionRange (statistics)Environmental scienceOcean EngineeringRainforestPrecipitationAtmospheric sciencesJournal of Atmospheric and Oceanic Technology
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A Precise Photometric Ratio via Laser Excitation of the Sodium Layer II: Two-photon Excitation Using Lasers Detuned from 589.16 nm and 819.71 nm Reso…

2020

This article is the second in a pair of articles on the topic of the generation of a two-color artificial star (which we term a "laser photometric ratio star," or LPRS) of de-excitation light from neutral sodium atoms in the mesosphere, for use in precision telescopic measurements in astronomy and atmospheric physics, and more specifically for the calibration of measurements of dark energy using type Ia supernovae. The two techniques respectively described in both this and the previous article would each generate an LPRS with a precisely 1:1 ratio of yellow (589/590 nm) photons to near-infrared (819/820 nm) photons produced in the mesosphere. Both techniques would provide novel mechanisms f…

Atmospheric physicsPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicslaw.inventionTelescopetechniques: photometricsymbols.namesakeOpticslawAstrophysics::Solar and Stellar AstrophysicsRayleigh scatteringdark energyInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsPhysicsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsSodium layerAstronomy and AstrophysicstelescopesPolarization (waves)Laser[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]instrumentation: miscellaneousWavelengthphotometric methods[SDU]Sciences of the Universe [physics]Space and Planetary SciencesymbolsAstrophysics::Earth and Planetary Astrophysicsmethods: observationalbusinesstechniquesAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Characterization of methyl orange and its photocatalytic degradation products by HPLC/UV–VIS diode array and atmospheric pressure ionization quadrupo…

2002

Abstract HPLC/UV–VIS diode array and HPLC/MS techniques were successfully applied to the analysis of sulfonated molecules present in samples coming from the photocatalytic degradation of the azo dye indicator, methyl orange. The substrate was chosen as a simple model for the study of reactions involving the more complex commercial products used for the dyeing of textile fibers. Unexpected MS fragmentation path was observed, due to the very stable methyl orange molecular structure. The chromatographic information were combined with the obtained MS, MS/MS data and the UV–VIS diode array spectra and allowed to rationalize the molecular structures attributable to the various degradation product…

Atmospheric pressureChemistryAnalytical chemistrySubstrate (chemistry)Condensed Matter PhysicsMass spectrometryHigh-performance liquid chromatographychemistry.chemical_compoundIonizationMethyl orangePhysical and Theoretical ChemistryQuadrupole ion trapDyeingInstrumentationSpectroscopyInternational Journal of Mass Spectrometry
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Beating Darwin-Bragg losses in lab-based ultrafast x-ray experiments

2017

The use of low temperature thermal detectors for avoiding Darwin-Bragg losses in lab-based ultrafast experiments has begun. An outline of the background of this new development is offered, showing the relevant history and initiative taken by this work. (C) 2017 Author(s). Funding Agencies|Knut and Alice Wallenberg Foundation; ERC [226136]; Finnish Funding Agency for Technology and Innovation TEKES; Academy of Finland [260880]; NIST Innovations in Measurement Science program; DOE Office of Basic Energy Sciences

Atom and Molecular Physics and OpticsPhysics::OpticsNanotechnology02 engineering and technology01 natural sciencesThermal detectorOpticsDarwin-Bragg loss0103 physical scienceslcsh:QD901-999010306 general physicsInstrumentationSpectroscopyPhysicsRadiationbusiness.industryArticleskidetiede021001 nanoscience & nanotechnologyCondensed Matter Physicsultrafast x-raysUltrafast Structural Dynamics—A Tribute to Ahmed H. ZewailDarwin (spacecraft)Atom- och molekylfysik och optiklcsh:Crystallography0210 nano-technologybusinessUltrashort pulseStructural Dynamics
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BASE-STEP: A transportable antiproton reservoir for fundamental interaction studies

2023

Currently, the only worldwide source of low-energy antiprotons is the AD/ELENA facility located at CERN. To date, all precision measurements on single antiprotons have been conducted at this facility and provide stringent tests of the fundamental interactions and their symmetries. However, the magnetic field fluctuations from the facility operation limit the precision of upcoming measurements. To overcome this limitation, we have designed the transportable antiproton trap system BASE-STEP to relocate antiprotons to laboratories with a calm magnetic environment. We anticipate that the transportable antiproton trap will facilitate enhanced tests of CPT invariance with antiprotons, and provide…

Atomic Physics (physics.atom-ph)FOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)
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Narrow-band pulsed electron source based on near-threshold photoionization of Cs in a magneto-optical trap

2019

The newly developed method of time-of-flight (ToF) momentum microscopy was used to analyse the cold electron emission from a Cs 3D magneto-optical trap (MOT). Three-step resonant photoionization was implemented via two intermediate states (6P3/2 pumped with 852 nm laser and 7S1/2 with 1470 nm) and a tuneable femtosecond Ti:sapphire laser for the final ionization step. The magnetic field of the MOT is switched off during the photoionization step. The natural bandwidth of the fs-laser is reduced to 4 meV using optical spectral filters. Precise tuning of the photon energy makes it possible to observe the transition regime between direct photoemission into the open continuum and field induced i…

Atomic Physics (physics.atom-ph)FOS: Physical sciencesPhysics::OpticsElectronPhotoionizationPhoton energy01 natural sciencesPhysics - Atomic Physics010305 fluids & plasmaslaw.inventionsymbols.namesake[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]lawIonizationMagneto-optical trap0103 physical sciencesPhysics::Atomic Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPhysicsCondensed Matter - Materials Science[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Materials Science (cond-mat.mtrl-sci)Laser3. Good healthFemtosecondRydberg formulasymbolsAtomic physics
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Searching for axion stars and $Q$-balls with a terrestrial magnetometer network

2018

Light (pseudo-)scalar fields are promising candidates to be the dark matter in the Universe. Under certain initial conditions in the early Universe and/or with certain types of self-interactions, they can form compact dark-matter objects such as axion stars or Q-balls. Direct encounters with such objects can be searched for by using a global network of atomic magnetometers. It is shown that for a range of masses and radii not ruled out by existing observations, the terrestrial encounter rate with axion stars or Q-balls can be sufficiently high (at least once per year) for a detection. Furthermore, it is shown that a global network of atomic magnetometers is sufficiently sensitive to pseudos…

Atomic Physics (physics.atom-ph)media_common.quotation_subjectScalar (mathematics)Dark matterFOS: Physical sciencesAstrophysicsParameter space01 natural sciencesPhysics - Atomic PhysicsQ-ballHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)media_commonPhysicsQuantum Physics010308 nuclear & particles physicsAstronomyUniversePseudoscalarStarsHigh Energy Physics - PhenomenologyAstrophysics - Instrumentation and Methods for AstrophysicsQuantum Physics (quant-ph)
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Deconvolution procedure of the UV-vis spectra. A powerful tool for the estimation of the binding of a model drug to specific solubilisation loci of b…

2015

UV-vis-spectra evolution of Nile Red loaded into Tween 20 micelles with pH and [Tween 20] have been analysed in a non-conventional manner by exploiting the deconvolution method. The number of buried sub-bands has been found to depend on both pH and bio-surfactant concentration, whose positions have been associated to Nile Red confined in aqueous solution and in the three micellar solubilisation sites. For the first time, by using an extended classical two-pseudo-phases-model, the robust treatment of the spectrophotometric data allows the estimation of Nile Red binding constant to the available loci. Hosting capability towards Nile Red is exalted by the pH enhancement. Comparison between bin…

Atomic and Molecular Physics and OpticOxazineAnalytical chemistrySpecific solubilisation lociTween 20PolysorbatesDeconvolutionNile RedMicelleSpectral lineUV-vis spectraAnalytical ChemistrySurface-Active Agentchemistry.chemical_compoundSurface-Active AgentsUltraviolet visible spectroscopycmc; Deconvolution; Nile Red; Specific solubilisation loci; Tween 20; UV-vis spectra; Binding Sites; Oxazines; Polysorbates; Solubility; Spectrophotometry Ultraviolet; Surface-Active Agents; Micelles; Instrumentation; Atomic and Molecular Physics and Optics; Analytical Chemistry; Spectroscopy; Medicine (all)Pulmonary surfactantOxazinesInstrumentationSpectroscopyMicellesAqueous solutionBinding SitesChemistryMedicine (all)Nile redBinding SiteBinding constantAtomic and Molecular Physics and OpticsPolysorbateSolubilitycmcSpectrophotometry UltravioletDeconvolutionMicelle
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The Athena X-ray Integral Field Unit (X-IFU)

2018

著者人数: 23名

Atomic and Molecular Physics and Optic[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Condensed Matter Physics01 natural sciencesAtomic and Molecular Physics and OpticsImaging spectroscopy[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010309 opticsX-ray astronomyMicrocalorimeter0103 physical sciencesGeneral Materials ScienceMaterials Science (all)010306 general physicsJournal of Low Temperature Physics
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