Search results for "Length"

showing 10 items of 2188 documents

Operational considerations to improve total ozone measurements with a Microtops II ozone monitor

2012

A Microtops II "ozone monitor" with UV channels centered at 305.5, 312.5, and 320 nm has been used routinely in six experimental campaigns carried out in several geographic locations and seasons, covering latitudes from 35 to 68° N during the last ten years (2001–2011). The total ozone content is retrieved by Microtops II by using different combinations (Channel I, 305.5/312.5 nm; Channel II, 312.5/320 nm; and Channel III, 305.5/312.5/320 nm) of the signals at the three ultraviolet wavelengths. The long-term performance of the total ozone content determination has been studied taking into account the sensitivities to the calibration, airmass, temperature and aerosols. When a calibration was…

Atmospheric ScienceOzoneMeteorologylcsh:TA715-787lcsh:Earthwork. FoundationsOzone monitorMicrotops IITotal ozoneGeofísicamedicine.disease_causelcsh:Environmental engineeringLatitudeRoot mean squarechemistry.chemical_compoundWavelengthAtmosferaUltraviolet solar radiationchemistrySunphotometerCalibrationmedicinelcsh:TA170-171Total column ozoneUltravioletCommunication channel
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Column-integrated aerosol optical properties in Sodankylä (Finland) during the Solar Induced Fluorescence Experiment (SIFLEX-2002).

2006

[1] A study has been made of the column aerosols using solar irradiance extinction measurements at ground level in a boreal region (Sodankyla, Finland) during spring 2002. The aerosol properties have been related to air mass origin. In general, the aerosol levels were observed to be very low, independent of the air mass origin, with an aerosol optical depth (AOD) value at 500 nm of less than 0.09 ± 0.03. Two characteristic patterns were observed depending on whether the air masses originated in the north and west or from the south and east. In the first case (north and west origins) the aerosol load was very small, with very low optical depths in the range 0.03 ± 0.02 to 0.09 ± 0.03 for 500…

Atmospheric ScienceRadiació solarMeteorologySoil ScienceAquatic ScienceOceanographySolar irradianceAtmospheric sciencesGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Air massEarth-Surface ProcessesWater Science and TechnologyAerosolsEcologySpring seasonPaleontologyForestryGeofísicaAerosolGround levelWavelengthGeophysicsBorealSpace and Planetary ScienceExtinction (optical mineralogy)Environmental science
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Surface temperature retrieval from Along Track Scanning Radiometer 2 data: Algorithms and validation

2004

[1] A study has been carried out using MODTRAN 3.5 simulations of the Along Track Scanning Radiometer 2 (ATSR-2) data at 3.7, 11, and 12 μm wavelengths to give a range of algorithms for estimating surface. Making use of the dual-angle feature of the ATSR-2, algorithms based on dual-angle, split-window, and mixed structure have been considered. The coefficients of the algorithms are derived by regression analysis using the MATLAB code. The evaluation of the sensitivity of each algorithm shows that in general, dual-angle algorithms provide smaller errors in the estimation of surface temperature than the split-window algorithms and that the algorithms with water vapor dependence give an improv…

Atmospheric ScienceRadiometerEcologyMODTRANComputer sciencePaleontologySoil ScienceForestryAquatic ScienceOceanographyWavelengthGeophysicsSpace and Planetary ScienceGeochemistry and PetrologyFeature (computer vision)Earth and Planetary Sciences (miscellaneous)TrajectoryRange (statistics)Sensitivity (control systems)AlgorithmWater vaporEarth-Surface ProcessesWater Science and TechnologyRemote sensingJournal of Geophysical Research
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Wavelength dependence of the effective cloud optical depth

2015

This study examines the wavelength dependence of cloud optical depth. To accomplish this task two different wavelength bands of the solar spectrum were considered in the cloud optical depth retrieval which was conducted in Valencia, Spain. The first retrieval used global irradiance measurements in the UVER range taken from a YES-UVB-1 radiometer in combination with multiple scattering model estimates; while the second retrieval was obtained in the Broadband range, with measurements of global solar surface irradiance from a CM6 pyranometer and a multiple scattering model. Whilst the dependence of the cloud optical depth (τ) on the wavelength is small, the best result was displayed by the SBD…

Atmospheric ScienceRadiometerPyranometerbusiness.industryScatteringIrradiancePhysics::OpticsWavelengthGeophysicsOpticsSpace and Planetary ScienceBroadbandRange (statistics)Environmental sciencebusinessOptical depthRemote sensingJournal of Atmospheric and Solar-Terrestrial Physics
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Optical properties of deep glacial ice at the South Pole

2006

We have remotely mapped optical scattering and absorption in glacial ice at the South Pole for wavelengths between 313 and 560 nm and depths between 1100 and 2350 m. We used pulsed and continuous light sources embedded with the AMANDA neutrino telescope, an array of more than six hundred photomultiplier tubes buried deep in the ice. At depths greater than 1300 m, both the scattering coefficient and absorptivity follow vertical variations in concentration of dust impurities, which are seen in ice cores from other Antarctic sites and which track climatological changes. The scattering coefficient varies by a factor of seven, and absorptivity (for wavelengths less than ∼450 nm) varies by a fact…

Atmospheric ScienceSoil ScienceMineralogyAquatic ScienceOceanographyLight scatteringPhysics::GeophysicsIce coreGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Absorption (electromagnetic radiation)Physics::Atmospheric and Oceanic PhysicsEarth-Surface ProcessesWater Science and Technologygeographygeography.geographical_feature_categoryEcologyScatteringPaleontologyForestryGlacierMolar absorptivityWavelengthGeophysicsSpace and Planetary ScienceAttenuation coefficientAstrophysics::Earth and Planetary AstrophysicsGeologyJournal of Geophysical Research
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Extreme, wintertime Saharan dust intrusion in the Iberian Peninsula: Lidar monitoring and evaluation of dust forecast models during the February 2017…

2019

The research leading to these results has received funding from the H2020 program from the European Union (grant agreement no. 654109, 778349) and also from the Spanish Ministry of Industry, Economy and Competitiviness (MINECO, ref. CGL2013-45410-R, CGL2016-81092-R, CGL2017-85344-R, TEC2015-63832-P), the Spanish Ministry of Science, Innovation and Universities (ref. CGL2017-90884-REDT); the CommSensLab "Maria de Maeztu" Unity of Excellence (ref. MDM-2016-0600) financed by the Spanish Agencia Estatal de Investigación. Co-funding was also provided by the European Union through the European Regional Development Fund (ref. POCI-01-0145-FEDER-007690, ALT20-03-0145-FEDER-000004, ALT20-03-0145-FED…

Atmospheric ScienceTeledeteccióPols mineral -- Tesis doctorals010504 meteorology & atmospheric sciencesBackscatterSun-photometer:Energies [Àrees temàtiques de la UPC]Particle optical propertiesForecast skill010501 environmental sciencesMineral dustAtmospheric sciencesExtreme Saharan dust intrusion01 natural sciencesSun photometerModel evaluation0105 earth and related environmental sciencesMulti-wavelength lidarRemote sensingVertical distributionDust forecast modelAERONETAerosolPlumeLidar:Enginyeria de la telecomunicació::Radiocomunicació i exploració electromagnètica::Teledetecció [Àrees temàtiques de la UPC]13. Climate actionEnvironmental scienceDust control
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Saharan dust absorption and refractive index from aircraft-based observations during SAMUM 2006

2009

During the Saharan Mineral Dust Experiment (SAMUM) conducted in summer 2006 in southeast Morocco, the complex refractive index of desert dust was determined from airborne measurements of particle size distributions and aerosol absorption coefficients at three different wavelengths in the blue (467 nm), green (530 nm) and red (660 nm) spectral regions. The vertical structure of the dust layers was analysed by an airborne high spectral resolution lidar (HSRL). The origin of the investigated dust layers was estimated from trajectory analyses, combined with Meteosat 2nd Generation (MSG) scenes and wind field data analyses. The real part n of the dust refractive index was found almost constant w…

Atmospheric Sciencerefractive indexMaterials science010504 meteorology & atmospheric sciencesaerosolAtmosphärische SpurenstoffeMineralogy010501 environmental sciencesMineral dust01 natural sciencesAerosolSAMUMTroposphereWavelengthLidarSpectral resolutionAbsorption (electromagnetic radiation)absorptionRefractive index0105 earth and related environmental sciencesRemote sensingTellus B: Chemical and Physical Meteorology
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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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Compact two-electron wave function for bond dissociation and Van der Waals interactions: A natural amplitude assessment

2014

Electron correlations in molecules can be divided in short range dynamical correlations, long range Van der Waals type interactions and near degeneracy static correlations. In this work we analyze for a one-dimensional model of a two-electron system how these three types of correlations can be incorporated in a simple wave function of restricted functional form consisting of an orbital product multiplied by a single correlation function $f(r_{12})$ depending on the interelectronic distance $r_{12}$. Since the three types of correlations mentioned lead to different signatures in terms of the natural orbital (NO) amplitudes in two-electron systems we make an analysis of the wave function in t…

Atomic Physics (physics.atom-ph)General Physics and AstronomyFOS: Physical sciencesPhysics - Atomic Physicssymbols.namesakeCondensed Matter - Strongly Correlated ElectronsAtomic orbitalQuantum mechanicsPhysics - Chemical PhysicsPhysics::Atomic PhysicsSDG 7 - Affordable and Clean EnergyPhysical and Theoretical ChemistryWave functionAnsatzPhysicsChemical Physics (physics.chem-ph)Quantum Physics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyta114Electronic correlationStrongly Correlated Electrons (cond-mat.str-el)Computational Physics (physics.comp-ph)Diatomic molecule3. Good healthBond lengthAmplitudesymbolsvan der Waals forceQuantum Physics (quant-ph)Physics - Computational Physics
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Observation of a narrow inner-shell orbital transition in atomic erbium at 1299 nm

2021

We report on the observation and coherent excitation of atoms on the narrow inner-shell orbital transition, connecting the erbium ground state $[\mathrm{Xe}] 4f^{12} (^3\text{H}_6)6s^{2}$ to the excited state $[\mathrm{Xe}] 4f^{11}(^4\text{I}_{15/2})^05d (^5\text{D}_{3/2}) 6s^{2} (15/2,3/2)^0_7$. This transition corresponds to a wavelength of 1299 nm and is optically closed. We perform high-resolution spectroscopy to extract the $g_J$-factor of the $1299$-nm state and to determine the frequency shift for four bosonic isotopes. We further demonstrate coherent control of the atomic state and extract a lifetime of 178(19) ms which corresponds to a linewidth of 0.9(1) Hz. The experimental findi…

Atomic Physics (physics.atom-ph)chemistry.chemical_elementFOS: Physical sciences01 natural sciences010305 fluids & plasmasPhysics - Atomic PhysicsErbium[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Polarizability0103 physical sciences010306 general physicsSpectroscopyPhysicsQuantum Physics[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]3. Good healthWavelengthchemistryCoherent controlQuantum Gases (cond-mat.quant-gas)Excited state[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physicsGround stateQuantum Physics (quant-ph)Condensed Matter - Quantum GasesExcitation
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