Search results for "Brightness"

showing 10 items of 162 documents

VLBA polarimetric monitoring of 3C 111

2018

Context. While studies of large samples of jets of active galactic nuclei (AGN) are important in order to establish a global picture, dedicated single-source studies are an invaluable tool for probing crucial processes within jets on parsec scales. These processes involve in particular the formation and geometry of the jet magnetic field as well as the flow itself. Aims. We aim to better understand the dynamics within relativistic magneto-hydrodynamical flows in the extreme environment and close vicinity of supermassive black holes. Methods. We analyze the peculiar radio galaxy 3C 111, for which long-Term polarimetric observations are available. We make use of the high spatial resolution of…

active [Galaxies]Radio galaxyAstrophysics::High Energy Astrophysical PhenomenaeducationFOS: Physical sciencesAstrophysicsgalaxies [Radio continuum]Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio continuum: galaxiesgalaxies: individual: 3C 111Coincident0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsSupermassive black holepolarizationGalaxies: magnetic fields010308 nuclear & particles physicsmagnetic fields [Galaxies]Astronomy and AstrophysicsGalaxies: activePolarization (waves)Astrophysics - Astrophysics of GalaxiesMonitoring programMagnetic fieldTransverse planeindividual: 3C 111 [galaxies]Space and Planetary ScienceGalaxies: jetsBrightness temperatureAstrophysics of Galaxies (astro-ph.GA)jets [Galaxies]
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Inverted Solution Processable OLEDs Using a Metal Oxide as an Electron Injection Contact.

2007

A new type of bottom-emission electroluminescent device is described in which a metal oxide is used as the electron-injecting contact. The preparation of such a device is simple. It consists of the deposition of a thin layer of a metal oxide on top of an indium tin oxide covered glass substrate, followed by the solution processing of the light-emitting layer and subsequently the deposition of a high-workfunction (air-stable) metal anode. This architecture allows for a low-cost electroluminescent device because no rigorous encapsulation is required. Electroluminescence with a high brightness reaching 5700 cd m–2 is observed at voltages as low as 8 V, demonstrating the potential of this new a…

chemistry.chemical_classificationBrightnessMaterials sciencebusiness.industryOxideFísicaPolymerElectroluminescenceCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsIndium tin oxideBiomaterialschemistry.chemical_compoundchemistryElectrochemistryOLEDOptoelectronicsbusinessMaterialsVoltageDiodeAdvanced Functional Materials
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Edges and Endpoints in 21-cm Observations from Resonant Photon Production

2020

Physical review letters 127(1), 011102 (1-7) (2021). doi:10.1103/PhysRevLett.127.011102

dark matter: interactionPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelbrightnesskineticGeneral Physics and AstronomyFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics53001 natural sciencesDark photonHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530010306 general physicsPhysicsphoton: productionCOSMIC cancer databasenew physicsproduction [photon]temperatureHigh Energy Physics - PhenomenologyBrightness temperatureDark Agesspectralinteraction [dark matter]signatureAstrophysics - Cosmology and Nongalactic Astrophysics
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Six-dimensional measurements of trains of high brightness electron bunches

2015

Trains of ultrashort electron pulses with THz repetition rate, so-called comblike beams, are assuming an ever growing interest in plasma-based acceleration. In particle-driven plasma wakefield acceleration (PWFA), a train of driver bunches with separation of the order of plasma wavelength, i.e., 300 μm, resonantly excites a plasma wake, which accelerates a trailing witness bunch, injected at the accelerating phase. Comblike beams have great potentialities in different fields of applications. In particular, radiation sources, such as free-electron lasers and THz radiation, take advantage from the possibility to tailor electron beams modulated both in time and energy, to customize emission ba…

electron beamNuclear and High Energy PhysicsBrightnessPhysics and Astronomy (miscellaneous)Terahertz radiationlaw.inventionacceleratorsOpticslawdiagnosticslcsh:Nuclear and particle physics. Atomic energy. RadioactivityPhysicsbusiness.industrySettore FIS/01 - Fisica Sperimentaleelectron beam diagnostics plasma accelerationSurfaces and InterfacesPlasmaPlasma accelerationLaserSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Bunchesplasma accelerationPhase spaceCathode raylcsh:QC770-798Physics::Accelerator PhysicsbusinessPhysical Review Special Topics - Accelerators and Beams
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SMOS-IC: An Alternative SMOS Soil Moisture and Vegetation Optical Depth Product

2017

© 2017 by the authors. The main goal of the Soil Moisture and Ocean Salinity (SMOS) mission over land surfaces is the production of global maps of soil moisture (SM) and vegetation optical depth (τ) based on multi-angular brightness temperature (TB) measurements at L-band. The operational SMOS Level 2 and Level 3 soil moisture algorithms account for different surface effects, such as vegetation opacity and soil roughness at 4 km resolution, in order to produce global retrievals of SM and τ. In this study, we present an alternative SMOS product that was developed by INRA (Institut National de la Recherche Agronomique) and CESBIO (Centre d'Etudes Spatiales de la BIOsphère). One of the main go…

environmental_sciencesL bandVegetation optical depth010504 meteorology & atmospheric sciencesNDVI[SDV]Life Sciences [q-bio]Science0211 other engineering and technologiesWeather forecasting0207 environmental engineeringSoil science02 engineering and technologycomputer.software_genre01 natural sciencesSMOS; L-band; Level 3; ECMWF; SMOS-IC; soil moisture; vegetation optical depth; MODIS; NDVINormalized Difference Vegetation IndexECMWFvegetation optical depthtempératurehumidité du solluminosity14. Life underwater020701 environmental engineeringWater content021101 geological & geomatics engineeringRemote sensing0105 earth and related environmental sciencessalinité des océansQBiosphereluminositéVegetationAlbedoL-bandSpectroradiometerMODIS13. Climate actionBrightness temperatureProduct (mathematics)General Earth and Planetary SciencesEnvironmental sciencesoil moistureSMOS;L-band;level 3;ECMWF;SMOS-IC;soil moisture;vegetation optical depth;MODIS;NDVISMOS-ICcomputerLevel 3SMOSRemote Sensing
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The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the Intracluster Medium out to $R_{200}$ in Abell 2319

2018

We present the joint analysis of the X-ray and SZ signals in A2319, the galaxy cluster with the highest signal-to-noise ratio in Planck maps and that has been surveyed within our XMM Cluster Outskirts Project (X-COP). We recover the thermodynamical profiles by the geometrical deprojection of the X-ray surface brightness, of the SZ comptonization parameter, and an accurate and robust spectroscopic measurements of the temperature. We resolve the clumpiness of the density to be below 20 per cent demonstrating that most of this clumpiness originates from the ongoing merger and can be associated to large-scale inhomogeneities. This analysis is done in azimuthally averaged radial bins and in eigh…

galaxies: clusters: general ; galaxies: clusters: intracluster medium – X-rays; galaxies: clusters – intergalactic mediumgalaxies: clusters: intracluster medium – X-raysCosmology and Nongalactic Astrophysics (astro-ph.CO)galaxies: clusters: intracluster medium[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionlawIntracluster medium0103 physical sciencesROSATCluster (physics)Surface brightnessTotal pressure010303 astronomy & astrophysicsGalaxy clusterComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgalaxies: clusters – intergalactic medium[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsSettore FIS/05Astronomy and AstrophysicsAstronomy and AstrophysicX-rays: galaxies: clusterGalaxySpace and Planetary Sciencegalaxies: clusters: generalX-rays: galaxies: clustersintergalactic mediumHydrostatic equilibrium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations

2018

Context. Asymmetries in atomic hydrogen (HI) in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project has demonstrated that isolated galaxies show the lowest level of asymmetry in their HI integrated profiles compared to even field galaxies, yet some present significant asymmetries. CIG 96 (NGC 864) is a representative case reaching a 16% level. Aims. Our aim is to investigate the HI asymmetries of the spiral galaxy CIG 96 and what processes have triggered the star-forming regions observed in the XUV pseudo-ring. Methods. We performed deep optical observations at CAHA1.23m, CAHA2.2m and V…

galaxies: spiralHIERARCHICAL SATELLITE ACCRETIONmedia_common.quotation_subjectFOS: Physical sciencesAstrophysicsI.01 natural sciences7. Clean energyAsymmetryAMIGA SAMPLElaw.inventionTelescopelaw0103 physical scienceskinematics and dynamics [galaxies]DARK-MATTER SUBSTRUCTURESurface brightness010303 astronomy & astrophysicsStellar evolutionComputingMilieux_MISCELLANEOUSevolution [galaxies]galaxies: kinematics and dynamicsLOPSIDED SPIRAL GALAXIESmedia_commonindividual: NGC 864 [galaxies]Physicsradio lines: galaxiesSpiral galaxy010308 nuclear & particles physicsgalaxies: individual: NGC864Astronomy and AstrophysicsDISK GALAXIESAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Galaxygalaxies [radio lines]RINGSTIDAL STREAMspiral [galaxies][SDU]Sciences of the Universe [physics]Space and Planetary ScienceGASAstrophysics of Galaxies (astro-ph.GA)structure [galaxies]galaxies: structureDIGITAL SKY SURVEYCirrusGalaxies: Individual: NGC 864galaxies: evolutionAstronomy & astrophysics
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2021

Abstract The spaceborne detection of volcanic ash clouds at infrared wavelengths helps to avoid regions with enhanced volcanic ash concentrations that pose a threat to aviation. Current volcanic ash data retrievals require detailed information on microphysical properties and the refractive index of volcanic ash, which are highly variable. Uncertainties in the latter currently limit the quality of volcanic ash nowcasts. Here, we introduce a novel method to calculate the complex refractive indices of volcanic ashes at wavelengths from 5 to 15 μm from measurements of their individual components based on generic petrological ash compositions. Thereby the refractive indices for volcanic glasses …

geographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesInfraredMineralogy010502 geochemistry & geophysics01 natural sciencesGeophysicsVolcano13. Climate actionGeochemistry and PetrologyBrightness temperatureParticle-size distributionParticlePorosityRefractive indexGeology0105 earth and related environmental sciencesVolcanic ashJournal of Volcanology and Geothermal Research
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Esa's SMOS Mission – Supporting Agricultural Applications

2018

The European Space Agency's (ESA) SMOS mission, in orbit since more than 8 years, carries a passive microwave interferometric radiometer measuring in L-Band and provides accurate global observations of emitted radiation originating from the Earth's surfaces since the atmosphere is almost transparent in this spectral range. In addition, over land the effect of vegetation on the measurements is smaller than for shorter wavelengths. The scientific objectives of the SMOS mission directly respond to the need for global observations of soil moisture and ocean salinity, two key variables used in predictive hydrological, oceanographic and atmospheric models. SMOS observations also provide informati…

geographygeography.geographical_feature_categoryAtmospheric modelsVegetationSnowPhysics::GeophysicsAtmosphereBrightness temperatureOrbit (dynamics)Sea iceEnvironmental scienceAstrophysics::Earth and Planetary AstrophysicsPhysics::Atmospheric and Oceanic PhysicsInterferometric radiometerRemote sensingIGARSS 2018 - 2018 IEEE International Geoscience and Remote Sensing Symposium
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Interactions between silver nanoparticles and fluorescent phytochromes from Deinococcus radiodurans

2017

Poikkitieteelliset sovellukset ovat viime aikoina yleistyneet tieteellisessä tutkimuksessa. Tämä näkyy hyvin esimerkiksi elävän kudoksen kuvantamisen kehittymisessä, jota varten etsitään jatkuvasti parempia biologisia leimoja fysiikan ja kemian keinoin. Tässä tutkielmassa on kehitetty ensimmäinen lähi-infrapuna-alueen fluoresenssileima, joka hyödyntää hopeananopartikkeleja ja fytokromeja. Kompleksi on syntetisoitu itse ja sen rakenne on todennettu optisen spektroskopian, elektroforeesin ja elektronimikroskopian keinoin. Lupaavat fluoresenssiominaisuudet saatiin käyttämällä monomeerisen Deinococcus radiodurans -fytokromin kromoforia sitovaa domeenia (CBDmon). Hopeapartikkelien läsnäollessa C…

lifetimefluorophoreelinaikakemialliset yhdisteetbrightnessfluoresenssiimagingsäteilykvanttisaantokirkkausfluoresenssimikroskopiaplasmonitabsorptioradiationplasmonfluoroforitkuvantaminenquantum yieldabsorptionCBDmon
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