Search results for "SCOPE"

showing 10 items of 2420 documents

Multiple accelerated particle populations in the Cygnus Loop with Fermi-LAT

2021

The Cygnus Loop (G74.0-8.5) is a very well-known nearby supernova remnant (SNR) in our Galaxy. Thanks to its large size, brightness, and angular offset from the Galactic plane, it has been studied in detail from radio to $\gamma$-ray emission. The $\gamma$ -rays probe the populations of energetic particles and their acceleration mechanisms at low shock speeds. We present an analysis of the $\gamma$-ray emission detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope over 11 years in the region of the Cygnus Loop. We performed detailed morphological and spectral studies of the $\gamma$-ray emission toward the remnant from 100 MeV to 100 GeV and compared it with X-ra…

Astrophysics::High Energy Astrophysical Phenomenabrightnesscosmic radiation: energyFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeV01 natural sciencesGLASTthermalX-raycosmic raysSpitzer Space Telescope0103 physical sciencesultravioletsupernovaRadiative transferopticalcloudcosmic radiation: acceleration010306 general physicsSupernova remnant010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsacceleration of particlesISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cygnus LoopAstronomy and Astrophysicsshock wavesGalactic planeGalaxy13. Climate actionSpace and Planetary Sciencegamma raystatisticsspectralgalaxyAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
researchProduct

The 2-μm spectroscopy of Huygens probe landing site on Titan with Very Large Telescope/Nasmyth Adaptive Optics System Near-Infrared Imager and Spectr…

2007

[1] Several ground-based telescopes followed the event of the Huygens probe descent through Titan's atmosphere (14 January 2005). We used the Nasmyth Adaptive Optics System Near-Infrared Imager and Spectrograph (NACO) adaptive optics system at the UT-4 of the Very Large Telescope in Chile to perform both spectroscopic and imaging measurements of Titan. We present here a selected sample of the spectra we acquired on 16 January 2005 in the K band between 2.03 and 2.40 μm. Our spectra include the Huygens landing site and surrounding dark and bright areas. We apply a radiative transfer code using new methane absorption coefficients calculated in the 2-μm region. The analysis of the data yields …

Atmospheric Science010504 meteorology & atmospheric sciencesSoil ScienceAquatic ScienceOceanography01 natural sciencesSpectral lineadaptive opticssymbols.namesakeOpticsGeochemistry and Petrology0103 physical sciencesEarth and Planetary Sciences (miscellaneous)Radiative transfersurfaceSpectroscopyAdaptive optics010303 astronomy & astrophysicsSpectrograph0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and TechnologyPhysicsVery Large TelescopeEcology[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]business.industryNear-infrared spectroscopyPaleontologyForestryhaze[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Geophysics13. Climate actionSpace and Planetary Scienceradiative transferHuygenssymbolsbusinessTitan (rocket family)Titan
researchProduct

Environmental scanning electron microscopy (ESEM) as a new technique to determine the ice nucleation capability of individual atmospheric aerosol par…

2007

Abstract Heterogeneous ice nucleation on synthetic silver iodide, natural kaolinite and montmorillonite particles via condensation, freezing and deposition modes was studied by environmental scanning electron microscopy (ESEM) in the temperature range of 250–270 K. By increasing the H2O pressure in the sample chamber at constant temperature, ice formation can be studied in situ and can be related to the chemical composition of the particles that can be determined simultaneously. For silver iodide and kaolinite, supersaturation values of first ice formation are in good agreement (1–2% absolute) with diffusion chamber experiments. For both substances, threshold temperatures for the condensati…

Atmospheric ScienceIce cloudSupersaturationIce crystalsChemistryAnalytical chemistrySilver iodideCloud physicsMineralogychemistry.chemical_compoundIce nucleusDeposition (phase transition)Environmental scanning electron microscopeGeneral Environmental ScienceAtmospheric Environment
researchProduct

Pore-space characterization of an altered tonalite by X-ray computed microtomography and the14C-labeled-polymethylmethacrylate method

2012

[1] The structure of geological materials strongly affects migration processes that take place in them and are also important in their weathering and alteration processes. Further information of that structure will also be important for many applications that involve geological materials. The emphasis of this study was thus to characterize the pore structure and porosity of altered tonalite by combining different measuring techniques: X-ray tomography, the14C-polymethylmethacrylate method, electron microscopy, and argon pycnometry. Intragranular porosities were determined using chemical staining of rock surfaces. Three-dimensional distributions of minerals and porosities were evaluated with…

Atmospheric ScienceMaterials scienceScanning electron microscope0207 environmental engineeringSoil ScienceMineralogy02 engineering and technologyAquatic Science010502 geochemistry & geophysicsOceanography01 natural sciencesTexture (geology)Geochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Diffusion (business)020701 environmental engineeringPorosity0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and TechnologyEcologyPaleontologyForestryMicrostructureCharacterization (materials science)GeophysicsSpace and Planetary ScienceGas pycnometerPorous mediumJournal of Geophysical Research: Solid Earth
researchProduct

2017

Abstract. Eleven particle samples collected in the polar stratosphere during SOLVE (SAGE III Ozone loss and validation experiment) from January until March 2000 were characterized in detail by high-resolution transmission and scanning electron microscopy (TEM/SEM) combined with energy-dispersive X-ray microanalysis. A total of 4202 particles (TEM  =  3872; SEM  =  330) were analyzed from these samples, which were collected mostly inside the polar vortex in the altitude range between 17.3 and 19.9 km. Particles that were volatile in the microscope beams contained ammonium sulfates and hydrogen sulfates and dominated the samples. Some particles with diameters ranging from 20 to 830 nm were re…

Atmospheric ScienceNanostructure010504 meteorology & atmospheric sciencesScanning electron microscopeChemistryAnalytical chemistryMineralogyElectron010501 environmental sciences01 natural sciencesMicroanalysisAmorphous solid13. Climate actionPolar vortexMixing ratioStratosphere0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
researchProduct

Individual-particle analysis of airborne dust samples collected over Morocco in 2006 during SAMUM 1

2011

During the course of SAMUM 1 in May and June 2006, airborne samples were collected in southern Morocco at altitudes between 830 and 3340 m above ground. We analysed approximately 22 500 particles of 1–30 μm by automated individual-particle analysis with a scanning electron microscope (SEM) and an energy-dispersive X-ray (EDX) analyser. The major difference between samples is due to the presence and amount of chlorine- and sulphur-bearing particles, pointing to a varying maritime influence and to different degrees of aging. In contrast, the desert dust component is very homogeneous independent of altitude, activated local source area, and dust storm intensity, implying very fast mixing of th…

Atmospheric ScienceRange (particle radiation)010504 meteorology & atmospheric sciencesScanning electron microscopePalygorskiteMineralogy010501 environmental sciencesMineral dust01 natural sciencesAerosolAltitudeDust stormmedicineParticleEnvironmental science0105 earth and related environmental sciencesmedicine.drugTellus B: Chemical and Physical Meteorology
researchProduct

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
researchProduct

Surface spectroscopic study of the corrosion of ultrathin57Fe-evaporated and Langmuir-Blodgett films in humid SO2 environments

2000

Integral conversion electron Mossbauer spectroscopy (ICEMS), x-ray photoelectron spectroscopy (XPS), Auger electron spectroscopy (AES) and scanning electron microscopy (SEM) have been used to carry out a comparative study of the corrosion resistance against humid SO2-aggressive environments of ultrathin 57Fe films. These films, having a thickness ≤ 2.5 nm, have been prepared by evaporation of 57Fe under vacuum and by 57Fe coating by a Langmuir–Blodgett (LB) technique on SiO2/Si wafers. The results have shown that the corrosion resistance of the evaporated films is similar to that of massive Fe. However, the LB films show a remarkably higher corrosion resistance. Thus, although the Fe films …

Auger electron spectroscopyChemistryScanning electron microscopeAnalytical chemistrySurfaces and InterfacesGeneral Chemistryengineering.materialCondensed Matter PhysicsEvaporation (deposition)Langmuir–Blodgett filmSurfaces Coatings and FilmsCorrosionX-ray photoelectron spectroscopyCoatingConversion electron mössbauer spectroscopyMaterials ChemistryengineeringSurface and Interface Analysis
researchProduct

Preparation by radio-frequency magnetron co-sputtering and characterization of thin films of lanthanum–strontium ferromanganites

2005

Abstract (La 0.8 Sr 0.2 )(Mn 1 −  y Fe y )O 3 ± δ films with y  = 0, 0.2, 0.5, 0.8 and 1, a few hundred nanometers thick, were deposited onto polycrystalline yttria-stabilized zirconia YSZ by a magnetron co-sputtering technique using individual targets of La 0.8 Sr 0.2 MnO 3 and La 0.8 Sr 0.2 FeO 3 . The deposition parameters, substrate temperature and gas pressure, were studied by scanning electron microscopy, energy dispersive X-ray spectrometry, X-ray diffraction and interferential microscopy for their effects on the morphological, chemical, topographic and crystallographic properties of films and YSZ-film interfaces. (La 0.8 Sr 0.2 )(Mn 1 −  y Fe y )O 3 ±  δ thin films were found to be …

Auger electron spectroscopyMaterials scienceScanning electron microscopeMetals and AlloysAnalytical chemistrySurfaces and InterfacesSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsSecondary ion mass spectrometrySputteringCavity magnetronMaterials ChemistryCrystalliteThin filmYttria-stabilized zirconiaThin Solid Films
researchProduct

Initial chemical transport of reducing elements and chemical reactions in oxide cathode base metal

2002

Abstract In the present work, the formation of compounds associated to the diffusion of reducing elements (Mg and Al) to the nickel surface of a one-piece oxide cathode has been studied. Those compounds have been evidenced after the annealing steps at high temperature performed on cathode base metal prior to the emitting coating deposition. Therefore, they form the “initial” interface between the nickel and the coating, in other words, the interface existing at the beginning of cathode life. Extensive analysis to characterize the nickel base prior to coating deposition has been performed by means of scanning electron microscopy (SEM) coupled with energy dispersive X-ray spectroscopy (EDX), …

Auger electron spectroscopyScanning electron microscopeAnalytical chemistryGeneral Physics and Astronomychemistry.chemical_elementSurfaces and InterfacesGeneral Chemistryengineering.materialCondensed Matter PhysicsCathodeSurfaces Coatings and Filmslaw.inventionNickelchemistryCoatinglawTransmission electron microscopyengineeringGrain boundary diffusion coefficientSpectroscopyApplied Surface Science
researchProduct