Search results for "Sorption"

showing 10 items of 4623 documents

Study of the reflection spectrum of the LMXB 4U 1702-429

2016

The source 4U 1702-429 (Ara X-1) is a low-mass X-ray binary system hosting a neutron star. Albeit the source is quite bright ( $\sim10^{37}$ erg s$^{-1}$) its broadband spectrum has never been studied. Neither dips nor eclipses have been observed in the light curve suggesting that its inclination angle is smaller than 60$^{\circ}$.We analysed the broadband spectrum of 4U 1702-429 in the 0.3-60 keV energy range, using XMM-Newton and INTEGRAL data, to constrain its Compton reflection component if it is present. After excluding the three time intervals in which three type-I X-ray bursts occurred, we fitted the joint XMM-Newton and INTEGRAL spectra obtained from simultaneous observations. A bro…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral lineAccretion accretion diskSettore FIS/05 - Astronomia E AstrofisicaIonization0103 physical sciencesStars: individual: 4U 1702-429Emission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsindividual: 4U 1702-429; Stars: neutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Stars]PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and AstrophysicLight curveX-rays: binarieAccretion (astrophysics)Stars: neutronNeutron starAbsorption edgeSpace and Planetary ScienceElectron temperatureAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Effects of radiation in accretion regions of classical T Tauri stars

2019

Models and observations indicate that the impact of matter accreting onto the surface of young stars produces regions at the base of accretion columns, in which optically thin and thick plasma components coexist. Thus an accurate description of these impacts requires to account for the effects of absorption and emission of radiation. We study the effects of radiation emerging from shock-heated plasma in impact regions on the structure of the pre-shock downfalling material. We investigate if a significant absorption of radiation occurs and if it leads to a pre-shock heating of the accreting gas. We developed a radiation hydrodynamics model describing an accretion column impacting onto the su…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsradiation: dynamics01 natural sciencesaccretion0103 physical sciencesThermalRadiative transferAstrophysics::Solar and Stellar Astrophysics010306 general physicsAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsultraviolet: starsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsstars: variables: T Tauristars: formationaccretion disksHerbig Ae/BeAstronomy and AstrophysicsPlasmaThermal conductionAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomena
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TeV gamma-ray survey of the Northern sky using the ARGO-YBJ detector

2013

The ARGO-YBJ detector is an extensive air shower array that has been used to monitor the northern $\gamma$-ray sky at energies above 0.3 TeV from 2007 November to 2013 January. In this paper, we present the results of a sky survey in the declination band from $-10^{\circ}$ to $70^{\circ}$, using data recorded over the past five years. With an integrated sensitivity ranging from 0.24 to $\sim$1 Crab units depending on the declination, six sources have been detected with a statistical significance greater than 5 standard deviations. Several excesses are also reported as potential $\gamma$-ray emitters. The features of each source are presented and discussed. Additionally, $95\%$ confidence le…

Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectFOS: Physical sciencesFluxField of viewAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGamma rays: general – surveys01 natural sciencesDeclination0103 physical sciencesAbsorption (logic)010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsgeneral – su [gamma rays]Air showerExtragalactic background light13. Climate actionSpace and Planetary ScienceSkygeneral – surveys [Gamma rays]Astrophysics - High Energy Astrophysical Phenomena
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Analysis of the aerosol radiative forcing over a Mediterranean urban coastal site

2014

Abstract The aerosol radiative forcing for the period 2003–2011 has been analyzed in Burjassot, Spain, an urban coastal site on the western Mediterranean, using measurements of global solar irradiance and aerosol properties, as well as simulated data. The aerosol radiative forcing was calculated at 5 minute intervals, and then integrated over 24 h to obtain daily mean values for 200 complete days under cloud-free skies. The monthly mean values of the aerosol radiative forcing showed a clear variation during the year, associated to the annual variability of the aerosol optical depth at 500 nm, ranging from − 6 to − 29 Wm− 2 at the surface, and from − 1.5 to − 3.9 Wm− 2 at the top of the atmo…

AtmosphereMediterranean climateCloud forcingAtmospheric ScienceAerosol radiative forcingClimatologyEnvironmental scienceRadiative forcingAbsorption (electromagnetic radiation)Solar irradianceAtmospheric sciencesAerosolAtmospheric Research
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Atmospheric water vapour content retrieval from visible and thermal data in the framework of the DAISEX campaigns

2005

In this paper three methods are presented that retrieve the atmospheric water vapour from DAIS (digital airborne imaging spectrometer) data in the framework of the DAISEX (DAIS Experiment) campaigns carried out by ESA (European Space Agency). The three methodologies analysed in the paper are: (i) the ratio technique, in which the water vapour is obtained from visible and near‐infrared bands; (ii) the split‐window technique; and (iii) the split‐window covariance‐variance ratio technique, in which the water vapour content is retrieved from thermal infrared bands. A comparison between the atmospheric water vapour content extracted from the DAIS images using these techniques and that obtained f…

AtmosphereMeteorologyThermalImaging spectrometerAtmospheric correctionGeneral Earth and Planetary SciencesAtmospheric water vapourEnvironmental scienceDaisAbsorption (electromagnetic radiation)Water vaporRemote sensingInternational Journal of Remote Sensing
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The novel HALO mini-DOAS instrument: inferring trace gas concentrations from airborne UV/visible limb spectroscopy under all skies using the scaling …

2017

Abstract. We report on a novel six-channel optical spectrometer (further on called mini-DOAS instrument) for airborne nadir and limb measurements of atmospheric trace gases, liquid and solid water, and spectral radiances in the UV/vis and NIR spectral ranges. The spectrometer was developed for measurements from aboard the German High-Altitude and Long-Range (HALO) research aircraft during dedicated research missions. Here we report on the relevant instrumental details and the novel scaling method used to infer the mixing ratios of UV/vis absorbing trace gases from their absorption measured in limb geometry. The uncertainties of the scaling method are assessed in more detail than before for …

Atmospheric Science010504 meteorology & atmospheric sciences0207 environmental engineering02 engineering and technology010502 geochemistry & geophysics01 natural sciencesUV/visible limb spectroscopylaw.inventionOpticslawErdsystem-Modellierungddc:550Nadirlcsh:TA170-171020701 environmental engineeringAbsorption (electromagnetic radiation)SpectroscopyScaling0105 earth and related environmental sciencesRemote sensingSpectrometerVerkehrsmeteorologielcsh:TA715-787business.industrylcsh:Earthwork. FoundationsAtmosphärische SpurenstoffeOptical spectrometerlcsh:Environmental engineeringTrace gasHALO mini-DOASEarth sciences13. Climate actionEnvironmental scienceHalobusinessAtmospheric Measurement Techniques
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Multiyear in-situ measurements of atmospheric aerosol absorption properties at an urban coastal site in western Mediterranean

2016

Abstract In-situ aerosol absorption properties measured in Valencia (Spain) for four years, from February 2011 to February 2015, have been analysed. Spectral absorption properties have been obtained using a seven-wavelength Aethalometer AE-31 which covers the range from UV (370 nm) to IR (950 nm). In order to obtain the absorption coefficients, compensation parameters have been calculated for the Aethalometer considering seasonal and spectral differences. For this multiyear measurement period, seasonal site-specific calibration parameters have been obtained. Furthermore, estimations of the absorption Angstrom Exponent (α abs ) have been calculated using the seven Aethalometer wavelengths. T…

Atmospheric Science010504 meteorology & atmospheric sciencesChemistry010501 environmental sciencesSeasonalitymedicine.diseaseAethalometerAtmospheric sciences01 natural sciencesStandard deviationWavelengthBoundary layerClimatologyAttenuation coefficientmedicineCalibrationAbsorption (electromagnetic radiation)0105 earth and related environmental sciencesGeneral Environmental ScienceAtmospheric Environment
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Electron microscopy of particles collected at Praia, Cape Verde, during the Saharan Mineral Dust Experiment: particle chemistry, shape, mixing state …

2011

A large field experiment of the Saharan Mineral Dust Experiment (SAMUM) was performed in Praia, Cape Verde, in January and February 2008. The aerosol at Praia is a superposition of mineral dust, sea-salt, sulphates and soot. Particles smaller than 500 nm are mainly mineral dust, mineral dust–sulphate mixtures, sulphates and soot–sulphate mixtures. Particles larger then 2.5 μm consist of mineral dust, sea-salt and few mineral dust–sulphate mixtures. A transition range exists in between. The major internal mixtures are mineral dust–sulphate and soot–sulphate. Mineral dust–sea-salt mixtures occur occasionally, mineral dust–soot mixtures were not observed. The aspect ratio was 1.3–1.4 for dry p…

Atmospheric Science010504 meteorology & atmospheric sciencesChemistryMineralogy010501 environmental sciencesMineral dustmedicine.disease_causecomplex mixtures01 natural sciencesSootAerosolCape verdeAbsorption edgemedicineParticleParticle sizeAbsorption (electromagnetic radiation)0105 earth and related environmental sciencesTellus B: Chemical and Physical Meteorology
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2016

Abstract. Gaseous formaldehyde (HCHO) is an important precursor of OH radicals and a key intermediate molecule in the oxidation of atmospheric volatile organic compounds (VOCs). Budget analyses reveal large discrepancies between modeled and observed HCHO concentrations in the atmosphere. Here, we investigate the interactions of gaseous HCHO with soil surfaces through coated-wall flow tube experiments applying atmospherically relevant HCHO concentrations of  ∼  10 to 40 ppbv. For the determination of uptake coefficients (γ), we provide a Matlab code to account for the diffusion correction under laminar flow conditions. Under dry conditions (relative humidity  =  0 %), an initial γ of (1.1 ± …

Atmospheric Science010504 meteorology & atmospheric sciencesChemistryRadicalDrop (liquid)Inorganic chemistry010501 environmental sciences01 natural sciencesChemical reactionTrace gasAdsorptionDesorptionMoleculeRelative humidity0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Inter-comparison of stratospheric O<sub>3</sub> and NO<sub>2</sub> abundances retrieved from …

2006

Abstract. Stratospheric O3 and NO2 abundances measured by different remote sensing instruments are inter-compared: (1) Line-of-sight absorptions and vertical profiles inferred from solar spectra in the ultra-violet (UV), visible and infrared (IR) wavelength ranges measured by the LPMA/DOAS (Limb Profile Monitor of the Atmosphere/Differential Optical Absorption Spectroscopy) balloon payload during balloon ascent/descent and solar occultation are examined with respect to internal consistency. (2) The balloon borne stratospheric profiles of O3 and NO2 are compared to collocated space-borne skylight limb observations of the Envisat/SCIAMACHY satellite instrument. The trace gas profiles are retr…

Atmospheric Science010504 meteorology & atmospheric sciencesDifferential optical absorption spectroscopyBalloonAtmospheric sciences01 natural sciencesOccultationTrace gasSCIAMACHY010309 opticsAtmosphereAltitude13. Climate action0103 physical sciencesEnvironmental scienceSatellite0105 earth and related environmental sciencesRemote sensingAtmospheric Chemistry and Physics
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