Search results for "BS"

showing 10 items of 20952 documents

ATR–FTIR Spectral Analysis and Soluble Components of PM10 And PM2.5 Particulate Matter over the Urban Area of Palermo (Italy) during Normal Days and …

2019

Several epidemiological studies have shown a close relationship between the mass of particulate matter (PM) and its effects on human health. This study reports the identification of inorganic and organic components by attenuated total reflectance-Fourier-transform infrared spectroscopy (ATR-FTIR) analysis in PM10 and PM2.5 filters collected from three air quality monitoring stations in the city of Palermo (Sicily, Italy) during non-Saharan dust events and Saharan events. It also provides information on the abundance and types of water-soluble species. ATR-FTIR analysis identified sulfate, ammonium, nitrate, and carbonate matter characterized by vibrational frequencies at 603, 615, 670, and …

010504 meteorology & atmospheric sciencesHealth Toxicology and Mutagenesissaharan dust eventsPM10 and PM2.5Infrared spectroscopychemistry.chemical_elementlcsh:Medicine[SDU.STU]Sciences of the Universe [physics]/Earth Sciencesionic soluble components010501 environmental sciencesMineral dust01 natural sciencesionic soluble componentSaharan dust eventPM<sub>10</sub> and PM<sub>2.5</sub>Absorbancechemistry.chemical_compound11. SustainabilitySulfate0105 earth and related environmental sciencesparticulate mattersirocco windsPM 10 and PM 2.5lcsh:RPublic Health Environmental and Occupational HealthSettore GEO/07 - Petrologia E PetrografiaParticulatesSettore GEO/08 - Geochimica E Vulcanologiachemistry13. Climate action[SDU]Sciences of the Universe [physics]Environmental chemistryCarbonateClay mineralsCarbonATR-FTIRInternational Journal of Environmental Research and Public Health
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A search for time-dependent astrophysical neutrino emission with IceCube data from 2012 to 2017

2020

Abstract High-energy neutrinos are unique messengers of the high-energy universe, tracing the processes of cosmic ray acceleration. This paper presents analyses focusing on time-dependent neutrino point-source searches. A scan of the whole sky, making no prior assumption about source candidates, is performed, looking for a space and time clustering of high-energy neutrinos in data collected by the IceCube Neutrino Observatory between 2012 and 2017. No statistically significant evidence for a time-dependent neutrino signal is found with this search during this period, as all results are consistent with the background expectation. Within this study period, the blazar 3C 279, showed strong var…

010504 meteorology & atmospheric sciencesHigh-energy astronomyAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectmodel [emission]FOS: Physical sciencesCosmic rayAstrophysics01 natural scienceslaw.inventionIceCube Neutrino ObservatoryIceCubeblazarlawemission [gamma ray]0103 physical sciencesCosmic ray sources; High-energy astrophysics; Particle astrophysicsenergy: high [neutrino]Blazar010303 astronomy & astrophysics0105 earth and related environmental sciencesmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstroparticle physicsPhysicsbackgroundAstronomy and AstrophysicsCosmic ray sourcesUniverseHigh-energy astrophysicsmessengerobservatorySpace and Planetary Scienceddc:520time dependenceacceleration [cosmic radiation]NeutrinoAstrophysics - High Energy Astrophysical PhenomenaParticle astrophysicsFlare
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High-resolution spectroscopy and analysis of the nu3/2nu4 dyad of CF4

2011

International audience; CF4 is a strong greenhouse gas of both anthropogenic and natural origin [D.R. Worton et al., Environ. Sci. Technol. 41, 2184 (2007)]. However, high-resolution infrared spectroscopy of this molecule has received only a limited interest up to now. Until very recently, the public databases only contained cross-sections for this species, but no detailed line list. We reinvestigate here the strongly absorbing ν3 region around 7.8 μm. New Fourier transform infrared (FTIR) spectra up to a maximal resolution of 0.0025 cm−1 have been recorded: (i) room-temperature spectra in a static cell and (ii) a supersonic expansion jet spectrum at a 23 K estimated temperature. Following …

010504 meteorology & atmospheric sciencesInfraredBiophysicsAnalytical chemistryInfrared spectroscopycarbon tetrafluoride01 natural sciencesSpectral linesymbols.namesake0103 physical sciencesPhysical and Theoretical ChemistryFourier transform infrared spectroscopySpectroscopyMolecular Biologyemi-classical analysis0105 earth and related environmental sciences010304 chemical physicsChemistryResolution (electron density)Condensed Matter Physics[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Fourier transform13. Climate actiongreenhouse gassymbolsinfrared absorption[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]tensorial formalismMicrowave
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Shallow vent architecture during hybrid explosive-effusive activity at Cordón Caulle (Chile, 2011-12): Evidence from direct observations and pyroclas…

2013

International audience; In June 2011, an eruption of rhyolite magma began at the Puyehue-Cordón Caulle volcanic complex, southern Chile. By January 2012, explosive activity had declined from sustained pyroclastic (Plinian to sub-Plinian) fountaining to mixed gas and ash jetting punctuated by Vulcanian blasts. This explosive activity was accompanied by synchronous effusion of obsidian lava in a hybrid explosive-effusive eruption. Fortuitous climatic conditions permitted ground-based observation and video recording of transient vent dynamics as well as real-time collection of proximal juvenile ash as it sedimented from the active plume. The main eruptive vent complex and site of lava effusion…

010504 meteorology & atmospheric sciencesLava[SDE.MCG]Environmental Sciences/Global ChangesSilicicPyroclastic rockMineralogyrhyolite010502 geochemistry & geophysics01 natural sciencestube pumiceobsidianGeochemistry and PetrologyPuyehue-Cordón CaulleRhyolite[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologyTephraPetrology0105 earth and related environmental sciencesgeographyVulcanian eruptiongeography.geographical_feature_categoryPeléan eruptionexplosive-effusive transitionGeophysicsVolcanopermeabilityGeologyVulcanian
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The 2009 Edition of the GEISA Spectroscopic Database

2011

The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques; Management and Study of Atmospheric Spectroscopic Information) is described in this paper. GEISA is a computer-accessible system comprising three independent sub-databases devoted, respectively, to: line parameters, infrared and ultraviolet/visible absorption cross-sections, microphysical and optical properties of atmospheric aerosols. In this edition, 50 molecules are involved in the line parameters sub-database, including 111 isotopologues, for a total of 3,807,997 entries, in the spectral range from 10-6 to 35,877.031cm-1.The successful performances of the new …

010504 meteorology & atmospheric sciencesMeteorologyTélédétectionPhysique atomique et moléculaireMolecular spectroscopyInfrared atmospheric sounding interferometercomputer.software_genre01 natural sciencesLine parametersAtmospheric radiative transfer0103 physical sciences010303 astronomy & astrophysicsSpectroscopy0105 earth and related environmental sciencesRemote sensingWeb site[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]RadiationSpectroscopic database[ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]DatabaseGEISAOptically activeAtmospheric aerosolsMolecular spectroscopyAtomic and Molecular Physics and Optics[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistryOn boardSpectroscopie [électromagnétisme optique acoustique][ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistryEarth's and planetary atmospheresEnvironmental scienceAtmospheric absorptionAtmospheric absorptionCross-sectionscomputer
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ARES. III. Unveiling the Two Faces of KELT-7 b with HST WFC3

2020

We present the analysis of the hot-Jupiter KELT-7b using transmission and emission spectroscopy from the Hubble Space Telescope (HST), both taken with the Wide Field Camera 3 (WFC3). Our study uncovers a rich transmission spectrum which is consistent with a cloud-free atmosphere and suggests the presence of H2O and H-. In contrast, the extracted emission spectrum does not contain strong absorption features and, although it is not consistent with a simple blackbody, it can be explained by a varying temperature-pressure profile, collision induced absorption (CIA) and H-. KELT-7 b had also been studied with other space-based instruments and we explore the effects of introducing these additiona…

010504 meteorology & atmospheric sciencesOpacityFOS: Physical sciencesEFFICIENTTransmission spectroscopy; Exoplanet atmospheres; Astronomy data analysisAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstronomy & Astrophysics01 natural sciencesAtmosphereHubble space telescope0103 physical sciencesTransmission spectroscopyEMISSION-SPECTRUMWATERBlack-body radiationEmission spectrumAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsScience & TechnologyHOT JUPITERSAstronomy and AstrophysicsBIASESEXOPLANETSTransmission (telecommunications)13. Climate actionSpace and Planetary SciencePhysical SciencesAstronomy data analysisHD 209458BAstrophysics::Earth and Planetary AstrophysicsATMOSPHERESWide Field Camera 3Astrophysics - Earth and Planetary AstrophysicsExoplanet atmospheresThe Astronomical Journal
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Ray optics for absorbing particles with application to ice crystals at near-infrared wavelengths

2018

Abstract Light scattering by particles large compared to the wavelength of incident light is traditionally solved using ray optics which considers absorption inside the particle approximately, along the ray paths. To study the effects rising from this simplification, we have updated the ray-optics code SIRIS to take into account the propagation of light as inhomogeneous plane waves inside an absorbing particle. We investigate the impact of this correction on traditional ray-optics computations in the example case of light scattering by ice crystals through the extended near-infrared (NIR) wavelength regime. In this spectral range, ice changes from nearly transparent to opaque, and therefore…

010504 meteorology & atmospheric sciencesOpacityspektroskopiaIce crystalsPhysics::OpticsRay optics01 natural sciencesPOLARIZED-LIGHT SCATTERING114 Physical sciencesLight scattering010309 opticsScatteringMEDIAOptics0103 physical sciencesABSORPTIONInhomogeneous wavesCIRRUSray opticsSpectroscopy0105 earth and related environmental sciencesPhysicsta113absorbing mediaRadiationta115Geometrical opticsIce crystalsta114Scatteringbusiness.industryscatteringCLOUDSkiteetRayAtomic and Molecular Physics and OpticsoptiikkaSOLAR-RADIATIONWavelengthMAXWELLS EQUATIONSAbsorbing mediainhomogeneous wavesLight scattering by particlesPHASE MATRIXGEOMETRIC-OPTICSbusinessice crystalsAPPROXIMATION
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The high overtone and combination levels of SF6 revisited at Doppler-limited resolution: A global effective rovibrational model for highly excited vi…

2017

Abstract Sulfur hexafluoride is an important prototypal molecule for modeling highly excited vibrational energy flow and multi quanta absorption processes in hexafluoride molecules of technological importance. It is also a strong greenhouse gas of anthropogenic origin. This heavy species, however, features many hot bands at room temperature (at which only 30% of the molecules lie in the ground vibrational state), especially those originating from the lowest, v 6 =1 vibrational state. Using a cryogenic long path cell with variable optical path length and temperatures regulated between 120 and 163 K, coupled to Synchrotron Radiation and a high resolution interferometer, Doppler-limited spectr…

010504 meteorology & atmospheric sciencesOvertoneInfrared spectroscopylow temperature01 natural sciences7. Clean energyHot bandSpectral linechemistry.chemical_compoundHexafluorideFar infraredhot bandRotation-vibration spectroscopy of SF 60103 physical sciencesSpectroscopy0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Radiation[ PHYS ] Physics [physics]010304 chemical physicsRotational–vibrational spectroscopyAtomic and Molecular Physics and Opticschemistry13. Climate actiongreenhouse gasExcited stateinfrared absorptionAtomic physicstensorial formalismLong path cell
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Oscillations on Width and Intensity of Slender Ca ii H Fibrils from Sunrise/SuFI

2017

R. Gafeira et. al.

010504 meteorology & atmospheric sciencesPhase (waves)FOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencesMolecular physics0103 physical sciencesWave modeSunriseSun: oscillationsTechniques: imaging spectroscopySun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSolar observatoryoscillations [Sun]imaging spectroscopy [Techniques]Sun: chromosphereAstronomy and AstrophysicsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]Space and Planetary ScienceIntensity (heat transfer)The Astrophysical Journal Supplement Series
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Spectropolarimetric evidence for a siphon flow along an emerging magnetic flux tube

2016

©2017 The American Astronomical Society. All rights reserved.We study the dynamics and topology of an emerging magnetic flux concentration using high spatial resolution spectropolarimetric data acquired with the Imaging Magnetograph eXperiment on board the sunrise balloon-borne solar observatory. We obtain the full vector magnetic field and the line of sight (LOS) velocity through inversions of the Fe i line at 525.02 nm with the SPINOR code. The derived vector magnetic field is used to trace magnetic field lines. Two magnetic flux concentrations with different polarities and LOS velocities are found to be connected by a group of arch-shaped magnetic field lines. The positive polarity footp…

010504 meteorology & atmospheric sciencesPolarity (physics)photosphere [Sun]FOS: Physical sciencesAstrophysicspolarimetric [Techniques]01 natural sciencesMethods: observational0103 physical sciencesSunriseAstrophysics::Solar and Stellar Astrophysicsobservational [Methods]010303 astronomy & astrophysicsSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsSolar observatoryPolarity symbolsTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsMagnetic fluxMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsFlow (mathematics)magnetic fields [Sun]Space and Planetary Science
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