Search results for " Atmosphere"

showing 10 items of 292 documents

Dried-Fruit Storage: An Analysis of Package Headspace Atmosphere Changes

2019

The quality of packaged dried foods depends on storage conditions and is determined largely by the initial gas composition inside and the transference through the container. The aim of this work was to analyze the O2 and CO2 concentrations within the internal atmosphere of the packaging. In this study, dried apricots and raisins were packaged in glass jars and polypropylene trays thermosealed with different polymers, and stored at 5, 15, 25, and 35 &deg

Health (social science)Dried fruit030309 nutrition & dieteticschemistry.chemical_elementPlant Sciencefruit storagefood qualitylcsh:Chemical technologyHealth Professions (miscellaneous)MicrobiologyArticle03 medical and health scienceschemistry.chemical_compound0404 agricultural biotechnologyCo2 concentrationlcsh:TP1-1185Gas compositionPolypropylene0303 health sciencesmodified atmosphere packagingEmbalatgeAliments Conservació04 agricultural and veterinary sciencesPulp and paper industry040401 food scienceNitrogenFood packagingFruitachemistryModified atmosphereEnvironmental sciencepermeabilityFood qualityfood packagingFood ScienceFoods
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VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), σ Oph, BM Sco, and HD 206859

2017

Aims. We add four warmer late-type supergiants to our previous spectro-interferometric studies of red giants and supergiants. Methods. We measure the near-continuum angular diameter, derive fundamental parameters, discuss the evolutionary stage, and study extended atmospheric atomic and molecular layers. Results. V766 Cen (=HR 5171 A) is found to be a high-luminosity (log L/L = 5.8 ± 0.4) source of effective temperature 4290 ± 760 K and radius 1490 ± 540 R, located in the Hertzsprung-Russell (HR) diagram close to both the Hayashi limit and Eddington limit; this source is consistent with a 40 M evolutionary track without rotation and current mass 27-36 M. V766 Cen exhibits Na i in emission a…

Hertzsprung–Russell diagramindividual: BM Sco [Stars]FOS: Physical sciencesAstrophysics01 natural sciencesLuminositysymbols.namesake0103 physical sciencesStars: individual: BM ScoRed supergiantStars: mass-lossYellow hypergiantatmospheres [Stars]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Physicsmass-loss [Stars]010308 nuclear & particles physicsAstronomy and AstrophysicsEffective temperatureStars: individual: V766 CenAstrophysics - Solar and Stellar AstrophysicsSupergiantsSpace and Planetary ScienceEddington luminosityTechniques: interferometricsymbolsCircumstellar dustinterferometric [Techniques]individual: V766 Cen [Stars]Stars: atmospheresSupergiant
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Temperature dependence of sodium and ionized calcium resonance lines perturbed by helium

2014

International audience; Traces of heavy metals in cool DZ white dwarf stars may be attributed to the accretion of circumstellar dust thought to originate from tidal disruption of rocky parent bodies. Spectra of such stars therefore provide a unique opportunity to study the composition of extrasolar planetary systems. The determination of metal abundances from stellar spectra depends on stellar atmospheric parameters and an accurate prior knowledge of the collision broadening of the line profiles by the most common constituents of the stellar atmosphere. For this purpose, we present theoretical absorption spectra of Na and Ca+ broadened by He for the conditions prevailing in cool white dwarf…

HistoryAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsHelium01 natural sciencesAstronomical spectroscopySpectral lineEducation0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics][PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]ChemistryStellar atmosphereWhite dwarfAstronomyPlanetary system[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Accretion (astrophysics)Computer Science ApplicationsStars13. Climate actionCircumstellar dustAtomic and molecular collisions[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Astrophysics::Earth and Planetary AstrophysicsMolecular physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Journal of Physics: Conference Series
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Influence of SMSI effect on the catalytic activity of a Pt(1%)/ Ce0.6Zr0.4O2 catalyst: SAXS, XRD, XPS and TPR investigations

2004

Abstract The steady-state activity of NO reduction by C3H6, in lean conditions, was studied on a Pt(1%)/Ce0.6Zr0.4O2 catalyst, in a plug-flow reactor, in the temperature range 100–500 °C. The influence of reductive pre-treatments on the catalytic performance at low temperature (250 °C) was investigated. Enhancement of the activity was found for the catalyst pre-treated in hydrogen at 350 °C as compared to the sample pre-treated in H2 at 800 and 1050 °C. Moreover, transient reactivity tests of NO reduction by hydrogen were also carried out. As previously observed, the sample reduced at 350 °C was the most active catalyst. In both types of reactions the temperature and the nature of pre-treat…

HydrogenProcess Chemistry and TechnologyReducing atmosphereInorganic chemistryAnalytical chemistrychemistry.chemical_elementAtmospheric temperature rangeCatalysisCatalysischemistryTransition metalX-ray photoelectron spectroscopyTemperature-programmed reductionPlatinumCerium compounds Catalysts capacity OSCGeneral Environmental Science
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A conceptual dynamic vegetation-soil model for arid and semiarid zones

2007

Plant ecosystems in arid and semiarid zones show high complexity from the point of view of water resources, since they depend on water availability to carry out their vital processes. In these climates, water stress is the main factor controlling vegetation development. The available water in the system results from a water balance where the soil, vegetation and the atmosphere are the key issues; but it is the vegetation which modulates (to a great extent) the total balance of water and the mechanisms of the feedback between soil and atmosphere, being the knowledge about soil moisture quite relevant for assessing available water and, as a consequence, for growth and plants maintenance and t…

Hydrologylcsh:GE1-350Moisturelcsh:T[SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmospherelcsh:Geography. Anthropology. RecreationVegetationAridlcsh:Technologylcsh:TD1-1066[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentWater balancelcsh:GEvapotranspirationSoil water[SDU.STU] Sciences of the Universe [physics]/Earth SciencesEnvironmental sciencelcsh:Environmental technology. Sanitary engineeringWater contentlcsh:Environmental sciencesTranspiration
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Volcanic gas emissions and degassing dynamics at Ubinas and Sabancaya volcanoes; implications for the volatile budget of the central volcanic zone

2017

Abstract Emission of volcanic gas is thought to be the dominant process by which volatiles transit from the deep earth to the atmosphere. Volcanic gas emissions, remain poorly constrained, and volcanoes of Peru are entirely absent from the current global dataset. In Peru, Sabancaya and Ubinas volcanoes are by far the largest sources of volcanic gas. Here, we report the first measurements of the compositions and fluxes of volcanic gases emitted from these volcanoes. The measurements were acquired in November 2015. We determined an average SO 2 flux of 15.3 ± 2.3 kg s − 1 (1325-ton day − 1 ) at Sabancaya and of 11.4 ± 3.9 kg s − 1 (988-ton day − 1 ) at Ubinas using scanning ultraviolet spectr…

IASI010504 meteorology & atmospheric sciencesSabancayaEarth scienceGeochemistry010502 geochemistry & geophysics01 natural sciencesVolcanic GasesAtmospherechemistry.chemical_compoundFlux (metallurgy)Geochemistry and Petrology[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologyVolcanic degassingeventGeophysic0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphereevent.disaster_typeTrail By Firegeographygeography.geographical_feature_categoryGas emissionsUV-cameraUbinaGeophysicsCarbon dioxidechemistryVolcanoUbinasDOAS13. Climate actionCarbon dioxideMulti-GASGeologyEarth (classical element)Journal of Volcanology and Geothermal Research
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High-Resolution Spectroscopy and Preliminary Global Analysis of C–H Stretching Vibrations of C2H4 in the 3000 and 6000 cm-1 Regions

2010

International audience; Ethylene (ethene, H2C=CH2) is a naturally occurring compound in ambient air that affects atmospheric chemistry and global climate. The C2H4 spectrum is available in databases only for the 1000 and 3000 cm−1 ranges. In this work, the ethylene absorption spectrum was measured in the 6030- 6250 cm−1 range with the use of a high resolution Bruker IFS 125HR Fourierspectrometer and a two-channel opto-acoustic spectrometer with a diode laser. As a secondary standard of wavelengths, the methane absorption spectrum was used in both cases. A preliminary analysis was realized thanks to the tensorial formalism developed by the Dijon group that is implemented in the XTDS software…

Infrared absorption[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistryEthyleneDiode laser spectroscopy[ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistryFourier transform spectroscopyEarth and planetary atmospheres
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Interfacial photochemistry of biogenic surfactants: a major source of abiotic volatile organic compounds

2017

Films of biogenic compounds exposed to the atmosphere are ubiquitously found on the surfaces of cloud droplets, aerosol particles, buildings, plants, soils and the ocean. These air/water interfaces host countless amphiphilic compounds concentrated there with respect to in bulk water, leading to a unique chemical environment. Here, photochemical processes at the air/water interface of biofilm-containing solutions were studied, demonstrating abiotic VOC production from authentic biogenic surfactants under ambient conditions. Using a combination of online-APCI-HRMS and PTR-ToF-MS, unsaturated and functionalized VOCs were identified and quantified, giving emission fluxes comparable to previous …

Lysis010504 meteorology & atmospheric sciencesRadical010501 environmental sciencesPhotochemistry01 natural sciencesMatrix (chemical analysis)AtmosphereSurface-Active AgentsPhysical and Theoretical Chemistry0105 earth and related environmental sciencesAbiotic componentAerosols[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereVolatile Organic CompoundsChemistryAtmosphere[CHIM.CATA]Chemical Sciences/CatalysisPhotochemical Processes[SDE.ES]Environmental Sciences/Environmental and SocietyAerosol13. Climate actionAtmospheric chemistryEnvironmental chemistrySoil water[CHIM.OTHE]Chemical Sciences/Other
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The Hamburg/ESO R-process Enhanced Star survey (HERES):XI. The highly r-process-enhanced star CS 29497-004

2017

We report an abundance analysis for the highly r-process-enhanced (r-II) star CS 29497-004, a very metal-poor giant with Teff = 5013K and [Fe/H]=-2.85, whose nature was initially discovered in the course of the HERES project. Our analysis is based on high signal-to-noise, high-resolution (R~75000) VLT/UVES spectra and MARCS model atmospheres under the assumption of local thermodynamic equilibrium, and obtains abundance measurements for a total of 46 elements, 31 of which are neutron-capture elements. As is the case for the other 25 r-II stars currently known, the heavy-element abundance pattern of CS 29497-004 well-matches a scaled Solar System second peak r-process-element abundance patter…

MODEL ATMOSPHERESSolar SystemPopulation II [stars]Thermodynamic equilibriumMETAL-POOR STARSFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciences7. Clean energySpectral lineGalactic halochemically peculiar [stars]CORE-COLLAPSE SUPERNOVAELABORATORY TRANSITION-PROBABILITIES0103 physical sciencesEXPERIMENTAL OSCILLATOR-STRENGTHShalo [Galaxy]NeutronEARLY GALAXY010306 general physics010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPROCESS-RICHGALACTIC CHEMICAL EVOLUTIONAstronomy and Astrophysicsindividual: CS 29497-004 [stars][PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Astrophysics - Astrophysics of Galaxiesabundances [stars]StarsHIGH-ENTROPY-WIND[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)r-processNEUTRON-CAPTURE
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Association of childhood adversities and home atmosphere with functioning in old age: the Helsinki birth cohort study

2019

Objectivechildhood adversities have been linked with adverse health outcomes, but less is known about the long-term consequences of childhood home atmosphere. We investigated whether childhood adversities and home atmosphere were associated with physical and mental functioning in older age.Methodsin the Helsinki Birth Cohort Study 2003, participants born in the year 1934–44 had data available on nine childhood home atmosphere items, e.g. whether it was supportive and warm (sum score ranged between 0 and 36, higher score indicating better atmosphere), and nine childhood adversities, e.g. unemployment and divorce (sum score 0–9, coded into no; one; and two or more adversities) assessed in 200…

MaleAgingHealth Statusmental functioningchildhood adversitiesPhysical functionolder people0302 clinical medicinePhysical functioningAdverse Childhood ExperiencesSurveys and QuestionnairesActivities of Daily LivingPsychologyMedicine030212 general & internal medicineParent-Child RelationsFinlandta3142General MedicineMiddle AgedMental HealthFemalehealthy ageingBirth cohortpsyykkinen toimintakykyikääntyneetelinolotfyysinen toimintakykyShort form 36home atmosphereHealth outcomesArticle03 medical and health sciencesHumansphysical functioningAssociation (psychology)Geriatric AssessmentAgedMental functioningbusiness.industrylapsuuskasvuympäristöMental healthkotiympäristöikääntyminenSocioeconomic FactorsGeriatrics and Gerontologybusiness030217 neurology & neurosurgeryDemographyAge and Ageing
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