Search results for "ATMOSPHERE"

showing 10 items of 673 documents

The Amazonian boundary layer and mesoscale circulations

2009

Numerous biogenic volatile organic compounds (VOC) species are released into the atmosphere from tropical forests. Measuring all those which are relevant for atmospheric chemistry or for the carbon budget is challenging. Large-Scale Biosphere-Atmosphere (LBA) Experiment field campaigns substantially increased the number of field studies of isoprene and monoterpene emissions, as well as of the exchange of several other VOC species. This chapter reports about the progress made within LBA from primary emission measurements at the plant species level up to discussions of the oxidative capacity of the atmosphere and formation of secondary organic aerosol particles and cloud condensation nuclei f…

chemistry.chemical_classificationHydrologyAmazonianchemistry.chemical_elementAerosolAtmospherechemistry.chemical_compoundchemistryEnvironmental chemistryAtmospheric chemistryCloud condensation nucleiEnvironmental scienceVolatile organic compoundCarbonIsoprene
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Seasonal variation of average phytoplankton concentration in the Kattegat—a periodical point model

2003

Abstract Seasonal variations in primary production, phytoplankton biomass, chlorophyll-a, dissolved inorganic phosphorus and nitrogen concentrations in the upper 10 m of the Kattegat were analysed by means of monitoring data from 1993–1997. Spatial optimal analysis, based on a stochastic model, was used to reconstruct weekly constituent fields onto a spatial grid. The reconstructed fields were spatially integrated, resulting in a relatively smooth seasonal variability of the average variables. A simple dynamical model, set up as a periodical boundary problem, is suggested for the average phytoplankton concentration, dissolved inorganic nitrogen and entrainment depth as state variables. The …

chemistry.chemical_elementInflowForcing (mathematics)Aquatic ScienceSeasonalityOceanographyAtmospheric sciencesmedicine.diseaseNitrogenAtmospherechemistryClimatologyPhytoplanktonmedicineEnvironmental sciencePhotic zoneEntrainment (chronobiology)Ecology Evolution Behavior and SystematicsJournal of Sea Research
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IEL.21-22-Unit 5. The Protection of the Atmosphere

2022

Zambrano González, K. (2022). The Protection of the Atmosphere. Powerpoint of the International Environmental Law subject. Academic course 2021-2022. 19. UNIT 5.-THE PROTECTION OF THE ATMOSPHERE. 1. General aspects: Long-Range Transboundary Air Pollution Convention, 1979. 2. Vienna Convention for the Protection of the Ozone Layer. 3. Legal instruments regulating Climate Change: UNFCCC; Kyoto Protocol; Paris Agreement; COP26 - Glasgow Climate Pact

climate changeprotection of the atmosphereUNESCO::CIENCIAS JURÍDICAS Y DERECHOinternational environmental protection
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Partitioning ET measurements for sparse vegetation: application to an olive orchard.

2011

continuum Soil-Plant-Atmosphere Actual Evapotranspiration Eddy covariance Sap Flow
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Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

2019

Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming τ neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in ∼ 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an Eν -2 spectrum in the energy range 1.0 × 1017 eV -2.5 × 1019 eV is E2 dNν/dEν < 4.4 × 10-9 GeV cm-2 s-1 sr-1, placing str…

cosmological neutrinosAstronomyFluxAstrophysics01 natural sciences7. Clean energycosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic rayssurface [detector]Ultra-high-energy cosmic rayPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)cosmological neutrinoSettore FIS/01 - Fisica SperimentaleDETETORESneutrino: UHEUHE [neutrino]Augerobservatorytrajectoryneutrino: flavorProduction (computer science)NeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencescosmic ray experimentCosmic rayultra high energy cosmic raysneutrino: productionneutrino astronomyproduction [neutrino]TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesddc:530model [neutrino]High Energy Physicscosmic radiation: UHEZenithAstrophysiqueneutrino: modelPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsdetector: surfaceHigh Energy Physics::Phenomenologyflavor [neutrino]Astronomy and AstrophysicsAstronomiefluxExperimental High Energy PhysicsatmosphereHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

2019

With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 1017 eV and 1020 eV from point-like sources across the sky, from close to the Southern Celestial Pole up to 60 in declination, with peak sensitivities at declinations around ∼-53 and ∼+55, and an unmatched sensitivity for arrival directions in the Northern hemisphere. A search has been performed for highly-inclined air showers induced by neutrinos of all flavours with no candidate events found in data taken between 1 Jan 2004 and 31 Aug 2018. Upper limits on the neutrino flux from point-like steady sources have been derived as a function of source declination. An unrivaled sensit…

cosmological neutrinosAstronomypoleFluxAstrophysics01 natural sciencesneutrino: fluxcosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic raysmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSastro-ph.HEcosmological neutrinoSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAYSneutrino: UHEAugerobservatoryNEUTRINOSNeutrinoAstrophysics - High Energy Astrophysical Phenomenaairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesultra high energy cosmic raysDeclinationneutrino astronomyCelestial pole0103 physical sciencesflux: upper limitHigh Energy PhysicsDETECTORZenithAstrophysiquePierre Auger Observatoryflavorshowers: atmosphere010308 nuclear & particles physicsdetector: surfaceNorthern HemisphereAstronomy and AstrophysicsAstronomiesensitivitySkyExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Modeling the Effect of Modified Atmospheres on Conidial Germination of Fungi from Dairy Foods

2017

Modified atmosphere packaging (MAP) is commonly applied to extend food shelf-life. Despite growth of a wide variety of fungal contaminants has been previously studied in relation to modified-atmospheres, few studies aimed at quantifying the effects of dioxygen (O2) and carbon dioxide (CO2) partial pressures on conidial germination in solid agar medium. In the present study, an original culture method was developed, allowing microscopic monitoring of conidial germination under modified-atmospheres in static conditions. An asymmetric model was utilized to describe germination kinetics of Paecilomyces niveus, Mucor lanceolatus, Penicillium brevicompactum, Penicillium expansum, and Penicillium …

dioxygen reductionMicrobiology (medical)carbon dioxide increaselcsh:QR1-502predictive mycologydairy foodsMicrobiologylcsh:Microbiologymodified atmosphereOriginal ResearchFrontiers in Microbiology
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Effects of Tray-Drying on the Physicochemical, Microbiological, Proximate, and Sensory Properties of White- and Red-Fleshed Loquat (Eriobotrya Japoni…

2022

Loquat fruits, highly valued by consumers for their characteristic aroma and pleasant taste, have a short post-harvest life and are susceptible to mechanical damage, loss of firmness, and initial organoleptic characteristics. The aim of this work was to develop a drying method suitable for storing loquat fruits in polyamide/polyethylene (PA/PE) bags containing two gaseous mixtures (treatments): MAPN2 (100% N2) and MAPP (21% O2 and 0.04% CO2), at room temperature (20 ± 1 °C) for at least 2 months. The effects of these conditions on the physico-chemical, microbiological, proximate, and sensory properties of fruit stored over a 50-day time interval were studied. The results showed that convect…

dried fruitfood safetymodified atmosphere packagingmineralfruit qualityloquatvitaminloquat; dried fruit; modified atmosphere packaging; fruit quality; food safety; vitamins; minerals; sensory analysisAgronomy and Crop Sciencesensory analysisAgronomy
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Microbiota of sliced cooked ham packaged in modified atmosphere throughout the shelf life

2019

Abstract Fourteen lots of cooked ham in modified atmosphere packaging (CH) were analyzed within a few days from packaging (S) and at the end of the shelf-life (E), after storage at 7 °C to simulate thermal abuse. Five more lots, rejected from the market because spoiled (R), were included in the study. Quality of the products was generally compromised during the shelf life, with only 4 lots remaining unaltered. Analysis of 16S rRNA gene amplicons resulted in 801 OTUs. S samples presented a higher diversity than E and R ones. At the beginning of the shelf life, Proteobacteria and Firmicutes dominated the microbiota, with Acinetobacter, Brochothrix, Carnobacterium, Lactobacillus, Prevotella, P…

education.field_of_studyWeissellabiologyChemistryLactobacillalesPopulationGeneral MedicineCarnobacteriumbiology.organism_classificationMicrobiologyModified atmosphereLactobacillusLeuconostocLeuconostoc carnosumFood scienceeducationFood ScienceInternational Journal of Food Microbiology
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Total volatile flux from Mount Etna

2008

[1] The Total Volatile (TV) flux from Mount Etna volcano has been characterised for the first time, by summing the simultaneously-evaluated fluxes of the three main volcanogenic volatiles: H2O, CO2 and SO2. SO2 flux was determined by routine DOAS traverse measurements, while H2O and CO2 were evaluated by scaling MultiGAS-sensed H2O/SO2 and CO2/SO2 plume ratios to the UV-sensed SO2 flux. The time-averaged TV flux from Etna is evaluated at ∼21,000 t·day−1, with a large fraction accounted for by H2O (∼13,000 t·day−1). H2O dominates (≥70%) the volatile budget during syn-eruptive degassing, while CO2 and H2O contribute equally to the TV flux during passive degassing. The CO2 flux was observed to…

event.disaster_typeBasaltgeographygeography.geographical_feature_categoryVOLCANIC IMPUT IN ATMOSPHERECo2 fluxGeophysicsAtmospheric sciencesPlumeSettore GEO/08 - Geochimica E VulcanologiaVolcanic GasesGeophysicsFlux (metallurgy)VolcanoTotal volatileGeneral Earth and Planetary ScienceseventGas compositionGeology
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