Search results for "Ham"

showing 10 items of 2612 documents

Julma ja kiehtova itä : muslimit englanninkielisissä maantieteen teoksissa 1700-luvun jälkimmäisellä puoliskolla

2010

Eurooppa ja islam ovat olleet toistensa kanssa tekemisissä jo vuosisatojen ajan. Kanssakäyminen on ollut sekä vihamielistä, että rauhanomaista, mutta eurooppalaisten asenteita on aina värittänyt pelko kristinuskon vanhentuneena kieltänyttä itäistä naapuria kohtaan. Tässä työssä tarkastellaan Euroopassa 1700-luvun loppupuolella vallinnutta muslimikuvaa. Tutkimuksessa selvitetään, miten muslimeihin suhtauduttiin maallistuvassa yhteiskunnassa, millaisia representaatioita heistä rakennettiin, sekä eroteltiinko muslimikansallisuudet toisistaan, vai tarkasteltiinko heitä yhtenäisenä ryhmänä. Alkuperäislähteenä käytetään 1700-luvun jälkimmäisellä puoliskolla kirjoitettuja englanninkielisiä maantie…

ArabiahaaremitPersiamaantiedeislamMuhammeditämainen despotiaOsmanien valtakuntarepresentaatiomuslimittoiseuden representaatiottoiseusEurooppamuslimikuva1700-luku
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De la nature juridique du référé pré-arbitral de la CCI

2003

International audience; (Paris, 1re ch. C, 29 avr. 2003, Sté Nationale des Pétroles du Congo et République du Congo c/ Sté Total Fina Elf TEP Congo, inédit)

Arbitrage internationalChambre de commerce internationale[SHS.DROIT]Humanities and Social Sciences/LawRéféré pré-arbitral[SHS.DROIT] Humanities and Social Sciences/LawARBITRAGENature juridique
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Exotic insect pests: The impact of the Red Palm Weevil on natural and cultural heritage in Palermo (Italy)

2013

Abstract The impact of invasive exotic pests is increasingly recognised as a global issue. A global strategy to address the exotic pest problem is beginning to evolve, albeit slowly. The International Plant Protection Convention (FAO) has begun the process of harmonizing standards for pest risk analysis to minimise the spread of exotic pests without adversely impacting global trade. However if the impacts of insect invasive species on human health and on agriculture have attracted worldwide attention, researchers and policymakers address directly the connection between invasive species and damage to natural and cultural heritages. The cost of these losses is generally neglected or underesti…

ArcheologybiologyEcologybusiness.industryAgroforestryMaterials Science (miscellaneous)BiodiversityGlobal strategyConservationbiology.organism_classificationInvasive speciesInternational Plant Protection ConventionCultural heritageRhynchophorusSettore AGR/11 - Entomologia Generale E ApplicataRhynchophorus ferrugineus Phoenix canariensis Chameropsis humilis Protected areas BiodiversityGlobal issueChemistry (miscellaneous)AgricultureSettore BIO/03 - Botanica Ambientale E ApplicatabusinessGeneral Economics Econometrics and FinanceSpectroscopyJournal of Cultural Heritage
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Early induction of genetic instability and apoptosis by arsenic in cultured Chinese hamster cells

2002

In order to assess at what time from the beginning of exposure inorganic arsenic can give rise to genetic instability and trigger apoptosis, V79-C13 Chinese hamster cells were treated with 10 microM sodium arsenite for 24 h. Under these conditions, cell survival was >70% and cells showed neither an increase in chromosome aberration frequency nor a delay in cell cycle progression. Investigations, which were carried out every 6 h during the treatment, revealed an early appearance of genetically unstable cells, namely micronucleated, multinucleated and mononucleated 'giant' cells, as well as apoptotic cells. Indirect immunostaining using anti-beta-tubulin antibody showed severe alterations in …

ArsenitesCell SurvivalHealth Toxicology and MutagenesisPopulationMitosisHamsterApoptosisToxicologyChromosome aberrationChromosomesChinese hamsterCricetulusMultinucleateCricetinaeGeneticsAnimalseducationMitosisGenetics (clinical)Chromosome Aberrationseducation.field_of_studybiologyAneuploidybiology.organism_classificationSodium CompoundsMolecular biologyCell biologySettore BIO/18 - GeneticaCell cultureApoptosisCytogenetic AnalysisMutationarsenic genomic instability apoptosisFluorescein-5-isothiocyanate
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Discovery potential of xenon-based neutrinoless double beta decay experiments in light of small angular scale CMB observations

2013

The South Pole Telescope (SPT) has probed an expanded angular range of the CMB temperature power spectrum. Their recent analysis of the latest cosmological data prefers nonzero neutrino masses, with Sigma m(nu) = (0.32 +/- 0.11) eV. This result, if con firmed by the upcoming Planck data, has deep implications on the discovery of the nature of neutrinos. In particular, the values of the effective neutrino mass m(beta beta) involved in neutrinoless double beta decay (beta beta 0 nu) are severely constrained for both the direct and inverse hierarchy, making a discovery much more likely. In this paper, we focus in xenon-based beta beta 0 nu experiments, on the double grounds of their good perfo…

AstrofísicaPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsCosmic microwave backgroundchemistry.chemical_elementdouble beta decayFOS: Physical sciences7. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicssymbols.namesakeHigh Energy Physics - Experiment (hep-ex)XenonHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesPlanck010306 general physicsPhysicsCosmologiaTime projection chamber010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsneutrino masses from cosmologyInstrumentation and Detectors (physics.ins-det)3. Good healthHigh Energy Physics - PhenomenologyMAJORANASouth Pole Telescopechemistry13. Climate actionsymbolsNeutrino
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The Gaia-ESO survey: Metallicity of the chamaeleon i star-forming region

2014

Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun and older clusters in the solar vicinity. However, these results are based on small statistics and inhomogeneous analyses. The Gaia-ESO Survey is observing and homogeneously analyzing large samples of stars in several young clusters and star-forming regions, hence allowing us to further investigate this issue. Aims. We present a new metallicity determination of the Chamaeleon I star-forming region, based on the products distributed in the first internal release of the Gaia-ESO Survey. Methods. 48 candidate member…

AstrofísicaStars: abundanceMetallicityFOS: Physical sciencesTechniques: spectroscopicContext (language use)AstrophysicsOpen clusters and associations: individual: Chamaeleon ISolar and Stellar Astrophysics (astro-ph.SR)Line (formation)Physics85A04open clusters and associations: individual: Chamaeleon I stars: pre-main sequence stars: abundances techniques: spectroscopicStars: abundancesAstronomy and AstrophysicsSurface gravityAstronomíaStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceChamaeleonStars: pre-main sequenceOpen clusters and associations: individual: Chamaeleon I; Stars: abundances; Stars: pre-main sequence; Techniques: spectroscopicindividual: Chamaeleon I stars: pre-main sequence stars: abundances techniques: spectroscopic [open clusters and associations]Equivalent widthOpen cluster
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The Gaia-ESO Survey: Chromospheric emission, accretion properties, and rotation in gamma Velorum and Chamaeleon

2015

Aims: One of the goals of the Gaia-ESO Survey (GES), which is conducted with FLAMES at the VLT, is the census and the characterization of the low-mass members of very young clusters and associations. We conduct a comparative study of the main properties of the sources belonging to γ Velorum (γ Vel) and Chamaeleon I (Cha I) young associations, focusing on their rotation, chromospheric radiative losses, and accretion. Methods: We used the fundamental parameters (effective temperature, surface gravity, lithium abundance, and radial velocity) delivered by the GES consortium in the first internal data release to select the members of γ Vel and Cha I among the UVES and GIRAFFE spectroscopic obser…

Astrofísicastars: chromospheresAstrophysics::High Energy Astrophysical PhenomenaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRotationStars: chromosphereOpen clusters and associations: individual:γVelorumstars: low-massStars: low-maAstrophysics::Solar and Stellar AstrophysicsOpen clusters and associations: individual: Chamaeleon Iopen clusters and associations: individual: γ VelorumQCAstrophysics::Galaxy AstrophysicsQBLine (formation)PhysicsAccretion (meteorology)stars: chromospheres ; stars: low-mass; open clusters and associations: individual: γ VelorumDiagramStars: rotationSpectral densityAstronomy and AstrophysicsAstronomy and AstrophysicStarsDistribution (mathematics)Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceChamaeleonStars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsOpen clusters and associations: individual: Chamaeleon I; Open clusters and associations: individual:γVelorum; Stars: chromospheres; Stars: low-mass; Stars: pre-main sequence; Stars: rotation
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History and results of the Riga dynamo experiments

2008

On 11 November 1999, a self-exciting magnetic eigenfield was detected for the first time in the Riga liquid sodium dynamo experiment. We report on the long history leading to this event, and on the subsequent experimental campaigns which provided a wealth of data on the kinematic and the saturated regime of this dynamo. The present state of the theoretical understanding of both regimes is delineated, and some comparisons with other laboratory dynamo experiments are made.

Astrophysics (astro-ph)Fluid Dynamics (physics.flu-dyn)General EngineeringFOS: Physical sciencesEnergy Engineering and Power TechnologyChamp magnetiqueGeophysicsPhysics - Fluid DynamicsAstrophysicsPhysics::GeophysicsPhysics::Fluid DynamicsNuclear magnetic resonanceDynamo theoryMagnetohydrodynamicsGeologyDynamo
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The pre-outburst flare of the A 0535+26 August/September 2005 outburst

2008

We study the spectral and temporal behavior of the High Mass X-ray Binary A 0535+26 during a `pre-outburst flare' which took place ~5 d before the peak of a normal (type I) outburst in August/September 2005. We compare the studied behavior with that observed during the outburst. We analyse RXTE observations that monitored A 0535+26 during the outburst. We complete spectral and timing analyses of the data. We study the evolution of the pulse period, present energy-dependent pulse profiles both at the initial pre-outburst flare and close to outburst maximum, and measure how the cyclotron resonance-scattering feature (hereafter CRSF) evolves. We present three main results: a constant period P=…

Astrophysics::High Energy Astrophysical PhenomenaX-ray binarymagnetic fields [Stars]FOS: Physical sciencesChamp magnetiqueAstrophysicsPhoton energyAstrophysicslaw.inventionPulse periodAccretion disclaw:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]X-rays : binaries; Stars : magnetic fields; Stars : individual : A 0535+26UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos XAstrophysics::Solar and Stellar AstrophysicsSpectral analysisPhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsSpace and Planetary ScienceHigh massbinaries [X-rays]individual : A 0535+26 [Stars]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasFlare:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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Atmospheric aging of small-scale wood combustion emissions (model MECHA 1.0) – is it possible to distinguish causal effects from non-causal ass…

2020

Abstract. Primary emissions of wood combustion are complex mixtures of hundreds or even over a thousand compounds, which pass through a series of chemical reactions and physical transformation processes in the atmosphere (aging). This aging process depends on atmospheric conditions, such as concentration of atmospheric oxidizing agents (OH radical, ozone and nitrate radicals), humidity and solar radiation, and is known to strongly affect the characteristics of atmospheric aerosols. However, there are only few models that are able to represent the aging of emissions during its lifetime in the atmosphere. In this work, we implemented a model (Model for aging of Emissions in environmental CHAm…

AtmosphereWork (thermodynamics)Scale (ratio)Differential equationScientific methodEnvironmental chamberCausal effectEnvironmental scienceAtmospheric sciencesCombustion
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