Search results for "Climate"

showing 10 items of 4934 documents

Characterizing a hybrid zone between a cryptic species pair of freshwater snails.

2015

Characterizing hybrid zones and their dynamics is a central goal in evolutionary biology, but this is particularly challenging for morphologically cryptic species. The lack of conspicuous divergence between parental types means intermediate hybrid forms often go undetected. We aimed to detect and characterize a suspected hybrid zone between a pair of morphologically cryptic lineages of the freshwater snail, Radix. We sampled Radix from across a contact zone between two mitochondrial lineages (Radix balthica and an undescribed lineage termed 'MOTU3') and detected admixture between two nuclear genotype clusters, which were significantly but not categorically associated with the mitochondrial …

Species complexEcological selectionGenotypeClimate ChangeMolecular Sequence DataSnailsFresh WaterDNA MitochondrialFreshwater snailHybrid zoneGeographical distanceGenetic variationGeneticsAnimalsDNA Barcoding TaxonomicSelection GeneticEcology Evolution Behavior and SystematicsbiologyGeographyModels GeneticEcologyTemperatureGenetic VariationBayes TheoremCline (biology)biology.organism_classificationBiological EvolutionRadix balthicaHybridization GeneticMicrosatellite RepeatsMolecular ecology
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Evenness, biodiversity, and ecosystem function of intertidal communities along the Italian coasts: Experimental short-term response to ambient and ex…

2023

Biodiversity can promote ecosystem functioning in both terrestrial and marine environments, emphasizing the neces- sity ofbiodiversity conservation in order to preserve critical ecosystem functions and associated services. However, the role of biodiversity in buffering ecosystem functioning under extreme events caused by climate change remains a major scientific issue, especially for intertidal systems experiencing stressors from both terrestrial and marine drivers. We performed a regional-scale field experiment along the Italian coast to investigate the response of unmanipulated intertidal communities (by using a natural biodiversity gradient) to low tide aerial exposure to both ambient an…

Species richneEnvironmental EngineeringChlorophyll AEvennessFunctional richneAmbient temperature; Climate change; Ecosystem functioning; Evenness; Extreme warming conditions; Functional richness; Intertidal biodiversity; Mediterranean Sea; Species richnessExtreme warming conditionsPollutionFunctional richnessEcosystem functioningMediterranean SeaClimate changeEnvironmental ChemistryAmbient temperatureIntertidal biodiversityWaste Management and DisposalEvenneEcosystemSpecies richnessScience of The Total Environment
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Model, software and database for line-mixing effects in the nu3 and nu4 bands of CH4 and tests using laboratory and planetary measurements - II : H2 …

2006

International audience; The absorption shapes of the nu(2), nu(3) and nu(4) infrared bands of CH4 perturbed by H-2 in large ranges of pressure and temperature have been measured in the laboratory. In order to model these spectra, the theoretical approach accounting for line-mixing effects proposed for CH4-N-2 and CH4-air and successfully tested in the companion paper (1), is used. As before, state-to-state rotational rates are used together with some empirical parameters that are deduced from a fit of a single room temperature spectrum of the nu(3) band at about 50 atm. The comparisons between measured and calculated spectra in the nu(3) and nu(4) regions under a vast variety of conditions …

Spectral shape analysis010504 meteorology & atmospheric sciencesInfraredcomputer.software_genre01 natural sciences7. Clean energyJovianSpectral line0103 physical sciencesRadiative transferAbsorption (electromagnetic radiation)Spectroscopy0105 earth and related environmental sciencesLine (formation)Physics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Radiation010304 chemical physicsSpectrometerDatabasemethane infrared spectraAtomic and Molecular Physics and Optics[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]13. Climate actionAstrophysics::Earth and Planetary Astrophysicscomputergiant planets emission
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INTEGRAL and RXTE observations of accreting millisecond pulsar IGR J00291+5934 in outburst

2005

Simultaneous observations of the accretion-powered millisecond pulsar IGR J00291+5934 by International Gamma-Ray Astrophysics Laboratory and Rossi X-ray Timing Explorer during the 2004 December outburst are analysed. The average spectrum is well described by thermal Comptonization with an electron temperature of 50 keV and Thomson optical depth tau_T ~ 1 in a slab geometry. The spectral shape is almost constant during the outburst. We detect a spin-up of the pulsar with nudot=8.4x10E-13 Hz/s. The ISGRI data reveal the pulsation of X-rays at a period of 1.67 milliseconds up to ~150 keV. The pulsed fraction is shown to increase from 6 per cent at 6 keV to 12--20 per cent at 100 keV. This is n…

Spectral shape analysisAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesHot spot (veterinary medicine)Astrophysicsaccretion accretion discs binaries: close stars: individual: IGR J00291+5934 stars: neutron X-rays: binariesAstrophysics01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]symbols.namesakestars: neutronPulsaraccretionMillisecond pulsar0103 physical sciencesOptical depth (astrophysics)010306 general physics010303 astronomy & astrophysicsPhysicsMillisecondbinaries: close[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Astrophysics (astro-ph)Astronomy and Astrophysicsaccretion discspulsars: individual (IGR J00291+5934)13. Climate actionSpace and Planetary SciencesymbolsElectron temperatureDoppler effectX-ray: binaries
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SPEECH AND SILENCE IN CICERO'S FINAL DAYS

2014

Composed in spring of 46 BC, Cicero's Brutus emphasizes oratorical silence, in stark contrast with the prominence of the speech act found in the Pro Marcello and first Philippic. Yet in the face of those difficult times and amidst the silence that such times engender, Cicero ironically finds his voice. This paper will demonstrate Cicero's acute awareness, in his final days, of the need to employ his rediscovered voice in light of eloquence's changed role in Rome's new political climate.

Speech actLiteratureSilenceHistorybusiness.industryFace (sociological concept)Political climateContrast (music)ClassicsbusinessCiceroThe Classical Journal
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Reduction of stored-particle background by a magnetic pulse method at the KATRIN experiment

2018

Arenz, M., et al. “Reduction of Stored-Particle Background by a Magnetic Pulse Method at the KATRIN Experiment.” The European Physical Journal C, vol. 78, no. 9, Sept. 2018. © 2018 The Authors

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Field (physics)Physics::Instrumentation and DetectorsFOS: Physical scienceslcsh:AstrophysicsElectronKATRIN01 natural sciencesradon: nuclideNeutrino mass0103 physical scienceslcsh:QB460-466coillcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsnumerical calculationsEngineering (miscellaneous)background: radioactivitybackground: suppressionPhysicsSpectrometer010308 nuclear & particles physicsPhysicsOrder (ring theory)Monte Carlo methodsInstrumentation and Detectors (physics.ins-det)Radon backgroundPulse (physics)13. Climate actionBackground reduction methodsPartículaslcsh:QC770-798spectrometerAtomic physicsElectricidadElectron neutrinoKATRIN
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Sulfuric acid speleogenesis (SAS) close to the water table: Examples from southern France, Austria, and Sicily

2016

Caves formed by rising sulfuric waters have been described from all over the world in a wide variety of climate settings, from arid regions to mid-latitude and alpine areas. H2S is generally formed at depth by reduction of sulfates in the presence of hydrocarbons and is transported in solution through the deep aquifers. In tectonically disturbed areas major fractures eventually allow these H2S-bearing fluids to rise to the surface where oxidation processes can become active producing sulfuric acid. This extremely strong acid reacts with the carbonate bedrock creating caves, some of which are among the largest and most spectacular in the world. Production of sulfuric acid mostly occurs at or…

Speleogenesi010504 meteorology & atmospheric sciencesWater tableSettore GEO/04 - Geografia Fisica E GeomorfologiaGeochemistry[SDU.STU]Sciences of the Universe [physics]/Earth SciencesAquifer010502 geochemistry & geophysics01 natural scienceschemistry.chemical_compoundPaleontologyCaveSpeleogenesis0105 earth and related environmental sciencesEarth-Surface ProcessesCondensation-corrosiongeographygeography.geographical_feature_categoryHypogenic karstBedrockAuthigenicchemistry13. Climate actionSulfuric acid caveSubaerialCave morphologyCarbonateSulfuric acid caves Hypogenic karst Cave morphology Speleogenesis Condensation–corrosionGeology
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Abundance of cellular material and proteins in the atmosphere.

2005

Suspended atmospheric particles play a crucial role in any global climate scenario: They can both enforce and suppress radiative forcing. In developing climate modeling further, a deeper understanding of atmospheric aerosol is needed. Because of extreme local and temporal variations, proper incorporation of aerosols into models requires modeling of the aerosol itself. It turns out that cellular material and proteins compose up to 25% of the atmospheric aerosol. Consequently, the source strength of the biogenic aerosol in general must be corrected and should be estimated on the order of other major aerosol sources.

SporesMeteorologyCellsAir MicrobiologyEnvironmentAtmospheric sciencesTroposphereAtmosphereAnimalsHumansParticle SizeAerosolsMultidisciplinaryBacteriaAtmosphereFungiBiogeochemistryEukaryotaProteinsRadiative forcingAerosolAtmospheric chemistryVirusesEnvironmental sciencePollenClimate modelSeasonsBioaerosolScience (New York, N.Y.)
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The effect of ISM absorption on stellar activity measurements and its relevance for exoplanet studies

2017

Past UV and optical observations of stars hosting hot Jupiters have shown that some of these stars present an anomalously low chromospheric activity, significantly below the basal level. For WASP-13, observations have shown that the apparent lack of activity is possibly caused by absorption from the intervening ISM. Inspired by this result, we study the effect of ISM absorption on activity measurements (S and logR'$_{\rm HK}$ indices) for main-sequence late-type stars. To this end, we employ synthetic stellar photospheric spectra combined with varying amounts of chromospheric emission and ISM absorption. We present the effect of ISM absorption on activity measurements by varying several ins…

Stars: activity010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstrophysicsStars: late-typeAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral linePlanets and satellites: general0103 physical sciencesHot JupiterAstrophysics::Solar and Stellar AstrophysicsAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesISM: generalPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Astronomy and AstrophysicsExoplanetStars: chromospheresStarsActivity measurementsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceStars: activity; Stars: chromospheres; Stars: late-type; ISM: general; Planets and satellites: generalAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Earth and Planetary Astrophysics
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Photometric and spectroscopic variability of the B5IIIe star HD 171219

2017

We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characteristics. Classical Be stars are main-sequence objects of mainly B-type, whose spectra show, or have shown at some epoch, Balmer lines in emission and an infrared excess. Both characteristics are attributed to an equatorially concentrated circumstellar disk fed by non-periodic mass-loss episodes (outbursts). Be stars often show nonradial pulsation gravity modes and, as more recently discovered, stochastically excited oscillations. Applying the CLEANEST algorithm to the high-cadence and highly photometrically precis…

Stars: individual: HD 171219Stars: emission-line BeAstrophysics::High Energy Astrophysical PhenomenaFísica matemàticaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineStars: early-typesymbols.namesakeearly-type [Stars]Stars: oscillationsStars: rotation0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsVariation (astronomy)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLine (formation)Physics[PHYS]Physics [physics]Infrared excess010308 nuclear & particles physicsASTROFÍSICA ESTELARBalmer seriesFísicaAstronomy and AstrophysicsoscillationsStars: rotation [Stars]Light curveCiència EnsenyamentStarsAstrophysics - Solar and Stellar Astrophysicsindividual: HD 171219 [Stars]emission-line Be [Stars]13. Climate actionSpace and Planetary ScienceExcited statesymbolsAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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