Search results for " nucleus"

showing 10 items of 1270 documents

The Origin of Isolated Populations of the Mountain Weevil, Liparus glabrirostris—The Flagship Species for Riparian Habitats

2020

AbstractLiparus glabrirostris is one of the largest European weevils, and it has been recently proposed as the flagship species for threatened riparian habitats in the mountains. For effective conservation of its populations (and associated habitats), it is crucial to understand its history, contemporary distribution, genetic diversity and predict changes in the range, including its highly isolated populations on the Baltic coast. Here, we examined numerous populations of L. glabrirostris across almost the entire species range using phylogeography and species niche modeling (SNM) approaches. Analyses of mtDNA and nucDNA markers revealed the existence of 2 major mitochondrial lineages genera…

Conservation geneticsGenetic MarkersConservation of Natural ResourcesRange (biology)Species distributionBiologyphylogeographyspecies distribution modelingDNA MitochondrialCurculionidaeGeneticsFlagship speciesAnimalsMolecular BiologyGenetics (clinical)EcosystemRiparian zoneCell Nucleusgeographygeography.geographical_feature_categoryEcologyEnvironmental niche modellingEuropeColeopteraPhylogeographyGenetics PopulationRefugiumconservation geneticsThreatened speciesWeevilsBiotechnologyJournal of Heredity
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Aryl hydrocarbon receptor activation by cAMP vs. dioxin: divergent signaling pathways.

2005

Even before the first vertebrates appeared on our planet, the aryl hydrocarbon receptor ( AHR ) gene was present to carry out one or more critical life functions. The vertebrate AHR then evolved to take on functions of detecting and responding to certain classes of environmental toxicants. These environmental pollutants include polycyclic aromatic hydrocarbons (e.g., benzo[ a ]pyrene), polyhalogenated hydrocarbons, dibenzofurans, and the most potent small-molecular-weight toxicant known, 2,3,7,8-tetrachlorodibenzo- p -dioxin (TCDD or dioxin). After binding of these ligands, the activated AHR translocates rapidly from the cytosol to the nucleus, where it forms a heterodimer with aryl hydroc…

Conservation of Natural ResourcesAryl hydrocarbon receptor nuclear translocatorPolychlorinated DibenzodioxinsTime FactorsTranscription GeneticGenetic VectorsGreen Fluorescent ProteinsImmunoblottingActive Transport Cell NucleusEnvironmentDioxinsLigandschemistry.chemical_compoundMiceCytosolGenes ReporterCell Line TumorCyclic AMPAnimalsImmunoprecipitationReceptorFluorescent Antibody Technique IndirectCell NucleusMultidisciplinarybiologyChemistryColforsinEndogenous mediatorrespiratory systemBiological SciencesAryl hydrocarbon receptorCyclic AMP-Dependent Protein KinasesCytosolProtein TransportBiochemistryBucladesineMicroscopy FluorescenceReceptors Aryl HydrocarbonSecond messenger systembiology.proteinProstaglandinsEnvironmental PollutantsSignal transductionDimerizationToxicantPlasmidsProtein BindingSignal TransductionProceedings of the National Academy of Sciences of the United States of America
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Intercomparing different devices for the investigation of ice nucleating particles using Snomax<sup>®</sup> as test subst…

2015

Abstract. Seven different instruments and measurement methods were used to examine the immersion freezing of bacterial ice nuclei from Snomax® (hereafter Snomax), a product containing ice-active protein complexes from non-viable Pseudomonas syringae bacteria. The experimental conditions were kept as similar as possible for the different measurements. Of the participating instruments, some examined droplets which had been made from suspensions directly, and the others examined droplets activated on previously generated Snomax particles, with particle diameters of mostly a few hundred nanometers and up to a few micrometers in some cases. Data were obtained in the temperature range from −2 to …

Contact angleAtmospheric ScienceRange (particle radiation)CrystallographyChemistrySlow coolingIce nucleusAnalytical chemistryParticleNanometreOrders of magnitude (numbers)Atmospheric temperature rangeAtmospheric Chemistry and Physics
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Small ice particles at slightly supercooled temperatures in tropical maritime convection

2020

In this paper we show that the origin of the ice phase in tropical cumulus clouds over the sea may occur by primary ice nucleation of small crystals at temperatures just between 0 and −5 ∘C. This was made possible through use of a holographic instrument able to image cloud particles at very high resolution and small size (6 µm). The environment in which the observations were conducted was notable for the presence of desert dust advected over the ocean from the Sahara. However, there is no laboratory evidence to suggest that these dust particles can act as ice nuclei at temperatures warmer than about −10 ∘C, the zone in which the first ice was observed in these clouds. T…

ConvectionAtmospheric Science010504 meteorology & atmospheric sciencesAtmospheric sciences01 natural scienceslcsh:QC1-999010309 opticslcsh:Chemistrylcsh:QD1-99913. Climate actionPhase (matter)0103 physical sciencesIce nucleusEnvironmental sciencePrecipitationGlacial periodDiffusion (business)SupercoolingDesert dustlcsh:Physics0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Numerical sensitivity studies on the impact of aerosol properties and drop freezing modes on the glaciation, microphysics, and dynamics of clouds

2006

[1] Numerical simulations were performed to investigate the effects of drop freezing in immersion and contact modes for a convective situation. For the description of heterogeneous drop freezing, new approaches were used considering the significantly different ice nucleating efficiencies of various ice nuclei. An air parcel model with a sectional two-dimensional description of the cloud microphysics was employed. Sensitivity studies were undertaken by varying the insoluble particle types as well as the soluble fraction of the aerosol particles showing the effects of these parameters on drop freezing and their possible impact on the vertical cloud dynamics. The soluble fraction ɛ decides whe…

ConvectionAtmospheric ScienceMaterials scienceNuclear TheorySoil ScienceMineralogyAquatic ScienceOceanographyGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Nuclear ExperimentPhysics::Atmospheric and Oceanic PhysicsEarth-Surface ProcessesWater Science and TechnologyEcologyMicrophysicsDrop (liquid)PaleontologyCloud physicsForestryMechanicsFreezing pointAerosolGeophysicsSpace and Planetary ScienceIce nucleusFreezing-point depressionJournal of Geophysical Research
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Ice Initiation for Various Ice Nuclei Types and its Infl uence on Precipitation Formation in Convective Clouds

2007

ConvectionIce nucleusConvective cloudPrecipitationAtmospheric sciencesGeology
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Model emulation to understand the joint effects of ice-nucleating particles and secondary ice production on deep convective anvil cirrus

2021

Abstract. Ice crystal formation in the mixed-phase region of deep convective clouds can affect the properties of climatically important convectively generated anvil clouds. Small ice crystals in the mixed-phase cloud region can be formed by heterogeneous ice nucleation by ice-nucleating particles (INP) and secondary ice production (SIP) by, for example, the Hallett-Mossop process. We quantify the effects of INP number concentration, the temperature dependence of the INP number concentration at mixedphase temperatures, and the Hallett-Mossop splinter production efficiency on the anvil of an idealised deep convective cloud using a Latin hypercube sampling method, which allows optimal coverage…

ConvectionMass fluxAtmospheric ScienceMaterials scienceIce crystalsPhysicsQC1-999AerosolPhysics::GeophysicsChemistryDeposition (aerosol physics)Chemical physicsIce nucleusParticleCirrusQD1-999Physics::Atmospheric and Oceanic PhysicsAtmospheric Chemistry and Physics
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High-spin levels in 63 145 Eu82

1996

The level scheme of theN=82 nucleus145Eu has been extended toI=(55/2) andEx=11.2 MeV in an experiment with the Tessa Compton-suppressed Ge detector array using the127I(22Ne,4n) reaction. Most of the complicated and irregular level scheme of145Eu can be interpreted as proton multi-quasiparticle states in comparison to the64146Gd82 core nucleus but also excitations across the neutronN=82 core have been observed.

Core (optical fiber)PhysicsNuclear and High Energy PhysicsProtonHalo nucleusDetector arrayAtomic physicsSpin-½Zeitschrift für Physik A: Hadrons and Nuclei
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Studies of Relativistic Jets in Active Galactic Nuclei with SKA

2014

Relativistic jets in active galactic nuclei (AGN) are among the most powerful astrophysical objects discovered to date. Indeed, jetted AGN studies have been considered a prominent science case for SKA, and were included in several different chapters of the previous SKA Science Book (Carilli & Rawlings 2004). Most of the fundamental questions about the physics of relativistic jets still remain unanswered, and await high-sensitivity radio instruments such as SKA to solve them. These questions will be addressed specially through analysis of the massive data sets arising from the deep, all-sky surveys (both total and polarimetric flux) from SKA1. Wide-field very-long-baseline-interferometri…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleus010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsJet (particle physics)01 natural sciencesAstrophysical jet0103 physical sciencesVery-long-baseline interferometryInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsStar formationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstrophysics - Astrophysics of GalaxiesGalaxyCharacterization (materials science)13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Brightness temperatureAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsProceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14)
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Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping

2015

By means of zoom-in hydrodynamic simulations we quantify the amount of neutral hydrogen (HI) hosted by groups and clusters of galaxies. Our simulations, which are based on an improved formulation of smoothed particle hydrodynamics (SPH), include radiative cooling, star formation, metal enrichment and supernova feedback, and can be split in two different groups, depending on whether feedback from active galactic nuclei (AGN) is turned on or off. Simulations are analyzed to account for HI self-shielding and the presence of molecular hydrogen. We find that the mass in neutral hydrogen of dark matter halos monotonically increases with the halo mass and can be well described by a power-law of th…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsmiscellaneous [cosmology]01 natural sciences7. Clean energymethods: numericalSettore FIS/05 - Astronomia e Astrofisicamethods: numerical; galaxies: clusters: general; cosmology: miscellaneous0103 physical sciencesclusters: general [galaxies]010303 astronomy & astrophysicsGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsStar formationAstronomynumerical [methods]Astronomy and AstrophysicsCosmology: Miscellaneous; Galaxies: Clusters: General; Methods: NumericalAstrophysics - Astrophysics of GalaxiesGalaxyRedshiftSupernovagalaxies: clusters: general13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Halocosmology: miscellaneousAstrophysics - Cosmology and Nongalactic Astrophysics
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