Search results for "dynamics."

showing 10 items of 9637 documents

Molecular Basis for Endocrine Disruption by Pesticides Targeting Aromatase and Estrogen Receptor

2020

The intensive use of pesticides has led to their increasing presence in water, soil, and agricultural products. Mounting evidence indicates that some pesticides may be endocrine disrupting chemicals (EDCs), being therefore harmful for the human health and the environment. In this study, three pesticides, glyphosate, thiacloprid, and imidacloprid, were tested for their ability to interfere with estrogen biosynthesis and/or signaling, to evaluate their potential action as EDCs. Among the tested compounds, only glyphosate inhibited aromatase activity (up to 30%) via a non-competitive inhibition or a mixed inhibition mechanism depending on the concentration applied. Then, the ability of the thr…

aromatasemedicine.drug_classHealth Toxicology and Mutagenesislcsh:MedicineEstrogen receptorMixed inhibitionEndocrine Disruptors010501 environmental sciencesPharmacology01 natural sciencesArticle03 medical and health scienceschemistry.chemical_compoundImidaclopridReceptorsmedicineHumansAromataseestrogenic activity030304 developmental biology0105 earth and related environmental sciences0303 health sciencesAromatase inhibitorendocrine disrupting chemicalbiologyAromatase Inhibitorslcsh:RPublic Health Environmental and Occupational HealthEstrogenspesticidesPesticideThiaclopridEstrogenmolecular dynamicsReceptors EstrogenchemistryEstrogenMELN allosteric inhibitionbiology.proteingene reporter assayAromatase; Endocrine disrupting chemical; Estrogen receptor; Estrogenic activity; Gene reporter assay; MELN allosteric inhibition; Molecular dynamics; Neonicotinoids; Pesticides; Aromatase; Aromatase Inhibitors; Estrogens; Humans; Receptors Estrogen; Endocrine Disruptors; Pesticidesneonicotinoidsestrogen receptorInternational Journal of Environmental Research and Public Health
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Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection

2020

Predicting the large-scale eruptions from the solar corona and their propagation through interplanetary space remains an outstanding challenge in solar- and helio-physics research. In this article, we describe three dimensional magnetohydrodynamic simulations of the inner heliosphere leading up to and including the extreme interplanetary coronal mass ejection (ICME) of 23 July 2012, developed using the code PLUTO. The simulations are driven using the output of coronal models for Carrington rotations 2125 and 2126 and, given the uncertainties in the initial conditions, are able to reproduce an event of comparable magnitude to the 23 July ICME, with similar velocity and density profiles at 1 …

astro-ph.SRSpace weather010504 meteorology & atmospheric sciencesMHDSolar windSTORMFOS: Physical sciencesMagnitude (mathematics)Context (language use)PROPAGATIONAstronomy & AstrophysicsDisturbancesSpace weatherPROTON01 natural sciencesEVENTSMagnetohydrodynamicsPhysics - Space Physicsphysics.plasm-ph0201 Astronomical and Space Sciences0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsScience & TechnologySUNAstronomy and AstrophysicsARRIVALGeophysicsEVOLUTIONSpace Physics (physics.space-ph)Physics - Plasma PhysicsPlasma Physics (physics.plasm-ph)PlutoSolar windAstrophysics - Solar and Stellar Astrophysicsphysics.space-ph13. Climate actionSpace and Planetary ScienceDragPhysical Sciencesastro-ph.EPMagnetohydrodynamicsInterplanetary coronal mass ejectionsHeliosphereAstrophysics - Earth and Planetary AstrophysicsSolar Physics
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The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon i

2017

Investigating the physical mechanisms driving the dynamical evolution of young star clusters is fundamental to our understanding of the star formation process and the properties of the Galactic field stars. The young (~2 Myr) and partially embedded cluster Chamaeleon I is one of the closest laboratories for the study of the early stages of star cluster dynamics in a low-density environment. The aim of this work is to study the structural and kinematical properties of this cluster combining parameters from the high-resolution spectroscopic observations of the Gaia-ESO Survey with data from the literature. Our main result is the evidence of a large discrepancy between the velocity dispersion …

astro-ph.SRStellar populationopen clustersand associations: individual: Chamaeleon IIndividual: Chamaeleon I [Open clusters and associations]Open clusters and associations: Individual: Chamaeleon I; Stars: Kinematics and dynamics; Stars: Pre-main sequence; Techniques: Spectroscopicastro-ph.GAstars: kinematics and dynamicsFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstars: pre-main sequence01 natural sciencesVirial theoremKinematics and dynamics [Stars]Stars: Kinematics and dynamic0103 physical sciencesCluster (physics)Mass segregationAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsStellar evolutionQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysicsPre-main sequence [Stars]open clusters and associations: individual: Chamaeleon I010308 nuclear & particles physicsVelocity dispersionAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxies[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]stars: kinematics and dynamics; stars: pre-main sequence; open clustersand associations: individual: Chamaeleon I; techniques: spectroscopicStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsSpectroscopic [Techniques]Equivalent widthtechniques: spectroscopicQB799
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Contribution of observed multi frequency spectrum of Alfvén waves to coronal heating

2019

Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves carry enough energy to maintain the thermal structure of the solar corona, it is not clear whether such energy can be efficiently and effectively converted into heating. Phase-mixing of Alfvén waves is considered a candidate mechanism, as it can develop transverse gradient where magnetic energy can be converted into thermal energy. However, phase-mixing is a process that crucially depends on the amplitude and period of the transverse oscillations, and only recently have we obtained a complete measurement of the power spectrum for transverse oscillations in the corona. Aims. We aim to investig…

atmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]T-NDASContext (language use)Astrophysics01 natural sciences03 medical and health sciences0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsSun: oscillationsQASun: magnetic fields010303 astronomy & astrophysicsQCQB030304 developmental biologyPhysics0303 health sciencesMagnetic energySun: coronaoscillations [Sun]Spectral densityAstronomy and AstrophysicsTransverse waveCoronal loopComputational physicsTransverse planeQC PhysicsAmplitudemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsSun: atmosphereAstronomy & Astrophysics
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L'Oscillation de Madden-Julian et la variabilité pluviométrique régionale en Afrique Subsaharienne

2007

The role of the Madden-Julian Oscillation ("MJO") on rainfall variability in Sub-Saharan Africa is examined, based on daily rain-gauge records and the NCEP-DOE AMIP-II reanalyses. The convective and dynamical signal associated with the MJO is extracted using two differing methodologies, the BMRC daily indices (Wheeler & Hendon 2004) on the one hand, and a Local Mode Analysis ("LMA", Goulet & Duvel 2000) on the other hand. The temporal variability of the MJO (in terms of period, amplitude, seasonality and location of the convective anomalies) is first analysed. Though the overall amplitude of the signal is not related to El Niño, the oscillations occurring under El Niño (La Niña) conditions …

atmospheric <br />dynamicsintraseasonal variabilityinteractions d'échelleSub-Saharan Africavariabilité intrasaisonnièrerainfall<br />dynamique atmosphériqueclimate diagnosticAfrique Subsaharienne[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/Climatology[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatologydiagnostic climatiqueMadden-Julian Oscillationpluviométriescale interactions[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyOscillation de Madden-Julian
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ELEKTROMAGNĒTISKI IETEKMĒTU HIDRODINAMISKO PROCESU EKSPERIMENTĀLI PĒTĪJUMI ŠĶIDRU METĀLU NOSLĒGTOS TILPUMOS

2014

Elektroniskā versija nesatur pielikumus

augstfrekvences magnētiskais lauksFizika materiālzinātne matemātika un statistikaŠķidrumu un gāzu mehānikamagnetic fieldfluid dynamicshigh frequencyšķidri metāliFizika astronomija un mehānikathermoelectricityMagnetohydrodynamicstermokapilārā konvekcijaMagnetohidrodinamikathermocapillary convectiontermoelektrībaFizikaliquid metals
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Estimates for Divergence Velocities of Axially Moving Orthotropic Thin Plates

2014

Some models for axially moving orthotropic thin plates are investigated analytically via methods of complex analysis to derive estimates for critical plate velocities. Linearised Kirchhoff plate theory is used, and the energy forms of steady-state models are considered with homogeneous and inhomogeneous tension profiles in the cross direction of the plate. With the help of the energy forms, some limits for the divergence velocity of the plate are found analytically. In numerical examples, the derived lower limits for the divergence velocity are analysed for plates with small flexural rigidity. peerReviewed

axially movingPhysics::Instrumentation and DetectorsGeneral MathematicsAerospace EngineeringOcean EngineeringGeometry02 engineering and technologyOrthotropic material01 natural sciencesPhysics::Fluid Dynamics0203 mechanical engineering0103 physical sciencesorthotropicta216Divergence (statistics)010301 acousticsCivil and Structural EngineeringMathematicsTension (physics)Mechanical Engineeringkalvot (biologia)Flexural rigidityMechanicsstabilityPhysics::Classical PhysicsCondensed Matter Physicslautaset (astiat)020303 mechanical engineering & transportsplatesmembranesMechanics of MaterialsHomogeneousAutomotive EngineeringPlate theoryAxial symmetryMechanics Based Design of Structures and Machines
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Comparison between simulated and observed LHC beam backgrounds in the ATLAS experiment at E beam =4 TeV

2018

Results of dedicated Monte Carlo simulations of beam-induced background (BIB) in the ATLAS experiment at the Large Hadron Collider (LHC) are presented and compared with data recorded in 2012. During normal physics operation this background arises mainly from scattering of the 4 TeV protons on residual gas in the beam pipe. Methods of reconstructing the BIB signals in the ATLAS detector, developed and implemented in the simulation chain based on the FLUKA Monte Carlo simulation package, are described. The interaction rates are determined from the residual gas pressure distribution in the LHC ring in order to set an absolute scale on the predicted rates of BIB so that they can be compared qua…

background [beam]background: inducedPhysics::Instrumentation and DetectorsCiencias FísicasMonte Carlo method01 natural sciencesHigh Energy Physics - ExperimentSubatomär fysik//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)beam lossesSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]and programsInstrumentationQCMathematical PhysicsPhysicsLarge Hadron ColliderRadiation calculationsAtlas (topology)Accelerator modelling and simulations (multi-particle dynamics; single-particle dynamics)DetectorATLAS experimentSettore FIS/01 - Fisica SperimentaleSimulation methods and programBeams (radiation) Accelerator modelling and simulations (multi-particle dynamics;; single-particle dynamics); Radiation calculations; Simulation methods; and programs; DETECTOR; SEARCHObservableAccelerator modelling and simulations (multi-particle dynamicMonte Carlo [numerical calculations]ATLASNuclear & Particles PhysicsAccelerator modelling and simulationsCERN LHC Coll collimators beam: backgroundcolliding beams [p p]numerical calculations: Monte CarloCIENCIAS NATURALES Y EXACTASParticle Physics - Experimentp p: scatteringAccelerator modelling and simulations (multi-particle dynamics; Radiation calculations; Simulation methods and programs; single-particle dynamics); Instrumentation; Mathematical Physics530 PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesFísica de Partículas y CamposAccelerator Physics and InstrumentationNuclear physicsFLUKAsingle-particle dynamics)ATLAS LHC High Energy PhysicsHIGH ENERGY PHYSICSSEARCH0103 physical sciencesddc:610010306 general physicsAbsolute scaleDETECTORpressure [gas]Science & Technology010308 nuclear & particles physicsScatteringhep-exRadiation calculationscatteringAcceleratorfysik och instrumentering//purl.org/becyt/ford/1.3 [https]ghostAccelerator modelling and simulations (multi-particle dynamicsSimulation methodscorrelationinduced [background]Experimental High Energy Physicsgas: pressureSimulation methods and programsp p: colliding beamsexperimental results
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Stochastic model for a biological complex system: analysis of the bacterial growth in food products

2012

The Physics of Complex Systems has recently taken a more and more important role in the description of natural systems because of the interactions, both deterministic and noisy, between such systems and the environment. In particular the noise plays a relevant role in biological systems, whose dynamics is strongly influenced by environmental variables subject to random fluctuations. In this work a stochastic model is exploited to reproduce the growth of bacteria in food of animal origin. Specifically the dynamics of a bacterial species, Listeria monocytogenes, is analyzed in the presence of lactic acid bacteria (LAB) during the period of the fermentation of meat products. The model, based o…

bacterial dynamicfood safetyPredictive microbiologyinterspecific competitionenvironmental noisestochastic modelSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Predictive microbiology; bacterial dynamics; interspecific competition; stochastic model; environmental noise; food safety
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Design of Reliable and Efficient Banki-Type Turbines

2020

A new shape for the external surface of the Crossflow turbine blades is proposed, which allows for the preservation of hydraulic efficiency in spite of a significant maximum blade thickness providing mechanic robustness and reliability. The final shape of the blades is assessed using an iterative solution for two uncoupled models: a 2D computational fluid dynamic (CFD) and a structural 3D finite element method (FEM) analysis of a single blade. Application of the proposed methodology to the design of a power recovery system (PRS) turbine, a new backpressure Crossflow-type inline turbine for pressure regulation, and energy production in a real Sicilian site follows.

banki turbinecrossflow turbineHydraulic efficiencyTurbine bladebusiness.industryComputer scienceMechanical engineeringComputational fluid dynamicsTurbineFinite element methodSettore ICAR/01 - Idraulicalaw.inventioncrossflow blade shapeRobustness (computer science)lawbusinessThe 4th EWaS International Conference: Valuing the Water, Carbon, Ecological Footprints of Human Activities
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