Search results for "SCAD"

showing 10 items of 348 documents

SECURE SOLUTION FOR MODERN SEMANTIC SCADA

2013

International audience; NOUS TRAVAILLONS SUR LA SECURITE DES SYSTEMES SCADA (SUPERVI-SORY CONTROL AND DATA AQUISITION) MODERNE EXPLOITANT DES EQUI-PEMENTS MODRNE AVEC DE L’INTELLIGENCE EMBARQUE COMME LES RTU (REMOTE TERMINAL UNIT), LES CAPTEURSINTELLIGENTS, LES ACTIONNEURS INTELLIGENTS, LES EQUIPEMENTS DE L’INSTRUMENTATION GAZIERE MODERNE COMME LES COMPTEURS NUME-RIQUE, LES CORECTEURS ELECTONIQUE, LES POMPES DOSEUSES AVEC CARTE ELECTRONIQUE, LES CHROMATOGRAPHES...ECT. AVEC LES AVANCES TECHNLOGIQUES DE L’INFORMATIQUE EMBARQUE COMME LES SERVICES WEB ET LES APPLICATION CONCU SELON LES ARCHITECTURES MODERNE (SOA- SERVICE ORIENTED ARCHITECTURE), LES ONTOLOGIES ET LE WEB SEMANTIQUE, LES BASES DE …

[INFO.INFO-NI]Computer Science [cs]/Networking and Internet Architecture [cs.NI][INFO.INFO-NI] Computer Science [cs]/Networking and Internet Architecture [cs.NI][ INFO.INFO-NI ] Computer Science [cs]/Networking and Internet Architecture [cs.NI](IT-SCADA) PLATFORMSCADASECURITY PROTOCOL
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Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

2009

From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (at 95% c.l.) are obtained on the fraction of cosmic-ray photons above 2, 3, 5 and 10 EeV (1 EeV equivalent to 10(18) eV), respectively. These are the first experimental limits on ultra-high energy photons at energies below 10 EeV. The results complement previous constraints on top-down models from array data and they reduce systematic uncertainties in the interpretation of shower data in terms of primary flux, nuclear composition and proton-air cross-section.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhotonAstronomyFOS: Physical sciencesFluxCosmic rayFotonesAstrophysicsEXTENSIVE AIR-SHOWERS01 natural sciences7. Clean energyNuclear physicsCascada atmosféricaUltra high energy (UHE)0103 physical sciencesLimit (mathematics)FLUORESCENCEUltra-high energy cosmic ray010303 astronomy & astrophysicsDETECTORCosmic raysCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysics010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomy and AstrophysicsPierre Auger ObservatoryPROFILESRadiación cósmicaPhotonLongitudinal development13. Climate actionphoton fractionComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical Phenomena
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Search for neutrino-induced cascades with five years of AMANDA data

2010

Contains fulltext : 97339.pdf (Publisher’s version ) (Closed access) We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of v(e):v(mu):v(tau) = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Phi proportional to E(-2) is less than 5.0 x…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHadronFluxCosmic rayContext (language use)Cascades; NeutrinosAstrophysicsAetiology screening and detection [ONCOL 5]01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Cascades0103 physical sciencesNeutrinos010306 general physicsPhysicsFluxMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyAstronomy and AstrophysicsCosmic-RaysNucleiHigh-Energy NeutrinosNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory

2009

Atmospheric parameters, such as pressure (P), temperature (T) and density (ρ ∝ P/T), affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a ∼ 10% seasonal modulation and ∼ 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and ρ. The former affects the longitudinal development of air showers while the latter influences the Molière radius and hence the lateral distribution of the shower particles. The model is val…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]: 96.50.sdRadiación CósmicaIMPACTAstronomyExtensive air showerFOS: Physical sciencesCosmic rayAstrophysicsExtensive air showers; UHECR; Atmosphere; Weather01 natural sciencesCOSMIC-RAY CASCADESAugerAtmosphereENERGYObservatory0103 physical sciencesExtensive air showersRECONSTRUCTION96.50.sf010303 astronomy & astrophysicsMolière radiusWeatherInstrumentation and Methods for Astrophysics (astro-ph.IM)96.50.sbPierre Auger ObservatoryPhysics010308 nuclear & particles physicsAtmosphereUHECRDetectorFísicaAstronomy and AstrophysicsPresión AtmosféricaPROFILES[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Longitudinal developmentATMOSFERA (ESTUDO)13. Climate actionExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGClimaAstrophysics - Instrumentation and Methods for Astrophysics
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Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector

2010

The ANTARES high energy neutrino telescope is a three-dimensional array of about 900 photomultipliers distributed over 12 mooring lines installed in the Mediterranean Sea. Between February and November 2007 it acquired data in a 5-line configuration. The zenith angular distribution of the atmospheric muon flux and the associated depth-intensity relation are measured and compared with previous measurements and Monte Carlo expectations. An evaluation of the systematic effects due to uncertainties on environmental and detector parameters is presented.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsMonte Carlo methodAtmospheric muonsFluxNeutrino telescope01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)WATER010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)DetectorAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAY CASCADES NEUTRINO TELESCOPE PERFORMANCE GENERATOR SYSTEM MODULE LIGHT WATER SITESITEMUON FLUXLIGHTddc:540Física nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsMODULEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayParticle detectorCOSMIC-RAY CASCADESNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]depth-intensity relation0103 physical sciencesatmospheric muons; depth-intensity relation; neutrino telescope14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithRemote sensingatmospheric muonsDepth-intensity relation010308 nuclear & particles physicsneutrino telescopeAstronomy and AstrophysicsCOSMIC RAYSPERFORMANCEGENERATORMeasuring instrumentHigh Energy Physics::ExperimentUNDERWATER DETECTORSYSTEM
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Pharmacogenomic identification of small molecules for lineage specific manipulation of subventricular zone germinal activity

2017

Strategies for promoting neural regeneration are hindered by the difficulty of manipulating desired neural fates in the brain without complex genetic methods. The subventricular zone (SVZ) is the largest germinal zone of the forebrain and is responsible for the lifelong generation of interneuron subtypes and oligodendrocytes. Here, we have performed a bioinformatics analysis of the transcriptome of dorsal and lateral SVZ in early postnatal mice, including neural stem cells (NSCs) and their immediate progenies, which generate distinct neural lineages. We identified multiple signaling pathways that trigger distinct downstream transcriptional networks to regulate the diversity of neural cells …

animal diseasesGene Identification and AnalysisGenetic NetworksAPC-PAIDMiceNeural Stem CellsCell SignalingLateral VentriclesDatabases GeneticGene Regulatory NetworksBiology (General)WNT Signaling CascadeNotch SignalingOrganic CompoundsBB/M029379/1GenomicsSignaling CascadesOligodendrogliaChemistryBBSRCPhysical Sciences[SDV.NEU]Life Sciences [q-bio]/Neurons and Cognition [q-bio.NC]Network AnalysisNeurovetenskaperSignal TransductionResearch ArticleBiotechnologyComputer and Information SciencesSignal InhibitionQH301-705.5NeurogenesisResearch and Analysis MethodsSmall Molecule LibrariesGenetics/dk/atira/pure/core/subjects/biomedicalsciencesAnimalsAdultsCell LineageComputer Simulation[SDV.NEU] Life Sciences [q-bio]/Neurons and Cognition [q-bio.NC]Molecular Biology TechniquesMolecular BiologyOrganic ChemistryGene MappingChemical CompoundsNeurosciencesBiology and Life SciencesRCUKBiomedical SciencesCell BiologyNerve RegenerationSignaling NetworksGene Expression Regulationnervous systemSmall MoleculesAge GroupsPeople and PlacesPopulation GroupingsTranscriptome
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Cabut, a C2H2 zinc finger transcription factor, is required during Drosophila dorsal closure downstream of JNK signaling.

2005

AbstractDuring dorsal closure, the lateral epithelia on each side of the embryo migrate dorsally over the amnioserosa and fuse at the dorsal midline. Detailed genetic studies have revealed that many molecules are involved in this epithelial sheet movement, either with a signaling function or as structural or motor components of the process. Here, we report the characterization of cabut (cbt), a new Drosophila gene involved in dorsal closure. cbt is expressed in the yolk sac nuclei and in the lateral epidermis. The Cbt protein contains three C2H2-type zinc fingers and a serine-rich domain, suggesting that it functions as a transcription factor. cbt mutants die as embryos with dorsal closure …

animal structuresMorphogenesisBiologyCabutZinc fingerMorphogenesismedicineAnimalsDrosophila ProteinsDorsal closureYolk sacMolecular BiologyTranscription factorYolk nucleiCytoskeletonGeneticsZinc fingerEpidermis (botany)C2H2 Zinc FingerJNK Mitogen-Activated Protein KinasesZinc FingersCell BiologyDorsal closureCell biologymedicine.anatomical_structureDrosophila melanogasterEpidermal Cellsembryonic structuresMutationJNK cascadeDrosophilaJNKDevelopmental BiologySignal TransductionTranscription FactorsDevelopmental biology
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Plexin-B1 activates NF-κB and IL-8 to promote a pro-angiogenic response in endothelial cells.

2011

Background The semaphorins and their receptors, the plexins, are proteins related to c-Met and the scatter factors that have been implicated in an expanding signal transduction network involving co-receptors, RhoA and Ras activation and deactivation, and phosphorylation events. Our previous work has demonstrated that Semaphorin 4D (Sema4D) acts through its receptor, Plexin-B1, on endothelial cells to promote angiogenesis in a RhoA and Akt-dependent manner. Since NF-κB has been linked to promotion of angiogenesis and can be activated by Akt in some contexts, we wanted to examine NF-κB in Sema4D treated cells to determine if there was biological significance for the pro-angiogenic phenotype o…

animal structuresRHOAProto-Oncogene Proteins c-aktAngiogenesisSignaling in cellular processesG-protein signalingCancer TreatmentSEMA4Dlcsh:MedicineSignal transductionBiology03 medical and health sciencesMolecular cell biology0302 clinical medicineSemaphorinSettore BIO/10 - BiochimicaAkt Signaling CascadeMembrane Receptor SignalingInterleukin 8lcsh:ScienceBiologyProtein kinase BGTPase signalingRas signaling030304 developmental biology0303 health sciencesMultidisciplinaryMechanisms of Signal Transductionlcsh:RSignaling Cascades3. Good healthCell biologyPlexin B1RNA interferencepro-angiogenicendothelial cellsOncology030220 oncology & carcinogenesisembryonic structuresCancer researchbiology.proteinMedicinelcsh:QAntiangiogenesis TherapyAntiapoptotic signalingSignal transductionResearch ArticlePLoS ONE
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Cargamentos de conservas de pescado béticas en el Mediterráneo Occidental durante la época Julio-Claudia

2023

A lo largo del Alto Imperio, la ciudad de Roma cuenta con aproximadamente un millón de habitantes, población que no igualará ninguna otra ciudad europea hasta el Londres del siglo XVIII, ni ninguna otra ciudad mediterránea hasta el Estambul del siglo XX. Con el fin de preservar su estabilidad, el Estado ha de atender tanto a las necesidades alimenticias de la megalópolis, como a las de las de las legiones diseminadas en las fronteras del Imperio. En este contexto, las provincias romanas como la Bética (actual Andalucía grosso modo) contribuyeron al aprovisionamiento alimenticio de la plebs y el ejército, implicando en ello numerosos barcos para la rápida y eficiente exportación de sus biene…

bou ferrerdressel 9dressel 8dressel 7dressel 14dressel 7/11dressel 12peciodressel 10dressel 11salsassalazonesépoca Julio-Claudiacediterráneo occidentalpescadobeltrán IIAdressel 17beltrán IIBbéticailles formigues IIUNESCO::HISTORIA::Ciencias auxiliares de la historia::Arqueología
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Ensemble feature selection with the simple Bayesian classification

2003

Abstract A popular method for creating an accurate classifier from a set of training data is to build several classifiers, and then to combine their predictions. The ensembles of simple Bayesian classifiers have traditionally not been a focus of research. One way to generate an ensemble of accurate and diverse simple Bayesian classifiers is to use different feature subsets generated with the random subspace method. In this case, the ensemble consists of multiple classifiers constructed by randomly selecting feature subsets, that is, classifiers constructed in randomly chosen subspaces. In this paper, we present an algorithm for building ensembles of simple Bayesian classifiers in random sub…

business.industryBayesian probabilityFeature selectionPattern recognitionMachine learningcomputer.software_genreLinear subspaceRandom subspace methodNaive Bayes classifierBayes' theoremComputingMethodologies_PATTERNRECOGNITIONHardware and ArchitectureSignal ProcessingArtificial intelligencebusinesscomputerClassifier (UML)SoftwareCascading classifiersInformation SystemsMathematicsInformation Fusion
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