Search results for " naturale"

showing 10 items of 438 documents

Evaluación multicriterio de políticas de uso y gestión de recursos naturales

2014

The purpose of this work is show the characteristics of different environmental economic assessment methodologies, and exposes a case study where possible alternatives addressed to reduce the contamination of a bay with multicriteria approach are evaluated. The results obtained show the effectiveness of multicriteria analysis to evaluate the alternatives for solution of contamination problem in a bay. Economic evaluation of the contamination effects integrated to the environmental, social and economic dimensions through multicriteria techniques allows an alternative planning to solve the environmental problem studied, providing the right decision.

Valorização Econômica Ambiental; Métodos Multicritério; Recursos Naturais; Meio Ambiente.ComputingMethodologies_PATTERNRECOGNITIONValoración Económica Ambiental; Métodos Multicriterio; Recursos Naturales; Medio Ambiente.GeneticsAnimal Science and ZoologyEnvironmental Economic Valuation; Multicriteria Methods; Natural Resources; Environment.Revista Eletrônica de Estratégia & Negócios
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La Europa social / 3. Bután como modelo

2005

Vidal-Beneyto JoséEducaciónEsperanza de vidaEvaluación alternativaSaludIndicadores ecológicosCrecimientoDominante financieraPatrimonioAlfabetizaciónEUROPAEconomía realInmigrantesPráctica sanitariaViolencia domésticaPublicaciones: Obra periodística: Columnas y artículos de opiniónCostes naturalesSalud públicaECONOMÍAPobrezaEndeudamientoDefensa de la vidaContabilidad NacionalButánALTERNATIVASEconomía cualitativaRiquezaEuropa socialFelicidad colectivaFinanciarizaciónActividades culturalesTrabajo clandestinoCuentas NacionalesProgreso socialNecesidades básicasVida económicaSiniestralidad laboralLibertadMedio ambienteModelo liberal-conservadorBienestar
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Pyrosequencing vs. culture-dependent approaches to analyze lactic acid bacteria associated to chicha, a traditional maize-based fermented beverage fr…

2015

The diversity of lactic acid bacteria (LAB) associated with chicha, a traditional maize-based fermented alcoholicbeverage from Northwestern Argentina, was analyzed using culture-dependent and culture-independent approaches.Samples corresponding to 10 production steps were obtained from two local producers at Maimará(chicha M) and Tumbaya (chicha T). Whereas by culture-dependent approach a few number of species(Lactobacillus plantarum and Weissella viridescens in chicha M, and Enterococcus faecium and Leuconostocmesenteroides in chicha T) were identified, a higher quantitative distribution of taxa was found in both beveragesby pyrosequencing. The relative abundance of OTUs was higher in chic…

WeissellaCHICHAOtras Ciencias BiológicasLactococcusPopulationDIVERSITYArgentinaColony Count MicrobialPYROSEQUENCINGMicrobiologyPolymerase Chain ReactionZea maysMicrobiologyCiencias BiológicasBeveragesLACTIC ACID BACTERIALactobacillalesRNA Ribosomal 16SLactic acid bacteriaLeuconostoceducationDiversityeducation.field_of_studybiologyISR RAPD PROFILESfood and beveragesGeneral MedicineBiodiversitySequence Analysis DNAbiology.organism_classificationBacterial Typing TechniquesRandom Amplified Polymorphic DNA TechniqueLeuconostoc mesenteroidesSettore AGR/16 - MICROBIOLOGIA AGRARIAFermentationChichabacteria16S rRNA SEQUENCINGPediococcusIdentification by molecular techniques High-throughput sequencing (HTS)HIGH-TROUGHPUT SEQUENCING (HTS)CIENCIAS NATURALES Y EXACTASLactobacillus plantarumFood ScienceEnterococcus faeciumInternational journal of food microbiology
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Umbilical cord revisited: from Wharton’s jelly myofibroblasts to mesenchymal stem cells

2013

The umbilical cord (UC) is an essential part of the placenta, contributing to foetal development by ensuring the blood flow between mother and foetus. The UC is formed within the first weeks of gestation by the enclosure of the vessels (one vein and two arteries) into a bulk of mucous connective tissue, named Wharton’s jelly (WJ) and lined by the umbilical epithelium. Since their first identification, cells populating WJ were described as unusual fibroblasts (or myofibroblasts). Recent literature data further highlighted the functional interconnection between UC and the resident cells. The UC represents a reservoir of progenitor populations which are collectively grouped into MSCs (mesenchy…

Wharton’s jelly:5 - Ciencias puras y naturales::57 - Biología::576 - Biología celular y subcelular. Citología [CDU]Mesenchymal stem cellsUmbilical cord
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Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

2013

We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 – 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 – 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Ciencias FísicasAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesultra-high energy cosmic raysCosmic rayAstrophysicsultra high energy cosmic raysAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAugerNUMBERObservatoryCosmic ray experiments0103 physical sciencesultra-high energy cosmic rayUltra-high-energy cosmic ray010303 astronomy & astrophysicsDETECTORLuminosity functionPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)FÍSICA DE PARTÍCULASRange (particle radiation)SPECTRUMCosmologia010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsUltra high energy cosmic raysAstronomíaLUMINOSITY FUNCTIONMagnitude (astronomy)Experimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstronomiaFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical Phenomenacosmic ray experiments; ultra high energy cosmic raysCIENCIAS NATURALES Y EXACTAS
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Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory

2013

To interpret the mean depth of cosmic ray air shower maximum and its dispersion, we parametrize those two observables as functions of the first two moments of the ln A distribution. We examine the goodness of this simple method through simulations of test mass distributions. The application of the parameterization to Pierre Auger Observatory data allows one to study the energy dependence of the mean ln A and of its variance under the assumption of selected hadronic interaction models. We discuss possible implications of these dependences in term of interaction models and astrophysical cosmic ray sources.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Ciencias FísicasAstronomyAstrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesCosmic rayultra high energy cosmic rays01 natural sciencesultra high energy cosmic rayInterpretation (model theory)//purl.org/becyt/ford/1 [https]Nuclear physics0103 physical sciencesPARTICLES010306 general physicsDispersion (water waves)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryCOMPOSICIÓN DE MASAEXPERIMENTO AUGER010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsObservableASTROFÍSICA//purl.org/becyt/ford/1.3 [https]RAYOS COSMICOSAstronomíaENERGY COSMIC-RAYSMODELDistribution (mathematics)Air showerParticlesUltra High Energy Cosmic RaysExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGEnergy cosmic-raysFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASSimulationcosmic ray experiments; ultra high energy cosmic raysModel
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Identifying clouds over the Pierre Auger Observatory using infrared satellite data

2013

We describe a new method of identifying night-time clouds over the Pierre Auger Observatory using infrared data from the Imager instruments on the GOES-12 and GOES-13 satellites. We compare cloud. identifications resulting from our method to those obtained by the Central Laser Facility of the Auger Observatory. Using our new method we can now develop cloud probability maps for the 3000 km(2) of the Pierre Auger Observatory twice per hour with a spatial resolution of similar to 2.4 km by similar to 5.5 km. Our method could also be applied to monitor cloud cover for other ground-based observatories and for space-based observatories. (C) 2013 Elsevier B.V. All rights reserved.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Atmospheric MonitoringSatellitesInfraredAstronomyCloud coverFOS: Physical sciencesAtmospheric monitoring01 natural sciencesCiencias de la Tierra y relacionadas con el Medio AmbienteAuger//purl.org/becyt/ford/1 [https]//purl.org/becyt/ford/1.5 [https]ObservatoryClouds0103 physical sciencesExtensive air showers010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Image resolutionCiencias ExactasPhysicsPierre Auger ObservatoryUHE Cosmic Rays atmosphere010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomyPierre Auger ObservatoryAstronomy and AstrophysicsUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]INFRAVERMELHOExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGPierre Auger observatoryultra-high energy cosmic rays; Pierre Auger Observatory; extensive air showers; atmospheric monitoring; clouds; satellitesFísica nuclearSatelliteCentral Laser FacilityExtensive Air ShowersAstrophysics - Instrumentation and Methods for AstrophysicsMeteorología y Ciencias AtmosféricasSYSTEMCIENCIAS NATURALES Y EXACTASAstroparticle Physics
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Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

2015

We analyze the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to $80^\circ$, thus covering from $-90^\circ$ to $+45^\circ$ in declination. After updating the fraction of events correlating with the active galactic nuclei (AGNs) in the V��ron-Cetty and V��ron catalog, we subject the arrival directions of the data with energies in excess of 40 EeV to different tests for anisotropy. We search for localized excess fluxes and for self-clustering of event directions at angular scales up t…

acceleration of particles; astroparticle physicsNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Upper LimitAstronomyCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias Físicas01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareSettore FIS/05 - Astronomia e AstrofisicaObservatorySpectrum0103 physical sciencesacceleration of particles astroparticle physicsSurface Detector010303 astronomy & astrophysicsacceleration of particleAstrophysics::Galaxy Astrophysicsacceleration of particlesPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleArrayAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicAstronomy and AstrophysicsASTROFÍSICANucleiSpace and Planetary Scienceastroparticle physicsExperimental High Energy Physicsacceleration of particles; astroparticle physics; Nuclear and High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearCatalogSkyAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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La interpretación de los riesgos naturales y el cambio climático en postgrado. Ejemplos de casos de estudio en la provincia de Alicante (España)

2020

Esta investigación tiene el objetivo de exponer una experiencia didáctica sobre la interpretación de los riesgos naturales y el cambio climático a partir de la propuesta de diferentes estudios de caso de la provincia de Alicante (España). Dicha propuesta se lleva a cabo en la asignatura de Cambio Climático y Riesgo en el Mediterráneo del Máster en Planificación y Gestión de Riesgos Naturales (Universidad de Alicante). Metodológicamente se han expuesto diferentes ejemplos de análisis sobre las temáticas de: 1) Las sequías; 2) La explotación y sangrado de cursos fluviales; 3) Tendencias climáticas; y 4) Medidas de adaptación al cambio climático. Con estos ejemplos se pretende que los discente…

alicante.ahmad s. & numan s.m. (2015). potentiality of disaster management education through open and distance learning system in bangladesh open university vol. 16 (1) pp. 249-260. alberola:GEOGRAFÍA [UNESCO]experiencia didácticalcsh:G1-922cambio climáticolcsh:Geography (General)UNESCO::GEOGRAFÍAriesgos naturalesCuadernos de Geografía de la Universitat de València
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Direct C-H metalation with chromium(ii) and iron(ii): transition- metal host/benzenediide guest magnetic inverse-crown complexes

2009

Check M(etal)ate: The chessboard and the figures represent a special reaction in which different low-polarity metals can metalate arenes directly when they are brought into the right position. In a combination of queen (sodium) and knight (chromium or iron), it is possible for the knight (usually the weaker piece) to make a direct deadly hit on the king (benzene) in this game of elemental chess. Fil: Alborés, Pablo. Johannes Gutenberg Universitat Mainz; Alemania. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Carrella, Luca M.. Johannes Gutenberg Universitat Mainz; Alemania Fil: Clegg, William. University of Newcastle; Reino Unido Fil: García Álvarez, Pablo. Univ…

alkali metalsMetalationchemistry.chemical_elementMineralogyALKALI METALSmetalationCatalysisQueen (playing card)Chromiumchemistry.chemical_compoundironTransition metalCHROMIUMinverse crown compoundsBenzeneIRONOtras Ciencias QuímicasCiencias QuímicasGeneral ChemistryAlkali metalCommunicationsCrystallographychemistrychromiumINVERSE CROWN COMPOUNDSCIENCIAS NATURALES Y EXACTAS
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