981 resultados para Propeller Jets, Scour, Ports, Dock and Harbours, Hydraulics


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Un escenario habitualmente considerado para el uso sostenible y prolongado de la energa nuclear contempla un parque de reactores rpidos refrigerados por metales lquidos (LMFR) dedicados al reciclado de Pu y la transmutacin de actnidos minoritarios (MA). Otra opcin es combinar dichos reactores con algunos sistemas subcrticos asistidos por acelerador (ADS), exclusivamente destinados a la eliminacin de MA. El diseo y licenciamiento de estos reactores innovadores requiere herramientas computacionales prcticas y precisas, que incorporen el conocimiento obtenido en la investigacin experimental de nuevas configuraciones de reactores, materiales y sistemas. A pesar de que se han construido y operado un cierto nmero de reactores rpidos a nivel mundial, la experiencia operacional es todava reducida y no todos los transitorios se han podido entender completamente. Por tanto, los anlisis de seguridad de nuevos LMFR estn basados fundamentalmente en mtodos deterministas, al contrario que las aproximaciones modernas para reactores de agua ligera (LWR), que se benefician tambin de los mtodos probabilistas. La aproximacin ms usada en los estudios de seguridad de LMFR es utilizar una variedad de cdigos, desarrollados a base de distintas teoras, en busca de soluciones integrales para los transitorios e incluyendo incertidumbres. En este marco, los nuevos cdigos para clculos de mejor estimacin ("best estimate") que no incluyen aproximaciones conservadoras, son de una importancia primordial para analizar estacionarios y transitorios en reactores rpidos. Esta tesis se centra en el desarrollo de un cdigo acoplado para realizar anlisis realistas en reactores rpidos crticos aplicando el mtodo de Monte Carlo. Hoy en da, dado el mayor potencial de recursos computacionales, los cdigos de transporte neutrnico por Monte Carlo se pueden usar de manera prctica para realizar clculos detallados de ncleos completos, incluso de elevada heterogeneidad material. Adems, los cdigos de Monte Carlo se toman normalmente como referencia para los cdigos deterministas de difusin en multigrupos en aplicaciones con reactores rpidos, porque usan secciones eficaces punto a punto, un modelo geomtrico exacto y tienen en cuenta intrnsecamente la dependencia angular de flujo. En esta tesis se presenta una metodologa de acoplamiento entre el conocido cdigo MCNP, que calcula la generacin de potencia en el reactor, y el cdigo de termohidrulica de subcanal COBRA-IV, que obtiene las distribuciones de temperatura y densidad en el sistema. COBRA-IV es un cdigo apropiado para aplicaciones en reactores rpidos ya que ha sido validado con resultados experimentales en haces de barras con sodio, incluyendo las correlaciones ms apropiadas para metales lquidos. En una primera fase de la tesis, ambos cdigos se han acoplado en estado estacionario utilizando un mtodo iterativo con intercambio de archivos externos. El principal problema en el acoplamiento neutrnico y termohidrulico en estacionario con cdigos de Monte Carlo es la manipulacin de las secciones eficaces para tener en cuenta el ensanchamiento Doppler cuando la temperatura del combustible aumenta. Entre todas las opciones disponibles, en esta tesis se ha escogido la aproximacin de pseudo materiales, y se ha comprobado que proporciona resultados aceptables en su aplicacin con reactores rpidos. Por otro lado, los cambios geomtricos originados por grandes gradientes de temperatura en el ncleo de reactores rpidos resultan importantes para la neutrnica como consecuencia del elevado recorrido libre medio del neutrn en estos sistemas. Por tanto, se ha desarrollado un mdulo adicional que simula la geometra del reactor en caliente y permite estimar la reactividad debido a la expansin del ncleo en un transitorio. ste mdulo calcula automticamente la longitud del combustible, el radio de la vaina, la separacin de los elementos de combustible y el radio de la placa soporte en funcin de la temperatura. ste efecto es muy relevante en transitorios sin insercin de bancos de parada. Tambin relacionado con los cambios geomtricos, se ha implementado una herramienta que, automatiza el movimiento de las barras de control en busca d la criticidad del reactor, o bien calcula el valor de insercin axial las barras de control. Una segunda fase en la plataforma de clculo que se ha desarrollado es la simulaci dinmica. Puesto que MCNP slo realiza clculos estacionarios para sistemas crticos o supercrticos, la solucin ms directa que se propone sin modificar el cdigo fuente de MCNP es usar la aproximacin de factorizacin de flujo, que resuelve por separado la forma del flujo y la amplitud. En este caso se han estudiado en profundidad dos aproximaciones: adiabtica y quasiesttica. El mtodo adiabtico usa un esquema de acoplamiento que alterna en el tiempo los clculos neutrnicos y termohidrulicos. MCNP calcula el modo fundamental de la distribucin de neutrones y la reactividad al final de cada paso de tiempo, y COBRA-IV calcula las propiedades trmicas en el punto intermedio de los pasos de tiempo. La evolucin de la amplitud de flujo se calcula resolviendo las ecuaciones de cintica puntual. Este mtodo calcula la reactividad esttica en cada paso de tiempo que, en general, difiere de la reactividad dinmica que se obtendra con la distribucin de flujo exacta y dependiente de tiempo. No obstante, para entornos no excesivamente alejados de la criticidad ambas reactividades son similares y el mtodo conduce a resultados prcticos aceptables. Siguiendo esta lnea, se ha desarrollado despus un mtodo mejorado para intentar tener en cuenta el efecto de la fuente de neutrones retardados en la evolucin de la forma del flujo durante el transitorio. El esquema consiste en realizar un clculo cuasiestacionario por cada paso de tiempo con MCNP. La simulacin cuasiestacionaria se basa EN la aproximacin de fuente constante de neutrones retardados, y consiste en dar un determinado peso o importancia a cada ciclo computacial del clculo de criticidad con MCNP para la estimacin del flujo final. Ambos mtodos se han verificado tomando como referencia los resultados del cdigo de difusin COBAYA3 frente a un ejercicio comn y suficientemente significativo. Finalmente, con objeto de demostrar la posibilidad de uso prctico del cdigo, se ha simulado un transitorio en el concepto de reactor crtico en fase de diseo MYRRHA/FASTEF, de 100 MW de potencia trmica y refrigerado por plomo-bismuto. ABSTRACT Long term sustainable nuclear energy scenarios envisage a fleet of Liquid Metal Fast Reactors (LMFR) for the Pu recycling and minor actinides (MAs) transmutation or combined with some accelerator driven systems (ADS) just for MAs elimination. Design and licensing of these innovative reactor concepts require accurate computational tools, implementing the knowledge obtained in experimental research for new reactor configurations, materials and associated systems. Although a number of fast reactor systems have already been built, the operational experience is still reduced, especially for lead reactors, and not all the transients are fully understood. The safety analysis approach for LMFR is therefore based only on deterministic methods, different from modern approach for Light Water Reactors (LWR) which also benefit from probabilistic methods. Usually, the approach adopted in LMFR safety assessments is to employ a variety of codes, somewhat different for the each other, to analyze transients looking for a comprehensive solution and including uncertainties. In this frame, new best estimate simulation codes are of prime importance in order to analyze fast reactors steady state and transients. This thesis is focused on the development of a coupled code system for best estimate analysis in fast critical reactor. Currently due to the increase in the computational resources, Monte Carlo methods for neutrons transport can be used for detailed full core calculations. Furthermore, Monte Carlo codes are usually taken as reference for deterministic diffusion multigroups codes in fast reactors applications because they employ point-wise cross sections in an exact geometry model and intrinsically account for directional dependence of the ux. The coupling methodology presented here uses MCNP to calculate the power deposition within the reactor. The subchannel code COBRA-IV calculates the temperature and density distribution within the reactor. COBRA-IV is suitable for fast reactors applications because it has been validated against experimental results in sodium rod bundles. The proper correlations for liquid metal applications have been added to the thermal-hydraulics program. Both codes are coupled at steady state using an iterative method and external files exchange. The main issue in the Monte Carlo/thermal-hydraulics steady state coupling is the cross section handling to take into account Doppler broadening when temperature rises. Among every available options, the pseudo materials approach has been chosen in this thesis. This approach obtains reasonable results in fast reactor applications. Furthermore, geometrical changes caused by large temperature gradients in the core, are of major importance in fast reactor due to the large neutron mean free path. An additional module has therefore been included in order to simulate the reactor geometry in hot state or to estimate the reactivity due to core expansion in a transient. The module automatically calculates the fuel length, cladding radius, fuel assembly pitch and diagrid radius with the temperature. This effect will be crucial in some unprotected transients. Also related to geometrical changes, an automatic control rod movement feature has been implemented in order to achieve a just critical reactor or to calculate control rod worth. A step forward in the coupling platform is the dynamic simulation. Since MCNP performs only steady state calculations for critical systems, the more straight forward option without modifying MCNP source code, is to use the flux factorization approach solving separately the flux shape and amplitude. In this thesis two options have been studied to tackle time dependent neutronic simulations using a Monte Carlo code: adiabatic and quasistatic methods. The adiabatic methods uses a staggered time coupling scheme for the time advance of neutronics and the thermal-hydraulics calculations. MCNP computes the fundamental mode of the neutron flux distribution and the reactivity at the end of each time step and COBRA-IV the thermal properties at half of the the time steps. To calculate the flux amplitude evolution a solver of the point kinetics equations is used. This method calculates the static reactivity in each time step that in general is different from the dynamic reactivity calculated with the exact flux distribution. Nevertheless, for close to critical situations, both reactivities are similar and the method leads to acceptable practical results. In this line, an improved method as an attempt to take into account the effect of delayed neutron source in the transient flux shape evolutions is developed. The scheme performs a quasistationary calculation per time step with MCNP. This quasistationary simulations is based con the constant delayed source approach, taking into account the importance of each criticality cycle in the final flux estimation. Both adiabatic and quasistatic methods have been verified against the diffusion code COBAYA3, using a theoretical kinetic exercise. Finally, a transient in a critical 100 MWth lead-bismuth-eutectic reactor concept is analyzed using the adiabatic method as an application example in a real system.

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In shallow waters, such as those found close to berth structures, the wash from a manoeuvring ships propeller can cause erosion of the seabed. This erosion can be increased if the wash intersects a berth structure. A number of researchers have undertaken model studies and used regression analysis to develop predictive relationships for the scouring action. This paper presents an experimental investigation with Artificial Neural Networks (ANNs), used to analyse the results. The purpose of using ANNs was to examine the prediction accuracy of the Networks in comparison with previous regression analysis methods. ANNs were found to provide a more accurate method of predicting propeller wash scour than the equations presented by previous investigators.

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Scour and deposition have been measured in two small cobble-bedded upland streams, for two years. Grids of scour chains were inserted in the bed and relocated after the passage of individual hydrographs. Scour, fill and the area of the bed affected by these processes were recorded. The relationship between mean scour or fill and maximum scour or fill is assessed. In addition, the relationship between the depth of scour and the sediment transport rate as bedload is discussed briefly.

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Predicting the velocity within the ships propeller jet is the initial step to investigate the scouring made by the propeller jet. Albertson et al. (1950) suggested the investigation of a submerged jet can be undertaken through observation of the plain water jet from an orifice. The plain water jet investigation of Albertson et al. (1950) was based on the axial momentum theory. This has been the basis of all subsequent work with propeller jets. In reality, the velocity characteristic of a ships propeller jet is more complicated than a plain water jet. Fuehrer and Rmisch (1977), Blaauw and van de Kaa (1978), Berger et al. (1981), Verhey (1983) and Hamill (1987) have carried out investigations using physical model. This paper reviews the state-of-art of the equations used to predict the time-averaged axial, tangential and radial components of velocity within the zone of flow establishment and the zone of established flow of a ships propeller jet.

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The influence of surface waves and an applied wind stress is studied in an ensemble of large eddy simulations to investigate the nature of deeply penetrating jets into an unstratified mixed layer. The influence of a steady monochromatic surface wave propagating parallel to the wind direction is parameterized using the wave-filtered Craik-Leibovich equations. Tracer trajectories and instantaneous downwelling velocities reveal classic counterrotating Langmuir rolls. The associated downwelling jets penetrate to depths in excess of the wave's Stokes depth scale, s. Qualitative evidence suggests the depth of the jets is controlled by the Ekman depth scale. Analysis of turbulent kinetic energy (tke) budgets reveals a dynamical distinction between Langmuir turbulence and shear-driven turbulence. In the former, tke production is dominated by Stokes shear and a vertical flux term transports tke to a depth where it is dissipated. In the latter, tke production is from the mean shear and is locally balanced by dissipation. We define the turbulent Langmuir number Lat = (v*/Us)0.5 (v* is the ocean's friction velocity and Us is the surface Stokes drift velocity) and a turbulent anisotropy coefficient Rt = /( + ). The transition between shear-driven and Langmuir turbulence is investigated by varying external wave parameters s and Lat and by diagnosing Rt and the Eulerian mean and Stokes shears. When either Lat or s are sufficiently small the Stokes shear dominates the mean shear and the flow is preconditioned to Langmuir turbulence and the associated deeply penetrating jets.

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Conselho Nacional de Desenvolvimento Cientfico e Tecnolgico (CNPq)

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A search for squarks and gluinos in final states containing jets, missing transverse momentum and no high-p(T) electrons or muons is presented. The data represent the complete sample recorded in 2011 by the ATLAS experiment in 7 TeV proton-proton collisions at the Large Hadron Collider, with a total integrated luminosity of 4.7 fb(-1). No excess above the Standard Model background expectation is observed. Gluino masses below 860 GeV and squark masses below 1320 GeV are excluded at the 95% confidence level in simplified models containing only squarks of the first two generations, a gluino octet and a massless neutralino, for squark or gluino masses below 2 TeV, respectively. Squarks and gluinos with equal masses below 1410 GeV are excluded. In minimal supergravity/constrained minimal supersymmetric Standard Model models with tan beta = 10, A(0) = 0 and mu > 0, squarks and gluinos of equal mass are excluded for masses below 1360 GeV. Constraints are also placed on the parameter space of supersymmetric models with compressed spectra. These limits considerably extend the region of supersymmetric parameter space excluded by previous measurements with the ATLAS detector.

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A search for squarks and gluinos in final states containing high-pT jets, missing transverse momentum and no electrons or muons is presented. The data were recorded in 2012 by the ATLAS experiment in s = 8TeV proton-proton collisions at the Large Hadron Collider, with a total integrated luminosity of 20.3 fb1. Results are interpreted in a variety of simplified and specific supersymmetry-breaking models assuming that R-parity is conserved and that the lightest neutralino is the lightest supersymmetric particle. An exclusion limit at the 95% confidence level on the mass of the gluino is set at 1330GeV for a simplified model incorporating only a gluino and the lightest neutralino. For a simplified model involving the strong production of first- and second-generation squarks, squark masses below 850GeV (440GeV) are excluded for a massless lightest neutralino, assuming mass degenerate (single light-flavour) squarks. In mSUGRA/CMSSM models with tan = 30, A0 = 2m0 and > 0, squarks and gluinos of equal mass are excluded for masses below 1700GeV. Additional limits are set for non-universal Higgs mass models with gaugino mediation and for simplified models involving the pair production of gluinos, each decaying to a top squark and a top quark, with the top squark decaying to a charm quark and a neutralino. These limits extend the region of supersymmetric parameter space excluded by previous searches with the ATLAS detector.

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Aims. The OSIRIS camera onboard the Rosetta spacecraft obtained close-up views of the dust coma of comet 67P. The jet structures can be used to trace their source regions and to examine the possible effect of gas-surface interaction. Methods. We analyzed the wide-angle images obtained in the special dust observation sequences between August and September 2014. The jet features detected in different images were compared to study their time variability. The locations of the potential source regions of some of the jets are identified by ray tracing. We used a ring-masking technique to calculate the brightness distribution of dust jets along the projected distance. Results. The jets detected between August and September 2014 mostly originated in the Hapi region. Morphological changes appeared over a timescale of several days in September. The brightness slope of the dust jets is much steeper than the background coma. This might be related to the sublimation or fragmentation of the emitted dust grains. Interaction of the expanding gas flow with the cliff walls on both sides of Hapi could lead to erosion and material down-fall to the nucleus surface.

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The small element spacing of compact multiport arrays introduces strong mutual coupling between the antenna ports. Due to this coupling, the input impedance of the array changes when elements excitations are varied, and consequently, the array cannot be matched for an arbitrary excitation. Decoupling networks have in the past been used to provide an additional connection between antenna ports in order to cancel the coupling between elements. An alternative approach is to design the antenna so that each port does not excite a single element, but all elements simultaneously instead. The geometry of the antenna is optimized so that this direct excitation of elements counteracts the mutual coupling, thus yielding decoupled ports. This paper describes the design of such a 4-port antenna.