997 resultados para steady 2D Navier-Stokes equations


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Centrifugal compressors are widely used for example in refrigeration processes, the oil and gas industry, superchargers, and waste water treatment. In this work, five different vaneless diffusers and six different vaned diffusers are investigated numerically. The vaneless diffusers vary only by their diffuser width, so that four of the geometries have pinch implemented to them. Pinch means a decrease in the diffuser width. Four of the vaned diffusers have the same vane turning angle and a different number of vanes, and two have different vane turning angles. The flow solver used to solve the flow fields is Finflo, which is a Navier-Stokes solver. All the cases are modeled with the Chien's k – έ- turbulence model, and selected cases are modeled also with the k – ώ-SST turbulence model. All five vaneless diffusers and three vaned diffusers are investigated also experimentally. For each construction, the compressor operating map is measured according to relevant standards. In addition to this, the flow fields before and after the diffuser are measured with static and total pressure, flow angle and total temperature measurements. When comparing the computational results to the measured results, it is evident that the k – ώ-SST turbulence model predicts the flow fields better. The simulation results indicate that it is possible to improve the efficiency with the pinch, and according to the numerical results, the two best geometries are the ones with most pinch at the shroud. These geometries have approximately 4 percentage points higher efficiency than the unpinched vaneless diffusers. The hub pinch does not seem to have any major benefits. In general, the pinches make the flow fields before and after the diffuser more uniform. The pinch also seems to improve the impeller efficiency. This is down to two reasons. The major reason is that the pinch decreases the size of slow flow and possible backflow region located near the shroud after the impeller. Secondly, the pinches decrease the flow velocity in the tip clearance, leading to a smaller tip leakage flow and therefore slightly better impeller efficiency. Also some of the vaned diffusers improve the efficiency, the increment being 1...3 percentage points, when compared to the vaneless unpinched geometry. The measurement results confirm that the pinch is beneficial to the performance of the compressor. The flow fields are more uniform with the pinched cases, and the slow flow regions are smaller. The peak efficiency is approximately 2 percentage points and the design point efficiency approximately 4 percentage points higher with the pinched geometries than with the un- pinched geometry. According to the measurements, the two best geometries are the ones with the most pinch at the shroud, the case with the pinch only at the shroud being slightly better of the two. The vaned diffusers also have better efficiency than the vaneless unpinched geometries. However, the pinched cases have even better efficiencies. The vaned diffusers narrow the operating range considerably, whilst the pinch has no significant effect on the operating range.

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Supersonic axial turbine stages typically exhibit lower efficiencies than subsonic axial turbine stages. One reason for the lower efficiency is the occurrence of shock waves. With higher pressure ratios the flow inside the turbine becomes relatively easily supersonic if there is only one turbine stage. Supersonic axial turbines can be designed in smaller physical size compared to subsonic axial turbines of same power. This makes them good candidates for turbochargers in large diesel engines, where space can be a limiting factor. Also the production costs are lower for a supersonic axial turbine stage than for two subsonic stages. Since supersonic axial turbines are typically low reaction turbines, they also create lower axial forces to be compensated with bearings compared to high reaction turbines. The effect of changing the stator-rotor axial gap in a small high (rotational) speed supersonic axial flow turbine is studied in design and off-design conditions. Also the effect of using pulsatile mass flow at the supersonic stator inlet is studied. Five axial gaps (axial space between stator and rotor) are modeled using threedimensional computational fluid dynamics at the design and three axial gaps at the off-design conditions. Numerical reliability is studied in three independent studies. An additional measurement is made with the design turbine geometry at intermediate off-design conditions and is used to increase the reliability of the modelling. All numerical modelling is made with the Navier-Stokes solver Finflo employing Chien’s k ¡ ² turbulence model. The modelling of the turbine at the design and off-design conditions shows that the total-to-static efficiency of the turbine decreases when the axial gap is increased in both design and off-design conditions. The efficiency drops almost linearily at the off-design conditions, whereas the efficiency drop accelerates with increasing axial gap at the design conditions. The modelling of the turbine stator with pulsatile inlet flow reveals that the mass flow pulsation amplitude is decreased at the stator throat. The stator efficiency and pressure ratio have sinusoidal shapes as a function of time. A hysteresis-like behaviour is detected for stator efficiency and pressure ratio as a function of inlet mass flow, over one pulse period. This behaviour arises from the pulsatile inlet flow. It is important to have the smallest possible axial gap in the studied turbine type in order to maximize the efficiency. The results for the whole turbine can also be applied to some extent in similar turbines operating for example in space rocket engines. The use of a supersonic stator in a pulsatile inlet flow is shown to be possible.

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It is well known that the numerical solutions of incompressible viscous flows are of great importance in Fluid Dynamics. The graphics output capabilities of their computational codes have revolutionized the communication of ideas to the non-specialist public. In general those codes include, in their hydrodynamic features, the visualization of flow streamlines - essentially a form of contour plot showing the line patterns of the flow - and the magnitudes and orientations of their velocity vectors. However, the standard finite element formulation to compute streamlines suffers from the disadvantage of requiring the determination of boundary integrals, leading to cumbersome implementations at the construction of the finite element code. In this article, we introduce an efficient way - via an alternative variational formulation - to determine the streamlines for fluid flows, which does not need the computation of contour integrals. In order to illustrate the good performance of the alternative formulation proposed, we capture the streamlines of three viscous models: Stokes, Navier-Stokes and Viscoelastic flows.

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Das von Maz'ya eingeführte Approximationsverfahren, die Methode der näherungsweisen Näherungen (Approximate Approximations), kann auch zur numerischen Lösung von Randintegralgleichungen verwendet werden (Randpunktmethode). In diesem Fall hängen die Komponenten der Matrix des resultierenden Gleichungssystems zur Berechnung der Näherung für die Dichte nur von der Position der Randpunkte und der Richtung der äußeren Einheitsnormalen in diesen Punkten ab. Dieses numerisches Verfahren wird am Beispiel des Dirichlet Problems für die Laplace Gleichung und die Stokes Gleichungen in einem beschränkten zweidimensionalem Gebiet untersucht. Die Randpunktmethode umfasst drei Schritte: Im ersten Schritt wird die unbekannte Dichte durch eine Linearkombination von radialen, exponentiell abklingenden Basisfunktionen approximiert. Im zweiten Schritt wird die Integration über den Rand durch die Integration über die Tangenten in Randpunkten ersetzt. Für die auftretende Näherungspotentiale können sogar analytische Ausdrücke gewonnen werden. Im dritten Schritt wird das lineare Gleichungssystem gelöst, und eine Näherung für die unbekannte Dichte und damit auch für die Lösung der Randwertaufgabe konstruiert. Die Konvergenz dieses Verfahrens wird für glatte konvexe Gebiete nachgewiesen.

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The discontinuities in the solutions of systems of conservation laws are widely considered as one of the difficulties in numerical simulation. A numerical method is proposed for solving these partial differential equations with discontinuities in the solution. The method is able to track these sharp discontinuities or interfaces while still fully maintain the conservation property. The motion of the front is obtained by solving a Riemann problem based on the state values at its both sides which are reconstructed by using weighted essentially non oscillatory (WENO) scheme. The propagation of the front is coupled with the evaluation of "dynamic" numerical fluxes. Some numerical tests in 1D and preliminary results in 2D are presented.

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The performance of a 2D numerical model of flood hydraulics is tested for a major event in Carlisle, UK, in 2005. This event is associated with a unique data set, with GPS surveyed wrack lines and flood extent surveyed 3 weeks after the flood. The Simple Finite Volume (SFV) model is used to solve the 2D Saint-Venant equations over an unstructured mesh of 30000 elements representing channel and floodplain, and allowing detailed hydraulics of flow around bridge piers and other influential features to be represented. The SFV model is also used to corroborate flows recorded for the event at two gauging stations. Calibration of Manning's n is performed with a two stage strategy, with channel values determined by calibration of the gauging station models, and floodplain values determined by optimising the fit between model results and observed water levels and flood extent for the 2005 event. RMS error for the calibrated model compared with surveyed water levels is ~±0.4m, the same order of magnitude as the estimated error in the survey data. The study demonstrates the ability of unstructured mesh hydraulic models to represent important hydraulic processes across a range of scales, with potential applications to flood risk management.

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Waves with periods shorter than the inertial period exist in the atmosphere (as inertia-gravity waves) and in the oceans (as Poincaré and internal gravity waves). Such waves owe their origin to various mechanisms, but of particular interest are those arising either from local secondary instabilities or spontaneous emission due to loss of balance. These phenomena have been studied in the laboratory, both in the mechanically-forced and the thermally-forced rotating annulus. Their generation mechanisms, especially in the latter system, have not yet been fully understood, however. Here we examine short period waves in a numerical model of the rotating thermal annulus, and show how the results are consistent with those from earlier laboratory experiments. We then show how these waves are consistent with being inertia-gravity waves generated by a localised instability within the thermal boundary layer, the location of which is determined by regions of strong shear and downwelling at certain points within a large-scale baroclinic wave flow. The resulting instability launches small-scale inertia-gravity waves into the geostrophic interior of the flow. Their behaviour is captured in fully nonlinear numerical simulations in a finite-difference, 3D Boussinesq Navier-Stokes model. Such a mechanism has many similarities with those responsible for launching small- and meso-scale inertia-gravity waves in the atmosphere from fronts and local convection.

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In decaying two-dimensional Navier-Stokes turbulence, Batchelor's similarity hypothesis fails due to the existence of coherent vortices. However, it is shown that decaying two-dimensional turbulence governed by the Harney-Hasegawa-Mima (CHM) equation ∂/∂t (V^2 φ-λ^2 φ)+J(φ,∇^2 φ)=D where D is a damping, is described well by Batchelor's similarity hypothesis for wave numbers k ≪ λ (the so-called AM regime). It is argued that CHM turbulence in the AM regime is a more `ideal' form of two-dimensional turbulence than is Navier-Stokes turbulence itself.

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The region of sea ice near the edge of the sea ice pack is known as the marginal ice zone (MIZ), and its dynamics are complicated by ocean wave interaction with the ice cover, strong gradients in the atmosphere and ocean and variations in sea ice rheology. This paper focuses on the role of sea ice rheology in determining the dynamics of the MIZ. Here, sea ice is treated as a granular material with a composite rheology describing collisional ice floe interaction and plastic interaction. The collisional component of sea ice rheology depends upon the granular temperature, a measure of the kinetic energy of flow fluctuations. A simplified model of the MIZ is introduced consisting of the along and across momentum balance of the sea ice and the balance equation of fluctuation kinetic energy. The steady solution of these equations is found to leading order using elementary methods. This reveals a concentrated region of rapid ice flow parallel to the ice edge, which is in accordance with field observations, and previously called the ice jet. Previous explanations of the ice jet relied upon the existence of ocean currents beneath the ice cover. We show that an ice jet results as a natural consequence of the granular nature of sea ice.

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We design consistent discontinuous Galerkin finite element schemes for the approximation of the Euler-Korteweg and the Navier-Stokes-Korteweg systems. We show that the scheme for the Euler-Korteweg system is energy and mass conservative and that the scheme for the Navier-Stokes-Korteweg system is mass conservative and monotonically energy dissipative. In this case the dissipation is isolated to viscous effects, that is, there is no numerical dissipation. In this sense the methods are consistent with the energy dissipation of the continuous PDE systems. - See more at: http://www.ams.org/journals/mcom/2014-83-289/S0025-5718-2014-02792-0/home.html#sthash.rwTIhNWi.dpuf

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We consider incompressible Stokes flow with an internal interface at which the pressure is discontinuous, as happens for example in problems involving surface tension. We assume that the mesh does not follow the interface, which makes classical interpolation spaces to yield suboptimal convergence rates (typically, the interpolation error in the L(2)(Omega)-norm is of order h(1/2)). We propose a modification of the P(1)-conforming space that accommodates discontinuities at the interface without introducing additional degrees of freedom or modifying the sparsity pattern of the linear system. The unknowns are the pressure values at the vertices of the mesh and the basis functions are computed locally at each element, so that the implementation of the proposed space into existing codes is straightforward. With this modification, numerical tests show that the interpolation order improves to O(h(3/2)). The new pressure space is implemented for the stable P(1)(+)/P(1) mini-element discretization, and for the stabilized equal-order P(1)/P(1) discretization. Assessment is carried out for Poiseuille flow with a forcing surface and for a static bubble. In all cases the proposed pressure space leads to improved convergence orders and to more accurate results than the standard P(1) space. In addition, two Navier-Stokes simulations with moving interfaces (Rayleigh-Taylor instability and merging bubbles) are reported to show that the proposed space is robust enough to carry out realistic simulations. (c) 2009 Elsevier B.V. All rights reserved.

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Simulações Numéricas são executadas em um código numérico de alta precisão resolvendo as equações de Navier-Stokes e da continuidade para regimes de escoamento incompressíveis num contexto da turbulência bidimensional. Este código utiliza um esquema compacto de diferenças finitas de sexta ordem na aproximação das derivadas espaciais. As derivadas temporais são calculadas usando o esquema de Runge-Kuta de terceeira ordem com baixo armazenamento. Tal código numérico fornece uma representação melhorada para uma grande faixa de escalas de comprimento e de tempo. As técnicas dos contornos imersos acopladas ao método dos contornos virtuais permitem modelar escoamentos não-estacionários sobre geometrrias complexas, usando simplesmente uma malha Cartesiana uniforme. Por meio de procedimentos de aproximação/interpolação, as técnicas dos contornos imersos (aproximação Gaussiana, interpolação bilinear e redistribuição Gaussiana), permitem a representação do corpo sólido no interior do campo de escoamento, com a superfície não coincidindo com a malha computacional. O método dos contornos virtuais, proposto originalmente por Peskin, consiste, basicamente, na imposição na superfície e/ou no interior do corpo, de um termo de força temporal acrescentando às equações do momento. A aplicação deste campo de força local leva o fluido ao repouso na superfície do corpo, permitindo obter as condições de contorno de não-deslizamento e de não penetração de fluido na parede. A análise das oscilações induzidas no escoamento-contorno pelo processo de desprendimento de vórtices na esteira do cilindro circular e de geometria retangulares na incidência, para números de Reybolds variando de 40 a 400, confirma a eficiência computacional e a aplicabilidade das técncias implementadas.

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O objetivo deste trabalho é estudar os efeitos eletromagnéticos e fluido-dinâmicos induzidos no aço, decorrentes do uso de um agitador eletromagnético. Para tal, foi proposta a construção de um modelo numérico que resolva, de forma acoplada, os problemas de eletromagnetismo e fluido-dinâmica. O modelo numérico do problema eletromagnético, em elementos finitos, foi construído utilizando-se o software Opera-3d/Elektra da Vector Fields. O mesmo foi validado com medidas experimentais de densidade de fluxo magnético feitas na usina. O escoamento decorrente da agitação eletromagnética foi resolvido fazendo-se o acoplamento das forças de Lorentz com as equações de Navier-Stokes. Essas últimas foram resolvidas pelo método de volumes finitos, usando-se o software CFX-4 da AEA Technology. O modelo eletromagnético mostrou que existe um torque máximo dependente da freqüência do campo magnético. Também foi observado que a força magnética aumenta em quatro vezes seu valor, quando a corrente é duplicada. O perfil de escoamento produzido no molde, sob agitação eletromagnética, indica, que as situações de lingotamento testadas, não propiciam o arraste da escória. A velocidade crítica de arraste, determinada via modelo físico, não foi atingida para nenhum caso testado. O modelo fluido-dinâmico e térmico apresentou um aumento do fluxo de calor cedido pelo fluido para a casca solidificada com o uso do agitador eletromagnético. Como conseqüência, observou-se uma queda na temperatura do banho. Também foi observado, que o uso do agitador propicia a remoção de inclusões das camadas mais externas do tarugo. Ao mesmo tempo, notou-se que o uso do agitador aumenta o índice de remoção de inclusões para as duas seções de molde analisadas.

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Este trabalho desenvolve um método numérico para a solução de escoamentos bidimensionais em torno de geometrias automobilísticas utilizando o método de diferenças finitas. O código computacional resolve as equações de Navier-Stokes e de Euler para uma distribuição adequada dos pontos discretos na malha. O método de integração empregado baseia-se no esquema explícito de Runge-Kutta de 3 estágios para as equações da quantidade de movimento e no de sub-relaxações sucessivas para a pressão na base Gauss-Seidel. Utilizou-se a técnica dos contornos virtuais em coordenadas cartesianas para resolver o escoamento sobre uma geometria simplificada, com a superfície coincidente com a malha computacional, e uma geometria automobilística mais complexa (BMW). Para a certificação da técnica empregada, optou-se pela utilização da teoria do escoamento potencial e pela comparação com dados experimentais encontrados na literatura e outros coletados em túnel de vento em escala reduzida. Houve dificuldade nesta comparação devido à falta de artigos relativos às simulações numéricas de escoamentos sobre automóveis e na aplicação da técnica dos contornos virtuais em geometrias complexas. Os resultados foram satisfatórios, com boas perspectivas para trabalhos futuros, contribuindo assim para o desenvolvimento da área.

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Neste trabalho, discutimos o movimento de uma macromolécula carregada em um fluido ionizado. A interação do campo elétrico é descrita pela equação de Poisson-Boltzmann acoplada às equações governantes para a dinâmica do fluido e às equações dinâmicas da partícula. Uma formulação fraca é introduzida no caso em que o domínio ocupado pelo fluido é finito e um teorema de existência de soluções fracas, local em tempo, é estabelecido. Dois modelos são considerados: fluxos não-estacionários e estacionários. No primeiro caso, a hidrodinâmica do sistema é governada pelas equações de Navier-Stokes, considerando-se um termo forçante relacionado ao potencial elétrico; no segundo caso, uma velocidade de deslizamento, a qual depende não linearmente sobre os potenciais, é introduzida como uma condição de contorno para um problema estacionário de Stokes. O caso de um fluido ocupando uma região infinita é também discutido supondo-se uma hipótese de aproximação sobre o campo elétrico.