2019
DOI: 10.1002/num.22404
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The method of fundamental solutions for the Oseen steady‐state viscous flow past obstacles of known or unknown shapes

Abstract: In this paper, the steady-state Oseen viscous flow equations past a known or unknown obstacle are solved numerically using the method of fundamental solutions (MFS), which is free of meshes, singularities, and numerical integrations. The direct problem is linear and well-posed, whereas the inverse problem is nonlinear and ill-posed. For the direct problem, the MFS computations of the fluid flow characteristics (velocity, pressure, drag, and lift coefficients) are in very good agreement with the previously publ… Show more

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Cited by 12 publications
(12 citation statements)
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“…For simplicity, we only consider the two-dimensional case. The MFS for the exterior stationary Oseen fluid flow past an arbitrary obstacle has been recently introduced in [12]. For our interior problem in the annular domain Ω\D, it approximates the fluid velocity u = (u 1 , u 2 ) and pressure p as…”
Section: The Methods Of Fundamental Solutions (Mfs)mentioning
confidence: 99%
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“…For simplicity, we only consider the two-dimensional case. The MFS for the exterior stationary Oseen fluid flow past an arbitrary obstacle has been recently introduced in [12]. For our interior problem in the annular domain Ω\D, it approximates the fluid velocity u = (u 1 , u 2 ) and pressure p as…”
Section: The Methods Of Fundamental Solutions (Mfs)mentioning
confidence: 99%
“…Example 3: Bean-shaped obstacle. We attempt to reconstruct a more irregular shape than the previous example, given by a bean-shaped obstacle D with the parametrisation [3,12,14] r(ϑ) = 1 + 0.9 cos(ϑ) + 0.1 sin(ϑ) 1 + 0.75 cos(ϑ) , ϑ ∈ [0, 2π).…”
Section: Niter=1 Niter=10 Niter=100 Niter=1000mentioning
confidence: 99%
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“…In terms of the perturbations u and p, the inverse problem requires solving for the unknown triplet (u, p, Ω) satisfying (1.7)-(1.11) and (4.2). This problem and its MFS combined nonlinear minimization is similar to that previously treated in [7] for Oseen flow. We assume that Ω is starshaped with respect to the origin, parametrised by the radial polar coordinate r(ϑ) ∈ (0, r max ] for ϑ ∈ [0, 2π), where r max > 0 is an a priori known upper bound of the size of the obstacle, namely,…”
Section: Inverse Obstacle Problemmentioning
confidence: 96%