“…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,…”