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An overview is given for identification criteria of tip vortices, trailing from lifting surfaces of aircraft. $Q$-distribution is used as the main vortex identification method in this work. According to the definition of Q-criterion, the vortex core is bounded by a surface on which the norm of the vorticity tensor is equal to the norm of the strain-rate tensor. Moreover, following conditions are satisfied inside of the vortex core: (i) net (non-zero) vorticity tensor; (ii) the geometry of the identified vortex core should be Galilean invariant. Based on the existing analytical vortex models, a vortex center of a twodimensional vortex is defined as a point, where the $Q$-distribution reaches a maximum value and it is much greater than the norm of the strain-rate tensor (for an axisymmetric 2D vortex, the norm of the vorticity tensor tends to zero at the vortex center). Since the existence of the vortex axis is discussed by various authors and it seems to be a fairly natural requirement in the analysis of vortices, the above-mentioned conditions (i), (ii) can be supplemented with a third condition (iii): the vortex core in a three-dimensional flow must contain a vortex axis. Flows, having axisymmetric or non-axisymmetric (in particular, elliptic) vortex cores in 2D cross-sections, are analyzed. It is shown that in such cases $Q$-distribution can be used to obtain not only the boundary of the vortex core, but also to determine the axis of the vortex. These concepts are illustrated using the numerical simulation results for a finite span wing flow-field, obtained using the Reynolds-Averaged Navier – Stokes (RANS) equations with $k-\omega$ turbulence model.

The article presents the results of numerical modeling of the vortex spatial non-stationary motion of the medium arising near the lateral and bottom surfaces of the descent module during its movement in the atmosphere of Mars. The numerical study was performed for the high-speed streamline regime at various angles of attack. Mathematical modeling was carried out on the basis of the Navier – Stokes model and the model of equilibrium chemical reactions for the Martian atmosphere gas. The simulation results showed that under the considered conditions of the descent module motion, a non-stationary flow with a pronounced vortex character is realized near its lateral and bottom surfaces. Numerical calculations indicate that, depending on the angle of attack, the nonstationarity and vortex nature of the flow can manifest itself both on the entire lateral and bottom surfaces of the module, and, partially, on their leeward side. For various angles of attack, pictures of the vortex structure of the flow near the surface of the descent vehicle and in its near wake are presented, as well as pictures of the gas-dynamic parameters fields. The non-stationary nature of the flow is confirmed by the presented time dependences of the gas-dynamic parameters of the flow at various points on the module surface. The carried out parametric calculations made it possible to determine the dependence of the aerodynamic characteristics of the descent module on the angle of attack. Mathematical modeling is carried out on the basis of the conservative numerical method of fluxes, which is a finitevolume method based on a finite-difference writing of the conservation laws of additive characteristics of the medium using «upwind» approximations of stream variables. To simulate the complex vortex structure of the flow over descent module, the nonuniform computational grids are used, including up to 30 million finite volumes with exponential thickening to the surface, which made it possible to reveal small-scale vortex formations. Numerical investigations were carried out on the basis of the developed software package based on parallel algorithms of the used numerical method and implemented on modern multiprocessor computer systems. The results of numerical simulation presented in the article were obtained using up to two thousand computing cores of a multiprocessor complex.

This paper is devoted to investigation of the swirl flows. Such flows are widely used in various industrial processes. Swirl flows can be accompanied by time-dependent effects, for example, precession of the vortex core. In turn, the large-scale fluctuations due to the precession of the vortex can cause damage of structures and reduce of equipment reliability. Thus, for engineering calculations approaches that sufficiently well described such flows are required. This paper presents the technique of swirl flows calculation, tested for CFD packages Fluent and SigmaFlow. A numerical simulation of several swirl flow test problems was carried out. Obtained results are compared with each other and with the experimental data.