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The paper deals with a heat wave motion problem for a degenerate second-order nonlinear parabolic equation with power nonlinearity. The considered boundary condition specifies in a plane the motion equation of the circular zero front of the heat wave. A new numerical-analytical algorithm for solving the problem is proposed. A solution is constructed stepby- step in time using difference time discretization. At each time step, a boundary value problem for the Poisson equation corresponding to the original equation at a fixed time is considered. This problem is, in fact, an inverse Cauchy problem in the domain whose initial boundary is free of boundary conditions and two boundary conditions (Neumann and Dirichlet) are specified on a current boundary (heat wave). A solution of this problem is constructed as the sum of a particular solution to the nonhomogeneous Poisson equation and a solution to the corresponding Laplace equation satisfying the boundary conditions. Since the inhomogeneity depends on the desired function and its derivatives, an iterative solution procedure is used. The particular solution is sought by the collocation method using inhomogeneity expansion in radial basis functions. The inverse Cauchy problem for the Laplace equation is solved by the null field method as applied to a circular domain with a circular hole. This method is used for the first time to solve such problem. The calculation algorithm is optimized by parallelizing the computations. The parallelization of the computations allows us to realize effectively the algorithm on high performance computing servers. The algorithm is implemented as a program, which is parallelized by using the OpenMP standard for the C++ language, suitable for calculations with parallel cycles. The effectiveness of the algorithm and the robustness of the program are tested by the comparison of the calculation results with the known exact solution as well as with the numerical solution obtained earlier by the authors with the use of the boundary element method. The implemented computational experiment shows good convergence of the iteration processes and higher calculation accuracy of the proposed new algorithm than of the previously developed one. The solution analysis allows us to select the radial basis functions which are most suitable for the proposed algorithm.

A 2D numerical model of the immersion of a cold oceanic plate into the thickness of the Earth’s upper mantle has been developed, where the stage of the initial immersion of the plate is preceded by the establishment of a regime of thermogravitational convection of the mantle substance. The model approximation of the mantle is a two-dimensional image of an incompressible Newtonian quasi-liquid in a Cartesian coordinate system, where, due to the high viscosity of the medium, the equations of mantle convection are accepted in the Stokes approximation. It is assumed that seawater that has leaked here enters the first horizons of the mantle together with the plate. With depth, the increase in pressure and temperature leads to certain losses of its light fractions and fluids, losses of water and gases of water-containing minerals of the plate, restructuring of their crystal lattice and, as a consequence, phase transformations. These losses cause an increase in the plate density and an uneven distribution of stresses along the plate (the initial sections of the plate are denser), which subsequently, together with the effect of mantle currents on the plate, causes its fragmentation. The state of mantle convection is considered when the plate and its individual fragments have descended to the bottom of the upper mantle. Computational schemes for solving the model equations have been developed. Mantle convection calculations are performed in terms of the Stokes approximation for vorticity and the stream function, and SPH is used to calculate the state and subsidence of the plate. A number of computational experiments have been performed. It is shown that fragmentation of the plate occurs due to the effect of mantle convection on the plate and the development of inhomogeneous stress fields along the plate. Following the equations of the model, the time of the final stage of subduction is estimated, i.e. the time of the entire oceanic plate reaching the bottom of the upper mantle. In geodynamics, this process is determined by the collision of plates that immediately follows subduction and is usually considered as the final stage of the Wilson cycle (i. e., the cycle of development of folded belts).

The article presents a systematic investigation of the capabilities of the lattice Boltzmann method (LBM) for modeling the propagation of acoustic waves. The study considers the problem of wave propagation from a point harmonic source in an unbounded domain, both in a quiescent medium (Mach number $M=0$) and in the presence of a uniform mean flow ($M=0.2$). Both scenarios admit analytical solutions within the framework of linear acoustics, allowing for a quantitative assessment of the accuracy of the numerical method.

The numerical implementation employs the two-dimensional D2Q9 velocity model and the Bhatnagar – Gross – Krook (BGK) collision operator. The oscillatory source is modeled using Gou’s scheme, while spurious high-order moment noise generated by the source is suppressed via a regularization procedure applied to the distribution functions. To minimize wave reflections from the boundaries of the computational domain, a hybrid approach is used, combining characteristic boundary conditions based on Riemann invariants with perfectly matched layers (PML) featuring a parabolic damping profile.

A detailed analysis is conducted to assess the influence of computational parameters on the accuracy of the method. The dependence of the error on the PML thickness ($L_{\text{PML}}^{}$) and the maximum damping coefficient ($\sigma_{\max}^{}$), the dimensionless source amplitude ($Q'_0$), and the grid resolution is thoroughly examined. The results demonstrate that the LBM is suitable for simulating acoustic wave propagation and exhibits second-order accuracy. It is shown that achieving high accuracy (relative pressure error below $1\,\%$) requires a spatial resolution of at least $20$ grid points per wavelength ($\lambda$). The minimal effective PML parameters ensuring negligible boundary reflections are identified as $\sigma_{\max}^{}\geqslant 0.02$ and $L_{\text{PML}}^{} \geqslant 2\lambda$. Additionally, it is shown that for source amplitudes $Q_0' \geqslant 0.1$, nonlinear effects become significant compared to other sources of error.

The paper presents a mathematical model to be used for design of cooling tanks for vapor desublimation. Results of calculations for the process of cooling of two tanks in a block of four are presented. Chart of the cooling air flow in the piping network is presented.

A mathematical model for the numerical study of thermal destruction of the "Chelyabinsk" meteorite when entering the Earth’s atmosphere is presented in the article. The study was conducted in the framework of an integrated approach, including the calculation of the meteorite trajectory associated with the physical processes connected with the meteorite motion. Together with the trajectory the flow field and radiation-convective heat
transfer were determined as well as warming and destruction of the meteorite under the influence of the calculated heat load. An integrated approach allows to determine the trajectories of space objects more precisely, predict the area of their fall and destruction.

The question on improvement of quality of images obtained in a tomography problem is considered. The problem consists in finding of boundaries of inhomogeneities (inclusions) in a continuous medium by results of X-ray radiography of this medium. A nonlinear integral transformation of a special kind is proposed which allows to improve quality of images obtained earlier at a set of papers. The method is realized numerically by the use of computer modelling. Some calculations are carried out with use of data for concrete materials. The results obtained are presented by drawings and graphic images.

WENO schemes (weighted, essentially non oscillating) are currently having a wide range of applications as approximate high order schemes for discontinuous solutions of partial differential equations. These schemes are used for direct numerical simulation (DNS) and large eddy simmulation in the gas dynamic problems, problems for DNS in MHD and even neutron kinetics. This work is dedicated to clarify some characteristics of WENO schemes and numerical simulation of specific tasks. Results of the simulations can be used to clarify the field of application of these schemes. The first part of the work contained proofs of the approximation properties, stability and convergence of WENO5, WENO7, WENO9, WENO11 and WENO13 schemes. In the second part of the work the modified wave number analysis is conducted that allows to conclude the dispersion and dissipative properties of schemes. Further, a numerical simulation of a number of specific problems for hyperbolic equations is conducted, namely for advection equations (one-dimensional and two-dimensional), Hopf equation, Burgers equation (with low dissipation) and equations of non viscous gas dynamics (onedimensional and two-dimensional). For each problem that is implying a smooth solution, the practical calculation of the order of approximation via Runge method is performed. The influence of a time step on nonlinear properties of the schemes is analyzed experimentally in all problems and cross checked with the first part of the paper. In particular, the advection equations of a discontinuous function and Hopf equations show that the failure of the recommendations from the first part of the paper leads first to an increase in total variation of the solution and then the approximation is decreased by the non-linear dissipative mechanics of the schemes. Dissipation of randomly distributed initial conditions in a periodic domain for one-dimensional Burgers equation is conducted and a comparison with the spectral method is performed. It is concluded that the WENO7–WENO13 schemes are suitable for direct numerical simulation of turbulence. At the end we demonstrate the possibility of the schemes to be used in solution of initial-boundary value problems for equations of non viscous gas dynamics: Rayleigh–Taylor instability and the reflection of the shock wave from a wedge with the formation a complex configuration of shock waves and discontinuities.

The article discusses the model of the anthropomorphic type of mechanism of the exoskeleton with links of variable length. Four models of parts of variable length are considered comprehensively: the model link of the exoskeleton of variable length with a resilient member and a rigid strong core; the model of the telescopic link; the model link with the masses in the hinge-joint between them; the link model with an arbitrary number of masses. The differential equations of motion in the form of Lagrange equations of the second kind are made. On the basis of analysis of differential equations of motion for multi-link rod of a mechanical system type, exoskeleton revealed their structure, which allowed us to represent them in vector-matrix form. The General pattern of building matrices are established for the first time and the generalization of the expressions for elements of matrices in two-dimensional case are obtained. New recursive and matrix methods of composing of differential equations of motion are given. A unified approach to constructing differential equations of motion of the exoskeleton based on the developed recursive and matrix methods write differential equations of motion of the proposed exoskeleton. Comparison of the time of writing the differential equations of motion proposed methods, in comparison with the Lagrange equations of the second kind, in the system of computer mathematics Mathematica conducted. An analytical study of the model of the exoskeleton carried out. It was found that for mechanisms with n movable links of the Cauchy problem for systems of differential equations of motion for any initial conditions there is no single and unlimited continue. Control of the exoskeleton is accomplished using the torques which are located in the hinge-joints in the joints of the links and simulating control actions. Numerical investigation of a model of the exoskeleton is made, a comparison of results of calculations for exoskeletons with various models of units is held. A numerical study of the empirical evidence about the man and his movements is used. It is established that the choice structure of the exoskeleton model with lumped masses is more preferable to a model with perfectly rigid strong core. As an exoskeleton, providing comfortable movement of people, and you should repeat the properties of the musculoskeletal system.

The paper develops a new mathematical method of the joint signal and noise parameters determination at the Rice statistical distribution by method of moments based upon the analysis of data for the 1-st and the 3-rd raw moments of the random rician value. The explicit equations’ system have been obtained for required parameters of the signal and noise. In the limiting case of the small value of the signal-to-noise ratio the analytical formulas have been derived that allow calculating the required parameters without the necessity of solving the equations numerically. The technique having been elaborated in the paper ensures an efficient separation of the informative and noise components of the data to be analyzed without any a-priori restrictions, just based upon the processing of the results of the signal’s sampled measurements. The task is meaningful for the purposes of the rician data processing, in particular in the systems of magnetic-resonance visualization, in ultrasound visualization systems, at the optical signals’ analysis in range measuring systems, in radio location, etc. The results of the investigation have shown that the two parameter task solution of the proposed technique does not lead to the increase in demanded volume of computing resources compared with the one parameter task being solved in approximation that the second parameter of the task is known a-priori There are provided the results of the elaborated technique’s computer simulation. The results of the signal and noise parameters’ numerical calculation have confirmed the efficiency of the elaborated technique. There has been conducted the comparison of the accuracy of the sought-for parameters estimation by the technique having been developed in this paper and by the previously elaborated method of moments based upon processing the measured data for lower even moments of the signal to be analyzed.

The Richtmyer–Meshkov and the Rayleigh–Taylor instabilities of viscoplastic (or the Bingham) fluids are studied in the three–dimensional formulation of the problem. A numerical modeling of the intermixing of two fluids with different rheology, whose densities differ twice, as a result of instabilities development process has been carried out. The development of the Richtmyer–Meshkov and the Rayleigh–Taylor instabilities of the Bingham fluids is analyzed utilizing the MacCormack and the Volume of Fluid (VOF) methods to reconstruct the interface during the process. Both the results of numerical simulation of the named instabilities of the Bingham liquids and their comparison with theory and the results of the Newtonian fluid simulation are presented. Critical amplitude of the initial perturbation of the contact boundary velocity field at which the development of instabilities begins was estimated. This critical amplitude presents because of the yield stress exists in the Bingham fluids. Results of numerical calculations show that the yield stress of viscoplastic fluids essentially affects the nature of the development of both Rayleigh–Taylor and Richtmyer–Meshkov instabilities. If the amplitude of the initial perturbation is less than the critical value, then the perturbation decays relatively quickly, and no instability develops.When the initial perturbation exceeds the critical amplitude, the nature of the instability development resembles that of the Newtonian fluid. In a case of the Richtmyer–Meshkov instability, the critical amplitudes of the initial perturbation of the contact boundary at different values of the yield stress are estimated. There is a distinction in behavior of the non-Newtonian fluid in a plane case: with the same value of the yield stress in three-dimensional geometry, the range of the amplitude values of the initial perturbation, when fluid starts to transit from rest to motion, is significantly narrower. In addition, it is shown that the critical amplitude of the initial perturbation of the contact boundary for the Rayleigh–Taylor instability is lower than for the Richtmyer–Meshkov instability. This is due to the action of gravity, which helps the instability to develop and counteracts the forces of viscous friction.