This paper is aimed at studying the efficiency of the electromagnetic radiation generation in various nonlinear processes occurring during the beamplasma interaction. The beam and plasma parameters were chosen close to the parameters in the experiment on the GOL-3 facility (BINP SB RAS). The…
In order to simplify the development of high-performance plasma physics codes for hybrid supercomputers, a template implementation of the Particlein-Cell (PIC) method was created. The template parameters are the problemspecific implementations of "particle" and "cell" (as C++ classes).
Thus, it is…
In this paper, a new hydrodynamic numerical simulation of interacting galaxies is proposed. The main subgrid physics processes are: the star formation, the supernovae feedback, the cooling function and the molecular hydrogen formation. The collisionless hydrodynamic approach was used for the…
The problem of network reliability calculation is studied. It is assumed that a network has unreliable communication links and perfectly reliable nodes. The diameter-constrained reliability for such a network is defined as probability that every pair of terminals of network is connected by…
The atmospheric chemistry dynamics with a convection-diffusion model is studied. The numerical Data Assimilation (DA) algorithm presented is based on the additive-averaged splitting schemes. It carries out "fine-grained" variational data assimilation at separate splitting stages with respect to the…
The main point of the performance of a code for a GPU (Graphical Processing Unit) is data locality. For the PIC method this means that all the particles belonging to one cell must be located closely in memory. During the particle push the particles might move to other cells, and must be transported…
We compare two algorithms for solving the Poisson equation: the first one is based on domain decomposition with direct coupling of subdomains (DDCS) and the second one is based on multidimensional Fast Fourier Transform and data transposition (FFTT).
Results of the comparison made helped us to…
We present a new parallel algorithm for supercomputer simulation of gas-dust circumstellar gravitating disks. The algorithm uses the domain decomposition technique and combines numerical methods of smooth particle hydrodynamics (SPH), particle-in-cell (PIC) and grid-based gravitational solver with…
We present a 2D hybrid numerical plasma model for the simulation of the physical processes in supernova remnant shock precursor. In simulation, a shock is generated by sending a supersonic ow against a reflecting wall. The interaction between the incoming and reflected streams produces a sharp…