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Numerical methods and programming
Tome 17 (2016)
no. 3
Précédent
Suivant
Volume 17 (2016) no. 3
Sommaire
Application of polynomial transforms for fast 2D convolutions
I. A. Kalinovskii
;
V. G. Spitsyn
p. 197-203
Solution of a model inverse spectral problem for the Sturm--Liouville operator on a graph
N. F. Valeev
;
Yu. V. Martynova
;
Ya. T. Sultanaev
p. 204-211
Study of properties of a finite-difference scheme for the advection stage implementation in the lattice Boltzmann method
G. V. Krivovichev
;
E. S. Marnopolskaya
p. 212-223
Image processing algorithms for a light-field camera and their application for optical flow diagnostics
A. V. Seredkin
;
M. P. Tokarev
p. 224-233
A method of two-level parallelization of the Thomas algorithm for solving tridiagonal linear systems on hybrid computers with multicore coprocessors
A. A. Fedorov
;
A. N. Bykov
p. 234-244
Flow visualization with strong and weak gas dynamic discontinuities in computational fluid dynamics
P. V. Bulat
;
K. N. Volkov
;
M. S. Yakovchuk
p. 245-257
Mathematical modeling of inverse multipoint forming problems in the creep mode using a reconfigurable tool
K. S. Bormotin
;
S. V. Belykh
;
A. Vin
p. 258-267
Hybrid methods for modeling waveguides containing local inhomogeneous insets of multilayer structure
A. A. Petukhov
;
A. N. Bogolyubov
;
M. K. Trubetskov
p. 268-279
Some control and inverse problems for linear parabolic equations
N. L. Gol'dman
p. 280-290
2D and 3D algorithms of introcontinuation
Yu. V. Glasko
p. 291-298
Increasing regularity of generalized solutions to the wave equation for computing optimal boundary controls
D. A. Ivanov
p. 299-308
A study of coupling between viscoelastic parameters using the singular value decomposition analysis
E. S. Efimova
p. 309-317
Analysis and optimization of a
$k$
-chain reduction algorithm for distributed computer systems
M. G. Kurnosov
p. 318-328
Efficiency analysis of hydrodynamic calculations on GPU and CPU clusters
A. V. Sentyabov
;
A. A. Gavrilov
;
M. A. Krivov
;
A. A. Dekterev
;
M. N. Pritula
p. 329-338
Numerical simulation of gravitational instability development and clump formation in massive circumstellar disks using integral characteristics for the interpretation of results
O. P. Stoyanovskaya
p. 339-352