The pseudospectral method in thermal convection models of a rotating
Numerical methods and programming, Tome 12 (2011) no. 1, pp. 77-84
Voir la notice de l'article provenant de la source Math-Net.Ru
The numerical application and parallelization of the classical thermal
convection models for a spherical shell are discussed. These models are
used in the modern planetary dynamo models with consideration of the inner
core rotation due to the viscous forces. Several scaling tests for a parallel
model with the parallelization in the radial direction for a cluster computing
systems are considered. The test results confirm a good scalability of the
method for typical three-dimensional grids of $64^3$ nodes.
Keywords:
spherical functions; Chebyshev polynomials; geostrophic state; cluster systems.
@article{VMP_2011_12_1_a8,
author = {M. Yu. Reshetnyak},
title = {The pseudospectral method in thermal convection models of a rotating},
journal = {Numerical methods and programming},
pages = {77--84},
publisher = {mathdoc},
volume = {12},
number = {1},
year = {2011},
language = {ru},
url = {http://geodesic.mathdoc.fr/item/VMP_2011_12_1_a8/}
}
M. Yu. Reshetnyak. The pseudospectral method in thermal convection models of a rotating. Numerical methods and programming, Tome 12 (2011) no. 1, pp. 77-84. http://geodesic.mathdoc.fr/item/VMP_2011_12_1_a8/