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Two computational approaches for the simulation of fluid problems in rotating spherical shells

Author
Garcia, F.; Dormy, E.; Sanchez, J.; Net, M.
Type of activity
Presentation of work at congresses
Name of edition
5th International Conference on Computational Methods - ICCM2014
Date of publication
2014
Presentation's date
2014-07
Book of congress proceedings
Proc. of the 5th International Conference on Computational Methods - ICCM2014
First page
1
Last page
13
Repository
http://hdl.handle.net/2117/27104 Open in new window
URL
http://www.sci-en-tech.com/ICCM2014/ICCM2014-Proceedings.pdf Open in new window
Abstract
Many geophysical and astrophysical phenomena such as magnetic fields generation, or the differential rotation observed in the atmospheres of the major planets are studied by means of numerical simulations of the Navier-Stokes equations in rotating spherical shells. Two different computational codes, spatially discretized using spherical harmonics in the angular variables, are presented. The first code, PARODY, solves the magneto-hydrodynamic anelastic convective equations with finite a differenc...
Citation
Garcia, F. [et al.]. Two computational approaches for the simulation of fluid problems in rotating spherical shells. A: 5th International Conference on Computational Methods - ICCM2014. "Proc. of the 5th International Conference on Computational Methods - ICCM2014". Cambridge: 2014, p. 1-13.
Keywords
Direct numerical simulation, Dynamical systems, Hydrodynamics, Parallelism, Spherical shells
Group of research
DF - Dinàmica de Fluids: formació d'estructures i aplicacions geofísiques

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