Pages that link to "Item:Q1606908"
From MaRDI portal
The following pages link to Computational aspects of a code to study rotating turbulent convection in spherical shells (Q1606908):
Displaying 13 items.
- ASH (Q18807) (← links)
- A compressible high-order unstructured spectral difference code for stratified convection in rotating spherical shells (Q349773) (← links)
- Numerical simulation of core convection by a multi-layer semi-implicit spherical spectral method (Q422498) (← links)
- Simulations of stellar convection with CO5BOLD (Q423801) (← links)
- A Fourier-spectral element algorithm for thermal convection in rotating axisymmetric containers (Q1775787) (← links)
- An assessment of implicit-explicit time integrators for the pseudo-spectral approximation of Boussinesq thermal convection in an annulus (Q2137962) (← links)
- Helicity generation and subcritical behaviour in rapidly rotating dynamos (Q2893751) (← links)
- Linear theory of compressible convection in rapidly rotating spherical shells, using the anelastic approximation (Q3550344) (← links)
- Development of a Simulation Code for MHD Dynamo Processes Using the GeoFEM Platform (Q4661260) (← links)
- Advances in geodynamo modelling (Q5063539) (← links)
- Implementation of a high-order combined compact difference scheme in problems of thermally driven convection and dynamo in rotating spherical shells (Q5875282) (← links)
- Magnetohydrodynamic simulations of the elliptical instability in triaxial ellipsoids (Q5875303) (← links)
- Comparison of the anelastic approximation with fully compressible equations for linear magnetoconvection and magnetic buoyancy (Q5876533) (← links)
