Pages that link to "Item:Q422498"

The following pages link to Numerical simulation of core convection by a multi-layer semi-implicit spherical spectral method (Q422498):

Displaying 8 items.

• A compressible high-order unstructured spectral difference code for stratified convection in rotating spherical shells (Q349773) (← links)
• Curvilinear grids for WENO methods in astrophysical simulations (Q525764) (← links)
• Radial collocation methods for the onset of convection in rotating spheres (Q729463) (← links)
• A semi-implicit spectral method for compressible convection of rotating and density-stratified flows in Cartesian geometry (Q2375012) (← links)
• Modelling the core convection using finite element and finite difference methods (Q3649097) (← links)
• A multiple shooting approach for the numerical treatment of stellar structure and evolution (Q4861371) (← links)
• Radius ratio dependency of the instability of fully compressible convection in rapidly rotating spherical shells (Q5154669) (← links)
• Onset of fully compressible convection in a rapidly rotating spherical shell (Q5229703) (← links)