Pages that link to "Item:Q2863827"
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The following pages link to Introduction to modeling convection in planets and stars. Magnetic field, density stratification, rotation (Q2863827):
Displaying 10 items.
- Rotating shallow water modeling of planetary, astrophysical and plasma vortical structures. (Plasma transport across a magnetic field, model of the Jupiter's GRS, prediction of existence of giant vortices in spiral galaxies) (Q1585759) (← links)
- Multi-physics adjoint modeling of Earth structure: combining gravimetric, seismic, and geodynamic inversions (Q2068861) (← links)
- Full-wave anelastic and compressible Fourier methods for gravity waves in the thermosphere (Q2124146) (← links)
- An assessment of implicit-explicit time integrators for the pseudo-spectral approximation of Boussinesq thermal convection in an annulus (Q2137962) (← links)
- A semi-implicit spectral method for compressible convection of rotating and density-stratified flows in Cartesian geometry (Q2375012) (← links)
- A model of thermal convection in the major planets with a strongly density-stratified atmospheric layer (Q3710276) (← links)
- Large-scale vortices and zonal flows in spherical rotating convection (Q4965292) (← links)
- On the equatorial Ekman layer (Q4976846) (← links)
- Validity of sound-proof approaches in rapidly-rotating compressible convection: marginal stability versus turbulence (Q5063509) (← links)
- The onset of thermo-compositional convection in rotating spherical shells (Q5065638) (← links)
