Pages that link to "Item:Q2947694"
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The following pages link to Thermal shallow water models of geostrophic turbulence in Jovian atmospheres (Q2947694):
Displaying 12 items.
- A well-balanced central-upwind scheme for the thermal rotating shallow water equations (Q777618) (← links)
- A quasi-Hamiltonian discretization of the thermal shallow water equations (Q2169492) (← links)
- Deep two-dimensional turbulence: An idealized model for atmospheric jets of the giant outer planets (Q3081177) (← links)
- Jupiter's zonal winds: are they bands of homogenized potential vorticity organized as a monotonic staircase? (Q3090269) (← links)
- Statistical equilibrium predictions of jets and spots on Jupiter (Q4547684) (← links)
- Structure-Preserving Reduced- Order Modeling of Non-Traditional Shallow Water Equation (Q5014032) (← links)
- Thermal versus isothermal rotating shallow water equations: comparison of dynamical processes by simulations with a novel well-balanced central-upwind scheme (Q5065742) (← links)
- Two-dimensional partially ionized magnetohydrodynamic turbulence (Q5115987) (← links)
- Super- and sub-rotating equatorial jets in shallow water models of Jovian atmospheres: Newtonian cooling versus Rayleigh friction (Q5364814) (← links)
- Flux Globalization Based Well-Balanced Path-Conservative Central-Upwind Scheme for the Thermal Rotating Shallow Water Equations (Q6143619) (← links)
- Equatorial modons in thermal rotating shallow water model (Q6491302) (← links)
- The QG limit of the rotating thermal shallow water equations (Q6584902) (← links)
