Thermal shallow water models of geostrophic turbulence in Jovian atmospheres

DOI10.1063/1.4861123zbMath1321.85002OpenAlexW1993910466MaRDI QIDQ2947694

Paul J. Dellar, Emma S. Warneford

Publication date: 28 September 2015

Published in: Physics of Fluids (Search for Journal in Brave)

Full work available at URL: https://semanticscholar.org/paper/042be04643fe5893e178e5339e385d48436313dd

Mathematics Subject Classification ID

Water waves, gravity waves; dispersion and scattering, nonlinear interaction (76B15) Planetary atmospheres (85A20) Stratification effects in turbulence (76F45)

Related Items (7)

Thermal versus isothermal rotating shallow water equations: comparison of dynamical processes by simulations with a novel well-balanced central-upwind scheme ⋮ A quasi-Hamiltonian discretization of the thermal shallow water equations ⋮ Flux Globalization Based Well-Balanced Path-Conservative Central-Upwind Scheme for the Thermal Rotating Shallow Water Equations ⋮ Two-dimensional partially ionized magnetohydrodynamic turbulence ⋮ Super- and sub-rotating equatorial jets in shallow water models of Jovian atmospheres: Newtonian cooling versus Rayleigh friction ⋮ A well-balanced central-upwind scheme for the thermal rotating shallow water equations ⋮ Structure-Preserving Reduced- Order Modeling of Non-Traditional Shallow Water Equation

Cites Work

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