scispace - formally typeset
Open AccessJournal ArticleDOI

Thermal instability in rotating shallow water with horizontal temperature/density gradients

Reads0
Chats0
TLDR
In this paper, a specific instability of vortices is found in rotating shallow water equations with horizontal density/temperature gradients, which is used for modelling atmospheric and oceanic mixed layers.
Abstract
A specific instability of vortices is found in rotating shallow water equations with horizontal density/temperature gradients, which is used for modelling atmospheric and oceanic mixed layers. The model is re-interpreted as dynamics of rotating non-isentropic two-dimensional gas. The instability, which was not reported previously, develops in a way suggesting its convective character. It appears when anomaly of buoyancy at the center of the vortex and the vorticity have opposite signs (for positive Coriolis parameters), and coexists with the standard barotropic instability, having higher growth rates in a wide range of parameters and leading to efficient mixing at a nonlinear stage.

read more

Citations
More filters
Journal ArticleDOI

Moist-convective thermal rotating shallow water model

TL;DR: In this paper, a self-consistent way, horizontal gradients of potential temperature and changes of the latter due to the condensation heating, radiative cooling, and ocean-atmosphere heat fluxes are introduced.
Journal ArticleDOI

A well-balanced central-upwind scheme for the thermal rotating shallow water equations

TL;DR: An analysis of the TRSW model based on the use of Lagrangian variables is presented, allowing one to obtain criteria of existence and uniqueness of the equilibrium state, of the wave-breaking and shock formation, and of instability development out of given initial conditions.
Journal ArticleDOI

A Quasi-Hamiltonian Discretization of the Thermal Shallow Water Equations

TL;DR: This work presents a quasi-Hamiltonian discretization of the thermal shallow water equations using compatible Galerkin methods, building on previous work done for the shallowWater equations.
Journal ArticleDOI

Thermal versus isothermal rotating shallow water equations: comparison of dynamical processes by simulations with a novel well-balanced central-upwind scheme

TL;DR: In this paper, a well-balanced central-upwind scheme for two-dimensional rotating shallow water equations with horizontal temperature/density gradients is proposed, based on thermal rotating shallow.
Journal ArticleDOI

Numerical dissipation switch for two-dimensional central-upwind schemes

TL;DR: In this article, a numerical dissipation switch is proposed to control the amount of dissipation present in central-upwind schemes without risking oscillations, which is achieved with the help of a more accurate estimate of the local propagation speeds in the parts of the computational domain.
References
More filters
Journal ArticleDOI

A numerical investigation of dynamics, thermodynamics and mixed-layer processes in the Indian Ocean

TL;DR: In this article, a 212-layer, thermodynamic numerical model is used to study the dynamics, thermodynamics and mixed-layer physics of Indian Ocean circulation, and a surface mixed layer of temperature Tm is imbedded in the upper layer of the model, and entrainment and detrainment in the mixed layer are determined by wind stirring and surface cooling.
Journal ArticleDOI

The Dynamics of Finite-Difference Models of the Shallow-Water Equations

TL;DR: In this paper, two simple numerical models of the shallow-water equations identical in all respects but for their conservation properties have been tested regarding their internal mixing processes, showing that violation of enstrophy conservation results in a spurious accumulation of rotational energy in the smaller scales, reflected by an unrealistic increase of enstroke, which ultimately produces a finite rate of energy dissipation in the zero viscosity limit, thus violating the well-known dynamics of two-dimensional flow.
Journal ArticleDOI

On Non-Geostrophic Baroclinic Stability

TL;DR: In this article, growth rates for various types of perturbations are found as a function of the Richardson number, and it is suggested that symmetric instabilities may play an important role in the dynamics of the atmospheres of the major planets of the solar system.
Journal ArticleDOI

A Mesoseale Numerical Model of Lake-Fffect Storms

TL;DR: In this paper, the atmospheric structure upwind of the Great takes during arctic air outbreaks is represented by three layers: a lower constant flux layer in contact with the ground, a well-mixed planetary boundary layer surmounted by an inversion, and a deep stratum of overlying stable air.
Journal ArticleDOI

Intense submesoscale upwelling in anticyclonic eddies

TL;DR: In this paper, high-resolution simulations of anticyclonic eddies are presented, showing that upwelling of nutrient-rich water occurs within the eddy, but such upwellings is not captured by models that resolve mesoscale processes.
Related Papers (5)