Quasigeostrophic models of convection in rotating spherical shells

59Citations
Citations of this article
22Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

The use of a quasigeostrophic, two-dimensional approximation in the problem of convection in a rapidly rotating spherical shell has been limited so far to investigations of the qualitative behavior of the solution. In this study, we build a quasigeostrophic model that agrees quantitatively with full threedimensional solutions of the onset of convection in the case of differential heating. Reducing the dimensionality of the problem also permits the simulation of finite amplitude regimes of convection, up to quasigeostrophic turbulence. The nonlinear behavior of the system is studied in detail and compared to ultrasonic Doppler velocimetry measurements performed in a convecting, rapidly rotating spherical shell filled with water and liquid gallium. The results are quantitatively satisfactory and open the way to less computer-demanding, and still accurate, simulations of the geodynamo. © 2003 by the American Geophysical Union.

Cite

CITATION STYLE

APA

Aubert, J., Gillet, N., & Cardin, P. (2003). Quasigeostrophic models of convection in rotating spherical shells. Geochemistry, Geophysics, Geosystems, 4(7). https://doi.org/10.1029/2002GC000456

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free