Skip to main content Accessibility help
×
Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-05T09:58:19.409Z Has data issue: false hasContentIssue false

3 - Fast singular oscillating limits of stably-stratified 3D Euler and Navier–Stokes equations and ageostrophic wave fronts

Published online by Cambridge University Press:  04 February 2010

John Norbury
Affiliation:
University of Oxford
Ian Roulstone
Affiliation:
University of Reading
Get access

Summary

Introduction

Flows that are stably-stratified or are rotating have certain distinct characteristics which, unlike many flows, vary greatly in their form depending on how the flows are initiated. The characteristics also change as the flows move towards their respective equilibrium or quasi-equilibrium states. The initial effects of rotational and buoyancy forces with time scales 1/f0 and 1/N0, respectively, are to produce internal waves on those time scales and hence to exchange energy between distant points in the flow leading to significant changes in the form of the imposed flow. Here N0 is the Brunt-Väisälä wave frequency and f0 = 2Ω0 is the Coriolis parameter. The significance of the wave motion depends on the relative magnitude of the flow's time scale, T, to the rotational and buoyancy time scales. The length scales L and geometric shape (especially the ratio of the vertical to horizontal scale, H/L) of the initial disturbances are equally significant in determining the anisotropic form of the wave motion and the orientation of the constrained equilibrium forms, such as the ‘Taylor’ columns parallel to the rotation axis in rotation-dominated regimes, or the horizontal ‘pancakes’ or fronts characteristic of strong stable stratification in stratification-dominated regimes with rotation.

Type
Chapter
Information
Large-Scale Atmosphere-Ocean Dynamics
Analytical Methods and Numerical Models
, pp. 126 - 201
Publisher: Cambridge University Press
Print publication year: 2002

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure [email protected] is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×