The University of Southampton
University of Southampton Institutional Repository

Long extra-tropical planetary wave propagation in the presence of slowly varying mean flow and bottom topography. II: ray propagation and comparison with observations

Long extra-tropical planetary wave propagation in the presence of slowly varying mean flow and bottom topography. II: ray propagation and comparison with observations
Long extra-tropical planetary wave propagation in the presence of slowly varying mean flow and bottom topography. II: ray propagation and comparison with observations
Ray theory is used to predict phase and group velocities for long planetary waves under realistic, albeit slowly varying, oceanic conditions. The results are compared with local theory using fields smoothed to the same amount (9° latitude/longitude) as well as those with much less smoothing (1°). The agreement is excellent, showing that local theory forms a good proxy for ray theory results. The predicted speeds agree well with observations of planetary waves deduced from sea surface height data. The theory uses purely baroclinic mean flow; the inclusion of barotropic flow has little effect except at high latitudes.
0022-3670
802-821
Killworth, Peter D.
cdb4e8d3-c5eb-48b8-860a-0b16473b5d44
Blundell, Jeffrey R.
88114f32-6b76-46b2-b2d8-d6ef64a82b0d
Killworth, Peter D.
cdb4e8d3-c5eb-48b8-860a-0b16473b5d44
Blundell, Jeffrey R.
88114f32-6b76-46b2-b2d8-d6ef64a82b0d

Killworth, Peter D. and Blundell, Jeffrey R. (2003) Long extra-tropical planetary wave propagation in the presence of slowly varying mean flow and bottom topography. II: ray propagation and comparison with observations. Journal of Physical Oceanography, 33 (4), 802-821. (doi:10.1175/1520-0485(2003)33<802:LEPWPI>2.0.CO;2).

Record type: Article

Abstract

Ray theory is used to predict phase and group velocities for long planetary waves under realistic, albeit slowly varying, oceanic conditions. The results are compared with local theory using fields smoothed to the same amount (9° latitude/longitude) as well as those with much less smoothing (1°). The agreement is excellent, showing that local theory forms a good proxy for ray theory results. The predicted speeds agree well with observations of planetary waves deduced from sea surface height data. The theory uses purely baroclinic mean flow; the inclusion of barotropic flow has little effect except at high latitudes.

Text
rossby2.pdf - Other
Download (1MB)

More information

Published date: 2003

Identifiers

Local EPrints ID: 11231
URI: http://eprints.soton.ac.uk/id/eprint/11231
ISSN: 0022-3670
PURE UUID: de5e96f4-1a3b-4719-8253-833bae8a72a3

Catalogue record

Date deposited: 04 Nov 2004
Last modified: 15 Mar 2024 05:03

Export record

Altmetrics

Contributors

Author: Peter D. Killworth

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×