Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
4533935 | Continental Shelf Research | 2006 | 19 Pages |
Abstract
The additional eddy kinetic energy of the residual flow (defined here as the kinetic energy contained in the spatial scales between 3 and 20Â km) in general is around two orders of magnitude smaller than the mean kinetic energy. However, there are several areas where the eddy kinetic energy reaches the same order of magnitude as the mean kinetic energy, for instance in the Southern Bight. From the fact that largest eddy kinetic energy rates occur in areas of strongest gradients of the mean flow it could be deduced that barotropic instabilities play the dominant role. Contrarily, baroclinic instabilities seem to be only of minor importance since areas of strongest density gradients only exhibit very localised maxima.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geology
Authors
Thomas Pohlmann,