Ocean Mixing by Kelvin-Helmholtz Instability
Kelvin-Helmholtz (KH) instability, characterized by the distinctive finite-amplitude billows it generates, is an important mechanism in the development of turbulence in the stratified interior of the ocean. In particular, it is often assumed that the onset of turbulence in internal waves begins in t...
| Main Authors: | , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
The Oceanography Society
2012-06-01
|
| Series: | Oceanography |
| Subjects: | |
| Online Access: | http://tos.org/oceanography/archive/25-2_smyth.pdf |