Flow structure and variability in the subtropical Indian Ocean: Instability of the South Indian Ocean Countercurrent

Details Flow structure and variability in the subtropical Indian Ocean: Instability of the South Indian Ocean Countercurrent Flow structure and variability in the subtropical Indian Ocean: Instability of the South Indian Ocean Countercurrent

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jgrc..11201001p&link_type=abstract

Journal of Geophysical Research, Volume 112, Issue C1, CiteID C01001

Physics

13

Oceanography: Physical: Currents, Oceanography: Physical: Fronts And Jets, Oceanography: Physical: General Circulation (1218, 1222), Oceanography: Physical: Planetary Waves

Scientific paper

The origin of the eddy variability around the 25°S band in the Indian Ocean is investigated. We have found that the surface circulation east of Madagascar shows an anticyclonic subgyre bounded to the south by eastward flow from southwest Madagascar, and to the north by the westward flowing South Equatorial Current (SEC) between 15° and 20°S. The shallow, eastward flowing South Indian Ocean Countercurrent (SICC) extends above the deep reaching, westward flowing SEC to 95°E around the latitude of the high variability band. Applying a two-layer model reveals that regions of large vertical shear along the SICC-SEC system are baroclinically unstable. Estimates of the frequencies (3.5-6 times/year) and wavelengths (290-470 km) of the unstable modes are close to observations of the mesoscale variability derived from altimetry data. It is likely then that Rossby wave variability locally generated in the subtropical South Indian Ocean by baroclinic instability is the origin of the eddy variability around 25°S as seen, for example, in satellite altimetry.

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