by Pierre Flament, Laurence Armi and Libe Washburn
Scripps Institution of Oceanography, University of California San Diego, La Jolla CA 92093
(J. Geophys. Res. vol. 90 no. C6 pp 11,765-11,778 and 11,835-11,837, 1985)
Received 16 May 1985; accepted 19 June 1985.
The evolution of an upwelling filament was studied over a 2-week period by using satellite infrared images, and its thermohaline structure was mapped in situ. The surface velocity field consisted of a large meander extending offshore for at least 300 km. The northern branch was ∼40 km wide, flowing offshore at a peak velocity of 0.55 m/s; the southern branch was flowing inshore at 0.35 m/s. The offshore transport was more than 106 m3 s−1, larger than the Ekman transport. The meander was unstable to barotropic instabilities at a scale of ∼15 km. From a succession of images a surface convergence γ ≈ 8·10−6 s−1 over 20 km was observed near the sharp front limiting the filament to the south. The ∼350 m width of the front indicates a separation of scales between the large-scale strain field and the mixed-layer turbulence parameterized with an eddy diffusion coefficient K H ≈ 0.25 m2 s−1. Thermohaline layers that originated at the convergence near the sharp front suggest a secondary circulation subducting denser waters to the south underneath the lighter northern water.