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 &ggr;≈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 KH≈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.