Abstract
The authors describe a method utilizing short-duration drifter tracks to compute rotary velocity amplitudes and phases for tidal frequency bands. These are compared to amplitudes and phases from a tidal model, revealing the regions where strong internal tides dominate the observed record or the times when inertial motions compete with the tidal signals. This method therefore enables a direct comparison between Lagrangian drifter data and Eulerian model simulations, while providing information on possible origin and spatial variability of tidal currents.
Corresponding author address: Dr. William Crawford, Institute of Ocean Sciences, P.O. Box 6000, Sidney, BC V8L 4B2, Canada.
Email: crawford@dfo-mpo.gc.ca