The authors describe a method utilizing short-duration drifter tracks
to compute rotary velocity amplitudes and phases for tidal frequency b
ands. These are compared to amplitudes and phases from a tidal model,
revealing the regions where strong internal tides dominate the observe
d record or the times when inertial motions compete with the tidal sig
nals. This method therefore enables a direct comparison between Lagran
gian drifter data and Eulerian model simulations, while providing info
rmation on possible origin and spatial variability of tidal currents.