Thrust-producing harmonically oscillating foils are studied through fo
rce and power measurements, as well as visualization data, to classify
the principal characteristics of the flow around and in the wake of t
he foil. Visualization data are obtained using digital particle image
velocimetry at Reynolds number 1100, and force and power data are meas
ured at Reynolds number 40 000. The experimental results are compared
with theoretical predictions of linear and nonlinear inviscid theory a
nd it is found that agreement between theory and experiment is good ov
er a certain parametric range, when the wake consists of an array of a
lternating vortices and either very weak or no leading-edge vortices f
orm. High propulsive efficiency, as high as 87%, is measured experimen
tally under conditions of optimal wake formation. Visualization result
s elucidate the basic mechanisms involved and show that conditions of
high efficiency are associated with the formation on alternating sides
of the foil of a moderately strong leading-edge vortex per half-cycle
, which is convected downstream and interacts with trailing-edge vorti
city, resulting eventually in the formation of a reverse Karman street
. The phase angle between transverse oscillation and angular motion is
the critical parameter affecting the interaction of leading-edge and
trailing-edge vorticity, as well as the efficiency of propulsion.