Microstructure measurements in the equatorial Pacific at 140¿W in late 1984 show a pronounced diurnal variation in both high-frequency internal wave energy and kinetic energy dissipation rate. Observations indicated that after sunset, internal waves (presumably generated by convective overturns in the mixed layer) propagate downward and increase turbulence levels in the pycnocline. It is proposed that large mixed layer eddies in the South Equatorial Current interact with the large shear caused by the Equatorial Undercurrent to generate a westward going anisotropic wave field. The momentum transport in the radiated wave field results in a drag force on the equatorial mean flow field. The observed mean wind stress at 140¿W during Tropic Heat I (which is twice as large as the annual mean wind) is closer to the estimated radiation stress (~-10-4 m2 s-2) at the base of the mixed layer (≈30 m) than to the estimated turbulent stress (~-10-5 m2 s-2). A wave dissipation model based on the observed turbulent kinetic energy dissipation rate is introduced in order to estimate the wave momentum flux divergence in the stratified region above the undercurrent core. The model predicts that most of the downward wave momentum flux penetrates through the undercurrent core. It is hypothesized that when the wind stress is strong, the equatorial Pacific Ocean responds by generating a westward traveling internal wave field which transports much of the surface wind stress below the actively mixing surface layer. ¿1991 American Geophysical Union