Nonlinear and linear 41/2-layer ocean models are used to explore the dynami
cs of intraseasonal (20-90 day periods) zonal flow in the equatorial Indian
Ocean. The model simulations suggest that the observed 40-60 day zonal sur
face current is forced primarily by wind associated with the Madden-Julian
Oscillation (MJO), which peaks at 4060 days. The strongest spectral peak of
zonal flow, however, occurs at 90-day period in the model and a correspond
ing 90-day peak appears in the observed sea level data. The 90-day current
results from the preferential excitation of Kelvin and Rossby waves by the
lower-frequency component of intraseasonal wind and from the enhancement by
Rossby waves reflected from the eastern ocean boundary.