Wind-driven Equatorial Oscillations in the Meridional Overturning Circulation
Abstract:
We present analysis of a set of integrations of a global configuration of the numerical ocean model, which show very large amplitude oscillations in the MOCs in the Atlantic, Indian and Pacific oceans confined to the equatorial region. The amplitude of these oscillations is proportional to the width of the ocean basin, typically about 100 (200) Sv in the Atlantic (Pacific). We show that these oscillations are driven by surface winds within 10\degree N/S of the Equator, and their periods (typically 4-10 days) correspond to a small number of low mode equatorially trapped planetary waves. These high frequency fluctuations in the MOC can be accurately simulated by linearising the equations of motion about a stably stratified state of rest and projecting the wind forcing onto the meridional and vertical normal modes. Although no direct observations of these MOC oscillations exist, previous studies using data from the TAO/TRITON identified the existence of equatorially trapped planetary waves in the Pacific basin, exciting vertical displacement of the 500 db dynamic height, giving confidence that this MOC variability occurs in reality.