Southern mid- to high-latitude variability, a zonal wavenumber-3 pattern, and the Antarctic circumpolar wave in the CSIRO coupled model

Variability in the southern atmospheric circulation at mid- to high latitud es with a dominant quasi-stationary wavenumber-3 pattern has been reported in many observational studies. The variability is barotropic in nature with signals in the middle troposphere as well as at the atmosphere-ocean inter face. Moreover, there are preferred Fixed centers for the strongest anomali es. These features are well reproduced by the Commonwealth Scientific and I ndustrial Research Organisation coupled model on various timescales. On the interannual timescale. an index of the modeled wavenumber-3 pattern shows little correlation with the modeled Southern Oscillation index, suggesting that the variability associated with wavenumber 3 anomalies is separate to modeled ENSO-like events. However, the variation of the pattern index is st rikingly similar to, and highly correlated with, the modeled oceanic variab ility. The associated oceanic anomalies move eastward and are similar to th ose of the observed Antarctic circumpolar wave (ACW). The modeled ACW-like anomalies exist not only at the surface but also through middle ocean depth s, with a similar barotropic nature to those of the atmospheric anomalies. The oceanic anomalies also display a wavenumber-3 pattern. The essential elements of the dynamics of the modeled ACW are the advection of SST anomalies by the surface Antarctic Circumpolar Current (ACC), and t he interactions between anomalies of SST and mean sea level pressure (MSLP) . Associated with the standing wavenumber-3 pattern, there are fixed center s for the strongest MSLP anomalies. As a positive SST anomaly advected by s urface ACC approaches a center of a positive MSLP anomaly, the MSLP decreas es. The positive (negative) SST anomalies are generated by anomalous latent and heat fluxes, which are in turn induced by southward (northward) meridi onal wind stress anomalies resulting from geostrophic balance. These MSLP a nomalies change sign when the positive (negative) SST anomalies move to a l ocation near the centers. Once MSLP anomalies change sign, positive (negati ve) SST anomalies are generated again reinforcing the anomalies entering fr om the west. The time for the surface ACC to advect one-sixth of the circui t around the pole corresponds to the time of a half-cycle of the standing M SLP oscillations. Thus the surface ACC determines the frequency of the stan ding oscillation. In the present model, the speed of the surface ACC is suc h that the period of the standing oscillation is 4-5 yr, and it would take 12-16 yr for an anomaly to encircle the pole. These and other features of t he modeled ACW, together with associated dynamic processes, are analyzed an d discussed.