Using a nearly one-thousand-year pre-industrial control simulation from the CESM2 Earth System Model in the CMIP6 archive, we identify positive Indian Ocean Dipole (pIOD) events and categorize them into single-year and consecutive multi-year (two- and three-year) types based on their duration. Direct comparisons between different types are conducted to reveal their impacts on Antarctic spring sea ice and atmospheric circulation. Results show that sea ice anomaly patterns triggered by pIOD events are strongly duration-dependent. Single-year events lead to a dipole pattern in the west Antarctic, whereas multi-year events are characterized by an eastward shift and meridional expansion of the anomaly centers. The lower-tropospheric circulation anomalies, guided by Rossby wave trains, are the key mechanism underlying these differences. Sea ice anomalies are modulated by both dynamic processes (Ekman transport and thermal advection) and thermodynamic processes (downwelling shortwave and longwave radiation). Compared with single-year events, multi-year events tend to generate more persistent and stronger Rossby wave trains, which increase and maintain impacts on Antarctic sea ice. Furthermore, quantitative sea ice mass budget analysis shows that the changes in sea ice mass are mainly attributed to dynamic processes, basal melting, and snow-to-ice conversion.
 

Antarctic sea ice,Indian Ocean Dipole,Circulation anomalies,Sea ice mass budget