The dynamics of the meridional cells in the Southern Ocean simulated b
y a primitive equation model are investigated. Particular attention is
drawn to the Deacon cell, which transports about 15 Sv (Sv = 10(6) m3
s-1) from the surface between 45-degrees-S and 35-degrees-S down to 2
500 m without crossing any isopycnals. A theory of the Deacon cell is
presented using a Sverdrup-Munk-based model with an Ekman layer at the
surface. The simple model successfully simulates a Deacon cell when a
pplied to the Southern Ocean. The explanation of the Deacon cell appea
rs to be the depth differences of the western boundary current and the
Sverdrupian interior flow. The theory is extended to the other cells
in the Southern Ocean by replacing the Sverdrup solution with a Luyten
, Pedlosky, and Stommel solution. These other cells are driven at the
surface by the ventilation provided by the Ekman pumping.