A fine resolution numerical model of the Southern Ocean (the Fine Reso
lution Antarctic Model (FRAM)) has been used to investigate the way in
which heat is supplied to the South Atlantic. The heat budget in the
model is compared with other estimates and is found to be broadly real
istic. The temperature structure in the Atlantic, and therefore the me
ridional heat transport, depend heavily on the input of heat from the
Indian Ocean via the Agulhas Retroflection region. FRAM is compared wi
th three models which do not exhibit a significant input of heat from
the Indian Ocean. These models also have a lower equatorward heat tran
sport in the South Atlantic. Horizontal resolution affects the amount
of Agulhas transfer with coarser resolution leading to lower heat tran
sport in the Atlantic, a result which has implications for ocean model
s used in climate simulations.