The formation process of intermediate water in baroclinic current under coo
ling is investigated using a nonhydrostatic numerical model. After baroclin
ic instability develops into finite amplitude in a short time, strong downd
rafts with a horizontal scale of I km are generated near the density front
and subduct surface water to depths (similar to 400 m) along isopycnals. As
a result, patches of ventilated water of 10 similar to 20 km horizontal sc
ale with anticyclonic circulation are formed at intermediate depths. Combin
ed effects of baroclinic instability and convection are key dynamics for th
ese phenomena. Convection acts as an initiator for baroclinic instability a
t the onset and accelerates its subsequent growth by reducing stratificatio
n. Developed baroclinic wave forms an intense density front, and downdraft
along isopycnals is generated through the frontogenetic process. Density ch
ange due to convection intensifies this frontal downdraft by strengthening
the geostrophic forcing (tendency to destroy the geostrophic balance) and b
y reducing potential vorticity (static stability). Further, symmetric insta
bility induced by the density change due to convection and intensified by t
he frontogenetic process drives slantwise convection, which in turn, enhanc
es the frontal downdraft. Consequent downward velocity becomes > 20 times a
s large as that of the frontal downdraft without convection (cooling) and t
wice larger than that of pure convection. Since the intensified frontal dow
ndraft moves its position with time and induces divergent how at depths, a
patch of ventilated water with a horizontal scale much larger than that of
the frontal downdraft is formed. The role of convection (cooling) in the fo
rmation process of intermediate water in this context is to enhance the fro
ntal downdraft rather than to deepen the mixed layer This scenario is quite
different from the one realized when baroclinic instability and convection
do not coexist.