The effect of the fan-shaped divergence of isopycnals in the permanent halo
cline of the Stolpe Channel observed in the sections across the channel is
studied numerically with the use of the known Blumberg-Mellor model. The ci
rculation induced by the force of the wind along the channel is also studie
d. The results prove the observed fan-shaped effect, which disappears in th
e absence of bottom friction, and support the hypothesis on the formation o
f the fan-shaped structure by circulation across the channel due to the Ekm
an transport in the near-bottom boundary layer.