A form of the evolution equation for the dissipation showing the effec
ts of rotation is derived directly from the Navier-Stokes equations. R
otation affects the dissipation if the flow is inhomogeneous or compre
ssible. This is due to the fact that pressure scales with inverse Ross
by number and certain pressure correlations usually neglected have to
be retained when Re Ro almost-equal-to 1. The term reflecting the effe
cts of rotation on the dissipation is a volume integral of the two-poi
nt velocity correlation similar in structure to the ''rapid-pressure''
correlation appearing in the second-moment equations. Some of its pro
perties are indicated.