“…The parameters and the data that differ in the three cases considered, viz. </> 0 = 0.111 and uj = 146.4 rad/s; (j> 0 = 0.138 and w = 146.4 rad/s; 4> 0 = 0.138 and u = 104.9 rad/s, were chosen in such a way that the simulated supernate-suspension interfaces could be compared with measurements by Sambuichi et al [19], which are shown as open circles (o). While in the compression zone, where <j > > (j) c is valid and hence (16) is parabolic, the solutions are similar to those of the pure gravity case [2,5], there are some distinctive features visible in the hindered settling zone (</> < 4> c ) where (16) is hyperbolic, due to the rotating frame of reference.…”