This work describes a one-dimensional (1-D) steady-state model of the
Hartmann boundary layers appropriate to a high-density rotating plasma
which is in local thermodynamic equilibrium. The purpose of the model
is to predict the performance of high-pressure plasma centrifuges, an
d approximations appropriate to magnetohydrodynamic plasmas are made,
Transport properties are calculated using a chemical equilibrium appro
ximation which should apply at high densities in a plasma centrifuge.
As well as rotation in the azimuthal direction, the model shows that t
here is plasma circulation in the radial direction, arising both from
convection of the neutral particles with the ions (''ion wind'') and t
he nonuniform distribution of the centrifugal force in the axial direc
tion (conventional secondary how), Calculated results have been compar
ed with experimental data from a rotating argon plasma, The agreement
is reasonable.