  A two-fluid model developed originally to describe wave oscillations in the
vacuum arc centrifuge, a cylindrical, rapidly rotating, low temperature and
confined plasma column, is applied to interpret plasma oscillations in a RF
generated linear magnetised plasma (WOMBAT), with similar density and field
strength. Compared to typical centrifuge plasmas, WOMBAT plasmas have slower
normalised rotation frequency, lower temperature and lower axial velocity.
Despite these differences, the two-fluid model provides a consistent
description of the WOMBAT plasma configuration and yields qualitative agreement
between measured and predicted wave oscillation frequencies with axial field
strength. In addition, the radial profile of the density perturbation predicted
by this model is consistent with the data. Parameter scans show that the
dispersion curve is sensitive to the axial field strength and the electron
temperature, and the dependence of oscillation frequency with electron
temperature matches the experiment. These results consolidate earlier claims
that the density and floating potential oscillations are a resistive drift
mode, driven by the density gradient. To our knowledge, this is the first
detailed physics model of flowing plasmas in the diffusion region away from the
RF source. Possible extensions to the model, including temperature
non-uniformity and magnetic field oscillations, are also discussed.
