When a cylindrically-symmetric magnetized plasma compresses or expands,
velocity-space anisotropy is naturally generated as a result of the different
adiabatic conservation laws parallel and perpendicular to the magnetic field.
When the compression timescale is comparable to the collision timescale, and
both are much longer than the gyroperiod, this pressure anisotropy can become
significant. We show that this naturally-generated anisotropy can dramatically
affect the transport of impurities in the compressing plasma, even in the
absence of scalar temperature or density gradients, by modifying the azimuthal
frictions that give rise to radial particle transport. Although the impurity
transport direction depends only on the sign of the pressure anisotropy, the
anisotropy itself depends on the pitch magnitude of the magnetic field and the
sign of the radial velocity. Thus, pressure anisotropy effects can drive
impurities either towards or away from the plasma core. These
anisotropy-dependent terms represent a qualitatively new effect, influencing
transport particularly in the sparse edge regions of dynamically-compressing
screw pinch plasmas. Such plasmas are used for both X-ray generation and
magneto-inertial fusion, applications which are sensitive to impurity
concentrations.Comment: 11 pages, 3 figure