Abstract
A novel fluid/gyro-kinetic hybrid model to study drift waves in
low-pressure stellarator plasmas is presented. The ion population is modeled
with the collisionless gyro-kinetic equation and the electron population is
described using fluid equations. The model equations are written in
straight-field-line coordinates and are valid for any magnetic configuration
with closed, nested magnetic surfaces. The geometrical effects which enter the
final eigenmode equations are derived and discussed in some detail. The
numerical method used to solve the coupled, time-dependent,
along-the-field-line equations is described. The geometrical effects are
discussed in some detail. Numerical calculations are carried out for a
three-field period toroidal heliac with small global magnetic shear.
Subject
General Physics and Astronomy