A computational model has been developed that allows calculation of
the radiofrequency (RF) power reflected by grill waveguide antennas,
employed for additional heating of tokamak plasmas. The plasma surface
impedance is evaluated using a full wave analysis with the SEMAL code
(Sauter, O., Vaclavik, J., Comput. Phys. Commun. 84 (1994) 226),
which solves
the integrodifferential equations for the electric field of the wave in
configuration space, in an inhomogeneous plasma, for any cyclotron
harmonic and without any approximation with respect to the Larmor
radius. These features are necessary for solving the problem of the
antenna coupling of the ion Bernstein wave (IBW) plasma heating
experiment, operating at an ion cyclotron harmonic higher than the second.
In this experiment, the antenna coupling has to be carefully
considered, in order to find suitable antenna-plasma conditions
for avoiding parametric instabilities, a phenomenon that inhibits
wave propagation in the plasma interior. As a result, for an IBW
experiment on the FTU tokamak, a good antenna coupling is expected by
assuming a low plasma density near the antenna-plasma interface.
Nevertheless, by considering higher plasma densities, so that a low
activity of the parametric instabilities is expected, a marginal
antenna coupling has been found, with about 40% of RF power reflected
at the antenna.