In a Doppler reflectometry experiment the line of sight is chosen to be non
perpendicular with respect to the reflecting layer. This type of diagnostic
is able to probe density perturbations with the wave number in the reflect
ing layer selected by the tilt angle. The propagation velocity of the pertu
rbations is calculated from the Doppler shift of the returning microwave si
gnal whereas its intensity contains information about the perturbation ampl
itude. The diagnostic capability of Doppler reflectometry is demonstrated a
t the W7-AS stellarator using an antenna system with variable tilt angle. T
he measured values of the propagation velocity of density perturbations and
its radial dependence are in good agreement with the ExB velocity of the p
lasma obtained from spectroscopy. Transient states can be followed with a t
emporal resolution less than 50 mus. Therefore Doppler reflectometry allows
one to test the interdependence of sheared flow and turbulence on that tim
escale. (C) 2001 American Institute of Physics.