The half-zone model is investigated for unit aspect ratio, zero gravity, an
d Prandtl numbers Pr = 1.5...7 by numerical simulations. For thermocapillar
y Reynolds numbers Re > Re-c, the 2D stationary flow is unstable to 3D trav
elling waves. In the simulations, standing waves can be generated slightly
above Re,. It is found, that these states are unstable and decay into eithe
r a clock or a counter-clockwise propagating wave. Amplitude equations are
used to quantitatively describe the instability of the standing wave states
and to estimate the range of Pr within which only travelling waves are sta
ble.