We observed the quasar 0917+624 at three epochs at a wavelength of 6 cm in
order to study its short-timescale variability. In December 1997 and Februa
ry 1999, the source showed its usual characteristics: variations on a 10-15
% level have been found on timescales less than or equal to 1.5 days. In c
ontrast, in September 1998 the source exhibited a monotonic increase of abo
ut 7 % during a five-day-observing campaign. Assuming an intrinsic origin o
f the variations, this corresponds to a change in brightness temperature of
at least two orders of magnitude. We discuss shortly several mechanisms wh
ich may cause the observed change of the variability properties of 0917+624
.