  The BLLac object S4 0954+65 is one of the main targets of the Urumqi
monitoring program targeting IntraDay Variable (IDV) sources. Between August
2005 and December 2009, the source was included in 41 observing sessions,
carried out at a frequency of 4.8 GHz. The time analysis of the collected light
curves, performed by applying both a structure function analysis and a
specifically developed wavelet-based algorithm, discovered an annual cycle in
the variability timescales, suggesting that there is a fundamental contribution
by interstellar scintillation to the IDV pattern of the source. The combined
use of the two analysis methods also revealed that there was a dramatic change
in the variability characteristics of the source between February and March
2008, at the starting time of a strong outburst phase. The analysis' results
suggest that the flaring state of the source coincides with the appearance of
multiple timescales in its light curves, indicating that changes in the
structure of the relativistically moving emitting region may strongly influence
the variability observed on IDV timescales.
