  We performed a multi-wave study of the oscillation dynamic in short-lived
facula regions during their lifetime. We studied oscillations in five regions,
three of which belonged to the beginning of the current solar activity cycle,
and two of them existed at the end of the previous cycle. We found that in the
facula regions of the current cycle, low-frequency 1-2 mHz oscillation
dominated at the early stages of the faculae formation, while in the regions of
the previous cycle, five-minute oscillations dominated at this stage. At the
maximal development phase of all the facula regions, the locations of observed
low frequencies are closely related to those of the coronal loops. These
results support the version that the sources of the low-frequency oscillations
in loops lie loops' foot points.
