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We performed a multi-wave study of the oscillation dynamic in short-livedfacula 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 thefacula regions of the current cycle, low-frequency 1-2 mHz oscillationdominated at the early stages of the faculae formation, while in the regions ofthe previous cycle, five-minute oscillations dominated at this stage. At themaximal development phase of all the facula regions, the locations of observedlow frequencies are closely related to those of the coronal loops. Theseresults support the version that the sources of the low-frequency oscillationsin loops lie loops' foot points.

Oscillation Dynamics in Short-Lived Facula Regions during Their Lifetime