  One of the most exciting benefits of solar small-scale brightening is their
oscillations, this study investigated the properties of small-scale brightening
(SSBs) in different regions of the Sun and found that there are differences and
similarities in the properties of oscillated and non-oscillated SSBs in
different regions of the Sun, including quiet Sun (QS), the adjacent to active
regions (AAR), and coronal hole (CH). The damping per period (Q-factor) and
maximum Doppler velocity of SSBs varied depending on the region, with the less
bright internetwork SSBs in QS having lower damping time (120 seconds) and
higher maximum Doppler velocities (47 km/s) compared to the brighter network
SSBs (with 216 seconds & 37 km/s, respectively), while in AAR, internetwork
SSBs tend to have higher damping time (about of 220 seconds) and wider maximum
Doppler velocity (10 to 140 km/s) ranges compared to network SSBs (130 seconds
& 10 to 85 km/s). In CH, both types of SSBs show similar damping time (120
seconds), but internetwork SSBs tend to have higher maximum Doppler velocities
(100 km/s) compared to network SSBs (85 km/s). Also, it was pointed out that
the majority of network SSBs in AARs are in the overdamping mode, while in QS,
internetwork SSBs demonstrate overdamping behavior and oscillated network SSBs
exhibit critical damping behavior. It is important to bear in mind, however,
that the physical mechanisms underlying the damping of SSBs may vary depending
on the local plasma conditions and magnetic environment.
