We present observations of a small-scale Extreme-ultraviolet ( EUV ) wave that was associated with a mini-filament eruption and a GOES B1.9 micro-flare in the quiet Sun region .
The initiation of the event was due to the photospheric magnetic emergence and cancellation in the eruption source region , which first caused the ejection of a small plasma ejecta , then the ejecta impacted on a nearby mini-filament and thereby led to the filament ’ s eruption and the associated flare .
During the filament eruption , an EUV wave at a speed of 182 – 317 km s ^ { -1 } was formed ahead of an expanding coronal loop , which propagated faster than the expanding loop and showed obvious deceleration and reflection during the propagation .
In addition , the EUV wave further resulted in the transverse oscillation of a remote filament whose period and damping time are 15 and 60 minutes , respectively .
Based on the observational results , we propose that the small-scale EUV wave should be a fast-mode magnetosonic wave that was driven by the the expanding coronal loop .
Moreover , with the application of filament seismology , it is estimated that the radial magnetic field strength is about 7 Gauss .
The observations also suggest that small-scale EUV waves associated with miniature solar eruptions share similar driving mechanism and observational characteristics with their large-scale counterparts .