CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption

We present Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observation of three types fast-mode, propagating, magnetosonic waves in a GOES C3.0 flare on 23 April 2013, which was accompanied by prominence eruption and broad coronal mass ejection (CME). During the fast-rising phase prominence, large-scale, dome-shaped, extreme-ultraviolet (EUV) wave firstly formed ahead CME bubble propagated at speed about 430 km s−1 CME’s lateral direction. One can identify separation process EUV from bubble. The reflection effect on-disk counterpart this also observed when it interacted with remote active region. Six minutes after first appearance wave, quasi-periodic train period 120 seconds, emanated epicenter outward an average up to 1100 s−1, appeared inside In addition, another narrow, train, epicenter, 475 110 along closed-loop system connecting two adjacent regions. propose that all are fast-mode waves, dome-shaped driven expansion bubble, while within narrow were excited intermittent energy-releasing flare. Coronal seismology application energy carried estimated based measured parameters.