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We report on the first simultaneous observation of an H-alpha Moreton wave,the corresponding EUV fast coronal waves, and a slow and bright EUV wave(typical EIT wave). Associated with an X6.9 flare that occurred on 2011 August9 at the active region NOAA 11263, we observed a Moreton wave in the H-alphaimages taken by the Solar Magnetic Activity Research Telescope (SMART) at HidaObservatory of Kyoto University. In the EUV images obtained by the AtmosphericImaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) we foundnot only the corresponding EUV fast "bright" coronal wave, but also the EUVfast "faint" wave that is not associated with the H-alpha Moreton wave. We alsofound a slow EUV wave, which corresponds to a typical EIT wave. Furthermore, weobserved, for the first time, the oscillations of a prominence and a filament,simultaneously, both in the H-alpha and EUV images. To trigger the oscillationsby the flare-associated coronal disturbance, we expect a coronal wave as fastas the fast-mode MHD wave with the velocity of about 570 - 800 km/s. Thesevelocities are consistent with those of the observed Moreton wave and the EUVfast coronal wave.

First Simultaneous Observation of H-alpha Moreton Wave, EUV Wave, and Filament/Prominence Oscillations