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Authors: Asai, Ayumi  kyouindb  KAKEN_id  orcid (unconfirmed)
Ishii, Takako T.
Isobe, Hiroaki  kyouindb  KAKEN_id
Kitai, Reizaburo
Ichimoto, Kiyoshi  kyouindb  KAKEN_id
UeNo, Satoru  kyouindb  KAKEN_id  orcid (unconfirmed)
Nagata, Shin'ichi  kyouindb  KAKEN_id
Morita, Satoshi  kyouindb  KAKEN_id
Nishida, Keisuke
Shiota, Daikou
Oi, Akihito
Akioka, Maki
Shibata, Kazunari
Author's alias: 浅井, 歩
Keywords: magnetohydrodynamics (MHD)
shock waves
Sun: corona
Sun: filaments, prominences
Sun: flares
Issue Date: 1-Feb-2012
Publisher: IOP Publishing
Journal title: The Astrophysical Journal
Volume: 745
Issue: 2
Thesis number: L18
Abstract: We report on the first simultaneous observation of an Hα Moreton wave, the corresponding EUV fast coronal waves, and a slow and bright EUV wave (typical EIT wave). We observed a Moreton wave, associated with an X6.9 flare that occurred on 2011 August 9 at the active region NOAA 11263, in the Hα images taken by the Solar Magnetic Activity Research Telescope at Hida Observatory of Kyoto University. In the EUV images obtained by the Atmospheric Imaging Assembly on board the Solar Dynamic Observatory we found not only the corresponding EUV fast "bright" coronal wave, but also the EUV fast "faint" wave that is not associated with the Hα Moreton wave. We also found a slow EUV wave, which corresponds to a typical EIT wave. Furthermore, we observed, for the first time, the oscillations of a prominence and a filament, simultaneously, both in the Hα and EUV images. To trigger the oscillations by the flare-associated coronal disturbance, we expect a coronal wave as fast as the fast-mode MHD wave with the velocity of about 570-800 km s[–1]. These velocities are consistent with those of the observed Moreton wave and the EUV fast coronal wave.
Rights: © IOP Publishing 2012
This is not the published version. Please cite only the published version.
DOI(Published Version): 10.1088/2041-8205/745/2/L18
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