Proceedings of the International Astronomical Union


Multi-Wavelength Investigations of Solar Activity
Contributed Papers

Moreton waves observed at Hida Observatory


Noriyuki Narukage a1, Shigeru Eto a2, Miwako Kadota a1, Reizaburo Kitai a1, Hiroki Kurokawa a1 and Kazunari Shibata a1
a1 Kwasan and Hida Observatories, Kyoto University, Yamashina, Kyoto 607-8471, Japan email: naru@kwasan.kyoto-u.ac.jp
a2 Department of Astronomy, Kyoto University, Sakyo, Kyoto 606-8502, Japan

Article author query
narukage n   [Google Scholar] 
eto s   [Google Scholar] 
kadota m   [Google Scholar] 
kitai r   [Google Scholar] 
kurokawa h   [Google Scholar] 
shibata k   [Google Scholar] 
 
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Abstract

Moreton waves are flare-associated waves observed to propagate across the solar disk in H$\alpha$, especially in the wing of H$\alpha$. The Flare Monitoring Telescope at Hida Observatory of Kyoto University observed 12 events associated with flare waves (i.e., Moreton waves and/or filament oscillations) in H$\alpha$ from 1997 to 2002. We review our studies of Moreton waves based on these observations;

  1. relation between EIT wave and Moreton wave (Eto et al. 2002),
  2. simultaneous observation with X-ray wave (Narukage et al. 2002),
  3. three dimensional structure of flare-associated wave (Narukage et al. 2004),
  4. relation between Moreton waves and filament eruptions.



Footnotes

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