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A Converging View on EIT Waves

Published online by Cambridge University Press:  27 June 2012

M. Faurobert ,
C. Fang ,
T. Corbard ,
P.F. Chen  and
C. Fang
P.F. Chen
Affiliation:
School of Astronomy and Space Science, Nanjing University, Nanjing, China. e-mail: [email protected] Key Laboratory of Modern Astronomy and Astrophysics, Nanjing, University, China
C. Fang
Affiliation:
School of Astronomy and Space Science, Nanjing University, Nanjing, China. e-mail: [email protected] Key Laboratory of Modern Astronomy and Astrophysics, Nanjing, University, China
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Abstract

Coronal “EIT wave” is a large-scale wavelike phenomenon propagating across the major part of the Sun. Debates are being continued regarding a more suitable name for it, its source driver, and its nature. “EIT waves” have been widely explained in terms of fast-mode waves, despite that the model contradicts with many observational features. Two-types of EUV waves were predicted 10 years ago. With the recent high-cadence observations, mainly from SDO/AIA telescope, more and more evidence has been revealed in favor of the two-wave model. In this paper, after summarizing different names used for EIT waves in the literature, we show how the community are getting close to reaching a consensus on the nature of EIT waves.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 55: 4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges , 2012 , pp. 313 - 320
Copyright
© EAS, EDP Sciences 2012

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