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Observation and simulation of a filament eruption associated with the contraction of the overlying coronal loops and the filament rotation

Published online by Cambridge University Press:  06 January 2014

X. L. Yan ,
Z. K. Xue  and
Z. X. Mei
X. L. Yan
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
Z. K. Xue
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China email: [email protected] University of Chinese Academy of Sciences, Zhongguancun Beijing 100049, China
Z. X. Mei
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China email: [email protected]
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Abstract

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By using the data of Solar Dynamics Observatory (SDO), we present a case study of the contraction of the overlying coronal loop and the rotation motion of a sigmoid filament on 2012 May 22. At the beginning of the filament eruption, the overlying coronal loop experienced a significant contraction. In the following, the filament started to rotate counterclockwise. We also carried the simulation to investigate the process of the filament eruption.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 504 - 506
Copyright
Copyright © International Astronomical Union 2013 

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