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Helicity Pattern of CME Source Active Regions

Published online by Cambridge University Press:  30 March 2016

Jingxiu Wang ,
Guiping Zhou  and
Jun Zhang
Jingxiu Wang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences Beijing 100012, China
Guiping Zhou
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences Beijing 100012, China
Jun Zhang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences Beijing 100012, China

Extract

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Coronal mass ejections are thought to originate from the over accumulation of magnetic helicity (Rust & Kumar, 1994). While recent studies revealed the incompetence of CME associated active regions in creating enough helicity for CMEs (Nindos, Zhang, & Zhang, 2003 and references therein), we have tried to seek, on the other hand, if particular helicity patterns are retained by CME-associated active regions.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 125
Copyright
Copyright © Astronomical Society of Pacific 2005

References

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