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Observations of Coronal Mass Ejections

Published online by Cambridge University Press:  01 November 2006

Louise K Harra
Affiliation:
UCL-Mullard Space Science Laboratory, Holmbury St Mary, Dorking, Surrey, RH5 6NT, UK email: [email protected]
Jingxiu Wang
Affiliation:
National Astronomical Observatory, Chinese Academy of Sciences, Beijing, China email: [email protected]
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Abstract

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Observations of source regions of coronal mass ejections have progressed enormously in the past decade with the observations from SOHO and Yohkoh. Progress has been made on understanding magnetic helicity, coronal dimming, coronal waves and flares in terms of their relationship to CMEs. Observations have been used to verify and disagree with models such as tether-cutting, kink instabilities and the breakout model. We will describe the observations, recent models, and how future observations from the Solar-B and STEREO missions will address many unanswered questions.

Type
Contributed Papers
Copyright
© 2006 International Astronomical Union