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Neoclassical Effects on Solar Plasma Loops

Published online by Cambridge University Press:  03 June 2005

B.L. Tan  and
G.L. Huang
B.L. Tan
Affiliation:
Purple Mountain Observatory CAS, Nanjing 210008, China email: bltan@pmo.ac.cn Graduate School of the CAS, Beijing, China Present address: No.2, West Beijing road, Nanjing 210008, China.
G.L. Huang
Affiliation:
Purple Mountain Observatory CAS, Nanjing 210008, China email: bltan@pmo.ac.cn
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Abstract

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Tokamak physics shows that there will be a neoclassical effect in current-carrying plasma loops. We apply the theory to solar coronal loops and hope to find a fast magnetic reconnection mechanism for understanding solar flares and CMEs.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)flaresmagnetic fieldsMHD
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 279 - 280
Copyright
© 2005 International Astronomical Union