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Prominence Formation Processes

Published online by Cambridge University Press:  30 March 2016

B.T. Welsch ,
C. R. DeVore  and
S. K. Antiochos
B.T. Welsch
Affiliation:
Space Sciences Lab, University of California, 7 Gauss Way, Berkeley, CA 94720-7450
C. R. DeVore
Affiliation:
Laboratory for Computational Physics and Fluid Dynamics, Code 6440, Naval Research Laboratory, Washington DC 20375-5344
S. K. Antiochos
Affiliation:
E. O. Hulburt Center for Space Research, Code 7675, Naval Research Laboratory, Washington DC 20375-5352

Abstract

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We summarize our attempts simulate the prominence formation model proposed by Martens & Zwaan (2001, ApJ, 558, 872) in which differential rotation drives reconnection between two initially unconnected bipolar active regions to form helical field lines along the polarity inversion line (PIL) between the flux systems.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 127
Copyright
Copyright © Astronomical Society of Pacific 2005