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Solar cycle variation of magnetic flux ropes in a quasi-static coronal evolution model

Yeates, A.R.; Constable, J.A.; Martens, P.C.H.


J.A. Constable

P.C.H. Martens


The structure of electric current and magnetic helicity in the solar corona is closely linked to solar activity over the 11-year cycle, yet is poorly understood. As an alternative to traditional current-free “potential-field” extrapolations, we investigate a model for the global coronal magnetic field which is non-potential and time-dependent, following the build-up and transport of magnetic helicity due to flux emergence and large-scale photospheric motions. This helicity concentrates into twisted magnetic flux ropes, which may lose equilibrium and be ejected. Here, we consider how the magnetic structure predicted by this model – in particular the flux ropes – varies over the solar activity cycle, based on photospheric input data from six periods of cycle 23. The number of flux ropes doubles from minimum to maximum, following the total length of photospheric polarity inversion lines. However, the number of flux rope ejections increases by a factor of eight, following the emergence rate of active regions. This is broadly consistent with the observed cycle modulation of coronal mass ejections, although the actual rate of ejections in the simulation is about a fifth of the rate of observed events. The model predicts that, even at minimum, differential rotation will produce sheared, non-potential, magnetic structure at all latitudes.


Yeates, A., Constable, J., & Martens, P. (2010). Solar cycle variation of magnetic flux ropes in a quasi-static coronal evolution model. Solar Physics, 263(1-2), 121-134.

Journal Article Type Article
Acceptance Date Mar 24, 2010
Publication Date May 1, 2010
Deposit Date Oct 17, 2011
Publicly Available Date Apr 29, 2015
Journal Solar Physics
Print ISSN 0038-0938
Electronic ISSN 1573-093X
Publisher Springer
Peer Reviewed Peer Reviewed
Volume 263
Issue 1-2
Pages 121-134
Keywords Coronal mass ejections, theory, Magnetic fields, corona, Magnetic fields, models, Solar cycle, models.


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