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Cited article:

How Should One Optimize Nonlinear Force-Free Coronal Magnetic Field Extrapolations from SDO/HMI Vector Magnetograms?

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Solar Physics (2012)
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DOES THE COMPRESSION OR THE EXPANSION OF A SIMPLE TOPOLOGY POTENTIAL MAGNETIC FIELD LEAD TO THE DEVELOPMENT OF CURRENT SHEETS?

J. J. Aly and T. Amari
The Astrophysical Journal 709 (2) L99 (2010)
https://doi.org/10.1088/2041-8205/709/2/L99

Effects of line-tying on magnetohydrodynamic instabilities and current sheet formation

Yi-Min Huang, A. Bhattacharjee and Ellen G. Zweibel
Physics of Plasmas 17 (5) (2010)
https://doi.org/10.1063/1.3398486

THE TOPOLOGICAL CHANGES OF SOLAR CORONAL MAGNETIC FIELDS. I. SPONTANEOUS CURRENT SHEETS IN THREE-DIMENSIONAL FIELDS

Å. M. Janse and B. C. Low
The Astrophysical Journal 690 (2) 1089 (2009)
https://doi.org/10.1088/0004-637X/690/2/1089

Nonlinear force-free modeling of the solar coronal magnetic field

T. Wiegelmann
Journal of Geophysical Research: Space Physics 113 (A3) n/a (2008)
https://doi.org/10.1029/2007JA012432

The Topological Nature of Boundary Value Problems for Force‐Free Magnetic Fields

B. C. Low and N. Flyer
The Astrophysical Journal 668 (1) 557 (2007)
https://doi.org/10.1086/520503