Magnetic field extrapolation is the construction of a model solution for the coronal magnetic field in active regions from magnetic boundary data originating close to the Sun's surface. The nonlinear force-free model (in which the electric current density is parallel to the magnetic field) is often adopted to describe the coronal field. The solution of the nonlinear force-free equations is a challenging computational task, and the application of codes to available boundary data has revealed a number of significant problems with nonlinear force-free extrapolation. This paper summarises the present status of coronal field extrapolation, and describes some recent developments. © 2013 Published under licence by IOP Publishing Ltd.
CITATION STYLE
Wheatland, M. S., & Gilchrist, S. A. (2013). The state of nonlinear force-free magnetic field extrapolation. In Journal of Physics: Conference Series (Vol. 440). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/440/1/012037
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