Volume 584, December 2015
|Number of page(s)||8|
|Published online||23 November 2015|
Limitations of force-free magnetic field extrapolations: Revisiting basic assumptions
Max Planck Institute for Solar System Research, 37077 Göttingen, Germany
Received: 24 July 2015
Accepted: 14 October 2015
Context. Force-free extrapolations are widely used to study the magnetic field in the solar corona based on surface measurements.
Aims. The extrapolations assume that the ratio of internal energy of the plasma to magnetic energy, the plasma β, is negligible. Despite the widespread use of this assumption observations, models, and theoretical considerations show that β is of the order of a few percent to more than 10%, and thus not small. We investigate what consequences this has for the reliability of extrapolation results.
Methods. We use basic concepts starting with force and energy balance to infer relations between plasma β and free magnetic energy to study the direction of currents in the corona with respect to the magnetic field, and to estimate the errors in the free magnetic energy by neglecting effects of the plasma (β ≪ 1). A comparison with a 3D magneto-hydrodynamics (MHD) model supports our basic considerations.
Results. If plasma β is of the order of the relative free energy (the ratio of the free magnetic energy to the total magnetic energy) then the pressure gradient can balance the Lorentz force. This is the case in solar corona, and therefore the currents are not properly described. In particular, the error in terms of magnetic energy by neglecting the plasma is of the order of the free magnetic energy, so that the latter cannot be reliably determined by an extrapolation.
Conclusions. While a force-free extrapolation might capture the magnetic structure and connectivity of the coronal magnetic field, the derived currents and free magnetic energy are not reliable. Thus quantitative results of extrapolations on the location and amount of heating in the corona (through current dissipation) and on the energy storage of the magnetic field (e.g. for eruptive events) are limited.
Key words: Sun: corona / Sun: magnetic fields / Sun: atmosphere / methods: data analysis
© ESO, 2015
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