Abstract
The development of the kink instability in line-tied coronal loops is studied using a cylindrical MHD code. When the twist of magnetic field lines of the initial configuration exceeds a critical value, an ideal kink mode develops and drives this unstable equilibrium towards a secondary bifurcated equilibrium containing an electric current concentration. Contrary to a periodic untied configuration where a current sheet is ideally generated, the current layer is non-singular with a non-zero thickness and a finite amplitude. This current concentration extends along all the loop length and takes the form of an helical ribbon of intense current. The numerical results give an algebraic linear-like scaling of the characteristics of the current layer (amplitude and thickness) as a function of the aspect ratio of the loop. An interpretation in terms of axial field-line bending of the three-dimensional kinked equilibrium is proposed.
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BATY, H. IDEAL CURRENT LAYERS AND KINK INSTABILITY IN LINE-TIED CORONAL LOOPS. Solar Physics 172, 249–256 (1997). https://doi.org/10.1023/A:1004920632763
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DOI: https://doi.org/10.1023/A:1004920632763