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Transverse oscillations of coronal loops

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Figure

Fig. 1 The background state consisting of an infinite magnetic tube.
Fig. 2 Typical dependences of mode phase speeds on the wavenumber under coronal condi-tions (CS0,e ≪ VA0, VA0 < VAe)
Fig. 3 The equilibrium state and the perturbed tube. The dashed lines show the tube in theequilibrium, while the solid lines show the tube perturbed by the fundamental mode of theglobal fast kink wave.
Fig. 4 The equilibrium configuration with a twisted magnetic tube. When the tube is thinand the Shafranov-Kruskal stability criterion is satisfied, Biz = Bez + O(a2/L2) in the coldplasma approximation.
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