Fig. 1.
Overview of the modelled coronal loop. (a) Volume rendering of the modulus of the current density together with selected magnetic field lines at t = 92 s. (b) Synthesised Fe XII emission for the whole loop with LOS along y. Over-plotted are boxes showing the fields-of-view used in Fig. 4. Axis markers are in Mm and the intensity is normalised to 1.
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