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Fig. 2
Profiles along the radial direction above the centre of the LHS bipole at t = 0 min of a) Log10(ρ), b) Log10(T), c) Log10(p). d) Profile along the φ direction across the centre of the bipoles of Log10(T). The dashed lines show the equivalent profiles for a coronal atmosphere in hydrostatic equilibrium at T = 2 MK.
This figure is made of several images, please see below:
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