Fig. 11.
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Space–time heatmaps of total density ρ (left), velocity v (centre), and temperature T (right) are shown for non-linear MPI-AMRVAC evolution of the bipolar isobaric perturbation (σ = 1 Mm). The negative-temperature pulse (right half, s ≳ 25 Mm) drives condensation and a dense blob that slides towards the left footpoint, while the positive-temperature pulse (left half, s ≲ 25 Mm) drives rarefaction and heating of the evacuated region under the fixed balanced-heating prescription.
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