The nature of small-scale extreme ultraviolet solar brightenings investigated as impulsive heating of short loops in 1D hydrodynamics simulations

Open Access

Fig. D.2.

Same as for Fig.10, zoomed-in to the right side of the loop, for the model m₁₉ (Table A.3). This model consists of an initial hot loop submitted to an impulsive heating with a narrow deposition function (σ_ev = 0.1L) localized at the center of the loop (s_ev = L_c + L/2).

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