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

Open Access

Fig. 5.

Evolution with time of the electron temperature and density at the loop center (s = L_c + L/2) for two models with an initial cool loop (m₄) and an initial hot loops (m₂₃) of similar length (L = 3 Mm). The dotted vertical line indicates the starting time of the impulsive heating.

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