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Fig. 6


Time variation of the surface luminosity emitted by the hot slab for the reference (blue), the dynamical chromosphere (green), and the hybrid (red) cases. These quantities are computed assuming an optically thin coronal plasma. To allow comparison, the time is reported in reduced units of tτcycle and the luminosity is normalised to the incoming mechanical energy flux FM defined in Eq. (10). The values of the cycle duration for each setup are reported in Table 1.

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