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Fig. 6.

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Horizontally and temporally averaged values of the kinetic energy (blue), internal energy (yellow), and magnetic energy (green) in the solar atmosphere. The shaded regions cover two standard deviations. We included the magnetic energy of a potential field above z = 0 (dot-dashed line). The vertical dashed lines represent the height of the photosphere (z = 0) and the base of the chromosphere (z = 800 km).

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