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Fig. 19

image

Scaling test simulating the solar corona above AR 1429. We show the temporal evolution of thermal, kinetic, and magnetic energies within corona above the transition region. The energy fluxes of the thermal, kinetic, and magnetic energies from the chromosphere are denoted by flux. For the meaning of the different lines see the line form legend. After t ~ 16 min the background resistivity is enhanced, causing Joule heating.

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