3D radiative-MHD simulations reveal that chromospheric heating rises with magnetic flux while coronal base temperature responds non-monotonically due to enhanced mass loading and radiative cooling.
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Chromosphere of the quiet sun: II. Atmospheric response to small-scale magnetic flux emergence
3D radiative-MHD simulations reveal that chromospheric heating rises with magnetic flux while coronal base temperature responds non-monotonically due to enhanced mass loading and radiative cooling.