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Mass and energy supply of a cool coronal loop near its apex

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Coronal energy input and dissipation in a solar active region 3D MHD model

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A model for the formation of the active region corona driven by magnetic flux emergence

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What can large-scale magnetohydrodynamic numerical experiments tell us about coronal heating?

H. Peter
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 373 (2042) 20150055 (2015)
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