Data-driven MURaM simulations of emerging active region 11640 reproduce key EUV features and find volumetric coronal heating proportional to B squared along with ubiquitous MHD waves.
Evidence for small-scale torsional Alfvén waves in the solar corona,
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Kappa=2.5 plasmas in the quiet solar corona invalidate the Spitzer-Harm conductive closure and render standard EUV DEM inversions insensitive to the electron distribution type.
citing papers explorer
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Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: Coronal Heating and Dynamics in an Emerging Active Region
Data-driven MURaM simulations of emerging active region 11640 reproduce key EUV features and find volumetric coronal heating proportional to B squared along with ubiquitous MHD waves.
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The Quiet-Sun DEM Under Kappa: Diagnostic Degeneracy and the Failure of the Conductive Closure
Kappa=2.5 plasmas in the quiet solar corona invalidate the Spitzer-Harm conductive closure and render standard EUV DEM inversions insensitive to the electron distribution type.