For κ≈2.5 quiet-corona electrons the Spitzer-Härm conductivity integral diverges and AIA DEM inversion cannot distinguish single-T kappa, multi-T kappa, or multi-T Maxwellian sources.
Evidence for small-scale torsional Alfvén waves in the solar corona,
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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.
citing papers explorer
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The Quiet-Sun DEM Under Kappa: Diagnostic Degeneracy and the Failure of the Conductive Closure
For κ≈2.5 quiet-corona electrons the Spitzer-Härm conductivity integral diverges and AIA DEM inversion cannot distinguish single-T kappa, multi-T kappa, or multi-T Maxwellian sources.
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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.