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December 1, 2019Solar Physics50 citationsOpen Access

The Distinction Between Thermal Nonequilibrium and Thermal Instability

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Abstract

Abstract For some forms of steady heating, coronal loops are in a state of thermal nonequilibrium and evolve in a manner that includes accelerated cooling, often resulting in the formation of a cold condensation. This is frequently confused with thermal instability, but the two are in fact fundamentally different. We explain the distinction and discuss situations where they may be interconnected. Large-amplitude perturbations, perhaps associated with MHD waves, likely play a role in explaining phenomena that have been attributed to thermal nonequilibrium but also seem to require cross-field communication.

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synapsesocial.com/papers/6a7d248e7786afdcaca00247https://doi.org/10.1007/s11207-019-1562-z
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