English

The Distinction Between Thermal Nonequilibrium and Thermal Instability

Solar and Stellar Astrophysics 2020-01-08 v1

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.

Keywords

Cite

@article{arxiv.1911.11849,
  title  = {The Distinction Between Thermal Nonequilibrium and Thermal Instability},
  author = {James A. Klimchuk},
  journal= {arXiv preprint arXiv:1911.11849},
  year   = {2020}
}

Comments

accepted by Solar Physics 16 pages, 1 figure

R2 v1 2026-06-23T12:28:19.952Z