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.
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