The effects of numerical resolution, heating timescales and background heating on thermal non-equilibrium in coronal loops (2019)

First Author: Johnston C

Attributed to: Solar and Magnetospheric Magnetohydrodynamics and Plasmas: Theory and Application funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1904.07287

Publication URI: https://arxiv.org/abs/1904.07287

Type: Other