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