Modelling the solar transition region using an adaptive conduction method (2020)
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.2002.01887
Publication URI: https://arxiv.org/abs/2002.01887
Type: Other