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/10.1051/0004-6361/201936979
Publication URI: http://dx.doi.org/10.1051/0004-6361/201936979
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics