How numerical treatments of the transition region modify energy flux into the solar corona (2023)
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/10.1093/mnras/stad2802
Publication URI: http://dx.doi.org/10.1093/mnras/stad2802
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1