Simulating the Coronal Evolution of AR 11437 Using SDO/HMI Magnetograms (2018)
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/10.3847/1538-4357/aa9f20
Publication URI: http://dx.doi.org/10.3847/1538-4357/aa9f20
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2