Evolution of the Transverse Density Structure of Oscillating Coronal Loops Inferred by Forward Modeling of EUV Intensity (2018)
Attributed to:
Solar and Magnetospheric Plasma Theory
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aad3cc
Publication URI: http://dx.doi.org/10.3847/1538-4357/aad3cc
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2