Multi-Stranded Coronal Loops: Quantifying Strand Number and Heating Frequency from Simulated Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA) Observations (2021)
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/10.1007/s11207-021-01848-8
Publication URI: http://dx.doi.org/10.1007/s11207-021-01848-8
Type: Journal Article/Review
Parent Publication: Solar Physics
Issue: 6