The Flare-Energy Distributions Generated by Kink-Unstable Ensembles of Zero-Net-Current Coronal Loops (2011)
Attributed to:
Magnetohydrodynamic and kinetic models of magnetic reconnection applied to solar coronal activity
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1007/s11207-011-9832-4
Publication URI: http://dx.doi.org/10.1007/s11207-011-9832-4
Type: Journal Article/Review
Parent Publication: Solar Physics
Issue: 1