The effects of resistivity and viscosity on the Kelvin- Helmholtz instability in oscillating coronal loops (2017)
Attributed to:
Solar and Magnetospheric Plasma Theory
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201630259
Publication URI: http://dx.doi.org/10.1051/0004-6361/201630259
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics