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/10.48550/arxiv.1703.02423
Publication URI: https://arxiv.org/abs/1703.02423
Type: Other