Ideal MHD Instabilities, with a Focus on the Rayleigh-Taylor and Kelvin-Helmholtz Instabilities
Attributed to:
Magnetism and Fluid Flows in our Solar-Planetary Environment
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1007/978-3-030-16343-3_1
Publication URI: https://api.elsevier.com/content/abstract/scopus_id/85069761153
Type: Book Chapter
Book Title: Topics in Magnetohydrodynamic Topology, Reconnection and Stability Theory (2020)
Page Reference: 1-36