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On the nature of the magnetic Rayleigh-Taylor instability in astrophysical plasma: the case of uniform magnetic field strength (2016)

First Author: Hillier A

Attributed to: Dynamics in solar prominences - connecting from small to large scale funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stw1805

Publication URI: http://dx.doi.org/10.1093/mnras/stw1805

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2