Alfvén wave phase-mixing in flows Why over-dense, solar coronal, open magnetic field structures are cool (2016)

First Author: Tsiklauri D

Attributed to: Astronomy Research at Queen Mary 2012-2015 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201527105

Publication URI: http://dx.doi.org/10.1051/0004-6361/201527105

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics