Alfvén wave phase-mixing in flows Why over-dense, solar coronal, open magnetic field structures are cool (2016)
Attributed to:
The Plasma-CCP Network
funded by
EPSRC
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