High-frequency torsional Alfvén waves as an energy source for coronal heating. (2017)
Attributed to:
Fundamental plasma physics of the sun and heliosphere: CFSA Warwick
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1038/srep43147
PubMed Identifier: 28256538
Publication URI: http://europepmc.org/abstract/MED/28256538
Type: Journal Article/Review
Volume: 7
Parent Publication: Scientific reports
ISSN: 2045-2322