Alfven wave phase-mixing in flows Why over-dense, solar coronal, open magnetic field structures are cool

View/Open
Volume
586
DOI
10.1051/0004-6361/201527105
Journal
ASTRONOMY & ASTROPHYSICS
ISSN
1432-0746
Metadata
Show full item record
Authors
Tsiklauri, D
URI
http://qmro.qmul.ac.uk/xmlui/handle/123456789/11782
Collections
Licence information
“The final publication is available at http://www.aanda.org/articles/aa/abs/2016/02/aa27105-15/aa27105-15.html”
Copyright statements
© ESO, 2016