| dc.contributor.author | Tsiklauri, D | en_US |
| dc.date.accessioned | 2016-04-12T12:30:51Z | |
| dc.date.issued | 2016-02 | en_US |
| dc.date.submitted | 2016-03-23T12:14:18.306Z | |
| dc.identifier.issn | 1432-0746 | en_US |
| dc.identifier.other | ARTN A95 | en_US |
| dc.identifier.uri | http://qmro.qmul.ac.uk/xmlui/handle/123456789/11782 | |
| dc.description | Accepted for publication in Astron. Astrophys. -- final accepted version | |
| dc.description.sponsorship | Computational facilities: Astronomy Unit, Queen Mary University of London and UK’s STFC Dirac-2 HPC via UKMHD consortium. The author was financially supported by STFC consolidated Grant No. ST/J001546/1 and Leverhulme Trust Research Project Grant No. RPG-311. The author would also like to thank Dr. T. R. Arter for providing crucially important IT support. | en_US |
| dc.relation.ispartof | ASTRONOMY & ASTROPHYSICS | en_US |
| dc.rights | “The final publication is available at http://www.aanda.org/articles/aa/abs/2016/02/aa27105-15/aa27105-15.html” | |
| dc.subject | magnetohydrodynamics (MHD) | en_US |
| dc.subject | Sun: activity | en_US |
| dc.subject | Sun: corona | en_US |
| dc.subject | solar wind | en_US |
| dc.title | Alfven wave phase-mixing in flows Why over-dense, solar coronal, open magnetic field structures are cool | en_US |
| dc.type | Article | |
| dc.rights.holder | © ESO, 2016 | |
| dc.identifier.doi | 10.1051/0004-6361/201527105 | en_US |
| pubs.author-url | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000369715900106&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
| pubs.notes | Not known | en_US |
| pubs.publication-status | Published | en_US |
| pubs.volume | 586 | en_US |
