Relationship between the topological skeleton, current concentrations, and 3D magnetic reconnection sites in the solar atmosphere (2008)
Attributed to:
Parallel Computing Resources for the UK MHD Community
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361:20078664
Publication URI: http://dx.doi.org/10.1051/0004-6361:20078664
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics
Issue: 1