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Relationship between the topological skeleton, current concentrations, and 3D magnetic reconnection sites in the solar atmosphere (2008)

First Author: Maclean R

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