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Cited article:

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

R. C. Maclean, J. Büchner, E. R. Priest

A&A, 501 1 (2009) 321-333

Published online: 2008-10-30

DOI: https://doi.org/10.1051/0004-6361:20078664

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Determining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null points

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Type III Solar Radio Burst Source Region Splitting due to a Quasi-separatrix Layer

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How skeletons turn into quasi-separatrix layers in source models

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