By Steven Tomczyk, Jie Zhang, Timothy Bastian

Captures advances being made within the box of coronal magnetism, from thought to observations and instrumentation.

This quantity is a suite of analysis articles with regards to the sun corona, and especially, coronal magnetism. The publication used to be inspired via the Workshop on Coronal Magnetism: Connecting types to information and the Corona to the Earth, which used to be held 21 - 23 may well 2012 in Boulder, Colorado, united states. This workshop used to be attended through nearly 60 researchers. Articles from this assembly are contained during this topical factor, however the topical factor additionally includes contributions from researchers now not current on the workshop.

This quantity is geared toward researchers and graduate scholars energetic in sunlight physics.

Originally released in Solar Physics, Vol. 288, factor 2, 2013 and Vol. 289, factor eight, 2014.

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The findings using field extrapolations are summarised in the previous section. , 2008). During flares, the chromospheric brightenings (localised patches or ribbons) have been identified as the 31 Reprinted from the journal S. Régnier footpoints of magnetic field lines linked to the flare process such as reconnection events or post-flare loop growth. Masson et al. (2009) used a potential field extrapolation to show the correlation between magnetic field lines involved in the flare process and chromospheric ribbons.

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