Global Non-Potential Magnetic Models of the Solar Corona

Main publication of the work of our ISSI team:

A.R. Yeates, T. Amari, I. Contopoulos, X. Feng, D.H. Mackay, Z. Mikic, T. Wiegelmann, J. Hutton, C.A. Lowder, H. Morgan, G. Petrie, L.A. Rachmeler, L.A. Upton, A. Canou, P. Chopin, Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse, Space Sci. Rev. 214, 99, 2018.

The following additional publications have arisen or benefited from our ISSI team:

T. Whitbread, A.R. Yeates, A. Munoz-Jaramillo and G.J.D. Petrie, Parameter optimization for surface flux transport models, Astron. Astrophys. 607, A76, 2017.
M. Weinzierl, D.H. Mackay, A.R. Yeates and A.A. Pevtsov, The possible impact of L5 magnetograms on non-potential solar coronal magnetic field simulations, Astrophys. J. 828, 102, 2016.
D.H. Mackay, A.R. Yeates and F.-X. Bocquet, Impact of an L5 magnetograph on nonpotential solar global magnetic field modeling, Astrophys. J. 825, 131, 2016.
C. Jiang, S.T. Wu, X. Feng, Q. Hu, Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption, Nature Comm. 7, 11522, 2015.
C. Jiang, S.T. Wu, V. Yurchyshyn, H. Wang, X. Feng, Q. Hu, How did a major confined flare occur in super solar active region 12192?, Astrophys. J. 828, 62, 2016.