Computational modelling of stellar magnetic fields from observational b oundary values M. S. Wheatland Scho ol of Physics Sydney Institute for Astronomy The University of Sydney Cosmic Magnetism Kiama 8 June 2010 Model for solar AR 10953 from Hinode/SOT data Overview Background Zeeman effect on spectral lines The Sun Modelling active regions The data vector magnetograms Nonlinear force-free ... 1987) 1 For more details see e.g. Landi degl'Innocenti & Landolfi (2004). ...
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