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Modeling coronal magnetic field using spherical geometry: cases with several active regions

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Wiegelmann,  T.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Tadesse, T., Wiegelmann, T., MacNeice, P. J., & Olson, K. (2013). Modeling coronal magnetic field using spherical geometry: cases with several active regions. Astrophysics and Space Science, 347(1), 21-27. doi:10.1007/s10509-013-1493-3.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0015-0B4D-9
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