Abstract
The magnetostatic modeling provides a simple and speedy method to model the erupted magnetic features. The assumption of magnetostatic equilibrium is reasonable for any periods smaller than the average life time of sunspots.
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Tiwari, P.B. (2001). The Effect of Azimuthal Magnetic Field on the Magnetostatic Models of Sunspots. In: Hanslmeier, A., Messerotti, M., Veronig, A. (eds) The Dynamic Sun. Astrophysics and Space Science Library, vol 259. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0760-3_33
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DOI: https://doi.org/10.1007/978-94-010-0760-3_33
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