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A fast method for constructing magnetic field models of solar active regions
Published online by Cambridge University Press: 27 June 2012
Abstract
A new method is proposed for automatic choosing the so-called magnetic “charges” that are necessary to model the coronal magnetic field in solar ARs. The method makes the quantitative analysis of large-scale magnetic field fast, easy, and reliable that allows us to study the evolution of ARs on short time scales.
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- Research Article
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- © EAS, EDP Sciences 2012