On the complexity and reactivity of magnetic features in solar active regions.

Computer Science

Scientific paper

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Scientific paper

In this paper an empirical method of a semi quantitative analysis of the complexity and of the reactivity of ensembles of magnetic features in the solar photosphere in the considered active regions is proposed and briefly discussed. For this analysis the author uses photospheric photoheliograms and vector magnetograms as material of observations and the possibilities of the two-dimensional topology as theoretical tool.

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