Abstract:The magnetic network extending from the photosphere (solar radius R ) to lower corona (R + 10 Mm) plays an important role in the heating mechanisms of the solar atmosphere.Here we further develop the models with realistic open magnetic flux tubes of the authors in order to model more complicated configurations. Closed magnetic loops, and combinations of closed and open magnetic flux tubes are modelled. These are embedded within a stratified atmosphere, derived from observationally motivated semi-empirical and … Show more
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