SIMULATIONS OF THE SOLAR CHROMOSPHERE IN THE TWO-FLUID APPROXIMATION
This work presents the study of wave propagation and the Rayleigh-Taylor instability in the solar atmosphere using a two-fluid model. The solar atmosphere is strongly stratified and permeated by magnetic fields with a complex configuration, thus creating very different regimes throughout its layers. Of the different layers of the solar atmosphere
Beatrice Popescou Braileau
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4
2020