Dion Donné
2.5D MHD Simulation of an Eruption Prominence with Stochastic Heating
Solar prominences are still not understood and even less how they erupt into a coronal mass ejection (CME). Recently, literature has shown that stochastic heating plays a crucial role in realistically simulating solar prominences, retrieving their fibril structure as well as counterstreaming flows. Yet, up to now stochastic heating has not been carried out in the context of an erupting prominence.
Here, we elaborate on our findings by performing a high resolution 2.5D MHD simulation of an erupting prominence with stochastic heating and outline its effects on the morphology and dynamics of an erupting prominence.
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2.5D MHD Simulation of an Eruption Prominence with Stochastic Heating