Rotational Flows in Solar Coronal Flux Rope Cavities

Rotational Flows in Solar Coronal Flux Rope Cavities

We present a 2.5D magnetohydrodynamic simulation of a systematically rotating prominence inside its coronal cavity using the open-source MPI-AMRVAC code. Our simulation starts from a nonadiabatic, gravitationally stratified corona, permeated with a sheared arcade magnetic structure. The flux rope (F...

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Bibliographic Details
Main Authors: Valeriia Liakh, Rony Keppens
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Magnetohydrodynamics
Solar atmosphere
Solar prominences
Magnetohydrodynamical simulations
Solar activity
Online Access:https://doi.org/10.3847/2041-8213/acea78

Internet

https://doi.org/10.3847/2041-8213/acea78

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