Origins of Flow and Magnetic Structure Involved in
Formation and Eruption of Solar Prominence
To clarify origins of the flow and magnetic structure involved in evolution of a solar prominence, we performed a
three-dimensional magnetohydrodynamic simulation of an emerging twisted flux tube, where both flow and magnetic field passed freely through a solar surface. By analyzing Lagrangian displacements of magnetized
plasma elements, we demonstrated how interactions between the
flow and magnetic field proceeded during the formation and eruption of the prominence, which led to clarifying those dynamic processes responsible for the evolution of the prominence: diverging
flow on U-loop, helical downdraft along rotating loop, acceleration and deceleration of downflow along S-loop, and partial emergence of W-loop, all of which
played roles in dynamics and magnetism of the prominence.
Reference
Magara, T.
Journal of the Korean Astronomical Society, 54, 157
movie
movie1, movie2, movie3
movie1, movie2
Prominence in the solar sky (solar plasma cloud).