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Formation and Eruption of a Vortex-driven Magnetic Flux Rope in the Simulated Quiet Sun

  • Authors: Zhizhen Ye, Feng Chen

Zhizhen Ye and Feng Chen 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 8.

Left panel: spatial distribution of ﹩\left|{{\bf{B}}}_{{\bf{z}}}\right|{\boldsymbol{\gt }}{\bf{50}}﹩ G concentrations at z = 1.584 Mm in the full simulation domain. The green contours mark the edges of all concentrations that evolved in the statistical analysis. Right panel: joint distribution of magnetic flux and vorticity flux for all concentrations at all time instants. Different colors of dots represent concentrations at different times, while the circles connected by the black line represent the temporal evolution of the core positive concentration.

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