The magneto-convective nature of dark striations and moving bright grains at the edge of pores

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Fig. 7.

Continuum-intensity snapshot of the MURaM simulation at the optical surface τ₅₀₀ = 1. Left: Complete simulation domain. Middle: Zoom of the pore. Right: Zoom filtered to a diffraction-limited frame from an ideal 1.6 m telescope. The white rectangles mark the locations of the striations and grains shown in Figures 8 and B.2.

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