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Numerical Simulations of Active Region Scale Flux Emergence: From Spot Formation to Decay

  • Authors: M. Rempel and M. C. M. Cheung

Rempel & Cheung 2014 The Astrophysical Journal 785 90.

  • Provider: AAS Journals

Caption: Figure 4.

Subsurface structure of the developing right spot at t = 16 hr. The azimuthally averaged magnetic field is shown in orange ( in logarithmic scale from 10 G to 10 kG). The contour lines show flux surfaces enclosing flux content ranging from Φ = 1021 to Φ = 1.2 × 1022 Mx in intervals of ΔΦ = 1021 Mx. Overlaid vectors display components of the azimuthally averaged velocity field in the rz plane. The yellow arrow at the bottom of the plot corresponds to 2 km s−1. The average flow field is roughly aligned with the average magnetic field, which loads the subsurface layers with buoyant, predominantly horizontal magnetic flux ready to emerge.

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