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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 5.

Magnetograms at τ = 1 (left), smoothed vertical velocity at τ = 1 (middle), and vertical flow velocity in 8 Mm depth (right) for three different times during the spot formation phase (t = 24, 28, and 32 hr). In the velocity plots black contours indicate vertical magnetic field with more than 1.5 kG in the photosphere. Positive velocity values (blue colors) indicate upflows.

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