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Subsurface Magnetic Field and Flow Structure of Simulated Sunspots

  • Authors: Matthias Rempel

Rempel 2011 The Astrophysical Journal 740 15.

  • Provider: AAS Journals

Caption: Figure 3.

Radial and vertical flow velocities at three depth levels for the snapshot at t = 46.4 hr. The top row shows radial flow velocity and the bottom row shows vertical flow velocity. Left to right the depth levels z = −11.5 Mm, z = −3.3 Mm, and z = −1.3 Mm. The ring-like arrangement of convection cells is present at all depth levels, and the diameter of the region in which the presence of the sunspot modifies the convection pattern is increasing with depth as the intrinsic scale of convection is increasing with pressure scale height.

(An animationanimation and a color version of this figure are available in the online journal.)

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