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Three‐dimensional Spherical Simulations of Solar Convection. I. Differential Rotation and Pattern Evolution Achieved with Laminar and Turbulent States

  • Authors: Mark S. Miesch, Julian R. Elliott, Juri Toomre, Tom L. Clune, Gary A. Glatzmaier, and Peter A. Gilman

Miesch et al. 2000 The Astrophysical Journal 532 593.

  • Provider: AAS Journals

Caption: Fig. 8.

Similar to Fig. 7 but for case LAM. Again, upper, middle, and lower images correspond to latitudes of about 70°, 40°, and 0°, respectively (see Table 2).

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