Fig. 10 from Three‐dimensional Spherical Simulations of Solar Convection. I. Differential Rotation and Pattern Evolution Achieved with Laminar and Turbulent States

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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. 10.

Shown are (a) an instantaneous snapshot, (b) a one–rotation‐period average, and (c) a ten–rotation‐period average of the angular velocity in case LAM (averaged over longitude). The color table and contour levels are the same as those used for the simulations in Fig. 9b–9d.

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