Fig. 3 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. 3.

Similar to Fig. 2 but for case LAM. The white dotted lines in the upper and middle zoomed‐in radial velocity images indicate the latitude corresponding to the cylinder tangent to the base of the convection zone and aligned with the rotation axis.

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