Fig. 7 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. 7.

Shown is the radial velocity in the mid convection zone (﹩r=0.84\,R_{\odot }﹩) as a function of longitude and time at high, mid, and low latitudes. The upper image corresponds approximately to a latitude of 70°, the middle image to 40°, and the lower image to the equator (see Table 2).

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