Fig. 19 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. 19.

Energy flux through the outer boundary, ﹩F_{u}+F_{r}﹩, is shown for case TUR (solid line) and case LAM (dashed line), averaged over longitude and over a time interval of one rotation period.

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