Fig. 11
Radial profiles taken at various times of the azimuthal velocity in the equatorial plane of the star for E = 10-5, B = 102, ϵ = 10-7, λ = 10-4, and Ro = 10-5. Profiles are scaled as in Fig. 10. The dimensionless time τ is specified for each curve. Dashed lines are profiles for baroclinicly dominated dynamics while solid lines are for spin-up dominated dynamics. The dashed bold curve shows the initial profile and the solid bold curve shows the last profile.
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