Fig. 6
Meridional circulation in a stably stratified rotating fluid in a sphere when the spin-down forcing Csd is increased (Csd = 0,10-6,10-5from left to right). Streamlines of the meridional circulations are shown in the same way as in Fig. 4. As in Fig. 5, E = 10-7, Pr = 10-4, and β ≫ 1. Numerical resolution is the same as in Fig. 5.
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