Fig. 1.
(a) Schematic of the radiative and convective zones, colored as yellow and orange, respectively, for the configuration of low-mass stars rotating with angular speed Ω0. (b) Horizontal shear flow U(y) in a local nontraditional f-plane at a colatitude θ in the radiative zone; zc denotes the transition altitude between the radiative and convective zones.
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