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Mechanisms of Superrotation in Slowly Rotating and Tidally Locked Planets

  • Authors: Quentin Nicolas, Geoffrey K. Vallis

Quentin Nicolas and Geoffrey K. Vallis 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Numerical solution of the Matsuno–Gill problem (Equations (17a)–(17d)) with E = 0.02 and ﹩{ \mathcal S }{{\rm{Ro}}}_{T}{T}_{{\rm{rad}}}=1﹩, and its EMFC. (a) Upper-layer geopotential ﹩{{\rm{\Phi }}}_{1}^{{\prime} }﹩ (shading) and wind ﹩{{\boldsymbol{u}}}_{1}^{{\prime} }﹩ (arrows). (b) EMFC in the upper layer (solid), its horizontal convergence component (red dashed), and its vertical convergence component (red dotted line; see Equation (14), flux-form expression). (c, d) Same as panels (a) and (b), except for the lower layer.

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