Image Details

Choose export citation format:

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 3.

Gill model properties on the sphere with different input parameters. (a) Scaled upper-layer EMFC. (b) Scaled lower-layer zonal wind ﹩{u}_{2}^{{\prime} }﹩ at the equator. Note the eastward shift in ﹩{u}_{2}^{{\prime} }﹩ with increased E and ﹩{ \mathcal S }{{\rm{Ro}}}_{T}{T}_{{\rm{rad}}}﹩. The black line shows the vertically integrated reference potential temperature profile at the equator. Drag-free solutions (dashed) are obtained analytically in Appendix A. Solutions with low-level drag (solid) are obtained numerically.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse