Degree-1 convection in the Martian mantle and the origin of the hemispheric dichotomy

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A benchmark study on mantle convection in a 3‐D spherical shell using CitcomS (2008, background): “…in studying the planform of mantle convection [e.g., Zhong and Gurnis, 1993; Tackley et al., 1993; Bunge et al., 1996; Harder and Christensen, 1996; Roberts and Zhong, 2006; Zhong et al., 2007a] and in incorporating more realistic physical and chemical conditions in the mantle including…”
Long-Term Stability of a Subsurface Ocean on Enceladus (2007, background): “Degree-1 convection has been successfully modeled for the Earth (McNamara and Zhong, 2005) and Mars (Harder and Christensen, 1996; Breuer et al., 1997; Harder, 2000; Roberts and Zhong, 2006).”
Supercontinent cycles, true polar wander, and very long-wavelength mantle convection (2007, background): “, coefficient of thermal expansion and thermal conductivity) may affect convective planform (Zhang and Yuen, 1995), but their effects may not be as strong as the depth-dependent viscosity (Roberts and Zhong, 2006).”
Asymmetric thermal evolution of the Moon (2012, methodology): “[13] The diffusion creep viscosity , normalized by 0 can be written in nondimensional form as follows [Roberts and Zhong, 2006]:”