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Modeling Titan’s Planetary Boundary Layer at the Huygens Landing Site: Evidence for the Role of Subsurface Methane Evaporation in Limiting Convective Growth

  • Authors: Victoria L. Hartwick, Scot C. R. Rafkin, Alejandro Soto

Victoria L. Hartwick et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 10.

Methane table depth (z) exerts a more significant control on methane evaporation rates than the regolith porosity (ϕ). Shown here is the diurnal evolution of the (a) methane evaporation rate [kg m−2 s−1] scaled by 1E–6, (b) latent heat flux [W m−2], (c) skin temperature [K], (d) sensible heat flux [W m−2], and (e) PBL depth [m] for four NSMT simulations (labeled in panel (c)). The maximum depth of the PBL on Tsol 3 is listed in the text in panel (e). Note that panel (a) is scaled by ﹩1\times {10}^{-6}﹩. Individual simulations are labeled in panel (a) and include simulations with prescribed porosity, methane table depth pairs (pink line: ﹩\phi ﹩ = 0.15, z = 0.005 m; green line: ﹩\phi ﹩ = 0.5, z = 0.1 m; blue line: ﹩\phi ﹩ = 0.35, z = 0.06 m; orange line: ﹩\phi ﹩ = 0.25, z = 0.04 m).

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