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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 9.

In all porosity ﹩\phi ﹩ = 0.02 simulations, methane evaporation increases the near-surface methane vapor mass mixing ratio. The rate and magnitude of this increase are determined by the initial methane profile (shown as different lines). Dashed lines show the final simulated time step (Tsol 5); solid lines show the initial time step. Individual lines show outcomes from simulations with different initial methane profiles.

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