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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 A5.

Multi-Tsol (simulated Tsols 2–5) evolution of (a) net downward shortwave flux (solid lines) and net downward infrared flux (dashed lines), (b), surface skin temperature (solid lines) and air temperature in the lowest atmospheric layer (dashed lines), (c) thermal conduction in the shallowest subsurface layer, (d) surface sensible heat flux, (e) net residual energy in the shallowest subsurface layer, and (f) PBL depth for dry simulations with varied deep subsurface fixed temperatures. The maximum PBL depth on Tsol 3 is listed in the main text.

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