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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 A1.

Comparison of surface energy and PBL depth for simulations with two different subsurface layer structures but all other parameters equal (e.g., initial surface temperature, deep subsurface temperature, thermal conductivity, volumetric heat capacity). The baseline layer structure is shown in Table 1. The S. Han & J. M. Lora (2025) layer structure is shown in Table A1.

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