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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 15.

Same as Figure 12, but for the MRPS results. (a–d) The diurnal maximum planetary boundary depth for each methane table depth, regolith porosity simulation pair; (e) the average diurnal maximum PBL depth. Cyan outlines indicate maximum PBL depths that fall within the target range (600–1200 m).

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