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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 4.

(a) HASI potential temperature profile (dashed black line) compared with baseline simulation results on Tsol 2 vs. altitude [m]. The reference pressure and temperature are 1.5 bars and 100 K, respectively. (b) Zoomed-in plot of the lower atmosphere (up to 3 km).

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