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 Journal7.
Provider: AAS Journals
Caption: Figure 14.
As in Figures 7 and 12, (a) HASI potential temperature profile (dashed black line) compared with ﹩\phi ﹩ = 0.3, ﹩\beta ﹩ = 0.04 simulation results on Tsol 2 vs. altitude [m]. (b) Zoomed-in plot of the lower atmosphere (up to 3 km).
