Image Details

Choose export citation format:

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 A3.

Multi-Tsol evolution of the (a) sensible heat flux, (b) surface temperature, (c) net surface downward infrared flux (negative values indicate radiative cooling), (d) upward and downward infrared radiative fluxes in the nearest-surface atmosphere layer, and (e) PBL height for the baseline simulation (blue line) and a simulation with an artificially damped sensible heat flux (orange line).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse