The impact of lake shape and size on lake breezes and air-lake exchanges on Titan

Audrey Chatain (1, 2) , Scot C R Rafkin (2) , Alejandro Soto (2) , Enora Moisan (2, 3) , Juan M Lora (4) , Alice Le Gall (5, 6) , Ricardo Hueso (1) , Aymeric Spiga (7)

1 Departamento de Fisica Aplicada [Bilbao]
2 Department of Space Studies [Boulder]
3 LGL-TPE - Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement
4 Department of Earth and Planetary Sciences [New Haven]
5 PLANETO - LATMOS
6 IUF - Institut universitaire de France
7 LMD - Laboratoire de Météorologie Dynamique (UMR 8539)

Titan, the largest moon of Saturn, has many lakes on its surface, formed mainly of liquid methane. Like water lakes on Earth, these methane lakes on Titan likely profoundly affect the local climate. Previous studies (Rafkin and Soto, 2020; Chatain et al., 2022) showed that Titan's lakes create lake breeze circulations with characteristic dimensions similar to the ones observed on Earth. However, such studies used a model in two dimensions; this work investigates the consequences of the addition of a third dimension to the model. Our results show that 2D simulations tend to overestimate the extension of the lake breeze over the land, and underestimate the strength of the subsidence over the lake, due to divergence/convergence geometrical effects in the mass conservation equations. In addition, 3D simulations including a large scale background wind show the formation of a pocket of accelerated wind behind the lake, which did not form in 2D simulations. An investigation of the effect of shoreline concavity on the resulting air circulation shows the formation of wind currents over peninsulas. Simulations with several lakes can either result in the formation of several individual lake breeze cells (during the day), or the emergence of a large merged cell with internal wind currents between lakes (during the night). Simulations of several real-shaped lakes located at a latitude of 74°N on Titan at the autumn equinox show that larger lakes trigger stronger winds, and that some sections of lakes might accumulate enough methane vapor to form a thin fog. Additionally, we adapted the Turbulent Kinetic Energy closure scheme of the model to better represent the extremely low turbulence at the surface of Titan, of 2 10−4 m2.s−2 above the land, and inferior to 3 10−5 m2.s−2 above the lake. The addition of a third dimension, along with adjustments in the parametrizations of turbulence and subsurface land temperature, results in a reduction in the magnitude of the average lake evaporate rate, namely to ~6 cm/Earth year.

Domaines: Planète et Univers [physics]

Audrey Chatain, Scot C R Rafkin, Alejandro Soto, Enora Moisan, Juan M Lora, et al.. The impact of lake shape and size on lake breezes and air-lake exchanges on Titan. Icarus, 2024, 41, pp.115925. ⟨10.1016/j.icarus.2023.115925⟩. ⟨insu-04263607v2⟩