Superrotation of Titan's stratosphere driven by the radiative heating of the haze layer
Motoki Sumi, Shin-ichi Takehiro, Wataru Ohfuchi, Hideko Nomura, Yuka, Fujii

TL;DR
This study uses a General Circulation Model to investigate how Titan's haze layer influences its superrotating stratosphere, revealing a balance between meridional circulation and eddy momentum transport that sustains superrotation.
Contribution
It demonstrates that Titan's stratospheric superrotation can be maintained by atmospheric dynamics independent of surface momentum transfer, highlighting the role of haze-induced radiative effects.
Findings
The model reproduces observed superrotation velocities at high altitudes.
Superrotation is maintained by a balance between meridional circulation and eddy momentum transport.
A no-wind region at about 80 km altitude is explained by the dynamics.
Abstract
Titan's stratosphere has been observed in a superrotation state, where the atmosphere rotates many times faster than the surface does. Another characteristics of Titan's atmosphere is the presence of thick haze layer. In this paper, we performed numerical experiments using a General Circulation Model (GCM), to explore the effects of the haze layer on the stratospheric superrotation. We employed a semi-gray radiation model of Titan's atmosphere following McKay et al. (1999), which takes account of the sunlight absorption by haze particles. The phase change of methane or the seasonal changes were not taken into account. Our model with the radiation parameters tuned for Titan yielded the global eastward wind around the equator with larger velocities at higher altitudes except at around 70 km after Earth days. Although the atmosphere is not in an equilibrium state, the zonal wind…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
