Global circulation as the main source of cloud activity on Titan
S\'ebastien Rodriguez (AIM, LPGN), St\'ephane Le Mou\'elic (LPGN),, Pascal Rannou (GSMA, LATMOS), Gabriel Tobie (LPGN), Kevin H. Baines (JPL),, Jason W. Barnes, Caitlin A. Griffith (LPL), Mathieu Hirtzig (LESIA,, AOSS-PSL), Karly M. Pitman (JPL), Christophe Sotin (LPGN, JPL)

TL;DR
This study confirms that Titan's cloud activity is primarily driven by global atmospheric circulation, with observations generally matching models but revealing some discrepancies in seasonal cloud distribution and atmospheric response.
Contribution
The paper provides observational validation of global circulation models for Titan's cloud activity and highlights discrepancies indicating a need to refine thermal and seasonal response assumptions.
Findings
Cloud coverage aligns with circulation model predictions
Discrepancies in cloud presence at 40°N latitude
Titan's atmosphere shows greater seasonal inertia than models suggest
Abstract
Clouds on Titan result from the condensation of methane and ethane and, as on other planets, are primarily structured by circulation of the atmosphere. At present, cloud activity mainly occurs in the southern (summer) hemisphere, arising near the pole and at mid-latitudes from cumulus updrafts triggered by surface heating and/or local methane sources, and at the north (winter) pole, resulting from the subsidence and condensation of ethane-rich air into the colder troposphere. General circulation models predict that this distribution should change with the seasons on a 15-year timescale, and that clouds should develop under certain circumstances at temperate latitudes (~40\degree) in the winter hemisphere. The models, however, have hitherto been poorly constrained and their long-term predictions have not yet been observationally verified. Here we report that the global spatial cloud…
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.
