Alongside Earth and Mars, Titan is the third planetary body in the solar system to show evidence for widespread and diverse sedimentary environments, including lakes (Hayes, 2016), rivers (Langhans et al., 2012, alluvial fans or deltas (Birch et al., 2016), eroded canyonlands (Poggiali et al., 2016), dissected plateaux (Malaska et al., 2020, and sand dunes (Lorenz, Wall et al., 2006). The latitudinal distribution of Titan's terrains, with sand dunes largely concentrated around the moon's equatorial belt, undifferentiated plains at mid-latitudes, and labyrinth terrains and lakes near the poles (Lopes et al., 2020), suggests a strong control of climate on Titan's surface processes and landscape formation (Figure 1a). Climate models predict that Titan's single-celled, pole-to-pole Hadley circulation splits into two cells as atmospheric circulation reverses near equinox (Hörst 2017), possibly leading to intense mid-latitude and equatorial storms that drive significant sediment transport by winds and rivers. Global circulation model (GCM) predictions (