Early warnings of the transition to a superrotating atmospheric state
- Department of Mathematics and Statistics, University of Exeter, Exeter, UK (m.s.williamson@exeter.ac.uk)
A superrotating atmosphere, one in which the angular momentum of the atmosphere exceeds the solid body rotation of the planet occurs on Venus and Titan. However, it may have occurred on the Earth in the hot house climates of the Early Cenozoic and some climate models have transitioned abruptly to a superrotating state under the more extreme global warming scenarios. Applied to the Earth, the transition to superrotation causes the prevailing easterlies at the equator to become westerlies and accompanying large changes in global circulation patterns. Although current thinking is that this scenario is unlikely, it shares features of other global tipping points in that it is a low probability, high risk event.
Using an idealized general circulation model developed for exoplanet research here at Exeter, we simulate the transition from a normal to a superrotating atmospheric state. We look at the changes in typical early warning indicators of tipping which show critical slowing down as well as oscillatory behaviour close to the transition. Inspired by the studies of phase transitions we also look at the critical spatial modes and correlation lengths close to the transition.
How to cite: Williamson, M.: Early warnings of the transition to a superrotating atmospheric state, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-6501, https://doi.org/10.5194/egusphere-egu23-6501, 2023.