Effects of model resolution, physics, and coupling on Southern Hemisphere storm tracks in CESM1.3

The CESM1.3 versions are documented, and the consequences of model resolution, air-sea coupling, and physics in the atmospheric models are studied with regards to storm tracks in the Southern Hemisphere as represented by 850 hPa eddy kinetic energy.

Increasing the resolution from 1 degree to 0.25 degree in the atmosphere (same physics) coupled to the 1 degree ocean intensifies the strength of the storm tracks closer to observations. The 0.25 degree atmosphere with the older CESM1.1 physics coupled to the 0.1 degree ocean has fewer low clouds, warmer Southern Ocean SSTs, a weaker meridional temperature gradient, and a degraded storm track simulation compared to the 0.25 degree atmosphere with CESM1.3 physics coupled to the 1 degree ocean.