11.3 Extending Tropical Cyclone Potential Intensity Over Land to Predict Heat Low Dynamics in West Africa

Wednesday, 31 January 2024: 2:15 PM
342 (The Baltimore Convention Center)
Aaron Kruskie, Purdue University, West Lafayette, IN; and D. R. Chavas

Heat lows are low pressure systems formed from localized intense sensible heat emitted from the Earth’s surface. Their structure has previously been qualitatively compared to that of a dry tropical cyclone, as both are warm core vortices which exhibit low level cyclonic circulation and anticyclonic circulation aloft – though heat lows are given energy through surface sensible heat flux rather than latent heat flux. This work draws a quantitative comparison between the physics governing western Saharan heat lows and tropical cyclones by extending the concept of tropical cyclone potential intensity over land. Using parameters from the ERA5 reanalysis, we develop a method calculating potential intensity over land in assuming surface sensible heat flux as the main energy source for heat lows in the Sahara. We filter a dataset of low pressure systems in ERA5 from 1979-2019 to extract idealized heat low cases occurring over land in West Africa, and observe that tracks are most frequent in summer months and in regions with relatively smooth surface orography. Applying the potential intensity calculation method to monthly averaged ERA5 parameters shows a distribution of heat low potential intensity that correlates well with the spatial density of heat low tracks for JJA. Seasonal averaged potential intensity by hour reveals a strong dependence on the changes in buoyancy and surface heating over the diurnal cycle. Hourly potential intensity calculated around the center point of individual heat low track cases captures the magnitude of surface winds observed in ERA5. The diurnal cycle dependence is present in individual heat lows as well as seasonal, showing a delay between the time of maximum potential intensity and the peak in surface wind speed of a heat low. Overall, our results suggest that the seasonal distribution and surface wind speeds of Saharan heat lows are well predicted by applying tropical cyclone potential intensity theory over land.
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