Airborne in-situ and remotely sensed satellite measurements have indicated that a preexisting positive perturbation in soil moisture (upwards of 150 km2) over a vegetatively sparse region in the African Sahel likely contributed to the initiation of a long-lived MCS on 31 July 2006. Observations showed that the perturbations in sensible and latent heat fluxes over the wetter soil produced a markedly cooler and moister planetary boundary layer (PBL) than over the dryer unperturbed areas. Using the vast array of observations and a high resolution WRF simulation (horz resolution of 1.66-km), this study will evaluate and attempt to simulate the impact of the soil moisture perturbations on the development of a thermally direct mesoscale circulation which contributed to the initiation of the MCS. A detailed assessment of the modeled surface fluxes and PBL evolution against observations will also be performed.
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