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The elevated heat source of the EH surface and the surrounding moisture sources of the Red Sea and the Congolese rain forests are shown to be crucial to the initiation of the scattered afternoon convection, and the eventual maturity of the convection into an MCC, with the no-sensible-heat-flux (NSH) and no-latent-heat-flux (NLH) experiments. The reduced-terrain (RT) experiment indicates that convection alone produces a weak wave signature, and that the local orography contributes significantly to the development of the convection and of the pre-Alberto AEW. Additional sensitivity experiments excluding the effects of the planetary boundary layer (NPBL) and the presence of the Turkana Channel (NTCH) will be performed to investigate more precisely the formation mechanisms for the pre-Alberto AEW.
Comparing simulation results with satellite data, the development of this AEW appears to take place in four stages: 1) cellular convection develops in the local afternoon over higher mountain peaks of the EH, 2) convective cells conglomerate into an MCC during the local nighttime at the lee slopes of the EH, 3) an MV develops from the remnants of the MCC, and 4) the convectively-generated MV combines with a pre-existing lee trough to form the AEW.