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Results show that the vertical temperature structure of IV4 is characterized by a warm anomaly around 100 hPa and a cold anomaly that extends from 200 hPa to the surface. The strongest circulation of IV4 is in the upper-levels around 200 hPa. The quasi-geostrophic (QG) vertical motion pattern indicates that IV4 forces weak subsidence (weak rising motion) to the west (east) of the upper-level low center. In particular, the Laplacian of thermal advection overwhelms the vorticity advection forcing term in the QG omega equation. There is a midlevel cyclonic circulation associated with IV4, with northeasterly (southeasterly) midlevel flow to the west (east) of the low. Analysis of individual synoptic times reveals that significant mesoscale convective system activity along the Sierra Madre Occidental (SMO) foothills is collocated with regions of anomalous northeasterly midlevel flow and increased northeasterly shear on the western (leading) flank of IV4. It is proposed that IV4 induces northeasterly midlevel flow on its leading flank, thereby creating an environment that is favorable for convective storms to grow upscale as they move off the high terrain of the SMO.