Strong nocturnal inversions can form in the basin, particularly below the height of the Lechner Saddle. Downslope winds along the basin sidewalls are not able to penetrate the strong inversion and thus separate from the sidewall near the top of the inversion to flow toward the basin center. The flow continues through the Lechner Saddle, where it produces a steady outflow of air. We will present a detailed analysis of the structure and mass flux of the downslope flows, the flow above the basin-floor inversion, and the outflow through the gap in the surrounding topography. We will also show how changes in surface characteristics can impact the strength of nocturnal cooling and subsequently the strength of the outflow.
 - Indicates paper has been withdrawn from meeting
 - Indicates an Award Winner