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An examination of observations and model analyses indicate that this precipitation formed in a region of strong forcing for ascent associated with an upper-trough-jet system and a strong lower-tropospheric frontal zone. Above the stable surface airmass, conditional gravitational instability and conditional symmetric instability (CSI) were present, consistent with the observational evidence which suggests that elevated gravitational and/or slantwise convection were occurring. It is hypothesized that operational model forecasts of this precipitation feature were poor in part because the models were unable to properly resolve or parameterize the elevated and/or slantwise convection.
The Betts-Miller-Janjić (BMJ) convective parameterization (CP) scheme used in the operational Eta model at the time of this event the only examined the lowest 130 hPa above the model surface for instability, therefore the deep convection scheme would not activate if instability was located above this level. Additionally, slantwise convection is not parameterized in any operational model, and at the time of this event the Eta model was run with a horizontal grid-spacing of 32 km, which is unlikely to properly resolve this phenomenon on the grid scale. To test the above hypothesis, the ability of a mesoscale NWP model to simulate the formation of this precipitation will be tested with high-resolution model forecasts designed to examine the sensitivity to model initial conditions, CP scheme choice, and grid-spacing.