Zhe Feng

and 17 more

Global kilometer-scale models are the future of Earth system models as they can explicitly simulate organized convective storms and their associated extreme weather. Here, we comprehensively examined tropical mesoscale convective system (MCS) characteristics in the DYAMOND (DYnamics of the atmospheric general circulation modeled on non-hydrostatic domains) models for both summer and winter phases by applying eight different feature trackers to the simulations and satellite observations. Although different trackers produce substantial differences (a factor of 2-3) in observed MCS frequency and their contribution to total precipitation, model-observation differences in MCS statistics are more consistent among the trackers. DYAMOND models are generally skillful in simulating tropical mean MCS frequency, with multi-model mean biases of 2.9% over land and -0.5% over ocean. However, most models underestimate the MCS precipitation amount (23%) and their contribution to total precipitation (17%) relative to observations. These biases show large inter-model variability, but are generally smaller over land (13%) than over ocean (21%) on average. MCS diurnal cycle and cloud shield characteristics are better simulated than precipitation. Most models overestimate MCS precipitation intensity and underestimate stratiform rain contribution (up to a factor of 2), particularly over land. Models also predict a wide range of precipitable water in the tropics compared to reanalysis and satellite observations, and many models simulate a greater sensitivity of MCS precipitation intensity to precipitable water. The MCS metrics developed in this work provide process-oriented diagnostics for future model development efforts.

Chanil Park

and 3 more

The initiation of springtime mesoscale convective systems (MCSs) over the U.S. Great Plains is strongly supported by synoptically forced uplift. In this study, we first quantify these uplift mechanisms by numerically solving the quasi-geostrophic omega equation in Q-vector form. To provide a process-based assessment, Q vectors are decomposed into shearwise and transverse components, representing changes in the direction and magnitude of the potential temperature gradient along the geostrophic motion. The composite analysis reproduces the upper- and lower-tropospheric synoptic conditions favorable for MCS initiation, which have been well documented in the literature. We reveal that shearwise ascent, induced by a baroclinically organized trough–ridge couplet, is the leading contributor to total dynamical ascent. The contribution of an upper-level jet, which induces upward motion in its right entrance region through geostrophic frontogenesis by confluent motion, is minor as indicated by weaker transverse ascent. Likewise, the lower-tropospheric transverse ascent, induced by warm frontogenesis at the exit of the Great Plains low-level jet, plays a secondary role compared to shearwise ascent. Furthermore, MCSs initiated under stronger shearwise ascent tend to grow into larger, more precipitating storms, while no significant sensitivity to initial transverse ascent is observed throughout the MCS lifecycle. This study underscores the critical role of baroclinic wave amplification not only in the genesis but also in the subsequent evolution of MCSs, offering operational insights for their prediction.