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Which cloud-resolving model results are robust to basic changes in microphysics and dynamics schemes to guide climate model parameterization development?.

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  1. Which cloud-resolving model results are robust to basic changes in microphysics and dynamics schemes to guide climate model parameterization development? Climate model grid meshes are too coarse to explicitly simulate storm system winds and therefore must rely on simplified models referred to as parameterizations to represent all storm properties and effects. Cloud-resolving models (CRMs), on the other hand, can explicitly resolve the wind circulations within storm systems. For decades CRMs have been an important tool to help evaluate and improve climate model parameterizations. However, CRMs still contain parameterizations, such as simplifications of the properties and behavior of hydrometeors (cloud droplets, raindrops, ice crystals, snow, graupel, and hail). CRMs therefore themselves remain unreliable to an unknown degree, owing at least in part to large remaining uncertainties in the representation of such microphysics. In this study the properties of three simulations of a strong mesoscale convective system observed during the TWP-ICE campaign were analyzed from a large-scale modeling perspective. The objective was to determine which CRM results are robust and therefore relatively more confidently used for parameterizations development and which are more model-dependent. The greatest difference found among the simulations is in the partitioning of ice among different species, which may depend primarily on microphysical formulation, in particular in the stratiform region. However, a consistent pattern is seen across the simulations insofar as the slowest-falling ice hydrometeor species (cloud ice) is roughly 90% as abundant in the stratiform regions as in the convection region, whereas the fastest-falling hydrometeor species (graupel or hail) is least abundant. In both convective and stratiform regions, downdrafts consistently contain precipitation below about 10 km and updrafts consistently contain cloud ice above the melting level (or at least the homogeneous freezing level in one of the simulations). Substantial differences in cold pool coverage and intensity can likely be attributed to microphysical, and possibly to some extent the dynamical formulation. Although hydrometeor mass loadings and cold pool properties diverge, several commonalities of convective regions are remarkably consistent across the simulations. First, both convective updraft and downdraft mass fluxes are nearly linearly correlated with convective area. Second, the ratio of ice in convective downdrafts to that in updrafts is about 0.5, independent of ice species. Third, the ratio of downdraft to updraft mass flux is about 0.5-0.6, which can be interpreted as a evaporation efficiency of roughly one-half in convective regions. Ultimately, some these findings may lead to improved convective parameterizations in large-scale models. Reference: Mrowiec AA, C Rio, AM Fridlind, AS Ackerman, AD Del Genio, OM Pauluis, AC Varble, and J Fan. 2012. "Analysis of cloud-resolving simulations of a tropical mesoscale convective system observed during TWP-ICE: Vertical fluxes and draft properties in convective and stratiform regions." Journal of Geophysical Research, 117, D19201, doi:10.1029/2012JD017759.

  2. Result: • Both convective updraft and downdraft mass fluxes are nearly linearly correlated with convective area. • The ratio of ice in convective downdrafts to that in updrafts is about 0.5, independent of ice species. • The ratio of downdraft to updraft mass flux is about 0.5–0.6, as shown in figure to the right. Mass flux in convective downdrafts versus mass flux in convective updrafts for three simulations (D1, D2, and S2). The fluxes are each computed at 10-minute intervals, with strongest fluxes occurring in the mature stage of the storm life cycle. Which cloud-resolving model results are robust to basic changes in microphysics and dynamics schemes to guide climate model parameterization development? • Motivation: • Climate model grid meshes are too coarse to explicitly simulate storm system winds and therefore must rely on parameterizations. • Cloud-resolving models (CRMs) can explicitly resolve the circulations within storm systems. However, CRMs contain simplifications, for example, of the properties and behavior of hydrometeors (cloud droplets, raindrops, ice crystals, snow, graupel, and hail). • CRMs therefore remain unreliable to an unknown degree, because of uncertainties in the representation of such microphysics. Convective updrafts (red) and downdrafts (dark blue) and stratiform updrafts (yellow) and downdrafts (light blue) identified over a storm life cycle (mostly convective at the start, mostly stratiform at the end). Approach: The properties of three simulations of a strong mesoscale convective system observed during the TWP-ICE campaign. The properties were viewed from a large-scale modeling perspective. Since models and observations commonly consider convective and stratiform precipitating regions and many GCM parameterizations are based on mass flux closure, we consider primarily the mass fluxes and properties of updrafts and downdrafts in convective and stratiform areas. For this purpose, we use three 3D CRM simulations that include one- and two-moment microphysics and an aerosol size distribution profile based on observations. Mrowiec AA, C Rio, AM Fridlind, AS Ackerman, AD Del Genio, OM Pauluis, AC Varble, and J Fan. 2012. "Analysis of cloud-resolving simulations of a tropical mesoscale convective system observed during TWP-ICE: Vertical fluxes and draft properties in convective and stratiform regions."Journal of Geophysical Research, 117, D19201, doi:10.1029/2012JD017759.

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