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Convectively Driven High Wind Events

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On a day when the potential instability is sufficient, it is possible to initiate storms from rising air parcels. One estimate of the intensity of these buoyant plumes (also an indicator of the severity of the storm) is based on parcel theory (Bluestein et al. 1988, 1989; Holton 1992). These rising parcels of air rapidly cool until saturation occurs. Further lifting results in condensation and, in a short period of time, precipitation develops. It is often at this stage that another fundamental element of a storm commonly forms: the convective downdraft.
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... The basic forcing mechanisms for downdrafts are given by the vertical momentum equation; the significance of the individual terms is summarized in the literature review by Wakimoto (2001). He notes that the vertical gradient of perturbation pressure and the perturbation pressure buoyancy term were, in most cases, less important than the precipitation induced changes in buoyancy. ...
... Srivastava (1985) notes that in the extreme case of an environmental lapse rate close to a dry adiabatic lapse rate, even light precipitation can lead to significant downdrafts. The dependence on ambient environmental humidity is less clear (see also Wakimoto, 2001). While a moister environment increases the virtual temperature difference between downdraft and environment, thus strengthening the downdraft, this effect can be reversed when the effect of entrainment of environmental air is considered. ...
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One important component of precipitating convection is the formation of convective downdrafts. They can terminate the initial updraft, affect the mean properties of the boundary layer, and cause strong winds at the surface. While the basic forcing mechanisms for downdrafts are well understood, it is difficult to formulate general relationships between updrafts, environmental conditions, and downdrafts. To better understand what controls different downdraft properties, we analyze downdrafts over tropical oceans in a global storm resolving simulation. Using a global model allows us to examine a large number of downdrafts under naturally varying environmental conditions. We analyze the various factors affecting downdrafts using three alternative methods. First, hierarchical clustering is used to examine the correlation between different downdraft, updraft, and environmental variables. Then, either random forests or multiple linear regression are used to estimate the relationships between downdraft properties and the updraft and environmental predictors. We find that these approaches yield similar results. Around 75% of the variability in downdraft mass flux and 37% of the variability in downdraft velocity are predictable. Analyzing the relative importance of our various predictors, we find that downdrafts are coupled to updrafts via the precipitation generation argument. In particular, updraft properties determine rain amount and rate, which then largely control the downdraft mass flux and, albeit to a lesser extent, the downdraft velocity. Among the environmental variables considered, only lapse rate is a valuable predictor: a more unstable environment favors a higher downdraft mass flux and a higher downdraft velocity.
... Several recent works have brought forward methods to track cold pools, in particular their gust fronts, in numerical simulations (Drager & van den Heever, 2017;Fournier & Haerter, 2019;Henneberg et al., 2020;Hirt et al., 2020;Rochetin et al., 2021;Schlemmer & Hohenegger, 2016). Yet, the detection of cold pools in numerical simulations is far from trivial: (a) the area affected by rainfall, where the CP is fed by rain evaporation, is often not cleanly delimited and subject to setting a threshold value, for example, on the precipitation rate; (b) the CP density current, as a highly dynamic object, experiences turbulent mixing and heat exchange with the surface and ambient environment, and is subject to spontaneous symmetry breaking, such as under the formation of "lobe-and-cleft" instabilities-again feeding back on the dynamics (Härtel et al., 2000;Markowski & Richardson, 2010;Simpson, 1972;Wakimoto, 2001); (c) the larger-scale pattern of cold pools and the rain cells produced by their collisions, is highly complex, with families formed by CP-rain cell networks making for a challenging tracking problem. ...
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Recent observations and modeling increasingly reveal the key role of cold pools in organizing the convective cloud field. Several methods for detecting cold pools in simulations exist, but are usually based on buoyancy fields and fall short of reliably identifying the active gust front. The current cold pool (CP) detection and tracking algorithm (CoolDeTA), aims to identify cold pools and follow them in time, thereby distinguishing their active gust fronts and the “offspring” rain cells generated nearby. To accomplish these tasks, CoolDeTA utilizes a combination of thermodynamic and dynamical variables and examines the spatial and temporal relationships between cold pools and rain events. We demonstrate that CoolDeTA can reconstruct CP family trees. Using CoolDeTA we can contrast radiative convective equilibrium (RCE) and diurnal cycle CP dynamics, as well as cases with vertical wind shear and without. We show that the results obtained are consistent with a conceptual model where CP triggering of children rain cells follows a simple birth rate, proportional to a CP's gust front length. The proportionality factor depends on the ambient atmospheric stability and is lower for RCE, in line with marginal stability as traditionally ascribed to the moist adiabat. In the diurnal case, where ambient stability is lower, the birth rate thus becomes substantially higher, in line with periodic insolation forcing—resulting in essentially run‐away mesoscale excitations generated by a single parent rain cell and its CP.
... Such patterns, which can be characterized as eddies forming along the azimuthal direction along the GF, have previously been referred to as lobe-and-cleft instabilities (Härtel, Carlsson & Thunblom, 2000;Markowski & Richardson, 2010;J. E. Simpson, 1972;Wakimoto, 2001). Based on numerical simulations it was suggested that the activation of these azimuthal features could affect the radial spreading of the CPs by causing a transition from a power law r(t) ∼ t α with α ≈ 0.6 at times before, but α ≈ 0.4 after the transition . ...
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Plain Language Summary Convective cold pools (CPs) are regions of cool air forming beneath precipitating clouds. As rain droplets evaporate during their fall, they cool down the surrounding air, thereby increasing its weight and causing it to sink down. As the cold sinking airflow hits the ground, it spreads outward in all directions, creating strong wind gusts which are important mediators of the weather system. Indeed, such gust fronts can suppress cloud formation in some locations, by cooling the near‐surface air, while simultaneously triggering cloud formation along their edges by wedging underneath and lifting the ambient air. Numerical weather models should ideally account for these effects. Unfortunately, the models' grid resolution is often too coarse to represent the thin CPs, and it is not yet known what resolution should be used. In this study, high‐resolution simulations of idealized CPs are carried out at different mesh resolutions, allowing a systematic exploration of CPs' sensitivity to grid resolution. Our simulation results may help reveal configuration requirements for high‐resolution simulations and guide climate model development.
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