Warm clouds form precipitation when droplets of roughly 10-20 μm radius cross the 'size gap' to sizes where gravitational collection is efficient; deterministic collection theory predicts crossing times far longer than the 15-20 minutes sometimes observed, and air turbulence is known to enhance collisions through the droplet radial distribution function, the radial relative velocity, and the collision efficiency. The source paper (Wang, Xue, Ayala and Grabowski, 2006, Atmospheric Research) posed the problem of turning these effects into predictive capability through five linked directions: parameterizing the radial distribution function at cloud-relevant Reynolds numbers with gravitational settling, determining the true turbulent collision efficiency, justifying the extrapolation of finite-Reynolds-number direct numerical simulations to atmospheric turbulence, closing the higher-order moments of the true stochastic coalescence equation, and integrating all of these into computationally tractable cloud-scale schemes.
Background
Warm (ice-free) clouds are turbulent suspensions of water droplets that grow first by condensation of water vapor and then by collision and coalescence, in which two colliding droplets merge into a larger one. Condensation growth slows as droplets approach roughly 10-20 μm in radius, while gravitational collection, in which larger droplets fall fast enough to sweep up smaller ones, becomes efficient only at radii of order 50 μm. Crossing this 10-50 μm 'size gap' is the rate-limiting step of warm-rain formation: deterministic collection calculations typically predict an hour or more, whereas some cumuli are observed to produce drizzle-sized particles within 15-20 minutes.
The standard predictive tool is the kinetic collection equation (KCE), a Smoluchowski-type mean-field equation for the average number of droplets in each mass bin, driven by a collection kernel that multiplies mean droplet numbers. The KCE assumes that instantaneous droplet counts in two bins factorize into products of their means; for the finite droplet populations and narrow initial spectra of real clouds this assumption is uncontrolled. The exact description is a continuous-time Markov process (a master equation) for the joint probability of all bin populations; its first-moment equation, the 'true stochastic coalescence equation' (TSCE) derived in the source paper, governs the mean bin populations but contains unclosed second moments whose correlations can approach magnitude unity in sparsely populated bins, invalidating the KCE factorization precisely where early droplet growth matters.
Air turbulence enters the kernel through three separable effects. First, turbulent velocity differences increase the mean radial (approach) relative velocity between droplet pairs. Second, because droplets have inertia they cluster preferentially in turbulent straining and vortical regions; this preferential concentration is quantified by the radial distribution function , the pair density at the collision distance normalized by its value in a spatially uniform suspension. Third, the aerodynamic disturbance flows of the two droplets and of their neighbors deflect trajectories and drain momentum from the approach; this is collected into the collision efficiency , the ratio of the actual collision rate to the geometric rate for undisturbed straight trajectories. The geometric collision kernel is built from and , and multiplying by gives the collection kernel. The regime is set by the turbulent kinetic-energy dissipation rate (roughly 10-400 cm^2 s^-3 in convective clouds, higher in vigorous updrafts) and by the flow Reynolds number, conventionally the Taylor-microscale Reynolds number (a standard turbulence Reynolds number built from the root-mean-square velocity fluctuation and the Taylor microscale, the effective small-scale correlation length of the turbulent velocity field), which in the atmosphere is of order 10^3-10^4, far beyond what direct numerical simulation (DNS) can reach (). Hybrid DNS (HDNS) couples DNS of the carrier turbulence with an approximate superposition treatment of the droplets' disturbance flows so that many-body hydrodynamic interactions can be included at feasible cost.
The source paper (Wang, Xue, Ayala and Grabowski 2006) combined the TSCE derivation, Monte Carlo simulations of stochastic coalescence driven by DNS-based kinematic parameterizations, and HDNS computations of the collision efficiency, concluding that turbulence raises both the geometric collision rate and the collision efficiency, most strongly for similar-size pairs where gravitational collection is weakest. Reviews a few years later (Devenish et al. 2012; Grabowski and Wang 2013) summarized total kernel enhancements of up to about a factor of five for such pairs, and discussed these unresolved directions among the open problems of warm-cloud droplet growth.
Problem Statement
Construct a physically grounded, validated, and computationally tractable quantitative treatment of droplet collision-coalescence in turbulent cloud air, following the future-work program of Wang, Xue, Ayala and Grabowski (2006). The problem has five jointly linked components serving one common scientific objective, the quantitative prediction of cloud droplet size-distribution evolution and drizzle/rain initiation in warm clouds: (1) parameterize the pair radial distribution function and the mean radial relative velocity , equivalently the geometric collision kernel, for droplet pairs in the roughly 10-50 μm size range at cloud-relevant turbulence intensities with gravitational settling included, valid at or demonstrably extrapolable to atmospheric flow Reynolds numbers; (2) determine the true collision efficiency , including short-range hydrodynamic and lubrication interactions in turbulent many-droplet suspensions, as a function of droplet sizes, size ratio, and dissipation rate, in a form usable in bulk and bin models; (3) provide a theoretical and/or experimental justification for extrapolating finite-Reynolds-number DNS results to atmospheric turbulence; (4) develop a systematic treatment of the higher-order moments of the stochastic coalescence process, a closure or other quantitative correction achieving the same validity, so that a deterministic mean-field collection equation remains quantitatively valid, or is explicitly corrected, in regimes where stochastic correlations and finite-number fluctuations matter; and (5) integrate components (1)-(4) into computationally tractable collision-coalescence schemes for cloud-scale models. A resolution requires an integrated treatment addressing all five components jointly; work on a single component is a partial result.
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