Abstract

Abstract. The increase in the spectral width of an initially monodisperse population of cloud droplets in homogeneous isotropic turbulence is investigated by applying a finite-difference fluid flow model combined with either Eulerian bin microphysics or a Lagrangian particle-based scheme. The turbulence is forced applying a variant of the so-called linear forcing method that maintains the mean turbulent kinetic energy (TKE) and the TKE partitioning between velocity components. The latter is important for maintaining the quasi-steady forcing of the supersaturation fluctuations that drive the increase in the spectral width. We apply a large computational domain (643 m3), one of the domains considered in Thomas et al. (2020). The simulations apply 1 m grid length and are in the spirit of the implicit large eddy simulation (ILES), that is, with small-scale dissipation provided by the model numerics. This is in contrast to the scaled-up direct numerical simulation (DNS) applied in Thomas et al. (2020). Two TKE intensities and three different droplet concentrations are considered. Analytic solutions derived in Sardina et al. (2015), valid for the case when the turbulence integral timescale is much larger than the droplet phase relaxation timescale, are used to guide the comparison between the two microphysics simulation techniques. The Lagrangian approach reproduces the scalings relatively well. Representing the spectral width increase in time is more challenging for the bin microphysics because appropriately high resolution in the bin space is needed. The bin width of 0.5 µm is only sufficient for the lowest droplet concentration (26 cm−3). For the highest droplet concentration (650 cm−3), an order of magnitude smaller bin size is barely sufficient. The scalings are not expected to be valid for the lowest droplet concentration and the high-TKE case, and the two microphysics schemes represent similar departures. Finally, because the fluid flow is the same for all simulations featuring either low or high TKE, one can compare point-by-point simulation results. Such a comparison shows very close temperature and water vapor point-by-point values across the computational domain and larger differences between simulated mean droplet radii and spectral width. The latter are explained by fundamental differences in the two simulation methodologies, numerical diffusion in the Eulerian bin approach and a relatively small number of Lagrangian particles that are used in the particle-based microphysics.

Highlights

  • Cloud droplet spectra in natural ice-free clouds significantly affect such key processes as drizzle or rain formation and the transfer of solar radiation through the cloudy atmosphere

  • This paper presents a modeling study addressing the impact of homogeneous isotropic turbulence on the broadening of an initially monodisperse distribution of cloud droplets in response to local fluctuations of the supersaturation field

  • This problem has been considered previously in modeling studies of Lanotte et al (2009) applying direct numerical simulation (DNS), Thomas et al (2020) using the scaled-up DNS, and Sardina et al (2015) employing theoretical analysis combined with DNS and stochastic model simulations

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Summary

Introduction

Cloud droplet spectra in natural ice-free clouds significantly affect such key processes as drizzle or rain formation and the transfer of solar radiation through the cloudy atmosphere. The Lagrangian methodology has clear benefits when compared to the bin scheme These include the lack of numerical diffusion, the realistic representation of the stochastic nature of the cloud droplet growth, the possibility of including a physically based representation of the unresolved scales’ impact on droplet growth (i.e., allowing the multiscale simulation of a turbulent cloud), and the provision of a better framework for aerosol–cloud interactions and the representation of ice processes. G20a argued that the good agreement was because of the constant chamber pressure assumed in the simulations This agrees with the Morrison et al (2018) conjecture that the artificial spectral broadening comes from the coupling between vertical advection in a stratified environment (that provides the supersaturation source) and advection in the bin space that represents the response of the droplet population to the supersaturation forcing.

The model and model forcing
The setup of dynamic simulations
Thermodynamics in ILES moist simulations
ILES moist simulations with droplets
Lagrangian and Eulerian microphysics schemes
Lagrangian microphysics
Eulerian bin microphysics
Grid-volume by grid-volume analysis of macro- and microphysical properties
Summary and conclusions
Bin microphysics
Super-droplets
Full Text
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