Instability driven by settling and evaporation in a shear flow: A model for asperitas clouds
S. Ravichandran and Rama Govindarajan
Phys. Rev. Fluids 7, 010501 (2022) - Published 5 January, 2022
Designated a new cloud feature in 2017, asperitas clouds are wave-like formations on the underside of layer clouds. We propose a mechanism for asperitas cloud formation: an instability driven by the settling and evaporation of water droplets. For suitable droplet size and liquid water content, a layer of dense air forms, which in moderate ambient shear gives rise to cloud structures of the asperitas type.
Framework for idealized climate simulations with spatiotemporal stochastic clouds and planetary-scale circulations
Tianhong Huang, Samuel N. Stechmann, and Jason L. Torchinsky
Phys. Rev. Fluids 7, 010502 (2022) - Published 20 January, 2022
In climate predictions, clouds are the leading source of uncertainty. For both predictions and basic understanding, a main challenge is to account for the vast range of scales, from the scales of individual clouds to the large-scale circulations. Here, an idealized simulation framework is investigated with stochastic clouds, so that some clouds are not subgrid-scale and are instead evolving on the numerical grid, albeit stochastically. The results show the possibility of following the influence of clouds on climate in idealized climate change simulations.
Dimensionless parameters for cloudy Rayleigh-Bénard convection: Supersaturation, Damköhler, and Nusselt numbers
Subin Thomas, Prasanth Prabhakaran, Fan Yang, Will H. Cantrell, and Raymond A. Shaw
Phys. Rev. Fluids 7, 010503 (2022) - Published 27 January, 2022
In this article we bridge between the Rayleigh-Bénard convection literature and the atmospheric literature by expressing the governing equations for cloudy convection in a dimensionless form. The governing parameters are Rayleigh, Prandtl, Schmidt, Damköhler, and sedimentation numbers for the cloudy case. We further connect to the atmospheric literature by obtaining an expression for the Nusselt number (dimensionless heat flux) for a cloud–convection system, directly from the conservation equations for temperature and water vapor, and illustrate the microphysics independence through large eddy simulation of an idealized cloudy Rayleigh-Bénard convection flow.































































