Turbulence Structure in a Stratocumulus Cloud
Department of Mechanical Engineering, University of Connecticut, Storrs, CT 06269, USA
Received: 16 July 2018 / Revised: 31 August 2018 / Accepted: 17 September 2018 / Published: 10 October 2018
The growth of computing power combined with advances in modeling methods can yield high-fidelity simulations establishing numerical simulation as a key tool for discovery in the atmospheric sciences. A fine-scale large-eddy simulation (LES) utilizing 1.25 m grid resolution and
horizontal domain is used to investigate the turbulence and liquid water structure in a stratocumulus cloud. The simulations capture the observed cloud morphology, including elongated regions of low liquid water path, cloud holes, and pockets of clear air within the cloud. The cloud can be partitioned into two broad layers with respect to the maximum mean liquid. The lower layer resembles convective turbulent structure with classical inertial range scaling of the velocity and scalar energy spectra. The top and shallower layer is directly influenced by the cloud top radiative cooling and the entrainment process. Near the cloud top, the liquid water spectra become shallower and transition to a
power law for scales smaller than about
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MDPI and ACS Style
Matheou, G. Turbulence Structure in a Stratocumulus Cloud. Atmosphere 2018, 9, 392.
Matheou G. Turbulence Structure in a Stratocumulus Cloud. Atmosphere. 2018; 9(10):392.
Matheou, Georgios. 2018. "Turbulence Structure in a Stratocumulus Cloud." Atmosphere 9, no. 10: 392.
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