Evolution and Features of Dust Devil?Like Vortices in Turbulent Rayleigh?Bénard Convection—A Numerical Study Using Direct Numerical Simulation

نویسندگان

چکیده

Dust devils are convective vortices with a vertical axis of rotation that made visible by entrained soil particles. These particles contribute to the atmospheric aerosol input, influencing Earth radiation budget. Quantifying this contribution requires reliable information about statistics dust devils, their formation process, and how they maintained. In past, was mainly derived from field experiments large-eddy simulations (LESs). Field suffer erratic occurrence limited area can be monitored reliably. LESs, cannot resolved completely, especially close ground. Additionally, affected numerical features surface boundary conditions, as well subgrid-scale models in an unknown way. To mitigate these limitations, we employ direct (DNSs) improve our understanding devils. We comprehensively investigate structure for Rayleigh numbers up 1011 using DNS Rayleigh-Bénard convection between two plates first time. find devil-like structures occur much lower than atmosphere (?107). results support previous studies which axes were observed but not further investigated. The devil strongly depend on number velocity little aspect ratio model domain. Simulated show very similar properties analyzed LESs layer.

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ژورنال

عنوان ژورنال: Journal Of Geophysical Research: Atmospheres

سال: 2021

ISSN: ['2169-8996', '2169-897X']

DOI: https://doi.org/10.1029/2020jd034334