Abstract
In this review, we address the use of numerical computations called Large-Eddy Simulations (LES) to study dust devils, and the more general class of atmospheric phenomena they belong to (convective vortices). We describe the main elements of the LES methodology. We review the properties, statistics, and variability of dust devils and convective vortices resolved by LES in both terrestrial and Martian environments. The current challenges faced by modelers using LES for dust devils are also discussed in detail.
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We acknowledge the logistic and financial help of the International Space Science Institute (ISSI, Bern, Switzerland) for the organization of a “dust devils” international workshop that led to the writing of this review chapter. We are indebted to two anonymous reviewers and associate editor Ralph Lorenz for constructive comments which helped to improve this review.
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Spiga, A., Barth, E., Gu, Z. et al. Large-Eddy Simulations of Dust Devils and Convective Vortices. Space Sci Rev 203, 245–275 (2016). https://doi.org/10.1007/s11214-016-0284-x
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DOI: https://doi.org/10.1007/s11214-016-0284-x