Abstract
As a phenomenon that occurs on Earth and on Mars, the diameter of a dust devil helps determine the amount of dust the devil injects into the atmosphere for both worlds—for a given dust flux density (dust lifted per area per time), a wider devil will lift more dust into the air. However, the factors that determine a dust devil’s diameter D and how it might relate to the ambient conditions have remained unclear. Moreover, estimating the contribution to an atmospheric dust budget from a population of dust devils with a range of diameters requires an accurate assessment of the differential diameter distribution, but considerable work has yet to reveal the best representation or explain its physical basis. In this study, we propose that this distribution follows a power law ∝D−5/3 and provide a simple physical explanation for why the distribution takes this form. By fitting diameter distributions of Martian dust devil diameters reported in several studies, we show that the data from several studies support this proposed form.
| Original language | English |
|---|---|
| Article number | 193 |
| Journal | Planetary Science Journal |
| Volume | 6 |
| Issue number | 8 |
| DOIs | |
| State | Published - 1 Aug 2025 |
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