Abstract
The essential dynamical characteristic of convective vortices, including dust devils, is a highly localized vorticity tube that extends into the vertical. This chapter is concerned with both the generation of vorticity and the subsequent focusing of that vorticity into a tight vortex, and with the environmental conditions that are conducive to the formation of convective vortices in general and dust devils in particular. A review of observations, theory, and modeling of dust devil formation is provided.
Original language | English |
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Pages (from-to) | 183-207 |
Number of pages | 25 |
Journal | Space Science Reviews |
Volume | 203 |
Issue number | 1-4 |
DOIs | |
Publication status | Published - 2016 Nov 1 |
Keywords
- Atmospheric dynamics
- Dust devils
- Earth atmosphere
- Mars atmosphere