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Quasi-electrostatic field analysis and simulation of Martian and terrestrial dust devils

Publication ,  Journal Article
Zhai, Y; Cummer, SA; Farrell, WM
Published in: Journal of Geophysical Research: Planets
June 20, 2006

Recent experimental and modeling studies show that large quasi-static electric fields (2-20 kV/m) can be developed in a Martian or terrestrial dust devil as a result of contact electrification and charge separation of dust grains with different sizes and compositions. Electric discharging occurs when the maximum electric field reaches breakdown values (∼20 kV/m on Mars and ∼3 MV/m on Earth, at surface altitudes). We derive a maximum electric field in a dust devil and develop a two-dimensional (2-D) cylindrically symmetric finite element model for Martian and terrestrial dust devil simulations. Unlike previous models with unlimited field growth, the tribocharging process and the time evolution of the dust devil electric field are self-consistently limited in our model and the saturated maximum electric fields in our simulations are comparable to past measurements. We study the saturated maximum electric fields for dust storms of different size, atmosphere conductivity and time rate of tribocharging. We also discuss the 2-D cylindrical field structures surrounding a dust devil and the conductivity gradient effect to the field growth of large Martian dust storms. Copyright 2006 by the American Geophysical Union.

Duke Scholars

Published In

Journal of Geophysical Research: Planets

DOI

ISSN

0148-0227

Publication Date

June 20, 2006

Volume

111

Issue

6

Related Subject Headings

  • Meteorology & Atmospheric Sciences
 

Citation

APA
Chicago
ICMJE
MLA
NLM
Zhai, Y., Cummer, S. A., & Farrell, W. M. (2006). Quasi-electrostatic field analysis and simulation of Martian and terrestrial dust devils. Journal of Geophysical Research: Planets, 111(6). https://doi.org/10.1029/2005JE002618
Zhai, Y., S. A. Cummer, and W. M. Farrell. “Quasi-electrostatic field analysis and simulation of Martian and terrestrial dust devils.” Journal of Geophysical Research: Planets 111, no. 6 (June 20, 2006). https://doi.org/10.1029/2005JE002618.
Zhai Y, Cummer SA, Farrell WM. Quasi-electrostatic field analysis and simulation of Martian and terrestrial dust devils. Journal of Geophysical Research: Planets. 2006 Jun 20;111(6).
Zhai, Y., et al. “Quasi-electrostatic field analysis and simulation of Martian and terrestrial dust devils.” Journal of Geophysical Research: Planets, vol. 111, no. 6, June 2006. Scopus, doi:10.1029/2005JE002618.
Zhai Y, Cummer SA, Farrell WM. Quasi-electrostatic field analysis and simulation of Martian and terrestrial dust devils. Journal of Geophysical Research: Planets. 2006 Jun 20;111(6).

Published In

Journal of Geophysical Research: Planets

DOI

ISSN

0148-0227

Publication Date

June 20, 2006

Volume

111

Issue

6

Related Subject Headings

  • Meteorology & Atmospheric Sciences