Integration of electrostatic and fluid dynamics within a dust devil

被引:23
作者
Farrell, WM
Renno, N
Delory, GT
Cummer, SA
Marshall, JR
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Univ Michigan, Ann Arbor, MI 48109 USA
[3] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[4] Duke Univ, Dept Elect & Comp Engn, Durham, NC 27708 USA
[5] SETI Inst, Mountain View, CA 94043 USA
关键词
D O I
10.1029/2005JE002527
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
[1] In this study we derive an analytical expression to describe the electrostatic field in a dust cloud with grain trajectories defined by fluid dynamics and grain charging via contact electrification. In order to solve for the electric field, we merge the fluid dynamic - driven grain motion directly into the basic electrostatic formalism to end up with an electric field dependent on meteorological variables within the dust cloud. We find that the E field is driven by two processes: the currents associated with the charging grains and the increasing velocity difference of varying-sized grains at early times. The resulting processes give rise to an exponentially growing electric field, which for Mars applications, quickly approaches breakdown values. Variations in the growth of the electric field are found with varying grains sizes and varying ambient atmospheric conductivity.
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页数:10
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