2017
DOI: 10.1002/2016jd026150
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The role of turbulence in thunderstorm, snowstorm, and dust storm electrification

Abstract: In this paper the contribution of turbulence into the electrification of thunderstorms, snowstorms, and dust storms is investigated for the first time. A model of large‐scale electric field generation in a weakly conducting medium, containing two types of particles charging by collisions, is used. Thunderstorm and snowstorm electrification are considered in detail in this paper; dust storm electrification is also considered, despite being substantially different from the two other cases, to demonstrate the uni… Show more

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Cited by 21 publications
(19 citation statements)
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“…Nevertheless, triboelectric charging is an exciting but so far not completely understood phenomenon. It has been investigated in many fields of research, such as contact electrification in dust devils (Farrell, 2004; Mareev and Dementyeva, 2017), in clouds after volcanic eruptions (Anderson et al, 1965; Mather and Harrison, 2006), in the formation of planets (Yair et al, 2008; Wang et al, 2017), and in almost every application dealing with fine and dry powders. Commonly, triboelectric charging is seen as a problem in industrial applications if particles are to be moved because charged particles tend to agglomerate and adhere on surfaces (Wong et al, 2015).…”
Section: Introductionmentioning
confidence: 99%
“…Nevertheless, triboelectric charging is an exciting but so far not completely understood phenomenon. It has been investigated in many fields of research, such as contact electrification in dust devils (Farrell, 2004; Mareev and Dementyeva, 2017), in clouds after volcanic eruptions (Anderson et al, 1965; Mather and Harrison, 2006), in the formation of planets (Yair et al, 2008; Wang et al, 2017), and in almost every application dealing with fine and dry powders. Commonly, triboelectric charging is seen as a problem in industrial applications if particles are to be moved because charged particles tend to agglomerate and adhere on surfaces (Wong et al, 2015).…”
Section: Introductionmentioning
confidence: 99%
“…One natural idea is to assume a linear dependence between the charge separation current density and CAPE: ffalse(εfalse)=εε00, where ε00 is the characteristic value of CAPE in intense convective systems. Another option is to use the quadratic formula ffalse(εfalse)=)(εε002; the reasoning behind this assumption is that the charge separation current is proportional to both the relative velocity of colliding particles and the charge transferred in each collision, which, in its turn, is also related to the relative velocity by a power law with the exponent about 2 or 3 (at least in the case of noninductive charging; see Mareev & Dementyeva, ; Norville et al, ); thus, the charging current is proportional to the third or fourth power of the relative velocity, or to εi3false/2 or εi2 (since CAPE is approximately proportional to the square of this velocity; see Williams & Stanfill, ). Figure e shows the diurnal variation of the IP computed with and ; it is clear that both these curves are similar in shape to our basic curve but reach their main maxima earlier.…”
Section: Resultsmentioning
confidence: 99%
“…The fact that at the end of the IRNL mode a large multitude of negative leaders have been created supports the picture of a small region with a very high space charge. The dense charge pocket is probably created by a local turbulence [26], with a typical size of order 5 km 2 . This dense space charge leads to a larger than usual amount of charge at its tip and an increased propagation velocity, both contributing to a strongly enhanced VHF power and strong broadband pulses when the propagation is in the vertical direction during the IRNL mode.…”
Section: Discussionmentioning
confidence: 99%