Effect of particle inertia on the alignment of small ice crystals in turbulent clouds

K. Gustavsson, M. Z. Sheikh, A. Naso, A. Pumir, B. Mehlig
{"title":"Effect of particle inertia on the alignment of small ice crystals in turbulent clouds","authors":"K. Gustavsson, M. Z. Sheikh, A. Naso, A. Pumir, B. Mehlig","doi":"10.1175/JAS-D-20-0221.1","DOIUrl":null,"url":null,"abstract":"Small non-spherical particles settling in a quiescent fluid tend to orient so that their broad side faces down, because this is a stable fixed point of their angular dynamics at small particle Reynolds number. Turbulence randomises the orientations to some extent, and this affects the reflection patterns of polarised light from turbulent clouds containing ice crystals. An overdamped theory predicts that turbulence-induced fluctuations of the orientation are very small when the settling number Sv (a dimensionless measure of the settling speed) is large. At small Sv, by contrast, the overdamped theory predicts that turbulence randomises the orientations. This overdamped theory neglects the effect of particle inertia. Therefore we consider here how particle inertia affects the orientation of small crystals settling in turbulent air. We find that it can significantly increase the orientation variance, even when the Stokes number St (a dimensionless measure of particle inertia) is quite small. We identify different asymptotic parameter regimes where the tilt-angle variance is proportional to different inverse powers of Sv. Parameter values for ice crystals in turbulent clouds lie near the boundaries between these regions; ice crystal-alignment in such clouds is thus unlikely to follow a simple power law. The theory predicts how the degree of alignment depends on particle size, shape, and turbulence intensity.","PeriodicalId":328276,"journal":{"name":"arXiv: Fluid Dynamics","volume":"24 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-07-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"8","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: Fluid Dynamics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1175/JAS-D-20-0221.1","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 8

Abstract

Small non-spherical particles settling in a quiescent fluid tend to orient so that their broad side faces down, because this is a stable fixed point of their angular dynamics at small particle Reynolds number. Turbulence randomises the orientations to some extent, and this affects the reflection patterns of polarised light from turbulent clouds containing ice crystals. An overdamped theory predicts that turbulence-induced fluctuations of the orientation are very small when the settling number Sv (a dimensionless measure of the settling speed) is large. At small Sv, by contrast, the overdamped theory predicts that turbulence randomises the orientations. This overdamped theory neglects the effect of particle inertia. Therefore we consider here how particle inertia affects the orientation of small crystals settling in turbulent air. We find that it can significantly increase the orientation variance, even when the Stokes number St (a dimensionless measure of particle inertia) is quite small. We identify different asymptotic parameter regimes where the tilt-angle variance is proportional to different inverse powers of Sv. Parameter values for ice crystals in turbulent clouds lie near the boundaries between these regions; ice crystal-alignment in such clouds is thus unlikely to follow a simple power law. The theory predicts how the degree of alignment depends on particle size, shape, and turbulence intensity.
粒子惯性对湍流云中小冰晶排列的影响
静止流体中的非球形小颗粒倾向于使其宽面朝下,因为这是小颗粒雷诺数下角动力学的稳定不动点。湍流在一定程度上随机化了方向,这影响了包含冰晶的湍流云中偏振光的反射模式。过阻尼理论预测,当沉降数Sv(沉降速度的无量纲度量)很大时,湍流引起的方向波动很小。相比之下,在小Sv下,过阻尼理论预测湍流使方向随机化。这种过阻尼理论忽略了粒子惯性的影响。因此,我们在这里考虑粒子惯性如何影响在湍流空气中沉降的小晶体的取向。我们发现,即使斯托克斯数St(粒子惯性的无量纲度量)很小,它也能显著增加取向方差。我们确定了不同的渐近参数区,其中倾角方差与Sv的不同逆幂成正比。湍流云中冰晶的参数值位于这些区域之间的边界附近;因此,这种云中的冰晶排列不太可能遵循简单的幂律。该理论预测了排列程度如何取决于颗粒大小、形状和湍流强度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信