行星大气中带电尘埃粒子动力学引起的电磁现象:实验室模拟和现场观测

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
Mohamad E. Abdelaal, Alexander V. Zakharov
{"title":"行星大气中带电尘埃粒子动力学引起的电磁现象:实验室模拟和现场观测","authors":"Mohamad E. Abdelaal,&nbsp;Alexander V. Zakharov","doi":"10.1134/S0038094625600519","DOIUrl":null,"url":null,"abstract":"<p>Dust electrification and its associated electromagnetic (EM) emissions play a critical role in atmospheric and near-surface dynamics across planetary environments. This study provides a synthesis of recent work under publication that investigates the mechanisms of charge accumulation, electrostatic discharge, and electromagnetic radiation generation in dust-laden flows under both terrestrial and Mars-analog conditions, using a combined approach of analytical modeling, laboratory experiments, and field measurements. Laboratory experiments were conducted in the Earth conditions and in low-pressure CO<sub>2</sub>-rich environments to simulate Martian conditions, employing silicate and basaltic samples across a range of grain sizes. The results demonstrate that triboelectric and tunneling charge transfer mechanisms, activated during vortex-driven particle dynamics, can induce transient discharges that generate broadband electromagnetic signals in the ~120–1500 kHz range. Under simulated Martian conditions, Paschen breakdown behavior was experimentally verified, confirming significantly lower breakdown thresholds compared to Earth’s atmosphere. Complementary field measurements carried out in the Kalmykian desert (Russia) further revealed that low humidity and intense solar radiation, even in the presence of moderate wind speeds, enhance dust electrification and discharge activity, leading to detectable EM emissions. Data were recorded using the Electromagnetic Analyzer (EMA), originally developed for Mars surface studies. Analysis of the recorded EM signal using time-domain analysis, Fast Fourier Transform (FFT), and continuous wavelet transform (CWT) revealed distinct amplitude-frequency signatures that correlate with particle properties and environmental drivers. These findings establish a new conceptual framework for understanding dust-driven EM phenomena in planetary atmospheres and underscore the applied relevance of electromagnetic diagnostics for future Mars, Moon, and Venus missions.</p>","PeriodicalId":778,"journal":{"name":"Solar System Research","volume":"59 7","pages":""},"PeriodicalIF":0.8000,"publicationDate":"2025-09-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Electromagnetic Phenomena Induced by Charged Dust Particles Dynamics in Planetary Atmospheres: Laboratory Simulations and Field Observations\",\"authors\":\"Mohamad E. Abdelaal,&nbsp;Alexander V. Zakharov\",\"doi\":\"10.1134/S0038094625600519\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Dust electrification and its associated electromagnetic (EM) emissions play a critical role in atmospheric and near-surface dynamics across planetary environments. This study provides a synthesis of recent work under publication that investigates the mechanisms of charge accumulation, electrostatic discharge, and electromagnetic radiation generation in dust-laden flows under both terrestrial and Mars-analog conditions, using a combined approach of analytical modeling, laboratory experiments, and field measurements. Laboratory experiments were conducted in the Earth conditions and in low-pressure CO<sub>2</sub>-rich environments to simulate Martian conditions, employing silicate and basaltic samples across a range of grain sizes. The results demonstrate that triboelectric and tunneling charge transfer mechanisms, activated during vortex-driven particle dynamics, can induce transient discharges that generate broadband electromagnetic signals in the ~120–1500 kHz range. Under simulated Martian conditions, Paschen breakdown behavior was experimentally verified, confirming significantly lower breakdown thresholds compared to Earth’s atmosphere. Complementary field measurements carried out in the Kalmykian desert (Russia) further revealed that low humidity and intense solar radiation, even in the presence of moderate wind speeds, enhance dust electrification and discharge activity, leading to detectable EM emissions. Data were recorded using the Electromagnetic Analyzer (EMA), originally developed for Mars surface studies. Analysis of the recorded EM signal using time-domain analysis, Fast Fourier Transform (FFT), and continuous wavelet transform (CWT) revealed distinct amplitude-frequency signatures that correlate with particle properties and environmental drivers. These findings establish a new conceptual framework for understanding dust-driven EM phenomena in planetary atmospheres and underscore the applied relevance of electromagnetic diagnostics for future Mars, Moon, and Venus missions.</p>\",\"PeriodicalId\":778,\"journal\":{\"name\":\"Solar System Research\",\"volume\":\"59 7\",\"pages\":\"\"},\"PeriodicalIF\":0.8000,\"publicationDate\":\"2025-09-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Solar System Research\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S0038094625600519\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar System Research","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S0038094625600519","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

尘埃电气化及其相关的电磁(EM)发射在整个行星环境的大气和近地表动力学中起着关键作用。本研究综合了最近发表的研究成果,利用分析建模、实验室实验和现场测量相结合的方法,研究了地面和火星模拟条件下含尘气流中电荷积累、静电放电和电磁辐射产生的机制。实验室实验是在地球条件和低压富含二氧化碳的环境中进行的,以模拟火星条件,使用了一系列颗粒大小的硅酸盐和玄武岩样品。结果表明,在涡旋驱动粒子动力学过程中激活的摩擦电和隧道电荷转移机制可以诱导瞬态放电,产生约120-1500 kHz范围内的宽带电磁信号。在模拟火星条件下,Paschen的击穿行为得到了实验验证,证实与地球大气相比,击穿阈值明显较低。在卡尔梅克沙漠(俄罗斯)进行的补充野外测量进一步表明,即使在中等风速的情况下,低湿度和强烈的太阳辐射也会增强粉尘的电气化和排放活动,从而导致可检测到的电磁辐射。数据记录使用电磁分析仪(EMA),最初是为火星表面研究开发的。利用时域分析、快速傅立叶变换(FFT)和连续小波变换(CWT)对记录的电磁信号进行分析,揭示了与粒子特性和环境驱动因素相关的不同幅频特征。这些发现为理解行星大气中尘埃驱动的电磁现象建立了一个新的概念框架,并强调了电磁诊断在未来火星、月球和金星任务中的应用相关性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Electromagnetic Phenomena Induced by Charged Dust Particles Dynamics in Planetary Atmospheres: Laboratory Simulations and Field Observations

Electromagnetic Phenomena Induced by Charged Dust Particles Dynamics in Planetary Atmospheres: Laboratory Simulations and Field Observations

Dust electrification and its associated electromagnetic (EM) emissions play a critical role in atmospheric and near-surface dynamics across planetary environments. This study provides a synthesis of recent work under publication that investigates the mechanisms of charge accumulation, electrostatic discharge, and electromagnetic radiation generation in dust-laden flows under both terrestrial and Mars-analog conditions, using a combined approach of analytical modeling, laboratory experiments, and field measurements. Laboratory experiments were conducted in the Earth conditions and in low-pressure CO2-rich environments to simulate Martian conditions, employing silicate and basaltic samples across a range of grain sizes. The results demonstrate that triboelectric and tunneling charge transfer mechanisms, activated during vortex-driven particle dynamics, can induce transient discharges that generate broadband electromagnetic signals in the ~120–1500 kHz range. Under simulated Martian conditions, Paschen breakdown behavior was experimentally verified, confirming significantly lower breakdown thresholds compared to Earth’s atmosphere. Complementary field measurements carried out in the Kalmykian desert (Russia) further revealed that low humidity and intense solar radiation, even in the presence of moderate wind speeds, enhance dust electrification and discharge activity, leading to detectable EM emissions. Data were recorded using the Electromagnetic Analyzer (EMA), originally developed for Mars surface studies. Analysis of the recorded EM signal using time-domain analysis, Fast Fourier Transform (FFT), and continuous wavelet transform (CWT) revealed distinct amplitude-frequency signatures that correlate with particle properties and environmental drivers. These findings establish a new conceptual framework for understanding dust-driven EM phenomena in planetary atmospheres and underscore the applied relevance of electromagnetic diagnostics for future Mars, Moon, and Venus missions.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
×
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:604180095
Book学术官方微信