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Surface Potential of Dust Grains at the Sheath Edge of Electronegative Dusty Plasmas
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作者 段萍 王正汹 +3 位作者 王文春 刘金远 刘悦 王晓钢 《Plasma Science and Technology》 SCIE EI CAS CSCD 2004年第6期2559-2563,共5页
In this paper we investigate the dust surface potential at the sheath edge of electronegative dusty plasmas theoretically, using the standard fluid model for the sheath and treating electrons and negative ions as Bolt... In this paper we investigate the dust surface potential at the sheath edge of electronegative dusty plasmas theoretically, using the standard fluid model for the sheath and treating electrons and negative ions as Boltzmann particles but positive ions and dust grains as cold fluids. The dust charging model is self-consistently coupled with the sheath formation criterion by the dust surface potential and the ion Mach number, moreover the dust density variation is taken into account. The numerical results reveal that the dust number density and negative ion number density as well as its temperature can significantly affect the dust surface potential at the sheath edge. 展开更多
关键词 electronegative plasma dust grain dust surface potential
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EQUILIBRIUM POTENTIAL OF DUST GRAINS IN COMETARY PLASMA ENVIRONMENTS
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作者 Chen Yao Li Zhongyuan Shi Zhidong (University of Science and Technology of China, Hefei 230026) (Advanced Center for Earth Science and Astronomy, Third World Academy of Science) 《中国科学院上海天文台年刊》 2000年第S1期189-193,共5页
The equilibrium potential of fluffy dust grains in plasma are calculated for comet P/Halley and comet P/G-Z. It is found that the dust equilibrium potential linearly correlates with the logarithm of electron density. ... The equilibrium potential of fluffy dust grains in plasma are calculated for comet P/Halley and comet P/G-Z. It is found that the dust equilibrium potential linearly correlates with the logarithm of electron density. We propose this relationship can also be applied to comet Hale-Bopp. 展开更多
关键词 COMET - plasma - dust grains - CHARGING - EQUILIBRIUM potential
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The effect of positive/negative ion on the dust grain charging process in a Vasyliunas-Cairns (VC)-distributed dusty plasma system
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作者 N AHMAD A A ABID +2 位作者 Y AL-HADEETHI M N S QURESHI Saqib REHMAN 《Plasma Science and Technology》 SCIE EI CAS CSCD 2019年第6期58-62,共5页
Charging mechanism of dust particles has been considered as a growing research area in dusty plasma physics because of its exciting results.In this paper,we consider a low-temperature non-equilibrium multispecies plas... Charging mechanism of dust particles has been considered as a growing research area in dusty plasma physics because of its exciting results.In this paper,we consider a low-temperature non-equilibrium multispecies plasma model,which consists of Vasyliunas-Caims (VC) distributed electrons,negative/positive streaming ions,and negatively-charged dust grains to explain the charging mechanism of dust grains.The main theme of this work is to derive expressions of currents for negatively-charged dust grains (considering an equilibrium state position) in the plasma environment comprised of electrons and positive/negative streaming ions using the VC distribution function.Our proposed model shows that the dust grain surface potential is significantly affected by different plasma parameters such as the negative ion streaming velocity (Sn),positive ion streaming velocity (Si),spectral indices of VC distribution,negative ion charging state (Zn),positive ion charging state (Zi),and negative ion number density (ρ). 展开更多
关键词 dust grain surface potential vasyliunas-cairns power LAW velocity distribution function multi species plasma
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月球南极尘埃等离子体环境特性
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作者 李梦谣 夏清 +4 位作者 蔡明辉 杨涛 许亮亮 贾鑫禹 韩建伟 《物理学报》 SCIE EI CAS CSCD 北大核心 2024年第15期133-140,共8页
由于缺少大气和全球性磁场的保护,空间等离子体环境可直接作用于月球表面的月壤层,月壤中较小粒径的月尘带电后会在月面附近形成复杂的尘埃等离子体环境,影响探月任务的顺利实施.针对月球南极尘埃等离子体环境,本文利用SPIS(spacecraft ... 由于缺少大气和全球性磁场的保护,空间等离子体环境可直接作用于月球表面的月壤层,月壤中较小粒径的月尘带电后会在月面附近形成复杂的尘埃等离子体环境,影响探月任务的顺利实施.针对月球南极尘埃等离子体环境,本文利用SPIS(spacecraft plasma interactions software)软件,仿真研究了月球南极0—200 m高度范围的等离子体和月尘的空间分布情况及月面充电特性,揭示了月面附近尘埃等离子体环境特征及悬浮在月面附近的带电月尘对等离子体环境的影响.仿真结果与Apollo探测数据和Popel团队的理论数据吻合.研究结果:表明空间电位随着高度升高而增加,月球南极附近0—10 m电位约为–40 V,在100 m处空间电位约为–20 V;在10 m以下高度范围内月尘密度为10^(7.22)—10^(4.66) m^(–3);月表附近尘埃等离子体中的电子密度为10^(5.47) m^(–3),离子密度为10^(6.07) m–3,并随着高度升高而增大;带电月尘会影响月尘的空间分布,主要是通过影响空间电场的分布,进而导致电子分布差异,对离子的影响不大. 展开更多
关键词 月球南极 尘埃等离子体环境 SPIS 仿真 月面电位分布
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