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排序方式: 共有241条查询结果,搜索用时 46 毫秒
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Zhong Lingwei Liu Yu Li Juan Gu Zuo Jiang Haocheng Wang Haixing Tang Haibin 《中国航空学报》2010,23(1):15-21
Charge exchange(CEX) ions could inflict severe damages on the ion thruster optical system. This article is aimed at investigating the characteristics of the CEX ions and their influences upon the optical system by means of particle-in- cell(PIC) ion simulation and Monte Carlo collision(MCC) methods. The results from numerical simulation indicate that despite the fact that CEX ions appear in the entire beamlet region near the ion optical system, the ones that present themselves downstream of the accelerator grid have good reason for attracting more attention. As their trajectories are significantly affected by the local electric field, a great number of CEX ions are accelerated toward grids resulting in sputtering erosion. When the influences of the CEX ions are considered in the numerical simulation, there could hardly be observed augments in the screen grid current, but the accelerator grid current increases from zero to 1. 4% of the beamlet current. It can be understood from the numerical simulation that the CEX ions formed in the region far downstream of the accelerator grid should be blamed for the erosion on the downstream surface of the accelerator grid. 相似文献
104.
Energisation of O+ and O+
2 Ions at Mars: An Analysis of a 3-D Quasi-Neutral Hybrid Model Simulation
E. Kallio A. Fedorov S. Barabash P. Janhunen H. Koskinen W. Schmidt R. Lundin H. Gunell M. Holmström Y. Futaana M. Yamauchi A. Grigoriev J. D. Winningham R. Frahm J. R. Sharber 《Space Science Reviews》2006,126(1-4):39-62
We have studied the loss of O+ and O+
2 ions at Mars with a numerical model. In our quasi-neutral hybrid model ions (H+, He++, O+, O+
2) are treated as particles while electrons form a massless charge-neutralising fluid. The employed model version does not
include the Martian magnetic field resulting from the crustal magnetic anomalies. In this study we focus the Martian nightside
where the ASPERA instrument on the Phobos-2 spacecraft and recently the ASPERA-3 instruments on the Mars Express spacecraft
have measured the proprieties of escaping atomic and molecular ions, in particular O+ and O+
2 ions. We study the ion velocity distribution and how the escaping planetary ions are distributed in the tail. We also create
similar types of energy-spectrograms from the simulation as were obtained from ASPERA-3 ion measurements. We found that the
properties of the simulated escaping planetary ions have many qualitative and quantitative similarities with the observations
made by ASPERA instruments. The general agreement with the observations suggest that acceleration of the planetary ions by
the convective electric field associated with the flowing plasma is the key acceleration mechanism for the escaping ions observed
at Mars. 相似文献
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氧离子注入P型(100)单晶硅形成SIMOX样品,经俄歇电子能谱、扩展电阻仪测试,形成了SOI结构;经霍尔测试仪测试,制备的SIMOX样品表层硅膜反型为N型导电类型,SIMOX样品的反型是硅中的氧施主所致,由近自由电子的类氦模型计算,氧施主电离能力为0.15eV,该值与早期文献报道的实验值一致。 相似文献
109.
SAR卫星用能量功率兼顾型锂离子电池研究 总被引:3,自引:3,他引:0
未来大功率合成孔径雷达(SAR)卫星的发展对储能电池组提出了轻量化、倍率高及在轨寿命长等要求,而现有的SAR卫星用功率型锂离子电池产品已无法满足未来需求。通过优化正极材料和电池设计,加入功能电解液,在保证电池功率特性的同时,显著提升了电池的能量密度和循环稳定性。本文研制出的新一代能量功率兼顾型锂离子蓄电池,额定容量为25.0 Ah,初期放电比能量达到180.0 Wh·kg~(-1),2 C放电容量为0.2 C容量的91.0%,1 C-100%放电深度(DOD)和2 C-30%DOD循环性能优异,可以满足下一代大功率SAR卫星的供配电需求,且大幅降低了电源系统重量,提高了卫星储能系统的利用率和平台有效载荷能力。 相似文献
110.
固态电池具有高能量密度和高安全性等潜力,是未来航天器电源的重要解决方案。本文利用原位聚合方法,制备了聚甲基丙烯酸甲酯(PMMA)凝胶/Li_(6.5)La_3Zr_(1.5)Ta_(0.5)O_(12)(LLZT)复合电解质。通过选择与陶瓷相润湿性好的甲基丙烯酸甲酯单体(MMA)进行原位聚合,改善了电解质内部陶瓷与凝胶的两相界面。室温下,此复合电解质具有6.6×10~(-4)S·cm~(-1)的离子导电率。进一步采用原位聚合法,制备了Li/复合电解质/Li对称电池。与非原位方法相比,原位聚合将电解质与金属锂的界面比电阻从1 572Ω·cm~2降至367Ω·cm~2,对称电池在0.085 mA·cm~(-2)下能够稳定循环400圈,显示出良好的循环稳定性。 相似文献