共查询到13条相似文献，搜索用时 46 毫秒
1.
提出了一种原位探测月表电场的新技术及相应计算方法, 以满足探测南极月面电场环境特性的需求. 根据仿真结果, 月表电场精细测量需要低能散、高电流的平行电子束发射能力, 设计的低能层流电子枪在10–8～10–5 A的发射电流下, 能散<0.4 eV, 且随发射电流减弱而降低; 通过控制发射电流、调整阳极孔径, 可对电流进行调控; 采用pierce电子枪的阴阳极结构和静电透镜对电子束的平行度进行进一步控制, 仿真显示10–7 A电子束的扩散效果较弱, 各方面性能符合探测需求. 此外, 构建通过电子束返回时间测量垂直电场的探测方式, 模拟验证月表光照区向上发射电子束时相应的电场计算结果可反映背景电场, 返回电子式月表电场探测技术达到了执行月表电场测量所需的要求. 相似文献
2.
板式推进剂管理装置（PMD）是板式表面张力贮箱最重要的部件之一．为分析板式PMD管理推进剂能力,以某板式贮箱为研究对象,采用三维非定常流体（VOF）体积函数的两相流模型,对不同填充比时板式PMD的推进剂管理性能进行数值仿真,得到微重力下推进剂在PMD上及贮箱内部的分布情况,仿真结果与国外空间搭载试验结果比较吻合,数值仿真结果为板式贮箱的性能提供验证依据 相似文献
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介绍了一种微波及毫米波滤波器精确设计方法:由滤波器的原型参数,导出滤波器的广义阻抗变换系数;采用模匹配法或耦合积分方程技术等数值算法精确计算各个耦合结的S参数,进而转换成广义阻抗变换系数;通过插值,获得满足原型要求的滤波器各个耦合结的结构尺寸以及谐振腔长度,将结构参数代入模匹配程序、HFSS或CST软件进行分析,分析结果与预期值一致。设计了26GHz矩形波导带通滤波器,模匹配法和HFSS以及CST软件的仿真结果、测试数据与设计要求一致,说明该种设计方法是有效的。 相似文献
4.
针对外日球层低速、低密度、低温的拾起离子（PUIs）的高分辨探测需求,以带顶盖超环面静电分析器、阻滞势分析器和线性场飞行时间系统为基础设计了一种新型高分辨拾起离子探测器。经过有限元仿真分析,探测器可实现离子（氢）的速度范围15.7 ~1072.2 km/s,密度范围0.0001 ~100 cm?3,温度高于474.9 K的探测,同时可实现典型拾起离子（氢、氦、碳、氮、氧、氖）的成分分辨,质谱分辨率（M/ ΔM ）大于40。 相似文献
5.
Michael R. Collier William M. Farrell Timothy J. Stubbs 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
An analytic model for the motion of a positively charged lunar dust grain in the presence of a shadowed crater at a negative potential in vacuum is presented. It is shown that the dust grain executes oscillatory trajectories, and an expression is derived for the period of oscillation. Simulations used to verify the analytic expression also show that because the trajectories are unstable, dust grains are either ejected from the crater’s vicinity or deposited into the crater forming “dust ponds.” The model also applies to other airless bodies in the solar system, such as asteroids, and predicts that under certain conditions, particularly near lunar sunset, oscillating dust “canopies” or “swarms” will form over negatively charged craters. 相似文献
6.
基于SIMION软件的空间等离子体探测器的数值仿真 总被引：1，自引：0，他引：1
空间等离子体探测器采用带偏转板的柱形静电分析器作为传感器,具有大于320°探测视场,可探测约10eV～30keV的热等离子体。利用SIMION软件采用均匀随机抽样建立粒子源的方法仿真探测器的基本特性参数:静电分析器因子、能量分辨率、偏转板因子和偏转角。仿真结果与实测结果吻合很好。静电分析器因子的仿真与实测结果偏差为3.2%,能量分辨率仿真与实测结果偏差为1.5%,偏转角-偏转板因子的关系式与实测结果的相关系数为0.999 4。仿真结果可以有效地应用于该类仪器的设计和定标过程中。 相似文献
7.
月尘的静电悬浮和迁移是Apollo时期留下的最有争议的问题之一. 其既是研 究月球表面物质演化历史的重要线索, 也是探月工程必须考虑的重要因素. 月尘在月表环境下易因电子附着、光电效应、二次电子发射等过程带电, 并 在月球全球性静电场作用下发生迁移运动. 但目前对月尘静电迁移过程的认 识还不全面, 其主要原因在于对月尘静电特性的了解不够准确, 对静电迁移 过程的地面模拟不够充分以及对月球尘埃环境的探测较为缺乏. 未来需进一 步开展模拟月尘的研制, 月尘静电特性的分析, 静电迁移过程模拟以及尘埃 环境的探测等工作. 相似文献
8.
S.B. Rakesh Chandran G. Renuka Chandu Venugopal 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The Moon is immersed in plasma environment. The most interesting challenge of the lunar plasma– field environment is that it is alternatively dominated by the extended but variable outer atmosphere of the Earth – the magnetosphere – and by the extended but highly variable solar atmosphere – the solar wind. Understanding the plasma environment and its interaction with the lunar surface will be beneficial to both manned and robotic surface exploration activities and to scientific investigations. Presented is a preliminary map of variations of lunar surface electric potential over the day side and night side using probe equations and a discussion on dust dynamics in this E-field structure using the data from Electron Reflectometer in Lunar Prospector spacecraft during 1998–1999. On the day side, potential is around 5 V and on the night side it reaches up to −82 V. On the night side region, only highly energetic electrons can overcome this large negative potential. The variation at electron temperature (Te) strongly reflects in the surface potential. The potential reaches to a value of −82 V for Te = 58 eV. Surface charging causes the electrostatic transport of charged dust grains. Dust grain size of 0.1 μm shows a levitation height of 4.92 m on lunar day side, 748 m on terminator region and 3.7 km on the night side. The radius of maximum sized grain to be lofted, Rmax, peaks at the terminator region (Rmax = 0.83 μm). At the transition region dust levitation is almost absent. This region is most suited for exploration activities as the region is free from hazards caused by lunar dust. 相似文献
9.
建立准确、实用的月球着陆探测器动力学模型,是制导、导航和控制系统方案设计中的首要工作,文中月球软着陆探测器的推进剂贮箱采用横向对称分散布局的形式,并分析了布局方式对液体推进剂晃动的影响;将贮箱内液体考虑一阶弹簧质量模型,应用虚功率原理建立包含液体推进剂晃动的月球软着陆探测器从动力下降段至最终着陆段的动力学模型,并对动力学下降段进行了数值仿真,仿真结果可为月球软着陆探测器控制系统设计提供理论参考。 相似文献
10.
Yanwei Li Ralf Srama Hartmut Henkel Zoltan Sternovsky Sascha Kempf Yiyong Wu Eberhard Grün 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
One of the highest-priority issues for a future human or robotic lunar exploration is the lunar dust. This problem should be studied in depth in order to develop an environment model for a future lunar exploration. A future ESA lunar lander mission requires the measurement of dust transport phenomena above the lunar surface. Here, we describe an instrument design concept to measure slow and fast moving charged lunar dust which is based on the principle of charge induction. LDX has a low mass and measures the speed and trajectory of individual dust particles with sizes below one micrometer. Furthermore, LDX has an impact ionization target to monitor the interplanetary dust background. The sensor consists of three planes of segmented grid electrodes and each electrode is connected to an individual charge sensitive amplifier. Numerical signals were computed using the Coulomb software package. The LDX sensitive area is approximately 400 cm2. Our simulations reveal trajectory uncertainties of better than 2° with an absolute position accuracy of better than 2 mm. 相似文献
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12.
Nima Afshar-Mohajer Brian Damit Chang-Yu Wu Nicoleta Sorloaica-Hickman 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Lunar grains accumulate charges due to solar-based ionizing radiations, and the repelling action of like-charged particles causes the levitation of lunar dust. The lunar dust deposit on sensitive and costly surfaces of investigative equipment is a serious concern in lunar explorations. Inspired by electrostatic precipitators (ESPs), the Electrostatic Lunar Dust Collector (ELDC) was proposed for collecting already charged lunar dust particles to prevent the lunar dust threat. As the conditions for terrestrial counterparts are not valid in the lunar environment, equations developed for terrestrial devices yield incorrect predictions in lunar application. Hence, a mathematical model was developed for the ELDC operating in vacuum to determine its collection efficiency. The ratios of electrical energy over potential energy, kinetic energy over potential energy and the ratio of ELDC dimensions were identified to be the key dimensionless parameters. Sensitivity analyses of the relevant parameters showed that depending on ELDC orientation, smaller particles would be collected more easily at vertical orientation, whereas larger particles were easier to collect in a horizontal ELDC configuration. In the worst case scenario, the electrostatic field needed to be 10 times stronger in the vertical mode in order to adequately collect larger particles. The collection efficiency was very sensitive to surface potential of lunar dust and it reached the maximum when surface potential was between 30 and 120 V. 相似文献
13.
二维静电孤立波的粒子模拟研究 总被引：1，自引：0，他引：1
利用二维粒子模拟程序研究了双流不稳定性激发静电波并演化为静电孤立波的物理过程.计算结果表明,在线性增长阶段,主要激发的是沿磁场传播的静电波;在非线性演化阶段,相邻的静电波会互相合并,直至形成静电孤立波,并可激发静电哨声波.还研究了磁场强度和离子温度对此过程的影响.当磁场强度比较小时,无法形成静电孤立波,只有磁场强度达到一定程度后静电孤立波才能形成;同时,离子温度会影响静电孤立波的稳定性,当离子温度比较小时,静电孤立波的稳定性减弱,在演化一段时间后会逐渐瓦解. 相似文献