Late Stages of Stellar Evolution

A large fraction of ISO observing time was used to study the late stages of stellar evolution. Many molecular and solid state features, including crystalline silicates and the rotational lines of water vapour, were detected for the first time in the spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres and circumstellar environments. A surprising number of objects, particularly young planetary nebulae with Wolf-Rayet (WR) central stars, were found to exhibit emission features in their ISO spectra that are characteristic of both oxygen-rich and carbon-rich dust species, while far-IR observations of the PDR around NGC 7027 led to the first detections of the rotational line spectra of CH and CH⁺. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

月食过程月表太阳辐照和温度变化模拟

月食对月球轨道探测器的温度有重要的影响,分析月食时月表的太阳辐照和温度,具有重要意义。文章给出了通用的月表温度模型和月食时月表太阳辐照模型,根据某次月食的天文参数,用太阳辐照模型可求出月表任一点在月食时的太阳直接辐照变化过程,代入温度模型可求出任一点的温度变化过程。此模型和方法可用于对任何一次月食的分析,并以2007年8月28日的月食为例,模拟了该次月食的表面太阳直接辐照和温度的变化过程。     

利用高空科学气球收集宇宙尘粒

本文叙述了高空科学气球上一种自行研制的宇宙尘收集器以及气球吊篮系统。利用该系统进行了五次高空字宙尘粒的收集飞行,简述了对所收集的尘粒进行系统研究的结果。     

月球探测器姿态大角度机动的反作用轮控制

研究了月球探测器转速与控制力矩受限的姿态大角度机动问题。根据时间变尺度思想，提出了双回路反馈的姿态大角度机动控制方法。以某型月球控测器为例，对该方法进行了仿真验证。结果表明，利用该控制方法，可使探测器以期望的角速度转动，从而完成探测器的姿态大角度机动。     

模拟月壤研制的初步设想

模拟月壤是月球样品的地球化学复制品，作者总结世界上已有的5种模拟月壤JSC-1，MLS．1，MLS-2，MKS-1和FJS-1的研制过程、方法与基本理化性质，认为系列化模拟月壤研制对中国首次月球探测有重要意义，在此基础上，作者提出系列化模拟月壤研制的基本思路．     

Experimental investigation on silica dust lofting due to charging within micro-cavities and surface electric field in the vacuum chamber

The charged dust particles can be mobilized electrostatically by the repulsion between the adjacent grains and the surface electric field due to the incoming electron current and the charge accumulation within the micro-cavities. In this study, the experimental results of the initial vertical launching velocities and the maximum dust heights are compared with the estimated values for the lofted spherical dust grains by the patch surface charging equations. Silica particles with the sizes between <6 and 45?µm in radius are loaded on a graphite plate, and they are exposed to the electron beam with 450?eV energy under 4?×?10^?3?Pa vacuum chamber pressure. During the first set of the experiments, the dust samples are tested without an initial compression process and an additional horizontal electric field. Second, the dust samples are compressed by two different weights in order to increase the packing density under approximately 780.7?Pa and 3780?Pa. Finally, the dust grains are placed between the two parallel aluminum plates to apply approximately 2000?V/m and 4800?V/m horizontal electric field. A high-speed camera is used to record the transportation of the dust grains together with a microscopic telescope, and the results point out that the patch surface dust-charging model estimations are in agreement with the first experiments. On the other hand, the dust particles from the compressed samples are lofted with higher velocities than the estimations, and the number of the dust lofting observations decreases significantly, which demonstrates the importance of the micro-cavities and the increased charging requirement to overcome the contact forces. When the horizontal electric field is present, the initial vertical launching velocities are measured to be lower than the other experiments, which can be attributed to the decreased charging requirement for the dust lofting as a result of inter-particle collisions and rolling motion. According to the experimental results, the electrostatic dust transportation can be controlled not only by the ambient plasma and the solar irradiation on the airless planetary bodies, but also by the surface properties such as the contact surfaces between the dust grains, the number of the micro-cavities related to the packing density, and the presence of the horizontal electric field contributing to the external forces by other particle motions.     

卷簧式浅层月壤取样器设计及动力学分析

面向浅层月壤取样,文章设计了新颖的卷簧式可伸缩小型月壤取样器,它包括柔性取样臂和振动式取样头。对取样器进行了动力学有限元分析,研究了取样臂为不同长度时取样头的振动模态及频率响应,得出取样臂一阶横振频率与取样臂长度呈负幂函数关系;对取样器测控系统进行了振动试验,通过扫频方式测量取样臂为不同长度时的自振频率,给出了取样臂长...     

载人月球探测月面活动发展设想

载人月球探测是浩大的系统工程,组成复杂,关键技术多,研制周期长,经费投入高,任务风险大.月面活动是载人月球探测任务体现能力、保障安全、提升效益的重要组成部分,必须回答"为什么""去哪里""怎么干"等问题.本文从国内外月球探测历程出发,结合当今世界月球探测领域趋势与局势,从月球战略布局、月球科学内涵开展分析.针对月面驻留...     

崎岖地形中关节式月球车姿态估计数值求解方法

 以被动关节式地形自适应月球车为研究对象,融合关节机器人D-H坐标建模方法构建了月球车悬架运动学模型和以侧倾、俯仰和偏转角表示姿态的欧拉角方式建立了车轮到世界坐标系的悬架完整表达模型。利用悬架完整表达模型,用带有迭代因子的连续迭代和离散迭代数值求解方法,建立了光滑和离散崎岖地形姿态估计算法。最后以8轮扭杆双摇杆摇臂月球车原理样机为例来验证此模型求解方法。仿真结果验证了所建立的基于数值方法的崎岖地形被动关节式月球车姿态估计模型的正确性,其求解模型精度能够满足仿真要求。     

风量与风机的安全运行

本文阐明了离心式通风机在通风除尘(或排毒净化)系统中的作用,以及离心式通风机产生风压.风量的工作工程,从而引出风机的性能参数风量L、风压P、功率N、效率η等.文章突出地论述了风量对风压、功率、效率的影响;详尽地分析了离心式通风机的性能曲线,特别是N—L曲线;根据性能曲线分析得知,风量L为零(L=0)时,风消耗的功率N最小.从而得出结论;系统中的离心式通风机必须是在关闭状态下启动,以确保通风机的安全运行.