Design and experimental performance verification of a thermal property test-bed for lunar drilling exploration

Chinese Chang'e lunar exploration project aims to collect and return subsurface lunar soil samples at a minimum penetration depth of 2 m in 2017. However, in contrast to those on the Earth, automated drilling and sampling missions on the Moon raise the risk of burning bits.Test-beds are required for testing the thermal properties of drill tools in a lunar environment. In this paper, a novel temperature measuring method based on thermocouples and a slip ring was proposed. Furthermore, a data acquisition system for a drilling process was designed. A vacuous,cryogenic, and anhydrous soil environment simulating the lunar surface was established. A drilling test-bed that can reach a depth of 2.2 m was developed. A control strategy based on online monitoring signals was proposed to improve the drilling performance. Vacuum and non-vacuum experiments were performed to test the temperature rising effect on drill tools. When compared with the non-vacuum experiment, the vacuum temperature rise resulted in a 12 °C increase. These experimental results provide significant support for Chinese lunar exploration missions.     

气氮调温器Y型喷嘴实验及数值研究

基于FLUENT软件离散相模型及气体助力雾化模型,采用欧拉-拉格朗日方法研究通过Y型喷嘴雾化液氮的雾化特性.由于液氮液滴的蒸发相变,与水相比喷雾锥角更清晰且明显减小,约为10°,喷雾距离缩短.分析喷嘴气液工作压力对液氮雾化索太尔平均直径（SMD）、液滴体积分数和数量分数的影响.结果表明：SMD沿喷射方向变化幅度极小;SMD主要受气相速度及气液比影响,气压低时气相速度影响较大,气压高时气液比影响较大;由于相变作用,液氮雾化粒径分布更为集中.数值研究Y型喷嘴用于不同流量需求的气氮调温器的调温效果,出口温度低于98K,进出口温差达到12K,且整个出口温差在±1K以内,能够实现精确控温要求.     

行星际空间环境对探测器可靠性影响分析

空间环境是影响航天器可靠性的重要因素。与地球轨道航天器相比,行星际探测任务可能会遭受更加恶劣的空间环境,例如极端温度环境,辐射环境,腐蚀性大气环境、宇宙尘等,再加上行星际任务寿命长,采用先进的器件和材料,空间环境对行星际探测器的可靠性构成严重的威胁,直接关系到探测目标能否实现。因此考虑空间环境对行星际探测器的影响,开展相关的预先研究无论是对于制定行星际空间探测计划,还是搭载仪器的设计都具有非常重要的意义。文章分析了极端温度、辐射环境和行星表面综合环境对探测器的影响,并对开展相关研究提出了建议。     

基于Globus Toolkit 4的网格服务开发环境

模拟网格环境以及开发网格服务应用程序,首先要配置Globus系统。Globus Toolkit 4．0(GT4)现已成为构建网格环境和开发网格服务的首选平台。讨论了网格服务的基本思想,分析了GT4的新特性及其在产业界的应用,探讨了在Linux上安装和配置GT4的方法和过程,并对该系统进行了测试。     

中小型环模试验设备中局域网应用的设计

文章规划了中小型环模试验设备的热真空系统、常压热循环系统、无油超高系统等组成的局域网,以期在不断的实践中完善系统,充实并扩大组网内涵,实现环模试验的现代化管理。     

基于特征的雷达信号环境仿真

通过分析装备的试验需求,解析雷达信号环境的特征,提出了具有针对性、适应性、可扩展性和层次化的雷达信号环境仿真策略。对实践应用具有较强的参考性。     

论航天器的综合环境试验

讨论了在航天器研制中综合环境试验的重要性和必要性,简单介绍了航天器研制中的各种综合环境试验,对如何设计和应用综合环境试验提出了一些看法。     

光纤光栅温度传感器研究进展

归纳了以光纤光栅为基础的温度传感器的研究现状,总结了这些温度传感器的基本原理,再现了它们的主要结构,展示了原文提到的实验过程和数据分析结果,并对这些传感器的优点和不足进行了分析,提出了部分改进方案。通过研究发现：光纤光栅温度传感器具有优良的特性,能够在恶劣环境下测量极高的温度,具有广阔的应用前景。     

基于工作过程的《制冷技术》课程教学设计

根据高等职业教育新的课程理念,对《制冷技术》课程的教学进行了改革。基于对实际工作过程的分析和思考,设计了学习情境,重构了课程内容,以学生为主体组织实施教学,创新了考核方法,有效地提高了教学效果。     

Characterization of the near Earth radiation environment by Liulin type spectrometers

Comprehensive study of the dose, flux and deposited energy spectra shape data obtained by Liulin type spectrometers on spacecraft (five different experiments) and aircraft since 2001 is performed with the aim of understanding how well these parameters can characterize the type of predominant particles and their energy in the near Earth radiation environment. Three different methods for characterisation of the incoming radiation from Liulin spectrometers are described. The results revealed that the most informative one is by the shape of the deposited energy spectra. Spectra generated by Galactic Cosmic Rays (GCR) protons and their secondaries are with linear falling shape in the coordinates deposited energy/deposited per channel dose rate. The position of the maximum of the deposited energy spectra inside the South Atlantic Anomaly (SAA) region depends on the incident energy of the incoming protons. Spectra generated by relativistic electrons in the outer radiation belt have a maximum in the first channels. For higher energy depositions these spectra are similar to the GCR spectra. Mixed radiation by protons and electrons and/or bremsstrahlung is characterized by spectra with 2 maxima. All type of spectra has a knee close to 6.2 MeV deposited energy, which correspond to the stopping energy of protons in the detector. Dose to flux ratio known also as specific dose is another high information parameter, which is given by experimentally obtained formulae [Heffner, J. Nuclear radiation and safety in space. M. Atomizdat. 115, 1971 (in Russian)] connecting the dose to flux ratio and the incident energy of the particles.