临近空间地面模拟装置等离子体源仿真研究

为了指导临近空间地面模拟装置中等离子体源结构设计及等离子体环境参数优化，围绕相关指标体系要求，采用数值模拟方法，分析临近空间等离子体环境地面模拟装置中的射流等离子体与下游目标模拟体相互作用。通过研究射流入口处等离子体状态与下游等离子体对钝体包覆效果的依赖关系，明确了影响包覆特性的关键等离子体参数、重要外控参量，及其对下游目标模拟体包覆特性的影响规律。仿真结果表明：相对于其他因素，射流入口的半径、气体流速、速度偏角、气体温度、钝体直径、环境背压等工况对有效实验区长度及厚度参数的影响较大。相关结果对于临近空间等离子体环境地面模拟装置中等离子体源优化设计及等离子体环境参数定向调控具有指导和借鉴意义。     

基于数字孪生的航天电推进器优化设计方法

针对以引力波探测为代表的空间科学任务和以“国网星座计划”为代表的商用卫星网络任务对推进器的特殊需求，本文提出了一种基于数字孪生的推进器优化设计方法。该方法首先建立由机理模型模块和测试数据集模块组成的数字孪生体。机理模型模块依据推进器的物理过程建立模型，对难以测量的数据进行仿真模拟；测试数据集模块通过实验对推进器进行测试，依靠测试数据建立可测参数的数学模型。将数字孪生体与实验进行对比，通过对比结果反馈调节机理模块从而不断提高孪生体的准确性，最终为优化设计提供依据。结果表明：(1)该方法能够构建微波离子推进器的数字孪生体；(2)该数字孪生体的预测结果存在一定差异，通过分析发现该差异与机理模型的精细度以及测试数据集的数据量有关。     

Development and coupling test of active spacecraft potential control – Next generation (ASPOC-NG)

The active spacecraft potential control (ASPOC) system developed in the 1990s emits positive ions to neutralise the spacecraft potential, such as used in several missions like Geotail, Equator-S, Cluster, Doublestar and MMS. With the experience gained, the next generation of the active spacecraft potential control (ASPOC-NG) instrument has been developed over the last three years. Thereby, three emission technologies were tested including Liquid Metal Ion Source (LMIS), Liquid Metal Electron Source (LMES) and Solid Metal Electron Source (SMES). The development of the emitter module by FOTEC and the corresponding electronics control unit by IWF is presented. Optimisations were carried out with the focus on the reduction of mass and power consumption to comply with the requirements of future scientific missions. Coupling tests of the modules and the electronics control unit were performed including range, accuracy and lifetime tests. Both ASPOC-NG instruments for positive and negative charge compensation and their performance values show excellent results.     

高频热等离子体法合成纳米ZrC粉体及其表征

以炭黑和甲烷分别作为碳源,四氯化锆作为锆源,采用高频热等离子体法合成了超细ZrC粉体。分别采用XRD、高频红外燃烧、SEM、化学重量法对实验产物进行了表征,分析了超细ZrC粉体的物相、纯度、粒径与碳源及进气量之间的影响规律。研究表明:采用不同碳源所合成的ZrC粉体粒径均在100 nm以下,相比较炭黑为碳源,甲烷作为碳源合成的产品纯度高,氧含量低,产率大,因此,甲烷作为碳源更适于批量制备超细ZrC粉体。     

基于双回路控制的电动负载模拟器研究

电动舵机负载模拟器可在实验条件下模拟飞行器飞行过程中舵机受到的空气动力铰链力矩,是半实物仿真的重要设备。在介绍电动负载模拟器研究进展并指出目前伺服系统研究所面临的难题的基础上,以改善系统动态频响为目标,设计基于双回路电机的加载方案并建立双回路系统的数学模型;通过系统仿真,分析系统输出力矩对指令力矩的跟踪能力,验证数学模型的准确性。结果表明:双回路方案有效地抑制了系统多余力,其工作频带在舵机扰动的情况下仍可达35 Hz,为电动负载模拟器提供了一种频带更高、匹配性更好的实现方案。     

2219 铝合金单、双道焊接头性能分析

通过对比2219 铝合金单道氩弧焊和氦弧打底+氩弧盖面双道焊接头的常温及液氮温度拉伸性
能、显微硬度分布、单向拉伸过程的数字散斑测量(DIC)结果,发现在常、低温条件下双道焊接头的拉伸强度和
延伸率均比单道焊接头高10% ~20%,单道焊接头焊缝及热影响区内材料的显微硬度值相比母材的降低程度
比双道焊接头更为显著,其主要原因是单道焊接头的一次性热输入大于双道焊,材料受热影响更严重,焊漏高
度及形状的可控性更差。     

电动膨胀循环液氧甲烷变推力发动机动态特性研究

电动泵压式液体火箭发动机受到了广泛的关注，然而电池有限的输出功率和过于沉重的质量成为限制电动泵压式发动机发展的重要因素。为此本文提出了一种电机驱动燃料泵和涡轮驱动氧泵的电动膨胀循环液体火箭发动机方案，并着重研究了该型发动机的动态响应特性。首先给出了20 kN级电动膨胀循环发动机的技术指标和部组件参数，进一步基于AMESim平台建立了全系统动力学模型，验证了方案的可行性和部组件动力学模型的准确性，并深入研究了单点工况和调节工况的动态响应特性。结果表明，针对启动过程而言，涡轮泵调整时间较电动泵长，这降低了系统响应速度，但工况越高，系统响应速度越快；高工况启动时，甲烷在冷却通道内的剧烈相变和跨临界状态的不连续物性相互耦合易引发系统振荡；就调节过程而言，推力调节时普遍存在超调或凹坑现象，且系统在两相同工况之间调节时，正调响应速度快于负调，这也导致阶跃幅值相等条件下的系统调整时间随目标工况升高而缩短。     

An atmosphere-breathing propulsion system using inductively coupled plasma source

CubeSats have attracted more research interest recently due to their lower cost and shorter production time. A promising technology for CubeSat application is atmosphere-breathing electric propulsion, which can capture the atmospheric particles as propulsion propellant to maintain long-term mission at very low Earth orbit. This paper designs an atmosphere-breathing electric propulsion system for a 3 U CubeSat, which consists of an intake device and an electric thruster based on the inductively coupled plasma. The capture performance of intake device is optimized considering both particles capture efficiency and compression ratio. The plasma source is also analyzed by experiment and simulation. Then, the thrust performance is also estimated when taking into account the intake performance. The results show that it is feasible to use atmosphere-breathing electric propulsion technology for CubeSats to compensate for aerodynamic drag at lower Earth orbit.     

Shocks and instabilities in the partially ionised solar atmosphere

The low solar atmosphere is composed of mostly neutral particles, but the importance of the magnetic field for understanding observed dynamics means that interactions between charged and neutral particles play a very important role in controlling the macroscopic fluid motions. As the exchange of momentum between fluids, essential for the neutral fluid to effectively feel the Lorentz force, is through collisional interactions, the relative timescale of these interactions to the dynamic timescale determines whether a single-fluid model or, when the dynamic frequency is higher, the more detailed two-fluid model is the more appropriate. However, as many MHD phenomena fundamentally contain multi-time-scale processes, even large-scale, long-timescale motions can have an important physical contribution from two-fluid processes. In this review we will focus on two-fluid models, looking in detail at two areas where the multi-time-scale nature of the solar atmosphere means that two-fluid physics can easily develop: shock-waves and instabilities. We then connect these ideas to observations attempting to diagnose two-fluid behaviour in the solar atmosphere, suggesting some ways forward to bring observations and simulations closer together.     

转子闭口槽在高效电机中的应用

高效电动机采用转子闭口槽工艺,可以减小转子齿槽产生的损耗,提高电机效率。通过闭口槽样机试制及样机试验数据,验证了转子闭口槽结构性能,得出该工艺可行,并提出相应的工艺措施。