深海潜水器推进器故障诊断技术研究进展

推进器是深海潜水器主要执行且负荷最重的部件,对其故障快速准确诊断是关系深海潜水器安全运行的关键技术之一。深海环境的复杂和深海潜水器自身的非线性、强耦合和模型的不确定性使其故障诊断成为一个研究的难点问题。从深潜器推进器主要类型、典型的故障模式、推进器故障诊断技术等方面对当前深潜器推进器故障诊断技术研究进展进行了综述,并对深海推进器及其故障诊断技术发展方向进行了探讨。     

同轴形微波等离子推力器数值计算

介绍了100W功率同轴形微波等离子推力器(MPT)的系统结构、谐振模式,采用耦合求解Maxwell方程、Saha方程和Navier-Stokes方程的方法,对100W同轴形MPT振腔内的电磁场、等离子体与流场间的耦合问题进行了数值计算并预估了原理实验样机的性能。计算结果表明,100W同轴形MPT结构系统的原理可行,性能较好,有较好的发展前景。      

基于多目标规划的交会对接推力器指令分配方法

将由控制律得到的控制量转化为推力器控制指令的过程称为推力器指令分配。由于交会对接涉及的推力器配置复杂,且对追踪航天器姿轨控精度的要求很高,因此其推力器指令分配问题十分重要。本文针对该问题,分析了基于线性规划的指令分配方法存在的不足,提出了将推力器指令分配问题转化为非线性多目标规划问题,并应用分枝定界法进行寻优的新方法。新方法可以在指令分配的误差和燃料消耗之间进行折衷,并且考虑了推力器最小开机时间的限制。仿真结果验证了新方法的有效性。     

离子推力器羽流特性及其污染分析

介绍了与电推进系统有关的空间环境效应的形成原因及其对航天器性能、寿命等的影响。阐述了离子火箭发动机羽流内束离子、中性推进剂原子、交换电荷（CEX）离子和电子等主要成分与航天器相互作用的过程及机理。分析表明，离子推力器出口处的中性推进剂原子与高速束离子流碰撞后产生的CEX离子Xe^＋，以及带电离子轰击推力器组件特别是加速极所产生的金属CEX离子，是造成离子火箭发动机羽流污染的主要成分。在此基础上提出了若干防污染措施。     

Relative ion Fe,C and O abundances in quiet time particle fluxes in the 23 SC

Using ACE and SOHO data the origin of quiet-time low-energy particle fluxes at 1 AU is studied in the 23rd solar cycle. One of the selection criteria of quiet-time periods is to demand that H/He < 10 provided that periods with noticeable contribution of remnants of gradual events have been excluded from consideration. Our results suggest different origin of 0.03–3 MeV/nucleon particles – different seed populations accelerated and different acceleration processes. During the ascending, maximum and descending phases of solar activity quiet-time ions consist of coronal particles accelerated to suprathermal energies in about a half of the quiet periods, the rest of quiet-time fluxes originates from particle acceleration in processes similar to those in small impulsive solar flares rich in Fe. At solar minimum the bulk solar wind particles serve as seed population.     

Modeling PSBL high speed ion beams observed by Cluster and Double Star

On October 8, 2004, the Cluster and Double Star spacecraft crossed the near-Earth (12–19 R_E) magnetotail neutral sheet during the recovery phase of a small, isolated substorm. Although they were separated in distance by ∼7 R_E and in time by ∼30 min, both Cluster and Double Star observed steady, but highly structured Earthward moving >1000 km/s high speed H⁺ beams in the PSBL. This paper utilizes a global magnetohydrodynamic (MHD) simulation driven by Wind spacecraft solar wind input to model the large-scale structure of the PSBL and large-scale kinetic (LSK) particle tracing calculations to investigate the similarities and differences in the properties of the observed beams. This study finds that the large-scale shape of the PSBL is determined by the MHD configuration. On smaller scales, the LSK calculations, in good qualitative agreement with both Cluster and Double Star observations, demonstrated that the PSBL is highly structured in both time and space, on time intervals of less than 2 min, and spatial distances of the order of 0.2–0.5 R_E. This picture of the PSBL is different from the ordered and structured region previously reported in observations.     

基于离子电流的爆震波压力非线性模型

为了实现爆震波压力的软测量,依据碳氢焰离子形成原理及爆震波高速传播的特点,在分析爆震波离子形成机理的基础上,根据爆震波离子电流与压力信号的相似性,提出基于离子电流的爆震波压力非线性模型建模思路。采用RBF网络建立爆震波非线性模型,并给出网络结构、样本选取原则和预处理方法。开展了单次脉冲爆震试验,利用试验数据建立该压力非线性模型,并通过试验数据和模型输出的对比校核模型的有效性和准确性。     

Constant thrust collision avoidance maneuver under thruster failure

In this paper, the collision avoidance maneuver under the chaser’s thruster failure in radial direction is investigated. First, based on the vision measurement, the relative position parameters of the target spacecraft are obtained and the target maneuvre positions are calculated through the isochronous interpolation method. Then, by using coupling effects, the thrusters working time intervals can be computed by the time series analysis method. The perturbations and fuel consumptions are addressed during the computation of the thrusters working time intervals. Next, the switching control law under constant thrust is designed for active collision avoidance maneuvres along a specified trajectory.     

霍尔电推进离子能量后加载设计及工作特性

典型的全电推进通信卫星通常设计使用寿命约为15年,对霍尔电推力器的使用寿命要求达到了104h量级,因此,长寿命设计技术是影响其能否工程应用的关键技术.简要调研了国内外霍尔推力器延寿技术的发展,分析得到壁面及磁极腐蚀程度是影响推力器寿命的核心物理过程.通过分析推力器放电过程离子加速场的建立过程,提出一种具有离子能量后加载...     

离子推力器小功率正高压屏栅电源研究

为了设计一种适用于小功率离子推力器的小功率正高压屏栅电源,本文提出了一种前级降压斩波电路后级全桥LLC谐振及全波倍压整流的两级式拓扑结构。在该主电路的基础上,设计了控制电路,并开展了试验研究。试验结果表明：设计的正高压屏栅电源在输入电压42 V、输出负载12.52 kΩ时,输出电压和输出功率分别为1050 V、88 W,且输出电压误差范围控制在2%以内,屏栅电源效率为90.44%。对于输出正负极高压短路、瞬时加减载具有自恢复功能。研究证明了该两级式拓扑结构的可行性,从而提供了一种小功率正高压屏栅电源的设计方法,对小功率离子推力器的发展具有推动作用。