航天器分子污染返回流计算方法

随着航天器对长寿命、高性能、高可靠要求的不断提高,污染逐渐成为影响任务成功的重要因素之一,数值模拟是评估分子污染的主要手段之一。文章对返回流计算方法进行了总结,详细介绍不同方法的理论基础、计算细节,对每种方法的优缺点、适用性等进行了比较分析。     

Assessing the Risk of Orbital Debris Impact

A Space Debris Impact Risk Analysis Tool (SDIRAT) was developed and implemented to assess the orbital debris impact risk on a specified target in Earth orbit, in terms of flux, relative velocity, impact velocity, direction of the incoming particles, debris mass and diameter. Based on a deterministic approach, SDIRAT uses a realistic orbital debris population where each representative particle is identified by its rectangular coordinates (position and velocity) at a reference epoch. Using this information, some geometrical algorithms were developed and implemented to evaluate the contribution of each particle to the incoming flux. The position of the particle with respect to a specified target drives the selection criteria to reject, or select, it as a possible projectile. On the other hand, the relative velocity vector can be used to estimate the impact direction of the incoming flux. SDIRAT was conceived as a general tool for a variety of scenarios, such as low circular and elliptical orbits, up to the geosynchronous ring. This paper presents some examples of possible applications, including the computation of the incoming debris flux on SAX (low Earth orbit), SIRIO (geosynchronous orbit) and the IRIS upper stage (elliptical orbit). Other applications assess the impact risk for the Soviet Radar Ocean Reconnaissance Satellites Cosmos 1900 and Cosmos 1932.     

一种实现干扰补偿的控制策略

提出了一种实现系统干扰补偿的控制策略。针对无界斜坡干扰情况，通过构造一个系统输出并为其设计观测器，实现了对状态和干扰的同时估计，并将干扰的估计量引入到控制律当中，从而实现系统对干扰的补偿控制。仿真结果验证了这一方法的有效性。     

基于鲁棒故障观测器的非线性离散系统容错控制设计

针对存在执行器故障以及未知干扰的非线性离散系统,提出了一种鲁棒故障估计与容错控制方法。首先在未知系统干扰作用下,设计鲁棒故障观测器实现系统状态和执行器故障的同步估计;然后根据鲁棒故障观测器得到的系统状态估计和故障估计信息设计容错控制器,进行状态反馈容错控制,同时基于D稳定与H_∞控制理论对鲁棒故障观测器和容错控制器进行设计,实现了多约束条件下的故障估计与容错控制;最后用飞行控制系统模型验证了所提方法的有效性。     

A new parameter to define interplanetary coronal mass ejections

The interplanetary manifestations of coronal mass ejections, ICMEs, have many signatures in the solar wind but none of these signatures in the velocity, density, temperature, magnetic field, plasma composition or energetic particles uniquely and unambiguously identifies the occurrence of an ICME. Different investigators identify different events when confronted with the same data. Herein, we present a single physical parameter that combines information from multiple plasma components and that holds the promise of defining a beginning and an end of the region of influence ICME and an indication of the location of the encounter with the ICME relative to its central meridian. This parameter is the total plasma pressure perpendicular to the magnetic field, consisting of the sum of the magnetic pressure and plasma kinetic or thermal pressure. It provides a vehicle for classifying the nature of the ICME encounter and, in many cases, provides an unambiguous start and stop time of the event. However, it does not provide a start and stop time for any embedded flux rope. This identification depends on examination of the magnetic field.     

Force-free magnetic field in a cylindrical flux rope without a constant alpha

It is generally assumed that magnetic fields inside interplanetary magnetic clouds and flux ropes in the solar photosphere are force-free. In order to model such fields, the solution of rot B = B is commonly used where  = const. But comparisons of this solutions with observations show significant difference. To treat this problem,we examine the solutions with .     

基于未知输入观测器的涡扇发动机直接推力控制

针对某型涡扇发动机,进行直接推力控制回路设计方法研究.基于未知输入观测器(UIO)原理建立了涡扇发动机机载模型和推力估计器,UIO通过解耦外界干扰实现了全飞行包线推力的准确估计;提出了直接推力闭环反馈控制的双回路结构设计方案,内环转速控制,外环推力控制,有利于实现各回路控制参数的独立设计.仿真验证结果表明:基于UIO的模型基涡扇发动机直接推力控制具有良好的控制稳定性和抗干扰性能,对于发动机不同工作点直接推力控制,推力控制误差不超过0.1%,转速控制偏差不超过0.2%.      

航天器再入大气层热力分析

以OREX（orbital reentry experiment vehicle）的飞行试验数据和相关的CFD数值模拟结果为基础,采用传热理论及相关公式,分析计算了OREX再入大气层过程中的轨迹,驻点处热流密度非平衡假设和平衡假设下的换热问题.所计算的轨迹、热流密度非平衡假设下计算的驻点温度和热流密度值同试验数据及相关的CFD数值结果取得了很好的一致,相应的计算方法可作为航天器驻点热力分析的通式.然而在平衡假设条件下,尽管计算所得到的驻点热流密度与之前的CFD数值结果差别不大,但这种情况下计算得到的温度与试验数据不符,这应归结于计算的热流密度结果对驻点处温度变化的不敏感.比较非平衡假设和平衡假设下的换热计算结果表明,对于航天器再入过程中的热力探讨不能仅仅满足于热流密度分析,对温度的考察或许更重要.      

Ground experimental investigations into an ejected spray cooling system for space closed-loop application

Spray cooling has proved its superior heat transfer performance in removing high heat flux for ground applications.However,the dissipation of vapor–liquid mixture from the heat surface and the closed-loop circulation of the coolant are two challenges in reduced or zero gravity space environments.In this paper,an ejected spray cooling system for space closed-loop application was proposed and the negative pressure in the ejected condenser chamber was applied to sucking the two-phase mixture from the spray chamber.Its ground experimental setup was built and experimental investigations on the smooth circle heat surface with a diameter of 5 mm were conducted with distilled water as the coolant spraying from a nozzle of 0.51 mm orifice diameter at the inlet temperatures of 69.2 °C and 78.2 °C under the conditions of heat flux ranging from 69.76 W/cm~2 to 311.45 W/cm~2,volume flow through the spray nozzle varying from 11.22 L/h to 15.76 L/h.Work performance of the spray nozzle and heat transfer performance of the spray cooling system were analyzed;results show that this ejected spray cooling system has a good heat transfer performance and provides valid foundation for space closed-loop application in the near future.