某型蒸发式稳定器气动及燃烧特性研究

为解决亚燃冲压发动机在高速低温来流条件下的可靠点火、火焰稳定和高效燃烧问题,对某型蒸发式火焰稳定器分别进行了冷态流场和燃烧流场的数值研究,并与常规V型火焰稳定器进行了对比分析。研究结果表明:在给定范围内,蒸发式稳定器随来流速度的增大,总压恢复系数和停留时间明显减小,回流区长度、回流率和燃烧效率变化不大;与相同槽宽的常规V型火焰稳定器相比,回流率明显减小,总压恢复系数、回流区长度和停留时间略有减小。蒸发式稳定器后部形成明显的回流区,且基本上不受外部主流流动的干扰,通过单独控制稳定器局部供油,可以使稳定器在最佳油气比下工作,有利于在高速来流条件下可靠工作。     

基于高效数值方法的一种高超声速飞行器外形气动力/热综合优化设计研究

基于所发展的高效气动力/热快速预测方法,建立了适用于高超声速飞行器的综合考虑气动力与气动热特性的外形优化设计技术,并在一种高超声速飞行器外形设计中应用,通过优化设计改变了初始外形纵向静不稳定特性,优化后外形实现了纵向静稳定、大攻角自配平和非驻点表面最大热流下降的设计目标。所发展的方法为适应气动外形快速选型设计需求提供了有效的途径。     

Accuracy enhancement of the spherical actuator with a two-level geometric calibration method

This paper presents a two-level geometric calibration method for the permanent magnet （PM） spherical actuator to improve its motion control accuracy. The proposed actuator is com- posed of a stator with circumferential coils and a rotor with multiple PM poles. Due to the assembly and fabrication errors, the real geometric parameters of the actuator will deviate from their design values. Hence, the identification of such errors is critical for the motion control tasks. A two-level geometric calibration approach is proposed to identify such errors. In the first level, the calibration model is formulated based on the differential form of the kinematic equation, which is to identify the geometric errors in the spherical joint. In the second level, the calibration model is formulated based on the differential form of torque formula, which is to calibrate the geometric parameters of the magnetization axes of PM poles and coils axes. To demonstrate the robustness and availability of the calibration algorithm, simulations are conducted. The results have shown that the proposed two-level calibration method can effectively compensate the geometric parameter errors and improve the positioning accuracy of the spherical actuator.     

大型回流边界层风洞的气动与结构设计

大型边界层风洞是开展风工程研究的必备装备。以浙江大学ZD-1边界层风洞的研制为背景,详细介绍了大型回流边界层风洞气动设计和立式结构设计中的关键问题,在风洞气动设计时采用了收缩比为4∶1的单回路单试验段气动轮廓,在试验段中设置了0．22°的当量扩散角,对拐角导流片外形作了特殊处理,并采用钢结构与混凝土结构相结合的立式结构。流场校验结果表明,大型回流边界层风洞的气动与结构设计能满足设计要求,某些指标甚至达到航空风洞的标准,在试验段中设置扩散角有利于降低轴向静压梯度,立式结构设计对提高试验段气流的水平均匀性有一定的作用,可为今后类似风洞的研制提供参考。     

一种折叠弹翼悬挂物的分离轨迹试验技术

提出了一种新的折叠弹翼悬挂物机弹分离轨迹试验技术,重点解决了在机弹分离过程中折叠弹翼动态展开时悬挂物的气动力获取问题。研究表明,提出的试验技术通过将悬挂物气动力修正方法引入到悬挂物分离安全性研究当中,准确地得到悬挂物的分离特性,解决了折叠弹翼悬挂物分离轨迹风洞试验技术瓶颈,为折叠弹翼悬挂物的投放分离安全性提供一套工程实用的解决方案。     

主/从动式组合旋翼悬停状态气动特性分析

针对传统直升机构型中主旋翼旋转时产生的扭矩需要尾翼或是反向旋转的共轴旋翼加以抵消,从而造成能量浪费的问题,以将主旋翼旋转时产生的扭矩转化为升力为出发点,提出了一种主旋翼带动下方无动力旋翼旋转的主/从动式组合旋翼气动布局构型。通过动量叶素理论以及CFD数值模拟中的多重参考系法,对主/从动式组合旋翼悬停状态的气动特性进行了初步分析,结果表明,此构型中的下方从动旋翼利用上方主动旋翼的扭矩产生了额外10%的升力,同时下方从动旋翼在上方主动旋翼引流的有利干扰下升力系数提高了35%。     

一种基于机动辨识预测的空空导弹导引律

现有的空空导弹导引头在有噪声和干扰的环境下获得目标精确信息存在时间延迟,且新一代目标的机动能力更强,不对导弹加以补偿会造成较大脱靶量,所以需对目标状态有效预测。针对新一代目标规避空空导弹常用的大机动模式,为满足新一代空空导弹发展需求,设计了一种新型复合导引律。从目标自身出发,研究高机动目标规避导弹采用的典型机动形式,对机动轨迹进行离线建模,构建具有扩展能力的目标机动模型库。设计自适应滤波器对测量噪声进行降噪。同时,利用模型库设计了机动辨识预测器,对目标实际机动进行在线辨识。基于在线辨识的结果对目标机动进行预测,并对时间延迟进行补偿和修正,实现对高机动目标的精确打击。仿真结果表明:该方法对不同类型的机动目标均有较高的预测精度和命中精度。     

航天器软件风险集成管理方法

为确保航天器软件产品功能、性能符合任务需求,安全、可靠地完成飞行任务,需要对其进行风险管理。文章首先介绍了软件风险管理理论研究现状;然后结合航天器软件强实时性、高可靠性和安全性、维护困难等问题,提出了基于系统集成思想的软件风险控制方法;最后以某航天器为例介绍了该套方法的应用成果。研究结果可为识别航天器软件风险,提高软件产品质量提供参考。     

Stability analysis of an aeroelastic system with friction

In this paper, harmonic balance method, exact formulation and numerical simulation method are adopted to study the effects of different friction stiffness on the stability of 1.5 degrees of freedom aeroelastic system. On this basis, the expressions of input energy and dissipated energy are deduced, and the energy method is used to reveal the mechanisms of the stable boundary and unstable boundary existing in the system and the effects of different friction stiffness on the stability of the system. Studies have shown that the stability region and the critical aerodynamic damping ratio of the system rise with the increase of the friction stiffness, while the friction stiffness has little effect on the stability boundary. In the analysis of the stability of system, the results of harmonic balance method, exact formulation and Newmark of numerical simulation method are in good agreement. Compared with exact formulation and numerical simulation method, the concept and conclusion of harmonic balance method are simple in the system stability analysis.     

Solar cycle and latitude dependence of high-beta suprathermal plasma conditions in interplanetary space between 1.3 and 5.4 AU

The analysis of energetic particles and magnetic field measurements from the Ulysses spacecraft has shown that in a series of events, the energy density contained in the suprathermal tail particle distribution is comparable to or larger than that of the magnetic field, creating conditions of high-beta plasma. In this work we analyze periods of high-beta suprathermal plasma occurrences (β_ep > 1) in interplanetary space, using the ratio (β_ep) of the energetic particle (20 keV to ∼5 MeV) and magnetic field energy densities from measurements covering the entire Ulysses mission lifetime (1990–2009) in order to reveal new or to reconfirm some recently defined interesting characteristics. The main key-results of the work are summarized as follows: (i) we verify that high-beta events are detected within well identified regions corresponding mainly to the vicinity of shock surfaces and magnetic structures, and associated with energetic particle intensity enhancements due to (a) reacceleration at shock-fronts and (b) unusually large magnetic field depressions. (ii) We define three considerable features for the high-beta events, concentrated on the next points: (a) there is an appreciable solar-activity influence on the high-beta events, during the maximum and middle solar-cycle phase, (b) the annual peak magnitude and the number of occurrences of high events are well correlated with the sunspot number, (c) the high-beta suprathermal plasma events present a spatial distribution in heliographic latitudes (HL) up to ∼±80°, and a specific important concentration on the low (−25° ? HL < −6°, 6° < HL ? 25°) and median (−45° ? HL < −25°, 25° < HL ? 45°) latitudes. We also reconfirm by a statistical analysis the results of Marhavilas and Sarris (2011), that the high-beta suprathermal plasma (β_ep > 1) events are characterized by a very large parameter β_ep (up to 1732.5), a great total duration (406 days) and a large percentage of the Ulysses-mission lifetime (which is equal to 6.34% of the total duration with usable measurements, and 11.3% of the duration in presence of suprathermal particles events).