计入畸变修正的旋翼尾迹前飞状态稳定性分析

现有的旋翼尾迹稳定性分析方法在涡线过近处会得出不现实的过大发散率结果,因而存在一定的局限性。为了消除这种前飞状态下尾迹高度畸变对其稳定性分析所造成的不合理干扰,提出了一个旋翼尾迹在正弦扰动下,结合涡线畸变修正的线性化稳定性分析方法。在该方法中,将尾迹涡线离散为一系列涡元,并对其端点施加沿尾迹涡线分布的正弦扰动;考虑了桨尖涡的自诱导、互诱导以及与桨叶的干扰作用,并创新地引入在伪涡核对稳定性分析中,因尾迹高度畸变产生的不合理干扰而进行的修正。以H-34型直升机旋翼模型为例,在前飞状态下,重点计算分析了尾迹向后飘移、涡核大小和前飞速度等对旋翼尾迹稳定性的影响。研究结果表明:引入伪涡核模型可以有效地修正在涡线过近处所产生的不现实稳定性分析结果;前飞速度、涡核大小等因素会在一定条件下有限地影响尾迹的不稳定性,但都不改变前飞状态旋翼尾迹的本质不稳定性。     

航天器红外成像检漏方法研究

红外成像检漏技术以其独特的优势在航天器检漏领域有良好的发展应用前景。文章分析了红外光谱吸收成像检漏方法、红外光声成像检漏方法及红外热成像检漏方法的基本原理与应用实例,分析研究了这几种不同红外检漏方法的特点及在航天器检漏中的应用范围,并为实施航天器红外检漏方法提供了研究思路与途径。     

Research and development version of computer-aided system of aircraft and rocket-space equipment vibration tests

In this paper, a research and development version of the computer-aided system of mass tensometry (SMT) for conduction of aircraft and rocket-space equipment vibration tests is considered. A technique of the system design and development that combines the advantages of the system and process approaches when using the modern element base around the high-performance integral microcircuits is a distinctive feature in this research and development problem solution. We describe the architecture and structure of the advanced computer-aided SMTs and present data on its basic components desigtn. Also determined are the list and functional parameters of ratio-measuring network modules as well as the scheme of their connection to the test object and the local computer network of the enterprise.     

基于非参数假设检验的程序缺陷定位方法

调查了西门子测试集中的程序失败用例的规模和谓词评估偏差的分布.结果表明,中心极限定理的前提和参数假设检验的假设条件无法得到普遍满足.所以,已有的基于参数假设检验的方法存在潜在的问题.针对这一现象,提出了基于非参数假设检验定位程序缺陷的方法.实验结果表明,该方法在非正态分布的样本集上仍具有较好的适用性,且在缺陷定位效率上优于已有的基于程序谓词的缺陷定位技术.同时比较了基于2种常用的非参数假设检验模型的缺陷定位方法的效率.一种方法基于Kolmogorov-Smirnov检验,另一种方法基于Cramér-von-Mises准则.比较结果表明,在西门子测试集上,基于Kolmogorov-Smirnov检验的方法在缺陷定位效率上优于基于Cramér-von-Mises准则的方法.     

环境减灾A、B星星座轨道维持技术与实践

为维持环境减灾A、B星星座的轨道构型,保证CCD相机48h对中国覆盖和对全球重访的特性,满足中国灾害与环境监测以及全球陆地观测的需求,制定了同时考虑地面轨迹和星座相位的轨道维持策略。在减灾和环保业务应用过程中,主要关注星座的重访和覆盖特性,严格的地面轨迹维持意义不大,因而形成了主要考虑星座相位的轨道维持方法。该方法能够减少轨道维持次数,降低操作风险,节省星上燃料,有利于延长卫星寿命。A、B星星座运行3年多,仅通过2次轨道调整就完成了星座轨道维持控制任务。     

基于雨衰环境下的多波束卫星资源分配策略

针对雨衰对高频段的卫星通信造成的不利影响,采用自适应前向纠错编码(FEC,Forward Error Correction)使传输的信息量减少,提出了一种雨衰下的自适应信道分配的策略.该方法是采用调整冗余信道来保障信息信道的传输量以满足系统对误码率的要求,达到可靠和有效地利用有限的卫星信道资源的目的.通过仿真分析了该策略针对不同的频段和降雨情况下对呼叫产生的影响,分析中考虑了话音业务享有比数据业务更高的优先权.仿真结果表明利用冗余信道传输用于纠错的冗余信息可以保证在不产生通信中断的前提下,可以满足系统对信道误码率的要求.     

基于多相滤波的跨信道宽带信号处理技术

首先介绍了实信号的多相滤波信道化体制,讨论了该体制下宽带信号跨信道接收时的信号检测技术以及邻信道虚假信号消除技术。然后详细讨论了各种跨信道宽带信号恢复算法,考虑到可行性和FPGA的硬件可实现性,选用综合滤波器算法进行宽带接收。最后通过MATLAB仿真验证算法的有效性。     

航空发动机密封组件平面度误差检测技术研究

针对航空发动机石墨密封组件结构特点和平面度测量技术要求,提出应用光波干涉法对航空发动机密封件平面度误差实施检测专用装置的设计、测量、平面度判读等。     

Activation of the tail open part during the magnetospheric storm

In each polar cap (PC) we mark out “old PC” observed during quiet time before the event under consideration, and “new PC” that emerges during the substorm framing the old one and expanding the PC total area. Old and new PCs are the areas for the magnetosphere old and new tail lobes, respectively. The new lobe variable magnetic flux Ψ₁ is usually assumed to be active, i.e. it provides the electromagnetic energy flux (Poynting flux) ɛ′ transport from solar wind (SW) into the magnetosphere. The old lobe magnetic flux Ψ₂ is supposed to be passive, i.e. it remains constant during the disturbance and does not participate in the transporting process which would mean the old PC electric field absolute screening from the convection electric field created by the magnetopause reconnection. In fact, screening is observed, but far from absolute. We suggest a model of screening and determine its quantitative characteristics in the selected superstorm. The coefficient of a screening is the β = Ψ₂/Ψ₀₂, where Ψ₀₂ = const is open magnetic flux through the old PC measured prior to the substorm, and Ψ₂ is variable magnetic flux through the same area measured during the substorm. We consider three various regimes of disturbance. In each, the coefficient β decreased during the loading phase and increased at the unloading phase, but the rates and amplitudes of variations exhibited a strong dependence on the regime. We interpreted decrease in β as a result of involving the old PC magnetic flux Ψ₂, which was considered to be constant earlier, in the Poynting flux ɛ′ transport process from solar wind into the magnetosphere. Transport process weakening at the subsequent unloading phase creates increase in β. Estimates showed that coefficient β during each regime and the computed Poynting flux ɛ′ varied manifolds. In general, unlike the existing substorm conception, the new scenario describes an unknown earlier of tail lobe activation process during a substorm growth phase that effectively increases the accumulated tail energy for the expansion and recovery phases.     

用于复杂装备费用驱动因子筛选的灰色凸关联模型

针对复杂装备费用预测中样本少和费用影响因素繁多的问题,分析以往灰色关联度的缺陷,运用改进的灰色凸关联度建立费用影响因素与费用之间的灰色关联模型。依据灰色凸关联度的大小和接近程度筛选费用驱动因子,利用所选择的驱动因子建立多元回归模型。与已有文献中的方法进行对比,结果表明本文方法具有较高的预测精度,说明改进的灰色凸关联度模型能够诊断复杂装备费用的关键影响因素。