叶片非线性瞬态响应计算方法与参数选择

在计算叶片的岛撞击响应时，为提高计算精度及降低计算成本，需要为待解的非线性动力方程组制定一个合理的求解方案，这包括选择系数矩阵的算法与非线性动力方程组的解法，以及选择主要计算参数，本文介绍了当使用ＡＤＩＮＡ程序计算平板叶片在冲载荷下的非线性瞬态响应时，对计算方法与计算参数的选择，算例说明了时间步长的重要影响作用。     

考虑部件约束的涡扇发动机循环参数分析方法研究

在涡扇发动机初步设计阶段,为了研究部件气动、结构、强度参数对于发动机循环参数求解域的约束,在发动机总体性能稳态计算模型以及尺寸流路计算模型的基础上,利用部件初步设计时采用的Smith图,基于牛顿迭代法构建了一种总体/部件耦合计算方法。在部件主要设计参数的约束边界基础上,采用该方法,能够获取同时满足总体和部件设计要求的循环参数求解域,并进一步获得部件的主要设计参数。使用该方法对第四代双轴混排涡扇发动机EJ200开展了算例验证,获取了部件约束条件下的发动机循环参数求解域,与公布的EJ200数据对比表明,主要部件设计参数误差<4%,表明该方法可以满足工程应用要求。     

透平叶片变切削加工工艺数据库设计与开发

透平叶片是透平机械的核心零件之一,因其复杂的曲面造型和低刚度性,被认为是机械加工中的难题.通过Visual Basic编程语言进行叶片切削工艺数据库开发,在功能上实现面向叶片工艺变切削参数智能推荐、相似工艺实例推理和数控加工工序卡片、程序清单的输出,方便企业用户使用,提高工作效率和准确性..     

难加工材料切削用量可优化区间的限定

针对传统切削用量优化方法在自动化程度较高以及大量使用难加工材料领域时局限,对刀具磨损随切削用量的变化趋势与广义刀具耐用度公式和马卡洛夫最优切削速度公式两种数学模型的符合程度进行比较,分析基于两种数学模型的优化方法的适用性和限制,提出使用磨损指数确定切削用量可优化区间边界条件的方法,分析多项切削用量可优化区域的特点.     

基于快速模糊干扰观测器的UASV再入Terminal滑模控制

针对无人空天飞行器再人大气层过程中气动参数变化剧烈、控制精度要求高的特点，设计了基于快速模糊干扰观测器的Terminal滑模控制方案。通过改进传统模糊干扰观测器的学习律，提出一种快速模糊干扰观测器，增强了其在线逼近干扰及系统不确定的能力。Terminal滑模的有限时间收敛特性提高了系统跟踪速度，同时采用快速模糊干扰观测器消除全部扰动的影响，从而保证了飞行品质。最后，仿真结果表明了快速模糊干扰观测器的优越性及闭环控制方案的有效性。     

CFCC的几种声学参量表征方法比较

化学气相渗透(CVI)制备的CFCC的质量控制非常困难。研究该材料质量的无损检测方法对材料使用及性能表征等都具有重要意义。针对声衰减严重的问题,采用穿透法测量各声学参量,用声速、衰减、非线性等相关参量评价材料的均匀性,同时用金相法进行对比测试。结果表明:声速、衰减、非线性等参量可准确地评价材料均匀性,其中声速评价是最成熟的表征方法。     

飞轮振源特征参数提取方法及其分布特性

为了从飞轮微振动输出中提取飞轮转子的振源信息，提出利用鲁棒回归辨识飞轮在升速过程中各主要阶次的振幅对转速的二次幂系数，并将其作为飞轮的振源幅值特征参数；为探究参数的分布特性，利用Weibull分布拟合多个飞轮在同一阶次的特征参数，并计算出特定概率点的分位数。振源特征参数的分位数既系统地展示了飞轮振源分布情况，亦可作为振源分级判据。将该方法成功应用于50 Nms飞轮的振源特征参数分布研究中，为该型飞轮的超静性能筛选和设计改进提供了判定准则和参考依据。     

Long-term changes in indices of geomagnetic activity at the auroral station Sodankylä

Here we compare the traditional analog measure of geomagnetic activity, Ak, with the more recent digital indices of IHV and Ah based on hourly mean data, and their derivatives at the auroral station Sodankylä. By this selection of indices we study the effects of (i) analog vs. digital technique, and (ii) full local-time vs. local night-time coverage on quantifying local geomagnetic activity. We find that all other indices are stronger than Ak during the low-activity cycles 15–16 suggesting an excess of very low scalings in Ak at this time. The full-day indices consistently depict stronger correlation with the interplanetary magnetic field strength, while the night-time indices have higher correlation with solar wind speed. The Ak index correlates better with the digital indices of full-day coverage than with any night-time index. However, Ak depicts somewhat higher activity levels than the digital full-day indices in the declining phase of the solar cycle, indicating that, due to their different sampling rates, the latter indices are less sensitive to high-frequency variations driven by the Alfvén waves in high-speed streams. On the other hand, the night-time indices have an even stronger response to solar wind speed than Ak. The results strongly indicate that at auroral latitudes, geomagnetic indices with different local time coverage reflect different current systems, which, by an appropriate choice of indices, allows studying the century-scale dynamics of these currents separately.     

Motion prediction of a non-cooperative space target

Capturing a non-cooperative space target is a tremendously challenging research topic. Effective acquisition of motion information of the space target is the premise to realize target capture. In this paper, motion prediction of a free-floating non-cooperative target in space is studied and a motion prediction algorithm is proposed. In order to predict the motion of the free-floating non-cooperative target, dynamic parameters of the target must be firstly identified (estimated), such as inertia, angular momentum and kinetic energy and so on; then the predicted motion of the target can be acquired by substituting these identified parameters into the Euler’s equations of the target. Accurate prediction needs precise identification. This paper presents an effective method to identify these dynamic parameters of a free-floating non-cooperative target. This method is based on two steps, (1) the rough estimation of the parameters is computed using the motion observation data to the target, and (2) the best estimation of the parameters is found by an optimization method. In the optimization problem, the objective function is based on the difference between the observed and the predicted motion, and the interior-point method (IPM) is chosen as the optimization algorithm, which starts at the rough estimate obtained in the first step and finds a global minimum to the objective function with the guidance of objective function’s gradient. So the speed of IPM searching for the global minimum is fast, and an accurate identification can be obtained in time. The numerical results show that the proposed motion prediction algorithm is able to predict the motion of the target.     

Simultaneous observations of some unusual whistlers and VLF hiss emission at a low L-value (L = 1.17)

The purpose of this paper is to describe some unusual whistlers (doublets and triplets) and VLF hiss emission recorded simultaneously on February 18, 1998 during nighttime at a low latitude Indian ground station Jammu (geomag. lat., 22° 26′ N; L = 1.17), and to make some discussions about their origin. The detailed structures of the observed VLF hiss emission clearly show that these emissions confined to a narrow continuous frequency band. Some times the frequency of hiss band oscillates and subsequently touches the upper edge of the first whistler component of the doublet. Detailed structures of the dynamic spectra of whistler and VLF hiss emission are briefly presented. From the dispersion analysis of the whistler doublets and triplets, it is found that the individual whistlers of the doublets and triplets simultaneously observed on the same day are one-hop whistlers having propagation path along higher and closely spaced L-values. Our result also shows that VLF hiss has been generated in the equatorial region of higher L-values. Generation and propagation mechanisms are briefly discussed.