叶片前缘仿形涡流检测仿真与试验设计

仿形涡流检测技术因其耦合性好可有效抑制检测过程晃动而特别适合对大曲率叶片前缘快速检测。针对涡轮叶片前缘仿形涡流检测建立前缘及仿形线圈有限元模型,运用有限元方法分析叶片前缘凹坑、长裂纹、边沿凹坑3种典型缺陷在内外两种激励、不同内径线圈、不同频率等模式下的检测信号特征。仿真结果表明：大曲率前缘实施仿形涡流检测,检测区域可有效覆盖整个前缘区域,检测频率越高,检测灵敏度越高。双线圈检测模式下,外激励内接收比内激励外接收灵敏高,当内检测线圈尺寸大于缺陷的尺度时,内接收线圈内径越小,其相对灵敏度越高。结合仿真结论,制作前缘缺陷试块,采用锁相放大及图形化编程技术,设计前缘仿形涡流检测系统,试验结果表明,仿形线圈可有效检出前缘典型缺陷,检测幅值相位输出结果与仿真结论相似。研究成果可用于指导大曲率叶片前缘的工程实践检测。     

大型民用客机管制与监视系统验证与测试平台的构建

目的在于研发大型民用客机航路管制与监视系统验证与测试平台,以实现机地数据通信系统环境下的航路管制与监视信息的数据地面接收和处理;同时,依照现有的空管航路管制与监视功能的国际标准和相关区域的运行要求,实现地面管制系统向机载系统的数据发布。该项研究成果能对口飞机机载数据链相关的ATC(Air Traffic Control空中交通管制)功能和部分监视功能ADS-C(Automatic Dependent Surveillance-Contract合同式自动相关监视)、ADS-B(Automatic Dependent Surveillance-Broadcast广播式自动相关监视),提供对应的地面收发端,监控机载系统数据状态。该成果可以配合飞机研发过程中的试验和排故,并为适航验证工作提供有力的准备和支持。     

用于微小卫星自主导航控制系统地面仿真的磁强计数学模型

对基于磁强计自主导航微小卫星控制系统地面仿真的磁强计数学模型建立进行了研究。给出了地磁场理论数据的生成模型及磁强计的测量模型,并据此建立了磁强计测量数据生成的数学模型。对低轨圆轨道微小卫星的仿真计算结果表明：由该磁强计数学模型获得的磁场强度测量值与文献中真实磁强计测量数据差异很小,验证了模型的有效性和准确性。     

复合材料飞机的电流回路接地技术研究

随着复合材料在飞机中所占比重的增大,诸多电磁兼容设计的问题也日趋凸显。本文分析了飞机复合材料结构对电流回路接地的影响,介绍了复合材料结构内接地网的应用及研究现状,提出了接地网设计及优化时的设计目标与方法。     

电流积分器对I/F转换性能的影响分析

本文介绍了带分流结构的电流/频率转换电路和电流积分器的工作原理,推导了电流积分器的误差,并分析了运放的几个关键参数对l/F电路性能的影响.通过理论推导和实验对比,得出了I/F电路设计时电流积分器电路选择运算放大器的参考依据,并对带分流结构的I/F电路作出了改进.     

Magnetosphere response to the 2005 and 2006 extreme solar events as observed by the Cluster and Double Star spacecraft

The four identical Cluster spacecraft, launched in 2000, orbit the Earth in a tetrahedral configuration and on a highly eccentric polar orbit (4–19.6 R_E). This allows the crossing of critical layers that develop as a result of the interaction between the solar wind and the Earth’s magnetosphere. Since 2004 the Chinese Double Star TC-1 and TC-2 spacecraft, whose payload comprise also backup models of instruments developed by European scientists for Cluster, provided two additional points of measurement, on a larger scale: the Cluster and Double Star orbits are such that the spacecraft are almost in the same meridian, allowing conjugate studies. The Cluster and Double Star observations during the 2005 and 2006 extreme solar events are presented, showing uncommon plasma parameters values in the near-Earth solar wind and in the magnetosheath. These include solar wind velocities up to ∼900 km s⁻¹ during an ICME shock arrival, accompanied by a sudden increase in the density by a factor of ∼5 and followed by an enrichment in He⁺⁺ in the secondary front of the ICME. In the magnetosheath ion density values as high as 130 cm⁻³ were observed, and the plasma flow velocity there reached values even higher than the typical solar wind velocity. These resulted in unusual dayside magnetosphere compression, detection of penetrating high-energy particles in the magnetotail, and ring current development following several successive injections of energetic particles in the inner magnetosphere, which “washed out” the previously formed nose-like ion structures.     

Tomographic reconstruction of the ionospheric electron density as a function of space and time

Electron density distribution is the major determining parameter of the ionosphere. Computerized Ionospheric Tomography (CIT) is a method to reconstruct ionospheric electron density image by computing Total Electron Content (TEC) values from the recorded Global Positioning Satellite System (GPS) signals. Due to the multi-scale variability of the ionosphere and inherent biases and errors in the computation of TEC, CIT constitutes an underdetermined ill-posed inverse problem. In this study, a novel Singular Value Decomposition (SVD) based CIT reconstruction technique is proposed for the imaging of electron density in both space (latitude, longitude, altitude) and time. The underlying model is obtained from International Reference Ionosphere (IRI) and the necessary measurements are obtained from earth based and satellite based GPS recordings. Based on the IRI-2007 model, a basis is formed by SVD for the required location and the time of interest. Selecting the first few basis vectors corresponding to the most significant singular values, the 3-D CIT is formulated as a weighted least squares estimation problem of the basis coefficients. By providing significant regularization to the tomographic inversion problem with limited projections, the proposed technique provides robust and reliable 3-D reconstructions of ionospheric electron density.     

开闭环PD型快速迭代学习控制方法及其在直流电动机中的应用

针对一类非线性系统的学习控制问题,提出了一种开闭环PD型快速迭代学习控制方法。此学习控制方法利用了系统当前的跟踪误差信号和前次迭代控制的跟踪误差信号,以及它们的微分信号,同时采用可调比例系数,根据系统误差的变化及时地调节比例系数,从而使目标的跟踪能力得到提高。通过分析给出了此快速迭代学习算法收敛的条件,直流电动机的仿真应用说明了此学习控制方法对于非线性系统具有较强的有效性和较好的可行性。     

环路热管地面实验平台的热设计

文章旨在建立环路热管的地面实验平台,模拟环路热管在太空轨道运行的热环境。首先建立了地面实验舱的物理模型,对其如何实现在地面模拟太空中该环路热管的热环境进行了热分析计算,其次确定了满足环路热管轨道运行最冷工况和最热工况下的实验舱的壁面温度,最后对实现该轨道环境所需要的壁面绝热材料、制冷剂、制冷设备进行了选择,初步完成了实验平台的热设计。计算结果表明,在同时考虑舱内对流和辐射换热的条件下,要实现空间热边界条件,实验舱内舱的壁温要保证在-62.1~-10.9℃之间变化。     

限制励磁方法在无刷交流发电机数字电压调节器中的应用

分析了限制励磁电流功能对无刷交流发电机加载过渡过程的影响,得到了设置励磁电流限制值的方法。采用了曲线拟合的方法对变速无刷交流发电机的励磁电流限制值进行了设置,而且拟合公式是与理论推导相一致的。按照本文的励磁电流限制值拟合方法可以保证无刷交流发电机在整个转速范围内都有良好的加载动态性能。