基于单机寿命管理的飞机维修方案调整

单机寿命管理可以对单架飞机疲劳损伤进行定期的计算分析,确定飞机的当量飞行小时数和剩余寿命.按照单机实际损伤,对飞机检查、大修、退役时间及修理方案的适当调整,可有效的保证飞机使用安全,减少维修成本,最大限度的发挥飞机的使用潜力.     

翼型动态失速影响因素及流动控制研究进展

深入认识翼型动态失速，结合有效流动控制手段，对解决直升机、风力机桨叶等动态失速引起的高阻力、大低头力矩等气动问题具有重要意义。本文首先介绍了翼型动态失速的流场特点和危害，进而分析了缩减频率、雷诺数、马赫数以及翼型型面等参数对动态失速的影响，并在此基础上总结了常见的动态失速流动控制方法及其研究进展。等离子体气动激励易于产生快速、可控的宽频带气动激励，在动态失速控制领域具有潜力，本文着重介绍了等离子体气动激励动态失速控制的概念和流动控制原理，总结了近来年等离子体激励在翼型动态失速控制上的进展。     

倾斜射流撞壁实验研究及液膜几何参数建模

倾斜射流撞壁在液体火箭发动机液膜冷却、射流撞壁雾化等领域具有广泛的应用。为了研究倾斜射流撞击壁面后形成的液膜的关键特征，开展单股圆柱射流撞击壁面的实验研究。从实验中研究各射流参数对液膜外形的影响规律，继而开展理论建模，获取液膜外形的关键几何参数表达式。实验研究发现随着射流倾角增大，液膜长度减小而宽度增大，随着射流孔径和射流速度增大液膜长度和宽度均增大这一定性规律。理论分析得到了液膜最大宽度位置与液膜对称面的夹角近似等于射流倾角α，液膜的长宽比近似等于1+cot α。通过进一步分析得到液膜宽度、最大宽度距撞击点的距离、液膜长度这几个液膜关键参数的表达式。建立的液膜几何参数表达式预测结果与实验结果的误差均在20%以内。     

谐振式陀螺全角模式误差来源与接口技术

全角模式是谐振式陀螺的新型接口技术，具有直接测量角度、动态范围大的优点，但其对陀螺元器件对称性要求极高的缺点限制了它的实际应用。首先，从谐振式陀螺全角模式的原理出发，讨论了各种不理想因素对全角模式运行造成的问题。然后，从器件设计和控制系统两方面出发，讨论了可行的技术路线。最后，通过数值仿真的方法证明了理论分析的正确性，并给出了谐振式陀螺的选型和控制系统的建议。     

VLBI observations to the APOD satellite

The APOD (Atmospheric density detection and Precise Orbit Determination) is the first LEO (Low Earth Orbit) satellite in orbit co-located with a dual-frequency GNSS (GPS/BD) receiver, an SLR reflector, and a VLBI X/S dual band beacon. From the overlap statistics between consecutive solution arcs and the independent validation by SLR measurements, the orbit position deviation was below 10?cm before the on-board GNSS receiver got partially operational. In this paper, the focus is on the VLBI observations to the LEO satellite from multiple geodetic VLBI radio telescopes, since this is the first implementation of a dedicated VLBI transmitter in low Earth orbit. The practical problems of tracking a fast moving spacecraft with current VLBI ground infrastructure were solved and strong interferometric fringes were obtained by cross-correlation of APOD carrier and DOR (Differential One-way Ranging) signals. The precision in X-band time delay derived from 0.1?s integration time of the correlator output is on the level of 0.1?ns. The APOD observations demonstrate encouraging prospects of co-location of multiple space geodetic techniques in space, as a first prototype.     

Satellite ocean colour algorithm for Prochlorococcus, Synechococcus, and picoeukaryotes concentration retrieval in the South China Sea

An algorithm for retrieval of surface waters cell concentrations (in cell/ml) for three picophytoplankton components, Prochlorococcus (Pro), Synechococcus (Syn), and picoeukaryotes (Peuk) in the South China Sea (SCS), from ocean colour satellite data was developed and tested. Level 3 merged multisensor Ocean Colour Climate Change Initiative satellite data is used. Training is performed using in situ data on abundances of the three phytoplankton components. Several predictors derived from satellite reflectance data were tested. The regression form that assures the highest accuracy of the algorithm was chosen based on cross-validation (CV). According to the CV on test data subset, the algorithm performance is characterized by the r value 0.89, 0.72, and 0.73 and MAPD 38, 71 and 51% for Peuk, Pro, and Syn respectively. This is one of the few studies aimed at the Peuk, Pro, and Syn distribution research in the northern SCS using ocean colour satellite data. This is the only research providing algorithm with accuracy estimates of the Peuk, Pro, and Syn concentrations retrieval from the ocean colour data. Analysis of the developed algorithm allows us to conclude that both mechanisms (specific spectral features caused by pigments composition and spectrum features sensitive to general primary productivity, e.g. band ratios in 443–510?nm range and spectrum absolute values) are important for getting accurate information on the picophytoplankton composition.     

非线性媒质无源交调电平预测

无源互调(PIM)作为地面基站天线、卫星天线系统中一种重要的干扰因数,在PIM问题的研究中,功率电平的预测是一个难点。文章对两种预测方法进行了深入的比较研究,建立了数学模型,并通过计算机仿真获得了在不同输出测量误差及相同输入工作电压情况下两种方案的3、5、7阶PIM的预测误差;通过与相关参考文献中实际测量值的比较分析,探讨了这两种预测方案的合理性、有效性。     

星座导航与控制分布式仿真系统设计

基于HLA/RTI和STK,设计了卫星星座导航与控制分布式仿真系统.仿真系统中每颗卫星均由单独的计算机模拟,可真实地反映星座的运行情况,更好地模拟星间链路;卫星轨道精确外推、星间链路优化、基于基准星和星间距离测量的分布式导航以及基于相对轨道根数的星座绝对站位保持等关键技术也融入到系统中;仿真系统还具有直观的二维、三维场景和曲线动态可视化演示功能.结合具体的WaIker星座实例,仿真星座稳定运行180天,系统运行结果表明所设计的仿真系统及采用的关键技术能够满足仿真与评估的需求.另外,在一定程度上该仿真系统还支持其它卫星星座的仿真与评估.     

基于相位重构的相位编码信号脉内特征分析

基于希尔伯特变换,提出了一种相位编码信号相位无模糊重构的脉内特征分析方法。该方法一方面利用魏格纳-威利变换对信号进行降噪处理,改善了在低信噪比下相位编码信号脉内特征识别和提取能力;另一方面对重构相位进行多阶差分处理来提高识别精度。仿真结果验证了该方法的正确性和有效性。