非线性调频信号参数估计算法

分析了非线性调频（NLFM）信号参数估计问题，提出了利用二次相位差分使相位降阶，使NLFM信号的参数估计转化为成熟的正弦波频率估计，而NLFM信号参数估计算法从三维搜索简化为三次一维搜索，既减少了计算复杂度，又有利于工程实现；另外从正弦波频率估计问题出发推导出对信号参数α3估计的最佳相关延迟量为2T/7,向时还考虑了延迟相关对信号信噪比的影响，发现一次延迟相关信号信噪比至少下降3dB，两次延迟相关至少下降7dB，而且信噪比越小，下降越多，因此该算法适用于高信噪比条件，仿真结果表明，该算法在较高的信噪比条件（RSN＞2dB)下具有较好的性能。     

基于蜂群算法的变循环发动机最小耗油率优化

性能寻优控制是使变循环发动机满足长寿命、低油耗和大推力需求的主要途径,也是实现飞机推进系统综合控制的关键技术.基于双外涵变循环发动机非线性数学模型,在满足发动机各部件物理约束条件和推力条件下,采用人工蜂群算法对变循环发动机典型亚声速巡航点(H=11 km,Ma=0.8)耗油率进行了寻优分析,找到了耗油率最小条件下发动机6个几何可调参数、5个发动机循环参数最优值.结果表明:亚声速巡航点的耗油率在优化后比优化前降低了4.5％,从而证实人工蜂群算法能够完成变循环发动机多维优化问题.     

基于比例因子的离心泵圆弧叶片造型研究

针对中低比转速离心泵,提出了能够统一各种圆弧叶片造型方法的比例因子法,推导了叶型参数的计算公式,分析了比例因子对叶片安放角、叶片长度等的影响,并采用数值模拟方法对不同比例因子下的泵内流场进行了性能预测.结果表明,不同比例因子下的叶型参数、流动参数及性能参数变化范围很大.比例因子较小时,节流损失较大,泵扬程较低;比例因子较大时,脱流损失较大,泵效率较低,存在较优的比例因子区间[0.15,0.35],使叶片安放角平滑变化,泵的综合性能较优,对应的曲率半径比为1.4～1.9.采用Pfleiderer方法及本文的角度平均法获得的叶片安放角变化较为平稳,可用于离心泵的初步设计.     

Modeling of the outer heliosphere with the realistic solar cycle

Time-dependent kinetic-continuum model of the solar wind interaction with the two-component local interstellar cloud (LIC) has been developed recently [Izmodenov, V., Malama, Y.G., Ruderman, M.S. Solar cycle influence on the interaction of the solar wind with local interstellar cloud. Astron. Astrophys. 429, 1069–1080, 2005a.]. Here, we adopted this model to the realistic solar cycle, when the solar wind parameters at the Earth’s orbit are taken from space data. This paper focuses on the results related to the termination shock (TS) excursion with the solar cycle that may help to understand Voyager 1 data obtained at and after the crossing of the termination shock and to predict the time of the TS crossing by Voyager 2.     

改善空中飞行模拟性能的有效方法

利用参数自适应控制技术，提出了一种能够自适应补偿飞机参数变化的快速采样控制律。这种控制律可使用迭代技术在不需要特殊“试验”信号又能自动折算依据检测输入激励而获得的原有数据下，对所需要的阶跃响应阵进行了在线辨识，仿真结果表明，在空中飞行模拟中采用这种参数自适应控制技术，尽管飞机参数突基或缓慢变化，但通过本机参数变化的自适应补偿，仍可有效地保持其跟踪性能，尽管飞机参数突然或缓慢变化，但通过本机参数变化     

最大飞行Ma=3.5的吸气式动力方案初步研究

针对某高超声速飞行器飞行任务对低速推进系统的需求(Ma≤3.5)，以某小涵道比加力混排涡扇发动机为背景机提出了两套布局方案。研究结果表明：对于加力涡扇发动机方案TF，通过对背景发动机控制规律的优化，能有效降低了发动机在高空大马赫数工作状态时混合器内外涵的总压差异，并且能获得更低的发动机单位耗油率。对于加力涡扇/亚燃冲压并联组合发动机方案，与TF方案相比，进气道和喷管的各自独立使其在结构上更加复杂,重量会大大增加，技术风险加大。     

Debris flux comparisons from the Goldstone Radar,Haystack Radar,and Hax Radar prior,during, and after the last solar maximum

The continual monitoring of the low Earth orbit (LEO) debris environment using highly sensitive radars is essential for an accurate characterization of these dynamic populations. Debris populations are continually evolving since there are new debris sources, previously unrecognized debris sources, and debris loss mechanisms that are dependent on the dynamic space environment. Such radar data are used to supplement, update, and validate existing orbital debris models. NASA has been utilizing radar observations of the debris environment for over a decade from three complementary radars: the NASA JPL Goldstone radar, the MIT Lincoln Laboratory (MIT/LL) Long Range Imaging Radar (known as the Haystack radar), and the MIT/LL Haystack Auxiliary radar (HAX). All of these systems are highly sensitive radars that operate in a fixed staring mode to statistically sample orbital debris in the LEO environment. Each of these radars is ideally suited to measure debris within a specific size region. The Goldstone radar generally observes objects with sizes from 2 mm to 1 cm. The Haystack radar generally measures from 5 mm to several meters. The HAX radar generally measures from 2 cm to several meters. These overlapping size regions allow a continuous measurement of cumulative debris flux versus diameter from 2 mm to several meters for a given altitude window. This is demonstrated for all three radars by comparing the debris flux versus diameter over 200 km altitude windows for 3 nonconsecutive years from 1998 to 2003. These years correspond to periods before, during, and after the peak of the last solar cycle. Comparing the year to year flux from Haystack for each of these altitude regions indicate statistically significant changes in subsets of the debris populations. Potential causes of these changes are discussed. These analysis results include error bars that represent statistical sampling errors.     

Solar spectral irradiance variability in the ultraviolet from SORCE and UARS SOLSTICE

The SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) has been measuring the solar spectral irradiance on a daily basis since early 2003. This time period includes near-solar maximum conditions, the Halloween storms of 2003, and solar minimum conditions. These results can be compared to observations from the SOLSTICE I experiment that flew on the Upper Atmosphere Research Satellite (UARS) during the decline of the previous solar cycle as well as with currently operating missions. We will discuss similarities and differences between the two solar cycles in the long-term ultraviolet irradiance record.     

YTQ-7氧气调节器性能参数调整分析与实验验证

情况下，实验数据通过对YTQ-7氧气调节器供氧浓度调节原理的分析，说明调整氧浓度调节机构后．在高空输入富氧可以达到输入纯氧时的供氧浓度要求。经测试并对比分析YTQ-7氧气调节器调整前后供氧性能参数验证调整后的氧气调节器供氧性能能够满足不同高度下供氧浓度生理学要求。     

基于EMD及PNN的航天器振动环境分析

针对航天器非平稳随机振动信号模态频率密集的特点,提出了基于经验模式分解EMD (Empirical Mode Decomposition)的多分量过程神经网络PNN(Process Neural Network)自回归模型.通过EMD对原始时间序列进行分解, 使之成为一组不同尺度的局部正交本征模函数IMF(Intrinsic Mode Functions),利用PNN对每个IMF分别进行时变参数分析并以此确定其时变自功率谱密度,对所有分量的时变自功率谱密度通过叠加进行重构, 以此得到原始信号的时变自功率谱密度.仿真结果和实例分析表明:和传统的时频分析法相比,该方法直接使用信号数据,避免了相关估计计算,减小了计算工作量;无交叉干扰项,提高了信号的时频分布特性,具有较高的时频分辨率;对各工况下航天器的振动信号能有效的进行分析,具有较强的信号特征提取能力.