Duffing振子临界态性能研究

During振子临界态相变对弱信号检测研究非常重要,文中研究During临界状态的性能。介绍了随机微分方程理论关于噪声对系统周期态影响的分析;然后为克服存在的过渡过程,建立改进的系统仿真模型。通过仿真试验分析During振子临界态的性能,混沌态与大尺度周期态表现的性能差别深化了对混沌现象的认识;重点研究受噪声干扰的系统运动状态变化情况,得出系统运动越接近临界态越对噪声敏感,噪声越强周期态运动容易再次跃迁回混沌态,说明随机微分方程理论分析临界状态结果不正确;实验结果还表明,噪声是在某些特定条件下导致处于临界大尺度周期态运动的系统发生突变分又跃迁回混沌状态,值得进一步深入研究。     

A model-scale test on noise from single-stream nozzle exhaust geometries in static conditions

A model-scale test with single-stream nozzle exhaust geometries was carried out at the anechoic chamber of Beihang University in Beijing, China. The spectral characteristics are investigated, and the effects of the following parametric variations are reported in this paper: impact of nozzle operating conditions on spectra; impact of the presence of a plug; and effectiveness of chevron configurations for noise mitigation. The measurement shows that the change of pressure values has more impact on spectra than the change of temperature values. The spectral change due to pressure is shown at all band numbers for unheated conditions whereas it is more pronounced at high-frequency ranges for heated conditions. An impact of the presence of a plug is also clearly observed. The reduction of noise is moderate up to band number of 35, and becomes more significant at higher band numbers. It is observed that chevron nozzles are more efficient at high pressure and temperature values. It is expected that the quantified analysis will be used to develop an empirical model of single jet noise, which will be the baseline for the development of prediction of noise from turbofan engines of high bypass ratios.     

雷达接收机内部噪声特性研究

给出了一种雷达接收机抗内部噪声干扰的数学模型,研究结果适用于一般电子设备的热噪声问题,具有普遍的指导意义及实用价值。     

回转体流噪声相似律的实验研究

介绍了回转体流噪声实验的方法,并对实验测得的回转体流噪声声功率谱的谱特性进行了分析。测量结果表明:在高频段,回转体流噪声声功率谱按6dB/ 倍频程衰减;且其声功率谱与流速的7 次方成正比。基于本实验,验证了回转体流噪声相似律理论     

宽波束天线噪声温度的计算

探讨宽波束天线噪声温度的计算方法及噪声温度对系统灵敏度的影响 ;提出天线自身噪声源、天线自身噪声温度、天线直流电阻、天线交流阻抗等概念 ,给出自身噪声温度的计算公式 ;对典型的 GPS天线的噪声温度进行计算     

基于增广Burgers方程的音爆远场计算及应用

音爆的精确模拟对于超声速客机的低音爆研究与设计意义重大。由于计算能力的限制,客机巡航高度的音爆全场直接模拟目前还难以实现。现有的音爆预测方法一般分为两步,先通过超声速线化理论或计算流体力学的方法得到音爆近场的过压值（Over-pressure）分布,再通过声学理论将近场声压信号推进至远场,以获得飞行器的地面音爆信号。在远场计算中,传统的波形参数法没有考虑音爆传播过程中的经典吸收和分子驰豫效应所造成的声能损失,得到的激波没有厚度,导致计算得到的远场声压级不准确。基于算子分裂法,开展了非线性声学中的增广Burgers方程的数值解法研究。通过计算第二届音爆预测研讨会（SBPW-2）发布的两个标准算例,验证了该方法可以实现地面音爆波形的精确预测。发现在近场声压信号前加入一段无幅值的缓冲信号可以有效提升"N"波上升时间的模拟精度。网格收敛性研究表明适当加密计算网格是有必要的。在此基础上研究了大气声吸收对地面波形的影响,发现分子驰豫效应的影响要强于经典吸收。最后,研究了不同湿度、温度对地面音爆波形的影响,发现干燥、低温的环境对音爆信号的过压值有抑制作用。     

基于改进TCAR的高精度定位技术研究

模糊度解算是实现快速、高精度定位的关键,一直是全球卫星导航系统研究的热点。北斗系统提供三频信号,可以进行不同形式的组合,实现高精度定位和模糊度解算。通过分析现有的无电离层三频模糊度解算方法(TCAR)和组合观测值的噪声特征,提出一种低噪声无电离层影响的宽巷与IF组合相结合的TCAR算法,选取低噪声长波长的宽巷组合观测值,在几何模型下用最小二乘法逐级解算模糊度,最终实现静态定位。为了验证组合噪声的影响和各种TCAR算法的性能,对北斗中基线的实测数据进行实验,并且比较提出方法与现有算法的模糊度解算情况及位置精度。结果表明,提出方法可以有效提高模糊度解算的成功率,实现高精度定位。     

多段翼型前缘缝翼位置的优化设计研究

本文讨论优化前缘缝翼位置的位流设计方法。优化变量为缝翼相对于主翼的缝隙(Gap)、覆盖量(Ouerlap)和偏角δ_s,目标函数为主翼上的压力峰值。应用高阶面元法计算多段翼型压强分布。用Powell优化法使主翼上压力峰值减至最小,以延迟多段翼型的失速,增大最大升力系数。本方法已用于计算NACA64A010两段和四段翼型以及Foster三段翼型,所得结果与实验数据和位流/边界层耦合设计法的结果有很好的一致性。     

Finding the suitable drag-free acceleration noise level for future low-low satellite-to-satellite tracking geodesy missions

This paper evaluates the impact of residual acceleration noise on the estimation of the Earth’s time-varying gravity field for future low-low satellite-to-satellite tracking missions. The goal is to determine the maximum level of residual acceleration noise that does not adversely affect the estimation error. The Gravity Recovery And Climate Experiment (GRACE) has provided monthly average gravity field solutions in spherical harmonic coefficients for more than a decade. It provides information about land and ocean mass variations with a spatial resolution of ～350?km and with an accuracy within 2?cm throughout the entire Earth. GRACE Follow-on was launched in May 2018 to advance the work of GRACE and to test a new laser ranging interferometer, which measures the range between the two satellites with higher precision than the K-Band ranging system used in GRACE. Moreover, there have been simulation studies that show, an additional pair of satellites in an inclined orbit increases the sampling frequency and reduces temporal aliasing errors. Given the fact that future missions will likely continue to use the low-low satellite-to-satellite tracking formation with laser ranging interferometry, it is expected that the residual acceleration noise will become one of the largest error contributor for the time-variable gravity field solution. We evaluate three different levels of residual acceleration noise based on demonstrated drag-free systems to find a suitable drag-free performance target for upcoming geodesy missions. We analyze both a single collinear polar pair and the optimal double collinear pair of drag-free satellites and assume the use of a laser ranging interferometer. A partitioned best linear unbiased estimator that was developed, incorporating several novel features from the ground up is used to compute the solutions in terms of spherical harmonics. It was found that the suitable residual acceleration noise level is around 2?×?10^?12?ms^?2?Hz^?1/2. Decreasing the acceleration noise below this level did not result in more accurate gravity field solutions for the chosen mission architecture.     

宽带转发器的功率利用率和交调干扰

动用统计分析的方法，给出了转发器功放的非线性与交调干扰的关系；可在保证一定信噪比的情况下得到较高的利用率，克服了在一般设计中为减少交调干扰，而尽可能提高功率输出地范围的盲目性，为宽带转发器的设计提出了一条新途径。