基于随机时延的弹射式干扰研究

针对传统噪声压制技术对合成孔径雷达形成有效干扰需要功率比较大的特点,研究了一种随机时延的弹射式干扰方法。该方法是在传统的弹射式干扰基础上,采用随机的干扰机转发时延。由于采用随机时延,方位向不同的回波时延不同而不能被压缩,干扰信号的距离向的压缩虽能成像,但已经是随机分布的。改进后的弹射式干扰能够覆盖整个成像区域,形成类噪...     

基于HOSVD局部重组的利噪抑噪经验模式分解及应用

及时准确地识别航天机构萌生和发展的损伤故障特征信息,可为机构故障诊断评估、科学任务调整以及未来在轨维修提供科学决策依据。集成噪声重构经验模式分解(ENEMD)及其衍生方法都是基于噪声利用机制以原信号中估计噪声改善模式混淆并实现信号降噪。然而,该方法中奇异值拐点难以获取、阈值处理中噪声不连续等带来的噪声估计偏差,将降低微弱特征提取准确性。为此,提出一种基于高阶奇异值分解(HOSVD)局部重组的噪声估计技术。研究基于滑动窗截断和Hankel矩阵相结合的张量构建,然后将奇异值曲率谱上的最大峰值点作为合理奇异阶,最后根据选取的奇异阶重构张量分解模型得到所需的估计噪声分量。在此基础上,将HOSVD局部重组引入ENEMD方法中,提出利噪抑噪经验模式分解方法。该方法可进一步提高微弱噪声估计精确度,实现对航天机构损伤微弱特征的增强提取。仿真分析和某航天轴承试验案例验证了该方法在损伤微弱特征提取和识别上具有实用性与有效性。     

Evaluation and analysis on positioning performance of BDS/QZSS satellite navigation systems in Asian-Pacific region

By using the observation data and products of precise obit and clock offset from Multi-GNSS Experiment (MGEX) of the International GNSS Service (IGS) and GNSS Research Centre, Curtin University in this paper, the positioning performance of BDS/QZSS satellite navigation system has been analyzed and evaluated in aspects of the quantity of visible satellites, DOP value, multipath effect, signal-to-noise ratio, static PPP and kinematic PPP. The analysis results show that compared to BDS single system when the cutoff angle are 30°and 40°, the DOP value of BDS/QZSS combined system has decreased above 20%, and the quantity of visible satellites increased about 16–30% respectively, because of the improved spatial geometric configuration. The magnitude of satellite multipath effect of BDS system shows the trend of MEO?>?IGSO?>?GEO, which is consistent with that of QZSS satellite system, as the constellation structure of the two systems is similar. The variation tendencies of signal-to-noise ratio with respect to elevation angle of the two systems are almost the same at all frequencies, showing that at the same elevation angle the signal-to-noise ratio of MEO satellites is higher than that of IGSO satellites, as the higher obit is the lower transmitting power is obtained. For having a specially designed obit, the variation of signal-to-noise ratio of BDS system is more stable. However, the magnitude of signal-to-noise ratio of QZSS system appears the trend of frequency 3?>?frequency 2?>?frequency 1. The static PPP performance of the BDS/QZSS combination system has been improved more significantly than the BDS single system in E, N and U directions. When the cutoff angle are at 7°, 15° and 30°, the PPP accuracy is increased about 25–34% in U direction, 10–13% and 23–34% in E and N directions respectively. When the elevation angle is large (40°), compared to BDS single system at lower elevation angles (7° and 15°) the PPP accuracy of the BDS/QZSS combination system is improved above 30% in U direction. In kinematic PPP performance, compared to BDS single system, the accuracy, availability and reliability of the BDS/QZSS combination system has been improved too, especially at large elevation angles (30° and 40°), the kinematic PPP accuracy in E and U directions has been improved about 10–50%, and above 50% in U direction. It can be concluded that the combination with QZSS system can improve the positioning accuracy, reliability and stability of BDS system. In the future, with the improvement of the satellite construction of Japan’s QZSS system and the global networking of China’s BDS satellites, the QZSS satellites will contribute greatly to improve the positioning accuracy, reliability, availability and stability of GNSS systems in areas such as cities, mountains, densely-packed buildings and severely covered areas in Asian-Pacific region.     

单体建筑在点声源环境中对预测点噪声等级的影响

为了提高噪声评价方法的可靠性，减化噪声评价工作程序，实现环境噪声评价自动化，从几何角度分析了点声源环境中，单体建筑随空间位置不同，对预测点噪声等级的不同影响。介绍了用VC 6．0语言对点声源环境中只有单体建筑存在时，预测点的噪声等级进行程序设计的方法及流程，编写的程序操作简单，实现了相关参数输入后(手工输入或从AutoCAD图纸读入)，计算机自动处理、输出结果，通过与外部程序接口调用Matlab，绘制等声级图，结果直观明了。     

频率源振动对测速精度的影响

针对频率源振动会影响测速精度的问题,按照国军标车载设备的振动要求,对频率源振动带来的相位噪声进行仿真分析和实际测试。并以振动频率为5Hz为例,对10 MHz频率源进行测试计算得到相应短稳;然后计算频率源在静止和振动环境下的测速随机误差;最后通过比较得到频率源在振动时测速精度会恶化几个数量级的结果。建议在动中测速时,通过使用加速度灵敏度低的晶振,安装减震器,优化环路设计,采用数字补偿技术等措施以减少振动对测速精度的影响。     

风扇出口导向叶片低噪声设计Ⅱ:数值验证

作为风扇出口导向叶片（Outlet Guide Vanes，OGV）低噪声设计系列文章的第2篇，本文对气动/声学一体化设计获得的2个OGV低噪声方案的降噪效果进行了数值验证。为了对低噪声优化方案的降噪效果进行详细评估，首先，采用非线性谐波法对优化前后的风扇/增压级开展了数值仿真，对OGV不同截面和叶片表面脉动压力进行了对比分析，发现低噪声优化设计方案有效降低了转/静干涉引起的脉动压力；然后，通过掠形和倾斜的合理组合，改变了叶片表面的相位分布，沿径向的相位变化增加了OGV对尾迹响应相互抵消的机会，从而有利于噪声的降低；最后，采用Wilson的波分解方法开展了对各方案的模态分析，对降噪效果进行了量化评估。结果显示，优化后的低噪声方案除起飞状态1BPF外，降噪量均超过了5 dB。     

集成运算放大器的噪声及其简化计算

介绍了运算放大器产生的机构，运放的Ｅｎ－Ｉｎ噪声等效电路模型，在等效电路的基础上求出了运放的噪声系数及最佳噪声电阻的估算公式。     

吸尘器振动与噪声试验分析

针对某型号吸尘器噪音和振动大的问题进行试验研究,用声强法对吸尘器的噪音进行测量分析,同时对吸尘器的振动进行了测量并对振动信号用DASP软件进行了频谱分析,识别了吸尘器的主要振动源和噪声源.在试验分析的基础上,提出了一些改善其振动和噪音性能的措施.     

Electron acoustic solitary waves in the Earth’s magnetotail region

Satellite observations have revealed solitary potential structures in the Earth’s magnetotail region. These structures have both positive (compressive) and negative (rarefactive) electrostatic potentials. In this paper we study the electron-acoustic solitary waves (EASWs) in an unmagnetized plasma consisting of cold plasma electrons and isothermal ions with two different temperatures. Using the reductive perturbation method, the nonlinear evolution of such structures is studied. The numerical computations are performed to study the role of two temperature ions in the generation of EASWs. In this case, the model supports the existence of both positive and negative electrostatic potentials with bipolar pulses. The electric field associated with these positive and negative solitary structures are numerically computed. The present study could be useful to construe the compressive and rarefactive electric field bipolar pulses associated with the BEN type emissions in the magnetospheric regions where the electron beams are not present.     

Correlation between the cosmic noise absorption calculated from the SARINET data and the energetic particles measured by MEPED: Simultaneous observations over SAMA region

The cosmic noise absorption is presented in terms of two-dimensional images obtained from the imaging riometers operated at the Southern Space Observatory (geographic coordinate: 29.4° S, 53.1° W), in São Martinho da Serra, Brazil, Concepcion (geographic coordinate: 36.5° S, 73.0° W) and Punta Arenas (geographic coordinate: 53.0° S, 70.5° W) in Chile, which belong to the South American Riometer Network and are located at the central and periphery regions of the South American Magnetic Anomaly. Correlations are performed between the maximum cosmic noise absorption observed at these stations and the energetic electron flux in two energy channels (>30 and >300 keV) and the proton flux in three energy channels (80–240, 800–2500 and >6900 keV) as measured by the Medium Energy Proton and Electron Detector, during a moderate geomagnetic storm that occurred on September 3, 2008. The results show high correlations between the cosmic noise absorption detected at São Martinho da Serra and the flux of protons with energy between 80 and 240 keV, and the flux of electrons with energies higher than 300 keV, while an additional ionization at Concepcion was correlated with electrons of energies higher than 30 keV. The cosmic noise absorption detected at Punta Arenas was probably caused by the increase of the protons flux with energy between 80 and 240 keV.