火箭发动机燃气射流喷水降噪研究

采用有限体积法预估喷水对火箭燃气射流气动噪声的抑制程度.建立并求解了守恒的控制体的质量、动量和能量方程,得到了燃气和水掺混后的等效射流参数,分析了水和燃气的质量流率比对等效射流参数和降噪效果的影响.计算结果和试验数据的结果基本吻合.结果显示,当水和燃气的质量流率比超过一个临界值之后,降噪效率会降低.      

基于有限元/边界元耦合方法的管道进口声传播及声辐射模型

发展了一种基于有限元和边界元耦合方法的管道进口声传播及声辐射计算模型.该模型将整个声场分为内部有限域和外部无界域,分别用有限元和边界元方法求解控制方程,在两者之间的界面上使用具有物理意义的声阻抗参数进行匹配,并通过一种快速迭代方法实现全声场求解.这种迭代方法可以保证有限元刚度矩阵等带宽以及对称的特性不被破坏,有助于提高计算效率.该模型先得到了Levine-Schwinger标准解的检验,进而在无流动情况下对于简化的航发短舱进口管道模型进行了噪声辐射现象的数值模拟,最后基于计算结果分析了声衬对远场声辐射的影响.      

三轴轮控航天器姿态大角度机动控制器设计

研究了飞轮作为执行机构的航天器姿态大角度机动问题。建立了飞轮控制的姿态动力学模型;基于Lya-punov稳定性定理,设计了闭环控制器并给出了参数自适应律的解析表达式;分析了有界噪声作用下该模型的控制效果。仿真结果表明,所设计的控制器具有较强的鲁棒性和抗干扰能力。     

一种无人机视觉导航方法及其滤波算法改进

设计了一种无人机视觉/惯性组合导航系统,将无人机和地标点的运动模型作为状态方程,视觉信息作为观测量构建了与之对应的滤波模型.在滤波处理上,采用了复杂加性噪声模型对系统噪声进行建模处理;将小波分析引入到UKF(Unscented Kalman Filter)滤波中得到小波-UKF滤波算法,以此克服视觉观测噪声对滤波的影响;采用最大后验概率准则(MAP,Maximum A Posterior)自适应估计观测噪声协方差阵,并将其反馈到滤波过程中克服了小波处理后观测噪声方差阵不易确定的不足.仿真结果证明:对滤波算法的改进可以有效地提高滤波估计的精度.     

传递对准中机翼弹性变形建模与滤波处理

针对机翼弹性变形对传递对准的较大影响,提出采用双激光测距方法对不同挂点弹载子惯导系统的机翼弹性变形进行在线量测,利用AR(n)模型来简化ARMA(p,q)模型进行机翼弹性变形的在线建模.建模中采用递推最小二乘法估计模型参数,利用模型估计残差的F检验法确定模型的阶数.最后,根据机翼弹性变形模型并结合快速对准匹配方法设计了考虑多阶有色观测噪声的传递对准滤波器.仿真试验验证了这种机翼弹性变形在线建模方法和考虑有色观测噪声的对准滤波器的可行性和有效性,为机载导弹提供了一种有效的快速精确传递对准方法.     

A new adaptive Kalman filter for navigation systems of carrier-based aircraft

The features of carrier-based aircraft’s navigation systems during the approach and landing phases are investigated. A new adaptive Kalman filter with unknown state noise statistics is proposed to improve the accuracy of the INS/GNSS integrated navigation system. The adaptive filtering algorithm aims to estimate and adapt the unknown state noise covariance Q in high dynamic conditions, when the measurement noise covariance R is assumed to be known empirically in advance. The new adaptive Kalman ...     

大型客机起飞着陆过程噪声辐射特性对比分析

 基于准稳态假设和分布点声源模型,并采用最新发展的噪声源半经验参数预测公式,发展和完善了用于飞机飞行过程中噪声辐射预测的计算模型和方法。该计算方法能够预测飞机起飞、着陆过程中的适航噪声,并能够对飞机不同噪声源的噪声辐射特性（声级、频谱特性和指向性等）进行计算分析。以某大型客机为对象,对飞机进场着陆过程和起飞过程中飞机噪声源进行了计算分析,计算结果表明,飞机进场着陆和起飞过程中,不同噪声源对远场噪声级的影响有明显的差异,起飞过程中发动机风扇噪声源是最主要的噪声辐射源,而在进场着陆过程中飞机机体噪声（包括起落架和襟翼等）是重要的飞机噪声源。文中也给出了不同噪声源频谱特性和指向特性等。     

基于乏信息系统的本征融合技术

提出基于乏信息系统的本征融合技术以模拟小样本条件下的未知分布.采用隶属函数法、最大隶属度法、自助法、灰自助法、算术平均值法和最大熵法等多种数学思想,从不同侧面分析各个个体的特征信息并进行融合,推断出总体的概率分布.滚动轴承噪声的试验研究表明,本征融合技术可以有效地模拟乏信息系统的概率分布.      

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.     

Scaling procedures of cabin noise generated by turbulent boundary layer excitation

This paper presents a new method for measuring the cabin noise of a structure in a wind tunnel. A method for scaling the cabin sound was derived to obtain the cabin noise of a structure, and the derivation of the scaling procedure was based on a theoretical hypothesis regarding the cabin noise prediction for a scaled model in a wind tunnel. A frequency offset was generated because of the error introduced by model manufacture and installation, and a proposed modal test method was used to eliminate the frequency offset. Both a full-scale structure and scaled structure were measured in the wind tunnel tests. The cabin noise of the full-scale model was compared with the results obtained using the scaling procedure based on the scaled model. The comparisons of the measurement results indicate that the scaling procedures developed in this paper are effective for vibro-acoustic predictions in wind tunnels. Moreover, background noise tended to affect the results of the cabin sound for the wind tunnel test, and thus background noise should be prevented through specific design efforts.