多级轴流压气机噪声源特性分析

某型轴流式压气机高压一级转子叶片出现大幅振动,并且振动频率不是转频的整阶次,即叶片非同步振动。对叶片的激励可能来源于气动和非定常流场,就包含了声场。为了研究叶片出现非同步振动时的压气机声场,在压气机机匣内壁上对压气机噪声进行测量。通过分析得知,噪声信号特征频率的出现与叶片非同步振动同时出现,主要影响因素有压气机转速、结构调节状态等参数。     

TC4 钛合金板材双晶探头超声波检测

研究了TC4钛合金板材高灵敏度双晶探头超声波检测中变型波、组织噪声的产生原因及影响.结果表明:变型波会给缺陷波定量评定带来影响,以缺陷波始脉冲波幅定量评定最为准确,对于缺陷波始脉冲之后的波幅超标应选用不同焦距的双晶探头进行对比检测.组织噪声的产生与板材中同取向粗大α相晶粒增多密切相关,通过减小脉冲宽度可有效降低组织噪声.     

“资源三号”卫星三线阵相机辐射质量评价

为了推动＂资源三号＂（ZY-3）卫星影像数据早日为相关领域提供服务,文章采用主观评价和客观评价相结合的方法,对资ZY-3卫星三线阵图像的辐射特性进行了全面评价。分析结果表明,ZY-3卫星三线阵相机图像清晰,信噪比高,能够有效反映不同地物的细节特征,在量化深度和细节表现等方面具有优势。     

导航卫星应用在双站雷达中的关键问题分析

对导航卫星应用到双站雷达中存在的功率、同步以及干涉等关键问题进行了分析。分析了双站雷达的信噪比的影响因素,得出目标散射面积和允许的最大接收机到目标斜距的关系。分析双站雷达面临的三大同步问题,给出了同步的思路和实现方法。分析了系统的干涉,并提出了解决思路。     

汽车发电机冷却风扇旋转噪声预测方法

以汽车发电机冷却风扇为对象,针对其修改叶片分布角度前后的旋转噪声预测问题,提出一套较精确且节约计算机时的预测方法.该方法结合了声类比法和矢量合成方法,首先,用大涡模拟(LES)和Ffowcs-Williams和Hawkings(FW-H)方程相结合的声类比方法对原风扇总噪声和主要阶次旋转噪声幅值进行预测;然后,针对只改变叶片分布角度情况下,提出一种矢量合成方法,用于对修改叶片分布前后主要阶次旋转噪声变化量的预测;最后,得到修改后主要阶次旋转噪声的幅值.计算和实验结果表明,原风扇总噪声最大预测误差4.3dB,第12阶和第18阶主要阶次旋转噪声幅值预测误差为1.24dB和4.26dB;修改后风扇第12阶和第18阶主要阶次旋转噪声分别变小了9.3dB和10.5dB,其变化量预测误差分别为0.36dB和0.43dB.结果表明,这一整套对修改前后风扇旋转噪声进行预测的方法是可行的,且大大节省计算时间,为风扇叶片周向分布角度设计提供了很好的依据.      

磁层电场仪前端信号处理电路研究

针对磁层稀薄等离子体环境中的电场测量,设计了一种电场仪前端信号处理电路方案.双探针电场仪通过向等离子体输出驱动电流,测量两探针间的电位差,从而测量空间电场的探测仪器.在磁层稀薄等离子体环境下,等离子体阻抗较高,电场仪探针将工作在较高的工作电压上.若探针电压接近或超过电路耐压值,则可能会影响探测结果,甚至损坏电场仪.本文结合低偏置电流的电压跟随方案和反馈悬浮电源控制方案,解决了稀薄等离子体环境中电场测量的弱电流采样和高动态电位处理问题,并采用低噪声元件和特殊电路设计,控制电路噪声.测试结果显示,本方案可使探针适应±100V的悬浮电位,实现150kHz带宽的电场信号测量,且噪声小于14nV·mHz-1/2,满足目前空间电场仪测量精度需求.      

主要参数对面齿轮传动噪声辐射的影响分析

为研究面齿轮传动力学特性及噪声辐射,通过建立面齿轮传动的弯扭耦合动力学模型,在分析轴承支承处动载荷的基础上,结合有限元法和边界元法,形成了面齿轮传动的噪声辐射计算流程.此外,利用该计算流程,开展了算例分析,讨论了单一几何参数和工况对面齿轮传动噪声辐射的影响规律.仿真结果表明:模数和传动比对改善面齿轮传动噪声辐射有益,压力角对其噪声辐射影响不明显.研究结果为低噪声面齿轮传动的设计奠定了必要的理论基础.      

一种用于深空通信的系统LT码

针对传统LT（Luby Transform）码用于深空通信时性能不理想的问题,通过重构LT码的二分图设计适用于深空通信环境的系统LT码,提出一种去环编码算法。采用外信息转移图分析系统LT码的收敛阈值,然后通过仿真试验评估系统LT码的性能。仿真结果表明,采用本文提出的编码方案的系统LT码能够明显降低错误平层,提高译码算法的性能。     

Investigation of rotor–stator interaction broadband noise using a RANS-informed analytical method

A Reynolds-Averaged Navier Stokes (RANS)-information analytical method for predicting Rotor-Stator Interaction (RSI) broadband noise is established in this paper. First, the turbulence information is deduced from RANS simulation result. Then, the unsteady load on the stator blade is calculated using a strip theory approach based on LINearized SUBsonic unsteady flow in cascade (LINSUB) and 2-D equivalence method. In the end, the sound power of RSI broadband noise is calculated by coupling the unsteady load on the stator blade with acoustic analogy and annular duct mode. The broadband noise model part of the RANS-information analytical method is validated against the upstream sound power of an annular cascade experimental bench. Besides, the RANS-information analytical method is used in predicting RSI broadband noise of a single-stage axial fan acoustic experimental bench, the results illustrate that the RANS-information analytical method can accurately predict the RSI broadband noise in different fan working conditions. After simplification the Wave Leading Edge (WLE) stator blade, the effect of WLE stator blade on RSI broadband noise is studies. Although the simplification may bring some discrepancies, the results illustrate that the RANS-information analytical method has the capability for further studies on the broadband noise reduction with WLE stator blade.     

Zero,minimum and maximum relative radial acceleration for planar formation flight dynamics near triangular libration points in the Earth–Moon system

Assume a constellation of satellites is flying near a given nominal trajectory around _L4$L_4$ or _L5$L_5$ in the Earth–Moon system in such a way that there is some freedom in the selection of the geometry of the constellation. We are interested in avoiding large variations of the mutual distances between spacecraft. In this case, the existence of regions of zero and minimum relative radial acceleration with respect to the nominal trajectory will prevent from the expansion or contraction of the constellation. In the other case, the existence of regions of maximum relative radial acceleration with respect to the nominal trajectory will produce a larger expansion and contraction of the constellation. The goal of this paper is to study these regions in the scenario of the Circular Restricted Three Body Problem by means of a linearization of the equations of motion relative to the periodic orbits around _L4$L_4$ or _L5$L_5$. This study corresponds to a preliminar planar formation flight dynamics about triangular libration points in the Earth–Moon system. Additionally, the cost estimate to maintain the constellation in the regions of zero and minimum relative radial acceleration or keeping a rigid configuration is computed with the use of the residual acceleration concept. At the end, the results are compared with the dynamical behavior of the deviation of the constellation from a periodic orbit.