小波去噪法在复合材料变形测量中的应用研究

为了提高数字散斑相关方法（DSCM）在复合材料变形测量中的精度,将数字散斑技术与小波去噪技术相结合,采用阈值去噪法对小波系数进行阈值量化处理,并进行复合材料的拉伸试验,同时使用DSCM及引伸计进行测量,再使用该小波去噪法对DSCM测量的结果进行去噪,并与引伸计所测结果相比较。结果表明：去噪后的DSCM的测量结果与引伸计测量的结果吻合得更好,精度更高,说明该小波去噪法能够较好地去除数字散斑相关测量和计算中的噪声。     

用小角度测量仪校准合象水平仪的不确定度问题探讨

介绍了微分筒式小角度测量仪的构造及测量原理 ,对使用该小角度测量仪校准合象水平仪时的测量不确定度进行了分析计算 ,指出使用微分筒法校准合象水平仪准确度高且操作方便。     

数字散斑干涉在振动测量中的应用

在动态测试领域中,数字散斑干涉技术常用到的相位处理方法有时问平均法和空间载波相移法.空间载波相移法因其简单性和实用性,被应用于双脉冲散斑干涉测量中.     

复合材料电子剪切散斑干涉无损检测

介绍了一种电子散斑干涉测量仪,对其测量原理和结构进行了描述。用此仪器对铝蜂窝夹层结构、树脂基复合材料等试样进行了检测,得到了满意的试验结果。     

基于视觉的模型烧蚀形貌实时测量方法

针对电弧风洞试验时模型烧蚀形貌实时的变化问题,使用数字散斑相关结合双目视觉的方法直接测量得到了模型烧蚀过程的形貌变化历程。利用散斑相关来进行图像数据的处理,同时综合了亚象素相关算法。通过测量获得了模型烧蚀过程的形貌实时变化情况。标定结果表明标定精度达到了0.02 mm;试验结果表明,测量方法可以为分析平板模型随烧蚀时间变化而变化的特性提供有效的试验数据。     

一种新型的非接触的变形场测量技术

数字散斑相关方法(DSCM)是一种新型非接触变形场测量技术。散斑是相干光被光学粗糙面或不均匀媒介散射而在空间形成的随机分布的光强场,它具有颗粒状特点。可认为物体表面随机分布着许多粒子,粒子在光照射下,反射光形成特有的光强场。DSCM是通过测量物体变形前后光强场概率统计相关性来确定物体变形。首先用光源照射试样,试样表面形成特定散斑图样,可用某一点周围微区内散斑子集的变形描述这一点的变     

球轴承接触角测量仪的动态不确定度

考虑球轴承接触角测量仪的自身动态特性、轴承外圈的试验转速、试验加载力对测量仪测量精度的影响,建立了测量仪的动态不确定度计算模型。针对小样本试验测试结果,采用灰色理论的方法评价了球轴承接触角测量结果的不确定度。基于不确定度的分离原理,分离出测量仪的自身动态特性、外圈转速、试验加载力对测量不确定度的影响规律,建立了接触角测量的动态不确定度计算模型,并通过实际算例验证了模型。建立的测量仪动态不确定度计算模型可用于预测不同工况下的接触角测量不确定度,有助于及时对测量仪进行相应的校准,以提高接触角测量结果的精度。      

基于可靠性指标的测试系统校准周期优化

通过对测试系统校准周期的直接反应法(SRM)和威布尔(Weibull)可靠性模型法的分析、改进,以及对校准过程中误判率的分析测算,解决了测试系统检定决策的风险问题.首先介绍了测试系统可靠性指标的相关计量技术规范,然后通过对常用的校准周期确定方法的介绍与分析,进一步给出了测量可靠性观测值的可靠性概率函数描述方法,并利用主元分析法来综合评价不同测量参数的影响,修正了最佳校准周期的计算.通过对自动测试系统DMM(数字万用表)测量通道的检定,表明这些优化措施是可行的.      

CS-01高空台推力测量和校准装置研制

推力是涡喷涡扇发动机高空模拟试验的重要测量参数之一。CS－01高空台原推力测量采用杠杆、砝码、测力秤系统，现采用原位校准，液压加载、应变式推力传感器来测量和校准，从而消除了“高度差”的影响，降低了稳态推力测量系统的测量不确定度。     

关于航空发动机测功机校准相关问题的探讨

以扭矩传感器测量原理为基础,阐述了航空发动机测试系统测功机的校准方法;通过分析航空发动机测试系统测功机校准方法存在的问题,提出了现场校准方法,探讨了量值传递过程中的误差来源及对策。     

全息测振干涉图的自动分析与处理

 研究数字条纹图象的自动检测与判读处理的理论与技术,在微型通用数字图象处理系统上建立了一套条纹自动检测与判读处理的软系统,实现了条纹图象的输入、定位、预处理、骨架化、细化、修补与光滑、计数、插值及三维振幅场输出等功能,对类似的散斑干涉条纹和莫尔条纹的判读处理有理论参考价值。     

位移传感器校准技术研究

介绍了一种直线位移传感器校准装置。该系统以自行研制开发的高准确度单频激光干涉仪为长度标准,通过可编程位移发生装置的配套使用实现了直线位移传感器的校准。     

ATS-6 Interferometer

The Applications Technology Satellite-6 (ATS-6) RF interferometer is utilized primarily as a precision 3-axis attitude sensor having an unambiguous field of view of 350°. This function requires two separated ground transmitters, each using one of the two available frequency channels or sharing a single channel by time multiplexing. For 3-axis control, one uplink transmitter can provide 2-axis attitude (pitch and roll) with other sensors (e.g., a Polaris tracker) providing yaw attitude. By utilizing two uplink transmitters and the Earth sensor or three time multiplexed uplink transmitters, the interferometer can also provide measurements of ATS-6 spacecraft orbit position. Uplink frequencies are 6.150 and 6.155 GHz. The receiving antennas are spaced at 19.95 wavelengths (?) for the vernier baseline and 1.66 ? for the coarse baseline. Spacecraft system weight is 8.39 kg (18.5 lb) and power requirement is 15.5 W. Flight evaluation results are given for the interferometer including R F link budgets, modulation of uplink carrier, signal-to-noise ratio, and dropout behavior. A hardware calibration model is described, containing major biases in the phase measurements. Techniques for flight calibration as both an attitude and spacecraft position sensor are outlined . Flight testing has shown that on-line calibration of receiver/converter biases must be performed on a short term routine basis. Interferometer resolution was found to be 0.00140 space angle with negligible noise (jitter) at transmitted power levels above 72 dBW. As an attitude sensor, the interferometer has demonstrated the ability to provide stabilization to better than 0.     

数字式活塞压力计的研制

介绍了一种集活塞压力计和数字压力计优点于一身的数字式活塞压力计,其改变了传统活塞压力计的设计方案,并在传动密封和系统校准技术方面有了很大的创新,对于现场校准和提高压力计量校准的自动化程度有深远意义。     

Polarization Mismatch Errors in Radio Phase Interferometers

An analysis is presented which deals with the effects of polarization mismatch errors on the accuracy of a phase interferometer used for position location of unknown emitters relative to known calibration emitters. Closed-form expressions for the induced phase difference between interferometer antennas are derived for several combinations of receiving and transmitting antenna polarizations. Errors contributed by mechanical misalignment between antennas, as well as effects of power loss attributable to polarization mismatch, are also considered. The analysis leads to the conclusion that circularly polarized interferometer and transmitter antennas are best suited for the position location application, if it is assumed that polarization tracking of the interferometer antennas is not available. It is shown that a reasonable amount of ellipticity can be tolerated before the phase error becomes significant.     

加速度计的校准

介绍了振动传感器——加速度计的校准方法及其误差分析,着重介绍了加速度计校准的最新方法,即随机校准,提出了改进的随机校准方法,并作了相应的误差分析。对各种校准方法如正弦比较法、激光干涉仪法、随机校准法进行了比较,作了试验研究。     

飞机系统模拟试验中热电阻及其数字显示仪表的现场校准技术研究

在飞机系统地面模拟试验中．热电阻及其数字显示仪表在液压、飞控等试验系统中广泛使用。针对各试验系统中某些位置的热电阻及其数字显示仪表接线复杂,不便拆卸和传统计量方式的种种弊端等问题,提出了一种由现场计量炉、便携式测温仪和温度校准器等设备组成的现场校准系统。实现对热电阻及其数字显示仪表的现场整体校准,同时亦可实现对热电阻及其数字显示仪表的分部校准,避免了拆卸和安装,提高了工作效率,具有实用价值。     

Space Interferometry Mission instrument model and astrometric performance validation

The Space Interferometry Mission (SIM), performed very accurate astrometric measurements to measure the positions of stars using a 10 m baseline optical interferometer. The lack of signal from the science targets precludes using the star as a feedback signal to control the science interferometer delay line. In order to solve this problem SIM uses pathlength feed forward (PFF) control of the science interferometer. In the case of controlling the science interferometer optical path, the information to position the science delay line comes from a combination of internal metrology, external metrology, and guide interferometer measurements. The accuracy of the internal and external metrology measurements and the guide interferometer measurements are important for the quality of the feed forward signal and also for the ultimate astrometric performance of the instrument. An instrument model of SIM has been built to evaluate optical performance and to emulate various observational scenarios. The effect of averaging methods to reduce metrology cyclic error and the viability of on-orbit calibration maneuvers are studied. The model consists of a real-time dynamics formulation of the spacecraft and a real-time attitude control system. Simulation results investigate the sensitivity of the feed forward signal to the various error sources and time-varying terms.