Flight Flutter Modal Parameters Identification with Atmospheric Turbulence Excitation Based on Wavelet Transformation

针对基于大气紊流激励的飞机颤振试验数据具有信噪比低以及测量数据以加速度响应形式给出等特点,将小波变换与随机减量法相结合对飞机颤振模态参数进行识别,首先利用随机减量法获得结构在非零初始加速度条件下的自由衰减响应,然后对该自由衰减响应进行Morlet连续小波变换,为使变换简单,本文采用了Parseval定理和留数定理,利用Morlet的带通滤波特性,通过搜索小波变换系数在不同的尺度区域内的极大值,再根据小波变换系数的极大值、相角与固有振动频率及阻尼系数间的关系,即可识别出各模态参数。并对利用小波变换识别颤振模态参数时,实现模态解耦应满足的条件进行了分析研究。通过仿真和飞机颤振试验数据分析,验证了该识别方法不仅简单、有效和可行,而且具有较强的抗噪性。     

Periodic Error Compensation for Quartz MEMS Gyroscope Drift of INS

In order to improve the navigation accuracy of an inertial navigation system （INS）, composed of quartz gyroscopes, the existing real-time compensation methods for periodic errors in quartz gyroscope drift and the periodic error term relationship between sampled original data and smoothed data are reviewed. On the base of the results, a new compensation method called using former period characteristics to compensate latter smoothness data （UFCL for short） method is proposed considering the INS working characteristics. This new method uses the original data without smoothing to work out an error conversion formula at the INS initial alignment time and then compensate the smoothed data errors by way of the formula at the navigation time. Both theoretical analysis and experimental results demonstrate that this method is able to cut down on computational time and raise the accuracy which makes it a better real-time compensation approach for periodic error terms of quartz micro electronic mechanical system （MEMS） gyroscope＇s zero drift.     

基于特征模型的火箭发动机伺服控制系统设计

以新型大推力火箭发动机为研究对象,提出了基于特征模型的伺服系统控制器设计方法。首先,介绍了特征建模理论并讨论了特征模型参数范围;其次,采用人工蜂群算法实时估计火箭发动机伺服系统特征模型参数,使其满足特征模型输出与实际系统输出特性等价条件;最后,使用黄金分割自适应控制律保证系统在参数估计过程中的闭环稳定性,同时引入前馈跟踪控制律,逻辑积分控制律和逻辑微分控制律使伺服控制系统快速、精确跟踪线位移指令并改善动态性能。仿真结果表明,设计的火箭发动机伺服控制系统指令跟踪精度高,动态特性良好,鲁棒性强。     

基于变刚度变阻尼的柔性喷管动态模型

针对柔性接头动态迟滞曲线受控制系统控制位置精度和动态响应速度影响较大的问题,基于电液伺服机构和柔性接头变刚度变阻尼模型,构建了柔性喷管的电液伺服机构-变刚度变阻尼模型,将其和电液伺服机构-定刚度定阻尼模型进行了对比。分析了电液伺服机构主要参数、柔性接头工作参数等对电液伺服机构-柔性接头系统动态特性的影响。分析结果表明:电液伺服机构-变刚度变阻尼模型所构造的迟滞曲线可更准确地与实验结果相吻合,并符合迟滞曲线随频率变化的规律,反馈系数、放大器静态放大系数、电液伺服机构增益、滑阀流量增益等参数对系统动态特性的影响更为明显。该模型为固体火箭发动机电液伺服机构-柔性接头系统动态特性的调整提供理论依据。     

多孔介质微燃烧器内的火焰驻定机理研究

为解释毫米尺度多孔介质燃烧器中火焰可在一个当量比范围内驻定的物理现象,搭建了二维非稳态数学物理模型,利用数值计算方法定性研究了氢气/空气预混气在部分填充不锈钢网的微通道内的火焰传播特性。通过分析浸没火焰及表面火焰的温度分布特点并量化燃烧室内的预热和散热发现：火焰驻定在多孔介质内的不同位置时对应的传热特性存在差异,是控制火焰传播速度在一定当量比范围内保持恒定的关键因素,而预热及散热的相对大小可作为衡量传热对火焰宏观影响的重要参数。对火焰的的总预热与总散热之比R越临近多孔介质入口边界变化越剧烈,导致浸没火焰易驻定在多孔介质的中上游区域;多孔介质对火焰的预热虽在多孔介质出口边界外减小,但与多孔介质散热之比Rp呈上升趋势,使得低流速工况下易形成表面火焰。同时,R随当量比的变化规律导致多孔介质下游火焰的稳定性相对较弱。     

Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan

Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5°N, 109.1°E; Geomagnetic coordinates: 178.95°E, 8.1°N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity.     

工艺参数对电弧增材制造2219铝合金微气孔缺陷的影响分析北大核心CSCD

微气孔是电弧增材制造2219铝合金面临的主要问题。采用Advanced CMT+P(变极性CMT+脉冲)熔滴过渡模式,研究了EP/EN(正负半周波数)、扫描速度、送丝速度等电弧增材工艺参数对成形2219铝合金微气孔缺陷的影响规律。结果表明:通过改变EP/EN、扫描速度、送丝速度等参数调控热输入可影响气孔率;在热输入较低时,气孔以形核和长大为主,随热输入增加微气孔数量增多、尺寸增大;在热输入较高时,气孔逸出开始占优,随热输入增加微气孔数量减少;在热输入低至230.5或高至439.5 J/mm时,平均气孔率均可降低至0.2%以下。     

GRACE gravity field modeling with an investigation on correlation between nuisance parameters and gravity field coefficients

The GRACE (Gravity Recovery And Climate Experiment) monthly gravity models have been independently produced and published by several research institutions, such as Center for Space Research (CSR), GeoForschungsZentrum (GFZ), Jet Propulsion Laboratory (JPL), Centre National d’Etudes Spatiales (CNES) and Delft Institute of Earth Observation and Space Systems (DEOS). According to their processing standards, above institutions use the traditional variational approach except that the DEOS exploits the acceleration approach. The background force models employed are rather similar. The produced gravity field models generally agree with one another in the spatial pattern. However, there are some discrepancies in the gravity signal amplitude between solutions produced by different institutions. In particular, 10%–30% signal amplitude differences in some river basins can be observed. In this paper, we implemented a variant of the traditional variational approach and computed two sets of monthly gravity field solutions using the data from January 2005 to December 2006. The input data are K-band range-rates (KBRR) and kinematic orbits of GRACE satellites. The main difference in the production of our two types of models is how to deal with nuisance parameters. This type of parameters is necessary to absorb low-frequency errors in the data, which are mainly the aliasing and instrument errors. One way is to remove the nuisance parameters before estimating the geopotential coefficients, called NPARB approach in the paper. The other way is to estimate the nuisance parameters and geopotential coefficients simultaneously, called NPESS approach. These two types of solutions mainly differ in geopotential coefficients from degree 2 to 5. This can be explained by the fact that the nuisance parameters and the gravity field coefficients are highly correlated, particularly at low degrees. We compare these solutions with the official and published ones by means of spectral analysis. It is found that our solutions are, in general, consistent with others in the spatial pattern. The water storage variations of the Amazon, Chari and Ganges river basins have also been computed. The variations computed with the NPARB approach are closer to those produced by JPL and DEOS solutions, while the variations produced with the NPESS approach are in good agreement with those produced by the CSR and GFZ solutions. A simulation study is implemented with considering realistic noise and low-frequency error. The two approaches are used to recover the true model. The NPESS solution appears closer to the true one. Therefore we are inclined to estimate the nuisance parameters simultaneously with the geopential coefficients.     

桁架结构的静动态特性有限元分析

通过对桁架结构的静、动态分析,探讨如何建立桁架的有限元模型及计算方法,并利用MSC．Patran／Nastran程序对该结构进行静、动态分析计算,计算结果与实际情况吻合。     

多孔层板换热特性实验研究

本实验选取了一种典型结构的多孔层板作为研究对象 ,进行了换热特性实验研究。研究了改变冷热气流吹风比对该型层板冷却效果的影响。另外 ,对该型多孔层板的冷却效果沿中轴线顺气流方向的变化规律也作了深入的研究。并给出了层板局部 N ux 和冷却效果 E关于局部 Rex 及冷热气流吹风比 M的数学拟合表达式。