基于TheoH方差的陀螺随机误差系数动态提取

针对运用动态Allan方差提取陀螺随机误差系数时,用截断窗截取原始信号造成方差估计置信度降低的问题,提出运用混合理论方差(Theo H方差)来代替Allan方差对截断窗内的数据进行分析,并提取出随时间变化的陀螺随机误差系数。Theo H方差改善了Allan方差计算时相关时间只能达到信号总时间的二分之一及长相关时间下方差估计置信度降低的问题,其计算的相关时间可以达到数据总时间的四分之三,有效改善了动态算法因数据截取造成误差系数估计置信度下降的缺陷。从对仿真信号和光学陀螺实测数据处理结果上来看,本文方法既能准确地对动态条件下陀螺量测信号的随机误差进行细化辨识,又能大幅提高中、长相关时间下方差估计的置信度。     

弹道靶中超高速发射弹的流场及空气动力特性研究(英)

本文描述的是研究爆炸成型发射弹（ＥＦＰ）模型的流场及超高速空气动力特性所用的弹道试验设备;简要报导了记录全尺寸干涉图形的技术;对径向密度分布再现的方法进行了讨论;在零攻角实验时不同模型的空气动力阻力是采用简化方法来计算的;对各种不同ＥＦＰ型式的气动稳定性提出了定性估计的方法;并阐述了用于组合体超高速飞行特性研究的数值计算技术的基本原理     

Measurement of mass diffusion coefficients of O_2 in aviation fuel through digital holographic interferometry

The experimental apparatus to measure the mass diffusion coefficients of O2 in aviation fuel was constructed based on the digital holographic interferometry method. The theory of mass diffusion coefficient and interference image processing were introduced in detail. The accuracy of the experiment was verified by measuring the mass diffusion coefficient of 0.33 mol/L KCl in aqueous solution at 298.15 K. The mass diffusion coefficients of O_2 in RP3 and RP5 aviation fuels were measured at temperature from 278.15 K to 333.15 K, and the Arrhenius equation was employed to fit the experimental data. In terms of the Stokes-Einstein equation, the viscosities of these two aviation fuels were tested to estimate the correlation among mass diffusion coefficient, viscosity and temperature. A uniform polynomial calculation correlation was proposed to predict the mass diffusion coefficients of O_2 in both RP3 and RP5 aviation fuels, and its accuracy is considerably higher than that of the Stokes-Einstein equation.     

双功能陶瓷膜生物反应器处理污水的实验研究

针对目前膜生物反应器运行过程中膜易污染的问题，研制了一种新型的双功能陶瓷膜生物反应器．该生物反应器的主要特点是采用一种具有双重功能的陶瓷膜作为生物反应器的主要元件，陶瓷膜可以交替地进行曝气和过滤，将膜的在线反冲清洗和生物反应器的供氧曝气结合在一起．考察了不同运行条件下该反应器对COD、氨氮的去除效果．对陶瓷膜的充氧能力进行了实验，测得小孔陶瓷膜、大孔陶瓷膜、砂型曝气头的氧传递系数分别为：0．2315min-1，0．1587min-1，0．0991min-1．     

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.     

Time-dependent cosmic ray modulation

Time-dependent cosmic ray modulation is calculated over multiple solar cycles using our well established two-dimensional time-dependent modulation model. Results are compared to Voyager 1, Ulysses and IMP cosmic ray observations to establish compatibility. A time-dependence in the diffusion and drift coefficients, implicitly contained in recent expressions derived by , ,  and , is incorporated into the cosmic ray modulation model. This results in calculations which are compatible with spacecraft observations on a global scale over consecutive solar cycles. This approach compares well to the successful compound approach of Ferreira and Potgieter (2004). For both these approaches the magnetic field magnitude, variance of the field and current sheet tilt angle values observed at Earth are transported time-dependently into the outer heliosphere. However, when results are compared to observations for extreme solar maximum, the computed step-like modulation is not as pronounced as observed. This indicates that some additional merging of these structures into more pronounced modulation barriers along the way is needed.     

空间群Pn3mPn3P23子群链耦合系数的计算

本文利用陈金全教授的本征函数法计算了Pn3m Pn3 P2 3空间群的母分系数。最后的计算结果表明 ,用陈金全教授的本征函数法所求得的母分系数确实满足幺正、归一性 ,同时也证明了本征函数法对于求母分系数同样适用     

求解非定常空气动力系数主导极点的近似方法

在计算与风洞实验的基础上, 提出了机翼剪切翼梢气动布局, 对平面形状与翼型进行了 优化设计, 达到了巡航状态与爬升阶段较高的增升减阻要求。计算采用涡格面元法与涡升力展向 分布吸力比拟法相结合的方法, 既能考虑气动力的非线性因素, 又有较高的计算精度与速度。计 算结果与实验数据十分吻合。通过分析得到, 在矩形翼翼梢处增加具有较大前缘后掠角的梯形剪 切翼梢有不仅增加机翼展弦比, 且可改变展向环量分布, 使其接近椭圆分布; 剪切翼梢上的前缘 涡可抑制翼端涡的作用(使翼端涡强度变弱) , 并在剪切翼梢上产生附加升力。     

弹射过程座舱盖抛放轨迹的预测

通过分析座舱盖在各个不同抛放阶段的受力关系,并着重考虑了抛放过程中气动系数的修正和铆钉剪切的影响,最终建立了座舱盖抛放轨迹的预测模型.该模型可广泛用于预测不同型号座舱盖在各种飞行状态下的抛放轨迹.算例表明计算结果与实验数据一致,证明了模型的实用性和有效性.     

Effects of sintering temperature and time on defect evolution and compression properties of Ti-Al3Ti laminated composites

For metal-intermetallic laminated composites, various types of defects often occur during the preparation process. This paper studied the evolution and formation mechanism of defects,such as pores, tunnel cracks, and delamination cracks in Ti-Al₃Ti laminated composites prepared by vacuum hot-pressing method. Moreover, quasi-static and dynamic compression tests were performed to study the effects of pores and delamination cracks on the compression properties of the composites. The resu...