纹影干涉图的图像处理方法研究

本文利用计算机存贮量大、运算能力强的特点研究了一种分析纹影干涉图,计算密度场的图像算法。这套算法包括使用低通滤波技术消除干涉图背景中的高频噪声,使用 Hilditch 算法细化宽度多于一个像素的干涉条纹,使用模式识别方法提取干涉条纹的位移量,最后应用数值积分技术求解密度场的空间分布。这里研究的图像处理方法提高了纹影干涉图定量分析的精度、加快了实验结果的处理速度,给出了直观可靠的数值结果,是一种实用有效的图像算法。     

基于Ansys Fluent的近场翼尖涡数值模拟与分析

为了进一步研究飞机远场尾涡,提供网格分配及湍流模型的参考,并为整机模拟提供必要的参考依据,通过基于Ansys Fluent的数值模拟方法,研究了NACA0012机翼的近场翼尖涡流场,采用有限体积法求解不可压缩雷诺平均Navier-Stokes方程,其中雷诺应力项分别以S-A和Realizable k-ε模型封闭,模拟了近场翼尖涡卷起的过程,分析了机翼表面压力以及涡核参数,包括轴向涡量、涡核位置、涡核粘性等,并与风洞实验结果进行了对比。结果分析表明:基于局部O-网的六面体网格,RKE模型要优于S-A模型,与实验值更为吻合。     

一种高灵敏度的电动舵机系统研究

本文研究了一种基于单片机的高灵敏、分体式小型电动舵机系统。首先分析了电动舵机的组成与功能,并分别从舵机结构、控制算法两方面对舵机系统的性能设计进行了分析和阐述。针对舵机高灵敏度的性能要求,对控制算法进行了优化并进行了相应仿真。最后经过试验验证,电动舵机满足了高灵敏度的指标要求,验证了控制算法的正确性。     

内外分区空间统一精度场建立方法研究

针对内外分区空间内结构和设备安装的数字化测量需求,研究内外参考点之间的关联技术,构建与外测量精度场相统一的内测量精度场。对于内外空间不同的开口数,利用多测点定位法、二测点和水平仪单站位定位法、二测点和水平仪双站位定位法等方法建立内精度场,实现与外精度场的统一。以某型设备为例进行试验表明,利用内外精度场测量同一检测点进行比较,测量的最大不一致误差为0.14 mm,证明构建模式可行、简单、可靠。     

空空导弹惯性开关中圆周磁场对导弹性能的影响

为了提高空空导弹的作战效能和可靠性,由弹载电源向开关电路进行大电流放电,可提高惯性开关中圆柱电极上周磁场的强度,增强抵抗磁钢对钢珠反向作用力的能力,当导弹撞击目标过载较小时,使惯性开关的导通时间也能够满足触发电路工作需要,因此,导弹遇目标不炸的故障概率可得到下降。     

航天器表面电荷激发空间静电场规律研究

从带电表面微元出发,通过求解泊松方程,得到带电介质平板表面邻近空间静电势的解析表达式,建立介质表面电位-介电常数模型,求得了带电介质平板表面电位、表面带电量和介质介电常数三者之间的关系式。结合典型的航天器表面介质材料带电案例,对此类圆盘结构介质平板带电问题进行了仿真分析,结果表明,在介质材料表面电位一定的情况下,表面电荷激发的空间静电势值随距离的增大而减小,并且距离介质表面越近,电势的空间变化率越大;在介质材料带电量相等的情况下,介质表面电位随着介质介电常数的增大而减小,并逐渐趋于一个稳定值,所以在一定范围内选择介电常数较大的介质材料可以降低介质的表面电位,减小介质间发生静电放电的几率。     

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.     

The geomagnetic solar flare effect identified by SIIG as an indicator of a solar flare observed by GOES satellites

This paper studies the efficiency of geomagnetic solar flare effects (gsfe) in X solar flare detection; so during the period 1999–2007 a comparison between solar flare (sf) observed by satellites of the Geostationary Operational Environmental Satellite (GOES) programme and gsfe published by the Service International des Indices Geomagnetiques (SIIG) is made.     

新电位移边界条件下的压电介质断裂问题

应用边界元法,并结合一种特殊的复变函数基本解,研究了压电介质的断裂问题。由于该基本解完全遵循本构方程没有对电位移边界作假设,所以结论同非穿透性裂纹假设的结果有较大差异。通过计算表明,外加力载荷不但会引起裂纹尖端应力奇异性,也会引起电场奇异性,同样,外加电压也会引起裂纹尖端应力奇异性。     

气体自发光在高超声速流场显示中的应用

提出了利用高焓气体自发光作为高超声速流场显示的方法,介绍了在使用高焓运行的激波风洞中,对二维模型的高超声速绕流流场使用此种方法的初步结果,可观察到二维棱形柱的尾流和马赫波的相交。结果表明此种方法不需外加光源,对于结构限制无法设置透明部件的模型,无疑是简单可行的。