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。     

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.     

The effects of the solar magnetic polarity and the solar wind velocity on Bz-component of the interplanetary magnetic field

We have studied the effect of both solar magnetic polarity and the solar wind velocity on the Bz-component of the interplanetary magnetic field, IMFBz, for the minimum activity of the solar cycles 21, 22, 23 and 24. We made a statistical study of IMFBz in the first section which is considered as an extension of Lyatsky et al. (2003). They made a statistical study of IMFBz for two periods of minimum solar activity 22 and 23 related to 1985–1987 and 1995–1997 when the solar magnetic field had opposite polarity. Our results seem to be consistent with the results obtained by Lyatsky et al. (2003). We found that there is a dependence of IMFBz on the IMFBx and the solar magnetic polarity for the minimum periods of the selected four solar cycles. In addition, we found that there is a dependence of IMFBz on the solar wind velocity.     

野战环境下大型飞机超低空气动特性分析

针对野战环境下的大型飞机超低空飞行,采用CFD方法对地面存在前向或横向不对称障碍物时地面效应对气动参数的影响进行了数值分析,包括纵向稳定性和侧向摇晃等问题.研究结果表明,野战等非常规飞行条件下,地面不确定障碍物会造成大型飞机稳定性变差,严重时可能出现纵向点头和横侧向摇晃现象,容易导致触地危险.最后,从现代飞行控制理论角度提出了对常规布局大型飞机进行闭环控制的研究思路.     

Subsidence rate monitoring of Aghajari oil field based on Differential SAR Interferometry

Land subsidence, due to natural or anthropogenic processes, causes significant costs in both economic and structural aspects. That part of subsidence observed most is the result of human activities, which relates to underground exploitation. Since the gradual surface deformation is a consequence of hydrocarbon reservoirs extraction, the process of displacement monitoring is amongst the petroleum industry priorities. Nowadays, Differential SAR Interferometry, in which satellite images are utilized for elevation change detection and analysis – in a millimetre scale, has proved to be a more real-time and cost-effective technology in contrast to the traditional surveying method. In this study, surface displacements in Aghajari oil field, i.e. one of the most industrious Iranian hydrocarbon sites, are being examined using radar observations. As in a number of interferograms, the production wells inspection reveals that surface deformation signals develop likely due to extraction in a period of several months. In other words, different subsidence or uplift rates and deformation styles occur locally depending on the geological conditions and excavation rates in place.     

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。     

位相物体的三维非对称温度场的重建

采用卷积背抽影公式实现了位相物体的三维非对称温度场的重建，为光线偏／折测量三维非对称温度场提供了高精度分析和处理实验数据的方法。     

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.     

大扫描视场飞行器共形光学系统设计

共形光学窗口外表面与飞行器轮廓相同,可以显著提升飞行器的整体性能,但在大扫描视场应用时,引入大量非对称动态像差,严重影响成像质量。针对大扫描视场的共形光学系统,提出了基于共形窗口内表面优化,以及分视场单元透镜阵列的动态像差校正方法,实现动态像差的静态化校正。在84°扫描视场范围内,对共形光学系统进行仿真验证,结果表明：该方法使共形光学系统在全扫描视场范围内的Zernike多项式系数绝对值从0~10.82λ减小到0~1λ（λ为波长）,同时各通道单元透镜阵列保持固定状态。与目前已有方法相比,本文显著提升了大扫描视场共形光学系统的成像质量和系统稳定性,有效简化了系统结构。本文的研究对实现大扫描视场、高成像质量和高稳定性的共形光学系统有重要意义。     

风洞T型冲击三通管道流场特性数值模拟

在24 m跨声速风洞进气管路T型冲击三通连接处和隔板位置,每隔一定时间会出现裂纹,影响了风洞的安全稳定运行。为了解裂纹出现的原因,同时为改进设计提供依据,采用CFD(computational fluid dynamics)对风洞现有三通和优化方案进行了对比。控制方程为三维黏性不可压缩Navier-Stokes方程。结果表明：无隔板时,三通内的流动为最常见的类型,支管内存在3个分离区,在转向过程中形成第1分离区,即马蹄涡;随后是第2分离区,一对反向旋转的旋涡,即Dean涡,及三通顶部壁面形成第3分离区。流场沿y=0 mm和z=0 mm平面基本呈对称分布。有隔板时,流场的左右和上下结构均不对称;在隔板和外侧壁面间的角点形成范围较小的驻涡,在支管内形成不稳定的螺旋状分离涡,致使气流振荡,从而使得三通连接和隔板处管壁出现裂纹。根据上述流态设计了管路优化方案和整流装置,优化后能有效减小或消除分离;其中去掉隔板最简单易行,可以解决裂纹的问题。