基于并行运算体系结构的星敏感器图像处理算法

采用FPGA构建星敏感器图像处理并行计算体系结构。星敏感器图像处理算法由高通滤波、星点提取和星点排序3个模块组成。高通滤波模块基于图像局部加窗计算阈值的方法,星点提取模块采用逐行扫描的计算方法,星点排序模块采用基数排序的计算方法。星敏感器图像处理算法基于四级流水并行计算体系结构,显著提高了星敏感器图像处理的效率和算法的可靠性。
     

热传导方程有限差分区域分裂：显—隐算法的注记

把Rodrigue和Wolitzer（1995）提出的一种新型显格式应用于热传导方程有限差分区域分裂算法的内边界点,并得到这类显—隐算法的收效性结果。新算法的逼近阶较好,而且较纯新型显式方法可以节省一倍左右的计算量。     

网格结构机上的并行填充算法

并行扫描转换算法,采用通过多边形顶点的扫描线对扫描转换区间进行划分,使划分在各个区域的子多边形都是梯形,这既在一定区域内保持了各种相关性,又消除了对奇点的处理,同时对梯形的扫描转换不需要求交计算而只进行增量计算,提高了扫描转换速度。     

喷管内流场并行计算方法研究

建立了基于区域分解的并行计算方法,将已有的后台阶喷管内流场三维ＴＶＤＭａｃ－Ｃｏｒｍａｃｋ显式格式的串行计算程序改造成为并行程序,获得了较高的并行加速比。并行计算结果同串行结果进行了对比,证明计算是成功的。     

数控机床切削力负载模拟器的显式力控制算法设计

为了对数控机床进行可靠性试验,设计了一种基于3P-(4S)并联机构的负载模拟器。基于PI反馈控制的显式力控制算法,并引入了模糊控制器,提高系统对不同加载误差的适应性。在控制系统中引入了力前馈控制器,提高控制系统的动态性能,减少实际加载力的滞后。同时,由于加载目标即机床主轴的进给运动轨迹未知,因此引入了主轴位置预测前馈以进行运动补偿,减少主轴运动所带来的干扰。最后设计并实施了静态与动态负载模拟试验,验证了所提控制算法的有效性。     

Testing the blast wave model with Swift GRBs

The complex structure of the light curves of Swift GRBs (e.g. superimposed flares and shallow decay) has made their interpretation and that of the blast wave caused by the burst, more difficult than in the pre-Swift era. We aim to constrain the blast wave parameters: electron energy distribution, p, density profile of the circumburst medium, k, and the continued energy injection index, q. We do so by comparing the observed multi-wavelength light curves and X-ray spectra of a Swift sample to the predictions of the blast wave model.     

航天器飞行控制仿真与平行系统

总结并分析了目前国内外航天器飞行控制仿真与平行技术的发展现状和任务需求,针对中国当前飞控仿真与平行系统的通用化和标准化不足的情况,提出了一种可组装的飞控仿真与平行系统的定义和系统架构,阐述了仿真与验证、决策与支持两个部分的设计方案,并通过嫦娥五号的飞控工作进行了检验,验证了系统的有效性。最后展望了未来航天器飞行控制仿真与平行技术的发展方向。     

An experimental investigation on static directional stability

A generic aircraft usually loses its static directional stability at moderate angle of attack (typically 20–30?). In this research, wind tunnel studies were performed using an aircraft model with moderate swept wing and a conventional vertical tail. The purpose of this study was to investigate flow mechanisms responsible for static directional stability. Measurements of force, surface pressure and spatial flow field were carried out for angles of attack from 0? to 46? and sideslip angles from ?8? to 8?. Results of the wind tunnel experiments show that the vertical tail is the main contributor to static directional stability, while the fuselage is the main contributor to static directional instabil-ity of the model. In the sideslip attitude for moderate angles of attack, the fuselage vortex and the wing vortex merged together and changed asymmetrically as angle of attack increased on the wind-ward side and leeward side of the vertical tail. The separated asymmetrical vortex flow around the vertical tail is the main reason for reduction in the static directional stability. Compared with the wing vortices, the fuselage vortices are more concentrated and closer to the vertical tail, so the yaw-ing moment of vertical tail is more unstable than that when the wings are absent. On the other hand, the attached asymmetrical flow over the fuselage in sideslip leads to the static directional instability of the fuselage being exacerbated. It is mainly due to the predominant model contour blockage effect on the windward side flow over the model in sideslip, which is strongly affected by angle of attack.     

对复杂平面连杆机构运动分析的研究

本文提出了用转化机构法进行单自由度复杂平面连杆机构的运动分析.基本思想是通过改变机构的原动件或机架或同时改变原动件和机架,以简化机构的运动分析.这种方法对常见的平面复杂连杆机构的运动分析非常有效,无需进行复杂的试凑或迭代.同时本文提出的这种解法有较为广泛的意义,对加深认识机构的组成以及对机构其它问题的研究都是+分重要的.     

Changes in radio emission from PSR J0737–3039B

The double pulsar system, J0737–3039, provides a unique probe of a pulsar magnetosphere due to its edge-on viewing geometry, a tight orbit and a significant rate of advance of the angle of periastron. In this paper, we report on the changes in radio emission from the long period pulsar in this system, J0737–3039B, over a period of 9 months. Observations of this system with Giant Metrewave Radio Telescope (GMRT) show that the duration of the first bright phase of the pulsar centered at 210° orbital longitude from the ascending node is shrinking. These observations will be useful to constrain the proposed models for this system.