旋转状态下S型带肋通道流动特性数值研究

为了更好地了解涡轮叶片内冷完整通道中流体的流动特性,数值研究了肋、转弯以及旋转对完整S型带肋通道流动特性的影响.雷诺数为17000,3个出口的出流比分别为27%,49%,24%,旋转数取0,0.03,0.06,0.09.结果表明:通道1靠近前缘侧阻塞比高,肋的扰流作用强,流体速度较低.转弯引起流体流动分离,使转弯下游通道中的主流发生偏移,通道3靠近分隔板侧存在较大范围低速区.旋转产生的切向哥氏力使流体向哥氏力指向面偏移,通道2与通道3主流分别偏向吸力面与压力面.旋转影响通道中二次流的分布,增强转弯下游低速回流涡区域流体的流动.      

基于MFT的非匀速转动目标干涉ISAR三维成像方法

非匀速转动目标各距离单元内的回波信号为多分量的多项式相位信号,采用傅里叶变换进行横向压缩得到的目标ISAR像会发生散焦,从而影响干涉ISAR三维成像质量。针对非匀速转动目标,提出了一种基于匹配傅里叶变换的InISAR三维成像方法。该方法对各天线接收回波的每个距离单元采用匹配傅里叶变换得到聚焦的目标ISAR像,进而得到散射点不同接收天线间的干涉相位,最后从干涉相位求解散射点三维位置重构目标的三维图像。由于非匀速转动目标多项式相位信号的相位系数之间的比值只与目标转动参数有关,因此该方法只需估计某一个散射点对应回波的多项式相位系数就可构造所有匹配傅里叶变换的积分路径,而且适用于任意阶的非匀速转动目标。仿真表明了该方法的有效性。     

“资源三号”卫星三线阵影像几何质量分析

文章首先简要叙述了基于＂资源三号＂（ZY-3）卫星三线阵TLC影像的严格几何成像模型,然后建立了针对外方位角元素的系统误差补偿模型与相机视向量几何检校模型。经地面系统检校后,采用地面高精度控制点数据对非同时相影像进行试验,并对影像平面精度进行分析评价。结果显示ZY-3三线阵TLC影像无控制点状态下外部定位精度优于6像元,内部几何变形优于1.5像元。     

单轴旋转式光纤陀螺惯导系统误差特性研究

通过对单轴旋转式光纤陀螺惯导系统误差特性进行研究,从理论上分析了旋转对系统中各个误差因素的影响。由分析结果知旋转调制对光纤陀螺输出的高频随机噪声不具有补偿效果;陀螺安装误差对导航系统精度的影响主要表现为与旋转运动之间耦合产生的周期性误差;由于单轴旋转需要引入规律性的旋转运动,不恰当的旋转方式会导致系统误差的放大。最后对以上结论进行了仿真研究和试验验证。     

Exponential Time-varying Sliding Mode Control for Large Angle Attitude Eigenaxis Maneuver of Rigid Spacecraft

An eigenaxis maneuver strategy with global robustness is studied for large angle attitude maneuver of rigid spacecraft. A sliding mode attitude control algorithm with an exponential time-varying sliding surface is designed, which guarantees the sliding mode occurrence at the beginning and eliminates the reaching phase of time-invariant sliding mode control. The proposed control law is global robust against matched external disturbances and system uncertainties, and ensures the eigenaxis rotation in the presence of disturbances and parametric uncertainties. The stability of the control law and the existence of global siding mode are proved by Lyapunov method. Furthermore, the system states can be fully predicted by the analytical solution of state equations, which indicates that the attitude error does not exhibit any overshoots and the system has a good dynamic response. A control torque command regulator is introduced to ensure the eigenaxis rotation under the actuator saturation. Finally, a numerical simulation is employed to illustrate the advantages of the proposed control law.     

机翼带外挂系统极限环颤振的区间分析

针对带有初偏间隙型非线性刚度的二元翼带外挂系统的极限环颤振,应用当量线化方法得出了颤振边界曲线,并根据颤振边界曲线用4阶Runge-Kutta法得到极限环相图,可明显看出极限环振动与普通周期振动的区别。然后引入了几个不确定量,通过区间分析方法给出了这些不确定量对机翼带外挂系统颤振边界曲线的影响,并用随机有限元法(FEM)验证区间分析方法的可靠性。进而可以得到一定来流速度下,具有不确定机翼外挂系统幅值的上下界,以及不确定参数对极限环相图的影响。知道机翼外挂幅值的上下界后,可以对外挂幅值进行适当控制。     

Apparent rotation properties of space debris extracted from photometric measurements

Knowledge about the rotation properties of space debris objects is essential for the active debris removal missions, accurate re-entry predictions and to investigate the long-term effects of the space environment on the attitude motion change. Different orbital regions and object’s physical properties lead to different attitude states and their change over time.Since 2007 the Astronomical Institute of the University of Bern (AIUB) performs photometric measurements of space debris objects. To June 2016 almost 2000 light curves of more than 400 individual objects have been acquired and processed. These objects are situated in all orbital regions, from low Earth orbit (LEO), via global navigation systems orbits and high eccentricity orbit (HEO), to geosynchronous Earth orbit (GEO). All types of objects were observed including the non-functional spacecraft, rocket bodies, fragmentation debris and uncorrelated objects discovered during dedicated surveys. For data acquisition, we used the 1-meter Zimmerwald Laser and Astrometry Telescope (ZIMLAT) at the Swiss Optical Ground Station and Geodynamics Observatory Zimmerwald, Switzerland. We applied our own method of phase-diagram reconstruction to extract the apparent rotation period from the light curve. Presented is the AIUB’s light curve database and the obtained rotation properties of space debris as a function of object type and orbit.     

快速精确调节稳频点的远共振线激光稳频方法

原子磁强计、激光冷却等技术需要将激光频率稳定在远离原子跃迁频率几兆赫兹的大失谐处,法拉第旋光光谱稳频方法能够实现远共振线的大失谐处的稳频,但是存在稳频点调节不便的问题。在法拉第旋光光谱稳频方法的基础上进行改进,提出了一种快速精确调节稳频点的远共振线激光稳频方法,能够在几十至几百兆赫兹范围内对稳频点频率进行快速精确的调节。基于该方法使失谐为-6.2 GHz的稳频点精确频移130 MHz,并实现频率漂移3.3 MHz/h,波动均方根值0.6 MHz/h的激光频率稳定度,满足原子磁强计对失谐及频率稳定性的要求。另外,分析了温度对该稳频方法的影响,推导了预估稳频点频率的物理参数,并将温度调节和声光调制器（AOM）调节相结合,以更好地实现在远共振线大失谐处对激光频率的长期稳定和精确控制。      

红外灯热流分布试验研究

文章采用蒙特卡罗法建立了红外灯单灯热流分布模型并在真空低温环境下进行了红外灯热流分布测试,以验证模型的准确性。测试在KM2空间环境模拟器中进行,采用黑片作为热流传感器。测试过程避免了空气对流对测试的影响,确保了测试数据的准确。对比分析表明,模型计算结果与实测结果偏差在5%以内,满足设计要求,可以作为红外灯阵热流分布模型的建立和红外灯阵热流优化的基础。     

地球自转对光机扫描仪摆扫成像的影响分析

地球自转会影响地物相对光机扫描仪的运动。不同纬度的地速不同,地速的变化会造成扫描条带畸变、相邻条带错动和重叠率的变化。文章研究了地球自转的变化规律,从扫描条带畸变、相邻条带错动和重叠率变化3方面因素研究了地速对光机扫描仪成像的影响。最后,针对这些影响提出了校正建议。