相关噪声背景下相干信源DOA估计算法研究

根据信号和噪声的非圆对称特性,利用除第一个阵元外的其它阵元接收数据的共轭信息,对原阵列进行有效地扩展,提出了一种相关噪声背景下相干信源波达方向（DOA）估计的新算法。由于对阵列进行了虚拟扩展并运用斜投影算法将非相干信源与相干信源分开分辨,因此该算法具有很强的信源过载能力及阵元节省能力,在一定程度上提高了空间分辨率DOA估计的性能,并可对消空间具有非圆对称性的相关噪声,适用于低信噪比环境。仿真结果证明了算法理论的正确性和有效性。     

基于最大似然多径估计的卫星导航信号码跟踪算法与实现

卫星导航接收机需要精确的估计信号的扩频码相位并进行跟踪,估计的精度直接影响 伪距的测量精度。卫星信号的多径传播使得传统的基于DLL的估计器存在较大误差,提 出了一种抗多径的估计算法,它基于最大似然参数估计方法,并给出了该算法的推导过程, 仿真的结果表明该算法比传统的DLL跟踪环在性能上有很大的改进。结合传统卫星导 航接收机的实现结构,给出了一种整合了该算法的实现方案。     

Quasiperiodic oscillations of the sub-mHz band in near-sun plasma according to the coherent radio occultation data

In 2013 and 2015, investigations of the internal solar wind were carried out using the method of two-frequency radio sounding by signals from the Mars Express European spacecraft. The values of the S- and X-bands’ frequency and the differential frequency were registered with a sampling rate of 1s at the American and European networks of ground-based tracking stations. The spatial distribution of the frequency fluctuation’s level has been studied. It has been shown that the intensity of frequency fluctuation considerably decreases at high heliolatitudes. In some radio sounding sessions, quasiperiodic oscillations of sub-mHz band have been observed in the temporal spectra of frequency fluctuations; they are supposed to be associated with the density inhomogeneities, the sizes of which are close to the turbulence outer scale.     

Modes of uncontrolled rotational motion of the <Emphasis Type="Italic">Progress M-29M</Emphasis> spacecraft

We have reconstructed the uncontrolled rotational motion of the Progress M-29M transport cargo spacecraft in the single-axis solar orientation mode (the so-called sunward spin) and in the mode of the gravitational orientation of a rotating satellite. The modes were implemented on April 3–7, 2016 as a part of preparation for experiments with the DAKON convection sensor onboard the Progress spacecraft. The reconstruction was performed by integral statistical techniques using the measurements of the spacecraft’s angular velocity and electric current from its solar arrays. The measurement data obtained in a certain time interval have been jointly processed using the least-squares method by integrating the equations of the spacecraft’s motion relative to the center of mass. As a result of processing, the initial conditions of motion and parameters of the mathematical model have been estimated. The motion in the sunward spin mode is the rotation of the spacecraft with an angular velocity of 2.2 deg/s about the normal to the plane of solar arrays; the normal is oriented toward the Sun or forms a small angle with this direction. The duration of the mode is several orbit passes. The reconstruction has been performed over time intervals of up to 1 h. As a result, the actual rotational motion of the spacecraft relative to the Earth–Sun direction was obtained. In the gravitational orientation mode, the spacecraft was rotated about its longitudinal axis with an angular velocity of 0.1–0.2 deg/s; the longitudinal axis executed small oscillated relative to the local vertical. The reconstruction of motion relative to the orbital coordinate system was performed in time intervals of up to 7 h using only the angularvelocity measurements. The measurements of the electric current from solar arrays were used for verification.     

Design of Interplanetary Transfers with Passive Gravity Assists and Deep Space Maneuvers

In the paper, the problem of designing interplanetary trajectories with several swing-bys and deep-space maneuvers is solved using the method of virtual trajectories developed by the authors. The algorithms for the calculation of both heliocentric and planetocentric trajectory arcs are presented, including the case of resonant trajectories. The results of applying the method of virtual trajectories to the problem of designing an interplanetary transfer to Jupiter are given and compared with the baseline trajectories for the Juno, Europa Clipper, and Laplace missions.     

基于脉冲交错的数字阵列雷达任务优化调度算法

针对数字阵列雷达搜索、跟踪和成像任务的资源调度问题,提出一种数字阵列雷达(DAR)任务的优化调度算法。该算法以脉冲交错技术为基础,在对目标搜索与跟踪的同时,利用基于压缩感知的稀疏孔径认知逆合成孔径雷达(ISAR)成像方法对部分精密跟踪目标成像,并采用观测时间动态调整策略以提高雷达系统的自适应能力。仿真结果表明,与传统雷达资源调度算法相比,该算法可以将成像任务考虑到优化调度模型中并合理分配资源,实现雷达多任务并行的调度,获得更高的资源利用率与期望的成像质量。     

航空涡轮发动机燃烧室内流场的PIV测量

设计了一种基于旋风分离原理的高压粒子发生器,并成功应用于高压状态下的航空涡轮发动机燃烧室内流场的PIV（粒子图像测速法）测量.在氢氧燃烧加热来流温度为813K、燃烧室压力为2.78MPa条件下,应用PIV技术开展了航空涡轮发动机单头部燃烧室复杂内流场测量研究,实现了高温高压条件下强旋流、强扰流、宽速域流场的PIV测量,获得了接近燃烧室工作压力工况下的流场速度和流场精细结构.结果表明:该型燃烧室内流场存在多处旋涡结构,形成回流区;流场旋流作用强,横截面流场存在顺时针大涡;主燃孔射流和掺混孔射流作用明显,射流穿透深度较大,对流场结构影响显著;高温高压状态下,流场结构与常温中压状态类似.