太阳同步卫星双星组网维持策略

某准共面星座由两颗相位差为 180°的太阳同步卫星组成。在对其进行轨道维持时 ,需综合考虑相位差和地面轨迹范围两方面的限制。然而 ,由于这两颗卫星的轨道倾角存在差异 ,使得在轨道维持过程中不能同时满足相位差和地面轨迹的要求。为解决上述问题 ,本文提出了调整地面参考轨迹的方法 ,实践证明有效。     

Ground experiments of Chang’e-5 lunar regolith penetrating radar

The Lunar Regolith Penetrating Radar (LRPR) is an Ultra-Wideband (UWB) array-based Ground penetrating radar (GPR) onboard the lander of Chang’e-5 (CE-5) mission. The primary scientific objectives of the LRPR are to probe the thickness and structure of lunar regolith of the landing site, and support the drilling and sampling process. In order to evaluate the performance of the LRPR, a series of ground experiments are performed using the LRPR prototype mounted on a CE-5 lander model. The performance of the LRPR is evaluated by comparing the experimental data with the simulated data. Data processing and imaging method are verified, and the interferences from the lander and other aspects are analyzed. The results of the ground experiments and simulation demonstrate that the LRPR is able to meet the design requirement of 2-m detection depth. They also indicate that the upper and lower interfaces of the stratified structure in the lunar regolith can be well distinguished by the LRPR when the dielectric constant difference is greater than 0.3, and the imaging effect of the location under the dense antennas is better than that of other positions. However, the identification capability of the LRPR to the independent blocky objects is relatively poor mainly due to the clutters caused by the lander, the sparsity of the antenna elements compared to the size of the basalt block, the limited aperture of the antenna array, and the tail of the transmitted waveform.     

Neural adaptive control for a ground experiment of the space proximity operation in a six-degree-of-freedom micro-gravity simulation system

In this study, a neural adaptive controller is developed for a ground experiment with a spacecraft proximity operation. As the water resistance in the experiment is highly nonlinear and can significantly affect the fidelity of the ground experiment, the water resistance must be estimated accurately and compensated using an active force online. For this problem, a novel control algorithm combined with Chebyshev Neural Networks (CNN) and an Active Disturbance Rejection Control (ADRC) is proposed. Specifically, the CNN algorithm is used to estimate the water resistance. The advantage of the CNN estimation is that the coefficients of the approximation can be adaptively changed to minimize the estimation error. Combined with the ADRC algorithm, the total disturbance is compensated in the experiment to improve the fidelity. The dynamic model of the spacecraft proximity maneuver in the experiment is established. The ground experiment of the proximity maneuver that considers an obstacle is provided to verify the efficiency of the proposed controller. The results demonstrate that the proposed method outperforms the pure ADRC method and can achieve close-to-real-time performance for the spacecraft proximity maneuver.     

核热推进地面试验技术研究

核热推进具有比冲高、推力大等特点,在载人深空探测和星际货运任务上具有广阔应用前景。核热推进技术的研发需要进行大量地面试验。首先回顾了美国与俄罗斯的核热推进地面试验技术的发展,对地面试验技术进行分类总结。然后基于一种小型核火箭方案,研究了燃料元件非核试验、燃料元件辐照考验试验和带核整机地面试验等关键地面试验技术,并提出了初步试验方案。最后对我国核热推进地面试验的发展提出了一些建议。     

硝化纤维素溶液冰冻过程中的折光指数增量

用定量体积排斥色谱（ＳＥＣ）的方法,以示差折光检测器的响应为基础,测定了硝化纤维素溶液冰冻及其加热以后的折光指数增量。结果表明：冰冻后,由于分子链发生链内凝聚（缠结）,硝化纤维素分子链周围溶剂化溶剂分子数减少,使硝化纤维素溶液的示差折光指数增量增加。加热后,由于硝化纤维素分子链获得能量,链内缠结点解开,溶剂化溶剂分子数增加,造成硝化纤维素溶液的折光指数增量降低。由此建立了以折光指数增量为基础,估算硝化纤维素分子在溶液中完全伸展时每个链段上的溶剂化溶剂分子数的理论公式,并且估算出常温下每个硝化纤维素链段就吸附有１３个溶剂化溶剂分子,这对建立硝化纤维素这类半刚性高分子链凝聚过程和凝聚态结构的物理图像具有重要意义。     

卫星通信地球站站址勘测的研究

介绍了卫星通信地球站站址勘测技术要求;讨论了方位角与俯仰角计算,微波干扰电平允许值计算,微波干扰测试以及发射协调距离的估算;从而得出建站最必要的技术结论。     

地面检测设备中数字逻辑电路干扰的分析和抑制

为了提高电子设备的性能,数字逻辑电路的设计必须十分可靠,通常设计数字逻辑电路只研究输入和输出的静态逻辑关系,这样设计出来的电路有时不可避免会产生毛刺,这些毛刺是事先没有估计的,因为设计者缺乏对数字逻辑电路过渡过程的考虑。本文提出了一种实用毛刺判别法,利用转移值表的方法分析一类时序电路,并从几个实例说明转移值法能够事先判别毛刺存在与否,使设计更加完善。本文还分析了开关对逻辑电路产生干扰的原因和抑制方法。并讨论了抑制毛刺的实用方法,指出竞争的可利用性。     

星间链路天线相对姿态的地面模拟

星间链路天线的相对姿态模拟为星间链路的测试验证提供近真实的动态姿态环境,是星间链路系统地面测试的重要组成部分。建立多个坐标系统将两颗卫星天线的位置和姿态联系起来,利用卫星星历将天线的相对姿态表示为一颗卫星天线在另一颗卫星天线坐标系中的方向向量,利用两个二轴转台实现此方向向量,最终通过控制转台的转角模拟卫星天线的相对姿态变化。同时计算天线波束的方向,分析了两颗卫星的可见性。天线相对姿态的模拟为星间链路的建立和保持提供动态测试环境。     

直连式喷气发动机试车台试验件进气的联接方式及有关问题

针对直连式喷气发动机试车台稳定段同试验件的联接问题，根据空气流量测量、补氧及推力测量等不同试验目的与要求，讨论了选择联接方案对试验结果的影响。结果认为，模拟总温较高时，音速喷嘴流量测量联接方式应慎重选用；采用能够测量进、出口压力的迷宫密封方式，可以根据喷嘴及回绕式阻隔件流动理论计算出空气泄漏量并可测出压力损失值，从而对试验所要求的补氧量及推力测量提供较准确的修正。     

Kink mode m = 1 in magnetic tube with discontinuous magnetic field

In this paper, we study conditions of realization and stability of kink modes with azimuthal wave numbers $m=\pm 1$ in cylindrical plasma flex with twisted magnetic field and homogeneous current along its axis. We assume permanent axial magnetic field both inside and outside the flex, surrounded by currentless plasma. Azimuthal magnetic field decreases inversely proportional to the distance from the boundary beyond the flex. We derived dispersion equations for stable and unstable modes in approximation of “thin” plasma flex. The analysis of equations has been provided for the case of discontinuous axial magnetic field on flex’s boundary. Conditions of propagation of wave modes have been defined. It was shown, that unstable modes can be implemented in certain interval of longitudinal wavenumbers. Results can be applied for the interpretation of solar magnetic tubes behavior, using measurements, provided by spacecrafts.