飞月轨道引力捕获设计方法研究

利用太阳引力摄动与月球绕飞设计的地月转移轨道（飞月轨道），与霍曼转移相比，虽然飞行时间较长（约三、四个月），但可显著节省速度增量（可达１５０米／秒），对无人月球探测器尤为适合。应用平面圆型限制性四体问题动力学模型，选择从月球出发的初始条件。借助“地心距－时间曲线”，从平面圆型限制性四体问题转换为一般的限制性四体问题。通过典型模拟计算，分析负向积分（从月球轨道出发）初始轨道参数及太阳方位对月球探测器     

Biaxial Mode of Rotation of a Satellite in the Orbit Plane

A mode of motion of a satellite with respect to its center of mass is studied, which is called the biaxial rotation in the orbit plane. In this mode of rotation, an elongated and nearly dynamically symmetric satellite rotates around the longitudinal axis, which, in turn, rotates around the normal to the plane of an orbit; the angular velocity of rotation around the longitudinal axis is several times larger than the orbital angular velocity, deviations of this axis from the orbit plane are small. Such a rotation is convenient in the case when it is required to secure a sufficiently uniform illumination of the satellite's surface by the Sun at a comparatively small angular velocity of the satellite. The investigation consists of the numerical integration of equations of the satellite's motion, which take into account gravitational and restoring aerodynamic moments, as well as the evolution of the orbit. At high orbits, the mode of the biaxial rotation is conserved for an appreciable length of time, and at low orbits it is destroyed due to the impact of the aerodynamic moment. The orbit altitudes and the method of constructing the initial conditions of motion that guarantee a sufficiently prolonged period of existence of this mode are specified.     

纤维增强陶瓷基复合材料中纤维增韧分析模型

对于单向纤维增强陶瓷基复合材料，在考虑纤维桥联和纤维拔出两种主要增韧机理的基础上，建立了研究紧凑拉伸试样断裂行为的理论模型，并利用该模型计算了裂纹扩展的Ｒ－阻力曲线和载荷／位移曲线，计算结果表明：由于纤维桥联与拔出，使得Ｒ－曲线和载荷／位移曲线呈现明显的非线性行为，纤维桥联是主要增韧机制。体积分数５０％ＳｉＣ１／ＬＡＳ复合材料断裂韧性的计算值与实验值吻合。     

铅化合物在双基推进剂燃烧过程的作用机理

本文提出了铅化合物催化双基推进剂燃烧的反应历程。充分说明这类化合物是最终通过提高燃烧表面处嘶嘶区温度梯度提高燃速的。本文还提出了“铅化合物有通过增加燃烧表面上碳质物量增加燃速的一面,还有通过减少碳质物抑制燃速增加的一面”这一新的论点及抑制碳质物增加的反应并阐明了压力对这种抑制能力的影响。最后根据本文提出的作用机理及传热原理圆满解释了超速、平平和/或麦撒效应。     

Statistical Relationships between Solar,Interplanetary, and Geomagnetic Disturbances, 1976–2000: 3

In this paper we continue the analysis of the influence of solar and interplanetary events on magnetic storms of the Earth that was started in [9, 10]. Different experimental results on solar-terrestrial physics are analyzed in the study and the effects are determined that arise due to differences in the methods used to analyze the data. The classifications of magnetic storms by the K _p and D _st indices, the solar flare classifications by optical and X-ray observations, and the classifications of different geoeffective interplanetary events are compared and discussed. It is demonstrated that quantitative estimations of the relationships between two types of events often depend on the direction in which the events are compared. In particular, it was demonstrated that the geoeffectiveness of halo CMEs (that is, the percentage of Earth-directed coronal mass ejections that result in geomagnetic storms) is 40–50%. Higher values given in some papers were obtained by another method, in which they were defined as the probability of finding candidates for a source of geomagnetic storms among CMEs, and, strictly speaking, these values are not true estimates of the geoeffectiveness. The latter results are also in contrast with the results of the two-stage tracing of the events: first a storm—an interplanetary disturbance, and then an interplanetary disturbance—a CME.     

新一代多光谱扫描仪高效率线性扫描系统研制

文章根据新一代多光谱扫描仪的总体技术要求,重点介绍了高效率线性扫描控制系统的设计实现。     

固体火箭发动机性能精度分析

根据固体火箭发动机内弹道计算模型，提出了内弹道计算中的独立随机变量，建立了随机变量的概率统计模型，确定了参数的分布规律，并用Ｍｏｎｔｅ—Ｃａｒｌｏ法进行了内弹道模拟计算。最后对发动机性能的均值。和标准差σ进行了分析和实验验证，得出了计算方法可行，数据可信的结论。     

固体火箭发动机喉衬材料

介绍和综合了固体火发动机机喉衬用主要材料，包括难熔金属，石墨等，并比较了其优缺点及适用范围，给出了这些材料的热震与烧蚀性能的一些研究进展。     

在轨运行热环境下的天线镜面热变形对空地激光通信链路的影响

针对光学天线镜面热变形对空地激光通信链路性能产生影响的问题进行了理论和仿真分析。采用ANSYS有限元分析软件仿真得到的结果表明：低轨卫星在轨运行热环境条件下，采用潜望式结构且暴露在卫星舱外的光学天线反射镜镜面热变形将导致天线镜面法向偏转，其偏转量在不能释放热应力条件下可达几十μrad量级，经其传输的光束将产生较大的指向偏差；对所提出的释放热应力效果较好的天线镜体安装方式进行的相应分析表明：镜面变形受到镜体固定方式的影响非常大，在一定的参数条件下，和压板法固定方式相比较，压圈固定方式受到热变形影响形成的法向角度偏转较小。