定速拉伸的固体推进剂双轴板条的应力分析

对固体推进剂双轴板条试件进行了有限元分析，并考虑了粘弹性对应力结果的影响，分析结果表明，双轴板条试件中心域为平面应变状态，与发动机药柱中部内孔表面相似，并给出了计算杨氏模量所需的修正系数。     

刚弹性复杂系统在重力场中的定点转动

本文研究了轴对称刚－弹系统在重力场中的定点运动。首先利用模态分析方法将偏微分方程转化为常微分方程组，然后引进小参数将藕合的长周期运动和短周期运动分离。得到了这个非线性刚弹藉合系统的一次近似解，并利用它研究了刚－弹系统运动特性。     

统计滤波理论在飞行器制导系统中的应用

本文叙述了统计滤波方法中具有典型代表性的卡尔曼滤波的基本方法。简要说明了它在惯性平台的自对准与自校准;复合制导中的信息综合以及飞行试验后的误差分离和弹道参数最佳估计中的应用。指出了应用中尚存的问题及今后的可能发展。     

固体火箭发动机点火过程内流场的二维预示

本文对固体火箭发动机点火过程的内场流进行了二维无粘非定常分析，计算得到了该阶段燃烧室中压强，温度和速度的分布。本文还提出了以近似预示复杂三维装药发动机内流场的有效积法。     

Production of neutrons from interactions of GCR-like particles

In order to help assess the risk to astronauts due to the long-term exposure to the natural radiation environment in space, an understanding of how the primary radiation field is changed when passing through shielding and tissue materials must be obtained. One important aspect of the change in the primary radiation field after passing through shielding materials is the production of secondary particles from the breakup of the primary. Neutrons are an important component of the secondary particle field due to their relatively high biological weighting factors, and due to their relative abundance, especially behind thick shielding scenarios. Because of the complexity of the problem, the estimation of the risk from exposure to the secondary neutron field must be handled using calculational techniques. However, those calculations will need an extensive set of neutron cross section and thicktarget neutron yield data in order to make an accurate assessment of the risk. In this paper we briefly survey the existing neutron-production data sets that are applicable to the space radiation transport problem, and we point out how neutron production from protons is different than neutron production from heavy ions. We also make comparisons of one the heavy-ion data sets with Boltzmann-Uehling-Uhlenbeck (BUU) calculations.     

航天飞行器防热部件烧蚀行为的数值模拟

对航天飞行器防热部件在氧－煤油发动机火焰喷吹下的烧蚀行为进行了有限元数值模拟。利用“杀死”单元的方法建立防热部件瞬态温度场的有限元模型，实现了烧蚀边界的退缩，从而完成了对烧蚀尺寸变化的定量描述。烧蚀开始于4．59s，到12s时线烧蚀量为1．47mm。计算结果与试验的实测结果一致。     

LISA — a study of the ESA cornerstone mission for observing gravitational waves

The primary objective of the Laser Interferometer Space Antenna (LISA) mission is to detect and observe gravitational waves from massive black holes and galactic binaries in the frequency range 10⁻⁴ to 10⁻¹ Hz. This low-frequency range is inaccessible to ground-based interferometers because of the unshieldable background of local gravitational noise and because ground-based interferometers are limited in length to a few km. LISA is an ESA cornerstone mission and recently had a system study (Ref. 1) carried out by a consortium led by Astrium, which confirmed the basic configuration for the payload with only minor changes, and provided detailed concepts for the spacecraft and mission design. The study confirmed the need for a drag-free technology demonstration mission to develop the inertial sensors for LISA, before embarking on the build of the flight sensors. With a technology demonstration flight in 2005, it would be possible to carry out LISA as a joint ESA-NASA mission with a launch by 2010 subject to the funding programmatics. The baseline for LISA is three disc-like spacecraft each of which consist of a science module which carries the laser interferometer payload (two in each science module) and a propulsion module containing an ion drive and the hydrazine thrusters of the AOCS. The propulsion module is used for the transfer from earth escape trajectory provided by the Delta II launch to the operational orbit. Once there the propulsion module is jettisoned to reduce disturbances on the payload. Detailed analysis of thermal and gravitational disturbances, a model of the drag-free control and of the interferometer operation confirm that the strain sensitivity of the interferometer will be achieved.     

飞行器姿态系统变结构控制的研究

对于具有纯延迟、惯性和由开关控制的非线性飞行器姿态系统，本文提出了采用解耦变结构控制的方法。计算机仿真结果表明，本方法行之有效，具有优良的鲁棒性，设计方法简单和易于实现数字控制等优点     

轴对称横向喷流强干扰流场的巨型机向量并行计算

本文在国产巨型计算机ＹＨ－１和ＹＨ－２上对ＭａｃＣｏｒｍａｃｋ显格式解轴对称横向喷流强干扰流场的计算程序进行了重构和向量优化使其能并行执行。得到该程序在ＹＨ－１上的向量加速比约为６．０，ＹＨ－２单机向量运行速度约为ＹＨ－１上的向量运行速度的３倍。与传统的串行计算相比较，并行计算大大缩短了程序运行的ＣＰＵ时间。     

ZN3火箭姿态测量用太阳角计

本文给出了用于ＺＮ３火箭姿态测量太阳角计的原理和测量结果，讨论了背景抑制和标定方法，分析了误差来源。该仪器采用选取适当探测波段和比值测量方法较好地消除了地外太阳辐照和大气消光的影响，也有效地抑制了背景辐射的干扰，大大提高了测量精度。实测结果表明，火箭姿态角测量的均方根误差约为０．７°。这一方法适用于各种自旋稳定飞行器的姿态测量。