高超声速小钝锥尾流化学非平衡辐射研究

本文主要目的是研究化学非平衡对高超声速小钝锥尾流辐射的影响。计算结果表明：激发发射辐射比化学发光辐射重要，红外辐射比可光辐射重要。结果还表明：由化学非平衡瞬时辐射模型计算求得的ＮＯ５．３μ的辐射能比由局部平衡辐射模型求得的辐射能大３０￣７０％。由此可知，小钝锥尾流的化学非平衡辐射模型对辐射的影响是不能忽略的。     

碳纤维增强陶瓷基复合材料抗氧化涂层研究进展

对碳纤维增强陶瓷材料抗氧化涂层的要求、组成与制备工艺以及最近抗氧化涂层体系的发展做了综述。并且对今后抗氧化涂层的发展作了一些展望。     

位置度测量最小二乘评定

就测量中无中心基准和无角向要求的位置评定问题，运用最小二乘法则对测量数据进行了误差分离优化评定，使此类位置度评定的稳定性和一致性得到改善。     

面外云纹法与相位法关系的研究

采用光学傅立叶函数分析法，论述了面外云纹法和相位法曲面三维测量的基本原理，深入研究了二者之间的本质联系，分析了这两种方法在曲面全场、无接触三维测量过程中的应用特点。     

低速风洞横向开槽壁试验段性能的研究

为探索减小洞壁干扰的试验方法，用环境风洞做了二维横向开槽壁试验段性能的试验研究。槽壁由等宽度薄板条在相对模型的两侧壁以零攻角等间距排放而构成，通过测量圆柱模型周向的表面压力对槽板宽度、驻室深度、试验段长度，模型在试验段中的轴向位置等与槽壁试验段性能有关的参量做了试验研究。模型堵塞比一直到０．２５的试验结果与无干扰的参考曲线符合良好，结果表明低速横向开槽壁具有洞壁干扰小且结构简单的特点。     

Stochastic Dynamic System Suboptimal Control with Uncertain Parameters

The control of a linear system with random coefficients is studied here. The cost function is of a quadratic form and the random coefficients are assumed to be partially observable by the controller. By means of the stochastic Bellman equation, the optimal control of stochastic dynamic models with partially observable coefficients is derived. The optimal control is shown to be a linear function of the observable states and a nonlinear function of random parameters. The theory is applied to an optimal control design of an aircraft landing in wind gust.     

9. The venus ionosphere and solar wind interaction

The current state of knowledge of the chemistry, dynamics and energetics of the upper atmosphere and ionosphere of Venus is reviewed together with the nature of the solar wind-Venus interaction. Because of the weak, though perhaps not negligible, intrinsic magnetic field of Venus, the mutual effects between these regions are probably strong and unique in the solar system. The ability of the Pioneer Venus Bus and Orbiter experiments to provide the required data to answer the questions outstanding is discussed in detail.     

Multipath-adaptive GPS/INS receiver

Multipath interference is one of the contributing sources of errors in precise global positioning system (GPS) position determination. This paper identifies key parameters of a multipath signal, focusing on estimating them accurately in order to mitigate multipath effects. Multiple model adaptive estimation (MMAE) techniques are applied to an inertial navigation system (INS)-coupled GPS receiver, based on a federated (distributed) Kalman filter design, to estimate the desired multipath parameters. The system configuration is one in which a GPS receiver and an INS are integrated together at the level of the in-phase and quadrature phase (I and Q) signals, rather than at the level of pseudo-range signals or navigation solutions. The system model of the MMAE is presented and the elemental Kalman filter design is examined. Different parameter search spaces are examined for accurate multipath parameter identification. The resulting GPS/INS receiver designs are validated through computer simulation of a user receiving signals from GPS satellites with multipath signal interference present The designed adaptive receiver provides pseudo-range estimates that are corrected for the effects of multipath interference, resulting in an integrated system that performs well with or without multipath interference present.     

快速凝固Al88Ce2Ni7Fe3非晶铝合金初生型晶化的研究

用X光衍射和透射电镜研究证实快速凝固Al88sCe2Ni7Fe3非晶铝合金晶化过程中的初期阶段为初生型晶化。初生相α－Al的结晶体积分数和纳米晶体尺寸随退火温度的升高表现出非同步增长行为：前者逐渐增加而后者变化不明显。不同退火态样品的小角X光散射结果表明，非晶基体中不断析出的纳米晶α－Al粒子，由开始的低温稀疏分布转向高温密集分布。根据实验结果，分析和讨论初生相α－Al的体积分数、晶粒数目、粒子尺寸及粒子分布在初生型晶化过程中的变化规律，为纳米晶α－Al粒子强化非晶基体提供了清晰的物理图像。     

Hydra — A 3-dimensional electron and ion hot plasma instrument for the POLAR spacecraft of the GGS mission

HYDRA is an experimental hot plasma investigation for the POLAR spacecraft of the GGS program. A consortium of institutions has designed a suite of particle analyzers that sample the velocity space of electron and ions between 2 keV/q – 35 keV/q in three dimensions, with a routine time resolution of 0.5 s. Routine coverage of velocity space will be accomplished with an angular homogeneity assumption of 16°, appropriate for subsonic plasmas, but with special 1.5° resolution for electrons with energies between 100 eV and 10 keV along and opposed to the local magnetic field. This instrument produces 4.9 kilobits s^–1 to the telemetry, consumes on average 14 W and requires 18.7 kg for deployment including its internal shielding. The scientific objectives for the polar magnetosphere fall into four broad categories: (1) those to define the ambient kinetic regimes of ions and electrons; (2) those to elucidate the magnetohydrodynamic responses in these regimes; (3) those to assess the particle populations with high time resolution; and (4) those to determine the global topology of the magnetic field. In thefirst group are issues of identifying the origins of particles at high magnetic latitudes, their energization, the altitude dependence of the forces, including parallel electric fields they have traversed. In thesecond group are the physics of the fluid flows, regimes of current, and plasma depletion zones during quiescent and disturbed magnetic conditions. In thethird group is the exploration of the processes that accompany the rapid time variations known to occur in the auroral zone, cusp and entry layers as they affect the flow of mass, momentum and energy in the auroral region. In thefourth class of objectives are studies in conjunction with the SWE measurements of the Strahl in the solar wind that exploit the small gyroradius of thermal electrons to detect those magnetic field lines that penetrate the auroral region that are directly open to interplanetary space where, for example, the Polar Rain is observed.