The WIND magnetic field investigation

The magnetic field experiment on WIND will provide data for studies of a broad range of scales of structures and fluctuation characteristics of the interplanetary magnetic field throughout the mission, and, where appropriate, relate them to the statics and dynamics of the magnetosphere. The basic instrument of the Magnetic Field Investigation (MFI) is a boom-mounted dual triaxial fluxgate magnetometer and associated electronics. The dual configuration provides redundancy and also permits accurate removal of the dipolar portion of the spacecraft magnetic field. The instrument provides (1) near real-time data at nominally one vector per 92 s as key parameter data for broad dissemination, (2) rapid data at 10.9 vectors s^–1 for standard analysis, and (3) occasionally, snapshot (SS) memory data and Fast Fourier Transform data (FFT), both based on 44 vectors s^–1. These measurements will be precise (0.025%), accurate, ultra-sensitive (0.008 nT/step quantization), and where the sensor noise level is <0.006 nT r.m.s. for 0–10 Hz. The digital processing unit utilizes a 12-bit microprocessor controlled analogue-to-digital converter. The instrument features a very wide dynamic range of measurement capability, from ±4 nT up to ±65 536 nT per axis in eight discrete ranges. (The upper range permits complete testing in the Earth's field.) In the FTT mode power spectral density elements are transmitted to the ground as fast as once every 23 s (high rate), and 2.7 min of SS memory time series data, triggered automatically by pre-set command, requires typically about 5.1 hours for transmission. Standard data products are expected to be the following vector field averages: 0.0227-s (detail data from SS), 0.092 s (detail in standard mode), 3 s, 1 min, and 1 hour, in both GSE and GSM coordinates, as well as the FFT spectral elements. As has been our team's tradition, high instrument reliability is obtained by the use of fully redundant systems and extremely conservative designs. We plan studies of the solar wind: (1) as a collisionless plasma laboratory, at all time scales, macro, meso and micro, but concentrating on the kinetic scale, the highest time resolution of the instrument (=0.022 s), (2) as a consequence of solar energy and mass output, (3) as an external source of plasma that can couple mass, momentum, and energy to the Earth's magnetosphere, and (4) as it is modified as a consequence of its imbedded field interacting with the moon. Since the GEOTAIL Inboard Magnetometer (GIM), which is similar to the MFI instrument, was developed by members of our team, we provide a brief discussion of GIM related science objectives, along with MFI related science goals.     

固体火箭发动机用新型涂料热防护设计和试验研究

介绍了某联合动力装置中的共底和环形点火器首次采用新研制的３５００Ｋ高温涂料进行热防护的配方设计、受热计算、涂层制备和试验考核。由环氧改性有机硅树脂基料、专用树脂固体体系和多种形状的硅酸盐填料制成的涂层具有优异的耐高温、隔热和抗烧蚀性能，还能常温固化成形，成功地解决了中型固体火箭发动机中大尺寸、薄壁、复杂型面零件的热防护和过烧蚀难题，有效地提高了发动机的工作可靠性。     

半波GLM方法封闭的湍流方程对转捩过程的数值模拟

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Pickup protons in the heliosphere

We calculate the conditions of pickup protons inside the termination shock. Outside 50 AU the partial pressure of pickup protons is greater than the magnetic pressure by a factor of > 10, and greater than the partial pressure of solar wind protons by a factor of > 100. Thus, pickup protons have a significant dynamical influence on the structures of the solar wind in the outer heliosphere.     

机翼的动态分离流动特性

本文对两个机翼等速上仰及下俯的动态分离流动特性在水槽中进行了流态研究。结果表明，动态滞后效应与折算频率关系很大。转轴位置对动态滞后的影响与增加上爷角速度的作用有某种相仿的效应。机翼的初始迎角对动态流动特性有不可忽视的“遗传”效应。     

Shock interactions in the outer heliosphere

Observations of plasma and magnetic fields by Pioneer 10 and 11 and Voyager 1 and 2 reveal that MHD shocks are an important component of the large-scale solar wind structures in the outer heliosphere. This review discusses recent progress in simulation studies of the nonlinear evolution of the solar wind structures, and in particular concentrates on the theoretical development and applications of the shock interactions model. Various stream propagation models, which do not use the Rankine-Hugoniot relations to calculate the jump conditions at shock crossings, have been used to simulate the essential evolution process of isolated streams and the formation and propagation of corotating and transient shocks. They produce fairly good results in the region up to a few AU. In 1984, the shock interactions model was introduced to study the evolution of large-scale solar wind structures in the region outside 1 AU up to several tens of AU. The model uses the exact Rankine-Hugoniot relations to calculate the shock speed and shock strength at all shock crossings. So that the model can more accurately calculate the shock speeds and the accumulated irreversible shock heating of plasma at several tens of AU. The applications of the shock interactions model are presented in three groups. (a) The first group covers the basic interaction of a shock with the ambient solar wind, the formation and propagation of shock pairs, and the collision and merging of shocks. (b) The second group covers the use of the shock interactions model to simulate the nonlinear evolution of large-scale solar wind structures in the outer heliosphere. These simulation results can provide the detailed evolution process for large-scale solar wind structures in the vast region not directly observed. Two selected studies are reported. (c) Finally, the shock interactions model is applied to studying the heating of the solar wind in the outer heliosphere. The model calculations support shocks being chiefly responsible for the heating of the solar wind plasma in the outer heliosphere at least up to 30 AU.     

Terminal control monitor for ATC using knowledge-based system

A knowledge-based system for air traffic control (ATC) in terminal control regions is designed for improving service and operation. Domain knowledge is established following rules, regulations, and comments from controllers. An expert system is adopted for approach control and airport control in the terminal control region. The proposed system was implemented in PC-AT with Turbo Prolog. The air terminal control monitor was checked with regard to flight information input, real-time data refreshment, air traffic rescheduling, constraint violation double checking, emergency responses, and normal monitoring. Simulation results are given     

鸟撞载荷下Y12飞机前风挡非线性动力响应分析

 本文利用VEP系统对Y12飞机6mm和8mm厚的前风挡上三点,在0.91kg鸟以56～61m/s撞击下的非线性动力响应进行了数值分析,并与实验结果进行了比较,其中二点情况与实验符合很好。     

微推偏火箭喷管非对称内流场数值模拟

研究了入流倾斜于喷管超音速段轴线的微推偏喷管内流场。数值方法是具有高分辨率高精度的三维隐式有限体积的ＴＶＤ格式。针对一系列典型锥形喷管和钟型喷管,数值模拟结果得出非对称内流场的侧向力和侧向力矩随喷管几何结构以及入流条件变化的一些特征,并同有关实验结果符合良好,对微推偏喷管设计具有一定的指导意义。     

飞机外形网格拓扑和多块网格拼接技术

多块网格方法成功的关键在于网格拓扑的选择和块与决之间的拼接方法。针对真实飞机外形多块网格生成,本文分析研究了翼类和体类部件的各种网格拓扑;论述了翼身组合体的多块网格非结构连续拼接技术;指出连续拼接方法的缺点,以及相应的解决方法;同时,还讨论了分块策略和确保块与块之间网格线完全连续拼接的方法;通过实例进一步阐述了本文工作的另外一些独到之处。