Interplanetary shock waves: Ulysses observations in and out of the ecliptic plane

Between its launch in October 1990 and the end of 1993, approximately 160 fast collisionless shock waves were observed in the solar wind by the Ulysses space probe. During the in-ecliptic part of the mission, to February 1992, the observed shock waves were first caused mainly by solar transient events following the solar maximum and the reorganisation of the large scale coronal fields. With the decay in solar activity, relatively stable Corotating Interaction Regions (CIRs) were observed betwen 3 and 5.4 AU, each associated with at least one forwardreverse shock pair. During the out-of-ecliptic phase of the orbit, from February 1992 onwards, CIRs and shock pairs associated with them continued to dominate the observations. From July 1992, Ulysses encountered the fast solar wind flow from the newly developed southern polar coronal hole, and from May 1993 remained in the unipolar magnetic region associated with this coronal hole. At latitudes beyond 30°, CIRs were associated almost exclusively with reverse shocks only. A comprehensive list of shock waves identified in the magnetic field and solar wind plasma data from Ulysses is given in Table 1. The principal characteristics were determined mainly from the magnetic field data. General considerations concerning the determination of shock characteristics are outlined in the Introduction.     

Design and characteristics of a multiband communication satelliteantenna system

Feasibility studies on a multiband communication satellite antenna system and the key technologies involved in devising this system are described. The proposed multiband communication satellite utilizes four frequency bands: Ka (30/20 GHz), Ku (14/12 GHz), C (6/4 GHz), and S (2.6/2.5 GHz). It has six beam configurations, three multibeam and three shaped-beam. The following key technologies are presented: (1) a low-loss frequency selective subreflector (FSR) for compact feeds, (2) a low-loss and broadband frequency selective surface (FSS), and (3) a highly accurate and reliable mesh reflector     

Neural controllers for systems with unknown dynamics

This study presents a methodology for specifying a neural controller for a system about which no a priori model information is available. The neural design presumes that a finite duration input/output (I/O) histogram on the system is available. The design procedure extracts from the histogram sufficient information to specify the neural feedback controller. The resultant controller will drive the system along a general output reference profile (unknown during the design). The resultant controller also exhibits the capability of disturbance rejection and the capacity to stabilize unstable plants     

液体火箭发动机基于时序分析的实时在线故障检测算法

针对液体火箭发动机主级稳态工作过程，采用时间序列分析理论，提出并实现了一种基于ＡＲＭＡ模型计算残差自相关函数置信区间检验的故障检测策略。经大量发动机实际热试车数据验证表明，本文所实现的故障检测算法是十分有效的。这一结果可望直接应用于工程。     

端弯叶片通道出口二次流的研究

实验并且采用考虑粘性的涡传输方程计算端弯压气机叶片通道出口二次流。给出了３种端弯叶片及对应的原始直叶片通道出口气流偏转角的实验值和计算预测值。研究表明：采用上述方程能比较准确地预测出口气流偏转角；叶片后缘减弯可减小流向二次涡强度。     

一类关联转子分离尺度与损失的工程模型

将分离与损失相关联，提出了利用转子进出口参数来确定跨音风扇转子内部分离流动的方法。应用该方法对几个转子流场计算的结果表明，在转子的叶尖区域，由于强的激波与附面层相互作用，使得流动在激波后不久便发生分离。叶尖漏流涡可能对激波与附面层的相互作用诱导流动分离有较大影响。     

端齿连接转子轴向松弛力（压紧力）计算

 将端齿连接转子的零部件简化归并为４类结构，利用弹性力学、壳体理论、有限元素法及多变量函数插值技术等手段，导出各类结构轴向柔度系数的工程计算表达式，并给出离心力、气动力、热载荷及机动载荷等在各端齿接触面处引起的轴向松弛力或压紧力的计算公式。还介绍了根据本文提出的方法及公式开发的计算机程序，并给出了其应用实例     

二维广义J积分

 本文从总位能差率出发推导出了在非均匀温度场中承受面力与体力的变厚度板的广义J积分,并证明了广义J积分的守恒性。     

X-Ray spectroscopic investigation of the coronal structure of capella

The binary system Capella (G6 III + F9 III) has been observed on 1979 March 15 and on 1980 March 15–17 with the Objective Grating Spectrometer (OGS) onboard theEinstein Observatory. The spectrum measured with the 1000 l/mm grating covers the range 5–30 Å with a resolution < 1 Å. The spectra show evidence for a bimodal temperature distribution of emission measure in an optically thin plasma with one component 5 million degrees and the other one 10 million degrees. Spectral features can be identified with line emissions from O VIII, Fe XVII, Fe XVIII, Fe XXIV, and Ne X ions. Good spectral fits have been obtained assuming standard cosmic abundances. The data are interpreted in terms of emission from hot static coronal loops rather similar to the magnetic arch structures found on the Sun. It is shown that the conditions required by this model exist on Capella. Mean values of loop parameters are derived for both temperature components.