SWE,a comprehensive plasma instrument for the WIND spacecraft

The Solar Wind Experiment (SWE) on the WIND spacecraft is a comprehensive, integrated set of sensors which is designed to investigate outstanding problems in solar wind physics. It consists of two Faraday cup (FC) sensors; a vector electron and ion spectrometer (VEIS); a strahl sensor, which is especially configured to study the electron strahl close to the magnetic field direction; and an on-board calibration system. The energy/charge range of the Faraday cups is 150 V to 8 kV, and that of the VEIS is 7 V to 24.8 kV. The time resolution depends on the operational mode used, but can be of the order of a few seconds for 3-D measurements. Key parameters which broadly characterize the solar wind positive ion velocity distribution function will be made available rapidly from the GGS Central Data Handling Facility.     

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     

复合材料在DCB试验中的裂纹尺寸效应

在许多关于复合材料Ⅰ型层间断裂韧性试验研究工作中，不同的作者所选取的有效裂纹长度有很大的差异，由此带来试验结果分散程度很大，试验结果无法相互比较等问题。本文对复合材料在Ⅰ型层间断裂ＤＣＢ试验中裂纹的预裂长度、裂纹尖端形状以及裂纹测量误差等问题进行了研究。     

多级涡轮S2流面的变比热气动热力计算方法

针对在多级涡轮流道中沿流动方向燃气温度变化较大这一特点，为了准确反映出温度变化对气动热力计算结果的影响，提出了一种考虑变比热影响的Ｓ２流面的气动热力计算方法。该方法摒弃了传统的定比热气动热力计算公式和由温度、密度确定压力的求解顺序，而是根据导出的变比热计算压力的关系式求解压力，然后用温度和压力计算密度。计算结果显示出本文的算法较传统的未能充分考虑变比热影响的气动热力计算方法可以改善多级涡轮联算时的计算准确度。     

The Rosat mission

The primary scientific objective of the ROSAT mission is to perform the first all sky survey with an imaging X-ray telescope leading to an improvement in sensitivity by several orders of magnitude compared with previous surveys. Consequently a large number of new sources (> 10⁵) will be discovered and located with an accuracy of 1 arcmin. After completion of the survey which will take about half a year the instrument will be used for detailed observations of selected targets.The X-ray telescope consists of a fourfold nested Wolter type I mirror system with 80 cm aperture and 240 cm focal length, and three focal plane detectors. In the baseline version these will be imaging proportional counters (0.1 – 2 keV) providing a field of view of 2⁰ × 2⁰.     

Optical observations of the X-ray source 2S0921-630

We report photometric observations of the optical counterpart of the X-ray source 2S0921-630. The data, obtained at the South African Astronomical Observatory during 3 weeks in 1980 and 1981, are consistent with a 17.9 day periodic modulation of the flux in the B band. Correlated variability of the (B-V) and (U-B) colour indices with the B mag. is demonstrated and quantified. The observed B mag. and colours at maximum and minimum light are used to compute some of the system parameters. A model of 2S0921-630 is proposed in terms of a binary system in which the variable inclination of a luminous accretion disc produces the long-term modulation of the optical flux.     

断裂力学在直升机桨毂上的应用

 本文用实验方法,得出了计算弯曲载荷下含表面裂纹圆轴、圆筒的应力强度因子（K_I）的表达式,并按照裂纹面积扩展率公式,分析了直升机桨毂转轴轴颈的临界裂纹面积和剩余疲劳寿命。为了校核断裂力学分析的可靠性,模拟飞行状况进行了实际桨毂支臂转轴轴颈的疲劳试验。实验结果与计算结果相当符合。     

The long term variability of 4U 1258-61 (GX304-1)

We present optical spectroscopy and photometry of 4U 1258-61 obtained over the course of six years. Evidence for the evolution of a circumstellar envelope throughout the course of the observations is presented.