高温天线罩材料研究进展

对目前主要几种高温天线罩材料体系，包括氧化铝陶瓷、石英陶瓷、微晶玻璃、纤维增强二氧化硅基复合材料、纤维增强磷酸盐基复合材料以及硅氧氮陶瓷材料的研究发展和应用情况进行了简要的综述。     

多层喷射沉积制备大尺寸耐热铝合金管坯的研究

采用多层喷射沉积工艺制备出了尺寸为Ф630 mm×250 mm×800 mm且质量较好的FVS0812耐热铝合金管坯,通过挤压获得了性能优良的大直径管材,并对管坯和挤压后管材的力学性能和微观结构进行了检测和分析.分析结果表明,多层喷射沉积制坯过程中,熔滴在沉积面的冷却速度约3.2×104 K@s-1～106K@s-1,熔滴凝固后在沉积坯中形成微细晶粒结构(200 nm～500 nm)和弥散分布的纳米析出相Al12(Fe,V)3Si(20nm～60 nm),使得沉积坯挤压致密后具有优异的性能.     

液体火箭爆炸地面推进剂残余量实验研究

为航天发射场安全技术文件的制定提供推进剂污染方面的数据，进行了四氧化二氮（N2O4）和偏二甲肼（UDMH）爆炸实验研究，获得了地面推进剂残余量和毒气扩散的实验测量数据，提出的液体火箭爆炸地面上推进剂污染范围和残余量等参数的计算公式可以用于工程估算。     

SAE线性令牌传输总线与光纤型分布式数据接口规约的比较

SAE LTPB与ANSI FDDI两种光纤高速总线规约很适合在分布式航空电子综合系统中使用,以满足下一代高性能军用飞机系统区域内、外数据的高传递速率的需要。本文从几个方面对其作了比较,旨在为设计者选择使用提供参考。     

逆升压电子设备冷却系统控制方案的研究

分析了目前国内一些飞机基于三点温度控制方案的逆升压电子设备冷却系统的缺陷 ,提出了一种新的系统控制方案 ,即基于飞行速度和高度的逆升压电子设备冷却系统的控制方案。这一方案不需要人工干预 ,可实现全自动化。     

Hectometric and kilometric solar radio emission observed from satellites in August 1972

Type II, III, and continuum solar radio events, as well as intense terrestrial magnetospheric radio emissions, were observed at low frequencies (10 MHz to 30 kHz) by the IMP-6 satellite during the period of high solar activity in August 1972. This review covers briefly the unique direction finding capability of the experiment, as well as a detailed chronology of the low frequency radio events, and, where possible, their association with both groundbased radio observations and solar flares. The attempted observation of solar bursts in the presence of intense magnetospheric noise may, as illustrated, lead to erroneous results in the absence of directional information. The problem of assigning an electron density scale and its influence on determining burst trajectories is reviewed. However, for the disturbed conditions existing during the period in question, we feel that such trajectories cannot be determined accurately by this method. In conclusion, the capabilities, limitations, and observing programs of present and future satellite experiments are briefly discussed.     

7. Dynamics,winds, circulation and turbulence in the atmosphere of venus

With the possible exception of the lowest one or two scale heights, the dominant mode of circulation of Venus' atmosphere is a rapid, zonal, retrograde motion. Global albedo variations in the ultraviolet may reflect planetary scale waves propagating relative to the zonal winds. Other special phenomena such as cellular convection in the subsolar region and internal gravity waves generated in the interaction of the zonal circulation with the subsolar disturbance may also be revealed in ultraviolet imagery of the atmosphere. We discuss the contributions of experiments on the Orbiter and Entry Probes of Pioneer Venus toward unravelling the mystery of the planet's global circulation and the role played by waves, instabilities and convection therein.     

Initial observations of low energy charged particles near the Earth's bow shock on ISEE-1

We report initial measurements from the ULECA sensor of the Max-Planck-Institut/University of Maryland experiment on ISEE-1. ULECA is an electrostatic deflection — total energy sensor consisting of a collimator, deflection analyzer and an array of solid state detectors. The position of a given detector, which determines the energy per charge of an incident particle, together with the measured energy determine the particle's charge state. We find that a rich variety of phenomena are operative in the transthermal energy regime (10 keV/Q to 100 keV/Q) covered by ULECA. Specifically, we present observations of locally accelerated protons, alpha particles, and heavier ions in the magnetosheath and upstream of the Earth's bow shock. Preliminary analysis indicates that the behavior of these locally accelerated particles is most similar at the same energy per charge.     

Crossarray Beamforming with a Parametric Receiving Array and a Line Array

A beamforming technique involving cross correlation of the outputs of two directional arrays is investigated. The performance characteristics of the crossarray system are determined and related to the characteristics of the two individual arrays. It is found that the crossarray beam pattern is the average (in decibels) of the beam patterns of the individual arrays, and that the crossarray gain (rejection of spatially distributed noise) is 1.5 dB greater than the average (in decibels) of the individual array gains. The most interesting applications for this system may be those where the two arrays are quite different, as in the case of a parametric acoustic receiving array (PARRAY) and a broadside line array.     

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.