扫描器运动多参数测试技术研究

新型图像扫描器具有较高的响应频率，可以实现高速扫描。在研究扫描器运动参数分离的基础上，利用对称放置的半导体位置探测器建立了扫描器的多运动参数测试系统，提出了光电二维位置传感器的非线性修正和补充方法，实现了四路模拟信号的DMA传送，提高了测试的速度和精度，实现扫描器在高频运动时的多运动参数测试。     

非线性传感器静态特性评估的极限点法

基于对测量过程、测量误差的认识，提出了一种利用极限点法评估非线性传感器静态特性的一种新方法。给出了利用该方法评估非线性传感器的两种模型。并以一电涡流式非线性位移传感器的标定数据进行了计算、分析。     

被动式引射器内两相流数值模拟

把气相二维欧拉方程的隐式矢通量分裂近似因子分解法与固相粒子的特征线解法进行耦合,对被动式引射器内两相流场进行数值模拟,确定产生激波的喷管出口压强,分析不同引射器结构对引射效果的影响,并获得了一种最佳结构。研究结果可以为被动式引射器的设计与使用提供依据。     

STUDY ON ALGORITHM OF SENSOR MANAGEMENT BASED ON FUNCTIONS OF EFFICIENCY AND WASTE

The sensor management system is a subsys-tem of a multisensor data fusion system,and itspurpose is to satisfy requests of multitarget andscanned space by using the limited sensor resourcesin order to gain optimal measurement values of allspecified characteristics ( detection and captureprobability,emission power of sensor,trackingprecision or target losing probability and so on) .By the optimal principle listed above,sensor re-sources are distributed in science and reason.In aword,itis a key p…     

旋转状态下带肋U形通道内换热的实验研究

用实验方法研究了涡轮叶片内带肋Ｕ形通道状态下的前缘、后缘及两侧面局部换热系数分布。结果表明,在旋转状态下此通道的努塞尔数随雷诺数的增大而增大。在进气通道的后缘和出气直通道前缘,努塞尔数随旋转数的增加而增加;在进气直通道的前缘和出气直通道的后缘,努塞尔数随着旋转数的变化出现几次反复。随着浮力数的增加,通道的平均努塞尔数是下降的。Ｕ形通道参旋转状态下的流动换热规律比静态下的复杂的多。     

变温热源内可逆布雷顿循环功率密度优化

计人工质与高、低温侧换热器的热阻损失，用有限时间热力学方法，导出了变温热源条件下内可逆布雷顿循环功率密度与压比间的解析式，借助于数值计算，研究了高、低温侧换热器的热导率分配和工质与热源间的热容率匹配对功率最大密度的影响。     

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.     

分区和有限容积法计算长尾喷管中的湍流流动

为了给长尾喷管热防护结构设计提供热边界条件，从轴对称二维雷诺平均N－S方程出发，采用分区算法和有限容积法计算了长尾喷管中的湍流流动，分析了流场的结构特性，提出了长尾喷管中燃气温度，压强和马赫数分布的某些规律以及燃气温度沿壁面的分布，计算和分析结果提出了长尾喷管热防护结构设计应注意的事项。     

吸热型碳氢燃料催化裂解热沉测定

报道了一套高温下测量吸热型碳氢燃料催化裂解热沉的稳态热导型流动热量计，仪器常数标定结果线性关系良好，符合Tian’s方程，可以正常工作；测定了500℃和600℃下吸热型碳氢燃料RL7及NNJ-150在SAPO-34分子筛催化剂上的催化裂解热沉，并与相同条件下热裂解热沉相比较，结果表明，吸热型碳氢燃料在SAPO-34分子筛催化剂上发生催化裂解能够比热裂解获得更高的热沉，燃料吸热工作温度可降低100℃。     

The Cassini Cosmic Dust Analyzer

The Cassini-Huygens Cosmic Dust Analyzer (CDA) is intended to provide direct observations of dust grains with masses between 10⁻¹⁹ and 10⁻⁹ kg in interplanetary space and in the jovian and saturnian systems, to investigate their physical, chemical and dynamical properties as functions of the distances to the Sun, to Jupiter and to Saturn and its satellites and rings, to study their interaction with the saturnian rings, satellites and magnetosphere. Chemical composition of interplanetary meteoroids will be compared with asteroidal and cometary dust, as well as with Saturn dust, ejecta from rings and satellites. Ring and satellites phenomena which might be effects of meteoroid impacts will be compared with the interplanetary dust environment. Electrical charges of particulate matter in the magnetosphere and its consequences will be studied, e.g. the effects of the ambient plasma and the magnetic field on the trajectories of dust particles as well as fragmentation of particles due to electrostatic disruption.The investigation will be performed with an instrument that measures the mass, composition, electric charge, speed, and flight direction of individual dust particles. It is a highly reliable and versatile instrument with a mass sensitivity 10⁶ times higher than that of the Pioneer 10 and 11 dust detectors which measured dust in the saturnian system. The Cosmic Dust Analyzer has significant inheritance from former space instrumentation developed for the VEGA, Giotto, Galileo, and Ulysses missions. It will reliably measure impacts from as low as 1 impact per month up to 10⁴ impacts per second. The instrument weighs 17 kg and consumes 12 W, the integrated time-of-flight mass spectrometer has a mass resolution of up to 50. The nominal data transmission rate is 524 bits/s and varies between 50 and 4192 bps.This revised version was published online in July 2005 with a corrected cover date.