The infrared space observatory (ISO)

The Infrared Space Observatory (ISO), a fully approved and funded project of the European Space Agency (ESA), is an astronomical satellite, which will operate at wavelengths from 2.5–240 m. ISO will provide astronomers with a unique facility of unprecedented sensitivity for a detailed exploration of the universe ranging from objects in the solar system right out to distant extragalactic sources. The satellite essentially consists of a large cryostat containing at launch over 2000 litres of superfluid helium to maintain the Ritchey-Chrétien telescope, the scientific instruments and the optical baffles at temperatures between 2 K and 8 K. The telescope has a 60-cm diameter primary mirror and is diffraction-limited at a wavelength of 5 m. A pointing accuracy of a few arc seconds is provided by a three-axis-stabilisation system consisting of reaction wheels, gyros and optical sensors. ISO's instrument complement consists of four instruments, namely: an imaging photo-polarimeter (2.5–240 m), a camera (2.5–17 m), a short wavelength spectrometer (3–45 m) and a long wavelength spectrometer (43–196 m). These instruments are being built by international consortia of scientific institutes and have been delivered to ESA for in-orbit operations. ISO will be launched in September 1995 by an Ariane 4 into an elliptical orbit (apogee 70000 km and perigee 1000 km) and will be operational for at least 18 months. In keeping with ISO's role as an observatory, the majority of its observing time is being made available to the general astronomical community via a Call for Observing Proposals.     

Windows 2000 Server的网络安全机制

文章分析了Windows2000Server的安全问题以及适用策略，为Windows2000Server局域网络的安全提供参考。     

基于B/S模式的煤矿物资信息管理系统设计

通过对龙宇股份公司陈四楼矿物资管理和内部市场化管理的分析和研究，探讨了煤矿物资信息管理系统的原理、开发、系统设计思想和系统结构。论述了采用“ASP＋SQL SERVER2000”进行系统设计的过程、步骤和安全性的实现。     

A new modeling method of solar energetic proton events for ISO specification

Solar energetic protons degrade performance and reliability of spacecraft systems due to single-event effects, total dose effects and displacement damage in electronics components including solar cells. On designing a solar cell panel, a total fluence of solar energetic protons (SEPs) which cause solar cell damage is needed to estimate power loss of the solar cells over mission life. Nowadays a solar panel area of spacecraft is increasing as spacecraft mission life becomes longer (15–18 years). Thus an accurate SEP model is strongly required for the cost-minimum design from the aerospace industry. The SEP model, JPL-91 proposed by Feynman et al., is currently used widely for solar cell designing. However, it is known that the JPL-91 model predicts higher fluences of protons than values actually experienced in space, especially after 7 years on orbit. In addition, the model is based on several assumptions, and also needs Monte-Carlo simulations for calculating fluences. In this study, we propose a new method for modeling SEPs especially focused on solar cell degradation. The newly-proposed method is empirical, which constructs a model based directly upon proton flux measurement data taken by instruments onboard spacecraft. This method has neither assumptions nor dependence on SEP event selection, both of which are needed in JPL-91. The model fluences derived from this method show lower fluences in longer missions compared to JPL-91. This method has been proposed to ISO (International Organization for Standardization) and has been discussed for a new standard SEP model.     

白光LED用VO4：Ce^3＋荧光粉的制备与表征

白光LED中YAG荧光粉专利权为日本Nichia所有,各国研究者为了规避专利,争相研究替代产品。本文首次采用高温固相法制备了YVO4：Ce^3＋荧光粉,对不同Ce^3＋掺杂浓度下XRD图样与国际标准衍射卡对比后发现在1100℃保温9小时合成的Ce^3＋：YVO4为四方晶系结构,随保温时间延长,结晶程度更好,但时间再长时,结晶变化已不大。荧光光谱表明,激发光谱为双峰结构,主峰在232nm和403nm。发射光谱为一宽带,峰值在424nm附近。发现最佳Ce^3＋掺杂浓度为5mol％。结论是Ce^3＋：YVO4荧光粉可以满足与蓝光LED复合产生自然白光的要求。     

某型起动机高温合金整体涡轮材料的改进与分析

针对某型起动机高温合金整体涡轮断裂故障率高的情况,本文从国内外涡轮材料的发展趋势和应用现状出发,介绍了一种新型涡轮材料,并通过对比新旧材料的性能证明了材料改进的可行性和有效性。     

适用于小型公司的 ISO 9000 质量管理系统(英文)

ＩＳＯ９０００质量管理系统往往存在一种神秘性。一般认为它只适用于大型公司，对小型公司而言，该系统实在是太昂贵了，本文澄清了这种错误的想法，并说明了ＩＳＯ９０００系统内在之属性事实上是灵活的，不论任何行业的小型公司均可适用。此外，它亦指出了认证审核员和质量管理顾问应对那些易犯的错误提高警觉。     

MDOE风洞试验方法研究

在介绍OFAT风洞试验方法和MDOE风洞试验方法概念的基础上,探讨研究了两种试验方法理念的本质区别;简述了MDOE风洞试验方法具体实施的三个过程;归纳分析了MDOE风洞试验方法的应用实例、效能评估和发展前景;意在为国内风洞试验领域科研人员拓展思路、创新方法提供参考。     

灵巧噪声干扰本质含义探讨

文章对灵巧噪声干扰概念的表述提出了质疑,在多项质疑中选取了SLB技术进行简要分析,并指出,SLC等抗干扰技术的作用与是否实施灵巧噪声干扰没有直接关系。进一步,基于匹配滤波器理论对灵工j噪声干扰的本质含义进行了分析,指出：灵巧噪声干扰的本质含义是使干扰由多个分量组成,并且使干扰中的每一个分量的频谱都与雷达发射信号的频谱相...     

面向海洋机动目标跟踪监视的卫星重构组网优化与仿真

摘要： 针对海洋机动目标跟踪监视问题，提出通过卫星相位重构调整进行机动目标搜索跟踪的监视策略，构建地理坐标系下机动目标航位预测模型及基于霍曼转移的卫星调相组网方式，并采用NSGA II算法进行优化求解，对比分析卫星重构组网前后的机动目标发现概率.仿真结果表明：在卫星能量消耗允许范围内进行重构组网，能够有效提升对机动目标的发现概率，为海洋机动目标的搜索跟踪问题提供了一定的方法支持.