Alta U9000图像数据由16位到8位的转换

科学级CCD图像一般是16位的,为了便于在Windows中显示处理过程中的16位图像,需要将16位图像转换为8位图像。介绍了2种转换算法:直接转换法和区间转换法。研究表明:直接转换法实现简单,但容易丢失信息,当原始图像中的有效信息区间较小时,应使用区间转换法;根据原始图像直方图确定用有效信息区间的算法,该算法与CCD的噪声点个数有关,通过对科学级CCD Alta U9000噪声情况的测试,给出了确定U9000图像有效信息区间的方法。     

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.     

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.     

Comets, Asteroids and Zodiacal Light as Seen by Iso

ISO performed a large variety of observing programmes on comets, asteroids and zodiacal light – covering about 1% of the archived observations – with a surprisingly rewarding scientific return. Outstanding results were related to the exceptionally bright comet Hale–Bopp and to ISO's capability to study in detail the water spectrum in a direct way. But many other results were broadly recognised: Discovery of new molecules in comets, the studies of crystalline silicates, the work on asteroid surface mineralogy, results from thermophysical studies of asteroids, a new determination of the asteroid number density in the main-belt and last but not least, the investigations on the spatial and spectral features of the zodiacal light.     

ISo航空航天标准化商业计划分析及其对我们的启示

介绍了ISO航空航天商业计划的主要内容 ;分析了航空航天商业计划的性质和作用 ,以及地区标准对国际标准的冲击 ,并分析了航空航天标准化工作面临的风险 ;在进行分析的同时 ,对我们航空工业标准化工作规划和今后的工作提出了自己的看法     

ISO/IEC 17025与ISO/IEC导则25的比照分析

本文主要介绍ISO/IEC 170251999的由来，及其与ISO9001、ISO9002的关系；ISO/IEC 17025的组成和构架以及与ISO/IEC导则25的对照、比较和分析。以帮助读者了解ISO/IEC 170251999与导则25的异同,从而有助于推进ISO/IEC 17025的实施。     

The ESA scientific programme

The ESA scientific programme has, so far, provided several significant astrophysics experiments and further important missions are scheduled for execution during the next decade. These missions are briefly summarised together with several astrophysics investigations presently under study.     

蓬勃发展中的小卫星国际标准

针对小卫星迅猛发展对标准化的需求,全面分析了现阶段国际标准化组织（International Standardization Organization,ISO）制定的小卫星方面的标准,给出了国际标准化工作中对小卫星的定义,小卫星与传统卫星的差异性分析,详细介绍了ISO/TC20/SC14组织制定的小卫星包括设计、发射、验证、运行4方面的国际标准和立方星标准。     

Disposal orbits for GEO spacecraft: A method for evaluating the orbit height distributions resulting from implementing IADC guidelines

Geostationary orbit (GEO) is the most commercially valuable Earth orbit. The Inter-Agency Space Debris Coordination Committee (IADC) has produced guidelines to help protect this region from space debris. The guidelines propose moving a satellite at the end of its operational life to a disposal orbit, which is designed so that satellites left there will not infringe the operational GEO region within a period of at least 100 yr.     

ISO的GPS基本概念与体系

概要介绍了ISO的产品几何技术规范产生的原由、基本概念与体系的构成、主要内容和今后的发展方向 ,以及我国采用产品几何技术规范的情况。