召开ISO9000、ISO/IEC导则25等国际标准宣贯会

中国航空工业总公司技术质量监督局于6月27日至7月3日在北京召开ISO9000、ISO／IEC导则25等国际标准宣贯会。航空工业系统有24个主要厂、所共55名代表参加会议。会议由三O四所丁叔丹副所长主持，中加航空工业总公司技术质量监督局杨育中局长和三O四所沈福核所长等领导出席会议，并讲了话。宣贵会邀请了原国家技术监督局副局长鲁绍曾同志着重宣讲了ISO9000国际质量管理标准与质量认证计量保证之间关系；还邀请了原航空工业总公司技术质量监督局王诉局长宣讲了ISO900O质量管理和质量保证体系的内容。会上还介绍了ISO／IEC导则25等国…     

我国参加ISO IEC活动近况

国际标准化组织(ISO)和国际电工委员会(IEC)是世界上两个最大的制订国际标准的机构,是联合国的甲级咨询机构。ISO负责制订除电工、电子以外的各领域的国际标准,IEC负责制订电工、电子方面的国际标准。ISO、IEC制订的国际标准被广泛采用为世界     

ISO/TC20/SC1第38届年会在京召开

<正>2014年8月25曰至27曰,ISO/TC20/SC1(航空航天电气要求分技术委员会)第38届年会及WG1/WG5/WG10/WG15工作组会议在北京召开。ISO/TC20/SC1现有7个活跃的工作组,24项注册工作项目,2项委员会内部工作项目。主席由来自法国的Louis Leblanc先生担任,秘书由中航工业综合技术研究所高     

参加ISO/TC20/SC1会议的汇报

我们中国代表团一行三人于1980年9月10日至12日在英国伦敦参加了国际标准化组织第二十技术委员会第一分技术委员会(ISO/TC20/SCl)召开的第十次工作会议。现将有关情况汇报如下:一、概况ISO/TC20/SCl是国际标准化组织航空航天器技术委员会下属的一个电气技术分委员会。参加这次工作会议的有:美国、英国、法国、西德和我国等五个国家共三十余名代表。TC20秘书及IEC代表也以观察员身份参加了会议。SCl分技术委员会的秘书国为英国。英国民航局的PERNY先生及英国标准化协会的NIGHTINGALE先生分别担任该分委员会的主席和秘书长。     

ISO9000系列标准

ISO9000系列标准是国际标准化组织为适应国际贸易发展需要而制定的国际品质保证标准。该标准分5个部分:ISO9000是该系列标准的选用导则;ISO9001～ISO9003是合同环境用于外部质量保证的标准;ISO9004是非合同环境下用于指导企业质量管     

ISO体系 值得信赖的伙伴——国际标准化组织(ISO)2007年度工作报告简介

介绍了国际标准化组织(ISO)2007年度工作报告主要内容,分析了ISO通过建立与发展全球伙伴关系不断提高ISO自身及ISO标准全球影响力的成功经验.     

参加ISO/TC20/SC10的工作汇报

我们三机部、七机部、八机部四名代表于1979年9月25～28日在莫斯科参加了国际标准化组织第二十技术委员会第十分技术委员会(ISO/TC20/SC10)召开的“航空管路联接和密封”会议。现将有关情况汇报如下:     

航空测试实验室管理体系及过程控制方法探讨

通过对ISO/IEC17025:2005<检测和校准实验室能力的通用要求>及DILAC/AC01:2005<检测实验室和校准实验室能力认可准则>的深入研究,结合实际工作经验,提出了应用过程的分析方法,建立了航空测试实验室管理体系,既满足了标准的要求,又符合航空测试实验室的实际,实现了航空测试试验的过程控制,确保了测试结果的准确可靠.     

参加ISO/TC20/SC4会议的汇报

由航空工业部二人组成的中国代表团出席了ISO/TC20/SC4航空航天紧固件分委员会六月在瑞典斯德哥尔摩召开的第25届会议。现将有关情况汇报如下:     

2000年版ISO／9001标准简介

ABriefofISO／90012000Version众所周知，2000年IS09000标准族新版将诞生。日前，国际标准化组织IS0／TC176委员会正在对1994年版IS09000族标准进行修订，并已完成第二稿委员会案，即CD2稿。由我国对口IS0／76的技术委员会──全国质量管理和质量保证标准化技术委员会（CSBTS／TC151），组织成立的“2000版ISO9000族标准跟踪与转化研究工作组”已在1999年3月将2000版ISO／CD19000、ISO／CDI9001、ISO／CD19004，三项标准翻译定稿并汇编成册。近期，又翻译出CD2稿。本人参阅了其中最受关注的ISO／CD29001标准译文，并与…     

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.     

试论企业开展ISO14001环境管理体系认证的必要性与可行性

为加强企业对开展ISO14001环境管理体系认证的认识,并加以实施,本文对ISO14001认证的必要性及可行性作了比较详细的论述。     

Pre-Main Sequence Stars Seen by ISO

Observations of pre-main sequence objects (T Tauri, Herbig Ae/Be and FU Orionis stars) obtained with the instrumentation on board the Infrared Space Observatory (ISO) are reviewed. All the observations have been mainly carried out by using the two spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to reconstruct the spectral energy distributions. Line emission and photometric behaviour of pre-main sequence objects have been analyzed in the framework of the current models, discussing the agreement (or disagreement) with them and trying to derive the questions which should be answered by the forthcoming FIR instrumentation. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

在高校后勤管理中建立ISO9000质量管理体系

ISO9000质量管理体系是目前国际上通用的质量管理标准体系，采用这个标准规范高校后勤管理和服务工作，能够提升管理服务水平，实现学校后勤管理规范化、标准化。     

ISO Observations of Pre-Stellar Cores and Young Stellar Objects

We summarize the observations of the Infrared Space Observatory (ISO) concerning the earliest stages of the stellar formation. The observations of samples of sources in different evolutionary stages are reviewed, addressing in particular how the physical and chemical properties of the protostellar environments change from the pre-stellar cores to the protostars at the end of their accretion phase. In addition, the mid-IR surveys in nearby star-forming regions are discussed, showing their implications for the understanding of the stellar initial mass function. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

ISO6507金属材料维氏硬度试验方法的测量不确定度评定实例

介绍了ISO6507金属材料维氏硬度试验方法的测量不确定度评定,并针对两种评定方法分别给出了评定实例。     

An ISO View on Interstellar and Cometary Ice Chemistry

The ISO-SWS instrument offering a large wavelength coverage and a resolution well adapted to the solid phase has changed our knowledge of the physical-chemical properties of ices in space. The discovery of many new ice features was reported and the comparison with dedicated laboratory experiments allowed the determination of more accurate abundances of major ice components. The presence of CO₂ ice has recently been confirmed with the SWS (Short Wavelength Spectrometer) as a dominant ice component of interstellar grain mantles. The bending mode of CO₂ ice shows a particular triple-peak structure which provides first evidence for extensive ice segregation in the line-of-sight toward massive protostars. A comparison of interstellar and cometary ices using recent ISO data and ground-based measurements has revealed important similarities but also indicated that comets contain, beside pristine interstellar material, admixtures of processed material. The investigation of molecules in interstellar clouds is essential to reveal the link between dust in the interstellar medium and in the Solar System. This revised version was published online in June 2006 with corrections to the Cover Date.     

The European Large Area ISO Survey

The European Large Area ISO Survey (ELAIS) was the largest Open Time survey on the Infrared Space Observatory (ISO). It was designed to explore obscured galaxies and hence quantify the recent star-formation history of the Universe. The final reanalysis of the data has been completed and a band-merged catalogue with associations across many wavelengths compiled and released the data to the global astronomical community (http://astro.imperial.ac.uk/Elais/). This paper summarises some of the key results. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Debris Discs Around Stars: The 2004 ISO Legacy

Debris discs around stars were first discovered by the Infrared Astronomical Satellite (IRAS) in 1983. For the first time material orbiting another star than the Sun, but distinct from a circumstellar envelope, was observed through its far infrared emission. This major discovery motivated astronomers to investigate those discs by further analyzing the IRAS data, using ground-based telescopes for the hunting of exoplanets, developing several projects using the Infrared Space Observatory (ISO), and now exploiting the ISO Data Archive (IDA). This review presents the main ISO results, statistical as well as individual, on debris discs in orbit around pre-main-sequence and main-sequence stars. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.