ISO 26000《社会责任指南》浅析

介绍了社会责任标准的起源及其演变,ISO 26000的制定和标准的概貌,在阐述了对ISO 26000认识的基础上,简要分析了标准实施会产生的影响.     

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.     

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。     

标准转换过程中必须做好的几项工作

比较分析了2000版ISO9000族标准与94版标准的差别,提出了经94版标准认证注册的组织在实施转换时必须做好的几项工作和应注意的问题.     

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。     

航空机载电源标准的发展研究

国际标准化组织(ISO)重新对ISO1540:1984进行了修订,颁布了ISO1540:2006,以适应现代飞机电源系统的发展要求,保证飞机电源系统的安全、可靠运行.本文就ISO1540的新旧版本差异进行研究,为航空机载电源的设计和维修提供参考.     

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。     

嵌入式测试系统中UDP/IP协议栈的移植与实现

根据分布式测发控系统单机的通信要求,基于DM9000以太网控制器芯片和BM3101嵌入式处理器进行了以太网网络接口的设计,实现了无操作系统的UDP/IP协议栈的移植,并详细介绍了数据发送和接收的具体实现过程。对系统通信进行了测试,结果表明UDP通信整体稳定可靠,能够满足实际应用需求。     

对2000版ISO 9000中几个概念的认识

通过对2000版ISO9000标准的学习,对质量管理体系审核、质量管理体系评审、自我评定以及质量策划等概念提出新的认识.     

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.