Obscured Activity: AGN, Quasars, Starbursts and ULIGs Observed by the Infrared Space Observatory

Some of the most ‘active’ galaxies in the Universe are obscured by large quantities of dust and emit a substantial fraction of their bolometric luminosity in the infrared. Observations of these infrared luminous galaxies with the Infrared Space Observatory (ISO) have provided a relatively unabsorbed view to the sources fuelling this active emission. The improved sensitivity, spatial resolution and spectroscopic capability of ISO over its predecessor Infrared Astronomical Satellite (IRAS) of enabled significant advances in the understanding of the infrared properties of active galaxies. ISO surveyed a wide range of active galaxies which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines as well as broad band features in the mid- and far-infrared. This was particularly useful, since it resulted in the understanding of the power production, excitation and fuelling mechanisms in the nuclei of active galaxies including the intriguing but so far elusive ultraluminous infrared galaxies. Detailed studies of various classes of AGN and quasars greatly improved our understanding of the unification scenario. Far-infrared imaging and photometry revealed the presence of a new very cold dust component in galaxies and furthered our knowledge of the far-infrared properties of faint starbursts, ULIGs and quasars. We summarise almost nine years of key results based on ISO data spanning the full range of luminosity and type of active galaxies.     

电泵起停控制与电机多功能保护电路

某些场合，电泵要在特殊的环境和条件下长期连续的工作，因此配置特殊的起停控制电路和保护电路是完全必要的，所以设计了本文介绍的电泵起停控制与多功能保护电路。电路主要由集成件构成。文中扼要介绍的是电泵欠载延时断电保护，过载分级延时断电保护电路，以及欠载停机后延时自动再起动电路。     

弹道靶红外辐射测量

为深入认识再入物理现象 ,在弹道靶上做了模型头部和近尾流红外辐射测量。发射器为 1 4.5mm口径的二级轻气炮 ,模型为1 0mm的球 ,材料为聚碳酸酯和铝 ,模型发射速度 4～6km/s,使用红外InSb探测器测量波长 3～ 5 .4μm的红外辐射 ,靶室压力 5 .32kPa。实验中使用光电法测量模型速度 ,两站阴影照相进行模型姿态监测和速度核实。实验结果表明 :球模型的红外辐射强度强烈依赖于模型材料和模型飞行速度。对不同材料模型头部和尾流部辐射强度的定性比较说明由于低温材料烧蚀产物的存在 ,极大地增强了头部和近尾流区的辐射强度 ,而且延长了尾流辐射长度     

红外隐身材料的研究进展

红外探测器的高度发展已使用于目标表面的热红外隐身材料成为飞行器隐身技术中的一个重要组成部分。但对这种材料的发展情况,以往的文献一向较少涉及。本文概括了这种材料的一般性能要求,较全面地评述了十余年来红外隐身材料研究中各主要方面的发展情况,并分析了一些重要材料品种的特点、性能水平、技术影响因素、存在的问题和发展趋势。     

基于XML的产品主模型技术研究

多学科设计优化方法是近年来发展的一种设计复杂系统的新方法。它充分考虑各个学科之间的相互影响和耦合作用,以获得系统的整体最优解。产品主模型技术是多学科设计优化的关键技术之一,能较好地解决应用模型之间的数据交换和通信。文章介绍了产品主模型的概念及其特点,对产品主模型技术及其实施过程进行了深入研究。回顾了可扩展标记语言的产生和发展历史,并对其特性进行了较详细介绍;研究了基于可扩展标记语言技术实现系统集成的技术路线;最后,提出了基于可扩展标记语言技术和产品主模型技术的卫星总体方案多学科设计优化集成框架。     

红外探测阵列对固体导弹尾焰跟踪定位的研究

通过分析研究建立了前视红外探测阵列ＦＬＩＲ（Ｆｏｒｗａｒｄ Ｌｏｏｋｉｎｇ Ｉｎｆｒａ－Ｒｅｄ）对导弹进行精确跟踪、定位的数学模型，其中包括导弹的运动模型、大气干扰模型和探测阵列的观测模型。利用探测阵列ＦＬＩＲ的原始观测数据，扩展卡尔曼滤波器（ＥＫＦ）精确跟踪导弹目标。由于导弹与探测器的距离较远，故为视为点目标。导弹在探测阵列上投影的位置由两部分组成：导弹真实运动位置和由于大气干扰造成的偏移。滤波     

INS／GPS组合导航系统的容错研究

本文研究了INS/GPS组合导航系统的容错问题,并提出了一个两级故障检测及分离方案。通过采用该方案,INS/GPS组合导航系统将具有较高的容错能力,并能为用户提供连续、精确的导航信息。     

基于CORBA实现专业领域软件在网络环境下的集成

如何有效地将已有系统集成或移植到新系统中 ,是集成系统开发中提出的一个重要问题。本文基于CORBA技术探讨如何实现遗留系统集成的方法 ,并通过实例重点阐述如何将已有的系统封装成CORBA对象的步骤。     

Expectations for Infrared Spectroscopy of 9P/Tempel 1 from Deep Impact

The science payload on the Deep Impact mission includes a 1.05–4.8 μm infrared spectrometer with a spectral resolution ranging from R∼200–900. The Deep Impact IR spectrometer was designed to optimize, within engineering and cost constraints, observations of the dust, gas, and nucleus of 9P/Tempel 1. The wavelength range includes absorption and emission features from ices, silicates, organics, and many gases that are known to be, or anticipated to be, present on comets. The expected data will provide measurements at previously unseen spatial resolution before, during, and after our cratering experiment at the comet 9P/Tempel 1. This article explores the unique aspects of the Deep Impact IR spectrometer experiment, presents a range of expectations for spectral data of 9P/Tempel 1, and summarizes the specific science objectives at each phase of the mission.     

高超声速小钝锥尾流化学非平衡辐射研究

本文主要目的是研究化学非平衡对高超声速小钝锥尾流辐射的影响。计算结果表明：激发发射辐射比化学发光辐射重要，红外辐射比可光辐射重要。结果还表明：由化学非平衡瞬时辐射模型计算求得的ＮＯ５．３μ的辐射能比由局部平衡辐射模型求得的辐射能大３０￣７０％。由此可知，小钝锥尾流的化学非平衡辐射模型对辐射的影响是不能忽略的。