光纤光栅温度传感器研究进展

归纳了以光纤光栅为基础的温度传感器的研究现状,总结了这些温度传感器的基本原理,再现了它们的主要结构,展示了原文提到的实验过程和数据分析结果,并对这些传感器的优点和不足进行了分析,提出了部分改进方案。通过研究发现：光纤光栅温度传感器具有优良的特性,能够在恶劣环境下测量极高的温度,具有广阔的应用前景。     

基于工作过程的《制冷技术》课程教学设计

根据高等职业教育新的课程理念,对《制冷技术》课程的教学进行了改革。基于对实际工作过程的分析和思考,设计了学习情境,重构了课程内容,以学生为主体组织实施教学,创新了考核方法,有效地提高了教学效果。     

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.     

Interplanetary medium – A dusty plasma

The average mass of dust per volume in space equals that of the solar wind so that the interplanetary medium should provide an obvious region to study dust plasma interactions. While dust collective behavior is typically not observed in the interplanetary medium, the dust component rather consists of isolated grains screened by and interacting with the plasma. Space measurements have revealed several phenomena possibly resulting from dust plasma interactions, but most of the dust plasma interactions are at present not quantified. Examples are the production of neutrals and pick-up ions from the dust, dust impact generated field variations at spacecraft and magnetic field variations possibly caused by solar wind interacting with dust trails. Since dust particles carry a surface charge, they are exposed to the Lorentz force in the interplanetary magnetic field and for grains of sub-micrometer sizes acceleration can be substantial.     

Characterization of the near Earth radiation environment by Liulin type spectrometers

Comprehensive study of the dose, flux and deposited energy spectra shape data obtained by Liulin type spectrometers on spacecraft (five different experiments) and aircraft since 2001 is performed with the aim of understanding how well these parameters can characterize the type of predominant particles and their energy in the near Earth radiation environment. Three different methods for characterisation of the incoming radiation from Liulin spectrometers are described. The results revealed that the most informative one is by the shape of the deposited energy spectra. Spectra generated by Galactic Cosmic Rays (GCR) protons and their secondaries are with linear falling shape in the coordinates deposited energy/deposited per channel dose rate. The position of the maximum of the deposited energy spectra inside the South Atlantic Anomaly (SAA) region depends on the incident energy of the incoming protons. Spectra generated by relativistic electrons in the outer radiation belt have a maximum in the first channels. For higher energy depositions these spectra are similar to the GCR spectra. Mixed radiation by protons and electrons and/or bremsstrahlung is characterized by spectra with 2 maxima. All type of spectra has a knee close to 6.2 MeV deposited energy, which correspond to the stopping energy of protons in the detector. Dose to flux ratio known also as specific dose is another high information parameter, which is given by experimentally obtained formulae [Heffner, J. Nuclear radiation and safety in space. M. Atomizdat. 115, 1971 (in Russian)] connecting the dose to flux ratio and the incident energy of the particles.     

浅谈银行信贷资产债权维护的配套设置

本文主要从强化商业银行内控、建立信贷资产债权保全机制、营造诚实信用环境三方面论述维护银行信贷资产债权的配套措施。     

Thermo-mechanical design and testing of a microbalance for space applications

This work focuses on the thermo-mechanical design of the microbalance used for the VISTA (Volatile In Situ Thermogravimetry Analyzer) sensor. VISTA has been designed to operate in situ in different space environments (asteroids, Mars, icy satellites). In this paper we focus on its application on Mars, where the expected environmental conditions are the most challenging for the thermo-mechanical design.     

舰载倾转旋翼机着舰域耦合流场数值模拟研究

倾转旋翼机是当前旋翼飞行器研究的热点,但有关舰载倾转旋翼机着舰域耦合流场的研究还很少。以两栖攻击舰(LHA)和V-22"鱼鹰"倾转旋翼机为研究对象,基于雷诺平均Navier-Stokes(RANS)方程和SST k-ω湍流模型对舰载倾转旋翼机着舰域耦合流场进行数值模拟研究,并探讨了不同着舰高度时机/舰耦合流场的相互作用。结果表明:倾转旋翼尾流会与舰船脱落涡、甲板舷涡以及舰岛艉涡发生较强的"涡-涡干扰"现象,加大了耦合流场的湍流强度;舰船流场的低频非稳态特征会导致旋翼桨盘气动载荷发生显著的波动,不利于飞行操纵;垂直降落过程中,舰船甲板会形成"前低后高"的压力分布特征,倾转旋翼RMS气动载荷值也会明显增加,降低了着舰安全性,且右旋翼RMS气动载荷值比左旋翼平均大一倍以上,这也表明右旋翼面临着更加严峻的气动环境。     

县域土地利用与生态环境关系探讨

以福建省云霄县作为探讨案例，根据存在的生态环境问题，并结合土地利用现状，提出创建环境友好型土地利用模式、大力加强生态建设、加强区域环境整治力度三点建议，从而探讨县域土地利用与生态环境协调发展的可行性。     

重庆都市经济圈土壤Cd元素含量分布特征与评价

通过重庆都市经济圈网格化深浅层土壤及评价样品的调查分析,阐述重金属Cd区域上的分布现状,并绘制土壤Cd元素环境质量分级图.研究区浅层土壤Cd背景平均值0.27μg/g,深层0.13μg/g.根据《土壤环境质量标准》对区内土壤进行统计分类,区内浅层土壤Cd元素Ⅱ类土及以上土类面积为83.97%.土壤Cd高含量值主要分布在金刀峡镇北、含谷—白市驿、木耳—王家和玉峰山镇等区域.含谷—白市驿、木耳—王家、西彭北等区域的高Cd含量受人类活动影响比较明显,其中含谷—白市驿区Cd主要来源于生活垃圾、排污底泥和降尘,而金刀峡镇北的高Cd含量属自然背景变化的范畴.