薄膜材料和纤维材料的热扩散率测量

介绍了激光热波技术用于测量薄膜材料和纤维材料热扩散率的测试系统，测试温度范围为２０－５００℃。讨论了测量中的各种试验条件、基本公式和误差分析。在理论上此系统可以应用于任何厚度样品面向热扩散率的测量。     

薄膜温度传感器的研制及应用

一种新型的薄膜温度传感器,采用真空镀膜的方法制作在涡轮叶片表面,两者构成一体,可以真实反应表面温度。传感器的质量小、响应快,对叶片内部换热和表面燃气流无干扰。 传感器的敏感元件为铂姥_(10)-铂热电偶,测温上限可达1000℃,测量精度为±3％。     

气、液组合膜流对壁面冷却效果的理论及试验研究

本文针对液膜及气膜组合流动的特点,提出了组合薄膜流动的“四层式流场物理模型”.根据所做简化、假设,对液膜区流场结构及冷却效果进行了理论计算,并通过分析方法,对其紧接的气膜段流动及冷却效果进行了理论预估.试验的结果表明:液膜段的理论计算与试验数据基本相符.并从试验中发现了液膜蒸干后气膜段冷却的一些特点.这对研究液体冷却时液膜及气膜组合流动的冷却效果提出了可行的途径.     

Energetic particles at high latitudes

We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path _r which is approximately constant as a function of distancer. When particle propagation in three dimensions in the heliosphere is considered it is not sufficient to consider _r only. Jovian electrons can be used as probes to determine the parameters of three-dimensional diffusion. In the polar regions diffusion is dominated by its parallel component. Some predictions how should vary with latitude are discussed. For different choices of this variation we present expectations for intensity-time profiles of solar particle events during the Ulysses polar passages.     

挤压油膜阻尼器的均匀两相流模型

在挤压油膜阻尼器内气穴现象实验研究的基础上，对挤压油膜因气穴现象而发生物理特性的变化进行了讨论。气液均相流模型作为挤压油膜的近似描述，导出了上述模型的密度和粘度与油膜压力之间的关系式。定性地分析了当挤压油膜采用这一可压缩模型时，其压力分布的描述更能与实际接近，对阻尼器的力学特性的准确预测有重要的参考价值。     

弹性环式挤压油膜阻尼器实验研究与应用

实验证实了弹性环式挤压油膜阻尼器（ＥＲＳＦＤ）的油膜阻尼的存在,并研究了ＥＲＳＦＤ的减振、调频特性。将ＥＲＳＦＤ应用于某核心机减振、调频,其效果很好,ＥＲＳＦＤ在某核心机上获得成功应用。实验和应用研究表明ＥＲＳＦＤ有优良的减振、调频性能。     

Solar Irradiance Variability Since 1978

Since November 1978 a set of total solar irradiance (TSI) measurements from space is available, yielding a time series of more than 25 years. Presently, there are three TSI composites available, called PMOD, ACRIM and IRMB, which are all constructed from the same original data, but use different procedures to correct for sensitivity changes. The PMOD composite is the only one which also corrects the early HF data for degradation. The results from the detailed analysis of the VIRGO radiometry allow a good understanding of the effects influencing the long-term behaviour of classical radiometers in space. Thus, a re-analysis of the behaviour of HF/NIMBUS-7 and ACRIM-I/SMM was indicated. For the former the situation is complicated by the fact that there are no in-flight means to determine changes due to exposure to solar radiation by comparison with a less exposed radiometer on the same spacecraft. The geometry and optical property of the cavity of HF is, however, very similar to the PMO6-type radiometers, so the behaviour of the PMO6V radiometers on VIRGO can be used as a model. ACRIM-I had to be revised mainly due to a henceforth undetected early increase and a more detailed analysis of its degradation. The results are not only important for solar radiometry from space, but they also provide a more reliable TSI during cycle 21. The differences between the revised PMOD composite and the ACRIM and IRMB are discussed by comparison with a TSI reconstruction from Kitt-Peak magnetograms. As the PMOD composite is the only one which has reliable data for cycle 21, the behaviour of the three solar cycles can now be compared and the similarities and differences discussed.     

Global Response of Martian Plasma Environment to an Interplanetary Structure: From Ena and Plasma Observations at Mars

As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board the Mars Express satellite. The “subsolar ENA jet” is generated by the interaction between the solar wind and the Martian exosphere, and is one of the most intense sources of ENA flux observed in the vicinity of Mars. On June 7, 2004 (orbit 485 of Mars Express), the NPD observed a very intense subsolar ENA jet, which then abruptly decreased within ∼10 sec followed by quasi-periodic (∼1 min) flux variations. Simultaneously, the plasma sensors detected a solar wind structure, which was most likely an interplanetary shock surface. The abrupt decrease of the ENA flux and the quasi-periodic flux variations can be understood in the framework of the global response of the Martian plasma obstacle to the interplanetary shock. The generation region of the subsolar ENA jet was pushed towards the planet by the interplanetary shock; and therefore, Mars Express went out of the ENA jet region. Associated global vibrations of the Martian plasma obstacle may have been the cause of the quasi-periodic flux variations of the ENA flux at the spacecraft location.     

带密布气膜冷却孔的涡轮叶片等效应力分析方法研究

以带气膜冷却孔的航空燃气涡轮发动机涡轮叶片为研究背景,引入了等效概念对密布小孔结构进行了详细的应力-应变分析。这种等效分析方法是把多孔材料转化为具有等效材料常数的等效实体材料。根据MARC大型通用软件的线弹性及弹-塑性有限元应力分析结果,将小孔效应转化为等效弹性常数及等效应力-应变曲线。最后以某发动机高压涡轮工作叶片为例,将得到的等效材料参数引入到叶片的有限元强度计算中,从而得到考虑密布孔影响的涡轮叶片应力应变场,并通过子模型计算得到更为准确的孔边最大应力。