HEDM－CMDB推进剂燃烧性能的理论预测

利用建立不久的双基系平台推进燃烧模型，对几种ＨＥＤＭ加入平台推进剂后的燃烧性能进行了理论计算。结果表明：在所计算的几种ＨＥＤＭ中，ＨＮＨＡＡ最有利于提高燃速；ＣＬ－２０最有利于降低燃速压力指数；ＣＬ－２０作为平台推进剂的高能填料综合性能最好。     

TRANSONIC WALL IN TERFERENCE CORRECTIONS FOR CIVIL AIRCRAFT MODEL TESTS

ＴＲＡＮＳＯＮＩＣＷＡＬＬＩＮＴＥＲＦＥＲＥＮＣＥＣＯＲＲＥＣＴＩＯＮＳＦＯＲＣＩＶＩＬＡＩＲＣＲＡＦＴＭＯＤＥＬＴＥＳＴＳＦａｎＺｈａｏｌｉｎ；ＣｕｉＮａｉｍｉｎｇ；ＹｕｎＱｉｌｉｎ；ＹｉｎＬｕｐｉｎ（ＣｈｉｎａＡｅｒｏｄｙｎａｍｉｃｓＲｅｓｅａｒ...     

哈尔滨空气动力研究所近期发展的几项流态观察与显示技术

本文介绍了哈尔滨空气动力研究所近期发展的三项流态观察与显示技术,即彩色氦气泡流态显示,复合式片光流态显示和计算机控制的彩色图像流态显示技术。给出了它们的基本工作原理,主要技术性能和应用。     

AP与HMX作用的“连锁互动”机制

研究了NEPE推进剂中AP与HMX的相互作用。基于凝相机理与热解实验,从分子层面和化学反应的角度,结合价键、形式电荷、链反应等理论和固体单元推进剂的燃烧状况,提出了AP与HMX间的“连锁互动”机制。有NH3与NO2等活性物种参与的“放热连锁、物种互动”过程,可以有效提高NEPE推进剂燃速并在一定程度上改善其燃烧性能。     

高性能铝基复合材料的颗粒分布及界面结合

采用常规粉末冶金和高能球磨粉末冶金法制备了B4Cp/Al复合材料，研究了B4C颗粒分布与界面结合特点、形成机制以及对材料性能的影响。结果表明，17％（体积分数）B4Cp/6061Al复合材料的屈服和抗拉强度分别为415MPa和470MPa，比常规粉末冶金复合材料分别提高了69％和70％。微观分析表明，高能球磨粉末冶金复合材料中B4C颗粒均匀分布、颗粒与基体之间存在近百纳米厚度的界面层，界面层由呈带状且有序分布的微细铝晶粒和弥散分布的纳米颗粒组成。高能球磨过程中，铝粉末在钢球表面形成冷焊层，B4C不断被挤入而均匀化是实现颗粒均匀分布的主要机制；球磨过程中铝粉末表面氧化层破碎暴露出新鲜铝表面且与镶嵌与铝粉末中的B4C颗粒形成界面结合是获得良好界面结合复合材料的重要条件     

新型太阳能利用装置的研究

对目前太阳能的几种常见的应用领域及相关装置进行了分析和研究,并在此基础上,结合相关理论,设计了利用太阳能的新型装置,如:太阳能房、太阳能热发电装置、聚光式太阳能电池发电装置等,这些装置将为更好地利用太阳能开辟新的途径.太阳能作为一种新兴的可再生能源有着不可限量的发展前景.     

Deep Impact: A Large-Scale Active Experiment on a Cometary Nucleus

The Deep Impact mission will provide the first data on the interior of a cometary nucleus and a comparison of those data with data on the surface. Two spacecraft, an impactor and a flyby spacecraft, will arrive at comet 9P/Tempel 1 on 4 July 2005 to create and observe the formation and final properties of a large crater that is predicted to be approximately 30-m deep with the dimensions of a football stadium. The flyby and impactor instruments will yield images and near infrared spectra (1–5 μm) of the surface at unprecedented spatial resolutions both before and after the impact of a 350-kg spacecraft at 10.2 km/s. These data will provide unique information on the structure of the nucleus near the surface and its chemical composition. They will also used to interpret the evolutionary effects on remote sensing data and will indicate how those data can be used to better constrain conditions in the early solar system.     

FL-9低速增压风洞主体结构有限元分析与气压试验

FL-9低速增压风洞是“十五”国家批准建设的大型航空基础设施，笔者简要介绍了该风洞基于有限元方法的应力、变形和模态分析，并与风洞气压试验结果进行了对比。结果表明：有限元计算中所采用的单元类型、模型简化、边界约束等处理方法合理可行，应力计算值与实测值比较一致，最大薄膜应力为147．6MPa，低于许用值42．1％，风洞结构具有较大的安全裕度。风洞的前六阶模态分析为风洞安全运行提供了参考依据。     

Influence of the Solar Cycle on the General Circulation of the Stratosphere and Upper Troposphere

The record of dynamical structure reveals a systematic variation that operates coherently with the 11-yr variation of UV irradiance. Involving periods shorter than 5 years, the systematic variation reflects the influence of the QBO on the polar-night vortex. It has the same basic structure as interannual changes associated with the residual mean circulation of the stratosphere. A signature of the solar cycle also appears in the direct correlation to solar flux, as recovered through regression of the entire monthly record. That signature, however, is sharply enhanced around solstice, when the residual circulation is active, and during extremal phases of the QBO. In the tropics, the solar signature follows, throughout the year, from a decadal modulation in the frequency of the QBO. The modulation is manifested to either side of the QBO’s mean frequency, in two spectral peaks where the QBO dwells: one at (24 months)⁻¹, reflecting a Biennial Oscillation (BO), and another at (36 months)^-1. Intrinsic to the QBO, those peaks are separated from its mean frequency by ∼11 years⁻¹.Through the QBO’s residual circulation, the decadal modulation introduces anomalies in the subtropics, with symmetry about the equator. Accompanying anomalous temperature in the subtropics is a stronger signature over the winter pole. Discovered by Labitzke and van Loon 1988, that solar signature reflects anomalous downwelling of the Brewer-Dobson circulation. It is shown to follow through the BO, which is intrinsic to the QBO and its modulation of the polar-night vortex.     

高超侧压式进气道参数分析及试验研究

分析了高超侧压式进气过第一、二溢流窗的溢流角随后掠角的变化规律，分析了溢流窗气流与主流相互作用而形成一道脱体曲面激波的原因，设计了侧压角为６°，后掠角３０°的直前缘及圆弧前缘两套高超侧压式进气道，在Ｍ５．３风洞中利用风洞壁面自然发展的附面层进行非均匀来流下进气道起动性能及总体性能试验，试验发现大量附面层吸入不仅对起动性能有重大影响，而且对总压恢复影响也极大。