翼型在自适应壁风洞中试验时的侧壁边界层三元效应研究

二元翼型试验时模型安装于侧壁转盘上会引起侧壁边界层三元效应，中国航空研究院西北工业大学和德国宇航院哥廷根流体力学研究所合作用计算和试验方法进行了研究。作者介绍了1995～1998年的研究，包含研究目的，方案，计算方法，在德国路德维希管风洞中的验证试验，结果分析和初步结论。     

PRD—149:一种应用于低变形增强和低回潮率的新型超高模量芳纶纤维

本文讨论了PRD—149这种新型超高模量Kevlar(芳纶)纤维的形貌及物理性能。该纤维结晶度高,具有独特的超晶态结构。其细纱的抗张强度为2.3～2.6GPa,抗张模量为162～175GPa,而市场供应的Kevlar—49纤维的抗张强度约为2.8GPa,抗张模量约为121GPa(与纤维型号和旦数有关)。PRD—149的高结晶度减小了纤维的蠕变和回潮率。纤维性能在复合材料中转化较好。其环氧浸渍原丝模量与高强碳纤维相近。预料它能在许多领域,从光导纤维电缆增强材料到芳纶/碳纤维混杂复合材料中得以应用。     

一个包括气相和亚表面反应的过氯酸铵复合推进剂的点火模型

本文提出了 Ap 基复合推进剂点火的一个综合模型及其数值解。这一分析模拟位于滞止区的推进剂试样在快速加压条件下的点火过程。本模型的特点包括:a)考虑了 Ap 基复合推进剂点火的详细的化学动力学资料;b)推进剂几何形状是二维(轴对称)的;c)考虑了气相中压力迅速增加对点燃过程的影响。使用隐式有限差分格式求解瞬态二阶联立、非齐次、非线性偏微分控制方程组。数值解揭示在点火阶段顺序发生的一系列重要事件,包括:点火器气体流入接近样品表面的区域;压缩波到达处未燃成份的燃烧;向推进剂传热;氧化剂和燃烧剂的高温分解;气相反应导致点燃。这个模型正确地预测了实验观察到的现象:随着增压速率提高,点火延迟时间缩短。采用文中考虑的不同点火准则都得到和试验一样的趋势。     

从聚硫到丁羧—固体推进剂粘合剂化学的主要变化

从1945年到1949年,液体聚硫粘合剂的复合同体推进剂,由于它在硫化前易于加工,在硫化后具有良好的机械性能和粘合强度,因而达到了可以扩大生产的工艺水平。这些发展导致了浇注——壳体粘结方法,在五十年代成功的用在一些火箭发动机上。到1954年,开始合成含有可固化官能团的液体聚丁二烯粘合剂。聚丁二烯最终取代聚硫粘合剂,有如下几个原因:较高的比冲、优良的老化性能及较好的高、低温机械性能。本文评述了这些配方的发展历史,并介绍了从乙基缩甲醛、丁基缩甲醛、丁醚聚硫到聚丁二烯丙烯酸(PBAA)、聚丁二烯丙烯腈(PBAN)和端羧聚丁二烯(CTPB)的变革原因。给出了典型配方实例、性能及其存在的问题。     

Early renal changes in 45 degrees HDT rats

Background: Both microgravity and simulated microgravity models, such as the 45HDT (45 degrees head-down tilt), cause a redistribution of body fluids indicating a possible adaptive process to the microgravity stressor. Understanding the physiological processes that occur in microgravity is a first step to developing countermeasures to stop its harmful effects, i.e., (edema, motion sickness) during long-term space flights. Hypothesis: Because of the kidneys' functional role in the regulation of fluid volume in the body, it plays a key role in the body's adaptation to microgravity. Methods: Rats were injected intramuscularly with a radioactive tracer and then lightly anesthetized in order to facilitate their placement in the 45HDT position. They were then placed in the 45HDT position using a specially designed ramp (45HDT group) or prone position (control group) for an experimental time period of 1 h. During this period, the 99mTc-DTPA (technetium-labeled diethylenepentaacetate, MW=492 amu, physical half-life of 6.02 h) radioactive tracer clearance rate was determined by measuring gamma counts per minute. The kidneys were then fixed and sectioned for electron microscopy. A point counting method was used to quantitate intracellular spaces of the kidney proximal tubules. Results: 45HDT animals show a significantly (p=0.0001) increased area in the interstitial space of the proximal tubules. Conclusions: There are significant changes in the kidneys during a 1 h exposure to a simulated microgravity environment that consist primarily of anatomical alterations in the kidney proximal tubules. The kidneys also appear to respond differently to the initial periods of head-down tilt.     

涡轮叶栅前缘上游端壁气膜冷却的流场实验研究

对前缘上游端壁有单排和双排孔冷却的大尺寸低速涡轮导向叶栅进行了气动测量、热示踪和端壁流场显示,在吹风比1～3范围获得了叶栅内的详细流场、冷气的空间分布和端壁上的流动图案。结合先前测得的没有冷却时的流场数据,这些结果表明端壁气膜冷却对叶栅流场结构有重大影响,吹风比是主宰射流与二次流间相互作用的主要因素,双排孔喷射使冷气比单排孔喷射更贴近端壁。低吹风比喷射冷气不能到达压力面并被二次流逐渐卷离端壁;中吹风比喷射有效的抑制了二次流的形成,并使端壁流线偏向于无粘流流线,冷气很均匀的覆盖在端壁上。      

Space-to-space Radio Interferometry System from Medium Earth Orbits

This paper presents a new concept to perform space-to-space Very Long Baseline Interferometry which enables the imaging of cosmic sources at high-resolution and high-sensitivity with small antennas. Several individual apertures are embarked on separate identical satellites staggered in height into Polar or Equatorial Circular Medium Earth Orbits (PECMEO orbits). These orbits are stable and allow GNSS-based on-the-fly centimeter-level relative positioning. Coherent operation is possible by exchanging local oscillator components and measured signals through Inter-Satellite Links (ISL). On-board cross correlation is performed at each satellite over a delay window compatible with the accuracy of the on-the-fly relative positioning and the result sent to the ground. Image reconstruction is completed on the ground thanks to sub-millimeter baseline retrieval from accurate GNSS orbits, ISL ranging and spacecraft attitude information. The application of this concept to image the Super Massive Black Hole Sgr A* is hinted.      

A reappraisal of the habitability of planets around M dwarf stars

Stable, hydrogen-burning, M dwarf stars make up about 75% of all stars in the Galaxy. They are extremely long-lived, and because they are much smaller in mass than the Sun (between 0.5 and 0.08 M(Sun)), their temperature and stellar luminosity are low and peaked in the red. We have re-examined what is known at present about the potential for a terrestrial planet forming within, or migrating into, the classic liquid-surface-water habitable zone close to an M dwarf star. Observations of protoplanetary disks suggest that planet-building materials are common around M dwarfs, but N-body simulations differ in their estimations of the likelihood of potentially habitable, wet planets that reside within their habitable zones, which are only about one-fifth to 1/50th of the width of that for a G star. Particularly in light of the claimed detection of the planets with masses as small as 5.5 and 7.5 M(Earth) orbiting M stars, there seems no reason to exclude the possibility of terrestrial planets. Tidally locked synchronous rotation within the narrow habitable zone does not necessarily lead to atmospheric collapse, and active stellar flaring may not be as much of an evolutionarily disadvantageous factor as has previously been supposed. We conclude that M dwarf stars may indeed be viable hosts for planets on which the origin and evolution of life can occur. A number of planetary processes such as cessation of geothermal activity or thermal and nonthermal atmospheric loss processes may limit the duration of planetary habitability to periods far shorter than the extreme lifetime of the M dwarf star. Nevertheless, it makes sense to include M dwarf stars in programs that seek to find habitable worlds and evidence of life. This paper presents the summary conclusions of an interdisciplinary workshop (http://mstars.seti.org) sponsored by the NASA Astrobiology Institute and convened at the SETI Institute.     

新时期航空航天工业的标准战略

本文是荣获美国庆祝2004年世界标准日论文竞赛头奖的作品,中心内容是在新世纪航空航天工业如何在广泛国际合作,信息技术迅猛发展的环境下结合本行业的实际,制定并适时调整其标准战略。文中分析问题的方法,解决问题的思路具有某种普遍意义,现将该文详细摘译刊登于下,供参考。     

Modelling of Geomagnetic Storm Effects in the Ionosphere of East Asia

This paper presents simulated results of the ionospheric behavior during few geomagnetic storms,which were occurred in the different seasons. The numerical model for ionosphere-plasmasphere coupling was used to interpret the observed variation of ionosphere structure. Reasons why the positive storms are dominant in the winter whereas the negative ones are dominant in the summer season present the special interest for the mid-latitude ionosphere. A theoretical analysis of the processes controlling the ionospheric response to the geomagnetic storms has showed a good agreement between the simulated results and measurements, as well as the crucial role of the neutral composition variations to fit the calculated and the observed ionospheric parameters.