接触热阻的研究进展

在航天器的热控设计中,接触热阻是重要参数之一,其取值准确与否直接关系到热控设计的质量。从理论及实验研究两个方面系统介绍了接触热阻研究的发展状况,在理论研究方面综合叙述了单点理论、多点接触理论这两种理论模型;在实验方面综合叙述了接触热阻的测量方法及导热填料的应用;最后还介绍了接触热阻研究的其它方面。     

一种接触热阻的数值计算方法

分别采用截锥体、圆弧形和三角形模型来模拟实际物体的接触面 ,利用DELAUNAY三角形非结构化网格离散温度场 ,并使用有限元法数值计算接触热阻。通过比较几种模型的计算结果 ,提出控制角为 30°的三角形模型有较高的精度。给出接触热阻的近似计算公式 ,并分析了表面粗糙度对接触热阻的影响 ,所得出的结论在工程实际应用上有一定的参考价值     

二维物体相交检验的线性四叉树方法

在物体的平面布局问题中，判别两个物体是否相交是一个难点，以往的方法数据结构不统一，计算量大，算法复杂，本文首先讨论了二值图象的线性四叉树的表示及其有关术语和性质，然后在此基础上首次提出了二维物体相交检验的线性四叉树方法及其实现的算法，最后进行了算法的时空分析，与以往的方法相经，本文所提方法具有数据结构统一，算法简单，时空效率高等优点。     

Constraints on a hadronic model for unidentified off-plane galactic gamma-ray sources

Recently the H.E.S.S. collaboration announced the detection of an unidentified gamma-ray source with an off-set from the galactic plane of 3.5°: HESS J1507-622. If the distance of the object is larger than about one kpc it would be physically located outside the galactic disk. The density profile of the ISM perpendicular to the galactic plane, which acts as target material for hadronic gamma-ray production, drops quite fast with increasing distance. This fact places distance dependent constraints on the energetics and properties of off-plane gamma-ray sources like HESS J1507-622 if a hadronic origin of the gamma-ray emission is assumed. For the case of this source it is found that there seems to be no simple way to link this object to the remnant of a stellar explosions.     

A sample collector for robotic sample return missions I: Temperature effect on collected mass

Sample return is playing an increasingly important role in solar system exploration. Among the possible mission on the horizon, are sample return from asteroids, comets, the Moon and Mars. A collector initially intended for near-Earth asteroids is the touch-and-go-impregnable-pad (TGIP). Here we explore the effect of temperature on its collection capabilities. Temperatures expected on near-Earth asteroid mission targets range from −43 to 36 °C. Experiments were conducted at −75, −50, −25, 23, 65, and 105 °C. It was found that the mass of sample collected by the TGIP increased almost linearly to 23 °C and then leveled off at higher temperatures. We also found that the collector did not lose its ability to collect samples after being subjected to −75 °C temperatures (essentially frozen) and then thawed. These experiments have shown that the TGIP can operate effectively at temperatures expected on near-Earth asteroids, especially if collection is performed on the sunward side of the asteroid.     

桥函数及广义桥函数的研究进展

桥函数和广义桥函数均为三值函数系,都是将初始序列经复制方式和移位方式变换后而形成的.它们包括了一些常见的非正弦正交函数,如沃尔什函数和方波函数等.简要介绍了近10年来北京航空航天大学通信与电子系统博士点在非正弦正交函数方面研究的一些新进展,重点介绍了复制理论和广义复制方法,桥函数、广义桥函数的复制生成方法、性质及其应用等专题.      

动态湿润与动态接触角的实验

利用精密步进电机、高速CCD图像采集系统、立体显微镜,采用液槽法测试硅酮油在玻璃、铝、不锈钢表面上的动态湿润行为。实验结果与前驱膜模型对比表明,无量纲参数λ在玻璃、铝和不锈钢表面上分别取值0.07,0.16和0.35时,二者吻合较好,表明动态接触角不仅是静接触角和毛细数的函数,也和固体表面性质有关。实验同时发现,对于低毛细数下成立的Hoffman-Voinov-Tanner定律(Cazabat推荐适用于CaD<1或θD<10°),直到动态接触角达到70°依然成立,用前驱膜模型可给出合理解释。      

橡胶"O"形密封圈结构参数和失效准则研究

利用大变形、接触的非线性有限元理论建立了某固体火箭发动机密封结构的二维轴对称模型,用有限元软件计算出该结构在工作状态下的变形和应力。通过计算可知,在橡胶“O”形密封圈与上下法兰接触的位置产生最大的接触压应力,在密封槽槽口转角位置产生最大的剪切应力。对密封性能的各结构参数进行了分析,讨论了上下法兰张开间隙、初始压缩率、密封槽槽口及槽底倒角半径、密封槽宽、密封圈材料等典型参数的影响:上下法兰张开间隙、密封圈的初始压缩率对最大接触压应力的影响较大,而密封槽槽口和槽底处倒角半径对剪切应力影响明显。三维壳体结构的有限元分析结果表明,上下法兰在内压作用下产生不均匀的张开间隙,体现了三维结构的特点。不均匀的张开间隙与二维轴对称结果对比可知,以最小间隙作为设计间隙,二维轴对称分析模型可取代三维模型来分析该结构的密封性能。最后,确定了“O”形圈密封结构的最大接触应力和剪切应力失效准则。     

A new eclipsing low-mass X-ray binary with a giant companion

We detected hard X-ray emission from the unidentified Galactic bulge source 1RXS J175721.2-304405 with ASCA. The observed absorption column, flux and power-law index led us to consider that 1RXS J175721.2-304405 may be a new low-mass X-ray binary located near the Galactic center. Furthermore, the X-ray light-curve shows a step-function-like time variability, which is likely due to the occultation of a companion star. Future follow-up observations by missions such as ASTROSAT may reveal a periodic eclipse from 1RXS J175721.2-304405 if it is covered long enough. Since the long orbital period suggests a giant companion, follow-up observations will give firm evidence that 1RXS J175721.2-304405 is a new and rare eclipsing low-mass X-ray binary with a giant companion.     

带冠预扭涡轮叶片模态分析及动应力测试验证

介绍了航空发动机带冠预扭涡轮叶片非线性接触预应力模态分析机理,并以ANSYS软件为平台,对某型涡轴发动机动力涡轮叶片进行了模态分析。结果表明：非线性接触预应力模态分析方法得到的叶片盘9～13节径1阶频率与动应力测试频率在变化规律上保持一致,差别基本稳定在12%～13%,计算精度较传统方法有了明显的提高。