多体全自由飞过程的数值模拟

以三维非结构粘性直角网格重构为构架,数值求解了固定空间网格瞬间运动边界的N-S方程,逼近了流场的非定常过程,结合六自由度的弹道方程,对单体或多体运动过程进行了全自由飞数值模拟,数值模拟结果和级间分离的风洞自由飞试验进行了对比,初步的计算结果说明,全自由飞数值模拟在一定程度上可以描述风洞试验的飞行轨迹,并且适应能力更强,整个全自由飞数值模拟系统可以为更复杂的单体机动飞行或多体运动过程提供快速实用的数值模拟方法.     

高超声速锥体表面凸起物分离干扰区气动力/热关联计算方法

针对高超声速锥体表面凸起物周围的分离干扰流动产生的气动力/热提供了关联计算方法,包括凸起物周围分离干扰区压力分布计算方法、分离干扰区几何特征的计算方法、分离干扰区附加气动力计算方法、分离干扰区气动热计算方法.对典型的钝锥加凸起物外形进行了计算,计算分析了由于凸起物周围分离干扰区压力升高引起的附加气动力、凸起物表面及干扰区的气动热,对气动热计算结果与激波风洞实验结果进行了比较,本文关联方法计算结果与实验结果符合较好.     

活塞裙部外圆复杂型面在位检测及其误差修正

提出了一种基于Windows环境下的活塞裙部外圆复杂型面在位检测的新方法,并设计了在位检测的软、硬件系统.同时,根据活塞裙部型面的特点,在现有常用误差处理算法的基础上进行了改进,新的误差处理方法具有更强的适用性.     

试用暗物质理论解释惯性和惯性力的物理机制(上)

基于对暗物质的多年探讨,我们认为宇宙空间是具有质量、相对均匀、连续稳定和有相当弹性暗物质群体(DMG)的空间.自然、宇宙万物终生处于群体引力制约之中,它们因此也获得了相应的惯性.本文立足于上述的宇宙空间,借助宇宙学原理、马赫原理和爱因斯坦等效原理,提出了物质客体的惯性机制和被称为虚力的惯性力机制 同时本文也解读所有惯...     

干涉测长中测量湿度的一种新方法

介绍了一种通过测量相对湿度和空气温度来计算湿度值的方法，并推导了计算公式。     

双满壳层附近原子核的双粒子能谱

采用由M-3Y力等效G矩阵,用格林函数方法对Ca42、Sc42、N i58和Cu58的双粒子能谱做了理论计算和讨论.结果表明:二级图中3p1h不可约顶角考虑多重散射后,使能级更趋于实验能级.因此用格林函数方法计算双粒子能谱是十分有效的。     

激光干涉正弦法小角度测量中有关问题探讨

分析了小角度正弦激光干涉仪的有关特性，叙述了这种方法的测量原理，计算了几种因素对测量准确度的影响，指出提高测量准确度的解决办法。     

卫星测控雷达校飞设备在飞机上的安装

介绍了某型卫星测控雷达的校飞设备以及这些设备在某型飞机上的安装方案，并对方案进行了分析，确保方案的可行性。     

Effective Coulomb force modeling for spacecraft in Earth orbit plasmas

Coulomb formation flight is a concept that utilizes electrostatic forces to control the separations of close proximity spacecraft. The Coulomb force between charged bodies is a product of their size, separation, potential and interaction with the local plasma environment. A fast and accurate analytic method of capturing the interaction of a charged body in a plasma is shown. The Debye–Hückel analytic model of the electrostatic field about a charged sphere in a plasma is expanded to analytically compute the forces. This model is fitted to numerical simulations with representative geosynchronous and low Earth orbit (GEO and LEO) plasma environments using an effective Debye length. This effective Debye length, which more accurately captures the charge partial shielding, can be up to 7 times larger at GEO, and as great as 100 times larger at LEO. The force between a sphere and point charge is accurately captured with the effective Debye length, as opposed to the electron Debye length solutions that have errors exceeding 50%. One notable finding is that the effective Debye lengths in LEO plasmas about a charged body are increased from centimeters to meters. This is a promising outcome, as the reduced shielding at increased potentials provides sufficient force levels for operating the electrostatically inflated membrane structures concept at these dense plasma altitudes.     

Silver Film Growth on Glass Ceramic by Radio Frequency Magnetron Sputtering

Thin silver films are deposited by radio frequency magnetron sputtering on glass ceramic at room temperature.Variations of sputtering power,bios voltage and power density are carried out for each deposition,then parts of as-deposited samples are subjected to annealing at 600 ℃ within a vacuum chamber.Structural properties are studied by X-ray diffraction(XRD),scanning electron microscope(SEM)and laser scanning confocal microscope(LSCM).It is shown that structural properties have a strong dependency on sputtering power and annealing temperature.Electrical contact resistance measured by a four point probe instrument is directly affected by the thickness of films.It is also found that the film conductivity,especially in thinner films,is improved by the increasing grain size.Finally,the film adhesion is observed by scratch tests.And the adhesive ability deposited by radio frequency magnetron sputtering shows a better performance than that produced by traditional methods.