Structural dynamic responses of a stripped solar sail subjected to solar radiation pressure

The stripped solar sail whose membrane is divided into separate narrow membrane strips is believed to have the best structural efficiency. In this paper, the stripped solar sail structure is regarded as an assembly made by connecting a number of boom-strip components in sequence. Considering the coupling effects between booms and membrane strips, an exact and semi-analytical method to calculate structural dynamic responses of the stripped solar sail subjected to solar radiation pressure is established. The case study of a 100 m stripped solar sail shows that the stripped architecture helps to reduce the static deflections and amplitudes of the steady-state dynamic response. Larger prestress of the membrane strips will decrease stiffness of the sail and increase amplitudes of the steady-state dynamic response. Increasing thickness of the boom will benefit to stability of the sail and reduce the resonant amplitudes. This proposed semi-analytical method provides an efficient analysis tool for structure design and attitude control of the stripped solar sail.     

An update global model of hmF2 from values estimated from ionosonde and COSMIC/FORMOSAT-3 radio occultation

In this paper, we present our recent work on developing an updated global model of the ionospheric F2 peak height hmF2 parameter by combining data from the Constellation Observing System for Meteorology, Ionosphere and Climate (COSMIC/FORMOSAT-3) radio occultation (RO) measurements and from the extended global ionosonde stations. In particular, 10 Chinese ionosonde stations’ data are newly introduced into this study. The modeling technique used is based on a two-layer empirical orthogonal function (EOF) expansion. Global distributions of hmF2 maps calculated using the newly constructed global model and the one provided by the International Reference Ionosphere model (IRI-ITU-R) are compared with the global distributions of hmF2 obtained by the COSMIC RO measurements and quantitative statistical analysis of the differences between the model results and those of the COSMIC RO measurements is made for the low (2008) and high (2012) solar activity years. The obtained average root-mean-square differences (RMSEs) for our model are 27.7 km (11.1%) and 31.0 km (9.8%), respectively for the years 2008 and 2012, whereas those for the IRI-ITU-R model are 39.9 km (16.9%) and 35.0 km (11.6%), respectively. Comparison of the results calculated both by our model and the IRI-ITU-R model with the digisonde observation is also made. The comparisons show that the newly constructed global hmF2 model can reproduce reasonably well the observations and perform better than IRI-ITU-R model.     

一种姿控动力装置热防护研究

酚醛树脂作为一种烧蚀材料,凭借其耐高温的特性应用于航天器防热系统,其防热性能在工程实际中需进行考核。以某航天器一段包覆80纤维布/酚醛树脂的液路管路作为研究对象,以定热流为边界条件,采用仿真计算和热流试验的研究方法对空导管以及注水导管的温度场进行研究:仿真计算得出导管表面平衡温度分布以及导管表面具有代表性某点瞬态温度变化;为验证仿真计算的准确性,进行了热流试验,得出了导管表面以及水中温度测点的瞬态温度变化;根据热流试验的温度结果,分析比对了热流试验对仿真计算的验证情况。研究结果表明:80纤维布/酚醛树脂的防热性能符合温度指标要求;仿真结果和热流试验结果一致度良好,证明了仿真计算的合理性和准确性。     

On extended thermonuclear functions through pathway model

The major problem in the cosmological nucleosynthesis is the evaluation of the reaction rate. The present scenario is that the standard thermonuclear function in the Maxwell–Boltzmann form is evaluated by using various techniques. The Maxwell–Boltzmannian approach to nuclear reaction rate theory is extended to cover Tsallis statistics (Tsallis, 1988) and more general cases of distribution functions. The main purpose of this paper is to investigate in some more detail the extended reaction probability integral in the equilibrium thermodynamic argument and in the cut-off case. The extended reaction probability integrals will be evaluated in closed form for all convenient values of the parameter by means of residue calculus. A comparison of the standard reaction probability integrals with the extended reaction probability integrals is also done.     

PCB电源地层腔模辐射快速算法

电路板电源总线的分析非常复杂,虽然传统腔模方法是分析电路板电源总线的一种非常有效的方法,但是该方法具有收敛速度慢,计算时间长和不能分析电源总线辐射发射的缺点.在该算法的基础上,改进二重级数和形式的电源总线辐射发射方法并提出了单一级数和形式的电源总线辐射发射表达式.在此基础上指出了单一级数腔模理论解的适用条件,并对该快速算法的收敛性进行了分析.分析表明,该方法减少了传统二重级数求和的计算工作量,提高了收敛效率并节省了计算时间,而且能够有效逼近双级数腔模辐射算法的计算结果.通过对电路板的辐射发射数值仿真验证了该算法的有效性和正确性.     

结构可靠度逐步逼近径向基神经网络响应面法

提出了逐步逼近径向基神经网络响应面法计算结构可靠度,这种数值方法较好地解决了结构功能函数非线性及结构随机变量非正态分布时采用结构可靠度指标度量结构可靠度存在误差的问题.经过多个数值试验表明,该算法迭代收敛迅速、计算准确性较高、应用过程简单.利用这种方法对含有多个随机变量的结构进行可靠性分析和设计,特别是当结构功能函数具有较强的非线性或结构随机变量分布具有较大的偏斜度时,具有一定的应用价值.      

基于一种匹配函数的ATS资源自动配置方法

提出采用匹配函数描述测试点与仪器端口的匹配程度,用来指导自动测试系统仪器选型和资源配置.匹配函数采用面向信号的方法构建,综合了测点信号属性与仪器性能参数、仪器可靠性、仪器成本、仪器操作复杂度等因素,使得仪器选型和资源配置策略的制定更符合工程需要.给出了资源配置策略和算法,并对资源配置进行了并行测试优化.通过给出一个典型实例,证明该方法能有效降低测试成本,增强系统可靠性,提高测试效率和吞吐量,并为自动测试系统硬件设计的自动化奠定了基础.      

氨质子化团簇红外振动光谱研究

运用Gaussian03W计算程序,在B3LYP／6—31G（d）方法水平上得到了氨质子化团簇（NH3）nH^＋（n=1～8）的最稳定构型,并对其相应红外振动光谱进行了研究。通过对红外振动光谱中谱峰位置与振动模式之间的关系的分析,发现光谱中的最强峰均来自于NH4^＋核中N—H键的反对称伸缩振动（n=2除外）。     

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.      

平滑粒子流体动力学(SPH)方法的进展

平滑粒子流体动力学(SPH)方法是一种无网格Lagrangian计算技术,在处理一些问题时,比以Lagrangian坐标系和Eulerian坐标系为基础的常规网格有独特的优越性,特别适用于处理物质质点的流动性极大的问题,如超高速碰撞问题.文章对SPH的理论和计算方法做了简单的介绍,并对其发展过程和现状做了简单的回顾.