适用于Ad hoc网络的EIGamal型门限数字签名方案

现有ElGamal型门限数字签名方案在签名前签名各方需要协商生成一个随机数,该过程计算量与通信量比较大,不能满足Ad hoc网络的需求.将组合公钥的思想引入到ElGamal型门限数字签名的随机数生成中,为Ad hoc网络提出一种门限数字签名的改进方案.方案由密钥初始化和门限签名两部分组成.密钥初始化时,签名各方使用分布式密钥生成协议协商出系统公/私钥对和一个随机数矩阵,每个节点掌握部分私钥和部分随机数矩阵;门限签名时,每个签名方使用相同的算法在掌握的部分随机数矩阵中选择随机数进行部分签名;最后将部分签名合成整体签名.对提出的方案在随机预言(RO, Random Oracle)模型中进行了安全性证明.实用性分析表明:方案计算复杂度低,交互次数少,通信量小,有很好的执行效率与签名成功率.     

基于点线关系的透视图消隐算法

准确获取建筑物的三维形体信息,在军事和民用上都有非常重要的意义.针对建筑物三维形体获取过程中的消隐问题,提出了一种基于点线关系的三维透视图消隐算法.结合后向面判别法和光线投射算法,利用三维表面模型中点、线、面的遮挡关系和视平面域上的包含性规则,进行边界线段的显、隐程度检查,实现对模型的消隐处理.实验结果表明,该算法数据结构简单,建立的透视投影计算模型正确且消隐算法有效,为地形地物透视图的消隐提供了一种新的方法与支持手段.     

基于有限体积法和SNBCK模型的红外辐射特性计算

耦合求解流场、组分浓度场、基于SNBCK模型的气体辐射传输/能量方程以求准确模拟飞行器排气系统气动热力及红外特性.窄带模型参数由HITEMP逐线计算数据库计算得到.通过CO₂4.3μm波段吸收率计算,圆柱炉膛辐射换热特性计算两个算例验证了所采用程序求解辐射传输/能量方程的准确性.最后计算了两种二元喷管的红外特性,结果表明大宽高比二元喷管地面和空中状态红外辐射特性差异巨大.     

无人机舵面负载模拟系统的小脑模型控制

为解决无人机舵面负载模拟系统中非线性和多余力矩扰动问题,利用小脑模型神经网络非线性逼近能力强、结构简单、适于实时控制等特点,采用小脑模型和传统PD(Proportional-Derivative)控制结合的复合控制策略,由小脑模型实现前馈控制,PD控制实现反馈控制,以保证在系统运行各阶段的控制精度.分析讨论了复合控制的不稳定性问题,研究了基于可信度分配和学习率自适应调整的改进型小脑模型的应用情况,提出一种适用于单输入单输出系统的简化小脑模型复合控制设计方法.仿真结果表明该方法有效地解决了小脑模型和PD复合控制的不稳定问题,改善了系统动态加载性能,并具有很好的抗干扰性能.     

月球软着陆器动力学建模研究

建立准确、实用的月球着陆探测器动力学模型,是制导、导航和控制系统方案设计中的首要工作,文中月球软着陆探测器的推进剂贮箱采用横向对称分散布局的形式,并分析了布局方式对液体推进剂晃动的影响;将贮箱内液体考虑一阶弹簧质量模型,应用虚功率原理建立包含液体推进剂晃动的月球软着陆探测器从动力下降段至最终着陆段的动力学模型,并对动力学下降段进行了数值仿真,仿真结果可为月球软着陆探测器控制系统设计提供理论参考。     

Upper limit of the total magnetic flux in an active region according to the photometric-magnetic dynamical model

The photometric-magnetic dynamical model handles the evolution of an individual sunspot as an autonomous nonlinear, though integrable, dynamical system. One of its consequences is the prediction of an upper limit of the sunspot areas. This upper limit is analytically expressed by the model parameters, while its calculated value is verified by the observational data. In addition, an upper limit for the magnetic strength inside the sunspot is also predicted, and then, we obtain the following significant result: The upper limit of the total magnetic flux in an active region is found to be of about 7.23 × 10²³ Mx, namely, phenomenologically equal to the magnetic flux concentrated in the totality of the granules of the quiet Sun, having a typical maximum magnetic strength of about 12G. Therefore, the magnetic flux concentrated in an active region cannot exceed the magnetic flux concentrated in the photosphere as a whole.     

Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan

Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5°N, 109.1°E; Geomagnetic coordinates: 178.95°E, 8.1°N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity.     

线性特征系统的标准形

本文在可控、可观测的条件下,建立了线性特征系统的标准形,并说明了系统结构参数d_1在建立标准形过程中的作用。对d_1=0的情况,通过上述标准形讨论了矩阵A的生成元所具有的独特性质。     

复合材料格栅结构的强度分析

复合材料格栅结构是由连续纤维缠绕的斜向及环向肋和蒙皮组成的结构。对ANSYS软件进行了二次开发,分别采用层合板和层合梁单元模拟复合材料格栅结构的蒙皮和肋。根据复合材料格栅结构的几何特征及其载荷分布特征,采用周期对称有限元模型,分别以最大应力准则、最大应变准则和蔡-吴准则和Chang刚度退化准则对轴压载荷作用下的复合材料格栅结构破坏过程进行了强度预测,计算结果表明采用蔡-吴准则预测并结合Chang刚度退化准则的计算结果与试验结果的一致性较好。     

幂律型流体射流破碎建模和实验问题探讨

简要回顾了射流破碎研究的现状,讨论了幂律型流体射流破碎建模和实验的相关问题。射流破碎建模的关键在于依据流体的胶凝结构和组份物性,射流与环境气体之间的作用关系,提炼主要影响因素。射流破碎实验研究的关键在于高分辨率和高速成像技术等光学测试技术。建模和实验的主要作用在于揭示射流破碎的机理,分析相关因素的影响,为喷注器雾化研究提供参考,为燃烧室冷却设计提供依据。