非列紧空间的一般非扩张映象的Ishikawa迭代序列

本文证明了Hilbert空间上的非列紧的一般非扩张映象的Ishikawa迭代序列的收敛性。     

基于EAB资源的交织编译码器的设计与实现

提出了一种新的基于EAB资源交织编译码设计方案，利用FPGA技术实现了数字通信中交织器和解交织器，构建了具体的算法模型，并说明了设计中实际产生的问题及解决方法。     

直扩测控系统抗多址能力分析与验证

为了防止多址干扰造成接收机出现误捕和假锁,改善直接序列扩频测控系统抗多址干扰性能,在Gold码特性和扩频接收机性能分析的基础上,结合最大似然原理,对采用扩频体制测控系统的抗干扰能力进行了分析。为契合工程应用,采用仿真遍历结合理论分析的方式,对Gold码的互相关抑制能力理论值进行了工程修正。在分析捕获阶段的抗干扰捕获门限后,还分析了载噪比估计结果在正常锁定和假锁两种状态下的差异,给出了接收机对假锁状态的判决方法和门限。根据分析和仿真的结果,给出了系统设计约束条件和优化的接收机设计流程,作为测控系统和接收机设计的参考。     

综合时序信息的试验优化设计及稀疏求解

考虑不同试验点的试验成本及试验时序信息,在性能指标与影响因素间的响应模型未知情况下,利用装备系统的先验信息构造模型驱动的基函数,构造相应的回归模型来刻画系统的内在关系,分析不同试验点成本及试验时序对试验方案的影响。定义了一种考虑空间权重及批序贯时序的非均匀最优设计模型,将稀疏理论引入到回归试验设计中,把不同批次试验下的回归试验设计模型参数估计问题转换为结构化稀疏重构问题,讨论了非均匀最优设计的构造定理,提出结构化稀疏参数求解算法。算例表明:利用本方法生成的试验点考虑了试验点空间权重和试验时序信息,更符合实际试验规程;采用本方法获得的响应函数得到的期望预测误差更小。     

凸轮逆序测量方法

目前各杂志所发表的关于凸轮测量的文章，所讨论的均是凸轮的顺序测量方法，有关凸轮的逆序测量(反求工程)方法，尚未见于文字。本文将对凸轮的逆序测量方法进行探讨。     

红外导引头光学系统的像质验收技术

从满足使用要求出发论述了红外导引头光学系统成像质量的验收原理、性能参数和方法。指出了性能验收的影响因素并提出了相应的解决措施。     

高密度栅测应变

将高密度光栅应用于力学参量的测量中。通过测得试件变形前后正交光栅衍射点阵的偏移移量，可逐点得到试件因载荷作用而引起的面内应变、离面位移和刚体传动分量。     

算术平均序列的收敛性

下述命题是熟知的:假设 {x_n)_(n=1)~∞是一数列且x_n=a 则1/n x_=a,并且我们知道它的逆命题是不真的。本文给出两个定理和两个推论,定理1断言S_n=1/nx_i 收敛于 a 和 b 的某种组合,这里 a 是(x_n)的子列极限,b 亦如此。在定理2中我们给出1/nx_i=0的一个充要条件,两个推论也是有趣的。     

期望状态序列导向的深空探测器规划修复方法

Aiming at the challenges caused by the persistence, concurrency and energy consumption of probe actions, a plan repair method of deep space probe based on the expected state sequence is proposed. In this method, the expected state sequence is formed of the expected effect of the unfinished action and the expected precondition of the unexecuted action in the pre designed plan, according to the execution status of the action. The expected state sequence is an ordered set of states with mixed logic and energy, providing subgoals for plan repair and also transforming the plan repair problem into the state transition path searching problem. During the search, the plan repair strategy with energy supply priority is proposed, which separates the logic repair from energy repair to reduce the difficulty of solving the problem. And this method enables the probe to recover from plan failure autonomously. Finally, the effectiveness and rationality of the proposed method are verified through simulation by taking the Mars Orbiter as an example.     

Latitudinal distribution of solar coronal active regions

We studied the cyclic evolution of the latitudinal distribution of solar coronal active regions based on daily images from SOHO EIT for the period 1995–2017. Fully automated software was used, which included the following steps: initial preparation of images in the data series, normalization of histograms and correction of limb brightening, segmentation of images using threshold intensity values obtained from their histograms, scanning of segmented images in heliographic coordinates and obtaining profiles of latitudinal distribution of coronal active regions for each image of the data series. From the output data, we obtained a temporary change in the latitudinal distribution profiles and the migration of activity centers on the solar disk. From the period of minimum activity to the next minimum in both hemispheres, activity centers begin to migrate from high latitudes towards the equator. At the same time, the general center of activity repeatedly changes the direction of migration. The latitudinal distribution of the so-called presence factor of coronal active regions closely resembles the magnetic butterfly diagram, which proves their direct causal relationships. Variations in the presence factor of coronal active regions are correlated with cyclic variations in the sunspot daily numbers.