basicpulseradar

熵权计算程序,本程序主要用于熵权的计算，可以直接使用。(The entropy weight calculation procedures, the procedures used for the calculation of the entropy weight can be used directly.)

这是一段matlab程序，主要目的是为了完成matlab的潮流计算(This is a period of matlab procedures are in order to achieve the main purpose of the power flow calculation matlab)

高斯列主元消去法求解线性方程组的程序 数值分析(Gauss )

ＴＥ波和TM波照射到二维导体柱上带你电流分布，各个方向的RCS以及总的ＲＣＳ随导体尺寸的变化(TE wave and TM wave illumination column take you to the two-dimensional conductor current distribution, in all directions of the RCS and the RCS with the total change of conductor size)

把鲁棒预测控问题转化为线性矩阵不等式来求解(Solving the problem of robust predictive control into a linear matrix inequality)

关于图像处理中的区域能量是matlab算法，此算法简单易行(Regional energy for image processing matlab algorithm, this algorithm is simple)

已知观测数据为A+W(n)，其中A为直流信号，W为复高斯噪声，服从CN（0， ），在统计N次下，计算X的统计平均值 ，求T(x)= 的pdf：p(T(x)|H0)、p(T(x)|H1)。 H0： W H1： A+W (Known observation data A+W (n), where A is the DC signal, W is the complex Gaussian noise, subject CN (0,), N times in the statistics, the calculation of the statistical mean of X, find T (x) = a pdf : p (T (x) | H0), p (T (x) | H1). H0: W H1: A+W)

太阳黑子是人类长久以来感兴趣的问题。此处运用matlab代码对太阳黑子的记录的数据进行处理，希望能提供帮助( Using archival records,astronomers have applied Wolfer s rule to determine sunspot activity back to the year 1700. Today the sunspot index is measured by many astronomers and the worldwide distribution of the data is coordinated by the Solar Influences Data Center at the Royal Observatory of Belgium. The text file sunspot.dat in the matlab/demos directory has two columns of numbers. The first column is the years from 1700 to 1987 and the second column is the average Wolfer sunspot number for each year.)

学习盲源分离的独立分量分离，可以作为学习盲源分离的基本程序(Learning blind source separation independent component can be used as learning the basic procedures for blind source separation)

神经网络在matlab中的使用说明书 也是新手上手的好东西(Neuron Network Architectures)