Neural networks and the separation of cosmic microwave background and astrophysical signals in sky maps

We implement an independent component analysis (ICA) algorithm to separate signals of different origin in sky maps at several frequencies. Owing to its self-organizing capability, it works without prior assumptions on either the frequency dependence or the angular power spectrum of the various signals; rather, it learns directly from the input data how to identify the statistically independent components, on the assumption that all but, at most, one of the components have non-Gaussian distributions.
We have applied the ICA algorithm to simulated patches of the sky at the four frequencies (30, 44, 70 and 100 GHz) used by the Low Frequency Instrument of the European Space Agency's Planck satellite. Simulations include the cosmic microwave background (CMB), the synchrotron and thermal dust emissions, and extragalactic radio sources. The effects of the angular response functions of the detectors and of instrumental noise have been ignored in this first exploratory study. The ICA algorithm reconstructs the spatial distribution of each component with rms errors of about 1 per cent for the CMB, and 10 per cent for the much weaker Galactic components. Radio sources are almost completely recovered down to a flux limit corresponding to ≃0.7 σ _CMB, where σ _CMB is the rms level of the CMB fluctuations. The signal recovered has equal quality on all scales larger than the pixel size. In addition, we show that for the strongest components (CMB and radio sources) the frequency scaling is recovered with per cent precision. Thus, algorithms of the type presented here appear to be very promising tools for component separation. On the other hand, we have been dealing here with a highly idealized situation. Work to include instrumental noise, the effect of different resolving powers at different frequencies and a more complete and realistic characterization of astrophysical foregrounds is in progress.     

TIFF图象文件格式分析及其TVGA显示

本文介绍了ＴＩＦＦ图象文件的文件结构和从ＴＩＦＦ格式文件复原图象的方法，以及该图象在ＴＶＣＡ上的各种调色板的设置及显示。     

E3D,the Euro3D visualization tool I: Description of the program and its capabilities

We present the first version of E3D, the Euro3D visualization tool for data from integral field spectroscopy. We describe its major characteristics, based on the proposed requirements, the current state of the project, and some planned future upgrades. We show examples of its use and capabilities. (© 2004 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

金相分析中消除划痕的两种方法

介绍了两种在金相分析中采用模式识别技术,以距离聚类和角度类消除划痕的方法,使主体更加突出,分类评级更加准确,也降低了对试样的磨制要求。     

陡倾斜脉状矿体隐伏深度计算

在研究广西 10 0个矿区地质资料基础上 ,建立了陡倾斜脉状矿体隐伏深度计算经验公式 ,从而为隐伏矿床预测、减少矿床勘查风险提供了信息     

用数学形态学变换实现空间分析中的数据处理

论述了数学形态学的基本算法, 并将这一方法引入空间分析的数据处理中。研究表明,该方法具有一定的可行性, 对于空间分析中一些问题的深入研究具有参考价值     

圆透视曲线类型及相对视点画面的位置的分析

圆曲线的透视根据圆曲线相对视点、画面的位置不同,可以有五种结果,分别为直线、圆、椭圆、双曲线、抛物线     

基于时域导频跟踪和频域插值的正交频分复用系统信道估计方法

针对下一代无线通信长期演进系统,提出了一种基于时域导频跟踪和频域迭代离散傅里叶变换插值的改进信道估计方法,首先利用导频符号进行信道估计,然后通过导频跟踪和迭代离散傅里叶变换插值获得时域和频域非导频位置的信道估计值。仿真结果表明,基于时域导频跟踪和频域迭代离散傅里叶变换插值的估计方法比传统的方法改善约2dB误比特率性能。     

Analysis on accuracy of Engineering Star RTK in cadastral survey based on SOUTH-CORS

Currently,with the fast development of GPS technique,GPS RTK is rapidly being applied to the cadastral survey.GPS RTK technique not only improves efficiency and accelerates the rate of mapping,but also increases economic efficiency.The authors introduced a method for GPS RTK rapid positioning,which uses continuous operational reference system (CORS) as a base station to change the method of previous map drawing by obtaining real-time three-dimensional coordinates of boundary points and statistically analyzing with the three-dimensional coordinates obtained by Total Station to get the accuracy of GPS RTK real-time coordinates.The application of GPS RTK in practical measurement was discussed when the data link had been lost especially.The results show that the three-dimensional coordinates measured by total station can be replaced by real-time three-dimensional coordinates measured by Engineering Star RTK in the CORS.     

基于中分辨率成像光谱仪数据的洋面云检测新方法的研究

提出了一种利用中分辨率成像光谱仪热红外窗区通道数据进行云、晴空分离的新方法。该云检测算法从热红外窗区通道亮温出发,并结合水汽廓线,运用水汽规度法计算规度因子的值,利用规度因子的数值状态实现分离云和晴空,从而达到云检测的目的。经过大量的实验,并将结果与中分辨率成像光谱仪官方云检测产品作对比分析,结果表明准确率为91％,算法具有可行性。