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341.
Hongwen Zheng Yanxia Zhang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(12):1960-1964
With an exponentially increasing amount of astronomical data, the complexity and dimension of astronomical data are likewise growing rapidly. Extracting information from such data becomes a critical and challenging problem. For example, some algorithms can only be employed in the low-dimensional spaces, so feature selection and feature extraction become important topics. Here we describe the difference between feature selection and feature extraction methods, and introduce the taxonomy of feature selection methods as well as the characteristics of each method. We present a case study comparing the performance and computational cost of different feature selection methods. For the filter method, ReliefF and fisher filter are adopted; for the wrapper method, improved CHAID, linear discriminant analysis (LDA), Naive Bayes (NB) and C4.5 are taken as learners. Applied on the sample, the result indicates that from the viewpoints of computational cost the filter method is superior to the wrapper method. Moreover, different learning algorithms combined with appropriate feature selection methods may arrive at better performance. 相似文献
342.
In this paper we review the current predictions of numerical simulations for the origin and observability of the warm hot
intergalactic medium (WHIM), the diffuse gas that contains up to 50 per cent of the baryons at z∼0. During structure formation, gravitational accretion shocks emerging from collapsing regions gradually heat the intergalactic
medium (IGM) to temperatures in the range T∼105–107 K. The WHIM is predicted to radiate most of its energy in the ultraviolet (UV) and X-ray bands and to contribute a significant
fraction of the soft X-ray background emission. While O vi and C iv absorption systems arising in the cooler fraction of the WHIM with T∼105–105.5 K are seen in FUSE and Hubble Space Telescope observations, models agree that current X-ray telescopes such as Chandra and XMM-Newton do not have enough sensitivity to detect the hotter WHIM. However, future missions such as Constellation-X and XEUS might be able to detect both emission lines and absorption systems from highly ionised atoms such as O vii, O viii and Fe xvii. 相似文献
343.
J. S. Kaastra F. B. S. Paerels F. Durret S. Schindler P. Richter 《Space Science Reviews》2008,134(1-4):155-190
We discuss the different physical processes that are important to understand the thermal X-ray emission and absorption spectra
of the diffuse gas in clusters of galaxies and the warm-hot intergalactic medium. The ionisation balance, line and continuum
emission and absorption properties are reviewed and several practical examples are given that illustrate the most important
diagnostic features in the X-ray spectra. 相似文献
344.
345.
李伟梁 《郑州航空工业管理学院学报(管理科学版)》2008,26(3):86-90
在社区各类资源中,物质资源最为重要,它是社区建设的物质基础和前提保障。社区物质资源的短缺极大地制约了社区建设和发展。因此,在建设和谐社区过程中,必须不断加强社区物质资源的整合。社区物质资源整合机制的构建主要包括社区资金的多元筹集机制和驻社区单位的资源共享机制。 相似文献
346.
C. Bouratzis P. Preka-Papadema X. Moussas C. Alissandrakis A. Hillaris 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
A complex radio event was observed on January 17, 2005 with the radio-spectrograph ARTEMIS-IV, operating at Thermopylae, Greece; it was associated with an X3.8 SXR flare and two fast Halo CMEs in close succession. We present dynamic spectra of this event; the high time resolution (1/100 s) of the data in the 450–270 MHz range, makes possible the detection and analysis of the fine structure which this major radio event exhibits. The fine structure was found to match, almost, the comprehensive Ondrejov Catalogue which it refers to the spectral range 0.8–2 GHz, yet seems to produce similar fine structure with the metric range. 相似文献
347.
“六性”、“七化”与“一品”——全国高职高专学报走向再探索 总被引:3,自引:0,他引:3
潘世东 《西安航空技术高等专科学校学报》2008,26(6):70-73
通过分析高职高专学报生存发展的现状和面临的主要问题,提出了高职高专学报的宗旨定位、作者定位、读者定位和特色定位;结合学报学会组织的功能和使命及高职高专学报的发展方向,归结出了“六性”、“七化”与“一品”的奋斗目标。 相似文献
348.
349.
新出现的RISC微处理器提供了超计算能力,采用i860XP超标量微处理器来增强已存在的Transputer系统的性能是一种切实可行的办法,它们构造了一种异构型多处理器系统。本文给出了该系统的设计和性能分析。 相似文献
350.