统计学习与知识发现

知识发现是将知识从隐性转化为显性的一个过程,它是知识管理的重要组成部分.为此阐述了利用统计学习的知识发现方法,以及统计学习中主要使用的分类学习,并强调了使用数据驱动指导知识构建的合理性和优越性,最后结合实例分析了几个主要的统计学习方法及其应用.     

基于小波的能源消费弹性系数预测方法

能源消费弹性系数反映了一个国家能源消费增长速度与国民经济增长速度之间的比例关系,是衡量一个国家能源利用效率的重要指标。鉴于数据中存在较多的噪声,首先用小波分析方法对数据进行滤波,然后用滤除了噪声的数据作为输入变量,用支持向量回归方法建模,并预测未来10年我国能源消费弹性系数变化的规律。实际数据检验表明,该预测方法还是可行的。     

毛细管内部核化过程分析

针对微细结构内部的核化沸腾特性进行理论和实验研究,利用统计理论分析并且导出受热工质内部沸腾发生所需的过热度,揭示出毛细管道内部空间尺度对核化的影响。实验中,对四种工质(去离子水、甲醇、乙醇、四氯化碳)在毛细管内部的沸腾现象进行了观察和测量,结果表明理论分析与实验观测结果吻合得较好。      

Internal fuselage noise: comparison of computations and tests on a Falcon airframe

An unequipped Falcon 2000 airframe, a complex heterogeneous structure reduced to the fuselage alone, was subjected to vibro-acoustic characterization within the framework of a cooperative effort by Aerospatiale, Dassault-Aviation, and Onera. Onera's Structural Dynamics and Coupled Systems Department measured the structure's vibro-acoustic responses for four mechanical excitation configurations, and analysed three structural configurations: fuselage alone without floor, with floor, and with floor and internal wall. The resulting database of vibratory and acoustic level measurements is used for validating numerical models in the low- and medium-frequency range, as well as statistical energy analysis (SEA) models in the medium- and high-frequency range.The database was analysed by Dassault-Aviation and Onera. We present here the computation/test comparisons and the limitations of the methods in use. All of the data and comparisons validate the predictive vibro-acoustic response models and methods for a Falcon fuselage subjected to a mechanical excitation.     

航空机电系统技术发展综述

文中总结了国际航空机电系统技术研究现状,以美国为代表的国际先进飞机研发体系,将机电系统技术提升至与飞机平台技术并重的地位,将综合推进、能源与热管理技术列为核心技术领域,持续开展了MEA、INVENT、INPPAT、AVEM、NGT-PAC等一系列面向机电领域的重大技术专项和演示验证计划;梳理了系统架构综合化、能源利用多电化、能量管理高效化的机电系统技术发展趋势;展开了机电系统技术研发思考,提出了强化机电系统技术发展规律和需求认识、升级机电系统技术基础研究,和仿真验证能力是引领机电系统技术发展的2个关键方向。     

基于误差模型的权重二值神经网络近似加速

针对智能识别系统精确度和硬件复杂度之间的均衡设计问题,提出了一种基于误差统计模型的权重二值神经网络近似加速方法.在提出了一种获得高精度轻量神经网络的权重二值化处理算法基础上,引入近似加法器、消除乘法器以进一步提高能效.最终提出了一种系统级误差统计模型用于系统评估和优化设计,该设计能够分析和预测权重二值神经网络近似加速系...     

Observations of the local interstellar medium with the Extreme Ultraviolet Explorer

Because of the strong absorption of extreme ultraviolet radiation by hydrogen and helium, almost every observation with the Extreme Ultraviolet Explorer (EUVE) satellite is affected by the diffuse clouds of neutral gas in the local interstellar medium (LISM). This paper reviews some of the highlights of the EUVE results on the distribution and physical state of the LISM and the implications of these results with respect to the interface of the LISM and the heliosphere. The distribution of sources found with the EUVE all-sky surveys shows an enhancement in absorption toward the galactic center. Individual spectra toward nearby continuum sources provide evidence of a greater ionization of helium than hydrogen in the Local Cloud with an mean ratio of H I/He I of 14.7. The spectral distribution of the EUV stellar radiation field has been measured, which provides a lower limit to local H II and He II densities, but this radiation field alone cannot explain the local helium ionization. A combination of EUVE measurements of H I, He I, and He II columns plus the measurement of the local He I density with interplanetary probes can place constraints on the local values of the H I density outside the heliosphere to lie between 0.15 and 0.34 cm^–3 while the H II density ranges between 0.0 and 0.14 cm^–3. The thermal pressure (P/k = nT) of the Local Cloud is derived to be between 1700 and 2300 cm^–3 K, a factor of 2 to 3 above previous estimates.     

应用微机校定三相变压器的联结组及标号

三相变压的联结组标号对其正常运行极为重要，必须校定，而目前变还缺少全面快捷的校定方法和设备。本文介绍采用微机系统来实现联结组桔的校定，首先把四类联结组差别区分开，然后分析指出同一类联结组中，除有六种正序标号外，存在六种逆序标号，提出用新的筛选法能简捷地判别校定同一类的十二种标号，当微机系统进行实际测试时，必须考虑电源电压三相不对称程序的影响，故经数学推导得出用实测计算值代替理想计算值作判别比较的基     

The Cool Interstellar Medium

Infrared spectroscopy and photometry with ISO covering most of the emission range of the interstellar medium has led to important progress in the understanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains. We review here the ISO results on the cool and low-excitation regions of the interstellar medium, where T _gas≲ 500 K, n _H∼ 100–10⁵ cm⁻³ and the electron density is a few 10⁻⁴. JEL codes: D24, L60, 047 Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Working group 3: Coronal streamers

The working group on coronal streamers convened on the first day of the 2nd SOHO Workshop, which took place in Marciana Marina, Isola d'Elba, 27 September –1 October 1993. Recent progress in streamer observational techniques and theoretical modeling was reported. The contribution of streamers to the mass and energy supply for the solar wind was discussed. Moreover, the importance of thin electric current sheets for determining both the gross dynamical properties of streamers and the fine-scale filamentary structure within streamers, was strongly emphasized. Potential advances to our understanding of these areas of coronal physics that could be made by the contingent of instruments aboard SOHO were pointed out.