我国农村义务教育财政专项投资若干问题探析

2006年开始的农村义务教育经费保障机制改革已经在全国全面铺开,自此,我国农村义务教育财政性经费第一次真正地被纳入公共财政的框架。而在这次改革中,财政专项投资发挥了非同寻常的作用,成为财政投入的主体形式。从义务教育财政专项投资的概念、现状和特点出发,解析农村义务教育经费保障机制改革条件下财政专项投资的资金安排、运营、支付和监管等若干问题,并对专项投资的功效和创新做出理论性的初探。     

应用ART1神经网络仿真车间分组

阐述了ART1神经网络在制造单元设计过程中形成零件族的基本方法,并在基于MATLAB的软件平台上,利用其神经网络工具箱对生产过程中的实际情况进行了仿真和应用。     

城市化发展的阶段性及其规律研究

文章提出了城市化发展一般经历初级、中级和高级三个阶段，并提出了城市化发展的一般规律；农业发展是城市化的初始动力，资本扩张是城市化的原动力，市场机制是加速城市化进程的基础性机制，大城市超前增长，城市经济要与农村经济协调发展，乡村人口进入城市门坎的高低直接影响着城市化的速度和水平。     

Expectations for Infrared Spectroscopy of 9P/Tempel 1 from Deep Impact

The science payload on the Deep Impact mission includes a 1.05–4.8 μm infrared spectrometer with a spectral resolution ranging from R∼200–900. The Deep Impact IR spectrometer was designed to optimize, within engineering and cost constraints, observations of the dust, gas, and nucleus of 9P/Tempel 1. The wavelength range includes absorption and emission features from ices, silicates, organics, and many gases that are known to be, or anticipated to be, present on comets. The expected data will provide measurements at previously unseen spatial resolution before, during, and after our cratering experiment at the comet 9P/Tempel 1. This article explores the unique aspects of the Deep Impact IR spectrometer experiment, presents a range of expectations for spectral data of 9P/Tempel 1, and summarizes the specific science objectives at each phase of the mission.     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

接触焊机理的探索

探讨了接触焊的机理，提出了以电位差选择电极材料的原则，以及焊接处的接触电阻和母材内阻在焊接中有一定作用，而且焊接处的总热能是各种能量产生的热量之和，焊接的总热量也应包括通电加热产生的热量和断电后（锻压时）产生的热量。     

先进的变载吸能器

传统的定载吸能器以50百分位男性乘员满足95％生存率为条件设计，它不能为全体乘员提供保护，变载吸能器能够根据乘员重量而调节动作载荷，为全体乘员提供最合理的保护，同时可以大大降低吸能器的冲击行程。     

一种无条件稳定的时域推进法与有限元混合分析瞬态热传导问题

本文将一种新的无条件稳定的时域推进法与有限元结合,用于分析瞬态热传导问题。根据微-积分型热传导控制方程,对时间变量在小区闻内插值积分,变初-边值问题为一系列离散时刻的边界值问题,再应用有限元法求解之。由于推进中的每一时刻的解,都严格满足原给定的初始条件,就消除了累积误差的影响。此外,这种时域推进法对时间变量的数值积分也优于数值微分。因而,与现行的基于微分型控制方程,采用时-空有限元模型同时离散,再逐步求解的直接积分算法相比,计算精度可大大提高。不难预料,当求解较长时间后的瞬态值时,本算法的优越性会更加明显。     

构建现代企业制度下的激励机制

国有企业改革的关键是要构建现代企业制度,而激励机制的陈旧落后将严重制约现代企业活力的发挥。本文结合我国过去计划经济体制下国有企业存在的激励问题,探讨了新时期构建现代企业制度下的激励机制的思路。     

CAPP中加工方法选择研究

研究在ＣＡＰＰ系统中，通过建立加工方法的知识库以及相关的推理机构，来实现对机械零件各表面的加工方法选择。