“读者接受”理论与《高级英语》教学自主学习模式研究

借鉴"读者接受"理论中以"读者为中心"的观点,研究《高级英语》课程教学的自主学习模式。本文认为,学生是审美活动的主体,在该教学模式中研究学生的元认知特点、教材、教学任务的设计和有效控制等因素,注重教学过程的研究,在实践中有效实现以学生为中心、培养学生综合素质的教学理念。     

试析马克思理论体系的两个思想资源

除了常说的三大理论来源以外,马克思的理论体系的形成还有很多丰富的思想资源,其中,基督教和<圣经>传统、古希腊神话和西方文学作品对马克思科学世界观、人生观、价值观的形成产生了深刻影响,马克思对他们采取了批判的借鉴的态度,从中汲取了丰富的营养,成为马克思理论体系重要的思想资源.     

高超声速非平衡流场多个振动温度模型的数值研究

利用数值求解热化学非平衡Navier-Stokes方程的方法,建立了考虑一个和多个振动温度的高超声速热化学非平衡流场的CFD计算程序,并对半球模型和球锥模型进行了数值计算,研究结果表明:(1)各个分子组分的振动温度分布于考虑一个振动温度模型的振动温度周围,即一个振动温度模型的振动温度是多个振动温度模型的各个分子组分振动温度的一种平均值;(2)在模型身部,振动温度的峰值高于平动温度的峰值;在模型近尾出现振动温度冻结并高于平动温度。     

Study of the 27-day variations of the galactic cosmic ray intensity and anisotropy

We demonstrate that the general features of the radial and azimuthal components of the anisotropy of galactic cosmic rays can be studied by the harmonic analysis method using data from an individual neutron monitor with cut off rigidity <5 GV. In particular, we study the characteristics of the 27-day (solar rotation period) variations of the galactic cosmic ray intensity and anisotropy, solar wind velocity, interplanetary magnetic field strength and sunspot number. The amplitudes of the 27-day variations of the galactic cosmic ray anisotropy are greater, and the phases more clearly established, in A > 0 polarity periods than in A < 0 polarity periods at times of minimum solar activity. The phases of the 27-day variations of the galactic cosmic rays intensity and anisotropy are opposite with respect to the similar changes of the solar wind velocity in A > 0 polarity periods. No significant dependence of the amplitude of the 27-day variation of the galactic cosmic ray anisotropy on the tilt angle of the heliospheric neutral sheet is found. Daily epicyclegrams obtained by Chree’s method show that the 27-day variations of the galactic cosmic ray anisotropy during A > 0 polarity periods follow elliptical paths with the major axes oriented approximately along the interplanetary magnetic field. The paths are more irregular during A < 0 polarity periods.     

Asteroid and comet hazard: Identification problem of observed space objects with the parental bodies

This article focuses on the genetic identification of observed small cosmic bodies with alleged parental bodies; namely, comets, asteroids and meteoroid swarms. There is a problem of the upper D-value limit as a measure of proximity between the orbits of the bodies in the five-dimensional phase space (Southworth and Hawkins, 1963). In the study of genetic relationships of the comet and meteor complexes, the D value is usually taken as equal to 0.2 for all meteor showers. However, the upper D limit should be investigated for each meteoroid complex. For example, such investigation was performed for the Taurid meteor complex (Porub?an et al., 2006). In this paper, the upper D-criterion limit value was investigated for the Perseid meteor shower. The 1862 III Swift–Tuttle comet is its parental comet.     

一种基于数字采样技术的电压波动测量系统CSCD

本文针对电能质量计量校准领域中电压波动参数的测量问题进行研究,通过比较现有电压波动信号的检测方法,结合数学模型分析,提出一种基于Agilent 3458A采样器的电压波动信号交流采样均方根值检测法。并搭建电压波动信号测量系统,通过实验,实现了测量电压波动频率范围可覆盖0.008Hz^40Hz,波动值范围为0.1%~30%。     

第21,22周峰年太阳射电爆发中毫秒级精细结构的分析

本文对第21周的2840MHz及22周峰年的2545MHz，2645MHz和2840MHz波段上所观测到的285个快速事件进行分析，发现两个峰年的快速事件具有多种多样的快速活动（快速精细结构）．它们与耀斑的对应关系也做了统计分析．     

洗流时差阻尼力矩研究

在分析飞机的纵向阻尼力矩时，除考虑俯仰角速度引起的俯仰阻尼力矩外，还应估算出迎角变化率引起的洗流时差阻尼力矩。根据洗流时差阻尼力矩产生的原理，推导并给出了它的计算方法。介绍了各种阻尼导数的表示方法及相互关系。最后较详细地分析了水平尾翼、马赫数、迎角变化率和下洗角随迎角的变化率诸因素对洗流时差阻尼力矩及阻尼导数的影响。     

应力腐蚀可靠性分析

本文阐明了应力腐蚀的基本概念，提出及阐明了应力腐蚀可靠性基本概念及其算法，做了应力腐蚀可靠性算例说明，并给出了应力腐蚀控制方法。     

钛硅共晶合金中硅化物及其对显微硬度的影响

观察了钛硅共晶系合金的微观组织。综合分析了X射线能谱（X－EDS）、透射电子显微镜（TEM）以及X射线衍射（XRD）结果，确认了铸态组织中析出的硅化物本质，并测得该硅化物的显微维氏硬度。结果表明，钛硅共晶合金铸态组织由α-Ti和Ti5Si3两相组成。亚共晶钛硅合金中共晶区比枝晶区具有更高的显微硬度，而共晶和过共晶合金的共晶区显微硬度明显高于亚共晶合金。