“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。     

大学英语考试方式方法改革与实践

要培养具有英语实际应用能力的学生，提升教学质量，改革现有的大学英语评价制度势在必行。本文提出，大学英语无纸化考试、人机对话、构建完善的课程评价机制，教考分离等方式方法，应该在大学英语教学中得到进一步加强。     

The damping of small-amplitude oscillations in quiescent prominences

The presence of small-amplitude oscillations in prominences is well-known from long time ago. These oscillations, whose exciters are still unknown, seem to be of local nature and are interpreted in terms of magnetohydrodynamic (MHD) waves. During last years, observational evidence about the damping of these oscillations has grown and several mechanisms able to damp these oscillations have been the subject of intense theoretical modelling. Among them, the most efficient seem to be radiative cooling and ion-neutral collisions. Radiative cooling is able to damp slow MHD waves efficiently, while ion-neutral collisions, in partially ionised plasmas like those of solar prominences, can also damp fast MHD waves. In this paper, we plan to summarize our current knowledge about the time and spatial damping of small-amplitude oscillations in prominences.     

多元系统论视角下的中国文化与美国诗歌

自19世纪以来中国诗歌的英译对美国诗歌产生了重大影响,但美国本土诗歌和文化思想仍然处于强势的主导地位,美国人接受的是他们心目中的中国文化。美国诗歌对中国文化和中国诗歌的吸收,并不等于东西文化的交流与结合。通过研究中美文化和文学交流的媒介,结合多元系统论和比较文学相关理论来对该问题进行分析。     

Modeling Pulsar Wind Nebulae

In the last few years, new observations by CHANDRA and XMM have shown that Pulsar Wind Nebulae present complex but similar inner features, with the presence of axisymmetric rings and jets, which are generally referred to as a jet-torus structure. Due to the rapid growth in accuracy and robustness of numerical schemes for relativistic fluid-dynamics, it is now possible to model the flow and magnetic structure of the relativistic plasma responsible for the emission. Recent results have clarified how the jet and rings are formed, suggesting that the morphology is strongly related to the wind properties, so that, in principle, it is possible to infer the conditions in the unshocked wind from the nebular emission. I will review here the current status in the modeling of Pulsar Wind Nebulae, and, in particular, how numerical simulations have increased our understanding of the flow structure, observed emission, polarization and spectral properties. I will also point to possible future developments of the present models.     

Solar Isotopic Composition as Determined Using Solar Energetic Particles

Solar energetic particles (SEPs) provide a sample of the Sun from which solar composition may be determined. Using high-resolution measurements from the Solar Isotope Spectrometer (SIS) onboard NASA’s Advanced Composition Explorer (ACE) spacecraft, we have studied the isotopic composition of SEPs at energies ≥20 MeV/nucleon in large SEP events. We present SEP isotope measurements of C, O, Ne, Mg, Si, S, Ar, Ca, Fe, and Ni made in 49 large events from late 1997 to the present. The isotopic composition is highly variable from one SEP event to another due to variations in seed particle composition or due to mass fractionation that occurs during the acceleration and/or transport of these particles. We show that various isotopic and elemental enhancements are correlated with each other, discuss the empirical corrections used to account for the compositional variability, and obtain estimated solar isotopic abundances. We compare the solar values and their uncertainties inferred from SEPs with solar wind and other solar system abundances and find generally good agreement.     

企业英语培训现状分析与对策

通过对国内涉外企业英语培训的市场需求及所存在问题的调研与分析，提出相应的对策与措施；在分析高校的优势与劣势的基础上，就高校参与英语培训市场的竞争提出了相关策略。     

英语翻译教学与能力训练的探索

在英译汉训练中，加强英文单词的辨析和理解，提高英语的分析能力是表达原著内容的基础；只有了解英语文化背景，掌握常用的翻译技巧，才能提高汉语水平使译文达意通顺。     

Tilts and polarity separation in the sunspot groups and active regions at the ascending and descending phases of the cycle 23

The Solar Feature Catalogues for sunspots and active regions measured with SOHO/MDI instrument and Ca II K3 spectroheliograph of the Paris-Meudon Observatory are analyzed with the automated classification technique for sunspot groups and active region polarities. We report the first classification results for daily variations of tilt angles (normal and trigonometric ones) in sunspot groups (SG) and active (AR) regions in the cycle 23. The average normal tilts are presented for every year at the ascending and descending phases of the cycle 23 which are similar to those deduced by other authors for the cycles 19–22. The normal tilts of both the sunspot groups and active regions are shown to increase in the ascending phase and a decrease in the descending phase. Similar to SG and AR areas, the trigonometric tilts are shown to have the noticeable North–South asymmetry with the Southern hemisphere dominant in the selected ascending and descending periods. The normal tilt variations with latitude follow Joy’s law revealing a periodicity along the meridian of about 10° and reaching the maximum of 14° at the latitude of about 32° corresponding to the top of the ‘royal zone’ where the sunspots appear. The variations of polarity separation with a latitude are in an anti-phase with those of the tilts reaching a maximum at the latitude of 35° and showing a small positive separation for the groups/active regions in a vicinity of the average tilts ±40°. The ratio R of the polarity separation to the trigonometric tilt fits the linear function of a latitude φ as R = −0.0213φ − 0.1245 confirming positive separation for the polarities of active regions with the average tilts, or the dominance of activity in the Southern hemisphere activity, for the selected period of observations.     

高职高专英语教学中的听力理解策略

在大学英语教学中,听力教学已成为相当重要的一部分,听力理解作为基本语言技能愈来愈受到重视,但是,我国的大学对听力教学从理论到实践都相对滞后,因此,通过以高职高专公共英语专业的学生为研究对象,分析了学生听力理解环节相对薄弱的因素,并针对听力教学存在的问题提出相应的教学策略,目的是使学生由消极被动地获取信息,转变为积极主动地对信息进行分析、解码,提高听力.