论儒家文化与现代企业文化

在经济全球化发展的今天,企业要保持持续发展的良好势头,离不开文化力量的支撑.而要建设好现代企业文化,需要对我国传统文化进行客观地、实事求是地分析、继承和发扬.儒家文化是中国传统文化的主流,对整个中华民族的民族心理和民族性格的影响是巨大的.文章分析了儒家文化和企业文化的内涵和特征,论述了儒家文化所提倡的以人为本、以和为贵、义利并重等内容对现代企业文化建设的积极作用.     

从物竞天择到族群和谐共处——马丁·雅克《当中国统治世界》一书探究

雅克在<当中国统治世界>一书中认为,中国将成为文化霸权,但是文化霸权并不是霸权文化.文化霸权应该是在认真反思和积极汲取"物竞天择"的西方工业文明价值观基础上,是以中国为典范的族群和谐共处的东方文化伟大的复兴.文化霸权不是"物竞天择"理念下另外一种形式的霸权主义和强权政治,而是要求在国际关系中遵循求同存异、合作共赢、相互尊重、和谐共生的价值观.     

北京奥运会中国传统文化元素解析

北京奥运会展现的许多具有代表性的中国传统文化元素，既是奥运会文化交流、彰显特色的成功保证，也让世人了解了悠久的华夏文明。后奥运时期，进一步挖掘这些传统文化元素符号背后的历史蕴涵及其在奥运会当中的文化寓意，有利于弘扬和保护中华民族的传统文化，更好地发展奥林匹克精神。     

论跨文化比较法在中国政治文化研究中的应用

当前,中国正处于社会转型的历史时期,社会正发生着深刻的变化。与此同时,中国的政治文化也发生着相应的变革。政治文化对一个国家或民族的政治现代化起着巨大的制约作用,每一个走向现代化的发展中国家都面临着发达国家政治文化的冲击和挑战。通过探讨跨文化比较研究方法在中国政治文化研究中的应用,把本国的政治文化与发达国家的政治文化进行比较,为我国政治文化建设提供一个参照系,以期进一步推动国内政治文化研究的深入发展。     

《红楼梦》中“杏花村”的跨文化翻译

对于中国古典文学作品《红楼梦》,目前有两个不同的英文全译本,本文试图就两个译本中的"杏花村"的两个不同译文为例进行分析和探究,力图客观地评析两个不同的译文本,以期在目前中国古典文学大量对外译介方面,探讨如何有效地解决古典文学作品中独特文化因子的跨文化传递。     

民航院校要自觉担负起行业文化传承创新的历史使命

胡锦涛总书记在庆祝清华大学建校100周年大会上的重要讲话中,鲜明地将文化传承创新与人才培养、科学研究、社会服务一起列为高校的四大重要职能,并突出强调:"高等教育是优秀文化传承的重要载体和思想文化创新的重要源泉。"党的十七届六中全会通过的《中共中央关于深化文化体制改革、推动社会主义文化大发展大繁荣若     

中西方文化差异在旅游主体上的反映

中西方文化差异对旅游主体——旅游者和旅游活动有着很大的影响，通过分析中西文化的差异性提出了旅游目的地的建设与发展的一些对策和建议。     

提高国家文化软实力的国际比较与借鉴

随着中国融入国际社会的不断深化,如何提升中国的国际形象和国家文化软实力具有越来越重要的意义.从国际经验来看,国家文化软实力的提高是一个长期的历史过程.尽管我国是一个有影响的文化大国,但与国外相比,我国文化软实力的建构还存在着缺乏学科支撑、文化建设不够,对外传播力不足等问题.应采取切实措施在构建主流文化、发展文化产业、提高对外传播力、开展海外汉语推广等方面着力提高我国的文化软实力,展现我国的国际形象和魅力.     

质量文化研究(上)——概念及结构化分析

定义了质量文化概念的涵义 ,并将其与企业文化和企业质量文化的涵义进行了比较和分析 ,以澄清人们在质量文化概念认识上的一些误区。分析并探讨了质量文化的结构特征、质量文化强度的评价方法以及质量文化的演变过程 ;说明了应用质量文化强度的评价方法可有效地考虑某一国家或地区经济的质量文化对该国家或地区经济的贡献 ,及质量文化将随着时间和客观条件的变化而不断地发生变革。     

文化创意人才培养的新模式

文化创意产业作为新兴产业形式,其发展需要大量的创意型人才。及时地分析和认清目前我国文化创意人才现状和存在问题,提出创意人才培养新模式已成为当务之急。基于此,在分析目前我国创意人才现状和存在问题的基础上,有针对性地从四个方面提出了创意人才培养的新模式。     

Radio emission from coronal streamers

Different models of coronal streamers are used to calculate the radio brightness temperature at the wavelengths of observation of the Nançays Radioheliograph. Calculation are performed assuming the location of the streamer both on the disk and at the limb. Their comparison with observations show that a satisfactory agreement with a particular model can be found in the shape and in the relative enhacement of the streamer with respect to the quiet Sun, although the absolute values of the computed brightness temperatures are much higher than the observed ones.     

孙中山晚年复归儒学原因初探

孙中山晚年复归儒学，根源于其坚定的民族立场，对西方“文明”的反省，以及建设革命党和从事政党政治的需要。     

怎样看待孙中山对马克思阶级斗争理论的批评

阶级斗争理论是马克思主义理论的重要组成部分,但这一理论遭到了孙中山的批评。孙中山的批评有错误之处,但谬误中包含着真理。阶级斗争并非历史发展的唯一动力,社会改革也是社会进步的重要途径。     

Solar mass flow in fine-scale structures

Observations of transient and steady velocities at chromospheric, transition region and coronal temperatures in the quiet Sun and coronal holes are reviewed. The relevance of fine-scale structures in governing the mass balance of the solar atmosphere is stressed. At present, a coherent picture of these mass flows does not exist. However, the current observational base of transition region and coronal velocity information is limited but should greatly improve with measurements from the SOHO satellite.     

Comparing Quiet Sun and Coronal Hole Regions with CDS/SOHO

Spectra from the Coronal Diagnostic Spectrometer on board SOHO are used to compare density and temperature in coronal hole and quiet Sun regions. This revised version was published online in June 2006 with corrections to the Cover Date.     

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.     

The Solar Quiet Chromosphere—Corona Transition Region

The chromosphere-corona transition region of the Sun enjoys both simplicities of character and complexities of character which result from its very thin geometrical extent. The simplicities derive from the reasonably clear view of the energy balance (both observationally and theoretically), while the complexities derive from both the proximity of the not-so-clearly viewed regions below and above, and the almost certain convolutions and perhaps discontinuities in the three dimensional geometry of the transition sheet. While observational resolution and spectral information has improved greatly in recent years, the problems associated with a single vantage point, the Earth and its environs, have not gone away. To understand the transition region we must resolve structures radially and temporally as well as in the plane of the sky. This revised version was published online in June 2006 with corrections to the Cover Date.     

孙中山与邓小平的社会主义本质论的相通性

孙中山的社会主义思想和邓小平的社会主义本质论,在发展生产力、变革生产关系和实现共同富裕等方面存在着相同性或相通性。这些相通性启迪我们必须坚持走社会主义道路,坚持马克思主义基本原理和中国的具体国情相结合,在实践中不断丰富和发展马克思主义。     

Spectroscopic Measurement of Coronal Compositions

Although the elemental composition in all parts of the solar photosphere appears to be the same this is clearly not the case with the solar upper atmosphere (SUA). Spectroscopic studies show that in the corona elemental composition along solar equatorial regions is usually different from polar regions; composition in quiet Sun regions is often different from coronal hole and active region compositions and the transition region composition is frequently different from the coronal composition along the same line of sight. In the following two issues are discussed. The first involves abundance ratios between the high-FIP O and Ne and the low-FIP Mg and Fe that are important for meaningful comparisons between photospheric and SUA compositions and the second involves a review of composition and time variability of SUA plasmas at heights of 1.0≤h≤1.5R _⊙.     

Standard Solar Composition

We review the current status of our knowledge of the chemical composition of the Sun, essentially derived from the analysis of the solar photospheric spectrum. The comparison of solar and meteoritic abundances confirms that there is a very good agreement between the two sets of abundances. They are used to construct a Standard Abundance Distribution. This revised version was published online in June 2006 with corrections to the Cover Date.