Evolution of the Protosolar Nebula and Formation of the Giant Planets

The formation of planetary systems is intimately tied to the question of the evolution of the gas and solid material in the early nebula. Current models of evolution of circumstellar disks are reviewed here with emphasis on the so-called “alpha models” in which angular momentum is transported outward by turbulent viscosity, parameterized by an dimensionless parameter α. A simple 1D model of protoplanetary disks that includes gas and embedded particles is used to introduce key questions on planetesimal formation. This model includes the aerodynamic properties of solid ice and rock grains to calculate their migration and growth. We show that the evolution of the nebula and migration and growth of its solids proceed on timescales that are generally not much longer than the timescale necessary to fully form the star-disk system from the molecular cloud. Contrary to a widely used approach, planet formation therefore can neither be studied in a static nebula nor in a nebula evolving from an arbitrary initial condition. We propose a simple approach to both account for sedimentation from the molecular cloud onto the disk, disk evolution and migration of solids. Giant planets have key roles in the history of the forming Solar System: they formed relatively early, when a significant amount of hydrogen and helium were still present in the nebula, and have a mass that is a sizable fraction of the disk mass at any given time. Their composition is also of interest because when compared to the solar composition, their enrichment in elements other than hydrogen and helium is a witness of sorting processes that occured in the protosolar nebula. We review likely scenarios capable of explaining both the presence of central dense cores in Jupiter, Saturn, Uranus and Neptune and their global composition. This revised version was published online in August 2006 with corrections to the Cover Date.     

应对学生能力差异不同策略的利弊分析

为解决高职高专院校英语课学生能力差异问题，在分析国内外教学中应对学生能力差异主要策略利弊的基础上，提出了混合班制是能够适应高职高专院校英语课学生能力差异的有效策略。     

高职教育技能竞赛与课程群建设互动机制研究

高职教育技能竞赛和课程群建设间普遍存在着相互独立运行、沟通渠道不畅、缺乏促进机制等问题.针对上述问题,提出了在技能竞赛与课程群建设间建立良性互动机制的构想,设计了互动机制的循环反馈调节模型,分析了互动要素的驱动关系,给出了互动机制在课程群建设中的实现思路和操作方法.     

网上考试系统的设计与实现

本文讨论了一种新的考试方法———网上考试 ,并讨论了一种基于B/S系统实现网上考试的思路和设计方法 ,并对实现网上考试系统的部分关键技术进行了分析     

基于ARMA模型在线辨识器的线性系统建模方法

线性系统的在线辨识是系统辨识领域中最感兴趣的问题之一。本文给出变阶式递推增广的最小二乘法及阶估计准则。在此基础上 ,给出一类ARMA模型在线辨识器。这种辨识器可用于在线或离线辨识。实例表明 ,建模计算量大大减小 ,并具有较高的精度     

高职院校开展野外生存生活训练的可行性

通过对我国大学生野外生存生活训练开展的现状与发展趋势分析，探讨在高职院校开展野外生存生活训练的可行性。开展野外生存生活训练可以完善体育课程体系，拓展体育课程内容，使学生掌握有关野外生存的基本知识和基本能力，促进高职学生身心健康和谐发展。     

以多元智力理论审视民办高校学生评价体系

民办高校如何构建合理的学生多元评价体系？依据多元智力理论，阐述了民办高校的学生管理者应形成积极乐观的“学生观”，突出学生评价体系的发展功能；树立新的“教育观”，突出学生评价体系的教育功能，结合民办高校学生实际，构建多元评价体系。     

数字化机载环控地面检测系统的研究

通过采用两片PIC18F448及其外围器件实现了机载环控地面检测系统的数字化设计。通过I^2C总线实现两片单片机之间的数据传输与协调，并利用其CAN接口模块实现多套检测系统的网络化和远程控制操作。     

变推力液体火箭发机系统仿真软件的研究

闸明了变推力液体火箭发动机系统仿真软件设计的指导思想,介绍了软件的结构,着重叙述了典型部件的运算模块。最后,简单地介绍丁在实现该软件时的一些技术处理。     

构建高职数控技术应用专业课程体系的改革与实践

课程体系是衡量学校办学水平和教学质量的重要标志，是实现培养目标的基本保证。从构建课程体系前提、人才培养目标、人才培养机制、课程体系构建、课程体系改革的效果等几个方面对数控技术应用专业课程体系建设进行了探讨，初步构建了产学研结合的人才培养途径，建立了理论体系和实践体系相结合的课程体系。