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.     

船载炮射击时的角度修正

分析了船在航行中的几种摇荡对火炮射击精度的影响 ,主要介绍了用于消除船体纵摇角和横摇角影响的数学平台的建立方法 ,以及射击角的修正。     

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。     

激光微推进器用于微小卫星的姿轨控仿真

为研究激光微推进器用于微小卫星在轨空间飞行任务的可行性,利用已建立的激光推进微小卫星仿真平台,对微小卫星在轨姿态调整、轨道维持和轨道转移等飞行任务进行了仿真和分析。仿真结果表明,星载激光微推进器可满足在轨微小卫星的高控制精度姿态调整、近地观测轨道维持以及较长时间要求的轨道转移等空间任务对推进系统的要求。     

Autonomous Control Reconfiguration of Aerospace Vehicle Based on Control Effectiveness Estimation

未来空天飞行器跨空天两域飞行,要求有较高的自主性以适应由故障和环境变化带来的不确定因素。针对空天飞行器的不确定性,提出了自主控制重构方案。研究了线性模型的时变控制效益的估计方法,提出并证明了效益矩阵可估计的充分条件,给出了相应的算法并证明了其收敛性和对噪声的鲁棒性;提出了基于线性规划和模糊逻辑的控制分配算法,通过冗余效应器实现了不确定条件下的自主控制重构。系统集成和仿真结果分析验证了方案和算法的有效性。