Diversity of Comets: Formation Zones and Dynamical Paths

The past dozen years have produced a new paradigm with regard to the source regions of comets in the early solar system. It is now widely recognized that the likely source of the Jupiter-family short-period comets (those with Tisserand parameters, T > 2 and periods, P, generally < 20 years) is the Kuiper belt in the ecliptic plane beyond Neptune. In contrast, the source of the Halley-type and long-period comets (those with T < 2 and P > 20 years) appears to be the Oort cloud. However, the comets in the Oort cloud almost certainly originated elsewhere, since accretion is very inefficient at such large heliocentric distances. New dynamical studies now suggest that the source of the Oort cloud comets is the entire giant planets region from Jupiter to Neptune, rather than primarily the Uranus-Neptune region, as previously thought. Some fraction of the Oort cloud population may even be asteroidal bodies formed inside the orbit of Jupiter. These comets and asteroids underwent a complex dynamical random walk among the giant planets before they were ejected to distant orbits in the Oort cloud, with possible interesting consequences for their thermal and collisional histories. Observational evidence for diversity in cometary compositions is limited, at best. This revised version was published online in June 2006 with corrections to the Cover Date.     

高校体育多媒体教学平台系统的建设研究

本文从当前高校体育教学的周期短、学时少、教学方法单一的特点出发,充分的利用现代计算机网路多媒体技术,设计一套符合高校体育教育的多媒体教学平台系统,以满足学生课余时间的自主学习,增加教学的延伸性、娱乐性,为高校体育教育目标的实现提供保障。     

改进体育课堂教学质量的几点思考

本文对现在体育教学方法提出了几点改进意见。目的是为了提高体育课的教学质量，增强学生的身体健康。     

Coupled Clouds and Chemistry of the Giant Planets— A Case for Multiprobes

In seeking to understand the formation of the giant planets and the origin of their atmospheres, the heavy element abundance in well-mixed atmosphere is key. However, clouds come in the way. Thus, composition and condensation are intimately intertwined with the mystery of planetary formation and atmospheric origin. Clouds also provide important clues to dynamical processes in the atmosphere. In this chapter we discuss the thermochemical processes that determine the composition, structure, and characteristics of the Jovian clouds. We also discuss the significance of clouds in the big picture of the formation of giant planets and their atmospheres. We recommend multiprobes at all four giant planets in order to break new ground.     

凝胶点官能度是重均官能度,还是数均官能度

Flory和Stockmayer等的凝胶化理论用重均官能度表示凝胶点或凝胶生成的临界条件,虽已有50多年的历史,并为各国学者所公认,但从分析凝胶点定义的物理意义出发,只要用简单的数学分析,即可证明用重均官能度而不用数均官能度表示凝胶点,与反应程度定义的物理意义和Flory的两个基本假设不符。凝胶化理论新概念用数均官能度表示凝胶点,则不存在不符的问题。     

刚体转动惯量的测量及数据处理

本文采用一元线性回归法进行刚体转动惯量实验的数据处理,对通常在测量中运用的简化条件作了分析,从而提高了实验课的教学水平,并使该实验具有实用价值。     

基于模型的系统工程方法在载人航天任务中的应用探讨

针对基于文档的航天任务设计中设计数据分散、一致性差、跟踪难度大等问题,引入了基于模型的系统工程(MBSE)方法。首先,介绍了MBSE方法理念,即通过构建图形化的模型来支持系统的需求捕获、设计、分析、验证和确认等全生命周期活动。然后,给出了MBSE方法的一般工作流程,即先构建系统的需求模型,用于指导功能模型、物理架构模型等的构建,按照事先制定好的逻辑规则建立模型间的关系,依靠模型间的关系实现设计过程中的关联性分析、参数查询等工作。最后,应用MBSE方法于载人飞船交会对接任务中。结果表明,此方法改善了人员沟通,提高了设计效率,降低了设计风险,可为MBSE方法在航天任务设计中的进一步应用提供参考。     

某飞翼布局隐身飞行器的翼型优化

对某飞翼布局无人机的翼型进行考虑隐身迎角的气动、隐身综合优化研究。采用基于非均匀有理B样条曲线的自由变形方法实现翼型的参数化表达;无限插值动网格方法生成气动求解的计算网格;分别采用基于雷诺平均N—S方程求解的计算流体力学方法及物理光学法计算翼型的气动、隐身性能;选择多目标遗传算法进行综合寻优设计研究。优化翼型兼顾了气动与隐身的要求,其综合性能优于原翼型。结果表明,方法具有较好的实用性。     

Passive inter-modulation scattering analysis of reflector considering contact nonlinearity

 Passive inter-modulation (PIM) is a form of nonlinear distortion caused by the inherent nonlinearities of the passive devices and components in RF/microwave system. It will degenerate the performance of communication system with broad-band channel and high-sensitivity receiver. Therefore, it is necessary to construct a model to simulate this process in order to predict the level of PIM. This paper is aimed at constructing some plate models with one-dimensional and two-dimensional contact nonlinearity sections illuminated by two-tone waves, and calculating the scattered field at a fixed-point in space using time-domain physical optics method. By taking fast Fourier transform (FFT), we get the spectrum of the scattered field and then analyze the generated PIM products. At the end of this paper, some numerical examples are presented to show the influence rules of the relative factors on PIM. The results indicate the variation of the level of PIM with the number of the nonlinear regions, the nonlinear spacing, and the incident power levels.