渤海动力环境研究应关注的新问题

回顾了近几年关于渤海动力环境的研究现状，分析了其中存在的问题。指出渤海盐度长期变化、年际尺度上变化的成因、过程；与此关联的渤海环流乃至黄海环流的变异及其过程；黄河入海的水、沙变化所引起发的渤海沉积物源汇的再调整等应是未来渤海动力环境研究中值得关注的重要问题。     

河南省电子政务空间信息服务系统建设与典型应用

介绍了河南省电子政务空间信息服务系统的项目背景、系统总体设计，论述了数据处理与集成建库所涉及的一些关键技术，并以中原城市群空间信息服务系统为典型应用，作了进一步的探讨。     

新建岩石地层单位的基本要求——以多索曲组的创建为例

本文介绍了岩石地层单位的基本概念,今后新创或修订岩石地层单位应提供的资料和说明,并以多索曲组的创建为例,对有关基本要求进一步予以说明。     

对死刑存废论争的思考

从辩证角度看,死刑存废论争有其自身的发展规律。论争的根源在于死刑自身所固有的矛盾性,因而论争的结果终将没有输家和赢家之分,争论将持续下去。然而,论争也有利于改变人们的观念和完善死刑制度。基于此,我们应汲取论争双方各自的合理之处,根据死刑内在发展规律和国家、社会发展的实际需要来灵活适用死刑。     

21cm波段太阳爆发中的精细结构

本文简要介绍了云南天文台新建立的21cm波段快速(不中断采样)记录系统,及使用该系统观测到的快速尖峰事件。系统得到的太阳分米波段爆发中不同时间尺度的精细结构与Stu-rroch等提出的太阳耀斑中能量释放的模式相一致。     

长江上游防护林体系建设要点

本区防护林体系的建设目标是:改善生态环境,发展山区经济。人口稠密区防护林体系建设成败的关健在于:能否掌握生态生产双重功能,是否具有生态社会经济三大效益。为此进行了防护林体系分类,提出了林种的生态功能指标和生产功能指标。防护林体系的生态经济分区要研究生态经济系绽的地域差异,有助于发挥各个林种的生态生产双重功能,是建设防护林体系的重要途径,为合理布局提供科学依据。     

Shock metamorphism on the moon

Shock metamorphism of the lunar samples is discussed. All types of lunar glasses formed by various-size collision-type impact are found as impact glass, ropy glass and agglutinates. The agglutinates bonded by crystal and glassy materials contain hydrogen and helium from the solar wind components. Lunar shocked minerals of plagioclase and silica show anomalous compositions and densities. There are typical two formation processes on planetary materials formed by shock events; that is (1) shocked quartz formed by silica-rich target rocks (esp. on evolved planets of the Earth and Mars), and (2) shocked silica with minor Al contents formed from plagioclase-rich primordial crusts of the Moon. The both shocked silica grows to coarse-grain normal crystals after high-temperature metamorphism which cannot distinguish the original main formation event of impact process.     

Modelling the outcomes of high-velocity impacts between small solar system bodies

We present a self-consistent numerical algorithm aimed at predicting the outcomes of high-velocity impacts between asteroids (or other small bodies of the solar system), based on a set of model input parameters which can be estimated from the available experimental evidence, and including the possible gravitational reaccumulation of ejected fragments whose velocity is less than a suitably defined escape velocity. All the fragment mass distributions are modelled by truncated power laws, and a possible correlation between fragment ejection velocity and mass is taken into account in different ways, including a probabilistic one. We analyze in particular the effectiveness of the gravitational reaccumulation process in terms of different choices of the collisional parameters and the assumed relationship between fragment speed and mass. Both the transition size beyond which solid targets are likely to reaccumulate a large fraction of the fragment mass and the collision energy needed to disperse most of the fragments are sensitive functions of the assumed fragment velocity versus mass relationship. We also give some examples of how our algorithm can be applied to study the origin and collisional history of small solar system bodies, including the asteroid 951 Gaspra (recently imaged by the Galileo probe) and the asteroid families.