跨断层的定点地壳形变研究及发展前景

新世纪内,在空间测地技术发展的同时,在现代地壳形变的监测和研究工作中,传统的大地测量方法仍具有不可替代的作用。全自动激光测量方法（ＥＤＭ）将是常规的跨断层定点的壳形变监测技术主要的发展方向。日本学者在２０世纪９０年代前后发展起来的中距离ＥＤＭ观测台获得了良好的成果。台湾花莲跨花东断层的ＥＤＭ观测台揭示了９．２１大地震有明显的中期和短临前兆,实践证明,这种方法不仅在成果质量和观测精度上可以和ＧＰＳ相     

磷灰石U-Th/He法——一种低温热年代计

回顾了U Th/He测年方法的发展过程 ,简要介绍了该方法测年的原理、分析流程和长α -粒子停止距离校正。然后介绍了近年来在磷灰石He扩散性研究及数值模拟方面取得的一些成果和磷灰石U Th/He热年代计在研究古地貌、岩体构造抬升、盆地热历史演化方面的应用。最后分析了U Th/He测年方法的优、缺点 ,说明这一方法既存在广阔的应用前景 ,又有待于进一步完善、提高。     

横向土运动作用下群桩的性状研究

以有限元与有限差分相结合,对横向土运动作用下的群桩工作性状,产生群桩效应的临界桩距、桩数及排列、桩顶边界条件等影响因素作出分析;并对沿桩排的应力分布作出初步探讨。     

加筋水泥土梁力学性能的试验研究

在对加筋水泥土进行力学试验的基础上, 初步得出其基本的力学性能, 以期为加筋水泥土用于支护工程提供试验依据。     

三维观测系统中横向覆盖次数及CDP间隔的计算方法

总结了三维观测系统中横向覆盖次数及CDP间隔计算的综合平面图法、坐标法、Z变换公式法,指出了3种方法各自的优、缺点和适用性。     

The most metal-poor galaxies

Summary. Metallicity is a key parameter that controls many aspects in the formation and evolution of stars and galaxies. In this review we focus on the metal deficient galaxies, in particular the most metal-poor ones, because they play a crucial r?le in the cosmic scenery. We first set the stage by discussing the difficult problem of defining a global metallicity and how this quantity can be measured for a given galaxy. The mechanisms that control the metallicity in a galaxy are reviewed in detail and involve many aspects of modern astrophysics: galaxy formation and evolution, massive star formation, stellar winds, chemical yields, outflows and inflows etc. Because metallicity roughly scales as the galactic mass, it is among the dwarfs that the most metal-poor galaxies are found. The core of our paper reviews the considerable progress made in our understanding of the properties and the physical processes that are at work in these objects. The question on how they are related and may evolve from one class of objects to another is discussed. While discussing metal-poor galaxies in general, we present a more detailed discussion of a few very metal-poor blue compact dwarf galaxies like IZw18. Although most of what is known relates to our local universe, we show that it pertains to our quest for primeval galaxies and is connected to the question of the origin of structure in the universe. We discuss what do QSO absorption lines and known distant galaxies tell us already? We illustrate the importance of star-forming metal-poor galaxies for the determination of the primordial helium abundance, their use as distance indicator and discuss the possibility to detect nearly metal-free galaxies at high redshift from Ly emission. Received 19 August 1999 / Published online: 15 February 2000     

贝叶斯统计方法在海浪方向谱研究中的应用

较详细介绍了贝叶斯统计方法在海浪方向谱估计中的应用,指出先验分布的不同对估计结果没有影响,由于均匀分布与最大熵原则相对应,使其具有某种特殊性.数值模拟表明贝叶斯方法对双峰方向分布估计的有效性,将其应用于黑海实测资料,证明双峰方向分布的出现依赖于估计方法分辨力的大小,而用最大似然法得到的双峰方向分布值得怀疑.最后给出出现双峰方向分布的一种可能物理解释.     

中等贫金属星的元素丰度分析

给出 １１颗中等贫金属星－１．３ ５［Ｆｅ／Ｈ］ ≤－０．６的观测资料,确定了这些样本星的恒星大气参数,得到了这些星中１４种元素的丰度．讨论了各类元素丰度比随金属丰度的变化。α元素（Ｍｇ、 Ｓｉ、 Ｃａ、 Ｔｉ）相对于铁均表现超丰,每一金属丰度处都存在不同程度的弥散．大部分的铁峰元素（Ｖ、Ｃｒ、Ｎｉ、Ｃｕ）也相对于铁超丰,不随［Ｆｅ／Ｈ］而变化,而［Ｍｎ／Ｆｅ］则随金属丰度的增加而增加．［Ｎａ／Ａｌ］在［Ｆｅ／Ｈ］＞－１．１的样本星中表现超车,在［Ｆｅ／Ｈ］＜－１．１的样本中却明显过贫．