温室效应、海平面上升与海岸地貌

温室效应引起全球增暖问题目前正受到科学家、工程技术人员、政治家和公众的广泛注意。最近的报告表明,对于全球增暖及其影响的确切性质尚不清楚(Schneider,1989)。然而,海岸带可能是一个关键而敏感的环境地带,全球增暖对海岸地貌会产生一系列后果。尽管到2100年全球海平面上升幅度的估计从56厘米到3.45米不等,但一般相差可能在44米和2.17米之间(Hoffman 等,1983:Titus,1987)。     

苏联经济区方案定量研究的经验

通常,经济区划的任务包括以下几个主要阶段:1) 确定作为基础区的地域;2)按照基础区选择区划指标系统及其定量评价;3) 选择区域系统模式;4) 阐明课题建立算法,直接把基础区进行分类计算;5)解释已获得的结果,选出最好的区划方案和有关进一步改善工作方法的结论等等。基础区的范围视所要解决的任务性质而定。     

自然-人为地理系统的主要原理

一、“自然—人为地理系统”概念的内容“地理系统”这一术语引入地理文献中虽然为时不久,但已牢固地确立下来了。“地理系统”概念的内容很广泛,它一般表示范围广阔的土地系统。本文只研究作为地理壳一部分的地理系统。这个系统的主要特征是它的地域性。谈到地理系统的划分,它主要分为两类:自然地理系统和人为地理系统。自然地理系统是指天然的,实际上没被人改变的系统,这就是自然地域综合体。     

对于进行地质普查、矿区找矿和勘探工作的几点基本要求

在这个报告中我准备讲一下苏联对于进行地质普查、矿区找矿和勘探工作方面的几点基本要求和工作方法上的一些原则。在谈到本题从前,我想简单地谈谈保证地质调查工作能够顺利进行的一些一般的原则。     

A 2D finite volume model for bebris flow and its application to events occurred in the Eastern Pyrenees

FLATModel is a 2D finite volume code that contains several original approaches to improve debris-flow simulation. Firstly, FLATModel incorporates a ＂stop-and-go＂ technique in each cell to allow continuous collapses and remobilizations of the debris-flow mass. Secondly, flow velocity and consequently yield stress is directly associated with the type of rheology to improve boundary accuracy. Thirdly, a simple approach for entrainment is also included in the model to analyse the effect of basal erosion of debris flows. FLATMODEL was tested at several events that occurred in the Eastern Pyrenees and simulation results indicated that the model can represent rather well the different characteristics observed in the field.     

NOTES ON THE GEOLOGY OF GREAT KHINGAN

In August 1933,I made geological investigations in the vicinity ofBarim station of Chinese Eastern Railway.This area was explored byDr.E.Ahnert in 1901~1,but my explorations were more in detail; I madegeological survey in the scale 1:10,000.All petrological determinations were     

现代大地构造理论中的某些重要问题

现状和问题现代大地构造中的问题与过去一样还没有完满地解决.其原因是缺乏能满足重大科学要求的统一的理论,因而对一直存在的大大小小的问题采用了各种不同的解决方式.在这种情况下自然更难以找到一个重要的基础或基点作为研究的起点,以致密观上使人们无所适从,并对大地构造学作了显然是虚无主义的评价.最近二十年,地质科学引入了大量精确的地球物理学概念,成功地解释了现代大洋的一系列特征,还引入了新全球构造说或岩石圈板块说.最初,似乎终于找到了解决所有构造学难题的灵丹妙药.全球构造是以行星演变的动力学和物质统一性为基础,对构造作用和现象     

Simulation Study on High Energy Cosmic Electron Detection by Shower Image

Many projects have recently been carried out and proposed for observing high energy electrons since it is realized that cosmic ray electrons are very important when study-ing the dark matter particles and the acceleration mechanism of cosmic rays. An imaging calorimeter,BETS (Balloon-borne Electron Telescope with Scintillator fiber),has been de-veloped for this purpose. Using pattern analysis of the shower development,the electrons can be selected from those primary cosmic ray proton events with flux heights one-tenth that of the electrons. The Monte-Carlo simulation is indispensable for the instrument design,the sig-nal trigger and the data analysis. We present different shower simulation codes and compare the simulation results with the beam test and the flight data of BETS. We conclude that the code FLUKA2002 gives the most consistent results with the experimental data.     

新疆及邻区Pn速度层析成像

利用新疆及邻区2万多条Pn射线的走时资料,采用层析成像的方法反演该地区上地幔顶部的Pn速度结构.主要结果是:①新疆地区平均h速度为.2km/s,高于中国大陆地区的平均值(.0km/s),速度变化量从-0.3km/s到0.2km/s.②准噶尔盆地是明显的高Pn速度区,高速区与地貌形状吻合较好,最大值达.4km/s;塔里木盆地整体上呈现高速异常二者都可能与盆地是稳定地块、构造活动和变形较弱有关.③在盆地与山脉的交接带即主要的构造活动带,存在较低的Pn速度,可达7.9km/s.④塔里木南缘中部存在一显著的低速区,可能与岩浆活动和构造活动较强有关.⑤上地幔顶部波速各向异性整体上盆地中心较弱,边缘地带较强.新疆南部波速的各向异性可能是因印度板块对欧亚大陆的碰撞使地幔物质向北蠕动的结果.     

Magnetic Field Strengths and Structures from Radio Observations of Solar Active Regions

Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field.