AN UPPER PLIOCENE FLORULE FROM THE SANMENIAN SERIES OF SHANSI PROVINCE

The recent discovery of fossil plants in association with fresh-watermollusca,at the type locality of the Sanmenian series at Sanmen Rapids,addsa brief though important chapter to our gradually increasing knowledge of the     

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     

On Tectonic History in Regions East of the Tibetan Plateau from Kansu to Yunnan

正 With 2 Plates During the recent five years I have joined several field parties in the carrying out of geological reconnaissances in regions between the valley of the Huangho and of the Yangtze and in the Sino-Tibetan borderland. This vast territory can be divided into six major geological units, e     

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     

THE OCCURRENCE OF CERCIS ASSOCIATED WITH THE REMAINS OF SINANTHROPUS

In a short paper entitled "Evidences of the Use of Fire by Sinanthropus",Dr.Davidson Black has discussed the occurrence of burned bone fragments andcharcoal debris in association with the remains of Sinanthropus at Chou KouTien,and has concluded that Sina     

О ГЕОЛОГИЧЕСКОМ СТРОЕНИИ И РАЗВИТИИ ОКЕАНИЧЕСКИХ ВПАДИН

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ALKALINE INTRUSIVES OF LUTINGSHAN AND CH''IAOSHAN IN S.SHANSI

In recent years several localities of highly alkaline rocks have been dis-covered in Shansi by the National Geological Survey of China and the Sino-Swedish Research Institute.The results of investigation in this line up to 1927are embodied in the paper:"S     

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.