思茅盆地河流地貌特征及其对构造活动的响应

河流地貌对构造活动具有极高的相关性、敏感性,是研究新构造活动最切实有效的地摘貌标要志之一。本文以30 m分辨率数字高程模型（DEM）为基础,利用ArcMap与Matlab软件提取的河流地貌因子（Horton定律比值和S-A双对数曲线）,先后分析了思茅盆地内部的李仙江、藤条江、勐戛河、威远江、南班河和南腊河等的河流地貌特征,揭示新生代晚期强烈构造活动对河流发育的影响。结果表明：1）思茅盆地的河流多沿或平行于走滑断裂发育,低级别河网较好的符合Horton定律中一般河网的发育规律,而沿活动断裂带发育的高级别河网则表现出了明显的偏差;2）各集水盆地 S-A双对数曲线均呈凹凸相间排列;3）各集水盆地河道的裂点分布特征与岩性变化不一致,这表明思茅盆地内部高级别河网的发育受岩性变化的影响较小,而主要受走滑断裂活动的影响。     

宝石表面光泽度的理论值

从光泽度的物理本质出发,导致出光泽度的理论公式,算出各种不同宝石的光泽度理论值,用此值去判断可能达到最佳的抛光效果。     

开鲁盆地陆家堡西部凹陷上侏罗统沉积体系研究

本文运用地质、地震和测井等资料对陆西凹陷上侏罗统沉积体系特征进行了综合研究。该区上侏罗统发育了近岸水下扇、三角洲和以凹陷中古隆起为沉积背景的高垒斜坡扇等3种沉积体系，其中近岸水下扇为上侏罗统分布最普遍的沉积类型，构成本区主要储层，高垒斜坡扇是与水下古隆起有关的由滑塌作用形成的重力流沉积体，构成本区极富特色的沉积体系。     

三个连续性台风特征分析

“榴莲”、“尤特”、“玉兔”三个台风前后相隔不到4天、20天在同一月份相继登陆广东沿海,且均严重影响粤西地区,在历史同期是首例。本文从有利台风形成、发展的大尺度环流背景、制约台风移向的有利环境场演变和台风登陆带来茂名地区风雨分布悬殊特点进行分析,为探讨热带气旋预报累积一定经验。     

重庆奉节天坑地缝喀斯特地质遗迹及发育演化

小寨天坑、天井峡地缝式喀斯特峡谷位于重庆市奉节县南部深切割峰丛谷地区,发育在一个流域面积280km2,落差1600m的喀斯特水文系统中,与巨大的地下河相连。前者深662m,口径626m,容积119×106m3,是目前世界上规模最大的天坑;后者长6162m,最大深度229m,最小宽度1m,为世界上罕见的地缝式喀斯特峡谷,具有很高的美学观赏价值和科研价值。天坑、地缝的形成条件,需要有连续沉积厚度巨大的碳酸盐岩层和平缓的岩层产状、高强度水动力作用地下河的存在、地表深切和地表地下排水基准面的长期大幅度下降、厚度相当大的包气带、地表与地下喀斯特作用协同等。天坑、地缝主要形成于峡谷期(三峡期),经历了3个演化阶段,即宽缓河流谷地阶段、峡谷及天坑地缝形成阶段和现代河谷持续深切阶段。     

Letters from Carlos Ibáñez e Ibáñez de Ibero to Aimé Laussedat: new sources for the history of nineteenth century geodesy

Recently found letters written by Carlos Ibáñez e Ibáñez de Ibero (1825–1891), first president of the International Geodetic Association, to geodesist–photogrammetrist Aimé Laussedat (1819–1907) are discussed. The contents of these epistolary conversations reflect their personal preoccupation with solving the geodetic problems of the time (1857–1889) and their desire to develop and propagate geodetic knowledge across all international boundaries.     

The Green Corona and Magnetic Fields

We present results of a study of the green corona (530.3 nm, Fexiv) and photospheric magnetic fields over the period 1976–1999 when both quantities were observed by ground-based observatories. By comparing both the limb green-line intensities and photospheric magnetograms we have found a relation between the strength of magnetic field and coronal intensities. This relation enables us to extend solar surface magnetic fields since 1976 back to 1939. From 1947 to 1992 the magnetic field strength grew at the cycle maxima by a factor of 1.5–2. On the other hand, both the green corona intensity and magnetic field strength in the present cycle are smaller compared to cycle 22, by a factor of 2. No relationship was found between the green corona intensities and magnetic field polarity as was previously supposed. Behavior for the green corona intensities is different between high-latitude and mid-latitude regions, and this break occurs at the heliographic latitude of ± 45°. Homogeneous coronal data set cannot be directly used to derive `the tilt angle', even though some similarities between the green coronal holes, poleward branches in the green corona and prominences and the tilt angle can be found.     

The North-South Asymmetry in the Green Corona

The north-south asymmetry of the Fe XIV 530.3 nm coronal emission line (the green corona) over cycle 22 was investigated. The green corona line brightness was dominant in the southern hemisphere during cycle 22 (A = –0.07), except for short periods of the ascending phase of the activity cycle. The asymmetry of the semi-annual mean over the period 1940 – 1996 was also studied. The asymmetry, during these years, reached its maximum in 1962 – 1966, and then decreased. Important periodicities of the asymmetry in cycle 22, e.g., 158 and 350 days, 2.39 years were found. Similar periodicities were also detected in the years 1940 – 1996. An FFT analysis was used to detect these periodicities.     

Prominences and the Green Corona Over the Solar Activity Cycle

Prominences, in contrast to other solar activity features, may appear at all heliographic latitudes. The position of zones where prominences are mainly concentrated depends on the cycle phase of solar activity. It is shown, for prominence observations made at Lomnický tít over the period 1967–1996, how the position of prominence zones changes over a solar cycle, and how these zones could be connected with other solar activity features. Our results obtained could be an additional source to do a better prediction of solar activity. Time-latitudinal distribution is also shown for the green corona (Fexiv, 530.3 nm). Distribution of the green coronal maxima shows that there are equator-migrating zones in the solar corona that migrate from latitudes of 45° (starting approximately 2–3 years after the cycle start) to higher latitudes 70°, and then turn (around the cycle maximum) towards the equator, reaching the equator in the next minimum (this duration lasts 18–19 years). Polar branches separate from these zones at the cycle minimum (2–3 years before above-mentioned zones) at latitudes of 50°, reaching the poles at the maximum of the present cycle. The picture becomes dim when more polar prominence zones are observed. Prominences show both the poleward and equatorward migration. Comparison between both solar activity features is also discussed.     

川西沙坝麻粒岩的Sm-Nd和Rb-Sr同位素年龄及其地质意义

首次测定扬子板块西缘古老的结晶基底岩石沙坝麻粒岩Sm Nd矿物等时线年龄为 114 0± 110Ma ,代表中元古代末期麻粒岩相变质作用时代。Rb -Sr矿物等时线年龄为 2 18± 11Ma ,可能为晚古生代至早中生代基性岩浆侵入的热扰动改造年龄。其亏损地幔模式年龄TDM 为115 8Ma ,表明沙坝麻粒岩的原岩在成岩之后不久即经受麻粒岩相变质作用。根据上述年龄以及紫苏辉石中Nd同位素封闭温度和40 Ar/ 3 9Ar年龄等资料的计算表明 ,以沙坝麻粒岩为代表的下地壳岩石抬升运动速率是缓慢的