鲜水河断裂带的构造大地测量   总被引：2，自引：2，他引：0  

刘本培  朱智勤  廖华  吕弋培 《大地测量与地球动力学》2001,21(4):17-25

利用短边GPS点阵、短基线标石阵和精密激光测距 ,在与鲜水河断裂带的断层破裂带垂直的剖面上和构造盆地内进行构造大地测量 ,获得了断层软弱带和断层蠕变带上的最佳形变分布。综合利用相关地学成果和理论 ,揭示了构造形变所隐含的动力学信息 ,识别了断层应变带、塑性流变带和主断面在地面的分布范围。用外围GPS远场联测成果探讨了该断裂带的驱动力机制 ,匡正了其“左旋”运动和现今活动速度的含义。最后 ,评估了该断裂的地震活动趋势  相似文献   

Possible Evidence of Long-Term Oscillations in the Solar Atmosphere     

Raju  K.P.  Singh  Jagdev  Srikanth  R.  Chou  Dean-Yi  Team  the Ton 《Solar physics》2001,199(1):1-11

We have obtained the temporal correlation function, Q(t), from time sequences of Caii K filtergrams and Dopplergrams from Antarctica, Taiwan Oscillation Network (TON) and Solar and Heliospheric Observatory (SOHO). Q(t) gives the time evolution of the pattern under examination, supergranulation in this case. It has been found that Q(t) shows oscillatory signals of both 5-min and long-term periods. The 5-min oscillations are suppressed by averaging the images over 10 min. An exponential decay curve which represents the lifetime trend of supergranules, is fitted to Q(t) and subtracted out. The Q(t) residuals thus obtained contain the oscillatory component and are then subjected to a periodogram analysis. Significant periodicities in the range of 1.4–10 hours have been noted. The causes of these oscillations are not fully known at present, but the instrumental and atmospheric factors can be ruled out, pointing to solar origin. Various possibilities are discussed. Some of the observed periodicities may be considered as probable candidates for long-term oscillations in the Sun, such as the elusive gravity modes.  相似文献   

西太平洋海山磷酸盐的常量、微量和稀土元素地球化学研究   总被引：8，自引：0，他引：8  

潘家华  刘淑琴  杨忆  刘学清 《地质论评》2002,48(5):534-541

本文对主要取自于西太平洋我国调查区内不同海山、不同水深、不同产状的13个磷酸盐样品进行了常量、微量和稀土元素测定,以探讨与大洋富钴结壳密切伴生的磷酸盐的常、微量和稀土元素地球化学的特征。分析结果表明,调查区磷酸盐中主要氧化物的平均值与赤道太平洋的相近,暗示两者可能有相似的形成环境和形成机制。磷酸盐中微量元素Sr、Ba、Co、Cu、Ni及U丰度分别变化于862×10~(-6)～2181×10~(-6)、29×10~(-6)～3429×10~(-6)、6.3×10~(-6)～115×10~(-6)、23×10~(-6)～263×10~(-6)、12×10~(-6)～825×10~(-6)及4×10~(-6)～11×10~(-6),丰度多数低于泥质岩平均值,其CaO/P_2O_5、F/CO_2、Sr/P_2O_5值及常量、微量元素间的相关关系,清晰地显示了磷酸盐的种类、成分与结构、形成的地质背景和元素的主要组合特征。磷酸盐的稀土丰度为136.50×10~(-6)～853.70×10~(-6);Ce~*变化于0.01～0.18之间;(Ce/Yb)_N值变化于0.01～0.21之间。研究证实,不同产状磷酸盐的稀土元素配分模式基本一致,曲线相互平行,基本不呈现交叉现象,均呈Ce强烈亏损,轻、重稀土分馏程度大及重稀土富集的型式。调查区、赤道太平洋、中太平洋磷酸盐的稀土元素丰度、Ce~*、Ce/Yb值以及它们与海水稀土元素配分模式相似的特征,也进一步显  相似文献   

中国地震学会地震学专业委员会工作及学术活动     

中国地震学会地震学专业委员会 《国际地震动态》2001,(1):17-18

中国地震学会第五届地震学专业委员会自1999年1月成立以来,在常务理事会和学会理事长的指导下,充分发挥委员在基础研究和战略研究方面的整体优势,围绕我国地震科学发展和防震减灾事业的一些重要问题,开展了多方面的工作。其中,将专业委员会活动的视野进一步扩大,与国内的有关机构和团体开展多方面的合作,并积极关注和参与国际性的学术活动,是本届专业委员会活动的一个特色。英国《自然》杂志(Nature)于1999年2月25日～4月8日在因特网上组织了主题为“Isthereliablepredictionofindividualearth-quakesarealisticscientificgoal?”的争论,引…  相似文献   

帕米尔东北缘及塔里木盆地西北部弧形构造的扩展特征   总被引：15，自引：0，他引：15  

沈军  汪一鹏  赵瑞斌  陈杰  曲国胜 《地震地质》2001,23(3):381-389

归纳了帕米尔东北缘弧形构造的基本特征 ,分析了塔里木盆地西北部EW向逆断裂背斜带与NNW向隐伏走滑断裂之间的关系。通过塔里木盆地与西南天山和帕米尔东北缘变形特征的对比 ,认为塔里木盆地西北部的变形样式与帕米尔东北缘的弧形构造类似 ,弧形构造具有由帕米尔东北缘向塔里木盆地扩展的特征 ,这种构造是帕米尔向北挤入运动所特有的变形样式  相似文献   

1989年大同—阳高地震现场分析预报工作回顾     

刘巍 《山西地震》1992,(1):8-18

叙述了1989大同—阳高地震的基本情况,回顾了此次地震现场的分析预报工作。按照《地震现场工作大纲和震情分析指南》所确定的原则,采用国内常用的一些方法,对此次地震的类型、震前活动、地震趋势、余震活动等做了分析。并对几次强余震的预报过程进行了讨论。  相似文献   

应用氢氧同位素方法研究兰州市傍河水源地地下水水体的形成和循环机理     

余振国  连炎清 《甘肃地质》1992,1(1):68-84

本文通过测定水中氢氧同位素的变化来对兰州市傍河水源地地下水体的形成和循环机理进行分析探讨。分析了兰州市马滩水源地水质恶化的程度,探讨了恶化的原因。对其工作原理及方法作了较详尽的论述。  相似文献   

采用阶梯抽水试验资料确定含水层参数     

王必刚 《上海国土资源》1993,(3):27-36

本文采用阶梯降深的有关公式,结合某矿区的一次多孔抽水试验资料进行试算,并和雅柯布直线法和恢复水位法求得的参数比较,汁算结果令人满意,表明该法是种简便、有效的求参手段。  相似文献   

Monte Carlo Radiative Transfer Modeling of Lightning Observed in Galileo Images of Jupiter   总被引：1，自引：0，他引：1  

U.A. DyudinaA.P. Ingersoll  A.R. VasavadaS.P. Ewald  the Galileo SSI Team 《Icarus》2002,160(2):336-349

We study lightning on Jupiter and the clouds illuminated by the lightning using images taken by the Galileo orbiter. The Galileo images have a resolution of ∼25 km/pixel and are able to resolve the shape of single lightning spots, which have half widths (radii) at half the maximum intensity in the range 45-80 km. We compare the shape and width of lightning flashes in the images with simulated flashes produced by our 3D Monte Carlo light-scattering model.The model calculates Monte Carlo scattering of photons in a 3D opacity distribution. During each scattering event, light is partially absorbed. The new direction of the photon after scattering is chosen according to a Henyey-Greenstein phase function. An image from each direction is produced by accumulating photons emerging from the cloud in a small range (bins) of emission angles. The light source is modeled either as a point or a vertical line.A plane-parallel cloud layer does not always fit the data. In some cases the cloud over the light source appears to resemble cumulus clouds on Earth. Lightning is estimated to occur at least as deep as the bottom of the expected water cloud. For the six flashes studied, we find that the clouds above the lightning are optically thick (τ>5). Jovian flashes are more regular and circular than the largest terrestrial flashes observed from space. On Jupiter there is nothing equivalent to the 30-40-km horizontal flashes that are seen on Earth.  相似文献   

Magnetic properties of soils from sites with different geological and environmental settings   总被引：7，自引：0，他引：7  

Hana Fialov  Günter Maier  Eduard Petrovský  Ale&#x; Kapi ka  Tetyana Boyko  Robert Scholger  MAGPROX Team 《Journal of Applied Geophysics》2006,59(4):273-283

Measurements of magnetic susceptibility of soils, reflecting magnetic enhancement of topsoils due to atmospherically deposited magnetic particles of industrial origin, are used recently in studies dealing with outlining polluted areas, as well as with approximate determination of soil contamination with heavy metals. One of the natural limitations of this method is magnetic enhancement of soils caused by weathering magnetically rich parent rock material. In this study we compare magnetic properties of soils from regions with different geological and environmental settings. Four areas in the Czech Republic and Austria were investigated, representing both magnetically rich and poor geology, as well as point-like and diffuse pollution sources. Topsoil and subsoil samples were investigated and the effect of geology and pollution was examined. Magnetic data including mass and volume magnetic susceptibility, frequency-dependent susceptibility, and main magnetic characteristics such as coercivity (Hc and Hcr) and magnetization (Ms and Mrs) parameters are compared with heavy metal contents. The aim of the paper is to assess the applicability of soil magnetometry under different geological-environmental conditions in terms of magnetic discrimination of dominant lithogenic/anthropogenic contributions to soil magnetic signature. Our results suggest that lithology represents the primary effect on soil magnetic properties. However, in case of significant atmospheric deposition of anthropogenic particles, this contribution can be clearly recognized, independent of the type of pollution source (point-like or diffuse), and discriminated from the lithogenic one. Different soil types apparently play no role. Possible effects of climate were not investigated in this study.  相似文献