用断裂力学模型对地震前兆进行分类     

I.G.Main邱泽华  张宝红 《地壳构造与地壳应力》1992,(2):48-55

目前在地震前兆的观测方面，普遍趋向于将最突出的地震前兆根据可能有的预警时间归类于一种地震发生的模型．例如，Rikitakc(1987)最近收集了418个日本的地震前兆异常，并按照前兆时间作了分类．虽然在可靠性和统计意义上变动很大，但是这种经验观测至少可以分出4种截然不同的类型，  相似文献   

什么是断层陡坎？     

I.S．Stewart侯治华  苏怡之 《地壳构造与地壳应力》1992,(3):20-27

近十年来，不断加强对构造活动性的仪器观测和历史记录。人们把注意力集中于根据地质，地貌的记录鉴别和研究古地震上，重要的是识别断层地貌特片，例如，断层陡坎，它可能是某一区域构造活动类型及其活动时间的明显标志。  相似文献   

爱琴地区新构造正断层带的构造非均匀性     

I.S.Stewart P.L.Hancock马保启  吴卫民 《地壳构造与地壳应力》1992,(5):40-53

一、引言 本文是对爱琴张性构造区新构造正断层带为期五年的野外调查结果所作的综台与分析(图1)．着重介绍爱琴地区的三个地带．(1)希腊大陆的科林斯地区(图1a)．(2)西土耳其的伊密兹尔地区(图1b)．(3)柯雷特的中部及西部(图1c)．在这三个地带正断层使中生代碳酸岩同第四纪沉积物直接相接，  相似文献   

椭球面上多边形的面积计算     

Gilli.  I 李晓桓 《测绘科技动态》1995,(1):39-42

本文给出了椭球面上多边形面积计算的一种新方法。这个多边形的边可能是大地线、恒向线、大圆线或是它们的组合。  相似文献   

波罗的地盾东部与构造有关的前寒武纪成矿作用     

S.I.Turchenko 《华北地质》1993,(4)

波罗的地盾东部的大部分地区为太古宙大陆壳,主要由具有不同构造环境的三个块体组成。1)科拉半岛省,由麻粒岩—片麻岩(含 Fe、Ni-Cu 矿床)、含 Ni-Cu 及条带状铁建造和 REE 矿床的绿岩带、含蓝晶石矿床的强烈变形的火山—沉积盆地和赋 Fe-Ti-V 矿床的晚太古宙辉长岩—斜长岩侵入体等组成。2)卡累利阿省,是典型的花岗岩—绿岩带地体。绿岩带是在洛平(Lopian)造山运动期间形成的(2.9—2.6Ga),其构造环境类似裂谷和岛弧。该省含有 Ni-Cu 和块状黄铁矿矿床,并有铜矿化,以及条带状铁建造。晚造山期花岗岩含有斑岩型的 Mo、Cu-Mo 矿床。3)自海省,是一个麻粒岩—片麻岩和  相似文献   

The possible influences of the increasing anthropogenic emissions in India on tropospheric ozone and OH   总被引：2，自引：0，他引：2  

LIU Yu  LI Weiliang  ZHOU Xiuji  I.S.A.ISAKSEN  J.K.SUNDET  HE Jinhai 《大气科学进展》2003,20(6):968-977

A 3-D chemical transport model (OSLO CTM2) is used to investigate the influences of the increasing anthropogenic emission in India. The model is capable of reproducing the observational results of the INDOEX experiment and the measurements in summer over India well. The model results show that when NOx and CO emissions in India are doubled, ozone concentration increases, and global average OH decreases a little. Under the effects of the Indian summer monsoon, NOx and CO in India are efficiently transported into the middle and upper troposphere by the upward current and the convective activities so that the NOx, CO, and ozone in the middle and upper troposphere significantly increase with the increasing NOx and CO emissions. These increases extensively influence a part of Asia, Africa, and Europe, and persist from June to September.  相似文献   

Total and methylmercury in a Brazilian estuary,Rio de Janeiro     

Kehrig HA  Costa M  Moreira I  Malm O 《Marine pollution bulletin》2002,44(10):1018-1023

Guanabara Bay, in Rio de Janeiro state, is impacted by organic matter, oil and heavy metals. The present study evaluated the total mercury (THg) and methylmercury (MeHg) concentrations and the MeHg to THg ratio (%MeHg) in water samples from different points of the bay and in 245 organisms of three different trophic levels sampled between 1990 and 2000. Dissolved mercury concentration in estuarine water samples ranged from 0.72 to 5.23 ngl(-1). THg and MeHg in mussel, ranging from 11.6 to 53.5 microg THg kg(-1) wet wt. and 4.5-21.0 microg MeHg kg(-1) wet wt., varied according to sampling point and water quality. Planktivorous fish and mussel presented similar MeHg concentrations, meanwhile THg in planktivorous fish were lower than in mussel. Carnivorous fish showed higher THg and MeHg concentrations (199.5 +/- 119.3, 194.7 +/- 112.7 microg kg(-1) wet wt. respectively) than organisms from other feeding habits and lower trophic levels. There was a significant difference in the %MeHg among trophic levels: mussel presented lower MeHg percentage (33%) than planktivorous fish (54%) and carnivorous fish (98%).  相似文献   

Environmental transformation of the Bilbao estuary,N. Spain: microfaunal and geochemical proxies in the recent sedimentary record     

Cearreta A  Irabien MJ  Leorri E  Yusta I  Quintanilla A  Zabaleta A 《Marine pollution bulletin》2002,44(6):487-503

The distribution and abundance of benthic foraminifera and a range of elements have been analysed in six long cores (up to 10 m long) from the Bilbao estuary, N. Spain, to document environmental transformation of this estuarine ecosystem and to determine sediment contamination levels. Three different environmental zones could be distinguished in the recent sedimentary record based on its microfaunal and geochemical contents. Initially, a pre-industrial zone containing very abundant and diverse foraminiferal assemblages together with baseline metal levels. Secondly, an older industrial zone exhibiting co-existence of abundant and diverse foraminiferal assemblages with high concentrations of metals. Finally, a younger industrial zone with extreme concentrations of metals and barren of indigenous foraminifera. This environmental transformation has been caused by the discharge of untreated domestic and industrial effluents during the last 150 years. The occurrence of foraminifera in the two industrial zones and along the estuary is not related to defined levels of metals, and this seems to confirm oxygen limitation as the key factor to explain complete estuarine defaunation during deposition of the younger industrial zone (period 1950-2000). Effectiveness of current regeneration schemes could be assessed using microfaunal and geochemical proxies as environmental quality indicators.  相似文献   

A Model for the Quiescent Phase of the Recurrent Nova U Scorpii     

Hachisu I  Kato M  Kato T  Matsumoto K  Nomoto K 《The Astrophysical journal》2000,534(2):L189-L192

A theoretical light curve is constructed for the quiescent phase of the recurrent nova U Scorpii in order to resolve the existing distance discrepancy between the outbursts (d approximately 6 kpc) and the quiescences (d approximately 14 kpc). Our U Sco model consists of a very massive white dwarf (WD), an accretion disk (ACDK) with a flaring-up rim, and a lobe-filling, slightly evolved, main-sequence star (MS). The model properly includes an accretion luminosity of the WD, a viscous luminosity of the ACDK, and a reflection effect of the MS and the ACDK irradiated by the WD photosphere. The B light curve is well reproduced by a model of 1.37 M middle dot in circle WD + 1.5 M middle dot in circle MS (0.8-2.0 M middle dot in circle MS is acceptable) with an ACDK having a flaring-up rim and the inclination angle of the orbit i approximately 80&j0;. The calculated color is rather blue (B-V approximately 0.0) for a suggested mass accretion rate of 2.5x10-7 M middle dot in circle yr-1, thus indicating a large color excess of E(B-V) approximately 0.56 with the observational color of B-V=0.56 in quiescence. Such a large color excess corresponds to an absorption of AV approximately 1.8 and AB approximately 2.3, which reduces the distance to 6-8 kpc. This is in good agreement with the distance estimation of 4-6 kpc for the latest outburst. Such a large intrinsic absorption is very consistent with the recently detected period change of U Sco, which is indicating a mass outflow of approximately 3x10-7 M middle dot in circle yr-1 through the outer Lagrangian points in quiescence.  相似文献   

ASCA Observation of the Quiescent X-Ray Counterpart to SGR 1627-41     

Hurley K  Strohmayer T  Li P  Kouveliotou C  Woods P  van Paradijs J  Murakami T  Hartmann D  Smith I  Ando M  Yoshida A  Sugizaki M 《The Astrophysical journal》2000,528(1):L21-L23

We present a 2-10 keV ASCA observation of the field around the soft gamma repeater SGR 1627-41. A quiescent X-ray source, whose position is consistent both with that of a recently discovered BeppoSAX X-ray source and with the Interplanetary Network localization for this soft gamma repeater, was detected in this observation. In 2-10 keV X-rays, the spectrum of the X-ray source may be fit equally well by a power-law, blackbody, or bremsstrahlung function, with unabsorbed flux approximately 5x10-12 ergs cm-2 s-1. We do not confirm a continuation of a fading trend in the flux, and we find no evidence for periodicity, both of which were noted in the earlier BeppoSAX observations.  相似文献