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1.
Introduction Earthquake magnitude is the most common measure of an earthquake′s size,and is one of the basic parameters of an earthquake.There are three most familiar scales of earthquake magnitude:ML(local earthquake magnitude),MS(surface wave magnitude)and mB/mb(body wave magni-tude).Richter(1935)introduced ML when studying earthquakes in Southern California.In1945,Gutenberg(1945a)put forward surface wave magnitude scale to determine earthquake magnitude(MS)using surface waves(20s)of s… 相似文献
2.
Nicolas Thomas 《紫金山天文台台刊》1996,(3)
Amajor objective of the Infrared Space Observatory (ISO) is the determination of the sized and albedoes of several objects in the "Kuiper disc".The method by which this will be achieved is described.It is shown that the unknown shapes and surface thermal properties proviede additional complications to the interpretation of ISO data.The requirement for ground-based measurements of the visual light curves of these objects is demonstrated and the implications of the results of the ISO observ Vations is discussed. 相似文献
3.
Chongjiang DU Dr. Institute for Hydraulic Structures Agricultural Engineering University of Karlsruhe Kaiserstr. D- Karlsruhe Germany Franz NESTMANN Prof Dr. Institute for Hydraulic Structures Agricultural Engineering University of 《国际泥沙研究》1997,(3)
LINTRODUCTIONTerrainmodellingisatermtodescribetheprocessofrepresentingthesurfaceoftheEarth.Mathemahcally,theproblemcanbedescribedas;Givenasetofn(3sn相似文献
4.
Geochemical Characteristics of a Veinlet Kupferschiefer Profile from the Lubin Mine, Southwestern Poland 总被引:3,自引:0,他引:3
Previous studies have shown that the ascending, oxidizing brines play a very important role in Kupferschiefer mineralization. Fractures could be the pathway of the brines. In order to clarify the influences of the brines on bulk organic matter, aromatic hydrocarbons and Kupferschiefer mineralization, one veinlet Kupferschiefer profile from the Lubin mine, southwestern Poland was studied with the microscopic, geochemical and Rock-Eval methods. The microscopic results indicate that organic matter of the veinlet sample consists dominantly of bitumen. Its extract content is higher than in other samples. The dominant aromatic compounds are naphthalene and alkylated naphthalenes (Na-PAH), which have migrated into the veinlet sample from other sediments. The content of phenanthrene and its methylated derivatives (Ph-PAH) is much lower than in other samples. The reason may be due to their heavier mass than Na-PAH. It is more difficult for Ph-PAH to migrate. The Na-PAH was probably removed from the shale by dist 相似文献
5.
Rapid afterslip and short-term viscoelastic relaxation following the 2008 M_W7.9 Wenchuan earthquake
Zhigang Shao Rongjiang Wang Yanqiang Wu Langping Zhang Institute of Earthquake Science China Earthquake Administration Beijing China GFZ German Research Center for Geosciences D- Potsdam Germany 《地震学报(英文版)》2011,(2):163-175
Significant postseismic deformation of the 2008 M W 7.9 Wenchuan earthquake has been observed from GPS data of the first 14 days after the earthquake. The possible mechanisms for the rapid postseismic deformation are assumed to be afterslip on the earthquake rupture plane and viscoelastic relaxation of coseismiclly stress change in the lower crust or upper mantle. We firstly use the constrained least squares method to find an afterslip model which can fit the GPS data best. The afterslip model can explain n... 相似文献
6.
WU Zhenhan JIANG Wan Peter Blisniuk BI Siwen ZHANG Shukun Olaf Kuchel MAO Yi Institute of Geomechanics CAGS Minzu Xueyuan Nanlu Beijing Institut fur Geowissenschaften Universitat Potsdam Postfach D- Potsdam Germany Liu Xinzhu 《《地质学报》英文版》1999,73(3):289-293
The Shuanghu basin is a NE-trending rift basin bounded by NE-striking normal faults and NW-striking shear-extensional faults of the northern Tibetan Plateau. Four samples from calcite veins in marginal faults and one sample from mudstone (S-3) were collected for dating the evolution of the Shuanghu basin by using the ESR spectrograph of EXM-type. Ages were calculated according to the close-equilibrium model on the basis of the measured ESR signal spectra of samples, providing good chronological information. It is known from the ESR dating that the extensional faulting and rifting of the Shuanghu area began at 4.92 Ma B.P., followed by regional folding in 3.56-1.36 Ma, NW-striking faulting in 0.60 Ma and normal faulting in 0.024 Ma in the Shuanghu basin. 相似文献
7.
Stephan Schaal 《东北亚地学研究》2005,(Z1)
The paper reports sunthetically the Cocene fauna of the Messel Pit Fossil site of Germany, in detail, including its rich taxanomic compositions, geological and paleogeographic backgroud, and the studying and applying history. 相似文献
8.
Matthias Schmidt 《山地科学学报》2005,2(2)
IntroductionThe mountain forests of South Kyrgyzstan have a long history of human influence. The political and socio-economic conditions prevailing in the region have changed dramatically several times over the last century and have played animportant role in forest policy, management and use. To highlight the human-environment relationship, I have chosen here to use a political ecology approach as conceptual framework (cf. Bryant & Bailey 1997, Bryant 1998, Blaikie 1999). In this approach,… 相似文献
9.
本文利用 EISCAT-Svalbard 雷达1999年3月至2003年2月期间观测数据,对太阳活动高年前后极区电离层 F 区电子密度随高度和地方时的二维分布进行统计分析,研究极隙/极盖区背景电离层特征,并与 IRI-2001模式预测结果进行比较。分析结果表明,在 ESR 雷达所在纬度,不存在“冬季异常”现象;但首次发现,此处电离层冬季日变化存在磁午夜前主极大。另外,无论在什么季节,白天时段 ESR 雷达上空电子密度都在磁正午附近有一极大值。与 IRI 模式的比较表明,模式预测的 F 区电子密度与 ESR 实测结果存在较大偏差,在500km 高度以上的顶部电离层和冬季,差别尤其明显。简要讨论了软粒子沉降对造成电子密度日变化磁正午极大的作用和冬季磁午夜前主极大的形成机理。 相似文献
10.
We report results of our optical photometric observations of ten gamma-ray loud blazers, namely: 0219+428 (3C66A), PKS 0420-014 (OA 129), S5 0716+714, 0754+100 (OI 090.4), 0827+243 (OJ248), 1652+398 (Mrk 501), 2200+420 (BL Lacertae), 2230+114 (CTA 102), 2251+158 (3C 454.3) and 2344+514. The observations were carried out in September-October, 2000 using the 70 cm optical telescope at Abstumani Observatory, Georgia. We found intra-day variations in 0420-014, S5 0716+714, BL Lacertae and CTA 102. A variation of 0.3 magnitude over a time scale of about 3 hours was observed in the R passband in BL Lacertae on JD 2451827. We did not detect any variation in 3C 66A, Mrk 501, or 3C 454.3 during our observations. Nor did we detect any clear evidence of variation in 1ES 2344+514 during our two weeks' observing run of the TeV gamma-ray source. 相似文献