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排序方式: 共有181条查询结果,搜索用时 15 毫秒
11.
Li Zhonghua Su Youjing and Liu ZhuyinSeismological Bureau of Yunnan Province Kunming China 《中国地震研究》1998,(4)
Results of analysis of variation of cross fault short-baseline and short-range leveling in Western Yunnan Earthquake Test Site (WYETS), results show that among five observation stations of cross fault short-baseline and short-range leveling in WYETS before the Lijiang MS7.0 Earthquake occurred in February 1996 only Yongsheng observation station (epicentral distance 82 km) located at Chenghai fault shows great variation about one year before the earthquake. And the nearest observation station, Lijiang (epicentral distance 42 km); presents great coseismic variation, but does not show obvious anomalous variation before the earthquake. There are no significant variations related to the earthquake at the other three observation stations. Two methods are used in analysis of the observed data and some valuable results have been obtained. 相似文献
12.
Burst strain disturbance—A new test study on fracture precursor 总被引:1,自引:0,他引:1
ZHAO YONG XU ) RUN HAI YANG ) BIN WANG ) JIN MING ZHAO ) YU FENG YAO ) PEI ZHONG HUA ) SHI RONG MEI ) ) Seismological Bureau of Yunnan Province Kunming China ) Center for Analysi 《地震学报(英文版)》1998,(6)
IntroductionBeforeanearthquakeocuurs,deformationvariationsobviouslyappearinseismogenicareaandnearbywhichwerereportedalot.Earl... 相似文献
13.
含硬包体试样在破裂孕育过程中波速场的变化 总被引:2,自引:2,他引:0
含硬包体混凝土试样在底面支撑侧面双轴加压至主破裂的情况下波速场的变化图象为:加压初期,试样上的纵波平均速度在4175~4615m/s之间变化,随着压力升高,出现小于4175m/s的低速区,但范围甚小,位置在两个包体之间。随后出现大于4615m/s的高速区,范围大致与包体位置一致。随着σ1的增加,低速区在逐渐变大,高速区逐步减小后又重新变大,高速区与低速区在平面上相互重叠,在空间上看,高速区被低速区包围着。临近主破裂时,低速区变小并逐步形成条带,高速区也变小,主要集中在靠近未来出现破裂的一个包体位置上。最终的破裂面出现在此高速区与低速条带交界附近,包体也局部破裂了。 相似文献
14.
15.
Lithospheric Geothermal Structure in Yunnan, China 总被引:2,自引:0,他引:2
Zhou Zhenheng Xiang Caiying and Deng WanmingSeismological Bureau of Yunnan Province Kunming China Institute of Geology Chinese Academy of Sciences Beijing China 《中国地震研究》1998,(1)
In this paper,the characteristics of the lateral variations of the deep heat flow and Hthospheric geotemperature distribution in Yunnan have been studied,and the lithospheric geothermal structure has been divided into three types,i.e.the geothermal structure in the typical modern tectonically active region,transitional geological region and stable geological region.Finally,the relationship between the geotherm and seismicitv has been discussed. 相似文献
16.
山东省平邑县王家村金矿化体赋存于寒武纪地层与顺层侵入的二长斑岩接触部位,为鲁西铜石地区又一新类型金矿,找矿前景良好。传统方法估算矿化体的资源量效果不佳,该文借助Surpac软件工具,在研究王家村金矿(化)体地质特征的基础上,根据矿床以往的地质勘查工程资料,首次建立了王家村矿床地质数据库,构建了矿区的三维可视化地质模型,模型形象直观的展现了矿区地形地貌、矿体展布位置及形态。并应用距离幂次反比法对矿体进行了资源量估算。用此软件进行资源量估算简便且准确,可以根据不同品位实现资源量的动态统计分析。 相似文献
17.
18.
Xiang-Jun Lai Yan Li National Astronomical Observatories/ Yunnan Observatory Chinese Academy of Sciences Kunming China Key Laboratory for the Structure Evolution of Celestial Objects China Graduate University of Chinese Academy of Sciences Beijing China. 《中国天文和天体物理学报》2011,(10)
Based on the turbulent convection model (TCM) of Li & Yang, we have studied the characteristics of turbulent convection in the envelopes of 2 and 5M⊙ stars at the red giant branch and asymptotic giant branch phases. The TCM has been successfully applied over the entire convective envelopes, including the convective unstable zone and the overshooting regions. We find that the convective motions become progressively stronger when the stellar models are located farther up along the Hayashi line. In the convect... 相似文献
19.
Xi-Liang Zhang Zhong Liu National Astronomical Observatories/ Yunnan Observatory Joint Laboratory for Optical Astronomy Chinese Academy of Sciences Kunming China Graduate University of Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2011,(10)
Mutual events between natural satellites include mutual occultation and mutual eclipse. Mutual eclipse is another kind of mutual occultation as viewed from the center of the Sun instead of the Earth. Two mutual eclipses of J2 Europa by J1 Io (2009 Aug. 28 and Sept. 12) were observed at Yunnan Observatory during the PHEMU09 international campaign. We will calculate the astrometric data of these Galilean satellites by analyzing and fitting the light curves we obtained. The limb-darkening was considered during... 相似文献
20.
Yuan Ma De-Yu Wang Jun Lin Shuo Dai Xue-Fei Zhang National Astronomical Observatories of China / Yunnan Astronomical Observatory Chinese Academy of Sciences Kunming China Purple Mountain Observatory Nanjing China Harvard-Smithsonian Center for Astrophysics Cambridge MA USA 《中国天文和天体物理学报》2010,10(5)
We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed in the period from July 2000 to March2005.In total,we investigated 395 decimetric type Ⅲ radio burst events,21% of which showed apparent correlation to CMEs that were associated with Hα flares.We noticed that the Hα flares which were strongly associated with CMEs were gradual events,and82% of them took place before CMEs appeared in the field of view of LASCO C2;that most of the CME-associated radio bursts started in the frequency range around750 MHz with a frequency drifting rate of several hundred MHz s-1,of which both positive and negative ones were recognized; and that the correlation of type Ⅲ radio bursts to CMEs without associated flares is fairly vague,less than 9%. 相似文献