天灾研究中的当代物理新途径   总被引：2，自引：1，他引：1  

胡辉  张世杰 《云南天文台台刊》2001,(1):58-62

应用当代物理学中的量子化方法，将日－地空间量子化。借天体分层结构特征，对地震震级公式及天体引潮力激起的孤波储能触发地震的原理作了探索性讨论。  相似文献   

流动VLBI站氢原子钟的研制与性能测试     

张为群  林传富  于双林  张一平  王关忠  张健  杨佩红 《天文学报》2001,42(1):94-100

氢脉泽是射电天文所必需的频率标准.文中对为流动vLBI站研制的新一代氢脉泽的物理结构特点进行了讨论，包括对腔泡结构、磁屏蔽、原子束光学系统等.同时性能测试表明在80秒到1天之间频率稳定度优于1×10  相似文献   

优化发电能源结构的初探   总被引：1，自引：0，他引：1  

程地卫 《成都信息工程学院学报》2001,16(1):41-45

从我国电力工业发展的角度，浅析了国内外发电能源结构及其变化趋势，作者认为优化我国发电能源结构、采取必要的技术措施，是实现我国电力 工业可持续发的重要途径。  相似文献   

广州白云山常绿阔叶林的结构特征   总被引：2，自引：0，他引：2  

何冰  尹爱国等 《广东海洋大学学报》2001,21(3):48-53

在线路调查和样方调查的基础上分析了广州白云山常绿阔叶林的结构特征，群落主要由亚热带科属组成，优势科为芸香科，五加科，茜草科，山茶科，壳斗科，鼠刺科，樟科等。优势树种也以相应的优势科属树种为主，群落中胸径≥3cm的个体密度较小，只有1964株/hm^2；群落较为低矮，平均高度只有6m；乔木垂直分化不明显，树种水平分布不均，白云山的植被是次生植被和人工造林改造的结果，只在山谷少数植被没受人类干扰，其现状植被是天然次生植被和人工植被的混合体，在一些由马尾松发展起来的群落，天然侵入的阔叶树种已在主要层中居优势；群落中可见马尾松衰退的痕迹。  相似文献   

断层相关褶皱理论在准噶尔盆地南缘山前带构造研究的应用   总被引：8，自引：4，他引：4  

邵雨  陈伟  张伯友 《地球科学与环境学报》2005,27(1):26-29

利用断层相关褶皱的构造几何分析方法，对准噶尔盆地南缘山前复杂构造带内基于地震剖面进行了构造解析，搭建了中、东段的构造轮廓和构造组合样式，认为东段阜康断裂带主要表现为至地表的推覆逆掩。由于位移量大部分转移至地表，阜康断裂带的前陆部分无喜山期构造带；西段造山带内的挤压往前陆方向传递过程中以前列式不断释放其位移量，造成在纵向上呈现三排主要的断层相关褶皱带。根据正演平衡地质剖面制作技术对山前复杂构造区地震剖面反射波的构造识别进行了模拟与探讨。  相似文献   

Rhombic Cell Analysis. Ⅱ. Application to the IRAS／PSCz Catalogue     

Tao Kiang  Yong-Feng Wu  Xing-Fen Zhu Dunsink Observatory Dublin Institute for Advanced Studies Dublin Ireland Center for Astrophysics  University of Science  Technology of China  Hefei 《中国天文和天体物理学报》2004,4(3):209-220

Rhombic cell analysis as outlined in the first paper of the present seriesis applied to samples of varying depths and liming luminosities of the IRAS/PSCzCatalogue. Numerical indices are introduced to summarize essential information.Because of the discrete nature of the analysis and of the space distribution of galax-ies, the indices for a given sample must be regarded as each having an irreduciblescatter. Despite the scatter, the mean indices show remarkable variations acrossthe samples. The underlying factor for the variations is shown to be the limitingluminosity rather than the sampling depth. As samples of more and more luminousgalaxies are considered over a range of some 2.5 magnitudes (a factor of some 75in space density), the morphology of the filled and empty regions defined by thegalaxies degrades steadily towards insignificance, and the degrading is faster for thefilled than the empty region.  相似文献   

黑宝山─木耳气煤盆地含煤建造的垂向层序与旋回特征     

王喜臣  白昶生 《黑龙江地质》1992,3(4):32-37

  相似文献   

广东,海南土壤中微量元素的迁移累积及剖面分布特点     

李小彬  潘树荣 《热带地理》1991,11(1):62-70

  相似文献   

结构计算的地震荷载模型     

д.  ВМ 李锟 《世界地震工程》1989,(1):50-52,58

  相似文献   

VERTICAL PROFII,ES OF CHL-A AND PRIMARY PRODUCTIVITY IN THE MIDDLE CONTINENTAL SHELF AREA AND EDDY AREA OF THE EAST CHINA SEA     

Wu Yu-lin  Zhou Cheng-xu  Zhang Yong-shan 《中国海洋湖沼学报》2002,20(1):74-80

Vertical profiles of chl-a and primary productivity in the middle continental shelf area and eddy area of the East China Sea were studied using data from a cruise in the East China Sea in February to March, 1997 and a cruise in July, 1998. The results showed that chl-a vertical distribution closely related to in situ hydrological and nutrient conditions. Chla-a concentration ranged from 0.22 to 0.35 mg/m³ and 0.93–1.09 mg/m³ in the eddy area and in the middle continental shelf area, respectively. In both areas, chl-a concentrations in deep layers were slightly higher than those in shallow layers, but was of the same order of magnitude. In summer, when a thermocline existed in the water column, highest chl-a concentrations appeared at the base of the thermocline layers in both areas. In the eddy area, chl-a concentration maximized at 31.743 mg/m³, and averaged 1.143 mg/m³ below 30 m depth. In the middle continental shelf area, the highest chl-a concentration was 2.120 mg/m³, the average was 1.168 mg/m³. The primary productivity reached 1418.76 mgC/(m²·d) in summer and 1360.69 mgC/(m²·d) in winter. In the eddy area, the primary productivity was 787.50 mgC/(m²·d) in summer and 159.04 mgC/(m²·d) in winter. Vertical carbon sinking rate from the deep layer to the bottom in both areas is also discussed in this paper. Contribution NO. 4183 from the Institute of Oceanology, Chinese Academy of Sciences. Project No. 49636210 supported by NSFC.  相似文献