利用背景噪声的分形方法监控台站观测系统运行状态

使用全国23个国家测震台站和17个实验台站地震计记录的背景噪声数据,研究特定尺度(限定频带内)的背景噪声特性,分析利用分形方法监测台站观测系统运行状态的可行性.结果 表明,分形方法具有较强的时域性,定量化程度高、抗干扰能力强,基本不受观测系统参数约束,可用于台站观测系统运行状态检测,减少正常记录瞬间中断和引入人为干扰的...     

华北定点形变的小波分析与地震活动研究

利用小波分析方法对华北地区１９９０ 年到１９９８ 年的多台定点形变观测资料进行了分析计算,并将计算结果与该地区的地震活动进行了对比分析,同时讨论了不同阶的小波分解结果的物理意义及其与地震之间的对应关系。认为小波分解本质是窗口加权滑动平均,能有效地对各种不同频率成分的形变按不同的频段分离,为识别地震形变异常提供一种新的手段。在空间分布上,地形变的变化幅度与地震活动强度相对应,即在华北西北部地震活动性较强的包头、张家口一带,台站形变的强度明显高于华北东南部地震活动性较弱的泰安、营口等地区。在时间分布上,张北ＭＬ６ ．２ 级地震前大约两年东西方向的形变振幅随时间变化明显加大。     

Physical geographical background of the culture of traditional Chinese residential architecture

ThetheSisistoexplainthebasicfactorsreferringtothetraditionalChineseresidentialarchitecturebasicallyfinalizedintheMingandQingdynastiesinthecountry'sspecificphysicalenvironment.Restrainedbyaxialfactors,itadaptsitselftotheself-sufficientnatural~nomy.Itisfiexiblydesigned,rsoablyfunctioned,economicallyconstructedandfeaturedbyremarkablelocalcharacteristics.IINFLUENCEOFCLIMATEONTRADITIONalarSIOCNTIAnANCnITh~arNinetyPercentofChina'spopulationinhabitstheeasternareawithinthedemarcati…     

鲁西南聊考断裂带地震危险性评价与活动性分布

利用1970年以来沿聊考断裂带及周边50 km范围内的地震数据,结合历史强震与现今地震活动背景,分别运用最大似然法和最小二乘法对研究区进行b值计算,圈出高应力累积区,并借助时间相依的地震潜势概率评估方法以及地震活动性分布,得出以下结论：1）南段的范县、清丰、濮阳以及鄄城地区的b值维持在0.6～07之间,属于高应力积累区;2）未来50 a内南段危险性较高,100 a内整条断裂发生M5.0～6.0地震的可能性较大;3）地震活动主要集中在115.2°～115.6°E、34.9°～36°N区域内,且自2000年后地震活动性变强。     

STUDIES ON ENVIRONMENTAL BACKGROUND VALUES IN CHINA

An investigation on environmental background values was made in an area of about 1,140,000 km2, which included temperate and subtropical zones of China. The environmental background values of 142 soil environment units, 18 main soil types, 87 surface water environment units, 8 aquatic organism environment units and 20 underground water environment units were obtained. The rules, causes and effecting factors of regional differentiation of the environmental background values were deduced from over 200,000 various data.     

Cosmic microwave background polarization due to scattering in clusters

Scattering of the cosmic microwave background (CMB) in clusters of galaxies polarizes the radiation. We explore several polarization components which have their origin in the kinematic quadrupole moments induced by the motion of the scattering electrons, either directed or random. Polarization levels and patterns are determined in a cluster simulated by the hydrodynamical enzo code. We find that polarization signals can be as high as  ∼1 μK  , a level that may be detectable by upcoming CMB experiments.     

Can the unresolved X-ray background be explained by the emission from the optically-detected faint galaxies of the GOODS project?

The emission from individual X-ray sources in the Chandra Deep Fields and XMM – Newton Lockman Hole shows that almost half of the hard X-ray background above 6 keV is unresolved and implies the existence of a missing population of heavily obscured active galactic nuclei (AGN). We have stacked the 0.5–8 keV X-ray emission from optical sources in the Great Observatories Origins Deep Survey (GOODS; which covers the Chandra Deep Fields) to determine whether these galaxies, which are individually undetected in X-rays, are hosting the hypothesized missing AGN. In the 0.5–6 keV energy range, the stacked-source emission corresponds to the remaining 10–20 per cent of the total background – the fraction that has not been resolved by Chandra . The spectrum of the stacked emission is consistent with starburst activity or weak AGN emission. In the 6–8 keV band, we find that upper limits to the stacked X-ray intensity from the GOODS galaxies are consistent with the ∼40 per cent of the total background that remains unresolved, but further selection refinement is required to identify the X-ray sources and confirm their contribution.