The Abundance of QSOs in Various Cold Dark Matter Models

Based on the statistics of the peaks in the random Gaussian field, we put forward a method to model the evolution of quasars, which are assumed to be a phenomenon of the early stages for some massive galaxies. Our calculations show that the cold-hot mixed dark matter model with _h = 0.3 cannot match the observed quasar abundance at redshift z = 4.5, and other prevailing CDM models, such as the mixed dark matter model with _h = 0.2, the tilted CDM models with n = 0.7 or 0.8, and the flat CDM models with = 0.6 or 0.7, are compatible with the observation of the abundance of QSOs on the range of z = 2-5.     

HIGH INPUT IMPEDANCE TRANSISTOR AMPLIFIER FOR ACCELERATION MEASUREMENT

This paper describes a high input impedance preamplifier ,a main amplifier ,including its specification and the circuits theories .An acceleration measurement system consist of the piezoelectric acceleration 、preamplifier、cable 、main amplifier and oscilloscope for measureing the acceleration of vibration due to explosion .The features of the system are :1.good stability ,2.small zero shift ,3.The preamplifier is a new circuit which consists of four transistors 3DG6C,3DG4E. Its input impedance is as high as 1500MΩ and is able to undertake a high instantaneous impulse voltage ,4.There is no power supply set near the preamplifier .The signal transmiting cable is also the power supply cable so that the transmiting characteristic is very well .when the cable length is varied from 1 meter to 1000 meters ,the frequency response of system will not change .The decrement of output amplitude is less than 6% etc.     

A Theoretical and Experimental Investigation of Energy-Containing Scales in the Dynamic Sublayer of Boundary-Layer Flows

The existence of universal power laws at low wavenumbers (K) in the energy spectrum (E_u) of the turbulent longitudinal velocity (u) is examined theoretically and experimentally for the near-neutral atmospheric surface layer. Newly derived power-law solutions to Tchen's approximate integral spectral budget equation are tested for strong- and weak-interaction cases between the mean flow and turbulent vorticity fields. To verify whether these solutions reproduce the measured E_u at low wavenumbers, velocity measurements were collected in the dynamic sublayer of the atmosphere at three sites and in the inner region of a laboratory open channel. The atmospheric surface layer measurements were carried out using triaxial sonic anemometers over tall corn, short grass, and smooth desert-like sandy soil. The open channel measurements were performed using a two-dimensional boundary-layer probe above a smooth stainless steel bed. Comparisons between the proposed analytical solution for E_u, the dimensional analysis by Kader and Yaglom, and the measured Haar wavelet E_u spectra are presented. It is shown that when strong interaction between the mean flow and turbulent vorticity field occurs, wavelet spectra measurements, predictions by the analytical solution, and predictions by the dimensional analysis of Kader-Yaglom (KY) are all in good agreement and confirm the existence of a -1 power law in E_u(= C_uuu² _* K^-1, where C_uu is a constant and u_* is the friction velocity). The normalized upper wavenumber limit of the -1 power law (Kz = 1, where z is the height above the zero-plane displacement) is estimated using two separate approaches and compared to the open channel and atmospheric surface-layer measurements. It is demonstrated that the measured upper wavenumber limit is consistent with Tchen's budget but not with the KY assumptions. The constraints as to whether the mean flow and turbulent vorticity strongly interact are considered using a proposed analysis by Panchev. It is demonstrated that the arguments by Panchev cannot be consistent with surface-layer turbulence. Using dimensional analysis and Heisenberg's turbulent viscosity model, new constraints are proposed. The new constraints agree with the open channel and atmospheric surface-layer measurements, Townsend's inactive eddy motion hypothesis, and the Perry et al. analysis.     

阿拉善高原古湖岸堤释光测年与晚第四纪湖面变化

阿拉善高原位于现代西风环流与东亚季风环流过渡带,该地区分布的湖泊对全球性气候变化响应极为敏感,阿拉善高原广泛分布的古湖岸堤为较准确地重建晚第四纪湖泊水位变化提供了良好载体。近年对黑河、石羊河尾闾湖泊以及吉兰泰盐池、雅布赖盆地等地的古湖岸堤的沉积地层以及石英和钾长石释光测年研究,重建了不同区域较高分辨率的末次间冰期以来湖泊时空演化过程。发现早在300 ka以前阿拉善高原就已经形成了高水位湖泊,黑河尾闾额济纳盆地在MIS 11或更早、MIS 9、MIS 7、MIS 5和MIS 1形成了高湖面湖泊,高湖面湖泊形成存在100 ka的周期。阿拉善高原在末次间冰期及全新世形成了稳定高湖面湖泊,但间冰期内部湖面波动具有空间差异性,东部区域湖泊高湖面出现在MIS 5e~5c和中全新世,西部湖泊高湖面出现在MIS 5a~5c和晚全新世。湖面变化的空间差异性很可能与冰期-间冰期旋回尺度及间冰期内部东亚夏季风与西风气候系统在阿拉善高原的相互作用密切相关。

     

数字增城国土信息化建设的探讨

论述了增城市国土信息化建设的现状及存在的问题,提出了增城市国土综合业务信息系统的总体技术方案,以及主要建设内容和所需解决的关键技术。     

Local isotropy and anisotropy in the sheared and heated atmospheric surface layer

Longitudinal velocity and temperature measurements above a uniform dry lakebed were used to investigate sources of eddy-motion anisotropy within the inertial subrange. Rather than simply test the adequacy of locally isotropic relations, we investigated directly the sources of anisotropy. These sources, in a daytime desert-like climate, include: (1) direct interaction between the large-scale and small-scale eddy motion, and (2) thermal effects on the small-scale eddy motion. In order to explore these two anisotropy sources, we developed statistical measures that are sensitive to such interactions. It was found that the large-scale/small-scale interaction was significant in the inertial subrange up to 3 decades below the production scale, thus reducing the validity of the local isotropy assumption. The anisotropy generated by thermal effects was also significant and comparable in magnitude to the former anisotropy source. However, this thermal anisotropy was opposite in sign and tended to counteract the anisotropy generated by the large-scale/smallscale interaction. The thermal anisotropy was attributed to organized ramp-like patterns in the temperature measurements. The impact of this anisotropy cancellation on the dynamics of inertial subrange eddy motion was also considered. For that purpose, the Kolmogorov-Obukhov structure function equation, as derived from the Navier-Stokes equations for locally isotropic turbulence, was employed. The Kolmogorov-Obukhov structure function equation in conjunction with Obukhov's constant skewness closure hypothesis reproduced the measured second- and third-order structure functions. Obukhov's constant skewness closure scheme, which is also based on the local isotropy assumption, was verified and was found to be in good agreement with the measurements. The accepted 0.4 constant skewness value derived from grid turbulence experiments overestimated our measurements. A suggested 0.26 constant skewness value, which we derived from Kolmogorov's constant, was found to be adequate.     

甘肃北山红石山地区扫子山组构造变形特征及其动力学背景

甘肃北山地区扫子山组形成于早石炭世,是红石山蛇绿构造混杂岩的重要组成部分,记录并保存了红石山古洋盆形成及演化的地质信息,是讨论红石山地区晚古生代古地理环境及洋盆构造属性的重要窗口。详细的野外地质调查发现,该套地层构造变形强烈,原始层理难以辨识,为研究该套地层的沉积环境增添了难度。基于此,在查明扫子山组物质组成的基础上,通过详细的构造解析,厘定其构造序列,并通过剥离后期构造改造,恢复原始沉积层理。结果表明,扫子山组经历了3期构造变形,第1期为北北西—南南东向逆冲兼左行走滑,可能为洋壳向北俯冲的产物;第2期为北北东—南南西向挤压兼右行走滑脆−韧性变形,可能为碰撞阶段的产物;第3期构造变形以北东—南西向左行走滑为主,为次一级的晚期构造变形。变形样式及变质程度表明,扫子山组以中浅层次构造变形为主,地层未发生明显的倒转和缺失,该套地层物质成分及空间分布具有明显的规律性,显示裂谷型盆地向南趋于成熟的火山-沉积特征。 结合红石山−蓬勃山断裂以北发育石炭纪—二叠纪弧岩浆岩,揭示了红石山古洋盆向北俯冲的动力学过程,为进一步研究中亚造山带南缘构造演化过程提供地质依据。     

三峡地区水资源评价

在大量水文资料统计分析的基础上，对三峡地区主要水文要素的时空分布及变化特征、分区水资源的评价和开发利用条件进行了系统分析，可为三峡工程建设提供该地区社会经济发展的科学依据和基本的水文水资源数据。     

内蒙古西乌旗沙尔哈达晚侏罗世A型花岗岩：地球化学特征、岩石成因与动力学背景

内蒙古西乌旗沙尔哈达花岗岩侵入于贺根山缝合带蛇绿岩中。LA-ICP-MS锆石测年指示,沙尔哈达花岗岩岩株于晚侏罗世(154.6±1.2 Ma)侵位,矿物组合以石英、碱性长石和斜长石为主,富SiO2(74.86%~75.97%)、K2O(4.4%~4.95%),贫MgO(0.044%~0.22%)、CaO(0.38%~0.77%)、TiO2(0.046%~0.18%)和P2O5(0.007%~0.042%),A/CNK=1.03~1.09, 小于1.1,强烈亏损Ba、Sr、Eu、P、Ti,具有典型的右倾“海鸥型”稀土元素分配模式,表现出典型的铝质A型花岗岩的矿物组合及地球化学特征。沙尔哈达A型花岗岩具有低的(87Sr/86Sr)i值(0.7014~0.70374)、低正εNd(t)值(+3.96~+4.31)、高的εHf(t)值(+10.54~+14.72)。同位素地球化学特征指示,沙尔哈达花岗岩可能源于新生的中基性地壳物质部分熔融及其后的结晶分异作用。沙尔哈达A型花岗岩为晚侏罗世蒙古-鄂霍茨克洋闭合后造山伸展作用的产物,和蒙古-华北北部地块散布的其他A型花岗岩共同指示中晚侏罗世广泛的中下地壳伸展。