Energy Of The Universe In Bianchi-Type I Models In MØLler’S Tetrad Theory Of Gravity

In this paper, using the energy definition in MØller’s tetrad theory of gravity we calculate the total energy of the universe in Bianchi-type I cosmological models which includes both the matter and gravitational fields. The total energy is found to be zero and this result agrees with a previous works of Banerjee and Sen who investigated this problem using the general relativity version of the Einstein energy-momentum complex and Xulu who investigated same problem using the general relativity versions of the Landau and lifshitz, Papapetrou and Weinberg’s energy-momentum complexes. The result that total energy of the universe in Bianchi-type I universes is zero supports the viewpoint of Tryon.     

IGS事后精密星历产品不连续性分析及处理方法

IGS的事后精密钟差产品采取以天为单位的数据处理策略这导致在天与天之间的交界处卫星的钟差基准不连续 对需要进行跨天数据处理的精密单点定位用户会发生基准跳跃的卫星模糊度在交界历元处不连贯这无异于产生了一个无法修复的非整周的周跳使得滤波需要重新收敛 详细分析了30d每颗卫星跳跃的量级以及对精密单点定位用户的影响在详细阐述IGS钟差解算策略的基础上分析了产生这种不连续性的原因并提出了两种应对策略 在IGS精密钟差产品中加入钟差基准跳跃信息供用户使用 将钟差基准在多天连续估计 最后给出了这两种策略的数据处理结果验证了两种方法的有效性.     

Accuracy analysis, dem generation and validation using russian tk-350 stereo-images

TK-350 stereo-scenes of the Zonguldak testfield in the north-west of Turkey have been analysed. The imagery had a base-to-height ratio of 0·52 and covered an area of 200 km × 300 km, with each pixel representing 10 m on the ground. Control points digitised from 1:25 000 scale topographic maps were used in the test. A bundle orientation was executed using the University of Hanover program BLUH and PCI Geomatica OrthoEngine AE software packages. Tests revealed that TK-350 stereo-images can yield 3D geopositioning to an accuracy of about 10 m in planimetry and 17 m in height. A 40 m resolution digital elevation model (DEM) was generated by the PCI system and compared against a reference DEM, which was derived from digitised contour lines provided by 1:25 000 scale topographic maps. This comparison showed that accuracy depends mainly on the surface structure and the slope of the local terrain. Root mean square errors in height were found to be about 27 and 39 m outside and inside forested areas, respectively. The matched DEM demonstrated a systematic shift against the reference DEM visible as an asymmetric shift in the frequency distribution. This is perhaps caused by the presence of vegetation and buildings.     

Turning points in black holes astrophysics

Black hole astrophysics is expected to have a major breakthrough any day. Theoretical understanding is well advanced, so the breakthrough has to come from observers. Conclusive and direct evidence of event horizons, signatures of tidal deformation of gas clouds (and eventual disappearance of matter behind horizons) could be obtained in matter of months. At this juncture, we wish to summarize how the subject came to this stage and what is the state-of-the-art flow solution around a black hole. We touch upon the most crucial issue of (un)predictability of this subject. We believe that if viscosity is roughly what MRI simulations are pointing to us, we still require very detailed knowledge of properties of the companion, especially time dependent mass transfer from the companion to the black hole.     

山东东营凹陷古近系碎屑岩储层特征及控制因素

通过对大量储层物性数据的分析和整理,结合薄片观察和扫描电镜分析结果,研究了不同构造背景、不同沉积类型及不同埋深的储层物性特征及其控制因素。东营凹陷近系碎屑岩储层类型多样,大多形成在冲积扇-河流、扇三角洲、近岸水下扇、深水浊积扇、三角洲前缘滑塌浊积扇以及滨浅湖滩坝等多种沉积环境中。碎屑岩储层类型主要包括砾岩、含砾砂岩、中粗砂岩、细砂岩及粉砂岩。其中中砂岩和细砂岩是最好的储层。但是不同地区、不同类型储层物性存在较大的差异。物性最好的储层为河道、（扇）三角洲前缘水下分流河道及河口坝砂体。在相同深度条件下,中央隆起带的物性最好,北部和南部次之。另外,本区随埋藏深度增加,碎屑岩储层物性逐渐变差（剔除次生孔隙的影响）。根据碎屑岩储层物性差异性分析和储层成岩演化研究结果,其储层物性主要受压实作用、碳酸盐溶蚀与胶结作用及沉积条件四大因素控制,其中压实作用、溶蚀作用及胶结作用是主要控制因素,而沉积条件对物性的影响主要表现在控制原生孔隙的发育程度,并进一步控制溶蚀、胶结等成岩作用。     

准噶尔盆地西北缘侏罗系储层

准噶尔盆地西北缘侏罗系陆相碎屑岩储层的岩性差异较大，岩性对物性的控制作用明显。储层的孔隙类型多样，不同类型的孔隙在发育规模、丰度及有效性方面都存在显差异，次生溶蚀孔隙、原生粒间孔隙和残余粒间孔隙是最重要的有效孔隙类型。储层渗透率与孔隙度之间存在较好的半对数相关关系。通过设置一定的孔隙度和渗透率参数界线，对储层储集性能进行评价，将侏罗系储层的孔渗性能划分为5个级别，可与当前流行的砂岩储层孔渗性能分级相对应。通过对大量压汞参数样本的聚类分析，将储层的孔隙结构划分为4个类型。通过各类参数统计及曲线形态对比，对孔隙结构类型进行了定量结合定性的优劣评价。最后，结合孔渗性能级别、储集空间类型、孔隙结构类型、岩性等特征，对准噶尔盆地西北缘侏罗系储层进行了综合分类评价。     

Energy–Momentum In The Viscous Kasner-Type Universe In Teleparallel Gravity

Using the teleparallel gravity versions of the Einstein and Landau–Lifshitz’s energy and/or momentum complexes, I obtain the energy and momentum of the universe in viscous Kasner-type cosmological models. The energy and momentum components (due to matter plus field) are found to be zero and this agree with a previous work of Rosen and Johri et al., who investigated the problem of the energy in Friedmann–Robertson–Walker (FRW) universe. The result that the total energy and momentum components of the universe in these models is zero same as Bergmann–Thomson’s energy–momentum and props the viewpoint of Tryon. Rosen found that the energy of the FRW space–time is zero, which agrees with the studies of Tryon. PACs Numbers: 04.20.-q; 04.50.+h An erratum to this article is available at .     

绵竹三箭水S1井温泉补给源的同位素示踪研究

根据绵竹三箭水S1井相关地质区域内各水体的氢、氧同位素组成和放射性同位素氚浓度,结合该区的地质背景,利用同位素示踪手段,基本确定该井温泉地下水的成因为大气降水渗入补给主体含水层补给源在西北部1700m左右的“彭灌杂岩”高山区一带、补给量相对稳定,水温不会有大波动,有远期开发价值。     

The Gaojiacun Mafic-Ultramafic Complex （Sichuan, SW China）：Neoproterozoic Magmatic Activity at the Western Margin of the Yangtze Craton

1 Introduction The Gaojiacun intrusive complex is one of the numerous ultramafic-mafic intrusions in Sichuan Province of China. It was mapped during the 1970s and studied mainly by Chinese scientists (e.g. Geological Team 106, 1975; Shen et al., 1986, 1989; CGGJC, 1986; Yang et al., 1993; Li et al., 1995; Shen et al., 2003; Zhu et al., 2004a). Since the year 2000, China has become one of the largest PGE consumers. While the country can produce only less than 1 ton PGE/year, the Chin…     

Large-scale distribution of magnetic fields,green corona and prominences during an extended activity cycle

The interrelations of the latitudinal distribution of the coronal green emission maxima, maximal numbers and areas of prominences, magnetic fields, sunspots, and polar faculae in the 20th and 21st sunspot cycles have been investigated. It is again demonstrated how the behaviour of all studied data depends on their heliographic latitude. In the polar zone, well separated from the equatorial we observe following polarity magnetic fields transported only polewards, while the equatorial zone is occupied mostly by leading polarity fields, developed there, moving equatorwards, and crossing the equator to the other hemisphere with the new cycle during the minimum of sunspot activity.This magnetic field distribution is well emphasized by the places of maximal occurrence of prominences and by the distribution of coronal green emission maxima which also differ in dependence on latitude.The question of identifying the first and last evolutionary stages of an extended cycle of activity is discussed and the existence of a magnetic activity cycle lasting 15–17 years is suggested.