济南东部埠村超单元及其就位机制

分布于济南东部六山圈—大有一带的侵入岩,为燕山早期同一岩浆热事件多次侵入形成的杂岩体,依其形成顺序可划分为山张庄、西杜、大有、赵家鹊山四个单元,归并为埠村超单元。该超单元的形成与幔源基性岩浆上侵及同源岩浆分异产生的中偏基性—中性岩浆多次侵入有关,属热气球式膨胀与火山口塌陷复合就位机制。     

内蒙古乌达地区早二叠世早期植物群

通过对内蒙古乌达地区早二叠世早期山西组植物化石进行研究,共鉴定出植物化石７属１１种,即Ｔｉｎｇｉａｃａｒｂｏｎｉｃａ（Ｓｃｈｅｎｋ）Ｈａｌｅ,ＴｐａｒｔｉｔａＨａｌｅ,ＰｌａｇｉｏｚａｍｉｔｅｓｃｆｏｂｌｏｎｇｉｆｏｌｉｕｓＨａｌｅ,ＳｐｈｅｎｏｐｔｅｒｉｓｎｏｒｉｎｉＨａｌｅ,ＳｎｙｓｔｒｏｅｍｉＳｚｅ,ＳｔｅｎｕｉｓＳｃｈｅｎｋ,ＰｅｃｏｐｔｅｒｉｓａｎｄｅｒｓｏｎｉＨａｌｅ,ＰｌａｔｉｖｅｎｏｓａＨａｌｅ,Ｔａｅｎｉｏｐｔｅｒｉｓｓｐ,Ｃａｕｌｏｐｔｅｒｉｓｓｐ,ＰｔｅｒｏｐｈｙｌｕｍｄａｉｈｏｅｎｓｅＫａｗａｓａｋｉ。研究结果表明,这些植物化石均为华夏型分子,可以和华夏植物区的一些同期植物群进行对比。根据植物群的总体组成,该区山西组植物群的地质时代属于早二叠世早期,大致相当于阿谢尔期（Ａｓｅｌｉａｎ）至萨克马尔期（Ｓａｋｍａｒｉａｎ）。     

The unique nature in ore composition,geological backgroudd and metallogenic mechanism of non-conventional superlarge ore deposits: A preliminary discussion

The new plants documented here, including a representative of the trimerophytesPsilophyton primitiuum sp. nov., a questionable rhyniophyte or trimerophyteHedeia sinica sp. nov., a prelycopodBragwanathia sp. and two species of zosterophyllophytes,Zosterophyllum australianum Lang and Cookson 1930 and2. sp. 1, from the Posongchong Formation of southeastern Yunnan, China, add to the known floral diversity of the Early Devonian of this region. Two sections of the Posongchong Formation, Changputang section of Wenshan district and Gegu section of Mengzi district also are introduced. After comparing the plants with those of the coeval flora of Australia and considering the data of recent paleocontinental reconstructions, the authors suggest that there is a northeastern Gondwana phytogeographic unit during the early Devonian comprising Australia, South China Block and perhaps Shan-Thai Block. The similarity of the floral component between Australia and South China is discussed. Because both Australia and South China also have dominant or endemic taxa, each might be recognized as a subunit, separately characterized byHedeia for Australia andEophyllophyton for South China. Project supported by the National Natural Science Foundation of China (Grant Nos. 49372075 and 49742004)     

四川南部珙县早侏罗世一新蜥脚类恐龙

简介在珙县下侏罗统自流井组东岳庙段中,发现的原始蜥脚类恐龙化石的一新属种石碑珙县龙。成年个体长约１４ｍ。化石材料相当丰富,除头骨不完全外,其他部分乃至全部均保存完好。它是早期的原始的蜥脚类,但又和蜥脚类有不少共同点。它对研究蜥脚类的起源和进化,具有重要意义     

河北尚义侏罗系后城组节理研究

研究区侏罗系后城组地层发育着多组节理,根据其方位及相互关系,自早到晚分为５个节理组,其定向分别为１７４°、７７°、５８°、１４５°和１１９°,反映出节理形成的最大主压应力方向交替变化和偏转。岩石应变强度具有由弱至强,再由强至弱的演化趋势,而节理型式趋向不规则。区内节理多属构造成因,推测形成于侏罗纪末至白垩纪初近南北向的区域挤压过程。热液活动在区内节理形成之后,而后１１９°方位节理组发生右行走滑。     

Clustering of galaxies at high redshifts

Recent observations show a large concentration of galaxies at high redshift. At first sight, strong clustering of galaxies at high redshifts seems to be in contradiction with the models of structure formation. In this paper we show that such structures are a manifestation of the strong clustering of rare peaks in the density field. We compute the frequency of occurrence of such large concentrations of galaxies in some models of structure formation.     

Natural entropy production in an inflationary model for a polarized vacuum

Though entropy production is forbidden in standard FRW Cosmology, Berman and Som presented a simple inflationary model where entropy production by bulk viscosity, during standard inflation without ad hoc pressure terms can be accommodated with Robertson–Walker’s metric, so the requirement that the early Universe be anisotropic is not essential in order to have entropy growth during inflationary phase, as we show. Entropy also grows due to shear viscosity, for the anisotropic case. The intrinsically inflationary metric that we propose can be thought of as defining a polarized vacuum, and leads directly to the desired effects without the need of introducing extra pressure terms.     

Angular fluctuations in the cosmic microwave background owing to initial perturbations in the radiation temperature

A new method is proposed to account for multiple scattering by electrons in calculations of the correlation functions describing the angular fluctuations in the cosmic microwave background radiation (CMBR). The apparatus of the theory of radiative transport with Rayleigh scattering is used. The problem is reduced to solving an integral equation for the vector source function (dependent only on time), along with differential equations for the other quantities (scalar potentials, baryon velocities, etc.) which show up in the problem. The quantities which describe the angular fluctuations in the CMBR (in the temperature and in the polarization) are then calculated by integrating the vector source function along the line of sight. As an illustration, the correlation functions and power spectra are calculated for the case where the fluctuations are produced by some initial gaussian perturbations of the CMBR. __________ Translated from Astrofizika, Vol. 50, No. 4, pp. 621–631 (November 2007).