内蒙古乌达地区早二叠世早期植物群   总被引：7，自引：2，他引：5  

孙克勤  张周良 《现代地质》1998,12(4):586-590

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）。  相似文献   

The unique nature in ore composition,geological backgroudd and metallogenic mechanism of non-conventional superlarge ore deposits: A preliminary discussion   总被引：3，自引：0，他引：3  

Guangzhi Tu 《中国科学D辑(英文版)》1998,41(1):1-13

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)  相似文献   

Gamma-ray bursts from stellar remnants: probing the Universe at high redshift     

Ralph A. M. J. Wijers  Joshua S. Bloom  Jasjeet S. Bagla  & Priyamvada Natarajan 《Monthly notices of the Royal Astronomical Society》1998,294(1):L13-L17

A gamma-ray burst (GRB) releases an amount of energy similar to that of a supernova explosion, which combined with its rapid variability suggests an origin related to neutron stars or black holes. Since these compact stellar remnants form from the most massive stars not long after their birth, GRBs should trace the star formation rate in the Universe; we show that the GRB flux distribution is consistent with this. Because of the strong evolution of the star formation rate with redshift, it follows that the dimmest known bursts have z  ∼ 6, much above the value usually quoted and beyond the most distant quasars. This explains the absence of bright galaxies in well-studied GRB error boxes. The increased distances imply a peak luminosity of 8.3 × 10⁵¹ erg s⁻¹ and a rate density of 0.025 per million years per galaxy. These values are 20 times higher and 150 times lower, respectively, than are implied by fits with non-evolving GRB rates. This means either that GRBs are caused by a much rarer phenomenon than mergers of binary neutron stars, or that their gamma-ray emission is often invisible to us due to beaming. Precise burst locations from optical transients will discriminate between the various models for GRBs from stellar deaths, because the distance between progenitor birth place and burst varies greatly among them. The dimmest GRBs are then the most distant known objects, and may probe the Universe at an age when the first stars were forming.  相似文献   

柞水原划泥盆系中发现早前寒武纪变质岩系   总被引：2，自引：1，他引：1  

崔建堂  赵长樱  计文华 《陕西地质》1998,(2)

本文阐述了作者在1：5万区调填图中,从柞水地区商丹断裂带南侧原划泥盆系刘岭群桐峪寺组中解体出前寒武纪中深变质岩系,取得了同位素全岩Sm－Nd年龄平均值2499．83Ma的数据,这对研究秦岭造山带的演化具有重要的地质意义。  相似文献   

Clustering of galaxies at high redshifts     

Bagla 《Monthly notices of the Royal Astronomical Society》1998,297(1):251-254

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.  相似文献   

华峰尖火山通道地球物理场地球化学异常特征及其与成矿作用的关系     

姚俭  王艳青 《浙江国土资源》1999,(1)

治岭头金银矿及杨梅岗铅锌矿、治岭头黄铁矿均生成在华峰尖火山通道的边缘断裂带内。研究火山构造不但对找矿和成矿预测有重要意义，而且对研究矿床的生成时代、成因类型也有重要意义。治岭头金银矿虽然生成在陈蔡群变质岩的糜棱岩带内，许多研究者认为是变质热液矿床。从矿体的产出部位与火山通道的关系看：应为火山热液矿床，生成时代应为燕山早期。  相似文献   

Natural entropy production in an inflationary model for a polarized vacuum     

Marcelo Samuel Berman  Murari M. Som 《Astrophysics and Space Science》2007,310(3-4):277-279

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.  相似文献   

谈早前寒武纪侵入岩定位、变形、变质的同期性     

仲卫国  宋奠南 《山东国土资源》1999,(4)

依据鲁西地区早前寒武纪花岗质侵入岩普遍具有塑性流变特征和退化变质特征，以及变质作用和变形作用相协调等现象，认为岩体的侵位与变形、变质是同一期构造岩浆作用形成的，是岩浆就位后逐渐冷凝过程中，在持续应力作用下发生的，与后期的地质构造作用无关；固态岩石只能发生脆性变形和局部的脆韧性变形。并从热力场、动力场和化学场的变化趋势对变形、变质作用的制约因素作了简要分析。  相似文献   

Formation and early development of tetraspores of Polysiphonia urceolata （Rhodomelaceae, Rhodophyta）     

姚建亭  李大鹏  于深辉  刘吉东  段德麟 《中国海洋湖沼学报》2009,27(2):365-369

Polysiphonia urceolata is one type of potential commercial red seaweeds used for breeding and cultivation, because of its significant biochemical and biomedical application. However, the information of breeding and seedling incubation for cultivation is limited, especially the early development. In this study, tetrasporohyte and gametophyte of P. urceolata were taken as the study materials in Huiquan Bay, Qingdao, China. The cleaned and sterilized tetrasporophytes and gametophytes were pre-cultured in sterilized seawater, then nurtured at 18°C, 25 μmol photons m⁻² s⁻¹ in 12:12 h (light:dark) photoperiod. Continuous observation under microscope showed that the early development consists of bipolar division stage and seedling stage. In the division stage, tetraspores germinate into bipolar sporelings that further differentiate into a colorless rhizoidal portion and a lightly pigmented upright shoot. The lightly pigmented rhizoidal cell develops to a rhizoid and the larger pigmented cell transforms to an erect axis. In the seedling stage, several quasi-protuberances appear on the erect axis and form juvenile seedlings. The results demonstrate the culture of P. urceolata from tetraspores under laboratory conditions. Supported by National Key Technology Support Program, Development Program of China (No.2006AA09Z21), National Natural Science Foundation of China (No. 40618001 and N_CUHK438/06) and Shandong Agricultural Seed Stock Breeding Project  相似文献   

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

S. I. Grachev 《Astrophysics》2007,50(4):515-524

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).  相似文献