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171.
对小秦岭地区熊耳群地层的分布作了概述。在熊耳群地层分布区划出了坝源—洛源(A区)、三岔—石门(B区)和西峪河—梧桐河(C区)三个火山岩型铁矿资源潜力区。阐述了各潜力区的铁矿成矿条件,对潜在资源量作了测算。预测全区300 m以上铁矿潜在资源量为≥9.4亿吨,钛铁矿≥300万吨。 相似文献
172.
TThe Roper Group is a cyclic, predominantly marine, siliciclastic succession of Calymmian (Early Mesoproterozoic) age. It has a distribution of at least 145 000 km2 and a maximum known thickness of ~5000 m. In the Roper River district the middle part of the Roper Group (~1300 m thick) is characterised by the cyclical alternation of mudstone and sandstone units, and can be divided into six third‐order depositional sequences. A typical sequence is broadly progradational in aspect, and comprises a lower, mudstone‐rich, storm‐dominated shelf succession (up to 330 m thick), and a sequence‐capping unit dominated by tidal‐platform cross‐bedded sandstone (up to 80 m thick); both are interpreted as highstand systems tracts. Transgressive strata are poorly represented but where present are characterised by paralic to fluvial redbed assemblages that include ooidal ironstone. Roper Group sequences lack a distinct condensed section and sequence boundaries are mostly conformable. Erosional contacts separate mud‐rich shelf facies from sequence‐capping sandstones. We infer that these erosion surfaces were generated by episodic flexural tectonism, which also generated the accommodation and sediment supply for Roper sequences. 相似文献
173.
Linella avis, an early to middle Neoproterozoic (Tonian to Cryogenian) stromatolite, occurs in the Eliot Range Dolomite, part of the Ruby Plains Group in the Wolfe Basin, east Kimberley. Previously, this dolomite was assigned to the Mesoproterozoic Bungle Bungle Dolomite in the Osmond Basin, which contains a different suite of stromatolites. Linella avis, which also occurs in the Neoproterozoic Bitter Springs Formation of the Amadeus Basin, central Australia, appears to be restricted to rocks aged around 850 to 800 Ma. The presence of L. avis indicates that the Ruby Plains Group is a probable correlative of the Heavitree Quartzite and Bitter Springs Formation, and is probably much younger than the Bungle Bungle Dolomite. If the correlation suggested here is correct, the Wolfe Basin, together with the Amadeus and Ngalia Basins, formed part of the Centralian Superbasin. 相似文献
174.
杨家喜 《地球科学与环境学报》1991,(4)
本文简略回顾了堇青石-石榴石-矽线石-石英地质温压计的研究历史,并介绍由Aranovich等人完成的最新实验研究。以内蒙古南部贺兰山群的麻粒岩相矽线石榴堇青片麻岩的温压计算为例,用Aranovich等人实验标定的温压计计算结果与石榴石-堇青石Fe-Mg交换反应温度计和石榴石-斜长石-矽线石-石英压力计的计算结果相当吻合;而应用含有假定的热力学参数的哈奇森的温压计与其它温压计计算结果有较大差别,温度明显偏低,与岩石形成于麻粒岩相变质条件这一地质事实不符。 相似文献
175.
We have modelled, for the cases of Milky Way and M31, the effects on the galactic discs, of the arrival at high velocity (≥150
km s−1) of giant HI clouds, with masses of up to 108M⊙. Predictions are compared with the detailed structure of the observed rotation curves for these two galaxies. The model
explains the rises and falls observed at large distances from the centre of each galaxy, distributed with a degree of regularity
in radius, in terms of a specific type of perturbations driven by the infall of the high velocity clouds (HVC's) arriving
from the intracluster medium of the Local Group. The underlying rotation curve is explained conventionally via the distribution
of the baryonic and dark matter components of the galaxy in question. This scenario, though tested here on the two major Local
Group objects, is in principle applicable to galaxies undergoing minor mergers with subgalactic mass gas clouds. 相似文献
176.
论辽南上前寒武系的划分与对比 总被引:1,自引:0,他引:1
辽南上元古界的区域对比的关键是如何与蓟县层型、峡东层型的衔接或对比。作者认为辽南群是介于北方的青白口群与南方的震旦系之间的层位,仅金县群才相当于震旦系,震旦系与寒武系的界线则应置于兴民村组与葛屯组之间。 相似文献
177.
J.Kleyna M. I.Wilkinson N. W.Evans G.Gilmore C.Frayn 《Monthly notices of the Royal Astronomical Society》2002,330(4):792-806
We present stellar radial velocity data for the Draco dwarf spheroidal (dSph) galaxy obtained using the AF2/WYFFOS instrument combination on the William Herschel Telescope. Our data set consists of 186 member stars, 159 of which have good quality velocities, extending to a magnitude V ≈19.5 with a mean velocity precision of ≈2 km s−1 . As this survey is based on a high-precision photometric target list, it contains many more Draco members at large radii. For the first time, this allows a robust determination of the radial behaviour of the velocity dispersion in a dSph.
We find statistically strong evidence of a rising velocity dispersion consistent with a dark matter halo that has a gently rising rotation curve. There is a <2 σ signature of rotation about the long axis, inconsistent with tidal disruption as the source of the rising dispersion. By comparing our data set with earlier velocities, we find that Draco probably has a binary distribution and fraction comparable to those in the solar neighbourhood.
We apply a novel maximum likelihood algorithm and fit the velocity data to a two parameter spherical model with an adjustable dark matter content and velocity anisotropy. Draco is best fit by a weakly tangentially anisotropic distribution of stellar orbits in a dark matter halo with a very slowly rising rotation law ( vcirc ∝ r 0.17 ) . We are able to rule out both a mass-follows-light distribution and an extended halo with a harmonic core at the 2.5 to 3 σ significance level, depending on the details of our assumptions about Draco's stellar binary population. Our modelling lends support to the idea that the dark matter in dwarf spheroidals is distributed in the form of massive, nearly isothermal haloes. 相似文献
We find statistically strong evidence of a rising velocity dispersion consistent with a dark matter halo that has a gently rising rotation curve. There is a <2 σ signature of rotation about the long axis, inconsistent with tidal disruption as the source of the rising dispersion. By comparing our data set with earlier velocities, we find that Draco probably has a binary distribution and fraction comparable to those in the solar neighbourhood.
We apply a novel maximum likelihood algorithm and fit the velocity data to a two parameter spherical model with an adjustable dark matter content and velocity anisotropy. Draco is best fit by a weakly tangentially anisotropic distribution of stellar orbits in a dark matter halo with a very slowly rising rotation law ( v
178.
辽宁省大石桥-吉洞峪一带出露的主要为古元古代的变质层状岩系,由云母片岩、长英质粒岩和大理类组成。区域上形成一大型北东向的复式向斜构造。复向斜南北两翼变质地层对比问题是辽吉东部辽河岩群研究的主要内容之一。作者根据五年来在大石桥-吉洞峪一带进行1∶5万区调所获得的新资料,从标志层及组合标志层、岩相学特征、主要标志层的岩石化学和稀土地球化学特征、变质作用演化等方面的研究入手,讨论了复向斜两翼变质地层对比的问题。结果表明,辽河岩群构成复向斜南北两翼的变质地层是完全可以对比的,从而进一步证实辽河岩群是一个不可分割的整体 相似文献
179.
河南省嵩箕地区登封群变质杂岩,原岩为一套造山带和岛弧的中基性、少部分为酸性的火山岩组合。其中郭家窑组为基性,常窑组、石牌河组逐渐向酸性火山岩过渡,石梯沟组属正常沉积岩系列。该群微量元素丰度值与地壳克拉克值相比,普遍偏低,其中Rb、Sr、Ba、F、Li等元素明显偏低。 相似文献
180.