Numerical simulations of protostellar encounters — II. Coplanar disc–disc encounters     

S. J. Watkins  A. S. Bhattal  H. M. J. Boffin  N. Francis  & A. P. Whitworth 《Monthly notices of the Royal Astronomical Society》1998,300(4):1205-1213

It is expected that an average protostar will undergo at least one impulsive interaction with a neighbouring protostar whilst a large fraction of its mass is still in a massive, extended disc. Such interactions must have a significant impact upon the evolution of the protostars and their discs.   We have carried out a series of simulations of coplanar encounters between two stars, each possessing a massive circumstellar disc, using an SPH code that models gravitational, hydrodynamic and viscous forces. We find that during a coplanar encounter, disc material is swept up into a shock layer between the two interacting stars, and the layer then fragments to produce new protostellar condensations. The truncated remains of the discs may subsequently fragment; and the outer regions of the discs may be thrown off to form circumbinary disc-like structures around the stars. Thus coplanar disc–disc encounters lead efficiently to the formation of multiple star systems and small- N clusters, including substellar objects.  相似文献   

Line emission from accretion discs around black holes: the analytic approach     

Andrej ?ade?  Claudio Fanton  Massimo Calvani 《New Astronomy》1998,3(8):528-654

The broad X-ray iron line observed in many active galactic nuclei spectra is thought to originate from the accretion disc surrounding the putative supermassive black hole. We show here how to perform the analytical integration of the geodesic equations that describe the photon trajectories in the general case of a rotating black hole (Kerr metric), in order to write a fast and efficient numerical code for modelling emission line profiles from accretion discs.  相似文献   

东天山秋格明塔什黄山韧性剪切带变形特征分析     

杨兴科  张连昌  姬金生  曾章仁  陶洪祥 《地球科学与环境学报》1998,20(3):42

东天山秋黄韧性剪切带位于新疆东部两大板块碰撞接合地带,东西延长逾６００ｋｍ,由石炭系组成,规模巨大,分带明显,宏微观变形标志清晰,石英Ｃ轴组构呈点极密型,分为四期变形,序列演化明显,应变测量属平面单剪,剪切位移量达７５ｋｍ以上,存在脆韧性变形转换,变形时代为海西中晚期,强弱应变相间排列的标度不变性特征明显,变形机制属地壳中深层次塑性流变和韧性剪切,与板块间的俯冲碰撞构造演化密切相关。控制着金铜矿分布。  相似文献   

三维空间实体间拓扑关系的矩阵描述   总被引：1，自引：0，他引：1  

陈军  郭薇 《武汉大学学报(信息科学版)》1998,(4)

三维空间实体及其间拓扑关系的语义描述和形式化表达是三维ＧＩＳ空间数据建模的重要理论基础。在ｋ－维流形的三维空间实体形式化描述方法的基础上,根据三维空间实体的可剖分性,采用顾及维数的九元组描述框架,研究用于构成三维实体的ｋ－单纯形（０≤ｋ≤３）之间的拓扑空间关系,继而研究三维实体间的拓扑空间关系。  相似文献   

三维地理信息系统中几何特征的误差模型   总被引：1，自引：0，他引：1  

史文中 《武汉大学学报(信息科学版)》1998,(1)

本文提出了三维地理信息系统中几何特征的误差模型。基于面表示的三维ＧＩＳ的特征被分为点、线段及线,该模型给出这些特征的一种误差描述,即围绕着这些几何特征的量测值的一个范围。  相似文献   

湘赣边地区走滑断裂带致矿异常的结构样式及分形特征   总被引：4，自引：1，他引：3  

李先福  李建威  傅昭仁  王学平 《地球科学》1998,23(2):11

湘赣边地区构造岩浆带是环太平洋成矿带内最重要的高值地质矿产异常区,其中ＮＮＥ向走滑断裂明显地控制了岩浆－断陷盆地和铀及钨、锡、铅、锌、锑等的成矿作用．在区域地质环境研究的基础上,根据典型矿田（床）控矿构造分析成果,将走滑断裂带内局部性致矿地质异常归纳为：帚尾式致矿异常,棋盘格式致矿异常、辫状结环式致矿异常和拉分盆缘式致矿异常．重点讨论了各类异常的结构样式和分维特点．  相似文献   

清江高坝洲地区古岩溶角砾岩特征及形成条件   总被引：5，自引：0，他引：5  

王增银  沈继方 《地球科学》1998,23(5):524-528

古岩溶角砾岩是在特定的地质和水文地质条件下形成的沉积岩,是记录岩溶发育环境和形成时代的“化石”通过对高坝洲地区古岩溶角砾岩发育特征及取样分析测试研究,查明该类岩角砾岩属于岩溶崩塌角砾岩,胶结物方解石晶体是中低温热水溶液中ＣａＣＯ３沉淀形成的,形成时间是上新世。  相似文献   

鲁南地区城市房屋震害预测     

何钧  杜宪宋 《高原地震》1998,(2)

在文献调查和现场调查的基础上,对鲁南地震重点监视防御区内城市房屋建筑的抗震能力做了分析,给出了抗震救灾重要房屋的单体预测结果、现有房屋的群体预测结果,并对房屋破坏造成的直接经济损失、人员伤亡进行了预测。文中指出了现有房屋的抗震薄弱环节,为该地区采取防震减灾对策提供了依据。  相似文献   

Inversion, error analysis, and validation of GPS/MET occultation data     

A. K. Steiner  G. Kirchengast  H. P. Ladreiter 《Annales Geophysicae》1998,17(1):122-138

The global positioning system meteorology (GPS/MET) experiment was the first practical demonstration of global navigation satellite system (GNSS)-based active limb sounding employing the radio occultation technique. This method measures, as principal observable and with millimetric accuracy, the excess phase path (relative to propagation in vacuum) of GNSS-transmitted radio waves caused by refraction during passage through the Earth’s neutral atmosphere and ionosphere in limb geometry. It shows great potential utility for weather and climate system studies in providing an unique combination of global coverage, high vertical resolution and accuracy, long-term stability, and all-weather capability. We first describe our GPS/MET data processing scheme from excess phases via bending angles to the neutral atmospheric parameters refractivity, density, pressure and temperature. Special emphasis is given to ionospheric correction methodology and the inversion of bending angles to refractivities, where we introduce a matrix inversion technique (instead of the usual integral inversion). The matrix technique is shown to lead to identical results as integral inversion but is more directly extendable to inversion by optimal estimation. The quality of GPS/MET-derived profiles is analyzed with an error estimation analysis employing a Monte Carlo technique. We consider statistical errors together with systematic errors due to upper-boundary initialization of the retrieval by a priori bending angles. Perfect initialization and properly smoothed statistical errors allow for better than 1 K temperature retrieval accuracy up to the stratopause. No initialization and statistical errors yield better than 1 K accuracy up to 30 km but less than 3 K accuracy above 40 km. Given imperfect initialization, biases ≫ 2 K propagate down to below 30 km height in unfavorable realistic cases. Furthermore, results of a statistical validation of GPS/MET profiles through comparison with atmospheric analyses of the European Centre for Medium-range Weather Forecasts (ECMWF) are presented. The comparisons indicate the high utility of the occultation data in that very good agreement of upper troposphere/lower stratosphere temperature (better than 1.5 K rms, ≪ 0.5 K bias) is found for a region (Europe+USA) where the ECMWF analyses are known to be good, but poorer agreement for a region (Southern Pacific) where the analyses are known to be degraded.  相似文献   

CUTLASS Finland radar observations of the ionospheric signatures of flux transfer events and the resulting plasma flows   总被引：1，自引：0，他引：1  

G. Provan  T. K. Yeoman  S. E. Milan 《Annales Geophysicae》1998,16(11):1411-1422

The CUTLASS Finland radar has been run in a two-beam special scan mode, which offered excellent temporal and spatial information on the flows in the high-latitude ionosphere. A detailed study of one day of this data revealed a convection reversal boundary (CRB) in the CUTLASS field of view (f.o.v) on the dayside, the direction of plasma flow either side of the boundary being typical of a dawn-cell convection pattern. Poleward of the CRB a number of pulsed transients are observed, seemingly moving away from the radar. These transients are identified here as the ionospheric signature of flux transfer events (FTEs). Equatorward of the CRB continuous backscatter was observed, believed to be due to the return flow on closed field lines. The two-beam scan offered a new and innovative opportunity to determine the size and velocity of the ionospheric signatures associated with flux transfer events and the related plasma flow pattern. The transient signature was found to have an azimuthal extent of 1900 ± 900 km and an poleward extent of 250 km. The motion of the transient features was in a predominantly westward azimuthal direction, at a velocity of 7.5 ± 3 km.  相似文献