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991.
We study the statistics of large-separation multiply-imaged quasars lensed by clusters of galaxies.In particular,we examine how the observed brightest cluster galaxies (BCGs) affect the predicted numbers of wide-separation lenses.We model the lens as an NFW-profiled dark matter halo with a truncated singular isothermal sphere to represent the BCG in its center.We mainly make predictions for the Sloan Digital Sky Survey Quasar Lens Search (SQLS) sample from the Data Release 5 (DR5) in two standard ΛCDM cosmo...  相似文献   
992.
We present broadband (radio,optical,X-ray and GeV) fits to the afterglow light curves and spectra of three long-duration gamma-ray bursts (GRBs 080916C,090902B,and 090926A) detected by the Gamma-Ray Burst Monitor and Large Area Telescope (LAT) instruments on the Fermi satellite.Using the observed broadband data,we study the origin of the high energy emission,and suggest that the early-time GeV emission and the late-time radio,optical,and X-ray afterglows can be understood as being due to synchrotron emissio...  相似文献   
993.
GRS 1915+105 is a prominent black hole system exhibiting variability over a wide range of time scales and its observed light curves have been classified into 12 temporal states. Here we undertake a complete analysis of these light curves from all the states using various quantifiers from nonlinear time series analysis, such as the correlation dimension (D2), the correlation entropy (K2), singular value decomposition (SVD) and the multifractal spectrum (f(α) spectrum). An important aspect of our analysis is ...  相似文献   
994.
X-ray dim isolated neutron stars are peculiar pulsar-like objects,characterized by their Planck-like spectrum.In studying their spectral energy distributions,optical/ultraviolet(UV) excess is a long standing problem.Recently Kaplan et al.measured the optical/UV excess for all seven sources,which is understandable in the resonant cyclotron scattering(RCS) model previously addressed.The RCS model calculations show that the RCS process can account for the observed optical/UV excess for most sources.The ?at spe...  相似文献   
995.
We present an efficient,robust computational method for modeling the Newtonian dynamics for rotation curve analysis of thin-disk galaxies.With appropriate mathematical treatments,the apparent numerical difficulties associated with singularities in computing elliptic integrals are completely removed.Using a boundary element discretization procedure,the governing equations are transformed into a linear algebra matrix equation that can be solved by straightforward Gauss elimination in one step without further ...  相似文献   
996.
The concept of degree of similarity(η),is proposed to quantitatively describe the similarity of a parameter(e.g.the maximum amplitude Rmax)of a solar cycle relative to a referenced one,and the prediction method of similar cycles is further developed.For two parameters,the solar minimum(Rmin)and rising rate(βa),which can be directly measured a few months after the minimum,a synthesis degree of similarity(ηs)is defined as the weighted-average of theηvalues around Rmin and βa,with the weights given by the coef...  相似文献   
997.
高铬红土型铝铁复合矿经钠盐还原焙烧-磁选-浸出后,铬等有价金属在赤泥中富集(Cr2O3含量达到3%~30%),属难熔复合矿物,目前主要以化学分析方法为主,但操作复杂,且步骤繁琐,分析周期长。而应用X射线荧光光谱法(XRF)分析测定,一般采用钠盐熔剂、较高稀释比等熔融制样,不利于钠以及低含量元素的测定。本文采用四硼酸锂-偏硼酸锂(67:33)作混合熔剂,硝酸铵作氧化剂,饱和溴化锂溶液作脱模剂制备玻璃熔片,建立了波长色散型XRF测定高铬赤泥中主次量组分(铬硅铝铁镁钙钠钾硫磷钛锰钒)的分析方法。研究表明,熔样稀释比低于24:1时,稀释比越低,对铂金坩埚腐蚀越严重;稀释比在24:1时制样方法的相对标准偏差(RSD,n=10)最低;熔样时间越长,温度越高,RSD越低。由此确定熔样最优条件为稀释比24:1,熔样时间15 min,熔样温度1100℃。分析中采用铬铁矿、铝土矿、黏土、铁矿石国家标准物质及人工标准样品校准,基本参数法进行基体校正,方法精密度(RSD,n=10)为0.3%~3.9%。与国内外其他含铬矿物的XRF分析方法相比,本方法采用不添加钠盐、一次熔片、常规熔样温度(1100℃)、低稀释比(24:1)等进行制样,制样方法的精密度和分析精密度均低,解决了高铬赤泥的XRF分析方法问题,还可扩展到高铬、铝、硅、铁等复合矿原矿及其钠盐处理焙烧矿、精矿及尾矿的XRF分析。  相似文献   
998.
昆仑山深部结构与造山机制   总被引:1,自引:0,他引:1       下载免费PDF全文
本文根据INDEPTH-Ⅳ剖面所做的地质?地球物理探测所取得的资料,进行综合研究,提出了一个新的昆仑山造山模式,论述了:(1)在早二叠世松潘—甘孜洋向昆仑—柴达木地块下俯冲使地块南缘形成陆缘弧和弧后拉张区,使昆仑—柴达木地块在持续碰撞挤压过程中,分别形成了造山带与古近—新近纪盆地的不同构造演化特征;(2)昆仑地段老结晶基底在地块对挤中不断向上抬升成山,同时又受到强烈剥蚀,使老结晶基底及深成岩呈现在地表;南昆仑地块则沿昆仑地块中央断裂向北逆冲到北昆仑地块之上,断裂深10 km;昆仑地块没有发生向北逆冲推覆到柴达木地块上;(3)昆仑地块地壳增厚主要发生在中地壳(6.2~6.6 km/s),是中基性岩石层的增厚;(4)柴达木盆地作为昆仑弧弧后拉张地带,随昆仑造山隆升而下沉,新生界陆相沉积达12~14 km厚,由“沉积”与“挤入”两个作用造成了地壳增厚;结晶基底发生断陷形成新裂谷,裂谷宽度约12 km,深度约4 km,导电带显示裂谷通过断裂与深部发生热流体联系;(5)再次确定了,柴达木盆地莫霍界面深52 km,昆仑山的莫霍界面深65~70 km,莫霍界面台阶位于格尔木附近(185 km距离处);(6)松潘—甘孜地体复理石层厚度为10~14 km,其下面的6.2~6.3 km/s 均匀速度层(同时有高导电性显示)是本地块所特有,推测为残留洋壳的堆积,约15 km厚;浅层通过古近—新近系风火山推覆系增厚,另在中地壳部位挤入了15 km厚岩层;(7)否定了亚洲岩石圈地幔向柴达木地块地幔岩石圈之下俯冲的模式,提出印度大陆地幔岩石圈从高喜马拉雅下拆离成两层,并沿高原地壳底部向北伸展,直到中祁连山之下,成为高原南北对挤过程中岩石圈地幔长度调节的新方式?  相似文献   
999.
Karst rocks from the Huanglong Formation exposed at the margin of the Eastern Sichuan Basin can be divided into four types:slightly corroded, moderately corroded porous, intensely corroded brecciated and intensely corroded and replaced secondary calcic karstic rocks. The carbon, oxygen and strontium isotope compositions of the various karst rocks are analyzed systematically and compared to rocks without karst corrosion. The results indicate that(1) the Huanglong Formation in the eastern Sichuan Basin was a restricted bay supplied and controlled by freshwater in which mudmicrite and mud-dolomicrite exhibit low δ13C and δ18O values and high 87Sr/86 Sr ratios;(2) all types of karstic rocks in the paleokarst reservoirs of the Huanglong Formation in the research area are affected by atmospheric freshwater with the δ13C and δ18O values and 87Sr/86 Sr ratios in the original formation approaching those of atmospheric freshwater, which reflects ancient hydrological conditions, fluid properties, isotopic source and the fractionation effect;(3) the intensely corroded and replaced secondary limestone is affected by a variety of diagenetic fluids, often reflected by δ13C and δ18O values, while the 87Sr/86 Sr ratios exhibit the strong degree of the corrosion;(4) after comparing the 87Sr/86 Sr ratios of each type of karst rock, the diagenetic fluids are determined to be mainly atmospheric freshwater, and depending on the strength of corrosion, and the low 87Sr/86 Sr ratio fluids in the layer will participate in the karst process. The carbon, oxygen, and strontium isotopes of different karstic reservoirs can provide meaningful geochemical information for forecasting and evaluating the development and distribution rules of the Huanglong Formation at the margin of the eastern Sichuan Basin in time and space.  相似文献   
1000.
Abstract: Soil water retention curves (SWRCs) provide an important means of describing the response of unsaturated soils during drying / wetting processes in terms of variations of degree of saturation, water content or void ratio with suction. A key consideration in generating these curves is how to measure the suction. Frequently the filter paper technique is adopted, especially when high suctions are developed, e.g. with plastic clays. As each measurement takes at least a week with this technique, it can take months or years to generate a full SWRC in drying and wetting. Developments in laboratory tensiometers now allow matrix suctions up to about 1.5 MPa to be measured. With such a device it is possible to develop SWRCs for granular soils such as silts and clays in hours or days by continuous measurement. This paper describes an experimental set-up that was developed to measure changes in volume, water content and matrix suction during drying of three granular soils. Limitations of the apparatus and usefulness of the curves are discussed.  相似文献   
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