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931.
The model of a presupernova’s carbon-oxygen (C-O) core with an initial mass of 1.33 M , an initial carbon abundance X C (0) =0.27, and a mean rate of increase in mass of 5 × 10?7 M yr?1 through accretion in a binary system evolved from the central density and temperature ρc=109 g cm?3 and T c=2.05 × 108K, respectively, by forming a convective core and its subsequent expansion to an explosive fuel ignition at the center. The evolution and explosion equations included only the carbon burning reaction 12C+12C with energy release corresponding to the complete conversion of carbon and oxygen (at the same rate as that of carbon) into 56Ni. The ratio of mixing length to convection-zone size αc was chosen as the parameter. Although the model assumptions were crude, we obtained an acceptable (for the theory of supernovae) pattern of explosion with a strong dependence of its duration on αc. In our calculations with sufficiently large values of this parameter, αc=4.0 × 10?3 and 3.0×10?3, fuel burned in the regime of prompt detonation. In the range 2.0×10?3≥αc≥3.0×10?4, there was initially a deflagration with the generation of model pulsations whose amplitude gradually increased. Eventually, the detonation regime of burning arose, which was triggered from the model surface layers (with m ? 1.33 M ) and propagated deep into the model up to the deflagration front. The generation of model pulsations and the formation of a detonation front are described in detail for αc=1.0 × 10?3.  相似文献   
932.
We analytically generalize the well-known solution of steady supersonic spherically symmetric gas accretion onto a star (Bondi 1952) for an iron atmosphere with completely degenerate electrons with an arbitrary degree of relativity. This solution is used for typical physical conditions in the vicinity of protoneutron stars produced by gravitational collapse with masses M 0=(1.4?1.8)M and over a wide range of nonzero “iron gas” densities at infinity, ρ=(104?5×106)g cm?3. Under these conditions, we determine all accretion parameters, including the accretion rate, whose value is ~(10?50)M s?1 at M 0=1.8M (it is a factor of 1.7 lower for M 0=1.4M , because the accretion rate is exactly ∝M 0 2 ). We take into account the effect of accreting-gas rotation in a quasi-one-dimensional approximation, which has generally proved to be marginal with respect to the accretion rate.  相似文献   
933.
Zedník  J.  Pospíšil  J.  Růžek  B.  Horálek  J.  Boušková  A.  Jedlička  P.  Skácelová  Z.  Nehybka  V.  Holub  K.  Rušajová  J. 《Studia Geophysica et Geodaetica》2001,45(3):267-282
In the time span from January 1995 to December 1999 the Czech National Seismological Network (CNSN), consisting of ten permanent digital broadband stations, several local networks and two data centers, detected and recorded 9530 regional natural seismic events, 27 greater than magnitude 2. Most of these events were located by the Czech Seismological Service (CSS), and the most prominent of them were analyzed in detail. A large number of quarry blasts were recorded as well but were not included in the analysis. We provide basic information on the configuration of the CNSN and on the way of routine data processing employed by the CSS in this paper. The over-all regional seismicity monitored by the CNSN in 1995–1999 is briefly reviewed. The main results of observations and evaluation of the local (NW-Bohemia/Vogtland, South Bohemia, Sudeten) and induced (Kladno, Píbram, Upper Silesia, Lubin/Poland) seismic activity within this period are presented in a condensed form. Finally, a summary on macroseismic observations on the territory of the Czech Republic in 1995–1999 is also presented.  相似文献   
934.
Low frequency electrostatic waves are studied in magnetized plasmas with an electron temperature which varies with position in a direction perpendicular to the magnetic field. For wave frequencies below the ion cyclotron frequency, the waves need not follow any definite dispersion relation. Instead a band of phase velocities is allowed, with a range of variation depending on the maximum and minimum values of the electron temperature. Simple model equations are obtained for the general case which can be solved to give the spatial variation of a harmonically time varying potential. A simple analytical model for the phenomenon is presented and the results are supported by numerical simulations carried out in a 2.5-dimensional particle-in-cell numerical simulation. We find that when the electron temperature is striated along B0 and low frequency waves (ci) are excited in this environment, then the intensity of these low frequency waves will be striated in a manner following the electron temperature striations. High frequency ion acoustic waves (ci) will on the other hand have a spatially more uniform intensity distribution.  相似文献   
935.
Approximately 70 km of new decimeter-resolution seismic reflection profile data from Owasco Lake, New York define a middle Holocene (4600 14C yr B.P.) erosion surface in the north end of the lake at water depths as great as 26 m. Beneath the lake, post-glacial sediments are up to 9 m thick and represent about 10% of the total sediment fill. Early to middle Holocene sediments, 6 m thick, contain biogenic gas at the south end of the basin and a large (4 km×300 m×15 m) subaqueous slide deposit along the east-central portion of the lake. Late Holocene sediments are thinner or absent, particularly at the north end of the lake. The middle Holocene erosion surface may have been produced by a drop in lake level. Alternatively, it may represent a change in climate during the transition between the relatively warm Holocene hypsithermal and cool neoglacial. At this time (4600 14C yr B.P.) circulation in Owasco Lake appears to have evolved from sluggish to active. The increased circulation, which persists today, probably resulted from atmospheric cold fronts with strong southwesterly winds that piled up water at the north end of the lake. The increased water circulation may have been ultimately driven by decreasing insolation, which produced an increased pole-to-equator thermal gradient and, thus, stronger global winds that began at the transition between the hypsithermal and neoglacial.  相似文献   
936.
地震定位研究及应用综述   总被引:10,自引:1,他引:10  
地震定位是地震学中最经典、最基本的问题之一,提高定位精度也一直是地震学应用研究的重要课题之一。本文就目前各种地震定位方法进行了大体分类并概述了基本原理及其应用,介绍了目前在国内各实时地震观测系统中应用的台网定位方法,同时将部分台网方法应用于黑龙江省绥棱爆破的定位。  相似文献   
937.
弦支穹顶结构的抗震性能研究   总被引:12,自引:2,他引:12  
弦支穹顶是一种受力性能优良的结构体系,它综合了单层网壳结构和索穹顶结构的优点,详细分析了影响弦支穹顶结构自振特性的各类参数,指出了边界条件对结构抗震性能的决定性影响。研究表明:当采用径向滑动边界时,即边界节点竖向和法向受到约束而容许径向在水平面滑动时,局部布索的弦支穹顶具有较佳的抗震性能;当边界条件相同时,弦支穹顶在水平地震和竖向地震作用下反应相似,只是程度上不同。  相似文献   
938.
具有悠久历史的石结构是砌体结构的重要组成部分,本文作者经广泛调研和试验分析:(1)提出以石粉为集料对石砌体进行抗震加固,寓环保与防灾于一体;(2)给出新型浆体配比和复合砂浆的强度等级,阐述加固技术和方法,建立灌浆石砌体抗震抗剪强度公式;(3)阐明抗震验算方法,提出基于模糊随机可靠理论的可靠性分析方法。  相似文献   
939.
本文将管线周围的土体视为固-液二相介质,采用考虑地震过程中土体内孔隙水压力的增长和消散的有效应力分析方法,并以非线性的土体本构模型模拟土体动力特性的改变以及在孔隙水压作用下的变形,以求接近土体的真实地震反应。研究表明随着土体软化程度的不同,受到土体约束的管线应力亦发生相应变化。文中详细研究了地震动峰值、管线直径、行波波速和入射角度等对管线应力的影响。  相似文献   
940.
不同型式暗支撑短肢剪力墙抗震性能试验研究   总被引:6,自引:0,他引:6  
本文选取短肢剪力墙结构体系中较为薄弱的抗震构件“一”形短肢剪力墙,采用不同的暗支撑型式进行了两个1/2缩尺的带暗支撑短肢剪力墙构件的低周反复荷载试验,比较分析了它们的承载力、刚度、延性、滞回特性、耗能能力及破坏机制,建立了其承载力计算模型与方法。计算结果与实测值符合较好。  相似文献   
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