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941.
经研究证明,前人建立的二郎坪群火神庙组确有少量的亚碱性双峰式火山岩。这些火山岩零星地分布在几个地区,走向不连续,出露宽度一般为数百米。构成该组主体的是一条规模宏伟的侵入岩带,其岩石组合为辉长岩-闪长岩-石英闪长岩-斜长花岗岩-花岗岩,总体上表现为正序岩浆演化序列。这些侵入岩普遍经历了三个阶段的变形变质作用,即第一阶段为韧性变形;第二阶段为静态重结晶;第三阶段为带状褶劈理,表现了复杂而漫长的构造演化史。 相似文献
942.
本文应用非线性谱分析中的最大熵谱分析方法(MEM)、和一般线性功率谱的分析方法,对固体潮潮汐因子的时间序列进行了综合研究,指出固体潮潮汐因子的时间序列中普遍存在明显的半月左右周期的特征频谱;将其应用于地震前兆的分析与探索,对固体潮潮汐因子特征频谱中的前兆变化特征进行了解释,得出结论:半月左右周期的频率域,是固体潮观测中前兆响应的一个重要主频域。 相似文献
943.
Contribution to diffuse gamma-rays in the Galactic Centre region from unresolved millisecond pulsars
W. Wang Z. J. Jiang K. S. Cheng 《Monthly notices of the Royal Astronomical Society》2005,358(1):263-269
Diffuse gamma-rays in the Galactic Centre region have been studied. We propose that there exists a population of millisecond pulsars in the Galactic Centre, which emit GeV gamma-rays through synchrotron-curvature radiation as predicted by outer gap models. These GeV gamma-rays from unresolved millisecond pulsars probably contribute to the diffuse gamma-ray spectrum detected by EGRET which displays a break at a few GeV. We have used a Monte Carlo method to obtain simulated samples of millisecond pulsars in the Galactic Centre region covered by EGRET (∼ 15) according to the different period and magnetic field distributions from observed millisecond pulsars in the Galactic field and globular clusters, and superposed their synchrotron-curvature spectra to derive the total GeV flux. Our simulated results suggest that there probably exist about 6000 unresolved millisecond pulsars in the region of angular resolution of EGRET, the emissions of which could contribute significantly to the observed diffuse gamma-rays in the Galactic Centre. 相似文献
944.
A. M. Chandler
G. L. Hutchinson
W. Jiang 《Soil Dynamics and Earthquake Engineering》1991,10(8):429-439This study aims to determine the influence of torsional coupling on the inelastic response of a series of models representing typical structural configurations in real buildings. The lake bed (SCT) east-west component of the 1985 Mexico City earthquake was employed in the analysis, and is representative of a severe ground motion known to have induced large inelastic structural deformations in a high proportion of those buildings having asymmetrical distributions of stiffness and/or strength. Material non-linearity in lateral load-resisting elements has been defined using a hysteretic Ramberg-Osgood model. Structural eccentricities have been introduced into the building models by (i) asymmetrical distributions of stiffness and/or strength, (ii) asymmetrical configuration of lateral load-resisting elements, or (iii) varying post-elastic material behaviour in the resisting elements. The dynamic inelastic response of these models has been obtained by a numerical integration of the relevant equations of motion, expressed in a non-dimensional incremental form.
In the elastic range, the results correlate well with those of previous studies. In the inelastic range, it is concluded that the peak ductility demand of the worst-affected element increases with the ground excitation level across the range of building periods considered, and that the influence of torsional coupling on the key response parameters is model dependent. Most significantly, the strength eccentricity relative to the centre of mass has been shown to influence the peak edge displacement response more than conventionally employed stiffness eccentricity. 相似文献
945.
As there are many heavily sediment-laden rivers in China, with high sediment concentration and a large quantity of sediment
load, the sedimentation problems of the reservoirs built on those rivers are so serious that the amount of sediment deposited
in the reservoirs is great and the rate of sedimentation is accelerated. According to the statistics, up to the end of 1981,
a total amount of 11.5×109m3 of sediment were accumulated in those reservoirs, i.e. 14.2% of the total designed capacity were lost. The average annual
loss in storage capacity reached 2.3 percent, being the highest in the world. Silting of impounding lakes not only has an
effect on the benefits of the reservoirs and seriously threatens the life of reservoirs, but also results in many environmental
problems which were not fully estimated in the planning of the reservoirs. In this paper, the situation of reservoir deposition
in China are described from the following aspects: 1) the characteristics of hydrology and sediment of the rivers; 2) the
seriousness of reservoir sedimentation in China; 3) problems caused by reservoir deposition; 4) the methods of minimizing
sediment deposition, etc. 相似文献
946.
本文研究墨吉对虾(Penaeus merguiensis)体长(L)与体重(W)的关系,经回归分析得其关系式。根据此关系式计算得体长和体重换算表,对指导生产具有现实意义。 相似文献
947.
辽西南天门断裂及其与北票组发育的关系 总被引:1,自引:0,他引:1
通过对辽西地区TM图像地质解译和对南天门断裂的研究表明,虽然南天门断裂现今在地形地貌上表现为其西的北票、朝阳、建昌盆地和其东的金羊盆地的区域性分隔断裂,但是实际上在早侏罗世末以前,则是一个统一盆地内的潜伏(基底)断裂,即非现今的盆地边缘断裂。由于盆地内普遍发育含有油气性良好的下侏罗统北票组,因此,辽西地区应具有良好的油气勘探开发前景。 相似文献
948.
对WCDMA直放站的原理、主要技术指标、覆盖半径计算及其对系统的干扰进行分析和阐述,并就如何最大限度发挥直放站作用进行了必要的工程和理论探讨,同时结合工程实际情况提出了相应的解决方案。 相似文献
949.
In this paper the researchers collected 28 times of maximum light including 4 times of those observed at the Xinglong station,
the National Astronomical Observation of China between May 27, 2004 and June 1, 2004 and 1 time of maximum light from a 60
cm telescope on May 4, 1984. It found that the O-C point distribution was more completely compared than in any papers published
before. The period is decreasing at the rate of about (1.4±0.1)×10−8 per year, which should not be caused by stellar evolution. It might be only part of a binary orbital light-time variation
or other unknown reason. The time scale is longer than Pocs and Szeidl’s suggestion; the star needs more observations before
we can be certain of the exact light-time variation. 相似文献
950.
Two-integral distribution functions for axisymmetric stellar systems with separable densities 总被引:1,自引:0,他引:1
Zhenglu Jiang Leonid Ossipkov 《Monthly notices of the Royal Astronomical Society》2007,382(4):1971-1981
We show different expressions of distribution functions (DFs) which depend only on the two classical integrals of the energy and the magnitude of the angular momentum with respect to the axis of symmetry for stellar systems with known axisymmetric densities. The density of the system is required to be a product of functions separable in the potential and the radial coordinates, where the functions of the radial coordinate are powers of a sum of a square of the radial coordinate and its unit scale. The even part of the two-integral DF corresponding to this type of density is in turn a sum or an infinite series of products of functions of the energy and of the magnitude of the angular momentum about the axis of symmetry. A similar expression of its odd part can be also obtained under the assumption of the rotation laws. It can be further shown that these expressions are in fact equivalent to those obtained by using Hunter & Qian's contour integral formulae for the system. This method is generally computationally preferable to the contour integral method. Two examples are given to obtain the even and odd parts of their two-integral DFs. One is for the prolate Jaffe model and the other for the prolate Plummer model.
It can be also found that the Hunter–Qian contour integral formulae of the two-integral even DF for axisymmetric systems can be recovered by use of the Laplace–Mellin integral transformation originally developed by Dejonghe. 相似文献
It can be also found that the Hunter–Qian contour integral formulae of the two-integral even DF for axisymmetric systems can be recovered by use of the Laplace–Mellin integral transformation originally developed by Dejonghe. 相似文献