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91.
三维层状场地的精确动力刚度矩阵及格林函数 总被引:3,自引:1,他引:3
本文对Wolf二维层状场地精确动力刚度矩阵进行推广,给出了三维层状场地的精确动力刚度矩阵。刚度矩阵具有对称的特点,且因刚度矩阵是精确的,计算结果不受土层单元厚度的影响,可以大大提高计算效率。文中对刚度矩阵进行了数值验证。利用三维层状场地动力刚度矩阵,计算分析了基岩上单一土层场地的动力响应。最后作为动力刚度矩阵的另一重要应用,给出了表面或埋置矩形均布荷载或集中荷载的动力格林函数计算方法。 相似文献
92.
An analysis of four-colour photographic images of Jupiter taken during 1970–1974 is presented. It is shown that major global and hemispheric changes in colour—mainly in the blue— occurred over this period. 相似文献
93.
Twenty nine samples of silica sinter, ranging in age from modern to Miocene, record temporal changes in both mineralogy and
texture. When first deposited, sinters consist largely of noncrystalline spheres (<1–8 μm diameter) of opal-A exhibiting varying
degrees of close-packing. Particle densities range from 1.5 to 2.1 g cm−3, total water 4–10 wt%, and porosities 35–60%. Changes over ∼10,000 years following deposition are slight although the spheres
may be invested by an additional film of secondary silica. For the next 10,000 to ∼50,000 years, the silica incrementally
crystallises to become poorly crystalline opal-CT and/or opal-C; spherical particles of thin-bladed crystals (lepispheres)
replace opal-A particles and coalesce in microbotryoidal aggregates (∼10–30 μm diameter). Amygdaloidal fibrous clusters occur
with lepispheres. As silica lattice ordering becomes enhanced, total water content drops to <7 wt%, particle density increases
to ∼2.3 g cm−3, and porosity reduces to <30%. The change from opal-A to opal-C takes place over a briefer periods (∼50 years) in silica
sinters that contain other materials (e.g. calcite, sulfur, alunite, plant remains). Sinters older than ∼50,000 years have
recrystallised to microcrystalline quartz. With the onset of quartz crystallisation at ∼20,000 years, total water is <0.2 wt%,
particle density approximates quartz (2.65 g cm−3), and porosity is <4%. The progressive changes in silica species and texture yield ageing profiles for sinters that may serve
as guides to the paleohydrology of geothermal systems and/or epithermal ore deposits in areas where surface thermal activity
has declined or ceased.
Received: 18 November 1998 / Accepted: 6 July 1999 相似文献
94.
N. Jackson E. Xanthopoulos I. W. A. Browne 《Monthly notices of the Royal Astronomical Society》2000,311(2):389-396
We present Hubble Space Telescope ( HST ) infrared images of four gravitational lens systems from the JVAS/CLASS gravitational lens survey and compare the new infrared HST pictures with previously published WFPC2 HST optical images and radio maps. Apart from the wealth of information that we get from the flux ratios and accurate positions and separations of the components of the lens systems, which we can use as inputs for better constraints on the lens models, we are able to discriminate between reddening and optical/radio microlensing as the possible cause of differences observed in the flux ratios of the components across the three wavelength bands. Substantial reddening has been known to be present in the lens system B1600+434 and has been further confirmed by the present infrared data. In the two systems B0712+472 and B1030+074 microlensing has been pinpointed as the main cause of the flux ratio discrepancy both in the optical/infrared and in the radio, the radio possibly caused by the substructure revealed in the lensing galaxies. In B0218+357, however, the results are still not conclusive. If we are actually seeing the two 'true' components of the lens system then the flux ratio differences are attributed to a combination of microlensing and reddening or are alternatively the result of some variability in at least one of the images. Otherwise the second 'true' component of B0218+357 may be completely absorbed by a molecular cloud and the anomalous flux density ratios and large difference in separation between the optical/infrared and radio that we see can be explained by emission either from a foreground object or from part of the lensing galaxy. 相似文献
95.
P. M. Phillips M. A. Norbury L. V. E. Koopmans I. W. A. Browne N. J. Jackson P. N. Wilkinson A. D. Biggs R. D. Blandford A. G. de Bruyn C. D. Fassnacht P. Helbig S. Mao D. R. Marlow S. T. Myers T. J. Pearson A. C. S. Readhead D. Rusin E. Xanthopoulos 《Monthly notices of the Royal Astronomical Society》2000,319(2):L7-L11
High-resolution MERLIN observations of a newly discovered four-image gravitational lens system, B0128+437, are presented. The system was found after a careful re-analysis of the entire CLASS data set. The MERLIN observations resolve four components in a characteristic quadruple-image configuration; the maximum image separation is 542 mas and the total flux density is 48 mJy at 5 GHz. A best-fitting lens model with a singular isothermal ellipsoid results in large errors in the image positions. A significantly improved fit is obtained after the addition of a shear component, suggesting that the lensing system is more complex and may consist of multiple deflectors. The integrated radio spectrum of the background source indicates that it is a gigahertz peaked spectrum source. It may therefore be possible to resolve structure within the radio images with deep VLBI observations and thus to constrain the lensing mass distribution better. 相似文献
96.
本文报道了雅鲁藏布江缝合带西段的东波蛇绿岩地幔橄榄岩中发现与罗布莎和普兰岩体相似的金刚石和特殊地幔矿物群。东波地幔橄榄岩体以方辉橄榄岩为主,含少量二辉橄榄岩和纯橄岩,辉石岩和辉长岩呈脉状产在方辉橄榄岩中。岩石地球化学特征表明东波岩体形成于MOR环境后受到SSZ环境的改造。通过重砂分选实验,在693 kg的地幔橄榄岩大样中发现了金刚石和碳硅石等30余种特殊矿物群,包括金刚石、自然铬、自然金、自然铁、自然硅、自然铜等自然元素矿物类;碳硅石等碳化物;铬尖晶石、金红石、铬铁矿、刚玉、黑钨矿、铌钽铁矿、磁铁矿、赤铁矿、方铁矿、锡石等氧化物;铁铬镍合金、镍铁合金、铜锌合金等合金互化物;辉钼矿、方铅矿、辉铋矿、黄铁矿、黄铜矿、毒砂和闪锌矿等硫化物;橄榄石、辉石、锆石、蓝晶石、白云母、蛇纹石、绿帘石等硅酸岩;萤石等氟化物。该矿物群与雅鲁藏布江缝合带的罗布莎和普兰两个岩体中发现的特殊矿物群非常类似,同时也为蛇绿岩型金刚石这一新类型提供了佐证。 相似文献
97.
一种有效的GNSS接收机载噪比估计方法 总被引:1,自引:0,他引:1
提出了一种I支路功率方差比方法(I branch power variance ratio,IBPVR),并详细推导了另外3种载噪比估计方法(NWPR、MM、SNV),比较了这4种方法在强信号和弱信号情况下的跟踪性能。实验结果显示,在载噪比超过50dBHz时,NWPR方法与SNV方法并未出现饱和现象,SNV方法在弱信号情况下会产生估计偏差,NWPR与IBPVR方法的估计性能比较好。 相似文献
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