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151.
论弱势群体的法律保护 总被引:3,自引:0,他引:3
毛晓华 《广东海洋大学学报》2005,25(2):20-23
弱势群体是社会分层的结果,对其进行保护是法律追求正义与秩序的必然要求,具体途径为通过法律再分配社会性资源,缩小强弱差距,保护弱势群体的正当权益。完善我国的弱势群体法律保护制度,须遵循“一个协调,两个结合”的指导原则,即效率与公平相协调,长远措施与短期措施相结合,全面保护与重点保护相结合。 相似文献
152.
153.
This paper concerns analysis of the impact of construction of urban tunnels on adjacent pile foundations. It is carried out using an elastoplastic three‐dimensional finite element modelling. Numerical simulations are performed in two stages, which concern, respectively, the application of the pile axial loading and the construction of the tunnel in presence of the pile foundations. Analysis is carried out for both single piles and groups of piles. Results of numerical simulations show that tunneling induces significant internal forces in adjacent piles. The distribution of internal forces depends mainly on the position of the pile tip regarding the tunnel horizontal axis and the distance of the pile axis from the centre of the tunnel. Analysis of the interaction between tunneling and a group of piles reveals a positive group effect with a high reduction of the internal forces in rear piles. Copyright © 2002 John Wiley & Sons, Ltd. 相似文献
154.
魏续占 《地球科学与环境学报》1996,(2)
用多种分析手段分析了Sol-gel法制取的Al2O3系陶瓷涂层在烧结过程中的组织变化以及烧结后涂层的成分和组织结构;对涂层的高温抗氧化性、耐蚀性、耐磨性以及涂层与金属基体的结合力进行了测试,结果表明,Sol-gel法制取的Al2O3系陶瓷涂层由氧化物晶体、过渡相和玻璃体混合而成,涂层与基体之间有很好的结合力,金属基体的抗氧性、耐蚀性、耐磨性能有明显提高. 相似文献
155.
为探究覆水饱和砂土场地中土-群桩基础-桥梁结构体系动力相互作用规律,自主设计并制作了直(斜)群桩基础-桥梁结构物理相似模型,开展了不同地震动强度和不同特性地震波输入下的离心机振动台试验,分析了群桩基础-桥梁结构动力特性指标,探究了覆水饱和砂土地基超孔隙水压力发展规律和桩-土相互作用动力响应特性。研究结果表明:覆水的存在对地基土-桥梁结构体系的基本周期和阻尼影响很小,但会导致直群桩基础桥梁结构的振动幅值增加20%,而斜群桩基础桥梁结构的振动幅值降低10%;斜群桩基础模型阻尼比是直群桩基础模型的2倍。上覆水导致饱和砂土地基由受低频振动液化深度更大变为受高频振动地基液化深度更大,同时导致小震作用下促进超孔隙水压力发展,而大震作用下则反之。上覆水会增大桥梁上部结构的动力响应和桩身弯矩。上述研究结果可为覆水场地中桥梁工程抗震设计提供关键参考依据。 相似文献
156.
XIAO Shuhai 《《地质学报》英文版》2022,96(6):1821-1829
Systematic extinctions can leave major morphological gaps between living crown-group clades. Such morphological gaps would be perceived, from a neontological point of view, as major evolutionary transitions. In order to fill these morphological gaps and to map the evolutionary steps toward major evolutionary transitions, we need to integrate extinct stem-group taxa in phylogenetic studies. However, the recognition of stem group has not been widely adopted in the study of early animal fossils, despite that all fossils are stem groups at one level or another. Part of the difficulty is that stem groups may not have all features that collectively diagnose the respective crown group, and they can have unique (autapomorphic) features, making them tantalizingly similar to and frustratingly different from the crown group (e.g., stem-group eukaryotes can be prokaryotic and stem-group animals can be protistan). The need to embrace stem groups and to implement the PhyloCode, in order to achieve phylogenetic clarity and to offer key paleontological insights into the origin and early animal evolution, is illustrated in debates on several controversial Ediacaran and Cambrian fossils. 相似文献
157.
Haitaite-(La), (La, Ce)(U4+, U6+, Fe2+)(Fe3+, Al)2(Ti, Fe2+, Fe3+)18O38, is a new member of the crichtonite group. It is named after the Haita Village in the Miyi County of Sichuan Province, China, where the mineral was discovered. The mineral occurs as black opaque centimeter-sized aggregates in the external contact zone between the Neoproterozoic (~800 Ma) alkali feldspar granite and the Mesoproterozoic (~1700 Ma) micaschist. In the studied sample, haitaite-(La) is associated with other minerals, including ilmenite, magnetite, rutile, zircon, brannerite and uraninite. The new mineral is a black, metallic phase and has a Mohs hardness of 6, with a density of 4.99 g/cm3 (calculated) and 5.03 g/cm3 (measured). Haitaite-(La) is opaque in transmitted light and grayish-white under reflected light, with a reflectivity between 22.5% and 16.42% in the 400–700 nm band (SiC, in the air). The compositions of the mineral were measured by EPMA, the U4+/U6+ ratio was determined by X-ray photoelectron spectroscopy and the Fe2+/Fe3+ ratio was determined by M?ssbauer spectroscopy. Haitaite-(La) is trigonal, belongs to R3ˉ and has unit-cell parameters a = 10.3678(5) ?, c = 20.8390(11) ?, V = 1939.9(2) ?3, Z = 3. The crystalline structure is composed of octahedra with 9 layers of close-packed octahedra (M1, M3, M4, M5), tetrahedra (M2) and contains large 12-coordinated M0 sites. 相似文献
158.
The itabirite-bearing metasedimentary sequence from Morro Escuro Ridge comprises the basal units of the Espinhaço Supergroup and makes up a small tectonic inlier developed during one of the Brasiliano orogenic events (800-500 Ma), amongst horses of the Archean TTG gneisses, including sheared granites of the anorogenic Borrachudos Suite (∼1700 Ma). The metasedimentary rocks are comprised of low-to intermediate-amphibolite facies schists, quartzites, conglomerates and banded iron formation (itabirite) correlatable with the sequences of the Serro Group, which underlies the metasedimentary rocks of the Espinhaço Supergroup in the Serra da Serpentina Ridge. A maximum Statherian deposition age (1668 Ma) was established using SHRIMP U–Pb isotopic constraints on zircon grains from conglomerate and quartzite units overlying the itabirite. The itabirite is predominantly hematitic and its geochemical characteristics are typical of a Lake Superior-type BIF deposited in a platformal, suboxic to anoxic environment distant from Fe-bearing hydrothermal vents. Close to the contact zone with amphibolites of the Early Neoproterozoic Pedro Lessa mafic suite, an increase of the magnetite content and crystallization of metasomatic Mg-hornblende and Ce-allanite can be observed. These mineralogical changes developed preferentially along the igneous contact zone but are probably co-genetic with the formation of alteration haloes in zircon grains during the Neoproterozoic Brasiliano orogeny (506 ± 6 Ma). 相似文献
159.
研究了灰区间偏好的群体决策问题.在专家灰区间偏好群体意见集结过程中,常规的灰区间运算会产生决策信息的失真.为了避免这一缺陷,首先引入了灰区间调节参数的概念,通过建立求解调节参数的二次规划模型,确定专家灰区间判断的真值.建立了专家客观权重求解的二次规划模型,并给出了专家客观权重的最优解.此外,从另外一个角度同时考虑调节参数与客观权重,建立求解灰区间真值与专家客观权重的群体最优决策模型.气象敏感性行业专家群体评估决策的算例表明,决策策略是有效的. 相似文献
160.
Based on high precision measurements of the distances to nearby galaxies with the Hubble telescope, we have determined the
radii of the zero velocity spheres for the local group, R0 = 0.96±0.03Mpc, and for the group of galaxies around M 81/M 82, 0.89±0.05Mpc. These yield estimates of MT = (1.29±0.14)· 1012 M⊙ and (1.03±0.17)· 1012 M⊙, respectively, for the total masses of these groups. The R0 method allows us to determine the mass ratios for the two brightest members in both groups, as well. By varying the position
of the center of mass between the two principal members of a group to obtain minimal scatter in the galaxies on a Hubble diagram,
we find mass ratios of 0.8:1.0 for our galaxy and Andromeda and 0.54:1.00 for the M82 and M81 galaxies, in good agreement
with the observed ratios of the luminosities of these galaxies.
__________
Translated from Astrofizika, Vol. 49, No. 1, pp. 5–22 (February 2006). 相似文献