锦州市规划区地质环境安全评价研究

地质环境问题是影响城市国土空间安全开发利用的重要因素,在城市规划开发阶段开展地质环境综合评价可有效控制地质灾害风险。锦州市规划区尚处于开发前期,本文基于该规划区的地质条件和开发需求,构建了地质环境安全评价指标和评价方法体系,基于主导因素综合法开展了地质环境安全综合评价。根据评价结果,锦州市规划区地质环境安全程度可划分为3级,空间分布上以相对安全区为主,其次为次不安全区和安全区。按照空间位置和区域构造稳定性、地质灾害易发性等不同成因划分为23个亚区,并指出了每个亚区安全程度主要影响因素。该评价结果反映了锦州市规划区的地质环境安全程度,确定了影响地质环境安全问题的关键因素,有助于规避该区国土空间规划开发可能面临的地质灾害风险。     

Palaeoproterozoic tectonothermal evolution and deep crustal processes in the Jiao‐Liao‐Ji Belt,North China Craton: a review

The Palaeoproterozoic Jiao‐Liao‐Ji Belt is located in the eastern margin of the Eastern Block of the North China Craton. In this paper, we synthesize the tectonothermal evolution and deep crustal processes in the Jiao‐Liao‐Ji Belt based on recent information. A mantle plume‐related underplating from 2.53 to 2.36 Ga is envisaged which led to the emplacement of the 2.47–2.33 Ga alkali granite plutons and mafic dyke swarms, followed by the development of the Jiao‐Liao‐Ji Rift and bi‐modal volcanism. The underplating resulted not only in different sedimentary environments in the upper crust, but also in a differentiation of the initial thermal structure in the rift. This controlled the metamorphism and style of P‐T‐t paths in the different parts of the rift. Subsequent underplating resulted in the emplacement of the A‐type Liaoji granites of ca. 2.17 Ga in the lower crust, and the formation of associated pegmatites of 2.2 and 2.0 Ga, together with the development of a bedding‐parallel extension. However, the main orogeny occurred between 1.93 and 1.88 Ga with closing of the rift, compressional deformation and high‐pressure granulite metamorphism in the southern part of the orogen. Subsequently, lithospheric blocks were possibly delaminated at ∼1.85 Ga; anorogenic magmatic rocks such as rapakivi granite, alkaline granites and syenite were intruded, and pegmatite veins and mafic dyke swarms were emplaced cross‐cutting all the earlier structural traces. We identify that the underplating styles, collision processes and delamination types in the deep lithosphere controlled the tectonothermal evolution of the crust in the Jiao‐Liao‐Ji region. Copyright © 2011 John Wiley & Sons, Ltd.     

峰峰矿区磁西三号勘查区地温异常分析

磁西三号勘查区详查阶段钻孔全部进行了井温测量工作,发现区内2、4号煤层处在高温热害区内,且同一水平地温变化较大,2号煤层-800m水平地温最大差值为5.1℃,显示勘查区可能存在地温异常。通过对钻孔测温资料的分析研究,确定本区地温梯度在1.8~2.6℃/100m,与峰峰矿区基本一致;高温区的出现是由于煤层埋藏深度加大和岩浆岩侵入带来的附加热效应而导致地温增加。结果认为,本区为正常地温背景下的高温热害区。     

The teratogenic effects of sediments from the Yangtze Estuary and adjacent bay, China, on frog embryos

In recent decades, the Yangtze (Changjiang) Estuary has suffered great environmental changes due to intensive human activities in the Yangtze River basin. This study assessed the ecotoxicity of sediments from the Yangtze Estuary with the frog embryo teratogenesis assay—Xenopus (FETAX). The results showed that the sediment extracts induced multiple malformations in embryos of Xenopus tropicalis. In the embryos treated with nearshore extracts, abnormal eyes, narrow fins and hypopigmentation were the dominant phenotypes, followed by enlarged proctodeums. In these embryos, the percentages of total malformations were greater than 50 % at five sampling sites and less than 40 % at the other seven sites. However, in the embryos treated with the offshore extracts, elongation of the proctodeums was the dominant phenotype, followed by bent tails. The percentages of total malformations ranged from 25 to 45 %. Comparatively, the embryos treated with extracts from the nearshore zone showed a greater variety of phenotypes than those treated with extracts from the offshore zone. These results suggest that the sediments showed high teratogenicity to the amphibian embryos. The results also indicate that the teratogencity to X. tropicalis embryos is a useful indicator of the pollution of sediments.     

SCI/SSCI期刊与中文权威核心期刊论文的学术价值评价——基于地理工作者的感知分析

进入信息全球化时代,SCI/SSCI 论文越来越成为中国各高校及科研院所等单位衡量其基础研究实力的评价标准,甚至出现“唯‘SCI/SSCI’论”的现象,中文权威核心期刊论文的学术价值评定和认可度则相应降低,这在一定程度上对中文权威核心期刊的发展造成了不小的冲击。基于探索性因子分析,构建了中文权威核心期刊论文学术价值认可度的结构方程假设模型,以地理科学工作者为例,通过验证性因子分析,实证研究了地理工作者对中文权威核心期刊论文学术价值认可度的影响因素。结果显示：① 学术成果影响力是影响中文权威核心期刊论文学术价值认可度的关键因素,科研评价和学术地位认定政策及学术影响力评价是影响中文权威核心期刊论文学术价值认可度的重要因素;② 学术成果影响力对认可度影响程度最大,其影响路径系数为0.52,其次为学术影响力评价,路径系数为0.25,科研评价和学术地位认定政策影响程度较小;③ 学术成果影响力和学术影响力评价与认可度表现为正相关关系,而科研评价和学术地位认定政策与认可度之间则表现为负相关关系。最后,提出了增强科研工作者对中文权威核心期刊论文学术价值认可度的相关对策,以期提升作者发表中文权威核心期刊论文的意愿度,来促进中文权威核心期刊的持续发展。     

海南岛早古生代大地构造格局:来自志留纪早期碎屑锆石年代学的约束

北东向乐东-定安断裂的具体位置及演化对海南岛大地构造单元划分及构造演化研究意义重大.本文采用碎屑锆石年代学方法,分析了乐东-定安断裂南西段两侧志留纪兰多维列世沉积物物源的特征及其差异,并讨论其中蕴含的大地构造意义.研究结果表明东方江边娜姆河地区志留纪兰多维列世陀烈组中碎屑锆石年龄介于1457～3124 Ma之间,显示1...     

Neutrino Dominated Accretion Flow Around a Strange Star

The “strange star - NDAF” model (NDAF: Neutrino Dominated Accretion Flow) is proposed as an alternative central engine of gamma-ray bursts for unifying the interpretation of the prompt emission and postburst activities of gamma-ray bursts. The structure of NDAF around a strange star is calculated. Different from other central compact objects, the strange star will feed back the phase transition energy of strangization on the accretion flow, with neutrinos as energy carriers. The friction between NDAF and strange star is ignored in this paper. The results indicate: firstly, the structure of NDAF around a strange star is sensitive to accretion rate; secondly, if accretion rate is larger than 0.18 M_? s^-1, the “strange star - NDAF” model can unify the explanation on the prompt emission and postburst activities of gamma-ray bursts, and the range of allowable accretion rates is wider than that in frictionless “neutron star - NDAF” models; thirdly, the range of annihilation energy of “strange star - NDAF” model is very wide, when the accretion rate is higher than 0.3 M_? s^-1, the annihilation energy is greater than 10⁵¹ erg; finally, if the accretion rate is greater than 0.3 M_? s^-1, the annihilation energy of “strange star - NDAF” model is larger than what of “black hole - NDAF” model at the same accretion rate by more than one order of magnitude, it is favorable to explaining some extremely energetic gamma-ray bursts.     

A Research on the Characteristics of Light Variation of Blazar 3C 273 in 2-10 keV

From the original observed data of RXTE (Rossi X-ray timing explorer), the data of 3C 273 in the X-ray band of 2-10 keV from February 2, 1996 (MJD 50115) to August 27, 2007 (MJD 54339) are analyzed. The photon spectral indexes and corresponding fluxes of the observational data from 1010 observations are obtained in total. The average time of each observation is 1666.76 seconds. By analyzing the spectral variation and behavior of the light variation of 3C 273 in the hard X-ray band of 2-10 keV during observational periods, it is found that there was a significant anti-correlation between the photon spectral index Γ and flux lgF_{2∼10 keV} in February 2000, March and April 2003, February, March and July 2004, as well as 2006 and 2007. During the observational periods in 1999 and from 2000 to 2007, there was also a significant anti-correlation between the monthly average behaviors of Γ and lgF_{2∼10 keV}. From the quantitative analysis of the behavior of light variation in the entire observational period, several relatively large light variations are found. The evidence of the existence of the Fe emission line with average width of 93.85±21.49 eV is also found by fitting a part of the spectra. Through analyzing the intensity of the light variation and features of Fe emission line, it is found that 3C 273 has some characteristics of blazars and Seyfert galaxies simultaneously.     

A photometric study of the detached binary WY Hydrae with twin components

We present a multicolor photometry for the eclipsing binary WY Hydrae, observed on four nights of 2008 December. From our new observations and Carr’s data, the photometric solutions were deduced by using the updated W–D program. The results show that WY Hya is a detached binary with a mass ratio of q = 0.970(±0.005).By analyzing the O–C curve, it is found that there exists either a continuous period increase or a cyclic variation. From Eq. (2), the orbital period of WY Hya secularly increases at a rate of dP/dt = +3.56(±0.37) × 10^?7 days/yr, which may be interpreted by some mass transfer for the near-contact configuration or tidal dissipation. From Eq. (3), the period and semi-amplitude of the periodic oscillation are P₃ = 95.4(±4.2) yr and A = 0^d.0087(±0^d.0003), respectively. This may be likely attributed by light-time effect via the presence of the assumed third body. Assumed in the coplanar orbit with the binary, the mass of the third body should be M₃ = 0.18 M_⊙. If the unseen additional companion exists, it will extract angular momentum from the binary system. Finally, WY Hya with high fill-out factors (i.e., f_1,2 > 80%), may evolve into a semi-detached configuration.     

Beyond density: municipal expenditures and the shape and location of development

A clear understanding of the relationship between development patterns and municipal expenditures is complicated by how one chooses to quantify these patterns. Extant literature often employs a single density measure to capture the low-density nature of sprawl. While density provides an intuitive link to economies of scale and congestion costs, it fails to capture other spatial characteristics of sprawl related to centrality, connectedness, and mixed use that may influence municipal expenditures according to Smart Growth and New Urbanism advocates. This study uses Massachusetts orthoimagery data to construct multidimensional measures of residential and commercial land use patterns. Municipal expenditures associated with public works, fire, and police are regressed on multidimensional measures of land use as well as a number of demand controls. Findings indicate that economies and diseconomies do exist with respect to the multidimensional metrics considered. Support is mixed for development patterns emphasized by Smart Growth and New Urbanism advocates.