Influencing factors for formation of urban and rural spatial structure in metropolis fringe area—Taking Shuangliu County of Chengdu in China as a case

With rapid urbanization process, the pace of urban sprawl has been quickened and most metropolises have experienced expansions in leaps and bounds in suburbanization, which has greatly changed the urban and rural spatial structure of the metropolis fringe area. In this paper, Shuangliu County is taken as a case, since it is a typical fringe area of Chengdu Metropolis. Based on Landsat TM images of Chengdu City and Shuangliu County obtained in 1985, 2000 and 2004, characteristics of urban and rural spatial structure in Shuangliu County were analyzed, such as core-periphery spatial structure and some obvious integration trends. Then the influencing factors for the formation of urban and rural spatial structure were identified, including some natural, social, economic and political factors. According to the discussion of this paper, Shuangliu County is undergoing a key transition and reform period. Its formation of urban and rural spatial structure was affected not only by such common factors as the location, natural background, industrial transition, migration, etc., but also by some unique factors such as city planning and policy guidance, which played an important role in accelerating its uneven spatial structure. The understanding of the role of the influencing factors would be useful for carrying out spatial management and development planning of metropolis fringe area.     

Molecular Characterization and Expression and DNA Methylation Analyses of a Galectin-Related Protein Gene from Cynoglossus semilaevis

Galectins,a family of ?-galactoside-binding proteins,participate in both innate immunity and adaptive immunity.This study identified one novel galectin-related protein from half-smooth tongue sole Cynoglossus semilaevis,which was designated as Cs GRP.The full-length c DNA of its encoding gene was 785 bp in length with a 528 bp open reading frame encoding a putative protein of 176 amino acids.The deduced Cs GRP contained a putative 131-aa galactoside-binding lectin domain and 3 critical residues responsible for carbohydrate binding(R~(93),W~(109) and R~(114)).Genomic structural analysis revealed that Cs GRP consisted of five exons and four introns.Cs GRP showed 68% similarity with Poecilia latipinna GRP and 67% similarity with Stegastes partitus GRP.Cs GRP showed the highest expression level in liver,although its expression was detected in all tested tissues.When challenged with Vibrio harveyi,the expression of Cs GRP was significantly down-regulated in liver(P 0.05).In addition,we found that in spleen and kidney of C.semilaevis,the Cp G island of Cs GRP showed significantly higher(P 0.05) methylation level in disease-resistant family of C.semilaevis(DR-Cs) than in disease-susceptible ones(DS-Cs).Our results suggested that Cs GRP may play important roles in the immune response of C.semilaevis.Moreover,DNA methylation patterns provided valuable data for understanding the relationship between epigenetic regulation and immunity,which would assist the animal genetic research and improve the animal breeding in the future.     

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空间同位模式支持下城市服务业关联发现及特征分析

空间同位模式分析是数据挖掘中一种常见的方法,可有效挖掘城市设施在空间位置上的关联特征,进而发现城市设施的分布规律.本文基于POI数据同位模式挖掘用来获取城市服务业空间关联结构:首先,通过邻近实例获取、同位候选模式存储与筛选,得到城市服务业二阶同位模式;然后,据此构造产业空间关联图,得到产业间的关联结构;最后,分别构造了...     

基于空间综合分析的长株潭城市群结构评价与优化策略

长株潭城市群空间特征及优化策略可作为我国多中心城市群空间优化的典型样本之一.本文运用多维度空间分析方法,对长株潭城市群空间展开现状测度与评价,尊重城市群阶段特征,选取针对性指标对比反映空间内在特征.在采用核密度法分析2013年和2017年湖南省152个区县第二产业与就业指标的空间变化后,得出长株潭城市群已初步形成空间—...     

利用ICESat/GLAS数据获取北极海冰出水高度的研究

利用ICESat激光测高卫星数据获取2003-10～2008-03北冰洋秋季与冬季海冰出水高度,结果与国外相关研究基本一致。出水高度数据的拟合结果表明,北极海冰出水高度以每年约2.3 cm的速度递减,该速度比此前的相关研究结果更快。在不同作者利用ICESat数据计算的北极海冰出水高度的对比中,不同方法得到的结果之间存在明显的系统误差。对引起系统误差的原因进行深入分析表明,高程滤波的窗口长度、确定海面高的范围以及海面观测值的选取方式都会使出水高度的计算产生cm级的误差。     

降雨对滑坡的影响与基于ANSYS的滑坡数值模拟研究

分析了四川理县一处山体滑坡2014-08～2015-08的监测数据。结果表明,滑坡处于缓慢发生中,滑移的主要方向指向山体旁的学校;1 a中3个监测点在该方向上的累积位移量分别为180 mm、262 mm和448 mm。分析降雨量资料发现,降雨对山体滑坡有延迟的影响。利用ANSYS软件对滑坡发生的过程进行数值模拟,并计算监测点的位移,结果与实际观测情况吻合较好,得到降雨量与弹性模量、密度、粘聚力、内摩擦角之间的关系。该数值模拟实验提供了一种预测滑坡的新方法。     

The evolution of the z distribution of normal neutron stars in the Galaxy

Under the two initial 1‐D one parameter velocity distribution forms (one is normal, the other is exponential), the z direction scale height evolution of normal neutron stars in the Galaxy is studied by numerical simulation. We do statistics for the cases at different time segments, also do statistics for the cumulative cases made of each time segment. The results show in the cumulative cases the evolution curves of the scale heights are smoother than in the each time segment, i.e., the cumulation improve the signal‐to‐noise ratio. Certainly the evolution cases are different at different Galactic disk locations, which also have very large difference from the average cases in the whole disk. In the initial stages of z evolution of normal neutron stars, after the beginning transient states, the cumulative scale heights increase linearly with time, and the cumulative scale height increasing rates have linear relationship with the initial velocity distribution parameters, which have larger fluctuation in the vicinity of the Sun than in the whole disk. We utilize the linear relationship of the cumulative scale height increasing rates vs. the initial velocity distribution parameters in the vicinity of the Sun to make comparison with the observation near the Sun. The results show if there is no magnetic decay, then the deserved initial velocity parameters are obvious lower than the present well known results from some authors; whereas if introducing magnetic decay, for the 1‐D normal case we can make consistence among concerning results using magnetic decay time values which are supported by some authors, while for the 1‐D exponential case the results show the lackness of young pulsar samples in the larger z in the vicinity of the Sun (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

北斗三号组网卫星数据质量分析及单系统定轨精度初步评估

选取2018-01-23起10 d内16个iGMAS测站观测数据,对北斗三号卫星的观测数据质量及BDS单系统精密定轨精度进行评估。初步结果表明,老信号B1I、B3I北斗三号卫星的信噪比略强于二号卫星,噪声与多路径基本相当,均在0.1 m量级,新卫星不存在星内多路径偏差。新信号B1C/L1/E1频点GPS信噪比最强,Galileo和BDS卫星相当,B2a/L5/E5a和B2b/E5b各系统基本相当;噪声及多路径方面,B1C/L1/E1频点GPS优于BDS、Galileo卫星0.1 m量级,B2a/L5/E5a和B2b/E5b各系统基本相当,均在0.1 m量级,新信号中北斗三号卫星星内多路径偏差基本消失。单系统精密定轨试验中,分别进行有/无GEO卫星策略、太阳光压模型ECOM 五/九参数策略的比较,并使用卫星激光测距数据进行独立检核。初步结果表明,有GEO卫星、ECOM五参数光压模型的定轨精度最好,C19号卫星7个重叠弧段的平均定轨精度在沿迹向、法向、径向的精度分别为32 cm、16 cm、8 cm,与试验卫星的定轨精度基本相当。     

Tracing the settlement region of massive floating green algae in the Yellow Sea

Outbreaks of large-scale green tides formed by Ulva prolifera in the Yellow Sea(YS)cause heavy ecological damages and huge economic losses.However,the ecological consequences of green tides remain poorly understood due to the lack of knowledge on the settlement region of massive green algae floating in the YS.In this study,we established a method to trace the settlement region of floating green algae,using 28-isofucosterol preserved in sediment as the specific biomarker for green algae.Sterols including 28-isofucosterol in surface sediment samples collected during an investigation in the YS and the Bohai Sea(BS)in August 2015 were analyzed using gas chromatography coupled with a mass spectrometer(GC-MS).Based on the content of 28-isofucosterol in sediment samples,the potential settlement region of loating green algae was identified in the sea area southeast to the Shandong Peninsula around the sampling site H06(122.66°E,36.00°N).This paper presents a first result on the settlement region of floating green algae in the YS for providing a solid basis to elucidate the ecological consequences of green tides in the area.