基于灰度共生矩阵的DEM地形纹理特征量化研究

 DEM的地形纹理以其表达地形表面的纯粹性与分析数据的可派生性受到越来越多关注。本文选取陕西省10个不同地貌类型区的25m分辨率DEM数据,引入空间灰度共生矩阵(GLCM)对地形表面纹理特征进行定量分析。研究表明,25m分辨率DEM数据的GLCM模型适宜分析间距是大于等于3个栅格大小。各纹理参数中,相关度可用于地形纹理的方向性量化;方差、差的方差、对比度可用于对地形纹理的周期性分析;熵、二阶角矩、逆差矩可用于对地形纹理的复杂性分析。在DEM及其派生数据中,光照模拟数据计算的各纹理参数的平均变异系数最高,表明光照模拟数据最适合于地形纹理特征的量化研究。同时本文提出了一种多参数综合的地形纹理量化方法,通过运用综合周期性和综合复杂性两个指标对不同地形区量化分析,结果表明,这两个指标对不同地形形态响应显著,可用于地形形态分类与识别研究。     

Heritability and genetic correlation of survival in turbot (Scophthalmus maximus)

We analyzed the survival data of the offspring from 21 sires and 42 dams of turbot. The results show that the cumulative survival rates for turbot from 2 to 18 months range from 17.5% to 28.5%; main mortality occurred during months 2–5; and the highest survival rates of families were 97.9%, 98.8%, 99.4%, 99.7% during months 2–5, 5–6, 6–8, 8–11, and 11–18, respectively, and 99.5%, being 53.5%, 23.8%, 19.5%, 14.9%, and 13.2% higher, respectively, than the mean values in each period. In all periods, the estimated heritabilities for survival were very low without significant difference from zero (P≫0.05) (values ranged from 0.06 to 0.12), indicating low additive genetic effects. The genetic correlations of survival among families in different periods were all positive, but low in magnitude (values range from 0.03 to 0.31). Genetic correlations between long-term survival and other periods’ survival had negative values (−0.06 and −0.15) and three positive values (0.16, 0.12 and 0.14). Genetic correlations between survival and weight were all positive, except for survival at months 2–5 and weight at 18 months, which was not significantly negative (−0.18).     

近20年来宜兴市域水稻土有机碳动态及其驱动因素

中国农业土壤有机碳的变化一直是国内外农业与全球气候变化研究中十分注意的问题。一些研究提示20世纪末以来我国水稻土尤其是太湖地区水稻土的有机碳储存出现了增长趋势。文章选择了2002年对江苏省宜兴市市域范围水稻土的61个土壤监测点进行系统采样和土壤分析,并与该市分别于1983年和1994年进行的土壤肥力调查结果相对比,从县市区域尺度分析、评价了近20年来太湖地区水稻土表土有机碳储存的变化。尽管20世纪80年代初以前土壤有机碳含量变化以下降为主,但20年来该市域内水稻土有机碳总体上呈上升趋势。统计表明,4个主要土属的表土有机碳密度的增幅以下序递增:湖白土(-2.80tChm2)2)2)2),因而全市74.2×103hm2水稻土表土的总有机碳库从1983年的1.37Tg增加到2002年的2.20Tg。该市水稻土的平均固碳速率达到0.5～0.8tChm2a,这种快速固碳作用与20世纪80年代以来土壤中氮素的富集、秸秆还田的推广和90年代以来该地区不断扩大的冬季休闲有关。目前该市水稻土的固碳潜力仍很大,太湖地区的高产高投入农业不能排除在碳固定上的积极意义。然而,这种快速固碳作用的土壤过程和机理值     

阿尔金成矿带的归属及成矿特征

合理划分成矿区带对矿产资源预测评价和勘查具有指导价值,而正确认识构造单元性质和成矿时期的构造环境是成矿带划分的重要前提。本文从地质建造、地球物理、卫星遥感等多角度全面分析了阿尔金山的内部组成及其边界断裂特征,认为阿尔金山原属于南塔里木地块的组成部分,阿尔金造山带是在古老地块基础上活化以后形成的特殊造山带,其特点明显不同于秦祁昆造山系,阿尔金成矿带应划归塔里木成矿省。阿尔金成矿带可进一步划分为三个次级成矿单元:红柳沟-喀腊大湾(裂谷)成矿亚带主要形成海相火山岩型铅锌矿、火山-沉积变质型铁矿;阿尔金(陆缘地块)成矿亚带主要形成石棉矿和玉石矿;迪木那里克-苏巴里克(裂陷槽)成矿亚带则以沉积变质型铁矿和石棉矿为主。     

The Manyas fault zone (southern Marmara region,NW Turkey): active tectonics and paleoseismology

The Manyas fault zone (MFZ) is a splay fault of the Yenice Gönen Fault, which is located on the southern branch of the North Anatolian Fault System. The MFZ is a 38 km long, WNW–ESE-trending and normal fault zone comprised of three en-echelon segments. On 6 October 1964, an earthquake (Ms = 6.9) occurred on the Salur segment. In this study, paleoseismic trench studies were performed along the Salur segment. Based on these paleoseismic trench studies, at least three earthquakes resulting in a surface rupture within the last 4000 years, including the 1964 earthquake have been identified and dated. The penultimate event can be correlated with the AD 1323 earthquake. There is no archaeological and/or historical record that can be associated with the oldest earthquake dated between BP 3800 ± 600 and BP 2300 ± 200 years. Additionally, the trench study performed to the north of the Salur segment demonstrates paleoliquefaction structures crossing each other. The surface deformation that occurred during the 1964 earthquake is determined primarily to be the consequence of liquefaction. According to the fault plane slip data, the MFZ is a purely normal fault demonstrating a listric geometry with a dip of 64°–74° to the NNE.     

剖面法测量近岸水体遥感反射率的新方法

光学剖面法是测量遥感反射率的首选方法。根据我国近岸水体的特点,提出采用下行辐照度剖面补偿剖面测量时环境影响的方法,估算水面之下遥感反射率[rrs(λ)]。从对实际测量数据的应用效果可见,同站位多次测量的rrs(λ),其相对偏差可控制在10％之内。     

尾矿砂的动力特性研究

目前国内许多尾矿坝的初始坝本身不透水且无排渗设施,因而整个尾矿坝体浸润线很高,坝内大部分尾矿砂处于饱和状态。在动荷载的作用下,这些尾矿砂的动力特性对尾矿坝的安全稳定具有重要的意义。本文利用液压式振动三轴仪,研究了某尾矿坝内尾矿砂的动力特性,讨论了影响尾矿砂液化的因素。     

Evaluation of site effects in the Aterno river valley (Central Italy) from aftershocks of the 2009 L��Aquila earthquake

A temporary network of 33 seismic stations was deployed in the area struck by the 6th April 2009, Mw 6.1 (Scognamiglio et?al. in Seism Res Lett 6/81, 2010), L??Aquila earthquake (central Italy), with the aim to investigate the site amplification within the Aterno river Valley. The seismograms of 18 earthquakes recorded by 14 of the 33 stations were used to evaluate the average horizontal to vertical spectral ratio (HVSR) for each site and the standard horizontal spectral ratio (SSR) between a site and a reference station. The obtained results have been compared to the geological and geophysical information in order to explain the resonance frequencies and the amplification levels with respect to surface geology of the valley. The results indicate that there is no uniform pattern of amplification, because of the complex geologic setting, as the thickness and degree of cementation of the deposits is highly variable.     

边坡岩体疏干巷道排水动态过程的数值模拟

渗流数值计算是岩体排水设施和仿真模拟、动态分析、效果评价及预测的有效工具。应用边界元数值方法模拟研究了巷道疏干边坡地下水的动态过程。结果表明,岩体的渗透系数张量、可疏干孔隙率对疏干排水效果及其动态过程变化产生显著影响。同时可见边界元数值方法模拟断面尺寸较小的排水设施时,十分有效。     

Few Comments on the Relation Between the Initial Proto-planetary Disc Model and the Oort Cloud Formation

A fraction of small bodies from the once existing proto-planetary disc was ejected, by the giant planets, to large heliocentric distances and start to build the comet Oort cloud. Considering four models of initial proto-planetary disc, we attempt to roughly map a dependence between the initial disc’s structure and some properties of the Oort cloud. We find that it is difficult to construct the proto-planetary disc if (i) the amount of heavy chemical elements in Jupiter and Saturn is as high as currently accepted and (ii) the total mass of the minimum-mass solar nebula is assumed to be lower than $\approx0.05\,\hbox{M}_{\odot}.$ The behaviour of the Oort cloud formation does not crucially depend on the initial disc model. Some differences in its structure are obvious: since the cloud is known to be filled mainly by Uranus and Neptune, the efficiency of its formation is higher when the initial amount of particles in the Uranus-Neptune region is relatively higher. A significantly large number of Jupiter Trojans in our simulation appears, however, only in the case of the initially non-gapped disc, with the particles situated also close to the Jupiter’s orbit.