北冰洋楚科奇海浮游细菌丰度和生产力及其分布特征

2012年夏季中国第5次北极科学考察期间,对北冰洋楚科奇海及其北部边缘海浮游细菌丰度和生产力进行了测定,并将其与环境因子进行了相关性分析。结果显示,楚科奇海浮游细菌丰度的变化范围为0.56×108~6.41×108 cells/dm3,平均为2.25×108 cells/dm3;细菌生产力介于0.042~1.92mg/(m3·d)(以碳计)之间,平均为0.54mg/(m3·d)(以碳计),与已有研究结果基本相当。陆架区细菌丰度和生产力要明显高于北部边缘区,但前者的单位细菌生产力则较低。与环境因子的相关性分析显示,细菌丰度与温度和叶绿素a浓度存在显著正相关(p0.01),表明北极变暖导致的海水升温及浮游植物生物量的增加均会促进细菌的生长,从而进一步提高细菌在海洋生态系统和碳循环中的作用。但陆架区的细菌生产力与环境参数均没有显著相关性,表明其影响因素较为复杂;生产力在北部边缘区则仅与叶绿素a存在显著正相关(p0.01),表明浮游植物生长过程产生的溶解有机碳(DOC)是细菌生长最为主要的碳源,碳源的单一可能制约细菌的生产从而导致该海域无冰状态下细菌丰度的增加不如预期,但融冰过程带来的大量DOC将促进细菌活性的增加。     

长江口九段沙潮沟系统分维研究

以长江口九段沙为研究区,采用2013年8月13日的Landsat-8遥感全色波段得到的九段沙潮沟分布图,利用Horton-Strahler原则将九段沙潮沟进行了分级。然后使用网格法对各个等级的潮沟进行了分维研究,计算了九段沙不同等级的每个潮沟左右两侧的维数值,并结合潮沟的宽度大小,对其维数值进行了比较和分析。研究结果表明,九段沙相同等级潮沟中,潮沟左侧维数的变化范围大于右侧,即潮沟左侧发育的复杂程度大于右侧;不同等级潮沟宽度的最小值变化幅度不大,但潮沟宽度的最大值变化幅度较大;不同等级潮沟宽度的变化和其潮沟左右两侧维数差值变化的相关性较小;不同等级潮沟,无论左侧还是右侧,潮沟维数大小随着潮沟的等级数和潮沟的平均宽度的增大而增大。     

天地图·河南影像数据关键技术研究

天地图·河南是"天地图"的有机组成部分保质保量实现天地图.河南影像数据一年更新两次目标,需要研究如何快速处理影像数据,提高工作效率,有必要从软件与硬件应用两个方面探讨影像数据处理关键技术。     

Purification of a Diatom and Its Identification to Cylindrotheca closterium

A diatom was purified with colony selection and continuous dilution methods. It was identified to Cylindrotheca closterium according to its morphological characteristics and rbc L and 18 s r RNA gene sequences. The alga was not sensitive to ampicillin and neomycin, but sensitive to chloramphenicol which inhibited its growth at concentrations ranging from 50 to 150 μg m L-1. The purified alga was easy to culture and its specific growth rate was 0.207 ± 0.002(d-1). It was resistant to pollution and could be harvested in an easy way. It was relatively high in lipid content(20.08% ± 0.67% of dry weight) and the combined amount of its 16:0 and 16:1(n-7), the most suitable resource of biodiesel, was as high as 64% of the total fatty acids, while the amount of polyunsaturated fatty acids reached 19.96%–20% of the total fatty acids. Thus the purified C. closterium can be cultured as a biodiesel producer or a nutrition supplement producer.     

智慧黄山时空大数据建设与应用实践

基于时空大数据技术、面向服务模式、高性能计算和分布式计算等相关理论和技术,本文设计并实现了时空大数据平台,集合了时空数据整合、处理、存储、分析、可视化等功能,并具备后台资源弹性分配和管理能力.规划了适合本地情况的时空大数据重点应用方向,基于大数据空间分析模型,分析了土地利用现状数据变化情况;运用机器学习的方法构建地价预测模型,实现了远期地价预测能力;利用大数据分析及存储手段,实现了基于手机信令数据的旅游景区流量分析.为黄山市提供了统一的时空大数据服务基础设施,并为智慧城市全面应用积累了经验.     

基于SRTM-ASTER融合数据的河网提取

在分析SRTM、ASTER GDEM数据源基本特征的基础上,融合了一种直接面向河网提取的数据——SRTM-ASTER,利用SRTM数据较高的垂直分辨率修正ASTER GDEM,弥补了SRTM水平分辨率上的不足;引入Landsat-8遥感卫星数据提取真实河网,分析在有(无)河网辅助条件下融合数据的提取效果,并以总长度、支流数目、套合差为特征指标进行分析.研究结果表明:1)SRTM-ASTER数据提取的河网能综合SRTM和ASTER GDEM数据的优势,提取精度较好,但河流长度以及支流数目有所减少;2)有河网辅助的条件下,经过AGREE算法进行河网纠正以后,提取结果的精度有显著提高.     

Evidence for high‐temperature fractionation of lithium isotopes during differentiation of the Moon

Lithium isotope and abundance data are reported for Apollo 15 and 17 mare basalts and the LaPaz low‐Ti mare basalt meteorites, along with lithium isotope data for carbonaceous, ordinary, and enstatite chondrites, and chondrules from the Allende CV3 meteorite. Apollo 15 low‐Ti mare basalts have lower Li contents and lower δ⁷Li (3.8 ± 1.2‰; all uncertainties are 2 standard deviations) than Apollo 17 high‐Ti mare basalts (δ⁷Li = 5.2 ± 1.2‰), with evolved LaPaz mare basalts having high Li contents, but similar low δ⁷Li (3.7 ± 0.5‰) to Apollo 15 mare basalts. In low‐Ti mare basalt 15555, the highest concentrations of Li occur in late‐stage tridymite (>20 ppm) and plagioclase (11 ± 3 ppm), with olivine (6.1 ± 3.8 ppm), pyroxene (4.2 ± 1.6 ppm), and ilmenite (0.8 ± 0.7 ppm) having lower Li concentrations. Values of δ⁷Li in low‐ and high‐Ti mare basalt sources broadly correlate negatively with ¹⁸O/¹⁶O and positively with ⁵⁶Fe/⁵⁴Fe (low‐Ti: δ⁷Li ≤4‰; δ⁵⁶Fe ≤0.04‰; δ¹⁸O ≥5.7‰; high‐Ti: δ⁷Li >6‰; δ⁵⁶Fe >0.18‰; δ¹⁸O <5.4‰). Lithium does not appear to have acted as a volatile element during planetary formation, with subequal Li contents in mare basalts compared with terrestrial, martian, or vestan basaltic rocks. Observed Li isotopic fractionations in mare basalts can potentially be explained through large‐degree, high‐temperature igneous differentiation of their source regions. Progressive magma ocean crystallization led to enrichment in Li and δ⁷Li in late‐stage liquids, probably as a consequence of preferential retention of ⁷Li and Li in the melt relative to crystallizing solids. Lithium isotopic fractionation has not been observed during extensive differentiation in terrestrial magmatic systems and may only be recognizable during extensive planetary magmatic differentiation under volatile‐poor conditions, as expected for the lunar magma ocean. Our new analyses of chondrites show that they have δ⁷Li ranging between ?2.5‰ and 4‰. The higher δ⁷Li in planetary basalts than in the compilation of chondrites (2.1 ± 1.3‰) demonstrates that differentiated planetary basalts are, on average, isotopically heavier than most chondrites.