富含古罗糖醛酸的褐藻多糖生产菌株的构建

为获得古罗糖醛酸(Guluronate)含量高的细菌胞外褐藻多糖,利用PCR从海洋细菌Pseudomonassp.QDA中克隆了其甘露糖醛酸C-5差向异构酶基因(algG),连接入质粒pMF 54Km,构建了重组表达载体pMF54 Km-algG。利用三亲接合法将pMF54 Km-algG转入菌株QDA中,获得algG过量表达重组菌株QDA-G1。H-NMR测定结果表明,QDA-G所产的褐藻多糖中β-D-甘露糖醛酸(M)与它的C-5差向异构体α-L-古罗糖醛酸(G)的比值为0.38,G的质量分数达到74.2%,比野生菌株QDA提高了26.4%。且重组菌株遗传稳定性良好,连续传代20代后,M/G的比值无明显变化。     

邻近算法在微地震震源位置和一维速度模型同时反演中的应用

微地震事件的空间分布可以用来监测水力压裂过程中裂缝的发育情况.因此,震源定位是微震监测中重要的环节.震源定位依赖准确的速度模型,而震源位置和速度模型的耦合易导致线性迭代的同时反演方法陷入局部极小值.邻近算法作为一种非线性全局优化算法,能够最大程度地避免陷入局部最优解.本文将邻近算法应用于单井监测的微震定位和一维速度模型...     

新疆库车盆地钾盐科探1井含盐系地球化学特征及找钾指示

在盐湖沉积演化过程中,钾盐矿物在盐类沉积的中晚期阶段才开始析出。因此,研究含盐系盐类的沉积地球化学特征,不仅可以从侧面获取岩盐的沉积物源和成盐古卤水蒸发浓缩程度等地球化学信息,而且更能揭示古盐湖钾盐富集趋势。文章通过对库车盆地钾盐科探1井钻取的岩芯样品进行高精度采样测试,得出岩盐中Mg×103/Cl、K×103/Cl、Li×103/Cl与K+、Mg2+、Li+、Ca2+、Cl-含量的垂向变化规律。并与库车盆地其他钻孔中的岩盐含钾性进行对比,同时,依据钻井剖面岩性特征,与潜江凹陷和大汶口凹陷含盐系剖面进行对比,论述研究区成盐的地球化学特征,对其钾盐成矿前景进行分析和评价。     

菏泽5.9级地震前后水准测量与承压水变化关系的研究

利用深层承压水头观测结果,对东明——菏泽长水准测线8——9号测段的高差变化进行了回归计算和相关分析。认为菏泽市城区9号测点下沉的主要原因是受深层承压水头变化的影响。排除地下水影响因素后证实,1983年11月7日菏泽5.9级地震前后仅3mm左右的升降变化,表明9号测点对这次中强地震仅能反映微弱的形变信息量。     

Integrating lysimeter drainage and eddy covariance flux measurements in a groundwater recharge model

Abstract

Field-scale water balance is difficult to characterize because controls exerted by soils and vegetation are mostly inferred from local-scale measurements with relatively small support volumes. Eddy covariance flux and lysimeters have been used to infer and evaluate field-scale water balances because they have larger footprint areas than local soil moisture measurements. This study quantifies heterogeneity of soil deep drainage (D) in four 12.5-m² repacked lysimeters, compares evapotranspiration from eddy covariance (ET_EC) and mass balance residuals of lysimeters (ETwb_Lys), and models D to estimate groundwater recharge. Variation in measured D was attributed to redirection of snowmelt infiltration and differences in lysimeter hydraulic properties caused by surface soil treatment. During the growing seasons of 2010, 2011 and 2012, ETwb_Lys (278, 289 and 269 mm, respectively) was in good agreement with ET_EC (298, 301 and 335 mm). Annual recharge estimated from modelled D was 486, 624 and 613 mm for three calendar years 2010, 2011 and 2012, respectively. In summary, lysimeter D and ET_EC can be integrated to estimate and model groundwater recharge.

Editor D. Koutsoyiannis     

Detection of nighttime sea fog/stratus over the Huanghai Sea using MTSAT-1R IR data

A dual channel difference (DCD) method is applied to detect nighttime sea fog/stratus over the Huanghai Sea using the infrared (IR) data of shortwave (3.5–4.0 μm) and longwave (10.3–11.3 μm) channels from the Multi-functional Transport Satellite (MTSAT)-1R, i.e., shortwave minus longwave brightness temperature difference (SLTD). Twenty-four sea fog events over the Huanghai Sea during March to July of 2006 and 2007 are chosen to determine a suitable value of SLTD for nighttime sea fog/stratus detection, and ...     

北京一号小卫星图像镶嵌处理技术研究

介绍北京一号小卫星数据的特点及应用情况,分析了卫星图像镶嵌处理技术流程,对其中的技术难点,如去条带处理、几何校正、图像拼接及色彩平衡等进行了重点探讨并提出解决办法。利用北京一号小卫星数据将两幅多光谱影像进行了镶嵌处理,得到了一幅覆盖整个研究区的新影像,镶嵌影像色彩丰富、层次感好、信息量大。     

一种带自由面的三维船体贴体网络的数值生成

本文提出了一个生成自由面的三维船体贴体网格的数值方法。文中以静水面以上的船体型线作为描述非定常自由面的计算网格域，进一步完善了我们以往开发的无法考虑兴波与静水面以上的船体型线相互作用对船舶粘性流动影响的网格生成方法。静水面以上的初始自由面网格分别沿船面法线η及切线ζ方向的曲线长的指数进行分布，即可极方便地调节自由面在船面及静水面附近的网格间距，也保证了在数值离散三维Ｐｏｉｓｓｏｎ方程时具有相当好的收敛性。这种方法的特点是计算量相当小，尤其能极方便地控制网格在船面簿粘性层中及静水面附近的分布。以Ｓｅｒｉｅｓ６０船模作为计算算例，带自由面的网格分布是相当满意的     

A unique Galactic planetary nebula with a [WN] central star

We report the discovery of the first probable Galactic [WN] central star of a planetary nebula (CSPN). The planetary nebula candidate was found during our systematic scans of the AAO/UKST Hα Survey of the Milky Way. Subsequent confirmatory spectroscopy of the nebula and central star reveals the remarkable nature of this object. The nebular spectrum shows emission lines with large expansion velocities exceeding 150 km s⁻¹, suggesting that perhaps the object is not a conventional planetary nebula. The central star itself is very red and is identified as being of the [WN] class, which makes it unique in the Galaxy. A large body of supplementary observational data supports the hypothesis that this object is indeed a planetary nebula and not a Population I Wolf–Rayet star with a ring nebula.     

重磁异常正反演可视化实时方法技术改进

摘 要 给出了2∙5D 多边形截面棱柱体重磁异常的简化表达式及其偏导数;提供了实用的可 视化模型建立、修改、实时正反演中的一些具体方法技术。借助这一操作方便、功能强大的 图形化实时反演系统‚资料解释工作者可以综合利用各种地质资料对计算过程实现引导和控 制‚使其解释思想及技术方案得到充分体现‚从而提高计算速度和质量。