三门湾表层沉积物黏土矿物特征及来源分析

利用XRD方法分析了三门湾表层沉积物中的黏土矿物组成和含量,结合沉积物粒径趋势分析及长江和三门湾流域中小河流的黏土矿物组合特征,开展了三门湾沉积物的来源分析。结果表明,三门湾表层沉积物中黏土矿物以伊利石为主,其次为高岭石和绿泥石,蒙脱石含量最低。其中,伊利石高值区位于海湾中部,高岭石和绿泥石高值区分布在港汊附近,蒙脱石则在近岸呈斑块状分布。三门湾现代表层沉积物主要来源于长江入海物质,海湾周边短源山溪性河流带来的物质仅影响了河口近岸区。     

一种灰树花菌丝体多糖GF4F1的结构特征及其抗肿瘤活性

以灰树花发酵菌丝体为原料,经过提取分离纯化得到1种水溶性多糖GF4F1,经高碘酸氧化、Smith降解、甲基化、红外光谱（IR）以及核磁共振波谱（NMR）等分析表明,该多糖是1种β-1, 3／1,6-葡聚糖,且小鼠体内实验结果表明其具有良好的抗肿瘤活性。在1mg／kg时,对小鼠抑制率为67.3％。     

广西钦州湾百年来红树林演变的有机碳同位素和孢粉示踪及其影响因素

气候变化和人类活动制约下的红树林演变是一种长时间尺度效应,而沉积物则是记录这种响应的最佳档案。采用古生态学研究思路,选择有效的示踪参数是解读这一档案的有效途径。本文通过广西钦州湾红树林区1根柱状沉积物中有机碳同位素(δ13C)、C/N分析和孢粉鉴定,以沉积物中的红树林源有机碳贡献和红树植物孢粉组合为示踪参数,在210Pb年龄框架构建的基础上,通过对比研究红树林源有机碳贡献和红树孢粉组合特征,揭示百年来钦州湾红树林兴衰和群落演替规律;进而重塑其红树林演变历史:兴盛期(1864-1918年)、衰退期(1918-1968年)和低谷期(1968-2007年),这与土地替代、遥感分析和现场勘测数据较为吻合。结合气候变化和人类活动资料,发现钦州湾红树林的近期衰退主要源于人类活动的影响,尤其是虾塘围垦;而与气候变化关系不大。     

厚叶切氏海带多糖的提取分离及其结构表征

本文以厚叶切氏海带(Kjellmaniella crassi folia)为原料,经提取分离获得4种多糖(KW1,KW2,KA1和KA2).运用电泳、高效液相色谱(HPLC)、高效凝胶渗透色谱(HPGPC)及核磁共振氢谱(1H-NMR)法分别对其单糖组成、相对分子量(Mr)以及结构进行分析.结果表明,KW1与KA1是Mr为520 kD和430 kD且M/G(6.14和1.90)显著不同的褐藻胶;KW2是以岩藻糖(82％)为主的岩藻糖硫酸酯;KA2是以半乳糖(34％)、岩藻糖(27％)和甘露糖(21％)为主的杂聚硫酸多糖.KW2和KA2的Mr和硫酸基含量分别为536 kD和427 kD及30％和21％.经1 H-NMR分析表明,KW2的硫酸酯基主要存在于岩藻糖残基的C2和C4位.     

Investigation of the hydrate reservoir production under different depressurization modes

Abstract

Large reserves of natural gas hydrates exist, and the depressurization method has the greatest potential for gas hydrate reservoir recovery. Currently, the most commonly adopted depressurization simulation method is a constant bottom-hole pressure production scheme. This study proposes a new depressurization mode with decreasing bottom-hole pressure. The production characteristic was numerically investigated using this method. The results show the following: (1) As the depressurization exponent (n) decreases, the development effect improves, and production indexes including cumulative gas production/dissociation and gas-water ratio increase. However, the reservoir energy consumption is higher and the hydrate reformation is more severe. (2) Compared to the proposed depressurization mode, the hydrate production index of the constant bottom-hole pressure production (n?=?0) is better. However, the hydrate reservoir energy consumption is higher and the hydrate reformation is more severe using constant bottom-hole pressure production. (3) To achieve a balance between production and reservoir energy consumption during depressurization production, the bottom-hole pressure should be controlled by selecting a suitable depressurization exponent between n_min and n_max, which can be determined through numerical simulations.     

周期性饥饿对褶皱臂尾轮虫实验种群特征参数的影响

实验设置了一直投喂、周期性饥饿1,2,3,4d和一直饥饿6个处理组,采用轮虫单个体培养,检验周期性饥饿对褶皱臂尾轮虫(Brachionus plicatilis)实验种群特征参数的影响.结果表明:一直投喂组的生殖价最高,对轮虫种群的潜在增长最有利,随饥饿强度的增大,生殖价减小.不同处理下,轮虫个体寿命与其生殖期之间存在显著的正相关(r=0.747).轮虫在受到饥饿后,寿命略有增长,但不同处理对轮虫的平均寿命(10.8~13.1d)和生殖期(6.3~8.3d)均未达到显著差异(P>0.05).饥饿强度增大时,轮虫个体的总产幼数、总产卵量显著下降(P<0.05),产第1幼、最后1幼、第1卵、最后1卵时间显著延长(P<0.05);同时,种群参数的世代时间(T)随饥饿强度增加而增大,内禀增长率(r_m)、周限增长率(λ)和净生殖率(R₀)却明显下降.     

太阳光球磁通量南北不对称性研究

运用统计方法系统研究了1978-2002年太阳光球磁通量南北不对称性变化特征，发现其与太阳活动周有关．不对称值在太阳活动极小年要明显高于太阳活动极大年，并且磁通量变化总是由上升段的北半球占优逐渐过渡到下降段的南半球占优．另外运用小波变换方法详细讨论了这种不对称性变化可能存在的周期信息．     

Researches in China on the Effects of Tides on the Earth Rotation

In this paper the tidal phenomena on the Earth are concisely specified, including solid tides, ocean tides and atmospheric tides due to the luni-solar tide-generating force, and the Earth pole tide due to the motion of the Earth's rotation axis (polar motion); as well as their effects on the Earth rotation. The outcomes of scientific researches of Chinese astronomers on these topics are described in some detail. These researches deal with the mechanisms responsible for tidal effects on the earth rotation, and on the measurements of the Earth rotation parameters. Finally, the effects discovered by Chinese researchers on the measurements of the period and change in period of pulsars are discussed. These effects are very small in magnitude but not negligible.     

Mid-to-Far Infrared Spectral Energy Distribution of Galaxies in the Spitzer First Look Survey Field

We made model fitting to the mid-to-far infrared spectral energy distributions (SEDs) for different categories of galaxies in the main extragalactic field of the Spitzer First Look Survey with the aid of spectroscopic information from the Sloan Digital Sky Survey. We find that the mid-to-far infrared SEDs of HII galaxies, mixture type galaxies and LINERs can be well fitted by the one-parameter (α) dust model of Dale et al. plus the 13 Gyr dust-free elliptical galaxy model. The statistics of α values indicates that all these galaxies tend to be quiescent, although the HII galaxies are relatively more active than the LINERs. The mid- infrared SEDs of absorption galaxies are well fitted simply by the 13 Gyr dust-free elliptical galaxy template, and the near-to-mid infrared SEDs of QSOs can be represented by AGN NGC 5506.