南海西缘断裂带右行走滑的地球动力学机制

南海西缘断裂带,北端始于17°30'N附近的海南岛南部,往南延伸止于北西走向的卢帕尔断裂,南北延伸长度约达1 600 km,十分壮观(见图1)。该断裂带除了其名称和延伸长度在不同研究者的文章中各有所不同[1—4]之外,其名称和作用至少在20世纪80年代初已得到广泛的应用,早已成习惯,如在《亚洲地质》[5]一书和杨树康等[1]、陈国达[4]等许多著名科学家的论著中不断地得到了应用。该断裂带的构造地位和作用得到地学界的普遍重视,到目前为止地学界基本上认为它就是印支亚板块与南海亚板块之间的区域性边界断裂。     

BTEX anomalies used as indicators of submarine oil and gas reservoirs

It is a conventional method for petroleum prospecting to generally use paraffin hydrocarbon as basic indexes of oil and gas. This conventional geochemical technology, however, shows some limits in the prospecting as paraffin is vulnerable to influences from human and biologic activities. Consequently, BTEX (short for benzene, toluene, ethyl benzene and xylem, which are direct biomarkers) among aromatic hydrocarbon series has been taken into account for the oil and gas prediction. Domestic and foreign study results demonstrate that BTEX is hardly disturbed and can well indicate oil and gas reservoirs. Based on measured data from a South China Sea area, the present authors have used self-developed visual assessment software for petroleum prospecting has been used to process data, strip background anomalies, and outline significant BTEX anomalies. By comparison with stratigraphic profiles of the target area, it is confirmed that BTEX is a good indication of marine oil and gas during the petroleum prospecting.     

蛋白质营养对高密度养殖凡纳滨对虾生长与免疫力的影响

在高密度养殖条件下,进行单因素随机设计动物试验.用5种饲料(蛋白质水平31%、35%、39%、43%、47%,以A～E组表示)分别投喂平均体质量6.2 g+0.2 g、平均养殖密度3.1 kg/m3的凡纳滨对虾(Litopenaeus vannamei),探寻蛋白质营养对虾生长、免疫、水质、抗胁迫的影响特征.结果表明:(1)中高蛋白质水平具有显著促进对虾生长的效果,随着蛋白水平的提高,特定生长率先增加后降低,饲料系数正好相反,D组两指标最佳,分另q为110.98%和2.54;C、D、E组差异不显著.(2)中高蛋白质水平有利于提高对虾多数免疫指标的活力,血淋巴中血细胞浓度、T-AOC活力、POD活力、总蛋白含量、白蛋白、血蓝蛋白含量,随着蛋白质水平提高先增加后降低,前5指标含量均以D组最高,比A组显著提高16.8%～33.9%;而血蓝蛋白含量C组最高,比A组提高15.0%.(3)高蛋白质水平有利于提高对虾SOD活力,也显著增强抗低盐胁迫的能力,但同时极显著加大了水环境中氨氮和亚硝氮的污染.(4)在我国北方集约化高密度养殖条件下,凡纳滨对虾中后期生长阶段适宜的饲料蛋白质营养水平为39%～43%.     

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Characteristics of dissolved organic matter in lakes with different eutrophic levels in southeastern Hubei Province,China

Dissolved organic matter (DOM) plays a crucial role in both the carbon cycle and geochemical cycles of other nutrient elements, which is of importance to the ma...     

企鹅珍珠贝游离珠培育技术的初步研究

2006 年 5 - 12 月,在广东省、湛江市、徐闻县芳华珍珠养殖场,采用贝龄 2 ～ 4 a 的企鹅珍珠贝作植核贝,以 1 ～ 3 a 贝作小片贝,进行游离珍珠培育试验.结果表明,植核母贝经 15 ～ 40 d 的术前处理,成活率为 95.33 % ～ 97.00 %;施术贝经过 6 个月培育后,吐核率为 63.00 % ～ 71.88 %,死亡率为 26.17 % ～ 35.00 %,成珠率为 1.95 % ～ 3.33 %.企鹅珍珠贝合适的植核母贝为 2 ～ 3 龄贝,小片贝为 1 ～ 2 龄贝.     

东亚地区春季一氧化碳的输送特征研究

以ECMWF ERA-40再分析资料构建的气象场为驱动场,利用全球三维大气化学模式MOZART-2,模拟了2001年3月大气污染物浓度的全球时空分布,并以一氧化碳(CO)作为示踪剂分析了春季东亚污染物向西太平洋地区输送的路线和机制.为了检验模拟结果的合理性,对TRACE-P 期间典型天气过程下的模拟结果与观测结果进行了比较.比较结果显示,模拟结果可以较好地再现2001年春季冷锋过境期间与东南亚深对流运动加强的天气形势下,东亚污染物向西太平洋地区输送的2大主要路径及其特征:(1) 污染物被冷锋系统提升后,在对流层中层向西太平洋快速传输;(2) 强烈的大气对流运动可以导致东南亚生物质燃烧产生的污染物在对流层上层向西太平洋输送.     

ICESat-2激光卫星与光学遥感影像融合水深测量

针对浅海测深的数据特点和应用需求,以我国南海甘泉岛为例,研究了利用ICESat-2(Ice,Cloud,and Land Elevation Satellite-2)激光卫星数据和光学遥感影像开展主被动融合水深测量的方法。首先通过信号点提取、水面/水底识别、水下点折射改正等步骤处理ICESat-2数据,获得水深值,随后以激光点作为控制,计算光学水深反演模型参数,最后由点及面地获取大范围高精度水深。实验表明,甘泉岛区域主被动融合测深中误差优于1.30m,基于激光卫星数据的主被动融合测深方法能够为浅水水深测量提供新手段。     

青藏铁路旅游线气候适宜性分析

本文利用10个气象站1991~2000年的气象观测数据,对青藏铁路旅游线的气候适宜性进行了评价。评价内容包括:生物气温指标、紫外辐射强度、大气含氧量以及障碍性天气等。得出如下结论:总的来看,青藏铁路沿线地区相对舒适的旅游气候条件集中出现于5~9月。该时段,生理气温舒适凉爽,空气含氧量比例较高,无炎热或热日,大风天气出现少。但是,紫外辐射较强,雷暴及冰雹出现的频率较高。旅游适宜期与适宜时段随海拔高度的上升而逐步缩短。位于铁路线两端的西宁、拉萨等地区的旅游气候条件最优,全年均较适宜旅游;五道梁、沱沱河、安多等高海拔地区的旅游适宜期较短,冬季的严寒和夏季(6、7月)的强紫外辐射对这些地区户外旅游活动的限制较大。     

Binary Star Fractions from the LAMOST DR4

Stellar systems composed of single, double, triple or higher-order systems are rightfully regarded as the fundamental building blocks of the Milky Way. Binary stars play an important role in formation and evolution of the Galaxy. Through comparing the radial velocity variations from multiepoch observations, we analyze the binary fraction of dwarf stars observed with LAMOST. Effects of different model assumptions, such as orbital period distributions on the estimate of binary fractions,are investigated. The results based on log-normal distribution of orbital periods reproduce the previous complete analyses better than the power-law distribution. We find that the binary fraction increases with Teff and decreases with [Fe/H]. We first investigate the relation between α-elements and binary fraction in such a large sample as provided by LAMOST. The old stars with high [α/Fe] dominate with a higher binary fraction than young stars with low [α/Fe]. At the same mass, earlier forming stars possess a higher binary fraction than newly forming ones, which may be related with evolution of the Galaxy.