银盘恒星运动学和化学丰度与银河系结构

大样本的银盘恒星的运动学数据和元素丰度特征是研究银河系结构及演化，尤其是银盘形成和演化的2个重要探针。本文首先介绍了银河系的总体结构特征，然后较详细的综述了以上2个探针的重要性。对我国LAMOST项目在研究银河系结构方面，尤其是银盘的形成和演化方面的能力作了合理的分析。     

星风吸积引起的钡星重元素超丰

首先指出目前星风吸积模型中理论上的不自洽，考虑到δｒ≠０，重新推导轨道参量变化方程，消去了理论上的不自洽．提出一个新模型：首次将星风吸积同内禀ＡＧＢ星核合成模型结合起来计算钡（Ｂａ）星的重元素超丰，并将计算结果与观测值进行了比较．各参量按标准情况取值时，计算结果不太理想．取Ｂｏｎｄｉｈｏｙｌｅ吸积率的０．５倍或取较大的星风速率时，对于较长轨道周期（Ｐ＞１０００天）的Ｂａ星，计算结果与观测值基本符合；而较短轨道周期（Ｐ＜６００天）的Ｂａ星，其重元素超丰机制可能是盘吸积     

原子吸收光度法测定金刚石钻头镀液中的主要成分

将原子吸收光谱法应用于电镀注保高含量组分分析。以空气－乙炔火焰次灵敏线测定镍，钴，锰，Ｎ２－Ｏ乙烯高温火焰测定硼，空气－乙炔火焰发射法测定钠，方法简便，快速，重现性好，加标回收率９６％－１０６％。已用于实际样品分析。     

延边东部五道沟岩群的单颗粒锆石SHRIMP U-Pb 年代学及其地质意义

通过对延边地区东部五道沟岩群黑云阳起石片岩的单颗粒锆石SHRIMP U-Pb年龄测定.获得21个单点年龄,其中包括7组谐和年龄和1组不谐和年龄.谐和年龄分别为1347.8 Ma、844.8 Ma、340.2～313.7 Ma(平均值为323±23 Ma,N=4,MSWD=0.23,置信度=0.88)、292.9～288.3 Ma(平均值=291±25 Ma,N=3,MSWD=0.031.置信度=0.86)、279.2～266.2 Ma(平均值为279±28 Ma,N=4,MSWD=0.031,置信度=0.86)、127.4～124.2 Ma(206Pb/208U年龄平均值为126.5±3.7 Ma,N=5,MSWD=0.12;置信度=O.97)、116.1～106.3 Ma(平均值为115±39 Ma,N=2,MSWD=1.2置信度=0.27),不谐和年龄的下交点年龄为(451±120)Ma、上交点年龄为(1811±400)Ma(MSWD=7.2);这一结果表明:阳起石片岩的原岩主要是来自中元古代、新元古代和早古生代的碎屑物,指示五道沟群的沉积成岩作用发生在石炭世(323±23 Ma),变质作用发生在晚二叠世(291±25 Ma),之后在279.2～266.2 Ma、126.5～106.3 Ma先后受两次岩浆用和蚀变作用的改造.     

唐山南堡开发区污水排海方案的优化选择研究

本文应用现场勘测和数据模拟相结合的方法，预测了开发区近期（２０００年）及远期（２０１０年）的开发建设对该海域的污染影响，探讨了对该海域污染影响较小且技术可行，经济合理的污水排海方案，为开发区的建设和海洋环境保护提供了科学依据和对策。     

同位素技术在海洋倾废区选划中的应用

本文从以往海洋倾废区选划中存在的问题出发，结合国内外海洋倾废区的选划实例，论述了同位素技术在海洋倾废区选划中的重要作用，为了提高倾废区的选划质量，作者建议尽快制定《海洋倾废区选划规范》，并将有关的同位素技术纳入该规范之中。     

雄性三倍体长牡蛎繁殖潜力的初步研究

国内外很多人做过三倍体长牡砺的诱导工作，但在三倍体性腺发育及配子活力方面的研究，目前仅见Ａｌｌｅｎ等１９８６年和１９９０年对三倍体的海螂和长蛎异常配子的发生报道。Ｃｏｘ１９９６年研究了悉尼岩牡蛎三倍体性腺发育情况，姜卫国等对三倍体合浦珠母贝的生殖腺进行了观察，李霞［１］对三倍体长牡蛎的性腺发育做了较系统的分析和总结。作者用流式细胞仪对长牡蛎Ｃｒａｓｓｏｓｔｒｅａ　ｇｉｇａｓ二、三倍体的性腺细胞进行了初步分析，回答了三倍体长牡蛎生殖潜力及性比方面的一些问题，为进一步研究三倍体长牡蛎的生长、繁殖、杂…     

Feeding of benthic foraminifera on diatoms and sewage-derived organic matter: an experimental application of lipid biomarker techniques

Foraminiferal ecology at sewage outfalls has been investigated in numerous field studies over the last 30 years. Foraminifera have been frequently used as biomonitors of sewage pollution since they are both abundant and ubiquitous. Sewage outfalls have been demonstrated to have both positive and negative effects on adjacent foraminiferal populations, but it has never been shown conclusively why sewage affects foraminifera in these ways. Such information on the impact mechanisms of sewage pollution is essential if foraminifera are to be used as sewage pollution biomonitors, and also to understand the ecology of these important protists. One possible cause of a positive effect is the direct consumption of sewage-derived particulate organic matter (POM) by the foraminifera themselves. However this hypothesis has never been tested experimentally. Here, lipid (fatty acid and sterol) biomarker techniques were applied to study the ingestion of two potential food items by the foraminiferan Haynesina germanica in the laboratory. An experiment was conducted to confirm that the laboratory conditions were conducive to the survival and feeding of the foraminifera. In this experiment, foraminifera were provided with the pennate diatom Phaeodactylum tricornutum, which was considered to be a suitable food source. After 2 weeks, a four-fold increase in the levels of the diatom fatty acid biomarker, 20:5(n-3), in the foraminifera suggested that they had fed actively on the diatoms and survived under the experimental conditions. These experimental conditions were used in the main experiment, where foraminifera were fed the POM from sewage. Lipid biomarker analysis indicated that H. germanica did not consume secondary treated sewage-derived POM. Neither fatty acid profiles in the sewage nor coprostanol, the diagnostic human faecal sterol, were detected in foraminifera after exposure to the potential sewage food source. However, foraminifera may have consumed bacteria associated with the sewage in the experiment. The findings are discussed in terms of current EU legislation on sewage treatment that has affected the composition of sewage discharges, and therefore possibly reduced the nutritive value of sewage to the marine benthos.     

Trophic accumulation and depuration of mercury by blue crabs (Callinectes sapidus) and pink shrimp (Penaeus duorarum)

Mercury concentrations in blue crabs (Callinectes sapidus) collected from an area of mercury-contaminated sediments in Lavaca Bay, TX, USA, are more than an order of magnitude greater than concentrations in penaeid shrimp from the same area. Laboratory feeding experiments using mercury-contaminated fish as food showed that both blue crabs and pink shrimp (Penaeus duorarum) could accumulate mercury concentrations comparable to those in their food in 28 days. Calculated mercury assimilation efficiencies averaged 76% for blue crabs and 72% for pink shrimp. Significant depuration of mercury by blue crabs was not observed during a subsequent 28-day period, but pink shrimp lost mercury at a rate of about 0.012 day-1. Model calculations predict biomagnification factors of mercury of about two to three at steady state for both species. The large difference in observed concentrations of mercury in field-collected blue crabs and penaeid shrimp does not result from differences in efficiency of mercury assimilation from their food or from differences in excretion rates. It is more likely the result of differences in residence times in the contaminated area and of differences in feeding habits.     

盘状星系结构与自转统计

通过对57个星系的光学和射电自转曲线等资料的分析,得出如下结论:(1)盘系沿哈勃序列从早型到晚型,其结构和自转等动力学量有系统的变化:星系核球与盘的质量比减小,自转速度达极大点r_m处速度V_m变慢、周期P_m增长,r_m相对于光学Holmberg半径r_H的位置外移,旋臂松卷,星系扁化。(2)星系诸动力学量在各形态型中的弥散与星系质量有关,较大质量星系的v_m和r_m较大,而k=V_m~2/r_m和β=r_H/r_m值较小。(3)潮汐作用也是影响星系动力学状态的重要因素,在同样形态型中潮汐星系有较大的k、β值和较小的r_m值。