4种重金属离子对海洋三角褐指藻生长影响的研究

于１９９３年４月－１９９３年５月以Ｚｎ＾２＋，Ｃｄ＾２＋，Ｐｂ＾２＋，Ｃｕ＾２＋不同浓度的海水对三角褐指藻进行生长影响的研究。实验表明，Ｃｕ＾２＋对三角褐指藻生长的毒性最大，其９６ｈＥＣ５０为０．０１７ｍｇ／Ｌ。Ｐｂ＾２＋的毒性最小，其９６ｈＥＣ５０为０．４６８ｍｇ／Ｌ。４种重金属离子的毒性顺序是Ｃｕ＾２＋＞Ｃｄ＾２＋＞Ｚｎ＾２＋＞Ｐｂ＾２＋，除Ｃｄ＾２＋外，其他３种金属离子对该单细胞藻的生长安全     

The effects of immobilization on physiology and ultrastructure of unicellular alga Platymonas subcordiformis

ＴｈｅｅｆｆｅｃｔｓｏｆｉｍｍｏｂｉｌｉｚａｔｉｏｎｏｎｐｈｙｓｉｏｌｏｇｙａｎｄｕｌｔｒａｓｔｒｕｃｔｕｒｅｏｆｕｎｉｃｅｌｌｕｌａｒａｌｇａＰｌａｔｙｍｏｎａｓｓｕｂｃｏｒｄｉｆｏｒｍｉｓ￥ＺｈａｎｇＸｕｅｃｈｅｎｇ；ＷｕＸｉａｏｎａｎａｎｄＬｉ...     

Semi-probabilistic method for evaluating system redundancy of existing offshore structures

Various forms of recently appeared concepts of structure system redundancy are studied. A new measure for existing structure redundancy is proposed. By introducing the concept of structure system failure at the mechanism level and the concept of equivalent reliability index, the evaluation of safety criteria for existing offshore structures is developed. By employing the method presented in this paper, system redundancy has been evaluated for some numerical examples and satisfactory results have been drawn.     

胶州湾底栖生物动态的研究

胶州湾底栖生物组成复杂,数量丰富,其中有些种为捕捞对象,如菲律宾蛤仔等开发潜力很大,有些种为鱼、虾类天然饵料,如多毛类的长吻沙蚕、索沙蚕,软体动物的金星碟铰蛤等。底栖生物对渔业资源的补充和开发利用以及增、养殖和海洋生态学的研究都具有重要意义。早在30年代,张玺教授等(1936)就对胶州湾的底栖生物进行了系统的研究。解放后,中国科学院海洋研究所在胶州湾进行了大量的调査研究(E.Φ.古丽娅诺娃、吴宝铃,1963),特别是刘瑞玉教授领导的底栖生物组在1980-1990年对胶州湾进行了长期的、连续的调査,积累了许多宝贵的资料,发表了很多文章(刘瑞玉等,1992a;刘瑞玉等,1992b;孙滨等,1992;孙道元,1990;吴耀泉等,1992),基本掌握了胶州湾底栖生物的全貌。作者自1991年5月至1994年2月在原来调查的基础上,在胶州湾6个不同底栖生物群落的分布区范围内设立了10个底栖生物监测取样站(图5),进行了3年调査。每年分春(5月)、夏(8月)、秋(11月)、冬(2月)四季在各站以取样面积为0.1㎡的表层采泥器取样2次,对胶州湾底梄生物的种类组成、数量变化及群落结构进行了研究。     

沉积物中重金属的归一化问题——以Al为例

沉积物的来源、粒度和矿物组成是影响重金属在动力沉积过程中的行为的最显著的因素,用某些参考元素（如Ａｌ、Ｌｉ等）归一化的目的是为了减小沉积物中重金属含量的波动,以揭示人文活动（例如污染）的影响。通过对国内一些河流沉积物中重金属的Ａｌ归一化结果的分析,认为在岩石的风化和变质过程中元素与Ａｌ的相对迁移能力的差异和各种生物过程均可使重金属的Ａｌ归一化值产生显著的变化,在某些情况下Ｍ／Ａｌ值并不一定能准确地描述人类活动对沉积物中重金属的影响。Ａｌ归一化仅能部分地校正粒度分布引起的重金属含量的变化,但不能消除矿物组成的影响。     

Is the jet of AO 0235+164 rotating?

We present the VLBI map of a superluminal radio source AO 0235+164 at 5 GHz. This shows that the object's radio structure is dominated by a strong, nearly unresolved core with two extended asymmetric weak jet components. Based on the variation of its flux density with time at 5 GHz, we suggest that the flux density of AO 0235+164 exhibits two periodic variations: a shorter-period variation of 1.81±0.06 yr and a longer-period one of 3.64±0.08 yr. These two periodic variations could be the result of the joint action of jet outbursts and jet rotation.     

行星天文学的重要地位及其热点

对1995年至2001年《Natue》和《Science》上发表的天文学论文的统计表明，行星天文学领域的论文数量明显超过天文学的其它分支学科，占天文学总论文数的1/3左右。从这个角度来看，行星天文学是天文学最活跃和重要的分支学科之一。对这些论文具体内容的分析可以给出当前行星天文学领域的若干热点问题。相比之下，我国对这一重要领域的关注和投入还远远不够。     

Using a New Sky Brightness Monitor to Observe the Annular Solar Eclipse on 15 January 2010

For the future development of Chinese Giant Solar Telescope (CGST) in Western China, a new sky brightness monitor (SBM) has been produced for the site survey for CGST. To critically examine the performance and sensitivity of SBM, we used it in the observation of the annular solar eclipse in Dali City, Yunnan, on 15 January 2010. The observation met good weather conditions with an almost clear sky during the eclipse. The SBM measurement translates into the solar illuminance changes at a level of 2.4×10^?4 I?s^?1 during the eclipse. The time of the minimal sky brightness in the field of view (FOV) is found consistent with the time of maximum eclipse. Two local sky regions in the FOV are chosen to make a time series of the calibrated skylight profiles. The evolution of the sky brightness thus calibrated also shows good consistency with the eclipse, particularly between the second and the third contacts. The minimal sky brightness in each local sky region took place within half a minute from the corresponding predicted contact time. Such small time delays were mainly caused by occasional cirri. The minimal sky brightness measured during the eclipse is a few millionths of I _?? with standard deviation of 0.11 millionths of I _??. The observation supports that the single-scattering process (optically thin conditions) is the main contributor to the atmospheric scattering. We have demonstrated that many important aerosol optical parameters can be deduced from our data. We conclude that the new SBM is a sensitive sky photometer that can be used for our CGST and coronagraph site surveys.     

Electron acceleration behind a wavy dipolarization front

In this paper, with the in-situ observations from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) probes we report a wavy dipolarization front (DF) event, where the DF has different magnetic structures and electron distributions at different \(y\) positions in the Geocentric Solar Magnetospheric (GSM) coordinates. At \(y \sim2.1R_{E}\) (\(R_{E}\) is the radius of Earth), the DF has a relatively simple structure, which is similar to that of a conventional DF. At \(y \sim3.0R_{E}\), the DF is revealed to have a multiple DF structure, where the plasma exhibits a vortex flow. Such a wavy DF could be the results of the interchange instability. The different structure of such a wavy DF at different sites has a great effect on electron acceleration. Fermi acceleration can occur at the site of the DF with a simple or multiple DF structure, while betatron acceleration as a local process has the contribution to energetic electrons only at the site of the DF with a simple structure.