近岸海域光合色素的生物标志作用研究Ⅰ.台湾海峡特征光合色素的分布及其对浮游植物类群结构的指示

１引言 由于高效液相色谱法（ＨＰＬＣ）的建立,利用光合色素,尤其是类胡萝卜素作为区分浮游植物类群的指示物,成为更方便和有效的化学分类法［１,２］．原因是色素能够很好地进行定量,可涵盖浮游植物的全部粒级范围;而且,适用于大批量样品的分析,甚至可实现现场的船上测定．海洋浮游植物光合色素的研究,比较多地集中在开放大洋,多为利用类胡萝卜素表征浮游植物的类群结构［３－５］;或以光合色素及其降解产物作为浮游植物参与的生物地球化学过程的生物标志物［６－８］．相比较而言,在近岸、陆架海域开展的此类研究较少,且多…     

渤海垂直湍流混合强度季节变化的数值模拟

渤海为极浅陆架海 ,其中湍流耗散作用显著。将三维斜压陆架海模式 HAMSOM应用于渤海 ,以渤海周边台站每天 4次的常规气象资料作为风和热驱动 ,渤海海峡开边界以 5个主要分潮调和常数计算水位强迫 ,计算了渤海 1982年水文要素和流场变化 ,并用模式以湍的局地平衡理论封闭计算出垂直湍流粘性的时空分布。结果表明 :渤海湍流混合冬强夏弱 ,变化幅度较大 ( 10～ 2 0 0 cm2 / s) ,这是风搅拌和潮混合的湍流输入在密度层化调整下的结果 ;风的作用在冬季强于潮的作用 ,而底层则由潮混合控制呈现半月周期 ;渤海湍粘性系数的空间分布十分复杂 ,这是在渤海地形和岸形轮廓限制下 ,由一定大气条件驱动的流场和密度场导致的湍流混合强度不同所致     

高纯河豚毒素对蛙坐骨神经动作电位的影响

用电生理学方法观察了4种不同浓度的高纯河豚毒素(tetrodotoxin,TTX)对蛙离体坐骨神经动作电位的影响.实验结果表明:1μmol/dm3TTX在给药后7 min能显著抑制动作电位的上相幅度(P<0.05),但在给药后10 min才显著抑制动作电位的下相幅度(P<0.01);20μmol/dm3TTX在给药后3 min内能完全抑制动作电位的形成.1μmol/dm3TTX在给药后1~5min对动作电位传导速度的影响没有统计学意义,5μmol/dm3TTX在5min时可显著抑制传导速度(P<0.05),而10μmol/dm3TTX在2min时便显著抑制传导速度(P<0.05).实验结果提示高纯河豚毒素对蛙离体坐骨神经动作电位的影响存在剂量效应关系.     

黄渤海海域贝类麻痹性贝毒的检测与分析

采用小白鼠生物测试法和高效液相色谱法对2002~2005年我国黄渤海海域采集的贝类样品进行了麻痹性贝毒毒性检测,结果显示大连海域的虾夷扇贝含有麻痹性贝毒,有毒样品均出现在5月和6月,部分虾夷扇贝样品的毒素含量已经超过食用安全标准。通过高效液相色谱法分析了有毒虾夷扇贝体内的毒素成分,共检出了6种麻痹性贝毒组分,主要以毒性较低的C1和C2毒素为主,GTX3和GTX2次之,STX和neoSTX含量很低。通过高效液相色谱法分析得到的各毒素组分毒性总和与小白鼠生物测试法毒性测试结果基本相当。     

台湾的弧陆碰撞研究及其地层沉积构造研究年表

对台湾及其邻近地区典型板块构造弧陆碰撞运动的研究历史沿革与代表性观点进行了较为全面的介绍;将1977年颜沧波有关台湾及其邻近地区典型板块构造弧陆碰撞运动研究的观点与30年后黄奇瑜教授的研究成果进行了对比性介绍;同时介绍了反映台湾及其邻近地区典型板块构造弧陆碰撞运动的地层沉积构造综合研究年表。     

褐牙鲆(♀)、夏鲆(♂)及其杂交子一代线粒体16S rDNA序列遗传特性的初步研究

以线粒体16S rRNA基因部分片段为代表研究雌褐牙鲆Paralichthys olivaceus、雄夏鲆P. dentatus及其杂交子一代间线粒体DNA的遗传特性。母本与父本序列差异较大,属种间差异,在590个位点中有28个变异位点,而且全部为简约信息位点。使用同一对引物扩增亲本与杂交子代,在杂交子代中未检测到父本的线粒体DNA类型,11个处于两种生长阶段的杂交样本仅检测到一种单倍型,而且与母本的一个单倍型为同一种,表明褐牙鲆与夏鲆杂交线粒体DNA遵循母系遗传规律。     

海区兵要地志信息系统的设计与开发

介绍了海区兵要地志信息系统的组成及功能,以及系统设计的关键点。系统实现了多媒体海量兵要地志信息存储与查询功能;成功地将GIS技术引入到兵要地志系统中,突破了传统纸质兵要地志的局限性;成功地将不同类型的兵要信息集成在同一个界面上表达,具有很好的兼容性。     

阿根廷滑柔鱼渔场的初步研究

根据2001年12月至2002年4月"辽渔1号"在西南大西洋(57°W—60°W,41°S—47°S)的柔鱼生产调查资料,对作业渔场的渔获量和水温垂直分布特点进行了初步分析,并运用逐步回归法探讨了周产量(t/week)与各水层温度之间的关系。结果表明:(1)周产量在70t以上的作业区域全部在60°02′W—60°40′W,44°59′S—46°04′S范围内(简称南渔场),周产量在70t以下的作业区域绝大多数集中在57°47′W—58°2′W,41°54′S—42°2′S范围内(简称北渔场);(2)南渔场渔获的表层水温在12.2℃~15.1℃,北渔场渔获的表层水温在10.0℃~12.3℃,两渔场在20~70m水体均出现了强度不等的温跃层;(3)整个作业区域,周产量与水温存在线性相关,相关系数R=0.8515,其中南渔场相关系数R=0.9985,北渔场相关系数R=0.9313。     

Evaluation of bending moments and shear forces at unit connections of very large floating structures using hydroelastic and rigid body analyses

This paper investigates the characteristics of bending moments, shear forces and stresses at unit connections of very large floating structures (VLFS) under wave loads. The responses of VLFS are calculated by solving multi-body motion equation considering hydroelasticity and connection stiffness. Hydroelastic responses are calculated by the direct method. Higher-order boundary element method (HOBEM) is used for fluid analysis and finite element method (FEM) is introduced for structural analysis. The equation of motion is modified to describe the unit connections by employing spring elements. Bending moments and shear forces at the connections are obtained from the dynamic equilibrium condition for pressures and inertia forces. Two types of VLFS units such as tandem arranged units and side-by-side arranged units are considered in the numerical examples. The influences of connection stiffness, wave frequency and heading angle on responses of VLFS are investigated through the numerical examples. Rigid body analysis along with hydroelastic analysis is also carried out in the numerical analysis and comparison of those two approaches is discussed.     

Estimates of AGN Black Hole Mass and Minimum Variability Timescale

Black hole mass is one of the fundamental physical parameters of active galactic nuclei (AGNs), for which many methods of estimation have been proposed. One set of methods assumes that the broad-line region (BLR) is gravitationally bound by the central black hole potential, so the black hole mass can be estimated from the orbital radius and the Doppler velocity. Another set of methods assumes the observed variability timescale is determined by the orbital timescale near the innermost stable orbit around the Schwarzschild black hole or the Kerr black hole, or by the characteristic timescale of the accretion disk. We collect a sample of 21 AGNs, for which the minimum variability timescales have been obtained and their black hole masses (Mσ) have been well estimated from the stellar velocity dispersion or the BLR size-luminosity relation. Using the minimum variability timescales we estimated the black hole masses for 21 objects by the three different methods, the results are denoted by Ms, Mk and Md, respectively. We compared each of them with Mσindividually and found that: (1) using the minimum variability timescale with the Kerr black hole theory leads to small differences between Mσand Mk, none exceeding one order of magnitude, and the mean difference between them is about 0.53 dex; (2) using the minimum variability timescale with the Schwarzschild black hole theory leads to somewhat larger difference between Mσand Ms: larger than one order of magnitude for 6 of the 21 sources, and the mean difference is 0.74 dex; (3) using the minimum variability timescale with the accretion disk theory leads to much larger differences between Mσand Md, for 13 of the 21 sources the differences are larger than two orders of magnitude; and the mean difference is as high as about 2.01 dex.