地球章动原因的分析与计算

介绍地球章动的特点,从理论上分析地球章动的主要原因,计算章动常数并给出了地球章动示意图的画法.所计算的章动常数与观测值相差仅2/10 000.     

与月球有关的引潮力

从简化的地月系统力学模型出发,严格推导出地表物体动力学方程在转动坐标系下的表示形式,通过对称性的分析,得到引潮力,从而有助于加深对引潮力和潮汐成因的理解.     

The Fundamental Experiments of Red Tide Chemical Forecast

Many food algae and red tide algae were cultivated in the f/2 medium, and the nitric oxide (NO) concentration of the medium and the cell density were determined. The experiments on algae were conducted when different concentrations of NO were added into the medium using two methods. The results show that low concentrations of NO were self-produced by marine algae during the exponential growth period and were about nmol/L level. But at the end of the period, i.e., 2 or 3 days before the cell density reaches the maximum, an NO peak appeared, with the NO concentration reaching 10 nmol/L. The NO threshold concentration exists according to the influence of exogenous NO on the marine phytoplankton growth. One type is the threshold concentration that can promote algae growth, and its value is between 10 and 1 nmol level, or even lower. The other type can inhibit the phytoplankton growth, which is about μmol level or higher. The results indicate that red tide algae are far more sensitive to NO than are food algae. The fundamental experimental outcome above may provide a new clue for red tide chemical forecast by inspecting the NO change.     

Treatment of Red Tide in Ocean Using Non-Thermal Plasma Based Advanced Oxidation Technology*

A Pilot-scale experiment for the treatment of red tide in the enclosure was done in sea area of Shandong Province, P.R. China on Aug. 25, 2002. With the method of micro-gap discharge, O₂ in air and H₂O in seawater are ionized and dissociated into large numbers of OH^• radicals, and then dissolved into a part of seawater to form OH^• solution of high concentration. With OH^• concentration of 0.68 mg/L, the kill efficiencies of 29 kinds of red tide organisms such as Chaetoceros lorenzianus and so on reached 99.89%, in which bacterium and vibrio were reduced below the detection limit, also Gonyaulax cysts and Prei. Cysts with the crust were done the lowest limit of test. At the same time, the content of chlorophyll-a was decreased below the detection limit. DO (dissolved oxygen) saturation of seawater was greatly increased to 100% because the residual OH^• radical was decomposed into H₂O and O₂ after 20 min. Therefore the treatment of red tide using OH^• radicals is a kind of advanced oxidation technology, which realizes zero pollution, zero emission and zero residual in the process of the production of OH^• radicals and the treatment of red tide.*Key project of National Foundation Research from Science and Technology Ministry of China, (2002CCC00900); key project of National Natural Science Foundation of China (NSFC; 60031001).     

Study on patterns and chemical features of NO effect on marine phytoplankton growth

With supernatural bioactivation, nitric oxide (NO), which was first regarded as an endothelium- derived relaxing factor, was recognized by Science as the “Molecule of the Year” in 1992. The Nobel Prize of Physiology & Medicine in 1998 was awarded jointly to Furchgatt, Ignarro, and Murad for their discoveries concerning the NO effects in the cardiovascular sys- tem. From then on, researchers have paid more and more attention to the special and diverse functions of NO in organism[1―18].…     

用流体静力学观点解释潮汐现象

考虑地球自转因素,用流体静力学的方法讨论海潮表面形状与涨落问题.     

多核环境下潮汐分析辅助软件并行绘制技术研究

为方便科研人员使用Baytap-G潮汐分析软件,基于C#.NET程序设计语言设计了一套潮汐分析辅助软件,实现了Baytap-G软件的封装,完成了输入数据格式的自动转换、输出数据的自动提取,以及水位、振幅、相位数据的可视化展示;在介绍C#.NET语言中任务(TASK)并行编程模型的基础上,详细讨论了绘制振幅、相位图任务分解、并行化程序设计考虑及其实现;实验结果表明,合理设计并行程序可以充分利用多核计算机的计算资源,提升程序运行效率,但是过多的任务数、不均匀的工作负载通常会影响并行程序的效率。     

转动双星同步和轨道圆化的物理过程研究

潮汐效应是影响恒星结构和演化非常重要的物理因素.本文研究了影响潮汐同步和轨道圆化的物理因素,如恒星质量、初始转速、轨道周期、金属丰度、对流超射等,并根据转动恒星的角动量转移和元素扩散方程,给出了这些因素对转动双星演化和元素混合的影响.结果表明：具有大质量子星、初始转速慢、对流超射小、轨道周期短的双星系统,能更早地达到平衡速度和轨道圆化;初始转速快的恒星,由于潮汐同步过程减速,双星系统中氮元素增丰没有单星的氮元素增丰显著;大质量星、高金属丰度、超射大和短周期的双星系统,氮增丰相对显著;质量小、金属丰度低、转速慢、超射大的恒星具有较小的恒星半径,而低金属丰度恒星表面却具有较高的有效温度,快速转动单星向低温和低光度端演化.     

平行因子分析在赤潮藻滤液三维荧光光谱特征提取中的应用

在实验室条件下培养我国沿海常见的10种赤潮藻,测定了赤潮藻生长过程中藻滤液的三维荧光光谱.用平行因子分析对光谱进行分解,获得每种赤潮藻滤液荧光峰的个数及类型,即每种赤潮藻的特征光谱.在此基础上比较每种藻特征光谱的相似性和差异性,并分析了赤潮藻生长过程中滤液的荧光峰强度和生长阶段的关系,为基于赤潮藻滤液三维荧光光谱的赤潮藻种类识别测定技术提供依据.结果表明:不同赤潮藻的特征光谱之间存在差异.在指数生长期,类蛋白和类腐殖质荧光峰强度与藻密度呈正相关,说明两类有机物在水体中不断积累;在稳定期和衰亡期,两类有机物的荧光强度迅速增大,这可能是衰老和死亡细胞的破碎释放,以及细菌降解作用所致.平行因子分析可以有效提取赤潮藻的荧光特征,考察了赤潮藻荧光峰强度和生长阶段的关系.     

赤潮光谱特征及其形成机制

采用海面以上光谱测量方法 (Above water method),利用美国FieldSpec® Dual VNIR光谱仪测量了丹麦细柱藻、中肋骨条藻、海洋褐胞藻等三种浮游植物赤潮以及红色中缢虫这一原生动物赤潮的离水辐射光谱数据。强调赤潮与正常海水的光谱差异在于687～728 nm波段的特征反射峰,指出了浮游植物赤潮与原生动物赤潮间的显著光谱差异,并认为可据此进行某些赤潮种类的遥感识别。给出了浮游植物赤潮光谱反射峰、吸收峰成因;红色中缢虫这一原生动物引起的水色异常,与其体内的共生藻类及浮游植物色素碎屑有关;其摄食偏好、与藻类的共生特性研究以及藻类常温下的荧光发射特性研究,将有助于加深对于红色中缢虫赤潮光谱成因的认识。