ASM1中污水水质参数与化学计量系数的估测     

王波 《海岸工程》2002,21(4):6-12

简要介绍了活性污泥1号模型中14个污水水质参数与5个化学计量系数的估测方法和典型取值。  相似文献   

饵料对中间球海胆生长发育的影响初探     

王波  张春利  高倩  张榭令  蔡世秋 《海洋科学进展》2002,20(1):54-59

实验结果表明 :单独投喂牟氏角毛藻或与三角褐指藻、绿色巴夫藻混投 ,中间球海胆幼虫成活率最高 ,其生长速度也最快 ,中间球海胆稚幼海胆培育的最好饵料是前期投喂的石莼等薄嫩的海藻 ,后期投喂海带其生长速度最快  相似文献   

Vertical Sound Velocity Transition in the Coral Reef Core and Its Significance of Indicating Facies     

李赶先  卢博 《海洋通报(英文版)》2002,4(1):19-26

On the basis of the sound velocity measurements of the coral reef core from Nanyong No.1 well of Yongshu Reef in the Nansha Islands,the paper studies the relations between the vertical sound velocity transition features in the coral reef core and the corresponding stratigraphic depositional facies change as well as stratigraphic gap of erosion,analyses the cause of the sound velocity transition,expounds the concrete process of the sea level change resulting in the stratigraphic gap of erosion and facies change in the coral reef and explains the relations between the vertical sound velocity transition in the coral reef core and the corresponding stratigraphic paleoclimate and the sea level change.This study is of important practical value and theoretical significance to the island and reef engineering construction and the acoustic logging for oil exploration in the reef limestone area as well as the paleoceanographic study of the marginal sea in the westerm Pacific Ocean.  相似文献   

白令海夏季浮游细菌和原生动物生物量及分布特征   总被引：4，自引：0，他引：4  

何剑锋  陈波  曾胤新  KANGS-H  王桂忠 《海洋学报》2005,27(4):127-134

1999年7月21日至8月1日在我国首次北极科学考察期间,考察了白令海中部的浮游细菌和原生动物,分析了其丰度、分布、生物量及其生态作用,结果显示,浮游细菌表层生物量为1.5～20.2μg/dm3,平均为浮游植物生物量的30%,100m以上水柱柱总生物量(720～3123mg/m2)平均为浮游植物柱总生物量的67%,因而是白令海夏季与浮游植物处同等量级的优势类群;原生动物表层生物量为1.2～27.4μg/dm3,100m以上水柱柱总生物量为189～1698mg/m2,平均为浮游植物柱总生物量的21%,其中粒径小于5,5～20μm和大于20μm的原生动物分别占其柱总生物量的13%,47%和40%;作为主要类群的异养腰鞭毛虫占原生动物柱总生物量的39%.浮游细菌和原生动物生物量的总体分布趋势从西部向东北和东部递减、从表层向深层衰减,20～25m水层温跃层和表层海流的存在对这一分布特性可能有较大的影响.原生动物受潜在的大、中型浮游动物捕食压力的制约,维持了一个相对较低的生物量水平,在一定程度上限制了微食物环(microbial food loop)在该海域夏季生态系统营养中的作用.  相似文献   

一类全局最优化问题的动态隧道方法     

李博  曹圣山 《中国海洋大学学报(自然科学版)》2003,33(1):160-164

研究了连续变量函数的全局最优化问题 ,给出了动态隧道方法。该动态隧道方法由局部搜索和动态隧道 2个阶段构成。在局部搜索阶段用了动态系统方法。对全局最优化问题的实例进行了数值实验 ,数值结果表明了该方法的稳健性和有效性。  相似文献   

Seasonal dynamics of elemental sulfur in two coastal sediments   总被引：1，自引：0，他引：1  

Henning Troelsen  Bo Barker Jørgensen 《Estuarine, Coastal and Shelf Science》1982,15(3):255-266

A spectrophotometric method for elemental sulfur (S⁰) analysis without interference from other reduced sulfur compounds was adapted for the use in reducing sediments. The S⁰ distribution in two coastal sediments was studied regularly from summer to winter and compared to factors regulating the S⁰ accumulation, such as redox potentials, the rate of bacterial sulfide production and the general sulfur chemistry. Dense coatings of sulfur bacteria developed on the sediment surface of a sulfuretum which had an S⁰ concentration of up to 41 μmol S cm^?3. The 2·5-mm thick bacterial coating contained 40% of all S⁰ in the sediment. A more typical marine sediment with a few cm thick oxidized surface layer had an S⁰ maximum of 1–3 μmol S cm^?3 at 2–4 cm depth. The S⁰ maximum in both sediments increased from summer to winter as the sediments gradually became more oxidized. The deeper layers maintained a low S⁰ concentration. Most of the S⁰ in the upper few mm of a laboratory sulfuretum was present inside sulfur bacteria and actively migrated up and down with the bacteria depending upon the changing light and oxygen conditions.  相似文献   

海底沉积物颗粒因素在不同频率下对声衰减的影响     

刘强  卢博  黄韶健  张福生 《热带海洋学报》2007,26(4):27-31

综合了多个沉积物声学测量的实验方案,提出适合研究柱状海底沉积物声衰减的实验方案。对黏土质粉砂的物理性质和声学性质作了相关处理,得到了在高、低两种测量频率下该类型沉积物的波形特性、频谱特性和与沉积颗粒因素有关的孔隙度对声衰减比的影响。进一步作了相应的回归分析,低频时方差为0.169—0.175,高频时方差为0.029—0.032,尝试总结出黏土质粉砂类型沉积物在两种频率下的声衰减趋势。  相似文献   

Hydrogen and Helium under high pressure: A case for a classical theory of dense matter     

Vladan čelebonović 《Earth, Moon, and Planets》1989,45(3):291-298

When subject to high pressure, H₂ and ³He are expected to undergo phase transitions, and to become metallic at a sufficiently high pressure. Using a semiclassical theory of dense matter proposed by Savi and Kaanin, calculations of phase transition and metallisation pressure have been performed for these two materials. In hydrogen, metallisation occurs at p _M= (3.0 ± 0.2) Mbar, while for helium the corresponding value is p _M= (106 ± 1) Mbar. A phase transition occurs in helium at p _tr= (10.0 ± 0.4) Mbar. These values are close to the results obtainable by more rigorous methods. Possibilities of experimental verification of the calculations are briefly discussed.  相似文献   

A comparison of Hα and soft X-ray characteristics of spotless and spot group flares     

V. Ruždjak  B. Vršnak  A. Schroll  R. Brajša 《Solar physics》1989,123(2):309-316

A comparative analysis of spotless and spot group flares recorded at Hvar and Kanzelhöhe Observatories during the 21st cycle of solar activity is presented. The rate of occurrence of two-ribbon flares was found to be significantly higher for the spotless flares. In comparison with spot group flares of corresponding H importance, the soft X-ray peak values have been systematically lower for the spotless flares. The highest peak values and the energy released in soft X-rays was found for flares with a H ribbon protruding over a major spot umbra. It was found that the effective plasma temperatures in spotless flares have been considerably lower than the temperatures in spot group flares.  相似文献   

The ionization balance of the Fe in the solar corona for a non-Maxwellian electron distribution function     

Elena Dzifčáková 《Solar physics》1992,140(2):247-267

The ionization equilibrium of the Fe in the solar corona for a non-Maxwellian electron distribution with an enhanced number of particles in the high-energy tail is presented. A parametric form of the distribution function is used to demonstrate the changes in the ionization equilibrium with changes in the shape of the distribution. The results over the range of temperature 10⁵ K T 10⁸ K for different deviations of the distribution from a Maxwellian are given in tabular form. The results can be used for specific applications in the solar corona, especially in the active corona, where deviations from the Maxwellian distribution can be significant.  相似文献