Structure and photosynthetic properties of phytoplankton assemblages in a highly dynamic system, the Northern Adriatic Sea     

O. Mangoni  M. Modigh  P. Mozeti   A. Bergamasco  P. Rivaro  V. Saggiomo 《Estuarine, Coastal and Shelf Science》2008,77(4):633-644

The photosynthetic properties of phytoplankton populations as related to physical–chemical variations on small temporal and spatial scales and to phytoplankton size structure and pigment spectra were investigated in the Northern Adriatic Sea off the Po River delta in late winter 1997. Large diatoms (fucoxanthin) dominated the phytoplankton in the coastal area whereas small phytoflagellates (mainly 19′-hexanoyloxyfucoxanthin, chlorophyll b, 19′-butanoyloxyfucoxanthin) occurred outside the front. The front was defined by the steep gradient in density in the surface layer separating low-salinity coastal waters from the offshore waters.Physical features of the area strongly influenced phytoplankton biomass distributions, composition and size structure. After high volumes of Po River discharge several gyres and meanders occurred in the area off the river delta in February. Decreasing river discharge and the subsequent disappearance of the gyres and the spreading dilution of the river plume was observed in March. The dynamic circulation of February resulted in high photosynthetic capacity of the abundant phytoplankton population (>3.40 mg m⁻³). In March, the slow circulation and an upper low-salinity water layer, segregated from the deeper layers, resulted in lack of renewal of this water mass. The huge phytoplankton biomass, up to 15.77 mg chl a m⁻³, became nutrient depleted and showed low photosynthetic capacity. In February, an exceptionally high P_max^B, 20.11 mg C (mg chl a)⁻¹ h⁻¹ was recorded in the Po River plume area and average P_max^B was three-fold in February as compared to the March recordings, 10.50 mg C (mg chl a)⁻¹ h⁻¹ and 3.22 mg C (mg chl a)⁻¹ h⁻¹, respectively.The extreme variability and values of phytoplankton biomass in the innermost plume area was not always reflected in primary production. Modeling of circulation patterns and water mass resilience in the area will help to predict phytoplankton response and biomass distributions. In the frontal area, despite a considerable variability in environmental conditions, our findings have shown that the phytoplankton assemblages will compensate for nutrient depression and hydrographic constraints, by means of size and taxonomic composition and, as a result, the variability in the photosynthetic capacity was much less pronounced than that observed for other parameters.  相似文献   

地磁测量参考场计算软件的设计与实现          下载免费PDF全文

田晋 《海洋测绘》2008,28(1):32-35

以IGRF全球地磁位模型为基础,设计地磁测量参考场计算软件,实现地磁场参数长波分量的时间域与空间域离散点计算,为野外磁力测量相关数据采集与仪器配置提供先验信息,使数据采集的作业效率及可靠性大大提高。  相似文献   

海底浅表层不同土类静力触探参数与物理力学性质对比研究   总被引：1，自引：0，他引：1  

陈培雄  潘国富  陈小玲 《海洋通报》2009,28(6)

海底土的物理、力学特性是海洋地质学、海洋土工学、海洋地质灾害等调查研究及海洋资源开发环境条件调查和评价等方面非常重要的资料,海底静力触探试验(CPT)是获取这方面资料的一种快速高效、成本低、测试精度高的原位测试方法。它可同时获取海底土锥尖阻力、侧摩阻力等方面的连续原位测试数据,这些数据与海底土取样样品测试分析资料及物探资料结合,可对海底土的工程特性等作比较全面的分析和评价。本文对采集的海底土样的静力触探参数与海底土样的物理力学指标进行相关分析,分粘性土和砂类土二类,建立了海底浅表层土的静力触探参数与物理力学指标之间的相关方程。利用相关方程可以通过静力触探的数据来推算土的物理力学指标,进而对海底土的工程情况作较全面的评价。  相似文献   

基于Global Mapper的地貌晕渲制图——以西安幅(Ⅰ-49)为例   总被引：1，自引：0，他引：1  

林松  程维明  乔玉良 《地球信息科学学报》2009,11(6):802-808

地貌晕渲图自动制图是以计算机软、硬件为基础,对DEM数据实现的一种三维立体可视化表达。本文从地貌晕渲的基本理论出发,以我国1:100万标准分幅的西安幅(1-49)为例,采用Global Mapper软件实现了计算机地貌晕渲自动制作的全过程,主要内容包括:计算机地貌晕渲关键技术的实现,地貌晕渲效果与参数设置之间的关系,Global Mapper软件中各种参数设置的合理性分析,使用分层设色的办法对晕渲图进行色彩的设计,并利用PHOTOSHOP软件对结果进行整饰等。该方法可实现地貌晕渲图的自动制图。  相似文献   

GPS卫星伪广播星历技术研究          下载免费PDF全文

何丽娜  王解先 《海洋测绘》2008,28(4):11-14

通过GPS广播星历求出一个时间段内间隔一定时间的离散卫星三维坐标,以这些卫星坐标序列为已知数据反求星历参数的方法,论述和验证了当卫星坐标发生旋转变化时,解算得到的相应地面点坐标的旋转矩阵与卫星坐标发生旋转变化的矩阵具有相同的值。这对于实现GPS加密具有很大的意义。  相似文献   

多类训练迭代法在沉积盆地圈闭评价中的应用     

《地球科学与环境学报》1999,(Z1)

本文介绍了多类训练迭代法计算的基本原理和计算过程。将此法成功地应用于某沉积盆地的圈闭评价中,结果表明未钻探的３８ 个圈闭可分三类,其中１０ 个圈闭为Ⅰ类,８ 个圈闭为Ⅱ类,其余的２０ 个圈闭为Ⅲ类  相似文献   

基于nRF9E5的无线网络控制应用设计方案     

王雄辉  沈玉利  林庆浩  郑甲任  吴东岳 《广东海洋大学学报》2008,28(3)

结合现代餐饮业自动化服务的需求,以无线Soc芯片nRF9E5和点阵型LCD模块ST7920为硬件核心,结合C++Builder软件编程环境,构建了一种基于nRF9E5芯片的无线网络自动化服务管理系统,该系统具有人机界面友好、数据管理软件完善、无线数据传输与控制稳定、高效等特点。可以推广应用到区域水质、土壤等环境的自动监测等领域。  相似文献   

Simulation of less‐mobile porosity dynamics in contrasting sediment water interface porous media          下载免费PDF全文

Farzaneh MahmoodPoor Dehkordy  Martin A. Briggs  Frederick D. Day‐Lewis  Amvrossios C. Bagtzoglou 《水文研究》2018,32(13):2030-2043

Considering heterogeneity in porous media pore size and connectivity is essential to predicting reactive solute transport across interfaces. However, exchange with less‐mobile porosity is rarely considered in surface water/groundwater recharge studies. Previous research indicates that a combination of pore‐fluid sampling and geoelectrical measurements can be used to quantify less‐mobile porosity exchange dynamics using the time‐varying relation between fluid and bulk electrical conductivity. For this study, we use macro‐scale (10 s of cm) advection–dispersion solute transport models linked with electrical conduction in COMSOL Multiphysics to explore less‐mobile porosity dynamics in two different types of observed sediment water interface porous media. Modeled sediment textures contrast from strongly layered streambed deposits to poorly sorted lakebed sands and cobbles. During simulated ionic tracer perturbations, a lag between fluid and bulk electrical conductivity, and the resultant hysteresis, is observed for all simulations indicating differential loading of pore spaces with tracer. Less‐mobile exchange parameters are determined graphically from these tracer time series data without the need for inverse numerical model simulation. In both sediment types, effective less‐mobile porosity exchange parameters are variable in response to changes in flow direction and fluid flux. These observed flow‐dependent effects directly impact local less‐mobile residence times and associated contact time for biogeochemical reaction. The simulations indicate that for the sediment textures explored here, less‐mobile porosity exchange is dominated by variable rates of advection through the domain, rather than diffusion of solute, for typical low‐to‐moderate rate (approximately 3–40 cm/day) hyporheic fluid fluxes. Overall, our model‐based results show that less‐mobile porosity may be expected in a range of natural hyporheic sediments and that changes in flowpath orientation and magnitude will impact less‐mobile exchange parameters. These temporal dynamics can be assessed with the geoelectrical experimental tracer method applied at laboratory and field scales.  相似文献   

Analysis of pile subjected to torsion in multi‐layered soil     

A. Misra  Rajni Saggu  D. Basu  T. Chakraborty 《国际地质力学数值与分析法杂志》2014,38(5):475-492

A new method of analysis of piles in multi‐layered elastic soil subjected to a torque at the head is developed. The differential equation governing the angle of twist in the pile is derived using the variational principles of mechanics. The method of initial parameters is used to obtain closed‐form solutions of the angle of twist and torque in the pile as a function of depth. The inputs required for the analysis are shear moduli of pile and soil, pile geometry and thickness of soil layers. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

Analyses of Wolf-Rayet ultraviolet spectra     

Krzysztof Rochowicz 《Astrophysics and Space Science》1996,238(1):71-74

Ultraviolet spectra of population I WR stars obtained from IUE archive are used to determine fundamental stellar parameters. Terminal velocities for 85 galactic and LMC Wolf-Rayet stars were obtained by means of the empirical relation between spectral quantities easily measured in low resolution and high-resolution terminal velocity measurements. Temperatures and so-called transformed radii were derived based on available contour plots of spectral characteristics for a grid of NLTE models. The effect of the reddening law on stellar far ultraviolet continua is emphasized and the revised extinction curve towards WR stars is used for dereddening. For the sample of stars attributed to open clusters or associations we construct the stellar distance scale and adopt it for the other WR stars. The remaining fundamental parameters are derived and HR diagram for population I WR stars is presented.  相似文献