军曹鱼营养成分的分析及评价   总被引：37，自引：1，他引：37  

李刘冬  陈毕生  冯娟  柯浩  蔡景心  范楷 《热带海洋学报》2002,21(1):76-82

对军曹鱼Rachycentron canadum Linnaeus进行解剖比较、营养分析和评价，结果显示，军曹鱼的含肉率为68．7％，肌肉蛋白质含量为21．2％，氨基酸总量为65．05％；蛋氨酸为第一限制氨基酸，其中赖氨酸含量高达591mg.gN^-1，军曹鱼的不饱和脂肪酸含量为65．2％，其中二十碳五烯酸（eicosapentaenoic acid，简称EPA）和二十二碳六烯酸（docosahexenoic acid简称DHA）的含量分别为4．5％和12．0％。研究结果表明，军曹鱼含肉率高，营养质量好，有较高的营养价值和药用价值。  相似文献   

Degradation of rope properties under increasing monotonic load     

Juan Felipe Beltran  Eric B. Williamson 《Ocean Engineering》2005,32(7):826-844

This paper describes the development of a computational model to predict the response of synthetic-fiber ropes under both monotonic and cyclic loads. The model addresses the issue of damage to a rope cross-section and its effect on rope response. Isotropic damage is assumed and is therefore characterized by a scalar quantity known as the damage index. The damage index is used to quantify the amount of deterioration that takes place in a damaged rope throughout its loading history. For the current study, data obtained from static tension tests are used to determine the evolution relationship for the damage index. This relationship is based on the stiffness ratio between experimental data and simulation of rope response without any source of damage and is assumed to be described by an exponential equation. Numerical simulations of damaged rope behavior compare well with experimental results.  相似文献   

水库浮游植物群落动态的人工神经网络方法   总被引：5，自引：0，他引：5  

邬红娟  郭生练  胡传林  刘跃 《海洋与湖沼》2001,32(3):267-273

根据辽宁大伙房水库1980－1997年的水文和湖沼学观测资料，分别建立浮游植物丰度和蓝藻优势度人工视经网络模型，将年降雨量，7－9月平均水温，7－8月入库水量与7－8月库容之比和磷酸盐作为输入，浮游植物量和丰度作为输出，建立浮游植物落消长的人工神经网络模型，将7－9月平均水温，7－8月入出库水量之比，磷酸盐和总氨作为输入，蓝藻优势度作为输出，建立浮游植物演替的人工神经网络预测模型，并进行检验，其模拟值与观测值平均相对误差分别2％和1％，结果表明，人工神经网络方法优于传统的统计学模型，可进行水库浮游植物群落动态的预测预报，并具有较高的精度。  相似文献   

基于多种生物指数的中国渤海莱州湾海域底栖生境健康评价     

王丽  罗先香  杨建强  张娟  樊玉清  沈佳裕 《海洋学报(英文版)》2020,39(2):49-58

As an important part of the Bohai economic rim, the Laizhou Bay has been stressed by serious eco-environmental problems in recent years. In this study, the Shannon-Wiener index(H′), AZTI's marine biotic index(AMBI) and the multivariate AMBI(M-AMBI) were used to assess the ecological quality status(EQS) of the Laizhou Bay according to macrobenthos data collected annually in August 2011–2014. The results showed that the overall benthic habitat quality in the Laizhou Bay was assessed as "Good". However, 25% of the samples were classified as"Moderate", "Bad" or "Poor" status under degraded conditions. Ecological group Ⅲ(EGⅢ) species which had a certain tolerance to environmental disturbances had a higher proportion in each station, and most of them had appeared the pollution indicator species Capitella capitata. This indicated that the benthic habitat in the Laizhou Bay had been disturbed and polluted to some extent. The comparison of the three indices evaluation result and the RDA analysis showed that the H′ and M-AMBI were more suitable when the relative abundance of the single species was high and the macrobenthic community was significantly imbalanced; when the relative abundance of opportunistic species(EGIV and EGV) was high, the AMBI and M-AMBI could reflected the EQS objectively; in an undisturbed and polluted environment, all the three indices could indicate the benthic habitats quality. In summary, the better correlation between the three indices and environmental factors showed that they were well responsive to the tendency of the benthic habitats quality in the Laizhou Bay.  相似文献   

Wave Dispersion Study in the Indian Ocean-Tsunami of December 26, 2004     

Juan Horrillo  Zygmunt Kowalik  Yoshinori Shigihara 《Marine Geodesy》2006,29(3):149-166

A numerical study which takes into account wave dispersion effects has been carried out in the Indian Ocean to reproduce the initial stage of wave propagation of the tsunami event that occurred on December 26, 2004. Three different numerical models have been used: the nonlinear shallow water (nondispersive), the nonlinear Boussinesq, and the full Navier-Stokes aided by the volume of fluid method to track the free surface. Numerical model results are compared against each other. General features of the wave propagation agreed very well in all numerical studies. However some important differences are observed in the wave patterns, i.e., the development in time of the wave front is shown to be strongly connected to the dispersion effects. Discussions and conclusions are made about the spatial and temporal distribution of the free surface reaffirming that the dispersion mechanism is important for tsunami hazard mitigation.  相似文献   

滨海砂土对可溶性油的吸附作用和影响因素研究     

孙娟  郑西来  吴俊文 《中国海洋大学学报(自然科学版)》2007,37(4):663-666,652

在现场自然地理、水文地质条件调查的基础上,对青岛海水浴场采集砂和海水样品进行主要物理化学性质分析,探讨吸附机理的影响因素,通过吸附试验建立砂样对可溶性油吸附的动力学方程和吸附等温线,经过批量试验确定温度、盐度和pH值对吸附量的影响。研究结果表明,砂土对可溶性油吸附的平衡吸附量为90~110 mg/kg,吸附平衡时间为14~16 h,符合Henry型直线等温物理吸附。对等温式进一步分析发现,当水相中可溶性油浓度低于一定数值时,不但不产生吸附,反而会使污染沙滩上的残留油分释放出来,造成二次污染。  相似文献   

The influence of some ship parameters on manoeuvrability studied at the design stage     

Francisco Lzaro Prez  Juan Antonio Clemente 《Ocean Engineering》2007,34(3-4):518-525

Collision and grounding are the most common accidents in ship operation. Some accidents are due to human failure, but several research projects have shown that a high percentage of these accidents could have been avoided if the ship have had better manoeuvrability characteristics. This paper describes how, when the shipyard select some important ship parameters and dimensions at the design stage, these set of parameters influence manoeuvrability characteristics. To obtain these effects, some IMO manoeuvres have been numerically simulated for a sample ship and a non-linear numerical model proposed by the authors to study ship manoeuvrability is described in this work. The day to day practice of a shipyard where fast modelisation and calculations are required, and modifications to the original design are quite common at the preliminary design stage, requires fast but accurate numerical models.  相似文献   

Multi-thermal observations of newly formed loops in a dynamic flare     

Zdeněk F. Švestka  Juan M. Fontenla  Marcos E. Machado  Sara F. Martin  Donald F. Neidig  Giannina Poletto 《Solar physics》1987,108(2):237-250

The dynamic flare of 6 November, 1980 (max 15:26 UT) developed a rich system of growing loops which could be followed in H for 1.5 hr. Throughout the flare, these loops, near the limb, were seen in emission against the disk. Theoretical computations of deviations from LTE populations for a hydrogen atom reveal that this requires electron densities in the loops close to, or in excess of 10¹² cm ^-3. From measured widths of higher Balmer lines the density at the tops of the loops was found to be 4 x 10¹² cm ^-3 if no non-thermal motions were present, or 5 × 10¹¹ cm ^-3 for a turbulent velocity of ~ 12 km s ^-1.It is now general knowledge that flare loops are initially observed in X-rays and become visible in H only after cooling. For such a high density, a loop would cool through radiation from 10⁷ to 10⁴ K within a few minutes so that the dense H loops should have heights very close to the heights of the X-ray loops. This, however, contradicts the observations obtained by the HXIS and FCS instruments on board SMM which show the X-ray loops at much higher altitudes than the loops in H. Therefore, we suggest that the density must have been significantly lower when the loops were formed and that the flare loops were apparently both shrinking and increasing in density while cooling.NAS/NRC Research Associate, on leave from CNIE, Argentina.Operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation. Partial support for the National Solar Observatory is provided by the USAF under a Memorandum of Understanding with the NSF.  相似文献   

An approximate analytical representation of the atmospheric gamma-ray flux at balloon altitudes     

Enrico Costa  Enrico Massaro  Marco Salvati  Antonio Appolloni 《Astrophysics and Space Science》1984,100(1-2):165-174

The general behaviour of the atmospheric -ray flux as a function of the residual atmosphere, zenith angle, and photon energy is approximated with simple analytical expressions. The free parameters are determined by comparison with the most recent models and the existing experimental measurements. The resulting formulae have an accuracy comparable to the mutual consistency of the available pieces of information, and at the same time are very convenient to use in numerical simulations.  相似文献   

Far-infrared emission from an intergalactic dust cloud?     

Bogdan Wszolek  Konrad Rudnicki  Silvia Masi  Paolo De Bernardis  Antonio Salvi 《Astrophysics and Space Science》1989,152(1):29-34

We used theIRAS All Sky Maps in order to search for infrared emission in the direction of the Okroy Cloud (R.A.=12^h50^m, =22°). An enhancement of 100 m diffuse emission is evident in such a region, with an anomalous value of the ratioI _v (100 m)/A _v ; hydrogen 21 cm emission is also present with low radial speed, thus suggesting that the cloud could be a satellite of our Galaxy.  相似文献