近场水下爆炸对背空圆板冲击作用仿真研究

在一定的假设条件下,圆板在空气中接触爆炸具有理论解;而在水介质中,近场条件下很难推导理论解。 通过 LS-Dyna 近场条件下全过程模拟计算技术研究水下爆炸载荷对水面圆板冲击作用,得到自由场压力、气泡脉动周期及最大半径、水射流速度等典型特征参数的变化规律,与理论分析结果一致。 揭示了气泡第一周期内脉动形态发展变化过程,获取了结构应力响应、圆板结构变形。 该技术可进一步应用于近场水下爆炸对水面舰船的毁伤评估工作。     

Antenna design and implementation for the future space Ultra-Long wavelength radio telescope

In radio astronomy, the Ultra-Long Wavelengths (ULW) regime of longer than 10 m (frequencies below 30 MHz), remains the last virtually unexplored window of the celestial electromagnetic spectrum. The strength of the science case for extending radio astronomy into the ULW window is growing. However, the opaqueness of the Earth’s ionosphere makes ULW observations by ground-based facilities practically impossible. Furthermore, the ULW spectrum is full of anthropogenic radio frequency interference (RFI). The only radical solution for both problems is in placing an ULW astronomy facility in space. We present a concept of a key element of a space-borne ULW array facility, an antenna that addresses radio astronomical specifications. A tripole–type antenna and amplifier are analysed as a solution for ULW implementation. A receiver system with a low power dissipation is discussed as well. The active antenna is optimized to operate at the noise level defined by the celestial emission in the frequency band 1 ? 30 MHz. Field experiments with a prototype tripole antenna enabled estimates of the system noise temperature. They indicated that the proposed concept meets the requirements of a space-borne ULW array facility.     

ENSO evolution asymmetry: EP versus CP El Niño

Through an oceanic mixed-layer heat budget analysis, the dominant processes contributing to the largest decay rate (− 0.37 °C/mon) in EP El Nino, the moderate delay rate (− 0.22 °C/mon) in CP El Nino and the smallest decay rate (0.13 °C/mon) in La Nina, are identified. The result shows that both dynamic (wind induced equatorial ocean waves and thermocline changes) and thermodynamic (net surface solar radiation and latent heat flux changes) processes contribute to a fast decay and thus phase transition in EP El Niño composite, whereas the thermodynamic process has less effect on the decay rate for both CP El Niño and La Niña due to the westward shift of sea surface temperature anomaly (SSTA) centers. Thus, the difference in surface wind stress forcing is critical in contributing to evolution asymmetry between CP El Niño and La Niña, while the difference in both the wind stress and heat flux anomalies contribute to evolution asymmetry between EP El Niño and La Niña. It is interesting to note that El Nino induced anomalous anticyclone over the western North Pacific is stronger and shifts more toward the east during EP El Niño than during CP El Niño, while compared to CP El Niño, the center of an anomalous cyclone during La Niña shifts further to the west. As a consequence, both EP and CP El Niño decay fast and transform into a La Niña episode in the subsequent year, whereas La Niña has a much slower decay rate and re-develops in the second year.

     

北黄海海底麻坑群形态的定量研究及控制因素

本文基于高分辨率多波束水深数据和反向散射强度数据,对北黄海海底麻坑群的形态参数进行定量研究,结合水深、地形坡度和后向散射强度的变化准确界定了麻坑的轮廓,识别出圆形、椭圆形、拉长型麻坑共282个,并在ArcGIS软件中对其形态参数进行了分析计算,麻坑的平均长轴1.36 km,短轴0.78 km,直径0.94 km,面积0.88 km2,平均周长3.82 km,长宽比1.83,深度0.3~2.5 m,平均面积密集度13%,麻坑的剖面形态有麻坑边缘凹陷、中部有明显凸起（W1型）,麻坑边缘凹陷、中部略凸起（W2型）,麻坑中部单纯凹陷（V型）,分别集中分布在麻坑群的北部、南部、西部。麻坑的平面规模大、深度小的原因与地层中形成麻坑的游离气体浓度较小有关,也可能受到了地震、海啸等外力的诱发。麻坑的长轴优势走向为ENE-WSW、NNE-SSW,底流对其形状的塑造起了较大作用,部分麻坑成串排列,形成串珠状的麻坑链,其排列方式受到海底古河道、古潟湖等沉积地层结构的控制。海底麻坑群发育区反向散射强度为-60~-71 dB,麻坑内部较麻坑外部平均高5 dB,可能为麻坑内部气体泄漏引起海底沉积物被剥蚀后残留下的粗颗粒物质或海底生物活动留下的遗迹导致的。     

基于空间自相关的阿根廷滑柔鱼CPUE标准化研究

CPUE的观测往往不是独立的,而是存在空间相关性的。但是,大多数的CPUE标准化方法通常都假设名义CPUE在空间上是相互独立的。为此,本研究以西南大西洋阿根廷滑柔鱼为例,采用2000-2014年1-5月中国大陆鱿钓生产统计数据以及对应的海表温度和叶绿素浓度数据,选择广义线性模型（general linear model,GLM）为基础模型,将空间自相关加入到GLM中,比较标准GLM和4种加入空间自相关的空间GLM的CPUE标准化。根据最小信息准则（Akaike Information Criterion,AIC）及贝叶斯信息准则（Bayesian Information Criterion,BIC）,空间自相关的GLM的CPUE标准化结果优于标准GLM,其中指数模型的CPUE标准化结果最佳。同时,标准GLM与空间自相关的GLM相比,存在精确度过高估计的问题。因此,在CPUE标准化中,应充分考虑空间自相关这一因素。     

基于碳、氮稳定同位素的雅浦海沟底栖生物食物来源和营养级初探

为了分析雅浦海沟中底栖生物群落的食物来源和营养级,本研究分析了雅浦海沟真光层中浮游植物和浮游动物、海底沉积物和巨型底栖生物（海绵、海参、海蛇尾、海星、海葵和钩虾）中的碳、氮稳定同位素组成。研究发现雅浦海沟真光层中的浮游植物和浮游动物δ13C值[（-22.8±0.4）‰和（-21.8±0.8）‰]和δ15N值[（5.4±0.4）‰和（6.8±0.2）‰]与巨型底栖生物的δ13C值（-20.1‰~-16.8‰）和δ15N值（11.9‰~17.9‰）的差异超过了一个营养级,表明作为底栖生物的初始食物来源的浮游植物和浮游动物在向下输送的过程中经历了食物链传递和细菌的降解。巨型底栖生物的δ15N和δ13C值之间无显著的相关性,此外不同物种之间营养级也存在明显差异,表现为海绵的营养级相对较高（3.4~4.7）,海参（3.3~3.6）、海蛇尾（3.4~3.5）和海星（3.2~3.7）的营养级较为接近,钩虾（2.9~3.3）和海葵（3.1）的营养级则相对略低,反映了底栖生物不同物种之间食物来源的多样化。     

不同气候模态下西北太平洋秋刀鱼资源丰度预测模型建立

秋刀鱼（Cololabis saira）资源对海洋环境因素极为敏感,不同气候模态可能对秋刀鱼资源丰度产生不同的影响。根据1990-2014年西北太平洋日本的秋刀鱼渔业中单位捕捞努力量渔获量（CPUE,以此作为资源丰度）,以及相应产卵场、索饵场的海表温（SST）遥感数据,探讨太平洋年际震荡（PDO）指数冷、暖年下,秋刀鱼资源丰度CPUE变化与产卵场、索饵场SST的关系,并分别建立资源丰度的预测模型。研究表明,PDO冷年索饵场4月SST与年CPUE显著相关（P<0.05）,PDO暖年索饵场11月的SST与年标准化CPUE显著相关（P<0.05）。PDO冷、暖年的秋刀鱼资源丰度的预测模型中,CPUE均与索饵场11月的SST、索饵场4月SST呈现正相关的关系,统计学上为显著相关（P<0.05）。PDO冷年（2012年）和PDO暖年（2014年）的CPUE预测值与实际值相对误差分别为14.03%、-16.26%,具有较好的拟合效果。研究认为,不同气候模态下,可用于秋刀鱼资源丰度预测的环境因子不同,上述建立资源丰度模型可用于业务化运行。     

Lateral Bearing Capacity of Modified Suction Caissons Determined by Using the Limit Equilibrium Method

The modified suction caisson (MSC) adds a short-skirted structure around the regular suction caissons to increase the lateral bearing capacity and limit the deflection. The MSC is suitable for acting as the offshore wind turbine foundation subjected to larger lateral loads compared with the imposed vertical loads. Determination of the lateral bearing capacity is a key issue for the MSC design. The formula estimating the lateral bearing capacity of the MSC was proposed in terms of the limit equilibrium method and was verified by the test results. Parametric studies on the lateral bearing capacity were also carried out. It was found that the lateral bearing capacity of the MSC increases with the increasing length and radius of the external skirt, and the lateral bearing capacity increases linearly with the increasing coefficient of subgrade reaction. The maximum lateral bearing capacity of the MSC is attained when the ratio of the radii of the internal compartment to the external skirt equals 0.82 and the ratio of the lengths of the external skirt to the internal compartment equals 0.48, provided that the steel usage of the MSC is kept constant.     

硅岩的Rb-Sr同位素组成特点及其地质意义

通过对扬子地台和东昆仑山地区的不同时代、不同成因、成分上差异较大的硅岩Rb-Sr同位素组成的对比研究，探讨其物源和形成环境，利用所测Rb-Sr等时线年龄，有效的解决硅岩的地层年代，开创硅岩测年的应用前景。     

Tilting Styx and Nix but not Uranus with a Spin-Precession-Mean-motion resonance

A Hamiltonian model is constructed for the spin axis of a planet perturbed by a nearby planet with both planets in orbit about a star. We expand the planet–planet gravitational potential perturbation to first order in orbital inclinations and eccentricities, finding terms describing spin resonances involving the spin precession rate and the two planetary mean motions. Convergent planetary migration allows the spinning planet to be captured into spin resonance. With initial obliquity near zero, the spin resonance can lift the planet’s obliquity to near 90\(^\circ \) or 180\(^\circ \) depending upon whether the spin resonance is first or zeroth order in inclination. Past capture of Uranus into such a spin resonance could give an alternative non-collisional scenario accounting for Uranus’s high obliquity. However, we find that the time spent in spin resonance must be so long that this scenario cannot be responsible for Uranus’s high obliquity. Our model can be used to study spin resonance in satellite systems. Our Hamiltonian model explains how Styx and Nix can be tilted to high obliquity via outward migration of Charon, a phenomenon previously seen in numerical simulations.