胶州湾水体镉的迁移过程和环境本底值结构

根据1979年的胶州湾水域调查资料,分析重金属Cd在胶州湾水域的水平分布、垂直分布和季节变化。研究结果表明:在整个胶州湾水域,水质没有受到任何Cd的污染。在胶州湾和湾口水域只有两个Cd的来源。一个是来源于地壳岩石风化,通过陆地径流把重金属Cd注入胶州湾水域;另一个是来源于海底,经过海洋水流的作用把重金属Cd注入湾口水域。作者提出了重金属在水域的环境本底值结构:基础本底值、陆地径流的输入量和海洋水流的输入量,并且应用于胶州湾水域。作者认为在来源的迁移过程中,有陆地来源迁移和海底来源迁移。根据杨东方的水域迁移过程研究,陆地径流决定了Cd的表、底层质量浓度变化。     

2009年秋季航次UCTD样机海上试验

UCTD(Underway Conductivity-Temperature-Depth)是一种新型船舶走航上层海洋温度盐度剖面调查设备。文中介绍了国内研制的UCTD样机参加2009年秋季航次海上试验情况,包括试验设备的组成、安装、试验结论和存在的问题等。为了海上现场检验UCTD样机探头测量性能、下降深度、速度和甲板设备的运行情况,共进行了42次投放试验。通过分析试验数据,UCTD样机的作业时间、测量深度、测量性能和可靠性均达到了预期的设计目标。试验数据经处理后可获取海洋上层温盐断面数据,实现了UCTD实际应用效果,最后对试验中发现的问题提出了解决办法。     

Second-Oorder Analytic Solutions of Nonlinear Interactions of Edge Waves on A Plane Sloping Bottom

Based on the full water-wave equation, a second-order analytic solution for nonlinear interaction of short edge waves on a constant plane sloping bottom is presented in this paper. For special case of slope angle b=p/2, this solution can be reduced to the same order solution of deep water gravity surface waves traveling along parallel coastline. Interactions between two edge waves including progressive, standing and partially reflected standing waves were also discussed. The unified analytic expressions with transfer functions for kinematic-dynamic elements of edge waves were also discussed. The random model of the unified wave motion processes for linear and nonlinear irregular edge waves is formulated, and the corresponding theoretical autocorrelation and spectral density functions of the first and second orders are derived. The boundary conditions for the determining determination of the parameters of short edge wave are suggested, that may be seen as one special simple edge wave excitation mechanism and an extension to the sea wave refraction theory. Finally some computation results are demonstrated.     

南海西北陆缘新型多金属结核的发现及意义

近年南海西北陆缘西沙东北海域发现大型多金属结核,尽管其外观与大洋结核别无二致,具有个体大、外部形态规整、层状结构清晰的特点,但其地球化学组成与大洋多金属结核存在明显差别:TMn/TFe的比值小,仅为0.73,富Fe、Si、Al、稀土元素而贫Mn、Cu、Co、Ni。Be同位素质谱法测年和钙质超微生物地层学方法研究表明,结核生长速度达7.41～15.38 mm/Ma,远大于大洋多金属结核的平均生长速率和以前发现于南海北部的多金属结核。依据其综合特征,初步认定其为边缘海区域赋存的一种新型多金属结核。该类型结核所蕴含丰富的边缘海区域古海洋、古气候、古环境信息,有助于探讨新生代末期青藏高原隆升、东亚季风加强、北半球冰期发生等重大地质事件所引起的区域沉积响应。     

流式影像术在海洋浮游植物分类研究中的应用

海洋浮游植物支撑着海洋生态系统的正常运转,对其种类的定性识别、鉴定和细胞数量的定量分析是海洋科学研究中最为关键的科学问题之一。流式影像术在海洋浮游植物形态特征识别与快速定量检测上是目前先进和可行的方法,它综合了流式细胞术和图像显微识别的技术优点,不但能够对快速流动状态中的海洋浮游植物进行相应的参数检测,而且可以获取流动过程中清晰的图像,通过计算机软件的图像处理和特征筛选,实现海洋浮游植物有效的自动识别。通过对流式影像术的原理、测定方法、技术特点及其发展动态等的综述,认为基于流式影像术对高速运动的浮游植物图像的清晰实时采集,可以有效地对图像进行模式的识别和分类。它是一种理想和实用的方法,将为海洋生物学研究提供新的实时、快速、高效平台,有很好的应用前景。     

近20年京津唐主体城区地表热场空间特征变化分析

基于Landsat遥感影像获取京津唐主体城区1995~2015年地表温度(Land Surface Temperature, LST)和不透水地表盖度(Impervious Surface Percentage, ISP)数据。采用热点聚集和阈值分割法,依据地表的温度和不透水盖度属性将京津唐主体城区划分成9种地表热场类型,分析并探讨地表热场的发展规律、年际变化状况和区域贡献作用。研究发现,京津唐主体城区地表温度与不透水地表盖度间存在显著的正向相关关系,两者分别呈现“阶梯降”和“两端高、中间低”的变化特征。京津唐主体城区地表热场的发展主轴保持在西北-东南方向,且随时间推移沿主轴呈聚集态势。 京津唐主体城区地表热场的影响范围在空间上持续扩张,对于不同的主体城区,其在整体区域的热场贡献中有差异化表现。     

轨道交通沿线土地溢价归公的政策与实践——以东莞市为例

轨道交通周边土地开发和溢价归公有助于缓解城市财政压力,推动公交都市建设。结合国外实施溢价归公的政策和实践模式,以东莞市为例,在资料收集、政策分析、文本和案例解读的基础上,探讨了中国城市政府在规划和建设轨道交通中,以土地溢价归公反哺轨道交通融资的政策安排和实施效果。结果表明:1)溢价归公的本质是以特定方式实现正外部效应的内部化,由于土地制度和税收体系的差异,欧美地区溢价归公主要依赖多样化的土地税收体系,而中国城市的实践主要借鉴了“轨道+物业”的联合开发模式;2)东莞市溢价归公策略的形成是综合开发规划编制和审批、沿线土地控制和储备、土地发展权转移、土地增值分配等核心环节有效协调的结果;3)东莞轨道交通沿线土地开发能形成可观的财政收益,潜在土地收益占轨道资金总需求的比例超过20%,但在实施过程中仍面临较大困难。东莞市案例能为其他城市轨道交通融资、土地开发和溢价归公的政策体系编制和有效实施提供一定的参考。     

Diffusion of elements in the interstellar medium in early-type galaxies

The role of diffusion in the redistribution of elements in the hot interstellar medium of earlytype galaxies is considered. It is well known that gravitational sedimentation can affect significantly the abundances of helium and heavy elements in the hot intergalactic gas of massive galaxy clusters. The universal temperature profile in cool-core clusters and the theoretical mass–temperature relation suggest that the maximum effect of sedimentation must take place in the most massive virialized objects in the Universe. However, observational data from the Chandra and XMM-Newton observatories demonstrate more complex scaling relations between the masses of early-type galaxies and other parameters, such as the mass fraction and temperature of the interstellar gas. An important fact is that the radial temperature profile can have both falling and rising patterns. We have calculated the diffusion based on the observed gas density and temperature distributions for 13 early-type galaxies that have different envelope types and cover a wide range of X-ray luminosities. To estimate the maximum effect of sedimentation and thermal diffusion, we have solved the full set of Burgers equations for a non-magnetized interstellar plasma. The results obtained demonstrate a considerable increase of the He/H ratio within one effective radius for all galaxies of our sample. For galaxies with a falling or constant temperature profile the average increase of the helium abundance is 60% in one billion years of diffusion. The revealed effect can introduce a significant bias into the metal abundance estimate based on X-ray spectroscopy and can affect the evolution of stars that could be formed from a gas with a high helium abundance.     

Identification of X-ray lines in the spectrum of the arcsec-scale precessing jets of SS 433

The extended X-ray emission observed at arcsec scales along the propagation trajectory of the precessing relativistic jets of the Galactic microquasar SS 433 features a broad emission line, with the position of the centroid being significantly different for the approaching and receding jets (≈7.3 and ≈6.4 keV, respectively). These observed line positions are at odds with the predictions of the kinematic model for any of the plausible bright spectral lines in this band, raising the question of their identification. Here we address this issue by taking into account time delays of the emission coming from the receding regions of the jets relative to that from the approaching ones, which cause a substantial phase shift and distortion of the predicted line positions for the extended (~10¹⁷ cm) emission compared to the X-ray and optical lines observed from the central source (emitted at distances ~10¹¹ and ~10¹⁵ cm, respectively). We demonstrate that the observed line positions are fully consistent with the Fe XXVI Lyα (E ₀ = 6.96 keV) line emerging from a region of size ~6 × 10¹⁶ cm along the jet. This supports the idea that intensive reheating of the jets up to temperatures >10 keV takes place at these distances, probably as a result of partial deceleration of the jets due to interaction with the surrounding medium, which might cause collisions between discrete dense blobs inside the jets.