以海岸带综合管理为工具开展海洋生物多样性保护管理

生物多样性保护是当前全球面临的最重要问题之一,本文分析了我国海洋生物多样性面临的主要威胁,并对生物多样性丧失的原因进行了分析。在以上研究的基础上,基于海岸带综合管理（ICZM）的理念,提出了海洋生物多样性保护管理中急需解决的问题,主要包括海洋生物多样性保护管理的指导思想、管理机构机制、管理边界、海洋生物多样性评价技术、海洋生物多样性保护规划技术和基于GIS的管理决策支持系统等。     

浙闽沿岸流消退时期的浮游植物群落结构特征

浙闽沿岸流对台湾海峡的水文环境意义重大.依据国家海洋局"908"补充调查专项,通过对覆盖浙闽沿岸流海洋锋面过程的海洋生物调查研究,于2008年4月实施针对浙闽沿岸流消退时期(春季)台湾海峡锋面海域的浮游植物取样分析.结果共记录3门41属86种,其中硅藻35属76种.甲藻5属9种,蓝藻1属1种.种类组成以暖水性种类和广布...     

深海新型取样仪器-电视抓斗及使用方法

每一位海洋地质工作者都非常重视外业调查及第一手资料的获取,而这些往往得益于海洋地质调查仪器的帮助.以前我们常用的表层沉积物取样仪器,有普通蚌式抓斗、小箱式取样器、多管取样器等.这里介绍一种深海新型取样仪器--电视抓斗.目前,它在深海及大洋洋中脊资源调查,特别是在深海底块状硫化物、多金属结核、锰结壳调查等勘测中扮演着重要...     

老168平台海油陆采丛式井组关键钻井工艺

老168平台丛式井组是2009年中石化及胜利油田的重点产能建设项目之一,平台上共部署58口海油陆采定向井。该丛式井组的施工主要有以下难点：井网密集,防碰工作量大;造斜点浅、井斜大、造斜困难;位移大、裸眼稳斜段长,稳斜难度大;钻井液技术必须考虑环境保护问题,可借鉴经验非常少。因此钻井施工难度极大,通过实施优化井场布局及井眼轨道技术、大井眼松软浅地层定向技术、高精度轨迹控制技术、大位移井安全钻进技术,优质无污染海水钻井液技术,最终实现了老168钻完井一体化作业,节约了成本,提高了效率,为今后胜利油田丛式井组施工提供了宝贵经验。     

Predicting size effect on diffusion-limited current density of oxygen reduction by copper wire

The size effect of copper wire radius (0.04–0.82 mm) on the diffusion-limited current density of an oxygen reduction reaction in stagnant simulated seawater (naturally aerated 0.5 mol/L NaCl) is investigated by potentiodynamic polarization and electrochemical impedance spectroscopy (EIS) and compared with the results obtained in 0.5 mol/L H2SO4. In the oxygen diffusion-limited range, size effect is found to occur independent of electrolytes, which is attributed to non-linear diffusion. Additionally, to sati...     

时差对海洋磁力测量地磁日变改正的影响分析

为研究时差对磁测的影响,基于站间同步地磁日变曲线的特征,尝试采用同步比对法和相关分析法计算两站的时差.结论表明:同步比对法和相关分析法能反映站间真实的时差,当测区范围较小时(至少是在本文实例的两个地磁日变站之间),时差对地磁日变改正的影响很小,海洋磁力测量地磁日变改正时可以忽略其影响.     

福建省海洋环境保护规划信息系统设计与实现

以福建省海洋环境保护规划的方法和步骤为基础,以系统的应用需求分析为出发点,进行海洋环境保护规划信息系统开发模式分析、系统总体结构设计、系统界面与系统功能模块实现等研究,采用组件式设计方法,用C#4.0封装了ArcEngine地图引擎,实现海洋环境信息采集、存储、管理、分析和图形处理,以及查询、分析、评价和辅助决策等主要...     

世界地理研究回顾与展望——建所70周年世界地理研究成果与发展前景

中科院地理科学与资源研究所建所70年来,世界地理研究由于坚持了紧密为国家政治斗争和社会经济建设服务的正确方针,在地缘政治与地缘经济、国家与区域地理的综合研究、部门地理与专题研究、中外对比研究、世界地理知识普及等方面取得了一系列重要研究成果.研究工作中存在的问题为:超前性不够、系统性不强、研究手段落后、资料来源单一、成果...     

Proton flux and radiation dose from galactic cosmic rays in the lunar regolith and implications for organic synthesis at the poles of the Moon and Mercury

Galactic cosmic rays are a potential energy source to stimulate organic synthesis from simple ices. The recent detection of organic molecules at the polar regions of the Moon by LCROSS (Colaprete, A. et al. [2010]. Science 330, 463–468, http://dx.doi.org/10.1126/science.1186986), and possibly at the poles of Mercury (Paige, D.A. et al. [2013]. Science 339, 300–303, http://dx.doi.org/10.1126/science.1231106), introduces the question of whether the organics were delivered by impact or formed in situ. Laboratory experiments show that high energy particles can cause organic production from simple ices. We use a Monte Carlo particle scattering code (MCNPX) to model and report the flux of GCR protons at the surface of the Moon and report radiation dose rates and absorbed doses at the Moon’s surface and with depth as a result of GCR protons and secondary particles, and apply scaling factors to account for contributions to dose from heavier ions. We compare our results with dose rate measurements by the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) experiment on Lunar Reconnaissance Orbiter (Schwadron, N.A. et al. [2012]. J. Geophys. Res. 117, E00H13, http://dx.doi.org/10.1029/2011JE003978) and find them in good agreement, indicating that MCNPX can be confidently applied to studies of radiation dose at and within the surface of the Moon. We use our dose rate calculations to conclude that organic synthesis is plausible well within the age of the lunar polar cold traps, and that organics detected at the poles of the Moon may have been produced in situ. Our dose rate calculations also indicate that galactic cosmic rays can induce organic synthesis within the estimated age of the dark deposits at the pole of Mercury that may contain organics.