Biofouling confounds the uptake of trace organic contaminants by semi-permeable membrane devices (SPMDs)

The outer layers of layflat, low density polyethylene plastic tubing (the principal component of semi-permeable membrane devices, SPMDs) were biofouled at a clean site in Hong Kong coastal waters for periods of 1–4 weeks. Following pre-fouling, triolein was added to the SPMDs and, along with control (unfouled) devices, they were exposed to a range of organochlorine pesticides (-HCH, aldrin, p,p^′-DDT) and PAHs (anthracene, fluoranthene and benzo(a)pyrene) under laboratory conditions. Results showed that the uptake of contaminants by SPMDs was severely reduced by as much as 50% under fouling conditions in comparison to unfouled controls. The ultimate utility of SPMDs as passive monitors is thus reduced, although alternative measures, such as the use of permeability reference compounds may compensate, and allow for realistic evaluations of dissolved environmental concentrations in aquatic environments. However, due to the complexities involved in such procedures––especially as they need to be conducted on a case-by-case basis––the utility of SPMDs appears to be limited for estimates of bioavailability unless necessary calibrations are undertaken within each environment that the sampler is used.     

《深圳市地图集》地理基础底图的设计与编制

详细介绍了《深圳市地图集》地理基础底图的设计原理和编制方法。着重论述了其地理底图的总体设计,底图系统的设计,投影和比例尺的设计,各底图系统的编制方法,制作地理底图的技术路线设计。     

A Measurement of Omega from the North American Test Flight of Boomerang

We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain the geometry of the universe. Within the class of cold dark matter models, we find that the overall fractional energy density of the universe Omega is constrained to be 0.85相似文献   

Near-Surface Flow Fields Deduced Using Correlation Tracking and Time-Distance Analyses

Near-photospheric flow fields on the Sun are deduced using two independent methods applied to the same time series of velocity images observed by SOI-MDI on SOHO. Differences in travel times between f modes entering and leaving each pixel measured using time-distance helioseismology are used to determine sites of supergranular outflows. Alternatively, correlation tracking analysis of mesogranular scales of motion applied to the same time series is used to deduce the near-surface flow field. These two approaches provide the means to assess the patterns and evolution of horizontal flows on supergranular scales even near disk center, which is not feasible with direct line-of-sight Doppler measurements. We find that the locations of the supergranular outflows seen in flow fields generated from correlation tracking coincide well with the locations of the outflows determined from the time-distance analysis, with a mean correlation coefficient after smoothing of _s=0.890. Near-surface velocity field measurements can be used to study the evolution of the supergranular network, as merging and splitting events are observed to occur in these images. The data consist of one 2048-min time series of high-resolution (0.6 pixels) line-of-sight velocity images taken by MDI on 1997 January 16–18 at a cadence of one minute.     

An analysis of Pc3 and Pc4 pulsations at Terra Nova Bay (Antarctica)

We conducted a statistical analysis of the physical characteristics of the micropulsation activity (Pc3 and Pc4 range) detected, during the austral summer 1994/95, at Terra Nova Bay (Antarctica, corrected latitude 80.0°S), a station which is few degrees poleward of those where most of the Antarctic measurements in these frequency ranges have been performed. The emerging overview suggests that the correspondence between the pulsation power and the external parameters (solar wind speed, interplanetary magnetic field magnitude and orientation) is significantly stronger than at somewhat lower latitudes. The day-to-day power variability was found to be strictly related to the general level of the geomagnetic activity, and the power level sharply maximizes at local magnetic noon. In the Pc4 range peaks of correlation with the SW speed are found in the dawn and dusk sides of the Earths magnetosphere and the daily variation of the polarization pattern is closely consistent with that found at auroral latitudes and at lower frequencies. In the Pc3 range the correlation coefficient between the pulsation power and the SW speed has maximum values in the local morning, and the frequency of selected events reveals a strong IMF control during closed magnetospheric conditions. The local time dependence of the correlation coefficient between the pulsation power and the cone angle reveals an additional control by the IMF orientation, which becomes more explicit around local noon.     

黔东南锦屏-天柱地区构造控岩控金特征模拟实验及其力学分析

在前人工作基础上,侧重研究石英脉型金矿床成矿的地质背景,建立了该类型金矿的成矿模式。进而开展三轴温压条件下的成岩成矿实验,构造形变特征及其与成矿物质活化、迁移、富集之间的相互关系的模拟实验。实验结果表明:(1)该区岩石、矿石在高温高压条件下,产生塑性变形(褶皱)和脆性变形(破裂);(2)在变形过程中使成矿物质活化、迁移和富集,形成顺层及穿层的含金石英脉,并在多期多次变形过程中使成矿物质叠加富集;(3)在褶皱(背斜)轴部形成富矿体。模拟实验结果与所建立的该类型金矿构造控矿和成矿模式非常相似。实验资料的力学分析表明,由轴压所产生的构造附加压力大大地提高了实际围压,从而促进了岩石流变、变形和物质的迁移,由此促进含矿流体向构造附加压力小的部位定向迁移、充填和成矿。构造附加压力是促进该区金成矿的重要动力条件。     

阿拉斯加输油管的设计和施工方式方案变更过程及其背后的原因和哲学思想

阿拉斯加输油管道公司曾经研发和使用了3种主要施工方案和技术:传统地埋式、特殊埋设和地上敷设方式.在传统地埋式施工方案中,管顶埋深变化于0.9~2.7 m.这主要是考虑了地形变化,而不是沿途的岩性和土壤类型.在特殊埋设方案中,在原油管道必须埋设的地段,如大规模动物迁徙常用地段则使用通道冷液循环降(保)温系统和(或)热管(桩)降(保)温,来保护多年冻土.地上敷设方案包括桩基架设和地上洁净砾石管堤(垫护层).后者只在管道进入和离开多年冻土时采用.架设桩基横梁方案中使用有或没有热管保温的垂直支架梁(单元)(VSM).在初步规划和设计阶段,管道的业主公司(即横穿阿拉斯加管道系统,或TAPS)和随后的阿拉斯加管道服务公司(APSC)不容商量的坚决要求100%的埋设方案.但是,随着勘察工作的进展和设计方案的细化,施工设计方案在不断变化.1977年管道施工结束时,只有57%的管道采用了埋设方式.管道运行30 a后的今天(考虑运行期间维护中所产生的问题),很多经验丰富的工程师认为53%的埋设可能更合理.设计和施工方案变更的原因主要有:1)为了获得通过联邦政府所属的土地所需的许可证,政府有特殊的规定和要求;2)管道公司的设计、施工和管理人员进行了现场野外调查、研究,并积极参与了详细设计和研发;3)美国环境政策法案(NEPA)的最新要求(启用了核准制).阿拉斯加管道服务公司是7家主要石油公司的服务机构.由于这个项目的巨大规模和所涉及的高昂费用,致使各大石油公司的工程师非同寻常程度的参与.在文章中,笔者论述了与阿拉斯加管道施工有关的阿拉斯加管道服务公司、美国联邦和阿拉斯加州政府相关组织机构的形成历史,管道设计演变过程及其背后的哲学思想,以及阿拉斯加管道工程项目的经验和教训.     

利用场地观测计算地表通量

高原地表的感热和潜热通量在亚洲季风系统中有很重要的作用。由于高原地域辽阔，且自然环境较严酷，不利于建立完善的地面观测系统。因此，卫星遥感观测就成为测算高原整体感热和潜热通量的有效工具。地面场地的观测结果作为地表通量的真实值，对于卫星遥感测算是非常重要的。它也为构建陆面—大气模型提供了科学依据，是卫星资料的资料同化系统中的重要组成部分。 计算场地热量通量有几种不同的处理方法。最简单的方法利用有效的观测和试验的参数，可以给出稳定连续的估计。愈精确的Bowen比或者廓线的观测能给出愈精确的信息。综合了湍流测量及辐射测量、土壤热通量的观测结果的估计对陆面—大气相互作用进行了详细的描述，以适应模式的发展。从1998年开始，这些方法联合应用到青藏高原；场地通量观测方面的成果以及目前对其理解将在本文中做一概述。     

中国东北地区岩石圈结构的地震学特征与对矿产资源的动力控制作用

利用东北地区1°×1°深至400km的三维Vp(km/s)值数据,选择互相垂直的2条有代表性的剖面,初步建立研究区构造圈、均匀层基本结构模型;利用8套沿不同经纬线的剖面Vp值分布,勾绘出研究区深至过渡层的结构模型谱;进一步综合得到研究区三维岩石圈结构模型。东北地区的B″层可能由3部分组成,即下部的低速带,中上部的中速、低速相间互层带和上部的增速带,B″层底界面是区分B″与B'″层的稳定的标志,上部的增速带速度与B'下部速度值接近,按照传统认识,那里是岩石圈底界面的位置,东北地区B″层顶界面形态可能存在不连续或剧烈变化的部位。B″层上中部的宽广的分布边界形态及其变化,可能反映软流圈对周围地球物质的同化熔蚀作用;软流圈物质上涌为固体矿产提供物源,也对油气矿产形成起加速作用。岩石圈结构是壳幔物质相互作用的动态平衡结果,它包含软流圈层对上覆地球物质的影响,并对油气、固体矿产存在一种动力控制作用。     

内蒙古沙麦岩体：正εNd（t）值的过铝质花岗岩

内蒙古沙麦岩体位于大兴安岭中段西坡,是二连浩特-东乌珠穆沁旗花岗岩带的重要组成部分。岩体中脉岩和围岩捕虏体较为发育,岩性组合主要为中细粒黑云母花岗岩和细粒似斑状花岗岩。在化学成分上,沙麦岩体以铝弱过饱和,富硅,全碱含量中等和低磷为特点,标准矿物中刚玉分子大于1%,可归为过铝质 S 型花岗岩。在稀土元素和微量元素组成上,岩体富 Rb、Th、U、Ta,贫 Ba、Sr、P、Ti,Rb/Sr 比值高,K/Rb 比值低,Eu 负异常明显。在 Nd 同位素组成上,岩体 Nd 同位素组成变化较大,除一件样品ε_(Nd)(t)值为负值以外,普遍以具正ε_(Nd)(t)值为特点,T_(2DM)值介于275.79～1048.41Ma 之间。研究结果表明,沙麦岩体形成于晚中生代后造山的岩石圈伸展环境中,是幔源基性岩浆底侵及其诱发的壳-幔混合岩浆,同化中上地壳泥质围岩并经高程度分离结晶的产物。