Developing Effective Decision Support for the Application of “Gentle” Remediation Options: The GREENLAND Project

Gentle remediation options (GRO) are risk management strategies/technologies that result in a net gain (or at least no gross reduction) in soil function as well as risk management. They encompass a number of technologies, including the use of plant (phyto‐), fungi (myco‐), and/or bacteria‐based methods, with or without chemical soil additives or amendments, for reducing contaminant transfer to local receptors by in situ stabilization, or extraction, transformation, or degradation of contaminants. Despite offering strong benefits in terms of risk management, deployment costs, and sustainability for a range of site problems, the application of GRO as practical on‐site remedial solutions is still in its relative infancy, particularly for metal(loid)‐contaminated sites. A key barrier to wider adoption of GRO relates to general uncertainties and lack of stakeholder confidence in (and indeed knowledge of) the feasibility or reliability of GRO as practical risk management solutions. The GREENLAND project has therefore developed a simple and transparent decision support framework for promoting the appropriate use of gentle remediation options and encouraging participation of stakeholders, supplemented by a set of specific design aids for use when GRO appear to be a viable option. The framework is presented as a three phased model or Decision Support Tool (DST), in the form of a Microsoft Excel‐based workbook, designed to inform decision‐making and options appraisal during the selection of remedial approaches for contaminated sites. The DST acts as a simple decision support and stakeholder engagement tool for the application of GRO, providing a context for GRO application (particularly where soft end‐use of remediated land is envisaged), quick reference tables (including an economic cost calculator), and supporting information and technical guidance drawing on practical examples of effective GRO application at trace metal(loid) contaminated sites across Europe. This article introduces the decision support framework. ©2015 Wiley Periodicals, Inc.     

Die Hochwasserkatastrophen im Sommer 2002

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A directional passive air sampler for monitoring polycyclic aromatic hydrocarbons (PAHs) in air mass

A passive air sampler was developed for collecting polycyclic aromatic hydrocarbons (PAHs) in air mass from various directions. The airflow velocity within the sampler was assessed for its responses to ambient wind speed and direction. The sampler was examined for trapped particles, evaluated quantitatively for influence of airflow velocity and temperature on PAH uptake, examined for PAH uptake kinetics, calibrated against active sampling, and finally tested in the field. The airflow volume passing the sampler was linearly proportional to ambient wind speed and sensitive to wind direction. The uptake rate for an individual PAH was a function of airflow velocity, temperature and the octanol-air partitioning coefficient of the PAH. For all PAHs with more than two rings, the passive sampler operated in a linear uptake phase for three weeks. Different PAH concentrations were obtained in air masses from different directions in the field test.     

我国矿产资源态势与对策

我国矿产资源总量大,居世界第3位人均拥有量小,居世界第80位。我国要实现现代化建设的第二步战略目标,矿产资源供需存在着矛盾。为了解决供需矛盾,必须从地质找矿、矿山、一次资源回收、二次资源回收、节能和节材等方面挖掘潜力。改革资源耗费型经济发展旧模式,确立资源节约型经济发展新模式,废止“有水快流”的方针,确立开发与节约并重的方针,是缓解矿产资源供需矛盾的根本途径。具体对策有:(1)依靠科学技术进步开发节约(2)搞好资源进出口贸易取长补短(3)健全法制管理体系依法治矿(4)用好计划机制管好资源和矿山(5)用好市场机制搞活矿业经济。     

多环芳烃污染与儿童内暴露负荷的关系

为了更好地了解环境空气PAHs污染与儿童内暴露负荷之间的关系,该研究在儿童尿液中未代谢PAHs以及代谢PAHs研究的基础上,同时获取了连续3 d空气中PAHs污染浓度。对环境空气中PAHs和尿液中未代谢的PAHs的分析表明:除Nap和Phe以外的其它PAHs单体在环境空气和尿液中占比一致,而且环境空气和尿液中PAHs组成特征一致,均表现为2环PAHs>3环PAHs>4环PAHs的规律;3 d中仅有A-Nap和U-Nap之间存在相关性(P<0.05,R~2=0.999 6)。对尿液中代谢的PAHs和尿液中未代谢的PAHs分析表明:儿童尿液中排出的Nap、Flu和Phe主要以羟基代谢物为主,仅Pyr与OHPyr基本一致。尿液中未代谢PAHs与代谢的PAHs组成特征一致,表现为Nap>Phe>Flu>Pyr和OHNap>OHPhe>OHFlu>OHPyr的规律;仅U-Nap和OHNap 3 d中均存在相关性,U-Phe和OHPhe、U-Pyr和OHPyr仅1 d存在相关性。结合PAHs污染与儿童内暴露负荷的共同研究表明,PAHs内暴露标志物可以在一定程度上反映环境PAHs污染的时间变异性。     

Was wissen wir über Neutronensterne?

There are 10^9±0.5 neutron stars in the Galaxy. They are born in supernova explosions. Isolated neutron stars are observed as (radio-)pulsars, in some cases also as γ-ray pulsars and as IR-, optical and X-ray pulsars. Binary neutron stars, when accreting mass from their companion, become flickering, periodic and/or bursting X-ray sources, and probably also γ-ray bursters. They may all derive from binary star systems. The masses of population-I-neutron stars are compatible with (1.4 ±0.2)M _⊙; their surface magnetic fields fall almost exclusively within 10^12.2 and 10^13.2 Gauss (at birth). The radii of population-II-neutron stars are (10 _-3 ⁺⁶ )km. Even in exotic sources like SS 433 and Cyg X-1, the compact core may well be a neutron star.