无线电引信电磁辐射能量耦合路径研究

目的为了确定外界电磁能量究竟如何进入到引信电路内部,针对无线电引信的电磁能量耦合路径进行系统研究。方法通过对多种引信进行不同形式的连续波、强电磁脉冲电磁辐照效应试验,对比引信天线、孔缝、弹体、电源模块等部位的能量耦合可能性。分析连续波、强电磁脉冲电磁环境对无线电引信作用的耦合规律。结果确定了电磁信号类型和引信接地结构是影响电磁能量耦合通道的关键因素,揭示了前门耦合是连续波电磁辐射环境的最主要方式。结论弹体或引信前端与电路共地的金属部件是强电磁脉冲辐射环境的主要能量路径,从而为无线电引信抗电磁性能加固的实施提供了有益参考。     

水体中甲基汞光化学降解特征研究

为探究水体中甲基汞（MMHg）的光化学行为,采用室内模拟实验,以不同波长紫外灯及室内可见光为光源,探讨紫外光波长、光强度等因素对MMHg光降解的影响,并根据生成物Hg0的量变化分析MMHg光降解反应历程.研究表明,MMHg光降解最终产物中含有Hg0,且光照条件对MMHg光降解速率、Hg0的产量有影响.在反应器暴露于紫外光条件下时,MMHg光降解速率随紫外光波长的变短而增加,随紫外光强度的提高而增加,且MMHg光降解呈一级动力学反应,速率常数分别为KUVA 0.403～0.562 h-1、KUVB 0.961 h-1、KUVC 1.221 h-1和KVL＋UVA＋UVB 1.346 h-1;Hg0释放通量为0.166～0.392 ng·min-1.当反应器暴露于可见光条件下时,反应器内MMHg浓度下降速率较慢,KVL0.061 h-1;Hg0释放通量为0.008 ng·min-1.而在黑暗条件下没有发现反应器内MMHg浓度下降,无Hg0生成.可见紫外光是导致MMHg降解的主要原因,光波波长与强度对MMHg的环境地球化学行为有重要影响.     

不同流态下微波辐射对污水污泥性质的影响研究

通过对不同流态下微波辐射对污水污泥性质的影响进行研究,考察了不同流态下微波辐射作用处理后污泥沉降性能、脱水性能的变化,以及微波辐射作用下流态对污泥挥发性悬浮固体(VSS)溶解率、上清液中COD和污泥微观形态的影响.结果表明,流态对污泥的沉降性能和脱水性能有一定影响,微波辐射功率越高,流态对污泥沉降性能和脱水性能的影响越显著.微波辐射功率较低时,雷诺数Re越大,污泥的沉降比(SV)、比阻和泥饼含水率越小;微波辐射功率较高时,Re为2300的临界流态下污泥的沉降性能和脱水性能最好.随着Re的增大,VSS溶解率和上清液中COD升高,微波辐射功率分别为300、500、700和900W时,Re为3000的紊流流态下上清液中COD分别达到1.1、2.1、3.6和6.7g·L-1.SEM观察结果表明,微波辐射及流态产生的协同剪切应时适宜时,有利于污泥颗粒的絮凝反应,高强度的微波辐射和紊流产生的较大剪切应力导致污泥絮体被打碎.     

微波辐射对污水处理厂动态流活性污泥性能的影响研究

通过微波辐射对污水处理厂动态流活性污泥性能进行实验研究,考察了微波辐射3min内污泥沉降性能、脱水性能的变化,探讨了微波辐射对污泥挥发性悬浮固体(VSS)溶解率、上清液中COD和污泥微观形态的影响.结果表明,低强度的微波辐射对活性污泥相关性质的影响不显著,没有从根本上改善活性污泥的结构.适宜的微波辐射能显著改善活性污泥的沉降性能和脱水性能,500、700和900W微波辐射的适宜辐射时间分别为180、150和60s,此时,活性污泥的比阻为0.3×109S2·g-1左右,较原活性污泥减小了88%,泥饼含水率由原活性污泥直接抽滤的85.2%降低到70.0%.VSS溶解率和上清液COD都随着辐射功率及辐射时间的增加而升高.适宜的微波辐射能促进污泥的团聚絮凝,过度的辐射会破坏活性污泥结构,使活性污泥颗粒细小化,混合液黏度增大,导致脱水性能变差.通过动态流动下微波辐射对活性污泥性能影响的研究,可为微波辐射在活性污泥处理的实际应用提供理论依据.     

Sulfur speciation and bioaccumulation in camphor tree leaves as atmospheric sulfur indicator analyzed by synchrotron radiation XRF and XANES

Analyzing and understanding the effects of ambient pollution on plants is getting more and more attention as a topic of environmental biology.A method based on synchrotron radiation X-ray fluorescence and X-ray absorption near edge structure spectroscopy was established to analyze the sulfur concentration and speciation in mature camphor tree leaves (CTLs),which were sampled from 5 local fields in Shanghai,China.Annual SO2 concentration,SO42-concentration in atmospheric particulate,SO42-and sulfur concentration in soil were also analyzed to explore the relationship between ambient sulfur sources and the sulfur nutrient cycling in CTLs.Total sulfur concentration in mature camphor tree leaves was 766-1704 mg/kg.The mainly detected sulfur states and their corresponding compounds were +6 (sulfate,include inorganic sulfate and organic sulfate),+5.2 (sulfonate),+2.2 (suloxides),+0.6 (thiols and thiothers),+0.2 (organic sulfides).Total sulfur concentration was strongly correlated with sulfate proportion with a linear correlation coefficient up to 0.977,which suggested that sulfur accumulated in CTLs as sulfate form.Reduced sulfur compounds (organic sulfides,thiols,thioethers,sulfoxide and sulfonate) assimilation was sufficed to meet the nutrient requirement for growth at a balanced level around 526 mg/kg.The sulfate accumulation mainly caused by atmospheric sulfur pollution such as SO2 and airborne sulfate particulate instead of soil contamination.From urban to suburb place,sulfate in mature CTLs decreased as the atmospheric sulfur pollution reduced,but a dramatic increase presented near the seashore,where the marine sulfate emission and maritime activity pollution were significant.The sulfur concentration and speciation in mature CTLs effectively represented the long-term biological accumulation of atmospheric sulfur pollution in local environment.     

红外系统对点源目标作用距离的优化计算

作用距离是红外系统核心性能指标之一,受大气、背景等多方面因素的影响。针对传统作用距离计算方法存在的局限,综合考虑多个影响因素,提出了一种优化计算方法,首次精确计算了作用距离与实际距离之差的大气衰减值,并对计算方法进行了验证。结果表明,优化计算方法具有较好的计算精度,可用于红外系统性能预测和整体设计。     

输变电工程电磁辐射污染的初步探讨

为了解输变电工程对周边环境的影响,对南阳地区某110 kV输变电工程进行实地监测。结果表明,工频电场、工频磁场和无线电干扰远远低于国家相关标准限值,而且随着距离的递增呈衰减趋势。然而监测往往选在"好天气"的时间进行,不能反映"坏天气"的实际状况。结合输变电工程环境影响评价的实际工作经验,分析电磁污染和公众参与现状,发现问题并提出建议。     

Getting ready for the manned mission to Mars: the astronauts’ risk from space radiation

Space programmes are shifting towards planetary exploration and, in particular, towards missions by human beings to the Moon and to Mars. Radiation is considered to be one of the major hazards for personnel in space and has emerged as the most critical issue to be resolved for long-term missions both orbital and interplanetary. The two cosmic sources of radiation that could impact a mission outside the Earth’s magnetic field are solar particle events (SPE) and galactic cosmic rays (GCR). Exposure to the types of ionizing radiation encountered during space travel may cause a number of health-related problems, but the primary concern is related to the increased risk of cancer induction in astronauts. Predictions of cancer risk and acceptable radiation exposure in space are extrapolated from minimal data and are subject to many uncertainties. The paper describes present-day estimates of equivalent doses from GCR and solar cosmic radiation behind various shields and radiation risks for astronauts on a mission to Mars.     

地表UV-B辐射增强对土壤-冬小麦系统呼吸速率和N2O排放的影响

通过室外盆栽实验,用静态箱-气相色谱法测定土壤-冬小麦系统的呼吸速率和N₂O排放通量,研究了UV-B辐射增强20%对土壤-冬小麦系统的呼吸速率和N₂O排放的影响.结果表明,相同的气象条件和田间管理下,UV-B辐射增强处理对呼吸速率和N₂O排放的季节变化模式无明显影响.在返青期,UV-B辐射增强显著降低了土壤-冬小麦系统的呼吸速率,但对N₂O的排放通量没有产生显著影响;在拔节孕穗期,UV-B辐射增强处理显著降低了土壤-冬小麦系统的呼吸速率和N₂O的排放通量;在抽穗-成熟期,UV-B辐射增强处理对土壤-冬小麦系统的呼吸速率和N₂O的排放没有显著影响.返青-齐穗期,UV-B增强处理显著降低土壤-冬小麦系统的N₂O累积排放量;但从齐穗开始至小麦成熟,UV-B增强处理对土壤-冬小麦系统的N₂O累积排放量没有显著影响.     

Ce(Ⅲ)对UV-B辐射胁迫下大豆幼苗光化学反应的影响

用水培法研究Ce(Ⅲ)对UV-B辐射胁迫下大豆幼苗光化学反应的影响.结果表明, 20 mg·L^-1 CeCl₃使大豆幼苗净光合速率(Pn)、Hill反应、Mg²⁺-ATPase活性与光合磷酸化活力4项指标较对照提高23.2%～14.3%; 有效抑制UV-B辐射(T₁=0.15 W·m^-2和T₂=0.45 W·m^-2)胁迫下4项指标下降, 4项指标降幅［Ce(Ⅲ)+T₁为36.6%～15.9%,Ce(Ⅲ)+T₂为65.6%～33.2%］小于对应的UV-B辐射组(T₁为50.9%～23.3%,T₂为77.3%～51.4%). 动态变化显示, Ce(Ⅲ)减缓了胁迫期4项指标的下降趋势,促进了恢复期4项指标上升幅度. 说明Ce(Ⅲ)通过减轻UV-B辐射对大豆幼苗光化学反应的伤害, 遏制UV-B辐射胁迫下大豆幼苗Pn下降.