A Study of Photoelectricity Chemistry in Different Acidity Solution of Agglutination Ferric Oxide

采用了烧结的方法制备了氧化铁电极,并讨论了在不同的酸度中电极的光电化学行为.得到了不同酸度中的光电流谱图,并结合XPS分析研究,发现电极表面是不均匀的,存在着两种类型的晶粒.In this paper,the photoelectricity chemistry of sinter ferric oxide electrode in different acidity solution were studied and the photocurrent spectrorams in different acidity were gained.It comes to the conclusion that two type of crystal were found in the electrode surface that is not even by XPS analysis

黄土关键带深层土壤水分动态模拟与主控因素

地球关键带是维系地球生态系统功能和人类生存的关键区域,土壤水分是黄土高原关键带植被恢复与生态环境重建的关键因子之一。为探明黄土关键带深剖面土壤水分变化过程并进行模型模拟,对黄土高原长武塬区苹果地和小麦地的深层土壤水分(0~18m)进行监测(2011~2013年,共选择11个不同日期进行深剖面土壤水分监测),在此基础上,采用Hydrus-1D进行模型模拟,分析了深剖面土壤水分动态及其模拟效果的主控因素。结果表明:1)苹果地(6~18m)、小麦地(3~18m)的深层土壤含水量随时间变化很小;0~1m的土壤含水量随时间变化较大;不同土地利用类型会产生不同的土壤水分过程及运动机制;在根系及近根系区,土壤含水量变化受根系分布格局及土壤质地共同影响,接近地表时还同时受降雨、蒸发等上边界条件影响;在非根系区,土壤含水量的主要影响因素为土壤质地;2)利用前6次的实测数据进行调参和校正,后5次实测数据进行预测效果检验,取得了较好的深剖面土壤水分模拟效果&mdash;&mdash;苹果地的决定系数、相对误差绝对值、均方根误差分别介于0.5923~ 0.7637、3.33%~5.20%、0.0149~0.0168cm~3/cm~3之间,小麦地分别介于0.2414~0.6822、2.64%~4.58%、 0.0177~0.0247cm~3/cm~3之间;3)叶面积指数、根系深度与分布是影响深剖面土壤水分动态模拟效果的主控因素。相关结果可为黄土关键带深剖面土壤水分模拟与调控提供参考。</p

大连极紫外相干光源

先进光源的发展在前沿科学研究中发挥的作用越来越重要。近十年来,飞速发展的自由电子激光技术为科学家们提供了探索未知世界、发现新科学规律和实现技术变革的重要工具。建成的大连极紫外(EUV)相干光源的运行波段为50~150nm,单脉冲能量大于100μJ,且可提供10-12 s和10-13 s量级的超快激光脉冲,是我国第一台自由电子激光用户装置,并且是国际上唯一运行在极紫外波段的自由电子激光用户装置,在世界范围内为用户提供具有高峰值亮度和超短脉冲的极紫外激光。大连EUV相干光源是由国家自然科学基金委资助、由中国科学院大连化学物理研究所和上海应用物理研究所共同承担的重大科学仪器研制项目,目标是打造一个以先进极紫外光源为核心、主要用于能源基础科学研究的光子科学平台

JUNO Sensitivity on Proton Decay p→νˉK+p\to \bar\nu K^+ Searches

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this paper, the potential on searching for proton decay in $p\to \bar\nu K^+$ mode with JUNO is investigated.The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification. Moreover, the excellent energy resolution of JUNO permits to suppress the sizable background caused by other delayed signals. Based on these advantages, the detection efficiency for the proton decay via $p\to \bar\nu K^+$ is 36.9% with a background level of 0.2 events after 10 years of data taking. The estimated sensitivity based on 200 kton-years exposure is $9.6 \times 10^{33}$ years, competitive with the current best limits on the proton lifetime in this channel

JUNO sensitivity on proton decay p → ν K + searches*

The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this study, the potential of searching for proton decay in the $p\to \bar{\nu} K^+$ mode with JUNO is investigated. The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification. Moreover, the excellent energy resolution of JUNO permits suppression of the sizable background caused by other delayed signals. Based on these advantages, the detection efficiency for the proton decay via $p\to \bar{\nu} K^+$ is 36.9% ± 4.9% with a background level of $0.2\pm 0.05({\rm syst})\pm$$0.2({\rm stat})$ events after 10 years of data collection. The estimated sensitivity based on 200 kton-years of exposure is $9.6 \times 10^{33}$ years, which is competitive with the current best limits on the proton lifetime in this channel and complements the use of different detection technologies