Lithium Abundances in the Atmospheres of SLR C-Giants WZ Cas and WX Cyg from Resonance and Subordinate Li I Lines

Lithium abundances in the atmospheres of the super Li-rich C-giants WZ Cas and WX Cyg are derived by the spectral synthesis technique using the Li I resonance line at λ670.8 nm and three subordinate lines at λλ 812.6, 610.4 and 497.2 nm. The differences between the Li abundances derived from the λ670.8 nm line and the λλ 497.2, 812.6 nm lines do not exceed ±0.5 dex. The lithium line at λ610.4 nm provides typically lower abundances than the resonance line (by ≈ 1 dex). The mean LTE and NLTE Li abundances from three Li I lines (excluding λ610.4 nm) are 4.7, 4.9 for WZ Cas, and 4.6, 4.8 for WX Cyg, respectively. This revised version was published online in July 2006 with corrections to the Cover Date.     

Fractional crystallization models and B–Be–Li systematics at Mt Somma-Vesuvius volcano (Southern Italy)

A compilation of B–Be–Li data on rocks that cover the entire eruptive history of Somma-Vesuvius is presented and interpreted in the light of evolution models for the Somma-Vesuvius rocks. Using major and trace element data, fractional crystalllization models are presented for different geochemical units. These data were used to constrain the source mineralogy of the Somma-Vesuvius rocks (ol-opx-cpx-gar-amp of 0.4-0.3-0.1-0.1-0.1), the amount of sediment added (5–10%) and the melt fraction from batch partial melting computations (0.05–0.1). From the B–Li data it is inferred that the main process responsible for the B isotopic signature is sediment recycling. However, the B–Li data show a major variation in Li abundances respect to B which is explained with Li dehydration before the fluid enriched the mantle wedge that produced the arc magmas. The Somma-Vesuvius B isotope composition is intermediate between that of the Campi Flegrei and the broad field of the Eolian Island arc. A low Be isotopes in the recent volcanic rocks can be explained as: (a) the top 1–22 m of the incoming sediment is accreted, (b) large amounts of sediment erosion, (c) a slow rate of subduction which have provoked a long magmatic history for the Vesuvius magma, (d) the sediment component takes several Myr longer than the subducting plate to reach the magma source region beneath Italy.     

不同浓度Li2SO4水溶液结构的X射线衍射研究

用θ～ 2θ型粉末衍射仪反射法精确测量了不同浓度的Li2 SO4水溶液的衍射数据 ,通过数据处理给出了溶液的结构函数和径向分布函数 ,由几何结构模型的最小二乘法精修 ,得到了溶液中阳离子和阴离子第一、二水合层的结构参数。     

Precise/ Small Sample Size Determinations of Lithium Isotopic Compositions of Geological Reference Materials and Modern Seawater by MC-ICP-MS

The Li isotope ratios of four international rock reference materials, USGS BHVO-2, GSJ JB-2, JG-2, JA-1 and modern seawater (Mediterranean, Pacific and North Atlantic) were determined using multi-collector inductively coupled plasma-mass spectrometry (MC-ICP-MS). These reference materials of natural samples were chosen to span a considerable range in Li isotope ratios and cover several different matrices in order to provide a useful benchmark for future studies. Our new analytical technique achieves significantly higher precision and reproducibility (< ± O.3%o 2s) than previous methods, with the additional advantage of requiring very low sample masses of ca . 2 ng of Li.     

可见光下Li+/CNTS-TiO2光催化剂降解海洋柴油污染的研究

通过溶胶-凝胶法,以CNTS-TiO₂为前驱物制备了Li⁺掺杂CNTS-TiO₂的纳米复合光催化剂(以下均称为Li⁺/CNTS-TiO₂),采用X射线衍射(XRD)、扫描电镜(SEM)等测试手段对光催化剂进行表征,结果表明制得的催化剂为纳米材料且在TiO₂的基础上增大了比表面积。利用掺杂量为3%的Li⁺掺杂CNTS-TiO₂复合光催化剂(以下均称为3%Li⁺/CNTS-TiO₂)光催化降解海洋柴油污染,在可见光条件下考察了Li⁺掺杂量、煅烧温度、光催化剂投加量、柴油初始质量浓度、光催化反应时间、H₂O₂质量浓度等条件对光催化实验的影响。进行正交实验,确定最优化工艺条件为:Li⁺掺杂量为3%,光催化剂的煅烧温度为600 ℃,3%Li⁺/CNTS-TiO₂的投加量为0.1 g/L,降解柴油初始质量浓度为0.4 g/L,光催化反应时间为3 h,H₂O₂质量浓度为0.6 g/L,降解率可以达到95%以上。同时对此光催化剂进行应用试验,试验结果表明光催化剂去除效果优异,去除率可达91.87%。     

黎安港海水和沉积物中叶绿素a含量及与环境因子的关系分析

在2019年6月和9月对黎安港海域9个站点进行水质和沉积物采样调查,研究叶绿素a含量在潟湖内的空间分布,并探讨叶绿素a含量与相关环境因子的关系,为黎安省级海草特别保护区的海草资源保护与恢复提供基础数据及理论研究.结果表明:水体叶绿素a含量时空分布不均匀.6月,水体叶绿素a含量变化范围为3.34μg/L?14.64μg/...     

纪念李世雄教授

本文以笔者所能领悟到的李世雄教授对提升油气勘探科学水平做出的贡献,阐述他近20年来在地震成像、Wavelet、独立分量分析（ICA）和复杂条件下动力学问题的理论方法研究成果,并对李世雄教授为提升年青后学者科学判断力和促进研究群体有效成果产出的指导风范,深表敬意.     

集均衡;;汇集干扰;;屏蔽介绍了临钢

,CATV of Lingfen Iron and Steel Company,Lingfen Shanxi 041000,China)This article introduces the design idea and experiences in innovating process of bi-directional HFC network,the design ideas of light pitch point,the optical cable skeleton line and the assignment network.Also the     

区域气候模式侧边界的处理对东亚夏季风降水模拟的影响

在区域气候模式模拟中,侧边界的作用是引入大尺度强迫场。如何处理好侧边界,即大尺度强迫场和区域气候模式本身之间的关系问题,对于区域气候模式模拟和预报东亚夏季风降水具有重要意义。本文利用美国纽约州立大学Albany分校的区域气候模式（SUNYA-ReCM）,设计了两种不同的侧边界处理方法,来探讨侧边界对东亚夏季风降水模拟的影响。驱动区域模式的大尺度强迫场来自欧洲中期天气预报中心（ECMWF）及热带海洋大气研究计划（TOGA）的分析资料场。试验结果表明:（1）当模式的区域较大时,采用较小的侧边界缓冲区会在缓冲区与模式内部的交界处产生不连续;扩大缓冲区并且考虑不同尺度强迫在垂直方向上的不同作用,可以避免这一缺陷。（2）更重要的是采用后一种方案,即减少了区域气候模式在模拟大尺度环流场方面所起的作用,使得模式更多地依赖侧边界来得到更真实的、对东亚夏季风降水起重大影响的一些气流,如副高、西南季风和南海季风,对东亚夏季风降水无论是在大小上还是在雨带位置的演变上都能进行更好的模拟。     

明嘉靖六年《大统历》历书的气朔推步精度

历书是历法的民用本.考察了明嘉靖六年(1527年)<大统历>历书,根据历书所颁朔日和节气时刻,以及先期恢复的<授时历>和<大统历>推步术,并利用现代天文历算结果,可考校得出:(1)历书所载朔日和节气日期、时刻确由<大统历>推得;(2)<大统历>与<授时历>推步结果存在差异,推朔平均差33.35 min或34.93 min,推气平均差86.40 min,且两者均有差1日现象;(3)<大统历>与现代推算合朔时刻的平均误差为24.50 min或44.03 min,与现代推算节气时刻的差平均为1.25 d,若扣除太阳中心差则节气推步的误差将减少到86.40 min.