单道扫描电感耦合等离子体发射光谱法测定珊瑚礁中主量和微量元素

建立了用单道扫描电感耦合等离子体发射光谱法测定珊瑚礁中主量和微量元素的方法。珊瑚礁样品经酸溶解后,直接进行Ca、Mg、K、Na、V、Sr、Ba、Co、Ni、Pb、Li、Rb的测定,方法检出限为0.0004～0.1mg/L,精密度RSD<5%(n=6),样品的加标回收率为97%～105%。测定w(CaO)为50%的样品,结果与传统的EDTA容量法相符。方法经碳酸盐岩石国家一级标准物质验证可行,已用于大批量的珊瑚礁样品的测定。     

高温密闭溶样电感耦合等离子体质谱准确测定辉钼矿铼-锇地质年龄

采用Carius管高温密闭溶样,电感耦合等离子体质谱(ICP MS)法对采自两个不同金属矿床的辉钼矿样品的Re Os同位素地质年龄进行了准确测定。所得出的Re Os年龄的平均值分别为14.26±0.19Ma和34.39±0.81Ma,相对标准偏差分别为1.3%(以2s计算,n=6)和2.4%(以2s计算,n=7)。采用国际通用的ISOPLOT软件按Model1模式对这两组样品分别进行处理,所得Re Os等时线年龄分别为14.32±0.46Ma和34.52±0.38Ma(均为95%置信水平)。同批次样品中所带的内部管理样JDC的Re Os年龄与国际先进实验室采用负离子热表面电离质谱测量所得的结果吻合也较好。说明在严格的质量体系保证及有效地降低实验室空白水平的前提下,ICP MS完全可以准确地测定辉钼矿的Re Os年龄。     

薄层水流速度测量系统的研究

根据水流影响电解质扩散和其导电特性的分析,结合电解质脉冲在水流中迁移的数学模型,设计了薄层水流速度测试系统。用Visual Basic语言编写了操作系统,实现了数据采集、参数计算和分析自动化。实验和模拟结果表明,模拟水槽实验中用流量法测量的流速和电解质扩散法测量的水流速度误差很小,说明用此系统测量浅层水流的流速是可行的。     

CFRP对砖墙抗震加固对比试验研究与计算分析

结合一工程实践的需要，通过5片碳纤维布加固的新建墙体在周期反复荷载作用下的试验，研究了碳纤维布加固对砌体结构抗震性能的影响，以及砌砌体在碳纤维布加固后的受力特性，比较了不同加固方案对砖砌体加固效果的影响，在此基础上讨论了对碳纤维布加固砖墙抗剪承载力计算模型，并提出了简化计算公式。     

陕甘宁盆地陇东地区长8油组厚层非均质砂体的沉积学解剖

通过对延长统长8段厚层砂岩沉积岩石学和层序地层学研究,将其分为两类,一类是由多期单一成因的分流河道砂岩叠加构成;另一类是由三角洲前缘的水下分流河道、河口坝、坝顶席状砂和滑塌砂等多种沉积微相以不同的组合形式叠加构成。首次提出在“高可容纳空间,高沉积通量”背景下,只有经过特殊水动力条件(淘洗)改造后形成的被我们称之为坝顶席状砂的砂岩才有可能成为相对高孔、高渗的优质储层。     

长江流域一次暴雨过程中的不稳定条件分析

文中分析了 1998年 7月 2 0～ 2 3日发生于长江流域的持续性降水和暴雨过程 ,在分析大尺度降水和中小尺度暴雨相对应的环流场和天气实况的基础上 ,主要分析相应大气层结的对流不稳定和条件性对称不稳定条件 ,并对切变线上涡层不稳定做了重点介绍和分析 ,计算了条件性对称不稳定判据和涡层不稳定判据。结果表明 :降水期间大气低层有对流不稳定和对称不稳定能量的积聚 ,在这两类不稳定条件都基本满足的情况下 ,涡层不稳定的维持对此次降水过程中暴雨的发生提供了有利的不稳定环境场 ,具体的计算分析还表明环境场的配置制约着切变线上低涡扰动的发展 ,是造成降水的重要原因之一。     

The onset of Pleistocene glaciation in the Barents Sea: implications for glacial isostatic adjustment

In this paper the effect of a delayed onset of glaciation in the Barents Sea on glacial isostatic adjustment is investigated. The model calculations solve the sea-level equation governing the total mass redistributions associated with the last glaciation cycle on a spherically symmetric, linear, Maxwell viscoelastic earth for two different scenarios for the growth phase of the Barents Sea ice sheet. In the first ice model a linear growing history is used for the Barents Sea ice sheet, which closely relates its development to the build-up of other major Late Pleistocene ice sheets. In the second ice model the accumulation of the Barents Sea ice sheet is restricted to the last 6 ka prior to the last glacial maximum.
The calculations predict relative sea levels, present-day radial velocities, and gravity anomalies for the area formerly covered by the Weichselian ice sheet. The results show that observed relative sea levels in the Barents Sea are appropriate for distinguishing between the different glaciation histories. In particular, present-day observables such as the free-air gravity anomaly over the Barents Sea, and the present-day radial velocities are sensitive to changes in the glaciation history on this scale.
A palaeobathymetry derived from relative sea-level predictions before the last glacial maximum based on the second ice model essentially agrees with a palaeobathymetry derived by Lambeck (1995). The additional emerged areas provide centres for the build-up of an ice sheet and thus support the theory of Hald, Danielsen & Lorentzen (1990) and Mangerud et al. (1992) that the Barents Sea was an essentially marine environment shortly before the last glacial maximum.     

Variation of the plasma turbulence in the central plasma sheet during substorm phases observed by the interball/tail satellite

Fluctuations of the plasma bulk velocity across the plasma sheet are studied using single-point measurements from the Corall instrument on board the Interball/Tail satellite. Several hour-long intervals of continuous data corresponding to quiet geomagnetic conditions and different phases of isolated substorms are analyzed. The plasma sheet flow appears to be strongly turbulent, i.e. dominated by fluctuations that are unpredictable. Corresponding eddy diffusion coefficients were obtained as a function of the autocorrelation time and rms velocity of the fluctuations. It was found that the amplitude of the turbulence and the values of eddy-diffusion coefficients increase significantly during substorm growth and expansion phases and they decrease to their initial level during the recovery phase. We also studied a relationship between the eddy-diffusion coefficients and the absolute value of the geomagnetic field, also measured by the Interball/Tail satellite. It was found that this relationship varies depending on the phase of substorm, indicating possible change in the turbulence regimen with substorm phase.     

Energetic Particles Observed in the CUSP Region During a Storm Recovery Phase

In this paper we report energetic ion behavior and its composition variations observed by the Cluster/RAPID instrument when the spacecraft was travelling in the high latitude magnetospheric boundary region on the day of the 31 March, 2001, strongest magnetic storm in the past 50 years. The Dst index reached −360 nT at about 09:00 UT. During its early recovery phase, large amounts of oxygen and helium ions were observed; the ratio of oxygen to hydrogen in the RAPID energy range reached as high as 250%, which suggests that the observed energetic particles might be of magnetospheric origin. The observations further show that enhanced energetic electron fluxes are confined in a very narrow region, while protons have occupied a larger region, and heavy ions have been observed in an even larger region. The flux of energetic electrons show a slight enhancement in a region where the magnetic field magnitude is around zero. These observed energetic ions could be quasi-trapped by the current sheet in the stagnation region of the cusp.     

Low-Frequency Plasma Waves in the Outer Polar CUSP: A Review of Observations from Prognoz 8, Interball 1, Magion 4, and Cluster

This paper presents a review of the most interesting observations of low-frequency plasma waves together with plasma particles which were made by the Interball 1, Magion 4 and Prognoz 8 satellites in the outer polar cusp. Accelerated plasma particles, hot electron populations and very strong wave activity, particularly at low frequencies, are observed. A detailed study of the wave spectra together with the distribution function for electrons indicate the correlation between the presence of lower-hybrid waves and the population of the particles with higher energy than in the surrounding space. These experimental facts suggest that strong coupling between waves and particles is responsible for plasma heating. During polar cusp crossings by Interball 1 and Prognoz 8, FFT analysis of the wave form indicates many bursts of ULF emissions in both electric and magnetic components. These waves have highly non-stationary characteristics. To study the dynamics of changes in the spectral characteristics of the waves wavelet analysis has been used. Nonlinear interactions are studied using bispectral methods of analysis. This presentation gives the results of such an analysis for selected cusp crossings at different altitudes. An example of wave activity registered by the STAFF instrument onboard the CLUSTER spacecraft in the polar cusp is also presented.