深海主跃层环境对会聚区影响的数值分析

应用BELLHOP模式,对声速剖面的声跃层结构变化引起会聚区偏移特征进行了分析。结果表明,声速垂直结构的变化可导致会聚区位置出现不同程度的偏移:跃层强度增加0.01 s-1将使会聚区向远离声源方向偏移1.5~2.0km;跃层厚度增大50m将使会聚区向靠近声源方向偏移0.3~0.5km;跃层位置加深100m将使会聚区向远离声源方向偏移0.5~1.0km。在跃层的三个特征量中,跃层强度起主导作用。跃层强度变化引起的声线在海洋次表层的偏折差异,进而导致进入深海等温层的入射角差异,是使会聚区发生偏移的决定性因素。     

基于三维荧光光谱-平行因子技术联用的浮游藻化学分类学技术研究

An in vivo three-dimensional fluorescence method for the determination of algae community structure was developed by parallel factor analysis(PARAFAC) and CHEMTAX. The PARAFAC model was applied to fluorescence excitation-emission matrix(EEM) of 60 algae species belonging to five divisions and 11 fluorescent components were identified according to the residual sum of squares and specificity of the composition profiles of fluorescent. By the 11 fluorescent components, the algae species at different growth stages were classified correctly at the division level using Bayesian discriminant analysis(BDA). Then the reference fluorescent component ratio matrix was constructed for CHEMTAX, and the EEM–PARAFAC–CHEMTAX method was developed to differentiate algae taxonomic groups. The correct discrimination ratios(CDRs) when the fluorometric method was used for single-species samples were 100% at the division level, except for Bacillariophyta with a CDR of 95.6%. The CDRs for the mixtures were above 94.0% for the dominant algae species and above 87.0% for the subdominant algae species. However, the CDRs of the subdominant algae species were too low to be unreliable when the relative abundance estimated was less than 15.0%. The fluorometric method was tested using the samples from the Jiaozhou Bay and the mesocosm experiments in the Xiaomai Island Bay in August 2007. The discrimination results of the dominant algae groups agreed with microscopy cell counts, as well as the subdominant algae groups of which the estimated relative abundance was above 15.0%. This technique would be of great aid when low-cost and rapid analysis is needed for samples in a large batch. The fluorometric technique has the ability to correctly identify dominant species with proper abundance both in vivo and in situ.     

四酸溶矿——电感偶合等离子体发射光谱法测定钼矿中的钼

为了适应地质找矿和地质大普查工作对矿样测定速度和正确度的要求,对钼矿样品中的钼的测定方法进行试验,探讨在敞开体系中用盐酸+硝酸+氢氟酸+高氯酸的四酸溶矿体系消解钼矿样品,使用电感耦合等离子发射光谱仪(ICP-AES)测定钼的方法。     

iCAP 6300电感耦合等离子体发射光谱仪的常规维护方法

电感耦合等离子体发射光谱仪在使用过程中,由于控制气体流量的电磁阀出现机械性移位,致使工作气流量过于偏大或偏小,对进样系统及分析数据产生不利影响;长期频繁使用条件下,由于控制光学系统的机械定位装置的磨损,致使谱峰坐标偏离而影响仪器灵敏度;很长时间不能"引燃"等离子体,检查进样系统和氩气纯度并没有发现异常,需要验证RF发生器有无功率输出时有一定的困难;在等离子体工作时产生的高温尾气的长期作用下,难免造成点火头末端铜丝的锈蚀,致使点火头放电微弱,不能"引燃"等离子体。因此,为保证仪器的正常运行,提高工作效率,确保检测数据的准确度,实验室应建立健全电感耦合等离子体发射光谱仪维护保养方案,解决上述问题。本文结合实际工作经验,以iCAP 6300电感耦合等离子体发射光谱仪为例,提出可以借助"Manufacturing and Service.exe"程序校正工作气流量,验证RF发生器是否输出功率;利用C 193.091 nm谱线为基准校正谱线修正CID检测器的谱峰坐标系统;另外,对点火头、分析软件数据库及主机灰尘的清理也进行了详细的维护说明,这些措施有益于保障仪器的性能及提高设备的利用率。     

不同加载条件下陕西华山花岗岩破坏过程的声发射特性

对陕西华山花岗岩试样进行单轴和常规三轴破坏过程的声发射参数测试,研究单轴和三轴两种应力条件下花岗岩破坏过程的声发射特性差异。结果表明,两种加载条件下,声发射特征均基本符合岩石加载破坏过程中的4个阶段,单轴下峰值应力前声发射平台现象明显,三轴下未出现明显声发射平台。弹性阶段内声发射信号均比较少,进入塑性阶段后声发射信号开始密集出现;破坏过程中声发射幅值主要范围都集中在40~100dB;在岩样破坏之前,都会出现事件计数、振铃计数率和累计释放能量逐渐升高的过程;达到峰值强度时,均出现振铃计数率和累计释放能量跳跃性的增长,因此可以将振铃计数率和累计释放能量的突增作为岩样破坏的前兆。此外,研究发现此花岗岩的声发射特征与其承载的路径密切相关,从而进一步验证了岩石材料声发射中的Kaiser效应。     

多普勒气象雷达发射系统故障分析与处理

正1引言民航吉林空管分局气象台多普勒天气雷达是由安徽四创电子股份有限公司设计、研制的C波段全相参脉冲多普勒天气雷达。能够完成探测降水回波的位置、强度,定量测量200km范围内气象目标的强度。它是警戒强对流危险天气,分析中小尺度天气系统,制作短时天气预报的强有力的工具。多普勒天气雷达发射机是雷达系统的重要组成部分,相对其他单元,由于大量器件长期工作在大电流、高电压、高功率环境下,故障率较高。本文     

对脉冲星发射宇宙线能量的估计

S.Karakula等人根据Ostriker等人的脉冲星产生的宇宙线能谱依赖脉冲星年龄的理论模型,利用脉冲星发射宇宙线的最大能量:     

The Correlation between Gamma-ray and Radio Emissions in γ-ray Loud Blazars

We collect 119 v-ray-loud blazars (97 flat spectrum radio quasars (FSRQs) and 22 BL Lacertae objects (BL Lacs)), and investigate possible correlations between their γ-ray emission (maximum, minimum and average values) at 1 GeV and the radio emission at 8.4 GHz. Our main results are as follows. For the lower state γ-ray data, there is no correlation between the γ-ray and radio flux density; For the high state γ-ray data, there are good correlations for the whole 119 blazars and 97 FSRQs, and a weak correlation for the 22 BL Lac objects; For the average γ-ray data, there are good correlations. According to our analysis, we propose that the γ-rays are associated with the radio emission from the jet, and that the γ-ray emission is likely from the SSC process in this case.