基于RTP的矢量数据流式传输研究

针对WebGIS中大规模矢量数据的网络传输问题,提出采用流式传输方式分批次向客户端传输所需数据,从而达到矢量数据在线实时应用的目的。通过研究流式传输机制,建立了适应于矢量数据流式传输的服务框架;按照流式传输的要求,对矢量数据进行分块组织,保证每个批次的要素作为独立的单元传输并在客户端处理;在传输过程中,实时传输协议实现了矢量数据流式传输机制,并参照流媒体文件“边传边播”的模式,设计了矢量数据的封包和解包算法。该方法实现了矢量数据的发送和接收,达到了多次往复传输的目标,且能通过差错控制和压缩加密等手段提高数据传输效率、保证数据传输质量和安全。实验证明,矢量数据的流式传输能降低约一半的数据传输量,有效地提高了传输效率,降低了系统响应时间。     

Intricacies of the fine structure of the eclipse corona

The inner white-light corona (up to 2 solar radii) can only be observed during total solar eclipses. New mathematical methods of the corona image processing and digital photo cameras or CCD cameras allow us to detect very faint structures (of a few arcseconds) in this part of the corona, even from images taken with relatively small telescopes (1–2 meters in the focal length). In the present paper we will discuss such structures as observed during the last few solar eclipses, mainly those of 2001 and 2006. Obtained results show that the white-light corona is highly structured not only in the sense of a variety of different types of its classical “objects”, e.g., polar plumes, helmet streamers, threadlike streamers, etc, but also within these objects themselves. Voids, loops, radial and non-radial threads, and other yet-undefined dark structures (“empty space”?) are well visible especially inside helmet streamers. This strongly indicates that the classical picture of the corona characterized by a hydrostatic distribution of density and temperature is no longer a sufficient assumption. It is magnetic forces that play a dominant role in shaping and structuring this part the corona. Given a remarkable similarity between the EUV corona as observed by SOHO and the white-light corona observed by us during the above-mentioned eclipses up to two solar radii. We suggest that the “missing” observations of the white-light corona should be replaced by those of the EUV one. Moreover, the last eclipse’s observations also indicate that the knots of some prominences extend well into the white-light corona. So, the next total eclipses of the Sun, of 1 August 2008 and 22 July 2009, offer an excellent opportunity for preparing joint observations for space-borne and ground-based eclipse teams.     

Expression of Mammalian Metallothionein-I Gene in Cyanobacteria to Enhance Heavy Metal Resistance

Metallothionein (MT) from mammals is a low molecular weight (about 6–7 KD), and cystein-rich (20 cystein per molecular) protein (Vallee, 1991). So MT has the strong binding ability of metal such as Cd, Hg and Pd. Wild-typed cyanobacteria have their own metallothionein-like proteins, which are of low cysteine content and have weak ability to bind heavy metal. Therefore, it is imperative to transfer the MT-I gene from mammal into cyanobacteria cell for the absorption and accumulation of heavy metals in aqueous system including marine and lake ( Misra and Gedamu, 1989). We inserted the MT-I cDNA gene after the strong promoter PpsbA or Psmt into the intermediary vector pRL-439, and then pRL-MT was ligated with shuttle vector pKT-210 (a shuttle vector pDC-08 was used at an earlier time) to construct the shuttle expression vector pKT-MT. (The MT-I mutant -KKS- also was selected as aim gene.) Then the constructed vector was introduced into cyanobacterium Anabaena sp. PCC7120, Synechocystis sp. PCC6803 and Synechococcus sp. PCC7942 with triparental conjunctive transfer (Bryant, 1994). The expression efficiency is about 1%. We also used homologous recombination vector pTZ18-8 to introduce MT-I cDNA into chromosomes in cyanobacteria and got higher expression efficiency. Metal tolerance tests show that the transgenic cyanobacteria acquire metal resistance up to 60 μmol/g CdCl₂ and expression efficiency up to 1045 μg MT/g fresh cells according to the data of ELISA.     

Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method

Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered.     

海南三亚鹿回头虫黄藻(Effrenium voratum)的形态学和系统发育学研究

本文对分离于我国海南三亚鹿回头海域的两株虫黄藻SYSC-14-11和SYSC-2-8进行了分类学研究。通过光学显微镜、扫描电子显微镜和分子生物学方法描述了两株藻的形态和系统发育特征, 并与世界其他地理区系的Effrenium属虫黄藻进行了差异性比较, 发现本研究中的两株虫黄藻的形态和系统发育特征与Effrenium属虫黄藻模式种Effrenium voratum基本一致, 推测本文中的两株Effrenium属虫黄藻均为E. voratum。本研究丰富了我国热带海域虫黄藻的物种多样性, 为完善我国的虫黄藻种质资源奠定了基础。     

基于性能的黏弹性阻尼器减震结构抗震设计

根据黏弹性阻尼器的特点和抗震规范的要求,分别提出了用于黏弹性阻尼器减震结构抗震分析的弹性及弹塑性需求谱,前者是基于黏弹性阻尼器减震结构等效阻尼比的简化计算公式及规范规定的反应谱;后者是基于修正的V id icRμ-μ-T关系。在此基础上,借助模态推覆分析,提出了可以考虑高阶振型影响的黏弹性阻尼器消能减震结构体系的能力谱分析方法,并对一8层钢筋混凝土消能减震框架结构进行了"中震不坏,大震可修"性能水准下的抗震分析。算例结果表明,采用该方法分析黏弹性阻尼器减震结构体系是可行的、有效的。     

河流中污染物衰减系数影响因素分析

污染物衰减系数是反映河流水质污染变化情况、建立水质模型、计算水环境容量的重要参数之一,其确定的合理性直接影响到水环境容量以及水质模型的可靠性。通过查阅有关文献,概述了国内外部分河流的COD和BOD以及氨氮的衰减系数,并分析了影响污染物衰减系数的主要因素,为研究河流水体自净规律、计算水环境容量、区域排污总量控制计划的制定提供科学依据。     

新疆春季气温异常的区域特征

利用新疆52个测站1961～2000年3～5月逐日平均气温资料，采用旋转经验正交展开（REOF）方法对新疆春季气温场进行客观分区，分析了各区域春季气温的不同时间尺度变化趋势。结果表明：新疆春季气温场可分为3个区域，北疆区和南疆区的长期变化呈下降趋势，而东疆区呈上升趋势；各区域存在明显不同的年际、年代际方差构成和多尺度振荡周期。     

中国西北地区石炭系泥岩稀土元素地球化学特征及其地质意义

详细研究了中国西北地区石炭系泥岩的稀土元素地球化学特征。各样品稀土总量为18 86× 10 -6～ 6 2 0 4× 10 -6,变化较大 ,其中祁连地区REE总量为 76 49× 10 -6～ 6 2 0 4×10 -6,甘肃永昌煤山子剖面的稀土总量最高 ,新疆北部地区泥岩和灰岩 (泥灰岩 )的稀土总量均较低。各泥岩样品的轻稀土富集 ,Eu负异常 ,δEu介于 0 44～ 0 90之间 ,δCe部分为正异常 (>1) ,部分为负异常 (<1)。研究区样品的Sm含量与北美页岩样品相比为正异常 ,Dy出现负异常的样品较多。根据稀土元素δCe和Ceanow的变化 ,反映当时新疆北部地区水介质环境大部分为缺氧的还原条件 ;祁连地区为海陆过渡环境 ,部分为氧化条件 ,另一部分为缺氧的还原条件 ,这与其他相标志所显示的结果是一致的。根据稀土元素组合及比值的变化 ,显示物源区母岩为花岗岩和玄武岩的混合来源 ,稀土分布模式均为轻稀土富集、重稀土亏损型 ,重稀土配分曲线较为平坦 ,显示源岩为粘土岩、花岗岩和中性岩的混合来源。     

哈密地区一次大降水天气过程分析

对哈密2001年10月大降水天气过程的降水成因进行了分析，表明低空急流和上升运动是其形成的重要机制，同时在哈密地区大降水天气短期预报着眼点方面获得了一些有益的启示。