光学选射电噪类星体的射电性质

对类星体进行多波段的观测和研究,是了解类星体本质的一个重要途径．LBQS类星体是目前公认较为完备的一个光学选类星体样本,利用此样本与最新的485GHz全天射电源表进行了交叉证认,共找到了34个类星体的对应射电源．计算证明,这34个类星体都是射电噪的类星体．所得研究结果表明,射电噪类星体的射电光度与光学光度之间存在线性相关性．     

Radio Identifications of Markarian Galaxies and the Correlation between Radio and Far-Infrared Properties

By checking DSS optical images and NVSS radio images, 782 Markarian galaxies were identified to be NVSS radio sources. A comparison of the radio luminosity at 1.4 GHz and the far-infrared (FIR) luminosity for 468 "normal" galaxies shows a tight correlation. Most of the Seyfert galaxies and quasars follow the radio-FIR relation deduced from the "normal" galaxy sample, but with a somewhat larger scatter. A total 167 Markarian galaxies, comprising 100 "normal" galaxies, 66 Seyfert galaxies and one quasar, have either excess radio emission or much lower FIR spectral index α(25μm,60μm). These galaxies may be classified as "AGN-powered". For "normal" galaxies, the average q value (defined as the log ratio between FIR and radio luminosities) is 2.3. There seems a trend for q to slightly decrease with increasing radio luminosity. This may imply that the ongoing active star formation in galaxies with higher radio luminosities is more efficient in heating the cosmic-ray electrons.     

美国长岛湾缺氧现象及其治理对策综述

近年来,缺氧(hypoxia)现象成为世界范围大洋沿岸水域的一个主要环境问题.本文介绍了由美国环境保护署协调进行的“长岛湾研究”项目对缺氧现象的成因、影响及其与海洋富营养化的关系所做的研究,同时介绍了治理缺氧所采取的对策.     

基于北斗的全海深装备定位与通信系统设计与实现

基于北斗双模工作模式,设计一种将全海深海洋装备的地理位置信息提供给母船或控制中心的定位与通信系统。提出使用卫星无线电导航业务RNSS模式进行定位,并将位置及待传输信息通过卫星无线电测定业务RDSS模式发送至接收模块;采用光敏、倾角和温度多传感器组合冗余实现海洋装备作业环境的全天候有效检测,进而通过单片机控制北斗模块的休眠与唤醒及北斗系统RDSS／RNSS模式间切换。定位测试试验和马里亚纳海沟海试结果表明,所设计的全海深定位与通信系统不仅具有很高的快速定位成功率,而且能够有效节约电池电量和实现短报文信息传输。      

20马力玻璃钢渔船的总体设计

作者为开发新型渔船并改善其性能和节约木材,设计了20马力玻璃钢渔船。船体总长Loa=13.65米,船宽B=3.40米,型深D=1.15米,平均吃水T_m=0.82米,航速V=6.5节,满载排水量为17.19吨,自持力为10天。全船采用玻璃钢材料,并设计成折角线形横剖面、延伸甲板和收缩形舭龙骨。本船稳性满足规范要求。横摇性能及适航性能良好。     

海洋水团的Fisher型逐步判别预报

判别分析是多元分析方法之一,我们将其应用于海洋水团的判别预报。用逐步判别的方法挑选因子,依每个因子的Wilks量进行F—检验,逐步地将判别“能力”强的因子选入。同时将由于其他因子组合而相形见绌者及时剔除。根据矩阵变换的信息,给出了Fisher型逐步判别预报式。将北黄海冷水团强度预报作为示例,给出了筛选因子及建立判别式的全过程。用历史资料检验了预报效果。与习用的Bayes型逐步判别预报进行了对比。     

Cambrian Reefs in the Western North China Platform, Wuhai, Inner Mongolia

Mid to late Cambrian thrombolites and maze-like maceriate reefs from the western North China Platform, Wuhai, Inner Mongolia, northwestern China, occur in the middle of a succession dominated by thin-bedded lime mudstone-shale/marlstone alternations, and are laterally surrounded by limestone conglomerate and/or grainstone. Thrombolite, characterized by meter-scale lenticular mounds composed of millimeter- to centimeter-scale mesoclots and wackestone matrix, occurs in the lower middle part of the sequence. Thrombolite mesoclots are composed of microstromatolites with alternating dark gray and light gray micritic laminae. The maze-like maceriate reefs occur in the middle to the upper part of the sequence, commonly forming lenticular mounds up to 1 m thick. They are characterized by centimeter- to decimeter-scale branched maze-like structures, whose biogenic portions (maceria) are selectively dolomitized. The maceriae are composed of poorly preserved microstromatolites and siliceous sponges. Inter-macerial sediments consist of lime mud and scattered bioclasts. These Wuhai reefs are generally similar to but older than various other Cambrian reefs previously reported from the Shandong region, northeastern China.     

基于PixelGrid及ADS100新型航摄仪的1∶2000DOM生产

数字正射影像图大规模的制作与应用是基础测绘发展的基本要求,现已为数字城市、不动产登记基础数据建设等提供有力的信息支持和保障。随着航空遥感技术的快速发展,推扫式影像的应用因其优势而发展迅猛,ADS100推扫式大幅面影像数据的生产,减少了人工干预,降低了工作量,提高了生产效率。本文结合湖南省不动产统一登记基础数据建设项目,总结了ADS100推扫式影像正射影像图的生产工艺及质量控制。该方法已经在生产实践中得到了验证,既能够保证产品精度又能够提高生产效率,对推动不动产统一登记基础数据建设具有一定的借鉴意义。     

基于水文地球化学模拟的昆特依盐湖杂卤石成矿流体来源初步研究

摘 要: 柴达木盆地昆特依盐湖赋存大量杂卤石。研究结果显示,苏干湖湖水模拟蒸发析出的盐类矿物与研究区实际情况相符,但杂卤石析出量很少;油田卤水模拟析盐结果中没有发现杂卤石,且析出盐类矿物与实际情况差异很大。典型钻孔杂卤石饱和指数（SI）分析表明,卤水相对杂卤石而言是不饱和的。综合分析揭示,地表水应该是昆特依盐湖成盐物质的主要来源,而深部油田卤水对于杂卤石的形成具有重要作用,杂卤石的沉积是不同流体混合作用的结果。     

Research on magnetic fields of galaxies using RZ-model

The generation of magnetic fields of galaxies is usually described by the dynamo mechanism.This process is characterized by the Steenbeck-Krause-Radler equation,which is the result of averaging the magnetohydrodynamics equations by distances which are associated with the size of turbulent cells in the interstellar medium.This equation is quite difficult to solve both from an analytical and numerical point of view.For galaxies,the no-z approximation is widely used.It describes the magnetic fields in thin discs.For such objects,where it is important to study the vertical structure of the field,it is not very applicable,so it is quite useful to adopt the RZ-model,which takes into account the dependence of the distance from the equatorial plane.During our research we have obtained the critical values of the dynamo number for galaxies with large half-thickness.We have also described typical z-structure for the magnetic field.Moreover,we have demonstrated that it is possible to generate dipolar magnetic fields.