面向对象自适应渗流有限元分析软件的研究和实现

采用面向对象技术,应用C++研制了一个自适应渗流有限元分析系统。该软件系统的前处理过程用对象化建模,具有实现方便,界面友好的优点。自适应有限元模块的引入使该系统具有规范性和客观性,计算结果不会因人而异,且后处理界面形象直观。笔者还给出了一个土坝渗流的实例,验证了该软件的可用性和优点。     

基于模型的3D3C采集设计与评价

对目前三维三分量(3D3C)地震勘探数据采集设计的方法进行了系统分析,利用聚焦射束分析技术(CFP),提出了基于模型的3D3C采集设计方法及其评价的参数。从模型出发的设计方法,能够使3D3C的采集结果更加真实可靠。      

The carbon accumulation and dissipation features of sub—alpine woodland in Mt.Gongga

Based on biomass investigations,soil respiration and plant photosynthesis measurement of dominant trees in Hailuogou valley of Mt.Gongga,Southwest China,the carbon(C) storage,absorption and release for several typical woodlands in sub-alpine zones have been discussed.For Abies fahri forest of 3,000 m above sea level,the Cstorage amount is 177.4t/ha for above-ground biomass and 143.2 t/ha for soil below-ground biomass. The annual gross C fixed by vegetation photosynthesis is 20-24 t/ha. The C release by canopy respiration is 3.0-5.5 t/ha for arbors and 10-19 t/ha for surface soil and roots.The annual net C fixed of forest ecosystem is about 6.0-7.1 t/ha.At lower elevations,the amount of C released by woodlands is higher than that of woods at higher elevations.The C fixed capacity of renewed forest with middle-aged trees is higher than that of mature forest.Before becoming over-matured forest,woodland is an important sink of C whereas bareland in woods is the source of atmospheric C.     

云南程海现代沉积物环境记录研究

本文通过对程海沉积物Ｃ、Ｈ、Ｎ等元素含量及其比值的综合分析,辨识了程海沉积物有机质Ｈ／Ｃ及Ｃ／Ｎ值的环境指示意义,发现它们增可作为程海水位波动及区域气候干湿变迁的替代性指标。研究结果表明：程海的水位和区域气候干湿主为化明显以历了两个不同的阶段,但整体上程海水位一直呈下降趋势,反映区域气候整体上向干旱化方向发展。     

Zw 1718.10108: a highly disturbed galaxy cluster at low Galactic latitude

We report the discovery of highly distorted X-ray emission associated with the nearby cluster Zw 1718.10108, one of the dominant members of which is the powerful radio galaxy 3C353. This cluster has been missed by previous X-ray cluster surveys because of its low Galactic latitude ( b =19.5°), despite its brightness in the hard X-ray band (210 keV flux of 1.210¹¹ erg cm² s¹). Our optical charge-coupled device image of the central part of the cluster reveals many member galaxies which are dimmed substantially by heavy Galactic extinction. We have measured redshifts of three bright galaxies near the X-ray emission peak and they are all found to be around z =0.028. The ASCA gas imaging spectrometer and ROSAT high-resolution imager images show three aligned X-ray clumps embedded in low surface-brightness X-ray emission extended by 30 arcmin. The averaged temperature measured with ASCA is kT =4.3±0.2 keV, which appears to be hot for the bolometric luminosity when compared with the temperatureluminosity correlation of galaxy clusters. The irregular X-ray morphology and evidence for a non-uniform temperature distribution suggest that the system is undergoing a merger of substructures. Since the sizes and luminosities of the individual clumps are consistent with those of galaxy groups, Zw 1718.10108 is interpreted as an on-going merger of galaxy groups in a dark matter halo forming a cluster of galaxies and thus is in a transition phase of cluster formation.     

Extended X-ray emission in the radio-loud galaxy 3C 382

ROSAT /HRI observations of the powerful radio-loud galaxy 3C 382 reveal extended X-ray emission associated with the source. On the basis of this new spatial component, a previous ROSAT /PSPC spectral analysis of the source is revised. Allowing for the presence of an additional thermal component in the PSPC spectrum, the non-thermal component is found to be compatible with the extrapolation of the well-defined 3C 382, 2–10 keV, power-law spectrum into the soft X-ray region. The thermal – extended – component would then account for the soft excess emission previously reported for this source. The origin of this thermal component is not clear. Its luminosity compares with that of rich Abell clusters; yet, the galaxy environment in 3C 382 appears of moderate optical richness. An alternative is that it is the result of a massive extended gaseous atmosphere sustained by the deep gravitational potential well of 3C 382.     

BDS-3新频点单点定位研究

针对目前有关北斗卫星导航系统(BDS-3)中MEO卫星(BDS-3M)增加的B1C、B2a新频点单点定位研究较少的现状,本文开展了基于新频点B1C、B2a的双频单点定位试验,结合国际GNSS监测评估系统(iGMAS)5个跟踪站连续10 d的数据,对BDS-3的新频点进行数据质量分析、双频伪距单点定位(SPP)和双频静态...     

利用FY-3C折射率对大气边界层高度的反演与分析

2013年中国发射了首颗进行全球导航卫星系统(global navigation satellite system,GNSS)掩星观测的气象卫星风云3号C星(Fengyun-3C,FY-3C),且已发布自2014年6月以来的FY-3C掩星大气产品,但目前还未见将其应用于大气边界层的相关研究.首次尝试利用FY-3C折射率...     

基于民用航空规章的结冰气象条件探测数据分析方法

我国极度缺乏结冰气象条件中的云层数据,我国民用航空规章第25部附录C结冰条件只能复制于美国航空规章,对飞行探测得到的结冰云层数据进行附录C符合性分析的方法也少有研究。附录C结冰条件形成于20世纪40年代末,当时的探测手段与如今采用先进探测仪器所获取的数据形式有很大差异,因此首先明确附录C结冰条件参数的具体定义,根据当前探测仪器测量数据的高分辨率特性,对数据处理与分析方法进行研究。最后基于该方法对安庆结冰气象探测数据进行了分析,从分析结果看,该方法能够清晰呈现所探测结冰云层的结冰条件基本特征及其与附录C的符合性程度。