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1.
吉林大阳岔寒武系-奥陶系界线层型候选剖面再描述   总被引:1,自引:2,他引:1  
吉林大阳岔剖面是目前国际寒武系-奥陶系界线工作组(ICOBWG)所确认的全球唯一的寒武系-奥陶系界线层型候选剖面。运用坐标系统对大阳岔界线剖面进行重新测量、详细描述Cambrooistodus 带至 Cordylodus lindstromi 带45.9m 厚的地层序列,将不同学者在大阳岔剖面所采用的样品采集系统相应地标在新的坐标剖面上,以统一它们在新坐标剖面上的坐标位,置点。新的坐标剖面将为国际寒武系-奥陶系界线工作组在确定全球界线层型剖面和点位(GSSP)时提供一个共同的参照标准。  相似文献   
2.
太空资源的勘探及利用是深空探测的重要目的之一。火星是人类最容易到达和资源利用最为迫切的行星,对火星资源进行勘查和原位利用是未来火星载人探测及基地建设需要解决的重要问题。本文对火星大气资源、水资源、土壤与岩石矿物资源、风能与太阳能资源等可利用资源的类型及赋存状况进行了分析,制作了火星资源的全球分布图,并从资源分布的角度提出了未来火星资源探测及火星基地建设的首选区域。同时,本文也总结了火星原位资源利用技术的研究进展及问题,认为未来需要从以下几个方面开展进一步研究:加强火星资源的针对性勘查与评估;开发新的资源利用模式与技术;建立资源利用成本的综合评估模型;完善资源开发与利用相关的法律法规。  相似文献   
3.
基于模拟退火算法的自动地图注记配置研究   总被引:2,自引:0,他引:2  
本文将求解大规模组合优化问题最优解的一种新型算法模拟退火算法应用于地图注记的自动配置。该算法将地图各要素注记的配置作为一个统一的整体来对待,从而避免了一般局部搜索法可能终止于一个局部最优解的缺点,这样可使自动注记配置的结果更趋合理化。用模拟退火算法进行注记自动配置,理论体系完整,机理简单,通用性强,编程容易,而且与一般局部搜索法相比,超常规注记配置出现的数目大大降低,其缺点在于配置速度较慢  相似文献   
4.
The concept of candidate particle set is introduced in the MPS gridless numerical method to generate neighboring particle set matrix, which can reduce the CPU time to 1/11 of that before introduction. The Bi-CGSTAB (bi-conjugate gradient stabilized) algorithm is applied to solving the Poisson pressure equation, by which the solving speed is significantly accelerated. The process of solitary waves propagating over a numerical flume and interacting with a vertical wall is simulated. The simulated results of water surface elevation are in good agreement with the analytical solution as well as the measured data. The predicted maximum values of the run-up of solitary waves with various relative incident wave heights agree well with the measured results.  相似文献   
5.
The collapse of a section of the cliff at Stevns Klint, Denmark in 1986 provided a unique opportunity to collect about 50 kg of Fish Clay representing the Cretaceous-Tertiary (K-T) boundary layer. In this paper, details of the preparation of this sample are presented, together with preliminary analytical results to support the development of this sample as a reference material, particularly for the determination of iridium and the other platinum-group elements in clays and sediments associated with K-T boundary studies and in other environmental samples collected to study the effects of automobile exhaust catalysts.  相似文献   
6.
在发现陆相侏罗系—白垩系界线地层连续剖面的基础上,补充大北沟组和大店子组的含义,将2组系统分为7个岩段,命名4个标志层;确定年代地层层序,完善大北沟阶和义县阶定义内容;研究重点门类化石分布和演化,建立系统生物地层分带序列,包括7个介形虫带和6个叶肢介带;划分陆相生物群发展阶段,将侏罗系—白垩系界线置于“早期热河生物群”阶段的底部;开展旋回地层和层序地层学研究,建立地层等时格架,识别盆地演化的3个阶段和5个构造期;测得界线层型剖面点存在O同位素高值异常;锆石206Pb/238U测得张家口组顶部年龄为135.4Ma±1.6Ma,大北沟组中部为133.9Ma±2.5Ma和130.1Ma±2.5Ma。综合多学科研究成果,将界线层型剖面点定在张家沟剖面第9层底,以介形虫化石Cyprideastenolonga的首现为标志。  相似文献   
7.
具有高分辨率和连续表面的DEM数据是获取月球形貌特征并进行数字地形分析的主要数据源。本文选择嫦娥五号候选着陆区中的一个区域作为试验区,首先,基于LROC NAC立体影像、ISIS3和Stereo Pipeline软件生成高分辨率DOM影像及对应DEM数据,并将其与日本SELENE数据进行对比;然后,利用反距离权重、径向基函数和经验贝叶斯克里金3种插值方法对DEM数据的空洞区域进行修复,并对不同修复方法进行交叉验证分析。结果表明:生成的DOM和DEM分辨率约3.5 m,明显比7.4 m分辨率的日本SELENE数据清晰,并具有更强的地形表达能力;径向基函数插值法的空洞修复效果最好,交叉验证均方根误差为0.26 m。本文对准确获取月球形貌特征、探测器选址等具有一定作用,并能够为其他区域的高分辨率连续DEM数据生成提供参考。  相似文献   
8.
It is a practical approach to select candidate probiotic bacterial stains on the basis of their special traits. Production of digestive enzyme was used as a trait to select a candidate probiotic bacterial strain in this study. In order to select a bacterium with the ability to degrade both starch and protein, an ideal bacterial strain STE was isolated from marine shrimp (Litopenaeus vannamei) intestines by using multiple selective media.The selected isolate STE was identified on the basis of its morphological, physiological,and biochemical characteristics as well as molecular analyses. Results of degradation experiments confirmed the ability of the selected isolate to degrade both starch and casein. The isolate STE was aerobic, Gram-negative, rod-shaped, motile and non-spore-forming, and had catalase and oxidase activities but no glucose fermentation activity. Among the tested carbon/nitrogen sources, only Tween40, alanyl-glycine, aspartyl-glycine, and glycyl-l-glutamic acid were utilized by the isolate STE. Results of homology comparison analyses of the 16S rDNA sequences showed that the isolate STE had a high similarity to several Pseudoalteromonas species and, in the phylogenetic tree, grouped with P. ruthenica with maximum bootstrap support (100%). In conclusion, the isolate STE was characterized as a novel strain belonging to the genus Pseudoalteromonas.This study provides a further example of a probiotic bacterial strain with specific characteristics isolated from the host gastrointestinal tract.  相似文献   
9.
The black hole candidate Cyg X-1 was observed in ultra low state on march 30, 1997 using Large Area Scintillation counter Experiment (LASE) in the hard X-ray energy region of 20–180 keV. During the 30 minute exposure a combined signal of 68 sigma was obtained, however, the measured flux at 50 keV was lower by a factor of 2 than the minimum flux reported so far. Using the recent orbital ephemeris of the source, our snap-shot observations were made at ϕ5.6 = 0.915, which corresponds to the binary minimum revealed by the ASM light curves. The daily average data from the BATSE detectors give the source intensity level to be higher by a factor of 5. Very low flux values measured in the present experiment suggest that the hard X-ray source may have been partially occulted by the primary companion during its transit near the X-ray minimum.  相似文献   
10.
We present our 2-year-long photometric (V, R c, I c) observations of the T Tauri star V1184 Tau. They show that the relatively quiet “photometric life” of this object, which ended in 2004 with a sharp brightness decline by four magnitudes, was succeeded by a qualitatively new (in nature) period of activity characterized by high-amplitude irregular photometric variability. Judging by its color variations, the object belongs to the class of UX Ori stars and, hence, variable circumstellar extinction is responsible for its brightness variations. Moreover, the (V?I c)/V color-magnitude diagram for the object is identical to that for UX Ori itself, suggesting that the optical properties of dust grains in the circumstellar space of these stars are similar. At the same time, V1184 Tau is quite dissimilar to UX Ori stars in its light curve, variability amplitude (reaching 4.5 magnitudes in the V band), and some other parameters.  相似文献   
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