位移时空综合分析法及其在边坡工程中的应用

以往对监测位移数据分析方法主要是位移-时间关系分析。但监测数据包含了大量对工程设计和施工都很有用的信息,其中不乏位移-空间方面的信息;另一方面,从工程设计和施工角度看,除需要位移-时间信息外,还需要位移-空间信息。位移时空综合分析法的提出旨在综合位移-时间和位移-空间等两方面的信息,为工程设计和施工服务。该方法依表现形式不同又分为竖线法和曲面法两种。本文将通过五强溪船闸边坡工程实例,来进一步说明位移时空综合分析法的原理及其应用。     

C_(60)研究现状及前景

碳除了具有传统观念上的石墨和金刚石两种同素异形体外,近年来人们又发现了第三种同素异形体———Ｃ６０。Ｃ６０以其独特的类似足球状的结构及性能,吸引了各国的科学家,对Ｃ６０的研究在全世界范围内如火如荼地开展起来。笔者在总结Ｃ６０的合成技术、分子结构与性能的基础上,探索了Ｃ６０作为一种新型材料所具有的应用潜力;回顾了从Ｃ６０发现至今十多年的研究历程,并首次将Ｃ６０的研究过程分成三个阶段,即起步阶段（１９８５年～１９９０年）、起飞阶段（１９９１年～１９９３年）和成熟阶段（１９９４年以后）;预测了Ｃ６０及其化合物的应用性研究将成为今后研究的重点和热点。最后,对当前Ｃ６０研究中存在的问题和难点进行了讨论。     

T_(63)500hPa高度场的预报统计检验与分析

该文将T63500hPa高度切48小时、96小时预报场与客观分析和欧洲中心500hPa高度场,48小时、96小时预报场进行仔细的统计检验。分析结果认为,T63500hPa高度场对我省具有相当高的预报价值,超过了欧洲中心数值产品.     

Populations of Bright X-ray Sources in the Starburst Galaxies NGC 4038/4039

Assuming a naive star formation history, we construct synthetic X-ray source pop- ulations, using a population synthesis code, for comparison with the observed X-ray lumi- nosity function (XLF) of the interacting galaxies NGC 4038/4039. We have included high- and intermediate-mass X-ray binaries, young rotation-powered pulsars and fallback disk-fed black holes in modeling the bright X-ray sources detected. We find that the majority of the X-ray sources are likely to be intermediate-mass X-ray binaries, but for typical binary evolu- tion parameters, the predicted XLF seems to be steeper than observed. We note that the shape of the XLFs depends critically on the existence of XLF break for young populations, and suggest super-Eddington accretion luminosities or the existence of intermediate-mass black holes to account for the high luminosity end and the slope of the XLF in NGC 4038/4039.     

Seven-frequency VLBI Observations of the GHz-Peaked-Spectrum Source OQ 208

We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4,1.7,2.3,5.0,8.4,15.4GHz and the European VLBI Network at 6.7 GHz.The low frequency(1.4,1.7 and 2.3GHz)ob- servations reveal a weak and extended steep-spectrum component at about 30mas away at position angle-110°,which may be a remnant emission.The radio structure of OQ 208 con- sists of two mini-lobes at 5.0,6.7,8.4 and 15.4 GHz.Our spectral analysis further confirms that the southwest lobe undergoes free-free absorption and finds that the free-free absorption is stronger in the inner region.By fitting the 8.4 GHz images from 1994 to 2005,we obtain a separation speed of 0.031±0.006 mas yr~(-1)between the two mini-lobes.This indicates a jet proper motion of 0.105±0.020 c and a kinematic age of 219±42 yr for the radio source.     

层次分析法在彩票抽奖方案选择中的应用

采用层次分析法对29种彩票抽奖方案进行排序,较为科学地解决了比较多种方案优劣程度的问题,得到了彩票抽奖方案选择问题的优化解.     

A New Feature Vector Using Selected Line Spectra for Pulsar Signal Bispectrum Characteristic Analysis and Recognition

Average pulse profiles of pulsar signals are analyzed using the bispectrum tech-nique. The result shows that there are nonlinear phase couplings between the two frequency axes of the bispectrum charts, which indicate nonlinear factors in the generation and prop-agation of pulsar signals. Bispectra can be used as feature vectors of pulsar signals because of their being translation invariant. A one-dimension selected line spectrum algorithm for ex-tracting pulsar signal characteristic is proposed. Compared with selected bispectra, the pro-posed selected line spectra have the maximum interclass separability measurements from the point of view of the whole one-dimension feature vector. Recognition experiments on several pulsar signals received at several frequency bands are carried out. The result shows that the selected line spectrum algorithm is suitable for extracting pulsar signal characteristics and has a good classification performance.     

書報述評

Isentropic AnlysIs(等位温層分析)*,C.G.Rossby著,載美國氣象學會氣象業報,18卷,6-7期之201-210頁:應用位置溫度和比較濕度二因子來分析天氣,不過是氣象界近数年間的事,但他在氣象學演進的過程中,却放出了異樣的光彩,因為這兩因子,不但富保有守性,並且還有動力學的意義。現在我們分析天氣、不僅僅從經驗上或實際上可以體會得到,並且在理論上也奠定了鞏固的基礎,因為現在的分析法,已從平面進到立體,二度進入三度。在一九二八年Bergeron發表了‘天氣三度分析論’,我們對於天氣的