致密碎屑岩储层裂缝和产能预测的单井建模——以新场气田沙溪庙组为例

近年来，利用三维地震资料进行致密碎屑岩储层裂缝和产能的识别预测取得了一些进展，而这之中最重要也最基础的是单井裂缝和产能的建模工作。本以新场气田沙溪庙组致密储层为例，详细介绍了综合运用岩芯资料、测井资料和录井资料进行裂缝和产能单井建模的方法，为利用三维地震资料建立裂缝和产能的灰色遗传过程识别模式打下了良好的基础。     

河南铝土矿矿石结构构造和矿石类型

河南省铝土矿产于中石炭统本溪组中、上部,广泛分布在秦岭东段北侧,中条山南侧,以及嵩山、箕山周围的山前丘陵地带,面积约1.8万平方公里,已知矿区(点)92个,民采矿坑星罗棋布,以其分布广、埋藏浅、质佳量大著称全国。近年来,随着铝土矿地质勘探工作的发展,对铝土矿矿石的结构、构造和矿石类型的研究也逐步深入。现就我们的研究成果陈述如下,以供读者参考。     

MERLIN Images of Five Compact Symmetric Object Candidates at 1.6 GHz

1 INTRODUCTIONCompact Symmetric Objects (CSOs) are powerful and compact sources (overall size <1 bpc) with lobe emission on both sides of the central engine. The small size of these sourcesis almost certainly to be attributed to the youth of the sources themselves (ages < 104 yr) andnot due to a dense coallning medium (Readhead 1996). The unification scenario assumes thatCSOs evolve into compact steep spectrum (CSS) sotirces and then into Fanaroff-Riley type 11objects (Fanti 1995). …     

Magnetic Field Strengths and Structures from Radio Observations of Solar Active Regions

Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field.     

高频VLBI观测射电源的结构

高频VLBI观测揭示出河外射电源在pc或者亚pc尺度上大都有核-喷流的内部结构，尤其是对平谱致密射电源中毫角秒尺度的子源，能以相当高的概率观测到它的视超光速现象。多频观测可监测到一些新喷流子源的出现，特别在射电激变源中这些新喷流子源的出现与宽带内（从光学到γ射线）的爆发相关。且得到的一些源的核区谱指数分布，为确认源的VLBI核提供了支持。     

奶牛隐性乳房炎发生规律探讨

通过对某奶牛场泌乳牛群隐性乳房炎的调查和分析。研究了奶牛隐性乳房炎的发生规律。结果表明，该场奶牛隐性乳房炎的阳性率为31.42%。乳区临诊阳性率达到10.60%。隐性乳房炎的发生随着胎次和泌乳时间的增加而增加，左乳区阳性率高于右侧，前乳区高于后乳区，在牛群（场）里进行经常性的临床和实验室检验是必要的。     

On the Rd Edge of the δ Scuti Instability Strip

The δ Scuti star ctalogue is used to derive the observational locations of such stars on the HR diagram.The theoretical and observational instability strips are compared to check the theoretical red edge obtained by considering nonlocal time-dependent convection theory.The observational instability strip almost overlaps with the theoretical one,but the observed blue and red envelopes are hotter overlaps with the theoretical one,but the observed blue and red envelopes are hotter than the theoretical edges.The distribution of δ Scuti stars in the pulsation strip is not uniform.     

诗意的海洋学——记现代海洋科学创始人马修·莫里

马修·莫里(MatthewF.Maury,1806-1873),美国海军军官,海洋学创始人之一。他的《海洋自然地理》出版于1855年,至今已有150年的历史,是现代海洋科学最早的教科书,并成为世界科学出版物的一个里程碑。莫里从一名普通的海员成为一名海洋科学家,曾写下许多有关海洋科学的著作,《海洋自然地理》是他一生的巅峰之作。     

适用于中子活化分析的CQ程序

近几年,我国向美国CANBERRA公司引进了多台SCORPIO—3000系列计算机多道分析器系统。该公司为中子活化子谱的数据提供了CLASS语言编写的“GAMMAS”程序。“GAMMAS”程序在处理地质样品γ谱数据时存在着以下主要缺陷: 1.中子活化分析多采用相对比较法工作,当不进行效率刻度时该程序执行的结果仅得到目标核数的强度数据。