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.     

中国东部第四纪自然环境演化及庐山“冰碛层”堆积时期的自然环境研究

根据第四纪地层内孢粉组合和动物群等新资料恢复了我国东部各大区域第四纪各个时期的自然环境特征,其温暖期与干冷期的交替与深海沉积O~(18)温度变化趋势大致对应。庐山三次“冰期冰碛层”内孢粉组合表明均为温暖湿润针阔叶混交林景观,而不是寒冷的冰川环境。     

贵州玉屏彰寨奥陶纪红花园期障积岩隆礁

该障积岩隆礁的造礁生物主要为海绵和藻,岩石类型有海绵灰岩、藻席岩、核形石凝决石灰岩、生物屑灰岩等。本文系统介绍其造礁生物的生态特征、岩石组合并分析其沉积相和礁的生长发育阶段,最后运用马尔柯夫概型分析研究期旋回沉积发育较好的礁核相地层的学积特征。     

沉积钙质白云石带状面缺陷的择优取向

作者用透射电子显微镜研究了沉积钙质白云石中的带状面缺陷。在衍衬象中面缺陷呈现出特有的条纹衬度,并具有一定的择优取向,它们沿着｛018｝面排列。面缺陷也可分叉,分枝部分平等于｛2－／10｝面。根据白云石面缺陷的取向,本文提出了鞍状白云石宏观弯曲面和微观面缺陷的取向关系。     

近江牡蛎作为重金属污染生物指示种的初步研究

对近江牡砺作为监测广东岸海域Ｃｕ，Ｚｎ，Ｃｄ，Ｐｂ污染的生物指示种的可能性进行了初步研究和评价，应用ＰＯＬＹＤＩＶ统计技术对采自广东沿岩海域１４个站点的近江牡盛的重金属含量进行了统计分析，结果表明近江牡蛎受Ｃｕ，Ｚｎ，Ｃｄ污染的地理分布类型与广东沿海排放的工业废水的分布以及潮间带生物和表层沉积物的Ｃｕ，Ｚｎ，Ｃｄ含量分布相一致，因此，近江牡蛎可作为监测研究Ｃｕ，Ｚｎ，Ｃｄ污染的可靠生物指示种，但能     

海山磁性反演精度的研究

在均匀磁化的假设下,进行海山磁性的反演,有时能获得良好的效果,有时则不然.海山磁性的不均匀性是影响反演精度的主要因素,特别当海山内部的正反向磁化不是严格反平行时,反演精度很低.海山形状不准确、磁测资料的随机误差对反演精度的影响较小.可以用拟合度参数GFR(Goodness-of-Fit Ratio)来衡量反演结果的可靠程度.当GFR≥5时,均匀磁化假设下反演所得的磁化方向有很高的参考价值;GFR=2～5时,反演结果有一定的参考价值;GFR<2时,反演结果常含有很大的误差.本文用面积分计算磁异常.在AT微机上反演一个海山的磁性,约需1分钟.