MERLIN Images of Five Compact Symmetric Object Candidates at 1.6 GHz     

Hai－YanZhang  XiangLiu 《中国天文和天体物理学报》2001,1(2):129-132

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). …  相似文献   

白石坡银多金属矿区火山机构与成矿地质作用初探     

易成煌  年平国 《河南国土资源》1992,(3)

区内火山活动早期为火山爆发成岩;晚期演化为岩浆侵入或隐爆两种成岩方式。矿主要受控于潜火山岩带、放射状断裂破碎带中。成矿是在晚期岩浆活动过程中,所携带的含矿介质叠加和热液作用活化了围岩中有用矿质迁移聚集而成,成矿作用与火山作用有着内在联系。  相似文献   

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

Chang－XiZhang  G.B.Gelfreikh 《中国天文和天体物理学报》2002,2(3):266-276

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.  相似文献   

高频VLBI观测射电源的结构     

田文武  张海燕等 《云南天文台台刊》2001,(2):1-9

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。  相似文献   

奶牛隐性乳房炎发生规律探讨   总被引：4，自引：0，他引：4  

苏俊强  梁海锋等 《广东海洋大学学报》2002,22(6):65-68

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。  相似文献   

地球物理现象和太阳活动中的高频振荡   总被引：2，自引：0，他引：2  

顾震年 《天文学报》1995,36(1):65-72

本文用几种谱分析方法了从１９７６年７月－１９９２年９月期间的地球物理资料（日长变化，大气角动量）和太阳活动及１９７６年７月－１９８７年１２月的日冕指数。结果证实所有序列中呈现出４０－６０天的振荡，同时也表明：它们的振幅和周期是随时间变化的。本文研究了谱结构的时空分布和讨论地球物理象与太阳活动之间的可能联系。  相似文献   

On the Rd Edge of the δ Scuti Instability Strip     

Yan  Xu  Zhi-Ping  Li 《中国天文和天体物理学报》2002,2(5):441-448

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.  相似文献   

沉积钙质白云石带状面缺陷的择优取向     

胡梅生  唐玉梅等 《矿物学报》1991,11(1):9-12,T003,T004

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。  相似文献   

海洋石油管道单点提升分析   总被引：3，自引：0，他引：3  

邢静忠  柳春图等 《海洋工程》2002,20(3):29-33

基于管道微单元体平衡建立了海管单点提升的非线性力学模型的控制微分方程组 ,使用变弧长的无量纲代换将动边界问题化为固定边界的两点边值问题 ,利用Maple环境下编制的两点边值问题的打靶法程序得到了该问题在各个提升阶段的数值解答和在单点提升过程中管道的极限弯矩约为 0 .71q1 3(EI) 2 3。  相似文献   

Cleveland火山喷发     

今年月日  Aleutian群岛中部的Cleveland火山出现了爆炸性喷发。飞行员报告说火山灰云弥漫至英尺的高空。灰羽以大约.km/h的速度向Akutan的丹麦港移动  向北延伸了至少英里。卫星图像显示灰云的主要部分大都漂移至°N°W之间的地区。火山以东英里处Nikolski地区的居民看到火山灰“瀑布”持续了h。Cleveland火山的上一次喷发出现在年。自年以来已经喷发了次。月份的喷发在火山的北东翼堆积起了高大的灰山  而在火山的南翼有可能形成小的泥石流。　　　　…… 《海洋地质前沿》2001

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