用GPS全球卫星定位系统建立义马矿区测量控制网     

郭敏  刘刚 《河南测绘》2003,(1):22-22,25

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疏散星团M11的研究——相对自行和成员概率     

束成钢  赵君亮等 《中国科学院上海天文台年刊》1996,37(17):205-210

本给出了疏散星团M11中心25′×25′天区内872颗恒星的相对自行、自行测定误差以及团中心距r≤25′范围内785颗恒星的成员概率，并对有关问题作了简单的讨论。  相似文献   

Ellerman Bombs,Type Ⅱ White—light Flares and Magnetic Reconnection in the Solar Lower Atmosphere     

Peng－FeiChen  ChengFang 《中国天文和天体物理学报》2001,1(2):176-184

Ellerman bombs and type Ⅱ white-light flares share many common features despite the large energy gap between them.Both are considered to result from local heation in the solar lower atmosphere.This paper presents numerical simulations of magnetic reconnection occurring in such a deep atmosphere,with the aim to account for the common features of the two phenomena.Our numerical results manifest the following two typical characteristics of the assumed reconnection process:(1)magnetic reconnection saturates in-600-900s,which is just the lifetime of the two phenomens;(2)ionization in the upper chromosphere consumes quite a large part of the energy released through reconnection,making the heation effect most significant in the lower chromosphere.The applicationof the reconnection model to the two phenomena is discussed in detail.  相似文献   

广州白云山常绿阔叶林的结构特征   总被引：2，自引：0，他引：2  

何冰  尹爱国等 《广东海洋大学学报》2001,21(3):48-53

在线路调查和样方调查的基础上分析了广州白云山常绿阔叶林的结构特征，群落主要由亚热带科属组成，优势科为芸香科，五加科，茜草科，山茶科，壳斗科，鼠刺科，樟科等。优势树种也以相应的优势科属树种为主，群落中胸径≥3cm的个体密度较小，只有1964株/hm^2；群落较为低矮，平均高度只有6m；乔木垂直分化不明显，树种水平分布不均，白云山的植被是次生植被和人工造林改造的结果，只在山谷少数植被没受人类干扰，其现状植被是天然次生植被和人工植被的混合体，在一些由马尾松发展起来的群落，天然侵入的阔叶树种已在主要层中居优势；群落中可见马尾松衰退的痕迹。  相似文献   

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     

匡建超  邓少云等 《致密岩石气藏勘探开发》2001,(4):49-55

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。  相似文献   

日本著名数学家吉泽太郎教授来海院讲学     

李天明 《海洋湖沼通报》1985,(4)

应山东海洋学院邀请,日本著名数学家吉泽太郎教授已于今天开始讲学。吉泽太郎教授自五十年代以来,在常微分方程的稳定性、周期解及泛函微分方程方面作出重要贡献。他的两部专著曾做为教材在我国高等院校的数学专业使用,他的大量论文和专业著作在世界数学界亦有重大影响,是国际著名数学家。  相似文献   

比利时海洋环境专家代表团访问海洋学院     

李天明 《海洋湖沼通报》1986,(1)

以物理海洋和生物学家杰克斯博士为首的比利时海洋环境专家代表团一行四人1985年十一月廿九日抵达山东海洋学院。此次比利时海洋环境专家来访是根据中比两国政府间科技合作协定中海洋环境项目规定的专家互访交流。主要任务是通过考察访问来确定双方在海洋环境保护方面的应用与基础教学模型领域内的合作和项目。这对我国海洋资源开发利用和环境保护都有重要意义。比利时专家与海洋学院物理海洋和气象系、海洋生物系、水产系、微藻中心的科学家进  相似文献   

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   

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   

比利时卤虫专家访问海洋学院     

李天明 《海洋湖沼通报》1985,(2)

应山东海洋学院邀请,比利时肯特大学卤虫研究中心孛柯劳斯教授已于日前抵青到海洋学院讲学。孛柯劳斯教授是世界卤虫研究的权威人士。此次来华讲学的主要内容是: 1.世界卤虫研究和养殖概况; 2.海洋养殖中卤虫的应用; 3.卤虫综合利用展望;  相似文献