γ射线暴的logN(>P)～logP分布     

吴枚  宋黎明  余文飞  李惕碚  李毅 《中国天文和天体物理学报》1997,(1)

本文用简单的宇宙学模型 ,在标准烛光和均匀分布的假设下计算了γ射线暴的logN(>P)～logP分布 (大小谱 ) .在考虑了探测效率修正和死时间修正后 ,由宇宙学模型计算的理论结果和BATSE实测的大小谱没有显著的偏离  相似文献   

Study of a model for correcting the effects of horizontal advection on surface fluxes measurement based on remote sensing     

Tian  Jing  Zhang  Renhua  Sun  Xiaomin  Zhu  Zhilin  Zhou  Yanlian 《中国科学:地球科学(英文版)》2006,49(2):273-280

As well known, the methods of remote sensing and Bowen Ratio for retrieving surface flux are based on energy balance closure; however, in most cases, surface energy observed in experiment is lack of closure. There are two main causes for this: one is from the errors of the observation devices and the differences of their observational scale; the other lies in the effect of horizontal advection on the surface flux measurement. Therefore, it is very important to estimate the effects of horizontal advection quantitatively. Based on the local advection theory and the surface experiment, a model has been proposed for correcting the effect of horizontal advection on surface flux measurement, in which the relationship between the fetch of the measurement and pixel size for remote sensed data was considered. By means of numerical simulations, the sensitivities of the main parameters in the model and the scaling problems of horizontal advection were analyzed. At last, by using the observational data acquired in agricultural field with relatively homogeneous surface, the model was validated.

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吸积双星脉冲星EXO2030+375中回旋吸收线的迹象     

孙学军  程凌翔  李惕碚  吴枚 《中国天文和天体物理学报》1993,(2)

本文作者首次发现了EXO 2030+375的回旋吸收线迹象.这是迄今唯一一个同时有用回旋吸收线直接测量的磁场数据和用吸积演化方法间接测量的中子星磁矩数据的X射线脉冲星.两种测量方法的结果有很大差别,本文提出了可能导致这种差别的物理机制.  相似文献   

On determining membership of open clusters from relative proper motion     

Zhao Jun-liang  Tian Kai-ping 《Chinese Astronomy and Astrophysics》1985,9(4):300-306

We discuss the determination of membership of 42 open clusters. Our analysis shows that Vasilevskis' mathematical model can be reasonably applied to this case. Our improved version of Sanders' method and our definition of cluster member based on the principles of discriminatory analysis effectively exclude stars of low probabilities. It is important in the study of open cluster to use only those with high probabilities. The effectiveness of the statistical method is closely related to the velocity distributions of the member and field stars. For fields where the error rate is high, it is better to combine other data than proper motion in determining membership.  相似文献   

βCephei变星的脉动不稳定带的研究(英文)     

田斌 《紫金山天文台台刊》2003,(2)

在本文中我们对两种不同的 βCephei变星的理论脉动不稳定带作了比较。它们具有明显的不同之处。为了确定这种变星的脉动不稳定带的轮廓 ,我们根据 4 9颗 βCephei变星的观测资料作了统计研究。在从样本星的色指数 (B -V) ,(U -B)和视差得到它们的有效温度和光度之后 ,我们发现在赫罗图上它们大多数是位于主序带内的。而且这些样本星的质量都位于 7M⊙ 到 30M⊙ 之间。和理论模型的比较表明我们提出的具有光度上边界和红蓝边界的 βCephei变星的理论脉动不稳定带跟观测吻合得更好  相似文献   

河南省洛宁县寨凹钼矿床流体包裹体研究及矿床成因   总被引：10，自引：0，他引：10  

邓小华陈衍景  姚军明李文博李 诺王 运糜 梅张 颖 《中国地质》2008,35(6):1250-1266

寨凹钼矿床位于华北克拉通南缘的熊耳地体．矿床定位受马超营断裂带的次级断裂控制,矿体呈脉状贼存于太华超群石板沟组黑云角闪斜长片麻岩中。成矿过程包括3个阶段：石英-辉钼矿阶段（I）、石英-多金属硫化物阶段（Ⅱ）、石英-碳酸盐阶段（Ⅲ）,其中,I阶段为主成矿阶段。寨凹钼矿床可见2类流体包裹体,即水溶液型和含子晶包裹体;激光拉曼指示包裹体成分主要为H2O。从早到晚,流体包裹体均一温度从I阶段100～260℃,经Ⅱ阶段110～160℃．变化为Ⅲ阶段120—180℃．矿床总体属于低温热液矿床：流体包裹体盐度从I阶段的2～25wt％NaCl．eqv演化至Ⅱ阶段的6—30wt％NaCl．eqv．然后降为Ⅲ阶段的7～25wt％NaCl．eqv。I阶段均一温度范围宽广、流体包裹体盐度由双峰式演化为单峰式以及包裹体温度-盐度双变图的负相关性指示了流体混合是主要的成矿机制。寨凹钼矿流体包裹体以高密度、高盐度的低温低压流体为特征,是含CaCl,流体参与成矿的结果,热的岩浆流体与冷的含CaCl,的卤水的混合．导致了辉钼矿的沉淀。寨凹钼矿床地质和流体包裹体特征与侵入岩相关的成矿系统一致．指示其成因类型为与侵入岩有关的钼矿床．  相似文献   

敦化盆地上侏罗统-上新统地层划分对比讨论   总被引：1，自引：0，他引：1       下载免费PDF全文

王海峰  张廷山  戴传瑞  罗梅  胡雯雯  谢晓安 《中国地质》2008,35(1)

利用野外资料、地震资料、煤田钻孔资料以及古生物资料,对松辽盆地外围探区敦化盆地的代表性地层划分方案进行了梳理,通过敦化盆地与周缘盆地之间的对比和分析,得出下列认识:(1)明确了珲春组的时代为始新世—渐新世;(2)指出白垩系上统龙井组地层在敦化盆地内可能是不存在的;(3)将原帽儿山组上段和下段分别划归泉水村组和长财组;(4)认为大砬子组、泉水村组、长财组和屯田营组在敦化盆地内是存在的,并通过盆间岩性地层和古生物地层对比指出大砬子组的时代可能为早白垩世阿普特期(Aptian)—阿尔布期(Albian),长财组时代可能为早白垩世贝利阿斯期—阿普特期;(5)对敦化盆地内几个地方地层名称的使用进行了修正;(6)建立了敦化盆地内目前可供参考使用的地层序列。  相似文献   

山东小清河的原生动物   总被引：1，自引：1，他引：1  

田家怡 《海洋湖沼通报》1995,(1):33-37

本文根据对山东小清河多年的污染生态调整研究，报导了淡水原生动物１４种。  相似文献   

东海冲绳海槽深海鱼类报告   总被引：1，自引：0，他引：1  

田明诚  孙宝龄 《海洋科学集刊》1982,(19):115-128

冲绳海槽位于东海大陆架浅水区的外缘,是一北东一南西向延伸,在东南方向呈弧形突出的海槽。其北部水深在500-1000米间,南部最深达2000余米。1978年6,7月间我所“金星”号调查船在这一深水区及其附近进行了海洋综合考查。在进行底栖生物拖网时,获得一些深海鱼类标本。本文共报道深海鱼类14种,隶14属,12科,9目。  相似文献   

Simulations of Annual Cycle of Phytoplankton Production and the Utilization of Nitrogen in the Yellow Sea     

Tian?TianEmail author  Hao?Wei  Jian?Su  Changsoo?Chung 《Journal of Oceanography》2005,61(2):343-357

A nutrient dynamic model coupled with a 3D physical model has been developed to study the annual cycle of phytoplankton production in the Yellow Sea. The biological model involves interactions between inorganic nitrogen (nitrate and ammonium), phosphate and phytoplankton biomass. The model successfully reproduces the main features of phytoplankton-nutrient variation and dynamics of production. 1. The well-mixed coastal water is characterized by high primary production, as well as high new production. 2. In summer, the convergence of tidal front is an important hydrodynamic process, which contributes to high biomass at frontal areas. 3. The evolution of phytoplankton blooms and thermocline in the central region demonstrate that mixing is a dominant factor to the production in the Yellow Sea. In this simulation, nitrate- and ammonium-based productions are estimated regionally and temporally. The northern Yellow Sea is one of the highly ranked regions in the Yellow Sea for the capability of fixing carbon and nitrogen. The annual averaged f-ratio of 0.37 indicates that regenerated production prevails over the Yellow Sea. The result also shows that phosphate is the major nutrient, limiting phytoplankton growth throughout the year and it can be an indicator to predict the bloom magnitude. Finally, the relative roles of external nutrient sources have been evaluated, and benthic fluxes might play a significant role in compensating 54.6% of new nitrogen for new production consumption.  相似文献