Sequences in the Hardness Ratio-Peak Energy Plane of Gamma-Ray Bursts     

Xiao-Hong Cui  En-Wei Liang  Rui-Jing Lu National Astronomical Observatories/Yunnan Observatory  Chinese Academy of Sciences  Kunming  ciwei@.com Department of Physics  Guangxi University  Nanning Department of Astronomy  Nanjing University  Nanjing Graduate School of the Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(2):151-158

The narrowness of the distribution of the peak energy of the vFv spectrum of gamma-ray bursts (GRBs) and the unification of GRB populations are great puzzles yet to be solved. We investigate the two puzzles based on the global spectral behaviors of different GRB populations, the long GRBs, the short GRBs, and the X-ray flashes (XRFs), in the HR - Ep plane (HR the spectral hardness ratio) with BATSE and HETE-2 observations. It is found that the long GRBs and the XRFs observed by HETE-2 seem to follow the same sequence in the HR-Ep plane, with the XRFs at the low end of this sequence. We fit the sequence by a universal Band function, and find that this sequence is mainly defined by the low energy index α, and is insensitive to the high energy index,β. With fixed β=-5, a best fit is given by α=-1.00 with X^2min/dof=2.2. The long and short GRBs observed by BATSE follow significantly different sequences in the HR-Ep plane, with most of the short GRBs having a larger hardness ratio than the long GRBs at a given Ep. For the long GRBs a best-fit yields α=-0.30 and β=-2.05. For the short GRBs, a best fit gives α=-0.60 with x^2min=1.1 (withβfixed at-2.0 because it is numerically unstable). The α value for the short GRBs is significantly greater than that for the long GRBs. These results indicate that the global spectral behaviors of the long GRB sample and the XRF sample are similar, while that of the short GRBs is different. The short GRBs seem to be a unique subclass of GRBs, and they are not the higher energy extension of the long GRBs.  相似文献   

On the Period Variation of the W UMa-type Contact Binary V502 Ophiuchi     

Qing-Yao Liu  Yu-Lan Yang National Astronomical Observatories/Yunnan Observatory  Chinese Academy of Sciences  Kunming   《中国天文和天体物理学报》2006,6(3):331-337

The variation in the orbital period of the W UMa type contact binary V502 Oph is analyzed. The orbital period exhibits a wavelike variation with a periodicity of 23.0 years and an amplitude of △P = 1.24×10~(-6) days superimposed on secular decrease of dP/dt = 1.68×10-7 day per year. The long-term decrease may be accompanied by the contraction of the secondary at a rate of 83 m per year and a mass transfer rate from the primary to the secondary of 4.28×10~8 M per year. The short-term oscillation may be explained by the presence of a third component. Orbital elements of the third body and its possible mass are presented.  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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The inversion of anelastic coefficient,source parameters and site respond using genetic algorithm     

刘杰  郑斯华  黄玉龙 《地震学报(英文版)》2003,16(2):226-232

It gradually becomes a common work using large seismic wave data to obtain source parameters, such as seismic moment, break radius, stress drop, with completingof digital seismic network in China (Hough, et al, 1999; Bindi, et al, 2001). These parameters are useful on earthquake prediction and seismic hazard analysis.Although the computation methods of source parameters are simple in principle and the many research works have been done, it is not easy to obtain the parameters accurately. There are two factors affecting the stability of computation results. The first one is the effect of spread path and site respond on signal. According to the research results, there are different geometrical spreading coefficients on different epicenter distance. The better method is to introduce trilinear geometrical spreading model (Atkinson, Mereu, 1992; Atkinson, Boore, 1995; WONG, et al, 2002). In addition, traditional site respond is estimated by comparing with rock station, such as linear inversion method (Andrews, 1982), but the comparative estimation will introduce some errors when selecting different stations. Some recent research results show that site respond is not flat for rock station (Moya, et al, 2000; ZHANG,. et al, 2001; JIN, et al, 2000; Dutta, et al, 2001). The second factor is to obtain low-frequency level and corner frequency fromdisplacement spectrum. Because the source spectrum model is nonlinear function,these values are obtained by eye. The subjectivity is strong. The small change of corner frequency will affect significantly the result of stress drop.  相似文献   

会议消息          下载免费PDF全文

CNC-IGBP/PAGES工作组 《第四纪研究》2004,24(3):358-358

随着社会发展和人类进步,地球环境问题,尤其是近现代环境变化问题日益引起人们的关注。保护环境,走可持续发展的道路已成为世界各国的共识和我国的一项基本国策。最近几年我国在现代环境污染防治、区域和全球环境变化等方面开展了深入系统的研究,取得了一批重要成果。为了推动环境科学、第四纪地质学和同位素地球化学研究的相互渗透,促进学科交叉和方法借鉴,给相关领域的专家们提供一个互相交流的机会,中国第四纪研究委员会高分辨率气候记录专业委员会、中国地质学会岩溶地质专业委员会、中国地质学会同位素专业委员会和国际地圈-生物圈计划…  相似文献   

内蒙古中西部地区震源参数和场地响应反演   总被引：15，自引：0，他引：15       下载免费PDF全文

高立新  郑斯华  丁风和 《地震工程学报》2005,27(2):109-114

采用Atkinson方法，基于遗传算法，利用呼和浩特数字地震台网7个子台记录的9次质量较高的地震事件资料，计算了内蒙古中西部地区的品质因子Q值和非弹性衰减系数c（f）。在所研究的频率范围内，前者和频率．厂有很好的线形关系：Q（f）=116．8f^1.000后者与频率．厂的变化关系不明显。在此基础上采用Moya方法反演了7个地震台的场地响应和地震的震源参数，并对它们之间的相互关系进行了讨论。结果显示在所研究的频率域内7个基岩台站的场地均不同程度的存在放大作用，其次震源参数间具有较好的线性关系。本文还详细介绍了Atkinson方法和Moya方法的原理和计算步骤。  相似文献   

新疆北天山中东段地区震源参数研究   总被引：9，自引：2，他引：9  

赵翠萍  夏爱国  郑斯华  陈章立 《中国地震》2005,21(1):61-69

本文首先利用经验格林函数方法证明了新疆北天山中东段地区的震源谱基本满足ω-2 模型。在此基础上 ,通过对S波观测谱中的噪音、仪器、路径、场地等影响的逐一消除 ,得到了研究区 10 5次ML2 5～ 5 7地震的震源谱 ,进而根据Brune的圆盘震源模型计算了地震矩、应力降、震源半径等震源参数。结果表明 ,这些地震的标量地震矩M0 与ML 震级线性相关较好 ,关系为Log10 M0 =1 10ML+ 17 2 0 ;震源半径在 10 0～ 15 0 0m之间 ;应力降介于 1～ 16 0bar之间 ,优势分布于 1～ 10 0bar。地震矩与拐角频率的关系呈现出两段趋势 ,可能表明了研究区震源的多重标度特征 :当M0 小于 4× 10 2 1dyne cm时 (相当于ML4 0地震 ) ,应力降显示出对M0 有依赖关系 ;当M0 大于 4× 10 2 1dyne cm时 ,地震的应力降不依赖于M0 。  相似文献   

给学生一个空间,让他们自己去学习     

朱戈雅 《天文爱好者》2020,(4):87-90

从事天文教学工作后,我开始思考如何协调小学教着的深度和宇宙知识的复杂程度之间的关系。在不断地思考与实践中,我决定从教育目标、搭建平台和培养学生三个维度着手,一步步形成了目前中关村二小天文教学的初步格局。现仅此小文,跟大家探讨、交流。  相似文献   

Dyke Swarms: Keys to Paleogeographic Reconstructions, Preface for IDC7 2016 PENG Peng, Richard ERNST     

Regional maps/reviews of dyke swarms  related units 《《地质学报》英文版》2016,90(Z1)

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住建部、国土资源部:统筹地上地下空间开发,加快城市停车场规划建设     

<中国国土资源报>报社 《国土资源》2016,(9)

正日前,住房和城乡建设部、国土资源部联合印发《关于进一步完善城市停车场规划建设和用地政策的通知》,提出合理配置停车设施,提高空间利用效率,促进土地节约集约利用;充分挖潜利用地上地下空间,推进建设用地的多功能立体开发和复合利用;鼓励社会资本参与,加快城市停车场建设,逐步缓解停车难问题。  相似文献