Statistical Properties of the Highest Pulses in Gamma-Ray Bursts

We study the statistical properties of the highest pulses within individual gamma-ray bursts (GRBs). A wavelet package analysis technique and a developed pulse-finding algorithm have been applied to identify the highest pulses from burst profiles observed by BATSE on board CGRO from 1991 April 21 to 1999 January 26. The statistical light curves of the highest pulses in four energy channels have been derived by an aligning method, which illustrate the temporal evolution of the pulse emission. Our result that narrower pulses go with higher energies is consistent with previous findings. By normalizing both the pulse durations and counts to unity, “characteristic” profiles of the highest pulses in the four channels are also derived. The four characteristic profiles are turned out to be almost the same, thus strongly support the previous conclusion that the temporal profiles in different energy channels are self-similar and the previous conjecture on GRB pulses, implying that the emission process is similar at different energies. The cosmological time dilation effect is examined by investigating the relationship between the pulse flux and pulse duration. An anti-correlation between the two was found, which agrees with the expectation of the cosmological time dilation effect. Also, the evolution of the pulse duration with the observational epoch is studied. The result shows that the pulse duration tends to be shorter in later epochs. This trend cannot be explained by the present theoretical models, and may represent a great challenge to current theories.     

低质量X射线双星的毫秒级准周期信号——最近的进展

最近对低质量X射线双星中的千赫兹准周期振动的研究表明 ,是辐射压力 ,而不是盘和磁球的相互作用以及处于盘内边界的广义相对论效应在短时标的盘切断机制上起作用。本文给出了一些研究结果及讨论。     

History of Star Formation and Chemical Enrichment in the Milky Way Disk

Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have improved our two-component chemical evolution model for the Milky Way disk. Two gas infall rates are compared, one exponential, one Gaussian. It is shown that the star formation law adopted in this paper depends more strongly on the gas surface density than that in Chang et al. It has large effects on the history of star formation and gas evolution of the whole disk. In the solar neighborhood, the history of chemical evolution and star formation is not sensitive to whether the infall rate is Gaussian or exponential. For the same infall time scale, both forms predict the same behavior for the current properties of the Galactic disk. The model predictions do depend on whether or not the infall time scale varies with the radius, but current available observations cannot decide which case is the more realistic. Our results also show that it would be inadequate to describe the gradient evolution along the Gala     

使用小波技术自动搜寻天体谱线

使用小波技术对包括恒星、近邻星系和ＡＧＮ等不同的天体光谱进行了自动处理．用小波滤波的方法将光谱中的连续谱与诸线分离;然后使用小波域隐含马尔可夫模型（ＨＭＭ）,对已去掉连续谱的光谱进行降噪,同时得到了噪声在每个光谱中的分布;在训练ＨＭＭ的过程中,使用改进的Ｔｙｉｎｇ方法增加训练数据以保证训练的可靠性;利用噪声分布确定出谱线信号的局部阈值,在已经降噪的光谱中找到吸收线和发射线;用高斯函数拟会出谱线的形状,标出线心的波长值,作为自动证认的基础．     

1-（4-硝基苯基）-3-（3，5-二溴吡啶）三氮烯的合成及其与镍的显色反应

合成了1-(4-硝基苯基)-3-(3,5-二溴吡啶)三氮烯(NPDBPDT),并研究了NPD-BPDT与镍的显色反应。在pH 10.0的Na2B4O7-NaOH缓冲溶液介质中,表面活性剂Triton X-100存在下,镍与试剂生成摩尔比为1∶4的络合物在470 nm处有最大正吸收峰,表观摩尔吸光系数为1.02×105L.mol-1.cm-1;在540 nm处有最大负吸收峰,表观摩尔吸光系数为1.15×105L.mol-1.cm-1;以540 nm为参比波长、470 nm为测量波长进行双波长测定,表观摩尔吸光系数为2.17×105L.mol-1.cm-1。镍含量在0~480μg/L内符合比尔定律。方法用于合金样品中镍的测定,结果与原子吸收法相符,加标回收率为98.0%~102.0%;精密度小于5%(RSD,n=6)。     

土体原位测试法在岩土工程中的应用

土体原位测试是工程勘察和检测的有效手段，通过统计其数据可以得出有效的经验公式，在工程中有一定的实用性。     

广南堂上金矿多种金矿化的发现

在不到10km^2的范围内，集中发现了滇黔桂金三角地区常见的多种矿化类型：微细粒浸染型金矿、不整合面上金矿（大厂层）、基性火山岩金矿、火山碎屑沉积型金矿、石英脉型金矿、现代河流沉积中的砂金，且存在不同的找矿标志。     

K-Ar法地质年龄国家一级标准物质ZBH-25黑云母的研制

ZBH-25黑云母采自北京房山花岗闪长岩体。它的~(40)Ar/~(39)Ar 阶段加热实验结果表明,~(40)Ar~*在矿物晶格中保存均匀稳定,年龄谱平坦,~(39)Ar 析出量高达96%,~(40)K-~(40)Ar~*同位素体系封闭良好,证明该黑云母结晶以后未受过热扰动。坪年龄为133.0±0.3Ma,总气体年龄为132.1±0.6Ma;~(36)Ar/~(40)Ar-~(39)Ar/~(40)Ar 反等时线年龄为133.1±1.3 Ma,~(40)Ar/~(36)Ar 初始值为293.5±1.6,与大气氩丰度比(295.5±0.5)处于同一范围,表明样品不含过剩氩。激光显微探针单颗粒坪年龄为132.8±0.2Ma,年龄谱和 K/Ca 谱线平坦,激光熔样总气体年龄为131.3±0.2Ma(图6)。这几个 Ar-Ar 年龄的一致性,说明样品具有良好的均匀性和稳定性,是理想的 K-Ar 和 Ar-Ar 法年龄标准物质。对均匀性检验数据进行统计学方法检验,在0.05显著性水平下,证明 K 和~(40)Ar~*的 F 分布值小于 F 临界值,说明该样品是均匀的。国内外14个实验室参加了 K 含量的定值分析,15个实验室参加了~(40)Ar~*含量的定值分析,经统计学方法检验,结果显示全部定值数据都服从正态分布并具等精度。在置信概率为0.95时,~(40)Ar~*和 K 含量的相对标准偏差都小于0.5%。两个特性量值定值分析结果的一致值和不确定度分别为:~(40)Ar~*=1.817±0.013×10~(-9)mol/g,K=7.60±0.02%,K-Ar 年龄(标准值)=132.9±1.3Ma(2σ).此标准物质纯度为98.8%,粒度为0.25-0.63mm,总重量为5800g,缩分成最小样品单元共400瓶,每瓶重量为14.5g。可供我国 K-Ar 和 Ar-Ar 法同位素年代学实验室使用120年。     

关于上海地区金山群大地构造属性的思考

根据上海地区金山群的岩石组合、原岩及原岩建造、变质作用、构造形变特征,以及已有的同位素年龄值,认为金山群与浙东南陈蔡群基本一致,是华厦古陆块的基底组分。参照华厦古板块与扬子古板岩多期聚合的观点,推断分布在(?)径——川沙断裂南东侧的金山群块断体,是晋宁期末二古板块碰撞对接、于结合带内形成的构造推叠岩片。     

南半球热带外准半年振荡及IAP 9L AGCM模拟检验

基于1979—2000年的NCEP/NCAR海平面气压和位势高度场资料分析了南半球大气环流的准半年振荡 (半年波) 现象。结果表明:这一现象主要出现在南半球对流层低层的中高纬度和中高层的热带地区。对南半球热带外大气而言, 40°S和65°S是低层大气环流准半年振荡最为显著的两个纬度带, 半年波的贡献都超过了70%, 低层南半球中高纬度海平面气压场季节变化的反位相也主要体现为各自半年波分量变化的反位相。在此基础上, 检验了IAP 9L AGCM (大气物理研究所9层大气环流模式) 对这一现象模拟的能力, 模拟结果显示, 模式成功模拟了65°S处海平面气压场的准半年振荡现象, 其振幅略低于观测结果, 但模式对40°S处气压场准半年振荡的模拟效果较差。