Implementation of New OPAL Tables in Eggleton's Stellar Evolution Code

Based on previous works of OPAL, we construct a series of opacity tables for various metallicities Z=0, 0.000 01, 0.000 03, 0.000 1, 0.000 3, 0.001, 0.004, 0.01, 0.02, 0.03, 0.04, 0.05, 0.06, 0.08 and 0.1. These tables can be easily used in Eggleton's stellar evolution code in place of the old tables without changing the code. The OPAL tables are used for log10(T/K) > 3.95 and Alexander's for log10(T/K) < 3.95. At log10(T/K) = 3.95, the two groups' data fit well for all hydrogen mass fractions. Conductive opacities are included by reciprocal addition according to the formulae of Yakovlev and Urpin. A comparison of 1 and 5 M models constructed with the older OPAL tables of Iglesias and Rogers shows that the new opacities have most effect in the late stages of evolution, the extension of the blue loop during helium burning for intermediate-mass and massive stars.     

Optical Photometric Observations of 7-Ray Loud Blazars

We report results of our optical photometric observations of ten gamma-ray loud blazers, namely: 0219+428 (3C66A), PKS 0420-014 (OA 129), S5 0716+714, 0754+100 (OI 090.4), 0827+243 (OJ248), 1652+398 (Mrk 501), 2200+420 (BL Lacertae), 2230+114 (CTA 102), 2251+158 (3C 454.3) and 2344+514. The observations were carried out in September-October, 2000 using the 70 cm optical telescope at Abstumani Observatory, Georgia. We found intra-day variations in 0420-014, S5 0716+714, BL Lacertae and CTA 102. A variation of 0.3 magnitude over a time scale of about 3 hours was observed in the R passband in BL Lacertae on JD 2451827. We did not detect any variation in 3C 66A, Mrk 501, or 3C 454.3 during our observations. Nor did we detect any clear evidence of variation in 1ES 2344+514 during our two weeks' observing run of the TeV gamma-ray source.     

卡尔曼滤波在低轨卫星精密定轨中的应用

星上计算机的处理能力不断提高,地基控制系统资源日益紧张,这些都对卫星自主定轨提出了迫切的要求,利用卡尔曼滤波进行卫星自主定轨将具有十分广阔的应用前景。但由于低轨卫星受摄动力较大,使得其动力学方程十分复杂,本文对如何建立适当的模型进行了分析。标准卡尔曼滤波只有在满足一定约束条件时,才能得到最优解。但利用星载GPS进行卫星定轨时,这些约束条件并不能得到完全的满足,针对这些问题本文讨论了相关噪声和滤波发散,观测值粗差等问题。     

AN IMPROVED SEMI-IMPLICIT TIME DIFFERENCE SCHEME OF SPECTRAL MODEL AND NUMERICAL APPLICATIONS

In fact,the popular semi-implicit time difference scheme of spectral model still includes someimportant linear terms using time explicit difference scheme,and the major terms are directlyrelated to fast internal-and external-gravity waves in the atmospheric forecasting equation.Additionally,due to using time difference on two terms at different time.the popular schemeartificially introduces unbalance between pressure gradient force and Coriolis force terms whilenumerically computing their small difference between large quantities.According to thecomputational stability analysis conducted to the linear term time difference scheme in simpleharmonic motion equation,one improved semi-implicit time difference scheme is also designed inour study.By adopting a kind of revised time-explicit-difference scheme to these linear terms thatstill included in spectral model governing equations,the defect of spectral model which only partlyusing semi-implicit integrating scheme can be overcome effectively.Moreover,besides all spectralcoefficients of prognostic equations,especially of Helmholtz divergence equation,can be workedout without any numerical iteration,the time-step (computation stability) can also be enlarged(enhanced) by properly introducing an adjustable coefficient.     

控制网连接点坐标值粗差的可定位性研究

在原有测量控制网(称旧网)的基础上建立同级扩大网或低级加密网(称新网)时,新旧网之间的重合点(称连接点)坐标值粗差的检验是平差前的一个重要环节。本文将连接点坐标视为带协方差阵的观测值,采用数据探测法定位其粗差。借助于 Gauss-Markov模型下两个备选假设检验的理论,推导了连接点相关坐标观测值粗差可定位性基本公式,讨论了各类平面网中连接点坐标观测值粗差的可发现性和可区分性。     

地形图符号库的设计

地形图中符号可分为点状符号、面状符号和线状符号,不同比例尺的地形图,其符号的构造规律是一致的,只是符号的结构与尺寸不同。本文在于探索这些符号的构造规律,并进行有机组织。     

专题地图地理底图数据库的建立与管理

本地理底图数据库系统是一个小型的数据库系统,它具备了地图数据库的基本功能,适应同一底图服务多种专题图编制的要求,提供多种检索途径;运用大量的位操作,使得数据库结构具有动态性、灵活性。将频繁交换的数据纳入内存,加快了系统运进速度;通过多边形组织,可自行建立专题要素与底图要素的图形关系,建立区域间层次关系,减小数据采集工作量。     

大别山北部榴辉岩的Pb同位素特征

大别山北部榴辉岩的全岩 Pb同位素研究结果表明 ,Pb同位素比值 N(2 0 6 Pb) /N (2 0 4 Pb) =16 .773～ 18.339,N (2 0 7Pb) /N (2 0 4 Pb) =15 .346～ 15 .5 16 ,N (2 0 8Pb) /N (2 0 4 Pb) =37.133～ 38.346 ,平均值分别为 17.6 5 ,15 .4 5和 37.81)明显接近于下地壳成分 N(2 0 6 Pb) /N(2 0 4 Pb) ,N(2 0 7Pb) /N(2 0 4 Pb) ,N(2 0 8Pb) /N(2 0 4 Pb)值分别为 17.6 2 ,15 .35和 38.75 ) ,同时 ,北部榴辉岩的 U /Pb比 (0 .0 0 2～ 0 .0 0 9)及 U质量分数 (0 .0 4× 10 - 6 ～ 0 .2 3× 10 - 6 )稍低于下地壳平均值 ,而 Pb质量分数 (6 .72× 10 - 6～ 2 6 .6 4× 10 - 6 )则接近于或略高于地壳平均值 ,但是 ,U/Pb比则明显偏离上地壳平均值、也不同于大别山南部榴辉岩及有关岩石 (较低的 Pb质量分数和较高的 U/Pb比 )。此外 ,考虑到研究区榴辉岩的岩石地球化学及 Sr,Nd同位素年代学方面研究已证明它们大多数为印支期扬子陆壳俯冲变质成因。由此进一步表明 ,大别山北部榴辉岩的原岩大多数应来自于扬子大陆下地壳。这对正确认识大别山碰撞造山带的构造格局和演化具有重要意义。     

线状要素移位的研究

制图综合常要求将地形图要素从其正确的图面位置偏移一点。本文就线状要素的移位问题进行讨论。首先提出移位场的概念,这对于由于移位所产生的“连锁反应”能较好地解决;然后,提出一种栅格探测——矢量计算方祛,加快移位计算的速度。     

EXPERIMENTAL STUDY ON THE COHERENT STRUCTURE OF THE TURBULENT BOUNDARY LAYER IN OPEN-CHANNEL FLOW

1 INTRODUCTION The coherent structure of turbulence is the most important discovery of turbulence studies in the last several decades. The coherent structure is a joint spatial state (Liang, 1999). In this space, there exist all kinds of motions that are organized and related. Namely, strip structures, large vortical structures, and other organizing flows are present. In 1932, researchers found that turbulence wasn抰 a fully random phenomenon and came to realize that the repeated emergen…