基于主体功能区划的上海市国土空间结构研究

构建由资源环境承载力子系统、现有开发密度子系统、发展潜力子系统3个子系统组成的上海市主体功能区指标体系。运用2012年数据计算各指标体系的综合得分,并制作Moran散点图。同时,依据资源环境承载力、现有开发密度与发展潜力这3个因素的综合评分以及Moran散点图的象限把上海市各区县划分成六大功能亚类:核心功能提升亚区、核心功能优化亚区、战略发展亚区、都市发展亚区、城市拓展亚区与生态涵养亚区。最后,剖析这六大功能亚区与国家层面上的优化开发区、重点开发区与限制开发区之间的内在联系。     

Optimizing the reservoir operating rule curves by genetic algorithms

Genetic algorithms, founded upon the principle of evolution, are applicable to many optimization problems, especially popular for solving parameter optimization problems. Reservoir operating rule curves are the most common way for guiding and managing the reservoir operation. These rule curves traditionally are derived through intensive simulation techniques. The main aim of this study is to investigate the efficiency and effectiveness of two genetic algorithms (GAs), i.e., binary coded and real coded, to derive multipurpose reservoir operating rule curves. The curves are assumed to be piecewise linear functions where the coordinates of their inflection points are the unknowns and we want to optimize system performance. The applicability and effectiveness of the proposed methods are tested on the operation of the Shih‐Men reservoir in Taiwan. The current M‐5 operating curves of the Shih‐Men reservoir are also evaluated. The results show that the GAs provide an adequate, effective and robust way for searching the rule curves. Both sets of operating rule curves obtained from GAs have better performance, in terms of water release deficit and hydropower, than the current M‐5 operating rule curves, while the real‐coded GA is more efficient than the binary‐coded GA. Copyright © 2005 John Wiley & Sons, Ltd.     

Gravitational Waves and Gravitational-wave Sourcestwo

The recent discovery of gravitational-wave burst GW150914 marks the coming of a new era of gravitational-wave astronomy, which provides a new window to study the physics of strong gravitational field, extremely massive stars, extremely high energy processes, and extremely early universe. In this article, we introduce the basic characters of gravitational waves in the Einstein's general relativity, their observational effects and main generation mechanisms, including the rotation of neutron stars, evolution of binary systems, and spontaneous generation in the inflation universe. Different sources produce the gravitational waves at quite different frequencies, which can be detected by different methods. In the lowest frequency range (f < 10^?15 Hz), the detection is mainly dependent of the observation of B-mode polarization of cosmic microwave background radiation. In the middle frequency range (10^?9 < f < 10^?6 Hz), the gravitational waves are detected by analyzing the timing residuals of millisecond pulsars. And in the high frequency range (10 ? 4 < f < 10⁴ Hz), they can be detected by the space-based and ground-based laser interferometers. In particular, we focus on the main features, detection methods, detection status, and the future prospects for several important sources, including the continuous sources (e.g., the spinning neutron stars, and stable binary systems), the burst sources (e.g., the supernovae, and the merge of binary system), and the stochastic backgrounds generated by the astrophysical and cosmological process. In addition, we forecast the potential breakthroughs in gravitational-wave astronomy in the near future, and the Chinese projects which might involve in these discoveries.     

X-ray measurements of black hole X-ray binary source GRS 1915+105 and the evolution of hard X-ray spectrum

We report the spectral measurement of GRS 1915+105 in the hard X-ray energy band of 20–140keV. The observations were made on March 30th, 1997 during a quiescent phase of the source. We discuss the mechanism of emission of hard X-ray photons and the evolution of the spectrum by comparing the data with earlier measurements and an axiomatic model for the X-ray source.     

台风纳沙和海棠的预报着眼点分析

2017年7月的两个台风(1709号台风纳沙和1710号台风海棠)在近海发生罕见的近距离相互作用和环流合并,给登陆点的预报及二次登陆时的强度预报造成很大困难,包括ECMWF和NCEP等在内的大部分数值模式均未能较好地做出预报,但实际业务中的官方预报则较为准确。本文总结了实际业务中的预报经验,并对预报着眼点进行了分析归纳,主要包括:利用天气学模型、模式的偏差订正经验和集合预报结果等,分析模式对副热带高压等大尺度环流背景预报的合理性;通过分析双台风最靠近时刻的相对强度来确定主环流,从而判断两个台风的登陆时间差、各自的极值强度和陆上维持机制的差异;充分考虑登陆台湾的路径角度和过岛时间这两个影响因子,从而修订台风二次登陆时的强度。     

Observational manifestations of the change in the tilt of the accretion disk to the orbital plane in her X-1/HZ her with phase of its 35-day period

We analyze and interpret the RXTE/ASM X-ray light curves for the close binary system Her X-1/HZ Her obtained from February 1996 to September 2004. Some of the features found previously in the averaged X-ray light curves are confirmed by the new RXTE/ASM data. In particular, the anomalous dips and post-eclipse recoveries in two successive orbits in the short-on state are clearly distinguishable and are stable features of the X-ray light curves. We argue that to account for these features, the tilt of the accretion disk to the orbital plane must be assumed to change with phase of the 35-day period. We present a numerical model that can reproduce the observed features of the light curves.     

Photometric analysis of EL Aqr

We present an analysis of the Hipparcos and ASAS photometry of the W UMa star EL Aqr. The Wilson-Devinney code is employed in conjunction with recent spectroscopic mass ratio of 0.203 to model the V band light curve. We confirm that the system is an A type contact binary however our analysis suggests that it is over massive for its spectral class and has a relatively high fillout of 44%. This revised version was published online in August 2006 with corrections to the Cover Date.     

利用GPS高求取正常高的几种拟合方法

全面系统地研究了GPS点正常高的拟合方法,对平面拟合、二次多项式拟合、移动曲面拟合、多曲面拟合的GPS水准拟合方法,采用不同参数进行了论述。并结合实际测区,对GPS水准点进行了计算分析。提出了不同测区、不同地形、不同大地水准面的拟合方法,部分拟合方法已用于实际生产中,结果表明,这些方法是切实可行的。通过计算分析,得出结论：不同地形、不同面积的测区需要采用不同的拟合模型,并且拟合时采用的参数也不同。利用GPS高求定正常高,能够降低劳动强度和作业成本,提高作业效率。     

天体运动的轨道偏心率研究概述---从恒星系统到行星系统

偏心率是描述天体运动轨道的重要参数之一, 能够为揭示天体的动力学演化提供重要线索, 进而帮助理解天体形成与演化的过程及背后的物理机制. 随着天文观测技术的不断发展, 人们对于天体运动轨道的研究已经走出太阳系, 包含的系统也从大质量端的恒星系统延伸到了低质量端的行星系统. 聚焦天体轨道偏心率研究, 回顾了目前在恒星系统(包括主序恒星、褐矮星以及致密星)和行星系统(包括太阳系外巨行星以及``超级地球''、``亚海王星''等小质量系外行星)方面取得的进展, 总结了不同尺度结构下偏心率研究的一些共同之处和待解决的问题. 并结合当下和未来的相关天文观测设备和项目, 对未来天体轨道偏心率方面的研究工作进行了展望.     

确定大熊W型双星质量比的一个近似方法

本文给出了一个确定大熊W型双星质量比的近似方法。如果知道大熊W型双星的周期P、主子星表面有效温度T_p和主次食深差△m,可通过该文导出的一个公式算得质量比。对21个大熊W双星进行了计算,结果表明用该方法确定的质量比同分光或测光质量比符合较好。