The orbit of the visual binary ADS 8630 (γ Vir)

We present a new orbit for the visual binary ADS 8630 = γ Vir. Although it is one of the first visual double stars discovered, its orbital elements were still poorly known. Indeed the very high eccentricity of the orbit and the difficulty of observing the pair at periastron passage in 1836 has meant that it is only now that sufficient measures of the recent close approach in 2005 have allowed an orbital analysis which predicts the angular motion to an acceptable degree of accuracy. We present a series of 35 speckle measurements of ADS 8630 obtained with PISCO in Merate between 2004 and 2006. Those measures have been crucial for determining the new orbital elements since they cover an arc of 130 degrees in the apparent orbit and include the periastron passage of 2005. The masses of the individual F0V components of the binary are found to be 1.40 M_⊙ with an accuracy of about 3%. We also investigate in detail the possibility of the presence of a third body in the system, that was proposed by other authors. The high‐angular resolution infra‐red image of γ Vir that we obtained in June 2006 with the LuckyCam instrument on the ESO NTT shows the absence of any companion as faint as a M0V star at a distance larger than 0.4″. Combined with the analysis of the residuals of our orbit, the values found for the masses of the individual components and the radial velocity measurements, this observation rules out the presence in the system of a third companion with a mass larger than 0.3 M_⊙. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Low‐mass visual binaries in the solar neighbourhood: The case of HD 141272

We search for stellar and substellar companions of young nearby stars to investigate stellar multiplicity and formation of stellar and substellar companions. We detect common proper‐motion companions of stars via multi‐epoch imaging. Their companionship is finally confirmed with photometry and spectroscopy. Here we report the discovery of a new co‐moving (13 σ) stellar companion ∼17.8 arcsec (350AU in projected separation) north of the nearby star HD141272 (21 pc).With EMMI/NTT optical spectroscopy we determined the spectral type of the companion to be M3±0.5V. The derived spectral type as well as the near infrared photometry of the companion are both fully consistent with a M_⊙ dwarf located at the distance of HD141272 (21 pc). Furthermore the photometry data rules out the pre‐main sequence status, since the system is consistent with the ZAMS of the Pleiades. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

A search for wide visual companions of exoplanet host stars: The Calar Alto Survey

We have carried out a search for co‐moving stellar and substellar companions around 18 exoplanet host stars with the infrared camera MAGIC at the 2.2 m Calar Alto telescope, by comparing our images with images from the all sky surveys 2MASS, POSS I and II. Four stars of the sample namely HD80606, 55 Cnc, HD46375 and BD–10°3166, are listed as binaries in the Washington Visual Double Star Catalogue (WDS). The binary nature of HD80606, 55 Cnc, and HD46375 is confirmed with both astrometry as well as photometry, thereby the proper motion of the companion of HD46375 was determined here for the first time.We derived the companion masses as well as the longterm stability regions for additional companions in these three binary systems. We can rule out further stellar companions around all stars in the sample with projected separations between 270AU and 2500AU, being sensitive to substellar companions with masses down to ∼60 M_Jup (S /N = 3). Furthermore we present evidence that the two components of the WDS binary BD–10°3166 are unrelated stars, i.e this system is a visual pair. The spectrophotometric distance of the primary (a K0 dwarf) is ∼67 pc, whereas the presumable secondary BD–10°3166B (a M4 to M5 dwarf) is located at a distance of 13 pc in the foreground. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

新一代可视化气象数据库管理系统

介绍了气象数据库管理系统软件的研制方法,系统采用面向对象技术,选用流行的可视人载具的第四代计算机语言－－Ｖｉｓｕａｌ Ｆｏｘｐｒｏ５作为编程语言,实现气象数据库的建库、查询、修改、复制、连接、转换等功能。『     

船体强度载荷可视化计算

利用ＯｂｊｅｃｔＡＲＸ语言,在ＶｉｓｕａｌＣ＋＋５．０开发平台中仿制了船体强度载荷可视化计算程序,程序具有船体载荷计算、光顺原始数据、仿真船体整过程和图形化计算结果的功能。     

深海机器人视景仿真系统研究

以载人深潜器的各种水动力参数和实际尺寸为基础,根据几何空间坐标方程建立了其运动学模型,采用MultiGen公司的Creator建模工具和Vega视景环境完成了在深海虚拟环境下的系统仿真。该系统可以实现深海机器人的可视化,更加直观、生动和实时的反映其位姿状态和水面、水下巡航过程。该系统实际应用在中国科学技术馆深海机器人展馆项目上,一方面展示载人深潜器的水下工作过程,同时也使得观众有机会亲身体验潜水器的操纵与驾驶。实际运行结果表明,该系统逼真地演示了载人深潜器水面备航、无动力下潜以及近海底巡航等仿真过程,能够满足系统仿真的实时性要求。该系统还可以应用到深海环境模拟研究、水下机器人运动仿真、控制系统调试以及操纵驾驶训练等中。     

基于空间点模式分析的城市管理事件空间分布及演化——以武汉市江汉区为例

城市网格化管理系统经过多年运行积累了大量历史事件数据, 这类事件数据在空间上呈现明显集聚分布。确定事件发生的空间分布以及衡量空间分布的集聚程度, 能够为城市管理资源的合理调配、划分提供重要的决策支持。本文应用空间点模式分析方法, 对2011 年1-8 月间武汉市江汉区城市网格化管理系统中的两类主体事件(占道经营和垃圾处理类)进行分析, 研究发现:占道经营事件的“热点”区域1-8 月总体呈减少趋势, 而垃圾处理事件的“热点”区域整体呈递增趋势;两类事件呈现明显的空间集聚, 其特征空间尺度都为1000 m左右。研究表明, 空间点模式分析方法能够为城市管理者提供一种针对城市事件空间集聚模式的直观的可视化分析手段, 以及对空间集聚程度的定量分析方法, 并可为进一步统计建模分析奠定基础。     

菲与芘在砂基培养的红树植物秋茄中的分布与可视化定位

本研究采用系列浓度盆栽试验研究多环芳烃（PAHs）菲与芘在红树植物秋茄（Kandelia obova-ta）中的迁移与分布规律,采用加速溶剂萃取（ASE）法和气相色谱-质谱（GC-MS）方法测定秋茄叶片和根中的多环芳烃含量,应用倒置荧光显微镜对秋茄叶片中的多环芳烃进行定位表征.结果表明：秋茄能从培养液中吸收菲和芘,并将根系吸收的菲和芘向叶片运输.秋茄体内菲和芘含量随处理时间（4、8、21 d）呈现先上升后下降的趋势,在培养8 d达到最大值.与4 d和8 d处理相比,在21d试验完成后,秋茄根与叶中的菲和芘含量显著降低,表明在红树植物体内存在明显的PAHs降解或者挥发.秋茄根系中的菲和芘含量随处理浓度提高而增高,与叶片相比,PAHs更多地在根部累积.在叶片中,菲和芘主要储存在叶片的维管束及附近的海绵组织中.     

面向不同主题的犯罪大数据可视分析

大数据时代,传统犯罪分析将向探索式可视分析的方向转变。本文基于公安犯罪数据的特点和犯罪分析理论,结合可视化技术（Wordle图、故事线图、平行坐标图、散点图矩阵等）,从表示内容、表示方法、交互设计等提出面向不同主题的犯罪大数据可视分析方法,其中,包括系列犯罪时空轨迹数据的可视分析、犯罪实时态势数据的可视分析、犯罪时空过程数据的可视分析、时间序列犯罪统计数据的可视分析、犯罪案情文本数据的可视分析、犯罪多维属性数据的可视分析,以及犯罪相关统计数据的可视分析等。相关可视分析方法为案件侦查、犯罪趋势预测、犯罪热点分析等方面提供了支持,也为今后面向其他领域的可视化表达研究提供了借鉴和参考。     

航线设计与设计结果的可视化仿真

介绍了一种基于定向理论的航线设计方法,利用设计结果实现了航摄仿真的技术与过程,讨论了实现航摄过程仿真预演功能对航摄工作的重要影响。