长周期变星的演化及振动

长周期变星的演化和振动一直是引人入胜的课题。这不仅仅是因为在它们的变化过程中有丰富的物理内容 ,更重要的是可以用它们来做河外星系距离的定标者。在本文中详细的计算了在z=0 .0 0 0 5,z=0 .0 0 1 ,z=0 .0 0 5,z =0 .0 1和z=0 .0 2这样一个大的金属丰度跨度下 ,质量为 1 5M⊙ ,2 0M⊙ 和 3 0M⊙ 恒星的演化和振动。在计算中采用了最新的不透明度 ,考虑了星风损失对大质量星的影响 ,对于每一个模型都从零年龄主序演化到了中心氦燃烧结束。在文中仔细研讨了混合长参数以及中心对流核的对流超射对演化模型的影响 ,同时在中心氦燃烧阶段蓝超巨星和红超巨星的比值被用来限定模型的参数 (尤其是混合长和对流超射 )。尽管在文中并没有得到和观测一致的结论 ,即随着金属丰度的增加B/R增加。但是 ,通过在低金属丰度区采用对流超射 ,而在高金属丰度区放弃对流超射这一方法得到了与观测更相符合的比值。在新的演化模型的基础上 ,对于大质量星的振动进行了详细的计算。各项振动的性质用来和LMC ,M3 3以及MW中的RSGs做比较。对于LMC和M3 3中长周期变星 ,理论的周光关系和观测在基频振动模式下很好的符合 ;而对于MW中长周期变星 ,它们更可能在一阶模式下振动。最终 ,得到了金属丰度和周光关系的之间的联系 ,即随     

Modeling of atmospheres and spectral energy distributions of R CrB and V4334 Sgr (Sakurai's Object)

Procedures and results of computations of model atmospheres andspectral energy distributions of R CrB, V4334 Sgr and relatedobjects are discussed. The sequence of SEDs computed for a gridof model atmospheres with 4000 < T_eff < 7000, 0 < logg < 1 provides a unique possibility to analyze the temporalchanges of physical parameters of V 4334 Sgr and related objectsin the framework of a self-consistent approach.     

Star clusterings in the Carina complex: UBVRI photometry of Bochum 9, 10 and 11

We report on the first UBVRI CCD photometry of three poorly known star clusterings in the region of η Carinae: Bochum 9, 10 and 11. We find that they are young, rather poor, loose open clusters.
We argue that Bochum 9 is probably a small and loose open cluster with about 30 probable members having E ( B − V )=0.63±0.08 , located 4.6 kpc far from the Sun, beyond the Carina spiral arm.
Similarly, Bochum 10 is a sparse aggregate with 14 probable members having E ( B − V )=0.47±0.05 and at a distance of 2.7 kpc from the Sun.
Finally, Bochum 11 is a less than 4×10⁶ yr old cluster for which we identify 24 members. It has a reddening E ( B − V )=0.58±0.05 , and lies between Bochum 10 and 9, at 3.5 kpc from the Sun. We propose that in the field of the cluster some stars might be pre-main-sequence candidates.     

Fiber Optic Network Technology For Distributed Long Baseline Radio Telescopes

The construction costs of distributed radio telescopes are to a great extent determined by the deployment costs of the fiber optic data transport network that is needed to transport the received information to the data processor(s). As such, the baseline and data rates that are feasible for a specified amount of money are determined by the status of the technology and deployment costs of the communication network. In this paper the present day data transport status is described and, using a costing model, the most attractive data transport technologies are determined, taking the LOFAR telescope (ASTRON, 2005) as an example. In the outlook, the near-term data transport technology developments are described.     

Forecasting flood disasters using an accelerated genetic algorithm: Examples of two case studies for China

This article discusses a rescaled range analysis model, titled AGA-R/S, that is based on an accelerated genetic algorithm. The parameter a, Hurst index of rescaled range analysis, and the recurrent time of disaster in the next time-period, were directly computed using an accelerated genetic algorithm developed by the authors. As case studies, using the AGA-R/S model, a forecast was made of the tendency for change in a time series of annual precipitation for the city of Jinhua, China. The model also forecast flooding-disaster in the city of Wuzhou, China. Results indicate that it is a relatively efficient technique to forecast the change-tendency of flood and disaster time series using the AGA-R/S model. When time series is utilized, forecasted error of the AGA-R/S model is less than with a linear least square method. The Hurst indexes of the two cities are from 0.23 to 0.24, which indicates that these time series are fractal and relatively long-term. Their fractional Brownian motion shows anti-persistence. AGA-R/S has application in forecasting the change-tendency of other natural disaster for specific time series.     

多尺度空间数据索引方法研究

以多尺度空间数据为研究对象,讨论其混合索引结构的建立方法。对于多尺度矢量空间数据提出基于多层次网格与R 树混合索引结构,栅格数据进行分块并建立四叉树索引结构。利用双向链表结构连接同尺度下的矢栅空间数据,实现矢栅之间的无缝转化;并用地理数据编码及双向链表结构连接不同尺度下的同一空间对象,实现多尺度空间对象的纵向无缝连接。进而实现多尺度空间数据的快速可视化及空间对象的纵向无缝查询。     

Landmark‐based summarized messages for flood warning

In order to evacuate residents in time, flood warning systems must have rapid data processing algorithms to translate detailed numerical data into simple warnings and navigation aids. Although it is common to display warning messages by directly drawing red circles on a map embedded in a Web page to indicate the regions about to be inundated, such an approach has some drawbacks. We propose an alternative way by summarizing the warning messages based on landmarks, so that the messages can be short and convey even more information. We have designed two approaches to output such messages. They are the nearest landmark approach and the threshold approach, which differ in the way of determining which landmarks will be influenced by a certain flooded region. These two methods are implemented and we compare their performance through real and synthetic datasets. Experimental results show that the threshold approach usually takes less execution time than the nearest landmark approach. Its severity ranking of landmarks is also better suited to human behaviour.     

热带西北太平洋10~30 d振荡对南海夏季风影响

采用1958—2011年NCEP/NCAR再分析资料以及ERSST海温资料,分析热带西太平洋夏季对流10~30 d振荡对南海夏季风的影响。在年际变化尺度上,热带西北太平洋夏季10~30 d振荡强度指数 (TWPI) 与南海夏季风强度有很好的正相关关系。在TWPI增强年份,海温主要呈El Ni?o分布,南海周边区域增强的异常西风产生强的正涡度切变,导致异常气旋性环流,为季风槽的增强提供了热量和水汽,从而增强南海夏季风强度。反之,在TWPI减弱年份,海温主要呈La Ni?a分布,南海夏季风强度减弱。在不同的年代际背景下,垂直切变和水汽-对流的总体变化是影响TWPI总体变化的重要因子,但不能影响南海夏季风强度的总体变化。海陆热力对比的总体变化是导致南海夏季风强度总体变化的主要影响因素。     

三角洲前缘水下分流河道薄层单砂体成因类型及其叠置模式--以古城油田泌浅10区核三段Ⅳ-Ⅵ油组为例

泌阳凹陷古城油田泌浅10区核三段广泛发育三角洲前缘水下分流河道薄层砂体。在储层精细沉积微相研究的基础上,综合应用岩芯、密井网测井等资料,对古城水下分流河道单砂体进行了精细刻画,建立了单砂体规模定量预测模型。依据河道规模将古城水下分流河道分为Ⅰ型、Ⅱ型、Ⅲ型河道3类。运用高分辨率层序地层学短期基准面旋回原理,对研究层段水下分流河道砂体成因类型进行了研究。结果表明,在基准面低幅上升且A/S<<1时,形成削截式水下分流河道砂体;A/S<1(接近1)时,形成完整式水下分流河道砂体。识别出单一河道砂体的叠置类型主要包括垂向叠置、侧向叠置、垂向相切、侧向相切、垂向分隔5种垂向叠置模式以及间湾相隔式、水平搭接式、侧向切叠式3种平面接触样式,并总结了各自的测井相识别标志。