A possible active galactic nucleus in M82?

MERLIN and VLA observations of the galaxy M82 have detected a jet-like feature emanating from one of the compact sources, 44.01+59.6. The proximity of this source to the dynamical centre of M82 led us to suspect that it could be a weak active nucleus rather than an SNR. We imaged this source using the EVN at 15 mas and although it shows a compact shell-like structure which could be consistent with an SNR, we note that the EVN image shows a bright region within the source which is elongated along the jet direction. There are distinct similarities between this source and the Sgr A complex at the centre of our own Galaxy which contains the compact AGN, Sgr A^*.     

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安徽省地震会商地理信息系统的研制与实现

文章结合安徽省现有分析预报手段和数学模型,以Visual Studio2005.net作为开发语言,利用GIS技术对地震地质和基础地理等数据进行管理、分析,通过快速访问前兆数据库,对前兆数据进行查询和曲线调用出图,最终研制实现了一套满足日常及紧急会商需要,集"基础数据查询""前兆数据管理""前兆数据注释""应急会商报告...     

Head/Tail Breaks: A New Classification Scheme for Data with a Heavy-Tailed Distribution

This article introduces a new classification scheme—head/tail breaks—to find groupings or hierarchy for data with a heavy-tailed distribution. The heavy-tailed distributions are heavily right skewed, with a minority of large values in the head and a majority of small values in the tail, commonly characterized by a power law, a lognormal, or an exponential function. For example, a country's population is often distributed in such a heavy-tailed manner, with a minority of people (e.g., 20 percent) in the countryside and the vast majority (e.g., 80 percent) in urban areas. This new classification scheme partitions all of the data values around the mean into two parts and continues the process iteratively for the values (above the mean) in the head until the head part values are no longer heavy-tailed distributed. Thus, the number of classes and the class intervals are both naturally determined. I therefore claim that the new classification scheme is more natural than the natural breaks in finding the groupings or hierarchy for data with a heavy-tailed distribution. I demonstrate the advantages of the head/tail breaks method over Jenks's natural breaks in capturing the underlying hierarchy of the data.     

Assimilating data into open ocean tidal models

The problem of deriving tidal fields from observations by reason of incompleteness and imperfectness of every data set practically available has an infinitely large number of allowable solutions fitting the data within measurement errors and hence can be treated as ill-posed. Therefore, interpolating the data always relies on some a priori assumptions concerning the tides, which provide a rule of sampling or, in other words, a regularization of the ill-posed problem. Data assimilation procedures used in large scale tide modeling are viewed in a common mathematical framework as such regularizations. It is shown that they all (basis functions expansion, parameter estimation, nudging, objective analysis, general inversion, and extended general inversion), including those (objective analysis and general inversion) originally formulated in stochastic terms, may be considered as utilizations of one of the three general methods suggested by the theory of ill-posed problems. The problem of grid refinement critical for inverse methods and nudging is discussed.     

矿井水化学数据管理与综合应用实例

为有效管理和利用矿井长期积累的大量水化学数据,介绍了基于Microsoft Excel的数据管理方法。该方法既方便水化学特点分析,也有利于质量标准化建设,设计的数据表可作为模板供生产单位防治水技术人员使用。通过应用实例说明了水化学数据在防治水工作中的重要性,同时,也证明传统简单分析方法仍是常用且有效的方法。     

中巴地球资源一号卫星CCD图像质量评价和交叉定标研究

使用定量分析方法评价了中巴地球资源卫星CCD相机遥感数据质量 ,在此基础上利用LANDSAT 7ETM 对CCD的对应波段进行交叉定标计算 ,得到了一组CCD的参考定标系数。在遥感数据质量评价研究中 ,使用统计分析方法计算得到了CCD相机图像数据的条纹强度 ;应用结构函数方法计算获得了CCD的噪声数据 ;通过功率谱计算 ,对比分析了CCD和LANDSAT 7ETM 对应波段图像空间纹理特征。该文通过交叉定标计算 ,得到了CCD相机前 4个波段的参考定标系数、动态范围和噪声等效反射率等参考指标 ,并对这组定标系数进行了验证 ,从验证结果中发现CCD1,2 ,3和LANDSAT 7ETM 对应波段反射率最大相差 1 98% ,最小0 0 3% ,平均差要低于 1 31% ,而波段 4最大也仅相差 4 4 1% ,平均差 3 0 2 % ,证明计算得到的交叉定标系数具有较高的参考价值     

MODIS 1B影像几何纠正方法研究及软件实现

MODIS影像是一种新型和重要的数据。对MODIS 1B影像几何畸变原因进行了深入分析，选择了一种合适的纠正方法。对于1km分辨率MODIS 1B影像，直接采用1km分辨率的空间坐标进行几何纠正；对于250m和500m分辨率的MODIS 1B影像，先用三次样条曲线对坐标进行插值生成同分辨率的坐标，然后利用坐标插值结果对其进行几何纠正。由于MODIS影像在空问分布上的特殊性，采用前向和后向映射相结合的方式确定纠正后某一像素点在原始影像中的位置。根据该位置的条带重叠度，可以确定参与计算像素个数、搜索窗口的大小以及窗口的精确位置；采用归一化反距离加权插值法计算纠正后像素点的属性值。上述优化算法不仅保证了纠正后影像的质量，而且提高了数据处理速度。作者在Visual C 6．0环境下开发实现了上述算法。从坐标插值和几何纠正结果分析，无论是数据处理速度还是纠正后的影像质量和精度均达到要求。     

高光谱数据在数据库中的高效存储技术研究

通过分析高光谱数据的特点 ,结合数据库系统开发实践 ,提出了高光谱数据集 ,包括图像、光谱、属性等 ,在关系数据库中的存储规范。结合ORACLE数据平台 ,提出了 3种高光谱数据的存储模式 ,并结合应用实例进行对比 ,分析了各自的优缺点以及适用条件。