“苏定强星”命名仪式在浙江隆重举行

为表彰苏定强院士为我国乃至国际天文事业做出的贡献,值“第三届海峡两岸天文望远镜及仪器学术研讨会”期间,2009年7月21日下午,在浙江省海宁市隆重举行了”苏定强星”命名仪式。首先,南京天文光学技术研究所崔向群所长介绍了苏定强院士的学术贡献。     

让星光不再闪烁——提升星像质量的自适应光学

天文学家通过望远镜观测星空,无非想看得更深,更清楚。所以,评价一架天文望远镜的最重要的两个指标就是灵敏度与分辨率。其中,灵敏度可以通过扩大收集面积来提高,也就是增大望远镜的口径。分辨率与此类似,望远镜的口径与分辨能力成正比,即口径越大的望远镜的分辨率也就越高。     

射电星的光学位置和自行

1980－1981年期间，上海天台Ⅱ型光电等高仪和丹容等高仪（OPL No.14）共观测了15颗射电星。在FK5星表系统中得到了这些射电星的位置，并由这些观测位置与它们在其他星表例如G C，CAMC和W5／50中的相应位置进行比较，求得了这些射电星的自行。把我们求得的这些射电星的自行和PPM及CAMC星表中的相应自行作了比较，相互符合很一致。     

云南天文台太阳光学研究进展

总结和综述了云南天文台２０年来在太阳光学仪器研制和改造，太阳活动现象观测研究，太阳活动预报和国际交换合作方面的成果和进展。     

TROS-Ⅰ型流动人卫激光测距仪光学系统设计

介绍了车载流动型人卫激光测距仪光学系统(包括激光发射系统、接收系统及微光电视监视系统)的设计思想和方法,着重叙述了光学系统的结构设计、关键部件几何尺寸的确定及重要元器件的选取。设计基于流动型仪器应满足的防振、体积小、调校方便、抗环境干扰能力强等特点。多年的实测证明,这种光学系统不仅能满足流动型人卫激光测距仪总体设计要求,而且经济实用。     

The Difference between the α-disks of Seyfert 1 Galaxiesand Quasars

In a previous paper, it was suggested that contamination of the nuclear luminosity by the host galaxy plays an important role in determining the parameters of the standard a disk of AGNs. Using the nuclear absolute B band magnitude instead of the total absolute B band magnitude, we have recalculated the central black hole masses, accretion rates and disk inclinations for 20 Seyfert 1 galaxies and 17 Palomar-Green (PG) quasars. It is found that a small value of a is needed for the Seyfert 1 galaxies than for the PG quasars. This difference in a possibly leads to the different properties of Seyfert 1 galaxies and quasars. Furthermore, we find most of the objects in this sample are not accreting at super-Eddington rates if we adopt the nuclear optical luminosity in our calculation.     

分离式靶标摄影测量在LAMOST中的应用

为了获取LAMOST焦面板上光纤的零位位置,提出了一种基于分离式标准靶标的高精度摄影测量方法。首先,根据Tsai摄像机标定参数模型介绍了CCD相机的标定原理。然后介绍了用光重心算法求取靶标发光点像面坐标及通过球面三角公式计算靶标发光点物面坐标。接着,利用最小二乘法导出了含标定参数的方程组。最后,介绍了标准靶标的放置方法以及提高光纤位置测量精度的靶标取法。实验结果表明:CCD相机的标定残差平均值为8.8μm;标定残差的标准差为5.3μm。测量方法简单易行,通过仔细分析,找出了残差偏大的原因,对后续进一步测量实验有重要指导意义。     

Characterizing landscape spatial heterogeneity in multisensor images with variogram models

Most evaluation of the consistency of multisensor images have focused on Normalized Difference Vegetation Index （NDVI） products for natural landscapes, often neglecting less vegetated urban landscapes. This gap has been filled through quantifying and evaluating spatial heterogeneity of urban and natural landscapes from QuickBird, Satellite pour l＇observation de la Terre （SPOT）, Ad- vanced Spacebome Thermal Emission and Reflection Radiometer （ASTER） and Landsat Thematic Mapper （TM） images with variogram analysis. Instead of a logarithmic relationship with pixel size observed in the corresponding aggregated images, the spatial variability decayed and the spatial structures decomposed more slowly and complexly with spatial resolution for real multisensor im- ages. As the spatial resolution increased, the proportion of spatial variability of the smaller spatial structure decreased quickly and only a larger spatial structure was observed at very coarse scales. Compared with visible band, greater spatial variability was observed in near infrared band for both densely and less densely vegetated landscapes. The influence of image size on spatial heterogeneity was highly dependent on whether the empirical sernivariogram reached its sill within the original image size. When the empirical semivariogram did not reach its sill at the original observation scale, spatial variability and mean characteristic length scale would increase with image size; otherwise they might decrease. This study could provide new insights into the knowledge of spatial heterogeneity in real multisen- sor images with consideration of their nominal spatial resolution, image size and spectral bands.     

农作物遥感估产的方法综述

概述了遥感在农作物长势预测、种植面积测算和产量估算方面的原理、技术路线、研究进展,并分析了遥感估产在现实利用上存在的问题。