The tiling algorithm for the 6dF Galaxy Survey     

Lachlan Campbell  Will Saunders  Matthew Colless 《Monthly notices of the Royal Astronomical Society》2004,350(4):1467-1476

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Morphology and Luminosity Segregations in Galaxy Groups     

M. Girardi  F. Mardirossian  M. Mezzetti  E. Rigoni 《Astrophysics and Space Science》2003,285(1):31-35

We study morphology and luminosity segregation of galaxies in groups. We analyze the two catalogs of (∼2×400) groups which have been identified in the Nearby Optical Galaxy sample, by means of hierarchical and percolation `friends-of-friends' methods. We find that earlier-type (brighter) galaxies are more clustered and lie closer to the group centers, both in position and in velocity, than later-type (fainter) galaxies. Spatial segregations are stronger than kinematical segregations. These effects are generally detected at the ≳3-sigma level, with the exception of morphological segregation in velocity, which is the weakest effect. Our main results are confirmed by the analysis of statistically more reliable groups (with at least five members), and are strengthened by the detection of segregation in both hierarchical and percolation catalogs. Luminosity segregation is shown to be independent of morphology segregation. Our conclusions agree with a continuum of segregation properties of galaxies in systems, from low-mass groups to massive clusters. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

太阳活动区磁场观测的一种新方法     

崔连竖  季国平  方成 《中国天文和天体物理学报》1986,(3)

在太阳活动区的物理研究中,特别是在二维动力学光谱分析中,迫切需要相应活动区的磁图资料。本文介绍了在太阳光谱仪的入射狭缝后安装一种新型偏振器进行活动区二维磁场观测的新方法。这种方法不仅能获得日面上任一点的磁场强度,且可快速获得活动区的纵向场磁图。除此之外,还可利用多条谱线的同时观测,获得有关磁力线管结构等方面的资料。  相似文献   

Radio interferometers with wide bandwidths     

Ravi Subrahmanyan 《Monthly notices of the Royal Astronomical Society》2004,348(4):1208-1214

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北太平洋亚热带环流区表层水中226Ra和228Ra的分布与变化     

李艳平  陈敏  黄奕普  蔡毅华 《台湾海峡》2004,23(3):261-267

对1999年9～10月采自北太平洋亚热带环流区的19份表层海水样品的Ra同位素分析表明。研究海域表层水中的^226Ra、^228Ra放射性比度分别介于0．67～0．92、0．08～0．30Bq／m^3之间，平均值分别为0．74、0．11Bq/m^3．^226Ra/^228Ra)A．R．活度比的变化范围为0．11～0．44，平均值为0．19．上述数值明显低于近岸海域水体的相应值，表现为典型的开阔大洋水的特征．从空间分布的特征看，研究海域Ra同位素含量与^226Ra/^228Ra)A.R.值均呈均匀分布态势．将本研究结果与历史数据进行对比后发现，本研究获得的^226Ra、^228Ra放射性比度比20世纪60～80年代得到的数据来得低，可能与水体层化作用加强导致的Ra补充量的减少以及生物生产力升高导致的Ra迁出量的增加有关．北太平洋亚热带环流区表层水中Ra同位素的时间变化与文献报道的该海域叶绿素a、硅酸盐、磷酸盐含量与初级生产力的历史变化趋势相吻合．  相似文献   

浅谈水化数字观测仪器的使用   总被引：1，自引：0，他引：1  

杨玉光 《东北地震研究》2004,20(2):57-64

以朝阳地震台水化观测实践为基础，对使用水化数字仪器遇到的问题进行了详细讨论。  相似文献   

The Basic Shape Classification of Space Debris with Light Curves     

LU Yao  ZHAO Chang-yin 《Chinese Astronomy and Astrophysics》2021,45(2):190-208

We study the machine learning method for classifying the basic shape of space debris in both simulated and observed data experiments, where light curves are used as the input features. In the dataset for training and testing, simulated light curves are derived from four types of debris within different shapes and materials. Observed light curves are extracted from Mini-Mega TORTORA (MMT) database which is a publicly accessible source of space object photometric records. The experiments employ the deep convolutional neural network, make comparisons with other machine learning algorithms, and the results show CNN (Convolutional Neural Network) is better. In simulational experiments, both types of cylinder can be distinguished perfectly, and two other types of satellite have around 90% probability to be classified. Rockets and defunct satellites can achieve 99% success rate in binary classification, but in further sub-classes classifications, the rate becomes relatively lower.  相似文献   

兰州台FSQ自记水管倾斜仪与CZB-1型竖直摆倾斜仪的对比分析     

余飞龙  龙艳  梅东林 《高原地震》2006,18(2):42-48

将兰州台的FSQ与CZB-1仪的观测资料质量、变化趋势、潮汐响应函数及映震能力进行了对比分析,认为:FSQ的观测资料的质量比CZB-1要好,因CZB-1的资料存在漂移现象;在潮汐因子和相位滞后方面,FSQ比CZB-1反应灵敏;但CZB-1的映震能力比FSQ强。  相似文献   

障碍物对风速风向影响的观测试验     

田东霞  郭建侠  陈挺  关彦华  刘文忠  杨彬云  薛筝筝 《气象科技》2014,42(5):881-887

随着城市化进程的加大,测站周围障碍物的存在使风观测资料失去代表性、准确性和比较性。为定量化研究障碍物对风观测的影响,开展了河北沽源构筑物观测试验,通过对比构筑物修建前后各测点的风速风向资料,分析了障碍物对风速风向的影响。分析结果显示:1障碍物对风速的衰减作用与背景风速大小有关,风速越大,衰减作用越强;2背景风速在2~6m/s时,障碍物背风面测点风速衰减随距离增大而减小,在10倍障碍物高度距离处平均约衰减15%;背景风速大于6m/s时,背风面各测点风速衰减先增大后减小,在大约5倍障碍物高度的距离处衰减最大,10倍障碍物高度的距离处平均约衰减20%~30%;3障碍物的存在使主风向的风向频率减小,对风向的影响距离为6倍障碍物高度。  相似文献   

Research on Parallel Algorithms for uv-faceting Imaging     

《Chinese Astronomy and Astrophysics》2019,43(3):424-443

The uv-faceting imaging is one of the widely used large field of view imaging technologies, and will be adopted for the data processing of the low-frequency array in the first stage of the Square Kilometre Array (SKA1). Due to the scale of the raw data of SKA1 is unprecedentedly large, the efficiency of data processing directly using the original uv-faceting imaging will be very low. Therefore, a uv-faceting imaging algorithm based on the MPI (Message Passing Interface)+OpenMP (Open Multi-Processing) and a uv-faceting imaging algorithm based on the MPI+CUDA (Compute Unified Device Architecture) are proposed. The most time-consuming data reading and gridding in the algorithm are optimized in parallel. The verification results show that the results of the proposed two algorithms are basically consistent with that obtained by the current mainstream data processing software CASA (Common Astronomy Software Applications), which indicates that the proposed two algorithms are basically correct. Further analysis of the accuracy and total running time shows that the MPI+CUDA method is better than the MPI+OpenMP method in both the correctness rate and running speed. The performance test results show that the proposed algorithms are effective and have certain extensibility.  相似文献