天球参考架的稳定源选取及其最新实现  

Newly Realization of Celestial Reference Frame by Stable Sources Selection

作　　者：乔书波[1,2,3] 李金岭[1] 柴洪洲[3] 李军正[3] 李健[3] 

机构地区：[1]中国科学院上海天文台,上海200030 [2]中国科学院研究生院,北京100039 [3]信息工程大学测绘学院,河南郑州450052

出　　处：《测绘学报》2010年第2期120-128,共9页Acta Geodaetica et Cartographica Sinica

基　　金：国家自然科学基金(10903032;10973030;10778635)

摘　　要：天球参考架是对理想的天球参考系的实现,其稳定性直接决定了所描述天体运动规律及某些地球物理现象的精度。基于1979-2007年期间全球IVS(international VLBI service)网近30年的观测资料,利用上海天文台的Calc_Solve系统对天测与测地VLBI资料进行解算和分析,得到一系列由射电源坐标(赤经和赤纬)构成的时间序列。通过对该时间序列的稳定性的检验和分析,制定选择稳定源的标准,得到一套稳定的河外射电源表列,最终实现由173颗稳定的定义源与135颗补充源构建的稳定天球参考架。When the motion of celestial bodies and some geophysical phenomena is described,a high precision and steady celestial reference system（CRS） is needed.An ideal CRS is equivalent to an inertia reference system.Celestial reference frame（CRF） is the realization of ideal CRS,the stability of which will directly determine the precision of celestial objects＇ motion and some geophysical phenomena.Based on nearly 30 years astrometric/geodetic observations of global IVS（international VLBI service） during 1979 to 2007,it is processed and analyzed the data using Calc_Solve software system on Shanghai Astronomical Observatory,CAS.Then it is acquired a series of coordinates（right ascension and declination） of radio sources,which can be made up to time series for our research.Stability of sources were checked and analyzed by the time series,a set of standards for the selection of stable sources is worked out,and then a set of lists of stable sources acquired.At last,a newly stable CRF are realized by 173 stable defining sources and 135 supplemental sources.

关 键 词：VLBI 天球参考架 稳定性 Calc_Solve 

分 类 号：P228[天文地球—大地测量学与测量工程]