天体测量

反常折射已成为传统天体测量学的主要误差来源。

Anomalous refraction is believed to be the main error source for classical astrometry .

美国宇航局和欧洲空间局的空间天体测量计划

Space astrometry as NASA and ESA projects

b、相关处理的方法。天体测量定位问题的最大相关估计

( b ) the way of correlation . Astrometric Location with Maximum Correlation Procedure

CCD在空间天体测量上的应用

The CCD applications to space Astrometry

认为观测精度比较好的仪器，例如PZT，子午环，还有很多工作要做，在天体测量学以及地球物理学领域内，空间技术并不能完全取代经典手段。

In astrometric and geodynamic areas the classical instruments will not be fully replaced by space technology .

射电源结构对VLBI天体测量的影响

The Effects of Radio Source Structures on VLBI Astrometry

PDS在天体测量中的应用技术&Ⅲ.星像粗略坐标的测量

Applied techniques of PDS in photographic astrometry - ⅲ . measurement of rough coordinates for star images

最后介绍了空间天体测量卫星DIVA、GAIA、SIM和FAME计划的进展。

Finally , the progress of space astrometric satellites : DIVA , GAIA , SIM and FAME are introduced .

介绍由天体测量卫星GAIA和SIM给出的天球参考架可能逵到的精度。

The accuracy of the future international celestial reference frame obtained from astrometric satellites : SIM and GAlA are given .

本文系统地研究了VLBI天体测量和大地测量数据处理软件系统（CALC／SOLVK）。

The VLBI software ( CALC / SOLVK ) for astrometry and geodesy ware researched in detail .

在窄角天体测量方面，将来地面上的长基线红外干涉仪，如Keck干涉仪阵，具有10μas级观测精度的潜力。

Future ground-based infrared long-baseline interferometer , such as Keck interferometer array , would have potential of 10 μ as in narrow angle astrometry .

并讨论了在目前的天体测量新技术如甚长基线干涉仪（VLBI）、激光测卫（SLR）、激光测月（LLR）已成功地用于天文地球动力学的情况下，GPS发展的可能前景。

Under the recent situation that new astronomical technigues , for example , Very Long Baseline Interferometry ( VLBI ), Satellite Laser Ranging ( SLR ) and Lunar Laser Ranging ( LLR ), are successfully applied to astro-geodynamics , the possible trends of GPS are discussed .

叙述了未来10年可能实施的几个空间天体测量计划，如欧洲空间局的GAIA、美国喷气推进实验室的SIM、德国的DIVA、美国海军天文台的FAME和俄罗斯普尔科沃天文台的STRUVE等。

In the third section , some space astrometric projects , which will probably be carried on in the next decade , such as GAIA of ESA , SIM of US JPL , DIVA of Germany , FAME of US Naval Observatory and STRUVE of Pulkovo , Russia are described .

依巴谷卫星和哈勃空间望远镜的天体测量观测结果

Astrometric Observational Results of the Hipparcos Satellite and the Hubble Space Telescope

用于1.56米天体测量望远镜的微计算机控制系统

Using the microcomputer system for the 1.56 m astrometric telescope

未来10年我国天体测量研究方向的建议

Suggestions on astrometric research field in China in next decade

近10年我国天体测量的发展

Development of Astrometry in China in the Most Recent Decade

空间时代地面光学天体测量的意义

Ground-Based Optical Astrometry in the Time of Space Astrometry

人生的位置在卫星上的天体测量

Where Is the Proper Place in My Life ASTROMETRY FROM THE ARTIFICIAL SATELLITE

伊巴谷空间天体测量任务对天文学发展的意义

Scientific Objectives of HIPPARCOS Space Astrometry Mission for Astronomy

利用新编依巴谷天体测量资料研究银河系运动

A Kinematical Study for the Galaxy Based on the Revised Hipparcos Astrometric Data

今天，天体测量学家再也不能对相对论问题置之不理了。

At present , astrometrists can not pay no attention to relativity any longer .

昴星团天体测量标准区域441颗星的高精度位置和自行

High-precision positions and proper motions of 441 stars in the Pleiades astrometric standard region

云南天文台基本天体测量工作的发展

Development of the Fundamental Astrometry at Yunnan Observatory

相对论天体测量学中的基本概念和定义

Basic Conceptions and Definitions of Relativistic Astrometry

天体测量研究室对我国体育企业进行市场细分的必然性及对策

The Astrometry Division The necessity and countermeasures of elaborate market division of Chinese sports enterprises

未来10年天体测量的发展

Development of Astrometry in the Next Decade

毫秒脉冲星在天体测量中的应用

Application of Millisecond Pulsars in Astrometry

长基线光干涉与天体测量

Long Baseline Optical Interferometry and Astrometry

天体测量学需要在相对论框架下重新建立自己的理论体系。

A new theoretical system of astrometry in the frame of relativity ought to be finished .