Linkage of the Optical Reference Frame to the Radio Reference Frame

光学参考系与无线电参考系的链接

• 批准号: 63302008
• 负责人: MIYAMOTO M
• 金额: $ 4.74万
• 依托单位: National Astronomical Observatory of Japan
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Co-operative Research (A)
• 财政年份: 1988
• 资助国家: 日本
• 起止时间: 1988 至 1990
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-63302008/
• 关键词: Celestial Reference Frame; FK5; Radio Reference Frame; Earth Orientations; VLBI; Stellar Kinematics; Galactic Astronomy; 位置観測星表; 地球回転パラメ-タ; 光電子年環; 位置天文学; 子午環; スペ-スアストロメトリ; 光学基準座標系; 基本座標系; 天体力学; 歳差・章動; Space Astrometry

The aim of this cooperative research was to unite the Terrestrial, Dynamical, Stellar and Extragalactic reference frames together into a unique conventional celestial reference frame. The unique celestial reference frame thus established would be most appropriate for analyzing the kinematics of optical and radio objects in a consistent fashion. The individual researches for this aim were as follows :1) The extension of the optical fundamental reference frame FK5 to the fainter magnitude.2) The establishment of a global radio reference frame with high accuracy.3) The determination of the earth orientations under the international cooperation with VLBI networks.4) The re-construction of a basic theory of the celestial reference system for high precision observations.5) The future projects for constructing astrometric instruments on the ground and in the space.6) The galactic astronomy based on the modern kinematic data of stars.The results achieved by the individual members of this Research have been published in the Proceedings of Symposiums, edited by M.MIYAMOTO, "Linkage of Terrestrial, Dynamical, Stellar, and Extragalactic Reference Frames (I)-(III)" and "The Astrometry and the Galactic Astronomy."

这项合作研究的目的是将陆地，动力学，恒星和外层状参考框架团结成独特的常规天体参考框架。因此，因此建立的独特的天体参考框架最适合以一致的方式分析光学和无线电对象的运动学。该目的的个人研究如下：1）将光学基本参考框架FK5扩展到较弱的幅度。2）建立具有很高准确性的全球无线电参考框架。3）在国际合作下，与VLBI网络的国际合作确定地球方向的确定。4）构建了构建的始终构建的仪表范围，以构建高级构建，以构建高级构建。 6）基于星星的现代运动学数据的银河天文学。这项研究的各个成员的结果已在研讨会论文集中发表，由M.Miyamoto编辑，“地层，动态，动态，恒星，恒星和外层状参考框架（III） - （III） - 和callastry and anstry and anstry and anstry and anstry and and anstry and anstry and anstry and and anstry and anstry and anstry and anstry and anstry and anstry anstry and anstry anstrys”和“”。

项目成果

M.Yoshizawa and S.Suzuki: "The Tokyo PMC Catalog 86:Catalog of Positions of 3974 Stars Observed in 1986 with Tokyo Photoelectric Meridian Circle" Publications of the National Astronomical Observatory of Japan. Vol.1 NO.2. 127-176 (1989)

M.Yoshizawa 和 S.Suzuki：《东京 PMC 目录 86：1986 年用东京光电子午线观测到的 3974 颗恒星的位置目录》日本国家天文台出版物。

M. SOMA: "Toward Consistency in the Uses of Ephemerides" Astrophys. Space Sci. IAU Colloq.100. (1991)

M. SOMA：“星历表使用中的一致性”天体物理学。

M.Soma,S.Aoki: "Transformation from FK4 system to FK5 system" Astron.Astrophys.240. 150-158. (1990)

M.Soma，S.Aoki：“从 FK4 系统到 FK5 系统的转变”Astron.Astrophys.240。

藤下 光身,久慈 清助,笹夫 哲夫,佐藤 克久,田村 良明,鶴田 誠逸,佐藤 弘一,原 忠徳,高橋 幸雄: "6mアンテナによる測地VLBI観測とGPSとの結合" 1989年度「GPS研究会」集録. 113-116

Mitsumi Fujishita、Kiyosuke Kuji、Tetsuo Sasao、Katsuhisa Sato、Yoshiaki Tamura、Seitsu Tsuruta、Koichi Sato、Tadanori Hara、Yukio Takahashi：“耦合大地测量 VLBI 观测与 6m 天线和 GPS”1989 年“GPS 研究组”会议记录 .113- 116

M.Fujishita: "Observations of Proper Motions And Annual Parallaxes of Pulsars" 東北大学欧文報告. (1990)

M.Fujishita：“脉冲星固有运动和年度视差的观察”东北大学欧洲文献报告（1990）。