Radial, transverse and normal satellite position perturbations due to the geopotential

IF 1.6 3区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Celestial Mechanics & Dynamical Astronomy Pub Date : 1987-09-01 DOI:10.1007/BF01235855

G. Rosborough, B. Tapley

引用次数: 69

查看原文本刊更多论文

由地球势引起的径向、横向和正常卫星位置扰动

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

Celestial Mechanics & Dynamical Astronomy 地学天文-数学跨学科应用

CiteScore

3.00

自引率

12.50%

发文量

审稿时长

6 months

期刊介绍： The international journal Celestial Mechanics and Dynamical Astronomy is concerned with the broad topic of celestial mechanics and its applications, as well as with peripheral fields. The papers published in Celestial Mechanics and Dynamical Astronomy include treatments of the mathematical, physical and computational aspects of planetary theory, lunar theory, general and special perturbation theory, ephemerides, resonance theory, geodesy of the Earth and the planets, dynamics, the 3-body problem, the n-body problem, space mechanics, ring systems, galactic dynamics, reference frames, time, relativity, nongravitational forces, computer methods, computer languages for analytical developments, and database management. Celestial Mechanics and Dynamical Astronomy is the journal of record in its field and is an indispensable component of reference libraries on Dynamical Astronomy, Astrodynamics and Dynamical Systems.