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An analytic method for computing the state transition matrix which includes the first-order secular perturbations of planet oblateness

机译：一种计算状态转移矩阵的分析方法，包括行星扁率的一阶长期扰动

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Kirkpatrick, J. C.;
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年度 1968
页码 1-47
总页数 47
原文格式 PDF
正文语种 eng
中图分类工业技术;
关键词
ORBITAL ELEMENTS; TRAJECTORY OPTIMIZATION; TRANSFORMATIONS (MATHEMATICS); CARTESIAN COORDINATES; MATRICES (MATHEMATICS); OBLATE SPHEROIDS; ORBIT PERTURBATION;

机译：轨道元素;轨迹优化;转型（数学）; CaRTEsIaN COORDINaTEs; maTRICEs（maTHEmaTICs）;暴露的球形;轨道摄动;

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专利

1. Nonlinear theory of secular perturbations of satellites of an oblate planet [J] . Nikonchuk D.V. Astronomy letters . 2012,第12期

机译：扁圆卫星长期扰动的非线性理论
2. Planetocentric Gravitational Sphere of the Dominating Influence of Perturbations from Planet Oblateness over Perturbations from External Bodies [J] . V. I. Prokhorenko Cosmic research . 2010,第2期

机译：行星扁度扰动对外体扰动起主要作用的行星中心引力球
3. Integrable Cases of the Three-Body Problem at First-Order Resonance and Oblateness of a Central Planet [J] . V.N. Shinkin Космические исследования . 1999,第5期

机译：中心行星一阶共振和扁率下三体问题的可积情形
4. Analytic Solution to the Relative Orbital Motion Around an Oblate Planet [C] . D. Condurache, V. Martinusi AIAA Guidance, Navigation, and Control Conference and Exhibit;AIAA Atmospheric Flight Mechanics Conference;AIAA Modeling and Simulation Technologies Conference . 2009

机译：扁圆行星相对轨道运动的解析解
5. A SEMI-ANALYTIC THEORY FOR SATELLITE ORBIT PREDICTION (PERTURBATION METHODS, EQUIVALENCE PERTURBATION METHODS, GEOPOTENTIAL HAMILTONIAN, POINCARE ELEMENTS, DENSITY MODELS). [D] . AHMED, AHMED HUSSEIN. 1985

机译：卫星轨道预测的半解析理论（摄动方法，当量摄动方法，地势哈密顿量，庞加莱元素，密度模型）。
6. Compressed sensing based cone-beam computed tomography reconstruction with a first-order method [O] . Kihwan Choi, Jing Wang, Lei Zhu, -1

机译：基于压缩感测的锥束计算机层析成像的一阶重建
7. An Adaptive Analytic Continuation Method for Computing the Perturbed Two-Body Problem State Transition Matrix [O] . Tahsinul Haque Tasif, Tarek A. Elgohary 2020

机译：用于计算扰动双体问题状态转换矩阵的自适应分析延续方法

An analytic method for computing the state transition matrix which includes the first-order secular perturbations of planet oblateness

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