基于 Okhotsimsky-Egorov 弹道方法的欧拉-兰伯特问题求解

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Solar System Research Pub Date : 2024-10-15 DOI:10.1134/S0038094624700527
A. V. Ivanyukhin, V. V. Ivashkin
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引用次数: 0

摘要

本文提出了由 V.A. Egorov 提出并以 D.E. Okhotsimsky 的著作为基础的解决欧拉-兰伯特问题的方法,该方法专门用于分析牛顿中心场中两个给定点之间的一组飞行轨迹。将欧拉-兰伯特问题视为弹道学(动力学)的逆问题时,我们成功地开发出一种新的有效方法,用于确定与给定飞行时间相对应的轨道。将这种方法命名为 Okhotsimsky-Egorov 方法是合乎逻辑的。在所考虑的方法中,飞行集的参数是初始飞行路径角。所提方法的优点是:解的定义域结构有限且易于理解,算法简单明了,解与初速度的关系明确。通过该方法可以对飞行轨迹进行定性分析,并构建有效的数值方法。为了解决欧拉-兰伯特问题,使用了哈雷数值方法。对所考虑的算法进行了计算复杂性分析,结果表明其效率很高。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Solution of the Euler–Lambert Problem Based on the Okhotsimsky–Egorov Ballistic Approach

The paper propose the method for solving the Euler–Lambert problem proposed by V.A. Egorov and based on the works by D.E. Okhotsimsky, devoted to the analysis of a set of flight trajectories between two given points in the central Newtonian field. When considering the Euler–Lambert problem as the inverse problem of ballistics (dynamics), we have succeeded in developing a new effective method for determining the orbit corresponding to a given flight time. It is logical to name this approach the Okhotsimsky–Egorov method. In the considered approach, the parameter of the set of flights is the initial flight-path angle. The advantages of the proposed method are the limited and understandable structure of the domain of definition of solutions, the simplicity and clarity of the algorithm, and the clear dependence of the solution on the initial velocity. It enables a qualitative analysis of flight trajectories and the construction of effective numerical methods. To solve the Euler–Lambert problem Halley’s numerical method was used. A computational complexity analysis of considered algorithm was carried out and demonstrated its high efficiency.

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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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