当前位置:
X-MOL 学术
›
Solar Syst. Res.
›
论文详情
Our official English website, www.x-mol.net, welcomes your feedback! (Note: you will need to create a separate account there.)
Dynamic Structure of Near-Earth Orbital Space in the 1 : 2 Resonance Region with the Speed of Earth’s Rotation
Solar System Research ( IF 0.9 ) Pub Date : 2020-08-03 , DOI: 10.1134/s0038094620040085 I. V. Tomilova , D. S. Krasavin , T. V. Bordovitsyna
中文翻译:
地球自转速度在1:2共振区近地轨道空间的动态结构
更新日期:2020-08-03
Solar System Research ( IF 0.9 ) Pub Date : 2020-08-03 , DOI: 10.1134/s0038094620040085 I. V. Tomilova , D. S. Krasavin , T. V. Bordovitsyna
Abstract—
The paper presents the results of a study of the dynamic structure of near-Earth orbital space in the 1 : 2 resonance region with Earth’s rotation speed. The results of an extensive numerical-analytical experiment to study the orbital evolution of objects moving in the semimajor axis range from 26 550 to 26 570 km, with inclinations from 0° to 180°. In this region, the zones of action of the five components of the orbital resonance and aspidal–nodal secular resonances of low orders are revealed. The distribution maps of the revealed resonances are constructed. The dynamic structure of the orbital space was also investigated using the fast Lyapunov characteristic of MEGNO and represented by a MEGNO map of the region in the section by the plane (inclination of the orbit, major axis). It is shown that a feature of the dynamic evolution of most of the studied orbits is randomness arising under the influence of overlapping resonances of various types.中文翻译:
地球自转速度在1:2共振区近地轨道空间的动态结构