Solar System Research ( IF 0.6 ) Pub Date : 2021-07-17 , DOI: 10.1134/s0038094621030011 A. G. Aleksandrova 1 , E. V. Blinkova 1 , T. V. Bordovitsyna 1 , N. A. Popandopulo 1 , I. V. Tomilova 1
Abstract
The paper presents the results of identifying secular resonances that act on objects moving in the LEO–MEO regions. The results were obtained from the processing of data of an extensive numerical experiment on the study of the orbital evolution of objects moving in the range of the semi-major axes from 8000 km to the operation zone of the GLONASS navigation systems (25 500 km), with inclinations from 0° to 180° outside the zones of orbital resonances. The distribution maps of the identified secular resonances are given. The analysis of the orbital evolution of the objects is presented.
中文翻译:
近地轨道空间LEO-MEO区域运动物体动力学的长期共振
摘要
本文介绍了识别长期共振的结果,这些共振作用于在 LEO-MEO 区域移动的物体。这些结果是通过对在 8000 公里至 GLONASS 导航系统工作区(25 500 公里)范围内移动的物体的轨道演化进行研究的广泛数值实验的数据处理获得的,在轨道共振区外的倾角从 0° 到 180°。给出了确定的长期共振的分布图。提出了对物体轨道演化的分析。