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Stability of Extensible Cable Connected Satellite System under Environmental Perturbation Forces in Elliptical Orbit

机译:椭圆轨道环境扰动力下可扩展有线卫星系统的稳定性

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The effect of environmental perturbation forces of the earth on the motion and stability of two cable-connected satellites in the earth's central gravitational field of force in elliptical orbit has been studied. In this paper the perturbation forces are the solar radiation pressure, the magnetic field of the Earth and the atmospheric resistance. The cable connecting the two satellites is assumed to be a light, flexible, non-conducting and extensible in nature. The effects of the Earth shadow have been considered during the analysis. The equations of motion of the system have been deduced with respect to the centre of mass, which is assumed to move along a Keplerian elliptical orbit. Hence a set of non-linear, non-homogeneous and non-autonomous differential equations in a rotating frame of reference in Nechvile's coordinates has been obtained for the motion of the system.rnThe Jacobi integral exists for the problem and with the help of this integral, we have discussed analytical and numerical stability of the system, we have used Liapunov sufficient condition for the stability of the system in elliptical orbit.
机译:研究了地球的环境扰动力对椭圆轨道上地球中央引力场中两颗连接卫星的运动和稳定性的影响。在本文中,摄动力是太阳辐射压力,地球磁场和大气电阻。假设连接两个卫星的电缆本质上是轻便,灵活,不导电且可扩展的。在分析过程中已考虑了地球阴影的影响。已经相对于质心推导了系统的运动方程,假定质心沿着开普勒椭圆轨道运动。因此,已获得Nechvile坐标中旋转参考系中的一组非线性,非齐次和非自治微分方程,用于系统的运动.rn Jacobi积分针对该问题而存在,并借助该积分,我们讨论了系统的解析和数值稳定性,我们使用Liapunov充分条件满足系统在椭圆轨道上的稳定性。

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