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USING EQUINOCTIAL ORBITAL ELEMENTS AND QUASI-AVERAGE ELEMENT METHOD TO CONSTRUCT ANALYTICAL SOLUTIONS FOR GEOSTATIONARY SATELLITE

机译:利用等值轨道单元和准平均单元法构造对地静止卫星的解析解

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The eccentricity and the inclination of the satellite in geosynchronous orbit are both small, under this condition, perturbations from the Earth's non-spherical gravitational field result in orbit resonances due to incommensurable small denominators, that is, the problem of small eccentricity, small inclination and commensurability small incommensurable denominator exist simultaneously. Usually we adopt the classic Kepler orbital elements to describe an orbit, However, in the case of small eccentricities and small inclinations, the geometric meaning of the perigee and ascending node of an GEO is no longer clear, and the equations of motion have small denominators which results in the failure of the usual mean orbit element perturbation solution. This phenomenon of singularity is caused by the inappropriate choice of independent variables and has nothing to do with the dynamics. Such singularities can be avoided by choosing the appropriate independent variables (called non-singularity orbital elements). Incommensurable singularity appears in the process of solving the perturbation equations by the mean element methodology. The quasi-average element methodology retains the main advantages of the mean element method and reasonably revises its definition. Quasi-average orbits, without short periodic terms, while including the long-term items are taken as the reference orbit. The reference orbit in this transformation has long-term variations which are similar to the long periodic terms within a short-time duration. So we can avoid the failure of the perturbation solution caused by the periodic terms when using the classical perturbation method or the mean element method. Prom the perspective of mechanics, it can eliminate the incommensurable singularity, and the perturbation solution will remain valid. This paper aims at introducing the calculation method to eliminate the singularity problem of e=0,i=0 and commensurability singularity by using the quasi-average element methodology based on equinoctial orbital elements. Also, considering the perturbation of J2 J3 J4 and J2,2 terms of Earth's non-spherical gravitational field, the lunar gravitational field and solar gravitational field, we try to derive a general perturbation solution, which can be applied in different conditions. Thus "zero mistake" in application can be realized to improve the security of the satellite operation. Also, this method can be extended to solve the problems of singularity caused by other perturbations.
机译:卫星在地球同步轨道上的偏心率和倾角都很小,在这种情况下,由于非分母较小的分母,来自地球非球面重力场的扰动会导致轨道共振,即,偏心率小,倾角小和可比性小不可比分母同时存在。通常,我们采用经典的开普勒轨道元素来描述轨道,但是,在小偏心率和小倾角的情况下,GEO的近地点和上升节点的几何含义不再明确,并且运动方程的分母也很小这导致通常的平均轨道元素摄动解失败。这种奇异现象是由于自变量选择不当引起的,与动力学无关。通过选择适当的自变量(称为非奇异轨道元素),可以避免这种奇异性。用均值单元法求解微分方程的过程中出现了难以估量的奇异性。准平均元素方法保留了均值元素方法的主要优点,并合理地修改了其定义。不包括短周期项的准平均轨道,而包括长期项在内,则作为参考轨道。此转换中的参考轨道具有长期变化,类似于短期内的长周期项。因此,在使用经典摄动法或均值单元法时,可以避免由周期项引起的摄动解的失败。从力学的角度出发,它可以消除不可估量的奇异性,并且摄动解将仍然有效。本文旨在介绍一种计算方法,通过使用基于等位轨道元素的准平均元素方法消除e = 0,i = 0的奇异性问题和可比性奇异性。另外,考虑地球非球面引力场,月球引力场和太阳引力场的J2,J3,J4和J2,2项的摄动,我们试图推导一个通用的摄动解,该解可以在不同的条件下应用。因此,可以实现应用中的“零错误”,以提高卫星运行的安全性。而且,可以扩展该方法以解决由其他扰动引起的奇异性问题。

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