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Solution of the Problem of Optimal Spacecraft Launching into Orbit Using Reactive Acceleration and Solar Sail in Kustaanheimo-Stiefel Variables

机译:用反应加速和太阳能帆在浅景海姆 - Stieafel变量中发射进入轨道的最佳航天器启动问题

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摘要

Using the Pontryagin maximum principle and the Kustaanheimo–Stiefel variables, the spatial problem of optimal launching into a given orbit of a spacecraft (SC) controlled by a solar sail and limited or impulsive reactive acceleration of the SC’s center of mass has been solved. The minimized functional is a linear combination with weight factors of two criteria: time and the integral sum of the values of the reactive acceleration impulses of the SC’s center of mass spent on the control process. The first integrals of the equations of the problem and formulas for determining the increments of the phase and conjugate variables under the action of the imparted impulse of reactive acceleration are given. Numerical solutions of the problem are obtained for limited or impulsive acceleration with or without a solar sail. An assessment of the influence of the presence of a solar sail on the duration of the process, on the total impulse of the reactive acceleration value and on the value of the minimized functional is given. Cases of orbit correction and cases when the elements of the new orbit differ significantly from the elements of the initial spacecraft orbit are considered. The optimality of the reactive acceleration, orthogonal to the plane of the osculating orbit of the spacecraft, for the considered small values of the angular element deviations of the orbit from their initial values, i.e., the optimality of such acceleration in the considered examples of the problem of correcting the angular elements of the SC orbit.
机译:利用Pontryagin最大原理和kustaan​​heimo-stieafel变量,已经解决了由太阳能帆和Sc的喧嚣的限制或冲动或冲动的反应加速度控制的给定轨道的最佳发射轨道的空间问题。最小化的功能是与两个标准的权重因子的线性组合:时间和SC在控制过程上花费的反应加速度脉冲的值的数量和积分。给出了问题和用于确定在反应加速度的赋予脉冲的动作下的相位和缀合物变量的增量的问题的第一种积分。有关或没有太阳帆的有限或冲动加速度,获得了问题的数值解。给出了对过程的持续时间的评估,对过程的持续时间,对反应加速度值的总脉冲和最小化功能的值。轨道校正和案例的案例,当新轨道的元素显着不同地不同于初始航天器轨道的元素。对于航天器的横向轨道的平面正交的反应加速度的最优性,用于轨道的角质元素偏差从其初始值,即,在所考虑的例子中的这种加速度的最优性校正SC轨道角元素的问题。

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  • 来源
    《Cosmic research》 |2021年第4期|280-290|共11页
  • 作者单位

    Institute of Precision Mechanics and Control Problems Russian Academy of Sciences;

    Institute of Precision Mechanics and Control Problems Russian Academy of Sciences;

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  • 正文语种 eng
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