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arXiv 1405.4411astro-ph.IM
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利用地磁洛伦兹力的航天器姿态动力学与控制

Attitude dynamics and control of spacecraft using geomagnetic Lorentz force

Yehia A. Abdel-Aziz, Muhammad Shoaib

摘要:

研究了利用洛伦兹力在俯仰和滚转方向上产生的力矩来稳定近地轨道上带电刚体航天器的姿态。在地球磁场中,航天器表面产生静电荷时,会受到洛伦兹力的扰动。作用在带静电的航天器上的洛伦兹力可以提供用于控制航天器定向的有用推力。假设航天器在地球磁场中沿椭圆轨道运动,受到重力、地磁和洛伦兹力矩的作用。地球的磁场被建模为非倾斜偶极子。在电场和磁场的基础上,建立了一个将所有洛伦兹力矩作为轨道根数函数的模型。研究了航天器定向的稳定性问题。平衡位置的存在性和稳定性的电荷质量比($α^*$)的不同值进行了研究。稳定轨道被确定为各种值的$α^*$。航天器稳定的主要参数是$α^*$和航天器转动惯量各分量之间的差值。

英文摘要:

The attitude stabilization of a charged rigid spacecraft in Low Earth Orbit (LEO) using torques due to Lorentz force in pitch and roll directions is considered. A spacecraft that generates an electrostatic charge on its surface in the Earth magnetic field will be subject to perturbations from Lorentz force. The Lorentz force acting on an electrostatically charged spacecraft may provide a useful thrust for controlling a spacecraft's orientation. We assume that the spacecraft is moving in the Earth's magnetic field in an elliptical orbit under the effects of the gravitational, geomagnetic and Lorentz torques. The magnetic field of the Earth is modeled as a non-tilted dipole. A model incorporating all Lorentz torques as a function of orbital elements has been developed on the basis of electric and magnetic fields. The stability of the spacecraft orientation is investigated both analytically and numerically. The existence and stability of equilibrium positions is investigated for different values of the charge to mass ratio ($α^*$). Stable orbits are identified for various values of $α^*$. The main parameters for stabilization of the spacecraft are $α^*$ and the difference between the components of the moment of inertia of spacecraft.

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