Simulating the earth magnetic field according to the 10th generation of IGRF coefficients for spacecraft attitude control applications

M. Navabi, N. Nasiri
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引用次数: 15

Abstract

In recent decades utilizing satellites in low earth orbits have had increasing tendency. These satellites experience the earth magnetic field more than others. The earth magnetic is used to control the attitude of spacecraft by the interaction between the earth magnetic field and magnetic dipoles. First of all, in order to use this phenomenon the intensity and the direction of the earth magnetic field have to be obtained. There are various ways in order to simulate the earth magnetic field and among these ways the most accurate one is the harmonic coefficients and the earth magnetic field mathematical model. In this study, the earth magnetic field is modeled based on the 10th generation of the IGRF coefficients and the results are verified with a valid reference. To utilize the earth magnetic field in the attitude control of a spacecraft, it is necessary to transform the magnetic filed into the spacecraft body frame. The transformation between orbital and body frame could be linear or nonlinear. In the next step, based on the comparison of the results of the spacecraft attitude dynamics with linear and nonlinear transformation, the validity of linear transformation is studied regarding spacecraft attitude angles.
根据第10代IGRF系数模拟地球磁场,用于航天器姿态控制
近几十年来,利用近地轨道卫星有日益增长的趋势。这些卫星比其他卫星更容易受到地球磁场的影响。地磁是利用地球磁场与磁偶极子之间的相互作用来控制航天器的姿态。首先,为了利用这一现象,必须获得地球磁场的强度和方向。模拟地磁场的方法有很多种,其中最准确的方法是谐波系数和地磁场数学模型。本研究基于第10代IGRF系数建立了地球磁场模型,并对结果进行了有效的验证。为了利用地磁场进行航天器姿态控制,需要将地磁场转化为航天器的体架。轨道和体架之间的转换可以是线性的,也可以是非线性的。在比较了线性变换和非线性变换航天器姿态动力学结果的基础上,研究了线性变换对航天器姿态角的有效性。
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