Attitude estimation or determination is a fundamental task for satellites to remain effectively operational. This task is furthermore complicated on small satellites by the limited space and computational power available on-board. This, coupled with a usually low budget, restricts small satellites from using high precision sensors for its especially important task of attitude estimation. On top of this, small satellites, on account of their size and weight, are comparatively more sensitive to environmental or orbital disturbances as compared to their larger counterparts. Magnetic disturbance forms the major contributor to orbital disturbances on small satellites in Lower Earth Orbits (LEO). This magnetic disturbance depends on the Residual Magnetic Moment (RMM) of the satellite itself, which for higher accuracy should be determined in real-time. This paper presents a method for in-orbit estimation of the satellite magnetic dipole using a Random Walk Model in order to circumnavigate the inaccuracy arising due to unknown orbital magnetic disturbances. It is also ensured that the dipole as well as attitude estimation of the satellite is done using only a magnetometer as the sensor.
翻译:姿态估计或确定是卫星继续有效运行的一项基本任务,这一任务在小型卫星上由于空间有限和机载计算力有限而更加复杂,这加上预算通常较低,限制了小型卫星使用高精度传感器进行姿态估计这一特别重要的任务。此外,小型卫星由于其大小和重量,相对较大的卫星而言,对环境或轨道扰动比较敏感。磁扰动是低地球轨道小卫星轨道上轨道扰动的主要促成因素。这种磁扰动取决于卫星本身的残余磁力动力(RMM),这种磁扰动取决于卫星本身的剩余磁力动力(RMM),而这种磁力动能的精度应实时确定。本文介绍了一种使用随机行走模型在轨估计卫星磁性顶点的方法,以便将未知轨道磁力扰动引起的不准确性加以环绕开。另外,还确保仅使用磁力计作为传感器对卫星进行浮度和姿态估测。