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In-orbit offline estimation of the residual magnetic dipole biases of the POPSAT-HIP1 nanosatellite

机译:POPSAT-HIP1纳米卫星残余磁偶极子偏置的在轨离线估计

摘要

The nanosatellite POPSAT-HIP1 is a Cubesat-class spacecraft launched on the 19th of June 2014 to test cold-gas based micro-thrusters; it is, as of April 2015, in a low Earth orbit at around 600 km of altitude and is equipped, notably, with a magnetometer. In order to increment the performance of the attitude control of nanosatellites like POPSAT, it is extremely useful to determine the main biases that act on the magnetometer while in orbit, for example those generated by the residual magnetic moment of the satellite itself and those originating from the transmitter. Thus, we present a methodology to perform an in-orbit offline estimation of the magnetometer bias caused by the residual magnetic moment of the satellite (we refer to this as the residual magnetic dipole bias, or RMDB). The method is based on a genetic algorithm coupled with a simplex algorithm, and provides the bias RMDB vector as output, requiring solely the magnetometer readings. This is exploited to compute the transmitter magnetic dipole bias (TMDB), by comparing the computed RMDB with the transmitter operating and idling. An experimental investigation is carried out by acquiring the magnetometer outputs in different phases of the spacecraft life (stabilized, maneuvering, free tumble). Results show remarkable accuracy with an RMDB orientation error between 3.6°and 6.2°, and a module error around 7%. TMDB values show similar coherence values. Finally, we note some drawbacks of the methodologies, as well as some possible improvements, e.g. precise transmitter operations logging. In general, however, the methodology proves to be quite effective even with sparse and noisy data, and promises to be incisive in the improvement of attitude control systems.
机译:纳米卫星POPSAT-HIP1是Cubesat级航天器,于2014年6月19日发射升空,用于测试基于冷气的微型推力器;截至2015年4月,它位于海拔约600公里的低地球轨道上,并配备了磁力计。为了提高诸如POPSAT之类的纳米卫星的姿态控制性能,确定在轨道上作用于磁力计的主要偏置非常有用,例如,由卫星本身的剩余磁矩产生的偏置以及源自卫星的剩余磁矩。发射器。因此,我们提出了一种方法,用于对由卫星的剩余磁矩引起的磁力计偏置进行在轨离线估计(我们将其称为剩余磁偶极偏置或RMDB)。该方法基于遗传算法和单纯形算法,并提供偏置RMDB向量作为输出,仅需要磁力计读数即可。通过将计算出的RMDB与发射机工作和空载进行比较,可以利用它来计算发射机磁偶极偏置(TMDB)。通过获取航天器寿命不同阶段(稳定,机动,自由滚动)的磁力计输出进行实验研究。结果表明,RMDB方向误差在3.6°至6.2°之间,模块误差在7%左右,具有卓越的精度。 TMDB值显示相似的相干值。最后,我们注意到该方法的一些缺点以及可能的改进,例如精确的变送器操作记录。但是,总的来说,该方法即使在数据稀少和嘈杂的情况下也被证明是非常有效的,并且有望在改善姿态控制系统方面发挥敏锐的作用。

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