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Calibration of the OLFAR space-based radio telescope using an alternating least squares approach

机译:使用交替最小二乘法对OLFAR天基射电望远镜进行校准

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Radio astronomy below 30 MHz has never been properly performed because the ionosphere inhibits this on Earth. The Orbiting Low-Frequency Antennas for Radio Astronomy (OLFAR) project aims to build a radio telescope consisting of 50 or more nano-satellites in space, forming a swarm-like array. The observational antenna systems need to be calibrated to successfully detect astronomical signals. However, a satellite swarm presents a unique calibration challenge, which is outlined in this paper. An approach is proposed for the calibration of several important system parameters, based on alternating least squares (ALS). In the proposed method, polarization is taken into account without the common simplifications, such as only considering fully linear polarization, and a good convergence rate is achieved. For validation, Monte Carlo simulations are compared with the Cramer-Rao bound.
机译:从未适当地执行低于30 MHz的射电天文学,因为电离层抑制了地球上的射电天文学。用于射电天文学的低频轨道天线(OLFAR)项目旨在建造由50个或更多纳米卫星组成的射电望远镜,形成一个类似蜂群的阵列。观测天线系统需要进行校准以成功检测天文信号。但是,卫星群提出了独特的校准挑战,本文概述了这一挑战。根据交替最小二乘(ALS),提出了一种用于校准几个重要系统参数的方法。在所提出的方法中,考虑了极化而没有通常的简化,例如仅考虑完全线性极化,并且实现了良好的收敛速度。为了进行验证,将蒙特卡洛模拟与Cramer-Rao界线进行比较。

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