Imaging method of synthetic aperture radio telescope based on minimum-maximum concave penalty
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摘要: 在综合孔径射电望远镜中,从测量的可见度函数重构出辐射信号是一个病态的反问题。虽然压缩感知技术已成功地应用于综合孔径射电望远镜成像中,但是传统的压缩感知算法利用L1范数来近似取代L0范数,带来了一定的偏差。针对此问题,提出了一种基于最小最大凹惩罚的综合孔径射电望远镜成像方法。该方法利用最小最大凹惩罚来近似L0范数,并利用快速迭代软阈值算法求解最小化模型。在求解过程中,采用最大似然估计来自适应选取正则化参数,并采用重启和自适应策略来提高算法的收敛速度。实验结果表明,该方法在重建精度和对噪声鲁棒性方面优于目前典型的压缩感知算法,证明了其有效性。Abstract: In the synthetic aperture radio telescope, the reconstruction of the radiation signal from the measured visibility function is an ill-posed inverse problem. Although compressed sensing technology has been successfully applied in synthetic aperture radio telescope imaging, the traditional compressed sensing algorithm uses L1 norm to approximately replace L0 norm, which brings some bias. To address this problem, a new imaging method of synthetic aperture radio telescope based on min-max concave penalty is proposed. The method uses the min-max concave penalty to approximate the L0 norm and the fast iterative shrinkage-thresholding algorithm to solve the minimization model. In the iterative process, the regularization parameter is selected adaptively by using maximum likelihood estimation, and the convergence speed is improved by using restart and adaptive strategies. The experimental results show that the proposed method is superior to the current typical compressed sensing algorithms in terms of reconstruction accuracy and noise suppression, which proves its effectiveness.
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Key words:
- Radio telescope /
- aperture synthesis /
- compressed sensing /
- min-max concave penalty
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