Abstract

In order to compensate for any failure on the use of point spread function (blur kernel) estimation and image estimation priors, we propose a novel regularization priors scheme with adapting the parameter for image restoration involving adaptive optics (AO) images. Our scheme uses a maximum a posteriori estimation with Gaussian statistics on the image and point spread function (blur kernel). An efficient regularization prior method associated with alternating minimization method is described to obtain the optimal solution recursively. Our method is applied to synthetic and real adaptive optics images. After applying our restoration method, satisfying results are obtained. Experimental results demonstrate that our proposed model and method performs better for restoring images in terms of both subjective results and objective assessments than the current state-of-the-art restoring methods. In addition, our proposed method can be a new way to promote their performances for AO image restoration.

Highlights

  • Seeing is the primary obstacle to obtaining high resolution astronomy observations from the ground

  • EXPERIMENTAL RESULTS we demonstrate the performance of our algorithm on simulated images and real adaptive optics images

  • The performance of our method is evaluated on adaptive optics images taken by a 1.2 m Adaptive optics (AO) telescope from Yunnan

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Summary

Introduction

Seeing is the primary obstacle to obtaining high resolution astronomy observations from the ground. Atmospheric turbulence along the line of sight randomly distorts the wavefronts [1]. The result is geometrical distortions and blurring in the collected images. Adaptive optics (AO) is an important tool that allows solar astronomers to achieve diffraction limited observations from existing ground based telescopes [2], [3]. Adaptive optics facilitates solar imaging with expressively reduced low-order aberrations. Due to the time scale of seeing evolution, AO only copes with limited high-order corrections

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