Modern ground-based telescopes like the planned extremely large telescope (ELT) depend
heavily on adaptive optics (AO) systems to correct for atmospheric turbulence. Even though …

Ground-based astronomy utilizes modern telescopes to obtain information on the universe
by analyzing recorded signals. Due to atmospheric turbulence, the reconstruction process …

Blind deconvolution (BD), which aims to separate unknown convolved signals, is a
fundamental problem in signal processing. Due to the ill-posedness and underdetermination …

Point spread function (PSF) is important for evaluating an optical system and image
deblurring. In this paper, we proposed a method to measure space-variant PSF at any depth …

Military applications such as optical space surveillance and civilian applications such as
astronomical imaging often require adaptive optics to compensate images of distant objects …

In ground-based astronomy, images of objects in outer space are acquired via ground-
based telescopes. However, the imaging system is generally interfered by atmospheric …

High-resolution imaging with large ground-based telescopes is limited by atmospheric
turbulence. The observed images are usually blurred with unknown point spread functions …

We propose a simplified method to calculate the optical spread function of a paradigmatic
system constituted by a pupil-lens with a line-shaped illumination ('line-spread-function') …

Deconvolution from wave-front sensing (DWFS) is an imaging compensation technique for
turbulence degraded images based on simultaneous recording of short exposure images …

Adaptive optics is a commonly used technique to correct the phase distortions caused by the
Earth's atmosphere to improve the image quality of the ground-based imaging systems …