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We propose a multi-frame blind deconvolution method using an in-plane rotating sample optimized for X-ray microscopy, where the application of existing deconvolution methods is technically difficult. Untrained neural networks are employed as the reconstruction algorithm to enable robust reconstruction against stage motion errors caused by the in-plane rotation of samples. From demonstration experiments using full-field X-ray microscopy with advanced Kirkpatrick-Baez mirror optics at SPring-8, a spatial resolution of 34 nm (half period) was successfully achieved by removing the wavefront aberration and improving the apparent numerical aperture. This method can contribute to the cost-effective improvement of X-ray microscopes with imperfect lenses as well as the reconstruction of the phase information of samples and lenses.
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http://dx.doi.org/10.1038/s41598-024-79237-x | DOI Listing |
Appl Opt
February 2025
Multi-frame blind deconvolution (MFBD) can obtain high-resolution images degraded by the atmospheric turbulence with limited prior information, but it is time-consuming. To improve the efficiency of MFBD, we integrate the macopt minimizer into the alternate minimization framework and investigate the detailed parallelization methods using a message passing interface (MPI) and open multiprocessing (OpenMP) based on a multicore architecture. Three sets of simulated seasat images with sizes of 128 ∗ 128, 256 ∗ 256, 512 ∗ 512, and one set of real solar observations with size of 1600 ∗ 1600 are used for restoration experiments.
View Article and Find Full Text PDFSci Rep
March 2025
Faculty of Automatic Control, Electronics and Computer Science, Silesian University of Technology, Akademicka 16, 44-100, Gliwice, Poland.
Heliophysics phenomena on the Sun, such as radio bursts, can strongly affect satellites and ground-based electronic systems. Therefore, an insight into the actual image of the Sun with good spatial and temporal resolution is crucial. In this paper, we explore the possibility of using fully convolutional networks (FCNs) to improve the images acquired from remotely operated small solar telescopes whose resolution is limited by the size of the lens aperture and by atmospheric turbulence.
View Article and Find Full Text PDFSci Rep
November 2024
Department of Materials Physics, Graduate School of Engineering, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi, 464-8603, Japan.
We propose a multi-frame blind deconvolution method using an in-plane rotating sample optimized for X-ray microscopy, where the application of existing deconvolution methods is technically difficult. Untrained neural networks are employed as the reconstruction algorithm to enable robust reconstruction against stage motion errors caused by the in-plane rotation of samples. From demonstration experiments using full-field X-ray microscopy with advanced Kirkpatrick-Baez mirror optics at SPring-8, a spatial resolution of 34 nm (half period) was successfully achieved by removing the wavefront aberration and improving the apparent numerical aperture.
View Article and Find Full Text PDFMed Phys
December 2023
Department of Radiology and Nuclear Medicine, University Medical Center Utrecht, Utrecht, The Netherlands.
Background: With the introduction of prostate specific membrane antigen (PSMA) PET/CT, the detection rate of prostate cancer metastases has improved significantly, both for primary staging and for biochemical recurrence. EANM/SNMMI guidelines recommend a 60 min time interval between [ Ga]Ga-PSMA administration and acquisition.
Purpose: This study evaluates the possibility of a shorter time interval by investigating the dynamic change in image quality measures.
IEEE Trans Image Process
December 2022
Blind visual quality assessment (BVQA) on 360° video plays a key role in optimizing immersive multimedia systems. When assessing the quality of 360° video, human tends to perceive its quality degradation from the viewport-based spatial distortion of each spherical frame to motion artifact across adjacent frames, ending with the video-level quality score, i.e.
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