• Home
  • Search
  • Neural blind deconvolution to reconstruct high-resolution ground-based solar observations
  • https://doi.org/10.1051/0004-6361/202658932Copy DOI Icon

Neural blind deconvolution to reconstruct high-resolution ground-based solar observations

Show More
  • Abstract
  • Literature Map
  • Similar Papers
Abstract

Ground-based solar observations enable unprecedented spatial, spectral, and temporal resolution of the lower solar atmosphere, yet Earth’s turbulent atmosphere imposes significant limitations, requiring advanced post facto image reconstruction. State-of-the-art reconstruction methods are based on restoring a burst of short exposure frames to a single observation. Limitations of these techniques arise due to the sparse information available concerning the atmospheric point spread function (PSF), which degrades the observations and, consequently, the quality of reconstructions. Developing new reconstruction methods is essential for providing high-quality data products for the study of the lower solar atmosphere on the smallest scales. We aim to develop a novel image-reconstruction method to achieve unprecedented spatial resolution from short exposure image bursts. This can provide high-quality reconstructions and therefore advance the study of the smallest spatial scales from the solar photosphere to the chromosphere. In this paper, we present a novel approach for high-resolution solar-image reconstruction based on physics-informed neural networks. In the training process, the neural network maps coordinate points $(x,y)$ directly to their corresponding intensity values o(x,y), while simultaneously updating the PSF parameters. The method convolves the "true" object from the neural network with the estimated PSFs and optimizes the network by minimizing the loss between the synthesized and real short-exposure image burst. This approach enabled the simultaneous estimation of both the degrading PSF and the real high-resolution intensity distribution. We demonstrate the method on synthetic intensity data derived from a radiative magnetohydrodynamics (MHD) simulation, where we applied PSF convolution and noise to obtain a realistic synthetic input data set, similar to observational short-exposure observations. Quantitative comparisons using image quality metrics, histograms, and power spectral analysis confirm that the model can reliably reconstruct the original image from the stack of synthetic short-exposure frames. Finally, we applied our method to high-resolution observations from GREGOR and DKIST and compare to state-of-the-art speckle reconstructions and multi-frame blind deconvolutions. Our results demonstrate the ability to reconstruct small-scale solar features that exceed the reconstruction performance of state-of-the-art reconstruction methods. With this approach, we lay the foundation for future spatially varying PSFs.

Similar Papers
  • Research Article

PiLocNet: physics-informed neural network on 3D localization with a rotating point spread function.

  • Jun 13, 2025
  • Applied optics
  • Mingda Lu +4
  • Research Article

Modeling and Estimation of Adaptive Optics-Corrected long-exposure Point Spread Function Using Gaussian Sum Approximation

  • Nov 15, 2024
  • Monthly Notices of the Royal Astronomical Society
  • Pedro Escárate +6
  • Conference Article

Advancing Multiphase Flow Measurement: Machine Learning Vs. Traditional MPFM in Flow Loop Testing

  • Oct 13, 2025
  • Hao Jin +1
  • Research Article
  • Citations12

Lesion Detection and Interobserver Agreement with Advanced Image Reconstruction for 18F-DCFPyL PET/CT in Patients with Biochemically Recurrent Prostate Cancer.

  • Sep 03, 2019
  • Journal of Nuclear Medicine
  • Bernard H.E Jansen +10
  • Dissertation

3D Concrete Printing Material Prediction and Flow Simulation Using Physics-Informed Neural Network

  • May 01, 2024
  • Tianjie Zhang
  • Research Article
  • Citations10

Model-based restoration and reconstruction for underwater range-gated imaging

  • Nov 01, 2011
  • Optical Engineering
  • Yuzhang Chen
  • Research Article
  • Citations24

Local perturbation responses and checkerboard tests: Characterization tools for nonlinear MRI methods.

  • Jun 03, 2021
  • Magnetic Resonance in Medicine
  • Chin‐Cheng Chan +1
  • Research Article

Rapid Inverse Parameter Inference Using Physics-Informed Neural Networks

  • Aug 09, 2024
  • Electrochemical Society Meeting Abstracts
  • Malik Hassanaly +4
  • Research Article
  • Citations236

A novel sequential method to train physics informed neural networks for Allen Cahn and Cahn Hilliard equations

  • Jan 04, 2022
  • Computer Methods in Applied Mechanics and Engineering
  • Revanth Mattey +1
  • Dissertation

Comparing Parameter Estimation and State Prediction Performance of Physics Informed Neural Networks in Relation to Bayesian Inference

  • Jan 01, 2025
  • Michael Francesco Pantano
  • Research Article
  • Citations1

Physics-informed neural networks based on source term decoupled and its application in discharge plasma simulation

  • Jan 01, 2024
  • Acta Physica Sinica
  • Ze Fang +3
  • Dissertation

Baking physics into deep learning for modeling scientific problems

  • Jan 01, 2021
  • Chengping Rao
  • Research Article
  • Citations28

Identifying optimal architectures of physics-informed neural networks by evolutionary strategy

  • Jul 26, 2023
  • Applied Soft Computing
  • Ana Kaplarević-Mališić +6
  • Conference Article
  • Citations23

Physics Informed Neural Network using Finite Difference Method

  • Oct 09, 2022
  • Kart Leong Lim +2
  • Research Article
  • Citations10

A pair of noisy/blurry patches-based PSF estimation and channel-dependent deblurring

  • Nov 01, 2011
  • IEEE Transactions on Consumer Electronics
  • Chang-Hwan Son +1
Cactus Communications logo

Copyright 2026 Cactus Communications. All rights reserved.