Photography is the cornerstone of modern astronomical and space research. However, most astronomical images captured by ground-based telescopes suffer from atmospheric turbulence, resulting in degraded imaging quality. While multi-frame strategies like lucky imaging can mitigate some effects, they involve intensive data acquisition and complex manual processing. In this paper, we propose AstroDiff, a generative restoration method that leverages both the high-quality generative priors and restoration capabilities of diffusion models to mitigate atmospheric turbulence. Extensive experiments demonstrate that AstroDiff outperforms existing state-of-the-art learning-based methods in astronomical image turbulence mitigation, providing higher perceptual quality and better structural fidelity under severe turbulence conditions.
Our training process is divided into two stages. In the first stage, we perform extensive pre-training separately for the generative prior branch and the restoration branch. In the second stage, we jointly combine these two models through a fusion module using Stochastic Gradient Langevin Dynamics inference.
AstroDiff's performance comparison against 3 state-of-the-art turbulence mitigation models (DATUM, TMT, ESTRNN) on planetary images with strong synthetic turbulence
Moon - AstroDiff
Moon - DATUM
Moon - TMT
Moon - ESTRNN
Mercury - AstroDiff
Mercury - DATUM
Mercury - TMT
Mercury - ESTRNN
Jupiter - AstroDiff
Jupiter - DATUM
Jupiter - TMT
Jupiter - ESTRNN
Slide to compare the original and enhanced images of celestial bodies. Our method significantly improves the image quality while preserving important details.
Jupiter collected by ZWOASI224MC
Venus collected by QHY5LII-C
Saturn collected by Skywatcher
Jupiter collected by ZWOASI462MC
Saturn collected by Hubble
Mars collected by iphone 12
Images BRISQUE ↓ | |
---|---|
Original Images | 95.64 |
Enhanced Images | 22.78 |