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 |