TY - JOUR
T1 - Revealing real-world hidden 3D atmospheric turbulence from imaging
AU - An, Yitong
AU - Jiang, Xingbo
AU - Li, Tongkai
AU - Bai, Xiangzhi
N1 - Publisher Copyright:
© 2025 The Authors
PY - 2026/5/4
Y1 - 2026/5/4
N2 - Learning the 3D structure of atmospheric turbulence poses challenges due to randomness, complex dynamics, and spatiotemporal coupling. We propose a turbulence effects-induced probing and evolutionary framework (TEPEF) that leverages optical degradation in multi-view images to learn real-world 3D turbulence. Trained on a large-scale dataset of 131,240 sequences (2,327,540 frames) and enhanced by a semi-supervised strategy, TEPEF estimates the refractive index structure constant (Cn2), a key measure of turbulence strength. TEPEF demonstrates high accuracy in quantifying atmospheric turbulence, achieving excellent agreement between predictions and ground truth for both probing and evolution tasks and substantially outperforming existing methods. When applied to predicting atmospheric coherence length and “seeing,” TEPEF achieves results with errors below 3%, offering a precise and cost-effective approach to astronomical site selection. These results highlight the promise of deep learning from turbulence-induced imaging for advancing atmospheric turbulence research.
AB - Learning the 3D structure of atmospheric turbulence poses challenges due to randomness, complex dynamics, and spatiotemporal coupling. We propose a turbulence effects-induced probing and evolutionary framework (TEPEF) that leverages optical degradation in multi-view images to learn real-world 3D turbulence. Trained on a large-scale dataset of 131,240 sequences (2,327,540 frames) and enhanced by a semi-supervised strategy, TEPEF estimates the refractive index structure constant (Cn2), a key measure of turbulence strength. TEPEF demonstrates high accuracy in quantifying atmospheric turbulence, achieving excellent agreement between predictions and ground truth for both probing and evolution tasks and substantially outperforming existing methods. When applied to predicting atmospheric coherence length and “seeing,” TEPEF achieves results with errors below 3%, offering a precise and cost-effective approach to astronomical site selection. These results highlight the promise of deep learning from turbulence-induced imaging for advancing atmospheric turbulence research.
KW - 3D field probing and evolution prediction
KW - C
KW - atmospheric turbulence
KW - multi-view imaging
KW - refractive index structure constant
KW - semi-supervised learning
KW - turbulence effects-induced deep learning framework
UR - https://www.scopus.com/pages/publications/105027104824
U2 - 10.1016/j.newton.2025.100364
DO - 10.1016/j.newton.2025.100364
M3 - 文章
AN - SCOPUS:105027104824
SN - 2950-6360
VL - 2
JO - Newton
JF - Newton
IS - 5
M1 - 100364
ER -