Credit: CC0 Public Domain

Researchers from the Yunnan Observatories of the Chinese Academy of Sciences and Southwest Forestry University have developed an advanced neural network-based method to improve the compression of spectral data from the New Vacuum Solar Telescope (NVST).

Published in , this technique addresses challenges in data storage and transmission for high-resolution solar observations.

The NVST produces vast amounts of spectral data, creating significant storage and transmission burdens. Traditional compression techniques, such as (PCA), achieved modest compression ratios (~30) but often introduced distortions in reconstructed data, limiting their utility.

To overcome these limitations, the researchers implemented a using a Convolutional Variational Autoencoder (VAE) for compressing Ca II (8542 Ã…) spectral data.

Their method achieves a compression ratio of up to 107 while preserving . Crucially, the decompressed data maintains errors within the inherent noise level of the original observations, ensuring scientific reliability. At the highest compression ratio, Doppler velocity errors remain below 5 km/s—a threshold critical for accurate solar physics analysis.

This breakthrough enables more efficient NVST data transmission and sharing while providing a scalable solution for other solar observatories facing similar challenges. Enhanced facilitates broader scientific collaboration and reduces infrastructure constraints.

More information: Yan Dong et al, Neural-Based Compression for the Spectral Data of the New Vacuum Solar Telescope, Solar Âé¶¹ÒùÔºics (2025).

Journal information: Solar Âé¶¹ÒùÔºics