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Neural-Based Compression Scheme for Solar Image DataStudying the solar system and especially the Sun relies on the data gathered daily from space missions. These missions are data-intensive and compressing this data to make them efficiently transferable to the ground station is a twofold decision to make. Stronger compression methods, by distorting the data, can increase data throughput at the cost of accuracy which could affect scientific analysis of the data. On the other hand, preserving subtle details in the compressed data requires a high amount of data to be transferred, reducing the desired gains from compression. In this work, we propose a neural network-based lossy compression method to be used in NASA’s data-intensive imagery missions. We chose NASA’s Solar Dynamics Observatory (SDO) mission which transmits 1.4 terabytes of data each day as a proof of concept for the proposed algorithm. In this work, we propose an adversarially trained neural network, equipped with local and non-local attention modules to capture both the local and global structure of the image resulting in a better trade-off in rate-distortion (RD) compared to conventional hand-engineered codecs. The RD variational autoencoder used in this work is jointly trained with a channel-dependent entropy model as a shared prior between the analysis and synthesis transforms to make the entropy coding of the latent code more effective. We also studied how optimizing perceptual losses could help our neural compressor to preserve high-frequency details of the data in the reconstructed compressed image. Our neural image compression algorithm outperforms currently-in-use and state-of-the-art codecs such as JPEG and JPEG-2000 in terms of the RD performance when compressing extreme-ultraviolet (EUV) data. As a proof of concept for use of this algorithm in SDO data analysis, we have performed coronal hole (CH) detection using our compressed images, and generated consistent segmentations, even at a compression rate of ∼ 0.1 bits per pixel (compared to 8 bits per pixel on the original data) using EUV data from SDO.
Document ID
20240002437
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Ali Zafari ORCID
(West Virginia University Morgantown, West Virginia, United States)
Atefeh Khoshkhahtinat ORCID
(West Virginia University Morgantown, West Virginia, United States)
Jeremy A Grajeda ORCID
(New Mexico State University Las Cruces, United States)
Piyush M Mehta ORCID
(West Virginia University Morgantown, West Virginia, United States)
Nasser M Nasrabadi ORCID
(West Virginia University Morgantown, West Virginia, United States)
Laura E Boucheron ORCID
(New Mexico State University Las Cruces, United States)
Barbara J Thompson ORCID
(Goddard Space Flight Center Greenbelt, United States)
Michael S F Kirk
(Goddard Space Flight Center Greenbelt, United States)
Daniel E da Silva ORCID
(University of Maryland, Baltimore County Baltimore, Maryland, United States)
Date Acquired
February 26, 2024
Publication Date
November 13, 2023
Publication Information
Publication: IEEE Transactions on Aerospace and Electronic Systems
Publisher: Institute of Electrical and Electronics Engineers
Volume: 60
Issue: 1
Issue Publication Date: February 1, 2024
ISSN: 0018-9251
e-ISSN: 1557-9603
Subject Category
Solar Physics
Computer Operations and Hardware
Funding Number(s)
WBS: 936723.02.35.01.01.01
CONTRACT_GRANT: 80NSSC21M0180
CONTRACT_GRANT: 80NSSC21M0322
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
External Peer Committee
Keywords
Image coding
Training
Transforms
Vector quantization
NASA
Entropy
Codecs
Attention-based networks
Coronal hole (SH) segmentation
Generative adversarial network (GAN)
Learned lossy image compression
Solar Dynamics Observatory (SDO)
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