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Physically Motivated Deep Learning to Superresolve and Cross Calibrate Solar Magnetograms

Abstract:
Superresolution (SR) aims to increase the resolution of images by recovering detail. Compared to standard interpolation, deep learning-based approaches learn features and their relationships to leverage prior knowledge of what low-resolution patterns look like in higher resolution. Deep neural networks can also perform image cross-calibration by learning the systematic properties of the target images. While SR for natural images aims to create perceptually convincing results, SR of scientific data requires careful quantitative evaluation. In this work, we demonstrate that deep learning can increase the resolution and calibrate solar imagers belonging to different instrumental generations. We convert solar magnetic field images taken by the Michelson Doppler Imager (resolution ∼2″ pixel−1; space based) and the Global Oscillation Network Group (resolution ∼2.″5 pixel−1; ground based) to the characteristics of the Helioseismic and Magnetic Imager (resolution ∼0.″5 pixel−1; space based). We also establish a set of performance measurements to benchmark deep-learning-based SR and calibration for scientific applications
Publication status:
Published
Peer review status:
Peer reviewed

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Files:
Publisher copy:
10.3847/1538-4365/ad12c2
Publication website:
https://ir.cwi.nl/pub/34111/34111.pdf

Authors

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Role:
Author
ORCID:
0000-0002-4716-0840
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0002-9888-6262
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Role:
Author
ORCID:
0000-0002-6648-0225
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Role:
Author
ORCID:
0000-0001-9021-611X
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Role:
Author
ORCID:
0000-0002-3689-6959


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal: Supplement Series More from this journal
Volume:
271
Issue:
2
Pages:
46-46
Publication date:
2024-03-26
DOI:
EISSN:
1538-4365
ISSN:
0067-0049


Language:
English
Keywords:
Pubs id:
1980100
Local pid:
pubs:1980100
Source identifiers:
W4393201222
Deposit date:
2026-06-10
ARK identifier:
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