Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D). I. Overview, Magnetohydrodynamic Modeling, and Stokes Profile Synthesis Article Swipe
Kai Yang
,
Lucas A. Tarr
,
M. Rempel
,
S. Curt Dodds
,
Sarah A. Jaeggli
,
Peter Sadowski
,
Thomas A. Schad
,
Ian Cunnyngham
,
Jiayi 嘉奕 Liu 刘
,
Yannik Glaser
,
Xudong Sun
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ad865b
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ad865b
The National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST) will provide high-resolution, multiline spectropolarimetric observations that are poised to revolutionize our understanding of the Sun. Given the massive data volume, novel inference techniques are required to unlock its full potential. Here, we provide an overview of our “SPIn4D” project, which aims to develop deep convolutional neural networks (CNNs) for estimating the physical properties of the solar photosphere from DKIST spectropolarimetric observations. We describe the magnetohydrodynamic (MHD) modeling and the Stokes profile synthesis pipeline that produce the simulated output and input data, respectively. These data will be used to train a set of CNNs that can rapidly infer the four-dimensional MHD state vectors by exploiting the spatiotemporally coherent patterns in the Stokes profile time series. Specifically, our radiative MHD model simulates the small-scale dynamo actions that are prevalent in quiet-Sun and plage regions. Six cases with different mean magnetic fields have been explored; each case covers six solar-hours, totaling 109 TB in data volume. The simulation domain covers at least 25 × 25 × 8 Mm, with 16 × 16 × 12 km spatial resolution, extending from the upper convection zone up to the temperature minimum region. The outputs are stored at a 40 s cadence. We forward model the Stokes profile of two sets of Fe i lines at 630 and 1565 nm, which will be simultaneously observed by DKIST and can better constrain the parameter variations along the line of sight. The MHD model output and the synthetic Stokes profiles are publicly available, with 13.7 TB in the initial release.
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Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/ad865b
- OA Status
- gold
- Cited By
- 5
- References
- 129
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4404701120
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4404701120Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/ad865bDigital Object Identifier
- Title
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Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D). I. Overview, Magnetohydrodynamic Modeling, and Stokes Profile SynthesisWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-11-25Full publication date if available
- Authors
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Kai Yang, Lucas A. Tarr, M. Rempel, S. Curt Dodds, Sarah A. Jaeggli, Peter Sadowski, Thomas A. Schad, Ian Cunnyngham, Jiayi 嘉奕 Liu 刘, Yannik Glaser, Xudong SunList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4357/ad865bPublisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-4357/ad865bDirect OA link when available
- Concepts
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Physics, Magnetohydrodynamics, Photosphere, Helioseismology, Magnetohydrodynamic drive, Astrophysics, Radiative transfer, Solar observatory, Computational physics, Astronomy, Geophysics, Magnetic field, Optics, Spectral line, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
- Cited by
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5Total citation count in OpenAlex
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2025: 4, 2024: 1Per-year citation counts (last 5 years)
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129Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| primary_location.license_id | https://openalex.org/licenses/cc-by |
| primary_location.is_accepted | True |
| primary_location.is_published | True |
| primary_location.raw_source_name | The Astrophysical Journal |
| primary_location.landing_page_url | https://doi.org/10.3847/1538-4357/ad865b |
| publication_date | 2024-11-25 |
| publication_year | 2024 |
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