SPIN4D Data Release 1
Data and Resources
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SPIN4D-DR1 HTTPother
Web (HTTP) access to the SPIND4D-DR1 dataset
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SPIN4D-DR1 OSDFother
OSDF/Pelican access to the SPIN4D-DR1 dataset
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SPIN4D-DR1 Globusother
Globus access to the SPIN4D-DR1 dataset
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SPIN4D-DR1 Data Exploration Jupyter Notebookgithub
Jupyter notebook tutorial for accessing and exploring the SPIN4D-DR1 dataset
| Field | Value |
|---|---|
| data size | 13 TB |
| other extra information about data | Project website: https://ifauh.github.io/SPIN4D/ |
| point of contact phone number | 8089567613 |
| Groups |
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| Tags |
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| author | Stanley Curtis Dodds |
| author_email | dodds@hawaii.edu |
| isopen | False |
| metadata_created | 2026-10-30T17:28:59.639123 |
| metadata_modified | 2026-10-30T17:28:59.639128 |
| notes | This is the Critical Early DKIST Science: Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIN4D) "Data Release 1" (SPIN4D-DR1). This dataset is a 13TB subset of 109TB of simulations that accompanied our first paper (DOI 10.3847/1538-4357/ad865b). We performed simulations of the small-scale dynamo actions that are prevalent in quiet-Sun and plage regions using Rempel's 2014 version of the Max-Planck University-of-Chicago Radiative MHD code (MURaM). Six simulation cases with different mean magnetic fields were conducted. These are: SPIN4D_SSD, SPIN4D_SSD_100G, SPIN4D_SSD_200G, SPIN4D_SSD_50G, SPIN4D_SSD_50G_V, SPIN4D_SSD_Large. Each case covers six solar-hours with output snapshots stored at a 40s cadence. For each case we forward model the Stokes profiles for two sets of Fe I lines at 630 and 1565 nm for snapshots at 12 minute intervals with two opposite magnetic field orientations due to the inherent LOS ambiguity. |
| num_resources | 4 |
| num_tags | 7 |
| title | SPIN4D Data Release 1 |
| version | DR1 |