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4 papers

astro-ph.SR2026

Probing the Physics of the Solar Corona with High-Resolution Observations using SKA-Mid

Mark C. M. Cheung, John S. Morgan, Rohit Sharma +3

The paper evaluates how the SKA-Mid radio telescope can be used to observe fine‑scale structures and plasma processes in the solar corona by synthesizing radio emission from radiat…

astro-ph.SR2026

Measuring the Coronal Magnetic Field with 2D Coronal Seismology: A Forward-Modeling Validation

Zihao Yang, Sarah Gibson, Matthias Rempel +1

In recent years, a two-dimensional (2D) coronal seismology technique applied to spectral-imaging data from the Coronal Multi-channel Polarimeter (CoMP) and UCoMP has enabled routin…

astro-ph.SR2025

Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D): II. A Physics-Informed Machine Learning Method for 3D Solar Photosphere Reconstruction

Kai E. Yang, Xudong Sun, Lucas A. Tarr +9

Inferring the three-dimensional (3D) solar atmospheric structures from observations is a critical task for advancing our understanding of the magnetic fields and electric currents…

astro-ph.SR2025

Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D): I. Overview, Magnetohydrodynamic Modeling, and Stokes Profile Synthesis

Kai E. Yang, Lucas A. Tarr, Matthias Rempel +8

The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will provide high-resolution, multi-line spectropolarimetric observations that are poised to revolutioniz…