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Cutting-edge SPIn4D project combines AI and Astronomy

SPin4D model workflow

Magnetic Field Evolution of the Solar Active Region 13664

Magnetic field configuration and parameters

Annular Eclipse Expedition at Hovenweep

Cool effect when trying to capture the eclipse through the telescope.

Comprehensive Radiative MHD Simulations of Eruptive Flares above Collisional Polarity Inversion Lines

Rempel model image of Sunspots, publication highlighted by NOVA

Comprehensive Radiative MHD Simulations of Eruptive Flares above Collisional Polarity Inversion Lines

Erupting magnetic flux rope

Small-scale dynamos: From idealized models to solar and stellar applications

Comparison of Bz at optical depth

A Comprehensive Radiative Magnetohydrodynamics Simulation of Active Region Scale Flux Emergence from the Convection Zone to the Corona

Coronal dimming

Eruption of a Magnetic Flux Rope in a Comprehensive Radiative Magnetohydrodynamic Simulation of flare-productive active regions

Synthetic AIA

Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code

Ground Truth and Data Driven simulations

Limitations and biases in the retrieval of the polar magnetic field I: the role of the magnetic filling factor in Milne-Eddington inversions of simulated Hinode/SP data

synthetic spectra continuum

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This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.