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A deep learning framework for instrument-to-instrument translation of solar observation data

comparison between AI-enhanced images and high-quality reference data

Image instabilities and polarization cross-talk

polarization cross-talk

Cutting-edge SPIn4D project combines AI and Astronomy

SPin4D model workflow

A Magnetohydrodynamic Mechanism for the Formation of Solar Polar Vortices

Simulation of an evolving polar vortex

Global and Local Dynamics of X-flare Producing Active Regions During Solar Cycle 25 Peak-Phase

21st February 2024 synoptic map

On the intermittency of hot plasma loops in the solar corona

SDO and DKIS data

Erratum: Analysis of Seeing-Induced Polarization Cross-Talk and Modulation Scheme Performance

Graph of polarimetric errors

A unifying polarization formalism for electric- and magnetic-multipole interactions

Hanle diagrams

Observing the evolution of the Sun’s global coronal magnetic field

Gibson Coronal Activity

Magnetic fields beneath active region coronal loops

Instead heating arises within primarily unipolar fields above the chromosphere.

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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.