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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

Evaluating F10.7 and F30 radio fluxes as long-term solar proxies of energy deposition in the thermosphere

Averaged mass density

Holly Gilbert awarded the 2025 Irene González Hernández Prize

Holly Gilbert portrait from SPD announcement

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

Magnetic Field Evolution of the Solar Active Region 13664

Magnetic field configuration and parameters

Spectra of solar shallow-water waves from bright point observations

Hovmoller (time × longitude) diagram at 30◦ latitudes

Evolution Of Amplitude And Longitude Phase Of Tachocline Rossby Waves Diffusing To The Photosphere

Rosby Wave penetration

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

21st February 2024 synoptic map

A Study on the Nested Rings CME Structure Observed by the WISPR Imager Onboard Parker Solar Probe

CME analysis

Pagination

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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.