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The improvements to the next-gen TIEGCM

Probing dynamic solar wind and realistic CME model with Icarus model and PUNCH observations

Probing the solar corona with the Solar Orbiter/Metis coronagraph: from instrumentation to CME diagnostics

Stellar Evidence of a Collapsing Solar Dynamo

Coordinated Multi-Instrument Diagnostics of the 2024 April Total Solar Eclipse: Enhanced Low-Corona Plasma Properties from DKIST Cryo-NIRSP, MLSO UCoMP, K-Cor, Hinode EIS, SDO AIA Observations, and Global Models

Satellite Drag and Sustainable Space Operations in a Dynamic Thermosphere

The NASA SWORD Space Weather Center of Excellence: a template for modern space weather research

Solar prominences in 2026: magnetic support, multiphase plasma, and the state of the art

Predictive EUV Signatures: Leveraging Coronal Dimmings and Flare Precursors for Advanced Space Weather Forecasting

Image reconstruction methods for high-resolution ground-based solar observations with deep learning

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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.