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Energetic Electron Precipitation into Earth’s Upper Atmosphere by Plasma Waves: The Role of Nonlinear Interactions

Neural Enhancement of the Traditional WSA Solar Wind Relation

What is that? Observing in the Sun’s corona at 63 kilometers resolution…

Introduction to Surya: A Foundation Model in Heliophysics

Flashes, Flares, and Aftershocks: Uncovering Unique Solar Flare Signatures with the Dunn Solar Telescope

Invert Everything Everywhere All at Once

Multiscale features in ICMEs and CIRs and Their Space Weather Implications

The magnetic origin of the solar wind and CMEs

Helicity turbulence model: Validations and application to stellar angular-momentum transport

Inter-hemispheric asymmetry in the high-latitude electrodynamics and its impact on the coupled magnetosphere-ionosphere-thermosphere

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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.