Solar Flux Origins, Emergence, and Eruptions | High Altitude Observatory

Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D): II. A Physics-Informed Machine Learning Method for 3D Solar Photosphere Reconstruction

Machine Learning Flowchart

Analysis Of Short-term Solar Activity Variability and Estimating Timings of Next Enhanced Bursts

Zoomed-in burst-envelope forecasts from January 2024 to April 2026

The ASPIICS solar coronagraph aboard the Proba-3 formation flying mission. Scientific objectives and instrument design

Two spacecraft of the Proba-3 mission

MHD simulations of CME with associated prominence eruption

Snapshots of the magnetic field lines & the synthetic SDO/AIA 304 Å images

The Striated Solar Photosphere Observed at 0.″03 Resolution

DKIST-MURaM observations

The role of the Lorentz force in sunspot equilibrium

Scatter plot image

HAO research featured on AAS Nova

Mother’s Day Superstorms

Mother's Day Superstorms: Pre- and Post-storm Evolutionary Patterns of AR 13664/8

Global-scale toroid patterns

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

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

The Yin-Yang Magnetic Flux Eruption (Yin-Yang-MFE) Code: A Global Corona Magnetohydrodynamic Code with the Yin-Yang grid

quasi-steady state solution from a global MHD simulation of the solar wind

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