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Steadiness of coronal heating

Solar Orbiter EUI revelations

Deciphering Pre-solar-storm Features Of September-2017 Storm From Global And Local Dynamics

Evolution of the magnetic fields (left) and helicity density (right) for AR 12673

The Sun's Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)

Magnetic Reconnection

Recent Progress on Understanding Coronal Mass Ejection / Flare Onset by a NASA Living with a Star Focused Science Team

Results from a data-driven MHD simulation

Comprehensive Radiative MHD Simulations of Eruptive Flares above Collisional Polarity Inversion Lines

Erupting magnetic flux rope

Hybrid data-driven magnetofrictional and magnetohydrodynamic simulations of an eruptive solar active region

Ribbon evolution

Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code

Ground Truth and Data Driven simulations

A Mosaic of the inner heliosphere:

McIntosh style coronal hole maps

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.