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A data-driven MHD simulation of the 2011-02-15 coronal mass ejection from Active Region NOAA 11158

MHD simulation of the 2011-02-15 coronal mass ejection (CME)

Comprehensive analysis of a filament-embedding solar active region at different stages of evolution

NVST and CHASE observations, Feb 14

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

A Comprehensive Radiative Magnetohydrodynamics Simulation of Active Region Scale Flux Emergence from the Convection Zone to the Corona

Coronal dimming

Eruption of a Magnetic Flux Rope in a Comprehensive Radiative Magnetohydrodynamic Simulation of flare-productive active regions

Synthetic AIA

An improved MHD simulation of the 2006 December 13 coronal mass ejection of active region NOAA 10930

MHD simulation of the 2006 December 13 coronal mass ejection

Synthetic Lyman-α Emissions for the coronagraph aboard the ASO-S mission I: an Eruptive Prominence-cavity System

Lyman-alpha emission

Coronal Cavities in CoMP Observations

Cavity widths observed by SDO/AIA

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.