2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events Archives

June 14, 2026 Mari Paz Miralles

Solar SMA: A New Solar Surveyor of the Sun

Authors: Mari Paz Miralles, Garrett Keating, Katharine Reeves, Chad Madsen, Mark Gurwell (Center for Astrophysics | Harvard & Smithsonian) The Solar Submillimeter Array (Solar SMA)View More

2026 Session 01. CHSKP at 50 years: Towards a Next-Generation 3D Solar Flare Model 2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events 2026 Session 05. The Era of Large-N Radio Arrays: Democratizing SHINE Science with Next-Generation Radio Interferometers 2026 Session 17. Coronal Heating and Acceleration near the Sun: What Have We Learned and What Remains to Reach Closure?

June 6, 2026 C. R. Gilly

PUNCH in Place: Variations on Multi-Observatory Composites

Authors: C. Gilly (NWRA) The PUNCH mission images the young solar wind across a field of view that spans several orders of magnitude in heliocentricView More

2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events 2026 Session 03. The Hidden Region of CME Evolution: What Are We Still Missing?2026 Session 06. The Multi-Source Origin of the Solar Wind in a Global Magnetic Context 2026 Session 07. New Insights and New Unknowns in the Coupled Corona-Heliosphere System 2026 Session 08. The Evolution of Solar Magnetic Open Flux and Its Implications for the Solar Cycle 2026 Session 11. Evolution of Large-Scale Solar Structures in the Inner Heliosphere: Space Weather at Earth and Mars 2026 Session 17. Coronal Heating and Acceleration near the Sun: What Have We Learned and What Remains to Reach Closure?

June 6, 2026 yfan@ucar.edu

MHD simulations of a prominence-forming coronal flux rope and its observational signatures

Authors: Yuhong Fan (HAO/NSF NCAR) We present magnetohydrodynamic simulations of the evolution of a prominence-forming coronal flux rope from quasi-equilibrium to eruption beneath a coronalView More

2026 WG1: Solar (including interior) and coronal

2026 Invited Speaker Abstract (No Poster)2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events

June 6, 2026 bin.chen@njit.edu

Solar Radio Observing Capabilities at the Owens Valley Radio Observatory: Status Update

Authors: Bin Chen (NJIT), Sijie Yu (NJIT), Peijin Zhang (NJIT), Owen Giersch (NJIT), Caius Selhorst (NJIT), Yuqian Wei (NJIT), Jonas Flygare (Caltech), Meiqi Wang (NJIT),View More

2026 Session 01. CHSKP at 50 years: Towards a Next-Generation 3D Solar Flare Model 2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events 2026 Session 03. The Hidden Region of CME Evolution: What Are We Still Missing?2026 Session 05. The Era of Large-N Radio Arrays: Democratizing SHINE Science with Next-Generation Radio Interferometers 2026 Session 06. The Multi-Source Origin of the Solar Wind in a Global Magnetic Context 2026 Session 12. Recent Extreme Particle Events and SHINE Mini-Challenge 2026 Session 14. Shock Waves and Energetic Particles Across the Heliosphere: Evolution of Structure and Processes from the Sun to the Outer Heliosphere 2026 Session 17. Coronal Heating and Acceleration near the Sun: What Have We Learned and What Remains to Reach Closure?

June 5, 2026 andres.munoz@swri.org

The VOCAL Framework: Conceptual Vocabulary as the Binding Constraint on Human-AI Collaboration Quality

Authors: Andres Munoz-Jaramillo (Southwest Research Institute), Isabel Tejada-Sanchez (Universidad de los Andes), Phoebe Mahlin (Universidad de California – Berkeley), Claudia Holland (Universidad de California –View More

2026 Session 01. CHSKP at 50 years: Towards a Next-Generation 3D Solar Flare Model 2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events 2026 Session 03. The Hidden Region of CME Evolution: What Are We Still Missing?2026 Session 04. Flux Emergence from the Deep Interior Through the Solar Atmosphere 2026 Session 05. The Era of Large-N Radio Arrays: Democratizing SHINE Science with Next-Generation Radio Interferometers 2026 Session 06. The Multi-Source Origin of the Solar Wind in a Global Magnetic Context 2026 Session 07. New Insights and New Unknowns in the Coupled Corona-Heliosphere System 2026 Session 08. The Evolution of Solar Magnetic Open Flux and Its Implications for the Solar Cycle 2026 Session 09. Understanding Complex CME Interactions as drivers of Extreme Space Weather 2026 Session 10. Data-driven Time-Dependent Inner Heliospheric Modeling: Methods and Uncertainties 2026 Session 11. Evolution of Large-Scale Solar Structures in the Inner Heliosphere: Space Weather at Earth and Mars 2026 Session 12. Recent Extreme Particle Events and SHINE Mini-Challenge 2026 Session 13. Dynamics of Particle Populations Throughout the Inner Heliosphere 2026 Session 14. Shock Waves and Energetic Particles Across the Heliosphere: Evolution of Structure and Processes from the Sun to the Outer Heliosphere 2026 Session 15. How is Machine Learning helping us improve space weather prediction?2026 Session 16. The Grand SEP Debate – Flares shocks drift cross-field and all that 2026 Session 17. Coronal Heating and Acceleration near the Sun: What Have We Learned and What Remains to Reach Closure?2026 Session 18. Routes to Dissipation in the Near-Sun Solar Wind 2026 Session 19. Solar Wind Turbulence Across Scales: From MHD to Kinetic Physics

June 5, 2026 Don Kolinski

We’re back! What’s new at the Mauna Loa Solar Observatory

Authors: Don Kolinski (HAO / NFS NCAR), Tom Berger (HAO / NFS NCAR), Ben Berkey (HAO / NFS NCAR), Joan Burkepile (HAO / NFS NCAR),View More

2026 WG1: Solar (including interior) and coronal

2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events 2026 Session 03. The Hidden Region of CME Evolution: What Are We Still Missing?2026 Session 09. Understanding Complex CME Interactions as drivers of Extreme Space Weather

June 1, 2026 ewraback@ucar.edu

Coronal Cavity Magnetic Fields Inferred by DKIST/CryoNIRSP

Authors: Elizabeth Wraback (HAO/NSF NCAR), Samaiyah Faird (Alabama A&M University), Thomas Schad (NSO), Urszula Bak-Steslicka (University of Wroclaw), Giuliana de Toma (HAO/NSF NCAR), Yuhong FanView More

2026 WG1: Solar (including interior) and coronal

2026 Session 02. Coronal Cavities and Their Implications for Eruptive Events