April 12, 2025 ktindiana Abstract Submission 2025 Your Name Affiliation Email Address Cell Phone Poster Title Author List in format Author1 (affiliation), Author2 (affiliation) INCLUDING FIRST AUTHOR Post Category 2026 Other 2026 WG1: Solar (including interior) and coronal 2026 WG2: Interplanetary 2026 WG3: Solar energetic particles (including suprathermal and GCR) 2026 WG4: Microphysics (reconnection, turbulence, etc) Tags (select all relevant options; use delete button to remove any unwanted tags) Please select.. 2026 Invited Speaker Abstract (No Poster) 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 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 2026 Student Poster Abstract (minimum of 50 characters), text only with no media (upload poster and images below) Visual Code Upload Poster as PDF, PNG, or JPG (max size 10 MB or 3000x3000 px) Add another file
