June 1, 2024 ktindiana Abstract Submission 2024 Your Name Affiliation Email Address Cell Phone Poster Title Author List in format Author1 (affiliation), Author2 (affiliation) INCLUDING FIRST AUTHOR Post Category 2024 Other 2024 WG1: Solar (including interior) and coronal 2024 WG2: Interplanetary 2024 WG3: Solar energetic particles (including suprathermal and GCR) 2024 WG4: Microphysics (reconnection, turbulence, etc) Tags (select all relevant options; use delete button to remove any unwanted tags) Please select.. 2024 Invited Speaker Abstract (no poster) 2024 Session 1. Exploring the Solar and Stellar Connection: Investigating Solar and Stellar Winds in Relation to Magnetic Fields and Eruptions 2024 Session 10. Seeing the Unseen: Sun in radio wavelengths 2024 Session 11. Neutron Monitors and GLEs—The Big Picture 2024 Session 12. Particle Acceleration in Solar Flares and at CME-driven Shocks: Their Interconnection in Producing SEPs and Gamma-rays 2024 Session 13. Solar Energetic Particle (SEP) acceleration near the Sun 2024 Session 14. Understanding the role of turbulence and diffusion in SEP transport in the inner heliosphere 2024 Session 15. Machine learning-based predictions of solar flares and SEP events 2024 Session 16. The role of the Helicity Barrier: Impact on Solar Wind Imbalanced Turbulence and Heating 2024 Session 17. Making Cross-Heliospheric and Cross-Scale Connections with Global Modeling and Observations 2024 Session 18. Multiscale Nature of Plasma Turbulence from Inertial Scales to Dissipation Range 2024 Session 19. Unraveling Turbulence Dynamics in the Very Local Interstellar Medium (VLISM) and the Connection with Heliophysics 2024 Session 2. Understanding Variations in Sun's Global Flows 2024 Session 20. The Things I Wish the Community Would Stop Getting Wrong: Facilitating Knowledge Dissemination (Town Hall) 2024 Session 21. Small Missions Big Results 2024 Session 22. Pickup Ions in the Heliosphere and Beyond 2024 Session 3. Small-scale magnetism and dynamics in the lower solar atmosphere 2024 Session 4. Beyond the Standard Flare Model 2024 Session 5. Flare- & CME-Associated Evolution of Active-Region Coronal Currents 2024 Session 6. Modern approaches to investigate larger scale structures in the heliosphere 2024 Session 7. Achieving coronal and solar wind science closure with multi-mission collaboration 2024 Session 8. Unifying the Physical Understanding of CMEs through Remote Sensing and In-Situ Observations in the PSP/SolO Era 2024 Session 9. Addressing your SHINE Science Questions with Radio Data 2024 Student Poster Abstract (minimum of 50 characters), text only with no media (upload poster and images below) Visual Text Upload Poster as PDF, PNG, or JPG (max size 10 MB or 3000x3000 px) Add another file
