April 30, 2022 ktindiana Abstract Submission Your Name Affiliation Email Address Cell Phone Poster Title Author List in format Author1 (affiliation), Author2 (affiliation) Scientific Category Please select.. 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; Students please choose Student Poster; use delete button to remove any unwanted tags) Please select.. 2022 Invited Speaker Abstract (no poster) 2022 PSP and SO: Origin and Acceleration of the Solar Wind(s) 2022 Session 01. Do we understand the role of turbulence and diffusion in cosmic ray transport in the heliosphere? 2022 Session 02. Multi-messenger Heliophysics with DKIST 2022 Session 02. Multi-messenger Heliophysics with DKIST, PSP and SO: Origin and Acceleration of the Solar Wind(s) 2022 Session 03. Energy dissipation processes in space plasmas 2022 Session 04. Heliospheric Turbulence I – Interplay of Large-scale Structure with Turbulence 2022 Session 05. Understanding and Quantifying the Performance and Uncertainties in Solar and Heliospheric Models 2022 Session 06. Connecting the Sun and Heliosphere through interdisciplinary coordinated observing campaigns and modeling 2022 Session 07. Data Mining for Science of the Sun-Earth Connection as a Single System 2022 Session 08. Connecting the Heliosphere with the Interstellar Medium 2022 Session 09. SHINE Challenge: SEP Model Validation Community Effort – Forecasting the “Non-event” 2022 Session 10. Machine Learning and Data Assimilation in Heliophysics: Capturing the Current Picture 2022 Session 11. Modeling CME initiation and propagation through the heliosphere 2022 Session 12. Flux Ropes and their Dynamics 2022 Session 13. How can we improve our current understanding of the nature of pre-eruptive configurations and the genesis of solar eruptions? 2022 Session 14. Identifying Science and Instrumentation Gaps in the Coronal – Solar Wind Connection 2022 Session 15. Suprathermal Ions in the Heliosphere and Surrounding Very Local Interstellar Medium 2022 Session 16. Heliospheric Turbulence II: Multiscale Nature of Turbulence from Inertial Scales to Dissipation Range 2022 Session 17. Models and observations for the contributions from SEPs and GCRs to the radiation background in the heliosphere 2022 Session 18. The kinetic physics of collisionless shock waves in the heliosphere 2022 Session 19. Data-driven models of solar flares: where are we and what’s next? 2022 Student Poster 2023 Invited Speaker Abstract (no poster) 2023 Session 01. Where in the solar interior lies the seat of the dynamo? 2023 Session 02. The Structure & Evolution of Active-Region Coronal Currents 2023 Session 03. Solar-stellar eruption analogy: observations and models 2023 Session 04. Multiwavelength diagnostics of the magnetic environment of coronal mass ejections (CMEs) and their precursors 2023 Session 05. Quantification and clustering of different CME initiation methods – numerical and observational analysis 2023 Session 06. Revisiting the Three-Part Structure of Coronal Mass Ejections by Combining the Advanced Remote-sensing and In-situ Observations 2023 Session 07. Multipoint probing of large-scale structures and their impact in the inner heliosphere 2023 Session 08. Understanding the solar wind from its origin to heliosphere through the lens of heavy ion composition 2023 Session 09. Advancing Space Weather Forecasting: Addressing Knowledge Gaps and Leveraging Modern Techniques 2023 Session 10. SHINE SEP Model Validation Challenge: Cross-Model Validation 2023 Session 11. Understanding the role of turbulence and diffusion in SEP and GCR transport in the heliosphere 2023 Session 12. Secondary neutral emission from solar flares to probe energetic particle acceleration 2023 Session 13. Energy release in the lower corona and its connection with the slow solar wind 2023 Session 14. The Kinetic Physics of Energy Conversion in Weakly Collisional Space Plasmas 2023 Session 15. What are the Basic Building Blocks of Solar Wind Turbulence? 2023 Session 16. Multiscale Nature of Heliospheric Turbulence from Inertial Scales to Dissipation Range 2023 Session 17. The Interaction Between the Heliosphere and the Local Interstellar Medium 2023 Session 18. What radio data can do for you! 2023 Session 19. Heliospheric Physics and Neutron Monitors 2023 Session 20. Concepts for Future Solar and Solar Wind Missions 2023 Student Poster 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) Visual Text Upload Poster as PDF, PNG, or JPG (max size 10 MB or 3000x3000 px) Add another file
