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.. 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; 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 2025 Invited Speaker Abstract (no poster) 2025 Session 01. Entropy and its role in space plasmas 2025 Session 02. Turbulence reconnection shock and particle energization 2025 Session 03. New insights into particle access and transport in the inner heliosphere 2025 Session 04. Pickup ions electrons and energetic neutral atoms in the heliosphere and local interstellar medium 2025 Session 05. What are the radiation risks from SEPs for humans in space 2025 Session 06. Multispacecraft new era: novel multipoint & multiscale techniques 2025 Session 07. What we know about the solar Alfvén surface in the era of “Touching the Sun” 2025 Session 08. Micro- Meso- and Macro-: Relating the Full Spectrum of Scale Sizes in Remote-Sensing Imaging and Coronal/Heliospheric Models 2025 Session 09. Moving Towards a Unified Perspective on Coronal Hole Boundaries 2025 Session 10. Revisiting Interacting Coronal Mass Ejections: Understanding Evolution and Associated Predictive Challenges 2025 Session 11. Enhancing CME modeling in the new solar missions era: Current challenges and future directions 2025 Session 12. Intertwining Physics-Based Simulations and Machine Learning in Heliophysics: How Can We Do It and Why Do We Need It? 2025 Session 13. Advancing Our Global Understanding of CMEs from In Situ and Remote Observations and Models 2025 Session 14. Secondary neutral emission from solar flares to probe energetic particle acceleration 2025 Session 15. Modern approaches in particle kinetics: bridging observations reconstructions and simulations throughout the heliosphere 2025 Session 16. SHINE Science with FASR and Next-Generation Radio Arrays 2025 Session 18. Far-side of the Sun: Observation Modeling and Application to Space-Weather 2025 Session 19. The Structure & Evolution of Coronal Currents in CME Source Regions 2025 Session 20. Neutron Monitors and Space Weather 2025 Session 21. [TOWN HALL] Instrumentation Necessary for a Future LWS Solar Polar Orbiter Mission 2025 Student Poster 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 jobs permanent positions sounding rockets Abstract (minimum of 50 characters) Visual Code Upload Poster as PDF, PNG, or JPG (max size 10 MB or 3000x3000 px) Add another file
