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Tags
- 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
Events
Tags
- 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