The AGU annual meeting will take place from 15 – 19 December 2025 in New Orleans, Louisiana.
Here is a list of all Solar and Heliospheric Physics sessions:
- SH001 – Across the Heliospheric Boundaries and Regions: In-situ Observations and Modeling as Tools for Probing the Outer Heliosphere
- SH002 – Advances in Understanding the Innermost Heliosphere
- SH003 – Beyond the Sun-Earth Line: Solar Orbiter, VIGIL, and Future Solar Polar Missions
- SH004 – Collisionless Shocks in Heliospheric and Astrophysical Plasmas and their Effects on Planetary Magnetospheres
- SH005 – Development and use cases of reusable Artificial Intelligence infrastructure in Heliophysics
- SH006 – Exploring the Connections between the Sun, Outer Heliosphere, and Local Interstellar Medium Including First-Light Results from NASA’s IMAP Mission
- SH007 – Exploring Space Weather Impacts Throughout the Heliosphere using Advanced Energetic Particle and Dosimetry Instrumentation
- SH008 – Exploring the engineering challenges facing space flight missions in heliophysics, translating recent anecdotes to lessons learned, and providing discussion on the strategies and best practices improve future space flight experiments
- SH009 – From Initiation to Impact: Understanding CMEs as Drivers of Space Weather
- SH010 – Fundamental Mechanisms in Highly Collisionless Plasmas: Wave-Particle Interactions, Turbulence, Structures, and Instabilities with Applications to Heliospheric, Magnetospheric, and Laboratory Plasma Physics
- SH011 – Fundamental Physics of the Solar Corona and Inner Heliosphere
- SH012 – Galactic Cosmic Ray Transport in the Heliosphere: From the Interstellar Medium to the Solar Atmosphere
- SH013 – High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond
- SH014 – Interior Dynamics to Surface Magnetism: Probing the Full Sun with Observations from the Sun-Earth Line Augmented with New Data from the Poles, the Far Side, and Other Vantage Points
- SH015 – Intermittent Structures and Wave Modes in Plasmas: From Turbulent Dynamics to Particle Transport
- SH016 – Monitoring and Forecasting Space and Terrestrial Weather with Ground-Based Measurements of Cosmic Rays
- SH017 – Multiscale Description of Solar Wind Dynamics: Quasilinear Theory, Simulations, and Observations
- SH018 – MULTISCALE processes in planetary, space and astrophysics: turbulence, magnetic reconnection, and shocks
- SH019 – Observations and modeling of turbulence in the solar photosphere, chromosphere,and low corona
- SH020 – Prediction of Solar Transient Events: Data-Driven, Physics-Based, and Hybrid Approaches
- SH021 – Radio Observations of Plasma Dynamics from Sun to Earth
- SH022 – Radio Solar and Heliospheric Observations, Instruments, and Modelling for Space Weather Research, Applications, and Forecasting
- SH023 – Revealing the structure of the corona and the young solar wind: new imaging capabilities
- SH024 – SOHO: Thirty Years of Solar and Heliospheric Science
- SH025 – Solar and Heliospheric Physics: General Contributions
- SH026 – Solar Energetic Particles in the Inner Heliosphere and Beyond
- SH027 – Solar Flare Particle Acceleration: Observations, Models, and Multi-mission Synergies
- SH028 – Solar Flares in the High-Resolution, High-Cadence Era: Observations, Modelling and future prospects
- SH029 – Solar Orbiter: Solar-Heliospheric Connections and First Out-of-the-Ecliptic Observations
- SH030 – Space and Heliophysics Science Undergraduate and Graduate Education Resources
- SH031 – The Future of the International Sunspot Number
- SH032 – The Long March: Heliosphere Modeling with Operations in Mind
- SH033 – The role of low-latency data for space weather and future human exploration
- SH034 – Toward a Unified Understanding of Particle Acceleration and Transport throughout the Heliosphere
- SH035 – Turbulence, magnetic reconnection, and non-thermal particles in space plasmas
- SH036 – Understanding Space Weather for Human and Robotic Exploration to the Moon, Mars, and Beyond
- SH037 – Velocity Distributions and Kinetic Wave Activity in Space Plasma: Theory, Simulation, and Machine Learning
- SH038 – Why We Need to Keep Funding Space-Weather Research!
- SM007 – From the Sun to the Earth: Exploring The Impacts of Plasma Waves and Instabilities on Solar-Terrestrial Interactions
- SM023 – Physics of Current Sheets in Planetary Magnetospheres and Solar Wind: Plasma Kinetics, Magnetic Reconnection, and Particle Acceleration
See also the Space Policy and Advocacy session.
Abstract Submission before July 30st, 2025 on the abstract submission website.