The upcoming annual meeting will only be held in-person. There will be a scientific conference as well as an exhibition. Additionally, there will be a general assembly, a general election for the 2026-2028 office bearers, along with the presentation of the usual annual society honours and awards.
Abstract deadline: 18 Feb 2025
The eight geoscience disciplines of the society—Atmospheric (AS), Biogeoscience (BG), Hydrological (HS) Interdisciplinary (IG), Ocean (OS), Planetary (PS), Solar & Terrestrial (ST), and Solid Earth (SE) —are the focus of the annual meeting, which is open to scientists, researchers, and practitioners in these fields.
All ST sessions:
- ST01: Particle Acceleration and Transport at the Sun and in the Heliosphere
- ST02: Advance the Understanding of the Atmosphere, Ionosphere, and Magnetosphere
- ST03: Multiscale Solar-wind-magnetosphere Interactions
- ST07: A New View Into The Magnetospheric Dynamics And Wave Phenomena Observed During The Event on May 10-12, 2024
- ST08: Auroral Dynamics and their impact on the geospace system
- ST09: General Session in Solar and Terrestrial Sciences Including Space Weather
- ST10: Advances in Magnetic Reconnection and Related Magnetic Structures: Observations, Theories, and Simulations
- ST11: Recent Progress in Observation and Modeling for Pre-eruptive Magnetic Configuration of Solar Eruptive Events
- ST12: Coupling Between Inner-magnetospheric, Ionospheric, and Thermospheric Particle Populations
- ST13: Space Instrumentation and Mission Concepts for Solar Terrestrial and Planetary Sciences
- ST14: Plasma Waves in the Terrestrial and Planetary Space Environment
- ST15: Modeling and Mitigation Techniques for Ionospheric Disturbance Effects on GNSS
- ST16: Space Weather Links from Sun to Earth Including May and October 2024 Events
- ST17: Advances in Our Understanding of Plasma Flows and Waves in the Solar Atmosphere from Single, Multi-fluid, and Kinetic Model Perspectives
- ST18: Observations and Simulations of the Ionospheric Electrodynamic Processes Driven by the External Drivers
- ST19: Solar Activity and Its Coupling with the Inner Heliosphere
- ST21: Small-scale Transients in the Solar Atmosphere and Beyond
- ST22: Advances in Monitoring, Modeling, and Forecasting Equatorial Plasma Bubbles
- ST24: Fundamental Physics in Heliospheric Plasmas: Waves, Turbulence, Reconnection, Structures, Shocks, and Field-particle Interactions
- ST25: Upper Atmosphere Disturbances Driven by Natural Events in the Solar Terrestrial Environment
- ST26: Enhancing Understanding of Upper Atmosphere Coupling Processes and Their Societal Impacts
- ST27: Solar-planetary Environment Observations and Modeling
- ST28: Precipitation of Energetic Particles: Magnetospheric Drivers and Their Impact on the Ionosphere
- ST29: Enhance Space Weather Prediction: Advanced Monitoring Techniques and Innovative Modeling
- ST30: Elemental Abundances and Dynamic Solar Activity from the Low Solar Atmosphere Into the Interplanetary Space
- ST31: Solar Cycle 25 and the Geomagnetic Field
- ST32: Coupling Processes from Space to the Atmosphere and Surface: Insights from Multi-instrument Observations
- ST33: Dynamics and Coupling in the Ionosphere, Thermosphere, and Mesosphere Driven by Forcing from Above and Below
- ST34: Understanding and Monitoring Space Weather and Geospace Hazards with the International Meridian Circle Project (imcp) and Related Facilities
- ST35: Solar Wind Dynamics Controlled by Collisions and Instabilities Influenced by Radial Expansion and the Background Large-amplitude Turbulence
- ST36: New Results from Low Earth Orbit (LEO) Space Environment Monitoring Satellites
- ST37: Space Weather Research and Operation in Asia-Oceania