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How Does Solar Wind Control Earth’s Radiation Belt Dynamics?

London, 🇬🇧 United Kingdom
Oct 16, 2026
Onye Dike
Added by Onye Dike
Published Oct 6, 2026

Summary

Join the Royal Astronomical Society in London for a hybrid event exploring how solar wind influences Earth's radiation belt dynamics. This academic conference will feature discussions on solar-terrestrial coupling, wave-particle interactions, and future research directions.

Details

Location
London, 🇬🇧 United Kingdom & Online
Date
October 16th, 2026
Type
In Person & Online
Website
Registration

Learn more

Event Overview

This hybrid event is part of the Royal Astronomical Society's Specialist Discussion Meeting (SDM) program, scheduled for October 16, 2026, from 10:30 AM to 3:35 PM. It aims to unite experts from the UK and international communities to delve into the complexities of how solar wind affects Earth's radiation belts.

Key Topics

Participants will engage in discussions covering:

  • Solar-terrestrial coupling and radiation belt response: Examining dynamics driven by Coronal Mass Ejections (CMEs) and Corotating Interaction Regions (CIRs), along with substorm activities and particle acceleration.
  • Wave-particle interactions: Investigating how solar wind conditions influence plasma wave generation and subsequent particle acceleration and loss.
  • Modelling and future directions: Identifying gaps in current physics-based and data-driven models, and strategizing future missions to enhance understanding of these phenomena.

This event promises to be a significant opportunity for networking and collaboration among researchers and practitioners in the field. For more information and to register, visit the event page.


Onye Dike
Added by:
Onye Dike
Sustainability Research Analyst
Onye Dike is a Sustainability Research Analyst at Net Zero Compare, where he contributes to research and analysis on environmental regulations, carbon accounting, and emerging sustainability trends.
Added on Oct 6, 2026 by Onye Dike ·