SM003
Advances in Radiation Belt Physics: Challenges in Models and Observations
Advances in Radiation Belt Physics: Challenges in Models and Observations
Session ID#: 72929
Session Description:
The energetic particles which form the Earth’s radiation belts are dynamically controlled by both microscopic and macroscopic acceleration, transport and loss processes. Recent spacecraft missions have provided unprecedented insights into the radiation belt response to driving conditions, and fast-increasing computational capabilities have allowed models to better explain these measurements. State-of-the-art models are now being used for radiation belt flux forecasting, as well as for studying more extreme scenarios for which fewer data are available. However, competing ideas for particle energisation and transport, and various physical and statistical modelling approaches, lead to the question, “what physics and processes are necessary to accurately predict radiation belt behaviour?” This session calls for all observational, modelling and theoretical contributions focussing on the radiation belts, and especially encourages efforts which contrast observational data with modelling results and vice versa, to help define the direction of radiation belt research into the space weather forecasting era.
Index Terms:
2720 Energetic particles: trapped [MAGNETOSPHERIC PHYSICS]
2722 Forecasting [MAGNETOSPHERIC PHYSICS]
2774 Radiation belts [MAGNETOSPHERIC PHYSICS]
7984 Space radiation environment [SPACE WEATHER]
Primary Convener: Ravindra Tobias Desai, Imperial College London, Physics, London, SW7, United Kingdom
Conveners: Richard Bertram Horne1, Nigel Peter Meredith1 and Wen Li2, (1)British Antarctic Survey, Cambridge, United Kingdom(2)Boston University, Boston, MA, United States
Primary Liaison: Ravindra Tobias Desai, Imperial College London, Physics, London, SW7, United Kingdom
See more of: SPA-Magnetospheric Physics
