The EMERALD Model for the Estimation of the Radial Diffusion Coefficients in the Outer Belt

The EMERALD Model for the Estimation of the Radial Diffusion Coefficients in the Outer Belt

Abstract Radial diffusion is one of the dominant physical mechanisms driving acceleration and loss of electrons in the outer radiation belt. Therefore, the accurate estimation of radial diffusion coefficients (DLL) is crucial for detailed radiation belt modeling. In recent years several semi‐empiric...

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Bibliographic Details
Main Authors: S. Aminalragia‐Giamini, C. Katsavrias, C. Papadimitriou, I. A. Daglis, A. Nasi, A. Brunet, S. Bourdarie, N. Dahmen, G. Balasis
Format: Article
Language:English
Published: Wiley 2023-01-01
Series:Space Weather
Subjects:
neural networks
radial diffusion
ULF waves
radiation belts
solar wind
Online Access:https://doi.org/10.1029/2022SW003283
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https://doi.org/10.1029/2022SW003283

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