Estimating Inner Magnetospheric Radial Diffusion Using a Hybrid-Vlasov Simulation

Estimating Inner Magnetospheric Radial Diffusion Using a Hybrid-Vlasov Simulation

Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagnetic field fluctuations in planetary radiation belts. Theoretically, radial diffusion occurs for an ensemble of particles that experience irreversible violation of their third adiabatic invariant, whi...

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Bibliographic Details
Main Authors: H. George, A. Osmane, E. K. J. Kilpua, S. Lejosne , L. Turc, M. Grandin, M. M. H. Kalliokoski, S. Hoilijoki, U. Ganse, M. Alho, M. Battarbee, M. Bussov, M. Dubart, A. Johlander, T. Manglayev, K. Papadakis, Y. Pfau-Kempf, J. Suni, V. Tarvus, H. Zhou, M. Palmroth
Format: Article
Language:English
Published: Frontiers Media S.A. 2022-05-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
radial diffusion coefficient
ULF waves
radiation belt
L-star
hybrid-Vlasov simulation
inner magnetosphere
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2022.866455/full

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https://www.frontiersin.org/articles/10.3389/fspas.2022.866455/full

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