EGU26-5350, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-5350
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 07 May, 11:00–11:10 (CEST)
 
Room 0.15
Enhanced radial diffusion of radiation belt electrons caused by field line 
Yiwei Hao
Yiwei Hao
  • Beihang University, School of Space and Earth Sciences, Beijing, China (tghyw0987@buaa.edu.cn)

The radial diffusion of radiation belt electrons due to interacting with ultra-low frequency (ULF) waves has traditionally been studied by assuming either a constant wave frequency at specific L drift-resonating with the electron or broad-band waves, resonating across a wider L range. We investigate a special case of radial diffusion caused by narrow-band ULF waves, generated by field line resonance (FLR), whose frequency varies with L in a manner that continuously satisfies the drift resonance condition throughout an electron’s radial motion. The conditions for this continuous resonance are derived for both non-relativistic and relativistic electrons in a dipolar magnetic field, which are further validated by two-dimensional test-particle simulations. The results show that, under conditions with inverse power-law relationship of -0.3~-0.5 between the wave frequency and L, relativistic electrons experience significantly enhanced radial diffusion, with the diffusion coefficient exceeding that of constant-frequency conditions by more than an order of magnitude.

How to cite: Hao, Y.: Enhanced radial diffusion of radiation belt electrons caused by field line , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5350, https://doi.org/10.5194/egusphere-egu26-5350, 2026.