Diffusion Coefficients of Chorus, Hiss, and High Latitude Whistler-mode Waves at Jupiter

The electron diffusion coefficients due to whistler-mode chorus, hiss, and high-latitude whistler-mode waves at Jupiter are calculated. The calculation covers equatorial pitch angles from 0.5 to 89.5 degrees, energies from 30 eV to 30 MeV, and M shells from 5.5 to 13. The wave power distributions and frequency spectra are from Ma et al. (2024). The full diffusion code at Jupiter is used to calculate the diffusion coefficients (Ma et al., 2020). The diffusion coefficients can be used to analyze the electron scattering and acceleration due to whistler-mode waves in Jupiter's radiation belt.Ma,Q., Li,W., Zhang,X.-J., Bagenal,F. (2020). Energetic electron scattering due to whistler mode chorus waves using realistic magnetic field and density models in Jupiter's magnetosphere. Journal of Geophysical Research: Space Physics, 125, e2020JA027968. https://doi.org/10.1029/2020JA027968Ma,Q., Li,W., Zhang,X.-J., Kang,N., Bortnik,J., Qin,M., et al. (2024). Survey of whistler-mode wave amplitudes and frequency spectra in Jupiter's magnetosphere. Geophysical Research Letters, 51, e2024GL111882. https://doi.org/10.1029/2024GL111882.