Cargando…
Formation of electron radiation belts at Saturn by Z-mode wave acceleration
At Saturn electrons are trapped in the planet’s magnetic field and accelerated to relativistic energies to form the radiation belts, but how this dramatic increase in electron energy occurs is still unknown. Until now the mechanism of radial diffusion has been assumed but we show here that in-situ a...
Autores principales: | Woodfield, E. E., Horne, R. B., Glauert, S. A., Menietti, J. D., Shprits, Y. Y., Kurth, W. S. |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2018
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6265320/ https://www.ncbi.nlm.nih.gov/pubmed/30498204 http://dx.doi.org/10.1038/s41467-018-07549-4 |
Ejemplares similares
-
Rapid Electron Acceleration in Low‐Density Regions of Saturn's Radiation Belt by Whistler Mode Chorus Waves
por: Woodfield, E. E., et al.
Publicado: (2019) -
Acceleration of Electrons by Whistler‐Mode Hiss Waves at Saturn
por: Woodfield, E. E., et al.
Publicado: (2022) -
Saturn Anomalous Myriametric Radiation, a New Type of Saturn Radio Emission Revealed by Cassini
por: Wu, S. Y., et al.
Publicado: (2022) -
Strong whistler mode waves observed in the vicinity of Jupiter’s moons
por: Shprits, Y. Y., et al.
Publicado: (2018) -
Electron Acceleration to MeV Energies at Jupiter and Saturn
por: Kollmann, P., et al.
Publicado: (2018)