Favored regions for chorus-driven electron acceleration to relativistic energies in the Earth's outer radiation belt
Pitch angle and energy diffusion rates for scattering by whistler‐mode chorus waves are proportional to the wave magnetic field intensity and are strongly dependent on the frequency distribution of the waves and to the ratio between the electron plasma frequency (fpe) and the electron gyrofrequency...
Gespeichert in:
Veröffentlicht in: | Geophysical research letters 2003-08, Vol.30 (16), p.SSC7.1-n/a |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Schreiben Sie den ersten Kommentar!