Ultra‐relativistic acceleration of electrons in planetary magnetospheres
- 25 December 2007
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 34 (24)
- https://doi.org/10.1029/2007gl032226
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- Global MHD test particle simulations of >10 MeV radiation belt electrons during storm sudden commencementJournal of Geophysical Research, 2007
- Relativistic particle acceleration in the process of whistler‐mode chorus wave generationGeophysical Research Letters, 2007
- Dynamics of high‐energy electrons interacting with whistler mode chorus emissions in the magnetosphereJournal of Geophysical Research, 2006
- A revised model of Jupiter's inner electron belts: Updating the Divine radiation modelGeophysical Research Letters, 2005
- Relativistic electrons in the outer radiation belt: Differentiating between acceleration mechanismsJournal of Geophysical Research, 2004
- Rebuilding process of the outer radiation belt during the 3 November 1993 magnetic storm: NOAA and Exos‐D observationsJournal of Geophysical Research, 2003
- Model of the energization of outer‐zone electrons by whistler‐mode chorus during the October 9, 1990 geomagnetic stormGeophysical Research Letters, 2002
- Relativistic theory of wave‐particle resonant diffusion with application to electron acceleration in the magnetosphereJournal of Geophysical Research, 1998
- Comparative observations of plasma waves at the outer planetsAdvances in Space Research, 1992
- Detection of Jovian whistler mode chorus; Implications for the Io torus auroraGeophysical Research Letters, 1980