Relativistic electrons near geostationary orbit: Evidence for internal magnetospheric acceleration

Geophysical Research Letters

Volumn 16, Issue 6, 1989, Pages 559-562

  Baker, D N ^a   Blake, J B ^b   Callis, L B ^c   Belian, R D ^d   Cayton, T E ^d  

^a NASA GODDARD SPACE FLIGHT CENTER   (United States)

^b AEROSPACE CORPORATION   (United States)

^c NASA LANGLEY RESEARCH CENTER   (United States)

^d LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 84989555020     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/GL016i006p00559     Document Type: Article

References (19)

1. High‐resolution energetic particle measurements at 6.6 RE
2. Do Jovian electrons influence the terrestrial outer radiation zone?
3. Highly relativistic electrons in the Earth's outer magnetosphere: 1
4. Highly relativistic magnetospheric electrons: A role in coupling to the middle atmosphere?
5. Theory of extragalactic radio sources
6. ULF electromagnetic turbulence in the high‐latitude topside ionosphere
7. Long term behavior of relativistic electrons observed in geostationary orbit
8. Energetic electron components at geosynchronous orbit
9. Equilibrium structure of radiation belt electrons
10. “Space weather forecase”: Prediction of relativistic electron intensity at synchronous orbit
11. Outward diffusion of energetic particles from the Jovian radiation belt
12. Recirculation of energetic particles in Jupiter's magnetosphere
13. Correction to “Recirculation of energetic particles in Jupiter's magnetosphee”
14. Energetic heavy ions with z > 4 in the equatorial radiation belts of the Earth: Magnetic storms
15. Electron pitch angle distributions throughout the magnetosphere as observed on Ogo 5