Pitch angle distribution of relativistic electrons in the inner radiation belt and its relation to equatorial plasma wave turbulence phenomena

Geophysical Research Letters

Volumn 28, Issue 5, 2001, Pages 931-934

  Morioka, Akira ^a   Misawa, Hiroaki ^a   Miyoshi, Yoshizumi ^a   Oya, Hiroshi ^a   Iizima, Masahide ^a   Nagai, Tsugunobu ^b  

^a TOHOKU UNIVERSITY   (Japan)

^b TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

PLASMA WAVES; RADIATION; SATELLITES; TURBULENCE;

RELATIVISTIC ELECTRONS;

ELECTRONS;

MAGNETOSPHERE; PLASMA;

EID: 0035267467     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL011886     Document Type: Article

References (13)

1. Electron scattering loss in Earth's inner magnetosphere 1. Dominant physical processes
2. Electron scattering loss in Earth's inner magnetosphere 2. Sensitivity to model parameter
3. Electron and proton observations
4. The quiet time structure of energetic (35-560 keV) radiation belt electrons
5. Plasma wave observation and stimulation experiments (PWS) using Akebono (EXOS-D) satellite - Instrumentation and initial results including discovery of the high altitude equatorial plasma turbulence
6. Plasma turbulence disc circulating the equatorial regions of the plasmaphere identified by the plasma wace detector (PWS) onboard the Akebono (EXOS-D) satellite
7. Observation of space radiation environment with EXOS-D
8. Electromagnetic hiss and relativistic electron losses in the inner zone
9. Natural variations in the geomagnetically trapped electron population
10. The effect of atmospheric collisions on geomagnetically trapped electrons
11. Electron pitch angle distributions through-out the magnetosphere as observed on OGO 5
12. Observations of trapped electrons at low and high altitude