Physical modeling of radiation belt response to geomagnetic storm: 2. On a 10 hour-10 day time scale

Advances in Space Research

Volumn 20, Issue 3, 1997, Pages 381-384

  Bourdarie, S ^a   Boscher, D ^a   Beutier, T ^b   Sauvaud, J A ^b   Blanc, M ^c  

^a ONERA   (France)

^b IRAP   (France)

^c OBSERVATOIRE MIDI PYRÉNÉES   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0041041482     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(97)00696-0     Document Type: Article

References (6)

1. Baker D.N., T.A. Fritz, B. Wilken, P.R. Higbie, S.M. Kaye, M.G. Kivelson, T.E. Moore, W. Stüdemann, A.J. Masley, P.H. Smith and A.L. Vampola, Observation and Modeling of Energetic Particles at Synchronous Orbit on July 29, 1977, J. Geophys. Res., 87, 5917, (1982).
2. E, J. Geophys. Res., 95, 15133, (1990).
3. Beutier T., and D. Boscher, A Three-Dimentional Analysis of the Electron Radiation Belt by the Salammbô Code, J. Geophys. Res., 100, 14853, (1995).
4. Lyons L.R., R.M. Thorne and C.F. Kennel, Pitch-Angle Diffusion of Radiation Belt Particles by Ion Cyclotron Waves, J. Geophys. Res., 77, 3455, (1972).
5. Schulz M. and L.J. Lanzerotti, Particle Diffusion in the Radiation Belts, Physics & Chemistry in space N 7, Springer-Verlag, (1974).
6. Schulz M., The Magnetosphere, in Geomagnetism, 4, 87, Academic Press, London, (1991).