Characteristics of the Pitch-Angle Anisotropy of Energetic Protons in the Daytime Magnetosphere due to Particle Drift in the Nondipole Magnetic Field
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Geophysics
Link
https://link.springer.com/content/pdf/10.1134/S001679322004009X.pdf
Reference28 articles.
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2. Anderson, B.J., Erlandson, R.E., and Zanetti, L.J., A statistical study of Pc1–2 magnetic pulsations in the equatorial magnetosphere: 1. Equatorial occurrence distributions, J. Geophys. Res., 1992, vol. 97, no. A3, pp. 3075–3088. https://doi.org/10.1029/91JA02706
3. Ganushkina, N.Yu., Liemohn, M.W., and Pulkkinen, T.I., Storm-time ring current: Model-dependent results, Ann. Geophys., 2012, vol. 30, pp. 177–202. https://doi.org/10.5194/angeo-30-177-2012
4. Hamlin, D.A., Karplus, R., Vik, R.C., and Watson, K.M., Mirror and azimuthal drift frequencies for geomagnetically trapped particles, J. Geophys. Res., 1961, vol. 66, pp. 1–5. https://doi.org/10.1029/JZ066i001p00001
5. Kennel, C.F. and Petschek, H.E., Limit of stably trapped particle fluxes, J. Geophys. Res., 1966, vol. 71, no. 1, pp. 1–28. https://doi.org/10.1029/JZ071i001p00001
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