Temporal variation of the distribution function and acceleration of O+ ions during substorm dipolarization
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[1] Wolfgang Baumjohann,et al. The terrestrial ring current: Origin, formation, and decay , 1999 .
[2] Junru Shi,et al. Theoretical study on the magnetospheric distribution of up-flowing ions , 1999 .
[3] W. E. Francis,et al. Distribution in magnetotail of O+ ions from cusp/cleft ionosphere: A possible substorm trigger , 1992 .
[4] I. Daglis,et al. Ionospheric contribution to the cross-tail current enhancement during the substorm growth phase , 1991 .
[5] T. Moore. Origins of magnetospheric plasma , 1991 .
[6] J. Sauvaud,et al. Cleft contribution to ring current formation , 1990 .
[7] J. Sauvaud,et al. Dynamics of single‐particle orbits during substorm expansion phase , 1990 .
[8] T. Moore,et al. A three‐dimensional numerical model of ionospheric plasma in the magnetosphere , 1989 .
[9] B. Mauk. Quantitative modeling of the “convection surge” mechanism of ion acceleration , 1986 .
[10] Donald J. Williams. Dynamics of the earth's ring current: Theory and observation , 1985 .
[11] N. Maynard,et al. Observations of large magnetospheric electric fields during the onset phase of a substorm , 1983 .
[12] J. Quinn,et al. Observations of parallel ion energization in the equatorial region , 1982 .
[13] A. Nishida. Origin of Magnetospheric Plasma , 1982 .
[14] E. Shelley,et al. Satellite observations of an ionospheric acceleration mechanism , 1976 .
[15] D. H. Fairfield,et al. A quantitative magnetospheric model derived from spacecraft magnetometer data , 1975 .
[16] E. Shelley,et al. SATELLITE OBSERVATIONS OF ENERGETIC HEAVY IONS DURING A GEOMAGNETIC STORM. , 1972 .