The nonlinear response of AE to the IMF BS driver: A spectral break at 5 hours
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Edward J. Smith | Toshihiko Iyemori | Bruce T. Tsurutani | S.-I. Akasofu | Masahisa Sugiura | Walter D. Gonzalez | B. Tsurutani | W. Gonzalez | E. Smith | T. Iyemori | B. Goldstein | S. Akasofu | M. Sugiura | Bruce E. Goldstein
[1] J. Slavin,et al. Processes influencing the diurnal variation of the AL index and its reliability , 1981 .
[2] B. Tsurutani,et al. The cause of high-intensity long-duration continuous AE activity (HILDCAAs): Interplanetary Alfvén wave trains , 1987 .
[3] Syun-Ichi Akasofu,et al. The development of the auroral substorm. , 1964 .
[4] J. W. Dungey,et al. The length of the magnetospheric tail , 1965 .
[5] B. Tsurutani,et al. Solar wind-magnetosphere coupling during intense magnetic storms (1978-1979) , 1989 .
[6] B. Tsurutani,et al. Observations of the interplanetary sector structure up to heliographic latitudes of 16°: Pioneer 11 , 1978 .
[7] B. Tsurutani,et al. Interplanetary Alfvén waves and auroral (substorm) activity: IMP 8 , 1990 .
[8] Daniel N. Baker,et al. Magnetospheric Impulse Response for Many Levels of Geomagnetic Activity , 1985 .
[9] Robert L. McPherron,et al. Semiannual variation of geomagnetic activity , 1973 .
[10] D. Savoie,et al. Response of magnetosphere-ionosphere current systems to changes in the interplanetary magnetic field , 1988 .
[11] H. W. Kroehl,et al. Spatial and temporal distributions of magnetic effects of auroral electrojets as derived from AE indices , 1975 .