Great geomagnetic storms in the rise and maximum of solar cycle 23

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Abstract

Geomagnetic storms are intervals of time when a sufficiently intense and long-lasting interplanetary convection electric field leads, through a substantial injection of energy into the magnetosphere-ionosphere system, to an intensified ring current, strong enough to exceed some key threshold of the quantifying storm time Dst index. We have studied all the 9 great magnetic storms (peak Dst

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Dal Lago, A., Vieira, L. E. A., Echer, E., Gonzalez, W. D., De Clúa Gonzalez, A. L., Guarnieri, F. L., … Schuch, N. J. (2004). Great geomagnetic storms in the rise and maximum of solar cycle 23. In Brazilian Journal of Physics (Vol. 34, pp. 1542–1546). Sociedade Brasileira de Fisica. https://doi.org/10.1590/S0103-97332004000800008

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